⁵ AA1J 18AM search for $H \to \mu\tau$ in 2.0 fb⁻¹ of pp collisions at $E_{cm} = 8$ TeV. The limit constrains the $Y_{\mu\tau}$ Yukawa coupling to $\sqrt{|Y_{\mu\tau}|^2 + |Y_{\tau\mu}|^2} < 1.7 \times 10^{-2}$ at 95% CL assuming SM production cross sections.

⁶ SIRUNYAN 18BH search for $H \to \mu\tau$ in 35.9 fb⁻¹ of pp collisions at $E_{cm} = 13$ TeV. The limit constrains the $Y_{\mu\tau}$ Yukawa coupling to $\sqrt{|Y_{\mu\tau}|^2 + |Y_{\tau\mu}|^2} < 1.43 \times 10^{-3}$ at 95% CL (see their Fig. 10).

⁷ AAD 17 search for $H \to \mu\tau$ in 20.3 fb⁻¹ of pp collisions at $E_{cm} = 8$ TeV.

⁸ KHACHATRYAN 15Q search for $H \to \mu\tau$ with $\tau$ decaying electronically or hadronically in 19.7 fb⁻¹ of pp collisions at $E_{cm} = 8$ TeV. The fit gives $B(H \to \mu\tau) = (0.84 \pm 0.39)\%$ with a significance of 2.4 $\sigma$.

$$ \Gamma(\text{invisible})/\Gamma_{\text{total}} $$

$$ \Gamma_{31}/\Gamma $$

Invisible final states.

<table><thead><tr><th>VALUE</th><th>CL%</th><th>DOCUMENT ID</th><th>TECN</th><th>COMMENT</th></tr></thead><tbody><tr><td>&lt;0.107</td><td>95</td><td>1 AAD</td><td>23A ATLS</td><td>pp, T, 8, 13 TeV</td></tr><tr><td colspan="5">• • • We do not use the following data for averages, fits, limits, etc. • • •</td></tr><tr><td>&lt;0.113</td><td>95</td><td>2 AAD</td><td>23A ATLS</td><td>pp, 13 TeV</td></tr><tr><td>&lt;0.38</td><td>95</td><td>3 AAD</td><td>23AF ATLS</td><td>pp → t<span style="text-decoration: overline">T</span>H, 13 TeV</td></tr><tr><td>&lt;0.54</td><td>95</td><td>4 TUMASYAN</td><td>23BA CMS</td><td>pp → t<span style="text-decoration: overline">T</span>H, V(→ q<span style="text-decoration: overline">q</span>)<br>H, 13 TeV</td></tr><tr><td>&lt;0.15</td><td>95</td><td>5 TUMASYAN</td><td>23BA CMS</td><td>pp, 7, 8, 13 TeV</td></tr><tr><td>&lt;0.19</td><td>95</td><td>6 AAD</td><td>22D ATLS</td><td>pp → ZH, 13 TeV</td></tr><tr><td>&lt;0.145</td><td>95</td><td>7 AAD</td><td>22P ATLS</td><td>pp → qqH, 13 TeV</td></tr><tr><td>&lt;0.37</td><td>95</td><td>8 AAD</td><td>22S ATLS</td><td>pp → qqH<span style="text-decoration: overline">H</span>, 13 TeV</td></tr><tr><td>&lt;0.13</td><td>95</td><td>9 ATLAS</td><td>22 ATLS</td><td>pp, 13 TeV</td></tr><tr><td>&lt;0.16</td><td>95</td><td>10 CMS</td><td>22 CMS</td><td>pp, 13 TeV</td></tr><tr><td>&lt;0.18</td><td>95</td><td>11 TUMASYAN</td><td>22G CMS</td><td>pp → qqH, 8, 13 TeV</td></tr><tr><td>&lt;0.18</td><td>95</td><td>12 TUMASYAN</td><td>22G CMS</td><td>pp → qqH, 13 TeV</td></tr><tr><td>&lt;0.34</td><td>95</td><td>13 AAD</td><td>21F ATLS</td><td>pp, 13 TeV</td></tr><tr><td>&lt;0.29</td><td>95</td><td>14 SIRUNYAN</td><td>21A CMS</td><td>pp → ZH, 13 TeV</td></tr><tr><td>&lt;0.278</td><td>95</td><td>15 TUMASYAN</td><td>21D CMS</td><td>pp, 13 TeV, jet or V(→ q<span style="text-decoration: overline">q</span>)</td></tr><tr><td>&lt;0.37</td><td>95</td><td>16 AABOUD</td><td>19AI ATLS</td><td>pp → qqH, 13 TeV</td></tr><tr><td>&lt;0.38</td><td>95</td><td>17 AABOUD</td><td>19AL ATLS</td><td>pp, 13 TeV</td></tr><tr><td>&lt;0.26</td><td>95</td><td>18 AABOUD</td><td>19AL ATLS</td><td>pp, 7, 8, 13 TeV</td></tr><tr><td>&lt;0.22</td><td>95</td><td>19 SIRUNYAN</td><td>19AT CMS</td><td>pp, 13 TeV</td></tr><tr><td>&lt;0.33</td><td>95</td><td>20 SIRUNYAN</td><td>19BO CMS</td><td>pp → qqH, 13 TeV</td></tr><tr><td>&lt;0.26</td><td>95</td><td>21 SIRUNYAN</td><td>19BO CMS</td><td>pp, 13 TeV</td></tr><tr><td>&lt;0.19</td><td>95</td><td>22 SIRUNYAN</td><td>19BO CMS</td><td>pp, 7, 8, 13 TeV</td></tr><tr><td>&lt;0.67</td><td>95</td><td>23 AABOUD</td><td>18 ATLS</td><td>pp → ZH, 13 TeV</td></tr><tr><td>&lt;0.83</td><td>95</td><td>24 AABOUD</td><td>18CA ATLS</td><td>pp → WH/ZH,<br>W/Z → jj, 13 TeV</td></tr><tr><td>&lt;0.40</td><td>95</td><td>25 SIRUNYAN</td><td>18BV CMS</td><td>pp → ZH, 13 TeV</td></tr><tr><td>&lt;0.53</td><td>95</td><td>26 SIRUNYAN</td><td>18S CMS</td><td>pp, 13 TeV, jet or V(→ q<span style="text-decoration: overline">q</span>)</td></tr><tr><td>&lt;0.46</td><td>95</td><td>27 AABOUD</td><td>17BD ATLS</td><td>pp, Hj, qqH, 13 TeV</td></tr><tr><td>&lt;0.24</td><td>95</td><td>28 KHACHATRY..17f CMS</td><td>pp, T, 8, 13 TeV</td><td></td></tr><tr><td>&lt;0.28</td><td>95</td><td>29 AAD</td><td>16AF ATLS</td><td>pp → qqH, 8 TeV</td></tr><tr><td>&lt;0.34</td><td>95</td><td>30 AAD</td><td>16AN LHC</td><td>pp, T, 8 TeV</td></tr><tr><td>&lt;0.78</td><td>95</td><td>31 AAD</td><td>15BD ATLS</td><td>pp → WH/ZH, 8 TeV</td></tr><tr><td>&lt;0.25</td><td>95</td><td>32 AAD</td><td>15CX ATLS</td><td>pp, T, 8 TeV</td></tr><tr><td>&lt;0.75</td><td>95</td><td>33 AAD</td><td>140 ATLS</td><td>pp → ZH, 7, 8 TeV</td></tr><tr><td>&lt;0.58</td><td>95</td><td>34 CHATRCHYAN 14B CMS</td><td>pp → ZH, qqH</td><td></td></tr><tr><td>&lt;0.81</td><td>95</td><td>35 CHATRCHYAN 14B CMS</td><td>pp → ZH, 7, 8 TeV</td><td></td></tr><tr><td>&lt;0.65</td><td>95</td><td>36 CHATRCHYAN 14B CMS</td><td>pp → qqH, 8 TeV</td><td></td></tr></tbody></table>

¹ AAD 23A report the combined results of 7, 8 (AAD 15Cx) and 13 TeV assuming the Standard Model cross section ($m_H = 125$ GeV). See their Table 1 and Fig. 3.

² AAD 23A report the combined results using 139 fb⁻¹ of data at $E_{cm} = 13$ TeV, where $H$ decaying to invisible final states in VBF (AAD 22p), $ZH, Z \to e, \mu, \mu$ (AAD 22d), $pp \to t<span style="text-decoration: overline">T</span>H (AAD 23AF), VBF + $\gamma$ (AAD 22s) and gluon-fusion production with an energetic jet (AAD 21f) assuming the Standard Model cross section ($m_H = 125$ GeV). See their Table 1 and Fig. 3.

³ AAD 23A search for $pp \to t<span style="text-decoration: overline">T</span>H with $H$ decaying to invisible final states using 139 fb⁻¹ of data. The quoted limit on the branching ratio is given for $m_H = 125$ GeV and assumes the Standard Model cross section. See their Table 3 for different decay topologies.

⁴ TUMASYAN 23BA search for $H$ decaying to invisible final states produced in association with a $t\bar{t}$ or a $V$, which decay to a fully hadronic final state. 138 fb⁻¹ of data is used. The quoted limit on the branching ratio is given for $m_H = 125$ GeV and assumes the Standard Model cross section. See their Fig. 6 for the results of individual topologies.

⁵ TUMASYAN 23BA report the combined results of 7, 8, and 13 TeV assuming the Standard Model cross section ($m_H = 125$ GeV). They combine results from TUMASYAN 22G, SIRUNYAN 21A, SIRUNYAN 21b, TUMASYAN 21D, SIRUNYAN 20AH, KHACHATRYAN 17F, CHATRCHYAN 14B as shown in their Table 8. See their Fig. 7 and Table 9 for the results of individual topologies.

⁶ AAD 22d search for $H$ decaying to invisible final states associated with a $Z$ decaying $ee/\mu\mu$ using 139 fb⁻¹ at 13 TeV. The limit is obtained for $m_H = 125$ GeV and assuming the SM $ZH$ production cross section. The branching ratio is obtained to be $(0.3 \pm 9.0)\%$.

⁷ AAD 22p search for $pp \to qqH\chi$ (VBF) with $H$ decaying to invisible final states using 139 fb⁻¹ of data. The quoted limit on the branching ratio is given for $m_H = 125$ GeV and assumes the Standard Model cross section.

⁸ AAD 22s observe electroweak $Z(\to \nu\nu)\gamma+2$jets production process with 139 fb⁻¹ of data. This result is applicable to search for $pp \to qqH\gamma\chi$ (VBF + $\gamma$) with $H$ decaying to invisible final states. The quoted limit on the branching ratio is given for $m_H = 125$ GeV and assumes the Standard Model cross section.

⁹ ATLAS 22 report the combined results using 139 fb⁻¹ of data at $E_{cm} = 13$ TeV, where $H$ decaying to invisible final states in VBF (AAD 22p), and $ZH, Z \to e, \mu, \mu$ (AAD 22d), assuming $\kappa_V \le 1$ and $B_{undetected} \ge 0$.

¹⁰ CMS 22 report the combined results using (a part of) 138 fb⁻¹ of data at $E_{cm} = 13$ TeV, where $H$ decaying to invisible final states in VBF (SIRUNYAN 19bO), associated with an energetic jet or a $V(\to q\bar{q})$ (TUMASYAN 21D), and $ZH, Z \to e, \mu, \mu$ (SIRUNYAN 21A) and assuming $\kappa_V \le 1$ and $B_{undetected} \ge 0$.

¹¹ TUMASYAN 22G combine 13 TeV 101 fb⁻¹ results with 8 TeV (KHACHATRYAN 17f) and other 13 TeV (KHACHATRYAN 17f for 2015 and SIRUNYAN 19bO for 2016) for $H$ decaying to invisible final states with VBF topology. The quoted limit on the branching ratio is given for $m_H = 125.38$ GeV and assumes the Standard Model production rates. The branching ratio is obtained to be $0.086 \pm 0.054$. See their Figs. 11 and 12.

¹² TUMASYAN 22G search for $pp \to qqH\chi$ (VBF) with $H$ decaying to invisible final states using 101 fb⁻¹ of data (2017 and 2018). The quoted limit on the branching ratio is given for $m_H = 125.38$ GeV and assumes the Standard Model cross section. See their Figs. 11 and 12.

¹³ AAD 21F search for an invisibly decaying Higgs boson with an energetic jet ($p_T > 150$ GeV) and missing transverse momentum ($> 200$ GeV) in 139 fb⁻¹ at $E_{cm} = 13$ TeV. The quoted limit on the branching ratio is given for $m_H = 125$ GeV.

¹⁴ SIRUNYAN 21A search for $H$ decaying to invisible final states associated with a $Z$ decaying $ee/\mu\mu$ using 137 fb⁻¹ at 13 TeV. The limit is obtained for $m_H = 125$ GeV and assuming the SM $ZH$ production cross section.

¹⁵ TUMASYAN 21D search for $H$ decaying to invisible final states associated with an energetic jet or a $V, V \to q\bar{q}$ using 101 fb⁻¹ at 13 TeV and the result is combined with SIRUNYAN 18s.

¹⁶ AABOUD 19AI search for $pp \to qqH\chi$ (VBF) with $H$ decaying to invisible final states using 36.1 fb⁻¹ of data. The quoted limit on the branching ratio is given for $m_H = 125$ GeV and assumes the Standard Model rates for VBF and gluon-fusion production.

¹⁷ AABOUD 19AL combine results of $H$ decaying to invisible final states with VBF (AABOUD 19AI), $ZH$, and $WH$ productions (AABOUD 18, AABOUD 18CA), which use 36.1 fb⁻¹ of data at 13 TeV. The quoted limit is given for $m_H = 125$ GeV and assumes the Standard Model rates for gluon fusion, VBF, $ZH$, and $WH$ productions.

¹⁸ AABOUD 19AL combine results of 7, 8 (AAD 15Cx), and 13 TeV for $H$ decaying to invisible final states.

¹⁹ SIRUNYAN 19AT perform a combined fit with visible decay using 35.9 fb⁻¹ of data at 13 TeV.

²⁰ SIRUNYAN 19BO search for $pp \to qqH\chi$ (VBF) with $H$ decaying to invisible final states using 35.9 fb⁻¹ of data. The quoted limit on the branching ratio is given for $m_H = 125.09$ GeV and assumes the Standard Model production rates.

²¹ SIRUNYAN 19BO combine the VBF channel with results of other 13 TeV analyses: SIRUNYAN 18BV and SIRUNYAN 18s. The quoted limit on the branching ratio is given for $m_H = 125.09$ GeV and assumes the Standard Model production rates.

²² SIRUNYAN 19BO combine 13 TeV 35.9 fb⁻¹ results with 7, 8, 13 TeV (KHACHATRYAN 17f) for $H$ decaying to invisible final states. The quoted limit on the branching ratio is given for $m_H = 125.09$ GeV and assumes the Standard Model production rates. The branching ratio is obtained to be $0.05 \pm 0.03$ (stat) $\pm 0.07$ (syst).

²³ AABOUD 18 search for $pp \to HZX, Z \to e, \mu, \mu$ with $H$ decaying to invisible final states in 36.1 fb⁻¹ at $E_{cm} = 13$ TeV. The quoted limit on the branching ratio is given for $m_H = 125$ GeV and assumes the Standard Model rate for $HZ$ production.

²⁴ AABOUD 18CA search for $H$ decaying to invisible final states using $WH$, and $ZH$ productions, where $W$ and $Z$ hadronically decay. The data of 36.1 fb⁻¹ at $E_{cm} = 13$ TeV is used. The quoted limit assumes SM production cross sections with combining the contributions from $WH, ZH, ZgF$ and VBF production modes.

²⁵ SIRUNYAN 18BV search for $H$ decaying to invisible final states associated with a $Z, Z \to \ell\ell$ using 35.9 fb⁻¹ at 13 TeV. The limit is obtained for $m_H = 125$ GeV and assuming the SM $ZH$ production cross section.

²⁶ SIRUNYAN 18s search for $H$ decaying to invisible final states associated with an energetic jet or a $V, V \to q\bar{q}$ using 35.9 fb⁻¹ at 13 TeV.

²⁷ AABOUD 17BD search for $H$ decaying to invisible final states with $\ge 1$ jet and VBF events using 3.2 fb⁻¹ of $pp$ collisions at $E_{cm} = 13$ TeV. A cross-section ratio $R^{\text{miss}}$ is used in the measurement. The quoted limit is given for $m_H = 125$ GeV.

²⁸ KHACHATRYAN 17F search for $H$ decaying to invisible final states with gluon fusion, VBF, $ZH$, and $WH$ productions using 2.3 fb⁻¹ of $pp$ collisions at $E_{cm} = 13$ TeV, 19.7 fb⁻¹ at 8 TeV, and 5.1 fb⁻¹ at 7 TeV. The quoted limit is given for $m_H = 125$ GeV and assumes the Standard Model rates for gluon fusion, VBF, $ZH$, and $WH$ productions.

²⁹ AAD 16AF search for $pp \to qqH\chi$ (VBF) with $H$ decaying to invisible final states in 20.3 fb⁻¹ at $E_{cm} = 8$ TeV. The quoted limit on the branching ratio is given for $m_H = 125$ GeV and assumes the Standard Model rates for VBF and gluon-fusion production.

³⁰ AAD 16AN perform fits to the ATLAS and CMS data at $E_{cm} = 7$ and 8 TeV. The branching fraction of decays into BSM particles that are invisible or into undetected decay modes is measured for $m_0 = 125.09$ GeV.

³¹ AAD 15BD search for $pp \to HWX$ and $pp \to HZX, W \to Z$ decaying hadronically and $H$ decaying to invisible final states using data at $E_{cm} = 8$ TeV. The quoted limit is given for $m_H = 125$ GeV, assumes the Standard Model rates for the production processes and is based on a combination of the contributions from $WH, HZ$ and the gluon-fusion process.

³² AAD 15Cx search for $H$ decaying to invisible final states with VBF, $ZH$, and $WH$ productions using 20.3 fb⁻¹ at 8 TeV, and 4.7 fb⁻¹ at 7 TeV. The quoted limit is given for $m_H = 125.36$ GeV and assumes the Standard Model rates for gluon fusion, VBF, $ZH$, and $WH$ productions. The upper limit is improved to 0.23 by adding the measured visible decay rates.

³³ AAD 14O search for $pp \to HZX, Z \to \ell\ell$, with $H$ decaying to invisible final states in 4.5 fb⁻¹ at $E_{cm} = 7$ TeV and 20.3 fb⁻¹ at $E_{cm} = 8$ TeV. The quoted limit on the branching ratio is given for $m_H = 125.5$ GeV and assumes the Standard Model rate for $HZ$ production.

³⁴ CHATRCHYAN 14B search for $pp \to HZX, Z \to \ell\ell$ and $Z \to b\bar{b}$, and also $pp \to qqH\chi$ with $H$ decaying to invisible final states using data at $E_{cm} = 7$ and 8 TeV. The quoted limit on the branching ratio is obtained from a combination of the limits from $HZ$ and $qqH$. It is given for $m_H = 125$ GeV and assumes the Standard Model rates for the two production processes.

³⁵ CHATRCHYAN 14B search for $pp \to HZX$ with $H$ decaying to invisible final states and $Z \to \ell\ell$ in 4.9 fb⁻¹ at $E_{cm} = 7$ TeV and 19.7 fb⁻¹ at $E_{cm} = 8$ TeV, and also with $Z \to b\bar{b}$ in 18.9 fb⁻¹ at $E_{cm} = 8$ TeV. The quoted limit on the branching ratio is given for $m_H = 125$ GeV and assumes the Standard Model rate for $HZ$ production.

³⁶ CHATRCHYAN 14B search for $pp \to qqH\chi$ (vector boson fusion) with $H$ decaying to invisible final states in 19.5 fb⁻¹ at $E_{cm} = 8$ TeV. The quoted limit on the branching ratio is given for $m_H = 125$ GeV and assumes the Standard Model rate for $qqH$ production.
$\Gamma(\gamma\text{invisible})/\Gamma_{\text{total}}$

$\Gamma_{32}/\Gamma$

<table><thead><tr><th>VALUE</th><th>CL%</th><th>DOCUMENT ID</th><th>TECN</th><th>COMMENT</th></tr></thead><tbody><tr><td>&lt;0.029</td><td>95</td><td>1,2 SIRUNYAN</td><td>21L CMS</td><td>VBF, HZ, H → γ + invisible, 13 TeV</td></tr></tbody></table>

• • • We do not use the following data for averages, fits, limits, etc. • • •

<table><tbody><tr><td>&lt;0.035</td><td>95</td><td>1 SIRUNYAN</td><td>21L CMS</td><td>VBF, H → γ + invisible, 13 TeV</td></tr><tr><td>&lt;0.046</td><td>95</td><td>3 SIRUNYAN</td><td>19CG CMS</td><td>pp → HZ, H → γ + invisible, Z → ℓℓ, 13 TeV</td></tr></tbody></table>

¹SIRUNYAN 21L search for H decaying to an invisible final state plus a γ in the VBF production using 130 fb⁻¹ data at $E_{cm} = 13$ TeV. The invisible state is called a dark photon. The quoted limit on the branching ratio is given for $m_H = 125$ GeV assuming the Standard Model rates.

²The result of the VBF production is combined with the $pp \to HZ$ result (SIRUNYAN 19CG).

³SIRUNYAN 19CG search for $pp \to HZ, Z \to ee, \mu\mu$ with H decaying to invisible final states plus a γ in 137 fb⁻¹ at $E_{cm} = 13$ TeV. The quoted limit on the branching ratio is given for $m_H = 125$ GeV assuming the Standard Model rate for HZ production and is obtained in the context of a theoretical model, where the undetected (invisible) particle is massless.

## H SIGNAL STRENGTHS IN DIFFERENT CHANNELS

The H signal strength in a particular final state xx is given by the cross section times branching ratio in this channel normalized to the Standard Model (SM) value, $\sigma \cdot B(H \to xx) / (\sigma \cdot B(H \to xx))_{SM}$, for the specified mass value of H. For the SM predictions, see DITTMAIER 11, DITTMAIER 12, and HEINEMEYER 13A. Results for fiducial and differential cross sections are also listed below.

### Combined Final States

<table><thead><tr><th>VALUE</th><th>DOCUMENT ID</th><th>TECN</th><th>COMMENT</th></tr></thead><tbody><tr><td>1.03 ±0.04</td><td colspan="3">OUR AVERAGE</td></tr><tr><td>1.05 ±0.06</td><td>1 ATLAS</td><td>22 ATLS</td><td>pp, 13 TeV</td></tr><tr><td>1.002±0.057</td><td>2 CMS</td><td>22 CMS</td><td>pp, 13 TeV</td></tr><tr><td>1.09 ±0.07</td><td>3,4 AAD</td><td>16AN LHC</td><td>pp, 7, 8 TeV</td></tr><tr><td>1.44</td><td>5 AALTONEN</td><td>13M TEVA</td><td>p<span style="text-decoration: overline">p</span> → HX, 1.96 TeV</td></tr><tr><td>1.11</td><td>6 AAD</td><td>20 ATLS</td><td>pp, 13 TeV</td></tr><tr><td>1.17</td><td>7 SIRUNYAN</td><td>19AT CMS</td><td>pp, 13 TeV</td></tr><tr><td></td><td>8 SIRUNYAN</td><td>19BA CMS</td><td>pp, 13 TeV, differential cross sections</td></tr><tr><td>1.20 ±0.10</td><td>4 AAD</td><td>16AN ATLS</td><td>pp, 7, 8 TeV</td></tr><tr><td>0.97 ±0.09</td><td>4 AAD</td><td>16AN CMS</td><td>pp, 7, 8 TeV</td></tr><tr><td>1.18 ±0.10</td><td>9 AAD</td><td>16K ATLS</td><td>pp, 7, 8 TeV</td></tr><tr><td>0.75</td><td>9 AAD</td><td>16K ATLS</td><td>pp, 7 TeV</td></tr><tr><td>1.28 ±0.11</td><td>9 AAD</td><td>16K ATLS</td><td>pp, 8 TeV</td></tr><tr><td>1.00 ±0.09</td><td>10 AAD</td><td>15P ATLS</td><td>pp, 8 TeV, cross section</td></tr><tr><td>1.33</td><td>11 AAD</td><td>13K ATLS</td><td>pp, 7, 8 TeV</td></tr><tr><td>1.54</td><td>12 AAD</td><td>13AK ATLS</td><td>pp, 7 and 8 TeV</td></tr><tr><td>1.40</td><td>13 AALTONEN</td><td>13L CDF</td><td>p<span style="text-decoration: overline">p</span> → HX, 1.96 TeV</td></tr><tr><td>1.40</td><td>14 ABAZOV</td><td>13L D0</td><td>p<span style="text-decoration: overline">p</span> → HX, 1.96 TeV</td></tr><tr><td>1.4</td><td>15 AAD</td><td>12AI ATLS</td><td>pp → HX, 7, 8 TeV</td></tr><tr><td>1.2</td><td>15 AAD</td><td>12AI ATLS</td><td>pp → HX, 7 TeV</td></tr><tr><td>1.5</td><td>15 AAD</td><td>12AI ATLS</td><td>pp → HX, 8 TeV</td></tr><tr><td>0.87 ±0.23</td><td>16 CHATRCHYAN 12N CMS</td><td>pp → HX, 7, 8 TeV</td><td></td></tr></tbody></table>

¹ATLAS 22 report combined results (see their Extended Data Table 1) using up to 139 fb⁻¹ of data at $E_{cm} = 13$ TeV, assuming $m_H = 125.09$ GeV. The Higgs production cross-sections, branching fractions and several ratios are found in their Figs. 2 and 3.

²CMS 22 report combined results (see their Extended Data Table 2) using 138 fb⁻¹ of data at $E_{cm} = 13$ TeV, assuming $m_H = 125.38$ GeV. Signal strengths for production modes and decay channels are found in their Fig. 2.

³AAD 16AN perform fits to the ATLAS and CMS data at $E_{cm} = 7$ and 8 TeV. The signal strengths for individual production processes are 1.03±0.16 for gluon fusion, 1.18±0.25 for vector boson fusion, 0.89±0.40 for W H production, 0.79±0.36 for Z H production, and 2.3±0.6 for $t\bar{t}H$ production.

⁴AAD 16AN: The uncertainties represent statistics, experimental systematics, and added in quadrature theory systematics on the background and on the signal. The quoted signal strengths are given for $m_H = 125.09$ GeV. In the fit, relative branching ratios and relative production cross sections are fixed to those in the Standard Model.

⁵AALTONEN 13M combine all Tevatron data from the CDF and D0 Collaborations with up to 10.0 fb⁻¹ and 9.7 fb⁻¹, respectively, of $p\bar{p}$ collisions at $E_{cm} = 1.96$ TeV. The quoted signal strength is given for $m_H = 125$ GeV.

⁶AAD 20 combine results of up to 79.8 fb⁻¹ of data at $E_{cm} = 125.09$ GeV: $\gamma\gamma, ZZ^*, WW^*, \tau\tau, b\bar{b}, \mu\mu$, invisible, and off-shell analyses (see their Table I). The signal strengths for individual production processes are 1.04±0.09 for gluon fusion, 1.21±0.24 for vector boson fusion, 1.30±0.40 for W H production, 1.05±0.31 for $t\bar{t}H$, and 1.21±0.26 for $t\bar{t}H+tH$ production (see their Fig. 2 and Table IV). Several results with the simplified template cross section and $\kappa$-frameworks are presented: see their Figs. 9–11, Figs. 20, 21 and Table VIII for stage-1 simplified template cross sections, their Figs. 12–17 and Tables X–XII for the $\kappa$-framework.

⁷SIRUNYAN 19AT combine results of 35.9 fb⁻¹ of data at $E_{cm} = 13$ TeV, assuming $m_H = 125.09$ GeV. The signal strengths for individual production processes are 1.22±0.14 for gluon fusion, 0.73±0.30 for vector boson fusion, 2.18±0.58 for W H production, 0.87±0.44 for Z H production, and 1.18±0.30 for $t\bar{t}H$ production. Several results with the simplified template cross section and $\kappa$-frameworks are presented: see their Fig. 8 and Table 5 for stage-0 simplified template cross sections, their Figs. 9–18 and Tables 7–11 for the $\kappa$-framework.

⁸SIRUNYAN 19BA measure differential cross sections for the Higgs boson transverse momentum, the number of jets, the rapidity of the Higgs boson and the transverse momentum of the leading jet using 35.9 fb⁻¹ of data at $E_{cm} = 13$ TeV with $H \to \gamma\gamma, H \to ZZ^*$, and $H \to b\bar{b}$. The total cross section for Higgs boson production is measured to be 61.1±6.0±3 pb using $H \to \gamma\gamma$ and $H \to ZZ^*$ channels. Several coupling measurements in the $\kappa$-framework are performed.

⁹AAD 16K use up to 4.7 fb⁻¹ of $pp$ collisions at $E_{cm} = 7$ TeV and up to 20.3 fb⁻¹ at $E_{cm} = 8$ TeV. The third uncertainty in the measurement is theory systematics. The signal strengths for individual production modes are 1.23±0.14±0.09±0.16 for gluon fusion, 1.23±0.28±0.13±0.11 for vector boson fusion, 0.80±0.31±0.10 for $t\bar{t}H$ production, 1.16±0.37±0.38 for W H production, and 1.81±0.52±0.58±0.31 for $t\bar{t}H$ production. The quoted signal strengths are given for $m_H = 125.36$ GeV.

¹⁰AAD 15P measure total and differential cross sections of the process $pp \to HX$ at $E_{cm} = 8$ TeV with 20.3 fb⁻¹. $\gamma\gamma$ and $4\ell$ final states are used. $\sigma(pp \to HX) = 33.0 \pm 5.3 \pm 1.6$ pb is given. See their Figs. 2 and 3 for data on differential cross sections.

¹¹KHACHATRYAN 15AM use up to 5.1 fb⁻¹ of $pp$ collisions at $E_{cm} = 7$ TeV and up to 19.7 fb⁻¹ at $E_{cm} = 8$ TeV. The third uncertainty in the measurement is theory systematics. Fits to each production mode give the value of 0.85±0.19 for gluon fusion, 1.16±0.37 for vector boson fusion, 0.92±0.38 for W H, Z H production, and 2.90±0.94 for $t\bar{t}H$ production.

¹²AAD 13AK use 4.7 fb⁻¹ of $pp$ collisions at $E_{cm} = 7$ TeV and 20.7 fb⁻¹ at $E_{cm} = 8$ TeV. The combined signal strength is based on the $\gamma\gamma, ZZ^* \to 4\ell$, and $WW^* \to \ell\nu\ell\nu$ channels. The quoted signal strength is given for $m_H = 125.5$ GeV. Reported statistical error value modified following private communication with the experiment.

¹³AALTONEN 13L combine all CDF results with 9.45–10.0 fb⁻¹ of $p\bar{p}$ collisions at $E_{cm} = 1.96$ TeV. The quoted signal strength is given for $m_H = 125$ GeV.

¹⁴ABAZOV 13L combine all D0 results with up to 9.7 fb⁻¹ of $p\bar{p}$ collisions at $E_{cm} = 1.96$ TeV. The quoted signal strength is given for $m_H = 125$ GeV.

¹⁵AAD 12AI obtain results based on 4.6–4.8 fb⁻¹ of $pp$ collisions at $E_{cm} = 7$ TeV and 5.8–5.9 fb⁻¹ at $E_{cm} = 8$ TeV. An excess of events over background with a local significance of 5.9 $\sigma$ is observed at $m_H = 126$ GeV. The quoted signal strengths are given for $m_H = 126$ GeV. See also AAD 12DA.

¹⁶CHATRCHYAN 12N obtain results based on 4.9–5.1 fb⁻¹ of $pp$ collisions at $E_{cm} = 7$ TeV and 5.1–5.3 fb⁻¹ at $E_{cm} = 8$ TeV. An excess of events over background with a local significance of 5.0 $\sigma$ is observed at about $m_H = 125$ GeV. The combined signal strength is based on the $\gamma\gamma, ZZ^*, WW^*, \tau^+\tau^-$, and $b\bar{b}$ channels. The quoted signal strength is given for $m_H = 125.5$ GeV. See also CHATRCHYAN 13Y.

## W W* Final State

<table><thead><tr><th>VALUE</th><th>DOCUMENT ID</th><th>TECN</th><th>COMMENT</th></tr></thead><tbody><tr><td>1.00±0.08</td><td colspan="3">OUR AVERAGE</td></tr><tr><td>0.97±0.09</td><td>1 CMS</td><td>22 CMS</td><td>pp, 13 TeV</td></tr><tr><td>1.09±0.18</td><td>2,3 AAD</td><td>16AN LHC</td><td>pp, 7, 8 TeV</td></tr><tr><td>0.94±0.85</td><td>4 AALTONEN</td><td>13M TEVA</td><td>p<span style="text-decoration: overline">p</span> → HX, 1.96 TeV</td></tr><tr><td>1.28±0.17</td><td>5 AAD</td><td>23AP ATLS</td><td>pp, 13 TeV, cross sections</td></tr><tr><td>1.28±0.18</td><td>6 AAD</td><td>23BV ATLS</td><td>pp, 13 TeV, cross sections</td></tr><tr><td>1.22±0.23</td><td>3 AAD</td><td>16AN CMS</td><td>pp, 7, 8 TeV</td></tr><tr><td>0.90±0.23</td><td>3 AAD</td><td>16AN CMS</td><td>pp, 7, 8 TeV</td></tr><tr><td>1.18±0.16</td><td>21 AAD</td><td>16AO ATLS</td><td>pp, 8 TeV, cross sections</td></tr><tr><td>1.09±0.16</td><td>22 AAD</td><td>16K ATLS</td><td>pp, 7, 8 TeV</td></tr><tr><td>1.09±0.17</td><td>23 AAD</td><td>15AA ATLS</td><td>pp, 7, 8 TeV</td></tr></tbody></table>
<table><tbody><tr><td>3.0</td><td>+1.3<br>-1.1</td><td>+1.0<br>-0.7</td><td>24 AAD</td><td>15AQ ATLS</td><td>pp → HW/ZX, 7, 8 TeV</td></tr><tr><td>1.16</td><td>+0.16+0.18<br>-0.15-0.15</td><td></td><td>25 AAD</td><td>15AQ ATLS</td><td>pp, 7, 8 TeV</td></tr><tr><td>0.72</td><td>+0.12±0.10<br>-0.10-0.12</td><td></td><td>26 CHATRCHYAN 14G</td><td>CMS</td><td>pp, 7, 8 TeV</td></tr><tr><td>0.99</td><td>+0.31<br>-0.28</td><td></td><td>27 AAD</td><td>13AK ATLS</td><td>pp, 7 and 8 TeV</td></tr><tr><td>0.00</td><td>+1.78<br>-0.00</td><td></td><td>28 AALTONEN</td><td>13L CDF</td><td>p<span style="text-decoration: overline">p</span> → HX, 1.96 TeV</td></tr><tr><td>1.90</td><td>+1.63<br>-1.52</td><td></td><td>29 ABAZOV</td><td>13L D0</td><td>p<span style="text-decoration: overline">p</span> → HX, 1.96 TeV</td></tr><tr><td>1.3</td><td>±0.5</td><td></td><td>30 AAD</td><td>12AI ATLS</td><td>pp → HX, 7, 8 TeV</td></tr><tr><td>0.5</td><td>±0.6</td><td></td><td>30 AAD</td><td>12AI ATLS</td><td>pp → HX, 7 TeV</td></tr><tr><td>1.9</td><td>±0.7</td><td></td><td>30 AAD</td><td>12AI ATLS</td><td>pp → HX, 8 TeV</td></tr><tr><td>0.60</td><td>+0.42<br>-0.37</td><td></td><td>31 CHATRCHYAN 12N</td><td>CMS</td><td>pp → HX, 7, 8 TeV</td></tr></tbody></table>

¹CMS 22 report combined results (see their Extended Data Table 2) using up to 138 fb⁻¹ of data at $E_{cm} = 13$ TeV, assuming $m_H = 125.38$ GeV. See their Fig. 2 right.

²AAD 16AN perform fits to the ATLAS and CMS data at $E_{cm} = 7$ and 8 TeV. The signal strengths for individual production processes are $0.84 \pm 0.17$ for gluon fusion, $1.2 \pm 0.4$ for vector boson fusion, $1.6 \pm 1.2 \pm 2.6$ for WH production, $5.9 \pm 2.2$ for ZH production, and $5.0 \pm 1.8 \pm 1.7$ for $t\bar{t}H$ production.

³AAD 16AN: In the fit, relative production cross sections are fixed to those in the Standard Model. The quoted signal strength is given for $m_H = 125.09$ GeV.

⁴AALTONEN 13M combine all Tevatron data from the CDF and D0 Collaborations with up to 10.0 fb⁻¹ and 9.7 fb⁻¹, respectively, of $p\bar{p}$ collisions at $E_{cm} = 1.96$ TeV. The quoted signal strength is given for $m_H = 125$ GeV.

⁵AAD 23AP measure cross-sections times the $H → WW^*$ branching fraction in the $H → WW^*$ → $e\nu\mu\nu$ channel using 139 fb⁻¹ of pp collisions at $E_{cm} = 13$ TeV: $\sigma_{ggF} \times B(H → WW^*) = 12.0 \pm 1.4$ pb, $\sigma_{VBF} \times B(H → WW^*) = 0.75 \pm 0.19$ pb, and $\sigma_{ggF+VBF} \times B(H → WW^*) = 12.3 \pm 1.3$ pb. The results are given for $m_H = 125.09$ GeV. Measured cross sections and ratios to the SM predictions in the reduced stage-1.2 (see their Fig. 5) simplified template cross section framework are shown in their Table VII and Fig. 15.

⁶AAD 23BV measure fiducial total and differential cross sections of VBF process at $E_{cm} = 13$ TeV with 139 fb⁻¹ using $H → WW^* → e\nu\mu\nu$. The measured total fiducial cross section is $1.68 \pm 0.33(\text{stat}) \pm 0.23(\text{syst})$ fb in their fiducial region (Table II and Section V). See their Fig. 9 for the comparison with theory predictions. The fiducial differential cross sections are shown in their Figs. 11, 12, and 13. Wilson coefficients in the Warsaw basis at 95% confidence interval are measured; see their Table V and Fig. 16.

⁷TUMASYAN 23w measure Higgs production rates with $H → WW^*$ at $E_{cm} = 13$ TeV with 138 fb⁻¹ data. The quoted results are given for $m_H = 125.38$ GeV.

⁸The quoted global signal strength is obtained assuming the relative ratios of different Higgs production modes fixed to the SM values.

⁹The 4 signal strengths for gluon-fusion (ggF), VBF, WH and ZH modes are fit assuming $t\bar{t}H$ and $b\bar{b}H$ fixed to the SM values.

¹⁰The quoted result is for ggF production mode.

¹¹The quoted result is for VBF production mode.

¹²The quoted result is for WH production mode.

¹³The quoted result is for ZH production mode.

¹⁴Measured cross sections and ratios to the SM predictions in the reduced stage-1.2 (see their Fig. 17) simplified template cross section framework (6 ggF, 4 VBF, and 4 VH) are shown in their Table 18 and Fig. 26.

¹⁵AAD 22v measure the signal strength for ggF+2jets with 36.1 fb⁻¹ data at 13 TeV.

¹⁶AAD 22v probe the Higgs couplings to longitudinally and transversely polarized W and Z using VBF ($H → WW^* → e\nu\mu\nu$ plus two jets) with 36.1 fb⁻¹ of data at $E_{cm} = 13$ TeV. The ratios of the polarization-dependent couplings $g_H V_L V_L$ and $g_H V_T V_T$ to the Higgs-V coupling predicted by the SM, $a_L = g_H V_L V_L / g_H V_V$ and $a_T = g_H V_T V_T / g_H V_V$ are measured to be $0.91 \pm 0.10 \pm 0.09 \pm 0.18 \pm 0.17$ and $1.2 \pm 0.4 \pm 0.2 \pm 0.3 \pm 0.13$ respectively, assuming the standard Hg g coupling. These measurements are translated into pseudo-observables of $\kappa_{VV}$ and $\epsilon_{VV}$: $\kappa_{VV} = 0.91 \pm 0.10 \pm 0.09 \pm 0.18 \pm 0.17$ and $\epsilon_{VV} = 0.13 \pm 0.28 \pm 0.08 \pm 0.20 \pm 0.10$, where $\kappa_{VV} = 1$ and $\epsilon_{VV} = 0$ for the SM. See their Tables 9 and 10.

¹⁷AABOUD 19f measure cross-sections times the $H → WW^*$ branching fraction in the $H → WW^* → e\nu\mu\nu$ channel using 36.1 fb⁻¹ of pp collisions at $E_{cm} = 13$ TeV: $\sigma_{ggF} \times B(H → WW^*) = 11.4 \pm 1.2 \pm 1.8$ pb and $\sigma_{VBF} \times B(H → WW^*) = 0.50 \pm 0.24 \pm 0.22 \pm 0.17$ pb.

¹⁸AAD 19a use 36.1 fb⁻¹ data at 13 TeV. The cross section times branching fraction values are measured to be $0.67 \pm 0.31 \pm 0.18 \pm 0.27 \pm 0.14$ pb for WH, $H → WW^*$ and $0.54 \pm 0.31 \pm 0.15 \pm 0.24 \pm 0.07$ pb for ZH, $H → WW^*$.

¹⁹SIRUNYAN 19AT perform a combine fit to 35.9 fb⁻¹ of data at $E_{cm} = 13$ TeV.

²⁰SIRUNYAN 19AX measure the signal strengths, cross sections and so on using gluon fusion, VBF and VH production processes with 35.9 fb⁻¹ of data. The quoted signal strength is given for $m_H = 125.09$ GeV. Signal strengths for each production process is found in their Fig. 9. Measured cross sections and ratios to the SM predictions in the stage-0 simplified template cross section framework are shown in their Fig. 10. $\kappa_F = 1.52 \pm 0.48 \pm 0.41$ and $\kappa_V = 1.10 \pm 0.08$ are obtained (see their Fig. 11 (right)).

²¹AAD 16AQ measure fiducial total and differential cross sections of gluon fusion process at $E_{cm} = 8$ TeV with 20.3 fb⁻¹ using $H → WW^* → e\nu\mu\nu$. The measured fiducial total cross section is $36.0 \pm 9.7$ fb in their fiducial region (Table 7). See their Fig. 6 for fiducial differential cross sections. The results are given for $m_H = 125.36$ GeV.

²²AAD 16k use up to 4.7 fb⁻¹ of pp collisions at $E_{cm} = 7$ TeV and up to 20.3 fb⁻¹ at $E_{cm} = 8$ TeV. The quoted signal strength is given for $m_H = 125.36$ GeV.

²³AAD 15AA use 4.5 fb⁻¹ of pp collisions at $E_{cm} = 7$ TeV and 20.3 fb⁻¹ at $E_{cm} = 8$ TeV. The signal strength for the gluon fusion and vector boson fusion mode is

1.02 ± 0.19 ± 0.22 and 1.27 ± 0.44 ± 0.30, respectively. The quoted signal strengths are given for $m_H = 125.36$ GeV.

²⁴AAD 15AQ use 4.5 fb⁻¹ of pp collisions at $E_{cm} = 7$ TeV and 20.3 fb⁻¹ at $E_{cm} = 8$ TeV. The quoted signal strength is given for $m_H = 125.36$ GeV.

²⁵AAD 15AQ combine their result on W/ZH production with the results of AAD 15AA (gluon fusion and vector boson fusion, slightly updated). The quoted signal strength is given for $m_H = 125.36$ GeV.

²⁶CHATRCHYAN 14G use 4.9 fb⁻¹ of pp collisions at $E_{cm} = 7$ TeV and 19.4 fb⁻¹ at $E_{cm} = 8$ TeV. The last uncertainty in the measurement is theory systematic. The quoted signal strength is given for $m_H = 125.6$ GeV.

²⁷AAD 13AK use 4.7 fb⁻¹ of pp collisions at $E_{cm} = 7$ TeV and 20.7 fb⁻¹ at $E_{cm} = 8$ TeV. The quoted signal strength is given for $m_H = 125.5$ GeV. Superseded by AAD 15AA.

²⁸AALTONEN 13L combine all CDF results with 9.45–10.0 fb⁻¹ of $p\bar{p}$ collisions at $E_{cm} = 1.96$ TeV. The quoted signal strength is given for $m_H = 125$ GeV.

²⁹ABAZOV 13L combine all D0 results with up to 9.7 fb⁻¹ of $p\bar{p}$ collisions at $E_{cm} = 1.96$ TeV. The quoted signal strength is given for $m_H = 125$ GeV.

³⁰AAD 12AI obtain results based on 4.7 fb⁻¹ of pp collisions at $E_{cm} = 7$ TeV and 5.8 fb⁻¹ at $E_{cm} = 8$ TeV. The quoted signal strengths are given for $m_H = 126$ GeV. See also AAD 12DA.

³¹CHATRCHYAN 12N obtain results based on 4.9 fb⁻¹ of pp collisions at $E_{cm} = 7$ TeV and 5.1 fb⁻¹ at $E_{cm} = 8$ TeV. The quoted signal strength is given for $m_H = 125.5$ GeV. See also CHATRCHYAN 13Y.

## Z Z* Final State

<table><thead><tr><th>VALUE</th><th>CL%</th><th>DOCUMENT ID</th><th>TECN.</th><th>COMMENT</th></tr></thead><tbody><tr><td colspan="5" style="text-align: center;">1.02±0.08 OUR AVERAGE</td></tr><tr><td>0.97<sup>+0.12</sup><sub>-0.11</sub></td><td></td><td>1 CMS</td><td>22 CMS</td><td>pp, 13 TeV</td></tr><tr><td>1.01±0.11</td><td></td><td>2.3 AAD</td><td>20AQ ATLS</td><td>pp, 13 TeV</td></tr><tr><td>1.29<sup>+0.26</sup><sub>-0.23</sub></td><td></td><td>4.5 AAD</td><td>16AN LHC</td><td>pp, 7, 8 TeV</td></tr><tr><td>0.94±0.07<sup>+0.09</sup><sub>-0.08</sub></td><td></td><td></td><td></td><td></td></tr><tr><td colspan="5" style="text-align: center;">6 HAYRAPETY...23 CMS</td></tr><tr><td>1.06<sup>+0.19</sup><sub>-0.17</sub></td><td></td><td>7 SIRUNYAN</td><td>21AE CMS</td><td>pp, 13 TeV, couplings</td></tr><tr><td>1.28<sup>+0.21</sup><sub>-0.19</sub></td><td></td><td>8 SIRUNYAN</td><td>21S CMS</td><td>pp, 13 TeV</td></tr><tr><td>1.52<sup>+0.40</sup><sub>-0.34</sub></td><td></td><td>9 AAD</td><td>20AQ ATLS</td><td>pp, 13 TeV</td></tr><tr><td>1.04<sup>+0.32</sup><sub>-0.26</sub></td><td></td><td>10 AAD</td><td>20BA ATLS</td><td>pp, 13 TeV cross sections</td></tr><tr><td>1.46<sup>+0.35</sup><sub>-0.31</sub></td><td></td><td>11 AABOUD</td><td>19N ATLS</td><td>pp, 13 TeV, off-shell</td></tr><tr><td>1.44<sup>+0.34</sup><sub>-0.31</sub></td><td></td><td>12 SIRUNYAN</td><td>19AT CMS</td><td>pp, 13 TeV</td></tr><tr><td>1.43<sup>+0.40</sup><sub>-0.35</sub></td><td></td><td>13 AABOUD</td><td>18AJ ATLS</td><td>pp, 13 TeV</td></tr><tr><td>0.80<sup>+0.35</sup><sub>-0.28</sub></td><td></td><td>14 AABOUD</td><td>18BP ATLS</td><td>pp, 13 TeV, off-shell</td></tr><tr><td>1.2 ± 0.6</td><td></td><td>15 SIRUNYAN</td><td>17AV CMS</td><td>pp, 13 TeV</td></tr><tr><td>1.4 ± 1.1</td><td></td><td>5 AAD</td><td>16AN ATLS</td><td>pp, 7, 8 TeV</td></tr><tr><td>1.1 ± 0.8</td><td></td><td>5 AAD</td><td>16AN CMS</td><td>pp, 7, 8 TeV</td></tr><tr><td>0.73<sup>+0.45</sup><sub>-0.33</sub></td><td></td><td>16 AAD</td><td>16K ATLS</td><td>pp, 7, 8 TeV</td></tr><tr><td>0.93<sup>+0.26</sup><sub>-0.23</sub></td><td></td><td>17 KHACHATRY...16AR CMS</td><td>pp, 7, 8 TeV cross sections</td><td></td></tr><tr><td>1.44<sup>+0.34</sup><sub>-0.31</sub></td><td></td><td>18 AAD</td><td>15F ATLS</td><td>pp → HX, 7, 8 TeV</td></tr><tr><td>0.93<sup>+0.26</sup><sub>-0.23</sub></td><td></td><td>19 AAD</td><td>14AR ATLS</td><td>pp, 8 TeV, cross sections</td></tr><tr><td>0.80<sup>+0.35</sup><sub>-0.28</sub></td><td></td><td>20 CHATRCHYAN 14AA CMS</td><td>pp, 7, 8 TeV</td><td></td></tr><tr><td>1.2 ± 0.6</td><td></td><td>21 AAD</td><td>13AK ATLS</td><td>pp, 7 and 8 TeV</td></tr><tr><td>1.4 ± 1.1</td><td></td><td>22 CHATRCHYAN 13J CMS</td><td>pp → HX, 7, 8 TeV</td><td></td></tr><tr><td>1.1 ± 0.8</td><td></td><td>23 AAD</td><td>12AI ATLS</td><td>pp → HX, 7, 8 TeV</td></tr><tr><td>0.73<sup>+0.45</sup><sub>-0.33</sub></td><td></td><td>23 AAD</td><td>12AI ATLS</td><td>pp → HX, 7 TeV</td></tr><tr><td>0.73<sup>+0.45</sup><sub>-0.33</sub></td><td></td><td>23 AAD</td><td>12AI ATLS</td><td>pp → HX, 8 TeV</td></tr><tr><td>0.73<sup>+0.45</sup><sub>-0.33</sub></td><td></td><td>24 CHATRCHYAN 12N CMS</td><td>pp → HX, 7, 8 TeV</td><td></td></tr></tbody></table>

¹CMS 22 report combined results (see their Extended Data Table 2) using up to 138 fb⁻¹ of data at $E_{cm} = 13$ TeV, assuming $m_H = 125.38$ GeV. See their Fig. 2 right.

²AAD 20AQ perform analyses using $H → ZZ^* → 4\ell$ ($\ell = e, \mu$) with data of 139 fb⁻¹ at $E_{cm} = 13$ TeV. Results are given for $m_H = 125$ GeV.

³AAD 20AQ measured the inclusive cross section times branching ratio for $H → ZZ^*$ decay ($|y(H)| < 2.5$) to be $1.34 \pm 0.12$ pb (with $1.33 \pm 0.08$ pb expected in the SM).

⁴AAD 16AN perform fits to the ATLAS and CMS data at $E_{cm} = 7$ and 8 TeV. The signal strengths for individual production processes are $1.13 \pm 0.34 \pm 0.11 \pm 0.6$ for gluon fusion and for vector boson fusion.

⁵AAD 16AN: In the fit, relative production cross sections are fixed to those in the Standard Model. The quoted signal strength is given for $m_H = 125.09$ GeV.

⁶HAYRAPETY 23 measure the cross sections for $pp → H → ZZ^* → 4\ell$ ($\ell = e, \mu$) using 138 fb⁻¹ at $E_{cm} = 13$ TeV. They give $\sigma = 2.73 \pm 0.22(\text{stat}) \pm 0.15(\text{syst})$ fb in their fiducial region (see their Section5 and Table 2), where $2.86 \pm 0.15$ fb is expected in the Standard Model for $m_H = 125.38$ GeV. 26 differential and 6 double-differential cross sections are given; see their Figs. 6-23 and 24-25.

⁷SIRUNYAN 21AE obtains constraints on anomalous couplings to vector bosons (W, Z, and gluon) and top quark using $H → ZZ^* → 4\ell$ ($\ell = e, \mu$) with data of 137 fb⁻¹ at $E_{cm} = 13$ TeV. Their Table 5 and Figs 14–17 show (effective) couplings to gluon and top with combining gluon fusion, $t\bar{t}H$ and $tH$ production channels and the result of $t\bar{t}H, H → γγ$ (SIRUNYAN 20AS). Their Tables 6–9 and Figs 18–22 show couplings to W and Z for different assumptions and bases (Higgs and Warsaw).
⁸SIRUNYAN 21s measure cross sections with the $H \to ZZ^* \to 4\ell (\ell = e, \mu)$ channel using 137 fb⁻¹ data at $E_{cm} = 13$ TeV. Results are given for $m_H = 125.38$ GeV. The signal strengths for individual production processes in their Table 4. Cross sections are given in their Table 6 and Fig. 14, which are based on the simplified template cross section framework (reduced stage-1.2).

⁹AAD 20AQ present several results for the channel $H \to ZZ^* \to 4\ell (\ell = e, \mu)$ with the simplified template cross section with $\kappa$-frameworks and the effective field theory (EFT) approach; see their Table 8 and Fig. 10 for simplified template cross sections. $\kappa_V = 1.02 \pm 0.06$ and $\kappa_F = 0.88 \pm 0.16$ are obtained, see their Fig. 12 for the $\kappa$-framework. See their Tables 9 and 10 and Figs. 16–18 for the EFT-framework.

¹⁰AAD 20BA measure the cross section for $pp \to H \to ZZ^* \to 4\ell (\ell = e, \mu)$ using 139 fb⁻¹ at $E_{cm} = 13$ TeV. They give $\sigma \cdot B = 3.28 \pm 0.30 \pm 0.11$ fb in their fiducial region, where $3.41 \pm 0.18$ fb is expected in the Standard Model for $m_H = 125$ GeV. Various differential cross sections are also given; see their Figs. 19-39. Constraints on Yukawa couplings for bottom and charm quarks are given in their Table 9 and Fig. 41.

¹¹AABOUD 19n measure the spectrum of the four-lepton invariant mass $m_{4\ell}$ ($\ell = e$ or $\mu$) using 36.1 fb⁻¹ of data at $E_{cm} = 13$ TeV. The quoted signal strength upper limit is obtained from 180 GeV < $m_{4\ell}$ < 1200 GeV.

¹²SIRUNYAN 19AT perform a combined fit to 35.9 fb⁻¹ of data at $E_{cm} = 13$ TeV.

¹³AABOUD 18AJ perform analyses using $H \to ZZ^* \to 4\ell (\ell = e, \mu)$ with data of 36.1 fb⁻¹ at $E_{cm} = 13$ TeV. Results are given for $m_H = 125.09$ GeV. The inclusive cross section times branching ratio for $H \to ZZ^*$ decay ($|\eta(H)| < 2.5$) is measured to be 1.73$^{+0.26}_{-0.24}$ pb (with 1.34$^{+0.09}_{-0.09}$ pb expected in the SM).

¹⁴AABOUD 18BP measure an off-shell Higgs boson production using $ZZ \to 4\ell$ and $ZZ \to 2\ell\nu (\ell = e, \mu)$ decay channels with 36.1 fb⁻¹ of data at $E_{cm} = 13$ TeV. The quoted signal strength upper limit is obtained from a combination of these two channels, where 220 GeV < $m_{4\ell}$ < 2000 GeV for $ZZ \to 4\ell$ and 250 GeV < $m_{4\ell}^{ZZ}$ < 2000 GeV for $ZZ \to 2\ell\nu$ ($m_{4\ell}^{ZZ}$ is defined in their Table 5). See their Table 2 for each measurement.

¹⁵SIRUNYAN 17AV use 35.9 fb⁻¹ of $pp$ collisions at $E_{cm} = 13$ TeV. The quoted signal strength, obtained from the analysis of $H \to ZZ^* \to 4\ell (\ell = e, \mu)$ decays, is given for $m_H = 125.09$ GeV. The signal strengths for different production modes are shown in their Table 3. The fiducial and differential cross sections are shown in their Fig. 10.

¹⁶AAD 16k use up to 4.7 fb⁻¹ of $pp$ collisions at $E_{cm} = 7$ TeV and up to 20.3 fb⁻¹ at $E_{cm} = 8$ TeV. The quoted signal strength is given for $m_H = 125.36$ GeV.

¹⁷KHACHATRYAN 16AR use data of 5.1 fb⁻¹ at $E_{cm} = 7$ TeV and 19.7 fb⁻¹ at 8 TeV. The fiducial cross sections for the production of 4 leptons via $H \to 4\ell$ decays are measured to be 0.56$^{+0.67}_{-0.21}$, 0.44$^{+0.06}_{-0.04}$ fb at 7 TeV and 1.11$^{+0.41}_{-0.14}$ fb at 8 TeV in their fiducial region (Table 2). The differential cross sections at $E_{cm} = 8$ TeV are also shown in Figs. 4 and 5. The results are given for $m_H = 125$ GeV.

¹⁸AAD 15f use 4.5 fb⁻¹ of $pp$ collisions at $E_{cm} = 7$ TeV and 20.3 fb⁻¹ at $E_{cm} = 8$ TeV. The quoted signal strength is given for $m_H = 125.36$ GeV. The signal strength for the gluon fusion production mode is 1.66$^{+0.45}_{-0.25}$, 0.41$^{+0.15}_{-0.10}$, while the signal strength for the vector boson fusion production mode is 0.26$^{+1.60}_{-0.36}$, 0.91$^{+0.23}_{-0.21}$.

¹⁹AAD 14AR measure the cross section for $pp \to H \to ZZ^* \to 4\ell (\ell = e, \mu)$ using 20.3fb⁻¹ at $E_{cm} = 8$ TeV. They give $\sigma \cdot B = 2.11^{+0.53}_{-0.47}$ ± 0.08 fb in their fiducial region, where 1.30 ± 0.13 fb is expected in the Standard Model for $m_H = 125.4$ GeV. Various differential cross sections are also given; see their Fig. 2.

²⁰CHATRYCHAN 14AA use data of 5.1 fb⁻¹ of $pp$ collisions at $E_{cm} = 7$ TeV and 19.7 fb⁻¹ at $E_{cm} = 8$ TeV. The quoted signal strength is given for $m_H = 125.6$ GeV. The signal strength for the gluon fusion and $t\bar{t}H$ production mode is 0.80$^{+0.46}_{-0.36}$, while the signal strength for the vector boson fusion and $WH, ZH$ production mode is 1.7$^{+2.2}_{-2.1}$.

²¹AAD 13AK use 4.7 fb⁻¹ of $pp$ collisions at $E_{cm} = 7$ TeV and 20.7 fb⁻¹ at $E_{cm} = 8$ TeV. The quoted signal strength is given for $m_H = 125.5$ GeV.

²²CHATRYCHAN 13j obtain results based on $ZZ \to 4\ell$ final states in 5.1 fb⁻¹ of $pp$ collisions at $E_{cm} = 7$ TeV and 12.2 fb⁻¹ at $E_{cm} = 8$ TeV. The quoted signal strength is given for $m_H = 125.8$ GeV. Superseded by CHATRYCHAN 14AA.

²³AAD 12AI obtain results based on 4.7–4.8 fb⁻¹ of $pp$ collisions at $E_{cm} = 7$ TeV and 5.8 fb⁻¹ at $E_{cm} = 8$ TeV. The quoted signal strengths are given for $m_H = 126$ GeV. See also AAD 12DA.

²⁴CHATRYCHAN 12N obtain results based on 4.9–5.1 fb⁻¹ of $pp$ collisions at $E_{cm} = 7$ TeV and 5.1–5.3 fb⁻¹ at $E_{cm} = 8$ TeV. An excess of events over background with a local significance of 5.0 $\sigma$ is observed at about $m_H = 125$ GeV. The quoted signal strengths are given for $m_H = 125.5$ GeV. See also CHATRYCHAN 12BY and CHATRYCHAN 13Y.

## γγ Final State

VALUE

1.10±0.06 OUR AVERAGE

DOCUMENT ID

TECN

COMMENT

1.04$^{+0.10}_{-0.09}$

1 AAD

23Y ATLS

pp, 13 TeV

1.13$^{+0.09}_{-0.09}$

2 CMS

22 CMS

pp, 13 TeV

1.14$^{+0.19}_{-0.18}$

3,4 AAD

16AN LHC

pp, 7, 8 TeV

5.97$^{+3.39}_{-3.12}$

5

13M TEVA $p\bar{p} \to HX, 1.96$ TeV

• • • We do not use the following data for averages, fits, limits, etc. • • •

1.12$^{+0.18}_{-0.14}$

6

23Q CMS

pp, 13 TeV, cross sections

0.99$^{+0.15}_{-0.14}$

7 AAD

22N ATLS

pp, 13 TeV, diff. x-sections

1.18$^{+0.17}_{-0.14}$

8

21Q CMS

pp, 13 TeV

1.20$^{+0.18}_{-0.14}$

9

19AT CMS

pp, 13 TeV

0.99$^{+0.15}_{-0.14}$

10

19L CMS

pp, 13 TeV, diff. x-section

1.18$^{+0.17}_{-0.14}$

11

18BO ATLS

pp, 13 TeV

1.14$^{+0.27}_{-0.25}$

12

18DS CMS

pp, H → γγ, 13 TeV, floated $m_H$

1.14$^{+0.27}_{-0.25}$

4 AAD

16AN ATLS

pp, 7, 8 TeV

1.11$^{+0.25}_{-0.23}$

4

16AN CMS

pp, 7, 8 TeV

1.17$^{+0.23}_{-0.08}$ $^{+0.10}_{-0.08}$

13

KHACHATRY...16G CMS

pp, 8 TeV, diff. x-section

1.14$^{+0.21}_{-0.09}$

15

14BJ ATLS

pp, 8 TeV, diff. x-section

1.15$^{+0.33}_{-0.28}$

16

KHACHATRY...14P CMS

pp, 7, 8 TeV

1.55$^{+0.33}_{-0.28}$

17

17AAD 13AK ATLS

pp, 7 and 8 TeV

7.81$^{+4.61}_{-4.42}$

18

AALTONEN 13L CDF

$p\bar{p} \to HX, 1.96$ TeV

4.20$^{+4.60}_{-4.20}$

19

ABAZOV 13L D0

$p\bar{p} \to HX, 1.96$ TeV

1.8 $^{+0.5}_{-0.5}$

20

AAD 12AI ATLS

pp, HX, 7, 8 TeV

2.2 $^{+0.7}_{-0.7}$

20

AAD 12AI ATLS

pp, HX, 7 TeV

1.5 $^{+0.6}_{-0.6}$

20

AAD 12AI ATLS

pp, HX, 8 TeV

1.5 $^{+0.6}_{-0.6}$

20

AAD 12AI ATLS

pp, HX, 8 TeV

1.54$^{+0.46}_{-0.42}$

21

CHATRYCHAN 12N CMS

pp, HX, 7, 8 TeV

¹AAD 23Y use 139 fb⁻¹ of $pp$ collisions at $E_{cm} = 13$ TeV. The quoted results are given for $m_H = 125.09$ GeV and $\Gamma_H = 4.07$ MeV. Measured $\sigma_B$ and ratios to the SM predictions for the different production modes are shown in their Table 9 and Fig. 9. Measured cross sections and ratios to the SM predictions in the reduced stage-1.2 (see their Fig. 11) simplified template cross section framework are shown in their Table 10 and Fig. 12. Wilson coefficients in the Warsaw basis (see their Table 11) at 95% CL are measured; see their Table 16 and Fig. 17.

²CMS 22 report combined results (see their Extended Data Table 2) using up to 138 fb⁻¹ of data at $E_{cm} = 13$ TeV, assuming $m_H = 125.38$ GeV. See their Fig. 2 right.

³AAD 16AN perform fits to the ATLAS and CMS data at $E_{cm} = 7$ and 8 TeV. The signal strengths for individual production processes are $1.10^{+0.23}_{-0.22}$ for gluon fusion, $1.3 \pm 0.5$ for vector boson fusion, $0.5^{+1.3}_{-1.2}$ for WH production, $0.5^{+3.0}_{-2.5}$ for ZH production, and $2.2^{+1.6}_{-1.3}$ for $t\bar{t}H$ production.

⁴AAD 16AN: In the fit, relative production cross sections are fixed to those in the Standard Model. The quoted signal strength is given for $m_H = 125.09$ GeV.

⁵AALTONEN 13M combine all Tevatron data from the CDF and D0 Collaborations with up to 10.0 fb⁻¹ and 9.7 fb⁻¹, respectively, of $p\bar{p}$ collisions at $E_{cm} = 1.96$ TeV. The quoted signal strength is given for $m_H = 125$ GeV.

⁶TUMASYAN 23Q measure fiducial and differential cross sections at $E_{cm} = 13$ TeV with 137 fb⁻¹ data. The quoted results are given for $m_H = 125.38$ GeV. The inclusive fiducial $\sigma_B$ is 73.4$^{+5.4}_{-5.3}$ (stat) $^{+2.4}_{-2.2}$ (syst) fb with their defined fiducial region (see their Section 7 and Table 2), where 75.4 $^{+4.1}_{-3.5}$ fb is expected in the Standard Model. See their Fig. 8 including other fiducial $\sigma_B$ defined in their Table 3. Differential $\sigma_B$ are shown in their Figs. 10-15. Double-differential $\sigma_B$ are in their Figs. 16 and 17.

⁷AAD 22N measure fiducial and differential cross sections of $pp \to H \to \gamma\gamma$ at $E_{cm} = 13$ TeV with 139 fb⁻¹ data. The quoted results are given for $m_H = 125.09$ GeV. The inclusive fiducial $\sigma_B$ is 67 $^{+5}_{-4}$ fb with their defined fiducial region. Other fiducial $\sigma_B$ are in their Table 3. Differential $\sigma_B$ are shown in their Figs. 8-13, 15, 25-32, 35, 36. Double-differential $\sigma_B$ are in their Figs. 14, 33, 34. Modifications of the b- and c-quark Yukawa couplings to $H$, $\kappa_D$ and $\kappa_C$ at 95% CL are in their Table 6 and Fig. 18. Wilson coefficients at 95% CL are in their Table 7 and Fig. 21.

⁸SIRUNYAN 21O measures cross sections and couplings with the $H \to \gamma\gamma$ channel using 137 fb⁻¹ data at $E_{cm} = 13$ TeV. Results are given for $m_H = 125.38$ GeV. The signal strengths for individual production processes are given in their Fig. 16. Cross sections are given in their Tables 12 and 13 and Figs. 18 and 20, which are based on the simplified template cross section framework (reduced stage-1.2). Results in the $\kappa$-framework are given in their Fig. 22.

⁹SIRUNYAN 19T perform a combine fit to 35.9 fb⁻¹ of data at $E_{cm} = 13$ TeV.

¹⁰SIRUNYAN 19T measure fiducial and differential cross sections of the process $pp \to HX, H \to \gamma\gamma$ at $E_{cm} = 13$ TeV with 35.9 fb⁻¹. See their Figs. 4-6 and Table 1 for data.

¹¹AABOUD 18BO use 36.1 fb⁻¹ of $pp$ collisions at $E_{cm} = 13$ TeV. The signal strengths for the individual production modes are: $0.81^{+0.19}_{-0.18}$ for gluon fusion, $2.0^{+0.6}_{-0.5}$ for vector boson fusion, $0.7^{+0.9}_{-0.8}$ for $VH$ production ($V = W, Z$), and $0.5 \pm 0.6$ for $t\bar{t}H$ and $tH$ production. Other measurements of cross sections and couplings are summarized in their Section 10. The quoted values are given for $m_H = 125.09$ GeV.

¹²SIRUNYAN 18DS use 35.9 fb⁻¹ of $pp \to H$ collisions with $H \to \gamma\gamma$ at $E_{cm} = 13$ TeV. The Higgs mass is floated in the measurement of a signal strength. The result is $1.18^{+0.12}_{-0.11}$ (stat.) $^{+0.09}_{-0.07}$ (syst.) $^{+0.07}_{-0.06}$ (theory), which is largely insensitive to the Higgs mass around 125 GeV.

¹³KHACHATRYAN 166 measure fiducial and differential cross sections of the process $pp \to HX, H \to \gamma\gamma$ at $E_{cm} = 8$ TeV with 19.7 fb⁻¹. See their Figs. 4-6 and Table 1 for data.

¹⁴AAD 14BC use 4.5 fb⁻¹ of $pp$ collisions at $E_{cm} = 7$ TeV and 20.3 fb⁻¹ at $E_{cm} = 8$ TeV. The last uncertainty in the measurement is theory systematics. The quoted signal strength is given for $m_H = 125.4$ GeV. The signal strengths for the individual production modes are: $1.32 \pm 0.38$ for gluon fusion, $0.8 \pm 0.7$ for vector boson fusion, $1.0 \pm 1.6$ for $WH$ production, $0.1^{+3.1}_{-0.1}$ for $ZH$ production, and $1.6^{+2.7}_{-1.8}$ for $t\bar{t}H$ production.

¹⁵AAD 14BJ measure fiducial and differential cross sections of the process $pp \to HX, H \to \gamma\gamma$ at $E_{cm} = 8$ TeV with 20.3 fb⁻¹. See their Table 3 and Figs. 3-12 for data.

¹⁶KHACHATRYAN 14P use 5.1 fb⁻¹ of $pp$ collisions at $E_{cm} = 7$ TeV and 19.7 fb⁻¹ at $E_{cm} = 8$ TeV. The last uncertainty in the measurement is theory systematics. The quoted signal strength is given for $m_H = 124.7$ GeV. The signal strength for the gluon fusion and $t\bar{t}H$ production mode is $1.13^{+0.37}_{-0.31}$, while the signal strength for the vector boson fusion and $WH, ZH$ production mode is $1.16^{+0.63}_{-0.58}$.

¹⁷AAD 13AK use 4.7 fb⁻¹ of $pp$ collisions at $E_{cm} = 7$ TeV and 20.7 fb⁻¹ at $E_{cm} = 8$ TeV. The quoted signal strength is given for $m_H = 125.5$ GeV.

¹⁸AALTONEN 13L combine all CDF results with 9.45–10.0 fb⁻¹ of $p\bar{p}$ collisions at $E_{cm} = 1.96$ TeV. The quoted signal strength is given for $m_H = 125$ GeV.

¹⁹ABAZOV 13L combine all D0 results with up to 9.7 fb⁻¹ of $p\bar{p}$ collisions at $E_{cm} = 1.96$ TeV. The quoted signal strength is given for $m_H = 125$ GeV.
20 AAD 12AI obtain results based on 4.8 fb⁻¹ of pp collisions at $E_{cm} = 7$ TeV and 5.9 fb⁻¹ at $E_{cm} = 8$ TeV. The quoted signal strengths are given for $m_H = 126$ GeV. See also AAD 12DA.

21 CHATRCHYAN 12N obtain results based on 5.1 fb⁻¹ of pp collisions at $E_{cm} = 7$ TeV and 5.3 fb⁻¹ at $E_{cm} = 8$ TeV. The quoted signal strength is given for $m_H = 125.5$ GeV. See also CHATRCHYAN 13Y.

## cτ Final State

<table><thead><tr><th>VALUE</th><th>CL%</th><th>DOCUMENT ID</th><th>TECN</th><th>COMMENT</th></tr></thead><tbody><tr><td>&lt; 14</td><td>95</td><td>1 TUMASYAN</td><td>23AH CMS</td><td>pp → W/H/ZH, 13 TeV</td></tr><tr><td colspan="5">• • • We do not use the following data for averages, fits, limits, etc. • • •</td></tr><tr><td></td><td></td><td>9.4 +20.3<br/>-19.9</td><td>2 TUMASYAN</td><td>pp → W/H/ZH<br/>(boosted), 13 TeV</td></tr><tr><td>&lt; 47</td><td>95</td><td>2 TUMASYAN</td><td>23AD CMS</td><td>pp → W/H/ZH<br/>(boosted), 13 TeV</td></tr><tr><td>- 9 ±10 ±11</td><td>3,4 AAD</td><td>22W ATLS</td><td>pp → W/H/ZH, 13 TeV</td></tr><tr><td>- 9 ±10 ±12</td><td>3,5 AAD</td><td>22W ATLS</td><td>pp → W/H/ZH, 13 TeV</td></tr><tr><td>&lt; 26</td><td>95</td><td>3 AAD</td><td>22W ATLS</td><td>pp → W/H/ZH, 13 TeV</td></tr><tr><td>37 ±17 +11<br/>-9</td><td>6 SIRUNYAN</td><td>20AE CMS</td><td>pp, 13 TeV</td></tr><tr><td>&lt; 110</td><td>95</td><td>7 AABOUD</td><td>18M ATLS</td><td>pp, 13 TeV</td></tr></tbody></table>

2 TUMASYAN 23AH search for V H, $H \to c\bar{\tau}$ ($V = W, Z$) using 138 fb⁻¹ of pp collision data at $E_{cm} = 13$ TeV. The upper limit on $\sigma(pp \to V H) \cdot B(H \to c\bar{\tau})$ is 0.94 pb at 95% CL. See their Fig. 4. The quoted values are given for $m_H = 125.38$ GeV.

2 TUMASYAN 23AD search for Higgs produced with transverse momenta greater than 450 GeV and decaying to cτ using 138 fb⁻¹ of pp collision data at $E_{cm} = 13$ TeV.

3 AAD 22W search for V H, $H \to c\bar{\tau}$ ($V = W, Z$) using 139 fb⁻¹ of pp collision data at $E_{cm} = 13$ TeV. The results are given for $m_H = 125$ GeV.

4 The analysis of V H, $H \to c\bar{\tau}$ is combined with V H, $H \to b\bar{d}$ (AAD 21AB). The ratio $|\kappa_C/\kappa_b|$ is constrained to be less than 4.5 at 95% CL. See their Fig. 7.

5 The constraint on the charm Yukawa coupling modifier $\kappa_C$ is measured to be $|\kappa_C| < 8.5$ at 95% CL. See their Fig. 4.

6 SIRUNYAN 20AE use 35.9 fb⁻¹ at of pp collisions at $E_{cm} = 13$ TeV. The measured best fit value of $\sigma(pp \to V H) \cdot B(H \to c\bar{\tau})$ is 2.40⁺¹.12⁻⁰.65 pb (equivalent to < 4.5 pb at 95% CL upper limit, i.e. 70 times the standard model), where V is $W \to \ell\nu$, $Z \to \ell\ell$, or $Z \to \nu\nu$ ($\ell = e, \mu$). The quoted values are given for $m_H = 125$ GeV.

7 AABOUD 18M use 36.1 fb⁻¹ at of pp collisions at $E_{cm} = 13$ TeV. The upper limit on $\sigma(pp \to ZH) \cdot B(H \to c\bar{\tau})$ is 2.7 pb at 95% CL. This corresponds to 110 times the standard model. The quoted values are given for $m_H = 125$ GeV.

## b\bar{b} Final State

<table><thead><tr><th>VALUE</th><th>DOCUMENT ID</th><th>TECN</th><th>COMMENT</th></tr></thead><tbody><tr><td>0.99±0.12 OUR AVERAGE</td><td></td><td></td><td></td></tr><tr><td>1.05<sup>+0.22</sup><sub>-0.21</sub></td><td>1 CMS</td><td>22 CMS</td><td>pp, 13 TeV</td></tr><tr><td>1.02<sup>+0.12</sup><sub>-0.11</sub></td><td>2 AAD</td><td>21AB ATLS</td><td>pp → HW/HZ, H → b<span style="text-decoration: overline">b</span>,<br/>13 TeV, 139 fb<sup>-1</sup></td></tr><tr><td>0.95<sup>+0.32</sup><sub>-0.17</sub></td><td>3 AAD</td><td>21AJ ATLS</td><td>VBF, H → b<span style="text-decoration: overline">b</span>, pp, 13 TeV,<br/>126 fb<sup>-1</sup></td></tr><tr><td>0.70<sup>+0.29</sup><sub>-0.27</sub></td><td>4,5 AAD</td><td>16AN LHC</td><td>pp, 7, 8 TeV</td></tr><tr><td>1.59<sup>+0.69</sup><sub>-0.72</sub></td><td>6 AALTONEN</td><td>13M TEVA</td><td>p<span style="text-decoration: overline">p</span> → HX, 1.96 TeV</td></tr></tbody></table>

• • • We do not use the following data for averages, fits, limits, etc. • • •

<table><tbody><tr><td>0.8 ±3.2</td><td>7 AAD</td><td>22X ATLS</td><td>boosted H → b<span style="text-decoration: overline">b</span>, pp, 13 TeV</td></tr><tr><td>0.95<sup>+0.18</sup><sub>-0.18</sub></td><td>2 AAD</td><td>21AB ATLS</td><td>pp → HW, H → b<span style="text-decoration: overline">b</span>, 13 TeV, 139 fb<sup>-1</sup></td></tr><tr><td>1.08<sup>+0.17</sup><sub>-0.15</sub></td><td>2 AAD</td><td>21AB ATLS</td><td>pp → HZ, H → b<span style="text-decoration: overline">b</span>, 13 TeV, 139 fb<sup>-1</sup></td></tr><tr><td>0.72<sup>+0.29</sup><sub>-0.28</sub></td><td>8 AAD</td><td>21H ATLS</td><td>pp → HW/HZ, H → b<span style="text-decoration: overline">b</span>,<br/>boosted W/Z, 13 TeV,<br/>139 fb<sup>-1</sup></td></tr><tr><td>1.3 ±1.0</td><td>9 AAD</td><td>21M ATLS</td><td>VBF+γ, H → b<span style="text-decoration: overline">b</span>, pp, 13 TeV,<br/>132 fb<sup>-1</sup></td></tr><tr><td>3.7 ±1.2<sup>+0.11</sup><sub>-0.9</sub></td><td>10 SIRUNYAN</td><td>20BL CMS</td><td>boosted H → b<span style="text-decoration: overline">b</span>, pp, 13 TeV</td></tr><tr><td>1.12<sup>+0.29</sup><sub>-0.25</sub></td><td>11 AABOUD</td><td>19U ATLS</td><td>pp → V H, H → b<span style="text-decoration: overline">b</span>, 13 TeV, cross sections</td></tr><tr><td>1.16<sup>+0.27</sup><sub>-0.25</sub></td><td>12 SIRUNYAN</td><td>19AT CMS</td><td>pp, 13 TeV</td></tr><tr><td>0.98<sup>+0.22</sup><sub>-0.21</sub></td><td>13 AABOUD</td><td>18BN ATLS</td><td>pp → HW/HZ, H → b<span style="text-decoration: overline">b</span>,<br/>13 TeV, 79.8 fb<sup>-1</sup></td></tr><tr><td>1.01<sup>+0.20</sup></td><td>14 AABOUD</td><td>18BN ATLS</td><td>pp → HW/HZ, H → b<span style="text-decoration: overline">b</span>,<br/>7, 8, 13 TeV</td></tr><tr><td>2.5<sup>+1.4</sup><sub>-1.3</sub></td><td>15 AABOUD</td><td>18BN ATLS</td><td>pp → HX, ggF, VBF, V H,<br/>t<span style="text-decoration: overline">T</span> 7, 8, 13 TeV</td></tr><tr><td>3.0<sup>+1.7</sup><sub>-1.6</sub></td><td>16,17 AABOUD</td><td>18BQ ATLS</td><td>pp → HX, VBF, 13 TeV</td></tr><tr><td>1.19<sup>+0.40</sup><sub>-0.38</sub></td><td>16,18 AABOUD</td><td>18BQ ATLS</td><td>pp → HX, VBF, 13 TeV</td></tr><tr><td>1.06<sup>+0.31</sup><sub>-0.29</sub></td><td>19 AALTONEN</td><td>18C CDF</td><td>p<span style="text-decoration: overline">p</span> → HX, 1.96 TeV</td></tr><tr><td>1.06<sup>+0.29</sup><sub>-0.29</sub></td><td>20 SIRUNYAN</td><td>18AE CMS</td><td>pp → HW/HZ, H → b<span style="text-decoration: overline">b</span>,<br/>13 TeV</td></tr><tr><td>1.06<sup>+0.26</sup></td><td>21 SIRUNYAN</td><td>18AE CMS</td><td>pp → HW/HZ, H → b<span style="text-decoration: overline">b</span>,<br/>7, 8, 13 TeV</td></tr><tr><td>1.01<sup>+0.22</sup></td><td>22 SIRUNYAN</td><td>18DB CMS</td><td>pp → HW/HZ, H → b<span style="text-decoration: overline">b</span>,<br/>13 TeV, 77.2 fb<sup>-1</sup></td></tr><tr><td>1.01<sup>+0.22</sup></td><td>23 SIRUNYAN</td><td>18DB CMS</td><td>pp → HW/HZ, H → b<span style="text-decoration: overline">b</span>,<br/>7, 8, 13 TeV</td></tr></tbody></table>

<table><tbody><tr><td>1.04±0.20</td><td>24 SIRUNYAN</td><td>18DB CMS</td><td>pp → HX, ggF, VBF, V H,<br/>t<span style="text-decoration: overline">T</span> 7, 8, 13 TeV</td></tr><tr><td>2.3 +1.8<br/>-1.6</td><td>25 SIRUNYAN</td><td>18E CMS</td><td>pp → HX, boosted, 13 TeV</td></tr><tr><td>1.20<sup>+0.24</sup><sub>-0.23</sub></td><td>26 AABOUD</td><td>17BA ATLS</td><td>pp → HW/ZX, H → b<span style="text-decoration: overline">b</span>,<br/>13 TeV, 36.1 fb<sup>-1</sup></td></tr><tr><td>0.90±0.18<sup>+0.21</sup><sub>-0.19</sub></td><td>27 AABOUD</td><td>17BA ATLS</td><td>pp → HW/ZX, H → b<span style="text-decoration: overline">b</span>,<br/>7, 8, 13 TeV</td></tr><tr><td>-0.8 ±1.3<sup>+1.8</sup><sub>-1.9</sub></td><td>28 AABOUD</td><td>16X ATLS</td><td>pp → HX, VBF, 8 TeV</td></tr><tr><td>0.62±0.37</td><td>5 AAD</td><td>16AN ATLS</td><td>pp, 7, 8 TeV</td></tr><tr><td>0.81<sup>+0.45</sup><sub>-0.43</sub></td><td>5 AAD</td><td>16AN CMS</td><td>pp, 7, 8 TeV</td></tr><tr><td>0.63<sup>+0.31</sup><sub>-0.30</sub></td><td>29 AAD</td><td>16K ATLS</td><td>pp, 7, 8 TeV</td></tr><tr><td>0.52<sup>+0.32</sup><sub>-0.24</sub></td><td>30 AAD</td><td>15G ATLS</td><td>pp → HW/ZX, 7, 8 TeV</td></tr><tr><td>2.8 +1.6<br/>-1.4</td><td>31 KHACHATRY...15Z CMS</td><td>pp → HX, VBF, 8 TeV</td></tr><tr><td>1.03<sup>+0.44</sup><sub>-0.42</sub></td><td>32 KHACHATRY...15Z CMS</td><td>pp, 8 TeV, combined</td></tr><tr><td>1.0 ±0.5</td><td>33 CHATRCHYAN14AI CMS</td><td>pp → HW/ZX, 7, 8 TeV</td></tr><tr><td>1.72<sup>+0.92</sup><sub>-0.87</sub></td><td>34 AALTONEN</td><td>13L CDF</td><td>p<span style="text-decoration: overline">p</span> → HX, 1.96 TeV</td></tr><tr><td>1.23<sup>+1.24</sup><sub>-1.17</sub></td><td>35 ABAZOV</td><td>13L D0</td><td>p<span style="text-decoration: overline">p</span> → HX, 1.96 TeV</td></tr><tr><td>0.5 ±2.2</td><td>36 AAD</td><td>12AI ATLS</td><td>pp → HW/ZX, 7 TeV</td></tr><tr><td></td><td>37 AALTONEN</td><td>12T TEVA</td><td>p<span style="text-decoration: overline">p</span> → HW/ZX, 1.96 TeV</td></tr><tr><td>0.48<sup>+0.81</sup><sub>-0.70</sub></td><td>38 CHATRCHYAN12N CMS</td><td>pp → HW/ZX, 7, 8 TeV</td><td></td></tr></tbody></table>

1 CMS 22 report combined results (see their Extended Data Table 2) using up to 138 fb⁻¹ of data at $E_{cm} = 13$ TeV, assuming $m_H = 125.38$ GeV. See their Fig. 2 right.

2 AAD 21AB search for V H, $H \to b\bar{d}$ ($V = W, Z$) using 139 fb⁻¹ of pp collision data at $E_{cm} = 13$ TeV. The results are given for $m_H = 125$ GeV. Cross sections are given in their Table 13 and Fig. 7, which are based on the simplified template cross section framework (reduced stage-1.2). Wilson coefficients of the Warsaw-basis operators are given in their Fig. 9.

3 AAD 21AJ present measurements of $H \to b\bar{d}$ in the VBF production mode. The inclusive VBF cross sections with and without the branching ratio of $H \to b\bar{d}$ are 2.07 ± 0.70⁺0.46⁻0.37 fb and 3.56 ± 1.21⁺0.80⁻0.64 fb, respectively. The latter is obtained assuming the SM value of $B(H \to b\bar{d}) = 0.5809$ and $m_H = 125$ GeV.

4 AAD 16AN perform fits to the ATLAS and CMS data at $E_{cm} = 7$ and 8 TeV. The signal strengths for individual production processes are 1.0 ± 0.5 for W H production, 0.4 ± 0.4 for Z H production, and 1.1 ± 1.0 for t<span style="text-decoration: overline">T</span> H production.

5 AAD 16AN: In the fit, relative production cross sections are fixed to those in the Standard Model. The quoted signal strength is given for $m_H = 125.09$ GeV.

6 AALTONEN 13M combine all Tevatron data from the CDF and D0 Collaborations with up to 10.0 fb⁻¹ and 9.7 fb⁻¹, respectively, of p<span style="text-decoration: overline">p</span> collisions at $E_{cm} = 1.96$ TeV. The quoted signal strength is given for $m_H = 125$ GeV.

7 AAD 22X measure cross sections using a boosted $H \to b\bar{d}$ with large-radius jets. The data is 136 fb⁻¹ of pp collisions at $E_{cm} = 13$ TeV. All the results are given for $m_H = 125$ GeV. The inclusive signal strength is given using data with a H candidate jet $p_T > 250$ GeV. The fiducial H production cross section ($p_T(H) > 450$ GeV and $|y(H)| < 2)$ is <115 fb (95% CL) and the upper limits for other four different $p_T$ regions are shown in their Fig. 12. The measured fiducial H production cross section ($p_T(H) > 1$ TeV) is 2.3 ± 3.9(stat)±1.3(syst)±0.5(theory) fb.

8 AAD 21H present measurements of $H \to b\bar{d}$ with a boosted vector boson ($p_T > 250$ GeV) using 139 fb⁻¹ of pp collision data at $E_{cm} = 13$ TeV. Cross sections are given in their Table 6 and Fig. 4, which are based on the simplified template cross section framework (reduced stage-1.2). Wilson coefficients of the Warsaw-basis operators are given in their Fig. 5.

9 AAD 21M search for VBF+γ, $H \to b\bar{d}$ using 132 fb⁻¹ of pp collision data at $E_{cm} = 13$ TeV.

10 SIRUNYAN 20BL search for boosted $H \to b\bar{d}$ (a H candidate jet $p_T > 450$ GeV) using 137 fb⁻¹ of pp collision data at $E_{cm} = 13$ TeV. The quoted signal strength corresponds to a significance of 2.5 standard deviations and is given for $m_H = 125$ GeV. A differential fiducial cross section as a function of Higgs boson $p_T$ for ggF is shown in their Fig. 7, assuming the other production modes occur at the expected SM rates. The reported value is 3.7 ± 1.2⁺0.8⁺0.8⁻0.7⁻0.5 where the last uncertainty comes from theoretical modeling. We have combined the systematic uncertainties in quadrature.

11 AABOUD 19U measure cross sections of pp → V H, $H \to b\bar{d}$ production as a function of the gauge boson transverse momentum using data of 79.8 fb⁻¹. The kinematical fiducial volumes used is based on the simplified template cross section framework (reduced stage-1). See their Table 3 and Fig. 3.

12 SIRUNYAN 19AT perform a combine fit to 35.9 fb⁻¹ of data at $E_{cm} = 13$ TeV.

13 AABOUD 18BN search for V H, $H \to b\bar{d}$ ($V = W, Z$) using 79.8 fb⁻¹ of pp collision data at $E_{cm} = 13$ TeV. The quoted signal strength corresponds to a significance of 4.9 standard deviations and is given for $m_H = 125$ GeV.

14 AABOUD 18BN combine results of 79.8 fb⁻¹ at $E_{cm} = 13$ TeV with results of V H at $E_{cm} = 7$ and 8 TeV.

15 AABOUD 18BN combine results of V H at $E_{cm} = 7, 8$ and 13 TeV with results of VBF (+gluon fusion) and t<span style="text-decoration: overline">T</span> H at $E_{cm} = 7, 8$, and 13 TeV to perform a search for the $H \to b\bar{d}$ decay. The quoted signal strength assumes a SM production strength and corresponds to a significance of 5.4 standard deviations.

16 AABOUD 18BQ search for $H \to b\bar{d}$ produced through vector-boson fusion (VBF) and VBF+γ with 30.6 fb⁻¹ pp collision data at $E_{cm} = 13$ TeV. The quoted signal strength is given for $m_H = 125$ GeV.

17 The signal strength is measured including all production modes (VBF, ggF, V H, t<span style="text-decoration: overline">T</span> H).

18 The signal strength is measured for VBF-only and others (ggF, V H, t<span style="text-decoration: overline">T</span> H) are constrained to Standard Model expectations with uncertainties described in their Section VIII B.

19 AALTONEN 18C use 5.4 fb⁻¹ of p<span style="text-decoration: overline">p</span> collisions at $E_{cm} = 1.96$ TeV. The upper limit at 95% CL on p<span style="text-decoration: overline">p</span> → H → b<span style="text-decoration: overline">b</span> is 33 times the SM prediction, which corresponds to a cross section of 40.6 pb.
20 SIRUNYAN 18A8E use 35.9 fb⁻¹ of pp collision data at E<sub>cm</sub> = 13 TeV. The quoted signal strength corresponds to 3.3 standard deviations and is given for m<sub>H</sub> = 125.09 GeV.

21 SIRUNYAN 18A8E combine the result of 35.9 fb⁻¹ at E<sub>cm</sub> = 13 TeV with the results obtained from data of up to 5.1 fb⁻¹ at E<sub>cm</sub> = 7 TeV and up to 18.9 fb⁻¹ at E<sub>cm</sub> = 8 TeV (CHATRCHYAN 14AI and KHACHATRYAN 152). The quoted signal strength corresponds to 3.8 standard deviations and is given for m<sub>H</sub> = 125.09 GeV.

22 SIRUNYAN 18DB search for V̄H, H → bD̄ (V = W, Z) using 77.2 fb⁻¹ of pp collision data at E<sub>cm</sub> = 13 TeV. The quoted signal strength corresponds to a significance of 4.4 standard deviations and is given for m<sub>H</sub> = 125.09 GeV.

23 SIRUNYAN 18DB combine the result of 77.2 fb⁻¹ at E<sub>cm</sub> = 13 TeV with the results obtained from data of up to 5.1 fb⁻¹ at E<sub>cm</sub> = 7 TeV and up to 18.9 fb⁻¹ at E<sub>cm</sub> = 8 TeV. The quoted signal strength corresponds to a significance of 4.8 standard deviations and is given for m<sub>H</sub> = 125.09 GeV.

24 SIRUNYAN 18DB combine results of 77.2 fb⁻¹ at E<sub>cm</sub> = 13 TeV with results of gluon fusion (ggF), VBF and t<span style="text-decoration: overline">t</span>H at E<sub>cm</sub> = 7 TeV, 8 TeV and 13 TeV to perform a search for the H → b<span style="text-decoration: overline">b</span> decay. The quoted signal strength assumes a SM production strength and corresponds to a significance of 5.6 standard deviations and is given for m<sub>H</sub> = 125.09 GeV.

25 SIRUNYAN 18E use 35.9 fb⁻¹ at E<sub>cm</sub> = 13 TeV. The quoted signal strength is given for m<sub>H</sub> = 125 GeV. They measure σ · B for gluon fusion production of H → b<span style="text-decoration: overline">b</span> with p<sub>T</sub> >450 GeV, |η| < 2.5 to be 74 ± 48<sup>+17</sup><sub>-10</sub> fb.

26 AABOUD 17BA use 36.1 fb⁻¹ at E<sub>cm</sub> = 13 TeV. The quoted signal strength is given for m<sub>H</sub> = 125 GeV. They give σ(W H) · B(H → b<span style="text-decoration: overline">b</span>) = 1.08<sup>+0.54</sup><sub>-0.47</sub> pb and σ(Z H) · B(H → b<span style="text-decoration: overline">b</span>) = 0.57<sup>+0.26</sup><sub>-0.23</sub> pb.

27 AABOUD 17BA combine 7, 8 and 13 TeV analyses. The quoted signal strength is given for m<sub>H</sub> = 125 GeV.

28 AABOUD 16x search for vector-boson fusion production of H decaying to b<span style="text-decoration: overline">b</span> in 20.2 fb⁻¹ of pp collisions at E<sub>cm</sub> = 8 TeV. The quoted signal strength is given for m<sub>H</sub> = 125 GeV.

29 AAD 16k use up to 4.7 fb⁻¹ of pp collisions at E<sub>cm</sub> = 7 TeV and up to 20.3 fb⁻¹ at E<sub>cm</sub> = 8 TeV. The quoted signal strength is given for m<sub>H</sub> = 125.36 GeV.

30 AAD 15g use 4.7 fb⁻¹ of pp collisions at E<sub>cm</sub> = 7 TeV and 20.3 fb⁻¹ at E<sub>cm</sub> = 8 TeV. The quoted signal strength is given for m<sub>H</sub> = 125.36 GeV.

31 KHACHATRYAN 15z search for vector-boson fusion production of H decaying to b<span style="text-decoration: overline">b</span> in up to 19.8 fb⁻¹ of pp collisions at E<sub>cm</sub> = 8 TeV. The quoted signal strength is given for m<sub>H</sub> = 125 GeV.

32 KHACHATRYAN 15z combined vector boson fusion, WH, ZH production, and t<span style="text-decoration: overline">t</span>H production results. The quoted signal strength is given for m<sub>H</sub> = 125 GeV.

33 CHATRCHYAN 14AI use up to 5.1 fb⁻¹ of pp collisions at E<sub>cm</sub> = 7 TeV and up to 18.9 fb⁻¹ at E<sub>cm</sub> = 8 TeV. The quoted signal strength is given for m<sub>H</sub> = 125 GeV. See also CHATRCHYAN 14AJ.

34 AALTONEN 13l combine all CDF results with 9.45–10.0 fb⁻¹ of p<span style="text-decoration: overline">p</span> collisions at E<sub>cm</sub> = 1.96 TeV. The quoted signal strength is given for m<sub>H</sub> = 125 GeV.

35 ABAZOV 13l combine all D0 results with up to 9.7 fb⁻¹ of p<span style="text-decoration: overline">p</span> collisions at E<sub>cm</sub> = 1.96 TeV. The quoted signal strength is given for m<sub>H</sub> = 125 GeV.

36 AAD 12AI obtain results based on 4.6–4.8 fb⁻¹ of pp collisions at E<sub>cm</sub> = 7 TeV. The quoted signal strengths are given in their Fig. 10 for m<sub>H</sub> = 126 GeV. See also Fig. 13 of AAD 12DA.

37 AALTONEN 12T combine AALTONEN 12Q, AALTONEN 12R, AALTONEN 12S, ABAZOV 12Q, ABAZOV 12P, and ABAZOV 12K. An excess of events over background is observed which is most significant in the region m<sub>H</sub> = 120–135 GeV, with a local significance of up to 3.3 σ. The local significance at m<sub>H</sub> = 125 GeV is 2.8 σ, which corresponds to (σ(HW) + σ(HZ)) · B(H → b<span style="text-decoration: overline">b</span>) = (0.23<sup>+0.09</sup><sub>-0.08</sub>) pb, compared to the Standard Model expectation at m<sub>H</sub> = 125 GeV of 0.12 ± 0.01 pb. Superseded by AALTONEN 13M.

38 CHATRCHYAN 12N obtain results based on 5.0 fb⁻¹ of pp collisions at E<sub>cm</sub>=7 TeV and 5.1 fb⁻¹ at E<sub>cm</sub>=8 TeV. The quoted signal strength is given for m<sub>H</sub>=125.5 GeV. See also CHATRCHYAN 13Y.

μ⁺μ⁻ Final State

<table><thead><tr><th>VALUE</th><th>CL%</th><th>DOCUMENT ID</th><th>TECN</th><th>COMMENT</th></tr></thead><tbody><tr><td colspan="5"><strong>1.21<sup>+0.35</sup><sub>-0.42</sub> OUR AVERAGE</strong></td></tr><tr><td>1.21<sup>+0.45</sup><sub>-0.42</sub></td><td>1 CMS</td><td>22</td><td>CMS</td><td>pp, 13 TeV</td></tr><tr><td>1.2 ± 0.6</td><td>2 AAD</td><td>21</td><td>ATLS</td><td>pp, 13 TeV</td></tr><tr><td colspan="5"><strong>1.19<sup>+0.40</sup><sub>-0.39</sub> OUR AVERAGE</strong></td></tr><tr><td>1.19<sup>+0.40</sup><sub>-0.39</sub></td><td>3 SIRUNYAN</td><td>21C</td><td>CMS</td><td>pp, 13 TeV</td></tr><tr><td>0.68<sup>+1.25</sup><sub>-1.24</sub></td><td>4 SIRUNYAN</td><td>19AT</td><td>CMS</td><td>pp, 13 TeV</td></tr><tr><td>0.7 ± 1.0<sup>+0.2</sup><sub>-0.1</sub></td><td>5 SIRUNYAN</td><td>19E</td><td>CMS</td><td>pp, 13 TeV, 35.9 fb<sup>-1</sup></td></tr><tr><td>1.0 ± 1.0 ± 0.1</td><td>5 SIRUNYAN</td><td>19E</td><td>CMS</td><td>pp, 7, 8, 13 TeV</td></tr><tr><td>-0.1 ± 1.4</td><td>6 AABOUD</td><td>17Y</td><td>ATLS</td><td>pp, 7, 8, 13 TeV</td></tr><tr><td>-0.1 ± 1.5</td><td>6 AABOUD</td><td>17Y</td><td>ATLS</td><td>pp, 13 TeV</td></tr><tr><td>0.1 ± 2.5</td><td>7 AAD</td><td>16AN</td><td>LHC</td><td>pp, 7, 8 TeV</td></tr><tr><td>-0.6 ± 3.6</td><td>7 AAD</td><td>16AN</td><td>ATLS</td><td>pp, 7, 8 TeV</td></tr><tr><td>0.9 ± 3.6<sup>+3.6</sup><sub>-3.5</sub></td><td>7 AAD</td><td>16AN</td><td>CMS</td><td>pp, 7, 8 TeV</td></tr><tr><td>&lt; 7.4</td><td>95</td><td>8 KHACHATRY...15H</td><td>CMS</td><td>pp → HX, 7, 8 TeV</td></tr><tr><td>7.0</td><td>95</td><td>14AS</td><td>ATLS</td><td>pp → HX, 7, 8 TeV</td></tr></tbody></table>

1 CMS 22 report combined results (see their Extended Data Table 2) using up to 138 fb⁻¹ of data at E<sub>cm</sub> = 13 TeV, assuming m<sub>H</sub> = 125.38 GeV. See their Fig. 2 right.

2 AAD 21 search for H → μ⁺μ⁻ using 139 fb⁻¹ of pp collision data at E<sub>cm</sub> = 13 TeV. The quoted signal strength corresponds to a significance of 2.0 standard deviations and is given for m<sub>H</sub> = 125.09 GeV. The upper limit on the cross section times branching fraction is 2.2 times the SM prediction at 95% CL, which corresponds to the branching fraction upper limit of 4.7 × 10⁻⁴ (assuming SM production cross sections).

3 SIRUNYAN 21 search for H → μ⁺μ⁻ using 137 fb⁻¹ of pp collision data at E<sub>cm</sub> = 13 TeV. The quoted signal strength corresponds to a significance of 3.0 standard deviations and is given for m<sub>H</sub> = 125.38 GeV.

4 SIRUNYAN 19AT perform a combine fit to 35.9 fb⁻¹ of data at E<sub>cm</sub> = 13 TeV.

5 SIRUNYAN 19E search for H → μ⁺μ⁻ using 35.9 fb⁻¹ of pp collisions at E<sub>cm</sub> = 13 TeV and combine with results of 7 TeV (5.0 fb⁻¹) and 8 TeV (19.7 fb⁻¹). The upper limit at 95% CL on the signal strength is 2.9, which corresponds to the SM Higgs boson branching fraction to a muon pair of 6.4 × 10⁻⁴.

6 AABOUD 17Y use 36.1 fb⁻¹ of pp collisions at E<sub>cm</sub> = 13 TeV, 20.3 fb⁻¹ at 8 TeV and 4.5 fb⁻¹ at 7 TeV. The quoted signal strength is given for m<sub>H</sub> = 125 GeV.

7 AAD 16AN: In the fit, relative production cross sections are fixed to those in the Standard Model. The quoted signal strength is given for m<sub>H</sub> = 125.09 GeV.

8 KHACHATRYAN 15H use 5.0 fb⁻¹ of pp collisions at E<sub>cm</sub> = 7 TeV and 19.7 fb⁻¹ at 8 TeV. The quoted signal strength is given for m<sub>H</sub> = 125 GeV.

9 AAD 14AS search for H → μ⁺μ⁻ in 4.5 fb⁻¹ of pp collisions at E<sub>cm</sub> = 7 TeV and 20.3 fb⁻¹ at E<sub>cm</sub> = 8 TeV. The quoted signal strength is given for m<sub>H</sub> = 125.5 GeV.

τ⁺τ⁻ Final State

<table><thead><tr><th>VALUE</th><th>DOCUMENT ID</th><th>TECN</th><th>COMMENT</th></tr></thead><tbody><tr><td colspan="4"><strong>0.91<sup>+0.09</sup><sub>-0.07</sub> OUR AVERAGE</strong></td></tr><tr><td>0.85 ± 0.10</td><td>1 CMS</td><td>22</td><td>CMS</td><td>pp, 13 TeV</td></tr><tr><td>1.09<sup>+0.18</sup><sub>-0.17</sub> + 0.26 + 0.16</td><td>2 AABOUD</td><td>19AQ</td><td>ATLS</td><td>pp, 13 TeV</td></tr><tr><td>1.11<sup>+0.24</sup><sub>-0.22</sub></td><td>3,4 AAD</td><td>16AN</td><td>LHC</td><td>pp, 7, 8 TeV</td></tr><tr><td>1.68<sup>+2.28</sup><sub>-1.68</sub></td><td>5 AALTONEN</td><td>13M</td><td>TEVA</td><td>p<span style="text-decoration: overline">p</span> → HX, 1.96 TeV</td></tr><tr><td colspan="5">• • • We do not use the following data for averages, fits, limits, etc. • • •</td></tr><tr><td>0.82<sup>+0.11</sup><sub>-0.10</sub></td><td>6,7 TUMASYAN</td><td>23Y</td><td>CMS</td><td>pp, 13 TeV</td></tr><tr><td>0.67<sup>+0.20</sup><sub>-0.18</sub></td><td>6,8 TUMASYAN</td><td>23Y</td><td>CMS</td><td>pp, 13 TeV</td></tr><tr><td>0.81<sup>+0.17</sup><sub>-0.16</sub></td><td>6,9 TUMASYAN</td><td>23Y</td><td>CMS</td><td>pp, 13 TeV</td></tr><tr><td>1.79<sup>+0.47</sup><sub>-0.42</sub></td><td>6,10 TUMASYAN</td><td>23Y</td><td>CMS</td><td>pp, 13 TeV</td></tr><tr><td></td><td>11 AAD</td><td>22Q</td><td>ATLS</td><td>pp, 13 TeV</td></tr><tr><td></td><td>12 TUMASYAN</td><td>22AJ</td><td>CMS</td><td>pp, 13 TeV</td></tr><tr><td>2.5<sup>+1.4</sup><sub>-1.3</sub></td><td>13 SIRUNYAN</td><td>19AF</td><td>CMS</td><td>pp → HW/HZ, H → ττ, 13 TeV</td></tr><tr><td>1.24<sup>+0.29</sup><sub>-0.27</sub></td><td>14 SIRUNYAN</td><td>19AF</td><td>CMS</td><td>pp, 13 TeV</td></tr><tr><td>1.02<sup>+0.26</sup><sub>-0.24</sub></td><td>15 SIRUNYAN</td><td>19AT</td><td>CMS</td><td>pp, 13 TeV</td></tr><tr><td>1.09<sup>+0.27</sup><sub>-0.26</sub></td><td>16 SIRUNYAN</td><td>18Y</td><td>CMS</td><td>pp, 13 TeV</td></tr><tr><td>0.98 ± 0.18</td><td>17 SIRUNYAN</td><td>18Y</td><td>CMS</td><td>pp, 7, 8, 13 TeV</td></tr><tr><td>2.3 ± 1.6</td><td>18 AAD</td><td>16AC</td><td>ATLS</td><td>pp → HW/ZX, 8 TeV</td></tr><tr><td>1.41<sup>+0.40</sup><sub>-0.36</sub></td><td>4 AAD</td><td>16AN</td><td>ATLS</td><td>pp, 7, 8 TeV</td></tr><tr><td>0.88<sup>+0.30</sup><sub>-0.28</sub></td><td>4 AAD</td><td>16AN</td><td>CMS</td><td>pp, 7, 8 TeV</td></tr><tr><td>1.44<sup>+0.30</sup><sub>-0.29</sub> + 0.29</td><td>19 AAD</td><td>16K</td><td>ATLS</td><td>pp, 7, 8 TeV</td></tr><tr><td>1.43<sup>+0.27</sup><sub>-0.26</sub> + 0.32</td><td>20 AAD</td><td>15AH</td><td>ATLS</td><td>pp → HX, 7, 8 TeV</td></tr><tr><td>0.78 ± 0.27</td><td>21 CHATRCHYAN14K</td><td>CMS</td><td></td><td>pp → HX, 7, 8 TeV</td></tr><tr><td>0.00<sup>+8.44</sup><sub>-0.00</sub></td><td>22 AALTONEN</td><td>13L</td><td>CDF</td><td>p<span style="text-decoration: overline">p</span> → HX, 1.96 TeV</td></tr><tr><td>3.96<sup>+4.11</sup><sub>-3.38</sub></td><td>23 ABAZOV</td><td>13L</td><td>D0</td><td>p<span style="text-decoration: overline">p</span> → HX, 1.96 TeV</td></tr><tr><td>0.4 <sup>+1.6</sup><sub>-2.0</sub></td><td>24 AAD</td><td>12AI</td><td>ATLS</td><td>pp → HX, 7 TeV</td></tr><tr><td>0.09<sup>+0.76</sup><sub>-0.74</sub></td><td>25 CHATRCHYAN12N</td><td>CMS</td><td></td><td>pp → HX, 7, 8 TeV</td></tr></tbody></table>

1 CMS 22 report combined results (see their Extended Data Table 2) using up to 138 fb⁻¹ of data at E<sub>cm</sub> = 13 TeV, assuming m<sub>H</sub> = 125.38 GeV. See their Fig. 2 right.

2 AABOUD 19AQ use 36.1 fb⁻¹ of data. The first, second and third quoted errors are statistical, experimental systematic and theory systematic uncertainties, respectively. The quoted signal strength is given for m<sub>H</sub> = 125 GeV and corresponds to 4.4 standard deviations. Combining with 7 TeV and 8 TeV results (AAD 15AH), the observed significance is 6.4 standard deviations. The cross sections in the H → ττ decay channel (m<sub>H</sub> = 125 GeV) are measured to be 3.77<sup>+0.60</sup><sub>-0.59</sub> (stat) +0.87<sub>-0.74</sub> (syst) pb for the inclusive, 0.28 ± 0.09<sup>+1.01</sup><sub>-0.09</sub> pb for VBF, and 3.1 ± 1.0<sup>+1.6</sup><sub>-1.3</sub> pb for gluon-fusion production. See their Table XI for the cross sections in the framework of simplified template cross sections.

3 AAD 16AN perform fits to the ATLAS and CMS data at E<sub>cm</sub> = 7 and 8 TeV. The signal strengths for individual production processes are 1.0 ± 0.6 for gluon fusion, 1.3 ± 0.4 for vector boson fusion, -1.4 ± 1.4 for WH production, 2.2<sup>+2.2</sup><sub>-1.8</sub> for ZH production, and -1.9<sup>+3.7</sup><sub>-3.3</sub> for t<span style="text-decoration: overline">t</span>H production.

4 AAD 16AN: In the fit, relative production cross sections are fixed to those in the Standard Model. The quoted signal strength is given for m<sub>H</sub> = 125.09 GeV.

5 AALTONEN 13M combine all Tevatron data from the CDF and D0 Collaborations with up to 10.0 fb⁻¹ and 9.7 fb⁻¹, respectively, of p<span style="text-decoration: overline">p</span> collisions at E<sub>cm</sub> = 1.96 TeV. The quoted signal strength is given for m<sub>H</sub> = 125 GeV.

6 TUMASYAN 23Y measure Higgs production with p<span style="text-decoration: overline">p</span> → H → ττ at E<sub>cm</sub> = 13 TeV with 138 fb⁻¹ data. The quoted results are given for m<sub>H</sub> = 125.38 GeV.

7 The inclusive σ · B is 2800<sup>+356</sup><sub>-335</sub> fb (see their Figs. 10 and 14). See their Fig. 15 for the 68 % and 95 % CL contours in the κ<sub>V</sub> - κ<sub>F</sub> plane.
¹ATLAS 22 report combined results (see their Extended Data Table 1) using up to 139 fb⁻¹ of data at $E_{cm} = 13$ TeV, assuming $m_H = 125.09$ GeV.

²All modifiers($\kappa$) > 0, and $\kappa_c = \kappa_t$ ($B_{inv} = B_{undetected} = 0$) are assumed. Only SM particles assume to contribute to the loop-induced processes. See their Fig. 5, which shows both $\kappa_c = \kappa_t$ and $\kappa_c$ floating.

³$B_{inv} = B_{undetected} = 0$ is assumed. Coupling strength modifiers including effective photon, $Z\gamma$ and gluon are measured. See their Fig. 6.

⁴$B_{inv}$ floating, $B_{undetected} \ge 0$, and $\kappa_V \le 1$ are assumed. Coupling strength modifiers including effective photon, $Z\gamma$ and gluon are measured. See their Fig. 6.

⁵CMS 22 report combined results (see their Extended Data Table 2) using up to 138 fb⁻¹ of data at $E_{cm} = 13$ TeV, assuming $m_H = 125.38$ GeV.

⁶Only SM particles assume to contribute to the loop-induced processes. See their Fig. 3 right.

⁷Coupling strength modifiers including effective photon, $Z\gamma$ and gluon are measured. See their Fig. 4 left.

## Z boson coupling ($\kappa_Z$)

<table><thead><tr><th>VALUE</th><th>DOCUMENT ID</th><th>TECN</th><th>COMMENT</th></tr></thead><tbody><tr><td>0.99<sup>+0.06</sup><sub>-0.05</sub></td><td>1,2 ATLAS</td><td>22</td><td>ATLS pp, 13 TeV</td></tr><tr><td>0.99<sup>+0.06</sup><sub>-0.05</sub></td><td>1,3 ATLAS</td><td>22</td><td>ATLS pp, 13 TeV</td></tr><tr><td>0.98<sup>+0.02</sup><sub>-0.05</sub></td><td>1,4 ATLAS</td><td>22</td><td>ATLS pp, 13 TeV</td></tr><tr><td>1.04<sup>+0.07</sup><sub>-0.07</sub></td><td>5,6 CMS</td><td>22</td><td>CMS pp, 13 TeV</td></tr><tr><td>1.04<sup>+0.07</sup><sub>-0.07</sub></td><td>5,7 CMS</td><td>22</td><td>CMS pp, 13 TeV</td></tr></tbody></table>

¹ATLAS 22 report combined results (see their Extended Data Table 1) using up to 139 fb⁻¹ of data at $E_{cm} = 13$ TeV, assuming $m_H = 125.09$ GeV.

²All modifiers($\kappa$) > 0, and $\kappa_c = \kappa_t$ ($B_{inv} = B_{undetected} = 0$) are assumed. Only SM particles assume to contribute to the loop-induced processes. See their Fig. 5, which shows both $\kappa_c = \kappa_t$ and $\kappa_c$ floating.

³$B_{inv} = B_{undetected} = 0$ is assumed. Coupling strength modifiers including effective photon, $Z\gamma$ and gluon are measured. See their Fig. 6.

⁴$B_{inv}$ floating, $B_{undetected} \ge 0$, and $\kappa_V \le 1$ are assumed. Coupling strength modifiers including effective photon, $Z\gamma$ and gluon are measured. See their Fig. 6.

⁵CMS 22 report combined results (see their Extended Data Table 2) using up to 138 fb⁻¹ of data at $E_{cm} = 13$ TeV, assuming $m_H = 125.38$ GeV.

⁶Only SM particles assume to contribute to the loop-induced processes. See their Fig. 3 right.

⁷Coupling strength modifiers including effective photon, $Z\gamma$ and gluon are measured. See their Fig. 4 left.

## top Yukawa coupling ($\kappa_t$)

<table><thead><tr><th>VALUE</th><th>DOCUMENT ID</th><th>TECN</th><th>COMMENT</th></tr></thead><tbody><tr><td>&lt;1.8</td><td>1 AAD</td><td>23BC ATLS</td><td>pp, 13 TeV</td></tr><tr><td>0.87-1.20</td><td>2 AAD</td><td>23Y ATLS</td><td>pp, 13 TeV</td></tr><tr><td>0.65-1.25</td><td>3 AAD</td><td>23Y ATLS</td><td>pp, 13 TeV</td></tr><tr><td>-1.09- -0.74 or 0.77-1.3</td><td>4 TUMASYAN</td><td>23P CMS</td><td>pp, 13 TeV</td></tr><tr><td>0.86-1.26</td><td>4,5 TUMASYAN</td><td>23P CMS</td><td>pp, 13 TeV</td></tr><tr><td>0.95<sup>+0.07</sup></td><td>6,7 ATLAS</td><td>22</td><td>ATLS pp, 13 TeV</td></tr><tr><td>0.94<sup>+0.11</sup></td><td>6,8 ATLAS</td><td>22</td><td>ATLS pp, 13 TeV</td></tr><tr><td>0.94<sup>+0.11</sup></td><td>6,9 ATLAS</td><td>22</td><td>ATLS pp, 13 TeV</td></tr><tr><td>0.95<sup>+0.07</sup><sub>-0.08</sub></td><td>10,11 CMS</td><td>22</td><td>CMS pp, 13 TeV</td></tr><tr><td>1.01<sup>+0.11</sup><sub>-0.10</sub></td><td>10,12 CMS</td><td>22</td><td>CMS pp, 13 TeV</td></tr><tr><td>-0.9- -0.7 or 0.7-1.1</td><td>13 SIRUNYAN</td><td>21R CMS</td><td>pp, 13 TeV</td></tr><tr><td>&lt;1.7</td><td>14 SIRUNYAN</td><td>20C CMS</td><td>pp, 13 TeV</td></tr><tr><td>&lt;1.67</td><td>15 SIRUNYAN</td><td>19B CMS</td><td>pp, 13 TeV</td></tr><tr><td>&lt;2.1</td><td>16 SIRUNYAN</td><td>18BU CMS</td><td>pp, 13 TeV</td></tr></tbody></table>

¹AAD 23BC measure the production of four top quarks with same-sign and multilepton final states with 140 fb⁻¹ pp collision data at $E_{cm} = 13$ TeV. The results constraint the ratio of the top quark Yukawa coupling $y_t$ to its Standard Model value, yielding $|y_t/y_t^{SM}| < 1.8$ at 95% CL. See their Fig. 8 as a function of $\kappa_t$ and CP-mixing angle.

²AAD 23Y constrain $\kappa_t$ from Higgs production rates with $H \to \gamma\gamma$ with 139 fb⁻¹ pp collision data at $E_{cm} = 13$ TeV. The quoted result is obtained assuming the SM loop structure in $gg \to H$ and $H \to \gamma\gamma$. See their Fig. 14.

³AAD 23Y constrain $\kappa_t$ from Higgs production rates with $H \to \gamma\gamma$ with 139 fb⁻¹ pp collision data at $E_{cm} = 13$ TeV. The quoted result is obtained assuming effective couplings $\kappa_{gluon}$ and $\kappa_\gamma$ for $gg \to H$ and $H \to \gamma\gamma$, respectively. See their Fig. 14.

⁴TUMASYAN 23P constrain $\kappa_t$ from $t\bar{t}H$ and $tH$ decaying $H \to WW^*$ and $H \to \tau\tau$ (multilepton decay mode) with 138 fb⁻¹ pp collision data at $E_{cm} = 13$ TeV. The $\kappa_t$ is obtained by fixing $\kappa_t = 0$ and other couplings ($\kappa_V$ etc.) to the SM values. See their Fig. 9 for 2-dim contours and Table 6.

⁵The quoted result is obtained by combining with other $t\bar{t}H$ decaying $H \to \gamma\gamma$ (SIRUNYAN 20As) and $H \to 4\ell$ (SIRUNYAN 21AE) and $\kappa_t = 0$. See their Fig. 12 for 2-dim contours and Table 7.

⁶ATLAS 22 report combined results (see their Extended Data Table 1) using up to 139 fb⁻¹ of data at $E_{cm} = 13$ TeV, assuming $m_H = 125.09$ GeV.

⁷All modifiers($\kappa$) > 0, and $\kappa_c = \kappa_t$ ($B_{inv} = B_{undetected} = 0$) are assumed. Only SM particles assume to contribute to the loop-induced processes. See their Fig. 5, which shows both $\kappa_c = \kappa_t$ and $\kappa_c$ floating.

⁸$B_{inv} = B_{undetected} = 0$ is assumed. Coupling strength modifiers including effective photon, $Z\gamma$ and gluon are measured. See their Fig. 6.

⁹$B_{inv}$ floating, $B_{undetected} \ge 0$, and $\kappa_V \le 1$ are assumed. Coupling strength modifiers including effective photon, $Z\gamma$ and gluon are measured. See their Fig. 6.

¹⁰CMS 22 report combined results (see their Extended Data Table 2) using up to 138 fb⁻¹ of data at $E_{cm} = 13$ TeV, assuming $m_H = 125.38$ GeV.

¹¹Only SM particles assume to contribute to the loop-induced processes. See their Fig. 3 right.

¹²Coupling strength modifiers including effective photon, $Z\gamma$ and gluon are measured. See their Fig. 4 left.

¹³SIRUNYAN 21R constrain the ratio of the top quark Yukawa coupling $y_t$ to its Standard Model value from $t\bar{t}H$ and $tH$ production rates using 137 fb⁻¹ pp collision data at $E_{cm} = 13$ TeV. Assuming a SM Higgs couplings to $\tau$'s, the joint interval -0.9 < $\kappa_t$($y_t/y_t^{SM}$) < -0.7 and 0.7 < $\kappa_t$ < 1.1 is obtained at 95% CL (see their Fig. 17).

¹⁴SIRUNYAN 20C search for the production of four top quarks with same-sign and multilepton final states with 137 fb⁻¹ pp collision data at $E_{cm} = 13$ TeV. The results constrain the ratio of the top quark Yukawa coupling $y_t$ to its Standard Model value by comparing to the central value of a theoretical prediction (see their Refs. [1-2]), yielding $|y_t/y_t^{SM}| < 1.7$ at 95% CL. See their Fig. 5.

¹⁵SIRUNYAN 19BY measure the top quark Yukawa coupling from $t\bar{t}$ kinematic distributions, the invariant mass of the top quark pair and the rapidity difference between $t$ and $\bar{t}$, in the $\ell^+$jets final state with 35.8 fb⁻¹ pp collision data at $E_{cm} = 13$ TeV. The results constrain the ratio of the top quark Yukawa coupling to its Standard Model to be $1.07^{+0.34}_{-0.43}$ with an upper limit of 1.67 at 95% CL (see their Table III).

¹⁶SIRUNYAN 18BU search for the production of four top quarks with same-sign and multilepton final states with 35.9 fb⁻¹ pp collision data at $E_{cm} = 13$ TeV. The results constrain the ratio of the top quark Yukawa coupling $y_t$ to its Standard Model by comparing to the central value of a theoretical prediction (see their Ref. [16]), yielding $|y_t/y_t^{SM}| < 2.1$ at 95% CL.

## bottom Yukawa coupling ($\kappa_b$)

<table><thead><tr><th>VALUE</th><th>CL%</th><th>DOCUMENT ID</th><th>TECN</th><th>COMMENT</th></tr></thead><tbody><tr><td>-1.09 to -0.86 OR<br>0.81 to 1.09</td><td>95</td><td>1 AAD</td><td>23C ATLS</td><td>pp, 13 TeV, γγ, ZZ* →<br>4ℓ cross sections</td></tr><tr><td>-1.1 to 1.1</td><td>95</td><td>2 AAD<br>3 HAYRAPETY...23</td><td>23CD ATLS<br>CMS</td><td>pp, 13 TeV, H → T(nS)γ<br>pp, 13 TeV, ZZ* → 4ℓ<br>cross sections</td></tr><tr><td>0.90<sup>+0.11</sup></td><td>4.5 ATLAS</td><td>4.5 ATLAS</td><td>22 ATLS</td><td>pp, 13 TeV</td></tr><tr><td>0.89<sup>+0.11</sup></td><td>4.6 ATLAS</td><td>4.6 ATLAS</td><td>22 ATLS</td><td>pp, 13 TeV</td></tr><tr><td>0.82<sup>+0.09</sup><sub>-0.08</sub></td><td>4,7 ATLAS</td><td>4,7 ATLAS</td><td>22 ATLS</td><td>pp, 13 TeV</td></tr><tr><td>1.02<sup>+0.15</sup><sub>-0.17</sub></td><td>8,9 CMS</td><td>8,9 CMS</td><td>22 CMS</td><td>pp, 13 TeV</td></tr><tr><td>0.99<sup>+0.17</sup><sub>-0.16</sub></td><td>8,10 CMS</td><td>8,10 CMS</td><td>22 CMS</td><td>pp, 13 TeV</td></tr></tbody></table>

¹AAD 23C combine results of $H \to \gamma\gamma$ and $H \to ZZ^*$ → 4ℓ ($\ell(e, \mu)$) using 139 fb⁻¹ at $E_{cm} = 13$ TeV. The Higgs boson transverse momentum ($p_T^H$) distribution constrains $\kappa_b$ and $\kappa_c$, assuming other couplings fixed to the SM values. The $\kappa_b$ is obtained using the $p_T^H$ shape and normalisation. Other cases are given in their Tables 6 and 7.

²AAD 23CD search for $H \to T(nS)\gamma$, $\gamma(nS) \to \mu^+\mu^-$ (n=1,2,3) with 138 fb⁻¹ of pp collision data at $E_{cm} = 13$ TeV. They interpret the $H \to T(nS)\gamma$ search to constrain the bottom Yukawa coupling by comparing to $H \to \gamma\gamma$. An observed 95% CL interval of (-37, 40) is obtained for $\kappa_b/\kappa_\gamma$.

³HAYRAPETY 23 measure the cross sections for $pp \to H \to ZZ^*$ → 4ℓ ($\ell(e, \mu)$) using 138 fb⁻¹ at $E_{cm} = 13$ TeV. The $\kappa_b$ is obtained from the $p_T$ differential cross section of the $ggF$ production employing the dependence of the branching fraction on $\kappa_b$ and $\kappa_c$.

⁴ATLAS 22 report combined results (see their Extended Data Table 1) using up to 139fb⁻¹ of data at $E_{cm} = 13$ TeV, assuming $m_H = 125.09$ GeV.

⁵All modifiers ($\kappa$) > 0, and $\kappa_c = \kappa_t$ ($B_{inv} = B_{undetected} = 0$) are assumed. Only SM particles assume to contribute to the loop-induced processes. See their Fig. 5, which shows both $\kappa_c = \kappa_t$ and $\kappa_c$ floating.

⁶$B_{inv}$ = $B_{undetected} = 0$ is assumed. Coupling strength modifiers including effective photon, $Z\gamma$ and gluon are measured. See their Fig. 6.

⁷$B_{inv}$ floating, $B_{undetected} \ge 0$, and $\kappa_V \le 1$ are assumed. Coupling strength modifiers including effective photon, $Z\gamma$ and gluon are measured. See their Fig. 6.

⁸CMS 22 report combined results (see their Extended Data Table 2) using up to 138 fb⁻¹ of data at $E_{cm} = 13$ TeV, assuming $m_H = 125.38$ GeV.

⁹Only SM particles assume to contribute to the loop-induced processes. See their Fig. 3 right.

¹⁰Coupling strength modifiers including effective photon, $Z\gamma$ and gluon are measured. See their Fig. 4 left.

## charm Yukawa coupling ($\kappa_c$)

<table><thead><tr><th>VALUE</th><th>CL%</th><th>DOCUMENT ID</th><th>TECN</th><th>COMMENT</th></tr></thead><tbody><tr><td>|$\kappa_c$| < 2.27</td><td>95</td><td>1 AAD</td><td>23C ATLS</td><td>pp, 13 TeV, γγ, ZZ* →<br>4ℓ cross sections</td></tr><tr><td>-5.3 to 5.2</td><td>95</td><td>2 AAD<br>3 HAYRAPETY...23</td><td>23CD ATLS<br>CMS</td><td>pp, 13 TeV, H → J/ψγ<br>pp, 13 TeV, ZZ* → 4ℓ<br>cross sections</td></tr><tr><td>1.1 < |$\kappa_c$| < 5.5</td><td>95</td><td>4 TUMASYAN</td><td>23AH CMS</td><td>pp → W H/Z H, 13 TeV</td></tr><tr><td>0.03<sup>+3.02</sup><sub>-0.03</sub></td><td></td><td>5 ATLAS</td><td>22 ATLS</td><td>pp, 13 TeV</td></tr></tbody></table>

¹AAD 23C combine results of $H \to \gamma\gamma$ and $H \to ZZ^*$ → 4ℓ ($\ell(e, \mu)$) using 139 fb⁻¹ at $E_{cm} = 13$ TeV. The Higgs boson transverse momentum ($p_T^H$) distribution constrains $\kappa_b$ and $\kappa_c$, assuming other couplings fixed to the SM values. The $\kappa_c$ is obtained using the $p_T^H$ shape and normalisation. Other cases are given in their Tables 6 and 7. See their Table 8 for results combined with $V H, H \to b\bar{b}$ and $c\bar{c}$.

²AAD 23CD search for $H \to J/\psi\gamma, J/\psi \to \mu^+\mu^-$ with 138 fb⁻¹ of pp collision data at $E_{cm} = 13$ TeV. They interpret the $H \to J/\psi\gamma$ search to constrain the charm Yukawa coupling by comparing to $H \to \gamma\gamma$. An observed 95% CL interval of (-133, 175) is obtained for $\kappa_c/\kappa_\gamma$.
³HAYRAPETYAN 23 measure the cross sections for $pp \to H \to ZZ^* \to 4\ell$ ($\ell = e, \mu$) using 138 fb⁻¹ at $E_{cm} = 13$ TeV. The $\kappa_c$ is obtained from the $p_T$ differential cross section of the ggF production employing the dependence of the branching fraction of $\kappa_b$ and $\kappa_e$.

⁴TUMASYAN 23AH search for $VH, H \to c\bar{c} (V = W, Z)$ using 138 fb⁻¹ of $pp$ collision data at $E_{cm} = 13$ TeV. The quoted values are obtained from the measured signal strength in the $\kappa$-framework, where only the Higgs decay width for $H \to c\bar{c}$ is changed while assuming all the other decay widths and the production cross section to be SM ones. The quoted values are given for $m_H = 125.38$ GeV.

⁵ATLAS 22 report combined results (see their Extended Data Table 1) using up to 139 fb⁻¹ of data at $E_{cm} = 13$ TeV, assuming $m_H = 125.09$ GeV, and all modifiers ($\kappa$) > 0 ($B_{inv} = B_{undetected} = 0$). Only SM particles assume to contribute to the loop-induced processes. See their Fig. 5, which shows both $\kappa_c = \kappa_t$ and $\kappa_c$ floating.

### tau Yukawa coupling ($\kappa_\tau$)

<table><thead><tr><th>VALUE</th><th>DOCUMENT ID</th><th>TECN</th><th>COMMENT</th></tr></thead><tbody><tr><td>0.94±0.07</td><td>1,2 ATLAS</td><td>22</td><td>ATLS pp, 13 TeV</td></tr><tr><td>0.93±0.07</td><td>1,3 ATLAS</td><td>22</td><td>ATLS pp, 13 TeV</td></tr><tr><td>0.91±0.07<br>-0.06</td><td>1,4 ATLAS</td><td>22</td><td>ATLS pp, 13 TeV</td></tr><tr><td>0.93±0.08</td><td>5,6 CMS</td><td>22</td><td>CMS pp, 13 TeV</td></tr><tr><td>0.92±0.08</td><td>5,7 CMS</td><td>22</td><td>CMS pp, 13 TeV</td></tr></tbody></table>

¹ATLAS 22 report combined results (see their Extended Data Table 1) using up to 139 fb⁻¹ of data at $E_{cm} = 13$ TeV, assuming $m_H = 125.09$ GeV.

²All modifiers($\kappa$) > 0, and $\kappa_c = \kappa_t$ ($B_{inv} = B_{undetected} = 0$) are assumed. Only SM particles assume to contribute to the loop-induced processes. See their Fig. 5, which shows both $\kappa_c = \kappa_t$ and $\kappa_c$ floating.

³$B_{inv} = B_{undetected} = 0$ is assumed. Coupling strength modifiers including effective photon, $Z\gamma$ and gluon are measured. See their Fig. 6.

⁴$B_{inv}$ floating, $B_{undetected} \ge 0$, and $\kappa_V \le 1$ are assumed. Coupling strength modifiers including effective photon, $Z\gamma$ and gluon are measured. See their Fig. 6.

⁵CMS 22 report combined results (see their Extended Data Table 2) using up to 138 fb⁻¹ of data at $E_{cm} = 13$ TeV, assuming $m_H = 125.38$ GeV.

⁶Only SM particles assume to contribute to the loop-induced processes. See their Fig. 3 right.

⁷Coupling strength modifiers including effective photon, $Z\gamma$ and gluon are measured. See their Fig. 4 left.

### muon Yukawa coupling ($\kappa_\mu$)

<table><thead><tr><th>VALUE</th><th>DOCUMENT ID</th><th>TECN</th><th>COMMENT</th></tr></thead><tbody><tr><td>1.07<sup>+0.25</sup><sub>-0.31</sub></td><td>1,2 ATLAS</td><td>22</td><td>ATLS pp, 13 TeV</td></tr><tr><td>1.06<sup>+0.25</sup><sub>-0.30</sub></td><td>1,3 ATLAS</td><td>22</td><td>ATLS pp, 13 TeV</td></tr><tr><td>1.04<sup>+0.23</sup><sub>-0.30</sub></td><td>1,4 ATLAS</td><td>22</td><td>ATLS pp, 13 TeV</td></tr><tr><td>1.12<sup>+0.20</sup><sub>-0.22</sub></td><td>5,6 CMS</td><td>22</td><td>CMS pp, 13 TeV</td></tr><tr><td>1.12<sup>+0.21</sup><sub>-0.22</sub></td><td>5,7 CMS</td><td>22</td><td>CMS pp, 13 TeV</td></tr></tbody></table>

¹ATLAS 22 report combined results (see their Extended Data Table 1) using up to 139 fb⁻¹ of data at $E_{cm} = 13$ TeV, assuming $m_H = 125.09$ GeV.

²All modifiers($\kappa$) > 0, and $\kappa_c = \kappa_t$ ($B_{inv} = B_{undetected} = 0$) are assumed. Only SM particles assume to contribute to the loop-induced processes. See their Fig. 5, which shows both $\kappa_c = \kappa_t$ and $\kappa_c$ floating.

³$B_{inv} = B_{undetected} = 0$ is assumed. Coupling strength modifiers including effective photon, $Z\gamma$ and gluon are measured. See their Fig. 6.

⁴$B_{inv}$ floating, $B_{undetected} \ge 0$, and $\kappa_V \le 1$ are assumed. Coupling strength modifiers including effective photon, $Z\gamma$ and gluon are measured. See their Fig. 6.

⁵CMS 22 report combined results (see their Extended Data Table 2) using up to 138 fb⁻¹ of data at $E_{cm} = 13$ TeV, assuming $m_H = 125.38$ GeV.

⁶Only SM particles assume to contribute to the loop-induced processes. See their Fig. 3 right.

⁷Coupling strength modifiers including effective photon, $Z\gamma$ and gluon are measured. See their Fig. 4 left.

### photon effective coupling ($\kappa_\gamma$)

<table><thead><tr><th>VALUE</th><th>DOCUMENT ID</th><th>TECN</th><th>COMMENT</th></tr></thead><tbody><tr><td>1.02<sup>+0.08</sup><sub>-0.07</sub></td><td>1 AAD</td><td>23Y ATLS</td><td>pp, 13 TeV</td></tr><tr><td>1.01±0.06</td><td>2,3 ATLAS</td><td>22</td><td>ATLS pp, 13 TeV</td></tr><tr><td>0.98±0.05</td><td>2,4 ATLAS</td><td>22</td><td>ATLS pp, 13 TeV</td></tr><tr><td>1.10±0.08</td><td>5 CMS</td><td>22</td><td>CMS pp, 13 TeV</td></tr></tbody></table>

¹AAD 23Y constrain $\kappa_\gamma$ from Higgs production rates with $H \to \gamma\gamma$ with 139 fb⁻¹ $pp$ collision data at $E_{cm} = 13$ TeV. The quoted result is obtained assuming effective couplings $\kappa_{gluon}$ and $\kappa_\gamma$ for $gg \to H$ and $H \to \gamma\gamma$, respectively and other couplings fixed to the SM values. See their Fig. 15.

²ATLAS 22 report combined results (see their Extended Data Table 1) using up to 139 fb⁻¹ of data at $E_{cm} = 13$ TeV, assuming $m_H = 125.09$ GeV. Coupling strength modifiers including effective photon, $Z\gamma$ and gluon are measured. See their Fig. 6.

³$B_{inv} = B_{undetected} = 0$ is assumed.

⁴$B_{inv}$ floating, $B_{undetected} \ge 0$, and $\kappa_V \le 1$ are assumed.

⁵CMS 22 report combined results (see their Extended Data Table 2) using up to 138 fb⁻¹ of data at $E_{cm} = 13$ TeV, assuming $m_H = 125.38$ GeV. Coupling strength modifiers including effective photon, $Z\gamma$ and gluon are measured. See their Fig. 4 left.

### gluon effective coupling ($\kappa_{gluon}$)

<table><thead><tr><th>VALUE</th><th>DOCUMENT ID</th><th>TECN</th><th>COMMENT</th></tr></thead><tbody><tr><td>1.01<sup>+0.11</sup><sub>-0.09</sub></td><td>1 AAD</td><td>23Y ATLS</td><td>pp, 13 TeV</td></tr><tr><td>0.95±0.07</td><td>2,3 ATLAS</td><td>22</td><td>ATLS pp, 13 TeV</td></tr><tr><td>0.94<sup>+0.07</sup><sub>-0.06</sub></td><td>2,4 ATLAS</td><td>22</td><td>ATLS pp, 13 TeV</td></tr><tr><td>0.92±0.08</td><td>5 CMS</td><td>22</td><td>CMS pp, 13 TeV</td></tr></tbody></table>

¹AAD 23Y constrain $\kappa_{gluon}$ from Higgs production rates with $H \to \gamma\gamma$ with 139 fb⁻¹ $pp$ collision data at $E_{cm} = 13$ TeV. The quoted result is obtained assuming effective couplings $\kappa_{gluon}$ and $\kappa_\gamma$ for $gg \to H$ and $H \to \gamma\gamma$, respectively and other couplings fixed to the SM values. See their Fig. 15.

²ATLAS 22 report combined results (see their Extended Data Table 1) using up to 139 fb⁻¹ of data at $E_{cm} = 13$ TeV, assuming $m_H = 125.09$ GeV. Coupling strength modifiers including effective photon, $Z\gamma$ and gluon are measured. See their Fig. 6.

³$B_{inv} = B_{undetected} = 0$ is assumed.

⁴$B_{inv}$ floating, $B_{undetected} \ge 0$, and $\kappa_V \le 1$ are assumed.

⁵CMS 22 report combined results (see their Extended Data Table 2) using up to 138 fb⁻¹ of data at $E_{cm} = 13$ TeV, assuming $m_H = 125.38$ GeV. Coupling strength modifiers including effective photon, $Z\gamma$ and gluon are measured. See their Fig. 4 left.

### $Z\gamma$ effective coupling ($\kappa_{Z\gamma}$)

<table><thead><tr><th>VALUE</th><th>DOCUMENT ID</th><th>TECN</th><th>COMMENT</th></tr></thead><tbody><tr><td>1.38<sup>+0.31</sup><sub>-0.37</sub></td><td>1,2 ATLAS</td><td>22</td><td>ATLS pp, 13 TeV</td></tr><tr><td>1.35<sup>+0.29</sup><sub>-0.36</sub></td><td>1,3 ATLAS</td><td>22</td><td>ATLS pp, 13 TeV</td></tr><tr><td>1.65<sup>+0.34</sup><sub>-0.37</sub></td><td>4 CMS</td><td>22</td><td>CMS pp, 13 TeV</td></tr></tbody></table>

¹ATLAS 22 report combined results (see their Extended Data Table 1) using up to 139 fb⁻¹ of data at $E_{cm} = 13$ TeV, assuming $m_H = 125.09$ GeV. Coupling strength modifiers including effective photon, $Z\gamma$ and gluon are measured. See their Fig. 6.

²$B_{inv} = B_{undetected} = 0$ is assumed.

³$B_{inv}$ floating, $B_{undetected} \ge 0$, and $\kappa_V \le 1$ are assumed.

⁴CMS 22 report combined results (see their Extended Data Table 2) using up to 138 fb⁻¹ of data at $E_{cm} = 13$ TeV, assuming $m_H = 125.38$ GeV. Coupling strength modifiers including effective photon, $Z\gamma$ and gluon are measured. See their Fig. 4 left.

## OTHER H PRODUCTION PROPERTIES

### $t\bar{t}H$ Production

Signal strength relative to the Standard Model cross section.

<table><thead><tr><th>VALUE</th><th>DOCUMENT ID</th><th>TECN</th><th>COMMENT</th></tr></thead><tbody><tr><td>1.10±0.18 OUR AVERAGE</td><td></td><td></td><td></td></tr><tr><td>0.92±0.19<sup>+0.17</sup><sub>-0.13</sub></td><td>1 SIRUNYAN</td><td>21R CMS</td><td>pp, 13 TeV, $H \to \tau\tau$, WW*, ZZ*</td></tr><tr><td>1.2 ±0.3</td><td>2 AABOUD</td><td>18AC ATLS</td><td>pp, 13 TeV, $H \to b\bar{b} \tau\tau$, $\gamma\gamma$, WW*, ZZ*</td></tr><tr><td>1.9<sup>+0.8</sup><sub>-0.7</sub></td><td>3 AAD</td><td>16AN ATLS</td><td>pp, 7, 8 TeV</td></tr><tr><td>-0.27<sup>+0.86</sup><sub>-0.83</sub></td><td>4 TUMASYAN</td><td>23AI ATLS</td><td>pp, 13 TeV, boosted $H \to b\bar{b}$</td></tr><tr><td>0.35<sup>+0.36</sup><sub>-0.34</sub></td><td>5 AAD</td><td>22M ATLS</td><td>pp, 13 TeV, $H \to b\bar{b}$</td></tr><tr><td>1.43<sup>+0.33</sup><sub>-0.31</sub></td><td>6 AAD</td><td>20Z ATLS</td><td>pp, 13 TeV, $H \to \gamma\gamma$</td></tr><tr><td>1.38<sup>+0.36</sup><sub>-0.29</sub></td><td>7 SIRUNYAN</td><td>20AS CMS</td><td>pp, 13 TeV, $H \to \gamma\gamma$</td></tr><tr><td>0.72±0.24±0.38</td><td>8 SIRUNYAN</td><td>19R CMS</td><td>pp, 13 TeV, $H \to b\bar{b}$</td></tr><tr><td>1.6<sup>+0.5</sup><sub>-0.4</sub></td><td>9 AABOUD</td><td>18AC ATLS</td><td>pp, 13 TeV, $H \to \tau\tau$, WW*, ZZ*</td></tr><tr><td></td><td>10 AABOUD</td><td>18BK ATLS</td><td>pp, 13 TeV, $H \to b\bar{b} \tau\tau$, $\gamma\gamma$, WW*, ZZ*</td></tr><tr><td>0.84<sup>+0.64</sup><sub>-0.61</sub></td><td>11 AABOUD</td><td>18T ATLS</td><td>pp, 13 TeV, $H \to b\bar{b}$</td></tr><tr><td>0.9 ±1.5</td><td>12 SIRUNYAN</td><td>18BD CMS</td><td>pp, 13 TeV, $H \to b\bar{b}$</td></tr><tr><td>1.23<sup>+0.45</sup><sub>-0.43</sub></td><td>13 SIRUNYAN</td><td>18BQ CMS</td><td>pp, 13 TeV, $H \to \tau\tau$, WW*, ZZ*</td></tr><tr><td>1.26<sup>+0.31</sup><sub>-0.26</sub></td><td>14 SIRUNYAN</td><td>18L CMS</td><td>pp, 7, 8, 13 TeV, $H \to b\bar{b} \tau\tau$, $\gamma\gamma$, WW*, ZZ*</td></tr><tr><td>1.7 ±0.8</td><td>15 AAD</td><td>16AL ATLS</td><td>pp, 7, 8 TeV, $H \to b\bar{b}$, $\tau\tau$, $\gamma\gamma$, WW*, and ZZ*</td></tr><tr><td>2.3<sup>+0.7</sup><sub>-0.6</sub></td><td>3,16 AAD</td><td>16AN LHC</td><td>pp, 7, 8 TeV</td></tr><tr><td>2.9<sup>+1.0</sup><sub>-0.9</sub></td><td>3 AAD</td><td>16AN CMS</td><td>pp, 7, 8 TeV</td></tr><tr><td>1.81<sup>+0.52</sup><sub>-0.50</sub></td><td>17 AAD</td><td>16K ATLS</td><td>pp, 7, 8 TeV</td></tr><tr><td>1.4<sup>+2.1</sup><sub>-1.4</sub></td><td>18 AAD</td><td>15 ATLS</td><td>pp, 7, 8 TeV</td></tr><tr><td>1.5 ±1.1</td><td>19 AAD</td><td>15BC ATLS</td><td>pp, 8 TeV</td></tr><tr><td>2.1<sup>+1.4</sup><sub>-1.2</sub></td><td>20 AAD</td><td>15T ATLS</td><td>pp, 8 TeV</td></tr></tbody></table>
# Gauge & Higgs Boson Particle Listings

H

<table><tr><td>1.2</td><td>+1.6</td><td>21 KHACHATRY...15AN CMS</td><td>pp, 8 TeV</td></tr><tr><td>2.8</td><td>+1.0</td><td>22 KHACHATRY...14H CMS</td><td>pp, 7, 8 TeV</td></tr><tr><td>9.49</td><td>+6.60</td><td>23 AALTONEN 13L CDF</td><td>p<span style="text-decoration: overline">b</span>, 1.96 TeV</td></tr><tr><td>&lt; 5.8 at 95% CL</td><td></td><td>24 CHATRCHYAN 13x CMS</td><td>pp, 7, 8 TeV, H → b<span style="text-decoration: overline">b</span></td></tr></table>

1 SIRUNYAN 21R search for $t\bar{t}H$ in final states with electrons, muons and hadronically decaying $\tau$ leptons ($H \to WW^*, ZZ^*, \tau\tau$) with 137 fb⁻¹ of pp collision data at $E_{cm} = 13$ TeV. The quoted signal strength corresponds to a significance of 4.7 standard deviations and is given for $m_H = 125$ GeV.

2 AABOUD 18AC combine results of $t\bar{t}H, H \to \tau\tau, WW^*(\to \ell\nu\ell\nu, \ell\nu q\bar{q}), ZZ^*(\to \ell\nu\ell\nu, \ell\ell q\bar{q})$ with results of $t\bar{t}H, H \to b\bar{d}$ (AABOUD 18T), $\gamma\gamma$ (AABOUD 18B0), $ZZ^*(\to 4\ell)$ (AABOUD 18AJ) in 36.1 fb⁻¹ of pp collisions at $E_{cm} = 13$ TeV. The quoted signal strength is given for $m_H = 125$ GeV. See their Table 14.

3 AAD 16AN: In the fit, relative branching ratios are fixed to those in the Standard Model. The quoted signal strength is given for $m_H = 125.09$ GeV.

4 TUMASYAN 23AI measure boosted $H \to b\bar{d}(p_T > 200$ GeV) in $t\bar{t}H$ production using 138 fb⁻¹ of data at $E_{cm} = 13$ TeV. The differential cross section for the Higgs $p_T$ is shown in their Fig. 8 and Table V. Limits on eight Weyl coefficients at 68% and 95% CL are shown in their Fig. 10 and Table VI.

5 AAD 22m measure $H \to b\bar{d}$ in $t\bar{t}H$ production using 139 fb⁻¹ of data at $E_{cm} = 13$ TeV. See their Fig. 14. The signal strengths and 95% CL cross section upper limits with simplified template cross section bins are given in Figs. 18 and 19, respectively.

6 AAD 20z measure $\sigma_t t\bar{t}H \cdot B(H \to \gamma\gamma)$ to be $1.64^{+0.38}_{-0.17}$ fb in 139 fb⁻¹ of data at $E_{cm} = 13$ TeV.

7 SIRUNYAN 20AS measure $\sigma_t t\bar{t}H \cdot B(H \to \gamma\gamma)$ to be $1.56^{+0.34}_{-0.32}$ fb in 137 fb⁻¹ of data at $E_{cm} = 13$ TeV.

8 SIRUNYAN 19R search for $t\bar{t}H$ production with $H$ decaying to $b\bar{d}$ in 35.9 fb⁻¹ of data at $E_{cm} = 13$ TeV. The quoted signal strength is given for $m_H = 125$ GeV.

9 AABOUD 18AC search for $t\bar{t}H$ production with $H$ decaying to $\tau\tau, WW^*(\to \ell\nu\ell\nu, \ell\nu q\bar{q}), ZZ^*(\to \ell\nu\ell\nu, \ell\ell q\bar{q})$ in 36.1 fb⁻¹ of pp collisions at $E_{cm} = 13$ TeV. The quoted signal strength is given for $m_H = 125$ GeV. See their Table 13 and Fig. 13.

10 AABOUD 18BK use 79.8 fb⁻¹ data for $t\bar{t}H$ production with $H \to \gamma\gamma$ and $ZZ^* \to 4\ell$ ($\ell = e, \mu$) and 36.1 fb⁻¹ for other decay channels at $E_{cm} = 13$ TeV. A significance of 5.8 standard deviations is observed for $m_H = 125.09$ GeV and its signal strength without the uncertainty of the $t\bar{t}H$ cross section is $1.32^{+0.28}_{-0.26}$. Combining with results of 7 and 8 TeV (AAD 16K), the significance is 6.3 standard deviations. Assuming Standard Model branching fractions, the total $t\bar{t}H$ production cross section at 13 TeV is measured to be $670 \pm 90^{+110}_{-100}$ fb.

11 AABOUD 18T search for $t\bar{t}H$ production with $H$ decaying to $b\bar{d}$ in 36.1 fb⁻¹ of pp collisions at $E_{cm} = 13$ TeV. The quoted signal strength is given for $m_H = 125$ GeV.

12 SIRUNYAN 18BD search for $t\bar{t}H, H \to b\bar{d}$ in the all-jet final state with 35.9 fb⁻¹ pp collision data at $E_{cm} = 13$ TeV. The quoted signal strength is given for $m_H = 125$ GeV.

13 SIRUNYAN 18BQ search for $t\bar{t}H$ in final states with electrons, muons and hadronically decaying $\tau$ leptons ($H \to WW^*, ZZ^*, \tau\tau$) with 35.9 fb⁻¹ of pp collision data at $E_{cm} = 13$ TeV. The quoted signal strength corresponds to a significance of 3.2 standard deviations and is given for $m_H = 125$ GeV.

14 SIRUNYAN 18L use up to 5.1, 19.7 and 35.9 fb⁻¹ of pp collisions at $E_{cm} = 7, 8$, and 13 TeV, respectively. The quoted signal strength corresponds to a significance of 5.2 standard deviations and is given for $m_H = 125.09$ GeV. H decay channels of $WW^*, ZZ^*, \gamma\gamma, \tau\tau$, and $b\bar{d}$ are used. See their Table 1 and Fig. 2 for results on individual channels.

15 AAD 16AL search for $t\bar{t}H$ production with $H$ decaying to $\gamma\gamma$ in 4.5 fb⁻¹ of pp collisions at $E_{cm} = 7$ TeV and $b\bar{d}, \tau\tau, \gamma\gamma, WW^*, $ and $ZZ^*$ in 20.3 fb⁻¹ at $E_{cm} = 8$ TeV. The quoted signal strength is given for $m_H = 125$ GeV. This paper combines the results of previous papers, and the new result of this paper only is: $\mu = 1.6 \pm 2.6$.

16 AAD 16AN perform fits to the ALAS and CMS data at $E_{cm} = 7$ and 8 TeV.

17 AAD 16K use up to 4.7 fb⁻¹ of pp collisions at $E_{cm} = 7$ TeV and up to 20.3 fb⁻¹ at $E_{cm} = 8$ TeV. The third uncertainty in the measurement is theory systematics. The quoted signal strength is given for $m_H = 125.36$ GeV.

18 AAD 15 search for $t\bar{t}H$ production with $H$ decaying to $\gamma\gamma$ in 4.5 fb⁻¹ of pp collisions at $E_{cm} = 7$ TeV and 20.3 fb⁻¹ at $E_{cm} = 8$ TeV. The quoted result on the signal strength is equivalent to an upper limit of 6.7 at 95% CL and is given for $m_H = 125.4$ GeV.

19 AAD 15BC search for $t\bar{t}H$ production with $H$ decaying to $b\bar{d}$ in 20.3 fb⁻¹ of pp collisions at $E_{cm} = 8$ TeV. The corresponding upper limit is 3.4 at 95% CL. The quoted signal strength is given for $m_H = 125$ GeV.

20 AAD 15T search for $t\bar{t}H$ production with $H$ resulting in multilepton final states (mainly from $WW^*, \tau\tau, ZZ^*$) in 20.3 fb⁻¹ of pp collisions at $E_{cm} = 8$ TeV. The quoted result on the signal strength is given for $m_H = 125$ GeV and corresponds to an upper limit of 4.7 at 95% CL. The data sample is independent from AAD 15 and AAD 15BC.

21 KHACHATRY 15AN search for $t\bar{t}H$ production with $H$ decaying to $b\bar{d}$ in 19.5 fb⁻¹ of pp collisions at $E_{cm} = 8$ TeV. The quoted result on the signal strength is equivalent to an upper limit of 4.2 at 95% CL and is given for $m_H = 125$ GeV.

22 KHACHATRY 14H search for $t\bar{t}H$ production with $H$ decaying to $b\bar{d}, \tau\tau, \gamma\gamma, WW^*, $ and $ZZ^*$, in 5.1 fb⁻¹ of pp collisions at $E_{cm} = 7$ TeV and 19.7 fb⁻¹ at $E_{cm} = 8$ TeV. The quoted signal strength is given for $m_H = 125.6$ GeV.

23 AALTONEN 13L combine all CDF results with 9.45–10.0 fb⁻¹ of $p\bar{p}$ collisions at $E_{cm} = 1.96$ TeV. The quoted signal strength is given for $m_H = 125$ GeV.

24 CHATRCHYAN 13x search for $t\bar{t}H$ production followed by $H \to b\bar{d}$, one top decaying to $\ell\nu$ and the other to either $\ell\nu$ or $q\bar{q}$ in 5.0 fb⁻¹ and 5.1 fb⁻¹ of pp collisions at $E_{cm} = 7$ and 8 TeV. A limit on cross section times branching ratio which corresponds to (4.0–8.6) times the expected Standard Model cross section is given for $m_H = 140$ GeV at 95% CL. The quoted limit is given for $m_H = 125$ GeV, where 5.2 is expected for no signal.

## H H Production Cross Section in pp Collisions

The H H production cross section relative to the SM prediction.

<table><thead><tr><th>VALUE</th><th>CL%</th><th>DOCUMENT ID</th><th>TECN</th><th>COMMENT</th></tr></thead><tbody><tr><td>&lt; 2.4</td><td>95</td><td>1 AAD</td><td>23AT ATLS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span>, b<span style="text-decoration: overline">b</span>ττ, b<span style="text-decoration: overline">b</span>γγ</td></tr></tbody></table>

<table><thead><tr><th colspan="2">• • • We do not use the following data for averages, limits, etc.</th></tr></thead><tbody><tr><td>&lt;183</td><td>95</td><td>2 AAD</td><td>23AD ATLS</td><td>13 TeV, VHH, HH → b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span></td></tr><tr><td>&lt; 5.4</td><td>95</td><td>3 AAD</td><td>23BK ATLS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span></td></tr><tr><td>&lt; 4.7</td><td>95</td><td>4 AAD</td><td>23Z ATLS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>ττ</td></tr><tr><td>&lt; 9.9</td><td>95</td><td>5 TUMASYAN</td><td>23AE CMS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span></td></tr><tr><td>&lt; 3.3</td><td>95</td><td>6,7 TUMASYAN</td><td>23D CMS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>ττ</td></tr><tr><td>&lt;124</td><td>95</td><td>6,8 TUMASYAN</td><td>23D CMS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>ττ</td></tr><tr><td>&lt; 32.4</td><td>95</td><td>9 TUMASYAN</td><td>23I CMS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>ZZ* (ZZ* → 4ℓ)</td></tr><tr><td>&lt; 21.3</td><td>95</td><td>10 TUMASYAN</td><td>23O CMS</td><td>13 TeV, WW* WW*, WW*ττ, ττττ</td></tr><tr><td>&lt; 4.2</td><td>95</td><td>11 AAD</td><td>22Y ATLS</td><td>13 TeV, γγ b<span style="text-decoration: overline">b</span></td></tr><tr><td>&lt; 3.4</td><td>95</td><td>12 CMS</td><td>22 CMS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>ZZ*, b<span style="text-decoration: overline">b</span>γγ, b<span style="text-decoration: overline">b</span>ττ, b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span>, multilepton</td></tr><tr><td>&lt; 3.9</td><td>95</td><td>13 TUMASYAN</td><td>22AN CMS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span></td></tr><tr><td>&lt; 7.7</td><td>95</td><td>14 SIRUNYAN</td><td>21K CMS</td><td>13 TeV, γγ b<span style="text-decoration: overline">b</span></td></tr><tr><td>&lt; 6.9</td><td>95</td><td>15 AAD</td><td>20C ATLS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>γγ, b<span style="text-decoration: overline">b</span>ττ, b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span>, b<span style="text-decoration: overline">b</span>WW*, WW*γγ, WW*WW*</td></tr><tr><td>&lt; 40</td><td>95</td><td>16 AAD</td><td>20E ATLS</td><td>13 TeV, HH → b<span style="text-decoration: overline">b</span>ℓνℓν</td></tr><tr><td>&lt;840</td><td>95</td><td>17 AAD</td><td>20X ATLS</td><td>13 TeV, VBF, b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span></td></tr><tr><td>&lt; 12.9</td><td>95</td><td>18 AABOUD</td><td>19A ATLS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span></td></tr><tr><td>&lt;300</td><td>95</td><td>19 AABOUD</td><td>19O ATLS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>WW*</td></tr><tr><td>&lt;160</td><td>95</td><td>20 AABOUD</td><td>19T ATLS</td><td>13 TeV, WW* WW*</td></tr><tr><td>&lt; 24</td><td>95</td><td>21 SIRUNYAN</td><td>19 CMS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span></td></tr><tr><td>&lt; 75</td><td>95</td><td>22 SIRUNYAN</td><td>19AB CMS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span></td></tr><tr><td>&lt; 22.2</td><td>95</td><td>23 SIRUNYAN</td><td>19BE CMS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>γγ, b<span style="text-decoration: overline">b</span>ττ, b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span>, b<span style="text-decoration: overline">b</span>WW*, b<span style="text-decoration: overline">b</span>ZZ*</td></tr><tr><td>&lt;179</td><td>95</td><td>24 SIRUNYAN</td><td>19H CMS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span></td></tr><tr><td>&lt;230</td><td>95</td><td>25 AABOUD</td><td>18BU ATLS</td><td>13 TeV, γγ WW*</td></tr><tr><td>&lt; 12.7</td><td>95</td><td>26 AABOUD</td><td>18CQ ATLS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>ττ</td></tr><tr><td>&lt; 22</td><td>95</td><td>27 AABOUD</td><td>18CWATLS</td><td>13 TeV, γγ b<span style="text-decoration: overline">b</span></td></tr><tr><td>&lt; 30</td><td>95</td><td>28 SIRUNYAN</td><td>18A CMS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>ττ</td></tr><tr><td>&lt; 79</td><td>95</td><td>29 SIRUNYAN</td><td>18F CMS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>ℓνℓν</td></tr><tr><td>&lt; 43</td><td>95</td><td>30 SIRUNYAN</td><td>17CN CMS</td><td>8 TeV, b<span style="text-decoration: overline">b</span>ττ, γγ b<span style="text-decoration: overline">b</span>, b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span></td></tr><tr><td>&lt;108</td><td>95</td><td>31 AABOUD</td><td>16I ATLS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span></td></tr><tr><td>&lt; 74</td><td>95</td><td>32 KHACHATRY...16BQ CMS</td><td>15CE ATLS</td><td>8 TeV, γγ b<span style="text-decoration: overline">b</span></td></tr><tr><td>&lt; 70</td><td>95</td><td>33 AAD</td><td>15CE ATLS</td><td>8 TeV, b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span>, b<span style="text-decoration: overline">b</span>ττ, γγ b<span style="text-decoration: overline">b</span>, γγ WW</td></tr></tbody></table>

1 AAD 23AT combine results from 126–139 fb⁻¹ of data at $E_{cm} = 13$ TeV for $pp \to HH \to b\bar{d}b\bar{d}$ (AAD 23BK), $b\bar{d}\tau\tau$ (AAD 23Z), and $b\bar{d}\gamma\gamma$ (AAD 22Y).

2 AAD 23AD search for non-resonant H H production in association with a vector boson using $HH \to b\bar{d}b\bar{d}$ with data of 139 fb⁻¹ at $E_{cm} = 13$ TeV. The vector boson decays leptonically ($W \to \ell\nu, Z \to \ell\ell, \nu\nu, \ell = e, \mu$).

3 AAD 23BK search for non-resonant H H production using $HH \to b\bar{d}b\bar{d}$ with data of 126 fb⁻¹ at $E_{cm} = 13$ TeV.

4 AAD 23Z search for non-resonant H H production using $HH \to b\bar{d}\tau\tau$ with data of 139 fb⁻¹ at $E_{cm} = 13$ TeV. The upper limit on the $pp \to HH$ production cross section at 95% CL is measured to be 140 fb, which corresponds to 4.7 times the SM prediction (see their Table 6).

5 TUMASYAN 23AE search for H H production using $HH \to b\bar{d}b\bar{d}$, where both $b\bar{d}$ pairs are highly boosted, with data of 138 fb⁻¹ at $E_{cm} = 13$ TeV.

6 TUMASYAN 23D search for non-resonant H H production using $HH \to b\bar{d}\tau\tau$ with data of 138 fb⁻¹ at $E_{cm} = 13$ TeV.

7 The upper limit on the $pp \to HH$ production cross section (gluon fusion and VBF) at 95% CL is measured to be 102 fb, which corresponds to 3.3 times the SM prediction (see their Table 2).

8 The upper limit on the VBF $pp \to HH$ production cross section at 95% CL is measured to be 212 fb, which corresponds to 124 times the SM prediction (see their Table 3).

9 TUMASYAN 23i search for non-resonant H H production using $HH \to b\bar{d}ZZ^*$ ($ZZ^* \to 4\ell, \ell = e, \mu$) with data of 138 fb⁻¹ at $E_{cm} = 13$ TeV.

10 TUMASYAN 23o search for non-resonant H H production using $HH \to WW*WW*, WW*ττ$, and $ττττ$ (multilepton) with data of 138 fb⁻¹ at $E_{cm} = 13$ TeV. The upper limit on the $pp \to HH$ production cross section at 95% CL is measured to be 130 fb, which corresponds to 4.2 times the SM prediction.

11 AAD 22Y search for non-resonant H H production using $HH \to \gamma\gamma b\bar{d}$ with data of 139 fb⁻¹ at $E_{cm} = 13$ TeV. The upper limit on the $pp \to HH$ production cross section at 95% CL is measured to be 130 fb, which corresponds to 4.2 times the SM prediction.

12 CMS 22 report combined results (see their Extended Data Table 2) using 138 fb⁻¹ of data at $E_{cm} = 13$ TeV. See their Fig. 5 (left) for different final states and these combination.

13 TUMASYAN 22AN search for non-resonant H H production using $HH \to b\bar{d}b\bar{d}$ with data of 138 fb⁻¹ at $E_{cm} = 13$ TeV. The upper limit on the $pp \to HH$ production cross section at 95% CL is measured to be 120 fb, which corresponds to 3.9 times the SM prediction.

14 SIRUNYAN 21k search for non-resonant H H production using $HH \to \gamma\gamma b\bar{d}$ with data of 137 fb⁻¹ at $E_{cm} = 13$ TeV. The upper limit on the $pp \to HH \to \gamma\gamma b\bar{d}$ production cross section at 95% CL is measured to be 0.67 fb, which corresponds to about 7.7 times the SM prediction.

15 AAD 20C combine results of up to 36.1 fb⁻¹ data at $E_{cm} = 13$ TeV for $pp \to HH \to b\bar{d}\gamma\gamma, b\bar{d}\tau\tau, b\bar{d}b\bar{d}, b\bar{d}WW*, WW*γγ, WW*WW* (AABOUD 18CW, AABOUD 18CQ, AABOUD 19A, AABOUD 19O, AABOUD 18BU, and AABOUD 19T).

16 AAD 20E search for non-resonant H H production using $HH \to b\bar{d}\ell\nu\ell\nu$, where one of the Higgs bosons decays to $b\bar{d}$ and the other decays to either $WW^*, ZZ^*$, or $\tau\tau$, with data of 139 fb⁻¹ at $E_{cm} = 13$ TeV. The upper limit on the $pp \to HH$ production cross section at 95% CL is measured to be 1.2 pb, which corresponds to about 40 times the SM prediction.

17 AAD 20x search for $HH \to b\bar{d}b\bar{d}$ process via VBF with data of 126 fb⁻¹ at $E_{cm} = 13$ TeV. The upper limit on the SM non-resonant H H production cross section is 1460 fb at 95% CL, which corresponds to 840 times the SM prediction.
18 AABOUD 19A search for $HH$ production using $HH \to b\bar{b}b\bar{b}$ with data of 36.1 fb⁻¹ at $E_{cm} = 13$ TeV. The upper limit on the $pp \to HH \to b\bar{b}b\bar{b}$ production cross section at 95% is measured to be 147 fb, which corresponds to about 12.9 times the SM prediction.

19 AABOUD 19O search for $HH$ production using $HH \to b\bar{b}WW^*$ with data of 36.1 fb⁻¹ at $E_{cm} = 13$ TeV. The upper limit on the $pp \to HH \to b\bar{b}WW^*$ production cross section at 95% CL is calculated to be 10 pb from the observed upper limit on the $pp \to HH \to b\bar{b}WW^*$ production cross section 2.5 pb assuming the SM branching fractions. The former corresponds to about 300 times the SM prediction.

20 AABOUD 19T search for $HH$ production using $HH \to WW^*WW^*$ with data of 36.1 fb⁻¹ at $E_{cm} = 13$ TeV. The upper limit on the $pp \to HH$ production cross section at 95% is measured to be 5.3 pb, which corresponds to about 160 times the SM prediction.

21 SIRUNYAN 19 search for $HH$ production using $HH \to \gamma\gamma b\bar{b}$ with data of 35.9 fb⁻¹ at $E_{cm} = 13$ TeV. The upper limit on the $pp \to HH \to \gamma\gamma b\bar{b}$ production cross section at 95% CL is measured to be 2.0 fb, which corresponds to about 24 times the SM prediction.

22 SIRUNYAN 19AB search for $HH$ production using $HH \to b\bar{b}b\bar{b}$, where 4 heavy flavor jets from two Higgs bosons are resolved, with data of 35.9 fb⁻¹ at $E_{cm} = 13$ TeV. The upper limit on the $pp \to HH \to b\bar{b}b\bar{b}$ production cross section at 95% is measured to be 847 fb, which corresponds to about 75 times the SM prediction.

23 SIRUNYAN 19BE combine results of 13 TeV 35.9 fb⁻¹ data: SIRUNYAN 19, SIRUNYAN 18A, SIRUNYAN 19AB, SIRUNYAN 19H, and SIRUNYAN 18F.

24 SIRUNYAN 19H search for $HH$ production using $HH \to b\bar{b}b$, where one of $b\bar{b}$ pairs is highly boosted and the other one is resolved, with data of 35.9 fb⁻¹ at $E_{cm} = 13$ TeV. The upper limit on the $pp \to HH \to b\bar{b}b\bar{b}$ production cross section at 95% is measured to be 1980 fb, which corresponds to about 179 times the SM prediction.

25 AABOUD 18BU search for $HH$ production using $\gamma\gamma WW^*$ with the final state of $\gamma\gamma\ell\ell jj$ using data of 36.1 fb⁻¹ at $E_{cm} = 13$ TeV. The upper limit on the $pp \to HH$ production cross section at 95% CL is measured to be 7.7 pb, which corresponds to about 230 times the SM prediction. The upper limit on the $pp \to HH \to \gamma\gamma WW^*$ at 95% CL is measured to be 7.5 fb (see thisier Table 6).

26 AABOUD 18CQ search for $HH$ production using $HH \to b\bar{b}\tau\tau$ with data of 36.1 fb⁻¹ at $E_{cm} = 13$ TeV. The upper limit on the $pp \to HH \to b\bar{b}\tau\tau$ production cross section at 95% is measured to be 30.9 fb, which corresponds to about 12.7 times the SM prediction.

27 AABOUD 18CW search for $HH$ production using $HH \to \gamma\gamma b\bar{b}$ with data of 36.1 fb⁻¹ at $E_{cm} = 13$ TeV. The upper limit on the $pp \to HH$ production cross section at 95% is measured to be 0.73 pb, which corresponds to about 22 times the SM prediction.

28 SIRUNYAN 18A search for $HH$ production using $HH \to b\bar{b}\tau\tau$ with data of 35.9 fb⁻¹ at $E_{cm} = 13$ TeV. The upper limit on the $gg \to HH \to b\bar{b}\tau\tau$ production cross section is measured to be 75.4 fb, which corresponds to about 30 times the SM prediction.

29 SIRUNYAN 18F search for non-resonant for $HH$ production using $HH \to b\bar{b}\ell\ell\nu\nu$, where $\ell\nu\ell\nu$ is either $WW \to \ell\nu\ell\nu$ or $ZZ \to \ell\nu\ell\nu$ ($\ell$ is e, $\mu$ or a leptonically decaying $\tau$), with data of 35.9 fb⁻¹ at $E_{cm} = 13$ TeV. The upper limit on the $HH \to b\bar{b}\ell\ell\nu\nu$ production cross section at 95% CL is measured to be 72 pb, which corresponds to about 79 times the SM prediction.

30 SIRUNYAN 17CN search for $HH$ production using $HH \to b\bar{b}\tau\tau$ with data of 18.3 fb⁻¹ at $E_{cm} = 8$ TeV. Results are then combined with the published results of the $HH \to \gamma\gamma b\bar{b}$ and $HH \to b\bar{b}b\bar{b}$, which use data of up to 19.7 fb⁻¹ at $E_{cm} = 8$ TeV. The upper limit on the $gg \to HH$ production cross section is measured to be 0.59 pb from $b\bar{b}\tau\tau$, which corresponds to about 59 times the SM prediction (gluon fusion). The combined upper limit is 0.43 pb, which is about 43 times the SM prediction. The quoted values are given for $m_H = 125$ GeV.

31 AABOUD 16i search for $HH$ production using $HH \to b\bar{b}b\bar{b}$ with data of 3.2 fb⁻¹ at $E_{cm} = 13$ TeV. The upper limit on the $pp \to HH \to b\bar{b}b\bar{b}$ production cross section is measured to be 1.22 pb. This result corresponds to about 108 times the SM prediction (gluon fusion), which is 11.3 +0.9 -1.0 fb (NNLO+NLLN) including top quark mass effects. The quoted values are given for $m_H = 125$ GeV.

32 KHACHATRYAN 16BQ search for $HH$ production using $HH \to \gamma\gamma b\bar{b}$ with data of 19.7 fb⁻¹ at $E_{cm} = 8$ TeV. The upper limit on the $gg \to HH \to \gamma\gamma b\bar{b}$ production is measured to be 1.85 pb, which corresponds to about 74 times the SM prediction and is translated into 0.1 pb for $gg \to HH$ production cross section.

33 AAD 15CE search for $HH$ production using $HH \to b\bar{b}\tau\tau$ and $HH \to \gamma\gamma WW$ with data of 20.3 fb⁻¹ at $E_{cm} = 8$ TeV. These results are then combined with the published results of the $HH \to \gamma\gamma b\bar{b}$ and $HH \to b\bar{b}b\bar{b}$, which use data of up to 20.3 fb⁻¹ at $E_{cm} = 8$ TeV. The upper limits on the $gg \to HH$ production cross section are measured to be 1.6 pb, 11.4 pb, 2.2 pb and 0.62 pb from $b\bar{b}\tau\tau, \gamma\gamma WW, \gamma\gamma b\bar{b}$ and $b\bar{b}b\bar{b}$, respectively. The combined upper limit is 0.69 pb, which corresponds to about 70 times the SM prediction. The quoted results are given for $m_H = 125.4$ GeV. See their Table 4.

## Higgs trilinear self coupling modifier $\kappa_\lambda$

Signal strength relative to the SM prediction, $\kappa_\lambda = \lambda_{H/H} / \lambda_{H/H}^{SM}$.

<table><thead><tr><th>VALUE</th><th>CL%</th><th>DOCUMENT ID</th><th>TECN</th><th>COMMENT</th></tr></thead><tbody><tr><td colspan="5">● ● We do not use the following data for averages, fits, limits, etc. ● ● ●</td></tr><tr><td>-34.4 to 33.3</td><td>95</td><td>1 AAD</td><td>23AD ATLS</td><td>13 TeV<sub>V</sub>VHH, HH → b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span></td></tr><tr><td>- 0.6 to 6.6</td><td>95</td><td>2 AAD</td><td>23AT ATLS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span>, b<span style="text-decoration: overline">b</span>ττ, b<span style="text-decoration: overline">b</span>γγ</td></tr><tr><td>- 0.4 to 6.3</td><td>95</td><td>3 AAD</td><td>23AT ATLS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span>, b<span style="text-decoration: overline">b</span>ττ, b<span style="text-decoration: overline">b</span>γγ</td></tr><tr><td>- 3.5 to 11.3</td><td>95</td><td>4 AAD</td><td>23BK ATLS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span></td></tr><tr><td>- 5.4 to 14.9</td><td>95</td><td>5 HAYRAPETY...23</td><td>CMS</td><td>13 TeV, ZZ* → 4ℓ cross sections</td></tr><tr><td>- 9.9 to 16.9</td><td>95</td><td>6 TUMASYAN</td><td>23AE CMS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span></td></tr><tr><td>- 1.7 to 8.7</td><td>95</td><td>7 TUMASYAN</td><td>23D CMS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>ττ</td></tr><tr><td>- 8.8 to 13.4</td><td>95</td><td>8 TUMASYAN</td><td>23I CMS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>ZZ* (ZZ* → 4ℓ)</td></tr><tr><td>- 6.9 to 11.1</td><td>95</td><td>9 TUMASYAN</td><td>23O CMS</td><td>13 TeV, WW* WW*, WW*ττ, τττ</td></tr><tr><td>- 1.5 to 6.7</td><td>95</td><td>10 AAD</td><td>22Y ATLS</td><td>13 TeV, γγ b<span style="text-decoration: overline">b</span></td></tr><tr><td>- 1.24 to 6.49</td><td>95</td><td>11 CMS</td><td>22 CMS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>Z*<sup>2</sup>, b<span style="text-decoration: overline">b</span>γγ, b<span style="text-decoration: overline">b</span>ττ, b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span>, multilepton</td></tr></tbody></table>

<table><tbody><tr><td>- 2.3 to 9.4</td><td>95</td><td>12 TUMASYAN</td><td>22AN CMS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span></td></tr><tr><td>- 3.3 to 8.5</td><td>95</td><td>13 SIRUNYAN</td><td>21K CMS</td><td>13 TeV, γγ b<span style="text-decoration: overline">b</span></td></tr><tr><td>- 5.0 to 12.0</td><td>95</td><td>14 AAD</td><td>20C ATLS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>γγ, b<span style="text-decoration: overline">b</span>ττ, b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span>, b<span style="text-decoration: overline">b</span>WW*, WW*γγ, WW*W*W*</td></tr><tr><td>-11 to 17</td><td>95</td><td>15 SIRUNYAN</td><td>19 CMS</td><td>13 TeV, γγ b<span style="text-decoration: overline">b</span></td></tr><tr><td>-11.8 to 18.8</td><td>95</td><td>16 SIRUNYAN</td><td>19BE CMS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>γγ b<span style="text-decoration: overline">b</span>ττ, b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span>, b<span style="text-decoration: overline">b</span>WW*, b<span style="text-decoration: overline">b</span>ZZ*</td></tr><tr><td>- 8.2 to 13.2</td><td>95</td><td>17 AABOUD</td><td>18CW ATLS</td><td>13 TeV, γγ b<span style="text-decoration: overline">b</span></td></tr><tr><td>- 17 to 22.5</td><td>95</td><td>18 SIRUNYAN</td><td>18A CMS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>ττ</td></tr><tr><td>-</td><td></td><td>19 KHACHATRY...16BQ CMS</td><td>8 TeV, γγ b<span style="text-decoration: overline">b</span></td><td></td></tr></tbody></table>

1 AAD 23AD search for non-resonant $HH$ production in association with a vector boson using $HH \to b\bar{b}b\bar{b}$ with data of 139 fb⁻¹ at $E_{cm} = 13$ TeV. The vector boson decays leptonically ($W \to \ell\nu, Z \to \ell\ell, \nu\nu, \ell = e, \mu$). The quoted $\kappa_\lambda$ is measured assuming all other Higgs boson couplings are at their SM value.

2 AAD 23AT combine results from 126-139 fb⁻¹ of data at $E_{cm} = 13$ TeV for $pp \to HH \to b\bar{b}b\bar{b}$ (AAD 23BK), $b\bar{b}\tau\tau$ (AAD 23Z), and $b\bar{b}\gamma\gamma$ (AAD 22Y). The quoted values are obtained from the profile likelihood scan as a function of $\kappa_\lambda$ as shown in their Fig. 5(a). All other coupling modifiers are assumed to have their SM values.

3 AAD 23AT combine results from 126-139 fb⁻¹ of data at $E_{cm} = 13$ TeV for $pp \to HH \to b\bar{b}b\bar{b}$ (AAD 23BK), $b\bar{b}\tau\tau$ (AAD 23Z), and $b\bar{b}\gamma\gamma$ (AAD 22Y) with single-Higgs boson analyses ($\gamma\gamma, ZZ^*$, $WW^*$, $\tau\tau$, b<span style="text-decoration: overline">b</span>, see their Table 1). The quoted values are obtained from the profile likelihood scan as a function of $\kappa_\lambda$ as shown in their Fig. 5(a), assuming that all other Higgs boson couplings are at their SM values. Results with other assumptions are shown in their Table 2.

4 AAD 23BK search for non-resonant $HH$ production using $HH \to b\bar{b}b\bar{b}$ with data of 126 fb⁻¹ at $E_{cm} = 13$ TeV. The quoted values are obtained from the one-dimensional profile likelihood scan as a function of $\kappa_\lambda$. See their Fig. 12 (a). The $\mu_{qgf+F/VBF}$ measurement for different values of $\kappa_\lambda$ constrains -3.9 < $\kappa_\lambda$ < 11.1 at 95% CL as shown in their Fig. 10 (a). $\kappa_{2V} = \kappa_V = 1$ is assumed in both cases.

5 HAYRAPETY 23 measure the cross sections for $pp \to H \to ZZ^* \to 4\ell$ ($\ell = e, \mu$) using 138 fb⁻¹ at $E_{cm} = 13$ TeV.

6 TUMASYAN 23AE search for $HH$ production using $HH \to b\bar{b}b\bar{b}$, where both $b\bar{b}$ pairs are highly boosted, with data of 138 fb⁻¹ at $E_{cm} = 13$ TeV. The quoted $\kappa_\lambda$ is measured assuming all other Higgs boson couplings are at their SM values.

7 TUMASYAN 23D search for non-resonant $HH$ production using $HH \to b\bar{b}\tau\tau$ with data of 138 fb⁻¹ at $E_{cm} = 13$ TeV. The quoted values are obtained from the upper limit on the $HH$ production cross section times the $b\bar{b}\tau\tau$ branching fraction for different values of $\kappa_\lambda$. See their Fig. 8 (left). All other coupling modifiers are assumed to be 1. In addition, two-dimensional exclusion regions as a function of the $\kappa_\lambda$ and $\kappa_\ell$ couplings, with $\kappa_{2V} = \kappa_V = 1$, are shown in their Fig. 9 (left). The one-dimensional likelihood scan as a function of $\kappa_\lambda$ is given in their Fig 10 (left), from which a 95% confidence interval is -1.77 < $\kappa_\lambda$ < 8.73 is extracted.

8 TUMASYAN 23AI search for non-resonant $HH$ production using $HH \to b\bar{b}ZZ^*$ (ZZ* → 4ℓ, $\ell = e, \mu$) with data of 138 fb⁻¹ at $E_{cm} = 13$ TeV. See their Fig. 4.

9 TUMASYAN 23O search for non-resonant $HH$ production using $HH \to WW^*WW^*$, $WW^*\tau\tau$, and $\tau\tau\tau$ (multilepton) with data of 138 fb⁻¹ at $E_{cm} = 13$ TeV. See their Fig. 10 for different final states and these combination. Limits are set on a variety of new-physics models using an effective field theory approach. See their Figs. 11, 12, and 13.

10 AAD 22Y search for non-resonant $HH$ production using $HH \to \gamma\gamma b\bar{b}$ with data of 139 fb⁻¹ at $E_{cm} = 13$ TeV. The quoted $\kappa_\lambda$ is obtained from their Fig. 12 where the theory uncertainties are not included while a negative log-likelihood scan vs. $\kappa_\lambda$ is shown in their Fig. 13 with the theory uncertainties, which provides $\kappa_\lambda = 2.8 \pm 2.0$ for the 1σ confidence interval.

11 CMS 22 report combined results (see their Extended Data Table 2) using 138 fb⁻¹ of data at $E_{cm} = 13$ TeV. See their Fig. 6 (left).

12 TUMASYAN 22AN search for non-resonant $HH$ production using $HH \to b\bar{b}b\bar{b}$ with data of 138 fb⁻¹ at $E_{cm} = 13$ TeV. The upper limit on the $pp \to HH$ production cross section at 95% CL is shown as a function of $\kappa_\lambda$ in their Fig. 2 (top).

13 SIRUNYAN 21K search for non-resonant $HH$ production using $HH \to \gamma\gamma b\bar{b}$ with data of 137 fb⁻¹ at $E_{cm} = 13$ TeV.

14 AAD 20C combine results of up to 36.1 fb⁻¹ data at $E_{cm} = 13$ TeV for $pp \to HH \to b\bar{b}\gamma\gamma, b\bar{b}\tau\tau, b\bar{b}b\bar{b}$, b<span style="text-decoration: overline">b</span>WW*, WW*γγ, WW*WW* (AADBOUD 18CW, AABOUD 18CQ, AABOUD 19A, AABOUD 19O, AABOUD 18BU, and AABOUD 19T).

15 SIRUNYAN 19 search for $HH$ production using $HH \to \gamma\gamma b\bar{b}$ with data of 19.7 fb⁻¹ at $E_{cm} = 13$ TeV. The quoted $\kappa_\lambda$ is measured assuming all other Higgs boson couplings are at their SM value.

16 SIRUNYAN 19BE combine results of 13 TeV 35.9 fb⁻¹ data: SIRUNYAN 19, SIRUNYAN 18A, SIRUNYAN 19AB, SIRUNYAN 19H, and SIRUNYAN 18F.

17 AABOUD 18CW search for $HH$ production using $HH \to \gamma\gamma b\bar{b}$ with data of 36.1 fb⁻¹ at $E_{cm} = 13$ TeV. The quoted $\kappa_\lambda$ is measured assuming all other Higgs boson couplings are at their SM value.

18 SIRUNYAN 18A search for $HH$ production using $HH \to b\bar{b}\tau\tau$ with data of 35.9 fb⁻¹ at $E_{cm} = 13$ TeV. The upper limit on production cross section times branching fraction at 95% CL is shown as a function of $\kappa_\lambda/\kappa_\ell$ in their Fig. 6 (top) where $\kappa_\ell = y_t / y_t^{SM}$ (top Yukawa coupling $y_t$).

19 KHACHATRYAN 16BQ search for $HH$ production using $HH \to \gamma\gamma b\bar{b}$ with data of 19.7 fb⁻¹ at $E_{cm} = 8$ TeV.

## Higgs-gauge boson quartic coupling modifier $\kappa_{2V}$

Signal strength relative to the SM prediction, $\kappa_{2V} = \lambda_{V/VHH} / \lambda_{V/VHH}^{SM} = V = W, Z$.

<table><thead><tr><th>VALUE</th><th>CL%</th><th>DOCUMENT ID</th><th>TECN</th><th>COMMENT</th></tr></thead><tbody><tr><td colspan="5">● ● We do not use the following data for averages, fits, limits, etc. ● ● ●</td></tr><tr><td>-8.6 to 10.0</td><td>95</td><td>1 AAD</td><td>23AD ATLS</td><td>13 TeV<sub>V</sub>VHH, HH → b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span></td></tr><tr><td>0.1 to 2.0</td><td>95</td><td>2 AAD</td><td>23AT ATLS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span>, b<span style="text-decoration: overline">b</span>ττ, b<span style="text-decoration: overline">b</span>γγ</td></tr><tr><td>0.0 to 2.1</td><td>95</td><td>3 AAD</td><td>23BK ATLS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span></td></tr></tbody></table>
<table><tr><td>0.62 to 1.41</td><td>95</td><td>4 TUMASYAN</td><td>23AE CMS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span></td></tr><tr><td>-0.4 to 2.6</td><td>95</td><td>5 TUMASYAN</td><td>23D CMS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>τ<span style="text-decoration: overline">τ</span></td></tr><tr><td>0.67 to 1.38</td><td>95</td><td>6 CMS</td><td>22 CMS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>Z<span style="text-decoration: overline">Z</span>*, b<span style="text-decoration: overline">b</span>γγ, b<span style="text-decoration: overline">b</span>τ<span style="text-decoration: overline">τ</span>, b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span>, multilepton</td></tr><tr><td>-0.1 to 2.2</td><td>95</td><td>7 TUMASYAN</td><td>22AN CMS</td><td>13 TeV, b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span></td></tr><tr><td>-1.3 to 3.5</td><td>95</td><td>8 SIRUNYAN</td><td>21K CMS</td><td>13 TeV, γγ b<span style="text-decoration: overline">b</span></td></tr><tr><td>-0.43 to 2.56</td><td>95</td><td>9 AAD</td><td>20X ATLS</td><td>13 TeV, VBF, b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span></td></tr></table>

¹AAD 23AD search for non-resonant *HH* production in association with a vector boson using *HH* → b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b*<sup>+</sup></sup> with data of 139 fb⁻¹ at E<sub>cm</sub> = 13 TeV. The vector boson decays leptonically (W → ℓν, Z → ℓν, νℓ, νℓ, ℓ = e, μ). The constraints on κ<sub>2V</sub> and κ<sub>2Z</sub> are separately measured to be -12.3 < κ<sub>2V</sub> < 13.5 and -9.9 < κ<sub>2Z</sub> < 11.3 (95% CL). The quoted κ<sub>2V</sub> (V = W, Z) is measured assuming all other Higgs boson couplings are at their SM value.

²AAD 23AT combine results from 126-139 fb⁻¹ of data at E<sub>cm</sub> = 13 TeV for pp → HH → b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span> (AAD 23BK), b<span style="text-decoration: overline">b</span>ττ (AAD 23Z), and b<span style="text-decoration: overline">b</span>γγ (AAD 22Y). The quoted values are obtained from the 95% CL VBF *HH* cross-section upper limit as a function of κ<sub>2V</sub> as shown in their Fig. 4(b). All other coupling modifiers are assumed to have their SM values.

³AAD 23BK search for non-resonant *HH* production using *HH* → b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b*<sup>+</sup></sup> with data of 126 fb⁻¹ at E<sub>cm</sub> = 13 TeV. The quoted values are obtained from the one-dimensional profile likelihood scan as a function of κ<sub>2V</sub>. See their Fig. 12 (b). The μ<sub>V</sub>B<sub>F</sub>E measurement for different values of κ<sub>2V</sub> constrains -0.03 < κ<sub>2V</sub> < 2.11 at 95% CL as shown in their Fig. 10 (b). κ<sub>λ</sub> = κ<sub>L</sub> = 1 is assumed in both cases.

⁴TUMASYAN 23AE search for *HH* production using *HH* → b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b*<sup>+</sup></sup>, where both b<span style="text-decoration: overline">b</span>b pairs are highly boosted, with data of 138 fb⁻¹ at E<sub>cm</sub> = 13 TeV. The κ<sub>2V</sub> = 0 is excluded at 6.3 σ assuming all other Higgs boson couplings are at their SM values.

⁵TUMASYAN 23d search for non-resonant *HH* production using *HH* → b<span style="text-decoration: overline">b</span>τττ with data of 138 fb⁻¹ at E<sub>cm</sub> = 13 TeV. The quoted values are obtained from the upper limits on the *HH* production cross section times the b<span style="text-decoration: overline">b</span>ττ branching fraction for different values of κ<sub>2V</sub>. See their Fig. 8 (right). All other coupling modifiers are assumed to be 1. In addition, two-dimensional exclusion regions as a function of the κ<sub>2V</sub> and κ<sub>L</sub> couplings, with κ<sub>λ</sub> = κ<sub>L</sub> = 1, are shown in their Fig. 9 (right). The one-dimensional likelihood scan as a function of κ<sub>2V</sub> is given in their Fig. 10 (right), from which a 95% confidence interval of -0.34 < κ<sub>2V</sub> < 2.49 is extracted.

⁶CMS 22 report combined results (see their Extended Data Table 2) using 138 fb⁻¹ of data at E<sub>cm</sub> = 13 TeV. See their Fig. 6 (right).

⁷TUMASYAN 22AN search for non-resonant *HH* production using *HH* → b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span>b*<sup>+</sup> with data of 138 fb⁻¹ at E<sub>cm</sub> = 13 TeV. The upper limit on the pp → HH production cross section at 95% CL is shown as a function of κ<sub>2V</sub> in their Fig. 2 (bottom).

⁸SIRUNYAN 21K search for non-resonant *HH* production using *HH* → γγ b<span style="text-decoration: overline">b</span> with data of 137 fb⁻¹ at E<sub>cm</sub> = 13 TeV.

⁹AAD 20x search for *HH* → b<span style="text-decoration: overline">b</span>b<span style="text-decoration: overline">b</span>b* process via VBF with data of 126 fb⁻¹ at E<sub>cm</sub> = 13 TeV.

tH production

<table><thead><tr><th>VALUE</th><th>DOCUMENT ID</th><th>TECN</th><th>COMMENT</th></tr></thead><tbody><tr><td>5.7±2.7±3.0</td><td>1 SIRUNYAN</td><td>21R CMS</td><td>pp, 13 TeV</td></tr><tr><td>• • •</td><td>2 AAD</td><td>20Z ATLS</td><td>pp, 13 TeV</td></tr><tr><td>• • •</td><td>3 SIRUNYAN</td><td>19BK CMS</td><td>pp, 13 TeV</td></tr><tr><td>• • •</td><td>4 KHACHATRY...16AU CMS</td><td>pp, 8 TeV</td><td></td></tr></tbody></table>

¹SIRUNYAN 21R search for *tH* in final states with electrons, muons and hadronically decaying τ leptons (*H* → WW*, ZZ*, ττ) with 137 fb⁻¹ of *pp* collision data at E<sub>cm</sub> = 13 TeV. The quoted signal strength corresponds to a significance of 1.4 standard deviations and is given for m<sub>H</sub> = 125 GeV.

²AAD 202 search for the *tH* associated production using *H* → γγ in 139 fb⁻¹ of data at E<sub>cm</sub> = 13 TeV. An upper limit on its rate is set to be 12 times the Standard Model at 95% CL (m<sub>H</sub> = 125.09 GeV).

³SIRUNYAN 19BK search for the *tH* associated production using multilepton signatures (*H* → WW*, *H* → ττ, *H* → ZZ*) and signatures with a single lepton and a b<span style="text-decoration: overline">b</span> pair (*H* → b<span style="text-decoration: overline">b</span>) using 35.9 fb⁻¹ at E<sub>cm</sub> = 13 TeV. Results are combined with *H* → γγ (SIRUNYAN 18DS). The observed 95% CL upper limit on the *tH* production cross section times *H* → WW* + ττ + ZZ* + b<span style="text-decoration: overline">b</span> + γγ branching fraction is 1.94 pb (assuming SM t<span style="text-decoration: overline">t</span>H production cross section). See their Table X and Fig. 14. The values outside the ranges of [-0.9, -0.5] and [0.1, 2.1] times the standard model top quark Yukawa coupling are excluded at 95% CL.

⁴KHACHATRYAN 16AU search for the *tH* associated production in 19.7 fb⁻¹ at E<sub>cm</sub> = 8 TeV. The 95% CL upper limits on the *tH* associated production cross section is measured to be 600-1000 fb depending on the assumed γγ branching ratios of the Higgs boson. The γγ branching ratio is varied to be a factor of 0.5-3.0 of the Standard Model Higgs boson (m<sub>H</sub> = 125 GeV). The results of the signal strengths for a negative Higgs-boson trilinear coupling are given. The results are given for m<sub>H</sub> = 125 GeV.

H Production Cross Section in pp Collisions at $\sqrt{s}$ = 13 TeV

Assumes m<sub>H</sub> = 125 GeV

<table><thead><tr><th>VALUE (pb)</th><th>DOCUMENT ID</th><th>TECN</th><th>COMMENT</th></tr></thead><tbody><tr><td>56.8±3.4 OUR AVERAGE</td><td></td><td></td><td></td></tr><tr><td>55.5±4.0</td><td>1 AAD</td><td>23C ATLS</td><td>pp, 13 TeV, γγ, ZZ* → 4ℓ (ℓ = e, μ)</td></tr><tr><td>61.1±6.0±3.7</td><td>2 SIRUNYAN</td><td>19BA CMS</td><td>pp, 13 TeV, γγ, ZZ* → 4ℓ (ℓ = e, μ)</td></tr><tr><td>• • •</td><td></td><td></td><td>• • •</td></tr><tr><td>58±4±4</td><td>3 AAD</td><td>22N ATLS</td><td>pp, 13 TeV, γγ</td></tr><tr><td>53.5±4.9±2.1</td><td>4 AAD</td><td>20BA ATLS</td><td>pp, 13 TeV, ZZ* → 4ℓ (ℓ = e, μ)</td></tr><tr><td>57.0±6.0±4.0</td><td>5 AABOUD</td><td>18CG ATLS</td><td>pp, 13 TeV, γγ, ZZ* → 4ℓ (ℓ = e, μ)</td></tr></tbody></table>

<table><tr><td>47.9+9.1<br>8.6</td><td>5 AABOUD</td><td>18CG ATLS</td><td>pp, 13 TeV, γγ</td></tr><tr><td>68+11<br>-10</td><td>5 AABOUD</td><td>18CG ATLS</td><td>pp, 13 TeV, ZZ* → 4ℓ (ℓ = e, μ)</td></tr><tr><td>69+10<br>9±5</td><td>6 AABOUD</td><td>17C ATLS</td><td>pp, 13 TeV, ZZ* → 4ℓ</td></tr></table>

¹AAD 23C combine AAD 22n and AAD 20BA, where both use 139 fb⁻¹ of *pp* collisions at E<sub>cm</sub> = 13 TeV. The Higgs production cross sections at E<sub>cm</sub> = 7 and 8 TeV are obtained to be 34+11 pb and 33.3+5.4 pb, respectively. The quoted value is given for m<sub>H</sub> = 125.09 GeV. The differential cross sections are given in their Figs. 3 and 4.

²SIRUNYAN 19BA use 35.9 fb⁻¹ of *pp* collisions at E<sub>cm</sub> = 13 TeV.

³AAD 22N use 139 fb⁻¹ of *pp* collisions at E<sub>cm</sub> = 13 TeV. The quoted value is given for m<sub>H</sub> = 125.09 GeV.

⁴AAD 20BA use 139 fb⁻¹ of *pp* collisions at E<sub>cm</sub> = 13 TeV with *H* → ZZ* → 4ℓ where ℓ = e, μ. The quoted value is given for m<sub>H</sub> = 125 GeV and assumes the Standard Model branching ratio.

⁵AABOUD 18CG use 36.1 fb⁻¹ of *pp* collisions at E<sub>cm</sub> = 13 TeV.

⁶AABOUD 17C0 use 36.1 fb⁻¹ of *pp* collisions at E<sub>cm</sub> = 13 TeV with *H* → ZZ* → 4ℓ where ℓ = e, μ for m<sub>H</sub> = 125 GeV. Differential cross sections for the Higgs boson transverse momentum, Higgs boson rapidity, and other related quantities are measured as shown in their Figs. 8 and 9.

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Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>23Y JHEP 2307 088</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>23Z JHEP 2307 040</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>HAYRAPETY...23</td><td>JHEP 2308 040</td><td>A. Hayrapetyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>HAYRAPETY...23</td><td>PR D108 072004</td><td>A. Hayrapetyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>TUMASYAN</td><td>23AD PRL 131 041801</td><td>A. Tumasyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>TUMASYAN</td><td>23AE PRL 131 041803</td><td>A. Tumasyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>TUMASYAN</td><td>23AH PRL 131 061801</td><td>A. Tumasyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>TUMASYAN</td><td>23AI PR D108 032008</td><td>A. Tumasyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>TUMASYAN</td><td>23AJ PR D108 032013</td><td>A. Tumasyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>TUMASYAN</td><td>23AU PL B846 137783</td><td>A. Tumasyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>TUMASYAN</td><td>23BA EPJ C63 933</td><td>A. Tumasyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>TUMASYAN</td><td>23C PL P842 137534</td><td>A. Tumasyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>TUMASYAN</td><td>23D PL P842 137531</td><td>A. Tumasyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>TUMASYAN</td><td>23F JHEP 2305 233</td><td>A. Tumasyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>TUMASYAN</td><td>23I JHEP 2306 130</td><td>A. Tumasyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>TUMASYAN</td><td>23O JHEP 2307 095</td><td>A. Tumasyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>TUMASYAN</td><td>23P JHEP 2307 092</td><td>A. Tumasyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>TUMASYAN</td><td>23Q JHEP 2307 091</td><td>A. Tumasyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>TUMASYAN</td><td>23W EPJ C83 667</td><td>A. Tumasyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>TUMASYAN</td><td>23Y EPJ C83 562</td><td>A. Tumasyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>AAD</td><td>22D PL B829 137066</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>22M JHEP 2206 097</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>22N JHEP 2208 027</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>22P JHEP 2208 104</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>22Q JHEP 2208 175</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>22S JHEP C82 105</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>22T JHEP 2202 622</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>22W EPJ C82 717</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>22R PR D105 092003</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>22Y PR D106 052001</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>ATLAS</td><td>22 NAT 607 52</td><td>ATLAS Collaboration</td><td>(ATLAS Collab.)</td></tr><tr><td>Also</td><td>22 NAT 612 E24 (errat.)</td><td>ATLAS Collaboration</td><td>(ATLAS Collab.)</td></tr><tr><td>CMS</td><td>22A JHEP 128 08105</td><td>CMS Collaboration</td><td>(CMS Collab.)</td></tr><tr><td>TUMASYAN</td><td>22AM NATP 18 1329</td><td>A. Tumasyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>TUMASYAN</td><td>22AN PR D129 081802</td><td>A. Tumasyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>TUMASYAN</td><td>22G PR D105 092007</td><td>A. Tumasyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>TUMASYAN</td><td>22J JHEP 2206 012</td><td>A. Tumasyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>AAD</td><td>21 PL B812 135980</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>21AB EPJ C81 178</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>21AJ EPJ C81 537</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>21F PR D103 112006</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>21G PR B819 136204</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>21I PL B819 136412</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>21M JHEP 2103 268</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>21E PR D104 052004</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>21A EPJ C81 13</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>Also</td><td>21A PR D104 052004 (errat.)</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>21B EPJ C81 3</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>21C JHEP 2101 148</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>21K JHEP 2103 257</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>21L JHEP 2103 011</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>21O JHEP 2107 027</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>21R EPJ C81 378</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>21S EPJ C81 488</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>21Z PR D104 032013</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>TUMASYAN</td><td>21D JHEP 2111 153</td><td>A. Tumasyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>AAD</td><td>20A PL B800 135069</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>20AE PR L12 221802</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>20AG PL B809 135754</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>20AQ EPJ C80 957</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>Also</td><td>20A JHEP 29 (errat.)</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>20BA EPJ C81 398 (errat.)</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>20A C80 942</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>20C PL B800 135103</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>20E PL B801 135145</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>20F PL B801 135148</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr></table>
<table><tbody><tr><td>AAD</td><td>20N</td><td>PL B805 135426</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>20X</td><td>JHEP 2007 108</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>Also</td><td></td><td>JHEP 2101 145 (errat.)</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>Also</td><td></td><td>JHEP 2105 207 (errat.)</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>20Z</td><td>PRL 125 061802</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>20AE</td><td>JHEP 2003 131</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>20AH</td><td>JHEP 2005 032</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>20AS</td><td>PRL 125 061801</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>20BK</td><td>JHEP 2011 039</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>20BL</td><td>JHEP 2012 085</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>20C</td><td>EPJ C80 75</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>20L</td><td>PL B805 135425</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>AABOUD</td><td>19A</td><td>JHEP 1901 030</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AABOUD</td><td>19AI</td><td>PL B793 499</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AABOUD</td><td>19AL</td><td>PRL 122 231801</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AABOUD</td><td>19AQ</td><td>PR D99 072001</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AABOUD</td><td>19I</td><td>PL B789 508</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AABOUD</td><td>19N</td><td>JHEP 1904 048</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AABOUD</td><td>19T</td><td>JHEP 1904 092</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AABOUD</td><td>19T</td><td>JHEP 1904 125</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AABOUD</td><td>19U</td><td>JHEP 1905 141</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>19A</td><td>PL B798 134949</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>19</td><td>JHEP 1905 093</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>19AB</td><td>JHEP 1904 112</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>19AF</td><td>JHEP 1906 093</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>19AJ</td><td>EPJ C79 94</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>19AT</td><td>JHEP C79 421</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>19AY</td><td>JHEP C79 96</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>19BA</td><td>PL B792 369</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>19BE</td><td>PRL 122 121803</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>19BK</td><td>PR D99 092005</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>19BL</td><td>PR D99 112003</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>19BO</td><td>PL B793 520</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>19BA</td><td>JHEP 1904 04811</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>19BY</td><td>JHEP D100 072007</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>19BZ</td><td>PR D100 112002</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>19CG</td><td>JHEP 1910 139</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>19E</td><td>PRL 122 021801</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>19F</td><td>JHEP 1901 040</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>19L</td><td>PL B797 183</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>19R</td><td>JHEP 1903 026</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>AABOUD</td><td>18B</td><td>PL B776 318</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AABOUD</td><td>18AC</td><td>PR D97 072003</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AABOUD</td><td>18AD</td><td>JHEP 1904 095</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AABOUD</td><td>18AU</td><td>JHEP 1807 127</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>Also</td><td></td><td>JHEP 2312 158 (errat.)</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AABK</td><td>18BL</td><td>PL B784 173</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AABOUD</td><td>18BL</td><td>PL B786 134</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AABOUD</td><td>18BM</td><td>PL B786 345</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AABOUD</td><td>18B</td><td>PL B785 348</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AABOUD</td><td>18BO</td><td>PR D98 052005</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AABP</td><td>18BP</td><td>PL B83 223</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AABOUD</td><td>18BQ</td><td>PR D98 052003</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AABOUD</td><td>18BU</td><td>EPJ C78 1007</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AABOUD</td><td>18CA</td><td>JHEP 1810 180</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AABOUD</td><td>18CG</td><td>PL B786 114</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AABOUD</td><td>18CQ</td><td>PRL 121 191801</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AABOUD</td><td>18CW</td><td>JHEP 1811 040</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AABOUD</td><td>18M</td><td>PRL 120 211802</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AABOUD</td><td>18C</td><td>PR D97 072016</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AJAI</td><td>18AM</td><td>EPJ C78 1008</td><td>R. Aajil et al.</td><td>(LHCd Collab.)</td></tr><tr><td>AALTONEN</td><td>18C</td><td>PR D98 072002</td><td>T. Aaltonen et al.</td><td>(CDF Collab.)</td></tr><tr><td>SIRUNYAN</td><td>18A</td><td>PL B778 101</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>18AE</td><td>PL B780 501</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>18BD</td><td>JHEP 1806 101</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>18E</td><td>JHEP 1806 001</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>18BQ</td><td>JHEP 1808 066</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>18BU</td><td>EPJ C78 140</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>18BV</td><td>EPJ C78 291</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>18DB</td><td>PRL 121 121801</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>18D</td><td>JHEP 1811 152</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>18DS</td><td>JHEP 1811 185</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>18E</td><td>PRL 120 071802</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>18F</td><td>JHEP 1801 054</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>18L</td><td>PRL 120 231801</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>18S</td><td>PR D97 092005</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>18Y</td><td>PL B779 283</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>AABOUD</td><td>17AW</td><td>JHEP 1710 112</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AABOUD</td><td>17BA</td><td>JHEP 1712 024</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AABOUD</td><td>17BD</td><td>EPJ C77 765</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AABOUD</td><td>17CO</td><td>JHEP 1710 132</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AABOUD</td><td>17C</td><td>PR D97 072016</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>17</td><td>EPJ C77 70</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>KHACHRYT...</td><td>17F</td><td>JHEP 1702 135</td><td>V. Khachatryan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>17AM</td><td>PL B775 1</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>17AV</td><td>JHEP 1711 047</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>SIRUNYAN</td><td>17CN</td><td>PR D96 072004</td><td>A.M. Sirunyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>AABOUD</td><td>16I</td><td>PR D94 052002</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AABOUD</td><td>16K</td><td>PRL 117 111802</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AABOUD</td><td>16X</td><td>JHEP 1611 112</td><td>M. Aaboud et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>16</td><td>PL B753 69</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>16A</td><td>PR D93 092005</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>16AH</td><td>JHEP 1601 172</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>16AL</td><td>JHEP 1605 160</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>16AN</td><td>JHEP 1608 045</td><td>G. Aad et al.</td><td>(ATLAS and CMS Collabs.)</td></tr><tr><td>AAD</td><td>16AO</td><td>JHEP 1608 104</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>16BL</td><td>EPJ C76 658</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>16C</td><td>JHEP C76 6</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>KHACHRYT...</td><td>16AB</td><td>PL B759 672</td><td>V. Khachatryan et al.</td><td>(CMS Collab.)</td></tr><tr><td>KHACHRYT...</td><td>16AR</td><td>JHEP 1604 005</td><td>V. Khachatryan et al.</td><td>(CMS Collab.)</td></tr><tr><td>KHACHRYT...</td><td>16AU</td><td>JHEP 1606 177</td><td>V. Khachatryan et al.</td><td>(CMS Collab.)</td></tr><tr><td>KHACHRYT...</td><td>16B</td><td>PL B753 341</td><td>V. Khachatryan et al.</td><td>(CMS Collab.)</td></tr><tr><td>KHACHRYT...</td><td>16C</td><td>JHEP 1609 051</td><td>V. Khachatryan et al.</td><td>(CMS Collab.)</td></tr><tr><td>KHACHRYT...</td><td>16BQ</td><td>PRL D94 052012</td><td>V. Khachatryan et al.</td><td>(CMS Collab.)</td></tr><tr><td>KHACHRYT...</td><td>16CD</td><td>PL B763 472</td><td>V. Khachatryan et al.</td><td>(CMS Collab.)</td></tr><tr><td>KHACHRYT...</td><td>16G</td><td>EPJ C76 13</td><td>V. Khachatryan et al.</td><td>(CMS Collab.)</td></tr><tr><td>AAD</td><td>15</td><td>PL B740 222</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>15A</td><td>PR D92 012006</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>15AA</td><td>JHEP 1504 117</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>15AQ</td><td>JHEP 1508 137</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>15AX</td><td>EPJ C75 231</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>15B</td><td>PRL 114 191803</td><td>G. Aad et al.</td><td>(ATLAS and CMS Collabs.)</td></tr><tr><td>AAD</td><td>15BC</td><td>EPJ C75 349</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>15BD</td><td>PL B75 337</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>15BE</td><td>EPJ C75 335</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>15CE</td><td>PR D92 092004</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>15CI</td><td>EPJ C75 476</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>Also</td><td></td><td>JHEP C76 152 (errat.)</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>15CX</td><td>JHEP 1511 206</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>15F</td><td>PR D91 012006</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>15G</td><td>JHEP 1501 069</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>15I</td><td>PRL 114 121801</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr></tbody></table>

<table><tbody><tr><td>AAD</td><td>15P</td><td>PRL 115 091801</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>15T</td><td>PL B749 519</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AALTONEN</td><td>15</td><td>PRL 114 151802</td><td>T. Aaltonen et al.</td><td>(CDF and D0 Collabs.)</td></tr><tr><td>AALTONEN</td><td>15B</td><td>PRL 114 141802</td><td>T. Aaltonen et al.</td><td>(CDF Collab.)</td></tr><tr><td>AALTONEN</td><td>15B</td><td>15AM EPJ C75 212</td><td>V. Khachatryan et al.</td><td>(CMS Collab.)</td></tr><tr><td>AALTONEN</td><td>15B</td><td>15AN EPJ C75 251</td><td>V. Khachatryan et al.</td><td>(CMS Collab.)</td></tr><tr><td>AALTONEN</td><td>15B</td><td>15BA PR D92 072010</td><td>V. Khachatryan et al.</td><td>(CMS Collab.)</td></tr><tr><td>AALTONEN</td><td>15E</td><td>15H PR B744 184</td><td>V. Khachatryan et al.</td><td>(CMS Collab.)</td></tr><tr><td>AALTONEN</td><td>15E</td><td>15Q PL B749 337</td><td>V. Khachatryan et al.</td><td>(CMS Collab.)</td></tr><tr><td>AALTONEN</td><td>15E</td><td>15Y PR D92 012004</td><td>V. Khachatryan et al.</td><td>(CMS Collab.)</td></tr><tr><td>AALTONEN</td><td>15E</td><td>15Z PR D92 032008</td><td>V. Khachatryan et al.</td><td>(CMS Collab.)</td></tr><tr><td>AAD</td><td>14AR</td><td>PL B738 234</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>14AS</td><td>PL B738 68</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>14BC</td><td>PR D90 112015</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>14BJ</td><td>JHEP 1409 112</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>14J</td><td>PL B732 8</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>14D</td><td>PRL 113 018002</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>14E</td><td>PL D90 052004</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>ABAZOV</td><td>14F</td><td>PRL 113 161802</td><td>V.M. Abazov et al.</td><td>(D0 Collab.)</td></tr><tr><td>ABATCHYAN</td><td>14AA</td><td>PR D89 092007</td><td>S. Chatrchyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>ABATCHYAN</td><td>14AI</td><td>PR D89 012003</td><td>S. Chatrchyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>ABATCHYAN</td><td>14AJ</td><td>NAPT 10 557</td><td>S. Chatrchyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>ABATCHYAN</td><td>14B</td><td>EPI C74 2980</td><td>S. Chatrchyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>ABATCHYAN</td><td>14G</td><td>JHEP 1401 096</td><td>S. Chatrchyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>ABATCHYAN</td><td>14H</td><td>JHEP 1405 104</td><td>S. Chatrchyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>ABATCHYAN</td><td>14I</td><td>PL B736 64</td><td>V. Khachatryan et al.</td><td>(CMS Collab.)</td></tr><tr><td>ABATCHYAN</td><td>14J</td><td>JHEP 1409 087</td><td>V. Khachatryan et al.</td><td>(CMS Collab.)</td></tr><tr><td>ABATCHYAN</td><td>14K</td><td>EPI C74 3076</td><td>V. Khachatryan et al.</td><td>(CMS Collab.)</td></tr><tr><td>AAD</td><td>13AJ</td><td>PL B726 120</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>13AK</td><td>PL B726 88</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>Also</td><td></td><td>PL B734 406 (errat.)</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AALTONEN</td><td>13L</td><td>PR D88 052013</td><td>T. Aaltonen et al.</td><td>(CDF Collab.)</td></tr><tr><td>AALTONEN</td><td>13M</td><td>PR D88 052014</td><td>T. Aaltonen et al.</td><td>(CDF and D0 Collabs.)</td></tr><tr><td>ABAZOV</td><td>13N</td><td>JHEP 1904 092001</td><td>V.M. Abazov et al.</td><td>(CMS Collab.)</td></tr><tr><td>ABATCHYAN</td><td>13BK</td><td>JHEP 1276 587</td><td>S. Chatrchyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>ABATCHYAN</td><td>13J</td><td>PRL 110 081803</td><td>S. Chatrchyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>ABATCHYAN</td><td>13X</td><td>JHEP 1305 145</td><td>S. Chatrchyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>ABATCHYAN</td><td>13Y</td><td>JHEP 1306 081</td><td>S. Chatrchyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>ABATCHYAN</td><td>13Z</td><td>JHEP 1307 1347</td><td>S. Heinemeier et al.</td><td>(LHC Higgs CS Working Group)</td></tr><tr><td>AAD</td><td>12AI</td><td>PL B716 1</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AAD</td><td>12DA</td><td>SCI 338 1576</td><td>G. Aad et al.</td><td>(ATLAS Collab.)</td></tr><tr><td>AALTONEN</td><td>12Q</td><td>PRL 109 111803</td><td>T. Aaltonen et al.</td><td>(CDF Collab.)</td></tr><tr><td>AALTONEN</td><td>12R</td><td>PRL 109 111804</td><td>T. Aaltonen et al.</td><td>(CDF Collab.)</td></tr><tr><td>AALTONEN</td><td>12S</td><td>PRL 109 111805</td><td>T. Aaltonen et al.</td><td>(CDF Collab.)</td></tr><tr><td>AALTONEN</td><td>12T</td><td>PRL 109 071804</td><td>T. Aaltonen et al.</td><td>(CDF and D0 Collabs.)</td></tr><tr><td>ABAZOV</td><td>12K</td><td>PL B716 285</td><td>V.M. Abazov et al.</td><td>(D0 Collab.)</td></tr><tr><td>ABAZOV</td><td>12O</td><td>PRL 109 121803</td><td>V.M. Abazov et al.</td><td>(D0 Collab.)</td></tr><tr><td>ABAZOV</td><td>12P</td><td>PRL 109 121804</td><td>V.M. Abazov et al.</td><td>(D0 Collab.)</td></tr><tr><td>ABATCHYAN</td><td>12BY</td><td>SCI 338 1569</td><td>S. Chatrchyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>ABATCHYAN</td><td>12C</td><td>PL B716 1</td><td>S. Chatrchyan et al.</td><td>(CMS Collab.)</td></tr><tr><td>DITTTMAIER</td><td>12</td><td>arXiv:1201.3084</td><td>S. Dittmaier et al.</td><td>(LHC Higgs CS Working Group)</td></tr><tr><td>DITTTMAIER</td><td>11</td><td>arXiv:1101.0593</td><td>S. Dittmaier et al.</td><td>(LHC Higgs CS Working Group)</td></tr></tbody></table>

Neutral Higgs Bosons, Searches for

CONTENTS:

Mass Limits for Neutral Higgs Bosons in Supersymmetric Models

- Mass Limits for heavy neutral Higgs bosons ($H_0^0, A^0$) in the MSSM

- Mass Limits for $H_0^0$ (Higgs Boson) in Supersymmetric Models

Mass Limits for Neutral Higgs Bosons in Extended Higgs Models

- Mass Limits in General two-Higgs-doublet Models

- Mass Limits for $H_0^0$ with Vanishing Yukawa Couplings

- Mass Limits for $H_0^0$ Decaying to Invisible Final States

- Mass Limits for Light $A^0$

- Other Mass Limits

Electroweak Constraints on the Standard Model Higgs Boson Mass

MASS LIMITS FOR NEUTRAL HIGGS BOSONS
IN SUPERSYMMETRIC MODELS

The minimal supersymmetric model has two complex doublets of Higgs bosons. The resulting physical states are two scalars ($H_0^0$ and $H_0^0$, where we define $m_{H_0^0} < m_{H_0^0}$, a pseudoscalar ($A^0$), and a charged Higgs pair ($H^\pm$). $H_0^0$ and $H_0^0$ are also called $h$ and $H$ in the literature. There are two free parameters in the Higgs sector which can be chosen to be $m_{A^0}$ and $\tan\beta = v_2/v_1$, the ratio of vacuum expectation values of the two Higgs doublets. Tree-level Higgs masses are constrained by the model to be $m_{H_0^0} \le m_Z$, $m_{H_0^0} \ge m_Z$, $m_{H_0^0} \ge m_W$, and $m_{H^\pm} \ge m_W$. However, as described in the review on "Status of Higgs Boson Physics" in this Volume these relations are violated by radiative corrections.

The observed signal at about 125 GeV, see section "H", can be interpreted as one of the neutral Higgs bosons of supersymmetric models. Unless otherwise noted, we identify the lighter scalar $H_0^0$ with the Higgs discovered at 125 GeV at the LHC (AAD 12A1, CHATHRYAN 12N).

Unless otherwise noted, the experiments in $e^+e^-$ collisions search for the processes $e^+e^- \to H_0^0 Z^0$ in the channels used for the Standard Model Higgs searches and $e^+e^- \to H_0^0 A^0$ in the final states $b\bar{b}b\bar{b}$ and $b\bar{b}\tau^-\tau^-$. Unless otherwise stated, the following results assume no invisible $H_0^0$ or $A^0$ decays. Unless otherwise noted, the results are given in the $m_{H_0^0}$ scenario, CARENA 13.

In $p\bar{p}$ and $pp$ collisions the experiments search for a variety of processes, as explicitly specified for each entry. Limits on the $A^0$ mass arise from these direct searches, as well as from the relations valid in the minimal supersymmetric model between $m_{A^0}$ and $m_{H_0^0}$. As discussed in the review on "Status of Higgs Boson Physics" in this Volume, these relations
depend, via potentially large radiative corrections, on the mass of the $t$ quark and on the supersymmetric parameters, in particular those of the stop sector. These indirect limits are weaker for larger $t$ and $t\bar{t}$ masses. To include the radiative corrections to the Higgs masses, unless otherwise stated, the listed papers use theoretical predictions incorporating two-loop corrections and beyond (SLAVICH 21), and the results are given for the $M_h^{125}$ benchmark scenario, see BAGNASCHI 19.

### Mass Limits for heavy neutral Higgs bosons ($H_2^0, A^0$) in the MSSM

The limits rely on $pp \to H_2^0/A^0 \to \tau^+\tau^-$ and assume that $H_2^0$ and $A^0$ are (sufficiently) mass degenerate. The limits depend on $\tan\beta$.

<table><thead><tr><th>VALUE (GeV)</th><th>CL%</th><th>DOCUMENT ID</th><th>TECN</th><th>COMMENT</th></tr></thead><tbody><tr><td>&gt; 835</td><td>95</td><td>1 TUMASYAN</td><td>23s CMS</td><td>tan&beta; = 10 GeV</td></tr><tr><td>&gt;1240</td><td>95</td><td>1 TUMASYAN</td><td>23s CMS</td><td>tan&beta; = 20 GeV</td></tr><tr><td>&gt;1605</td><td>95</td><td>1 TUMASYAN</td><td>23s CMS</td><td>tan&beta; = 30 GeV</td></tr><tr><td>&gt;1820</td><td>95</td><td>1 TUMASYAN</td><td>23s CMS</td><td>tan&beta; = 40 GeV</td></tr><tr><td>&gt;1950</td><td>95</td><td>1 TUMASYAN</td><td>23s CMS</td><td>tan&beta; = 50 GeV</td></tr><tr><td>&gt;2062</td><td>95</td><td>1 TUMASYAN</td><td>23s CMS</td><td>tan&beta; = 60 GeV</td></tr><tr><td>&gt;1121</td><td>95</td><td>2 AAD</td><td>20AA ATLS</td><td>tan&beta; = 10 GeV</td></tr><tr><td>&gt;1475</td><td>95</td><td>2 AAD</td><td>20AA ATLS</td><td>tan&beta; = 20 GeV</td></tr><tr><td>&gt;1677</td><td>95</td><td>2 AAD</td><td>20AA ATLS</td><td>tan&beta; = 30 GeV</td></tr><tr><td>&gt;1826</td><td>95</td><td>2 AAD</td><td>20AA ATLS</td><td>tan&beta; = 40 GeV</td></tr><tr><td>&gt;1937</td><td>95</td><td>2 AAD</td><td>20AA ATLS</td><td>tan&beta; = 50 GeV</td></tr><tr><td>&gt;2033</td><td>95</td><td>2 AAD</td><td>20AA ATLS</td><td>tan&beta; = 60 GeV</td></tr><tr><td>&gt; 377</td><td>95</td><td>10 AABOUD</td><td>18G ATLS</td><td>tan&beta; = 10 GeV</td></tr><tr><td>&gt; 863</td><td>95</td><td>10 AABOUD</td><td>18G ATLS</td><td>tan&beta; = 20 GeV</td></tr><tr><td>&gt;1157</td><td>95</td><td>10 AABOUD</td><td>18G ATLS</td><td>tan&beta; = 30 GeV</td></tr><tr><td>&gt;1328</td><td>95</td><td>10 AABOUD</td><td>18G ATLS</td><td>tan&beta; = 40 GeV</td></tr><tr><td>&gt;1483</td><td>95</td><td>10 AABOUD</td><td>18G ATLS</td><td>tan&beta; = 50 GeV</td></tr><tr><td>&gt;1613</td><td>95</td><td>10 AABOUD</td><td>18G ATLS</td><td>tan&beta; = 60 GeV</td></tr><tr><td>&gt; 389</td><td>95</td><td>11 SIRUNYAN</td><td>18CX CMS</td><td>tan&beta; = 10 GeV</td></tr><tr><td>&gt; 832</td><td>95</td><td>13 SIRUNYAN</td><td>18CX CMS</td><td>tan&beta; = 20 GeV</td></tr><tr><td>&gt;1148</td><td>95</td><td>13 SIRUNYAN</td><td>18CX CMS</td><td>tan&beta; = 30 GeV</td></tr><tr><td>&gt;1341</td><td>95</td><td>13 SIRUNYAN</td><td>18CX CMS</td><td>tan&beta; = 40 GeV</td></tr><tr><td>&gt;1496</td><td>95</td><td>13 SIRUNYAN</td><td>18CX CMS</td><td>tan&beta; = 50 GeV</td></tr><tr><td>&gt;1613</td><td>95</td><td>13 SIRUNYAN</td><td>18CX CMS</td><td>tan&beta; = 60 GeV</td></tr><tr><td>&gt; 832</td><td>95</td><td>14 AABOUD</td><td>16AA ATLS</td><td>A<sup>0</sup> &rarr; &tau;<sup>+</sup>&tau;<sup>-</sup></td></tr><tr><td>&gt; 832</td><td>95</td><td>15 KHACHATRY...16A</td><td>CMS</td><td>H<sub>1,2</sub><sup>0</sup>/A<sup>0</sup> &rarr; &mu;<sup>+</sup>&mu;<sup>-</sup></td></tr><tr><td>&gt; 832</td><td>95</td><td>16 KHACHATRY...16P</td><td>CMS</td><td>H<sub>2</sub><sup>0</sup>/A<sup>0</sup> &rarr; H<sup>0</sup>H<sup>0</sup>, A<sup>0</sup> &rarr; ZH<sup>0</sup></td></tr><tr><td>&gt; 832</td><td>95</td><td>17 KHACHATRY...15AY</td><td>CMS</td><td>pp &rarr; H<sub>1,2</sub><sup>0</sup>/A<sup>0</sup> + b + X, H<sub>1,2</sub><sup>0</sup>/A<sup>0</sup> &rarr; b&bar{b}</td></tr><tr><td>&gt; 832</td><td>95</td><td>18 AAD</td><td>14AW ATLS</td><td>pp &rarr; H<sub>1,2</sub><sup>0</sup>/A<sup>0</sup> + X, H<sub>1,2</sub><sup>0</sup>/A<sup>0</sup> &rarr; &tau;&tau;</td></tr><tr><td>&gt; 832</td><td>95</td><td>19 KHACHATRY...14M</td><td>CMS</td><td>pp &rarr; H<sub>1,2</sub><sup>0</sup>/A<sup>0</sup> + X, H<sub>1,2</sub><sup>0</sup>/A<sup>0</sup> &rarr; &tau;&tau;</td></tr><tr><td>&gt; 832</td><td>95</td><td>20 AAD</td><td>130 ATLS</td><td>pp &rarr; H<sub>1,2</sub><sup>0</sup>/A<sup>0</sup> + X, H<sub>1,2</sub><sup>0</sup>/A<sup>0</sup> &rarr; &tau;<sup>+</sup>&tau;<sup>-</sup>, &mu;<sup>+</sup>&mu;<sup>-</sup></td></tr><tr><td>&gt; 832</td><td>95</td><td>21 AAIJ</td><td>13T LHCB</td><td>pp &rarr; H<sub>1,2</sub><sup>0</sup>/A<sup>0</sup> + X, H<sub>1,2</sub><sup>0</sup>/A<sup>0</sup> &rarr; &tau;<sup>+</sup>&tau;<sup>-</sup></td></tr><tr><td>&gt; 832</td><td>95</td><td>22 CHATRCHYAN</td><td>13AG CMS</td><td>pp &rarr; H<sub>1,2</sub><sup>0</sup>/A<sup>0</sup> + b + X, H<sub>1,2</sub><sup>0</sup>/A<sup>0</sup> &rarr; b&bar{b}</td></tr><tr><td>&gt; 832</td><td>95</td><td>23 AALTONEN</td><td>12AQ TEVA</td><td>p&bar{p} &rarr; H<sub>1,2</sub><sup>0</sup>/A<sup>0</sup> + b + X, H<sub>1,2</sub><sup>0</sup>/A<sup>0</sup> &rarr; b&bar{b}</td></tr><tr><td>&gt; 832</td><td>95</td><td>24 AALTONEN</td><td>12X CDF</td><td>p&bar{p} &rarr; H<sub>1,2</sub><sup>0</sup>/A<sup>0</sup> + b + X, H<sub>1,2</sub><sup>0</sup>/A<sup>0</sup> &rarr; b&bar{b}</td></tr><tr><td>&gt; 832</td><td>95</td><td>25 ABAZOV</td><td>12G D0</td><td>p&bar{p} &rarr; H<sub>1,2</sub><sup>0</sup>/A<sup>0</sup> + X, H<sub>1,2</sub><sup>0</sup>/A<sup>0</sup> &rarr; &tau;<sup>+</sup>&tau;<sup>-</sup></td></tr><tr><td>&gt; 832</td><td>95</td><td>26 CHATRCHYAN</td><td>12K CMS</td><td>pp &rarr; H<sub>1,2</sub><sup>0</sup>/A<sup>0</sup> + X, H<sub>1,2</sub><sup>0</sup>/A<sup>0</sup> &rarr; &tau;<sup>+</sup>&tau;<sup>-</sup></td></tr><tr><td>&gt; 832</td><td>95</td><td>27 ABAZOV</td><td>11K D0</td><td>p&bar{p} &rarr; H<sub>1,2</sub><sup>0</sup>/A<sup>0</sup> + b + X, H<sub>1,2</sub><sup>0</sup>/A<sup>0</sup> &rarr; b&bar{b}</td></tr><tr><td>&gt; 832</td><td>95</td><td>28 ABAZOV</td><td>11W D0</td><td>p&bar{p} &rarr; H<sub>1,2</sub><sup>0</sup>/A<sup>0</sup> + b + X, H<sub>1,2</sub><sup>0</sup>/A<sup>0</sup> &rarr; &tau;<sup>+</sup>&tau;<sup>-</sup></td></tr></tbody></table>

<table><tbody><tr><td>&gt; 90.4</td><td>29 AALTONEN</td><td>09AR CDF</td><td>p&bar{p} &rarr; H<sub>1,2</sub><sup>0</sup>/A<sup>0</sup> + X, H<sub>1,2</sub><sup>0</sup>/A<sup>0</sup> &rarr; &tau;<sup>+</sup>&tau;<sup>-</sup></td></tr><tr><td>&gt; 93.4</td><td>30 ABDALLAH</td><td>08B DLPH</td><td>E<sub>cm</sub> &le; 209 GeV</td></tr><tr><td>&gt; 93.4</td><td>31 SCHAEL</td><td>06B LEP</td><td>E<sub>cm</sub> &le; 209 GeV</td></tr><tr><td>&gt; 93.4</td><td>32 ACOSTA</td><td>05Q CDF</td><td>p&bar{p} &rarr; H<sub>1,2</sub><sup>0</sup>/A<sup>0</sup> + X</td></tr><tr><td>&gt; 85.0</td><td>95</td><td>33,34 ABBIENDI</td><td>04M OPAL</td><td>E<sub>cm</sub><sup>mod</sup> &le; 209 GeV</td></tr><tr><td>&gt; 85.0</td><td>95</td><td>35 ABBIENDI</td><td>03G OPAL</td><td>H<sub>1</sub><sup>0</sup>/A<sup>0</sup> &rarr; A<sup>0</sup>A<sup>0</sup></td></tr><tr><td>&gt; 86.5</td><td>95</td><td>33,36 ACHARD</td><td>02H L3</td><td>E<sub>cm</sub> &le; 209 GeV, tan&beta; &gt; 0.4</td></tr><tr><td>&gt; 90.1</td><td>95</td><td>37 AKEROYD</td><td>02 RVUE</td><td></td></tr><tr><td>&gt; 90.1</td><td>95</td><td>33,38 HEISTER</td><td>02 ALEP</td><td>E<sub>cm</sub> &le; 209 GeV, tan&beta; &gt; 0.5</td></tr></tbody></table>

1. TUMASYAN 23s search for production of $H_2^0/A^0 \to \tau^+\tau^-$ by gluon fusion and b-associated production using $138 \text{ fb}^{-1}$ of $pp$ collisions at $E_{cm} = 13$ TeV. See their Fig. 13 for excluded regions in the $m_{A^0}-\tan\beta$ plane in $H_2^{125}$ and $M_{H^0}^{125}$ MSSM scenarios. In both scenarios $m_{A^0} < 350$ GeV is excluded at 95% CL.

2. AAD 20AA search for $H_2^0/A^0 \to \tau^+\tau^-$ produced by gluon fusion or b-associated production using $139 \text{ fb}^{-1}$ of $pp$ collisions at $E_{cm} = 13$ TeV. See their Fig. 2(c) for excluded region in the $M_h^{125}$ scenario of MSSM. Values of $\tan\beta > 8$ (21) are excluded for $m_{A^0} = 1.0$ (1.5) TeV at 95% CL.

3. AAD 20 combine measurements on $H^0$ production and decay using data taken in years 2015–2017 (up to 79.8 fb$^{-1}$) of $pp$ collisions at $E_{cm} = 13$ TeV. See their Fig. 19 for excluded region in the hMSSM parameter space.

4. AAD 20C combine searches for a scalar resonance decaying to $H^0 H^0$ in 36.1 fb$^{-1}$ of $pp$ collisions at $E_{cm} = 13$ TeV from AABOUD 19A, AABOUD 19o, AABOUD 18cQ, AABOUD 19tA, AABOUD 18cw, and AABOUD 18bu. See their Fig. 7(b) for the excluded region in the hMSSM parameter space.

5. AAD 20L search for b-associated production of $H_2^0$ decaying to $b\bar{b}$ in 27.8 fb$^{-1}$ of $pp$ collisions at $E_{cm} = 13$ TeV. See their Fig. 9 for excluded regions in hMSSM, $m_h^{\text{mod+}}$ and $m_h^{\text{mod-}}$ scenarios of MSSM.

6. SIRUNYAN 20AC search for gluon-fusion and b-associated production of $A^0$ decaying to $ZH^0$ in 35.9 fb$^{-1}$ of $pp$ collisions at $E_{cm} = 13$ TeV. See their Fig. 6 for excluded regions in the $M_{H^0}^{125}$ and hMSSM scenarios of the MSSM.

7. SIRUNYAN 20AF search for $H_2^0/A^0 \to t\bar{t}$ with one or two charged leptons in the final state using kinematic variables in 35.9 fb$^{-1}$ of $pp$ collisions at $E_{cm} = 13$ TeV. See their Fig. 8 for excluded region in the hMSSM scenario of MSSM. Values of $\tan\beta$ below 1.0–1.5 are excluded for $m_{A^0} = 0.4–0.75$ TeV at 95% CL.

8. SIRUNYAN 20Y search for gluon-fusion and vector-boson-fusion production of $H_2^0$ decaying to $W^+W^-$ in the final states $\ell\nu\ell\nu$ and $\ell\nu q\bar{q}$ in 35.9 fb$^{-1}$ of $pp$ collisions at $E_{cm} = 13$ TeV. See their Figs. 8 and 9 for excluded regions in various MSSM scenarios.

9. SIRUNYAN 19CR search for production of $H_2^0/A^0$ in gluon fusion and in association with a $b\bar{b}$ pair, decaying to $\mu^+\mu^-$ in 35.9 fb$^{-1}$ of $pp$ collisions at $E_{cm} = 13$ TeV. See their Fig. 5 for the excluded region in the MSSM parameter space in the $m_h^{\text{mod+}}$ and hMSSM scenarios.

10. AABOUD 18G search for production of $H_2^0/A^0 \to \tau^+\tau^-$ by gluon fusion and b-associated production in 36.1 fb$^{-1}$ of $pp$ collisions at $E_{cm} = 13$ TeV. See their Fig. 10 for excluded regions in the $m_{A^0}-\tan\beta$ plane in several MSSM scenarios.

11. SIRUNYAN 18A search for production of a scalar resonance decaying to $H^0 H^0 \to b\bar{b}\tau^+\tau^-$ in 35.9 fb$^{-1}$ of $pp$ collisions at $E_{cm} = 13$ TeV. See their Fig. 5 (lower) for excluded regions in the $m_{A^0}-\tan\beta$ plane in the hMSSM scenario.

12. SIRUNYAN 18BP search for production of $H_2^0/A^0 \to b\bar{b}$ by b-associated production in 35.7 fb$^{-1}$ of $pp$ collisions at $E_{cm} = 13$ TeV. See their Fig. 6 for the limits on cross section times branching ratio for $m_{H_2^0}, m_{A^0} = 0.3–1.3$ TeV, and Fig. 7 for excluded regions in the $m_{A^0}-\tan(\beta)$ plane in several MSSM scenarios.

13. SIRUNYAN 18CX search for production of $H_2^0/A^0 \to \tau^+\tau^-$ by gluon fusion and b-associated production in 35.9 fb$^{-1}$ of $pp$ collisions at $E_{cm} = 13$ TeV. See their Fig. 9 for excluded regions in the $m_{A^0}-\tan(\beta)$ plane in several MSSM scenarios.

14. AABOUD 16AA search for production of a Higgs boson in gluon fusion and in association with a $b\bar{b}$ pair followed by the decay $A^0 \to \tau^+\tau^-$ in 3.2 fb$^{-1}$ of $pp$ collisions at $E_{cm} = 13$ TeV. See their Fig. 5(a, b) for limits on cross section times branching ratio for $m_{A^0} = 200–1200$ GeV, and Fig. 5(c, d) for the excluded region in the MSSM parameter space in the $m_h^{\text{mod+}}$ and hMSSM scenarios.

15. KHACHATRYAN 16A search for production of a Higgs boson in gluon fusion and in association with a $b\bar{b}$ pair followed by the decay $H_2^0/A^0 \to \mu^+\mu^-$ in 5.1 fb$^{-1}$ of $pp$ collisions at $E_{cm} = 7$ TeV and 19.3 fb$^{-1}$ at $E_{cm} = 8$ TeV. See their Fig. 7 for the excluded region in the MSSM parameter space in the $m_h^{\text{mod+}}$ benchmark scenario and Fig. 9 for limits on cross section times branching ratio.

16. KHACHATRYAN 16P search for gluon fusion production of an $H_2^0$ decaying to $H^0 H^0 \to b\bar{b}\tau^+\tau^-$ and an $A^0$ decaying to $ZH^0 \to \ell^+\ell^-\tau^+\tau^-$ in 19.7 fb$^{-1}$ of $pp$ collisions at $E_{cm} = 8$ TeV. See their Fig. 12 for excluded region in the $\tan\beta - \cos(\beta - \alpha)$ plane for $m_{H_2^0} = m_{A^0} = 300$ GeV.

17. KHACHATRYAN 15AY search for production of a Higgs boson in association with a $b$ quark in the decay $H_2^0/A^0 \to b\bar{b}$ in 19.7 fb$^{-1}$ of $pp$ collisions at $E_{cm} = 8$ TeV and combine with CHATRCHYAN 13AG 7 TeV data. See their Figs. 6 for the limits on cross section times branching ratio for $m_{A^0} = 100–900$ GeV and GeV. 7–9 for the excluded region in the MSSM parameter space in various benchmark scenarios.

18. AAD 14AW search for production of a Higgs boson followed by the decay $H_2^0/A^0 \to \tau^+\tau^-$ in 19.5–20.3 fb$^{-1}$ of $pp$ collisions at $E_{cm} = 8$ TeV. See their Fig. 11 for the limits on cross section times branching ratio and their Figs. 9 and 10 for the excluded region in the MSSM parameter space. For $m_{A^0} = 140$ GeV, the region $\tan\beta > 5.4$ is excluded at 95% CL in the $m_h^{\text{max}}$ scenario.