adsabs/AstroCLIMB huggingface dataset:
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: The velocity-integrated maps of deuterated and 13C isotopic molecular lines for BGPS 3110. The integrated-velocity range, shown at the bottom-right corner, is derived after combining the Gaussian-fitting line widths for each deuterated molecular line and 13C isotopologue. For H13CO+, HN13C, DNC, H13CN, DCN, N2D+ J = 1−0, and DCN J = 2−1, the contours start from 3σ in steps of 1σ, with σ = 0.21, 0.25, 0.12, 0.24, 0.12, 0.08, and 0.19 K km s−1, respectively. The crosses represent peaks in the velocity-integrated maps of different molecular lines and the red star represents the 1.1 mm continuum peak obtained from Svoboda et al. (2016). The beam sizes for H13CN, DCN J = 1−0 and DCN J = 2−1 of ∼28″, ∼34″, and ∼16″ are shown as red circles at the bottom-left corners in their integrated-intensity maps. The averaged spectra for column density estimation are derived in the regions enclosed by blue squares.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: The velocity-integrated maps of deuterated and 13C isotopic molecular lines for BGPS 3134. The integrated-velocity range, shown at the bottom-right corner, is derived after combining the Gaussian-fitting line widths for each deuterated molecular line and 13C isotopologue. For H13CO+, DCO+, HN13C, DNC, H13CN, DCN, N2D+ J = 1−0, DCO+, DNC, DCN, and N2D+ J = 2−1, the contours start from 3σ in steps of 1σ, with σ = 0.15, 0.10, 0.15, 0.08, 0.16, 0.08, 0.14, 0.21, 0.16, and 0.32 K km s−1, respectively. The crosses represent peaks in the velocity-integrated maps of different molecular lines and the red star represents the 1.1 mm continuum peak obtained from Svoboda et al. (2016). The beam sizes for H13CO+, DCO+ J = 1−0, and DCO+ J = 2−1 of ∼28″, ∼34″, and ∼16″ are shown as red circles at the bottom-left corners in their integrated-intensity maps. The averaged spectra for column density estimation are derived in the regions enclosed by blue squares.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: Averaged DCO+, H13CO+, DNC, HN13C, DCN, and H13CN J = 1−0 spectra of the 11 OTF sources. These spectra are averaged from the region enclosed by blue squares in Figures 10−20. These regions represent the peak regions of the deuterated molecular lines. The Gaussian-fitting result for each spectrum is shown in magenta. The x-axis is velocity in kilometers per second, and the y-axis is T mb in kelvin.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: Velocity field of deuterated molecules for BGPS 2986. The crosses represent integrated-intensity peaks of different lines and 1.1 mm continuum peak.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: The velocity-integrated maps of deuterated and 13C isotopic molecular lines for BGPS 2693. The integrated-velocity range, shown at the bottom-right corner, is derived after combining the Gaussian-fitting line widths for each deuterated molecular line and 13C isotopologue pair. For H13CO+, DCO+, HN13C, and DNC J = 1−0, the contours start from 3σ in steps of 1σ, with σ = 0.19, 0.12, 0.15, and 0.14 K km s−1, respectively. The crosses represent peaks in the velocity-integrated maps of different molecular lines and the red star represents the 1.1 mm continuum peak obtained from Svoboda et al. (2016). The beam sizes for H13CO+ and DCO+ J = 1−0 of ∼28″ and ∼34″ are shown as red circles at the bottom-left corners in their integrated-intensity maps. The averaged spectra for column density estimation are derived in the regions enclosed by blue squares.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: The velocity-integrated maps of deuterated and 13C isotopic molecular lines for BGPS 2986. The integrated-velocity range, shown at the bottom-right corner, is derived after combining the Gaussian-fitting line widths for each deuterated molecular line and 13C isotopologue. For H13CO+, DCO+, DNC J = 1−0, and DCO+ J = 2−1, the contours start from 6σ in steps of 2σ, with σ = 0.11, 0.08, 0.08, and 0.08 K km s−1, respectively. For HN13C, H13CN, DCN, N2D+ J = 1−0, DNC, DCN, and N2D+ J = 2−1, the contours start from 3σ in steps of 1σ, with σ = 0.14, 0.13, 0.09, 0.06, 0.28, 0.09, and 0.23 K km s−1, respectively. The crosses represent peaks in the velocity-integrated maps of different molecular lines and the red star represents the 1.1 mm continuum peak obtained from Svoboda et al. (2016). The beam sizes for H13CO+, DCO+ J = 1−0, and DCO+ J = 2−1 of ∼28″, ∼34″, and ∼16″ are shown as red circles at the bottom-left corners in their integrated-intensity maps. The averaged spectra for column density estimation are derived in the regions enclosed by blue squares.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: The velocity-integrated maps of deuterated and 13C isotopic molecular lines for BGPS 2984. The integrated-velocity range, shown at the bottom-right corner, is derived after combining the Gaussian-fitting line widths for each deuterated molecular line and 13C isotopologue pair. For H13CO+, DCO+, DNC J = 1−0, and DCO+ J = 2−1, the contours start from 3σ in steps of 2σ, with σ = 0.12, 0.09, 0.07, and 0.09 K km s−1, respectively. For HN13C, H13CN, DCN, N2D+ J = 1−0, and DNC J = 2−1, the contours start from 3σ in steps of 1σ, with σ = 0.11, 0.12, 0.09, 0.08, and 0.25 K km s−1, respectively. The crosses represent peaks in the velocity-integrated maps of different molecular lines and the red star represents the 1.1 mm continuum peak obtained from Svoboda et al. (2016). The beam sizes for H13CO+, DCO+ J = 1−0, and DCO+ J = 2−1 of ∼28″, ∼34″, and ∼16″ are shown as red circles at the bottom-left corners in their integrated-intensity maps. The averaged spectra for column density estimation are derived in the regions enclosed by blue squares.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: The velocity-integrated maps of deuterated and 13C isotopic molecular lines for BGPS 2945. The integrated-velocity range, shown at the bottom-right corner, is derived after combining the Gaussian-fitting line widths for each deuterated molecular line and 13C isotopologue pair. For H13CO+, DCO+, and DNC J = 1−0, the contours start from 3σ in steps of 2σ, with σ = 0.14, 0.09, and 0.08 K km s−1, respectively. For HN13C, H13CN, DCN, N2D+ J = 1−0, and DNC J = 2−1, the contours start from 3σ in steps of 1σ, with σ = 0.15, 0.13, 0.10, 0.09, and 0.32 K km s−1, respectively. The crosses represent peaks in the velocity-integrated maps of different molecular lines and the red star represents the 1.1 mm continuum peak obtained from Svoboda et al. (2016). The beam sizes for H13CO+, DCO+ J = 1−0, and DNC J = 2−1 of ∼28″, ∼34″, and ∼16″ are shown as red circles at the bottom-left corners in their integrated-intensity maps. The averaged spectra for column density estimation are derived in the regions enclosed by blue squares.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: The velocity-integrated maps of deuterated and 13C isotopic molecular lines for BGPS 2940. The integrated-velocity range, shown at the bottom-right corner, is derived after combining the Gaussian-fitting line widths for each deuterated molecular line and 13C isotopologue pair. For H13CO+ and DCO+ J = 1−0, the contours start from 3σ in steps of 2σ, with σ = 0.19 and 0.11 K km s−1, respectively. For HN13C, DNC, H13CN, DCN, and N2D+ J = 1−0, the contours start from 3σ in steps of 1σ, with σ = 0.18, 0.19, 0.17, 0.09, and 0.08 K km s−1, respectively. The crosses represent peaks in the velocity-integrated maps of different molecular lines and the red star represents the 1.1 mm continuum peak obtained from Svoboda et al. (2016). The beam sizes for H13CO+ and DCO+ J = 1−0 of ∼28″ and ∼34″ are shown as red circles at the bottom-left corners in their integrated-intensity maps. The averaged spectra for column density estimation are derived in the regions enclosed by blue squares.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: The velocity-integrated maps of deuterated and 13C isotopic molecular lines for BGPS 2931. The integrated-velocity range, shown at the bottom-right corner, is derived after combining the Gaussian-fitting line widths for each deuterated molecular line and 13C isotopologue pair. For H13CO+, DCO+, HN13C, DNC, H13CN, DCN, and N2D+ J = 1−0, the contours start from 3σ in steps of 1σ, with σ = 0 .21, 0.18, 0.16, 0.11, 0.16, 0.12, and 0.10 K km s−1, respectively. The crosses represent peaks in the velocity-integrated maps of different molecular lines and the red star represents the 1.1 mm continuum peak obtained from Svoboda et al. (2016). The beam sizes for H13CO+ and DCO+ J = 1−0 of ∼28″ and ∼34″ are shown as red circles at the bottom-left corners in their integrated-intensity maps. The averaged spectra for column density estimation are derived in the regions enclosed by blue squares.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: The velocity-integrated maps of deuterated and 13C isotopic molecular lines for BGPS 3018. The integrated-velocity range, shown at the bottom-right corner, is derived after combining the Gaussian-fitting line widths for each deuterated molecular line and 13C isotopologue. For H13CO+, DCO+, HN13C, DNC, H13CN, and DCN J = 1−0, the contours start from 3σ in steps of 1σ, with σ = 0.18, 0.12, 0.19, 0.11, 0.19, and 0.10 K km s−1, respectively. The crosses represent peaks in the velocity-integrated maps of different molecular lines and the red star represents the 1.1 mm continuum peak obtained from Svoboda et al. (2016). The beam sizes for H13CO+ and DCO+ J = 1−0 of ∼28″ and ∼34″ are shown as red circles at the bottom-left corners in their integrated-intensity maps. The averaged spectra for column density estimation are derived in the regions enclosed by blue squares.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: Line profiles of the 91 H2CO(1(0,1) −0(0,0)) detected clumps. The Gaussian-fitting result for each spectrum is shown in magenta. The blue dashed vertical line represents the LSR velocity of NH3 for each MSCC derived from Svoboda et al. (2016). The x-axis is velocity in kilometers per second, and the y-axis is T mb in kelvin.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: Left: The H44α (black contours and gray-scale maps) vs. deuterated line (colored contours) distributions for BGPS 3110 and BGPS 3125. Right: The H44α spectra for BGPS 3110 and BGPS 3125. The velocity range that we derived the velocity-integrated intensity maps are shown in the spectra with blue lines. The spectra are averaged from the regions enclosed by blue lines in the velocity-integrated intensity maps. The black contours start from 3σ in steps of 1σ, with σ = 1.5 and 0.2 K km s−1 for BGPS 3110 and BGPS 3125. The colored contours of the deuterated lines are the same as those in Figures 17 and 18.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: Line-width distribution of deuterated molecules for BGPS 3134.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: Left: D frac(HNC) vs. D frac(HCN). Middle: D frac(HNC) vs. D frac(HCO+). Right: D frac(HCN) vs. D frac(HCO+). The arrows show the upper limits of the estimated deuteration fractions. The green dashed lines represent x = y.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: HCO+, HCN, HNC, and N2H+ J = 1−0 integrated maps of BGPS 2931. The integrated-velocity range is shown at the bottom-right corner. For HCO+ and HNC J = 1−0, the contours start from 15σ in steps of 3σ, with σ = 0.20 and 0.15 K km s−1. For HCN and N2H+ J = 1−0, the contours start from 10σ in steps of 2σ, with σ = 0.17 and 0.17 K km s−1.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: HCO+, HCN, HNC, and N2H+ J = 1−0 integrated maps of BGPS 2693. The integrated-velocity range is shown at the bottom-right corner. For HCO+, HCN, HNC, and N2H+ J = 1−0, the contours start from 5σ in steps of 2σ, with σ = 0.20, 0.15, 0.16, and 0.17 K km s−1.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: Line-width distribution of deuterated molecules for BGPS 2986. The crosses represent integrated-intensity peaks of different lines and the 1.1 mm continuum peak.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: Line-width distribution of deuterated molecules for BGPS 3018.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: Line-width distribution of deuterated molecules for BGPS 4402.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: Line-width distribution of deuterated molecules for BGPS 2931.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: Line-width distribution of deuterated molecules for BGPS 3125.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: Line-width distribution of deuterated molecules for BGPS 2940.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: Line-width distribution of deuterated molecules for BGPS 2984.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: Line-width distribution of deuterated molecules for BGPS 2945.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: Line-width distribution of deuterated molecules for BGPS 3110.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: HCO+, HCN, HNC, and N2H+ J = 1−0 integrated maps of BGPS 2940. The integrated-velocity range is shown at the bottom-right corner. For HCO+, HCN, and HNC J = 1−0, the contours start from 20σ in steps of 5σ, with σ = 0.25, 0.17, and 0.21 K km s−1. For N2H+ J = 1−0, the contours start from 5σ in steps of 3σ, with σ = 0.24 K km s−1.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: HCO+, HCN, HNC, and N2H+ J = 1−0 integrated maps of BGPS 2945. The integrated-velocity range is shown at the bottom-right corner. For HCO+, HCN, and HNC J = 1−0, the contours start from 15σ in steps of 3σ, with σ = 0.25, 0.18, and 0.21 K km s−1. For N2H+ J = 1−0, the contours start from 5σ in steps of 2σ, with σ = 0.17 K km s−1.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: HCO+, HCN, HNC, and N2H+ J = 1−0 integrated maps of BGPS 3125. The integrated-velocity range is shown at the bottom-right corner. For HCO+, HNC, and N2H+ J = 1−0, the contours start from 15σ in steps of 3σ, with σ = 0.24, 0.26, and 0.24 K km s−1. For HCN J = 1−0, the contours start from 30σ in steps of 10σ, with σ = 0.19 K km s−1.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: HCO+, HCN, HNC, and N2H+ J = 1−0 integrated maps of BGPS 4402. The integrated-velocity range is shown at the bottom-right corner. For HCO+, HCN, HNC, and N2H+ J = 1−0, the contours start from 6σ in steps of 2σ, with σ = 0.27, 0.19, 0.21, and 0.19 K km s−1.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: HCO+, HCN, HNC, and N2H+ J = 1−0 integrated maps of BGPS 3134. The integrated-velocity range is shown at the bottom-right corner. For HCO+, HCN, HNC, and N2H+ J = 1−0, the contours start from 30σ in steps of 10σ, with σ = 0.17, 0.18, 0.15, and 0.15 K km s−1.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: HCO+, HCN, HNC, and N2H+ J = 1−0 integrated maps of BGPS 3110. The integrated-velocity range is shown at the bottom-right corner. For HCO+, HCN, HNC, and N2H+ J = 1−0, the contours start from 30σ in steps of 10σ, with σ = 0.33, 0.28, 0.27, and 0.26 K km s−1.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: HCO+, HCN, HNC, and N2H+ J = 1−0 integrated maps of BGPS 3018. The integrated-velocity range is shown at the bottom-right corner. For HCO+, HCN, HNC, and N2H+ J = 1−0, the contours start from 6σ in steps of 2σ, with σ = 0.20, 0.19, 0.18, and 0.22 K km s−1.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: HCO+, HCN, HNC, and N2H+ J = 1−0 integrated maps of BGPS 2986. The integrated-velocity range is shown at the bottom-right corner. For HCO+, HCN, HNC, and N2H+ J = 1−0, the contours start from 12σ in steps of 3σ, with σ = 0.12, 0.12, 0.12, and 0.15 K km s−1.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: HCO+, HCN, HNC, and N2H+ J = 1−0 integrated maps of BGPS 2984. The integrated-velocity range is shown at the bottom-right corner. For HCO+, HCN, HNC, and N2H+ J = 1−0, the contours start from 8σ in steps of 2σ, with σ = 0.18, 0.17, 0.14, and 0.15 K km s−1.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: Line profiles of the 10 DCN J = 2−1 detected clumps. The Gaussian-fitting result for each spectrum is shown in magenta. The blue dashed vertical line represents the LSR velocity of NH3 for each SCC derived from Svoboda et al. (2016). The x-axis is velocity in kilometers per second, and the y-axis is T mb in kelvin.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: The integrated intensities of DCO+ (left), DCN (middle), and N2D+ (right) J = 1−0 in relation to DNC J = 1−0. The colored dashed lines represent the fitting results. The black dashed lines represent y = x.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: 1.1 mm intensities vs. masses (left panel) and kinetic temperatures obtained from NH3 observations vs. distances (right panel) for SCCs with and without deuterated molecule detections. The dashed lines represent the median values.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: Line profiles of the 7 N2D+ J = 1−0 detected clumps. The Gaussian-fitting result for each spectrum is shown in magenta. The blue dashed vertical line represents the LSR velocity of NH3 for each SCC derived from Svoboda et al. (2016). The x-axis is velocity in kilometers per second, and the y-axis is T mb in kelvin.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: Line profiles of the 20 DCO+ J = 2−1 detected clumps. The Gaussian-fitting result for each spectrum is shown in magenta. The blue dashed vertical line represents the LSR velocity of NH3 for each SCC derived from Svoboda et al. (2016). The x-axis is velocity in kilometers per second, and the y-axis is T mb in kelvin.
Paper: Molecular Deuterations in Massive Starless Clump Candidates
Authors: Kai Yang, Junzhi Wang, Keping Qiu, Tianwei Zhang
Figure caption: Line-width distribution of deuterated molecules for BGPS 2693.
Paper: Cross Correlation between the Thermal Sunyaev–Zeldovich Effect and the Integrated Sachs–Wolfe Effect
Authors: Ayodeji Ibitoye, Wei-Ming Dai, Yin-Zhe Ma, Patricio Vielva, Denis Tramonte, Amare Abebe, Aroonkumar Beesham, Xuelei Chen
Figure caption: A comparison of the early- and late-time measurements of the Hubble constant. These studies include Planck data (Planck Collaboration et al. 2020), DES Year 1, BAO, and BBN data (DES+BAO+BBN; Abbott et al. 2018), SPT-SZ and BAO data (SPT-SZ+BAO; Addison et al. 2018), CCHP data (Freedman et al. 2019), lensed quasar data (H0LiCOW; Wong et al. 2020), the SN, CC, BAO, and H0LiCOW lenses sample (SN+CC+BAO+H0LiCOW; Bonilla et al. 2021), and Hubble Space Telescope observations (SH0ES; Riess et al. 2019).
Paper: Cross Correlation between the Thermal Sunyaev–Zeldovich Effect and the Integrated Sachs–Wolfe Effect
Authors: Ayodeji Ibitoye, Wei-Ming Dai, Yin-Zhe Ma, Patricio Vielva, Denis Tramonte, Amare Abebe, Aroonkumar Beesham, Xuelei Chen
Figure caption: Comparison of the estimate on baryon temperature from two-point correlation studies (FRBs×Planck tSZ; Muñoz & Loeb 2018), stacking analyses (Planck tSZ-LRGs DR12—Tanimura et al. 2019; Planck tSZ-CMASS—de Graaff et al. 2019; Planck tSZ–Planck lensing—Tanimura et al. 2020), and X-ray observations (X-Ray ROSAT; Wang 1993). Notice that the temperature values derived from different measurements correspond to cosmic structures on different scales; hence, this plot is only intended to provide a comparison between their orders of magnitude, which are found to be in broad agreement.
Paper: Cross Correlation between the Thermal Sunyaev–Zeldovich Effect and the Integrated Sachs–Wolfe Effect
Authors: Ayodeji Ibitoye, Wei-Ming Dai, Yin-Zhe Ma, Patricio Vielva, Denis Tramonte, Amare Abebe, Aroonkumar Beesham, Xuelei Chen
Figure caption: Posterior distributions from MCMC using both EMCEE and ULTRANEST with the full covariance matrix for the six free parameters in our model. The figures show the joint constraints for all parameter pairs and the marginalized distributions for each parameter along the table diagonal. Both results are compatible within uncertainties, and they have no obvious discrepancies. Therefore, for this analysis, we present the results obtained using the EMCEE package, a more versatile and widely employed MCMC engine.
Paper: Cross Correlation between the Thermal Sunyaev–Zeldovich Effect and the Integrated Sachs–Wolfe Effect
Authors: Ayodeji Ibitoye, Wei-Ming Dai, Yin-Zhe Ma, Patricio Vielva, Denis Tramonte, Amare Abebe, Aroonkumar Beesham, Xuelei Chen
Figure caption: Base ΛCDM model 68% and 95% posterior distribution constraint contours on the matter density parameter Ωm and on the structure amplitude parameter S 8.