<figure><img src="image_17.png" /><figcaption>**Fig. 16.** TESS observations of KIC 7955301 from 2019 to 2022. **Top panel:** time series processed with the software package FITSH (Pál 2012). **Bottom panel:** power spectral density of the times series for Sector 14 only. The vertical dot-dashed red line indicates $v_{max}$ and the vertical dashed blue line indicates Kepler's Nyquist frequency.</figcaption></figure>

ARCES at APO, we were able to first classify the system as an SB1 and monitor the RV shift of the RG component along its orbit. Then, with the dynamical model solution, we could disentangle and co-add the optical spectra to derive the atmospheric parameters of the three components, even though the parameters of the inner binary have a low S/N. By fixing the RG surface gravity to that found by the complete LIGHTCURVEFACTORY model, we were able to determine the RG temperature and metallicity at $T_A = 4720 \pm 105$ K and $[M/H] = -0.01 \pm 0.12$ (Table 2).

We computed the asteroseismic mass of the RG in three different manners. The first and most basic one, which consisted in applying the asteroseismic scaling laws tuned for RG stars by Mosser et al. (2013) from the values of $v_{max}$, $\Delta v$, and $T_A$, led to $M_{A,SL} = 1.27 \pm 0.05 M_{\odot}$. The second made use of the (PARAM) approach that fits the global asteroseismic parameters, including $\Delta\Pi_1$, and by including the metallicity on a grid of

stellar-evolution models. The mass appears to be exactly the same as with the asteroseismic scaling relation: $M_{A,PARAM} = 1.27 \pm 0.05 M_{\odot}$. Finally, the most sophisticated approach based on fitting individual oscillation frequencies led to a mass of $M_A = 1.281_{-0.004}^{+0.015} M_{\odot}$.

The RG mass that we derived from the purely dynamical modeling – independent from both asteroseismology and stellar evolution models – is $1.30_{-0.02}^{+0.03} M_{\odot}$. The uncertainty is thus about 2%, which is better than what can be obtained from asteroseismology or stellar evolution models based on atmospheric parameters, luminosity, and parallaxes. This type of system, a solar-like oscillator in an SB1 hierarchical triple system, should definitely be considered for helping to calibrate the asteroseismic masses. About ten of them are available in Gaulme et al. (2013) and Gaulme & Guzik (2019), even though none of them exhibit such clear ETVs, which means that a 2% accuracy on mass may not be achievable with those.

It is interesting to notice that in this system, the asteroseismic mass matches the dynamical one, contrary to what has been observed for most RGs in EBs (Gaulme et al. 2016; Brogaard et al. 2018; Benbakoura et al. 2021), where asteroseismology appeared to overestimate masses by about 15% on average. This puzzling fact may just be a case where the sample of RG oscillators with accurate independent mass estimates is small and the dispersion of the observed overestimation is large, but it could also highlight issues with RGs in EBs where the companion is an MS dwarf star. For an RG in an EB, the mass of the RG is driven by the low S/N Doppler shift that is measured by tracking the absorption lines of the companion star. In most cases, the flux coming from the companion is less than 5% of the total flux. We also note that a good agreement between dynamical and seismic masses was found with the double RG KIC 9246715 (Rawls et al. 2016), where there were no issues of noisy RVs.

In contrast, KIC 7955301 is a special target with respect to the bulk of RGs in EBs because it is the least evolved, and thus the smallest RG ($\approx 5.85 R_{\odot}$) for which we have an independent mass measurement. The radii of all of the RGs in EBs listed in Benbakoura et al. (2021), for example, range from 8 to 14 $R_{\odot}$. In addition, a significant fraction of them are red clump stars. So far, no significant overestimation of stellar masses and radii by asteroseismology has been observed for MS and subgiant stars. We may have an intermediate case here, for which asteroseismic measurements are unbiased. To clarify the question, our recommendation is to take new RV measurements of the RGs in EBs listed in Benbakoura et al. (2021) and Gaulme & Guzik (2019) with larger S/Ns, that is, longer exposure times, and with spectrometers that are dedicated to high-precision RV measurements.

## 7.2. Age of the system

One of the goals of the future ESA PLATO mission (Rauer et al. 2014) is to provide ages of solar-like MS stars hosting exoplanets with an accuracy of 10%. Many papers dealing with stellar physics report ages arising from stellar evolution codes with a similar precision, especially when asteroseismic measurements are available. With this paper, we could have run a single stellar evolution code and provided an age with a relatively low uncertainty. We decided to let four different modelers estimate the age in an independent fashion. We obtained $4.9 \pm 0.9$ Gyr with PARAM, $3.43_{-0.16}^{+0.62}$ Gyr with MESA, $4.5 \pm 0.2$ Gyr with YaPSI, and $4.5 \pm 0.2$ Gyr with LIGHTCURVEFACTORY, that is, with uncertainties of 18.4, 22.7, 4.4, and 4.4% respectively. Both the YaPSI and LIGHTCURVEFACTORY estimates have a better precision, likely because the three components of the system are included into the
optimization process. Ages determined for the RG only (component A), with the help of asteroseismic and classical parameters, have uncertainties of about 20%, despite RGs usually being considered good cases for age estimates thanks to their fast evolution along the RG branch.

Our age estimate thus ranges from 3.3 to 5.8 Gyr, which is quite broad given the unusually vast amount of information that we have. By looking more closely, the age is consistent between the three “standard” approaches that use the classical parameters (mass, metallicity, and effective temperature), and the global asteroseismic parameters (PARAM only). On the contrary, the model based on reproducing the individual oscillation frequencies with MESA stands apart. Even though a deeper understanding of the differences between the age estimates goes beyond the scope of this paper, we can already draw some conclusions. A careful inspection of the posterior PDF of the mass, radius, and age (Fig. 12) shows a good agreement between the mass and radius obtained with PARAM and MESA, whereas the age PDF appears to be bimodal with MESA. In fact, the secondary peak of the age distribution matches the PARAM estimate (at ≈4.5 Gyr). A key aspect of the MESA-model based optimization is that the helium abundance *Y* and metallicity *Z* are two free independent parameters of the model. The resulting *Y* value of 0.29 is quite large, considering the slightly subsolar value found for the metallicity (*Z* ≈ 0.012) and assuming a linear *Y* = *Y*(*Z*) relation, and that the Sun falls on that relation (see Fig. A.4, Miglio et al. 2021). A difference of about 0.02 in *Y* with respect to what we have in the grid used in PARAM would mean a difference of ~15% in age, which, considering also the slight difference in mass, could explain the different age estimate.

### 7.3. Formation of the system

Physical properties and the orbital configuration carry information about the formation process of the systems. We refer the reader to Borkovits et al. (2022) and references therein, where a connection between dynamical and orbital parameters and formation scenarios is discussed. An outer eccentricity of 0.27 for a 209-day period outer orbit is far from being exceptional. For example, Borkovits et al. (2016) reported 16 triple star candidates with a smaller outer period than that of KIC 7955301 and six of them have larger outer eccentricities. Since then, further highly eccentric systems amongst substantially more compact triply eclipsing triples were found in TESS data (Borkovits et al. 2022).

With an outer semimajor axis less than 10 AU, KIC 7955302 is considered to be a compact triple system. The formation of this type of system involves either a fragmentation of the accretion disk or a disk-mediated capture of the outer component. In both cases the outer star forms by being less massive than the inner binary. Then, thanks to its wider and eccentric orbit, it sweeps out a larger orbit, and thus accretes most of the infalling material from the accretion disk, which eventually leads $q_{out}$ toward larger values. Although it is expected that the total mass of the inner pair remains larger than the mass of the wide component by the end of the complete formation process, the third component may actually become the most massive star of the system (Tokovinin 2021), which is the case of KIC 7955301.

### 7.4. Evolution of the system

In the short term, we have shown that the inner binary components eclipse each other over a period of about 7.3 years, and stop eclipsing for the next 11.9 years. The RG will never eclipse the inner binary as seen from the Earth. This is why we were

<figure><img src="image_17.png" /><figcaption>**Fig. 17.** Top panel: radius evolution of the three components according to the MIST tracks (with masses and metallicity set equal to their nominal values from Table 4). The semimajor axis of the inner binary is indicated by the black dotted line, and the semimajor axis of the outer orbit with dashed lines. Bottom panel: zoom on the RG component around its RGB and AGB phases.</figcaption></figure>

able to study the eclipses of the inner binary from the *Kepler* data, and why we are not able to do so with TESS. The eclipses should be visible again during the ESA PLATO mission, whose nominal operations should take place between 2027 and 2031. The PLATO observations will certainly help fine-tune the model of the system.

In the long term and in general, stars are likely to merge in close multiple-star systems when the most massive component reaches the tip of the RG branch. This is especially true for low-mass stars that ignite helium only at the tip of the RGB, after reaching very large radii (~200 $R_\odot$). RGs may swallow planets or stars, converting their orbital momentum into spin and friction loss. There is indirect observational evidence for it. For example, about 3% of the solar-mass stars on the RGB and 11% of the helium-burning stars observed by *Kepler* display unusually fast rotation and magnetic fields (e.g., Tayar et al. 2015; Ceillier et al. 2017; Tayar & Pinsonneault 2018; Gaulme et al. 2020). This means that a fraction of the RGs in that mass range gain angular momentum between the RGB and the red clump (RC). Until alternative explanations are provided, a likely possibility is that these stars have engulfed a stellar or substellar companion. Recently, Price-Whelan et al. (2020) reported a notable dearth of close companions around the RC – where companions may have been engulfed when the primary star ascended the upper RGB – in the color-magnitude diagram produced by the APO Galactic Evolution Experiment (APOGEE, Majewski et al. 2017), which is part of the Sloan Digital Sky Survey IV (e.g., Blanton et al. 2017). The orbital configuration of KIC 7955301 represents a borderline case for this type of scenario. The current distance at periastron between the giant and the inner binary is about ≈142 $R_\odot$ according to the data from Table 4.
optimization process. Ages determined for the RG only (component A), with the help of asteroseismic and classical parameters, have uncertainties of about 20%, despite RGs usually being considered good cases for age estimates thanks to their fast evolution along the RG branch.

Our age estimate thus ranges from 3.3 to 5.8 Gyr, which is quite broad given the unusually vast amount of information that we have. By looking more closely, the age is consistent between the three “standard” approaches that use the classical parameters (mass, metallicity, and effective temperature), and the global asteroseismic parameters (PARAM only). On the contrary, the model based on reproducing the individual oscillation frequencies with MESA stands apart. Even though a deeper understanding of the differences between the age estimates goes beyond the scope of this paper, we can already draw some conclusions. A careful inspection of the posterior PDF of the mass, radius, and age (Fig. 12) shows a good agreement between the mass and radius obtained with PARAM and MESA, whereas the age PDF appears to be bimodal with MESA. In fact, the secondary peak of the age distribution matches the PARAM estimate (at ≈4.5 Gyr). A key aspect of the MESA-model based optimization is that the helium abundance *Y* and metallicity *Z* are two free independent parameters of the model. The resulting *Y* value of 0.29 is quite large, considering the slightly subsolar value found for the metallicity (*Z* ≈ 0.012) and assuming a linear *Y* = *Y*(*Z*) relation, and that the Sun falls on that relation (see Fig. A.4, Miglio et al. 2021). A difference of about 0.02 in *Y* with respect to what we have in the grid used in PARAM would mean a difference of ~15% in age, which, considering also the slight difference in mass, could explain the different age estimate.

### 7.3. Formation of the system

Physical properties and the orbital configuration carry information about the formation process of the systems. We refer the reader to Borkovits et al. (2022) and references therein, where a connection between dynamical and orbital parameters and formation scenarios is discussed. An outer eccentricity of 0.27 for a 209-day period outer orbit is far from being exceptional. For example, Borkovits et al. (2016) reported 16 triple star candidates with a smaller outer period than that of KIC 7955301 and six of them have larger outer eccentricities. Since then, further highly eccentric systems amongst substantially more compact triply eclipsing triples were found in TESS data (Borkovits et al. 2022).

With an outer semimajor axis less than 10 AU, KIC 7955302 is considered to be a compact triple system. The formation of this type of system involves either a fragmentation of the accretion disk or a disk-mediated capture of the outer component. In both cases the outer star forms by being less massive than the inner binary. Then, thanks to its wider and eccentric orbit, it sweeps out a larger orbit, and thus accretes most of the infalling material from the accretion disk, which eventually leads $q_{\text{out}}$ toward larger values. Although it is expected that the total mass of the inner pair remains larger than the mass of the wide component by the end of the complete formation process, the third component may actually become the most massive star of the system (Tokovinin 2021), which is the case of KIC 7955301.

### 7.4. Evolution of the system

In the short term, we have shown that the inner binary components eclipse each other over a period of about 7.3 years, and stop eclipsing for the next 11.9 years. The RG will never eclipse the inner binary as seen from the Earth. This is why we were

able to study the eclipses of the inner binary from the *Kepler* data, and why we are not able to do so with TESS. The eclipses should be visible again during the ESA PLATO mission, whose nominal operations should take place between 2027 and 2031. The PLATO observations will certainly help fine-tune the model of the system.

<figure><img src="image_18.png" /><figcaption>**Fig. 17.** Top panel: radius evolution of the three components according to the MIST tracks (with masses and metallicity set equal to their nominal values from Table 4). The semimajor axis of the inner binary is indicated by the black dotted line, and the semimajor axis of the outer orbit with dashed lines. Bottom panel: zoom on the RG component around its RGB and AGB phases.</figcaption></figure>

In the long term and in general, stars are likely to merge in close multiple-star systems when the most massive component reaches the tip of the RG branch. This is especially true for low-mass stars that ignite helium only at the tip of the RGB, after reaching very large radii (~200 $R_{\odot}$). RGs may swallow planets or stars, converting their orbital momentum into spin and friction loss. There is indirect observational evidence for it. For example, about 3% of the solar-mass stars on the RGB and 11% of the helium-burning stars observed by *Kepler* display unusually fast rotation and magnetic fields (e.g., Tayar et al. 2015; Ceillier et al. 2017; Tayar & Pinsonneault 2018; Gaulme et al. 2020). This means that a fraction of the RGs in that mass range gain angular momentum between the RGB and the red clump (RC). Until alternative explanations are provided, a likely possibility is that these stars have engulfed a stellar or substellar companion. Recently, Price-Whelan et al. (2020) reported a notable dearth of close companions around the RC – where companions may have been engulfed when the primary star ascended the upper RGB – in the color-magnitude diagram produced by the APO Galactic Evolution Experiment (APOGEE, Majewski et al. 2017), which is part of the Sloan Digital Sky Survey IV (e.g., Blanton et al. 2017). The orbital configuration of KIC 7955301 represents a borderline case for this type of scenario. The current distance at periastron between the giant and the inner binary is about ≈142 $R_{\odot}$ according to the data from Table 4.
We can formulate some broad predictions for the long-term evolution of the system, assuming that the dynamical interaction among the components can be neglected until they come into contact with each other because of post-MS evolution. Figure 17 shows the evolution of the radii of the three components according to evolutionary tracks generated with the MIST web interpolator (Choi et al. 2016), setting the masses to the central values given in Table 4 (1.29, 0.94, and 0.88 $M_\odot$ for components A, Ba, and Bb, respectively), and the metallicity to +0.06. Significant mass loss takes place during the RGB and asymptotic giant branch (AGB) phases, and as a result, all three stars reach a final mass of about 0.5 $M_\odot$ by the end of their respective AGB phases. Stellar rotation is not included in these models. At an age of approximately 5 Gyr, component A (already an RG at the present time) reaches the RGB tip, and shortly after (relative to the $10^9$ yr timescale) the AGB tip and thermal pulses phase. The peak radius reached at the tip of the RGB ($\approx 160 R_\odot$) is mostly equal to the distance at periastron, while the peak radius on some of the AGB pulses is significantly larger than the semimajor axis of the outer orbit, and thus merging can be expected to occur at one of those times. Should merging of component A with the inner binary be avoided because of some process not considered in this crude analysis, at around 15 Gyr, component Ba will evolve onto the RGB and merge with Bb. In light of this discussion, it is comforting that none of our age estimates is larger than 5 Gyr.

**Acknowledgements.** This paper includes data collected by the *Kepler* mission. Funding for the *Kepler* mission is provided by the NASA Science Mission Directorate. Some of the data presented in this paper were obtained from the Mikulski Archive for Space Telescopes (MAST). STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. This work is also based on observations obtained with the Apache Point Observatory 3.5-m telescope, which is owned and operated by the Astrophysical Research Consortium. Part of our spectroscopic observations were done at the Observatoire de Haute-Provence. We acknowledge the technical team for their onsite support as well as the “Programme National de Physique Stelлаire” (PNPS) of CNRS/INSU for their financial support. P.G. and F.S. were supported by the German space agency (Deutsches Zentrum für Luft- und Raumfahrt) under PLATO data grant 50001501. P.G. and J.J. acknowledge NASA grant NNX17AF74G for partial support. The research leading to these results has (partially) received funding from the KU Leuven Research Council (grant C16/18/005: PARADISE) and from the Belgian federal Science Policy Office (BELSPO) through PRODEX grant PLATO. M.B. acknowledges support from the “Deutscher Akademischer Austauschdiensl” (DAAD) and the Université Paris Diderot.

## References

Aizenman, M., Smeyers, P., & Weigert, A. 1977, A&A, 58, 41

Allard, F., Guillot, T., Ludwig, H. G., et al. 2003, in Brown Dwarfars, ed. E. Martín, IAU Symp., 211, 325

Appourchaux, T. 2020, A&A, 642, A226

Asplund, M., Grevesse, N., Sauval, A. J., & Scott, P. 2009, ARA&A, 47, 481

Bailer-Jones, C. A. L., Rybizki, J., Fouesneau, M., Demleitner, M., & Andrae, R. 2021, AJ, 161, 147

Beck, P. G., Hambleton, K., Vos, J., et al. 2014, A&A, 564, A36

Beck, P. G., Hambleton, K., Vos, J., et al. 2015, Eur. Phys. J. Web Conf., 101, 06004

Benbakoura, M., Gaulme, P., McKeever, J., et al. 2021, A&A, 648, A113

Blanton, M. R., Bershady, M. A., Abolfathi, B., et al. 2017, AJ, 154, 28

Borkovits, T., Érdi, B., Forgács-Dajka, E., & Kovács, T. 2003, A&A, 398, 1091

Borkovits, T., Csizmadia, S., Forgács-Dajka, E., & Hegedüs, T. 2011, A&A, 528, A53

Borkovits, T., Hajdu, T., Sztakovics, J., et al. 2016, MNRAS, 455, 4136

Borkovits, T., Rappaport, S., Kaye, T., et al. 2019, MNRAS, 483, 1934

Borkovits, T., Rappaport, S. A., Hajdu, T., et al. 2020, MNRAS, 493, 5005

Borkovits, T., Rappaport, S. A., Toonen, S., et al. 2022, MNRAS, 515, 3773

Borucki, W. J., Koch, D. G., Basri, G., et al. 2011, ApJ, 736, 19

Bressan, A., Marigo, P., Girardi, L., et al. 2012, MNRAS, 427, 127

Brogaard, K., Hansen, C. J., Miglio, A., et al. 2018, MNRAS, 476, 3729

Brown, J. A., Sneden, C., Lambert, D. L., & Dutchover, E., Jr. 1989, ApJS, 71, 293

Brown, T. M., Latham, D. W., Everett, M. E., & Esmerdo, G. A. 2011, AJ, 142, 112

Buder, S., Asplund, M., Duong, L., et al. 2018, MNRAS, 478, 4513

Carter, J. A., Fabrycky, D. C., Ragozzine, D., et al. 2011, Science, 331, 562

Castelli, F., & Kurucz, R. L., et al. 2003, in Modelling of Stellar Atmospheres, 210, A20

Ceillier, T., Tayar, J., Mathur, S., et al. 2017, A&A, 605, A111

Charbonnel, C., Lagarde, N., Jasniewicz, G., et al. 2020, A&A, 633, A34

Choi, J., Dotter, A., Conroy, C., et al. 2016, ApJ, 823, 102

Claret, A., & Bloemen, S. 2011, A&A, 529, A75

Cutri, R. M., Wright, E. L., Conrow, T., et al. 2013, Explanatory Supplement to the AllWISE Data Release Products, Explanatory Supplement to the AllWISE Data Release Products

Derekas, A., Kiss, L. L., Borkovits, T., et al. 2011, Science, 332, 216

Eggleton, P. 2006, Evolutionary Processes in Binary and Multiple Stars (Cambridge: Cambridge University Press)

Ford, E. B. 2005, AJ, 129, 1706

Ford, E. B., Kozinsky, B., & Rasio, F. A. 2000, ApJ, 535, 385

Frandsen, S., Lehmann, H., Hekker, S., et al. 2013, A&A, 556, A138

Gaia Collaboration (Brown, A. G. A., et al.) 2018, A&A, 616, A1

Gaia Collaboration (Brown, A. G. A., et al.) 2021, A&A, 649, A1

García, R. A., Pérez Hernández, F., Benomar, O., et al. 2014, A&A, 563, A84

Gaulme, P., & Guzik, J. A. 2019, A&A, 630, A106

Gaulme, P., McKeever, J., Rawls, M. L., et al. 2013, ApJ, 767, 82

Gaulme, P., Jackiewicz, J., Appourchaux, T., & Mosser, B. 2014, ApJ, 785, 5

Gaulme, P., McKeever, J., Jackiewicz, J., et al. 2016, ApJ, 832, 121

Gaulme, P., Jackiewicz, J., Spada, F., et al. 2020, A&A, 639, A63

Gehan, C., Mosser, B., Michel, E., Samadi, R., & Kallinger, T. 2018, A&A, 616, A24

Gehan, C., Mosser, B., Michel, E., & Cunha, M. S. 2021, A&A, 645, A124

Gehan, C., Campante, T. L., Cunha, M. S., & Pereira, F. 2022, A&A, submitted

Gizon, L., & Solanki, S. K. 2003, ApJ, 589, 1009

Grevesse, N., & Sauval, A. J. 1998, Space Sci. Rev., 85, 161

Hekker, S., Debosscher, J., Huber, D., et al. 2010, ApJ, 713, L187

Helminiak, K. G., Ukita, N., Kambe, E., et al. 2017, MNRAS, 468, 1726

Henden, A. A., Levine, S., Terrell, D., & Welch, D. L. 2015, Am. Astron. Soc. Meet. Abstr., 225, 336.16

Henden, A. A., Templeton, M., Terrell, D., et al. 2016, VizieR On-line Data Catalog: II/336.

Huber, D., White, T. R., Metcalfe, T. S., et al. 2022, AJ, 163, 79

Iliijic, S. 2004, ASP Conf. Ser., 318, 107

Kallinger, T., De Ridder, J., Hekker, S., et al. 2014, A&A, 570, A41

Khan, S., Miglio, A., Mosser, B., et al. 2019, A&A, 628, A35

Kjeldsen, H., & Bedding, T. R. 1995, A&A, 293, 87

Kolbas, V., Pavlovski, K., Southworth, J., et al. 2015, MNRAS, 451, 4150

Kuszlewicz, J. S., North, T. S. H., Chaplin, W. J., et al. 2019, MNRAS, 487, 14

Loeb, A., & Gaudi, B. S. 2003, ApJ, 588, L117

Luck, R. E., & Heiter, U. 2007, AJ, 133, 2464

Lucy, L. B. 1967, ZAp, 65, 89

Majewski, S. R., Schiavon, R. P., Frinchaboy, P. M., et al. 2017, AJ, 154, 94

Mandel, K., & Agol, E. 2002, ApJ, 580, L171

Marcadon, F., Appourchaux, T., & Marques, J. P. 2018, A&A, 617, A2

Maxted, P. F. L., Gaulme, P., Graczyk, D., et al. 2020, MNRAS, 498, 332

Metcalfe, T. S., van Saders, J. L., Basu, S., et al. 2020, ApJ, 900, 154

Mier, P. R. 2017, https://doi.org/10.5281/zenodo.848679

Miglio, A., Chiappini, C., Mackereth, J. T., et al. 2021, A&A, 645, A85

Miller, N. J., Maxted, P. F. L., & Smalley, B. 2020, MNRAS, 497, 2899

Mosser, B., & Appourchaux, T. 2009, A&A, 508, 877

Mosser, B., Belkacem, K., Goupil, M. J., et al. 2011, A&A, 525, L9

Mosser, B., Goupil, M. J., Belkacem, K., et al. 2012, A&A, 548, A10

Mosser, B., Michel, E., Belkacem, K., et al. 2013, A&A, 550, A126

Mosser, B., Benomar, O., Belkacem, K., et al. 2014, A&A, 572, L5

Mosser, B., Vrard, M., Belkacem, K., Deheuvels, S., & Goupil, M. J. 2015, A&A, 584, A50

Mosser, B., Pinçon, C., Belkacem, K., Takata, M., & Vrard, M. 2017, A&A, 600, A1

Mosser, B., Gehan, C., Belkacem, K., et al. 2018, A&A, 618, A109

Ong, J. M. J., & Basu, S. 2020, ApJ, 898, 127

Pál, A. 2012, MNRAS, 421, 1825

Pavlovski, K., & Hensberge, H. 2005, A&A, 439, 309

Pavlovski, K., Tamajo, E., Koubský, P., et al. 2009, MNRAS, 400, 791

Pavlovski, K., Southworth, J., & Tamajo, E. 2018, MNRAS, 481, 3129

Paxton, B., Bildsten, L., Dotter, A., et al. 2011, ApJS, 192, 3

Paxton, B., Cantiello, M., Arras, P., et al. 2013, ApJS, 208, 4

Paxton, B., Marchant, P., Schwab, J., et al. 2015, ApJS, 220, 15
We can formulate some broad predictions for the long-term evolution of the system, assuming that the dynamical interaction among the components can be neglected until they come into contact with each other because of post-MS evolution. Figure 17 shows the evolution of the radii of the three components according to evolutionary tracks generated with the MIST web interpolator (Choi et al. 2016), setting the masses to the central values given in Table 4 (1.29, 0.94, and 0.88 $M_\odot$ for components A, Ba, and Bb, respectively), and the metallicity to +0.06. Significant mass loss takes place during the RGB and asymptotic giant branch (AGB) phases, and as a result, all three stars reach a final mass of about 0.5 $M_\odot$ by the end of their respective AGB phases. Stellar rotation is not included in these models. At an age of approximately 5 Gyr, component A (already an RG at the present time) reaches the RGB tip, and shortly after (relative to the $10^9$ yr timescale) the AGB tip and thermal pulses phase. The peak radius reached at the tip of the RGB ($\approx 160 R_\odot$) is mostly equal to the distance at periastron, while the peak radius on some of the AGB pulses is significantly larger than the semimajor axis of the outer orbit, and thus merging can be expected to occur at one of those times. Should merging of component A with the inner binary be avoided because of some process not considered in this crude analysis, at around 15 Gyr, component Ba will evolve onto the RGB and merge with Bb. In light of this discussion, it is comforting that none of our age estimates is larger than 5 Gyr.

**Acknowledgements.** This paper includes data collected by the *Kepler* mission. Funding for the *Kepler* mission is provided by the NASA Science Mission Directorate. Some of the data presented in this paper were obtained from the Mikulski Archive for Space Telescopes (MAST). STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. This work is also based on observations obtained with the Apache Point Observatory 3.5-m telescope, which is owned and operated by the Astrophysical Research Consortium. Part of our spectroscopic observations were done at the Observatoire de Haute-Provence. We acknowledge the technical team for their onsite support as well as the “Programme National de Physique Stelлаire” (PNPS) of CNRS/INSU for their financial support. P.G. and F.S. were supported by the German space agency (Deutsches Zentrum für Luft- und Raumfahrt) under PLATO data grant 50001501. P.G. and J.J. acknowledge NASA grant NNX17AF74G for partial support. The research leading to these results has (partially) received funding from the KU Leuven Research Council (grant C16/18/005: PARADISE) and from the Belgian federal Science Policy Office (BELSPO) through PRODEX grant PLATO. M.B. acknowledges support from the “Deutscher Akademischer Austauschdiensl” (DAAD) and the Université Paris Diderot.

References

Aizenman, M., Smeyers, P., & Weigert, A. 1977, A&A, 58, 41

Allard, F., Guillot, T., Ludwig, H. G., et al. 2003, in Brown Dwarfars, ed. E. Martín, IAU Symp., 211, 325

Appourchaux, T. 2020, A&A, 642, A226

Asplund, M., Grevesse, N., Sauval, A. J., & Scott, P. 2009, ARA&A, 47, 481

Bailer-Jones, C. A. L., Rybizki, J., Fouesneau, M., Demleitner, M., & Andrae, R. 2021, AJ, 161, 147

Beck, P. G., Hambleton, K., Vos, J., et al. 2014, A&A, 564, A36

Beck, P. G., Hambleton, K., Vos, J., et al. 2015, Eur. Phys. J. Web Conf., 101, 06004

Benbakoura, M., Gaulme, P., McKeever, J., et al. 2021, A&A, 648, A113

Blanton, M. R., Bershady, M. A., Abolfathi, B., et al. 2017, AJ, 154, 28

Borkovits, T., Érdi, B., Forgács-Dajka, E., & Kovács, T. 2003, A&A, 398, 1091

Borkovits, T., Csizmadia, S., Forgács-Dajka, E., & Hegedüs, T. 2011, A&A, 528, A53

Borkovits, T., Hajdu, T., Sztakovics, J., et al. 2016, MNRAS, 455, 4136

Borkovits, T., Rappaport, S., Kaye, T., et al. 2019, MNRAS, 483, 1934

Borkovits, T., Rappaport, S. A., Hajdu, T., et al. 2020, MNRAS, 493, 5005

Borkovits, T., Rappaport, S. A., Toonen, S., et al. 2022, MNRAS, 515, 3773

Borucki, W. J., Koch, D. G., Basri, G., et al. 2011, ApJ, 736, 19

Bressan, A., Marigo, P., Girardi, L., et al. 2012, MNRAS, 427, 127

Brogaard, K., Hansen, C. J., Miglio, A., et al. 2018, MNRAS, 476, 3729

Brown, J. A., Sneden, C., Lambert, D. L., & Dutchover, E., Jr. 1989, ApJS, 71, 293

Brown, T. M., Latham, D. W., Everett, M. E., & Esmerdo, G. A. 2011, AJ, 142, 112

Buder, S., Asplund, M., Duong, L., et al. 2018, MNRAS, 478, 4513

Carter, J. A., Fabrycky, D. C., Ragozzine, D., et al. 2011, Science, 331, 562

Castelli, F., & Kurucz, R. L., et al. 2003, in Modelling of Stellar Atmospheres, 210, A20

Ceillier, T., Tayar, J., Mathur, S., et al. 2017, A&A, 605, A111

Charbonnel, C., Lagarde, N., Jasniewicz, G., et al. 2020, A&A, 633, A34

Choi, J., Dotter, A., Conroy, C., et al. 2016, ApJ, 823, 102

Claret, A., & Bloemen, S. 2011, A&A, 529, A75

Cutri, R. M., Wright, E. L., Conrow, T., et al. 2013, Explanatory Supplement to the AllWISE Data Release Products, Explanatory Supplement to the AllWISE Data Release Products

Derekas, A., Kiss, L. L., Borkovits, T., et al. 2011, Science, 332, 216

Eggleton, P. 2006, Evolutionary Processes in Binary and Multiple Stars (Cambridge: Cambridge University Press)

Ford, E. B. 2005, AJ, 129, 1706

Ford, E. B., Kozinsky, B., & Rasio, F. A. 2000, ApJ, 535, 385

Frandsen, S., Lehmann, H., Hekker, S., et al. 2013, A&A, 556, A138

Gaia Collaboration (Brown, A. G. A., et al.) 2018, A&A, 616, A1

Gaia Collaboration (Brown, A. G. A., et al.) 2021, A&A, 649, A1

García, R. A., Pérez Hernández, F., Benomar, O., et al. 2014, A&A, 563, A84

Gaulme, P., & Guzik, J. A. 2019, A&A, 630, A106

Gaulme, P., McKeever, J., Rawls, M. L., et al. 2013, ApJ, 767, 82

Gaulme, P., Jackiewicz, J., Appourchaux, T., & Mosser, B. 2014, ApJ, 785, 5

Gaulme, P., McKeever, J., Jackiewicz, J., et al. 2016, ApJ, 832, 121

Gaulme, P., Jackiewicz, J., Spada, F., et al. 2020, A&A, 639, A63

Gehan, C., Mosser, B., Michel, E., Samadi, R., & Kallinger, T. 2018, A&A, 616, A24

Gehan, C., Mosser, B., Michel, E., & Cunha, M. S. 2021, A&A, 645, A124

Gehan, C., Campante, T. L., Cunha, M. S., & Pereira, F. 2022, A&A, submitted

Gizon, L., & Solanki, S. K. 2003, ApJ, 589, 1009

Grevesse, N., & Sauval, A. J. 1998, Space Sci. Rev., 85, 161

Hekker, S., Debosscher, J., Huber, D., et al. 2010, ApJ, 713, L187

Helminiak, K. G., Ukita, N., Kambe, E., et al. 2017, MNRAS, 468, 1726

Henden, A. A., Levine, S., Terrell, D., & Welch, D. L. 2015, Am. Astron. Soc. Meet. Abstr., 225, 336.16

Henden, A. A., Templeton, M., Terrell, D., et al. 2016, VizieR On-line Data Catalog: II/336.

Huber, D., White, T. R., Metcalfe, T. S., et al. 2022, AJ, 163, 79

Iliijic, S. 2004, ASP Conf. Ser., 318, 107

Kallinger, T., De Ridder, J., Hekker, S., et al. 2014, A&A, 570, A41

Khan, S., Miglio, A., Mosser, B., et al. 2019, A&A, 628, A35

Kjeldsen, H., & Bedding, T. R. 1995, A&A, 293, 87

Kolbas, V., Pavlovski, K., Southworth, J., et al. 2015, MNRAS, 451, 4150

Kuszlewicz, J. S., North, T. S. H., Chaplin, W. J., et al. 2019, MNRAS, 487, 14

Loeb, A., & Gaudi, B. S. 2003, ApJ, 588, L117

Luck, R. E., & Heiter, U. 2007, AJ, 133, 2464

Lucy, L. B. 1967, ZAp, 65, 89

Majewski, S. R., Schiavon, R. P., Frinchaboy, P. M., et al. 2017, AJ, 154, 94

Mandel, K., & Agol, E. 2002, ApJ, 580, L171

Marcadon, F., Appourchaux, T., & Marques, J. P. 2018, A&A, 617, A2

Maxted, P. F. L., Gaulme, P., Graczyk, D., et al. 2020, MNRAS, 498, 332

Metcalfe, T. S., van Saders, J. L., Basu, S., et al. 2020, ApJ, 900, 154

Mier, P. R. 2017, https://doi.org/10.5281/zenodo.848679

Miglio, A., Chiappini, C., Mackereth, J. T., et al. 2021, A&A, 645, A85

Miller, N. J., Maxted, P. F. L., & Smalley, B. 2020, MNRAS, 497, 2899

Mosser, B., & Appourchaux, T. 2009, A&A, 508, 877

Mosser, B., Belkacem, K., Goupil, M. J., et al. 2011, A&A, 525, L9

Mosser, B., Goupil, M. J., Belkacem, K., et al. 2012, A&A, 548, A10

Mosser, B., Michel, E., Belkacem, K., et al. 2013, A&A, 550, A126

Mosser, B., Benomar, O., Belkacem, K., et al. 2014, A&A, 572, L5

Mosser, B., Vrard, M., Belkacem, K., Deheuvels, S., & Goupil, M. J. 2015, A&A, 584, A50

Mosser, B., Pinçon, C., Belkacem, K., Takata, M., & Vrard, M. 2017, A&A, 600, A1

Mosser, B., Gehan, C., Belkacem, K., et al. 2018, A&A, 618, A109

Ong, J. M. J., & Basu, S. 2020, ApJ, 898, 127

Pál, A. 2012, MNRAS, 421, 1825

Pavlovski, K., & Hensberge, H. 2005, A&A, 439, 309

Pavlovski, K., Tamajo, E., Koubský, P., et al. 2009, MNRAS, 400, 791

Pavlovski, K., Southworth, J., & Tamajo, E. 2018, MNRAS, 481, 3129

Paxton, B., Bildsten, L., Dotter, A., et al. 2011, ApJS, 192, 3

Paxton, B., Cantiello, M., Arras, P., et al. 2013, ApJS, 208, 4

Paxton, B., Marchant, P., Schwab, J., et al. 2015, ApJS, 220, 15
Paxton, B., Schwab, J., Bauer, E. B., et al. 2018, ApJS, 234, 34

Paxton, B., Smolec, R., Schwab, J., et al. 2019, ApJS, 243, 10

Pinçon, C., Takata, M., & Mosser, B. 2019, A&A, 626, A125

Piskunov, N. E., & Valenti, J. A. 2002, A&A, 385, 1095

Price-Whelan, A. M., Hogg, D. W., Rix, H.-W., et al. 2020, ApJ, 895, 2

Prša, A., & Zwitter, T. 2005, ApJ, 628, 426

Rappaport, S., Deck, K., Levine, A., et al. 2013, ApJ, 768, 33

Rauer, H., Catala, C., Aerts, C., et al. 2014, Exp. Astron., 38, 249

Rawls, M. L., Gaulme, P., McKeever, J., et al. 2016, ApJ, 818, 108

Rodrigues, T. S., Bossini, D., Miglio, A., et al. 2017, MNRAS, 467, 1433

Roxburgh, I. W. 2016, A&A, 585, A63

Rucinski, S. M. 2002, AJ, 124, 1746

Santerne, A., Bonomo, A. S., Hébrard, G., et al. 2011a, A&A, 536, A70

Santerne, A., Díaz, R. F., Bouchy, F., et al. 2011b, A&A, 528, A63

Shulyak, D., Tsymbal, V., Ryabchikova, T., Stütz, C., & Weiss, W. W. 2004, A&A, 428, 993

Simon, K. P., & Sturm, E. 1994, A&A, 281, 286

Skrutskie, M. F., Cutri, R. M., Stiening, R., et al. 2006, AJ, 131, 1163

Smith, K. C. 1992, PhD Thesis, University College London, UK

Spada, F., Demarque, P., Kim, Y. C., Boyajian, T. S., & Brewer, J. M. 2017, ApJ, 838, 161

Stassun, K. G., Oelkers, R. J., Pepper, J., et al. 2018, AJ, 156, 102

Tayar, J., & Pinsonneault, M. H. 2018, ApJ, 868, 150

Tayar, J., Ceillier, T., García-Hernández, D. A., et al. 2015, ApJ, 807, 82

Themeßl, N., Hekker, S., Southworth, J., et al. 2018, MNRAS, 478, 4669

Tkachenko, A. 2015, A&A, 581, A129

Tokovinin, A. A. 1997, Astron. Lett., 23, 727

Tokovinin, A. A. 2021, Universe, 7, 352

Torres, G., Sandberg Lacy, C. H., Pavlovski, K., et al. 2014, ApJ, 797, 31

Tout, C. A., Pols, O. R., Eggleton, P. P., & Han, Z. 1996, MNRAS, 281, 257

Townsend, R. H. D., & Teitler, S. A. 2013, MNRAS, 435, 3406

Twicken, J. D., Chandrasekaran, H., Jenkins, J. M., et al. 2010, Proc. SPIE, 7740, 77401U

van Kerkwijk, M. H., Rappaport, S. A., Breton, R. P., et al. 2010, ApJ, 715, 51

Vrard, M., Mosser, B., & Samadi, R. 2016, A&A, 588, A87

Wang, S. I., Hildebrand, R. H., Hobbs, L. M., et al. 2003, SPIE Conf. Ser., 4841, 1145

Yan, Z.-C., Tambasco, M., & Drake, G. W. F. 1998, Phys. Rev. A, 57, 1652
Paxton, B., Schwab, J., Bauer, E. B., et al. 2018, ApJS, 234, 34

Paxton, B., Smolec, R., Schwab, J., et al. 2019, ApJS, 243, 10

Pinçon, C., Takata, M., & Mosser, B. 2019, A&A, 626, A125

Piskunov, N. E., & Valenti, J. A. 2002, A&A, 385, 1095

Price-Whelan, A. M., Hogg, D. W., Rix, H.-W., et al. 2020, ApJ, 895, 2

Prša, A., & Zwitter, T. 2005, ApJ, 628, 426

Rappaport, S., Deck, K., Levine, A., et al. 2013, ApJ, 768, 33

Rauer, H., Catala, C., Aerts, C., et al. 2014, Exp. Astron., 38, 249

Rawls, M. L., Gaulme, P., McKeever, J., et al. 2016, ApJ, 818, 108

Rodrigues, T. S., Bossini, D., Miglio, A., et al. 2017, MNRAS, 467, 1433

Roxburgh, I. W. 2016, A&A, 585, A63

Rucinski, S. M. 2002, AJ, 124, 1746

Santerne, A., Bonomo, A. S., Hébrard, G., et al. 2011a, A&A, 536, A70

Santerne, A., Díaz, R. F., Bouchy, F., et al. 2011b, A&A, 528, A63

Shulyak, D., Tsymbal, V., Ryabchikova, T., Stütz, C., & Weiss, W. W. 2004, A&A, 428, 993

Simon, K. P., & Sturm, E. 1994, A&A, 281, 286

Skrutskie, M. F., Cutri, R. M., Stiening, R., et al. 2006, AJ, 131, 1163

Smith, K. C. 1992, PhD Thesis, University College London, UK

Spada, F., Demarque, P., Kim, Y. C., Boyajian, T. S., & Brewer, J. M. 2017, ApJ, 838, 161

Stassun, K. G., Oelkers, R. J., Pepper, J., et al. 2018, AJ, 156, 102

Tayar, J., & Pinsonneault, M. H. 2018, ApJ, 868, 150

Tayar, J., Ceillier, T., García-Hernández, D. A., et al. 2015, ApJ, 807, 82

Themeßl, N., Hekker, S., Southworth, J., et al. 2018, MNRAS, 478, 4669

Tkachenko, A. 2015, A&A, 581, A129

Tokovinin, A. A. 1997, Astron. Lett., 23, 727

Tokovinin, A. A. 2021, Universe, 7, 352

Torres, G., Sandberg Lacy, C. H., Pavlovski, K., et al. 2014, ApJ, 797, 31

Tout, C. A., Pols, O. R., Eggleton, P. P., & Han, Z. 1996, MNRAS, 281, 257

Townsend, R. H. D., & Teitler, S. A. 2013, MNRAS, 435, 3406

Twicken, J. D., Chandrasekaran, H., Jenkins, J. M., et al. 2010, Proc. SPIE, 7740, 77401U

van Kerkwijk, M. H., Rappaport, S. A., Breton, R. P., et al. 2010, ApJ, 715, 51

Vrard, M., Mosser, B., & Samadi, R. 2016, A&A, 588, A87

Wang, S. I., Hildebrand, R. H., Hobbs, L. M., et al. 2003, SPIE Conf. Ser., 4841, 1145

Yan, Z.-C., Tambasco, M., & Drake, G. W. F. 1998, Phys. Rev. A, 57, 1652
**Appendix A: Radial velocity data**

Table A.1 contains the RVs obtained at Apache Point and Haute-Provence observatories.

<table><caption>**Table A.1.** Radial velocity data obtained at Apache Point and Haute-Provence observatories.</caption><thead><tr><th>Date (KJD)</th><th>RV km s<sup>-1</sup></th></tr></thead><tbody><tr><td>1569.823526</td><td>-28.82</td></tr><tr><td>1591.832861</td><td>-12.50</td></tr><tr><td>1611.826703</td><td>-1.44</td></tr><tr><td>1648.831533</td><td>9.92</td></tr><tr><td>1704.641327</td><td>-18.59</td></tr><tr><td>1711.645679</td><td>-30.04</td></tr><tr><td>1737.619563</td><td>-53.19</td></tr><tr><td>1766.572107</td><td>-36.50</td></tr><tr><td>1958.878300</td><td>-48.28</td></tr><tr><td>3090.825370</td><td>4.65</td></tr><tr><td>3189.617802</td><td>-50.82</td></tr><tr><td>3195.587236</td><td>-53.95</td></tr><tr><td>3203.595970</td><td>-52.70</td></tr><tr><td>3216.717021</td><td>-45.36</td></tr><tr><td>3217.631558</td><td>-43.57</td></tr><tr><td>3219.657836</td><td>-42.14</td></tr><tr><td>3416.917213</td><td>-49.39</td></tr><tr><td>3444.847760</td><td>-28.94</td></tr><tr><td>3445.534184*</td><td>-27.26</td></tr><tr><td>3446.421966*</td><td>-26.49</td></tr><tr><td>3542.669669</td><td>8.53</td></tr><tr><td>3557.755987</td><td>3.53</td></tr><tr><td>3559.754443</td><td>3.12</td></tr><tr><td>3568.344058*</td><td>-2.24</td></tr><tr><td>3616.635254</td><td>-54.58</td></tr><tr><td>3617.597411</td><td>-54.06</td></tr></tbody></table>

**Notes.** Dates are mid-exposure times expressed in *Kepler* Julian dates (KJD). *Kepler* Julian dates KJD are related to barycentric Julian dates BJD by $KJD = BJD - 2,454,833$ days. The first spectrum was taken on April 20, 2013, and the last on November 28, 2018. Measurement errors are estimated to be $0.5$ km s$^{-1}$. Dates with an ★ sign are data taken at OHP.
**Appendix A: Radial velocity data**

Table A.1 contains the RVs obtained at Apache Point and Haute-Provence observatories.

<table><caption>**Table A.1.** Radial velocity data obtained at Apache Point and Haute-Provence observatories.</caption><thead><tr><th>Date (KJD)</th><th>RV km s<sup>-1</sup></th></tr></thead><tbody><tr><td>1569.823526</td><td>-28.82</td></tr><tr><td>1591.832861</td><td>-12.50</td></tr><tr><td>1611.826703</td><td>-1.44</td></tr><tr><td>1648.831533</td><td>9.92</td></tr><tr><td>1704.641327</td><td>-18.59</td></tr><tr><td>1711.645679</td><td>-30.04</td></tr><tr><td>1737.619563</td><td>-53.19</td></tr><tr><td>1766.572107</td><td>-36.50</td></tr><tr><td>1958.878300</td><td>-48.28</td></tr><tr><td>3090.825370</td><td>4.65</td></tr><tr><td>3189.617802</td><td>-50.82</td></tr><tr><td>3195.587236</td><td>-53.95</td></tr><tr><td>3203.595970</td><td>-52.70</td></tr><tr><td>3216.717021</td><td>-45.36</td></tr><tr><td>3217.631558</td><td>-43.57</td></tr><tr><td>3219.657836</td><td>-42.14</td></tr><tr><td>3416.917213</td><td>-49.39</td></tr><tr><td>3444.847760</td><td>-28.94</td></tr><tr><td>3445.534184*</td><td>-27.26</td></tr><tr><td>3446.421966*</td><td>-26.49</td></tr><tr><td>3542.669669</td><td>8.53</td></tr><tr><td>3557.755987</td><td>3.53</td></tr><tr><td>3559.754443</td><td>3.12</td></tr><tr><td>3568.344058*</td><td>-2.24</td></tr><tr><td>3616.635254</td><td>-54.58</td></tr><tr><td>3617.597411</td><td>-54.06</td></tr></tbody></table>

**Notes.** Dates are mid-exposure times expressed in *Kepler* Julian dates (KJD). *Kepler* Julian dates KJD are related to barycentric Julian dates BJD by $KJD = BJD - 2,454,833$ days. The first spectrum was taken on April 20, 2013, and the last on November 28, 2018. Measurement errors are estimated to be $0.5$ km s$^{-1}$. Dates with an ★ sign are data taken at OHP.
## Appendix B: Oscillation frequencies

Table B.1 displays the oscillation frequencies of the RG component, as performed by co-authors Appourchaux and Mosser.

<table><caption>**Table B.1.** Oscillation frequencies of KIC 7955301 by co-authors Appourchaux and Mosser (COR method). The columns report $v_{as}$ as an asymptotic fit (µHz), $v_{obs}$ are the observed peak (µHz) with uncertainties, $nm$ is the proxy of the mixed order ($nm = np - ng$; 0 for p-modes), $zeta$ = zeta factor of mixed modes (Mosser+2015, 2018), and HBR is the height-to-background ratio.</caption><thead><tr><th rowspan="2">l</th><th rowspan="2">m</th><th rowspan="2">n</th><th rowspan="2">nm<sub>TA</sub></th><th rowspan="2">nm<sub>BM</sub></th><th colspan="2">Appourchaux</th><th colspan="4">Mosser</th></tr><tr><th>v<sub>obs,TA</sub><br>µHz</th><th>err<br>µHz</th><th>v<sub>obs,BM</sub><br>µHz</th><th>err<br>µHz</th><th>v<sub>as</sub><br>µHz</th><th>ζ</th><th>HBR</th></tr></thead><tbody><tr><td>0</td><td>0</td><td>7</td><td>8</td><td>87</td><td>0.057</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>0</td><td>0</td><td>8</td><td>9</td><td>0</td><td>96.918</td><td>0.027</td><td>96.905</td><td>0.063</td><td>96.593</td><td>0.000</td><td>17.4</td></tr><tr><td>0</td><td>0</td><td>9</td><td>10</td><td>0</td><td>106.921</td><td>0.009</td><td>106.917</td><td>0.009</td><td>106.920</td><td>0.000</td><td>47.4</td></tr><tr><td>0</td><td>0</td><td>10</td><td>11</td><td>0</td><td>117.396</td><td>0.013</td><td>117.402</td><td>0.018</td><td>117.323</td><td>0.000</td><td>110.2</td></tr><tr><td>0</td><td>0</td><td>11</td><td>12</td><td>0</td><td>127.851</td><td>0.167</td><td>127.753</td><td>0.013</td><td>127.802</td><td>0.000</td><td>127.9</td></tr><tr><td>0</td><td>0</td><td>12</td><td>13</td><td>0</td><td>138.268</td><td>0.018</td><td>138.230</td><td>0.027</td><td>138.357</td><td>0.000</td><td>50.2</td></tr><tr><td>0</td><td>0</td><td>13</td><td>14</td><td>0</td><td>149.021</td><td>0.004</td><td>148.943</td><td>0.013</td><td>148.987</td><td>0.000</td><td>21.1</td></tr><tr><td>0</td><td>0</td><td>14</td><td>15</td><td>...</td><td>159.718</td><td>0.059</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>-1</td><td>...</td><td>-136</td><td>...</td><td>90.142</td><td>0.002</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>1</td><td>...</td><td>-132</td><td>...</td><td>92.323</td><td>0.022</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>-1</td><td>...</td><td>-132</td><td>...</td><td>92.626</td><td>0.052</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>1</td><td>8</td><td>...</td><td>-126</td><td>...</td><td>...</td><td>98.377</td><td>0.014</td><td>98.371</td><td>0.989</td><td>5.4</td></tr><tr><td>1</td><td>1</td><td>8</td><td>-120</td><td>...</td><td>101.235</td><td>0.004</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>-1</td><td>8</td><td>-120</td><td>-121</td><td>101.310</td><td>0.004</td><td>101.305</td><td>0.017</td><td>101.277</td><td>0.825</td><td>19.5</td></tr><tr><td>1</td><td>-1</td><td>8</td><td>-119</td><td>-120</td><td>101.874</td><td>0.006</td><td>101.880</td><td>0.026</td><td>101.831</td><td>0.614</td><td>64.9</td></tr><tr><td>1</td><td>1</td><td>8</td><td>-119</td><td>...</td><td>101.881</td><td>0.006</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>0</td><td>8</td><td>-119</td><td>...</td><td>102.112</td><td>0.001</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>1</td><td>8</td><td>-118</td><td>...</td><td>102.342</td><td>0.015</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>-1</td><td>8</td><td>-118</td><td>-119</td><td>102.401</td><td>0.006</td><td>102.391</td><td>0.011</td><td>102.390</td><td>0.825</td><td>14.5</td></tr><tr><td>1</td><td>-1</td><td>8</td><td>-117</td><td>...</td><td>103.061</td><td>0.002</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>1</td><td>8</td><td>-117</td><td>...</td><td>103.103</td><td>0.005</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>1</td><td>8</td><td>...</td><td>-118</td><td>...</td><td>...</td><td>103.840</td><td>0.014</td><td>103.853</td><td>0.973</td><td>7.3</td></tr><tr><td>1</td><td>-1</td><td>...</td><td>-113</td><td>...</td><td>106.245</td><td>0.000</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>1</td><td>...</td><td>-113</td><td>...</td><td>106.384</td><td>0.009</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>1</td><td>...</td><td>-112</td><td>...</td><td>107.164</td><td>0.012</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>-1</td><td>9</td><td>-110</td><td>-111</td><td>109.059</td><td>0.001</td><td>109.051</td><td>0.012</td><td>109.066</td><td>0.985</td><td>14.1</td></tr><tr><td>1</td><td>1</td><td>9</td><td>-109</td><td>-111</td><td>109.807</td><td>0.002</td><td>109.806</td><td>0.010</td><td>109.816</td><td>0.977</td><td>20.5</td></tr><tr><td>1</td><td>1</td><td>9</td><td>-108</td><td>-110</td><td>110.698</td><td>0.001</td><td>110.696</td><td>0.010</td><td>110.705</td><td>0.949</td><td>24.2</td></tr><tr><td>1</td><td>-1</td><td>9</td><td>-108</td><td>-109</td><td>110.863</td><td>0.002</td><td>110.837</td><td>0.021</td><td>110.868</td><td>0.938</td><td>5.6</td></tr><tr><td>1</td><td>1</td><td>9</td><td>...</td><td>-109</td><td>...</td><td>...</td><td>111.554</td><td>0.012</td><td>111.550</td><td>0.823</td><td>10.6</td></tr><tr><td>1</td><td>-1</td><td>9</td><td>-107</td><td>-108</td><td>111.717</td><td>0.001</td><td>111.719</td><td>0.016</td><td>111.693</td><td>0.770</td><td>34.8</td></tr><tr><td>1</td><td>1</td><td>9</td><td>-107</td><td>-108</td><td>112.305</td><td>0.013</td><td>112.254</td><td>0.035</td><td>112.188</td><td>0.567</td><td>59.1</td></tr><tr><td>1</td><td>-1</td><td>9</td><td>-106</td><td>-107</td><td>112.369</td><td>0.016</td><td>112.325</td><td>0.016</td><td>112.299</td><td>0.584</td><td>59.3</td></tr><tr><td>1</td><td>0</td><td>9</td><td>-118</td><td>-107</td><td>102.592</td><td>0.001</td><td>112.514</td><td>0.021</td><td>112.547</td><td>0.699</td><td>9.2</td></tr><tr><td>1</td><td>1</td><td>9</td><td>-106</td><td>-107</td><td>112.862</td><td>0.004</td><td>112.876</td><td>0.022</td><td>112.836</td><td>0.822</td><td>34.9</td></tr><tr><td>1</td><td>-1</td><td>9</td><td>-105</td><td>-106</td><td>113.013</td><td>0.011</td><td>113.041</td><td>0.016</td><td>113.014</td><td>0.870</td><td>26.1</td></tr><tr><td>1</td><td>1</td><td>9</td><td>-105</td><td>-106</td><td>113.699</td><td>0.010</td><td>113.703</td><td>0.012</td><td>113.718</td><td>0.949</td><td>20.3</td></tr><tr><td>1</td><td>-1</td><td>9</td><td>-104</td><td>-105</td><td>113.913</td><td>0.007</td><td>113.931</td><td>0.011</td><td>113.933</td><td>0.959</td><td>9.1</td></tr><tr><td>1</td><td>1</td><td>9</td><td>-104</td><td>-105</td><td>114.624</td><td>0.002</td><td>114.655</td><td>0.013</td><td>114.673</td><td>0.976</td><td>15.8</td></tr><tr><td>1</td><td>-1</td><td>9</td><td>...</td><td>-103</td><td>...</td><td>...</td><td>115.938</td><td>0.014</td><td>115.914</td><td>0.986</td><td>45.1</td></tr><tr><td>1</td><td>1</td><td>9</td><td>...</td><td>-103</td><td>...</td><td>...</td><td>116.647</td><td>0.017</td><td>116.668</td><td>0.988</td><td>6.1</td></tr><tr><td>1</td><td>-1</td><td>10</td><td>...</td><td>-102</td><td>...</td><td>...</td><td>116.953</td><td>0.011</td><td>116.941</td><td>0.988</td><td>14.6</td></tr><tr><td>1</td><td>-1</td><td>10</td><td>...</td><td>-101</td><td>...</td><td>...</td><td>117.977</td><td>0.015</td><td>117.988</td><td>0.988</td><td>5.2</td></tr><tr><td>1</td><td>1</td><td>10</td><td>...</td><td>-101</td><td>...</td><td>...</td><td>118.717</td><td>0.018</td><td>118.741</td><td>0.986</td><td>5.4</td></tr><tr><td>1</td><td>-1</td><td>10</td><td>-99</td><td>-100</td><td>119.028</td><td>0.002</td><td>119.032</td><td>0.013</td><td>119.051</td><td>0.984</td><td>31.0</td></tr><tr><td>1</td><td>1</td><td>10</td><td>-99</td><td>-100</td><td>119.782</td><td>0.002</td><td>119.779</td><td>0.015</td><td>119.801</td><td>0.978</td><td>9.1</td></tr></tbody></table>
Appendix B: Oscillation frequencies

Table B.1 displays the oscillation frequencies of the RG component, as performed by co-authors Appourchaux and Mosser.

<table><caption>**Table B.1.** Oscillation frequencies of KIC 7955301 by co-authors Appourchaux and Mosser (COR method). The columns report $\nu_{as}$ as an asymptotic fit (µHz), $\nu_{obs}$ are the observed peak (µHz) with uncertainties, $nm$ is the proxy of the mixed order ($nm = np - ng$; 0 for p-modes), $zeta = zeta$ factor of mixed modes (Mosser+2015, 2018), and HBR is the height-to-background ratio.</caption><thead><tr><th rowspan="2">l</th><th rowspan="2">m</th><th rowspan="2">n</th><th rowspan="2">nm<sub>TA</sub></th><th rowspan="2">nm<sub>BM</sub></th><th colspan="2">Appourchaux</th><th colspan="4">Mosser</th></tr><tr><th>ν<sub>obs,TA</sub><br>μHz</th><th>err<br>μHz</th><th>ν<sub>obs,BM</sub><br>μHz</th><th>err<br>μHz</th><th>ν<sub>as</sub><br>μHz</th><th>ζ</th><th>HBR</th></tr></thead><tbody><tr><td>0</td><td>0</td><td>7</td><td>8</td><td>87</td><td>0.057</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>0</td><td>0</td><td>8</td><td>9</td><td>0</td><td>96.918</td><td>0.027</td><td>96.905</td><td>0.063</td><td>96.593</td><td>0.000</td><td>17.4</td></tr><tr><td>0</td><td>0</td><td>9</td><td>10</td><td>0</td><td>106.921</td><td>0.009</td><td>106.917</td><td>0.009</td><td>106.920</td><td>0.000</td><td>47.4</td></tr><tr><td>0</td><td>0</td><td>10</td><td>11</td><td>0</td><td>117.396</td><td>0.013</td><td>117.402</td><td>0.018</td><td>117.323</td><td>0.000</td><td>110.2</td></tr><tr><td>0</td><td>0</td><td>11</td><td>12</td><td>0</td><td>127.851</td><td>0.167</td><td>127.753</td><td>0.013</td><td>127.802</td><td>0.000</td><td>127.9</td></tr><tr><td>0</td><td>0</td><td>12</td><td>13</td><td>0</td><td>138.268</td><td>0.018</td><td>138.230</td><td>0.027</td><td>138.357</td><td>0.000</td><td>50.2</td></tr><tr><td>0</td><td>0</td><td>13</td><td>14</td><td>0</td><td>149.021</td><td>0.004</td><td>148.943</td><td>0.013</td><td>148.987</td><td>0.000</td><td>21.1</td></tr><tr><td>0</td><td>0</td><td>14</td><td>15</td><td>...</td><td>159.718</td><td>0.059</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>-1</td><td>...</td><td>-136</td><td>...</td><td>90.142</td><td>0.002</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>1</td><td>...</td><td>-132</td><td>...</td><td>92.323</td><td>0.022</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>-1</td><td>...</td><td>-132</td><td>...</td><td>92.626</td><td>0.052</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>1</td><td>8</td><td>...</td><td>-126</td><td>...</td><td>...</td><td>98.377</td><td>0.014</td><td>98.371</td><td>0.989</td><td>5.4</td></tr><tr><td>1</td><td>1</td><td>8</td><td>-120</td><td>...</td><td>101.235</td><td>0.004</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>-1</td><td>8</td><td>-120</td><td>-121</td><td>101.310</td><td>0.004</td><td>101.305</td><td>0.017</td><td>101.277</td><td>0.825</td><td>19.5</td></tr><tr><td>1</td><td>-1</td><td>8</td><td>-119</td><td>-120</td><td>101.874</td><td>0.006</td><td>101.880</td><td>0.026</td><td>101.831</td><td>0.614</td><td>64.9</td></tr><tr><td>1</td><td>1</td><td>8</td><td>-119</td><td>...</td><td>101.881</td><td>0.006</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>0</td><td>8</td><td>-119</td><td>...</td><td>102.112</td><td>0.001</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>1</td><td>8</td><td>-118</td><td>...</td><td>102.342</td><td>0.015</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>-1</td><td>8</td><td>-118</td><td>-119</td><td>102.401</td><td>0.006</td><td>102.391</td><td>0.011</td><td>102.390</td><td>0.825</td><td>14.5</td></tr><tr><td>1</td><td>-1</td><td>8</td><td>-117</td><td>...</td><td>103.061</td><td>0.002</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>1</td><td>8</td><td>-117</td><td>...</td><td>103.103</td><td>0.005</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>1</td><td>8</td><td>...</td><td>-118</td><td>...</td><td>...</td><td>103.840</td><td>0.014</td><td>103.853</td><td>0.973</td><td>7.3</td></tr><tr><td>1</td><td>-1</td><td>...</td><td>-113</td><td>...</td><td>106.245</td><td>0.000</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>1</td><td>...</td><td>-113</td><td>...</td><td>106.384</td><td>0.009</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>1</td><td>...</td><td>-112</td><td>...</td><td>107.164</td><td>0.012</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>-1</td><td>9</td><td>-110</td><td>-111</td><td>109.059</td><td>0.001</td><td>109.051</td><td>0.012</td><td>109.066</td><td>0.985</td><td>14.1</td></tr><tr><td>1</td><td>1</td><td>9</td><td>-109</td><td>-111</td><td>109.807</td><td>0.002</td><td>109.806</td><td>0.010</td><td>109.816</td><td>0.977</td><td>20.5</td></tr><tr><td>1</td><td>1</td><td>9</td><td>-108</td><td>-110</td><td>110.698</td><td>0.001</td><td>110.696</td><td>0.010</td><td>110.705</td><td>0.949</td><td>24.2</td></tr><tr><td>1</td><td>-1</td><td>9</td><td>-108</td><td>-109</td><td>110.863</td><td>0.002</td><td>110.837</td><td>0.021</td><td>110.868</td><td>0.938</td><td>5.6</td></tr><tr><td>1</td><td>1</td><td>9</td><td>...</td><td>-109</td><td>...</td><td>...</td><td>111.554</td><td>0.012</td><td>111.550</td><td>0.823</td><td>10.6</td></tr><tr><td>1</td><td>-1</td><td>9</td><td>-107</td><td>-108</td><td>111.717</td><td>0.001</td><td>111.719</td><td>0.016</td><td>111.693</td><td>0.770</td><td>34.8</td></tr><tr><td>1</td><td>1</td><td>9</td><td>-107</td><td>-108</td><td>112.305</td><td>0.013</td><td>112.254</td><td>0.035</td><td>112.188</td><td>0.567</td><td>59.1</td></tr><tr><td>1</td><td>-1</td><td>9</td><td>-106</td><td>-107</td><td>112.369</td><td>0.016</td><td>112.325</td><td>0.016</td><td>112.299</td><td>0.584</td><td>59.3</td></tr><tr><td>1</td><td>0</td><td>9</td><td>-118</td><td>-107</td><td>102.592</td><td>0.001</td><td>112.514</td><td>0.021</td><td>112.547</td><td>0.699</td><td>9.2</td></tr><tr><td>1</td><td>1</td><td>9</td><td>-106</td><td>-107</td><td>112.862</td><td>0.004</td><td>112.876</td><td>0.022</td><td>112.836</td><td>0.822</td><td>34.9</td></tr><tr><td>1</td><td>-1</td><td>9</td><td>-105</td><td>-106</td><td>113.013</td><td>0.011</td><td>113.041</td><td>0.016</td><td>113.014</td><td>0.870</td><td>26.1</td></tr><tr><td>1</td><td>1</td><td>9</td><td>-105</td><td>-106</td><td>113.699</td><td>0.010</td><td>113.703</td><td>0.012</td><td>113.718</td><td>0.949</td><td>20.3</td></tr><tr><td>1</td><td>-1</td><td>9</td><td>-104</td><td>-105</td><td>113.913</td><td>0.007</td><td>113.931</td><td>0.011</td><td>113.933</td><td>0.959</td><td>9.1</td></tr><tr><td>1</td><td>1</td><td>9</td><td>-104</td><td>-105</td><td>114.624</td><td>0.002</td><td>114.655</td><td>0.013</td><td>114.673</td><td>0.976</td><td>15.8</td></tr><tr><td>1</td><td>-1</td><td>9</td><td>...</td><td>-103</td><td>...</td><td>...</td><td>115.938</td><td>0.014</td><td>115.914</td><td>0.986</td><td>45.1</td></tr><tr><td>1</td><td>1</td><td>9</td><td>...</td><td>-103</td><td>...</td><td>...</td><td>116.647</td><td>0.017</td><td>116.668</td><td>0.988</td><td>6.1</td></tr><tr><td>1</td><td>-1</td><td>10</td><td>...</td><td>-102</td><td>...</td><td>...</td><td>116.953</td><td>0.011</td><td>116.941</td><td>0.988</td><td>14.6</td></tr><tr><td>1</td><td>-1</td><td>10</td><td>...</td><td>-101</td><td>...</td><td>...</td><td>117.977</td><td>0.015</td><td>117.988</td><td>0.988</td><td>5.2</td></tr><tr><td>1</td><td>1</td><td>10</td><td>...</td><td>-101</td><td>...</td><td>...</td><td>118.717</td><td>0.018</td><td>118.741</td><td>0.986</td><td>5.4</td></tr><tr><td>1</td><td>-1</td><td>10</td><td>-99</td><td>-100</td><td>119.028</td><td>0.002</td><td>119.032</td><td>0.013</td><td>119.051</td><td>0.984</td><td>31.0</td></tr><tr><td>1</td><td>1</td><td>10</td><td>-99</td><td>-100</td><td>119.782</td><td>0.002</td><td>119.779</td><td>0.015</td><td>119.801</td><td>0.978</td><td>9.1</td></tr></tbody></table>
<table><caption>**Table B.1.** continued.</caption><thead><tr><th rowspan="2">l</th><th rowspan="2">m</th><th rowspan="2">n</th><th rowspan="2">nm<sub>TA</sub></th><th rowspan="2">nm<sub>BM</sub></th><th colspan="2">Appourchaux</th><th colspan="4">Mosser</th></tr><tr><th>ν<sub>obs,TA</sub><br>μHz</th><th>err<br>μHz</th><th>ν<sub>obs,BM</sub><br>μHz</th><th>err<br>μHz</th><th>ν<sub>as</sub><br>μHz</th><th>ζ</th><th>HBR</th></tr></thead><tbody><tr><td>1</td><td>-1</td><td>10</td><td>...</td><td>-99</td><td>...</td><td>...</td><td>120.157</td><td>0.019</td><td>120.127</td><td>0.974</td><td>9.3</td></tr><tr><td>1</td><td>1</td><td>10</td><td>-98</td><td>-99</td><td>120.854</td><td>0.003</td><td>120.858</td><td>0.010</td><td>120.864</td><td>0.954</td><td>21.1</td></tr><tr><td>1</td><td>-1</td><td>10</td><td>-97</td><td>-98</td><td>121.186</td><td>0.008</td><td>121.180</td><td>0.015</td><td>121.199</td><td>0.935</td><td>7.1</td></tr><tr><td>1</td><td>0</td><td>10</td><td>...</td><td>-98</td><td>...</td><td>...</td><td>121.558</td><td>0.014</td><td>121.549</td><td>0.899</td><td>6.3</td></tr><tr><td>1</td><td>1</td><td>10</td><td>-97</td><td>-98</td><td>121.893</td><td>0.004</td><td>121.897</td><td>0.011</td><td>121.881</td><td>0.831</td><td>94.6</td></tr><tr><td>1</td><td>-1</td><td>10</td><td>-96</td><td>-97</td><td>122.198</td><td>0.004</td><td>122.196</td><td>0.015</td><td>122.170</td><td>0.717</td><td>110.0</td></tr><tr><td>1</td><td>0</td><td>10</td><td>...</td><td>-97</td><td>...</td><td>...</td><td>122.385</td><td>0.020</td><td>122.417</td><td>0.586</td><td>25.2</td></tr><tr><td>1</td><td>1</td><td>10</td><td>-96</td><td>-97</td><td>122.695</td><td>0.007</td><td>122.708</td><td>0.044</td><td>122.622</td><td>0.523</td><td>275.3</td></tr><tr><td>1</td><td>-1</td><td>10</td><td>-95</td><td>...</td><td>122.891</td><td>0.009</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>0</td><td>10</td><td>...</td><td>-96</td><td>...</td><td>...</td><td>123.030</td><td>0.027</td><td>123.078</td><td>0.707</td><td>15.7</td></tr><tr><td>1</td><td>1</td><td>10</td><td>-95</td><td>-96</td><td>123.394</td><td>0.000</td><td>123.384</td><td>0.012</td><td>123.369</td><td>0.823</td><td>45.7</td></tr><tr><td>1</td><td>-1</td><td>10</td><td>-94</td><td>-95</td><td>123.685</td><td>0.022</td><td>123.723</td><td>0.009</td><td>123.721</td><td>0.897</td><td>35.3</td></tr><tr><td>1</td><td>0</td><td>10</td><td>-94</td><td>-95</td><td>124.054</td><td>0.006</td><td>124.054</td><td>0.013</td><td>124.069</td><td>0.933</td><td>14.4</td></tr><tr><td>1</td><td>1</td><td>10</td><td>-94</td><td>-95</td><td>124.409</td><td>0.001</td><td>124.416</td><td>0.010</td><td>124.430</td><td>0.953</td><td>72.8</td></tr><tr><td>1</td><td>-1</td><td>10</td><td>-93</td><td>-94</td><td>124.812</td><td>0.001</td><td>124.809</td><td>0.015</td><td>124.834</td><td>0.966</td><td>28.1</td></tr><tr><td>1</td><td>0</td><td>10</td><td>...</td><td>-94</td><td>...</td><td>...</td><td>125.187</td><td>0.017</td><td>125.204</td><td>0.973</td><td>5.1</td></tr><tr><td>1</td><td>1</td><td>10</td><td>-93</td><td>-94</td><td>125.555</td><td>0.007</td><td>125.557</td><td>0.014</td><td>125.577</td><td>0.978</td><td>15.7</td></tr><tr><td>1</td><td>-1</td><td>10</td><td>...</td><td>-93</td><td>...</td><td>...</td><td>125.982</td><td>0.018</td><td>126.011</td><td>0.981</td><td>10.8</td></tr><tr><td>1</td><td>-1</td><td>10</td><td>-91</td><td>-92</td><td>127.197</td><td>0.002</td><td>127.194</td><td>0.016</td><td>127.221</td><td>0.986</td><td>30.5</td></tr><tr><td>1</td><td>0</td><td>10</td><td>...</td><td>-92</td><td>...</td><td>...</td><td>127.627</td><td>0.017</td><td>127.598</td><td>0.986</td><td>40.7</td></tr><tr><td>1</td><td>1</td><td>11</td><td>...</td><td>-91</td><td>...</td><td>...</td><td>129.217</td><td>0.010</td><td>129.209</td><td>0.983</td><td>16.2</td></tr><tr><td>1</td><td>-1</td><td>11</td><td>-89</td><td>-90</td><td>129.760</td><td>0.051</td><td>129.689</td><td>0.015</td><td>129.714</td><td>0.980</td><td>28.7</td></tr><tr><td>1</td><td>0</td><td>11</td><td>-89</td><td>...</td><td>129.919</td><td>0.000</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>1</td><td>11</td><td>-89</td><td>-90</td><td>130.442</td><td>0.002</td><td>130.437</td><td>0.014</td><td>130.460</td><td>0.972</td><td>33.4</td></tr><tr><td>1</td><td>-1</td><td>11</td><td>-88</td><td>-89</td><td>130.954</td><td>0.005</td><td>130.957</td><td>0.016</td><td>130.982</td><td>0.961</td><td>16.4</td></tr><tr><td>1</td><td>1</td><td>11</td><td>-88</td><td>-89</td><td>131.653</td><td>0.026</td><td>131.697</td><td>0.012</td><td>131.704</td><td>0.924</td><td>9.5</td></tr><tr><td>1</td><td>-1</td><td>11</td><td>-87</td><td>-88</td><td>132.191</td><td>0.001</td><td>132.193</td><td>0.013</td><td>132.212</td><td>0.854</td><td>101.6</td></tr><tr><td>1</td><td>0</td><td>11</td><td>-87</td><td>-88</td><td>132.850</td><td>0.024</td><td>132.531</td><td>0.015</td><td>132.518</td><td>0.760</td><td>7.4</td></tr><tr><td>1</td><td>1</td><td>11</td><td>-87</td><td>-88</td><td>132.800</td><td>0.009</td><td>132.807</td><td>0.014</td><td>132.785</td><td>0.628</td><td>114.0</td></tr><tr><td>1</td><td>-1</td><td>11</td><td>-86</td><td>-87</td><td>133.083</td><td>0.017</td><td>133.051</td><td>0.025</td><td>133.095</td><td>0.486</td><td>27.4</td></tr><tr><td>1</td><td>0</td><td>11</td><td>...</td><td>-87</td><td>...</td><td>...</td><td>133.137</td><td>0.075</td><td>133.286</td><td>0.509</td><td>22.9</td></tr><tr><td>1</td><td>1</td><td>11</td><td>-86</td><td>-87</td><td>133.524</td><td>0.030</td><td>133.523</td><td>0.017</td><td>133.494</td><td>0.613</td><td>71.9</td></tr><tr><td>1</td><td>-1</td><td>11</td><td>-85</td><td>-86</td><td>133.923</td><td>0.001</td><td>133.924</td><td>0.010</td><td>133.934</td><td>0.811</td><td>101.8</td></tr><tr><td>1</td><td>1</td><td>11</td><td>-85</td><td>-86</td><td>134.598</td><td>0.003</td><td>134.593</td><td>0.011</td><td>134.608</td><td>0.923</td><td>66.9</td></tr><tr><td>1</td><td>-1</td><td>11</td><td>-84</td><td>-85</td><td>135.179</td><td>0.004</td><td>135.176</td><td>0.014</td><td>135.191</td><td>0.955</td><td>9.3</td></tr><tr><td>1</td><td>1</td><td>11</td><td>...</td><td>-85</td><td>...</td><td>...</td><td>135.924</td><td>0.010</td><td>135.928</td><td>0.972</td><td>11.9</td></tr><tr><td>1</td><td>1</td><td>1</td><td>-83</td><td>...</td><td>137.527</td><td>0.003</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>-1</td><td>1</td><td>-82</td><td>...</td><td>137.917</td><td>0.409</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>1</td><td>12</td><td>-82</td><td>-83</td><td>138.722</td><td>0.003</td><td>138.718</td><td>0.014</td><td>138.733</td><td>0.983</td><td>8.5</td></tr><tr><td>1</td><td>-1</td><td>12</td><td>-81</td><td>-82</td><td>139.410</td><td>0.004</td><td>139.411</td><td>0.015</td><td>139.432</td><td>0.982</td><td>12.3</td></tr><tr><td>1</td><td>-1</td><td>12</td><td>-80</td><td>-81</td><td>140.891</td><td>0.002</td><td>140.890</td><td>0.012</td><td>140.905</td><td>0.970</td><td>18.0</td></tr><tr><td>1</td><td>0</td><td>12</td><td>...</td><td>-81</td><td>...</td><td>...</td><td>141.292</td><td>0.016</td><td>141.274</td><td>0.963</td><td>6.1</td></tr></tbody></table>
<table><caption>**Table B.1.** continued.</caption><thead><tr><th rowspan="2">l</th><th rowspan="2">m</th><th rowspan="2">n</th><th rowspan="2">nm<sub>TA</sub></th><th rowspan="2">nm<sub>BM</sub></th><th colspan="2">Appourchaux</th><th colspan="4">Mosser</th></tr><tr><th>ν<sub>obs,TA</sub><br>μHz</th><th>err<br>μHz</th><th>ν<sub>obs,BM</sub><br>μHz</th><th>err<br>μHz</th><th>ν<sub>as</sub><br>μHz</th><th>ζ</th><th>HBR</th></tr></thead><tbody><tr><td>1</td><td>-1</td><td>10</td><td>...</td><td>-99</td><td>...</td><td>...</td><td>120.157</td><td>0.019</td><td>120.127</td><td>0.974</td><td>9.3</td></tr><tr><td>1</td><td>1</td><td>10</td><td>-98</td><td>-99</td><td>120.854</td><td>0.003</td><td>120.858</td><td>0.010</td><td>120.864</td><td>0.954</td><td>21.1</td></tr><tr><td>1</td><td>-1</td><td>10</td><td>-97</td><td>-98</td><td>121.186</td><td>0.008</td><td>121.180</td><td>0.015</td><td>121.199</td><td>0.935</td><td>7.1</td></tr><tr><td>1</td><td>0</td><td>10</td><td>...</td><td>-98</td><td>...</td><td>...</td><td>121.558</td><td>0.014</td><td>121.549</td><td>0.899</td><td>6.3</td></tr><tr><td>1</td><td>1</td><td>10</td><td>-97</td><td>-98</td><td>121.893</td><td>0.004</td><td>121.897</td><td>0.011</td><td>121.881</td><td>0.831</td><td>94.6</td></tr><tr><td>1</td><td>-1</td><td>10</td><td>-96</td><td>-97</td><td>122.198</td><td>0.004</td><td>122.196</td><td>0.015</td><td>122.170</td><td>0.717</td><td>110.0</td></tr><tr><td>1</td><td>0</td><td>10</td><td>...</td><td>-97</td><td>...</td><td>...</td><td>122.385</td><td>0.020</td><td>122.417</td><td>0.586</td><td>25.2</td></tr><tr><td>1</td><td>1</td><td>10</td><td>-96</td><td>-97</td><td>122.695</td><td>0.007</td><td>122.708</td><td>0.044</td><td>122.622</td><td>0.523</td><td>275.3</td></tr><tr><td>1</td><td>-1</td><td>10</td><td>-95</td><td>...</td><td>122.891</td><td>0.009</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>0</td><td>10</td><td>...</td><td>-96</td><td>...</td><td>...</td><td>123.030</td><td>0.027</td><td>123.078</td><td>0.707</td><td>15.7</td></tr><tr><td>1</td><td>1</td><td>10</td><td>-95</td><td>-96</td><td>123.394</td><td>0.000</td><td>123.384</td><td>0.012</td><td>123.369</td><td>0.823</td><td>45.7</td></tr><tr><td>1</td><td>-1</td><td>10</td><td>-94</td><td>-95</td><td>123.685</td><td>0.022</td><td>123.723</td><td>0.009</td><td>123.721</td><td>0.897</td><td>35.3</td></tr><tr><td>1</td><td>0</td><td>10</td><td>-94</td><td>-95</td><td>124.054</td><td>0.006</td><td>124.054</td><td>0.013</td><td>124.069</td><td>0.933</td><td>14.4</td></tr><tr><td>1</td><td>1</td><td>10</td><td>-94</td><td>-95</td><td>124.409</td><td>0.001</td><td>124.416</td><td>0.010</td><td>124.430</td><td>0.953</td><td>72.8</td></tr><tr><td>1</td><td>-1</td><td>10</td><td>-93</td><td>-94</td><td>124.812</td><td>0.001</td><td>124.809</td><td>0.015</td><td>124.834</td><td>0.966</td><td>28.1</td></tr><tr><td>1</td><td>0</td><td>10</td><td>...</td><td>-94</td><td>...</td><td>...</td><td>125.187</td><td>0.017</td><td>125.204</td><td>0.973</td><td>5.1</td></tr><tr><td>1</td><td>1</td><td>10</td><td>-93</td><td>-94</td><td>125.555</td><td>0.007</td><td>125.557</td><td>0.014</td><td>125.577</td><td>0.978</td><td>15.7</td></tr><tr><td>1</td><td>-1</td><td>10</td><td>...</td><td>-93</td><td>...</td><td>...</td><td>125.982</td><td>0.018</td><td>126.011</td><td>0.981</td><td>10.8</td></tr><tr><td>1</td><td>-1</td><td>10</td><td>-91</td><td>-92</td><td>127.197</td><td>0.002</td><td>127.194</td><td>0.016</td><td>127.221</td><td>0.986</td><td>30.5</td></tr><tr><td>1</td><td>0</td><td>10</td><td>...</td><td>-92</td><td>...</td><td>...</td><td>127.627</td><td>0.017</td><td>127.598</td><td>0.986</td><td>40.7</td></tr><tr><td>1</td><td>1</td><td>11</td><td>...</td><td>-91</td><td>...</td><td>...</td><td>129.217</td><td>0.010</td><td>129.209</td><td>0.983</td><td>16.2</td></tr><tr><td>1</td><td>-1</td><td>11</td><td>-89</td><td>-90</td><td>129.760</td><td>0.051</td><td>129.689</td><td>0.015</td><td>129.714</td><td>0.980</td><td>28.7</td></tr><tr><td>1</td><td>0</td><td>11</td><td>-89</td><td>...</td><td>129.919</td><td>0.000</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>1</td><td>11</td><td>-89</td><td>-90</td><td>130.442</td><td>0.002</td><td>130.437</td><td>0.014</td><td>130.460</td><td>0.972</td><td>33.4</td></tr><tr><td>1</td><td>-1</td><td>11</td><td>-88</td><td>-89</td><td>130.954</td><td>0.005</td><td>130.957</td><td>0.016</td><td>130.982</td><td>0.961</td><td>16.4</td></tr><tr><td>1</td><td>1</td><td>11</td><td>-88</td><td>-89</td><td>131.653</td><td>0.026</td><td>131.697</td><td>0.012</td><td>131.704</td><td>0.924</td><td>9.5</td></tr><tr><td>1</td><td>-1</td><td>11</td><td>-87</td><td>-88</td><td>132.191</td><td>0.001</td><td>132.193</td><td>0.013</td><td>132.212</td><td>0.854</td><td>101.6</td></tr><tr><td>1</td><td>0</td><td>11</td><td>-87</td><td>-88</td><td>132.850</td><td>0.024</td><td>132.531</td><td>0.015</td><td>132.518</td><td>0.760</td><td>7.4</td></tr><tr><td>1</td><td>1</td><td>11</td><td>-87</td><td>-88</td><td>132.800</td><td>0.009</td><td>132.807</td><td>0.014</td><td>132.785</td><td>0.628</td><td>114.0</td></tr><tr><td>1</td><td>-1</td><td>11</td><td>-86</td><td>-87</td><td>133.083</td><td>0.017</td><td>133.051</td><td>0.025</td><td>133.095</td><td>0.486</td><td>27.4</td></tr><tr><td>1</td><td>0</td><td>11</td><td>...</td><td>-87</td><td>...</td><td>...</td><td>133.137</td><td>0.075</td><td>133.286</td><td>0.509</td><td>22.9</td></tr><tr><td>1</td><td>1</td><td>11</td><td>-86</td><td>-87</td><td>133.524</td><td>0.030</td><td>133.523</td><td>0.017</td><td>133.494</td><td>0.613</td><td>71.9</td></tr><tr><td>1</td><td>-1</td><td>11</td><td>-85</td><td>-86</td><td>133.923</td><td>0.001</td><td>133.924</td><td>0.010</td><td>133.934</td><td>0.811</td><td>101.8</td></tr><tr><td>1</td><td>1</td><td>11</td><td>-85</td><td>-86</td><td>134.598</td><td>0.003</td><td>134.593</td><td>0.011</td><td>134.608</td><td>0.923</td><td>66.9</td></tr><tr><td>1</td><td>-1</td><td>11</td><td>-84</td><td>-85</td><td>135.179</td><td>0.004</td><td>135.176</td><td>0.014</td><td>135.191</td><td>0.955</td><td>9.3</td></tr><tr><td>1</td><td>1</td><td>11</td><td>...</td><td>-85</td><td>...</td><td>...</td><td>135.924</td><td>0.010</td><td>135.928</td><td>0.972</td><td>11.9</td></tr><tr><td>1</td><td>1</td><td>1</td><td>-83</td><td>...</td><td>137.527</td><td>0.003</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>-1</td><td>1</td><td>-82</td><td>...</td><td>137.917</td><td>0.409</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1</td><td>1</td><td>12</td><td>-82</td><td>-83</td><td>138.722</td><td>0.003</td><td>138.718</td><td>0.014</td><td>138.733</td><td>0.983</td><td>8.5</td></tr><tr><td>1</td><td>-1</td><td>12</td><td>-81</td><td>-82</td><td>139.410</td><td>0.004</td><td>139.411</td><td>0.015</td><td>139.432</td><td>0.982</td><td>12.3</td></tr><tr><td>1</td><td>-1</td><td>12</td><td>-80</td><td>-81</td><td>140.891</td><td>0.002</td><td>140.890</td><td>0.012</td><td>140.905</td><td>0.970</td><td>18.0</td></tr><tr><td>1</td><td>0</td><td>12</td><td>...</td><td>-81</td><td>...</td><td>...</td><td>141.292</td><td>0.016</td><td>141.274</td><td>0.963</td><td>6.1</td></tr></tbody></table>
<table><caption>**Table B.1.** continued.</caption><thead><tr><th rowspan="2">l</th><th rowspan="2">m</th><th rowspan="2">n</th><th rowspan="2">nm<sub>TA</sub></th><th rowspan="2">nm<sub>BM</sub></th><th colspan="2">Appourchaux</th><th colspan="4">Mosser</th></tr><tr><th>ν<sub>obs,TA</sub><br>μHz</th><th>err<br>μHz</th><th>ν<sub>obs,BM</sub><br>μHz</th><th>err<br>μHz</th><th>ν<sub>as</sub><br>μHz</th><th>ζ</th><th>HBR</th></tr></thead><tbody><tr><td>1</td><td>-1</td><td>12</td><td>-79</td><td>-80</td><td>142.366</td><td>0.007</td><td>142.362</td><td>0.014</td><td>142.356</td><td>0.906</td><td>5.7</td></tr><tr><td>1</td><td>1</td><td>12</td><td>-79</td><td>-80</td><td>143.050</td><td>0.024</td><td>142.984</td><td>0.018</td><td>143.008</td><td>0.770</td><td>8.7</td></tr><tr><td>1</td><td>-1</td><td>12</td><td>-78</td><td>-79</td><td>143.555</td><td>0.099</td><td>143.527</td><td>0.014</td><td>143.515</td><td>0.512</td><td>18.1</td></tr><tr><td>1</td><td>0</td><td>12</td><td>...</td><td>-79</td><td>...</td><td>...</td><td>143.527</td><td>0.087</td><td>143.698</td><td>0.447</td><td>18.1</td></tr><tr><td>1</td><td>1</td><td>12</td><td>-78</td><td>-79</td><td>143.940</td><td>0.003</td><td>143.882</td><td>0.013</td><td>143.874</td><td>0.469</td><td>21.5</td></tr><tr><td>1</td><td>-1</td><td>12</td><td>-77</td><td>-78</td><td>144.373</td><td>0.001</td><td>144.362</td><td>0.011</td><td>144.351</td><td>0.719</td><td>26.7</td></tr><tr><td>1</td><td>0</td><td>12</td><td>...</td><td>-78</td><td>...</td><td>...</td><td>144.661</td><td>0.014</td><td>144.643</td><td>0.820</td><td>14.1</td></tr><tr><td>1</td><td>1</td><td>12</td><td>-77</td><td>-78</td><td>144.972</td><td>0.002</td><td>144.968</td><td>0.012</td><td>144.963</td><td>0.882</td><td>8.9</td></tr><tr><td>1</td><td>-1</td><td>12</td><td>...</td><td>-76</td><td>...</td><td>...</td><td>147.329</td><td>0.013</td><td>147.339</td><td>0.976</td><td>7.8</td></tr><tr><td>1</td><td>1</td><td>12</td><td>...</td><td>-76</td><td>...</td><td>...</td><td>148.101</td><td>0.013</td><td>148.086</td><td>0.980</td><td>11.5</td></tr><tr><td>1</td><td>0</td><td>13</td><td>...</td><td>-75</td><td>...</td><td>...</td><td>149.337</td><td>0.019</td><td>149.362</td><td>0.981</td><td>5.0</td></tr><tr><td>1</td><td>1</td><td>13</td><td>...</td><td>-75</td><td>...</td><td>...</td><td>149.754</td><td>0.014</td><td>149.736</td><td>0.980</td><td>8.8</td></tr><tr><td>1</td><td>0</td><td>13</td><td>...</td><td>-74</td><td>...</td><td>...</td><td>151.029</td><td>0.015</td><td>151.044</td><td>0.972</td><td>6.1</td></tr><tr><td>1</td><td>1</td><td>13</td><td>...</td><td>-74</td><td>...</td><td>...</td><td>151.407</td><td>0.013</td><td>151.415</td><td>0.968</td><td>7.5</td></tr><tr><td>1</td><td>-1</td><td>13</td><td>...</td><td>-72</td><td>...</td><td>...</td><td>153.902</td><td>0.017</td><td>153.879</td><td>0.647</td><td>13.8</td></tr><tr><td>1</td><td>0</td><td>13</td><td>-71</td><td>-72</td><td>153.925</td><td>0.010</td><td>154.185</td><td>0.046</td><td>154.102</td><td>0.518</td><td>5.8</td></tr><tr><td>1</td><td>1</td><td>13</td><td>...</td><td>-72</td><td>...</td><td>...</td><td>154.398</td><td>0.060</td><td>154.283</td><td>0.431</td><td>7.9</td></tr><tr><td>1</td><td>-1</td><td>13</td><td>...</td><td>-71</td><td>...</td><td>...</td><td>154.823</td><td>0.040</td><td>154.750</td><td>0.539</td><td>7.8</td></tr><tr><td>1</td><td>0</td><td>13</td><td>...</td><td>-71</td><td>...</td><td>...</td><td>155.020</td><td>0.026</td><td>155.979</td><td>0.666</td><td>5.6</td></tr><tr><td>1</td><td>1</td><td>13</td><td>...</td><td>-71</td><td>...</td><td>...</td><td>155.272</td><td>0.018</td><td>155.254</td><td>0.779</td><td>5.1</td></tr><tr><td>2</td><td>0</td><td>6</td><td>7</td><td>...</td><td>85.387</td><td>0.120</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>2</td><td>0</td><td>7</td><td>8</td><td>0</td><td>95.395</td><td>0.036</td><td>95.449</td><td>0.135</td><td>94.778</td><td>0.000</td><td>8.4</td></tr><tr><td>2</td><td>0</td><td>8</td><td>9</td><td>0</td><td>105.537</td><td>0.026</td><td>105.579</td><td>0.095</td><td>105.106</td><td>0.000</td><td>14.0</td></tr><tr><td>2</td><td>0</td><td>9</td><td>10</td><td>0</td><td>116.058</td><td>0.004</td><td>116.072</td><td>0.112</td><td>115.512</td><td>0.000</td><td>95.1</td></tr><tr><td>2</td><td>0</td><td>10</td><td>11</td><td>0</td><td>126.474</td><td>0.018</td><td>126.462</td><td>0.095</td><td>125.988</td><td>0.000</td><td>68.9</td></tr><tr><td>2</td><td>0</td><td>11</td><td>12</td><td>0</td><td>136.935</td><td>0.028</td><td>136.986</td><td>0.089</td><td>136.544</td><td>0.000</td><td>34.0</td></tr><tr><td>2</td><td>0</td><td>12</td><td>13</td><td>0</td><td>147.637</td><td>0.035</td><td>147.676</td><td>0.102</td><td>147.170</td><td>0.000</td><td>22.7</td></tr><tr><td>2</td><td>0</td><td>13</td><td>14</td><td>...</td><td>158.462</td><td>0.099</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>3</td><td>0</td><td>9</td><td>9</td><td>...</td><td>119.568</td><td>0.098</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>3</td><td>0</td><td>10</td><td>10</td><td>...</td><td>130.013</td><td>0.026</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr></tbody></table>
<table><caption>Table B.1. continued.</caption><thead><tr><th rowspan="2">l</th><th rowspan="2">m</th><th rowspan="2">n</th><th rowspan="2">nm<sub>TA</sub></th><th rowspan="2">nm<sub>BM</sub></th><th colspan="2">Appourchaux</th><th colspan="4">Mosser</th></tr><tr><th>ν<sub>obs,TA</sub><br>μHz</th><th>err<br>μHz</th><th>ν<sub>obs,BM</sub><br>μHz</th><th>err<br>μHz</th><th>ν<sub>as</sub><br>μHz</th><th>ζ</th><th>HBR</th></tr></thead><tbody><tr><td>1</td><td>-1</td><td>12</td><td>-79</td><td>-80</td><td>142.366</td><td>0.007</td><td>142.362</td><td>0.014</td><td>142.356</td><td>0.906</td><td>5.7</td></tr><tr><td>1</td><td>1</td><td>12</td><td>-79</td><td>-80</td><td>143.050</td><td>0.024</td><td>142.984</td><td>0.018</td><td>143.008</td><td>0.770</td><td>8.7</td></tr><tr><td>1</td><td>-1</td><td>12</td><td>-78</td><td>-79</td><td>143.555</td><td>0.099</td><td>143.527</td><td>0.014</td><td>143.515</td><td>0.512</td><td>18.1</td></tr><tr><td>1</td><td>0</td><td>12</td><td>...</td><td>-79</td><td>...</td><td>...</td><td>143.527</td><td>0.087</td><td>143.698</td><td>0.447</td><td>18.1</td></tr><tr><td>1</td><td>1</td><td>12</td><td>-78</td><td>-79</td><td>143.940</td><td>0.003</td><td>143.882</td><td>0.013</td><td>143.874</td><td>0.469</td><td>21.5</td></tr><tr><td>1</td><td>-1</td><td>12</td><td>-77</td><td>-78</td><td>144.373</td><td>0.001</td><td>144.362</td><td>0.011</td><td>144.351</td><td>0.719</td><td>26.7</td></tr><tr><td>1</td><td>0</td><td>12</td><td>...</td><td>-78</td><td>...</td><td>...</td><td>144.661</td><td>0.014</td><td>144.643</td><td>0.820</td><td>14.1</td></tr><tr><td>1</td><td>1</td><td>12</td><td>-77</td><td>-78</td><td>144.972</td><td>0.002</td><td>144.968</td><td>0.012</td><td>144.963</td><td>0.882</td><td>8.9</td></tr><tr><td>1</td><td>-1</td><td>12</td><td>...</td><td>-76</td><td>...</td><td>...</td><td>147.329</td><td>0.013</td><td>147.339</td><td>0.976</td><td>7.8</td></tr><tr><td>1</td><td>1</td><td>12</td><td>...</td><td>-76</td><td>...</td><td>...</td><td>148.101</td><td>0.013</td><td>148.086</td><td>0.980</td><td>11.5</td></tr><tr><td>1</td><td>0</td><td>13</td><td>...</td><td>-75</td><td>...</td><td>...</td><td>149.337</td><td>0.019</td><td>149.362</td><td>0.981</td><td>5.0</td></tr><tr><td>1</td><td>1</td><td>13</td><td>...</td><td>-75</td><td>...</td><td>...</td><td>149.754</td><td>0.014</td><td>149.736</td><td>0.980</td><td>8.8</td></tr><tr><td>1</td><td>0</td><td>13</td><td>...</td><td>-74</td><td>...</td><td>...</td><td>151.029</td><td>0.015</td><td>151.044</td><td>0.972</td><td>6.1</td></tr><tr><td>1</td><td>1</td><td>13</td><td>...</td><td>-74</td><td>...</td><td>...</td><td>151.407</td><td>0.013</td><td>151.415</td><td>0.968</td><td>7.5</td></tr><tr><td>1</td><td>-1</td><td>13</td><td>...</td><td>-72</td><td>...</td><td>...</td><td>153.902</td><td>0.017</td><td>153.879</td><td>0.647</td><td>13.8</td></tr><tr><td>1</td><td>0</td><td>13</td><td>-71</td><td>-72</td><td>153.925</td><td>0.010</td><td>154.185</td><td>0.046</td><td>154.102</td><td>0.518</td><td>5.8</td></tr><tr><td>1</td><td>1</td><td>13</td><td>...</td><td>-72</td><td>...</td><td>...</td><td>154.398</td><td>0.060</td><td>154.283</td><td>0.431</td><td>7.9</td></tr><tr><td>1</td><td>-1</td><td>13</td><td>...</td><td>-71</td><td>...</td><td>...</td><td>154.823</td><td>0.040</td><td>154.750</td><td>0.539</td><td>7.8</td></tr><tr><td>1</td><td>0</td><td>13</td><td>...</td><td>-71</td><td>...</td><td>...</td><td>155.020</td><td>0.026</td><td>155.979</td><td>0.666</td><td>5.6</td></tr><tr><td>1</td><td>1</td><td>13</td><td>...</td><td>-71</td><td>...</td><td>...</td><td>155.272</td><td>0.018</td><td>155.254</td><td>0.779</td><td>5.1</td></tr><tr><td>2</td><td>0</td><td>6</td><td>7</td><td>...</td><td>85.387</td><td>0.120</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>2</td><td>0</td><td>7</td><td>8</td><td>0</td><td>95.395</td><td>0.036</td><td>95.449</td><td>0.135</td><td>94.778</td><td>0.000</td><td>8.4</td></tr><tr><td>2</td><td>0</td><td>8</td><td>9</td><td>0</td><td>105.537</td><td>0.026</td><td>105.579</td><td>0.095</td><td>105.106</td><td>0.000</td><td>14.0</td></tr><tr><td>2</td><td>0</td><td>9</td><td>10</td><td>0</td><td>116.058</td><td>0.004</td><td>116.072</td><td>0.112</td><td>115.512</td><td>0.000</td><td>95.1</td></tr><tr><td>2</td><td>0</td><td>10</td><td>11</td><td>0</td><td>126.474</td><td>0.018</td><td>126.462</td><td>0.095</td><td>125.988</td><td>0.000</td><td>68.9</td></tr><tr><td>2</td><td>0</td><td>11</td><td>12</td><td>0</td><td>136.935</td><td>0.028</td><td>136.986</td><td>0.089</td><td>136.544</td><td>0.000</td><td>34.0</td></tr><tr><td>2</td><td>0</td><td>12</td><td>13</td><td>0</td><td>147.637</td><td>0.035</td><td>147.676</td><td>0.102</td><td>147.170</td><td>0.000</td><td>22.7</td></tr><tr><td>2</td><td>0</td><td>13</td><td>14</td><td>...</td><td>158.462</td><td>0.099</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>3</td><td>0</td><td>9</td><td>9</td><td>...</td><td>119.568</td><td>0.098</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>3</td><td>0</td><td>10</td><td>10</td><td>...</td><td>130.013</td><td>0.026</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr></tbody></table>
## Appendix C: Eclipse properties

Table C.1 presents the eclipses properties obtained with the LIGHTCURVEFACTORY.

<table><caption>**Table C.1.** Eclipse properties.</caption><thead><tr><th>n</th><th>t<sub>1</sub><br>(KJD)</th><th>O<sub>1</sub> - nP - t<sub>0</sub><br>day</th><th>D<sub>1</sub><br>%</th><th>W<sub>1</sub><br>hour</th><th>t<sub>2</sub><br>(KJD)</th><th>O<sub>2</sub> - nP - t<sub>0</sub><br>day</th><th>D<sub>2</sub><br>%</th><th>W<sub>2</sub><br>hour</th></tr></thead><tbody><tr><td>8</td><td>127.4560</td><td>4.4034</td><td>-0.55</td><td>2.10</td><td>134.9905</td><td>11.9379</td><td>-0.50</td><td>2.24</td></tr><tr><td>9</td><td>142.8022</td><td>4.3911</td><td>-0.52</td><td>2.15</td><td>150.3368</td><td>11.9121</td><td>-0.51</td><td>2.20</td></tr><tr><td>10</td><td>158.1280</td><td>4.3778</td><td>-0.53</td><td>2.32</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>11</td><td>174.1688</td><td>4.3612</td><td>-0.62</td><td>2.48</td><td>181.7034</td><td>11.8727</td><td>-0.66</td><td>2.18</td></tr><tr><td>12</td><td>188.7792</td><td>4.3464</td><td>-0.65</td><td>2.38</td><td>196.3137</td><td>11.8560</td><td>-0.72</td><td>2.39</td></tr><tr><td>13</td><td>204.1046</td><td>4.3251</td><td>-0.77</td><td>2.31</td><td>211.6391</td><td>11.8481</td><td>-0.88</td><td>2.53</td></tr><tr><td>14</td><td>219.4298</td><td>4.3058</td><td>-0.84</td><td>2.40</td><td>226.9644</td><td>11.8495</td><td>-0.96</td><td>2.57</td></tr><tr><td>15</td><td>235.7970</td><td>4.3025</td><td>-0.87</td><td>2.40</td><td>243.3315</td><td>11.8809</td><td>-0.91</td><td>2.48</td></tr><tr><td>16</td><td>250.0798</td><td>4.4026</td><td>-0.89</td><td>2.43</td><td>257.6144</td><td>11.9343</td><td>-1.01</td><td>2.57</td></tr><tr><td>17</td><td>265.4046</td><td>4.4707</td><td>-1.15</td><td>2.67</td><td>272.9391</td><td>11.9343</td><td>-1.39</td><td>2.78</td></tr><tr><td>18</td><td>...</td><td>...</td><td>...</td><td>...</td><td>288.2638</td><td>11.9523</td><td>-1.56</td><td>2.69</td></tr><tr><td>19</td><td>296.0539</td><td>4.4538</td><td>-1.38</td><td>2.67</td><td>303.5884</td><td>11.9615</td><td>-1.62</td><td>2.71</td></tr><tr><td>20</td><td>311.3988</td><td>4.4533</td><td>-1.38</td><td>2.79</td><td>318.9334</td><td>11.9532</td><td>-1.58</td><td>2.80</td></tr><tr><td>21</td><td>327.9493</td><td>4.4437</td><td>-1.40</td><td>2.79</td><td>335.4839</td><td>11.9355</td><td>-1.53</td><td>2.81</td></tr><tr><td>22</td><td>342.0480</td><td>4.4350</td><td>-1.35</td><td>2.71</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>23</td><td>357.3727</td><td>4.4217</td><td>-1.42</td><td>2.63</td><td>364.9072</td><td>11.8882</td><td>-1.68</td><td>2.79</td></tr><tr><td>24</td><td>372.6975</td><td>4.4051</td><td>-1.39</td><td>2.55</td><td>380.2320</td><td>11.8657</td><td>-1.71</td><td>2.70</td></tr><tr><td>25</td><td>388.7172</td><td>4.3921</td><td>-1.52</td><td>2.81</td><td>396.2517</td><td>11.8462</td><td>-1.81</td><td>2.79</td></tr><tr><td>26</td><td>405.2275</td><td>4.3752</td><td>-1.60</td><td>2.75</td><td>412.7621</td><td>11.8327</td><td>-1.93</td><td>2.87</td></tr><tr><td>27</td><td>418.6730</td><td>4.3593</td><td>-1.64</td><td>2.70</td><td>426.2075</td><td>11.8260</td><td>-2.04</td><td>2.79</td></tr><tr><td>28</td><td>433.9985</td><td>4.3395</td><td>-1.75</td><td>2.65</td><td>441.5330</td><td>11.8378</td><td>-1.98</td><td>2.78</td></tr><tr><td>29</td><td>449.3241</td><td>4.3562</td><td>-1.68</td><td>2.73</td><td>456.8586</td><td>11.8931</td><td>-1.94</td><td>2.95</td></tr><tr><td>30</td><td>464.6703</td><td>4.4809</td><td>-1.73</td><td>2.74</td><td>472.2048</td><td>11.9169</td><td>-2.15</td><td>2.94</td></tr><tr><td>31</td><td>480.6909</td><td>4.5004</td><td>-1.97</td><td>2.85</td><td>488.2254</td><td>11.9218</td><td>-2.52</td><td>2.98</td></tr><tr><td>32</td><td>495.3219</td><td>4.4902</td><td>-2.16</td><td>2.88</td><td>502.8565</td><td>11.9427</td><td>-2.58</td><td>2.93</td></tr><tr><td>33</td><td>510.6478</td><td>4.4881</td><td>-2.15</td><td>2.79</td><td>518.1823</td><td>11.9468</td><td>-2.53</td><td>2.92</td></tr><tr><td>34</td><td>525.9735</td><td>4.4836</td><td>-2.15</td><td>2.80</td><td>533.5081</td><td>11.9353</td><td>-2.61</td><td>2.85</td></tr><tr><td>35</td><td>541.2992</td><td>4.4736</td><td>-2.10</td><td>2.81</td><td>548.8337</td><td>11.9158</td><td>-2.50</td><td>2.93</td></tr><tr><td>36</td><td>556.6248</td><td>4.4625</td><td>-2.13</td><td>2.79</td><td>564.1593</td><td>11.8930</td><td>-2.54</td><td>2.85</td></tr><tr><td>37</td><td>571.9502</td><td>4.4480</td><td>-2.11</td><td>2.81</td><td>579.4847</td><td>11.8694</td><td>-2.63</td><td>2.90</td></tr><tr><td>38</td><td>587.2755</td><td>4.4327</td><td>-2.21</td><td>2.79</td><td>594.8100</td><td>11.8469</td><td>-2.72</td><td>2.88</td></tr><tr><td>39</td><td>602.6006</td><td>4.4184</td><td>-2.26</td><td>2.82</td><td>610.1351</td><td>11.8267</td><td>-2.79</td><td>2.91</td></tr><tr><td>40</td><td>617.9255</td><td>4.4025</td><td>-2.34</td><td>2.82</td><td>625.4601</td><td>11.8149</td><td>-2.88</td><td>2.98</td></tr><tr><td>41</td><td>633.2504</td><td>4.3860</td><td>-2.35</td><td>2.82</td><td>640.7849</td><td>11.8126</td><td>-2.94</td><td>2.85</td></tr><tr><td>42</td><td>648.5955</td><td>4.3689</td><td>-2.40</td><td>2.78</td><td>656.1300</td><td>11.8403</td><td>-2.81</td><td>2.87</td></tr><tr><td>43</td><td>663.9201</td><td>4.4192</td><td>-2.28</td><td>2.77</td><td>671.4546</td><td>11.9076</td><td>-2.86</td><td>2.85</td></tr><tr><td>44</td><td>679.2446</td><td>4.5282</td><td>-2.46</td><td>2.82</td><td>686.7792</td><td>11.9015</td><td>-3.18</td><td>2.86</td></tr><tr><td>45</td><td>694.5692</td><td>4.5233</td><td>-2.60</td><td>2.87</td><td>702.1037</td><td>11.9192</td><td>-3.28</td><td>2.84</td></tr><tr><td>46</td><td>709.8938</td><td>4.5202</td><td>-2.61</td><td>2.83</td><td>717.4283</td><td>11.9373</td><td>-3.21</td><td>2.83</td></tr><tr><td>47</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>48</td><td>740.5432</td><td>4.5077</td><td>-2.61</td><td>2.83</td><td>748.0777</td><td>11.9246</td><td>-3.15</td><td>2.85</td></tr><tr><td>49</td><td>755.8682</td><td>4.4959</td><td>-2.57</td><td>2.83</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>50</td><td>771.1933</td><td>4.4826</td><td>-2.66</td><td>2.77</td><td>778.7278</td><td>11.8789</td><td>-3.26</td><td>2.86</td></tr><tr><td>51</td><td>786.5186</td><td>4.4682</td><td>-2.60</td><td>2.81</td><td>794.0531</td><td>11.8559</td><td>-3.27</td><td>2.83</td></tr><tr><td>52</td><td>801.8440</td><td>4.4541</td><td>-2.64</td><td>2.82</td><td>809.3786</td><td>11.8329</td><td>-3.30</td><td>2.86</td></tr><tr><td>53</td><td>817.1901</td><td>4.4394</td><td>-2.68</td><td>2.80</td><td>824.7246</td><td>11.8117</td><td>-3.26</td><td>2.82</td></tr><tr><td>54</td><td>832.5158</td><td>4.4247</td><td>-2.68</td><td>2.88</td><td>840.0503</td><td>11.8028</td><td>-3.35</td><td>2.82</td></tr><tr><td>55</td><td>847.8416</td><td>4.4062</td><td>-2.67</td><td>2.85</td><td>855.3761</td><td>11.8107</td><td>-3.34</td><td>2.85</td></tr><tr><td>56</td><td>863.1674</td><td>4.3991</td><td>-2.65</td><td>2.81</td><td>870.7020</td><td>11.8615</td><td>-3.31</td><td>2.84</td></tr><tr><td>57</td><td>878.4933</td><td>4.4867</td><td>-2.63</td><td>2.79</td><td>886.0278</td><td>11.9122</td><td>-3.37</td><td>2.82</td></tr><tr><td>58</td><td>893.8191</td><td>4.5508</td><td>-2.71</td><td>2.83</td><td>901.3536</td><td>11.9018</td><td>-3.52</td><td>2.82</td></tr><tr><td>59</td><td>909.1448</td><td>4.5441</td><td>-2.71</td><td>2.83</td><td>916.6793</td><td>11.9259</td><td>-3.40</td><td>2.80</td></tr><tr><td>60</td><td>924.4703</td><td>4.5415</td><td>-2.71</td><td>2.83</td><td>932.0049</td><td>11.9388</td><td>-3.46</td><td>2.78</td></tr></tbody></table>
## Appendix C: Eclipse properties

Table C.1 presents the eclipses properties obtained with the LIGHTCURVEFACTORY.

<table><caption>**Table C.1.** Eclipse properties.</caption><thead><tr><th>n</th><th>t<sub>1</sub><br>(KJD)</th><th>O<sub>1</sub> - nP - t<sub>0</sub><br>day</th><th>D<sub>1</sub><br>%</th><th>W<sub>1</sub><br>hour</th><th>t<sub>2</sub><br>(KJD)</th><th>O<sub>2</sub> - nP - t<sub>0</sub><br>day</th><th>D<sub>2</sub><br>%</th><th>W<sub>2</sub><br>hour</th></tr></thead><tbody><tr><td>8</td><td>127.4560</td><td>4.4034</td><td>-0.55</td><td>2.10</td><td>134.9905</td><td>11.9379</td><td>-0.50</td><td>2.24</td></tr><tr><td>9</td><td>142.8022</td><td>4.3911</td><td>-0.52</td><td>2.15</td><td>150.3368</td><td>11.9121</td><td>-0.51</td><td>2.20</td></tr><tr><td>10</td><td>158.1280</td><td>4.3778</td><td>-0.53</td><td>2.32</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>11</td><td>174.1688</td><td>4.3612</td><td>-0.62</td><td>2.48</td><td>181.7034</td><td>11.8727</td><td>-0.66</td><td>2.18</td></tr><tr><td>12</td><td>188.7792</td><td>4.3464</td><td>-0.65</td><td>2.38</td><td>196.3137</td><td>11.8560</td><td>-0.72</td><td>2.39</td></tr><tr><td>13</td><td>204.1046</td><td>4.3251</td><td>-0.77</td><td>2.31</td><td>211.6391</td><td>11.8481</td><td>-0.88</td><td>2.53</td></tr><tr><td>14</td><td>219.4298</td><td>4.3058</td><td>-0.84</td><td>2.40</td><td>226.9644</td><td>11.8495</td><td>-0.96</td><td>2.57</td></tr><tr><td>15</td><td>235.7970</td><td>4.3025</td><td>-0.87</td><td>2.40</td><td>243.3315</td><td>11.8809</td><td>-0.91</td><td>2.48</td></tr><tr><td>16</td><td>250.0798</td><td>4.4026</td><td>-0.89</td><td>2.43</td><td>257.6144</td><td>11.9343</td><td>-1.01</td><td>2.57</td></tr><tr><td>17</td><td>265.4046</td><td>4.4707</td><td>-1.15</td><td>2.67</td><td>272.9391</td><td>11.9343</td><td>-1.39</td><td>2.78</td></tr><tr><td>18</td><td>...</td><td>...</td><td>...</td><td>...</td><td>288.2638</td><td>11.9523</td><td>-1.56</td><td>2.69</td></tr><tr><td>19</td><td>296.0539</td><td>4.4538</td><td>-1.38</td><td>2.67</td><td>303.5884</td><td>11.9615</td><td>-1.62</td><td>2.71</td></tr><tr><td>20</td><td>311.3988</td><td>4.4533</td><td>-1.38</td><td>2.79</td><td>318.9334</td><td>11.9532</td><td>-1.58</td><td>2.80</td></tr><tr><td>21</td><td>327.9493</td><td>4.4437</td><td>-1.40</td><td>2.79</td><td>335.4839</td><td>11.9355</td><td>-1.53</td><td>2.81</td></tr><tr><td>22</td><td>342.0480</td><td>4.4350</td><td>-1.35</td><td>2.71</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>23</td><td>357.3727</td><td>4.4217</td><td>-1.42</td><td>2.63</td><td>364.9072</td><td>11.8882</td><td>-1.68</td><td>2.79</td></tr><tr><td>24</td><td>372.6975</td><td>4.4051</td><td>-1.39</td><td>2.55</td><td>380.2320</td><td>11.8657</td><td>-1.71</td><td>2.70</td></tr><tr><td>25</td><td>388.7172</td><td>4.3921</td><td>-1.52</td><td>2.81</td><td>396.2517</td><td>11.8462</td><td>-1.81</td><td>2.79</td></tr><tr><td>26</td><td>405.2275</td><td>4.3752</td><td>-1.60</td><td>2.75</td><td>412.7621</td><td>11.8327</td><td>-1.93</td><td>2.87</td></tr><tr><td>27</td><td>418.6730</td><td>4.3593</td><td>-1.64</td><td>2.70</td><td>426.2075</td><td>11.8260</td><td>-2.04</td><td>2.79</td></tr><tr><td>28</td><td>433.9985</td><td>4.3395</td><td>-1.75</td><td>2.65</td><td>441.5330</td><td>11.8378</td><td>-1.98</td><td>2.78</td></tr><tr><td>29</td><td>449.3241</td><td>4.3562</td><td>-1.68</td><td>2.73</td><td>456.8586</td><td>11.8931</td><td>-1.94</td><td>2.95</td></tr><tr><td>30</td><td>464.6703</td><td>4.4809</td><td>-1.73</td><td>2.74</td><td>472.2048</td><td>11.9169</td><td>-2.15</td><td>2.94</td></tr><tr><td>31</td><td>480.6909</td><td>4.5004</td><td>-1.97</td><td>2.85</td><td>488.2254</td><td>11.9218</td><td>-2.52</td><td>2.98</td></tr><tr><td>32</td><td>495.3219</td><td>4.4902</td><td>-2.16</td><td>2.88</td><td>502.8565</td><td>11.9427</td><td>-2.58</td><td>2.93</td></tr><tr><td>33</td><td>510.6478</td><td>4.4881</td><td>-2.15</td><td>2.79</td><td>518.1823</td><td>11.9468</td><td>-2.53</td><td>2.92</td></tr><tr><td>34</td><td>525.9735</td><td>4.4836</td><td>-2.15</td><td>2.80</td><td>533.5081</td><td>11.9353</td><td>-2.61</td><td>2.85</td></tr><tr><td>35</td><td>541.2992</td><td>4.4736</td><td>-2.10</td><td>2.81</td><td>548.8337</td><td>11.9158</td><td>-2.50</td><td>2.93</td></tr><tr><td>36</td><td>556.6248</td><td>4.4625</td><td>-2.13</td><td>2.79</td><td>564.1593</td><td>11.8930</td><td>-2.54</td><td>2.85</td></tr><tr><td>37</td><td>571.9502</td><td>4.4480</td><td>-2.11</td><td>2.81</td><td>579.4847</td><td>11.8694</td><td>-2.63</td><td>2.90</td></tr><tr><td>38</td><td>587.2755</td><td>4.4327</td><td>-2.21</td><td>2.79</td><td>594.8100</td><td>11.8469</td><td>-2.72</td><td>2.88</td></tr><tr><td>39</td><td>602.6006</td><td>4.4184</td><td>-2.26</td><td>2.82</td><td>610.1351</td><td>11.8267</td><td>-2.79</td><td>2.91</td></tr><tr><td>40</td><td>617.9255</td><td>4.4025</td><td>-2.34</td><td>2.82</td><td>625.4601</td><td>11.8149</td><td>-2.88</td><td>2.98</td></tr><tr><td>41</td><td>633.2504</td><td>4.3860</td><td>-2.35</td><td>2.82</td><td>640.7849</td><td>11.8126</td><td>-2.94</td><td>2.85</td></tr><tr><td>42</td><td>648.5955</td><td>4.3689</td><td>-2.40</td><td>2.78</td><td>656.1300</td><td>11.8403</td><td>-2.81</td><td>2.87</td></tr><tr><td>43</td><td>663.9201</td><td>4.4192</td><td>-2.28</td><td>2.77</td><td>671.4546</td><td>11.9076</td><td>-2.86</td><td>2.85</td></tr><tr><td>44</td><td>679.2446</td><td>4.5282</td><td>-2.46</td><td>2.82</td><td>686.7792</td><td>11.9015</td><td>-3.18</td><td>2.86</td></tr><tr><td>45</td><td>694.5692</td><td>4.5233</td><td>-2.60</td><td>2.87</td><td>702.1037</td><td>11.9192</td><td>-3.28</td><td>2.84</td></tr><tr><td>46</td><td>709.8938</td><td>4.5202</td><td>-2.61</td><td>2.83</td><td>717.4283</td><td>11.9373</td><td>-3.21</td><td>2.83</td></tr><tr><td>47</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>48</td><td>740.5432</td><td>4.5077</td><td>-2.61</td><td>2.83</td><td>748.0777</td><td>11.9246</td><td>-3.15</td><td>2.85</td></tr><tr><td>49</td><td>755.8682</td><td>4.4959</td><td>-2.57</td><td>2.83</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>50</td><td>771.1933</td><td>4.4826</td><td>-2.66</td><td>2.77</td><td>778.7278</td><td>11.8789</td><td>-3.26</td><td>2.86</td></tr><tr><td>51</td><td>786.5186</td><td>4.4682</td><td>-2.60</td><td>2.81</td><td>794.0531</td><td>11.8559</td><td>-3.27</td><td>2.83</td></tr><tr><td>52</td><td>801.8440</td><td>4.4541</td><td>-2.64</td><td>2.82</td><td>809.3786</td><td>11.8329</td><td>-3.30</td><td>2.86</td></tr><tr><td>53</td><td>817.1901</td><td>4.4394</td><td>-2.68</td><td>2.80</td><td>824.7246</td><td>11.8117</td><td>-3.26</td><td>2.82</td></tr><tr><td>54</td><td>832.5158</td><td>4.4247</td><td>-2.68</td><td>2.88</td><td>840.0503</td><td>11.8028</td><td>-3.35</td><td>2.82</td></tr><tr><td>55</td><td>847.8416</td><td>4.4062</td><td>-2.67</td><td>2.85</td><td>855.3761</td><td>11.8107</td><td>-3.34</td><td>2.85</td></tr><tr><td>56</td><td>863.1674</td><td>4.3991</td><td>-2.65</td><td>2.81</td><td>870.7020</td><td>11.8615</td><td>-3.31</td><td>2.84</td></tr><tr><td>57</td><td>878.4933</td><td>4.4867</td><td>-2.63</td><td>2.79</td><td>886.0278</td><td>11.9122</td><td>-3.37</td><td>2.82</td></tr><tr><td>58</td><td>893.8191</td><td>4.5508</td><td>-2.71</td><td>2.83</td><td>901.3536</td><td>11.9018</td><td>-3.52</td><td>2.82</td></tr><tr><td>59</td><td>909.1448</td><td>4.5441</td><td>-2.71</td><td>2.83</td><td>916.6793</td><td>11.9259</td><td>-3.40</td><td>2.80</td></tr><tr><td>60</td><td>924.4703</td><td>4.5415</td><td>-2.71</td><td>2.83</td><td>932.0049</td><td>11.9388</td><td>-3.46</td><td>2.78</td></tr></tbody></table>
<table><caption>Table C.1. continued.</caption><thead><tr><th>n</th><th>t<sub>1</sub><br>(KJD)</th><th>O<sub>1</sub> - nP - t<sub>0</sub><br>day</th><th>D<sub>1</sub><br>%</th><th>W<sub>1</sub><br>hour</th><th>t<sub>2</sub><br>(KJD)</th><th>O<sub>2</sub> - nP - t<sub>0</sub><br>day</th><th>D<sub>2</sub><br>%</th><th>W<sub>2</sub><br>hour</th></tr></thead><tbody><tr><td>61</td><td>939.7958</td><td>4.5342</td><td>-2.72</td><td>2.85</td><td>947.3303</td><td>11.9356</td><td>-3.36</td><td>2.83</td></tr><tr><td>62</td><td>955.1211</td><td>4.5223</td><td>-2.72</td><td>2.78</td><td>962.6557</td><td>11.9193</td><td>-3.40</td><td>2.78</td></tr><tr><td>63</td><td>970.4463</td><td>4.5100</td><td>-2.63</td><td>2.66</td><td>977.9808</td><td>11.8984</td><td>-3.42</td><td>2.79</td></tr><tr><td>64</td><td>985.7713</td><td>4.4957</td><td>-2.73</td><td>2.77</td><td>993.3058</td><td>11.8751</td><td>-3.40</td><td>2.80</td></tr><tr><td>65</td><td>...</td><td>...</td><td>...</td><td>...</td><td>1008.6307</td><td>11.8528</td><td>-3.60</td><td>2.87</td></tr><tr><td>66</td><td>1016.4413</td><td>4.4668</td><td>-2.79</td><td>2.83</td><td>1023.9758</td><td>11.8293</td><td>-3.54</td><td>2.78</td></tr><tr><td>67</td><td>1031.7659</td><td>4.4523</td><td>-2.74</td><td>2.79</td><td>1039.3004</td><td>11.8137</td><td>-3.44</td><td>2.78</td></tr><tr><td>68</td><td>1047.0905</td><td>4.4373</td><td>-2.75</td><td>2.85</td><td>1054.6250</td><td>11.8063</td><td>-3.44</td><td>2.79</td></tr><tr><td>69</td><td>1062.4150</td><td>4.4218</td><td>-2.71</td><td>2.86</td><td>1069.9495</td><td>11.8256</td><td>-3.51</td><td>2.78</td></tr><tr><td>70</td><td>1077.7396</td><td>4.4325</td><td>-2.60</td><td>2.78</td><td>1085.2741</td><td>11.9016</td><td>-3.38</td><td>2.81</td></tr><tr><td>71</td><td>1093.0642</td><td>4.5402</td><td>-2.74</td><td>2.80</td><td>1100.5987</td><td>11.9150</td><td>-3.39</td><td>2.83</td></tr><tr><td>72</td><td>1108.3889</td><td>4.5620</td><td>-2.70</td><td>2.88</td><td>1115.9235</td><td>11.9160</td><td>-3.42</td><td>2.85</td></tr><tr><td>73</td><td>1123.7138</td><td>4.5594</td><td>-2.70</td><td>2.78</td><td>1131.2484</td><td>11.9406</td><td>-3.36</td><td>2.83</td></tr><tr><td>74</td><td>1139.0389</td><td>4.5551</td><td>-2.74</td><td>2.85</td><td>1146.5734</td><td>11.9484</td><td>-3.48</td><td>2.78</td></tr><tr><td>75</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>76</td><td>1169.7100</td><td>4.5329</td><td>-2.74</td><td>2.82</td><td>1177.2446</td><td>11.9232</td><td>-3.41</td><td>2.79</td></tr><tr><td>77</td><td>1185.0356</td><td>4.5174</td><td>-2.71</td><td>2.83</td><td>1192.5701</td><td>11.9026</td><td>-3.45</td><td>2.77</td></tr><tr><td>78</td><td>1200.3613</td><td>4.5009</td><td>-2.71</td><td>2.81</td><td>1207.8958</td><td>11.8782</td><td>-3.48</td><td>2.82</td></tr><tr><td>79</td><td>1215.6870</td><td>4.4898</td><td>-2.61</td><td>2.64</td><td>1223.2216</td><td>11.8551</td><td>-3.42</td><td>2.83</td></tr><tr><td>80</td><td>1231.0129</td><td>4.4730</td><td>-2.66</td><td>2.83</td><td>1238.5474</td><td>11.8341</td><td>-3.45</td><td>2.78</td></tr><tr><td>81</td><td>1246.3387</td><td>4.4609</td><td>-2.68</td><td>2.85</td><td>1253.8732</td><td>11.8182</td><td>-3.38</td><td>2.76</td></tr><tr><td>82</td><td>1261.6645</td><td>4.4451</td><td>-2.77</td><td>2.91</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>83</td><td>1276.9903</td><td>4.4303</td><td>-2.79</td><td>2.83</td><td>1284.5248</td><td>11.8558</td><td>-3.42</td><td>2.72</td></tr><tr><td>84</td><td>...</td><td>...</td><td>...</td><td>...</td><td>1299.8504</td><td>11.9417</td><td>-3.43</td><td>2.72</td></tr><tr><td>85</td><td>1307.6414</td><td>4.5621</td><td>-2.64</td><td>2.90</td><td>1315.1759</td><td>11.9248</td><td>-3.34</td><td>2.83</td></tr><tr><td>86</td><td>1322.9667</td><td>4.5669</td><td>-2.66</td><td>2.96</td><td>1330.5013</td><td>11.9406</td><td>-3.40</td><td>2.75</td></tr><tr><td>87</td><td>1338.2920</td><td>4.5667</td><td>-2.74</td><td>2.87</td><td>1345.8265</td><td>11.9605</td><td>-3.44</td><td>2.75</td></tr><tr><td>88</td><td>1353.6170</td><td>4.5586</td><td>-2.74</td><td>2.83</td><td>1361.1515</td><td>11.9625</td><td>-3.41</td><td>2.75</td></tr><tr><td>89</td><td>1368.9623</td><td>4.5468</td><td>-2.74</td><td>2.85</td><td>1376.4969</td><td>11.9525</td><td>-3.62</td><td>2.77</td></tr><tr><td>90</td><td>1384.2871</td><td>4.5313</td><td>-2.83</td><td>2.85</td><td>1391.8216</td><td>11.9353</td><td>-3.55</td><td>2.70</td></tr><tr><td>91</td><td>1399.6117</td><td>4.5150</td><td>-2.82</td><td>2.79</td><td>1407.1463</td><td>11.9131</td><td>-3.55</td><td>2.75</td></tr><tr><td>92</td><td>...</td><td>...</td><td>...</td><td>...</td><td>1422.4708</td><td>11.8905</td><td>-3.43</td><td>2.74</td></tr><tr><td>93</td><td>1430.2608</td><td>4.4844</td><td>-2.72</td><td>2.84</td><td>1437.7954</td><td>11.8663</td><td>-3.43</td><td>2.76</td></tr><tr><td>94</td><td>1445.5854</td><td>4.4706</td><td>-2.73</td><td>2.86</td><td>1453.1199</td><td>11.8456</td><td>-3.43</td><td>2.78</td></tr><tr><td>95</td><td>1460.9100</td><td>4.4564</td><td>-2.71</td><td>2.91</td><td>1468.4445</td><td>11.8321</td><td>-3.41</td><td>2.73</td></tr><tr><td>96</td><td>1476.5208</td><td>4.4392</td><td>-2.71</td><td>2.89</td><td>1484.0553</td><td>11.9078</td><td>-3.43</td><td>2.70</td></tr><tr><td>97</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>98</td><td>1506.9050</td><td>4.5093</td><td>-2.77</td><td>2.85</td><td>1514.4395</td><td>11.9682</td><td>-3.47</td><td>2.78</td></tr><tr><td>99</td><td>1522.2302</td><td>4.5590</td><td>-2.73</td><td>2.92</td><td>1529.7647</td><td>11.9494</td><td>-3.47</td><td>2.75</td></tr><tr><td>100</td><td>1537.5556</td><td>4.5621</td><td>-2.64</td><td>2.94</td><td>1545.0901</td><td>11.9717</td><td>-3.49</td><td>2.77</td></tr><tr><td>101</td><td>1552.8811</td><td>4.5624</td><td>-2.69</td><td>2.90</td><td>1560.4156</td><td>11.9858</td><td>-3.36</td><td>2.72</td></tr><tr><td>102</td><td>1568.2067</td><td>4.5518</td><td>-2.66</td><td>2.89</td><td>1575.7413</td><td>11.9851</td><td>-3.37</td><td>2.74</td></tr></tbody></table>
<table><caption>Table C.1. continued.</caption><thead><tr><th>n</th><th>t<sub>1</sub><br>(KJD)</th><th>O<sub>1</sub> - nP - t<sub>0</sub><br>day</th><th>D<sub>1</sub><br>%</th><th>W<sub>1</sub><br>hour</th><th>t<sub>2</sub><br>(KJD)</th><th>O<sub>2</sub> - nP - t<sub>0</sub><br>day</th><th>D<sub>2</sub><br>%</th><th>W<sub>2</sub><br>hour</th></tr></thead><tbody><tr><td>61</td><td>939.7958</td><td>4.5342</td><td>-2.72</td><td>2.85</td><td>947.3303</td><td>11.9356</td><td>-3.36</td><td>2.83</td></tr><tr><td>62</td><td>955.1211</td><td>4.5223</td><td>-2.72</td><td>2.78</td><td>962.6557</td><td>11.9193</td><td>-3.40</td><td>2.78</td></tr><tr><td>63</td><td>970.4463</td><td>4.5100</td><td>-2.63</td><td>2.66</td><td>977.9808</td><td>11.8984</td><td>-3.42</td><td>2.79</td></tr><tr><td>64</td><td>985.7713</td><td>4.4957</td><td>-2.73</td><td>2.77</td><td>993.3058</td><td>11.8751</td><td>-3.40</td><td>2.80</td></tr><tr><td>65</td><td>...</td><td>...</td><td>...</td><td>...</td><td>1008.6307</td><td>11.8528</td><td>-3.60</td><td>2.87</td></tr><tr><td>66</td><td>1016.4413</td><td>4.4668</td><td>-2.79</td><td>2.83</td><td>1023.9758</td><td>11.8293</td><td>-3.54</td><td>2.78</td></tr><tr><td>67</td><td>1031.7659</td><td>4.4523</td><td>-2.74</td><td>2.79</td><td>1039.3004</td><td>11.8137</td><td>-3.44</td><td>2.78</td></tr><tr><td>68</td><td>1047.0905</td><td>4.4373</td><td>-2.75</td><td>2.85</td><td>1054.6250</td><td>11.8063</td><td>-3.44</td><td>2.79</td></tr><tr><td>69</td><td>1062.4150</td><td>4.4218</td><td>-2.71</td><td>2.86</td><td>1069.9495</td><td>11.8256</td><td>-3.51</td><td>2.78</td></tr><tr><td>70</td><td>1077.7396</td><td>4.4325</td><td>-2.60</td><td>2.78</td><td>1085.2741</td><td>11.9016</td><td>-3.38</td><td>2.81</td></tr><tr><td>71</td><td>1093.0642</td><td>4.5402</td><td>-2.74</td><td>2.80</td><td>1100.5987</td><td>11.9150</td><td>-3.39</td><td>2.83</td></tr><tr><td>72</td><td>1108.3889</td><td>4.5620</td><td>-2.70</td><td>2.88</td><td>1115.9235</td><td>11.9160</td><td>-3.42</td><td>2.85</td></tr><tr><td>73</td><td>1123.7138</td><td>4.5594</td><td>-2.70</td><td>2.78</td><td>1131.2484</td><td>11.9406</td><td>-3.36</td><td>2.83</td></tr><tr><td>74</td><td>1139.0389</td><td>4.5551</td><td>-2.74</td><td>2.85</td><td>1146.5734</td><td>11.9484</td><td>-3.48</td><td>2.78</td></tr><tr><td>75</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>76</td><td>1169.7100</td><td>4.5329</td><td>-2.74</td><td>2.82</td><td>1177.2446</td><td>11.9232</td><td>-3.41</td><td>2.79</td></tr><tr><td>77</td><td>1185.0356</td><td>4.5174</td><td>-2.71</td><td>2.83</td><td>1192.5701</td><td>11.9026</td><td>-3.45</td><td>2.77</td></tr><tr><td>78</td><td>1200.3613</td><td>4.5009</td><td>-2.71</td><td>2.81</td><td>1207.8958</td><td>11.8782</td><td>-3.48</td><td>2.82</td></tr><tr><td>79</td><td>1215.6870</td><td>4.4898</td><td>-2.61</td><td>2.64</td><td>1223.2216</td><td>11.8551</td><td>-3.42</td><td>2.83</td></tr><tr><td>80</td><td>1231.0129</td><td>4.4730</td><td>-2.66</td><td>2.83</td><td>1238.5474</td><td>11.8341</td><td>-3.45</td><td>2.78</td></tr><tr><td>81</td><td>1246.3387</td><td>4.4609</td><td>-2.68</td><td>2.85</td><td>1253.8732</td><td>11.8182</td><td>-3.38</td><td>2.76</td></tr><tr><td>82</td><td>1261.6645</td><td>4.4451</td><td>-2.77</td><td>2.91</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>83</td><td>1276.9903</td><td>4.4303</td><td>-2.79</td><td>2.83</td><td>1284.5248</td><td>11.8558</td><td>-3.42</td><td>2.72</td></tr><tr><td>84</td><td>...</td><td>...</td><td>...</td><td>...</td><td>1299.8504</td><td>11.9417</td><td>-3.43</td><td>2.72</td></tr><tr><td>85</td><td>1307.6414</td><td>4.5621</td><td>-2.64</td><td>2.90</td><td>1315.1759</td><td>11.9248</td><td>-3.34</td><td>2.83</td></tr><tr><td>86</td><td>1322.9667</td><td>4.5669</td><td>-2.66</td><td>2.96</td><td>1330.5013</td><td>11.9406</td><td>-3.40</td><td>2.75</td></tr><tr><td>87</td><td>1338.2920</td><td>4.5667</td><td>-2.74</td><td>2.87</td><td>1345.8265</td><td>11.9605</td><td>-3.44</td><td>2.75</td></tr><tr><td>88</td><td>1353.6170</td><td>4.5586</td><td>-2.74</td><td>2.83</td><td>1361.1515</td><td>11.9625</td><td>-3.41</td><td>2.75</td></tr><tr><td>89</td><td>1368.9623</td><td>4.5468</td><td>-2.74</td><td>2.85</td><td>1376.4969</td><td>11.9525</td><td>-3.62</td><td>2.77</td></tr><tr><td>90</td><td>1384.2871</td><td>4.5313</td><td>-2.83</td><td>2.85</td><td>1391.8216</td><td>11.9353</td><td>-3.55</td><td>2.70</td></tr><tr><td>91</td><td>1399.6117</td><td>4.5150</td><td>-2.82</td><td>2.79</td><td>1407.1463</td><td>11.9131</td><td>-3.55</td><td>2.75</td></tr><tr><td>92</td><td>...</td><td>...</td><td>...</td><td>...</td><td>1422.4708</td><td>11.8905</td><td>-3.43</td><td>2.74</td></tr><tr><td>93</td><td>1430.2608</td><td>4.4844</td><td>-2.72</td><td>2.84</td><td>1437.7954</td><td>11.8663</td><td>-3.43</td><td>2.76</td></tr><tr><td>94</td><td>1445.5854</td><td>4.4706</td><td>-2.73</td><td>2.86</td><td>1453.1199</td><td>11.8456</td><td>-3.43</td><td>2.78</td></tr><tr><td>95</td><td>1460.9100</td><td>4.4564</td><td>-2.71</td><td>2.91</td><td>1468.4445</td><td>11.8321</td><td>-3.41</td><td>2.73</td></tr><tr><td>96</td><td>1476.5208</td><td>4.4392</td><td>-2.71</td><td>2.89</td><td>1484.0553</td><td>11.9078</td><td>-3.43</td><td>2.70</td></tr><tr><td>97</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td><td>...</td></tr><tr><td>98</td><td>1506.9050</td><td>4.5093</td><td>-2.77</td><td>2.85</td><td>1514.4395</td><td>11.9682</td><td>-3.47</td><td>2.78</td></tr><tr><td>99</td><td>1522.2302</td><td>4.5590</td><td>-2.73</td><td>2.92</td><td>1529.7647</td><td>11.9494</td><td>-3.47</td><td>2.75</td></tr><tr><td>100</td><td>1537.5556</td><td>4.5621</td><td>-2.64</td><td>2.94</td><td>1545.0901</td><td>11.9717</td><td>-3.49</td><td>2.77</td></tr><tr><td>101</td><td>1552.8811</td><td>4.5624</td><td>-2.69</td><td>2.90</td><td>1560.4156</td><td>11.9858</td><td>-3.36</td><td>2.72</td></tr><tr><td>102</td><td>1568.2067</td><td>4.5518</td><td>-2.66</td><td>2.89</td><td>1575.7413</td><td>11.9851</td><td>-3.37</td><td>2.74</td></tr></tbody></table>