J/ApJS/275/32 Hot Jupiter planetary system masses with TESS obs. (Zhang+, 2024)

Constraining the presence of companion planets in hot Jupiter planetary systems using transit-timing variation observations from TESS. Zhang Z., Wang W., Ma X., Chen Z., Wang Y., Yu C., Liu S., Gao Y., Tang B., Ma Bo <Astrophys. J. Suppl. Ser., 275, 32 (2024)> =2024ApJS..275...32Z 2024ApJS..275...32Z
ADC_Keywords: Exoplanets; Stars, masses; Optical Keywords: Hot Jupiters ; Exoplanets ; Transits ; Transit timing variation method Abstract: The presence of another planetary companion in a transiting exoplanet system can impact its transit light curve, leading to sinusoidal transit-timing variations (TTV). By utilizing both χ2 and rms analysis, we have combined the TESS observation data with an N-body simulation to investigate the existence of an additional planet in the system and put a limit on its mass. We have developed CMAT, an efficient and user-friendly tool for fitting transit light curves and calculating TTV with a theoretical period, based on which we can give a limit on its hidden companion's mass. We use 260 hot Jupiter systems from the complete TESS data set to demonstrate the use of CMAT. Our findings indicate that, for most systems, the upper mass limit of a companion planet can be restricted to several Jupiter masses. This constraint becomes stronger near resonance orbits, such as the 1:2, 2:1, 3:1, and 4:1 mean-motion resonance, where the limit is reduced to several Earth masses. These findings align with previous studies suggesting that a lack of companion planets with resonance in hot Jupiter systems could potentially support the high-eccentricity migration theory. Additionally, we observed that the choice between χ2 or rms method does not significantly affect the upper limit on companion mass; however, χ2 analysis may result in weaker restrictions but is statistically more robust compared to rms analysis in most cases. Description: The data for this study are taken from the Transiting Exoplanet Survey Satellite (TESS) observations. We select transiting hot Jupiters observed by TESS based on the following criteria: an orbital period of less than 10 days and a mass greater than 0.3MJ. This results in a sample of 260 hot Jupiter systems. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tableb1.dat 127 260 The mass of the host star and the planet in the system; Appendix B -------------------------------------------------------------------------------- See also: IV/39 : TESS Input Catalog version 8.2 (TIC v8.2) (Paegert+, 2021) J/ApJ/640/1051 : 25pc sample of Sun-like stars (Grether+, 2006) J/A+A/482/L17 : CoRoT space mission. I. 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(Ikwut-Ukwa+, 2020) J/AJ/162/7 : LC and radial velocities for 7 host stars (Bakos+, 2021) J/ApJS/270/14 : Transit times of hot Jupiters from TESS (Wang+, 2024) http://heasarc.gsfc.nasa.gov/docs/tess/ : NASA TESS Science Support Center Byte-by-byte Description of file: tableb1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 15 A15 --- Planet Planet name 17- 21 F5.3 Msun Mstar [0.49/2.52] Star mass 23- 50 A28 --- Auth First Author's name for the reference of Mstar 52- 70 A19 --- BibCode Bibcode of the reference for Mstar 72- 80 F9.6 Mjup Mp [0.2/13.3] Planet mass 82 A1 --- f_Mp [c] c: Calculated from MSINI and I 84-107 A24 --- Auth2 First Author's name for the reference of Mp 109-127 A19 --- Bibcode2 Bibcode of the reference for Mp -------------------------------------------------------------------------------- History: From electronic version of the journal Licences: cc-by
(End) Emmanuelle Perret [CDS] 15-Oct-2025
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