TY - JOUR
T1 - VaTEST.
T2 - II. Statistical Validation of 11 TESS-detected Exoplanets Orbiting K-type Stars
AU - Mistry, Priyashkumar
AU - Pathak, Kamlesh
AU - Prasad, Aniket
AU - Lekkas, Georgios
AU - Bhattarai, Surendra
AU - Gharat, Sarvesh
AU - Maity, Mousam
AU - Kumar, Dhruv
AU - Collins, Karen A.
AU - Schwarz, Richard P.
AU - Mann, Christopher R.
AU - Furlan, Elise
AU - Howell, Steve B.
AU - Ciardi, David
AU - Bieryla, Allyson
AU - Matthews, Elisabeth C.
AU - Gonzales, Erica
AU - Ziegler, Carl
AU - Crossfield, Ian
AU - Giacalone, Steven
AU - Tan, Thiam-Guan
AU - Evans, Phil
AU - Hełminiak, Krzysztof G.
AU - Collins, Kevin I.
AU - Narita, Norio
AU - Fukui, Akihiko
AU - Pozuelos, Francisco J.
AU - Dressing, Courtney
AU - Soubkiou, Abderahmane
AU - Benkhaldoun, Zouhair
AU - Schlieder, Joshua E.
AU - Suarez, Olga
AU - Barkaoui, Khalid
AU - Palle, Enric
AU - Murgas, Felipe
AU - Srdoc, Gregor
AU - Goliguzova, Maria V.
AU - Strakhov, Ivan A.
AU - Gnilka, Crystal
AU - Lester, Kathryn
AU - Littlefield, Colin
AU - Scott, Nic
AU - Matson, Rachel
AU - Gillon, Michaël
AU - Jehin, Emmanuel
AU - Timmermans, Mathilde
AU - Ghachoui, Mourad
AU - Abe, Lyu
AU - Bendjoya, Philippe
AU - Guillot, Tristan
AU - Triaud, Amaury H. M. J.
PY - 2023/7/1
Y1 - 2023/7/1
N2 - NASA’s Transiting Exoplanet Survey Satellite (TESS) is an all-sky survey mission designed to find transiting exoplanets orbiting nearby bright stars. It has identified more than 329 transiting exoplanets, and almost 6000 candidates remain unvalidated. In this manuscript, we discuss the findings from the ongoing Validation of Transiting Exoplanets using Statistical Tools (VaTEST) project, which aims to validate new exoplanets for further characterization. We validated 11 new exoplanets by examining the light curves of 24 candidates using the LATTE and TESS-Plot tools and computing the false-positive probabilities using the statistical validation tool TRICERATOPS. These include planets suitable for atmospheric characterization using transmission spectroscopy (TOI-2194b), emission spectroscopy (TOI-3082b and TOI-5704b) and for both transmission and emission spectroscopy (TOI-672b, TOI-1694b, and TOI-2443b). Our validated planets have one super-Earth (TOI-2194b) orbiting a bright (V = 8.42 mag), metal-poor ([Fe/H] = −0.3720 ± 0.1) star, and one short-period Neptune-like planet (TOI-5704) in the hot-Neptune desert. In total, we validated one super-Earth, seven sub-Neptunes, one Neptune-like, and two sub-Saturn or super-Neptune-like exoplanets. Additionally, we identify five likely planet candidates (TOI-323, TOI-1180, TOI-2200, TOI-2408, and TOI-3913), which can be further studied to establish their planetary nature.
AB - NASA’s Transiting Exoplanet Survey Satellite (TESS) is an all-sky survey mission designed to find transiting exoplanets orbiting nearby bright stars. It has identified more than 329 transiting exoplanets, and almost 6000 candidates remain unvalidated. In this manuscript, we discuss the findings from the ongoing Validation of Transiting Exoplanets using Statistical Tools (VaTEST) project, which aims to validate new exoplanets for further characterization. We validated 11 new exoplanets by examining the light curves of 24 candidates using the LATTE and TESS-Plot tools and computing the false-positive probabilities using the statistical validation tool TRICERATOPS. These include planets suitable for atmospheric characterization using transmission spectroscopy (TOI-2194b), emission spectroscopy (TOI-3082b and TOI-5704b) and for both transmission and emission spectroscopy (TOI-672b, TOI-1694b, and TOI-2443b). Our validated planets have one super-Earth (TOI-2194b) orbiting a bright (V = 8.42 mag), metal-poor ([Fe/H] = −0.3720 ± 0.1) star, and one short-period Neptune-like planet (TOI-5704) in the hot-Neptune desert. In total, we validated one super-Earth, seven sub-Neptunes, one Neptune-like, and two sub-Saturn or super-Neptune-like exoplanets. Additionally, we identify five likely planet candidates (TOI-323, TOI-1180, TOI-2200, TOI-2408, and TOI-3913), which can be further studied to establish their planetary nature.
KW - Exoplanet systems
KW - Exoplanet detection methods
KW - Exoplanet astronomy
U2 - 10.3847/1538-3881/acd548
DO - 10.3847/1538-3881/acd548
M3 - Article
SN - 0004-6256
VL - 166
JO - The Astronomical Journal
JF - The Astronomical Journal
IS - 1
M1 - 9
ER -