학술논문
The TESS-Keck Survey. XX. 15 New TESS Planets and a Uniform RV Analysis of All Survey Targets
Document Type
article
Author
Alex S. Polanski; Jack Lubin; Corey Beard; Joseph M. Akana Murphy; Ryan Rubenzahl; Michelle L. Hill; Ian J. M. Crossfield; Ashley Chontos; Paul Robertson; Howard Isaacson; Stephen R. Kane; David R. Ciardi; Natalie M. Batalha; Courtney Dressing; Benjamin Fulton; Andrew W. Howard; Daniel Huber; Erik A. Petigura; Lauren M. Weiss; Isabel Angelo; Aida Behmard; Sarah Blunt; Casey L. Brinkman; Fei Dai; Paul A. Dalba; Tara Fetherolf; Steven Giacalone; Lea A. Hirsch; Rae Holcomb; Molly R. Kosiarek; Andrew W. Mayo; Mason G. MacDougall; Teo Močnik; Daria Pidhorodetska; Malena Rice; Lee J. Rosenthal; Nicholas Scarsdale; Emma V. Turtelboom; Dakotah Tyler; Judah Van Zandt; Samuel W. Yee; David R. Coria; Shannon D. Dulz; Joel D. Hartman; Aaron Householder; Sarah Lange; Andrew Langford; Emma M. Louden; Jared C. Siegel; Emily A. Gilbert; Erica J. Gonzales; Joshua E. Schlieder; Andrew W. Boyle; Jessie L. Christiansen; Catherine A. Clark; Rachel B. Fernandes; Michael B. Lund; Arjun B. Savel; Holden Gill; Charles Beichman; Rachel Matson; Elisabeth C. Matthews; E. Furlan; Steve B. Howell; Nicholas J. Scott; Mark E. Everett; John H. Livingston; Irina O. Ershova; Dmitry V. Cheryasov; Boris Safonov; Jorge Lillo-Box; David Barrado; María Morales-Calderón
Source
The Astrophysical Journal Supplement Series, Vol 272, Iss 2, p 32 (2024)
Subject
Language
English
ISSN
1538-4365
0067-0049
0067-0049
Abstract
The Transiting Exoplanet Survey Satellite (TESS) has discovered hundreds of new worlds, with TESS planet candidates now outnumbering the total number of confirmed planets from Kepler. Owing to differences in survey design, TESS continues to provide planets that are better suited for subsequent follow-up studies, including mass measurement through radial velocity (RV) observations, compared to Kepler targets. In this work, we present the TESS-Keck Survey’s (TKS) Mass Catalog: a uniform analysis of all TKS RV survey data that has resulted in mass constraints for 126 planets and candidate signals. This includes 58 mass measurements that have reached ≥5 σ precision. We confirm or validate 32 new planets from the TESS mission either by significant mass measurement (15) or statistical validation (17), and we find no evidence of likely false positives among our entire sample. This work also serves as a data release for all previously unpublished TKS survey data, including 9,204 RV measurements and associated activity indicators over our three-year survey. We took the opportunity to assess the performance of our survey and found that we achieved many of our goals, including measuring the mass of 38 small (