Kaz Gary

ORCID: 0009-0005-1681-6340
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About
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Research Areas
  • Stellar, planetary, and galactic studies
  • Astro and Planetary Science
  • Astrophysics and Star Formation Studies
  • Astronomy and Astrophysical Research

University of Kansas
2022

Abstract Exoplanet systems with multiple transiting planets are natural laboratories for testing planetary astrophysics. One such system is HD 191939 (TOI 1339), a bright ( V = 9) and Sun-like (G9V) star, which TESS found to host three (b, c, d). The have periods of 9, 29, 38 days each similar sizes from 3 3.4 R ⊕ . To further characterize the system, we measured radial velocity (RV) over 415 Keck/HIRES APF/Levy. We find that M b 10.4 ± 0.9 c 7.2 1.4 , low compared most known comparable...

10.3847/1538-3881/ac3d38 article EN cc-by The Astronomical Journal 2022-01-31
Steven Giacalone Courtney D. Dressing Christina Hedges Veselin B. Kostov Karen A. Collins and 95 more Eric L. N. Jensen Daniel A. Yahalomi Allyson Bieryla David R. Ciardi Steve B. Howell J. Lillo-Box Khalid Barkaoui Jennifer G. Winters Elisabeth C. Matthews John H. Livingston Samuel N. Quinn B. S. Safonov Charles Cadieux Elise Furlan Ian J. M. Crossfield Avi M. Mandell Emily A. Gilbert Ethan Kruse Elisa V. Quintana G. Ricker Sara Seager Joshua N. Winn Jon M. Jenkins Britt Duffy Adkins David Baker Thomas Barclay D. Barrado Natalie M. Batalha A. Belinski Z. Benkhaldoun Lars A. Buchhave Luca Cacciapuoti David Charbonneau Ashley Chontos Jessie L. Christiansen Ryan Cloutier Kevin I. Collins Dennis M. Conti Neil Cutting Scott Dixon René Doyon Mohammed El Mufti E. Esparza-Borges Zahra Essack Akihiko Fukui Tianjun Gan Kaz Gary Mourad Ghachoui M. Gillon Éric Girardin Ana Glidden Erica J. Gonzales P. Guerra Elliott P. Horch K. G. Hełminiak Andrew W. Howard Daniel Huber Jonathan Irwin Giovanni Isopi Emmanuël Jehin T. Kagetani Stephen R. Kane Kiyoe Kawauchi John F. Kielkopf Pablo Lewin Lindy Luker Michael B. Lund F. Mallia Shude Mao Bob Massey Rachel A. Matson Ismael Mireles M. Mori F. Murgas Norio Narita Tanner O’Dwyer Erik A. Petigura Alex S. Polanski F. J. Pozuelos Ε. Πάλλη H. Parviainen Peter Plavchan Howard M. Relles Paul Robertson Mark E. Rose Pamela Rowden Arpita Roy Arjun B. Savel Joshua E. Schlieder C. Schnaible Richard P. Schwarz Ramatholo Sefako A. Selezneva Brett Skinner Chris Stockdale

The James Webb Space Telescope (JWST) will be able to probe the atmospheres and surface properties of hot, terrestrial planets via emission spectroscopy. We identify 18 potentially planet candidates detected by Transiting Exoplanet Survey Satellite (TESS) that would make ideal targets for these observations. These cover a broad range radii ($R_{\rm p} \sim 0.6 - 2.0 R_\oplus$) orbit stars various magnitudes ($K_s = 5.78 10.78$, $V 8.4 15.69$) effective temperatures ($T_{\rm eff }\sim 3000...

10.3847/1538-3881/ac4334 article EN cc-by The Astronomical Journal 2022-01-28
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