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We present the discovery of 30 transiting giant planets that were initially detected using data from NASA's Transiting Exoplanet Survey Satellite (TESS) mission. These new planets orbit relatively bright ($G \leq 12.5$) FGK host stars with…

Earth and Planetary Astrophysics · Physics 2025-07-03 Samuel W. Yee , Joshua N. Winn , Joel D. Hartman , Joseph E. Rodriguez , George Zhou , David W. Latham , Samuel N. Quinn , Allyson Bieryla , Karen A. Collins , Jason D. Eastman , Kevin I. Collins , Dennis M. Conti , Eric L. N. Jensen , David R. Anderson , Özgür Baştürk , David Baker , Khalid Barkaoui , Matthew P. Battley , Daniel Bayliss , Thomas G. Beatty , Yuri Beletsky , Alexander A. Belinski , Zouhair Benkhaldoun , Paul Benni , Pau Bosch-Cabot , César Briceño , Andrzej Brudny , Matthew R. Burleigh , R. Paul Butler , Stavros Chairetas , Ashley Chontos , Jessie Christiansen , David R. Ciardi , Catherine A. Clark , Ryan Cloutier , Matthew W. Craig , Jeffrey D. Crane , Nicholas Dowling , Courtney D. Dressing , Jehin Emmanuel , Phil Evans , Mark E. Everett , Gareb Fernández-Rodríguez , Jorge Fernández Fernández , Raquel Forés-Toribio , Charles D. Fortenbach , Akihiko Fukui , Elise Furlan , Tianjun Gan , Mourad Ghachoui , Steven Giacalone , Samuel Gill , Michaël Gillon , Kylie Hall , Yuya Hayashi , Christina Hedges , Jesus Higuera , Eric G. Hintz , Lea Hirsch , Rae Holcomb , Keith Horne , Ferran Grau Horta , Andrew W. Howard , Steve B. Howell , Howard Isaacson , Jon M. Jenkins , Taiki Kagetani , Jacob Kamler , Alicia Kendall , Judth Korth , Maxwell A. Kroft , Gaia Lacedelli , Didier Laloum , Nicholas Law , Jerome Pitogo de Leon , Alan M. Levine , Pablo Lewin , Sarah E. Logsdon , Michael B. Lund , Madelyn M. Madsen , Andrew W. Mann , Christopher R. Mann , Nataliia A. Maslennikova , Sandra Matutano , Mason McCormack , Kim K. McLeod , Edward J. Michaels , Ismael Mireles , Mayuko Mori , Jose A. Muñoz , Felipe Murgas , Norio Narita , Sean M. O'Brien , Caroline Odden , Enric Palle , Yatrik G. Patel , Peter Plavchan , Alex S. Polanski , Adam Popowicz , Don J. Radford , Phillip A. Reed , Howard M. Relles , Malena Rice , George R. Ricker , Boris S. Safonov , Arjun B. Savel , Jack Schulte , Richard P. Schwarz , Heidi Schweiker , Sara Seager , Ramotholo Sefako , Stephen A. Shectman , Avi Shporer , Denise C. Stephens , Chris Stockdale , Stephanie Striegel , Thiam-Guan Tan , Johanna K. Teske , Mathilde Timmermans , Solène Ulmer-Moll , Gavin Wang , Peter J. Wheatley , Selçuk Yalcinkaya , Roberto Zambelli , Judah Van Zandt , Carl Ziegler

Of the nearby transiting exoplanets that are amenable to detailed study, TrES-2 is both the most massive and has the largest impact parameter. We present z-band photometry of three transits of TrES-2. We improve upon the estimates of the…

We report on the confirmation of a transiting giant planet around the relatively hot (Teff = 6801 $\pm$ 56 K) star HD2685, whose transit signal was detected in Sector 1 data of the TESS mission. We confirmed the planetary nature of the…

Hot Jupiters have been perceived as loners devoid of planetary companions in close orbital proximity. However, recent discoveries based on space-borne precise photometry have revealed that at least some fraction of giant planets coexists…

Earth and Planetary Astrophysics · Physics 2023-07-04 G. Maciejewski , J. Golonka , W. Łoboda , J. Ohlert , M. Fernandez , F. Aceituno

The exoplanet HD 118203 b, orbiting a bright (V = 8.05) host star, was discovered using the radial velocity method by da Silva et al. (2006), but was not previously known to transit. TESS photometry has revealed that this planet transits…

We revisit the TrES-4 system parameters based on high-precision HARPS-N radial-velocity measurements and new photometric light curves. A combined spectroscopic and photometric analysis allows us to determine a spectroscopic orbit with an…

We present an estimate of the occurrence rate of hot Jupiters ($7\ R_{\oplus}\leq R_{p}\leq 2\ R_{J}$, $0.8 \leq P_{b}\leq 10$ days) around early-type M dwarfs based on stars observed by TESS during its Primary Mission. We adopt stellar…

We report the discovery and characterization of TOI-2005b, a warm Jupiter on an eccentric (e~0.59), 17.3-day orbit around a V_mag = 9.867 rapidly rotating F-star. The object was detected as a candidate by TESS and the planetary nature of…

We present the discovery of EPIC 228735255b, a P= 6.57 days Jupiter-mass (M$_P$=1.019$\pm$0.070 M$_{Jup}$) planet transiting a V=12.5 (G5-spectral type) star in an eccentric orbit (e=$0.120^{+0.056}_{-0.046}$) detected using a combination…

Albeit at a lower frequency than around hotter stars, short-period gas giants around low-mass stars ($T_\mathrm{eff} < 4965$ K) do exist, despite predictions from planetary population synthesis models that such systems should be exceedingly…

NASA's Transiting Exoplanet Survey Satellite (TESS) has identified over 7,000 candidate exoplanets via the transit method, with gas giants among the most readily detected due to their large radii. Even so, long intervals between TESS…

We report on a spectroscopic determination of the stellar parameters and chemical abundances for the parent star of the transiting planet TrES-1. Based on a detailed analysis of iron lines in our Keck and HET spectra we derive…

We report the discovery of the massive hot Jupiter NGTS-13b by the Next Generation Transit Survey (NGTS). The V = 12.7 host star is likely in the subgiant evolutionary phase with log g$_{*}$ = 4.04 $\pm$ 0.05, T$_{eff}$ = 5819 $\pm$ 73 K,…

We calculate the planet-star flux-density ratios as a function of wavelength from 0.5 microns to 25 microns for the transiting extrasolar giant planets TrES-1 and HD209458b and compare them with the recent Spitzer/IRAC-MIPS secondary…

Astrophysics · Physics 2009-11-10 A. Burrows , I. Hubeny , D. Sudarsky

We present estimates for the occurrence rates of hot Jupiters around dwarf stars based on data from the Transiting Exoplanet Survey Satellite (TESS) Prime Mission. We take 97 hot Jupiters orbiting 198,721 AFG dwarf stars (ranging in mass…

Earth and Planetary Astrophysics · Physics 2022-08-09 Maya Beleznay , Michelle Kunimoto

The orbital parameters of warm Jupiters serve as a record of their formation history, providing constraints on formation scenarios for giant planets on close and intermediate orbits. Here, we report the discovery of TIC 237913194b, detected…

We report the detection of a hot Jupiter ($M_{p}=1.75_{-0.17}^{+0.14}\ M_{J}$, $R_{p}=1.38\pm0.04\ R_{J}$) orbiting a middle-aged star ($\log g=4.152^{+0.030}_{-0.043}$) in the Transiting Exoplanet Survey Satellite (TESS) southern…