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We report the discovery by the WASP transit survey of two new highly irradiated giant planets transiting moderately bright stars. WASP-64b is slightly more massive (1.271+-0.068 M_Jup) and larger (1.271+-0.039 R_Jup) than Jupiter, and is in…

We observed the hot Jupiter HAT-P-32b (also known as HAT-P-32Ab) to determine its optical transmission spectrum by measuring the wavelength-dependent planet-to-star radius ratios in the region between 518 - 918 nm. We used the OSIRIS…

Earth and Planetary Astrophysics · Physics 2016-10-19 L. Nortmann , E. Palle , F. Murgas , S. Dreizler , N. Iro , A. Cabrera-Lavers

Here we draw attention to a candidate system with one hot Jupiter and one small, nearby companion, revealed by the recent Kepler data release (DR25). The hot Jupiter, Kepler-730b, has radius $R_{\rm p}=11.36^{+1.14}_{-0.98}~R_\oplus$ and…

Earth and Planetary Astrophysics · Physics 2018-09-05 Wei Zhu , Fei Dai , Kento Masuda

We report the discovery of the transiting exoplanets WASP-95b, WASP-96b, WASP-97b, WASP-98b, WASP-99b, WASP-100b and WASP-101b. All are hot Jupiters with orbital periods in the range 2.1 to 5.7 d, masses of 0.5 to 2.8 Mjup, and radii of 1.1…

In this paper, we report a refined determination of the orbital parameters and the detection of the Rossiter-McLaughlin effect of the recently discovered transiting exoplanet HD147506b (HAT-P-2b). The large orbital eccentricity at the short…

We present Hubble Space Telescope near-infrared transmission spectroscopy of the transiting hot-Jupiter HAT-P-1b. We observed one transit with Wide Field Camera 3 using the G141 low-resolution grism to cover the wavelength range 1.087-…

We report the discovery by the WASP transit survey of a highly-irradiated, massive (2.242 +/- 0.080 MJup) planet which transits a bright (V = 10.6), evolved F8 star every 2.9 days. The planet, WASP-71b, is larger than Jupiter (1.46 +/- 0.13…

We report the discovery by the HATSouth exoplanet survey of three hot-Saturn transiting exoplanets: HATS-19b, HATS-20b, and HATS-21b. The planet host HATS-19 is a slightly evolved V = 13.0 G0 star with [Fe/H] = 0.240, a mass of 1.303 Msun,…

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 report the discovery of a transiting planet orbiting the star TYC 6446-326-1. The star, WASP-22, is a moderately bright (V=12.0) solar-type star (Teff = 6000 +/- 100 K, [Fe/H] = -0.05 +/- 0.08). The lightcurve of the star obtained with…

We report the discovery of eight hot-Jupiter exoplanets from the WASP-South transit survey. WASP-144b has a mass of 0.44 Mj, a radius of 0.85 Rj, and is in a 2.27-d orbit around a V = 12.9, K2 star which shows a 21-d rotational modulation.…

We present a new ground-based visible transmission spectrum of the high-gravity, hot Jupiter HAT-P-23b, obtained as part of the ACCESS project. We derive the spectrum from five transits observed between 2016 and 2018, with combined…

Exoplanet research is now target rich with a wide diversity of systems making it difficult for high demand observatories to undertake follow up observations over extended periods of time. We investigate the effectiveness of using 0.4m-class…

Earth and Planetary Astrophysics · Physics 2020-09-08 M. A. Salisbury , U. C. Kolb , A. J. Norton , C. A. Haswell

We report the discovery of Kepler-77b (alias KOI-127.01), a Saturn-mass transiting planet in a 3.6-day orbit around a metal-rich solar-like star. We combined the publicly available Kepler photometry (quarters 1-13) with high-resolution…

A 10.24 days Neptune-mass planet was recently announced to orbit the nearby M2 dwarf Gl 176, based on 28 radial velocities measured with the HRS spectrograph on the Hobby-Heberly Telescope (HET). We obtained 57 radial velocities of Gl 176…

We present the discoveries of KELT-25b (TIC 65412605, TOI-626.01) and KELT-26b (TIC 160708862, TOI-1337.01), two transiting companions orbiting relatively bright, early A-stars. The transit signals were initially detected by the KELT…

Earth and Planetary Astrophysics · Physics 2020-11-04 Romy Rodríguez Martínez , B. Scott Gaudi , Joseph E. Rodriguez , George Zhou , Jonathan Labadie-Bartz , Samuel N. Quinn , Kaloyan Minev Penev , Thiam-Guan Tan , David W. Latham , Leonardo A. Paredes , John Kielkopf , Brett C. Addison , Duncan J. Wright , Johanna K. Teske , Steve B. Howell , David R. Ciardi , Carl Ziegler , Keivan G. Stassun , Marshall C. Johnson , Jason D. Eastman , Robert J. Siverd , Thomas G. Beatty , Luke G. Bouma , Joshua Pepper , Michael B. Lund , Steven Villanueva , Daniel J. Stevens , Eric L. N. Jensen , Coleman Kilby , David H. Cohen , Daniel Bayliss , Allyson Bieryla , Phillip A. Cargile , Karen A. Collins , Dennis M. Conti , Knicole D. Colon , Ivan A. Curtis , Darren L. DePoy , Phil A. Evans , Dax Feliz , Joao Gregorio , Jason Rothenberg , David J. James , Matthew T. Penny , Phillip A. Reed , Howard M. Relles , Denise C. Stephens , Michael D. Joner , Rudolf B. Kuhn , Chris Stockdale , Mark Trueblood , Patricia Trueblood , Xinyu Yao , Roberto Zambelli , Roland Vanderspek , Sara Seager , Joshua N. Winn , Jon M. Jenkins , Todd J. Henry , Hodari-Sadiki James , Wei-Chun Jao , Sharon X. Wang , R. Paul Butler , Jeffrey D. Crane , Ian B. Thompson , Stephen Schectman , Robert A. Wittenmyer , Timothy R. Bedding , Jack Okumura , Peter Plavchan , Brendan P. Bowler , Jonathan Horner , Stephen R. Kane , Matthew W. Mengel , Timothy D. Morton , C. G. Tinney , Hui Zhang , Nicholas J. Scott , Rachel A. Matson , Mark E. Everett , Andrei Tokovinin , Andrew W. Mann , Diana Dragomir , Maximilian N. Guenther , Eric B. Ting , Michael Fausnaugh , Ana Glidden , Elisa V. Quintana , Mark Manner , Jennifer L. Marshall , Kim K. McLeod , Somayeh Khakpash

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…

We report the discovery of a new transiting planet in the Southern Hemisphere. It has been found by the WASP-south transit survey and confirmed photometrically and spectroscopically by the 1.2m Swiss Euler telescope, LCOGT 2m Faulkes South…

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