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Related papers: The Random Transiter -- EPIC 249706694/HD 139139

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The NASA mission Kepler has detected 28 transits with depths and durations hours in the light curve of HD139139 during a 87 days campaign . Their arrival times are erratic. Rappaport et al. (2019) discard ten explanations. It is not clear…

Earth and Planetary Astrophysics · Physics 2019-10-08 Jean Schneider

We present the first good evidence for exocomet transits of a host star in continuum light in data from the Kepler mission. The Kepler star in question, KIC 3542116, is of spectral type F2V and is quite bright at K_p = 10. The transits have…

Earth and Planetary Astrophysics · Physics 2018-01-24 S. Rappaport , A. Vanderburg , T. Jacobs , D. LaCourse , J. Jenkins , A. Kraus , A. Rizzuto , D. W. Latham , A. Bieryla , M. Lazarevic , A. Schmitt

We describe EPIC 205718330 and EPIC 235240266, two systems identified in the K2 data whose light curves contain episodic drops in brightness with shapes and durations similar to those of the young "dipper" stars, yet shallower by ~1-2…

A search for extrasolar planetary transits using the extended Kepler mission (K2) campaigns 9 and 11 revealed five new candidates towards the Galactic bulge. The stars EPIC 224439122, 224560837, 227560005, 230778501 and 231635524 are found…

Earth and Planetary Astrophysics · Physics 2019-04-10 C. C. Cortes , D. Minniti , S. Villanova

Doppler measurements of two G-type main-sequence stars, HD210277 and HD168443, reveal Keplerian variations that imply the presence of companions with masses (M sin i) of 1.28 and 5.04 M_Jup and orbital periods of 437 d and 58 d,…

Astrophysics · Physics 2009-10-31 Geoffrey W. Marcy , R. Paul Butler , Steven S. Vogt , Debra Fischer , Michael C. Liu

As revealed by its peculiar Kepler light curve, the enigmatic star KIC 8462852 undergoes short and deep flux dimmings at a priori unrelated epochs. It presents nonetheless all other characteristics of a quiet 1 Gyr old F3V star. These…

We report here on the discovery of stellar occultations, observed with Kepler, that recur periodically at 15.685 hour intervals, but which vary in depth from a maximum of 1.3% to a minimum that can be less than 0.2%. The star that is…

Earth and Planetary Astrophysics · Physics 2015-06-03 S. Rappaport , A. Levine , E. Chiang , I. El Mellah , J. Jenkins , B. Kalomeni , E. S. Kite , M. Kotson , L. Nelson , L. Rousseau-Nepton , K. Tran

KIC 2856960 is a star in the Kepler field which was observed by Kepler for 4 years. It shows the primary and secondary eclipses of a close binary of 0.258d as well as complex dipping events that last for about 1.5d at a time and recur on a…

Solar and Stellar Astrophysics · Physics 2015-06-22 T. R. Marsh , D. J. Armstrong , P. J. Carter

The Kepler Mission is monitoring the brightness of ~150,000 stars searching for evidence of planetary transits. As part of the "Hunt for Exomoons with Kepler" (HEK) project, we report a planetary system with two confirmed planets and one…

Earth and Planetary Astrophysics · Physics 2015-06-11 David Nesvorny , David M. Kipping , Lars A. Buchhave , Gáspár Á. Bakos , Joel Hartman , Allan Schmitt

EPIC 204278916 has been serendipitously discovered from its K2 light curve which displays irregular dimmings of up to 65% for ~25 consecutive days out of 78.8 days of observations. For the remaining duration of the observations, the…

Solar and Stellar Astrophysics · Physics 2016-09-07 S. Scaringi , C. F. Manara , S. A. Barenfeld , P. J. Groot , A. Isella , M. A. Kenworthy , C. Knigge , T. J. Maccarone , L. Ricci , M. Ansdell

In 2015, K2 observations of the bright (V = 8.9, K = 7.7) star HIP 41378 revealed a rich system of at least five transiting exoplanets, ranging in size from super-Earths to gas giants. The 2015 K2 observations only spanned 74.8 days, and…

We report the discovery of a unique object of uncertain nature -- but quite possibly a disintegrating asteroid or minor planet -- orbiting one star of the widely separated binary TIC 400799224. We initially identified the system in data…

Context: We present the transit and follow-up of a single transit event from Campaign 14 of K2, EPIC248847494b, which has a duration of 54 hours and a 0.18% depth. Aims: Using photometric tools and conducting radial velocity follow-up, we…

KIC 2835289 is a triple stellar system that consists of an inner ellipsoidal variable with an orbital period of ~0.86 days and an outer star that eclipses the inner pair every ~750 days. Two eclipse events were observed by the Kepler…

Solar and Stellar Astrophysics · Physics 2015-04-20 Kyle Conroy , Andrej Prsa , Keivan Stassun , Jerome Orosz

We describe the results of a search for transit-like events caused by giant planets occulting stars in the old, metal-rich open cluster NGC 6791 based on BVI-colour photometry from eight nights of observations with the 2.54m Nordic Optical…

Astrophysics · Physics 2009-11-10 H. Bruntt , F. Grundahl , B. Tingley , S. Frandsen , P. B. Stetson , B. Thomsen

Over the duration of the Kepler mission, KIC8462852 was observed to undergo irregularly shaped, aperiodic dips in flux of up to $\sim 20$\%. The dipping activity can last for between 5 and 80 days. We characterize the object with…

Observations of the main sequence F3 V star KIC 8462852 (also known as Boyajian's star) revealed extreme aperiodic dips in flux up to 20% during the four years of the Kepler mission. Smaller dips (< 2%) were also observed with ground-based…

Solar and Stellar Astrophysics · Physics 2018-08-06 Gary Sacco , Linh Ngo , Julien Modolo

We report the discovery of two planets transiting the bright stars HD 89345 (EPIC 248777106, $V=9.376$, $K=7.721$) in K2 Campaign 14 and HD 286123 (EPIC 247098361, $V=9.822$, $K=8.434$) in K2 Campaign 13. Both stars are G-type stars, one of…

This paper discusses an algorithm for detecting single transits in photometric time-series data. Specifically, we aim to identify asymmetric transits with ingress that is more rapid than egress, as expected for cometary bodies with a…

Earth and Planetary Astrophysics · Physics 2018-11-28 Grant M. Kennedy , Greg Hope , Simon T. Hodgkin , Mark C. Wyatt
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