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相关论文: Optical Phase Curves of Kepler Exoplanets

200 篇论文

The Kepler mission has provided high-accurate photometric data in a long time span for more than two hundred thousands stars, looking for planetary transits. Among the detected candidates, the planetary nature of around 15% has been…

地球与行星天体物理 · 物理学 2015-04-15 J. Lillo-Box , D. Barrado , L. Mancini , Th. Henning , P. Figueira , S. Ciceri , N. Santos

The Kepler mission has allowed the detection of numerous multi-planet exosystems where the planetary orbits are relatively compact. The first such system detected was Kepler-11 which has six known planets at the present time. These kinds of…

地球与行星天体物理 · 物理学 2015-06-19 Dawn M. Gelino , Stephen R. Kane

Kepler has detected numerous exoplanet transits by precise measurements of stellar light in a single visible-wavelength band. In addition to detection, the precise photometry provides phase curves of exoplanets, which can be used to study…

地球与行星天体物理 · 物理学 2015-06-23 Renyu Hu , Brice-Olivier Demory , Sara Seager , Nikole Lewis , Adam P. Showman

I measure the physical properties of 38 transiting extrasolar planetary systems, bringing the total number studied within the Homogeneous Studies project to 82. Transit light curves are modelled using JKTEBOP, with careful attention paid to…

地球与行星天体物理 · 物理学 2015-06-05 John Southworth

The Robo-AO \textit{Kepler} Planetary Candidate Survey is observing every \textit{Kepler} planet candidate host star with laser adaptive optics imaging to search for blended nearby stars, which may be physically associated companions and/or…

地球与行星天体物理 · 物理学 2017-01-18 Carl Ziegler , Nicholas M. Law , Tim Morton , Christoph Baranec , Reed Riddle , Dani Atkinson , Anna Baker , Sarah Roberts , David R. Ciardi

The Robo-AO Kepler Planetary Candidate Survey is designed to observe every Kepler planet candidate host star with laser adaptive optics imaging to search for blended nearby stars, which may be physically associated companions and/or…

We present the results of our Hubble Space Telescope program and describe how our analysis methods were used to re-evaluate the habitability of some of the most interesting Kepler planet candidates. Our program observed 22 Kepler Object of…

太阳与恒星天体物理 · 物理学 2015-05-20 Kimberly M. S. Cartier , Ronald L. Gilliland , Jason T. Wright , David R. Ciardi

KOI-13 was presented by the Kepler team as a candidate for having a giant planet - KOI-13.01, with orbital period of 1.7 d and transit depth of ~0.8%. We have analyzed the Kepler Q2 data of KOI-13, which was publicly available at the time…

地球与行星天体物理 · 物理学 2015-05-30 T. Mazeh , G. Nachmani , G. Sokol , S. Faigler , S. Zucker

We have systematically searched for the phase curves among the planets discovered by \textit{K2}. Using the reported planetary parameters, we screen out the best potential candidates, and examine their light curves in detail. For our work,…

地球与行星天体物理 · 物理学 2019-03-08 Prajwal Niraula , Seth Redfield , Julien de Wit , Fei Dai , Ismael Mireles , Dilovan Serindag , Avi Shporer

With only two functional reaction wheels, Kepler cannot maintain stable pointing at its original target field and entered a new mode of observation called K2. Our method is based on many years of experience in planet hunting for the CoRoT…

地球与行星天体物理 · 物理学 2016-10-19 S. C. C. Barros , O. Demangeon , M. Deleuil

The Robo-AO Kepler Planetary Candidate Survey is observing every Kepler planet candidate host star (KOI) with laser adaptive optics imaging to hunt for blended nearby stars which may be physically associated companions. With the…

地球与行星天体物理 · 物理学 2016-11-23 Carl Ziegler , Nicholas M. Law , Christoph Baranec , Tim Morton , Reed Riddle , Dani Atkinson , Larissa Nofi

We confirm 27 planets in 13 planetary systems by showing the existence of statistically significant anti-correlated transit timing variations (TTVs), which demonstrates that the planet candidates are in the same system, and long-term…

We have analyzed Kepler light curves for 849 stars with T_eff < 5200 K from our Cycle 1 Guest Observer program. We identify six new eclipsing binaries, one of which has an orbital period of 29.91 d, and two of which are probably W UMa…

太阳与恒星天体物理 · 物理学 2015-06-03 T. E. Harrison , J. L. Coughlin , N. M. Ule , M. Lopez-Morales

Context. During the primary Kepler mission, between 2009 and 2013, about 150,000 pre-selected targets were observed with a 29.42 minute-long cadence. However, a survey of background stars that fall within the field of view (FOV) of the…

地球与行星天体物理 · 物理学 2025-02-19 John Bienias , Robert Szabo

We visually inspected the light curves of 7557 Kepler Objects of Interest (KOIs) to search for single transit events (STEs) possibly due to long-period giant planets. We identified 28 STEs in 24 KOIs, among which 14 events are newly…

地球与行星天体物理 · 物理学 2016-05-04 Sho Uehara , Hajime Kawahara , Kento Masuda , Shin'ya Yamada , Masataka Aizawa

We analyze the full $\mathit{Kepler}$ phase curve of KOI-964, a binary system consisting of a hot white dwarf on an eclipsing orbit around an A-type host star. Using all 18 quarters of long-cadence photometry, we carry out a joint light…

Optical secondary eclipse measurements made by \emph{Kepler} reveal a diverse set of geometric albedos for hot Jupiters with equilibrium temperatures between $1550-1700$ K. The presence or absence of high altitude condensates, such as…

地球与行星天体物理 · 物理学 2022-03-02 Danica Adams , Tiffany Kataria , Natasha Batalha , Peter Gao , Heather Knutson

Three transiting exoplanet candidate stars were discovered in a ground-based photometric survey prior to the launch of NASA's {\it Kepler} mission. {\it Kepler} observations of them were obtained during Quarter 1 of the {\it Kepler}…