Eclipsing binaries and fast rotators in the Kepler sample. Characterization via radial velocity analysis from Calar Alto
arXiv:1501.05183 · doi:10.1051/0004-6361/201425272
Abstract
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 established or validated by different techniques. But additional data is needed to characterize the rest of the candidates and reject other possible configurations. We started a follow-up program to validate, confirm, and characterize some of the planet candidates. In this paper we present the radial velocity analysis (RV) of those presenting large variations, compatible with being eclipsing binaries. We also study those showing large rotational velocities, which prevents us from obtaining the necessary precision to detect planetary-like objects. We present new RV results for 13 Kepler objects of interest (KOIs) obtained with the CAFE spectrograph at the Calar Alto Observatory, and analyze their high-spatial resolution images and the Kepler light curves of some interesting cases. We have found five spectroscopic and eclipsing binaries. Among them, the case of KOI-3853 is of particular interest. This system is a new example of the so-called heartbeat stars, showing dynamic tidal distortions in the Kepler light curve. We have also detected duration and depth variations of the eclipse. We suggest possible scenarios to explain such effect, including the presence of a third substellar body possibly detected in our RV analysis. We also provide upper mass limits to the transiting companions of other six KOIs with large rotational velocities. This property prevents the RV method to obtain the necessary precision to detect planetary-like masses. Finally, we analyze the large RV variations of other two KOIs, incompatible with the presence of planetary-mass objects. These objects are likely to be stellar binaries but a longer timespan is still needed.
Accepted for publication in A&A. 18 pages, 9 figures, 17 tables. This version fixes an error affecting the values of tables A.1-A.13. The text remains unaltered
References in corpus (35)
- Analytic Lightcurves for Planetary Transit Searches
- The false positive rate of Kepler and the occurrence of planets
- Planetary Candidates Observed by Kepler, III: Analysis of the First 16 Months of Data
- Characteristics of planetary candidates observed by Kepler, II: Analysis of the first four months of data
- Kepler Presearch Data Conditioning II - A Bayesian Approach to Systematic Error Correction
- The NASA Exoplanet Archive: Data and Tools for Exoplanet Research
- Kepler Presearch Data Conditioning I - Architecture and Algorithms for Error Correction in Kepler Light Curves
- The CORALIE survey for southern extra-solar planets VII. Two short-period Saturnian companions to HD108147 and HD168746
- Revised Stellar Properties of Kepler Targets for the Quarter 1-16 Transit Detection Run
- On the Low False Positive Probabilities of Kepler Planet Candidates
- A Class of Eccentric Binaries with Dynamic Tidal Distortions Discovered with Kepler
- KOI-54: The Kepler Discovery of Tidally-Excited Pulsations and Brightenings in a Highly Eccentric Binary
- Efficient fitting of multiplanet Keplerian models to radial velocity and astrometry data
- SOPHIE velocimetry of Kepler transit candidates VII. A false-positive rate of 35% for Kepler close-in giant exoplanet candidates
- Kepler Eclipsing Binary Stars. III. Classification of Kepler Eclipsing Binary Light Curves with Locally Linear Embedding
- Cross-Correlation and Maximum Likelihood Analysis: A New Approach to Combine Cross-Correlation Functions
- Binarity of Transit Host Stars - Implications on Planetary Parameters
- Robotic Laser-Adaptive-Optics Imaging of 715 Kepler Exoplanet Candidates using Robo-AO
- High-resolution imaging of planet host candidates. A comprehensive comparison of different techniques
- Kepler-91b: a planet at the end of its life. Planet and giant host star properties via light-curve variations
- Contamination in the Kepler Field. Identification of 685 KOIs as False Positives Via Ephemeris Matching Based On Q1-Q12 Data
- Tidal Excitation of Modes in Binary Systems with Applications to Binary Pulsars
- Adaptive Optics Images of Kepler Objects of Interest
- Measurements of Stellar Inclinations for Kepler Planet Candidates
- Multiplicity in transiting planet host stars. A Lucky Imaging study of Kepler candidates
- Gas and dust in the Beta Pictoris Moving Group as seen by the Herschel Space Observatory
- Tidally induced radial-velocity variations in close binaries
- Kepler-432 b: a massive planet in a highly eccentric orbit transiting a red giant
- The Mass-Radius Relationship for Very Low Mass Stars: Four New Discoveries from the HATSouth Survey
- The Discovery of HD 37605c and a Dispositive Null Detection of Transits of HD 37605b
- CAFE: Calar Alto Fiber-fed Echelle spectrograph
- SOPHIE velocimetry of Kepler transit candidates. XIII. KOI-189 B and KOI-686 B: two very low-mass stars in long-period orbits
- Gas and dust in the TW Hydrae Association as seen by the Herschel Space Observatory
- Radial velocity confirmation of Kepler-91 b. Additional evidence of its planetary nature using the Calar Alto/CAFE instrument
- Detection of the secondary eclipse of WASP-10b in the Ks-band
Cited by in corpus (9)
- Radial velocity monitoring of Kepler heartbeat stars
- Spin-Orbit Misalignments of Three Jovian Planets via Doppler Tomography
- Kepler-539: a young extrasolar system with two giant planets on wide orbits and in gravitational interaction
- Kepler-447b: a hot-Jupiter with an extremely grazing transit
- Visual Analysis and Demographics of Kepler Transit Timing Variations
- CAFE2: an upgrade to the CAFE high-resolution spectrograph. Commissioning results and new public pipeline
- Regular and chaotic orbits in the dynamics of exoplanets
- KOI-3890: A high mass-ratio asteroseismic red-giantM-dwarf eclipsing binary undergoing heartbeat tidal interactions
- Modeling Stellar Surface Features on Subgiant Star with an M-dwarf Companion