Limits to the presence of transiting circumbinary planets in CoRoT data
arXiv:1610.08471 · doi:10.1051/0004-6361/201628244
Abstract
The CoRoT mission during its flight-phase 2007-2012 delivered the light-curves for over 2000 eclipsing binaries. Data from the Kepler mission have proven the existence of several transiting circumbinary planets. Albeit light-curves from CoRoT have typically lower precision and shorter coverage, CoRoT's number of targets is similar to Kepler, and some of the known circumbinary planets could potentially be detected in CoRoT data as well. The aim of this work has been a revision of the entire CoRoT data-set for the presence of circumbinary planets, and the derivation of limits to the abundances of such planets. We developed a code which removes the light curve of the eclipsing binaries and searches for quasi-periodic transit-like features in a light curve after removal of binary eclipses and instrumental features. The code needs little information on the sample systems and can be used for other space missions as well, like Kepler, K2, TESS and PLATO. The code is broad in the requirements leading to detections, but was tuned to deliver an amount of detections that is manageable in a subsequent, mainly visual, revision about their nature. In the CoRoT sample we identified three planet candidates whose transits would have arisen from a single pass across the central binary. No candidates remained however with transit events from multiple planetary orbits. We calculated the upper limits for the number of Jupiter, Saturn and Neptune sized planets in co-planar orbits for different orbital period ranges. We found that there are much less giant planets in short-periodic orbits around close binary systems than around single stars.
Accepted for publication in A&A, 11 pages, 4 figures and 4 tables. Updated to fix error in acknowledgement
References in corpus (12)
- The Transiting Circumbinary Planets Kepler-34 and Kepler-35
- Terrestrial Planet Occurrence Rates for the Kepler GK Dwarf Sample
- Planet Hunters X. KIC 8462852 - Where's the Flux?
- Exoplanet population inference and the abundance of Earth analogs from noisy, incomplete catalogs
- Eclipse Timing Variation Analyses of Eccentric Binaries with Close Tertiaries in the Kepler field
- Planets Transiting Non-Eclipsing Binaries
- On the Occurrence Rate of Hot Jupiters in Different Stellar Environments
- A triple origin for the lack of tight coplanar circumbinary planets around short-period binaries
- No circumbinary planets transiting the tightest Kepler binaries - a possible fingerprint of a third star
- Planet Hunters. VIII. Characterization of 41 Long-Period Exoplanet Candidates from Kepler Archival Data
- Circumbinary planets - why they are so likely to transit
- A study of the performance of the transit detection tool DST in space-based surveys. Application of the CoRoT pipeline to Kepler data
Cited by in corpus (12)
- The BEBOP radial-velocity survey for circumbinary planets I. Eight years of CORALIE observations of 47 single-line eclipsing binaries and abundance constraints on the masses of circumbinary planets
- Planets, candidates, and binaries from the CoRoT/Exoplanet programme: the CoRoT transit catalogue
- Populations of planets in multiple star systems
- SPOTS: The Search for Planets Orbiting Two Stars. III. Complete Sample and Statistical Analysis
- An Automated Method to Detect Transiting Circumbinary Planets
- Searching for Small Circumbinary Planets I. The STANLEY Automated Algorithm and No New Planets in Existing Systems
- CoRoT-TESS eclipsing binaries with light-travel-time effect
- Blackbody temperature of 200+ stellar flares observed with the CoRoT satellite
- Study of a Sample of Faint Be Stars in the Exofield of CoRoT. Part III. Global Spectroscopic Characterization and Astrophysical Parameters of the Central Stars
- CoRoT: The First Space-Based Transit Survey to Explore the Close-in Planet Population
- The Number of Transits Per Epoch for Transiting Misaligned Circumbinary Planets
- Optimized cutting off transit algorithm to study stellar rotation from PLATO mission light curves