Transiting exoplanets from the CoRoT space mission - IV. CoRoT-Exo-4b: a transiting planet in a 9.2 day synchronous orbit
CoRoT, the first space-based transit search, provides ultra-high-precision light curves with continuous time-sampling over periods of up to 5 months. This allows the detection of transiting planets with relatively long periods, and the simultaneous study of the host star's photometric variabili...
Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , |
---|---|
Format: | Journal article |
Language: | English |
Published: |
2008
|
_version_ | 1797106188678070272 |
---|---|
author | Aigrain, S Cameron, A Ollivier, M Pont, F Jorda, L Almenara, J Alonso, R Barge, P Borde, P Bouchy, F Deeg, H De la Reza, R Deleuil, M Dvorak, R Erikson, A Fridlund, M Gondoin, P Gillon, M Guillot, T Hatzes, A Lammer, H Lanza, A Leger, A Llebaria, A Magain, P |
author_facet | Aigrain, S Cameron, A Ollivier, M Pont, F Jorda, L Almenara, J Alonso, R Barge, P Borde, P Bouchy, F Deeg, H De la Reza, R Deleuil, M Dvorak, R Erikson, A Fridlund, M Gondoin, P Gillon, M Guillot, T Hatzes, A Lammer, H Lanza, A Leger, A Llebaria, A Magain, P |
author_sort | Aigrain, S |
collection | OXFORD |
description | CoRoT, the first space-based transit search, provides ultra-high-precision light curves with continuous time-sampling over periods of up to 5 months. This allows the detection of transiting planets with relatively long periods, and the simultaneous study of the host star's photometric variability. In this Letter, we report the discovery of the transiting giant planet CoRoT-Exo-4b and use the CoRoT light curve to perform a detailed analysis of the transit and determine the stellar rotation period. The CoRoT light curve was pre-processed to remove outliers and correct for orbital residuals and artefacts due to hot pixels on the detector. After removing stellar variability about each transit, the transit light curve was analysed to determine the transit parameters. A discrete autocorrelation function method was used to derive the rotation period of the star from the out-of-transit light curve. We determine the periods of the planetary orbit and star's rotation of 9.20205 0.00037 and 8.87 1.12 days respectively, which is consistent with this being a synchronised system. We also derive the inclination, in degrees, the ratio of the orbital distance to the stellar radius, , and the planet-to-star radius ratio . We discuss briefly the coincidence between the orbital period of the planet and the stellar rotation period and its possible implications for the system's migration and star-planet interaction history. © 2008 ESO. |
first_indexed | 2024-03-07T06:58:12Z |
format | Journal article |
id | oxford-uuid:fed942dd-9ed3-4dff-b9be-2e5bef7e24db |
institution | University of Oxford |
language | English |
last_indexed | 2024-03-07T06:58:12Z |
publishDate | 2008 |
record_format | dspace |
spelling | oxford-uuid:fed942dd-9ed3-4dff-b9be-2e5bef7e24db2022-03-27T13:39:52ZTransiting exoplanets from the CoRoT space mission - IV. CoRoT-Exo-4b: a transiting planet in a 9.2 day synchronous orbitJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:fed942dd-9ed3-4dff-b9be-2e5bef7e24dbEnglishSymplectic Elements at Oxford2008Aigrain, SCameron, AOllivier, MPont, FJorda, LAlmenara, JAlonso, RBarge, PBorde, PBouchy, FDeeg, HDe la Reza, RDeleuil, MDvorak, RErikson, AFridlund, MGondoin, PGillon, MGuillot, THatzes, ALammer, HLanza, ALeger, ALlebaria, AMagain, PCoRoT, the first space-based transit search, provides ultra-high-precision light curves with continuous time-sampling over periods of up to 5 months. This allows the detection of transiting planets with relatively long periods, and the simultaneous study of the host star's photometric variability. In this Letter, we report the discovery of the transiting giant planet CoRoT-Exo-4b and use the CoRoT light curve to perform a detailed analysis of the transit and determine the stellar rotation period. The CoRoT light curve was pre-processed to remove outliers and correct for orbital residuals and artefacts due to hot pixels on the detector. After removing stellar variability about each transit, the transit light curve was analysed to determine the transit parameters. A discrete autocorrelation function method was used to derive the rotation period of the star from the out-of-transit light curve. We determine the periods of the planetary orbit and star's rotation of 9.20205 0.00037 and 8.87 1.12 days respectively, which is consistent with this being a synchronised system. We also derive the inclination, in degrees, the ratio of the orbital distance to the stellar radius, , and the planet-to-star radius ratio . We discuss briefly the coincidence between the orbital period of the planet and the stellar rotation period and its possible implications for the system's migration and star-planet interaction history. © 2008 ESO. |
spellingShingle | Aigrain, S Cameron, A Ollivier, M Pont, F Jorda, L Almenara, J Alonso, R Barge, P Borde, P Bouchy, F Deeg, H De la Reza, R Deleuil, M Dvorak, R Erikson, A Fridlund, M Gondoin, P Gillon, M Guillot, T Hatzes, A Lammer, H Lanza, A Leger, A Llebaria, A Magain, P Transiting exoplanets from the CoRoT space mission - IV. CoRoT-Exo-4b: a transiting planet in a 9.2 day synchronous orbit |
title | Transiting exoplanets from the CoRoT space mission - IV. CoRoT-Exo-4b: a transiting planet in a 9.2 day synchronous orbit |
title_full | Transiting exoplanets from the CoRoT space mission - IV. CoRoT-Exo-4b: a transiting planet in a 9.2 day synchronous orbit |
title_fullStr | Transiting exoplanets from the CoRoT space mission - IV. CoRoT-Exo-4b: a transiting planet in a 9.2 day synchronous orbit |
title_full_unstemmed | Transiting exoplanets from the CoRoT space mission - IV. CoRoT-Exo-4b: a transiting planet in a 9.2 day synchronous orbit |
title_short | Transiting exoplanets from the CoRoT space mission - IV. CoRoT-Exo-4b: a transiting planet in a 9.2 day synchronous orbit |
title_sort | transiting exoplanets from the corot space mission iv corot exo 4b a transiting planet in a 9 2 day synchronous orbit |
work_keys_str_mv | AT aigrains transitingexoplanetsfromthecorotspacemissionivcorotexo4batransitingplanetina92daysynchronousorbit AT camerona transitingexoplanetsfromthecorotspacemissionivcorotexo4batransitingplanetina92daysynchronousorbit AT ollivierm transitingexoplanetsfromthecorotspacemissionivcorotexo4batransitingplanetina92daysynchronousorbit AT pontf transitingexoplanetsfromthecorotspacemissionivcorotexo4batransitingplanetina92daysynchronousorbit AT jordal transitingexoplanetsfromthecorotspacemissionivcorotexo4batransitingplanetina92daysynchronousorbit AT almenaraj transitingexoplanetsfromthecorotspacemissionivcorotexo4batransitingplanetina92daysynchronousorbit AT alonsor transitingexoplanetsfromthecorotspacemissionivcorotexo4batransitingplanetina92daysynchronousorbit AT bargep transitingexoplanetsfromthecorotspacemissionivcorotexo4batransitingplanetina92daysynchronousorbit AT bordep transitingexoplanetsfromthecorotspacemissionivcorotexo4batransitingplanetina92daysynchronousorbit AT bouchyf transitingexoplanetsfromthecorotspacemissionivcorotexo4batransitingplanetina92daysynchronousorbit AT deegh transitingexoplanetsfromthecorotspacemissionivcorotexo4batransitingplanetina92daysynchronousorbit AT delarezar transitingexoplanetsfromthecorotspacemissionivcorotexo4batransitingplanetina92daysynchronousorbit AT deleuilm transitingexoplanetsfromthecorotspacemissionivcorotexo4batransitingplanetina92daysynchronousorbit AT dvorakr transitingexoplanetsfromthecorotspacemissionivcorotexo4batransitingplanetina92daysynchronousorbit AT eriksona transitingexoplanetsfromthecorotspacemissionivcorotexo4batransitingplanetina92daysynchronousorbit AT fridlundm transitingexoplanetsfromthecorotspacemissionivcorotexo4batransitingplanetina92daysynchronousorbit AT gondoinp transitingexoplanetsfromthecorotspacemissionivcorotexo4batransitingplanetina92daysynchronousorbit AT gillonm transitingexoplanetsfromthecorotspacemissionivcorotexo4batransitingplanetina92daysynchronousorbit AT guillott transitingexoplanetsfromthecorotspacemissionivcorotexo4batransitingplanetina92daysynchronousorbit AT hatzesa transitingexoplanetsfromthecorotspacemissionivcorotexo4batransitingplanetina92daysynchronousorbit AT lammerh transitingexoplanetsfromthecorotspacemissionivcorotexo4batransitingplanetina92daysynchronousorbit AT lanzaa transitingexoplanetsfromthecorotspacemissionivcorotexo4batransitingplanetina92daysynchronousorbit AT legera transitingexoplanetsfromthecorotspacemissionivcorotexo4batransitingplanetina92daysynchronousorbit AT llebariaa transitingexoplanetsfromthecorotspacemissionivcorotexo4batransitingplanetina92daysynchronousorbit AT magainp transitingexoplanetsfromthecorotspacemissionivcorotexo4batransitingplanetina92daysynchronousorbit |