Search Publications

CSI 2264: Probing the inner disks of AA Tauri-like systems in NGC 2264
DOI: 10.1051/0004-6361/201425475 Bibcode: 2015A&A...577A..11M

Aigrain, S.; Dougados, C.; Bouvier, J. +20 more

Context. The classical T Tauri star (CTTS) AA Tau has presented photometric variability that was attributed to an inner disk warp, caused by the interaction between the inner disk and an inclined magnetosphere. Previous studies of the young cluster NGC 2264 have shown that similar photometric behavior is common among CTTS.
Aims: The goal of t…

2015 Astronomy and Astrophysics
CoRoT 113
CSI 2264: Characterizing Young Stars in NGC 2264 With Short-Duration Periodic Flux Dips in Their Light Curves
DOI: 10.1088/0004-6256/149/4/130 Bibcode: 2015AJ....149..130S

Song, Inseok; Gillen, Edward; Cody, Ann Marie +27 more

We identify nine young stellar objects (YSOs) in the NGC 2264 star-forming region with optical CoRoT light curves exhibiting short-duration, shallow periodic flux dips. All of these stars have infrared excesses that are consistent with their having inner disk walls near the Keplerian co-rotation radius. The repeating photometric dips have FWHMs ge…

2015 The Astronomical Journal
CoRoT 97
Transiting exoplanets from the CoRoT space mission⋆. XXVIII. CoRoT-33b, an object in the brown dwarf desert with 2:3 commensurability with its host star
DOI: 10.1051/0004-6361/201526763 Bibcode: 2015A&A...584A..13C

Mazeh, T.; Aigrain, S.; Alonso, R. +32 more

We report the detection of a rare transiting brown dwarf with a mass of 59 MJup and radius of 1.1 RJup around the metal-rich, [Fe/H] = +0.44, G9V star CoRoT-33. The orbit is eccentric (e = 0.07) with a period of 5.82 d. The companion, CoRoT-33b, is thus a new member in the so-called brown dwarf desert. The orbital period is w…

2015 Astronomy and Astrophysics
CoRoT 59
Stellar cycles from photometric data: CoRoT stars
DOI: 10.1051/0004-6361/201424900 Bibcode: 2015A&A...583A.134F

Catelan, M.; Ferreira Lopes, C. E.; De Medeiros, J. R. +3 more

Context. Until a few years ago, the amplitude variation in the photometric data had been explored to a limited extent mainly because of time resolution and photometric sensitivity limitations. This investigation is now possible thanks to the Kepler and CoRoT databases which provide a unique set of data for studying the nature of stellar variabilit…

2015 Astronomy and Astrophysics
CoRoT 42
CoRoT space photometry of seven Cepheids
DOI: 10.1093/mnras/stv1899 Bibcode: 2015MNRAS.454..849P

Poretti, E.; Rainer, M.; Baglin, A. +4 more

A few Galactic classical Cepheids were observed in the programmes of space missions as Coriolis, MOST, and Kepler. An appealing opportunity was to detect additional non-radial modes, thus opening the possibility to perform asteroseismic studies and making the pulsational content of Galactic Cepheids more similar to that of Magellanic Clouds ones. …

2015 Monthly Notices of the Royal Astronomical Society
CoRoT 29
MIARMA: A minimal-loss information method for filling gaps in time series. Application to CoRoT light curves
DOI: 10.1051/0004-6361/201425056 Bibcode: 2015A&A...575A..78P

Garrido, R.; Suárez, J. C.; Pascual-Granado, J.

Context. Gaps in time series cause spurious frequencies in the power spectra. In light curves of pulsating stars, this hampers identifying the theoretical oscillation modes. When these gaps are smaller than the total time span, the commonly used approach to overcome these difficulties involves linear interpolation. The original frequency content o…

2015 Astronomy and Astrophysics
CoRoT 22
BEER analysis of Kepler and CoRoT light curves. III. Spectroscopic confirmation of seventy new beaming binaries discovered in CoRoT light curves
DOI: 10.1051/0004-6361/201526425 Bibcode: 2015A&A...580A..21T

Mazeh, T.; Tal-Or, L.; Faigler, S.

Context. The BEER algorithm searches stellar light curves for the BEaming, Ellipsoidal, and Reflection photometric modulations that are caused by a short-period companion. These three effects are typically of very low amplitude and can mainly be detected in light curves from space-based photometers. Unlike eclipsing binaries, these effects are not…

2015 Astronomy and Astrophysics
CoRoT 19
Transiting exoplanets from the CoRoT space mission. XXVII. CoRoT-28b, a planet orbiting an evolved star, and CoRoT-29b, a planet showing an asymmetric transit
DOI: 10.1051/0004-6361/201424501 Bibcode: 2015A&A...579A..36C

Mazeh, T.; Aigrain, S.; Alonso, R. +50 more

Context. We present the discovery of two transiting extrasolar planets by the satellite CoRoT.
Aims: We aim at a characterization of the planetary bulk parameters, which allow us to further investigate the formation and evolution of the planetary systems and the main properties of the host stars.
Methods: We used the transit light curve …

2015 Astronomy and Astrophysics
CoRoT 16
Search for sub-kilometre trans-Neptunian objects using CoRoT asteroseismology data
DOI: 10.1093/mnras/stu1987 Bibcode: 2015MNRAS.446..932L

Chang, Hsiang-Kuang; Doressoundiram, Alain; Auvergne, Michel +3 more

We present the search for sub-kilometre trans-Neptunian objects (TNOs) by re-examining the CoRoT (Convection Rotation and Planetary Transits) asteroseismology observations. The total observation time employed in this work is about 144 000 star hours with signal-to-noise ratio larger than 1000 computed on 30-s intervals. 13 Possible Occultation Eve…

2015 Monthly Notices of the Royal Astronomical Society
CoRoT 15
The variability behaviour of CoRoT M-giant stars⋆
DOI: 10.1051/0004-6361/201425503 Bibcode: 2015A&A...583A.122F

Baglin, A.; Paz-Chinchón, F.; Janot-Pacheco, E. +8 more

Context. For six years the Convection, Rotation, and planetary Transits (CoRoT) space mission has been acquiring photometric data from more than 100 000 point sources towards and directly opposite the inner and outer regions of the Galaxy. The high temporal resolution of the CoRoT data, combined with the wide time span of the observations, enabled…

2015 Astronomy and Astrophysics
CoRoT 13