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623 results on '"Samadi, R"'

203. Mixed modes in red giants: a window on stellar evolution

Author

Mosser, B., primary, Benomar, O., additional, Belkacem, K., additional, Goupil, M. J., additional, Lagarde, N., additional, Michel, E., additional, Lebreton, Y., additional, Stello, D., additional, Vrard, M., additional, Barban, C., additional, Bedding, T. R., additional, Deheuvels, S., additional, Chaplin, W. J., additional, De Ridder, J., additional, Elsworth, Y., additional, Montalban, J., additional, Noels, A., additional, Ouazzani, R. M., additional, Samadi, R., additional, White, T. R., additional, and Kjeldsen, H., additional

Published
2014
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206. VizieR Online Data Catalog: Supervised classification of CoRoT variables (Debosscher+, 2009)

Author

Debosscher, J., Sarro, L.~m., Lopez, M., Deleuil, M., Aerts, C., Auvergne, M., Baglin, A., Baudin, F., Chadid, M., Charpinet, S., Cuypers, J., de Ridder, J., Garrido, R., Hubert, A.~m., Janot-Pacheco, E., Jorda, L., Kaiser, Andreas, Kallinger, T., Kollath, Z., Maceroni, C., Mathias, P., Michel, E., Moutou, C., Neiner, C., Ollivier, M., Samadi, R., Solano, E., Surace, C., Vandenbussche, B., Weiss, W.~w., Institute of Astronomy [Leuven], Catholic University of Leuven - Katholieke Universiteit Leuven (KU Leuven), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Instituut voor Sterrenkunde [Leuven], Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Division technique INSU/SDU (DTI), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Hippolyte Fizeau (FIZEAU), Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Astrophysique de Toulouse-Tarbes (LATT), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Royal Observatory of Belgium [Brussels] (ROB), Instituto de Astrofísica de Andalucía (IAA), Consejo Superior de Investigaciones Científicas [Madrid] (CSIC), Instituto de Astronomia, Geofisica e Ciencias Atmosfericas (IAGCAUSP), Universidade de São Paulo = University of São Paulo (USP), Institut d’Électronique, de Microélectronique et de Nanotechnologie - UMR 8520 (IEMN), Centrale Lille-Institut supérieur de l'électronique et du numérique (ISEN)-Université de Valenciennes et du Hainaut-Cambrésis (UVHC)-Université de Lille-Centre National de la Recherche Scientifique (CNRS)-Université Polytechnique Hauts-de-France (UPHF), Institute for Astronomy [Vienna], University of Vienna [Vienna], Laboratoire des Sciences du Climat et de l'Environnement [Gif-sur-Yvette] (LSCE), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Galaxies, Etoiles, Physique, Instrumentation (GEPI), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Departamento de Astrofisica [Madrid], Centro de Astrobiologia [Madrid] (CAB), Instituto Nacional de Técnica Aeroespacial (INTA)-Consejo Superior de Investigaciones Científicas [Madrid] (CSIC)-Instituto Nacional de Técnica Aeroespacial (INTA)-Consejo Superior de Investigaciones Científicas [Madrid] (CSIC), Spanish Virtual Observatory - Observatorio Virtual Español (SVO), and Spanish Virtual Observatory - Observatorio Virtual Español

Subjects
[INFO]Computer Science [cs], Stars: variable, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract

International audience; Light curve parameters and classification results are presented for all the objects measured in the first four CoRoT observing runs: IRa01, SRc01, LRc01, and LRa01. The information presented here should allow scientists to make candidate lists of their objects of study and to obtain some basic light curve information. We recall that we did not perform detailed light curve modelling, only a basic one, sufficient for producing variability class memberships for each target. We refer to the paper for a detailed description of the light curve parameters, and the classification results. It is strongly advised to read the paper prior to using the results presented here. (4 data files).

Published
2009

207. Automated supervised classification of variable stars in the CoRoT programme. Method and application to the first four exoplanet fields

Author

Debosscher, J., Sarro, L. M., Lxf3pez, M., Deleuil, M., Aerts, C., Auvergne, M., Baglin, A., Baudin, F., Chadid, M., Charpinet, S., Cuypers, J., De Ridder, J., Garrido, R., Hubert, A. M., Janot-Pacheco, E., Jorda, L., Kaiser, A., Kallinger, T., Kollath, Z., Maceroni, C., Mathias, P., Michel, E., Moutou, C., Neiner, C., Ollivier, M., Samadi, R., Solano, E., Surace, C., Vandenbussche, B., Weiss, W. W., Debosscher, Sarro, L. M., Lxf3pez, Deleuil, Aerts, Auvergne, Baglin, Baudin, Chadid, Charpinet, Cuypers, De Ridder, Garrido, Hubert, A. M., Janot-Pacheco, Jorda, Kaiser, Kallinger, Kollath, Maceroni, Mathias, Michel, Moutou, Neiner, Ollivier, Samadi, Solano, Surace, Vandenbussche, Weiss, and W. W.

Published
2009

208. Space observations of B stars with CoRoT

Author

Degroote, P., Miglio, A., Debosscher, J., Montalbxe1n, J., Cuypers, J., Briquet, M., De Cat, P., Thoul, A., Morel, T., Niemczura, E., Balaguer-Nxfaxf1ez, L., Maceroni, C., Ribas, I., Noels, A., Aerts, C., Auvergne, M., Baglin, A., Catala, C., Deleuil, M., Michel, E., Ollivier, M., Jorda, L., Samadi, R., Degroote, Miglio, Debosscher, Montalbxe1n, Cuypers, Briquet, De Cat, Thoul, Morel, Niemczura, Balaguer-Nxfaxf1ez, Maceroni, Ribas, Noels, Aerts, Auvergne, Baglin, Catala, Deleuil, Michel, Ollivier, Jorda, and Samadi

Published
2009

210. The B0.5IVe CoRoT target HD 49 330. I. Photometric analysis from CoRoT data

Author

Huat, A.L., Hubert, A.M., Floquet, M., Neiner, C., Frémat, Y., Gutiérrez Soto, Juan, Baudin, F., Andrade, L., De Batz, B., Diago Nebot, Pascual David, Emilio, M., Espinosa-Lara, F., Fabregat Llueca, Juan, Janot-Pacheco, E., Leroy, B., Martayan, C., Semaan, T., Suso, J., Michel, E., and Samadi, R.

Subjects
Astrophysics::High Energy Astrophysical Phenomena, Astronomia, Astrophysics::Solar and Stellar Astrophysics, Astrophysics::Earth and Planetary Astrophysics, Astrophysics::Galaxy Astrophysics, Ciència Ensenyament
Abstract

Context. Be stars undergo outbursts producing a circumstellar disk from the ejected material. The beating of non-radial pulsations has been put forward as a possible mechanism of ejection. Aims. We analyze the pulsational behavior of the early B0.5IVe star HD 49330 observed during the first CoRoT long run towards the Galactical anticenter (LRA1). This Be star is located close to the lower edge of the β Cephei instability strip in the HR diagram and showed a 0.03 mag outburst during the CoRoT observations. It is thus an ideal case for testing the aforementioned hypothesis. Methods. We analyze the CoRoT light curve of HD 49330 usin g Fourier methods and non-lin ear least square fitting. Results. In this star, we find pulsation modes typical of β Cep stars (p modes) and SPB stars (g modes) with amplitude variations along the run directly correlated with the outburst. These results provide new clues about the origin of the Be phenomenon as well as strong constraints on the seismic modelling of Be stars.

Published
2009

211. Asteroseismic analysis of the CoRoT ��-Scuti star HD174936

Author

Hern��ndez, A. Garc��a, Moya, A., Michel, E., Garrido, R., Su��rez, J. C., Rodr��guez, E., Amado, P. J., Mart��n-Ru��z, S., Rolland, A., Poretti, E., Samadi, R., Baglin, A., Auvergne, M., Catala, C., Lefevre, L., and Baudin, F.

Subjects
Astrophysics::Solar and Stellar Astrophysics, FOS: Physical sciences, Astrophysics::Earth and Planetary Astrophysics, Solar and Stellar Astrophysics (astro-ph.SR)
Abstract

We present an analysis of the ��-Scuti star object HD 174936 (ID 7613) observed by CoRoT during the first short run SRc01 (27 days). A total number of 422 frequencies we are extracted from the light curve using standard prewhitening techniques. This number of frequencies was obtained by considering a spectral significance limit of sig = 10 using the software package SigSpec. Our analysis of the oscillation frequency spectrum reveals a spacing periodicity of around 52 \muHz. Although modes considered here are not in the asymptotic regime, a comparison with stellar models confirms that this signature may stem from a quasi-periodic pattern similar to the so-called large separation in solar-like stars., 7 pages, 7 figures, 2 tables. Accepted for publication in A&A CoRoT Special Feature

Published
2009
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212. The pulsations of the B5IVe star HD 181 231 observed with CoRoT and ground-based spectroscopy

Author

Neiner, C., Gutiérrez Soto, Juan, Baudin, F., De Batz, B., Frémat, Y., Huat, A.L., Floquet, M., Hubert, A.M., Leroy, B., Diago Nebot, Pascual David, Poretti, E., Carrier, F., Rainer, M., Catala, C., Thizy, O., Buil, C., Ribeiro, J., Andrade, L., Emilio, M., Espinosa-Lara, F., Fabregat Llueca, Juan, Janot-Pacheco, E., Martayan, C., Semaan, T., Suso, J., Baglin, A., Michel, E., and Samadi, R.

Subjects
Astronomia, Astrophysics::Solar and Stellar Astrophysics, Astrophysics::Earth and Planetary Astrophysics, Ciència Ensenyament
Abstract

Context. HD 181231 is a B5IVe star, which has been observed with the CoRoT satellite during ∼5 consecutive months and simultaneously from the ground in spectroscopy and spectropolarimetry. Aims. By analysing these data, we aim to detect and characterize as many pulsation frequencies as possible, to search for the presence of beating effects possibly at the origin of the Be phenomenon. Our results will also pr ovide a basis for seismic modelling. Methods. The fundamental parameters of the star are determined from spectral fitting and from the study of the circumstellar emission. The CoRoT photometric data and ground-based spectroscopy are analysed using several Fourier Techniques: CLEAN-NG,PASPER,and TISAFT, as well as a time-frequency technique. A search for a magnetic field is performed by applying the LSD technique to the spectropolarimetric data. Results. We find that HD 181231 is a B5IVe star seen with an inclination of ∼45 degrees. No magnetic field is detected in its photo-sphere. We detect at least 10 independent significant frequencies of variations among the 54 detected frequencies, interpreted in termsof non-radial pulsation modes and rotation. Two longer-term variations are also detected: one at ∼14 days resulting from a beating effect between the two main frequencies of short-term variations, the other at ∼116 days due either to a beating of frequencies or to a zonal pulsation mode. Conclusions. Our analysis of the CoRoT light curve and ground-based spectroscopic data of HD 181231 has led to the determination of the fundamental and pulsational parameters of the star, including beating effects. This will allow a precise seismic modelling of this star.

Published
2009

213. Low-amplitude variations detected by CoRoT in the B8IIIe star HD 175 869

Author

Gutiérrez Soto, Juan, Floquet, M., Samadi, R., Neiner, C., Garrido, R., Fabregat Llueca, Juan, Frémat, Y., Diago Nebot, Pascual David, Huat, A. L., Leroy, B., Emilio, M., Hubert, A.M., Thizy, O., Andrade, L., De Batz, B., Janot-Pacheco, E., Espinosa-Lara, F., Martayan, C., Suso, J., Auvergne, M., Chaintreuil, S., Michel, E., and Catala, C.

Subjects
Esteroides, Astrophysics::Solar and Stellar Astrophysics, Astrophysics::Earth and Planetary Astrophysics
Abstract

Context.The origin of the short-term variability in Be stars remains a matter of controversy. Pulsations and rotational modulation are the components of the favored hypothesis.Aims.We present our analysis of CoRoT data of the B8IIIe star HD 175869 observed during the first short run in the center direction (SRC1).Methods.We review both the instrumental effects visible in the CoRoT light curve and the analysis methods used by the CoRoT Be team. We applied these methods to the CoRoT light curve of the star HD 175869. A search for line-profile variations in the spectroscopic data was also performed. We also searched for a magnetic field, by applying the LSD technique to spectropolarimetric data.Results.The light curve exhibits low-amplitude variations of the order of 300 μ mag with a double wave shape. A frequency within the range determined for the rotational frequency and 6 of its harmonics are detected. The main frequency and its first harmonic exhibit amplitude variations of a few days. Other significant frequencies of low-amplitude from 25 to a few μmag are also found. The analysis of line profiles from ground-based spectrosc opic data does not detect an y variation. In addition, no Zeeman signature was found.Conclusions.Inhomogeneities caused by stellar activity in or just above the photosphere are proposed to produce the photometric variability detected by CoRoT in the Be star HD 175869. The hypothesis that non-radial pulsations are the origin of these variations cannot be excluded.

Published
2009

214. AsteroFLAG - from the Sun to the Stars

Author

Chaplin, W.J., Appourchaux, T., Arentoft, Torben, Ballot, J., Baudin, F., Bazot, Michael, Bedding, T.R., Christensen-Dalsgaard, Jørgen, Creevey, O.L., Duez, V., Elsworth, Y., Fletcher, S.T., García, R.A., Gough, D.O., Jiménez, A., Jiménez-Reyes, S.J., Houdek, G., Kjeldsen, Hans, Lazrek, M., Leibacher, J.W., Monteiro, M.J.P.F.G., Neiner, C., New, R., Régulo, C., Salabert, D., Samadi, R., Sekii, T., Sousa, S.G., Toutain, T., and Turck-Chièze, S.

Published
2008

217. Studying solar-like oscillations in red giants: MOST spacebased photometry of epsilon Ophiuchi

Author

Barban, C., Matthews, J., Ridder, J., Baudin, F., Kuschnig, R., Anwesh Mazumdar, Samadi, R., Guenther, D. B., Moffat, A. F. J., Rucinski, S. M., Sasselov, D., Walker, G. A. H., Weiss, W. W., Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Pôle Astronomie du LESIA, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris

Subjects
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract

International audience

Published
2006

218. Why bothering to measure stellar rotation with CoRoT?

Author

Goupil, M. J., Moya, A., Suarez, J. C., Lochard, J., Barban, C., Dias Do Nascimento, J., Dupret, M. A., Samadi, R., Baglin, A., Zahn, J. P., Hubert, A. M., Brun, S., Boisnard, L., More, P., Garrido, R., Mathis, S., Michel, E., Renan De Medeiros, R., Palacios, A., Lignieres, F., Rieutord, M., Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Departement d'Astrophysique Stellaire et Galactique (DASGAL), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL), Laboratoire Univers et Théories (LUTH (UMR_8102)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Observatoire de Paris - Site de Meudon (OBSPM), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Astrophysique de Toulouse-Tarbes (LATT), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7), Centre National de la Recherche Scientifique (CNRS)-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées, Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC), PSL Research University (PSL)-PSL Research University (PSL), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), PSL Research University (PSL)-PSL Research University (PSL)-Centre National de la Recherche Scientifique (CNRS), and Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3)

Subjects
[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Astrophysics::Solar and Stellar Astrophysics, Astrophysics::Earth and Planetary Astrophysics
Abstract

International audience; One important goal of the CoRoT experiment is to obtain information about the internal rotation of stars, in particular the ratio of central to surface rotation rates. This will provide constraints on face the modelling of transport mechanisms of angular momentum acting in radiative (rotationally induced turbulent) and convective zones (plumes, extension beyond convectively unstable regions). Relations between the surface rotation period and age, magnetic activity, mass loss and other stellar characteristics can also be studied with a statistically significant set of data as will be provided by CoRoT. We present various theoretical efforts performed over the past years in order to develope the theoretical tools which will enable us to study rotation with CoRoT.

Published
2006

221. Seismic analysis of HD 43587Aa, a solar-like oscillator in a multiple system

Author

Boumier, P., primary, Benomar, O., additional, Baudin, F., additional, Verner, G., additional, Appourchaux, T., additional, Lebreton, Y., additional, Gaulme, P., additional, Chaplin, W., additional, García, R. A., additional, Hekker, S., additional, Regulo, C., additional, Salabert, D., additional, Stahn, T., additional, Elsworth, Y., additional, Gizon, L., additional, Hall, M., additional, Mathur, S., additional, Michel, E., additional, Morel, T., additional, Mosser, B., additional, Poretti, E., additional, Rainer, M., additional, Roxburgh, I., additional, do Nascimento Jr., J.-D., additional, Samadi, R., additional, Auvergne, M., additional, Chaintreuil, S., additional, Baglin, A., additional, and Catala, C., additional

Published
2014
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224. An in-depth study of HD 174966 with CoRoT photometry and HARPS spectroscopy

Author

García Hernández, A., primary, Moya, A., additional, Michel, E., additional, Suárez, J. C., additional, Poretti, E., additional, Martín-Ruíz, S., additional, Amado, P. J., additional, Garrido, R., additional, Rodríguez, E., additional, Rainer, M., additional, Uytterhoeven, K., additional, Rodrigo, C., additional, Solano, E., additional, Rodón, J. R., additional, Mathias, P., additional, Rolland, A., additional, Auvergne, M., additional, Baglin, A., additional, Baudin, F., additional, Catala, C., additional, and Samadi, R., additional

Published
2013
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225. Low-amplitude rotational modulation rather than pulsations in the CoRoT B-type supergiant HD 46769

Author

Aerts, C., primary, Simón-Díaz, S., additional, Catala, C., additional, Neiner, C., additional, Briquet, M., additional, Castro, N., additional, Schmid, V. S., additional, Scardia, M., additional, Rainer, M., additional, Poretti, E., additional, Pápics, P. I., additional, Degroote, P., additional, Bloemen, S., additional, Østensen, R. H., additional, Auvergne, M., additional, Baglin, A., additional, Baudin, F., additional, Michel, E., additional, and Samadi, R., additional

Published
2013
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227. Asymptotic and measured large frequency separations

Author

Mosser, B., primary, Michel, E., additional, Belkacem, K., additional, Goupil, M. J., additional, Baglin, A., additional, Barban, C., additional, Provost, J., additional, Samadi, R., additional, Auvergne, M., additional, and Catala, C., additional

Published
2013
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233. Study of HD 169392A observed by CoRoT and HARPS

Author

Mathur, S., primary, Bruntt, H., additional, Catala, C., additional, Benomar, O., additional, Davies, G. R., additional, García, R. A., additional, Salabert, D., additional, Ballot, J., additional, Mosser, B., additional, Régulo, C., additional, Chaplin, W. J., additional, Elsworth, Y., additional, Handberg, R., additional, Hekker, S., additional, Mantegazza, L., additional, Michel, E., additional, Poretti, E., additional, Rainer, M., additional, Roxburgh, I. W., additional, Samadi, R., additional, Stȩślicki, M., additional, Uytterhoeven, K., additional, Verner, G. A., additional, Auvergne, M., additional, Baglin, A., additional, Barceló Forteza, S., additional, Baudin, F., additional, and Roca Cortés, T., additional

Published
2012
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234. Spin down of the core rotation in red giants

Author

Mosser, B., primary, Goupil, M. J., additional, Belkacem, K., additional, Marques, J. P., additional, Beck, P. G., additional, Bloemen, S., additional, De Ridder, J., additional, Barban, C., additional, Deheuvels, S., additional, Elsworth, Y., additional, Hekker, S., additional, Kallinger, T., additional, Ouazzani, R. M., additional, Pinsonneault, M., additional, Samadi, R., additional, Stello, D., additional, García, R. A., additional, Klaus, T. C., additional, Li, J., additional, Mathur, S., additional, and Morris, R. L., additional

Published
2012
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235. Stochastic gravito-inertial modes discovered by CoRoT in the hot Be star HD 51452

Author

Neiner, C., primary, Floquet, M., additional, Samadi, R., additional, Espinosa Lara, F., additional, Frémat, Y., additional, Mathis, S., additional, Leroy, B., additional, de Batz, B., additional, Rainer, M., additional, Poretti, E., additional, Mathias, P., additional, Guarro Fló, J., additional, Buil, C., additional, Ribeiro, J., additional, Alecian, E., additional, Andrade, L., additional, Briquet, M., additional, Diago, P. D., additional, Emilio, M., additional, Fabregat, J., additional, Gutiérrez-Soto, J., additional, Hubert, A.-M., additional, Janot-Pacheco, E., additional, Martayan, C., additional, Semaan, T., additional, Suso, J., additional, and Zorec, J., additional

Published
2012
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236. Gravito-inertial and pressure modes detected in the B3 IV CoRoT target HD 43317

Author

Pápics, P. I., primary, Briquet, M., additional, Baglin, A., additional, Poretti, E., additional, Aerts, C., additional, Degroote, P., additional, Tkachenko, A., additional, Morel, T., additional, Zima, W., additional, Niemczura, E., additional, Rainer, M., additional, Hareter, M., additional, Baudin, F., additional, Catala, C., additional, Michel, E., additional, Samadi, R., additional, and Auvergne, M., additional

Published
2012
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237. The CoRoT B-type binary HD 50230: a prototypical hybrid pulsator with g-mode period and p-mode frequency spacings

Author

Degroote, P., primary, Aerts, C., additional, Michel, E., additional, Briquet, M., additional, Pápics, P. I., additional, Amado, P., additional, Mathias, P., additional, Poretti, E., additional, Rainer, M., additional, Lombaert, R., additional, Hillen, M., additional, Morel, T., additional, Auvergne, M., additional, Baglin, A., additional, Baudin, F., additional, Catala, C., additional, and Samadi, R., additional

Published
2012
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238. Pulsation spectrum ofδScuti stars: the binary HD 50870 as seen with CoRoT and HARPS

Author

Mantegazza, L., primary, Poretti, E., additional, Michel, E., additional, Rainer, M., additional, Baudin, F., additional, García Hernández, A., additional, Semaan, T., additional, Alvarez, M., additional, Amado, P. J., additional, Garrido, R., additional, Mathias, P., additional, Moya, A., additional, Suárez, J. C., additional, Auvergne, M., additional, Baglin, A., additional, Catala, C., additional, and Samadi, R., additional

Published
2012
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239. Probing the core structure and evolution of red giants using gravity-dominated mixed modes observed withKepler

Author

Mosser, B., primary, Goupil, M. J., additional, Belkacem, K., additional, Michel, E., additional, Stello, D., additional, Marques, J. P., additional, Elsworth, Y., additional, Barban, C., additional, Beck, P. G., additional, Bedding, T. R., additional, De Ridder, J., additional, García, R. A., additional, Hekker, S., additional, Kallinger, T., additional, Samadi, R., additional, Stumpe, M. C., additional, Barclay, T., additional, and Burke, C. J., additional

Published
2012
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240. Modelling a high-mass red giant observed by CoRoT

Author

Baudin, F., primary, Barban, C., additional, Goupil, M. J., additional, Samadi, R., additional, Lebreton, Y., additional, Bruntt, H., additional, Morel, T., additional, Lefèvre, L., additional, Michel, E., additional, Mosser, B., additional, Carrier, F., additional, De Ridder, J., additional, Hatzes, A., additional, Hekker, S., additional, Kallinger, T., additional, Auvergne, M., additional, Baglin, A., additional, and Catala, C., additional

Published
2012
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241. Characterization of the power excess of solar-like oscillations in red giants withKepler

Author

Mosser, B., primary, Elsworth, Y., additional, Hekker, S., additional, Huber, D., additional, Kallinger, T., additional, Mathur, S., additional, Belkacem, K., additional, Goupil, M. J., additional, Samadi, R., additional, Barban, C., additional, Bedding, T. R., additional, Chaplin, W. J., additional, García, R. A., additional, Stello, D., additional, De Ridder, J., additional, Middour, C. K., additional, Morris, R. L., additional, and Quintana, E. V., additional

Published
2011
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242. CoRoT’s view on variable B8/9 stars: spots versus pulsations

Author

Degroote, P., primary, Acke, B., additional, Samadi, R., additional, Aerts, C., additional, Kurtz, D. W., additional, Noels, A., additional, Miglio, A., additional, Montalbán, J., additional, Bloemen, S., additional, Baglin, A., additional, Baudin, F., additional, Catala, C., additional, Michel, E., additional, and Auvergne, M., additional

Published
2011
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243. Amplitudes and lifetimes of solar-like oscillations observed by CoRoT (Corrigendum)

Author

Baudin, F., primary, Barban, C., additional, Belkacem, K., additional, Hekker, S., additional, Morel, T., additional, Samadi, R., additional, Benomar, O., additional, Goupil, M.-J., additional, Carrier, F., additional, Ballot, J., additional, Deheuvels, S., additional, De Ridder, J., additional, Hatzes, A. P., additional, Kallinger, T., additional, and Weiss, W. W., additional

Published
2011
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244. Variability in the CoRoT photometry of three hot O-type stars

Author

Blomme, R., primary, Mahy, L., additional, Catala, C., additional, Cuypers, J., additional, Gosset, E., additional, Godart, M., additional, Montalban, J., additional, Ventura, P., additional, Rauw, G., additional, Morel, T., additional, Degroote, P., additional, Aerts, C., additional, Noels, A., additional, Michel, E., additional, Baudin, F., additional, Baglin, A., additional, Auvergne, M., additional, and Samadi, R., additional

Published
2011
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245. Mixed modes in red-giant stars observed with CoRoT

Author

Mosser, B., primary, Barban, C., additional, Montalbán, J., additional, Beck, P. G., additional, Miglio, A., additional, Belkacem, K., additional, Goupil, M. J., additional, Hekker, S., additional, De Ridder, J., additional, Dupret, M. A., additional, Elsworth, Y., additional, Noels, A., additional, Baudin, F., additional, Michel, E., additional, Samadi, R., additional, Auvergne, M., additional, Baglin, A., additional, and Catala, C., additional

Published
2011
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247. Accurate p-mode measurements of the G0V metal-rich CoRoT target HD 52265

Author

Ballot, J., primary, Gizon, L., additional, Samadi, R., additional, Vauclair, G., additional, Benomar, O., additional, Bruntt, H., additional, Mosser, B., additional, Stahn, T., additional, Verner, G. A., additional, Campante, T. L., additional, García, R. A., additional, Mathur, S., additional, Salabert, D., additional, Gaulme, P., additional, Régulo, C., additional, Roxburgh, I. W., additional, Appourchaux, T., additional, Baudin, F., additional, Catala, C., additional, Chaplin, W. J., additional, Deheuvels, S., additional, Michel, E., additional, Bazot, M., additional, Creevey, O., additional, Dolez, N., additional, Elsworth, Y., additional, Sato, K. H., additional, Vauclair, S., additional, Auvergne, M., additional, and Baglin, A., additional

Published
2011
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248. CoRoT high-precision photometry of the B0.5 IV star HD 51756

Author

Pápics, P. I., primary, Briquet, M., additional, Auvergne, M., additional, Aerts, C., additional, Degroote, P., additional, Niemczura, E., additional, Vučković, M., additional, Smolders, K., additional, Poretti, E., additional, Rainer, M., additional, Hareter, M., additional, Baglin, A., additional, Baudin, F., additional, Catala, C., additional, Michel, E., additional, and Samadi, R., additional

Published
2011
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249. An asteroseismic study of the O9V star HD 46202 from CoRoT space-based photometry

Author

Briquet, M., primary, Aerts, C., additional, Baglin, A., additional, Nieva, M. F., additional, Degroote, P., additional, Przybilla, N., additional, Noels, A., additional, Schiller, F., additional, Vučković, M., additional, Oreiro, R., additional, Smolders, K., additional, Auvergne, M., additional, Baudin, F., additional, Catala, C., additional, Michel, E., additional, and Samadi, R., additional

Published
2011
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