Zobrazeno 1 - 10
of 588
pro vyhledávání: '"Auvergne, M"'
Autor:
Cabrera, J., Csizmadia, Sz., Montagnier, G., Fridlund, M., Eiff, M. Ammler-von, Chaintreuil, S., Damiani, C., Deleuil, M., Ferraz-Mello, S., Ferrigno, A., Gandolfi, D., Guillot, T., Guenther, E. W., Hatzes, A., Hébrard, G., Klagyivik, P., Parviainen, H., Pasternacki, Th., Pätzold, M., Sebastian, D., Santos, M. Tadeu dos, Wuchterl, G., Aigrain, S., Alonso, R., Almenara, J. -M., Armstrong, J. D., Auvergne, M., Baglin, A., Barge, P., Barros, S. C. C., Bonomo, A. S., Bordé, P., Bouchy, F., Carpano, S., Chaffey, C., Deeg, H. J., Díaz, R. F., Dvorak, R., Erikson, A., Grziwa, S., Korth, J., Lammer, H., Lindsay, C., Mazeh, T., Moutou, C., Ofir, A., Ollivier, M., Pallé, E., Rauer, H., Rouan, D., Samuel, B., Santerne, A., Schneider, J.
Publikováno v:
Astronomy & Astrophysics, 2015, Volume 579, A36
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 sys
Externí odkaz:
http://arxiv.org/abs/1504.01532
Transiting exoplanets from the CoRoT space mission: XXVI. CoRoT-24: A transiting multi-planet system
Autor:
Alonso, R., Moutou, C., Endl, M., Almenara, J. M., Guenther, E. W., Deleuil, M., Hatzes, A., Aigrain, S., Auvergne, M., Baglin, A., Barge, P., Bonomo, A. S., Bordé, P., Bouchy, F., Cavarroc, C., Cabrera, J., Carpano, S., Csizmadia, Sz., Cochran, W. D., Deeg, H. J., Díaz, R. F., Dvorak, R., Erikson, A., Ferraz-Mello, S., Fridlund, M., Fruth, T., Gandolfi, D., Gillon, M., Grziwa, S., Guillot, T., Hébrard, G., Jorda, L., Léger, A., Lammer, H., Lovis, C., MacQueen, P. J., Mazeh, T., Ofir, A., Ollivier, M., Pasternacki, T., Patzold, M., Queloz, D., Rauer, H., Rouan, D., Santerne, A., Schneider, J., Santos, M. Tadeu dos, Tingley, B., Titz-Weider, R., Weingrill, J., Wuchterl, G.
Publikováno v:
A&A 567, A112 (2014)
We present the discovery of a candidate multiply-transiting system, the first one found in the CoRoT mission. Two transit-like features with periods of 5.11 and 11.76d are detected in the CoRoT light curve, around a main sequence K1V star of r=15.1.
Externí odkaz:
http://arxiv.org/abs/1406.1270
Autor:
Boumier, P., Benomar, O., Baudin, F., Verner, G., Appourchaux, T., Lebreton, Y., Gaulme, P., Chaplin, W., Garcia, R. A., Hekker, S., Regulo, C., Salabert, D., Stahn, T., Elsworth, Y., Gizon, L., Hall, M., Mathur, S., Michel, E., Morel, T., Mosser, B., Poretti, E., Rainer, M., Roxburgh, I., Nascimento Jr., J. -D. do, Samadi, R., Auvergne, M., Chaintreuil, S., Baglin, A., Catala, C.
Context. The object HD 43587Aa is a G0V star observed during the 145-day LRa03 run of the COnvection, ROtation and planetary Transits space mission (CoRoT), for which complementary High Accuracy Radial velocity Planet Searcher (HARPS) spectra with S/
Externí odkaz:
http://arxiv.org/abs/1402.5053
Autor:
Morel, T., Briquet, M., Auvergne, M., Alecian, G., Ghazaryan, S., Niemczura, E., Fossati, L., Lehmann, H., Hubrig, S., Ulusoy, C., Damerdji, Y., Rainer, M., Poretti, E., Borsa, F., Scardia, M., Schmid, V. S., Van Winckel, H., De Smedt, K., Papics, P. I., Gameiro, J. F., Waelkens, C., Fagas, M., Kaminski, K., Dimitrov, W., Baglin, A., Michel, E., Dumortier, L., Fremat, Y., Hensberge, H., Jorissen, A., Van Eck, S.
The existence of pulsations in HgMn stars is still being debated. To provide the first unambiguous observational detection of pulsations in this class of chemically peculiar objects, the bright star HD 45975 was monitored for nearly two months by the
Externí odkaz:
http://arxiv.org/abs/1311.4370
Autor:
Ozel, N., Mosser, B., Dupret, M. A., Bruntt, H., Barban, C., Deheuvels, S., García, R. A., Michel, E., Samadi, R., Baudin, F., Mathur, S., Régulo, C., Auvergne, M., Morel, P., Pichon, B.
The CoRoT short asteroseismic runs give us the opportunity to observe a large variety of late-type stars through their solar-like oscillations. We report the observation and modeling of the F5V star HD 175272. Our aim is to define a method for extrac
Externí odkaz:
http://arxiv.org/abs/1309.2009
Autor:
Paparó, M., Chadid, M., Chapellier, E., Benkő, J. M., Szabó, R., Kolenberg, K., Guggenberger, E., Regály, Zs., Auvergne, M., Baglin, A., Weiss, W. W.
Publikováno v:
Astronomy & Astrophysics (2011), Volume 531, A135, 12 pp
The star CoRoT102781750 reveals a puzzle, showing a very complex and altering variation in different `CoRoT colours'. We established without doubt that more than a single star was situated within the CoRoT mask. Using a search for periodicity as a to
Externí odkaz:
http://arxiv.org/abs/1308.3598
Autor:
Mathur, S., Bruntt, H., Catala, C., Benomar, O., Davies, G. R., Garcia, R. A., Salabert, D., Ballot, J., Mosser, B., Regulo, C., Chaplin, W. J., Elsworth, Y., Handberg, R., Hekker, S., Mantegazza, L., Michel, E., Poretti, E., Rainer, M., Roxburgh, I. W., Samadi, R., Steslicki, M., Uytterhoeven, K., Verner, G. A., Auvergne, M., Baglin, A., Forteza, S. Barcelo, Baudin, F., Cortes, T. Roca
The satellite CoRoT (Convection, Rotation, and planetary Transits) has provided high-quality data for almost six years. We show here the asteroseismic analysis and modeling of HD169392A, which belongs to a binary system weakly gravitationally bound a
Externí odkaz:
http://arxiv.org/abs/1308.0647
Autor:
Aerts, C., Simon-Diaz, S., Catala, C., Neiner, C., Briquet, M., Castro, N., Schmid, V. S., Scardia, M., Rainer, M., Poretti, E., Papics, I., Degroote, P., Bloemen, S., Oestensen, R. H., Auvergne, M., Baglin, A., Baudin, F., Michel, E., Samadi, R.
{We aim to detect and interpret photometric and spectroscopic variability of the bright CoRoT B-type supergiant target HD\,46769 ($V=5.79$). We also attempt to detect a magnetic field in the target.} {We analyse a 23-day oversampled CoRoT light curve
Externí odkaz:
http://arxiv.org/abs/1307.5791
Autor:
Hernández, A. García, Moya, A., Michel, E., Suárez, J. C., Poretti, E., Martín-Ruíz, S., Amado, P. J., Garrido, R., Rodríguez, E., Rainer, M., Uytterhoeven, K., Rodrigo, C., Solano, E., Rodón, J. R., Mathias, P., Rolland, A., Auvergne, M., Baglin, A., Baudin, F., Catala, C., Samadi, R.
The aim of this work was to use a multi-approach technique to derive the most accurate values possible of the physical parameters of the \delta Sct star HD174966. In addition, we searched for a periodic pattern in the frequency spectra with the goal
Externí odkaz:
http://arxiv.org/abs/1307.2739
Autor:
Paparo, M., Bognar, Zs., Benko, J. M., Gandolfi, D., Moya, A., Suarez, J. C., Sodor, A., Hareter, M., Poretti, E., Guenther, E. W., Auvergne, M., Baglin, A., Weiss, W. W.
The high accuracy of space data increased the number of the periodicities determined for pulsating variable stars, but the mode identification is still a critical point in the non-asymptotic regime. We use regularities in frequency spacings for ident
Externí odkaz:
http://arxiv.org/abs/1307.2553