Search Results - "Salabert, D."

Asteroseismic inference on rotation, gyrochronology and planetary system dynamics of 16 Cygni by Davies, G R, Chaplin, W J, Farr, W M, Garcia, R A, Lund, M N, Mathis, S, Metcalfe, T S, Appourchaux, T, Basu, S, Benomar, O, Campante, T L, Ceillier, T, Elsworth, Y, Handberg, R, Salabert, D, Stello, D

“…The solar analogues 16 Cyg A and B are excellent asteroseismic targets in the Kepler field of view and together with a red dwarf and a Jovian planet form an…”
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PROBING THE DEEP END OF THE MILKY WAY WITH KEPLER: ASTEROSEISMIC ANALYSIS OF 854 FAINT RED GIANTS MISCLASSIFIED AS COOL DWARFS by Mathur, S., García, R. A., Huber, D., Regulo, C., Stello, D., Beck, P. G., Houmani, K., Salabert, D.

“…ABSTRACT Asteroseismology has proven to be an excellent tool to determine not only global stellar properties with good precision, but also to infer the stellar…”
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Rotation periods and seismic ages of KOIs – comparison with stars without detected planets from Kepler observations by Ceillier, T., van Saders, J., García, R. A., Metcalfe, T. S., Creevey, O., Mathis, S., Mathur, S., Pinsonneault, M. H., Salabert, D., Tayar, J.

“…One of the most difficult properties to derive for stars is their age. For cool main-sequence stars, gyrochronology relations can be used to infer stellar ages…”
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TESTING SCALING RELATIONS FOR SOLAR-LIKE OSCILLATIONS FROM THE MAIN SEQUENCE TO RED GIANTS USING KEPLER DATA by HUBER, D, BEDDING, T. R, ELSWORTH, Y. P, HALE, S. J, KALLINGER, T, SILVA AGUIRRE, V, CHAPLIN, W. J, DE RIDDER, J, GARCIA, R. A, APPOURCHAUX, T, FRANDSEN, S, HOUDEK, G, STELLO, D, MOLENDA-ZAKOWICZ, J, MONTEIRO, M. J. P. F. G, CHRISTENSEN-DALSGAARD, J, GILLILAND, R. L, KAWALER, S. D, KJELDSEN, H, BROOMHALL, A. M, CORSARO, E, SALABERT, D, SANDERFER, D. T, HEKKER, S, SEADER, S. E, SMITH, J. C, MATHUR, S, MOSSER, B, VERNER, G. A, BONANNO, A, BUZASI, D. L, CAMPANTE, T. L

“…We have analyzed solar-like oscillations in ~1700 stars observed by the Kepler Mission, spanning from the main sequence to the red clump. Using evolutionary…”
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Improving the diameters of interferometric calibrators with MATISSE by Robbe-Dubois, S, Cruzalèbes, P, Berio, Ph, Meilland, A, Petrov, R-G, Allouche, F, Salabert, D, Paladini, C, Matter, A, Millour, F, Lagarde, S, Lopez, B, Burtscher, L, Jaffe, W, Hron, J, Percheron, I, van Boekel, R, Weigelt, G, Stee, Ph

“…ABSTRACT A good knowledge of the angular diameters of stars used to calibrate the observables in stellar interferometry is fundamental. As the available…”
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ERRATUM: "PROBING THE DEEP END OF THE MILKY WAY WITH KEPLER: ASTEROSEISMIC ANALYSIS OF 854 FAINT RED GIANTS MISCLASSIFIED AS COOL DWARFS" (2016, ApJ, 827, 50) by Mathur, S., García, R. A., Huber, D., Regulo, C., Stello, D., Beck, P. G., Houmani, K., Salabert, D.

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Measurement of Low Signal-To-Noise Ratio Solar p-Modes in Spatially Resolved Helioseismic Data by Salabert, D, Leibacher, J, Appourchaux, T, Hill, F

“…We present an adaptation of the rotation-corrected, m-averaged spectrum technique designed to observe low signal-to-noise ratio (S/N), low-frequency solar…”
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On the Determination and Constancy of the Solar Oblateness by Meftah, M., Irbah, A., Hauchecorne, A., Corbard, T., Turck-Chièze, S., Hochedez, J.-F., Boumier, P., Chevalier, A., Dewitte, S., Mekaoui, S., Salabert, D.

“…The equator-to-pole radius difference (Δ r = R eq − R pol ) is a fundamental property of our star, and understanding it will enrich future solar and stellar…”
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Picard SODISM, a Space Telescope to Study the Sun from the Middle Ultraviolet to the Near Infrared by Meftah, M., Hochedez, J.-F., Irbah, A., Hauchecorne, A., Boumier, P., Corbard, T., Turck-Chièze, S., Abbaki, S., Assus, P., Bertran, E., Bourget, P., Buisson, F., Chaigneau, M., Damé, L., Djafer, D., Dufour, C., Etcheto, P., Ferrero, P., Hersé, M., Marcovici, J.-P., Meissonnier, M., Morand, F., Poiet, G., Prado, J.-Y., Renaud, C., Rouanet, N., Rouzé, M., Salabert, D., Vieau, A.-J.

“…The Solar Diameter Imager and Surface Mapper (SODISM) onboard the Picard space mission provides wide-field images of the photosphere and chromosphere of the…”
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Extracting surface rotation periods of solar-like Kepler targets by Ceillier, T., García, R.A., Salabert, D., Mathur, S.

“…We use various method to extract surface rotation periods of Kepler targets exhibiting solar-like oscillations and compare their results…”
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Acoustic glitches in solar-type stars from Kepler by Mazumdar, A., Monteiro, M.J.P.F.G., Ballot, J., Antia, H.M., Basu, S., Houdek, G., Mathur, S., Cunha, M.S., Silva Aguirre, V., García, R.A., Salabert, D., Verner, G.A., Christensen-Dalsgaard, J., Metcalfe, T.S., Chaplin, W.J.

“…We report the measurement of the acoustic locations of layers of sharp variation in sound speed in the interiors of 19 solar‐type stars observed by the Kepler…”
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Damping and Excitation Variations of the Solar Acoustic Modes Using LOWL Observations by Salabert, D, Jiménez-Reyes, S. J

“…We have used observations made with the helioseismic instrument LOWL collected over 66 years to carry out an independent study of the variations of the p-mode…”
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Solar FLAG hare and hounds: on the extraction of rotational p-mode splittings from seismic, Sun-as-a-star data by Chaplin, W. J., Appourchaux, T., Baudin, F., Boumier, P., Elsworth, Y., Fletcher, S. T., Fossat, E., García, R. A., Isaak, G. R., Jiménez, A., Jiménez-Reyes, S. J., Lazrek, M., Leibacher, J. W., Lochard, J., New, R., Pallé, P., Régulo, C., Salabert, D., Seghouani, N., Toutain, T., Wachter, R.

“…We report on results from the first solar Fitting at Low-Angular degree Group (solar FLAG) hare-and-hounds exercise. The group is concerned with the…”
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solarFLAG hare and hounds: estimation of p-mode frequencies from Sun-as-star helioseismology data by Jiménez-Reyes, S. J., Chaplin, W. J., García, R. A., Appourchaux, T., Baudin, F., Boumier, P., Elsworth, Y., Fletcher, S. T., Lazrek, M., Leibacher, J. W., Lochard, J., New, R., Régulo, C., Salabert, D., Toutain, T., Verner, G. A., Wachter, R.

“…We report on the results of the latest solarFLAG hare-and-hounds exercise, which was concerned with testing methods for extraction of frequencies of low-degree…”
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MEASUREMENT OF ACOUSTIC GLITCHES IN SOLAR-TYPE STARS FROM OSCILLATION FREQUENCIES OBSERVED BY KEPLER by Mazumdar, A, MONTEIRO, M J P F G, Ballot, J, Antia, H M, Basu, S, Houdek, G, Mathur, S, Cunha, M S, Aguirre, V Silva, Garcia, R A

“…For the very best and brightest asteroseismic solar-type targets observed by Kepler, the frequency precision is sufficient to determine the acoustic depths of…”
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A UNIFORM ASTEROSEISMIC ANALYSIS OF 22 SOLAR-TYPE STARS OBSERVED BY KEPLER by MATHUR, S, METCALFE, T. S, STELLO, D, APPOURCHAUX, T, CAMPANTE, T. L, CHAPLIN, W. J, GARCIA, R. A, BEDDING, T. R, BENOMAR, O, BONANNO, A, DEHEUVELS, S, ELSWORTH, Y, WOITASZEK, M, GAULME, P, GUZIK, J. A, HANDBERG, R, HEKKER, S, HERZBERG, W, MONTEIRO, M. J. P. F. G, PIAU, L, QUIRION, P.-O, REGULO, C, ROTH, M, BRUNTT, H, SALABERT, D, SERENELLI, A, THOMPSON, M. J, TRAMPEDACH, R, WHITE, T. R, BALLOT, J, BRANDAO, I. M, MOLENDA-ZAKOWICZ, J, KJELDSEN, H, TWICKEN, J. D, VERNER, G. A, UDDIN, K, WOHLER, B, CHRISTENSEN-DALSGAARD, J, CREEVEY, O. L, DOGAN, G, BASU, S, KAROFF, C

“…Asteroseismology with the Kepler space telescope is providing not only an improved characterization of exoplanets and their host stars, but also a new window…”
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A Precise Asteroseismic Age and Radius for the Evolved Sun-like Star KIC 11026764 by Metcalfe, T. S, Monteiro, M. J. P. F. G, Thompson, M. J, Molenda-Żakowicz, J, Appourchaux, T, Chaplin, W. J, Doğan, G, Eggenberger, P, Bedding, T. R, Bruntt, H, Creevey, O. L, Quirion, P.-O, Stello, D, Bonanno, A, Silva Aguirre, V, Basu, S, Esch, L, Gai, N, Di Mauro, M. P, Kosovichev, A. G, Kitiashvili, I. N, Suárez, J. C, Moya, A, Piau, L, García, R. A, Marques, J. P, Frasca, A, Biazzo, K, Sousa, S. G, Dreizler, S, Bazot, M, Karoff, C, Frandsen, S, Wilson, P. A, Brown, T. M, Christensen-Dalsgaard, J, Gilliland, R. L, Kjeldsen, H, Campante, T. L, Fletcher, S. T, Handberg, R, Régulo, C, Salabert, D, Schou, J, Verner, G. A, Ballot, J, Broomhall, A.-M, Elsworth, Y, Hekker, S, Huber, D, Mathur, S, New, R, Roxburgh, I. W, Sato, K. H, White, T. R, Borucki, W. J, Koch, D. G, Jenkins, J. M

“…The primary science goal of the Kepler Mission is to provide a census of exoplanets in the solar neighborhood, including the identification and…”
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Global asteroseismic properties of solar-like oscillations observed by Kepler: a comparison of complementary analysis methods by Verner, G. A., Elsworth, Y., Chaplin, W. J., Campante, T. L., Corsaro, E., Gaulme, P., Hekker, S., Huber, D., Karoff, C., Mathur, S., Mosser, B., Appourchaux, T., Ballot, J., Bedding, T. R., Bonanno, A., Broomhall, A.-M., García, R. A., Handberg, R., New, R., Stello, D., Régulo, C., Roxburgh, I. W., Salabert, D., White, T. R., Caldwell, D. A., Christiansen, J. L., Fanelli, M. N.

“…We present the asteroseismic analysis of 1948 F-, G- and K-type main-sequence and subgiant stars observed by the National Aeronautics and Space Administration…”
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Asteroseismology of Solar-Type Stars with K2: Detection of Oscillations in C1 Data by Chaplin, W. J., Lund, M. N., Handberg, R., Basu, S., Buchhave, L. A., Campante, T. L., Davies, G. R., Huber, D., Latham, D. W., Latham, C. A., Serenelli, A., Antia, H. M., Appourchaux, T., Ball, W. H., Benomar, O., Casagrande, L., Christensen-Dalsgaard, J., Coelho, H. R., Creevey, O. L., Elsworth, Y., García, R. A., Gaulme, P., Hekker, S., Kallinger, T., Karoff, C., Kawaler, S. D., Kjeldsen, H., Lundkvist, M. S., Marcadon, F., Mathur, S., Miglio, A., Mosser, B., Régulo, C., Roxburgh, I. W., Silva Aguirre, V., Stello, D., Verma, K., White, T. R., Bedding, T. R., Barclay, T., Buzasi, D. L., Dehuevels, S., Gizon, L., Houdek, G., Howell, S. B., Salabert, D., Soderblom, D. R.

“…We present the first detections by the NASA K2 mission of oscillations in solar-type stars, using short-cadence data collected during K2 Campaign 1 (C1). We…”
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DETECTION OF SOLAR-LIKE OSCILLATIONS, OBSERVATIONAL CONSTRAINTS, AND STELLAR MODELS FOR θ CYG, THE BRIGHTEST STAR OBSERVED BY THE KEPLER MISSION by Guzik, J. A., Houdek, G., Chaplin, W. J., Smalley, B., Kurtz, D. W., Gilliland, R. L., Mullally, F., Rowe, J. F., Bryson, S. T., Still, M. D., Antoci, V., Appourchaux, T., Basu, S., Bedding, T. R., Benomar, O., Garcia, R. A., Huber, D., Kjeldsen, H., Latham, D. W., Metcalfe, T. S., Pápics, P. I., White, T. R., Aerts, C., Ballot, J., Boyajian, T. S., Briquet, M., Bruntt, H., Buchhave, L. A., Campante, T. L., Catanzaro, G., Christensen-Dalsgaard, J., Davies, G. R., Doğan, G., Dragomir, D., Doyle, A. P., Elsworth, Y., Frasca, A., Gaulme, P., Gruberbauer, M., Handberg, R., Hekker, S., Karoff, C., Lehmann, H., Mathias, P., Mathur, S., Miglio, A., Molenda- akowicz, J., Mosser, B., Murphy, S. J., Régulo, C., Ripepi, V., Salabert, D., Sousa, S. G., Stello, D., Uytterhoeven, K.

“…ABSTRACT θ Cygni is an F3 spectral type magnitude V = 4.48 main-sequence star that was the brightest star observed by the original Kepler spacecraft mission…”
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