Search Results - "Creevey, O."

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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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    Journal Article
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    PLATO as it is: A legacy mission for Galactic archaeology by Miglio, A., Chiappini, C., Mosser, B., Davies, G. R., Freeman, K., Girardi, L., Jofré, P., Kawata, D., Rendle, B. M., Valentini, M., Casagrande, L., Chaplin, W. J., Gilmore, G., Hawkins, K., Holl, B., Appourchaux, T., Belkacem, K., Bossini, D., Brogaard, K., Montalbán, J., Noels, A., Anders, F., Rodrigues, T., Piotto, G., Pollacco, D., Rauer, H., Prieto, C. Allende, Avelino, P. P., Babusiaux, C., Barban, C., Barbuy, B., Basu, S., Baudin, F., Benomar, O., Bienaymé, O., Binney, J., Bland‐Hawthorn, J., Bressan, A., Cacciari, C., Campante, T. L., Cassisi, S., Christensen‐Dalsgaard, J., Combes, F., Creevey, O., Cunha, M. S., Jong, R. S., Laverny, P., Degl'Innocenti, S., Deheuvels, S., Ridder, J., Matteo, P. Di, Mauro, M. P. Di, Dupret, M.‐A., Eggenberger, P., Elsworth, Y., Famaey, B., Feltzing, S., Gerhard, O., Gibson, B. K., Gizon, L., Haywood, M., Handberg, R., Heiter, U., Hekker, S., Huber, D., Ibata, R., Katz, D., Kawaler, S. D., Kurtz, D. W., Lagarde, N., Lebreton, Y., Lund, M. N., Majewski, S. R., Marigo, P., Martig, M., Mathur, S., Minchev, I., Morel, T., Ortolani, S., Pinsonneault, M. H., Plez, B., Moroni, P. G. Prada, Pricopi, D., Recio‐Blanco, A., Reylé, C., Robin, A., Roxburgh, I. W., Salaris, M., Schiavon, R., Serenelli, A., Sharma, S., Aguirre, V. Silva, Soubiran, C., Steinmetz, M., Stello, D., Strassmeier, K. G., Ventura, P., Ventura, R., Walton, N. A., Worley, C. C.

    Published in Astronomische Nachrichten (01-07-2017)
    “…Deciphering the assembly history of the Milky Way is a formidable task, which becomes possible only if one can produce high‐resolution chrono‐chemo‐kinematical…”
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    Journal Article Web Resource
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    A large sample of calibration stars for Gaia: log g from Kepler and CoRoT fields by Creevey, O. L., Thévenin, F., Basu, S., Chaplin, W. J., Bigot, L., Elsworth, Y., Huber, D., Monteiro, M. J. P. F. G., Serenelli, A.

    “…Asteroseismic data can be used to determine stellar surface gravities with precisions of <0.05 dex by using the global seismic quantities 〈Δν〉 and νmax along…”
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    Journal Article
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    The Complementary Roles of Interferometry and Asteroseismology in Determining the Mass of Solar-Type Stars by Creevey, O. L, Monteiro, M. J. P. F. G, Metcalfe, T. S, Brown, T. M, Jiménez-Reyes, S. J, Belmonte, J. A

    Published in The Astrophysical journal (10-04-2007)
    “…How important is an independent diameter measurement for the determination of stellar parameters of solar-type stars? When coupled with seismic observables,…”
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    Journal Article
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    Constraining the Properties of Delta Scuti Stars Using Spectroscopic Eclipsing Binary Systems by Creevey, O. L, Metcalfe, T. S, Brown, T. M, Jiménez-Reyes, S, Belmonte, J. A

    Published in The Astrophysical journal (20-05-2011)
    “…Many stars exhibit stellar pulsations, favoring them for asteroseismic analyses. Interpreting the oscillations requires some knowledge of the oscillation mode…”
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    Journal Article
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    A New Detached M Dwarf Eclipsing Binary by Creevey, O. L, Benedict, G. F, Brown, T. M, Alonso, R, Cargile, P, Mandushev, G, Charbonneau, D, McArthur, B. E, Cochran, W, O’Donovan, F. T, Jiménez-Reyes, S. J, Belmonte, J. A, Kolinski, D

    Published in The Astrophysical journal (01-06-2005)
    “…We describe a newly discovered detached M dwarf eclipsing binary system. This system was first observed by the TrES network during a long-term photometry…”
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    Journal Article
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    CHARACTERIZING TWO SOLAR-TYPE KEPLER SUBGIANTS WITH ASTEROSEISMOLOGY: KIC 10920273 AND KIC 11395018 by Dogan, G, Metcalfe, T S, Deheuvels, S, Di Mauro, M P, Eggenberger, P, Creevey, O L, MONTEIRO, M J P F G, Pinsonneault, M, Frasca, A, Karoff, C

    Published in The Astrophysical journal (20-01-2013)
    “…Determining fundamental properties of stars through stellar modeling has improved substantially due to recent advances in asteroseismology. Thanks to the…”
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    Journal Article
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    A semi–automatic procedure for abundance determination of A– and F–type stars by Hekker, S., Frémat, Y., Lampens, P., De Cat, P., Niemczura, E., Creevey, O. L., Zorec, J.

    “…A variety of physical processes leading to different types of pulsations and chemical compositions are observed between A– and F–type stars. To investigate the…”
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    Journal Article
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    Testing Asteroseismic Scaling Relations with Interferometry by White, T. R., Aguirre, V. Silva, Boyajian, T., Creevey, O., Huber, D., von Braun, K., Bedding, T. R., Elsworth, Y., Hekker, S., Stello, D., Weiss, A.

    Published in EPJ Web of conferences (01-01-2015)
    “…The asteroseismic scaling relations for the frequency of maximum oscillation power, vmax, and the large frequency separation, Δν, provide an easy way to…”
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    Journal Article Conference Proceeding
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    Benchmarking the effective temperature scale of red giant branch stellar models: the case of the metal-poor halo giant HD 122563 by Creevey, O. L, Cassisi, S, Thévenin, F, Salaris, M, Pietrinferni, A

    Published 05-04-2024
    “…A&A 689, A243 (2024) There is plenty of evidence in the literature of significant discrepancies between the observations and models of metal-poor red giant…”
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    Journal Article
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    Asteroseismic age constraints on the open cluster NGC 2477 using oscillating stars identified with TESS FFI by Palakkatharappil, D. B, Creevey, O. L

    Published 21-03-2023
    “…A&A 674, A146 (2023) The ages of pulsating stars in clusters can be determined by isochrone fitting and it can be further improved by asteroseismic modelling…”
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    Journal Article
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