Zobrazeno 1 - 10
of 111
pro vyhledávání: '"Rendle, B."'
Autor:
Worley, C. C., Jofre, P., Rendle, B., Miglio, A., Magrini, L., Feuillet, D., Gavel, A., Smiljanic, R., Lind, K., Korn, A., Gilmore, G., Randich, S., Hourihane, A., Gonneau, A., Francois, P., Lewis, J., Sacco, G., Bragaglia, A., Heiter, U., Feltzing, S., Bensby, T., Irwin, M., Solares, E. Gonzalez, Murphy, D., Bayo, A., Sbordone, L., Zwitter, T., Lanzafame, A. C., Walton, N., Zaggia, S., Alfaro, E. J., Morbidelli, L., Sousa, S., Monaco, L., Carraro, G., Lardo, C.
Publikováno v:
A&A 643, A83 (2020)
The extensive stellar spectroscopic datasets that are available for studies in Galactic Archeaology thanks to, for example, the Gaia-ESO Survey, now benefit from having a significant number of targets that overlap with asteroseismology projects such
Externí odkaz:
http://arxiv.org/abs/2007.10189
Autor:
Buldgen, G., Farnir, M., Pezzotti, C., Eggenberger, P., Salmon, S. J. A. J., Montalban, J., Ferguson, J. W., Khan, S., Bourrier, V., Rendle, B. M., Meynet, G., Miglio, A., Noels, A.
Context. The CoRoT and Kepler missions have paved the way for synergies between exoplanetology and asteroseismology. The use of seismic data helps providing stringent constraints on the stellar properties which directly impact the results of planetar
Externí odkaz:
http://arxiv.org/abs/1907.10315
Autor:
Rendle, B. M., Miglio, A., Chiappini, C., Valentini, M., Davies, G. R., Mosser, B., Elsworth, Y., García, R. A., Mathur, S., Jofré, P., Worley, C. C., Casagrande, L., Girardi, L., Lund, M. N., Feuillet, D. K., Gavel, A., Magrini, L., Khan, S., Rodrigues, T. S., Johnson, J. A., Cunha, K., Lane, R. L., Nitschelm, C., Chaplin, W. J.
Analyses of data from spectroscopic and astrometric surveys have led to conflicting results concerning the vertical characteristics of the Milky Way. Ages are often used to provide clarity, but typical uncertainties of $>$ 40\,\% restrict the validit
Externí odkaz:
http://arxiv.org/abs/1906.07489
Autor:
Bugnet, L., García, R. A., Mathur, S., Davies, G. R., Hall, O. J., Lund, M. N., Rendle, B. M.
Publikováno v:
A&A 624, A79 (2019)
The NASA's Transiting Exoplanet Survey Satellite (TESS) is about to provide full-frame images of almost the entire sky. The amount of stellar data to be analysed represents hundreds of millions stars, which is several orders of magnitude above the am
Externí odkaz:
http://arxiv.org/abs/1902.09854
Autor:
Rendle, B. M., Buldgen, G., Miglio, A., Reese, D., Noels, A., Davies, G. R., Campante, T. L., Chaplin, W. J., Lund, M. N., Kuszlewicz, J. S., Scott, L. J. A., Scuflaire, R., Ball, W. H., Smetana, J., Nsamba, B.
A key aspect in the determination of stellar properties is the comparison of observational constraints with predictions from stellar models. Asteroseismic Inference on a Massive Scale (AIMS) is an open source code that uses Bayesian statistics and a
Externí odkaz:
http://arxiv.org/abs/1901.02663
The recently launched NASA Transiting Exoplanet Survey Satellite (TESS) mission is going to collect lightcurves for a few hundred million of stars and we expect to increase the number of pulsating stars to analyze compared to the few thousand stars o
Externí odkaz:
http://arxiv.org/abs/1811.12140
Autor:
Bugnet, L., García, R. A., Davies, G. R., Mathur, S., Corsaro, E., Hall, O. J., Rendle, B. M.
Publikováno v:
A&A 620, A38 (2018)
Asteroseismology provides global stellar parameters such as masses, radii or surface gravities using the mean global seismic parameters as well as the effective temperature for thousands of low-mass stars $(0.8 M_\odot
Externí odkaz:
http://arxiv.org/abs/1809.05105
Autor:
Buldgen, Gaël, Rendle, B., Sonoi, T., Davies, G. R., Miglio, A., Salmon, S. J. A. J., Reese, D. R., Bossini, D., Eggenberger, P., Noels, A., Scuflaire, R.
Since the CoRoT and Kepler missions, the availability of high quality seismic spectra for red giants has made them the standard clocks and rulers for Galactic Archeology. With the expected excellent data from the TESS and PLATO missions, red giants w
Externí odkaz:
http://arxiv.org/abs/1808.08391
Autor:
Nsamba, B., Campante, T. L., Monteiro, M. J. P. F. G., Cunha, M. S., Rendle, B. M., Reese, D. R., Verma, K.
Asteroseismic forward modelling techniques are being used to determine fundamental properties (e.g. mass, radius, and age) of solar-type stars. The need to take into account all possible sources of error is of paramount importance towards a robust de
Externí odkaz:
http://arxiv.org/abs/1804.04935
Autor:
Miglio, A., Chiappini, C., Mosser, B., Davies, G. R., Freeman, K., Girardi, L., Jofre, 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., Goupil, M. -J., Montalban, 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., Bienayme, 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., de Jong, R. S., de Laverny, P., Degl'Innocenti, S., Deheuvels, S., Depagne, E., DeRidder, J., DiMatteo, P., Di Mauro, M. P., Dupret, M. -A., Eggenberger, P., Elsworth, Y., Famaey, B., Feltzing, S., Garcia, R. A., Gerhard, O., Gibson, B. K., Gizon, L., Haywood, M., Handberg, R., Heiter, U., Hekker, S., Huber, D., Ibata, R., Katz, D., Kawaler, S. D., Kjeldsen, H., 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., Reyle, C., Robin, A., Roxburgh, I. W., Salaris, M., Santiago, B. X., 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.
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 maps of the Galaxy. Data from large-scale astrometric and spectroscopic surveys will soon
Externí odkaz:
http://arxiv.org/abs/1706.03778