The<i>Kepler</i>characterization of the variability among A- and F-type stars
K. UytterhoevenAstrophysique, Instrumentation et ModélisationA. MoyaLaboratorio de Astrofísica Estelar y Exoplanetas, LAEX-CAB (INTA-CSIC), PO BOX 78, 28691 Villanueva de la Cañada, Madrid, SpainA. GrigahcèneCentro de Astrofísica, Faculdade de Ciências, Universidade do Porto, Rua das Estrelas, 4150-762 Porto, PortugalJ. A. GuzikLos Alamos National Laboratory, XTD-2, Los Alamos, NM 87545-2345, USAJ. Gutiérrez-SotoSorbonne UniversitéB. SmalleyAstrophysics Group, Keele University, Staffordshire, ST5 5BG, UKG. HandlerInstitut für Astronomie, Türkenschanzstraße 17, 1180 Wien, AustriaL. A. BalonaSouth African Astronomical Observatory, PO Box 9, Observatory 7935, South AfricaE. NiemczuraInstytut Astronomiczny, Uniwersytet Wrocławski, Kopernika 11, 51-622 Wrocław, PolandL. Fox MachadoS. BenattiCISAS, Padova University, via Venezia 15, 35131 Padova, ItalyE. ChapellierInstitut de Biologie ValroseA. TkachenkoInstituut voor Sterrenkunde, K.U.Leuven, Celestijnenlaan 200D, 3001 Leuven, BelgiumR. SzabóHungarian Academy of SciencesJ. C. SuárezInstituto de Astrofísica de Andalucía (CSIC), Apartado 3004, 18080 Granada, SpainV. RipepiINAF - Osservatorio Astronomico di Capodimonte, via Moiariello 16, 80131 Napoli, ItalyJ. PascualInstituto de Astrofísica de Andalucía (CSIC), Apartado 3004, 18080 Granada, SpainP. MathiasLab. d’Astrophysique de Toulouse-Tarbes, Université de Toulouse, CNRS, 57 avenue d’Azereix, 65000 Tarbes, FranceS. Martín-RuízInstituto de Astrofísica de Andalucía (CSIC), Apartado 3004, 18080 Granada, SpainH. LehmannThüringer Landessternwarte Tautenburg, 07778 Tautenburg, GermanyJ. JackiewiczDepartment of Astronomy, New Mexico State University, Las Cruces, NM 88001, USAS. HekkerUniversity of Birmingham, School of Physics and Astronomy, Edgbaston, Birmingham B15 2TT, UKM. GruberbauerDepartment of Astronomy and Physics, Saint Marys University, Halifax, NS B3H 3C3, CanadaR. A. GarcíaCentre National de la Recherche ScientifiqueX. DumusqueCentro de Astrofísica, Faculdade de Ciências, Universidade do Porto, Rua das Estrelas, 4150-762 Porto, PortugalD. Díaz-FraileInstituto de Astrofísica de Andalucía (CSIC), Apartado 3004, 18080 Granada, SpainP. BradleyLos Alamos National Laboratory, XCP-6, MS T-087, Los Alamos, NM 87545-2345, USAV. AntociM. RothKiepenheuer-Institut für Sonnenphysik, Schöneckstraße 6, 79104 Freiburg im Breisgau, GermanyB. LeroyDélégation Paris 7S. J. MurphyJeremiah Horrocks Institute of Astrophysics, University of Central Lancashire, Preston PR1 2HE, UKP. De CatRoyal Observatory of Belgium, Ringlaan 3, 1180 Brussel, BelgiumJ. CuypersRoyal Observatory of Belgium, Ringlaan 3, 1180 Brussel, BelgiumH. KjeldsenDepartment of Physics and Astronomy, University of Aarhus, bygn. 1520, Ny Munkegade, 8000 Aarhus C., DenmarkJ. Christensen-DalsgaardDepartment of Physics and Astronomy, University of Aarhus, bygn. 1520, Ny Munkegade, 8000 Aarhus C., DenmarkM. BregerDepartment of Astronomy, University of Texas, Austin, TX 78712, USAA. PigulskiInstytut Astronomiczny, Uniwersytet Wrocławski, Kopernika 11, 51-622 Wrocław, PolandL. L. KissSydney Institute for Astronomy, School of Physics, A28, The University of Sydney, NSW, 2006, AustraliaM. StillBay Area Environmental Research Inst./NASA Ames Research Center, Moffett Field, CA 94035, USAS. E. ThompsonSearch for Extraterrestrial IntelligenceJ. Van CleveSETI Institute/NASA Ames Research Center, Moffett Field, CA 94035, USA
2011en
ABI
Annotatsiya
Context. The Kepler spacecraft is providing time series of photometric data with micromagnitude precision for hundreds of A-F type stars.
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