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| Reference : CoRot B star frequency analysis (Degroote+, 2009) |
| Computer developments : Other | |||
| Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics | |||
| http://hdl.handle.net/2268/132628 | |||
| CoRot B star frequency analysis (Degroote+, 2009) | |
| English | |
| Degroote, P. [> > > >] | |
| Aerts, C. [> > > >] | |
| Ollivier, M. [> > > >] | |
Miglio, Andrea  [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie] | |
| Debosscher, J. [> > > >] | |
| Cuypers, J. [> > > >] | |
| Briquet, Maryline [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie >] | |
| Montalban Iglesias, Josefa [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie] | |
| Thoul, Anne [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie] | |
| Noels-Grötsch, Arlette [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Département d'astrophys., géophysique et océanographie (AGO) >] | |
| De Cat, P. [> > > >] | |
| Balaguer-Nunez, L. [> > > >] | |
| Maceroni, C. [> > > >] | |
| Ribas, I. [> > > >] | |
| Auvergne, M. [> > > >] | |
| Baglin, A. [> > > >] | |
| Deleuil, M. [> > > >] | |
| Weiss, W. [> > > >] | |
| Jorda, L. [> > > >] | |
| Baudin, F. [> > > >] | |
| Samadi, R. [> >] | |
| 1-Jun-2009 | |
| [en] Stars: early-type ; Stars: B-type ; Stars: variable | |
| [en] Results of frequency analyses for 352 candidate B pulsators (candidate Be stars are ommitted) from CoRoT's initial run. For each star, the following information is given: frequency number, amplitude + error, frequency value + error, phase + error. The error values for large amplitude frequencies can be slightly underestimated, as they are not corrected for correlation effects. Also given are comments about every frequency: if they are expected to be due to instrumental effects (e.g. orbit of the satellite), if they are harmonics or higher order combinations of previously identified frequencies. (2 data files). | |
| http://hdl.handle.net/2268/132628 | |
| http://adsabs.harvard.edu/abs/2009yCat..35060471D | |
| stars.dat 352x40 Star positions; data/* 352x186 Frequency analysis for each star | |
| VizieR On-line Data Catalog: J/A+A/506/471 |
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