Reference : The UVES Paranal Observatory Project: a public library of high resolution stellar spectra
Scientific congresses and symposiums : Paper published in a book
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/108088
The UVES Paranal Observatory Project: a public library of high resolution stellar spectra
English
Jehin, Emmanuel mailto [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique et traitement de l'image]
Bagnulo, S. [> > > >]
Melo, C. [> > > >]
Ledoux, C. [> > > >]
Cabanac, R. [> > > >]
FRANCOIS, Patricia [Centre Hospitalier Universitaire de Liège - CHU > > Radiothérapie]
Primas, F. [> > > >]
2005
From Lithium to Uranium: Elemental Tracers of Early Cosmic Evolution
Hill, V.
Cambridge University Press
IAU Symposium Proceedings of the international Astronomical Union 228
261-262
No
No
International
From Lithium to Uranium: Elemental Tracers of Early Cosmic Evolution
May 23-27, 2005
Hill, V.; François, P.; Primas, F.
Paris
France
[en] The UVES Paranal Observatory Project (POP), is an ESO public database of about 400 stars whose high quality spectra were obtained with UVES, the high resolution spectrometer of the VLT. All stars were observed with two instrument modes, in order to cover almost completely the optical region (300-1000 nm). The resolving power is about 80000, and for most of the spectra, the typical S/N ratio is 300-500 in the V band. Program stars fall into two groups, stars belonging to open clusters IC2391 and NGC6475, and bright field stars. For field stars, the only selection criterion applied was to cover the largest possible variety of spectral types in the HR diagram, including peculiar objects, e.g., Ap and Bp stars, Wolf-Rayet stars, Be stars, carbon stars and metal poor stars. The spectra have been reduced, coadded and merged and various products can be downloaded from a public area. For each star the final spectrum may be displayed through a dedicated user-friendly Spectral Preview Interface. The database is accessible at http://www.eso.org/uvespop
Researchers
http://hdl.handle.net/2268/108088
10.1017/S1743921305005739
http://adsabs.harvard.edu/abs/2005IAUS..228..261J

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