8500-8750{AA} high resolution spectroscopy. III. Virtual Observatory Resource

Authors

1. Castelli F.
2. Munari U.

Published by

CDS

Abstract

In this paper we complete the library of synthetic spectra for the range 7650-8750{AA}, which includes the 8500-8750{AA} interval currently base-lined for the spectroscopic observations by GAIA, candidate ESA Cornerstone 5 mission. As for Paper II (Munari & Castelli, Cat. <J/A+AS/141/141>), the spectra are based on Kurucz's codes and line data. The explored metallicity, gravity and temperature ranges are -2.5<=[Z/Z_{sun}_]<=+0.5, 4.5<=logg<=2.0 and 7750<=T_eff_<=50000K, respectively. The 698 new spectra are computed at the same {lambda}/{Delta}{lambda}=20000 resolving power of the observed spectra given in Paper I (Munari & Castelli, Cat. <J/A+AS/137/521>) (131 standard stars mapping the MKK spectral classification system) and the 254 synthetic spectra of Paper II (characterized by T_eff_<=7500K).

Keywords

1. astronomical-models
2. stellar-atmospheres
3. spectroscopy

Bibliographic source Bibcode

2001A&A...366.1003C

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IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/366/1003

Document Object Identifer DOI

doi:10.26093/cds/vizier.33661003

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