Libraries of High and Mid-Resolution Spectra of F, G, K, and M Field Stars

Details Libraries of High and Mid-Resolution Spectra of F, G, K, and M Field Stars Libraries of High and Mid-Resolution Spectra of F, G, K, and M Field Stars

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ap%26ss.263..275m&link_type=abstract

Astrophysics and Space Science, v. 263, Issue 1/4, p. 275-278 (1998).

Astronomy and Astrophysics

Astrophysics

5

Scientific paper

I have compiled here the three libraries of high and mid-resolution optical spectra of late-type stars I have recently published. The libraries include F, G, K and M field stars, from dwarfs to giants. The spectral coverage is from 3800 to 1000 Å, with spectral resolution ranging from 0.09 to 3.0 Å. These spectra include many of the spectral lines most widely used as optical and near-infrared indicators of chromospheric activity. The spectra have been obtained with the aim of providing a library of high and mid-resolution spectra to be used in the study of active chromosphere stars by applying a spectral subtraction technique. However, the data set presented here can also be utilized in a wide variety of ways. A digital version of all the fully reduced spectra is available via FTP and the World Wide Web (WWW) in FITS format.

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