SPECTRUM: A stellar spectral synthesis program

Details SPECTRUM: A stellar spectral synthesis program SPECTRUM: A stellar spectral synthesis program

Oct 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ascl.soft10002g&link_type=abstract

Astrophysics Source Code Library, record ascl:9910.002

Astronomy and Astrophysics

Astrophysics

Scientific paper

SPECTRUM ((C) Richard O. Gray, 1992-2008) is a stellar spectral synthesis program which runs on a number of platforms, including most flavors of UNIX and LINUX . It will also run under Windows 9x/XP/NT/2000/(VISTA?) using the Cygwin tools or the distributed Windows binaries. The code for SPECTRUM has been written in the "C" language. SPECTRUM computes the LTE synthetic spectrum given a stellar atmosphere model. SPECTRUM can use as input the fully blanketed stellar atmosphere models of Robert Kurucz including the new models of Castelli and Kurucz, but any other stellar atmosphere model which can be cast into the format of Kurucz's models can be used as well. SPECTRUM can be programmed with "command-line switches" to give a number of different outputs. In the default mode, SPECTRUM computes the stellar-disk-integrated normalized-intensity spectrum, but in addition, SPECTRUM will compute the absolute monochromatic flux from the stellar atmosphere or the specific intensity from any point on the stellar surface.

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