Population Synthesis Models at very low metallicities (Schaerer, 2003)

Details Population Synthesis Models at very low metallicities (Schaerer, 2003) Population Synthesis Models at very low metallicities (Schaerer, 2003)

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ycat.6109....0s&link_type=abstract

VizieR On-line Data Catalog: VI/109. Originally published in: 2003A&A...397..527S

Computer Science

Models: Atmosphere, Models: Evolutionary, Populations: Stellar, Spectra: Ultraviolet

Scientific paper

All the models used are included in the tar file "models.tar", which contains a README file describing the file naming conventions depending on the values of the parameters (see note (G1)). There are five different types of output for each set of parameter values, designated by a number between 20 and 24, which are also presented in tabular form in the files type20.dat to type24.dat.
All the quantities are normalised to a total burst mass of 1solMass; note that different normalisation conventions may be found elsewhere, e.g. Starburst99 (Leitherer et al., 1999ApJS..123....3L) which is normalised to a burst of 106^solMass.
The models are computed with the pop-iso-25 code Version 2.5.
(7 data files).

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