Spectrophotometry of simulated Stellar Populations (Schulz+, 2002)

Details Spectrophotometry of simulated Stellar Populations (Schulz+, 2002) Spectrophotometry of simulated Stellar Populations (Schulz+, 2002)

May 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ycat..33920001s&link_type=abstract

VizieR On-line Data Catalog: J/A+A/392/1. Originally published in: 2002A&A...392....1S

Mathematics

Logic

Clusters: Globular, Clusters: Open, Models: Evolutionary, Spectrophotometry, Colors

Scientific paper

Spectra, colors and luminosities in various filter-systems as well as cosmological and evolutionary corrections in 2 different cosmologies (H0=75, {Omega}0=0.1, {Lambda}0=0.9) (H0=65, {Omega0}=0.1, {Lambda0}=0.0). The total mass in stars of all SPSs are 1.6*109 solar masses at the beginning of evolution. The time-step is 4*106years. The UBV filters are from Buser & Kurucz (1978A&A....70..555B), the RI filter from Bessell (1990PASP..102.1181B) and JHK from Bessel & Brett (1988PASP..100.1134B).
Files are following the naming-convention: sa* = SSP with Salpeter IMF sc* = SSP with Scalo IMF The metallicities considered are: Z1 = 0.0004 = 0.02Z{sun} Z2 = 0.004 = 0.20Z{sun} Z3 = 0.008 = 0.40Z{sun} Z4 = 0.02 = 1.00Z{sun} Z5 = 0.05 = 2.50Z{sun}
(22 data files).

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