VizieR Online Data Catalog: SSP in NIR. II. Synthesis models (Meneses-Goytia+, 2015)

S. Meneses-Goytia, R. F. Peletier, S. C. Trager, A. Vazdekis

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Abstract

The present Single Stellar Populations (SSP) models are derived from my Ph.D.'s thesis and this paper. The following nomenclature is used throughout the paper and the website (http://smg.astro-research.net/ssp-models/the-models/) to describe the models, e.g. MarS models use the M08 isochrones (Mar) and the Salpeter (S) IMF. General information about the models is given in table1. For further information, please refer to the paper. Each set of models and their corresponding predictions are available in the website and VIZIER. The spectral energy distributions (SEDs) can be downloaded in a zip-file from those pages in ascii format . The spectral energy distributions (SEDs) can be downloaded in a zip-file from t hose pages in ascii format . The nomenclature of each SED is as follows: isochroneIMFsedXXXXHZX.XXXXXXXXXTgXX.XXXXXXXe+XX - where XXXX tells whether those models contain C-stars or no (COMBO or NOCS respectively) H is the spectral band in which normalization occurred Z_X.XXXXXXXXX is the metallicity in terms of Z Tg_XX.XXXXXXXe+XX is the age in years. Each set of models contains MarS - 96 SEDs GirS - 96 SEDs BaSS - 116 SEDs We have also included in the websites the Integrated colours and line-strength indices from all our models (MarS, GirS and BaSS). The SEDs were convolved to a velocity dispersion of 350km/s before calculating indices. (5 data files).
Original languageEnglish
Pages (from-to)20097
JournalVizieR On-line Data Catalog
Volume358
Publication statusPublished - 1-Aug-2015

Keywords

  • Models: evolutionary
  • Photometry: infrared

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