Publication date
March 2022
DOIAbstract
Simple stellar population spectra from Venkatesan et al. (2003; ApJ; 584; 621) in the Galacticus format. Two models are provided. Both assume a Salpeter IMF, one from 10-140M☉ and the other from 1-100M☉
Simple stellar population spectra from Venkatesan et al. (2003; ApJ; 584; 621) in the Galacticus format. Two models are provided. Both assume a Salpeter IMF, one from 10-140M☉ and the other from 1-100M☉
published in A&A. The arXiv version includes also the online tables. Reference spectra will later be...
We present synthetic spectral energy distributions (SEDs) for single-age, single-metallicity stellar...
Context. Models of stellar spectra are necessary for interpreting light from individual stars, plane...
Models from Bruzual & Charlot (2003; MNRAS; 344; 1000). Data was downloaded from http://www2.iap.fr/...
Models from Conroy & Gunn (2010; ascl:1010.043). SSP_Spectra_Conroy-et-al_v2.5_imfChabrier.hdf5...
Three basic ingredients are required to generate a simple stellar population (SSP) library, i.e. an ...
The present Single Stellar Populations (SSP) models are derived from my Ph.D.'s thesis and this pape...
We have compared simple stellar populations (SSPs) generated with different population synthesis too...
Context. Our ability to extract information from the spectra of stars depends on reliable models of ...
We study systematics associated with estimating simple stellar population (SSP) parameters – age, me...
We use the star counts model of Ortiz & Lépine (1993) to perform an unprecedented ex-ploration ...
Models from Maraston (2005, MNRAS, 362, 799); Maraston (1998, MNRAS, 300, 872). Data downloaded from...
We estimated the Galactic model parameters by means of a new approach based on the comparison of the...
We present simple stellar population (SSP) models with scaled-solar and α-element-enhanced abundance...
We perform a direct comparison of two state-of-the art single stellar population (SSP) models that h...
published in A&A. The arXiv version includes also the online tables. Reference spectra will later be...
We present synthetic spectral energy distributions (SEDs) for single-age, single-metallicity stellar...
Context. Models of stellar spectra are necessary for interpreting light from individual stars, plane...
Models from Bruzual & Charlot (2003; MNRAS; 344; 1000). Data was downloaded from http://www2.iap.fr/...
Models from Conroy & Gunn (2010; ascl:1010.043). SSP_Spectra_Conroy-et-al_v2.5_imfChabrier.hdf5...
Three basic ingredients are required to generate a simple stellar population (SSP) library, i.e. an ...
The present Single Stellar Populations (SSP) models are derived from my Ph.D.'s thesis and this pape...
We have compared simple stellar populations (SSPs) generated with different population synthesis too...
Context. Our ability to extract information from the spectra of stars depends on reliable models of ...
We study systematics associated with estimating simple stellar population (SSP) parameters – age, me...
We use the star counts model of Ortiz & Lépine (1993) to perform an unprecedented ex-ploration ...
Models from Maraston (2005, MNRAS, 362, 799); Maraston (1998, MNRAS, 300, 872). Data downloaded from...
We estimated the Galactic model parameters by means of a new approach based on the comparison of the...
We present simple stellar population (SSP) models with scaled-solar and α-element-enhanced abundance...
We perform a direct comparison of two state-of-the art single stellar population (SSP) models that h...
published in A&A. The arXiv version includes also the online tables. Reference spectra will later be...
We present synthetic spectral energy distributions (SEDs) for single-age, single-metallicity stellar...
Context. Models of stellar spectra are necessary for interpreting light from individual stars, plane...
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