1999
DOI: 10.1007/978-3-540-49460-7_56
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Semi-Analytic Models and Background Hydrogen-Ionizing Flux

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Cited by 204 publications
(333 citation statements)
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“…A well-calibrated model is clearly needed for the progenitor predictions to be reliable. Note that in the redshift interval (z < 1) and for the wavelength range (B and V band) studied in this paper, the population synthesis models employed by the fiducial GALICS model -STARDUST (Devriendt et al 1999) -provide virtually identical results to other commonly used models (Yi 2003;Bruzual & Charlot 2003;Maraston 2005).…”
Section: Reproduction Of the Early-type Galaxy Populationmentioning
confidence: 56%
“…A well-calibrated model is clearly needed for the progenitor predictions to be reliable. Note that in the redshift interval (z < 1) and for the wavelength range (B and V band) studied in this paper, the population synthesis models employed by the fiducial GALICS model -STARDUST (Devriendt et al 1999) -provide virtually identical results to other commonly used models (Yi 2003;Bruzual & Charlot 2003;Maraston 2005).…”
Section: Reproduction Of the Early-type Galaxy Populationmentioning
confidence: 56%
“…the "Santa Cruz SAM") that was combined with estimates for dust attenuation by both diffuse dust and stellar birth clouds surrounding young clusters. The energy absorbed by dust was assumed to be re-radiated in the infrared, and combined these with both theoretical SED templates by Devriendt et al (1999), as well as the locally-calibrated observed SED templates by Rieke et al (2009). These authors found that in order to reproduce the (rest) UV and optical luminosity functions at high-z, an evolving dust-to-metals ratio was necessary.…”
Section: Semi-analytic Methodsmentioning
confidence: 99%
“…This is possible only by combining the new FIR observational results with modeling techniques for the SED from the UV to the FIR/submillimeter range. Di †er-ent tools have been proposed for analyzing the energy budget of normal galaxies, starting with the pioneering works of Xu & Buat (1995) and Xu & Helou (1996) and continuing with more recent models, like those of Silva et al (1998), Devriendt, Guiderdoni, & Sadat (1999), and Bianchi, Davies, & Alton (2000a). However, most of these models have made severe simpliÐcations, which ultimately led to contradictory conclusions on the disk opacities and the origin of the FIR emission.…”
Section: Introductionmentioning
confidence: 99%