TP-AGB stars contribution in SFR

DOI

We study the debated contribution from thermally pulsing asymptotic-giant-branch (TP-AGB) stars in evolutionary population synthesis models. We investigate the spectral energy distributions (SEDs) of a sample of 51 spectroscopically confirmed, high-z (1.3

Identifier
DOI http://doi.org/10.26093/cds/vizier.74560790
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/456/790
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/456/790
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/456/790
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/456/790
Provenance
Creator Capozzi D.; Maraston C.; Daddi E.; Renzini A.; Strazzullo V.; Gobat R.
Publisher CDS
Publication Year 2016
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy