Dusty star-forming galaxies physical properties (Donevski+, 2020)

The catalogue contains main physical properties for 300 distant, dusty star-forming galaxies detected with ALMA that are analysed in this work. We make use of panchromatic data coverage of our sources in the COSMOS field and apply full SED (UV+IR) modelling with the newest release of code CIGALE. We note that for each parameter CIGALE makes a probability distribution function (PDF) analysis, and the output value is the likelihood-weighted mean of the PDF (and consequently, the associated error is likelihood-weighted standard deviation).

Source http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/644/A144
Related Identifier https://ui.adsabs.harvard.edu/abs/2020A&A...644A.144D
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_datacite&identifier=ivo://CDS.VizieR/J/A+A/644/A144
Creator Donevski D., Lapi A., Malek K., Liu D., Gomez-Guijarro C., Dave R., Kraljic K., Pantoni L., Man A., Fujimoto S., Feltre A., Pearson W., Li Q., Narayanan, D.
Publisher CDS
Contributor International Virtual Observatory Alliance (IVOA)
Publication Year 2021
Rights public
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Format text/xml+votable
Version 18-Sep-2020
Discipline Galactic and extragalactic Astronomy