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).

Identifier
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

Provenance
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>

Representation
Format	text/xml+votable
Version	18-Sep-2020
Discipline	Galactic and extragalactic Astronomy