FRESCO Halpha emitter catalogue

The H{alpha} nebular emission line is an optimal tracer for recent star formation in galaxies. With the advent of JWST, this line has recently become observable at z>3 for the first time. We present a catalog of 1050 H{alpha} emitters at 3.7

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/694/A178
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/694/A178
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/694/A178
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/694/A178
Provenance
Creator Covelo-Paz A.; Giovinazzo E.; Oesch P.A.; Meyer R.A.; Weibel A.,Brammer G.; Fudamoto Y.; Kerutt J.; Lin J.; Matharu J.; Naidu R.P.,Velichko A.; Bollo V.; Bouwens R.; Chisholm J.; Illingworth G.D.,Kramarenko I.; Magee D.; Maseda M.; Matthee J.; Nelson E.; Reddy N.,Schaerer D.; Stefanon M.; Xiao M.
Publisher CDS
Publication Year 2026
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; Cosmology; Galactic and extragalactic Astronomy; Natural Sciences; Observational Astronomy; Physics