Multi-frequency study of the Pavo field

We test the prediction of Hamilton and Helfand (1993ApJ...418...55H) that faint radio selected galaxies are a new class contributing to the diffuse X-ray background (XRB) radiation. The test is based on the correlation of X-ray, optical and radio positions for sources detected in ROSAT (S_0.08-2.4keV_>6x10^-15^erg/s/cm^2^, 69 sources) and ATCA (S_1.42GHz_>250uJy, 93 sources) observations of the Einstein Pavo field. A total of six ATCA radio sources inside the inner ring of the ROSAT image are located within 10" of the ROSAT X-ray positions, with one associated by random chance.

Cone search capability for table J/other/Ser/166.13/table2 (Measured ATCA properties of radio-continuum objects in the Pavo deep field)

Cone search capability for table J/other/Ser/166.13/table3 (ROSAT PSPC properties of objects in Pavo field)

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/other/Ser/166.13
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/other/Ser/166.13
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/other/Ser/166.13
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/other/Ser/166.13
Provenance
Creator Filipovic M.D.; Anderson M.; Ekers R.D.; Danziger I.J.; Zimmermann H.-U.,White G.L.; Jones P.A.; Borun B.C.P.; Payne J.L.; Dionne M.; Ganis M.,Ognjanovic M.
Publisher CDS
Publication Year 2011
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; Natural Sciences; Physics