ROSAT Ultra Deep Survey

DOI

The ROSAT Ultra Deep Survey in the Lockman Hole consists of a sample of 94 X-ray sources reaching a limiting flux of 1.2x10-15erg/s/cm^2^ in the 0.5-2.0keV energy band. About 90% of the X-ray sources have been spectroscopically identified using low-resolution Keck spectra.

Cone search capability for table J/A+A/371/833/table3 (X-ray source catalogue)

Cone search capability for table J/A+A/371/833/table4 (Photometric and spectroscopic properties of optical counterparts)

Identifier
DOI http://doi.org/10.26093/cds/vizier.33710833
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/371/833
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/371/833
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/371/833
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/371/833
Provenance
Creator Lehmann I.; Hasinger G.; Schmidt M.; Giacconi R.; Truemper J.,Zamorani G.; Gunn J.E.; Pozzetti L.; Schneider D.P.; Stanke T.,Szokoly G.; Thompson D.; Wilson G.
Publisher CDS
Publication Year 2003
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; High Energy Astrophysics; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy