Redshifts in Subaru/XMM Deep Field

DOI

We present multiobject spectroscopy of galaxies in the immediate (Mpc-scale) environments of four low-power (L_1.4GHz_~<10^25^W/Hz) radio galaxies at z~0.5, selected from the Subaru/XMM-Newton Deep Field. We use the spectra to calculate velocity dispersions and central redshifts of the groups the radio galaxies inhabit, and combined with XMM-Newton (0.3-10keV) X-ray observations investigate the L_X_-{sigma}v and T_X_-{sigma}v scaling relationships. All the radio galaxies reside in moderately rich groups - intermediate environments between poor groups and rich clusters, with remarkably similar X-ray properties.

Cone search capability for table J/MNRAS/381/1369/table3 (Spectroscopic targets with total z'-band magnitudes and cross-correlated redshifts)

Identifier
DOI http://doi.org/10.26093/cds/vizier.73811369
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/381/1369
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/381/1369
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/381/1369
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/381/1369
Provenance
Creator Geach J.E.; Simpson C.; Rawlings S.; Read A.M.; Watson M.
Publisher CDS
Publication Year 2008
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