J/MNRAS/506/473ivo://CDS.VizieR/J/MNRAS/506/473doi:10.26093/cds/vizier.75060473CDSPage M.J.Dwelly T.McHardy I.Seymour N.Mason K.O.Sharma M.,Kennea J.A.Sasseen T.P.Rawlings J.I.Breeveld A.A.Ferreras I.,Loaring N.S.Walton D.J.Symeonidis M.2024-11-06T20:34:17Z2024-06-24T13:15:00ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frx-ray-sourcesgalaxiesstar-forming-regionsactive-galactic-nucleiredshiftedultraviolet-photometryWe use ultraviolet (UV) imaging taken with the XMM-Newton Optical Monitor telescope (XMM-OM), covering 280 arcmin^2^ in the UVW1 band ({lambda}_eff_ = 2910 {AA}) to measure rest-frame UV 1500-{AA} luminosity functions of galaxies with redshifts z between 0.6 and 1.2. The XMM-OM data are supplemented by a large body of optical and infrared imaging to provide photometric redshifts. The XMM-OM data have a significantly narrower point spread function (resulting in less source confusion) and simpler K-correction than the GALEX data previously employed in this redshift range. UV-bright active galactic nuclei are excluded to ensure that the luminosity functions relate directly to the star-forming galaxy population. Binned luminosity functions and parametric Schechter-function fits are derived in two redshift intervals: 0.6 < z < 0.8 and 0.8 < z < 1.2. We find that the luminosity function evolves such that the characteristic absolute magnitude M* is brighter for 0.8 < z < 1.2 than for 0.6 < z < 0.8.2021MNRAS.506..473Phttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/506/473CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/MNRAS/342/802 : Chandra survey of 13-h XMM/ROSAT survey (McHardy+, 2003)J/MNRAS/362/1371 : XMM-Newton 13^H^ deep field (Loaring+, 2005)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/506/473https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/506/473http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/506/473https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/506/473https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/506/473http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/506/473GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/506/473/table3 (*UVW1-selected galaxies used to construct the luminosity functions)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/506/473/table3?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/506/473/table3?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/506/473/table3?GETtext/xml+votable180.050000true203.449208337.885750.0055555555555555566/10484https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/506/473?format=asciiX-rayUVdefaultJ/MNRAS/506/473/table3*UVW1-selected galaxies used to construct the luminosity functionsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainUVW1magApparent AB magnitude in UVW1 filter at an effective wavelength of 2910 {AA} (UVW1_mag_)magphot.mag;em.UVfloate_UVW1magMean error of UVW1mag (e_UVW1_mag_)magstat.error;phot.magfloatzMeasured redshift (z)src.redshiftfloatf_z[spec phot] Indicates whether the redshift is derived from spectroscopic or photometric data (spec/phot)meta.codechar