J/MNRAS/474/4151ivo://CDS.VizieR/J/MNRAS/474/4151doi:10.26093/cds/vizier.74744151CDSDrinkwater M.J.Byrne Z.J.Blake C.Glazebrook K.Brough S.,Colless M.Couch W.Croton D.J.Croom S.M.Davis T.M.Forster K.,Gilbank D.Hinton S.R.Jelliffe B.Jurek R.J.Li I.-H.Martin D.C.,Pimbblet K.Poole G.B.Pracy M.Sharp R.Smillie J.Spolaor M.,Wisnioski E.Woods D.Wyder T.K.Yee H.K.C.2024-08-18T20:17:29Z2021-04-15T08:40:00ZCDS support team

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

cds-question@unistra.frsurveysgalaxiescatalogsredshiftedultraviolet-photometryvisible-astronomysloan-photometryThe WiggleZ Dark Energy Survey measured the redshifts of over 200000 ultraviolet (UV)-selected (N_UV_<22.8mag) galaxies on the Anglo-Australian Telescope. The survey detected the baryon acoustic oscillation signal in the large-scale distribution of galaxies over the redshift range 0.2<z<1.0, confirming the acceleration of the expansion of the Universe and measuring the rate of structure growth within it. Here, we present the final data release of the survey: a catalogue of 225415 galaxies and individual files of the galaxy spectra. We analyse the emission-line properties of these UV-luminous Lyman-break galaxies by stacking the spectra in bins of luminosity, redshift, and stellar mass. The most luminous (-25mag<M_FUV_< -22mag) galaxies have very broad H{beta} emission from active nuclei, as well as a broad second component to the [OIII] (495.9nm, 500.7nm) doublet lines that is blueshifted by 100km/s, indicating the presence of gas outflows in these galaxies. The composite spectra allow us to detect and measure the temperature-sensitive [OIII] (436.3nm) line and obtain metallicities using the direct method. The metallicities of intermediate stellar mass (8.8<log(M*/M_{sun}_)<10) WiggleZ galaxies are consistent with normal emission-line galaxies at the same masses. In contrast, the metallicities of high stellar mass (10<log(M*/M_{sun}_)<12) WiggleZ galaxies are significantly lower than for normal emission-line galaxies at the same masses. This is not an effect of evolution as the metallicities do not vary with redshift; it is most likely a property specific to the extremely UV-luminous WiggleZ galaxies.2018MNRAS.474.4151Dhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/474/4151CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/MNRAS/401/1429 : WiggleZ dark energy survey (DR1) (Drinkwater+, 2010)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/474/4151https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/474/4151http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/474/4151https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/474/4151https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/474/4151http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/474/4151GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/474/4151/wigglez (The WiggleZ catalogue)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/474/4151/wigglez?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/474/4151/wigglez?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/474/4151/wigglez?GETtext/xml+votable180.050000true7.51655514.489120.0055555555555555563/270 4/257 512-514 1123 1126 1132 1174 1187 1193 1196 1621-1623 1628-1629 1691-1692 1694 1708 1710 1712-1714 2267 2288-2289 2291 5/1024-1025 1027 1036-1037 1040-1042 2060 2080 4279 4299 4302 4338 4344 4487 4498 4510 4516-4517 4519 4532-4534 4536-4537 4676-4677 4679 4685 4688 4690-4691 4693-4694 4700 4742-4743 4745-4747 4760 4762-4763 4768-4769 4771 4780-4781 4783 4788 4792 6477-6479 6481-6483 6500-6501 6503 6520-6521 6523-6524 6744 6746-6747 6757-6759 6761-6763 6772 6774-6775 6780-6782 6805-6807 6810 6813 6821-6823 6825-6829 6831 6838 6844-6846 6860-6862 6864-6866 6881 7848 7850-7851 7854 9067 9161 9168 9170-9171 9176 9178-9179 9181-9183 9200-9202 11261-11263 6/4104-4105 4107 4132-4133 4135 4152-4153 4155-4158 4172-4174 4176-4178 4192-4194 8244-8246 8248-8250 8258-8259 8264-8266 8324-8326 8328-8330 17111 17115 17140-17141 17143 17149 17191 17195 17202 17214 17346 17358 17380-17382 17384-17386 17403 17406 17947 17959 17965-17967 17986-17987 17998 18009 18011-18012 18014 18032-18034 18036 18046 18052-18053 18055 18072-18073 18075 18100-18101 18103 18140 18152-18153 18156 18160 18692-18693 18695 18712-18713 18715 18737 18749 18756 18758-18759 18769-18771 18780-18782 18808 18959 18963 18966-18967 18979 19018-19019 19044 19046-19047 19058 19064 19066-19067 19081 19109 19129 19156 19158 19160-19162 19172-19174 19176-19178 19458 19464 21844-21845 21847 23080 25886-25887 25902-25903 25905-25907 25922-25923 25988-25989 25991 26008-26009 26037 26039 26088-26089 26091 26100-26102 26104-26106 26436-26437 26877-26879 26941-26943 26982 27002 27021-27023 27025-27027 27041-27043 27094 27132-27134 27197-27199 27217-27219 27234-27235 27244 27246-27247 27249 27261 27277-27279 27281-27283 27297-27299 27320-27321 27323 27346-27347 27356 27358-27359 27388 27390 27452 27454 27468-27470 27472-27474 27488-27490 27521 27536-27538 27552 27554 27786 27808 27810 31396 31398-31399 31420 31422 36251 36254 36263 36267 36322 36328 36330-36331 36439 36445 36641 36653 36676 36678-36679 36696 36698 36708-36710 36721-36723 36753 36756-36757 36759 36765 36767 36812-36814 36816-36818 40957-40959 45039 45043 49023 491092.040811542443644e-19 1.4134638842407062e-18https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/474/4151?format=asciiUVOpticaldefaultJ/MNRAS/474/4151/wigglezThe WiggleZ cataloguezRedshiftsrc.redshiftdoubleSimbadSimbad column added by the CDSmeta.ref.urlcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameWiggleZ Name, NhhJHHMMSSsss+DDMMSSss (1)meta.id;meta.maincharRAJ2000Right ascension (J2000)degpos.eq.ra;meta.mainindexedDEJ2000Decliantion 9J2000(degpos.eq.dec;meta.mainindexede_z? rms uncertainty on zstat.error;src.redshiftdoublenullableq_zRedshift quality flag (2)meta.code.qual;src.redshiftintFUV? GALEX FUV magnitudemagphot.mag;em.UV.100-200nmfloatnullableNUV? GALEX NUV magnitudemagphot.mag;em.UVfloatnullableumag? SDSS u magnitudemagphot.mag;em.opt.Ufloatnullablegmag? SDSS g magnitudemagphot.mag;em.opt.Bfloatnullablermag? SDSS r magnitudemagphot.mag;em.opt.Rfloatnullableimag? SDSS i magnitudemagphot.mag;em.opt.Ifloatnullablezmag? SDSS z magnitudemagphot.mag;em.opt.Ifloatnullablee_FUV? rms uncertainty on FUVmagmagstat.errorfloatnullablee_NUV? rms uncertainty on NUVmagmagstat.errorfloatnullablee_umag? rms uncertainty on umagmagstat.error;phot.magfloatnullablee_gmag? rms uncertainty on gmagmagstat.error;phot.magfloatnullablee_rmag? rms uncertainty on rmagmagstat.error;phot.magfloatnullablee_imag? rms uncertainty on imagmagstat.error;phot.magfloatnullablee_zmag? rms uncertainty on zmagmagstat.error;phot.magfloatnullableE(B-V)? Redenning E(B-V)magphot.color.excessfloatnullableClassClass (1)meta.code.classcharComCommentsmeta.notecharDateUT date when the associated spectrum was observed at the Anglo-Australian Telescopetime.epochnullableindexedMFUV? Absolute FUX magnitudemagphys.magAbsfloatnullableMass? Stellar MasssolMassphys.massfloatnullablee_Mass? rms uncertainty on MasssolMassstat.error;phys.massfloatnullableSpecFileSpectrum file idmeta.id;meta.filechar