J/ApJ/835/166ivo://CDS.VizieR/J/ApJ/835/166doi:10.26093/cds/vizier.18350166CDSde Jaeger T.Gonzalez-Gaitan S.Hamuy M.Galbany L.Anderson J.P.,Phillips M.M.Stritzinger M.D.Carlberg R.G.Sullivan M.,Gutierrez C.P.Hook I.M.Howell D.A.Hsiao E.Y.Kuncarayakti H.,Ruhlmann-Kleider V.Folatelli G.Pritchet C.Basa S.2018-09-25T12:05:54Z2018-05-30T08:17:26ZCDS support team

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

cds-question@unistra.frsupernovaeredshiftedinterstellar-reddeningsurveysThe coming era of large photometric wide-field surveys will increase the detection rate of supernovae by orders of magnitude. Such numbers will restrict spectroscopic follow-up in the vast majority of cases, and hence new methods based solely on photometric data must be developed. Here, we construct a complete Hubble diagram of Type II supernovae (SNe II) combining data from three different samples: the Carnegie Supernova Project-I, the Sloan Digital Sky Survey II SN, and the Supernova Legacy Survey. Applying the Photometric Color Method (PCM) to 73 SNe II with a redshift range of 0.01-0.5 and with no spectral information, we derive an intrinsic dispersion of 0.35mag. A comparison with the Standard Candle Method (SCM) using 61 SNe II is also performed and an intrinsic dispersion in the Hubble diagram of 0.27mag, i.e., 13% in distance uncertainties, is derived. Due to the lack of good statistics at higher redshifts for both methods, only weak constraints on the cosmological parameters are obtained. However, assuming a flat universe and using the PCM, we derive the universe's matter density: {Omega}_m_=0.32_-0.21_^+0.30^ providing a new independent evidence for dark energy at the level of two sigma.2017ApJ...835..166Dhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/835/166CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toB/sn : Asiago Supernova Catalogue (Barbon et al., 1999-)J/A+A/477/717 : Spectroscopy of Type Ia supernovae (Bronder+, 2008)J/AJ/136/2306 : SDSS-II Supernova survey, 2005 (Holtzman+, 2008)J/A+A/507/85 : ESO/VLT 3rd year type Ia supernova data set (Balland+, 2009)J/A+A/506/999 : Photometric Calibration of SNLS (Regnault+, 2009)J/MNRAS/395/1409 : Type II-P SN progenitor constraints (Smartt+, 2009)J/AJ/139/519 : Carnegie supernova project. SNe Ia (Contreras+, 2010)J/ApJ/708/661 : SDSS-II SN Survey: SNe II-P standardization (D'Andrea+, 2010)J/A+A/523/A7 : Light curves of type Ia supernovae in SNLS (Guy+, 2010)J/ApJS/192/1 : Light-curve parameters from the SNLS (Conley+, 2011)J/AJ/142/156 : The CSP (DR2): photometry of SNe Ia (Stritzinger+, 2011)J/MNRAS/410/1262 : Supernova Legacy Survey. Type Ia supernovae (Walker+, 2011)J/ApJ/773/53 : Type Ia SNe spectroscopy by the CSP (Folatelli+, 2013)J/A+A/568/A22 : Joint analysis of the SDSS-II and SNLS SNe Ia (Betoule+, 2014)J/MNRAS/442/844 : BVRI light curves of type II-P supernovae (Faran+, 2014)J/ApJ/795/44 : PS1 SNe Ia (0.02<z<0.7) griz light curves (Rest+, 2014)J/ApJ/799/215 : 26 type II-Plateau supernovae parameters (Pejcha+, 2015)J/ApJ/799/208 : Type IIP supernovae from Pan-STARRS1 (Sanders+, 2015)J/A+A/589/A110 : SN II in host HII regions (Anderson+, 2016)J/AJ/151/33 : UBVRIz light curves of 51 Type II supernovae (Galbany+, 2016)J/A+A/587/L7 : Metallicity from Type II SN from (i)PTF (Taddia+, 2016)http://csp.obs.carnegiescience.edu/ : Carnegie Supernova Project home pagehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/835/166https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/835/166http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/835/166https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/835/166https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/835/166http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/835/166GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/835/166/table1 (Supernova sample)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/835/166/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/835/166/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/835/166/table1?GETtext/xml+votable180.050000true39.246-5.35547220.0055555555555555566/43 552 4182 4410 8306 8484 8700 11403 11425 12290 12471 16441 16652 17001 17509 17689 17692 17812 17831 17836 17841 17999 18023 18083 18405 18795 19097 19457 19584 19616 19710 21148 22613 23144 23190 24225 24873 25336 25438 25599 25645 25742 26303 27256 27258 27588 27840 28346 29348 30034 30038 30052 31107 35071 35313 35692 36210 36377 36799 36811 36827 36908 37436 38623 38956 39108 40300 40527 40531 40819 40847 40939 43233 43325 45433 45711 46004 46568 47028 47187 47386 47564 48478 48500 49097https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/835/166?format=asciidefaultJ/ApJ/835/166/table1Supernova sampleSimbadNameSimbad column added by the CDSmeta.idcharEpochThe explosion epoch (MJD)dtime.epochfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameSupernova identifiermeta.id;meta.maincharf_Name[c] Flag on Name (1)meta.codecharAvG[0.02/1.9] Reddening (2)magphys.absorptionfloatz[0.0008/0.6] Host-galaxy heliocentric recession velocity from NEDsrc.redshiftfloatzCMB[-0.0001/0.6] Host-galaxy velocity in the CMB frame (3)phys.veloc;pos.frame;pos.cmbfloate_zCMB[0.00001/0.005] zCMB uncertaintystat.errordoublee_Epoch[1/25] Epoch uncertaintydstat.error;time.epochfloats2[-2/3]? s2 value (the slope of the plateau) in the i band (defined in Section 4)stat.fit.paramfloatnullablee_s2[0.01/1.5]? s2 uncertaintystat.errorfloatnullableVHb[2420/8640]? H{beta} velocity (4)km/sspect.dopplerVelocintnullablee_VHb[160/700]? VHb uncertaintykm/sstat.errorintnullablemuPCM[33/42.2]? Distance modulus measured using the Photometric Color Method (PCM); see section 4magphot.mag.distModfloatnullablee_muPCM[0.05/0.7]? muPCM uncertaintymagstat.errorfloatnullablemuSCM[33/40]? Distance modulus measured using the Standard Candle Method (SCM); see section 5magphot.mag.distModfloatnullablee_muSCM[0.06/0.5]? muSCM uncertaintymagstat.errorfloatnullableCampSurvey from which the SN II originates (5)meta.notecharMethMethods (whether a spectrum is available or not)meta.notecharSloanDisplay the online SDSS data for the nearest objectmeta.ref.urlcharNEDNED column added by the CDSmeta.ref.urlchar_RAPositions from SIMBAD or from the author for the SNLS supernovae (right ascension part)degpos.eq.ra;meta.main_DEPositions from SIMBAD or from the author for the SNLS supernovae (declination part)degpos.eq.dec;meta.main