J/A+A/637/A73ivo://CDS.VizieR/J/A+A/637/A73doi:10.26093/cds/vizier.36370073CDSNyholm A.Sollerman J.Tartaglia L.Taddia F.Fremling C.,Blagorodnova N.Filippenko A.V.Gal-Yam A.Howell D.A.,Karamehmetoglu E.Kulkarni S.R.Laher R.Leloudas G.Masci F.,Kasliwal M.M.Mora K.Moriya T.J.Ofek E.O.Papadogiannakis S.,Quimby R.Rebbapragada U.Schulze S.2022-01-14T08:08:51Z2020-05-19T07:32:09ZCDS support team

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

cds-question@unistra.frsupernovaephotometryThe evolution of a Type IIn supernova (SN IIn) is governed by the interaction between the SN ejecta and a hydrogen-rich circumstellar medium (CSM). SNe IIn thus allow us to probe the late-time mass-loss history of their progenitor stars. We present optical photometry of a sample of 42 Type IIn supernovae, obtained by the Palomar Transient Factory (PTF) collaboration and its successor, the intermediate PTF (iPTF), from 2009 to 2017 using the 1.2m Samuel Oschin telescope and the 1.52m telescope at Palomar Observatory, California, USA.2020A&A...637A..73Nhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/637/A73CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/A+A/593/A68 : PTF12os & iPTF13bvn spectra and light curves (Fremling+, 2016)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/637/A73https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/637/A73http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/637/A73https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/637/A73https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/637/A73http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/637/A73GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/637/A73/sample (The 42 SNe IIn in the sample (from table4 of the paper))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/637/A73/sample?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/637/A73/sample?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/637/A73/sample?GETtext/xml+votable180.050000true206.733083361.55433330.0055555555555555566/459 550 1211 2147 3444 5987 5993 6625 8391 8682 8917 9292 9339 9416 9702 9813 10194 10453 10530 10569 11041 11120 11616 11628 11824 12019 12605 19036 19055 20703 22660 25771 26265 27244 27629 27728 28150 31442 31991 32507 32680 36712https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/637/A73?format=asciidefaultJ/A+A/637/A73/sampleThe 42 SNe IIn in the sample (from table4 of the paper)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintLCLight curvesmeta.ref.urlcharNameSN namemeta.id;meta.maincharRAJ2000Right ascension (J2000.0)pos.eq.ra;meta.mainDEJ2000Declination (J2000.0)pos.eq.dec;meta.mainzRedshift (1)src.redshiftdoubleMODDistance modulusmagphot.mag.distModfloatDiscDiscovery date, refers to the time of PTF/iPTF discovery (MJD) (2)dtime.epochdoubleE(B-V)MWMilky Way colour excess for each SN is obtained as described in Sect. 3.1magphot.color.excessfloatgMAGHostHost galaxy g-band absolute magnitude (3)magphys.magAbsfloatANameAlternative designationsmeta.idcharSimbadSimbad column added by the CDSmeta.ref.urlcharJ/A+A/637/A73/table2Type IIn SN photometryrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNamePTF/iPTF name of the supernovameta.id;meta.maincharJDEpoch (JD)dtime.epochdoubleindexedmag? Magnitude (AB) in filtermagphot.magfloatnullablee_mag? Magnitude statistical error (1 sigma)magstat.error;phot.magfloatnullablelmag? Upper limit magnitude (AB) in filtermagphot.magfloatnullableTelTelescope (P48 or P60)meta.id;instr.telcharCamCamera (CFH12K for P48, GRBCam or SEDM for P60)meta.id;instrcharFilter[RgrizB] Filter used (1)instr.setup;instr.filtercharRefReference frame (P48ref, P60ref, SDSS or PS1) (2)pos.framecharPipePipeline used (PTFIDE for P48, FPipe for P60)instr.setupchar