J/ApJ/855/107ivo://CDS.VizieR/J/ApJ/855/107doi:10.26093/cds/vizier.18550107CDSGalbany L.Anderson J.P.Sanchez S.F.Kuncarayakti H.Pedraz S.,Gonzalez-Gaitan S.Stanishev V.Dominguez I.Moreno-Raya M.E.,Wood-Vasey W.M.Mourao A.M.Ponder K.A.Badenes C.Molla M.,Lopez-Sanchez A.R.Rosales-Ortega F.F.Vilchez J.M.Garcia-Benito R.,Marino R.A.2019-04-08T14:51:00Z2019-03-06T13:09:17ZCDS support team

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

cds-question@unistra.frgalaxiessupernovaeline-intensitieschemical-abundancesvisible-astronomyspectroscopyWe present the PMAS/PPak Integral-field Supernova hosts COmpilation (PISCO), which comprises integral field spectroscopy (IFS) of 232 supernova (SN) host galaxies that hosted 272 SNe, observed over several semesters with the 3.5m telescope at the Calar Alto Observatory (CAHA). PISCO is the largest collection of SN host galaxies observed with wide-field IFS, totaling 466347 individual spectra covering a typical spatial resolution of ~380pc. Focused studies regarding specific SN Ia-related topics will be published elsewhere; this paper aims to present the properties of the SN environments, using stellar population (SP) synthesis, and the gas-phase interstellar medium, providing additional results separating stripped-envelope SNe into their subtypes. With 11270 HII regions detected in all galaxies, we present for the first time a statistical analysis of HII regions, which puts HII regions that have hosted SNe in context with all other star-forming clumps within their galaxies. SNe Ic are associated with environments that are more metal-rich and have higher EW(H{alpha}) and higher star formation rate within their host galaxies than the mean of all HII regions detected within each host. This in contrast to SNe IIb, which occur in environments that are very different compared to other core-collapse SNe types. We find two clear components of young and old SPs at SNe IIn locations. We find that SNe II fast decliners tend to explode at locations where the {Sigma}SFR is more intense. Finally, we outline how a future dedicated IFS survey of galaxies in parallel to an untargeted SN search would overcome the biases in current environmental studies.2018ApJ...855..107Ghttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/855/107CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toII/159 : Asiago Supernova Catalogue 1988 (Barbon+, 1989)J/A+AS/96/269 : Stellar Models from 0.8 to 120 Msolar (Schaller+, 1992)J/A+AS/101/415 : Grids of stellar models III. (Charbonnel+ 1993)J/A+AS/102/339 : Grids of stellar models IV (Schaerer+, 1993)J/A+AS/98/523 : Grids of stellar models. II. (Schaerer+ 1993)J/A+AS/141/371 : Low-mass stars evolutionary tracks (Girardi+, 2000)J/MNRAS/371/703 : MILES library of empirical spectra (Sanchez-Blazquez+, 2006)J/ApJ/689/377 : PAIRITEL SNIa as NIR standard candles (Wood-Vasey+, 2008)J/ApJ/707/1449 : Local hosts of SNe Ia (Neill+, 2009)J/ApJS/190/233 : Spectroscopy and abundances of SINGS gal. (Moustakas+, 2010)J/MNRAS/404/1639 : MILES base models & new line index system (Vazdekis+, 2010)J/AJ/141/126 : HST photometry of NGC 5471 (Garcia-Benito+, 2011)J/ApJ/759/107 : Core-collapse SNe and host galaxies (Kelly+, 2012)J/other/Sci/337.444 : RV curves of Galactic massive O stars (Sana+, 2012)J/A+A/546/A2 : Spectroscopy of HII regions in nearby gal. (Sanchez+, 2012)J/A+A/559/A114 : Updated O3N2 and N2 abundance indicators (Marino+, 2013)J/A+A/555/A10 : Light curves of 5 type IIn supernovae (Taddia+, 2013)J/A+A/568/A22 : Joint analysis of the SDSS-II and SNLS SNIa (Betoule+, 2014)J/MNRAS/438/1391 : Host galaxies of Type Ia SN from PTF (Pan+, 2014)J/MNRAS/448/732 : SNIa environment within host galaxies (Anderson+, 2015)J/A+A/584/A87 : CALIFA sample SFR calibration (Catalan-Torrecilla+, 2015)J/A+A/576/A135 : CALIFA DR2 (Garcia-Benito+, 2015)J/A+A/581/A103 : CALIFA survey across the Hubble sequence (Gonzalez+, 2015)J/ApJ/799/208 : Type IIP supernovae from Pan-STARRS1 (Sanders+, 2015)J/A+A/580/A131 : Circumstellar-interacting supernovae (Taddia+, 2015)J/MNRAS/448/2608 : UV & optical photometric data for SN 2013by (Valenti+, 2015)J/A+A/589/A110 : SN II in host HII regions (Anderson+, 2016)J/ApJ/825/L22 : BVRI LCs of type Ib supernova iPTF13bvn (Folatelli+, 2016)J/AJ/151/33 : UBVRIz light curves of 51 Type II SNe (Galbany+, 2016)J/A+A/594/A36 : CALIFA Survey DR3 list of galaxies (Sanchez+, 2016)J/MNRAS/459/3939 : Type II supernova light curves (Valenti+, 2016)J/ApJ/837/120 : Lick Observatory SN Search (LOSS) revisited (Graur+, 2017)J/A+A/602/A85 : SN 1998bw MUSE datacube (Kruehler+, 2017)J/ApJ/854/L14 : Photometry and spectra of SN 2017dio (Kuncarayakti+, 2018)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/855/107https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/855/107http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/855/107https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/855/107https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/855/107http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/855/107GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/855/107/pisco (Properties of the 232 galaxies and 272 SNe included in PISCO (tables 2 and 3))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/855/107/pisco?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/855/107/pisco?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/855/107/pisco?GETtext/xml+votable180.050000true0.7771667-1.91161110.0055555555555555566/43 50 471 552 620 621 626 635 738 908 909 948 995 1517 1596 1644 1688 2169 2251 2254 2372 2395 2408 2561 3105 3217 3519 3929 4114 4178 4472 4511 4583 4704 4716 4719 4806 4807 4813 4993 5028 5115 5148 5190 5399 5505 5593 5642 5715 5757 5975 5980 6000 6034 6082 6261 6335 6366 6501 6539 6549 6585 6637 6805 6970 6994 7014 7199 7210 7214 7297 7309 7458 7572 7599 7606 7735 7783 7824 7849 7983 8045 8064 8376 8391 8498 8537 8626 8700 8719 8728 8922 8973 9101 9220 9287 9452 9468 9471 9640 9736 9759 9812 9859 9891 9946 9974 10189 10379 10380 10381 10398 10422 10434 10438 10501 10523 10530 10566 10577 10595 10621 10628 10629 10642 10727 10739 10782 10984 11111 11164 11173 11247 11290 11392 11544 11769 11944 12497 13316 13459 13496 13511 13523 13545 13694 13780 13901 14560 14834 14962 14968 15264 15593 16091 16120 17237 17398 17571 17667 17748 17912 18009 18049 18081 18209 18300 18394 18398 18854 18935 19073 19084 19108 19227 19283 19490 19581 19661 19848 19954 19996 20014 20040 20060 20356 21857 21916 21953 22353 22654 22751 23051 23204 23356 23405 23895 24027 24055 24186 25491 25715 25888 25889 26068 26432 26563 26791 27239 27368 27373 27596 28112 28149 28213 28251 28263 28579 28599 28606 30044 31348 31537 31628 32400 32614 36793 36805https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/855/107?format=asciiOpticaldefaultJ/ApJ/855/107/piscoProperties of the 232 galaxies and 272 SNe included in PISCO (tables 2 and 3)SimbadNameSimbad column added by the CDSmeta.idcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintGalGalaxy namemeta.id.parentcharGalIDGalaxy ID in the CALIFA extended samplemeta.id.parentcharMorphMorphology of the galaxy (1)src.morphcharRAG[0/23] Hour of Right Ascension, galaxy (J2000)pos.eq.raDEGDegree of Declination, galaxy (J2000)pos.eq.decz[0.0001/0.09] galaxy redshift (1)src.redshiftdoubleSNSupernova namemeta.id;meta.maincharTypeSupernova typesrc.spTypecharRAJ2000[0/23] Hour of Right Ascension, SN (J2000)pos.eq.ra;meta.mainDEJ2000Degree of Declination, SN (J2000)pos.eq.dec;meta.mainSep[0.5/227] Supernova offset from galaxy corearcsecpos.angDistancefloatSet[1/8] Source (2)meta.codeintCommComments on parameters from previous columnsmeta.notecharANameAbbreviated galaxy name as used for the spectra file names; column added by CDS (3)meta.idcharSNameAbbreviated SN name as used for the spectra file names; column added by CDSmeta.idcharFHa[0.08/2645000]? H{alpha} flux (4)1e-18W.m**-2.nm**-1phot.fluxdoublenullablee_FHa[0.01/157000]? H{alpha} flux error1e-18W.m**-2.nm**-1stat.errordoublenullableFHb[0.06/924900]? H{beta} flux (4)1e-18W.m**-2.nm**-1phot.fluxdoublenullablee_FHb[0.01/59600]? H{beta} flux error1e-18W.m**-2.nm**-1stat.errordoublenullableFOIII[0.04/281200]? Oxygen III {lambda}5007 flux (4)1e-18W.m**-2.nm**-1phot.fluxdoublenullablee_FOIII[0.0/17860]? FOIII error1e-18W.m**-2.nm**-1stat.errordoublenullableFNII[0.09/1367000]? Nitrogen II {lambda}6548 flux (4)1e-18W.m**-2.nm**-1phot.fluxdoublenullablee_FNII[0.01/81750]? FNII error1e-18W.m**-2.nm**-1stat.errordoublenullableFSII[0.09/749000]? Sulphur II {lambda}{lambda}6719,6731 flux (4)1e-18W.m**-2.nm**-1phot.fluxdoublenullablee_FSII[0.01/32005]? FSII error1e-18W.m**-2.nm**-1stat.errordoublenullablelogSFR[-7/1.1]? log of star formation rate intensity, in Msun/yr/kpc^2^log(solMass.yr**-1.kpc**-2)phys.SFRfloatnullablee_logSFR[0.01/0.09]? logSFR uncertaintylog(solMass.yr**-1.kpc**-2)stat.error;phys.SFRfloatnullableEWHa[0/505]? H{alpha} equivalent width, in Angstroms units0.1nmspect.line.eqWidth;em.line.Halphafloatnullablee_EWHa[0/9]? EWHa uncertainty0.1nmstat.errorfloatnullablelogAge[6.5/10.2]? log of average luminosity weighted stellar agelog(yr)phys.luminosity;stat.meanfloatnullablee_logAge[0/0.3]? logAge uncertaintylog(yr)stat.error;time.agefloatnullableOHD16[7.51/9.17]? Oxygen abundance (5)log(Sun)phys.abundfloatnullablee_OHD16[0.0/0.05]? OHD16 uncertainty (5)log(Sun)stat.errorfloatnullablelogM[8.9/12]? log of stellar masslog(solMass)phys.massfloatnullable