J/ApJ/807/169ivo://CDS.VizieR/J/ApJ/807/169doi:10.26093/cds/vizier.18070169CDSAckermann M.Arcavi I.Baldini L.Ballet J.Barbiellini G.,Bastieri D.Bellazzini R.Bissaldi E.Blandford R.D.Bonino R.,Bottacini E.Brandt T.J.Bregeon J.Bruel P.Buehler R.Buson S.,Caliandro G.A.Cameron R.A.Caragiulo M.Caraveo P.A.Cavazzuti E.,Cecchi C.Charles E.Chekhtman A.Chiang J.Chiaro G.Ciprini S.,Claus R.Cohen-Tanugi J.Cutini S.D'Ammando F.de Angelis A.,de Palma F.Desiante R.Di Venere L.Drell P.S.Favuzzi C.Fegan S.J.,Franckowiak A.Funk S.Fusco P.Gal-Yam A.Gargano F.Gasparrini D.,Giglietto N.Giordano F.Giroletti M.Glanzman T.Godfrey G.,Grenier I.A.Grove J.E.Guiriec S.Harding A.K.Hayashi K.,Hewitt J.W.Hill A.B.Horan D.Jogler T.Johannesson G.Kocevski D.,Kuss M.Larsson S.Lashner J.Latronico L.Li J.Li L.Longo F.,Loparco F.Lovellette M.N.Lubrano P.Malyshev D.Mayer M.,Mazziotta M.N.Mcenery J.E.Michelson P.F.Mizuno T.Monzani M.E.,Morselli A.Murase K.Nugent P.Nuss E.Ofek E.Ohsugi T.Orienti M.,Orlando E.Ormes J.F.Paneque D.Pesce-rollins M.Piron F.Pivato G.,Raino S.Rando R.Razzano M.Reimer A.Reimer O.Schulz A.Sgro C.,Siskind E.J.Spada F.Spandre G.Spinelli P.Suson D.J.Takahashi H.,Thayer J.B.Tibaldo L.Torres D.F.Troja E.Vianello G.Werner M.,Wood K.S.Wood M.2017-10-11T05:13:54Z2015-12-11T12:09:24ZCDS support team

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

cds-question@unistra.frsupernovaegamma-ray-astronomyredshiftedapparent-magnitudeSupernovae (SNe) exploding in a dense circumstellar medium (CSM) are hypothesized to accelerate cosmic rays in collisionless shocks and emit GeV {gamma}-rays and TeV neutrinos on a timescale of several months. We perform the first systematic search for {gamma}-ray emission in Fermi Large Area Telescope data in the energy range from 100MeV to 300GeV from the ensemble of 147 SNe Type IIn exploding in a dense CSM. We search for a {gamma}-ray excess at each SNe location in a one-year time window. In order to enhance a possible weak signal, we simultaneously study the closest and optically brightest sources of our sample in a joint-likelihood analysis in three different time windows (1 year, 6 months, and 3 months). For the most promising source of the sample, SN 2010jl (PTF 10aaxf), we repeat the analysis with an extended time window lasting 4.5 years. We do not find a significant excess in {gamma}-rays for any individual source nor for the combined sources and provide model-independent flux upper limits for both cases. In addition, we derive limits on the {gamma}-ray luminosity and the ratio of {gamma}-ray-to-optical luminosity ratio as a function of the index of the proton injection spectrum assuming a generic {gamma}-ray production model. Furthermore, we present detailed flux predictions based on multi-wavelength observations and the corresponding flux upper limit at a 95% confidence level (CL) for the source SN 2010jl (PTF 10aaxf).2015ApJ...807..169Ahttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/807/169CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toB/sn : Asiago Supernova Catalogue (Barbon et al., 1999-)II/313 : Palomar Transient Factory (PTF) photometric catalog 1.0 (Ofek+, 2012)J/A+A/555/A10 : Light curves of 5 type IIn supernovae (Taddia+, 2013)J/ApJ/768/47 : Swift/XRT 0.2-10keV observations of SN2009ip (Ofek+, 2013)J/ApJ/763/42 : X-ray emission from 28 SNe (IIn, Ibn or SLSN-I) (Ofek+, 2013)J/AJ/144/131 : Photometry and spectroscopy of SN 2010jl (Zhang+, 2012)J/ApJS/183/46 : Fermi/LAT bright gamma-ray source list (0FGL) (Abdo+, 2009)http://fermi.gsfc.nasa.gov/ssc/data/ : Fermi data accesshttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/807/169https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/807/169http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/807/169https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/807/169https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/807/169http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/807/169GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/807/169/sncat (All supernovae included in this analysis)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/807/169/sncat?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/807/169/sncat?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/807/169/sncat?GETtext/xml+votable180.050000true348.55-2.780.0055555555555555566/51 172 459 543 568 835 2147 2504 3444 4181 4524 4545 4671 4740 4787 5136 5409 5758 5841 5877 5905 5987 5993 6048 6427 6625 7325 7701 7783 7977 8201 8829 9200 9292 9339 9375 9463 9702 9731 9859 10118 10194 10330 10530 10780 10800 10890 11041 11291 11314 11368 11408 11418 11428 11482 11519 11616 11628 11824 12019 12523 12599 12605 13518 15024 17235 17605 18214 18411 18431 18532 18610 18739 18919 18951 19004 19036 19055 19103 19127 19192 19591 19634 19667 19670 20089 20172 20177 20181 20245 20255 20298 20385 20703 20875 21130 21198 21868 22914 22934 22953 23027 23327 23882 24951 25046 25771 25830 26001 26117 26265 26805 26865 27024 27244 27332 27521 27712 27728 27939 28036 28224 28649 31359 31532 31991 32451 32462 32505 32507 32573 32620 32680 36656 36710 36712 40378 40648 43739 43942 43948 44648 46321 47765 485932.762881831355591e-19 3.3785437584409506e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/807/169?format=asciiGamma-rayOpticaldefaultJ/ApJ/807/169/sncatAll supernovae included in this analysisrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameSN namemeta.id;meta.maincharONameOther SN namemeta.idcharf_Name[a] Flag on Name (1)meta.codecharRAJ2000Right ascension in decimal degrees (J2000) (2)degpos.eq.ra;meta.mainDEJ2000Declination in decimal degrees (J2000) (2)degpos.eq.dec;meta.mainDatePeak datetime.epoch;stat.maxnullablef_Date[d] d: Discovery date (3)meta.codecharz[0.004/0.4]? Redsfhitsrc.redshiftfloatnullableRmag[13.2/21.1]? Apparent R-band peak magnitudemagphot.mag;em.opt.Rfloatnullablef_Rmag[D] D: Discovery magnitude (3)meta.codecharTS[0/14.4]? Test statisticstat.fit.goodnessfloatnullablep[0.006/0.6]? p-valuestat.fit.paramfloatnullableN[1]? 1: Nearby and/or bright SN used for the joint likelihood analysis (table 1); column added by CDSmeta.codeintnullableSimbadSimbad column added by the CDSmeta.ref.urlchar