2023ApJ...949L..12A


Query : 2023ApJ...949L..12A

2023ApJ...949L..12A - Astrophys. J., 949, L12 (2023/May-3)

Constraining High-energy Neutrino Emission from Supernovae with IceCube.

ABBASI R., ACKERMANN M., ADAMS J., AGARWALLA S.K., AGUILAR J.A., AHLERS M., ALAMEDDINE J.M., AMIN N.M., ANDEEN K., ANTON G., ARGUELLES C., ASHIDA Y., ATHANASIADOU S., AXANI S.N., BAI X., BALAGOPAL V.A., BARICEVIC M., BARWICK S.W., BASU V., BAY R., BEATTY J.J., BECKER K.-H., BECKER TJUS J., BEISE J., BELLENGHI C., BENZVI S., BERLEY D., BERNARDINI E., BESSON D.Z., BINDER G., BINDIG D., BLAUFUSS E., BLOT S., BONTEMPO F., BOOK J.Y., BOSCOLO MENEGUOLO C., BOSER S., BOTNER O., BOTTCHER J., BOURBEAU E., BRAUN J., BRINSON B., BROSTEAN-KAISER J., BURLEY R.T., BUSSE R.S., BUTTERFIELD D., CAMPANA M.A., CARLONI K., CARNIE-BRONCA E.G., CHATTOPADHYAY S., CHEN C., CHEN Z., CHIRKIN D., CHOI S., CLARK B.A., CLASSEN L., COLEMAN A., COLLIN G.H., CONNOLLY A., CONRAD J.M., COPPIN P., CORREA P., COUNTRYMAN S., COWEN D.F., DAVE P., DE CLERCQ C., DELAUNAY J.J., DELGADO LOPEZ D., DEMBINSKI H., DEOSKAR K., DESAI A., DESIATI P., DE VRIES K.D., DE WASSEIGE G., DEYOUNG T., DIAZ A., DIAZ-VELEZ J.C., DITTMER M., DOMI A., DUJMOVIC H., DUVERNOIS M.A., EHRHARDT T., ELLER P., ENGEL R., ERPENBECK H., EVANS J., EVENSON P.A., FAN K.L., FANG K., FAZELY A.R., FEDYNITCH A., FEIGL N., FIEDLSCHUSTER S., FINLEY C., FISCHER L., FOX D., FRANCKOWIAK A., FRIEDMAN E., FRITZ A., FURST P., GAISSER T.K., GALLAGHER J., GANSTER E., GARCIA A., GARRAPPA S., GERHARDT L., GHADIMI A., GLASER C., GLAUCH T., GLUSENKAMP T., GOEHLKE N., GONZALEZ J.G., GOSWAMI S., GRANT D., GRAY S.J., GRIFFIN S., GRISWOLD S., GUNTHER C., GUTJAHR P., HAACK C., HALLGREN A., HALLIDAY R., HALVE L., HALZEN F., HAMDAOUI H., HA MINH M., HANSON K., HARDIN J., HARNISCH A.A., HATCH P., HAUNGS A., HELBING K., HELLRUNG J., HENNINGSEN F., HEUERMANN L., HICKFORD S., HIDVEGI A., HILL C., HILL G.C., HOFFMAN K.D., HOSHINA K., HOU W., HUBER T., HULTQVIST K., HUNNEFELD M., HUSSAIN R., HYMON K., IN S., IOVINE N., ISHIHARA A., JACQUART M., JANSSON M., JAPARIDZE G.S., JAYAKUMAR K., JEONG M., JIN M., JONES B.J.P., KANG D., KANG W., KANG X., KAPPES A., KAPPESSER D., KARDUM L., KARG T., KARL M., KARLE A., KATZ U., KAUER M., KELLEY J.L., KHATEE ZATHUL A., KHEIRANDISH A., KIN K., KIRYLUK J., KLEIN S.R., KOCHOCKI A., KOIRALA R., KOLANOSKI H., KONTRIMAS T., KOPKE L., KOPPER C., KOSKINEN D.J., KOUNDAL P., KOVACEVICH M., KOWALSKI M., KOZYNETS T., KRUISWIJK K., KRUPCZAK E., KUMAR A., KUN E., KURAHASHI N., LAD N., LAGUNAS GUALDA C., LAMOUREUX M., LARSON M.J., LAUBER F., LAZAR J.P., LEE J.W., LEONARD DEHOLTON K., LESZCZYNSKA A., LINCETTO M., LIU Q.R., LIUBARSKA M., LOHFINK E., LOVE C., LOZANO MARISCAL C.J., LU L., LUCARELLI F., LUDWIG A., LUSZCZAK W., LYU Y., MA W.Y., MADSEN J., MAHN K.B.M., MAKINO Y., MANCINA S., MARIE SAINTE W., MARIS I.C., MARKA S., MARKA Z., MARSEE M., MARTINEZ-SOLER I., MARUYAMA R., MAYHEW F., McELROY T., McNALLY F., MEAD J.V., MEAGHER K., MECHBAL S., MEDINA A., MEIER M., MEIGHEN-BERGER S., MERCKX Y., MERTEN L., MICALLEF J., MOCKLER D., MONTARULI T., MOORE R.W., MORII Y., MORSE R., MOULAI M., MUKHERJEE T., NAAB R., NAGAI R., NAKOS M., NAUMANN U., NECKER J., NEUMANN M., NIEDERHAUSEN H., NISA M.U., NOELL A., NOWICKI S.C., OBERTACKE POLLMANN A., O'DELL V., OEHLER M., OEYEN B., OLIVAS A., ORSOE R., OSBORN J., O'SULLIVAN E., PANDYA H., PARK N., PARKER G.K., PAUDEL E.N., PAUL L., PEREZ DE LOS HEROS C., PETERSON J., PHILIPPEN S., PIEPER S., PIZZUTO A., PLUM M., POPOVYCH Y., PRADO RODRIGUEZ M., PRIES B., PROCTER-MURPHY R., PRZYBYLSKI G.T., RAAB C., RACK-HELLEIS J., RAWLINS K., RECHAV Z., REHMAN A., REICHHERZER P., RENZI G., RESCONI E., REUSCH S., RHODE W., RICHMAN M., RIEDEL B., ROBERTS E.J., ROBERTSON S., RODAN S., ROELLINGHOFF G., RONGEN M., ROTT C., RUHE T., RUOHAN L., RYCKBOSCH D., SAFA I., SAFFER J., SALAZAR-GALLEGOS D., SAMPATHKUMAR P., SANCHEZ HERRERA S.E., SANDROCK A., SANTANDER M., SARKAR S., SARKAR S., SAVELBERG J., SAVINA P., SCHAUFEL M., SCHIELER H., SCHINDLER S., SCHLUTER B., SCHMIDT T., SCHNEIDER J., SCHRODER F.G., SCHUMACHER L., SCHWEFER G., SCLAFANI S., SECKEL D., SEUNARINE S., SHARMA A., SHEFALI S., SHIMIZU N., SILVA M., SKRZYPEK B., SMITHERS B., SNIHUR R., SOEDINGREKSO J., SOGAARD A., SOLDIN D., SOMMANI G., SPANNFELLNER C., SPICZAK G.M., SPIERING C., STAMATIKOS M., STANEV T., STASIK A., STEIN R., STEZELBERGER T., STURWALD T., STUTTARD T., SULLIVAN G.W., TABOADA I., TER-ANTONYAN S., THOMPSON W.G., THWAITES J., TILAV S., TOLLEFSON K., TONNIS C., TOSCANO S., TOSI D., TRETTIN A., TUNG C.F., TURCOTTE R., TWAGIRAYEZU J.P., TY B., UNLAND ELORRIETA M.A., UPADHYAY A.K., UPSHAW K., VALTONEN-MATTILA N., VANDENBROUCKE J., VAN EIJNDHOVEN N., VANNEROM D., VAN SANTEN J., VARA J., VEITCH-MICHAELIS J., VENUGOPAL M., VERPOEST S., VESKE D., WALCK C., WATSON T.B., WEAVER C., WEIGEL P., WEINDL A., WELDERT J., WENDT C., WERTHEBACH J., WEYRAUCH M., WHITEHORN N., WIEBUSCH C.H., WILLEY N., WILLIAMS D.R., WOLF M., WREDE G., WULFF J., XU X.W., YANEZ J.P., YILDIZCI E., YOSHIDA S., YU F., YU S., YUAN T., ZHANG Z., ZHELNIN P. (The IceCube Collaboration)

Abstract (from CDS):

Core-collapse supernovae are a promising potential high-energy neutrino source class. We test for correlation between seven years of IceCube neutrino data and a catalog containing more than 1000 core-collapse supernovae of types IIn and IIP and a sample of stripped-envelope supernovae. We search both for neutrino emission from individual supernovae as well as for combined emission from the whole supernova sample, through a stacking analysis. No significant spatial or temporal correlation of neutrinos with the cataloged supernovae was found. All scenarios were tested against the background expectation and together yield an overall p-value of 93%; therefore, they show consistency with the background only. The derived upper limits on the total energy emitted in neutrinos are 1.7 × 1048 erg for stripped-envelope supernovae, 2.8 × 1048 erg for type IIP, and 1.3 × 1049 erg for type IIn SNe, the latter disfavoring models with optimistic assumptions for neutrino production in interacting supernovae. We conclude that stripped-envelope supernovae and supernovae of type IIn do not contribute more than 14.6% and 33.9%, respectively, to the diffuse neutrino flux in the energy range of about [ 103-105] GeV, assuming that the neutrino energy spectrum follows a power-law with an index of -2.5. Under the same assumption, we can only constrain the contribution of type IIP SNe to no more than 59.9%. Thus, core-collapse supernovae of types IIn and stripped-envelope supernovae can both be ruled out as the dominant source of the diffuse neutrino flux under the given assumptions.

Abstract Copyright: © 2023. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Neutrino astronomy - Core-collapse supernovae - Circumstellar matter - High-energy astrophysics

Simbad objects: 56

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Number of rows : 56
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 SN 2009mk SN* 00 06 21.37 -41 28 59.8           SNIIb 16 1
2 SN 2009gj SN* 00 30 28.56 -33 12 56.0           SNIIb 16 1
3 SN 2011dq SN* 00 59 47.75 -07 34 20.5           SNIIP 15 1
4 SN 2009mf SN* 01 00 55.88 +47 41 07.7           SNIIP 6 1
5 SN 2013ej SN* 01 36 48.16 +15 45 31.0           SNIIP 248 0
6 SN 2009js SN* 02 25 48.28 +18 29 25.8           SNIIP 36 1
7 M 77 Sy2 02 42 40.7091669408 -00 00 47.859690204 9.70 9.61 8.87 10.1 9.9 ~ 4897 2
8 SN 2007gr SN* 02 43 27.98 +37 20 44.7       12.77   SNIc 265 1
9 SN 2012ec SN* 02 45 59.89 -07 34 25.0         22.32 SNIIP 92 3
10 SN 2008dv SN* 03 37 51.43 +72 34 21.8           SNIc 16 1
11 SN 1999em SN* 04 41 27.04 -02 51 45.2   13.79 13.7     SNIIP 727 1
12 AT 2014gf SN* 04 42 12.20 +23 06 16.7           SNIIn 8 0
13 SN 2009kr SN* 05 12 03.30 -15 41 52.2           SNII 93 1
14 TCP J06043671-1237406 SN* 06 04 36.71 -12 37 40.6           SNIIn 3 0
15 2MASS J07371703+6535579 HXB 07 37 17.0432126424 +65 35 57.826001220           SNIIP 317 1
16 SN 2011an SN* 07 59 24.42 +16 25 08.2           SNIIn 11 1
17 SN 2013gc SN* 08 07 11.88 -28 03 26.3           SNIIn 17 1
18 SN 2010jl SN* 09 42 53.33 +09 29 41.8           SNIIn 350 1
19 SN 2009mu SN* 09 51 57.75 -33 04 42.4           SNIIb 4 1
20 PSN J10081059+5150570 s*b 10 08 10.58 +51 50 57.1           LBV 110 0
21 SN 2009dq SN* 10 08 49.94 -67 01 57.3           SNIIb 11 1
22 SN 2012cw SN* 10 13 47.95 +03 26 02.6           SNIc 12 2
23 SN 1999bw SN* 10 19 46.81 +45 31 35.0     17.8     SNIIn? 61 2
24 SN 2012A SN* 10 25 07.39 +17 09 14.6           SNIIP 135 0
25 SN 2013ge SN* 10 34 48.46 +21 39 41.9           SNIc 70 1
26 SN 2012fh SN* 10 43 34.05 +24 53 29.0           SNIc: 39 1
27 SN 2012aw SN* 10 43 53.735 +11 40 17.63       15   SNIIP 252 1
28 SN 2009md SN* 10 48 26.28 +12 32 02.8           SNIIP 75 2
29 SN 2014G SN* 10 54 34.13 +54 17 56.9           SNIIL 95 1
30 SN 2013am SN* 11 18 56.95 +13 03 49.4           SNII 52 1
31 SN 2010br SN* 12 03 10.95 +44 31 43.1           SNIb/c 25 1
32 SN 2014ge SN* 12 04 51.50 +26 59 46.6           SNIb 23 0
33 SN 2002bu SN* 12 17 37.18 +45 38 47.4     15.5     SNIIn? 58 2
34 SN 2014bc SN* 12 18 57.71 +47 18 11.3           SNIIP 25 1
35 SN 2006ov SN* 12 21 55.30 +04 29 16.7     14.9     SNIIP 88 1
36 SN 2012ab SN* 12 22 47.5 +05 36 24           SNII: 28 1
37 SN 2013df SN* 12 26 29.33 +31 13 38.3           SNIIb 142 1
38 SN 2008ax SN* 12 30 40.80 +41 38 16.1   23.6 23.5 14.1 22.6 SNIIb 295 1
39 SN 2011jm SN* 12 54 51.10 +02 39 14.9           SNIc 18 1
40 SN 2011ja SN* 13 05 11.12 -49 31 27.0           SNIIP 48 0
41 SN 2005cs SN* 13 29 53.37 +47 10 28.2   14.5       SNIIP 450 1
42 SN 2011dh SN* 13 30 05.10555 +47 10 10.9227           SNIIb 445 1
43 PSN J13375721-1754272 SN* 13 37 57.21 -17 54 27.2           SNIIp 4 0
44 SN 2015da SN* 13 52 24.16470 +39 41 27.9355           SNIIn 41 0
45 PSN J14041297-0938168 SN? 14 04 12.97 -09 38 16.8           ~ 3 0
46 SN 2013ab SN* 14 32 44.49 +09 53 12.3           SNIIP 71 1
47 SN 2012P SN* 14 59 59.04 +01 53 24.4           SNIb/c 51 1
48 iPTF 13bvn SN* 15 00 00.152 +01 52 53.17           SNIb 211 0
49 SN 2013by SN* 16 59 02.43 -60 11 41.8           SNII 83 1
50 SN 2019fdr SN* 17 09 06.859 +26 51 20.50           SLSN-II 48 0
51 SN 2010gi SN* 17 21 46.03 +75 50 44.4           SNIIb: 8 1
52 SN 2008S ev 20 34 45.33 +60 05 58.4   19.89 18.79 17.93   SNIIn? 253 1
53 SN 2004et SN* 20 35 25.33 +60 07 17.7   12.88       SNIIP 547 1
54 SN 2013bu SN* 22 37 02.17 +34 24 05.2           SNIIP 22 1
55 SN 2014C SN* 22 37 05.60 +34 24 31.9           SNIb 167 1
56 SN 2008bk SN* 23 57 50.42 -32 33 21.5           SNIIP 167 2

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