2017ApJ...849...67A

Query : 2017ApJ...849...67A

2017ApJ...849...67A - Astrophys. J., 849, 67-67 (2017/November-8)

Constraints on Galactic neutrino emission with seven years of IceCube data.

AARTSEN M.G., ACKERMANN M., ADAMS J., AGUILAR J.A., AHLERS M., AHRENS M., AL SAMARAI I., ALTMANN D., ANDEEN K., ANDERSON T., ANSSEAU I., ANTON G., ARGUELLES C., AUFFENBERG J., AXANI S., BAGHERPOUR H., BAI X., BARRON J.P., BARWICK S.W., BAUM V., BAY R., BEATTY J.J., BECKER TJUS J., BECKER K.-H., BENZVI S., BERLEY D., BERNARDINI E., BESSON D.Z., BINDER G., BINDIG D., BLAUFUSS E., BLOT S., BOHM C., BORNER M., BOS F., BOSE D., BOSER S., BOTNER O., BOURBEAU J., BRADASCIO F., BRAUN J., BRAYEUR L., BRENZKE M., BRETZ H.-P., BRON S., BURGMAN A., CARVER T., CASEY J., CASIER M., CHEUNG E., CHIRKIN D., CHRISTOV A., CLARK K., CLASSEN L., COENDERS S., COLLIN G.H., CONRAD J.M., COWEN D.F., CROSS R., DAY M., DE ANDRE J.P.A.M., DE CLERCQ C., DELAUNAY J.J., DEMBINSKI H., DE RIDDER S., DESIATI P., DE VRIES K.D., DE WASSEIGE G., DE WITH M., DEYOUNG T., DIAZ-VELEZ J.C., DI LORENZO V., DUJMOVIC H., DUMM J.P., DUNKMAN M., EBERHARDT B., EHRHARDT T., EICHMANN B., ELLER P., EVENSON P.A., FAHEY S., FAZELY A.R., FELDE J., FILIMONOV K., FINLEY C., FLIS S., FRANCKOWIAK A., FRIEDMAN E., FUCHS T., GAISSER T.K., GALLAGHER J., GERHARDT L., GHORBANI K., GIANG W., GLAUCH T., GLUSENKAMP T., GOLDSCHMIDT A., GONZALEZ J.G., GRANT D., GRIFFITH Z., HAACK C., HALLGREN A., HALZEN F., HANSON K., HEBECKER D., HEEREMAN D., HELBING K., HELLAUER R., HICKFORD S., HIGNIGHT J., HILL G.C., HOFFMAN K.D., HOFFMANN R., HOKANSON-FASIG B., HOSHINA K., HUANG F., HUBER M., HULTQVIST K., IN S., ISHIHARA A., JACOBI E., JAPARIDZE G.S., JEONG M., JERO K., JONES B.J.P., KALACYNSKI P., KANG W., KAPPES A., KARG T., KARLE A., KATZ U., KAUER M., KEIVANI A., KELLEY J.L., KHEIRANDISH A., KIM J., KIM M., KINTSCHER T., KIRYLUK J., KITTLER T., KLEIN S.R., KOHNEN G., KOIRALA R., KOLANOSKI H., KOPKE L., KOPPER C., KOPPER S., KOSCHINSKY J.P., KOSKINEN D.J., KOWALSKI M., KRINGS K., KROLL M., KRUCKL G., KUNNEN J., KUNWAR S., KURAHASHI N., KUWABARA T., KYRIACOU A., LABARE M., LANFRANCHI J.L., LARSON M.J., LAUBER F., LENNARZ D., LESIAK-BZDAK M., LEUERMANN M., LIU Q.R., LU L., LUNEMANN J., LUSZCZAK W., MADSEN J., MAGGI G., MAHN K.B.M., MANCINA S., MARUYAMA R., MASE K., MAUNU R., McNALLY F., MEAGHER K., MEDICI M., MEIER M., MENNE T., MERINO G., MEURES T., MIARECKI S., MICALLEF J., MOMENTE G., MONTARULI T., MOORE R.W., MOULAI M., NAHNHAUER R., NAKARMI P., NAUMANN U., NEER G., NIEDERHAUSEN H., NOWICKI S.C., NYGREN D.R., OBERTACKE POLLMANN A., OLIVAS A., O'MURCHADHA A., PALCZEWSKI T., PANDYA H., PANKOVA D.V., PEIFFER P., PEPPER J.A., PEREZ DE LOS HEROS C., PIELOTH D., PINAT E., PLUM M., PRICE P.B., PRZYBYLSKI G.T., RAAB C., RADEL L., RAMEEZ M., RAWLINS K., REIMANN R., RELETHFORD B., RELICH M., RESCONI E., RHODE W., RICHMAN M., ROBERTSON S., RONGEN M., ROTT C., RUHE T., RYCKBOSCH D., RYSEWYK D., SALZER T., SANCHEZ HERRERA S.E., SANDROCK A., SANDROOS J., SARKAR S., SARKAR S., SATALECKA K., SCHLUNDER P., SCHMIDT T., SCHNEIDER A., SCHOENEN S., SCHONEBERG S., SCHUMACHER L., SECKEL D., SEUNARINE S., SOLDIN D., SONG M., SPICZAK G.M., SPIERING C., STACHURSKA J., STANEV T., STASIK A., STETTNER J., STEUER A., STEZELBERGER T., STOKSTAD R.G., STOSSL A., STROTJOHANN N.L., SULLIVAN G.W., SUTHERLAND M., TABOADA I., TATAR J., TENHOLT F., TER-ANTONYAN S., TERLIUK A., TESIC G., TILAV S., TOALE P.A., TOBIN M.N., TOSCANO S., TOSI D., TSELENGIDOU M., TUNG C.F., TURCATI A., TURLEY C.F., TY B., UNGER E., USNER M., VANDENBROUCKE J., VAN DRIESSCHE W., VAN EIJNDHOVEN N., VANHEULE S., VAN SANTEN J., VEHRING M., VOGEL E., VRAEGHE M., WALCK C., WALLACE A., WALLRAFF M., WANDLER F.D., WANDKOWSKY N., WAZA A., WEAVER C., WEISS M.J., WENDT C., WESTERHOFF S., WHELAN B.J., WICKMANN S., WIEBE K., WIEBUSCH C.H., WILLE L., WILLIAMS D.R., WILLS L., WOLF M., WOOD J., WOOD T.R., WOOLSEY E., WOSCHNAGG K., XU D.L., XU X.W., XU Y., YANEZ J.P., YODH G., YOSHIDA S., YUAN T., ZOLL M. (The IceCube Collaboration)

Abstract (from CDS):

The origins of high-energy astrophysical neutrinos remain a mystery despite extensive searches for their sources. We present constraints from seven years of IceCube Neutrino Observatory muon data on the neutrino flux coming from the Galactic plane. This flux is expected from cosmic-ray interactions with the interstellar medium or near localized sources. Two methods were developed to test for a spatially extended flux from the entire plane, both of which are maximum likelihood fits but with different signal and background modeling techniques. We consider three templates for Galactic neutrino emission based primarily on gamma-ray observations and models that cover a wide range of possibilities. Based on these templates and in the benchmark case of an unbroken E–2.5 power-law energy spectrum, we set 90% confidence level upper limits, constraining the possible Galactic contribution to the diffuse neutrino flux to be relatively small, less than 14% of the flux reported in Aartsen et al. above 1 TeV. A stacking method is also used to test catalogs of known high-energy Galactic gamma-ray sources.

Abstract Copyright: © 2017. The American Astronomical Society. All rights reserved.

Journal keyword(s): gamma rays: ISM - gamma rays: ISM

Simbad objects: 42

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Number of rows : 42
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 1572A SN* 00 25 21.5 +64 08 27           B8 1254 1
2 M 1 SNR 05 34 31.8 +22 01 03           ~ 6516 1
3 IC 443 SNR 06 17 00.0000000 +22 34 11.998901           ~ 1314 1
4 NAME Vela Jr SN SNR 08 52.0 -46 20           ~ 507 2
5 ESO 134-11 HII 14 40 29 -62 38.7           ~ 585 1
6 NAME Lupus SN SNR 15 02 22.1 -42 05 49           ~ 1407 1
7 3A 1510-590 Psr 15 13 17.000 -59 04 54.00           ~ 434 3
8 HESS J1634-472 gam 16 34 51.11927 -47 14 01.9360           ~ 31 0
9 SNR G338.3-00.0 SNR 16 40 43.2 -46 31 48           ~ 175 2
10 HESS J1641-463 gam 16 41 01.7 -46 18 11           ~ 27 0
11 HESS J1708-410 gam 17 08 24.0 -41 05 24           ~ 21 0
12 SNR G347.3-00.5 SNR 17 12 27 -39 41.2     12.27     ~ 761 1
13 HESS J1718-385 gam 17 18 07 -38 33.0           ~ 32 0
14 NAME Galactic Center reg 17 45 39.60213 -29 00 22.0000           ~ 16269 0
15 NAME Sgr A* X 17 45 40.03599 -29 00 28.1699           ~ 4970 3
16 SNR G000.9+00.1 SNR 17 47.3 -28 09           ~ 222 1
17 Fermi J1808.2-2029 gam 18 08 00.0 -20 24 00           ~ 20 0
18 HESS J1809-193 gam 18 10 31 -19 18.0           ~ 70 1
19 NAME AGPS 273.4-17.8 SNR 18 13 35.05 -17 49 58.1           ~ 145 2
20 1HWC J1825-133 gam 18 25 -13.3           ~ 4 0
21 PSR B1823-13 Psr 18 26 13.06 -13 34 48.1           ~ 460 1
22 1HWC J1836-090c gam 18 36 -09.0           ~ 2 0
23 1HWC J1836-074c gam 18 36 -07.4           ~ 2 0
24 1HWC J1838-060 gam 18 38 -06.0           ~ 4 0
25 1HWC J1842-046c gam 18 42 -04.6           ~ 3 0
26 ARGO J1841-0332 gam 18 43.6 -03 36           ~ 40 0
27 1HWC J1844-031c gam 18 44 -03.1           ~ 4 0
28 1HWC J1849-017c gam 18 49 -01.7           ~ 4 0
29 MGRO J1852+01 gam 18 52 +01.0           ~ 2 0
30 1HWC J1857+023 gam 18 57 +02.3           ~ 3 0
31 HESS J1858+020 gam 18 58 20.0 +02 05 24           ~ 45 0
32 1HWC J1904+080c gam 19 04 +08.0           ~ 3 0
33 1HWC J1907+062c gam 19 07 +06.2           ~ 4 0
34 ARGO J1907+0627 gam 19 08 12.24 +06 23 30.8           ~ 94 0
35 SNR G054.1+00.3 SNR 19 30 10.6 +18 50 22           ~ 271 1
36 1LHAASO J2018+3643u gam 20 18.6 +36 43           ~ 67 0
37 MGRO J2032+37 gam 20 31.0 +36 31           ~ 1 0
38 TeV J2032+4130 gam 20 31.7 +41 31           ~ 148 0
39 NAME Cyg Complex reg 20 32 +45.0           ~ 667 0
40 MGRO J2043+36 gam 20 43.9 +36 18           ~ 1 0
41 NAME Cas A SNR 23 23 26.0 +58 48 41     14.30     ~ 3033 1
42 NAME Galactic Ridge ? ~ ~           ~ 543 1

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