2023ApJ...945L...8A


Query : 2023ApJ...945L...8A

2023ApJ...945L...8A - Astrophys. J., 945, L8 (2023/March-1)

Searches for Neutrinos from Large High Altitude Air Shower Observatory Ultra-high-energy γ-Ray Sources Using the IceCube Neutrino Observatory.

ABBASI R., ACKERMANN M., ADAMS J., AGGARWAL N., AGUILAR J.A., AHLERS M., ALAMEDDINE J.M., ALVES A.A.Jr, AMIN N.M., ANDEEN K., ANDERSON T., 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., BENDA S., BENZVI S., BERLEY D., BERNARDINI E., BESSON D.Z., BINDER G., BINDIG D., BLAUFUSS E., BLOT S., BONTEMPO F., BOOK J.Y., BOROWKA J., BOSCOLO MENEGUOLO C., BOSER S., BOTNER O., BOTTCHER J., BOURBEAU E., BRAUN J., BRINSON B., BROSTEAN-KAISER J., BURLEY R.T., BUSSE R.S., CAMPANA M.A., CARNIE-BRONCA E.G., CHANG Y.L., CHEN C., CHEN Z., CHIRKIN D., CHOI K., CLARK B.A., CLASSEN L., COLEMAN A., COLLIN G.H., CONNOLLY A., CONRAD J.M., COPPIN P., CORREA P., COUNTRYMAN S., COWEN D.F., DAPPEN C., 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., DUJMOVIC H., DUVERNOIS M.A., EHRHARDT T., ELLER P., ENGEL R., ERPENBECK H., EVANS J., EVENSON P.A., FAN K.L., FAZELY A.R., FEDYNITCH A., FEIGL N., FIEDLSCHUSTER S., FIENBERG A.T., 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., GREGOIRE T., 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., JANSSON M., JAPARIDZE G.S., 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., 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., 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., MICALLEF J., MOCKLER D., MONTARULI T., MOORE R.W., MORSE R., MOULAI M., MUKHERJEE T., NAAB R., NAGAI R., NAUMANN U., NAYERHODA A., NECKER J., NEUMANN M., NIEDERHAUSEN H., NISA M.U., NOELL A., NOWICKI S.C., OBERTACKE POLLMANN A., OEHLER M., OEYEN B., OLIVAS A., ORSOE R., OSBORN J., O'SULLIVAN E., PANDYA H., PANKOVA D.V., 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., PORCELLI A., PRADO RODRIGUEZ M., PRIES B., PROCTER-MURPHY R., PRZYBYLSKI G.T., RAAB C., RACK-HELLEIS J., RAMEEZ M., 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., RYSEWYK CANTU D., SAFA I., SAFFER J., SALAZAR-GALLEGOS D., SAMPATHKUMAR P., SANCHEZ HERRERA S.E., SANDROCK A., SANTANDER M., SARKAR S., SARKAR S., SAVELBERG J., SCHAUFEL M., SCHIELER H., SCHINDLER S., SCHLUETER 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., SPANNFELLNER C., SPICZAK G.M., SPIERING C., STAMATIKOS M., STANEV T., 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., UPSHAW K., VALTONEN-MATTILA N., VANDENBROUCKE J., VAN EIJNDHOVEN N., VANNEROM D., VAN SANTEN J., VARA J., VEITCH-MICHAELIS J., VERPOEST S., VESKE D., WALCK C., WANG W., 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 D.L., XU X.W., YANEZ J.P., YASUTSUGU M., YILDIZCI E., YOSHIDA S., YU S., YUAN T., ZHANG Z., ZHELNIN P. (The IceCube Collaboration)

Abstract (from CDS):

Galactic PeV cosmic-ray accelerators (PeVatrons) are Galactic sources theorized to accelerate cosmic rays up to PeV in energy. The accelerated cosmic rays are expected to interact hadronically with nearby ambient gas or the interstellar medium, resulting in γ-rays and neutrinos. Recently, the Large High Altitude Air Shower Observatory (LHAASO) identified 12 γ-ray sources with emissions above 100 TeV, making them candidates for PeVatrons. While at these high energies the Klein-Nishina effect exponentially suppresses leptonic emission from Galactic sources, evidence for neutrino emission would unequivocally confirm hadronic acceleration. Here, we present the results of a search for neutrinos from these γ-ray sources and stacking searches testing for excess neutrino emission from all 12 sources as well as their subcatalogs of supernova remnants and pulsar wind nebulae with 11 yr of track events from the IceCube Neutrino Observatory. No significant emissions were found. Based on the resulting limits, we place constraints on the fraction of γ-ray flux originating from the hadronic processes in the Crab Nebula and LHAASO J2226+6057.

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

Journal keyword(s): Neutrino astronomy - High energy astrophysics - Galactic cosmic rays

Simbad objects: 21

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Number of rows : 21
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 LHAASO J0534+2202 gam 05 34.0 +22 02           ~ 5 0
2 M 1 SNR 05 34 31.8 +22 01 03           ~ 6516 1
3 eHWC J1825-134 gam 18 25.0 -13 26           ~ 21 0
4 HAWC J1825-134 gam 18 25.8 -13 25           ~ 10 0
5 LHAASO J1839-0545 gam 18 39.0 -05 45           ~ 9 0
6 LHAASO J1843-0338 gam 18 43.0 -03 38           ~ 11 0
7 LHAASO J1849-0003 gam 18 49.0 -00 03           ~ 9 0
8 PSR J1849-0001 Psr 18 49 01.83 -00 01 19.1           ~ 76 0
9 eHWC J1907+063 gam 19 07 +06.3           ~ 10 0
10 LHAASO J1908+0621 gam 19 08.0 +06 21           ~ 21 0
11 ARGO J1907+0627 gam 19 08 12.24 +06 23 30.8           ~ 94 0
12 LHAASO J1929+1745 gam 19 29.0 +17 45           ~ 10 0
13 LHAASO J1956+2845 gam 19 56.2 +28 45           ~ 9 0
14 SH 2-104 HII 20 17 52.5 +36 49 24           ~ 97 0
15 LHAASO J2018+3651 gam 20 18.0 +36 51           ~ 10 0
16 1LHAASO J2018+3643u gam 20 18.6 +36 43           ~ 67 0
17 eHWC J2019+368 gam 20 19 +36.8           ~ 10 0
18 LHAASO J2032+4102 gam 20 32.0 +41 02           ~ 14 0
19 1FGL J2107.5+5202c Bz? 21 08 04.0 +51 55 39           ~ 39 0
20 LHAASO J2226+6057 gam 22 26.0 +60 57           ~ 16 0
21 SNR G106.3+02.7 SNR 22 27.5 +60 50           ~ 99 1

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