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2022ApJ...926...59A - Astrophys. J., 926, 59-59 (2022/February-2)

Search for High-energy Neutrinos from Ultraluminous Infrared Galaxies with IceCube.

ABBASI R., ACKERMANN M., ADAMS J., AGUILAR J.A., AHLERS M., AHRENS M., ALISPACH C., ALVES A.A., AMIN N.M., AN R., ANDEEN K., ANDERSON T., ANTON G., ARGUELLES C., ASHIDA Y., AXANI S., BAI X., BALAGOPAL V.A., BARBANO A., BARWICK S.W., BASTIAN B., BASU V., BAUR S., BAY R., BEATTY J.J., BECKER K.-H., BECKER TJUS J., BELLENGHI C., BENZVI S., BERLEY D., BERNARDINI E., BESSON D.Z., BINDER G., BINDIG D., BLAUFUSS E., BLOT S., BODDENBERG M., BONTEMPO F., BOROWKA J., BOSER S., BOTNER O., BOTTCHER J., BOURBEAU E., BRADASCIO F., BRAUN J., BRON S., BROSTEAN-KAISER J., BROWNE S., BURGMAN A., BURLEY R.T., BUSSE R.S., CAMPANA M.A., CARNIE-BRONCA E.G., CHEN C., CHIRKIN D., CHOI K., CLARK B.A., CLARK K., CLASSEN L., COLEMAN A., COLLIN G.H., CONRAD J.M., COPPIN P., CORREA P., COWEN D.F., CROSS R., DAPPEN C., DAVE P., DE CLERCQ C., DELAUNAY J.J., DEMBINSKI H., DEOSKAR K., DE RIDDER S., DESAI A., DESIATI P., DE VRIES K.D., DE WASSEIGE G., DE WITH M., DEYOUNG T., DHARANI S., DIAZ A., DIAZ-VELEZ J.C., DITTMER M., DUJMOVIC H., DUNKMAN M., DUVERNOIS M.A., DVORAK E., EHRHARDT T., ELLER P., ENGEL R., ERPENBECK H., EVANS J., EVENSON P.A., FAN K.L., FAZELY A.R., FIEDLSCHUSTER S., FIENBERG A.T., FILIMONOV K., 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., GOLDSCHMIDT A., GONZALEZ J.G., GOSWAMI S., GRANT D., GREGOIRE T., GRISWOLD S., GUNDUZ M., GUNTHER C., HAACK C., HALLGREN A., HALLIDAY R., HALVE L., HALZEN F., HA MINH M., HANSON K., HARDIN J., HARNISCH A.A., HAUNGS A., HAUSER S., HEBECKER D., HELBING K., HENNINGSEN F., HETTINGER E.C., HICKFORD S., HIGNIGHT J., HILL C., HILL G.C., HOFFMAN K.D., HOFFMANN R., HOINKA T., HOKANSON-FASIG B., HOSHINA K., HUANG F., HUBER M., HUBER T., HULTQVIST K., HUNNEFELD M., HUSSAIN R., IN S., IOVINE N., ISHIHARA A., JANSSON M., JAPARIDZE G.S., JEONG M., JONES B.J.P., KANG D., KANG W., KANG X., KAPPES A., KAPPESSER D., KARG T., KARL M., KARLE A., KATZ U., KAUER M., KELLERMANN M., KELLEY J.L., KHEIRANDISH A., KIN K., KINTSCHER T., KIRYLUK J., KLEIN S.R., KOIRALA R., KOLANOSKI H., KONTRIMAS T., KOPKE L., KOPPER C., KOPPER S., KOSKINEN D.J., KOUNDAL P., KOVACEVICH M., KOWALSKI M., KOZYNETS T., KUN E., KURAHASHI N., LAD N., LAGUNAS GUALDA C., LANFRANCHI J.L., LARSON M.J., LAUBER F., LAZAR J.P., LEE J.W., LEONARD K., LESZCZYNSKA A., LI Y., LINCETTO M., LIU Q.R., LIUBARSKA M., LOHFINK E., 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., MARIS I.C., MARUYAMA R., MASE K., McELROY T., McNALLY F., MEAD J.V., MEAGHER K., MEDINA A., MEIER M., MEIGHEN-BERGER S., MICALLEF J., MOCKLER D., MONTARULI T., MOORE R.W., MORSE R., MOULAI M., NAAB R., NAGAI R., NAUMANN U., NECKER J., NGUYEN L.V., NIEDERHAUSEN H., NISA M.U., NOWICKI S.C., NYGREN D.R., OBERTACKE POLLMANN A., OEHLER M., OLIVAS A., O'SULLIVAN E., PANDYA H., PANKOVA D.V., PARK N., PARKER G.K., PAUDEL E.N., PAUL L., PEREZ DE LOS HEROS C., PETERS L., PETERSON J., PHILIPPEN S., PIELOTH D., PIEPER S., PITTERMANN M., PIZZUTO A., PLUM M., POPOVYCH Y., PORCELLI A., PRADO RODRIGUEZ M., PRICE P.B., PRIES B., PRZYBYLSKI G.T., RAAB C., RAISSI A., RAMEEZ M., RAWLINS K., REA I.C., REHMAN A., REICHHERZER P., REIMANN R., RENZI G., RESCONI E., REUSCH S., RHODE W., RICHMAN M., RIEDEL B., ROBERTS E.J., ROBERTSON S., ROELLINGHOFF G., RONGEN M., ROTT C., RUHE T., RYCKBOSCH D., RYSEWYK CANTU D., SAFA I., SAFFER J., SANCHEZ HERRERA S.E., SANDROCK A., SANDROOS J., SANTANDER M., SARKAR S., SARKAR S., SATALECKA K., SCHARF M., SCHAUFEL M., SCHIELER H., SCHINDLER S., SCHLUNDER P., SCHMIDT T., SCHNEIDER A., SCHNEIDER J., SCHRODER F.G., SCHUMACHER L., SCHWEFER G., SCLAFANI S., SECKEL D., SEUNARINE S., SHARMA A., SHEFALI S., SILVA M., SKRZYPEK B., SMITHERS B., SNIHUR R., SOEDINGREKSO J., SOLDIN D., SPANNFELLNER C., SPICZAK G.M., SPIERING C., STACHURSKA J., STAMATIKOS M., STANEV T., STEIN R., STETTNER J., STEUER A., STEZELBERGER T., STURWALD T., STUTTARD T., SULLIVAN G.W., TABOADA I., TENHOLT F., TER-ANTONYAN S., TILAV S., TISCHBEIN F., TOLLEFSON K., TOMANKOVA L., TONNIS C., TOSCANO S., TOSI D., TRETTIN A., TSELENGIDOU M., TUNG C.F., TURCATI A., TURCOTTE R., TURLEY C.F., TWAGIRAYEZU J.P., TY B., UNLAND ELORRIETA M.A., VALTONEN-MATTILA N., VANDENBROUCKE J., VAN EIJNDHOVEN N., VANNEROM D., VAN SANTEN J., VERPOEST S., VRAEGHE M., WALCK C., WATSON T.B., WEAVER C., WEIGEL P., WEINDL A., WEISS M.J., WELDERT J., WENDT C., WERTHEBACH J., WEYRAUCH M., WHITEHORN N., WIEBUSCH C.H., WILLIAMS D.R., WOLF M., WOSCHNAGG K., WREDE G., WULFF J., XU X.W., XU Y., YANEZ J.P., YOSHIDA S., YU S., YUAN T., ZHANG Z. (The IceCube Collaboration)

Abstract (from CDS):

Ultraluminous infrared galaxies (ULIRGs) have infrared luminosities L IR >= 1012 L , making them the most luminous objects in the infrared sky. These dusty objects are generally powered by starbursts with star formation rates that exceed 100 M yr–1, possibly combined with a contribution from an active galactic nucleus. Such environments make ULIRGs plausible sources of astrophysical high-energy neutrinos, which can be observed by the IceCube Neutrino Observatory at the South Pole. We present a stacking search for high-energy neutrinos from a representative sample of 75 ULIRGs with redshift z <= 0.13 using 7.5 yr of IceCube data. The results are consistent with a background-only observation, yielding upper limits on the neutrino flux from these 75 ULIRGs. For an unbroken E –2.5 power-law spectrum, we report an upper limit on the stacked flux {Φ}_{ν_µ+{bar}ν_µ}^{90 % }=3.24×{10}{–14} TeV{-1} cm{–2} {s}{-1} {(E/10 TeV)}^{-2.5} at 90% confidence level. In addition, we constrain the contribution of the ULIRG source population to the observed diffuse astrophysical neutrino flux as well as model predictions.

Abstract Copyright: © 2022. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Ultraluminous infrared galaxies - Neutrino astronomy - High energy astrophysics

Simbad objects: 78

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