Back to Search Start Over

Evidence for neutrino emission from the nearby active galaxy NGC 1068.

Authors :
Abbasi R
Ackermann M
Adams J
Aguilar JA
Ahlers M
Ahrens M
Alameddine JM
Alispach C
Alves AA Jr
Amin NM
Andeen K
Anderson T
Anton G
Argüelles C
Ashida Y
Axani S
Bai X
Balagopal V A
Barbano A
Barwick SW
Bastian B
Basu V
Baur S
Bay R
Beatty JJ
Becker KH
Becker Tjus J
Bellenghi C
BenZvi S
Berley D
Bernardini E
Besson DZ
Binder G
Bindig D
Blaufuss E
Blot S
Boddenberg M
Bontempo F
Borowka J
Böser S
Botner O
Böttcher J
Bourbeau E
Bradascio F
Braun J
Brinson B
Bron S
Brostean-Kaiser J
Browne S
Burgman A
Burley RT
Busse RS
Campana MA
Carnie-Bronca EG
Chen C
Chen Z
Chirkin D
Choi K
Clark BA
Clark K
Classen L
Coleman A
Collin GH
Conrad JM
Coppin P
Correa P
Cowen DF
Cross R
Dappen C
Dave P
De Clercq C
DeLaunay JJ
Delgado López D
Dembinski H
Deoskar K
Desai A
Desiati P
de Vries KD
de Wasseige G
de With M
DeYoung T
Diaz A
Díaz-Vélez JC
Dittmer M
Dujmovic H
Dunkman M
DuVernois MA
Dvorak E
Ehrhardt T
Eller P
Engel R
Erpenbeck H
Evans J
Evenson PA
Fan KL
Fazely AR
Fedynitch A
Feigl N
Fiedlschuster S
Fienberg AT
Filimonov K
Finley C
Fischer L
Fox D
Franckowiak A
Friedman E
Fritz A
Fürst P
Gaisser TK
Gallagher J
Ganster E
Garcia A
Garrappa S
Gerhardt L
Ghadimi A
Glaser C
Glauch T
Glüsenkamp T
Goldschmidt A
Gonzalez JG
Goswami S
Grant D
Grégoire T
Griswold S
Günther C
Gutjahr P
Haack C
Hallgren A
Halliday R
Halve L
Halzen F
Ha Minh M
Hanson K
Hardin J
Harnisch AA
Haungs A
Hebecker D
Helbing K
Henningsen F
Hettinger EC
Hickford S
Hignight J
Hill C
Hill GC
Hoffman KD
Hoffmann R
Hokanson-Fasig B
Hoshina K
Huang F
Huber M
Huber T
Hultqvist K
Hünnefeld M
Hussain R
Hymon K
In S
Iovine N
Ishihara A
Jansson M
Japaridze GS
Jeong M
Jin M
Jones BJP
Kang D
Kang W
Kang X
Kappes A
Kappesser D
Kardum L
Karg T
Karl M
Karle A
Katz U
Kauer M
Kellermann M
Kelley JL
Kheirandish A
Kin K
Kintscher T
Kiryluk J
Klein SR
Koirala R
Kolanoski H
Kontrimas T
Köpke L
Kopper C
Kopper S
Koskinen DJ
Koundal P
Kovacevich M
Kowalski M
Kozynets T
Kun E
Kurahashi N
Lad N
Lagunas Gualda C
Lanfranchi JL
Larson MJ
Lauber F
Lazar JP
Lee JW
Leonard K
Leszczyńska A
Li Y
Lincetto M
Liu QR
Liubarska M
Lohfink E
Lozano Mariscal CJ
Lu L
Lucarelli F
Ludwig A
Luszczak W
Lyu Y
Ma WY
Madsen J
Mahn KBM
Makino Y
Mancina S
Mariş IC
Martinez-Soler I
Maruyama R
Mase K
McElroy T
McNally F
Mead JV
Meagher K
Mechbal S
Medina A
Meier M
Meighen-Berger S
Micallef J
Mockler D
Montaruli T
Moore RW
Morse R
Moulai M
Naab R
Nagai R
Nahnhauer R
Naumann U
Necker J
Nguyen LV
Niederhausen H
Nisa MU
Nowicki SC
Nygren D
Obertacke Pollmann A
Oehler M
Oeyen B
Olivas A
O'Sullivan E
Pandya H
Pankova DV
Park N
Parker GK
Paudel EN
Paul L
Pérez de Los Heros C
Peters L
Peterson J
Philippen S
Pieper S
Pittermann M
Pizzuto A
Plum M
Popovych Y
Porcelli A
Prado Rodriguez M
Price PB
Pries B
Przybylski GT
Raab C
Rack-Helleis J
Raissi A
Rameez M
Rawlins K
Rea IC
Rehman A
Reichherzer P
Reimann R
Renzi G
Resconi E
Reusch S
Rhode W
Richman M
Riedel B
Roberts EJ
Robertson S
Roellinghoff G
Rongen M
Rott C
Ruhe T
Ryckbosch D
Rysewyk Cantu D
Safa I
Saffer J
Sanchez Herrera SE
Sandrock A
Sandroos J
Santander M
Sarkar S
Sarkar S
Satalecka K
Schaufel M
Schieler H
Schindler S
Schmidt T
Schneider A
Schneider J
Schröder FG
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 GM
Spiering C
Stachurska J
Stamatikos M
Stanev T
Stein R
Stettner J
Steuer A
Stezelberger T
Stokstad R
Stürwald T
Stuttard T
Sullivan GW
Taboada I
Ter-Antonyan S
Tilav S
Tischbein F
Tollefson K
Tönnis C
Toscano S
Tosi D
Trettin A
Tselengidou M
Tung CF
Turcati A
Turcotte R
Turley CF
Twagirayezu JP
Ty B
Unland Elorrieta MA
Valtonen-Mattila N
Vandenbroucke J
van Eijndhoven N
Vannerom D
van Santen J
Verpoest S
Walck C
Watson TB
Weaver C
Weigel P
Weindl A
Weiss MJ
Weldert J
Wendt C
Werthebach J
Weyrauch M
Whitehorn N
Wiebusch CH
Williams DR
Wolf M
Woschnagg K
Wrede G
Wulff J
Xu XW
Yanez JP
Yoshida S
Yu S
Yuan T
Zhang Z
Zhelnin P
Source :
Science (New York, N.Y.) [Science] 2022 Nov 04; Vol. 378 (6619), pp. 538-543. Date of Electronic Publication: 2022 Nov 03.
Publication Year :
2022

Abstract

A supermassive black hole, obscured by cosmic dust, powers the nearby active galaxy NGC 1068. Neutrinos, which rarely interact with matter, could provide information on the galaxy's active core. We searched for neutrino emission from astrophysical objects using data recorded with the IceCube neutrino detector between 2011 and 2020. The positions of 110 known gamma-ray sources were individually searched for neutrino detections above atmospheric and cosmic backgrounds. We found that NGC 1068 has an excess of [Formula: see text] neutrinos at tera-electron volt energies, with a global significance of 4.2σ, which we interpret as associated with the active galaxy. The flux of high-energy neutrinos that we measured from NGC 1068 is more than an order of magnitude higher than the upper limit on emissions of tera-electron volt gamma rays from this source.

Details

Language :
English
ISSN :
1095-9203
Volume :
378
Issue :
6619
Database :
MEDLINE
Journal :
Science (New York, N.Y.)
Publication Type :
Academic Journal
Accession number :
36378962
Full Text :
https://doi.org/10.1126/science.abg3395