Evidence for neutrino emission from the nearby active galaxy NGC 1068

Publication type:

Journal article

Metadata:

Autoren

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

Autoren-URL

https://www.webofscience.com/api/gateway?GWVersion=2&SrcApp=fis-test-1&SrcAuth=WosAPI&KeyUT=WOS:000903333800005&DestLinkType=FullRecord&DestApp=WOS_CPL

DOI

10.1126/science.abg3395

eISSN

1095-9203

Externe Identifier

Clarivate Analytics Document Solution ID: 7H6TQ
PubMed Identifier: 36378962

ISSN

0036-8075

Ausgabe der Veröffentlichung

6619

Zeitschrift

SCIENCE

Paginierung

538 - +

Datum der Veröffentlichung

2022

Status

Published

Titel

Evidence for neutrino emission from the nearby active galaxy NGC 1068

Sub types

Article

Ausgabe der Zeitschrift

378

Data source: Web of Science (Lite)

Other metadata sources:

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 <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" overflow="scroll"> <mml:mrow> <mml:msubsup> <mml:mrow> <mml:mn>79</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>−</mml:mo> <mml:mn>20</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>+</mml:mo> <mml:mn>22</mml:mn> </mml:mrow> </mml:msubsup> </mml:mrow> </mml:math> 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.

Autoren

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

DOI

10.1126/science.abg3395

eISSN

1095-9203

ISSN

0036-8075

Ausgabe der Veröffentlichung

6619

Zeitschrift

Science

Sprache

Paginierung

538 - 543

Datum der Veröffentlichung

2022

Status

Published

Herausgeber

American Association for the Advancement of Science (AAAS)

Herausgeber URL

http://dx.doi.org/10.1126/science.abg3395

Datum der Datenerfassung

2024

Titel

Evidence for neutrino emission from the nearby active galaxy NGC 1068

Ausgabe der Zeitschrift

378

Data source: Crossref

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.

Autoren

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

DOI

10.1126/science.abg3395

eISSN

1095-9203

Externe Identifier

PubMed Identifier: 36378962

Open access

false

ISSN

0036-8075

Ausgabe der Veröffentlichung

6619

Zeitschrift

Science (New York, N.Y.)

Schlüsselwörter

IceCube Collaboration*†

Sprache

eng

Medium

Print-Electronic

Online publication date

2022

Paginierung

538 - 543

Datum der Veröffentlichung

2022

Status

Published

Datum der Datenerfassung

2022

Titel

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

Sub types

Research Support, Non-U.S. Gov't
Research Support, U.S. Gov't, Non-P.H.S.
Journal Article

Ausgabe der Zeitschrift

378

Data source: Europe PubMed Central

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.

Autoren

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

Autoren-URL

https://www.ncbi.nlm.nih.gov/pubmed/36378962

DOI

10.1126/science.abg3395

eISSN

1095-9203

Ausgabe der Veröffentlichung

6619

Zeitschrift

Science

Sprache

eng

Country

United States

Paginierung

538 - 543

Datum der Veröffentlichung

2022

Status

Published

Datum, an dem der Datensatz öffentlich gemacht wurde

2022

Titel

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

Sub types

Journal Article
Research Support, Non-U.S. Gov't
Research Support, U.S. Gov't, Non-P.H.S.

Ausgabe der Zeitschrift

378

Data source: PubMed

Beziehungen:

Has preprint

Evidence for neutrino emission from the nearby active galaxy NGC 1068

Property of

QUANTUM 2

Evidence for neutrino emission from the nearby active galaxy NGC 1068

Tools