Constraints on Populations of Neutrino Sources from Searches in the Directions of IceCube Neutrino Alerts
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- Journal article
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- Autoren
- R Abbasi
- M Ackermann
- J Adams
- N Aggarwal
- JA Aguilar
- M Ahlers
- JM Alameddine
- AA Alves
- NM Amin
- K Andeen
- T Anderson
- G Anton
- C Arguelles
- Y Ashida
- S Athanasiadou
- SN Axani
- X Bai
- A Balagopal
- M Baricevic
- SW Barwick
- V Basu
- R Bay
- JJ Beatty
- K-H Becker
- J Becker Tjus
- J Beise
- C Bellenghi
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- E Bernardini
- DZ Besson
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- J Boettcher
- E Bourbeau
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- B Brinson
- J Brostean-Kaiser
- RT Burley
- RS Busse
- MA Campana
- EG Carnie-Bronca
- C Chen
- Z Chen
- D Chirkin
- K Choi
- BA Clark
- L Classen
- A Coleman
- GH Collin
- A Connolly
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- P Coppin
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- P Dave
- C De Clercq
- JJ DeLaunay
- D Delgado Lopez
- H Dembinski
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- A Desai
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- KD de Vries
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- A Diaz
- JC Diaz-Velez
- M Dittmer
- H Dujmovic
- MA DuVernois
- T Ehrhardt
- P Eller
- R Engel
- H Erpenbeck
- J Evans
- PA Evenson
- KL Fan
- AR Fazely
- A Fedynitch
- N Feigl
- S Fiedlschuster
- AT Fienberg
- 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
- N Goehlke
- JG Gonzalez
- S Goswami
- D Grant
- SJ Gray
- T Gregoire
- S Griswold
- C Guenther
- P Gutjahr
- C Haack
- A Hallgren
- R Halliday
- L Halve
- F Halzen
- H Hamdaoui
- M Ha Minh
- K Hanson
- J Hardin
- AA Harnisch
- P Hatch
- A Haungs
- K Helbing
- J Hellrung
- F Henningsen
- L Heuermann
- S Hickford
- A Hidvegi
- C Hill
- GC Hill
- KD Hoffman
- K Hoshina
- W Hou
- 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
- JL Kelley
- A Kheirandish
- K Kin
- J Kiryluk
- SR Klein
- A Kochocki
- R Koirala
- H Kolanoski
- T Kontrimas
- L Koepke
- C Kopper
- DJ Koskinen
- P Koundal
- M Kovacevich
- M Kowalski
- T Kozynets
- E Krupczak
- E Kun
- N Kurahashi
- N Lad
- C Lagunas Gualda
- MJ Larson
- F Lauber
- JP Lazar
- JW Lee
- K Leonard
- A Leszczynska
- M Lincetto
- QR Liu
- M Liubarska
- E Lohfink
- C Love
- CJ Lozano Mariscal
- L Lu
- F Lucarelli
- A Ludwig
- W Luszczak
- Y Lyu
- WY Ma
- J Madsen
- KBM Mahn
- Y Makino
- S Mancina
- W Marie Sainte
- IC Maris
- S Marka
- Z Marka
- M Marsee
- I Martinez-Soler
- R Maruyama
- T McElroy
- F McNally
- JV Mead
- K Meagher
- S Mechbal
- A Medina
- M Meier
- S Meighen-Berger
- Y Merckx
- J Micallef
- D Mockler
- T Montaruli
- RW Moore
- R Morse
- M Moulai
- T Mukherjee
- R Naab
- R Nagai
- U Naumann
- A Nayerhoda
- J Necker
- M Neumann
- H Niederhausen
- MU Nisa
- A Noell
- SC Nowicki
- A Obertacke Pollmann
- M Oehler
- B Oeyen
- A Olivas
- R Orsoe
- J Osborn
- 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
- A Pizzuto
- M Plum
- Y Popovych
- A Porcelli
- M Prado Rodriguez
- B Pries
- R Procter-Murphy
- GT Przybylski
- C Raab
- J Rack-Helleis
- M Rameez
- K Rawlins
- Z Rechav
- A Rehman
- P Reichherzer
- G Renzi
- E Resconi
- S Reusch
- W Rhode
- M Richman
- B Riedel
- EJ Roberts
- S Robertson
- S Rodan
- G Roellinghoff
- M Rongen
- C Rott
- T Ruhe
- L Ruohan
- D Ryckbosch
- D Rysewyk Cantu
- I Safa
- J Saffer
- D Salazar-Gallegos
- P Sampathkumar
- SE Sanchez Herrera
- A Sandrock
- M Santander
- S Sarkar
- J Savelberg
- M Schaufel
- H Schieler
- S Schindler
- B Schlueter
- T Schmidt
- J Schneider
- FG Schroeder
- L Schumacher
- G Schwefer
- S Sclafani
- S Seunarine
- A Sharma
- S Shefali
- N Shimizu
- M Silva
- B Skrzypek
- B Smithers
- R Snihur
- J Soedingrekso
- A Sogaard
- D Soldin
- C Spannfellner
- GM Spiczak
- C Spiering
- M Stamatikos
- T Stanev
- R Stein
- T Stezelberger
- T Stuerwald
- T Stuttard
- GW Sullivan
- I Taboada
- S Ter-Antonyan
- WG Thompson
- J Thwaites
- S Tilav
- K Tollefson
- C Tonnis
- S Toscano
- D Tosi
- A Trettin
- CF Tung
- R Turcotte
- JP Twagirayezu
- B Ty
- MA Unland Elorrieta
- K Upshaw
- N Valtonen-Mattila
- J Vandenbroucke
- N van Eijndhoven
- D Vannerom
- J van Santen
- J Vara
- J Veitch-Michaelis
- S Verpoest
- D Veske
- C Walck
- W Wang
- TB Watson
- C Weaver
- P Weigel
- A Weindl
- J Weldert
- C Wendt
- J Werthebach
- M Weyrauch
- N Whitehorn
- CH Wiebusch
- N Willey
- DR Williams
- M Wolf
- G Wrede
- J Wulff
- XW Xu
- JP Yanez
- E Yildizci
- 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:001023878800001&DestLinkType=FullRecord&DestApp=WOS_CPL
- DOI
- 10.3847/1538-4357/acd2ca
- eISSN
- 1538-4357
- Externe Identifier
- Clarivate Analytics Document Solution ID: L5TC7
- ISSN
- 0004-637X
- Ausgabe der Veröffentlichung
- 1
- Zeitschrift
- ASTROPHYSICAL JOURNAL
- Artikelnummer
- ARTN 45
- Datum der Veröffentlichung
- 2023
- Status
- Published
- Titel
- Constraints on Populations of Neutrino Sources from Searches in the Directions of IceCube Neutrino Alerts
- Sub types
- Article
- Ausgabe der Zeitschrift
- 951
Data source: Web of Science (Lite)
- Other metadata sources:
-
- Abstract
- <jats:title>Abstract</jats:title> <jats:p>Beginning in 2016, the IceCube Neutrino Observatory has sent out alerts in real time containing the information of high-energy (<jats:italic>E</jats:italic> ≳ 100 TeV) neutrino candidate events with moderate to high (≳30%) probability of astrophysical origin. In this work, we use a recent catalog of such alert events, which, in addition to events announced in real time, includes events that were identified retroactively and covers the time period of 2011–2020. We also search for additional, lower-energy neutrinos from the arrival directions of these IceCube alerts. We show how performing such an analysis can constrain the contribution of rare populations of cosmic neutrino sources to the diffuse astrophysical neutrino flux. After searching for neutrino emission coincident with these alert events on various timescales, we find no significant evidence of either minute-scale or day-scale transient neutrino emission or of steady neutrino emission in the direction of these alert events. This study also shows how numerous a population of neutrino sources has to be to account for the complete astrophysical neutrino flux. Assuming that sources have the same luminosity, an <jats:italic>E</jats:italic> <jats:sup>−2.5</jats:sup> neutrino spectrum, and number densities that follow star formation rates, the population of sources has to be more numerous than 7 × 10<jats:sup>−9</jats:sup> Mpc<jats:sup>−3</jats:sup>. This number changes to 3 × 10<jats:sup>−7</jats:sup> Mpc<jats:sup>−3</jats:sup> if number densities instead have no cosmic evolution.</jats:p>
- Autoren
- R Abbasi
- M Ackermann
- J Adams
- N Aggarwal
- JA Aguilar
- M Ahlers
- JM Alameddine
- AA Alves
- NM Amin
- K Andeen
- T Anderson
- G Anton
- C Argüelles
- Y Ashida
- S Athanasiadou
- SN Axani
- X Bai
- A Balagopal V.
- M Baricevic
- SW Barwick
- V Basu
- R Bay
- JJ Beatty
- K-H Becker
- J Becker Tjus
- J Beise
- C Bellenghi
- S Benda
- S BenZvi
- D Berley
- E Bernardini
- DZ Besson
- G Binder
- D Bindig
- E Blaufuss
- S Blot
- F Bontempo
- JY Book
- J Borowka
- C Boscolo Meneguolo
- S Böser
- O Botner
- J Böttcher
- E Bourbeau
- J Braun
- B Brinson
- J Brostean-Kaiser
- RT Burley
- RS Busse
- MA Campana
- EG Carnie-Bronca
- C Chen
- Z Chen
- D Chirkin
- K Choi
- BA Clark
- L Classen
- A Coleman
- GH Collin
- A Connolly
- JM Conrad
- P Coppin
- P Correa
- S Countryman
- 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
- T DeYoung
- A Diaz
- JC Díaz-Vélez
- M Dittmer
- H Dujmovic
- MA DuVernois
- T Ehrhardt
- P Eller
- R Engel
- H Erpenbeck
- J Evans
- PA Evenson
- KL Fan
- AR Fazely
- A Fedynitch
- N Feigl
- S Fiedlschuster
- AT Fienberg
- 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
- N Goehlke
- JG Gonzalez
- S Goswami
- D Grant
- SJ Gray
- T Grégoire
- S Griswold
- C Günther
- P Gutjahr
- C Haack
- A Hallgren
- R Halliday
- L Halve
- F Halzen
- H Hamdaoui
- M Ha Minh
- K Hanson
- J Hardin
- AA Harnisch
- P Hatch
- A Haungs
- K Helbing
- J Hellrung
- F Henningsen
- L Heuermann
- S Hickford
- A Hidvegi
- C Hill
- GC Hill
- KD Hoffman
- K Hoshina
- W Hou
- 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
- JL Kelley
- A Kheirandish
- K Kin
- J Kiryluk
- SR Klein
- A Kochocki
- R Koirala
- H Kolanoski
- T Kontrimas
- L Köpke
- C Kopper
- DJ Koskinen
- P Koundal
- M Kovacevich
- M Kowalski
- T Kozynets
- E Krupczak
- E Kun
- N Kurahashi
- N Lad
- C Lagunas Gualda
- MJ Larson
- F Lauber
- JP Lazar
- JW Lee
- K Leonard
- A Leszczyńska
- M Lincetto
- QR Liu
- M Liubarska
- E Lohfink
- C Love
- CJ Lozano Mariscal
- L Lu
- F Lucarelli
- A Ludwig
- W Luszczak
- Y Lyu
- WY Ma
- J Madsen
- KBM Mahn
- Y Makino
- S Mancina
- W Marie Sainte
- IC Mariş
- S Marka
- Z Marka
- M Marsee
- I Martinez-Soler
- R Maruyama
- T McElroy
- F McNally
- JV Mead
- K Meagher
- S Mechbal
- A Medina
- M Meier
- S Meighen-Berger
- Y Merckx
- J Micallef
- D Mockler
- T Montaruli
- RW Moore
- R Morse
- M Moulai
- T Mukherjee
- R Naab
- R Nagai
- U Naumann
- A Nayerhoda
- J Necker
- M Neumann
- H Niederhausen
- MU Nisa
- A Noell
- SC Nowicki
- A Obertacke Pollmann
- M Oehler
- B Oeyen
- A Olivas
- R Orsoe
- J Osborn
- 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
- A Pizzuto
- M Plum
- Y Popovych
- A Porcelli
- M Prado Rodriguez
- B Pries
- R Procter-Murphy
- GT Przybylski
- C Raab
- J Rack-Helleis
- M Rameez
- K Rawlins
- Z Rechav
- A Rehman
- P Reichherzer
- G Renzi
- E Resconi
- S Reusch
- W Rhode
- M Richman
- B Riedel
- EJ Roberts
- S Robertson
- S Rodan
- G Roellinghoff
- M Rongen
- C Rott
- T Ruhe
- L Ruohan
- D Ryckbosch
- D Rysewyk Cantu
- I Safa
- J Saffer
- D Salazar-Gallegos
- P Sampathkumar
- SE Sanchez Herrera
- A Sandrock
- M Santander
- S Sarkar
- S Sarkar
- J Savelberg
- M Schaufel
- H Schieler
- S Schindler
- B Schlueter
- T Schmidt
- J Schneider
- FG Schröder
- L Schumacher
- G Schwefer
- S Sclafani
- S Seunarine
- A Sharma
- S Shefali
- N Shimizu
- M Silva
- B Skrzypek
- B Smithers
- R Snihur
- J Soedingrekso
- A Søgaard
- D Soldin
- C Spannfellner
- GM Spiczak
- C Spiering
- M Stamatikos
- T Stanev
- R Stein
- T Stezelberger
- T Stürwald
- T Stuttard
- GW Sullivan
- I Taboada
- S Ter-Antonyan
- WG Thompson
- J Thwaites
- S Tilav
- K Tollefson
- C Tönnis
- S Toscano
- D Tosi
- A Trettin
- CF Tung
- R Turcotte
- JP Twagirayezu
- B Ty
- MA Unland Elorrieta
- K Upshaw
- N Valtonen-Mattila
- J Vandenbroucke
- N van Eijndhoven
- D Vannerom
- J van Santen
- J Vara
- J Veitch-Michaelis
- S Verpoest
- D Veske
- C Walck
- W Wang
- TB Watson
- C Weaver
- P Weigel
- A Weindl
- J Weldert
- C Wendt
- J Werthebach
- M Weyrauch
- N Whitehorn
- CH Wiebusch
- N Willey
- DR Williams
- M Wolf
- G Wrede
- J Wulff
- XW Xu
- JP Yanez
- E Yildizci
- S Yoshida
- S Yu
- T Yuan
- Z Zhang
- P Zhelnin
- DOI
- 10.3847/1538-4357/acd2ca
- eISSN
- 1538-4357
- ISSN
- 0004-637X
- Ausgabe der Veröffentlichung
- 1
- Zeitschrift
- The Astrophysical Journal
- Online publication date
- 2023
- Paginierung
- 45 - 45
- Datum der Veröffentlichung
- 2023
- Status
- Published
- Herausgeber
- American Astronomical Society
- Herausgeber URL
- http://dx.doi.org/10.3847/1538-4357/acd2ca
- Datum der Datenerfassung
- 2024
- Titel
- Constraints on Populations of Neutrino Sources from Searches in the Directions of IceCube Neutrino Alerts
- Ausgabe der Zeitschrift
- 951
Data source: Crossref
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