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Scholarly Works (14 results)
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Article
Peer Reviewed
Marian Lyric in the Cistercian Monastery during the High Middle Ages
Noell, Brian
Comitatus: A Journal of Medieval and Renaissance Studies, Volume 30, Issue 1
(1999)
Multimedia
Peer Reviewed
Hole in Time
Noell, Thomas
CMPM 80K
(2020)
Hole in Time by Thomas Noell Hole in Time is about a commander whose ship is caught in a black hole's gravity and is being attacked by pirates. By helping the whole crew on the ship out, you can escape.
1 supplemental file
Article
Peer Reviewed
Herpes zoster as a cause of atypical chronic ulcerations associated with tofacitinib
Noell, Claire
;
Arbeit, Robert
;
Kanhoush, Rima
Dermatology Online Journal, Volume 24, Issue 1
(2018)
Tofacitinib is a targeted inhibitor of janus kinase (JAK), currently approved for the treatment of rheumatoid arthritis. We present a patient on treatment withtofacitinib who had an episode of classic dermatomal herpes zoster followed months later by atypical chronic cutaneous ulcers also caused by herpes zoster.
Article
Peer Reviewed
Search for sub-TeV Neutrino Emission from Novae with IceCube-DeepCore
Abbasi, R
;
Ackermann, M
;
Adams, J
;
Aggarwal, N
;
Aguilar, JA
;
Ahlers, M
;
Alameddine, JM
;
Alves, AA
;
Amin, NM
;
Andeen, K
;
Anderson, T
;
Anton, G
;
Argüelles, C
;
Ashida, Y
;
Athanasiadou, S
;
Axani, SN
;
Bai, X
;
V., A Balagopal
;
Baricevic, M
;
Barwick, SW
;
Basu, V
;
Bay, R
;
Beatty, JJ
;
Becker, K-H
;
Tjus, J Becker
;
Beise, J
;
Bellenghi, C
;
BenZvi, S
;
Berley, D
;
Bernardini, E
;
Besson, DZ
;
Binder, G
;
Bindig, D
;
Blaufuss, E
;
Blot, S
;
Bontempo, F
;
Book, JY
;
Borowka, J
;
Meneguolo, C Boscolo
;
Böser, S
;
Botner, O
;
Böttcher, J
;
Bourbeau, E
;
Braun, J
;
Brinson, B
;
Brostean-Kaiser, J
;
Burley, RT
;
Busse, RS
;
Campana, MA
;
Carnie-Bronca, EG
;
Chen, C
;
Chen, Z
;
Chirkin, D
;
Choi, S
;
Clark, BA
;
Classen, L
;
Coleman, A
;
Collin, GH
;
Connolly, A
;
Conrad, JM
;
Coppin, P
;
Correa, P
;
Countryman, S
;
Cowen, DF
;
Dappen, C
;
Dave, P
;
De Clercq, C
;
DeLaunay, JJ
;
López, D Delgado
;
Dembinski, H
;
Deoskar, K
;
Desai, A
;
Desiati, P
;
de Vries, KD
;
de Wasseige, G
;
DeYoung, T
;
Diaz, A
;
Díaz-Vélez, JC
;
Dittmer, M
;
Dujmovic, H
;
DuVernois, MA
;
Ehrhardt, T
;
Eller, P
;
Engel, R
;
Erpenbeck, H
;
Evans, J
;
Evenson, PA
;
Fan, KL
;
Fazely, AR
;
Fedynitch, A
;
Feigl, N
;
Fiedlschuster, S
;
Fienberg, AT
;
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
;
Goehlke, N
;
Gonzalez, JG
;
Goswami, S
;
Grant, D
;
Gray, SJ
;
Grégoire, T
;
Griffin, S
;
Griswold, S
;
Günther, C
;
Gutjahr, P
;
Haack, C
;
Hallgren, A
;
Halliday, R
;
Halve, L
;
Halzen, F
;
Hamdaoui, H
;
Minh, M Ha
;
Hanson, K
;
Hardin, J
;
Harnisch, AA
;
Hatch, P
;
Haungs, A
;
Helbing, K
;
Hellrung, J
;
Henningsen, F
;
Heuermann, L
;
Hickford, S
;
Hidvegi, A
;
Hill, C
;
Hill, GC
;
Hoffman, KD
;
Hoshina, K
;
Hou, W
;
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
;
Kelley, JL
;
Kheirandish, A
;
Kin, K
;
Kiryluk, J
;
Klein, SR
;
Kochocki, A
;
Koirala, R
;
Kolanoski, H
;
Kontrimas, T
;
Köpke, L
;
Kopper, C
;
Koskinen, DJ
;
Koundal, P
;
Kovacevich, M
;
Kowalski, M
;
Kozynets, T
;
Kruiswijk, K
;
Krupczak, E
;
Kumar, A
;
Kun, E
;
Kurahashi, N
;
Lad, N
;
Gualda, C Lagunas
;
Lamoureux, M
;
Larson, MJ
;
Lauber, F
;
Lazar, JP
;
Lee, JW
;
DeHolton, K Leonard
;
Leszczyńska, A
;
Lincetto, M
;
Liu, QR
;
Liubarska, M
;
Lohfink, E
;
Love, C
;
Mariscal, CJ Lozano
;
Lu, L
;
Lucarelli, F
;
Ludwig, A
;
Luszczak, W
;
Lyu, Y
;
Y., W
;
Madsen, J
;
Mahn, KBM
;
Makino, Y
;
Mancina, S
;
Sainte, W Marie
;
Mariş, IC
;
Marka, S
;
Marka, Z
;
Marsee, M
;
Martinez-Soler, I
;
Maruyama, R
;
Mayhew, F
;
McElroy, T
;
McNally, F
;
Mead, JV
;
Meagher, K
;
Mechbal, S
;
Medina, A
;
Meier, M
;
Meighen-Berger, S
;
Merckx, Y
;
Merten, L
;
Micallef, J
;
Mockler, D
;
Montaruli, T
;
Moore, RW
;
Morii, Y
;
Morse, R
;
Moulai, M
;
Mukherjee, T
;
Naab, R
;
Nagai, R
;
Naumann, U
;
Nayerhoda, A
;
Necker, J
;
Neumann, M
;
Niederhausen, H
;
Nisa, MU
;
Noell, A
;
Nowicki, SC
;
Pollmann, A Obertacke
;
Oehler, M
;
Oeyen, B
;
Olivas, A
;
Orsoe, R
;
Osborn, J
;
O’Sullivan, E
;
Pandya, H
;
Pankova, DV
;
Park, N
;
Parker, GK
;
Paudel, EN
;
Paul, L
;
de los Heros, C Pérez
;
Peterson, J
;
Philippen, S
;
Pieper, S
;
Pizzuto, A
;
Plum, M
;
Popovych, Y
;
Rodriguez, M Prado
;
Pries, B
;
Procter-Murphy, R
;
Przybylski, GT
;
Raab, C
;
Rack-Helleis, J
;
Rawlins, K
;
Rechav, Z
;
Rehman, A
;
Reichherzer, P
;
Renzi, G
;
Resconi, E
;
Reusch, S
;
Rhode, W
;
Richman, M
;
Riedel, B
;
Roberts, EJ
;
Robertson, S
;
Rodan, S
;
Roellinghoff, G
;
Rongen, M
;
Rott, C
;
Ruhe, T
;
Ruohan, L
;
Ryckbosch, D
;
Cantu, D Rysewyk
;
Safa, I
;
Saffer, J
;
Salazar-Gallegos, D
;
Sampathkumar, P
;
Herrera, SE Sanchez
;
Sandrock, A
;
Santander, M
;
Sarkar, S
;
Sarkar, S
;
Savelberg, J
;
Savina, P
;
Schaufel, M
;
Schieler, H
;
Schindler, S
;
Schlüter, B
;
Schmidt, T
;
Schneider, J
;
Schröder, FG
;
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
;
Søgaard, A
;
Soldin, D
;
Spannfellner, C
;
Spiczak, GM
;
Spiering, C
;
Stamatikos, M
;
Stanev, T
;
Stein, R
;
Stezelberger, T
;
Stürwald, T
;
Stuttard, T
;
Sullivan, GW
;
Taboada, I
;
Ter-Antonyan, S
;
Thompson, WG
;
Thwaites, J
;
Tilav, S
;
Tollefson, K
;
Tönnis, C
;
Toscano, S
;
Tosi, D
;
Trettin, A
;
Tung, CF
;
Turcotte, R
;
Twagirayezu, JP
;
Ty, B
;
Elorrieta, MA Unland
;
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
;
Watson, TB
;
Weaver, C
;
Weigel, P
;
Weindl, A
;
Weldert, J
;
Wendt, C
;
Werthebach, J
;
Weyrauch, M
;
Whitehorn, N
;
Wiebusch, CH
;
Willey, N
;
Williams, DR
;
Wolf, M
;
Wrede, G
;
Wulff, J
;
Xu, XW
;
Yanez, JP
;
Yildizci, E
;
Yoshida, S
;
Yu, S
;
Yuan, T
;
Zhang, Z
;
Zhelnin, P
;
Collaboration, IceCube
UC Berkeley Previously Published Works
(2023)
The understanding of novae, the thermonuclear eruptions on the surfaces of white dwarf stars in binaries, has recently undergone a major paradigm shift. Though the bolometric luminosity of novae was long thought to arise directly from photons supplied by the thermonuclear runaway, recent gigaelectronvolt (GeV) gamma-ray observations have supported the notion that a significant portion of the luminosity could come from radiative shocks. More recently, observations of novae have lent evidence that these shocks are acceleration sites for hadrons for at least some types of novae. In this scenario, a flux of neutrinos may accompany the observed gamma rays. As the gamma rays from most novae have only been observed up to a few GeV, novae have previously not been considered as targets for neutrino telescopes, which are most sensitive at and above teraelectronvolt (TeV) energies. Here, we present the first search for neutrinos from novae with energies between a few GeV and 10 TeV using IceCube-DeepCore, a densely instrumented region of the IceCube Neutrino Observatory with a reduced energy threshold. We search both for a correlation between gamma-ray and neutrino emission as well as between optical and neutrino emission from novae. We find no evidence for neutrino emission from the novae considered in this analysis and set upper limits for all gamma-ray detected novae.
Article
Peer Reviewed
Constraints on Populations of Neutrino Sources from Searches in the Directions of IceCube Neutrino Alerts
Abbasi, R
;
Ackermann, M
;
Adams, J
;
Aggarwal, N
;
Aguilar, JA
;
Ahlers, M
;
Alameddine, JM
;
Alves, AA
;
Amin, NM
;
Andeen, K
;
Anderson, T
;
Anton, G
;
Argüelles, C
;
Ashida, Y
;
Athanasiadou, S
;
Axani, SN
;
Bai, X
;
V., A Balagopal
;
Baricevic, M
;
Barwick, SW
;
Basu, V
;
Bay, R
;
Beatty, JJ
;
Becker, K-H
;
Tjus, J Becker
;
Beise, J
;
Bellenghi, C
;
Benda, S
;
BenZvi, S
;
Berley, D
;
Bernardini, E
;
Besson, DZ
;
Binder, G
;
Bindig, D
;
Blaufuss, E
;
Blot, S
;
Bontempo, F
;
Book, JY
;
Borowka, J
;
Meneguolo, C Boscolo
;
Böser, S
;
Botner, O
;
Böttcher, J
;
Bourbeau, E
;
Braun, J
;
Brinson, B
;
Brostean-Kaiser, J
;
Burley, RT
;
Busse, RS
;
Campana, MA
;
Carnie-Bronca, EG
;
Chen, C
;
Chen, Z
;
Chirkin, D
;
Choi, K
;
Clark, BA
;
Classen, L
;
Coleman, A
;
Collin, GH
;
Connolly, A
;
Conrad, JM
;
Coppin, P
;
Correa, P
;
Countryman, S
;
Cowen, DF
;
Cross, R
;
Dappen, C
;
Dave, P
;
De Clercq, C
;
DeLaunay, JJ
;
López, D Delgado
;
Dembinski, H
;
Deoskar, K
;
Desai, A
;
Desiati, P
;
de Vries, KD
;
de Wasseige, G
;
DeYoung, T
;
Diaz, A
;
Díaz-Vélez, JC
;
Dittmer, M
;
Dujmovic, H
;
DuVernois, MA
;
Ehrhardt, T
;
Eller, P
;
Engel, R
;
Erpenbeck, H
;
Evans, J
;
Evenson, PA
;
Fan, KL
;
Fazely, AR
;
Fedynitch, A
;
Feigl, N
;
Fiedlschuster, S
;
Fienberg, AT
;
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
;
Goehlke, N
;
Gonzalez, JG
;
Goswami, S
;
Grant, D
;
Gray, SJ
;
Grégoire, T
;
Griswold, S
;
Günther, C
;
Gutjahr, P
;
Haack, C
;
Hallgren, A
;
Halliday, R
;
Halve, L
;
Halzen, F
;
Hamdaoui, H
;
Minh, M Ha
;
Hanson, K
;
Hardin, J
;
Harnisch, AA
;
Hatch, P
;
Haungs, A
;
Helbing, K
;
Hellrung, J
;
Henningsen, F
;
Heuermann, L
;
Hickford, S
;
Hidvegi, A
;
Hill, C
;
Hill, GC
;
Hoffman, KD
;
Hoshina, K
;
Hou, W
;
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
;
Kelley, JL
;
Kheirandish, A
;
Kin, K
;
Kiryluk, J
;
Klein, SR
;
Kochocki, A
;
Koirala, R
;
Kolanoski, H
;
Kontrimas, T
;
Köpke, L
;
Kopper, C
;
Koskinen, DJ
;
Koundal, P
;
Kovacevich, M
;
Kowalski, M
;
Kozynets, T
;
Krupczak, E
;
Kun, E
;
Kurahashi, N
;
Lad, N
;
Gualda, C Lagunas
;
Larson, MJ
;
Lauber, F
;
Lazar, JP
;
Lee, JW
;
Leonard, K
;
Leszczyńska, A
;
Lincetto, M
;
Liu, QR
;
Liubarska, M
;
Lohfink, E
;
Love, C
;
Mariscal, CJ Lozano
;
Lu, L
;
Lucarelli, F
;
Ludwig, A
;
Luszczak, W
;
Lyu, Y
;
Y., W
;
Madsen, J
;
Mahn, KBM
;
Makino, Y
;
Mancina, S
;
Sainte, W Marie
;
Mariş, IC
;
Marka, S
;
Marka, Z
;
Marsee, M
;
Martinez-Soler, I
;
Maruyama, R
;
McElroy, T
;
McNally, F
;
Mead, JV
;
Meagher, K
;
Mechbal, S
;
Medina, A
;
Meier, M
;
Meighen-Berger, S
;
Merckx, Y
;
Micallef, J
;
Mockler, D
;
Montaruli, T
;
Moore, RW
;
Morse, R
;
Moulai, M
;
Mukherjee, T
;
Naab, R
;
Nagai, R
;
Naumann, U
;
Nayerhoda, A
;
Necker, J
;
Neumann, M
;
Niederhausen, H
;
Nisa, MU
;
Noell, A
;
Nowicki, SC
;
Pollmann, A Obertacke
;
Oehler, M
;
Oeyen, B
;
Olivas, A
;
Orsoe, R
;
Osborn, J
;
O’Sullivan, E
;
Pandya, H
;
Pankova, DV
;
Park, N
;
Parker, GK
;
Paudel, EN
;
Paul, L
;
de los Heros, C Pérez
;
Peters, L
;
Peterson, J
;
Philippen, S
;
Pieper, S
;
Pizzuto, A
;
Plum, M
;
Popovych, Y
;
Porcelli, A
;
Rodriguez, M Prado
;
Pries, B
;
Procter-Murphy, R
;
Przybylski, GT
;
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, EJ
;
Robertson, S
;
Rodan, S
;
Roellinghoff, G
;
Rongen, M
;
Rott, C
;
Ruhe, T
;
Ruohan, L
;
Ryckbosch, D
;
Cantu, D Rysewyk
;
Safa, I
;
Saffer, J
;
Salazar-Gallegos, D
;
Sampathkumar, P
;
Herrera, SE Sanchez
;
Sandrock, A
;
Santander, M
;
Sarkar, S
;
Sarkar, S
;
Savelberg, J
;
Schaufel, M
;
Schieler, H
;
Schindler, S
;
Schlueter, B
;
Schmidt, T
;
Schneider, J
;
Schröder, FG
;
Schumacher, L
;
Schwefer, G
;
Sclafani, S
;
Seunarine, S
;
Sharma, A
;
Shefali, S
;
Shimizu, N
;
Silva, M
;
Skrzypek, B
;
Smithers, B
;
Snihur, R
;
Soedingrekso, J
;
Søgaard, A
;
Soldin, D
;
Spannfellner, C
;
Spiczak, GM
;
Spiering, C
;
Stamatikos, M
;
Stanev, T
;
Stein, R
;
Stezelberger, T
;
Stürwald, T
;
Stuttard, T
;
Sullivan, GW
;
Taboada, I
;
Ter-Antonyan, S
;
Thompson, WG
;
Thwaites, J
;
Tilav, S
;
Tollefson, K
;
Tönnis, C
;
Toscano, S
;
Tosi, D
;
Trettin, A
;
Tung, CF
;
Turcotte, R
;
Twagirayezu, JP
;
Ty, B
;
Elorrieta, MA Unland
;
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, TB
;
Weaver, C
;
Weigel, P
;
Weindl, A
;
Weldert, J
;
Wendt, C
;
Werthebach, J
;
Weyrauch, M
;
Whitehorn, N
;
Wiebusch, CH
;
Willey, N
;
Williams, DR
;
Wolf, M
;
Wrede, G
;
Wulff, J
;
Xu, XW
;
Yanez, JP
;
Yildizci, E
;
Yoshida, S
;
Yu, S
;
Yuan, T
;
Zhang, Z
;
Zhelnin, P
;
Collaboration, IceCube
UC Berkeley Previously Published Works
(2023)
Beginning in 2016, the IceCube Neutrino Observatory has sent out alerts in real time containing the information of high-energy (E ≳ 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 E −2.5 neutrino spectrum, and number densities that follow star formation rates, the population of sources has to be more numerous than 7 × 10−9 Mpc−3. This number changes to 3 × 10−7 Mpc−3 if number densities instead have no cosmic evolution.
Article
Peer Reviewed
Limits on Neutrino Emission from GRB 221009A from MeV to PeV Using the IceCube Neutrino Observatory
Abbasi, R
;
Ackermann, M
;
Adams, J
;
Agarwalla, SK
;
Aggarwal, N
;
Aguilar, JA
;
Ahlers, M
;
Alameddine, JM
;
Amin, NM
;
Andeen, K
;
Anton, G
;
Argüelles, C
;
Ashida, Y
;
Athanasiadou, S
;
Axani, SN
;
Bai, X
;
V., A Balagopal
;
Baricevic, M
;
Barwick, SW
;
Basu, V
;
Bay, R
;
Beatty, JJ
;
Becker, K-H
;
Tjus, J Becker
;
Beise, J
;
Bellenghi, C
;
BenZvi, S
;
Berley, D
;
Bernardini, E
;
Besson, DZ
;
Binder, G
;
Bindig, D
;
Blaufuss, E
;
Blot, S
;
Bontempo, F
;
Book, JY
;
Borowka, J
;
Meneguolo, C Boscolo
;
Böser, S
;
Botner, O
;
Böttcher, J
;
Bourbeau, E
;
Braun, J
;
Brinson, B
;
Brostean-Kaiser, J
;
Burley, RT
;
Busse, RS
;
Campana, MA
;
Carloni, K
;
Carnie-Bronca, EG
;
Chen, C
;
Chen, Z
;
Chirkin, D
;
Choi, S
;
Clark, BA
;
Classen, L
;
Coleman, A
;
Collin, GH
;
Connolly, A
;
Conrad, JM
;
Coppin, P
;
Correa, P
;
Countryman, S
;
Cowen, DF
;
Dappen, C
;
Dave, P
;
De Clercq, C
;
DeLaunay, JJ
;
López, D Delgado
;
Dembinski, H
;
Deoskar, K
;
Desai, A
;
Desiati, P
;
de Vries, KD
;
de Wasseige, G
;
DeYoung, T
;
Diaz, A
;
Díaz-Vélez, JC
;
Dittmer, M
;
Domi, A
;
Dujmovic, H
;
DuVernois, MA
;
Ehrhardt, T
;
Eller, P
;
Engel, R
;
Erpenbeck, H
;
Evans, J
;
Evenson, PA
;
Fan, KL
;
Fazely, AR
;
Fedynitch, A
;
Feigl, N
;
Fiedlschuster, S
;
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
;
Goehlke, N
;
Gonzalez, JG
;
Goswami, S
;
Grant, D
;
Gray, SJ
;
Griffin, S
;
Griswold, S
;
Günther, C
;
Gutjahr, P
;
Haack, C
;
Hallgren, A
;
Halliday, R
;
Halve, L
;
Halzen, F
;
Hamdaoui, H
;
Minh, M Ha
;
Hanson, K
;
Hardin, J
;
Harnisch, AA
;
Hatch, P
;
Haungs, A
;
Helbing, K
;
Hellrung, J
;
Henningsen, F
;
Heuermann, L
;
Hickford, S
;
Hidvegi, A
;
Hill, C
;
Hill, GC
;
Hoffman, KD
;
Hoshina, K
;
Hou, W
;
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
;
Kelley, JL
;
Kheirandish, A
;
Kin, K
;
Kiryluk, J
;
Klein, SR
;
Kochocki, A
;
Koirala, R
;
Kolanoski, H
;
Kontrimas, T
;
Köpke, L
;
Kopper, C
;
Koskinen, DJ
;
Koundal, P
;
Kovacevich, M
;
Kowalski, M
;
Kozynets, T
;
Kruiswijk, K
;
Krupczak, E
;
Kumar, A
;
Kun, E
;
Kurahashi, N
;
Lad, N
;
Gualda, C Lagunas
;
Lamoureux, M
;
Larson, MJ
;
Lauber, F
;
Lazar, JP
;
Lee, JW
;
DeHolton, K Leonard
;
Leszczyńska, A
;
Lincetto, M
;
Liu, QR
;
Liubarska, M
;
Lohfink, E
;
Love, C
;
Mariscal, CJ Lozano
;
Lu, L
;
Lucarelli, F
;
Ludwig, A
;
Luszczak, W
;
Lyu, Y
;
Y., W
;
Madsen, J
;
Mahn, KBM
;
Makino, Y
;
Mancina, S
;
Sainte, W Marie
;
Mariş, IC
;
Marka, S
;
Marka, Z
;
Marsee, M
;
Martinez-Soler, I
;
Maruyama, R
;
Mayhew, F
;
McElroy, T
;
McNally, F
;
Mead, JV
;
Meagher, K
;
Mechbal, S
;
Medina, A
;
Meier, M
;
Meighen-Berger, S
;
Merckx, Y
;
Merten, L
;
Micallef, J
;
Mockler, D
;
Montaruli, T
;
Moore, RW
;
Morii, Y
;
Morse, R
;
Moulai, M
;
Mukherjee, T
;
Naab, R
;
Nagai, R
;
Naumann, U
;
Necker, J
;
Neumann, M
;
Niederhausen, H
;
Nisa, MU
;
Noell, A
;
Nowicki, SC
;
Pollmann, A Obertacke
;
Oehler, M
;
Oeyen, B
;
Olivas, A
;
Orsoe, R
;
Osborn, J
;
O’Sullivan, E
;
Pandya, H
;
Park, N
;
Parker, GK
;
Paudel, EN
;
Paul, L
;
de los Heros, C Pérez
;
Peterson, J
;
Philippen, S
;
Pieper, S
;
Pizzuto, A
;
Plum, M
;
Popovych, Y
;
Rodriguez, M Prado
;
Pries, B
;
Procter-Murphy, R
;
Przybylski, GT
;
Raab, C
;
Rack-Helleis, J
;
Rawlins, K
;
Rechav, Z
;
Rehman, A
;
Reichherzer, P
;
Renzi, G
;
Resconi, E
;
Reusch, S
;
Rhode, W
;
Richman, M
;
Riedel, B
;
Roberts, EJ
;
Robertson, S
;
Rodan, S
;
Roellinghoff, G
;
Rongen, M
;
Rott, C
;
Ruhe, T
;
Ruohan, L
;
Ryckbosch, D
;
Athanasiadou, S
;
Safa, I
;
Saffer, J
;
Salazar-Gallegos, D
;
Sampathkumar, P
;
Herrera, SE Sanchez
;
Sandrock, A
;
Santander, M
;
Sarkar, S
;
Sarkar, S
;
Savelberg, J
;
Savina, P
;
Schaufel, M
;
Schieler, H
;
Schindler, S
;
Schlüter, B
;
Schmidt, T
;
Schneider, J
;
Schröder, FG
;
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
;
Søgaard, A
;
Soldin, D
;
Sommani, G
;
Spannfellner, C
;
Spiczak, GM
;
Spiering, C
;
Stamatikos, M
;
Stanev, T
;
Stein, R
;
Stezelberger, T
;
Stürwald, T
;
Stuttard, T
;
Sullivan, GW
;
Taboada, I
;
Ter-Antonyan, S
;
Thompson, WG
;
Thwaites, J
;
Tilav, S
;
Tollefson, K
;
Tönnis, C
;
Toscano, S
;
Tosi, D
;
Trettin, A
;
Tung, CF
;
Turcotte, R
;
Twagirayezu, JP
;
Ty, B
;
Elorrieta, MA Unland
;
Upshaw, K
;
Valtonen-Mattila, N
;
Vandenbroucke, J
;
van Eijndhoven, N
;
Vannerom, D
;
van Santen, J
;
Vara, J
;
Veitch-Michaelis, J
;
Venugopal, M
;
Verpoest, S
;
Veske, D
;
Walck, C
;
Watson, TB
;
Weaver, C
;
Weigel, P
;
Weindl, A
;
Weldert, J
;
Wendt, C
;
Werthebach, J
;
Weyrauch, M
;
Whitehorn, N
;
Wiebusch, CH
;
Willey, N
;
Williams, DR
;
Wolf, M
;
Wrede, G
;
Wulff, J
;
Xu, XW
;
Yanez, JP
;
Yildizci, E
;
Yoshida, S
;
Yu, F
;
Yu, S
;
Yuan, T
;
Zhang, Z
;
Zhelnin, P
UC Berkeley Previously Published Works
(2023)
Gamma-ray bursts (GRBs) have long been considered a possible source of high-energy neutrinos. While no correlations have yet been detected between high-energy neutrinos and GRBs, the recent observation of GRB 221009A—the brightest GRB observed by Fermi-GBM to date and the first one to be observed above an energy of 10 TeV—provides a unique opportunity to test for hadronic emission. In this paper, we leverage the wide energy range of the IceCube Neutrino Observatory to search for neutrinos from GRB 221009A. We find no significant deviation from background expectation across event samples ranging from MeV to PeV energies, placing stringent upper limits on the neutrino emission from this source.
Article
Peer Reviewed
Search for Correlations of High-energy Neutrinos Detected in IceCube with Radio-bright AGN and Gamma-Ray Emission from Blazars
Abbasi, R
;
Ackermann, M
;
Adams, J
;
Agarwalla, SK
;
Aguilar, JA
;
Ahlers, M
;
Alameddine, JM
;
Amin, NM
;
Andeen, K
;
Anton, G
;
Argüelles, C
;
Ashida, Y
;
Athanasiadou, S
;
Axani, SN
;
Bai, X
;
V., A Balagopal
;
Baricevic, M
;
Barwick, SW
;
Basu, V
;
Bay, R
;
Beatty, JJ
;
Becker, K-H
;
Tjus, J Becker
;
Beise, J
;
Bellenghi, C
;
Benning, C
;
BenZvi, S
;
Berley, D
;
Bernardini, E
;
Besson, DZ
;
Binder, G
;
Blaufuss, E
;
Blot, S
;
Bontempo, F
;
Book, JY
;
Meneguolo, C Boscolo
;
Böser, S
;
Botner, O
;
Böttcher, J
;
Bourbeau, E
;
Braun, J
;
Brinson, B
;
Brostean-Kaiser, J
;
Burley, RT
;
Busse, RS
;
Butterfield, D
;
Campana, MA
;
Carloni, K
;
Carnie-Bronca, EG
;
Chattopadhyay, S
;
Chau, N
;
Chen, C
;
Chen, Z
;
Chirkin, D
;
Choi, S
;
Clark, BA
;
Classen, L
;
Coleman, A
;
Collin, GH
;
Connolly, A
;
Conrad, JM
;
Coppin, P
;
Correa, P
;
Countryman, S
;
Cowen, DF
;
Dave, P
;
De Clercq, C
;
DeLaunay, JJ
;
Delgado, D
;
Dembinski, H
;
Deng, S
;
Deoskar, K
;
Desai, A
;
Desiati, P
;
de Vries, KD
;
de Wasseige, G
;
DeYoung, T
;
Diaz, A
;
Díaz-Vélez, JC
;
Dittmer, M
;
Domi, A
;
Dujmovic, H
;
DuVernois, MA
;
Ehrhardt, T
;
Eller, P
;
Mentawi, S El
;
Engel, R
;
Erpenbeck, H
;
Evans, J
;
Evenson, PA
;
Fan, KL
;
Fang, K
;
Farrag, K
;
Fazely, AR
;
Fedynitch, A
;
Feigl, N
;
Fiedlschuster, S
;
Finley, C
;
Fischer, L
;
Fox, D
;
Franckowiak, A
;
Friedman, E
;
Fritz, A
;
Fürst, P
;
Gaisser, TK
;
Gallagher, J
;
Ganster, E
;
Garcia, A
;
Gerhardt, L
;
Ghadimi, A
;
Glaser, C
;
Glauch, T
;
Glüsenkamp, T
;
Goehlke, N
;
Gonzalez, JG
;
Goswami, S
;
Grant, D
;
Gray, SJ
;
Gries, O
;
Griffin, S
;
Griswold, S
;
Günther, C
;
Gutjahr, P
;
Haack, C
;
Hallgren, A
;
Halliday, R
;
Halve, L
;
Halzen, F
;
Hamdaoui, H
;
Minh, M Ha
;
Hanson, K
;
Hardin, J
;
Harnisch, AA
;
Hatch, P
;
Haungs, A
;
Helbing, K
;
Hellrung, J
;
Henningsen, F
;
Heuermann, L
;
Heyer, N
;
Hickford, S
;
Hidvegi, A
;
Hill, C
;
Hill, GC
;
Hoffman, KD
;
Hori, S
;
Hoshina, K
;
Hou, W
;
Huber, T
;
Hultqvist, K
;
Hünnefeld, M
;
Hussain, R
;
Hymon, K
;
In, S
;
Ishihara, A
;
Jacquart, M
;
Janik, O
;
Jansson, M
;
Japaridze, GS
;
Jayakumar, K
;
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
;
Kelley, JL
;
Zathul, A Khatee
;
Kheirandish, A
;
Kiryluk, J
;
Klein, SR
;
Kochocki, A
;
Koirala, R
;
Kolanoski, H
;
Kontrimas, T
;
Köpke, L
;
Kopper, C
;
Koskinen, DJ
;
Koundal, P
;
Kovacevich, M
;
Kowalski, M
;
Kozynets, T
;
Kruiswijk, K
;
Krupczak, E
;
Kumar, A
;
Kun, E
;
Kurahashi, N
;
Lad, N
;
Gualda, C Lagunas
;
Lamoureux, M
;
Larson, MJ
;
Latseva, S
;
Lauber, F
;
Lazar, JP
;
Lee, JW
;
DeHolton, K Leonard
;
Leszczyńska, A
;
Lincetto, M
;
Liu, QR
;
Liubarska, M
;
Lohfink, E
;
Love, C
;
Mariscal, CJ Lozano
;
Lu, L
;
Lucarelli, F
;
Ludwig, A
;
Luszczak, W
;
Lyu, Y
;
Madsen, J
;
Mahn, KBM
;
Makino, Y
;
Manao, E
;
Mancina, S
;
Sainte, W Marie
;
Mariş, IC
;
Marka, S
;
Marka, Z
;
Marsee, M
;
Martinez-Soler, I
;
Maruyama, R
;
Mayhew, F
;
McElroy, T
;
McNally, F
;
Mead, JV
;
Meagher, K
;
Mechbal, S
;
Medina, A
;
Meier, M
;
Merckx, Y
;
Merten, L
;
Micallef, J
;
Montaruli, T
;
Moore, RW
;
Morii, Y
;
Morse, R
;
Moulai, M
;
Mukherjee, T
;
Naab, R
;
Nagai, R
;
Nakos, M
;
Naumann, U
;
Necker, J
;
Neumann, M
;
Niederhausen, H
;
Nisa, MU
;
Noell, A
;
Nowicki, SC
;
Pollmann, A Obertacke
;
O’Dell, V
;
Oehler, M
;
Oeyen, B
;
Olivas, A
;
Orsoe, R
;
Osborn, J
;
O’Sullivan, E
;
Pandya, H
;
Park, N
;
Parker, GK
;
Paudel, EN
;
Paul, L
;
de los Heros, C Pérez
;
Peterson, J
;
Philippen, S
;
Pieper, S
;
Pizzuto, A
;
Plum, M
;
Pontén, A
;
Popovych, Y
;
Rodriguez, M Prado
;
Pries, B
;
Procter-Murphy, R
;
Przybylski, GT
;
Rack-Helleis, J
;
Rawlins, K
;
Rechav, Z
;
Rehman, A
;
Reichherzer, P
;
Renzi, G
;
Resconi, E
;
Reusch, S
;
Rhode, W
;
Richman, M
;
Riedel, B
;
Rifaie, A
;
Roberts, EJ
;
Robertson, S
;
Rodan, S
;
Roellinghoff, G
;
Rongen, M
;
Rott, C
;
Ruhe, T
;
Ruohan, L
;
Ryckbosch, D
;
Safa, I
;
Saffer, J
;
Salazar-Gallegos, D
;
Sampathkumar, P
;
Herrera, SE Sanchez
;
Sandrock, A
;
Santander, M
;
Sarkar, S
;
Sarkar, S
;
Savelberg, J
;
Savina, P
;
Schaufel, M
;
Schieler, H
;
Schindler, S
;
Schlickmann, L
;
Schlüter, B
;
Schlüter, F
;
Schmidt, T
;
Schneider, J
;
Schröder, FG
;
Schumacher, L
;
Schwefer, G
;
Sclafani, S
;
Seckel, D
;
Seikh, M
;
Seunarine, S
;
Shah, R
;
Sharma, A
;
Shefali, S
;
Shimizu, N
;
Silva, M
;
Skrzypek, B
;
Smithers, B
;
Snihur, R
;
Soedingrekso, J
;
Søgaard, A
;
Soldin, D
;
Soldin, P
;
Sommani, G
;
Spannfellner, C
;
Spiczak, GM
;
Spiering, C
;
Stamatikos, M
;
Stanev, T
;
Stezelberger, T
;
Stürwald, T
;
Stuttard, T
;
Sullivan, GW
;
Taboada, I
;
Ter-Antonyan, S
;
Thiesmeyer, M
;
Thompson, WG
;
Thwaites, J
;
Tilav, S
;
Tollefson, K
;
Tönnis, C
;
Toscano, S
;
Tosi, D
;
Trettin, A
;
Tung, CF
;
Turcotte, R
;
Twagirayezu, JP
;
Ty, B
;
Elorrieta, MA Unland
;
Upadhyay, AK
;
Upshaw, K
;
Valtonen-Mattila, N
;
Vandenbroucke, J
;
van Eijndhoven, N
;
Vannerom, D
;
van Santen, J
;
Vara, J
;
Veitch-Michaelis, J
;
Venugopal, M
;
Vereecken, M
;
Verpoest, S
;
Veske, D
;
Walck, C
;
Watson, TB
;
Weaver, C
;
Weigel, P
;
Weindl, A
;
Weldert, J
;
Wendt, C
;
Werthebach, J
;
Weyrauch, M
;
Whitehorn, N
;
Wiebusch, CH
;
Willey, N
;
Williams, DR
;
Wolf, A
;
Wolf, M
;
Wrede, G
;
Xu, XW
;
Yanez, JP
;
Yildizci, E
;
Yoshida, S
;
Young, R
;
Yu, F
;
Yu, S
;
Yuan, T
;
Zhang, Z
;
Zhelnin, P
;
Collaboration, IceCube
UC Berkeley Previously Published Works
(2023)
The IceCube Neutrino Observatory sends realtime neutrino alerts with a high probability of being astrophysical in origin. We present a new method to correlate these events and possible candidate sources using 2089 blazars from the Fermi-LAT 4LAC-DR2 catalog and with 3413 active galactic nuclei (AGNs) from the Radio Fundamental Catalog. No statistically significant neutrino emission was found in any of the catalog searches. The result suggests that a small fraction, <1%, of the studied AGNs emit neutrinos that pass the alert criteria, and is compatible with prior evidence for neutrino emission presented by IceCube and other authors from sources such as TXS 0506 + 056 and PKS 1502 + 106. We also present cross-checks to other analyses that claim a significant correlation using similar data samples.
Article
Peer Reviewed
Constraining High-energy Neutrino Emission from Supernovae with IceCube
Abbasi, R
;
Ackermann, M
;
Adams, J
;
Agarwalla, SK
;
Aguilar, JA
;
Ahlers, M
;
Alameddine, JM
;
Amin, NM
;
Andeen, K
;
Anton, G
;
Argüelles, C
;
Ashida, Y
;
Athanasiadou, S
;
Axani, SN
;
Bai, X
;
V., A Balagopal
;
Baricevic, M
;
Barwick, SW
;
Basu, V
;
Bay, R
;
Beatty, JJ
;
Becker, K-H
;
Tjus, J Becker
;
Beise, J
;
Bellenghi, C
;
BenZvi, S
;
Berley, D
;
Bernardini, E
;
Besson, DZ
;
Binder, G
;
Bindig, D
;
Blaufuss, E
;
Blot, S
;
Bontempo, F
;
Book, JY
;
Meneguolo, C Boscolo
;
Böser, S
;
Botner, O
;
Böttcher, J
;
Bourbeau, E
;
Braun, J
;
Brinson, B
;
Brostean-Kaiser, J
;
Burley, RT
;
Busse, RS
;
Butterfield, D
;
Campana, MA
;
Carloni, K
;
Carnie-Bronca, EG
;
Chattopadhyay, S
;
Chen, C
;
Chen, Z
;
Chirkin, D
;
Choi, S
;
Clark, BA
;
Classen, L
;
Coleman, A
;
Collin, GH
;
Connolly, A
;
Conrad, JM
;
Coppin, P
;
Correa, P
;
Countryman, S
;
Cowen, DF
;
Dave, P
;
De Clercq, C
;
DeLaunay, JJ
;
López, D Delgado
;
Dembinski, H
;
Deoskar, K
;
Desai, A
;
Desiati, P
;
de Vries, KD
;
de Wasseige, G
;
DeYoung, T
;
Diaz, A
;
Díaz-Vélez, JC
;
Dittmer, M
;
Domi, A
;
Dujmovic, H
;
DuVernois, MA
;
Ehrhardt, T
;
Eller, P
;
Engel, R
;
Erpenbeck, H
;
Evans, J
;
Evenson, PA
;
Fan, KL
;
Fang, K
;
Fazely, AR
;
Fedynitch, A
;
Feigl, N
;
Fiedlschuster, S
;
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
;
Goehlke, N
;
Gonzalez, JG
;
Goswami, S
;
Grant, D
;
Gray, SJ
;
Griffin, S
;
Griswold, S
;
Günther, C
;
Gutjahr, P
;
Haack, C
;
Hallgren, A
;
Halliday, R
;
Halve, L
;
Halzen, F
;
Hamdaoui, H
;
Minh, M Ha
;
Hanson, K
;
Hardin, J
;
Harnisch, AA
;
Hatch, P
;
Haungs, A
;
Helbing, K
;
Hellrung, J
;
Henningsen, F
;
Heuermann, L
;
Hickford, S
;
Hidvegi, A
;
Hill, C
;
Hill, GC
;
Hoffman, KD
;
Hoshina, K
;
Hou, W
;
Huber, T
;
Hultqvist, K
;
Hünnefeld, M
;
Hussain, R
;
Hymon, K
;
In, S
;
Iovine, N
;
Ishihara, A
;
Jacquart, M
;
Jansson, M
;
Japaridze, GS
;
Jayakumar, K
;
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
;
Kelley, JL
;
Zathul, A Khatee
;
Kheirandish, A
;
Kin, K
;
Kiryluk, J
;
Klein, SR
;
Kochocki, A
;
Koirala, R
;
Kolanoski, H
;
Kontrimas, T
;
Köpke, L
;
Kopper, C
;
Koskinen, DJ
;
Koundal, P
;
Kovacevich, M
;
Kowalski, M
;
Kozynets, T
;
Kruiswijk, K
;
Krupczak, E
;
Kumar, A
;
Kun, E
;
Kurahashi, N
;
Lad, N
;
Gualda, C Lagunas
;
Lamoureux, M
;
Larson, MJ
;
Lauber, F
;
Lazar, JP
;
Lee, JW
;
DeHolton, K Leonard
;
Leszczyńska, A
;
Lincetto, M
;
Liu, QR
;
Liubarska, M
;
Lohfink, E
;
Love, C
;
Mariscal, CJ Lozano
;
Lu, L
;
Lucarelli, F
;
Ludwig, A
;
Luszczak, W
;
Lyu, Y
;
Y., W
;
Madsen, J
;
Mahn, KBM
;
Makino, Y
;
Mancina, S
;
Sainte, W Marie
;
Mariş, IC
;
Marka, S
;
Marka, Z
;
Marsee, M
;
Martinez-Soler, I
;
Maruyama, R
;
Mayhew, F
;
McElroy, T
;
McNally, F
;
Mead, JV
;
Meagher, K
;
Mechbal, S
;
Medina, A
;
Meier, M
;
Meighen-Berger, S
;
Merckx, Y
;
Merten, L
;
Micallef, J
;
Mockler, D
;
Montaruli, T
;
Moore, RW
;
Morii, Y
;
Morse, R
;
Moulai, M
;
Mukherjee, T
;
Naab, R
;
Nagai, R
;
Nakos, M
;
Naumann, U
;
Necker, J
;
Neumann, M
;
Niederhausen, H
;
Nisa, MU
;
Noell, A
;
Nowicki, SC
;
Pollmann, A Obertacke
;
O’Dell, V
;
Oehler, M
;
Oeyen, B
;
Olivas, A
;
Orsoe, R
;
Osborn, J
;
O’Sullivan, E
;
Pandya, H
;
Park, N
;
Parker, GK
;
Paudel, EN
;
Paul, L
;
de los Heros, C Pérez
;
Peterson, J
;
Philippen, S
;
Pieper, S
;
Pizzuto, A
;
Plum, M
;
Popovych, Y
;
Rodriguez, M Prado
;
Pries, B
;
Procter-Murphy, R
;
Przybylski, GT
;
Raab, C
;
Rack-Helleis, J
;
Rawlins, K
;
Rechav, Z
;
Rehman, A
;
Reichherzer, P
;
Renzi, G
;
Resconi, E
;
Reusch, S
;
Rhode, W
;
Richman, M
;
Riedel, B
;
Roberts, EJ
;
Robertson, S
;
Rodan, S
;
Roellinghoff, G
;
Rongen, M
;
Rott, C
;
Ruhe, T
;
Ruohan, L
;
Ryckbosch, D
;
Safa, I
;
Saffer, J
;
Salazar-Gallegos, D
;
Sampathkumar, P
;
Herrera, SE Sanchez
;
Sandrock, A
;
Santander, M
;
Sarkar, S
;
Sarkar, S
;
Savelberg, J
;
Savina, P
;
Schaufel, M
;
Schieler, H
;
Schindler, S
;
Schlüter, B
;
Schmidt, T
;
Schneider, J
;
Schröder, FG
;
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
;
Søgaard, A
;
Soldin, D
;
Sommani, G
;
Spannfellner, C
;
Spiczak, GM
;
Spiering, C
;
Stamatikos, M
;
Stanev, T
;
Stasik, A
;
Stein, R
;
Stezelberger, T
;
Stürwald, T
;
Stuttard, T
;
Sullivan, GW
;
Taboada, I
;
Ter-Antonyan, S
;
Thompson, WG
;
Thwaites, J
;
Tilav, S
;
Tollefson, K
;
Tönnis, C
;
Toscano, S
;
Tosi, D
;
Trettin, A
;
Tung, CF
;
Turcotte, R
;
Twagirayezu, JP
;
Ty, B
;
Elorrieta, MA Unland
;
Upadhyay, AK
;
Upshaw, K
;
Valtonen-Mattila, N
;
Vandenbroucke, J
;
van Eijndhoven, N
;
Vannerom, D
;
van Santen, J
;
Vara, J
;
Veitch-Michaelis, J
;
Venugopal, M
;
Verpoest, S
;
Veske, D
;
Walck, C
;
Watson, TB
;
Weaver, C
;
Weigel, P
;
Weindl, A
;
Weldert, J
;
Wendt, C
;
Werthebach, J
;
Weyrauch, M
;
Whitehorn, N
;
Wiebusch, CH
;
Willey, N
;
Williams, DR
;
Wolf, M
;
Wrede, G
;
Wulff, J
;
Xu, XW
;
Yanez, JP
;
Yildizci, E
;
Yoshida, S
;
Yu, F
;
Yu, S
;
Yuan, T
;
Zhang, Z
;
Zhelnin, P
;
Collaboration, IceCube
UC Berkeley Previously Published Works
(2023)
Core-collapse supernovae are a promising potential high-energy neutrino source class. We test for correlation between seven years of IceCube neutrino data and a catalog containing more than 1000 core-collapse supernovae of types IIn and IIP and a sample of stripped-envelope supernovae. We search both for neutrino emission from individual supernovae as well as for combined emission from the whole supernova sample, through a stacking analysis. No significant spatial or temporal correlation of neutrinos with the cataloged supernovae was found. All scenarios were tested against the background expectation and together yield an overall p-value of 93%; therefore, they show consistency with the background only. The derived upper limits on the total energy emitted in neutrinos are 1.7 × 1048 erg for stripped-envelope supernovae, 2.8 × 1048 erg for type IIP, and 1.3 × 1049 erg for type IIn SNe, the latter disfavoring models with optimistic assumptions for neutrino production in interacting supernovae. We conclude that stripped-envelope supernovae and supernovae of type IIn do not contribute more than 14.6% and 33.9%, respectively, to the diffuse neutrino flux in the energy range of about [ 103-105] GeV, assuming that the neutrino energy spectrum follows a power-law with an index of −2.5. Under the same assumption, we can only constrain the contribution of type IIP SNe to no more than 59.9%. Thus, core-collapse supernovae of types IIn and stripped-envelope supernovae can both be ruled out as the dominant source of the diffuse neutrino flux under the given assumptions.
Article
Peer Reviewed
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, JA
;
Ahlers, M
;
Alameddine, JM
;
Alves, AA
;
Amin, NM
;
Andeen, K
;
Anderson, T
;
Anton, G
;
Argüelles, C
;
Ashida, Y
;
Athanasiadou, S
;
Axani, SN
;
Bai, X
;
V., A Balagopal
;
Baricevic, M
;
Barwick, SW
;
Basu, V
;
Bay, R
;
Beatty, JJ
;
Becker, K-H
;
Tjus, J Becker
;
Beise, J
;
Bellenghi, C
;
Benda, S
;
BenZvi, S
;
Berley, D
;
Bernardini, E
;
Besson, DZ
;
Binder, G
;
Bindig, D
;
Blaufuss, E
;
Blot, S
;
Bontempo, F
;
Book, JY
;
Borowka, J
;
Meneguolo, C Boscolo
;
Böser, S
;
Botner, O
;
Böttcher, J
;
Bourbeau, E
;
Braun, J
;
Brinson, B
;
Brostean-Kaiser, J
;
Burley, RT
;
Busse, RS
;
Campana, MA
;
Carnie-Bronca, EG
;
Chang, YL
;
Chen, C
;
Chen, Z
;
Chirkin, D
;
Choi, K
;
Clark, BA
;
Classen, L
;
Coleman, A
;
Collin, GH
;
Connolly, A
;
Conrad, JM
;
Coppin, P
;
Correa, P
;
Countryman, S
;
Cowen, DF
;
Dappen, C
;
Dave, P
;
De Clercq, C
;
DeLaunay, JJ
;
López, D Delgado
;
Dembinski, H
;
Deoskar, K
;
Desai, A
;
Desiati, P
;
de Vries, KD
;
de Wasseige, G
;
DeYoung, T
;
Diaz, A
;
Díaz-Vélez, JC
;
Dittmer, M
;
Dujmovic, H
;
DuVernois, MA
;
Ehrhardt, T
;
Eller, P
;
Engel, R
;
Erpenbeck, H
;
Evans, J
;
Evenson, PA
;
Fan, KL
;
Fazely, AR
;
Fedynitch, A
;
Feigl, N
;
Fiedlschuster, S
;
Fienberg, AT
;
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
;
Goehlke, N
;
Gonzalez, JG
;
Goswami, S
;
Grant, D
;
Gray, SJ
;
Grégoire, T
;
Griswold, S
;
Günther, C
;
Gutjahr, P
;
Haack, C
;
Hallgren, A
;
Halliday, R
;
Halve, L
;
Halzen, F
;
Hamdaoui, H
;
Minh, M Ha
;
Hanson, K
;
Hardin, J
;
Harnisch, AA
;
Hatch, P
;
Haungs, A
;
Helbing, K
;
Hellrung, J
;
Henningsen, F
;
Heuermann, L
;
Hickford, S
;
Hidvegi, A
;
Hill, C
;
Hill, GC
;
Hoffman, KD
;
Hoshina, K
;
Hou, W
;
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
;
Kelley, JL
;
Kheirandish, A
;
Kin, K
;
Kiryluk, J
;
Klein, SR
;
Kochocki, A
;
Koirala, R
;
Kolanoski, H
;
Kontrimas, T
;
Köpke, L
;
Kopper, C
;
Koskinen, DJ
;
Koundal, P
;
Kovacevich, M
;
Kowalski, M
;
Kozynets, T
;
Kruiswijk, K
;
Krupczak, E
;
Kun, E
;
Kurahashi, N
;
Lad, N
;
Gualda, C Lagunas
;
Lamoureux, M
;
Larson, MJ
;
Lauber, F
;
Lazar, JP
;
Lee, JW
;
DeHolton, K Leonard
;
Leszczyńska, A
;
Lincetto, M
;
Liu, QR
;
Liubarska, M
;
Lohfink, E
;
Love, C
;
Mariscal, CJ Lozano
;
Lu, L
;
Lucarelli, F
;
Ludwig, A
;
Luszczak, W
;
Lyu, Y
;
Y., W
;
Madsen, J
;
Mahn, KBM
;
Makino, Y
;
Mancina, S
;
Sainte, W Marie
;
Mariş, IC
;
Marka, S
;
Marka, Z
;
Marsee, M
;
Martinez-Soler, I
;
Maruyama, R
;
Mayhew, F
;
McElroy, T
;
McNally, F
;
Mead, JV
;
Meagher, K
;
Mechbal, S
;
Medina, A
;
Meier, M
;
Meighen-Berger, S
;
Merckx, Y
;
Micallef, J
;
Mockler, D
;
Montaruli, T
;
Moore, RW
;
Morse, R
;
Moulai, M
;
Mukherjee, T
;
Naab, R
;
Nagai, R
;
Naumann, U
;
Nayerhoda, A
;
Necker, J
;
Neumann, M
;
Niederhausen, H
;
Nisa, MU
;
Noell, A
;
Nowicki, SC
;
Pollmann, A Obertacke
;
Oehler, M
;
Oeyen, B
;
Olivas, A
;
Orsoe, R
;
Osborn, J
;
O’Sullivan, E
;
Pandya, H
;
Pankova, DV
;
Park, N
;
Parker, GK
;
Paudel, EN
;
Paul, L
;
de los Heros, C Pérez
;
Peterson, J
;
Philippen, S
;
Pieper, S
;
Pizzuto, A
;
Plum, M
;
Popovych, Y
;
Porcelli, A
;
Rodriguez, M Prado
;
Pries, B
;
Procter-Murphy, R
;
Przybylski, GT
;
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, EJ
;
Robertson, S
;
Rodan, S
;
Roellinghoff, G
;
Rongen, M
;
Rott, C
;
Ruhe, T
;
Ruohan, L
;
Ryckbosch, D
;
Cantu, D Rysewyk
;
Safa, I
;
Saffer, J
;
Salazar-Gallegos, D
;
Sampathkumar, P
;
Herrera, SE Sanchez
;
Sandrock, A
;
Santander, M
;
Sarkar, S
;
Sarkar, S
;
Savelberg, J
;
Schaufel, M
;
Schieler, H
;
Schindler, S
;
Schlueter, B
;
Schmidt, T
;
Schneider, J
;
Schröder, FG
;
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
;
Søgaard, A
;
Soldin, D
;
Spannfellner, C
;
Spiczak, GM
;
Spiering, C
;
Stamatikos, M
;
Stanev, T
;
Stein, R
;
Stezelberger, T
;
Stürwald, T
;
Stuttard, T
;
Sullivan, GW
;
Taboada, I
;
Ter-Antonyan, S
;
Thompson, WG
;
Thwaites, J
;
Tilav, S
;
Tollefson, K
;
Tönnis, C
;
Toscano, S
;
Tosi, D
;
Trettin, A
;
Tung, CF
;
Turcotte, R
;
Twagirayezu, JP
;
Ty, B
;
Elorrieta, MA Unland
;
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, TB
;
Weaver, C
;
Weigel, P
;
Weindl, A
;
Weldert, J
;
Wendt, C
;
Werthebach, J
;
Weyrauch, M
;
Whitehorn, N
;
Wiebusch, CH
;
Willey, N
;
Williams, DR
;
Wolf, M
;
Wrede, G
;
Wulff, J
;
Xu, DL
;
Xu, XW
;
Yanez, JP
;
Yasutsugu, M
;
Yildizci, E
;
Yoshida, S
;
Yu, S
;
Yuan, T
;
Zhang, Z
;
Zhelnin, P
;
Collaboration, IceCube
UC Berkeley Previously Published Works
(2023)
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.
Article
Peer Reviewed
D-Egg: a dual PMT optical module for IceCube
Abbasi, R
;
Ackermann, M
;
Adams, J
;
Aggarwal, N
;
Aguilar, JA
;
Ahlers, M
;
Alameddine, JM
;
Alves, AA
;
Amin, NM
;
Andeen, K
;
Anderson, T
;
Anton, G
;
Argüelles, C
;
Ashida, Y
;
Athanasiadou, S
;
Axani, SN
;
Bai, X
;
V., A Balagopal
;
Baricevic, M
;
Barwick, SW
;
Basu, V
;
Bay, R
;
Beatty, JJ
;
Becker, K-H
;
Tjus, J Becker
;
Beise, J
;
Bellenghi, C
;
BenZvi, S
;
Berley, D
;
Bernardini, E
;
Besson, DZ
;
Binder, G
;
Bindig, D
;
Blaufuss, E
;
Blot, S
;
Bontempo, F
;
Book, JY
;
Borowka, J
;
Meneguolo, C Boscolo
;
Böser, S
;
Botner, O
;
Böttcher, J
;
Bourbeau, E
;
Braun, J
;
Brinson, B
;
Brostean-Kaiser, J
;
Burley, RT
;
Busse, RS
;
Campana, MA
;
Carnie-Bronca, EG
;
Chen, C
;
Chen, Z
;
Chirkin, D
;
Choi, S
;
Clark, BA
;
Classen, L
;
Coleman, A
;
Collin, GH
;
Connolly, A
;
Conrad, JM
;
Coppin, P
;
Correa, P
;
Countryman, S
;
Cowen, DF
;
Dappen, C
;
Dave, P
;
De Clercq, C
;
DeLaunay, JJ
;
López, D Delgado
;
Dembinski, H
;
Deoskar, K
;
Desai, A
;
Desiati, P
;
de Vries, KD
;
de Wasseige, G
;
DeYoung, T
;
Diaz, A
;
Díaz-Vélez, JC
;
Dittmer, M
;
Dujmovic, H
;
DuVernois, MA
;
Ehrhardt, T
;
Eller, P
;
Engel, R
;
Erpenbeck, H
;
Evans, J
;
Evenson, PA
;
Fan, KL
;
Fazely, AR
;
Fedynitch, A
;
Feigl, N
;
Fiedlschuster, S
;
Fienberg, AT
;
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
;
Goehlke, N
;
Gonzalez, JG
;
Goswami, S
;
Grant, D
;
Gray, SJ
;
Grégoire, T
;
Griffin, S
;
Griswold, S
;
Günther, C
;
Gutjahr, P
;
Haack, C
;
Hallgren, A
;
Halliday, R
;
Halve, L
;
Halzen, F
;
Hamdaoui, H
;
Minh, M Ha
;
Hanson, K
;
Hardin, J
;
Harnisch, AA
;
Hatch, P
;
Haungs, A
;
Helbing, K
;
Hellrung, J
;
Henningsen, F
;
Heuermann, L
;
Hickford, S
;
Hidvegi, A
;
Hill, C
;
Hill, GC
;
Hoffman, KD
;
Hoshina, K
;
Hou, W
;
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
;
Kelley, JL
;
Kheirandish, A
;
Kin, K
;
Kiryluk, J
;
Klein, SR
;
Kochocki, A
;
Koirala, R
;
Kolanoski, H
;
Kontrimas, T
;
Köpke, L
;
Kopper, C
;
Koskinen, DJ
;
Koundal, P
;
Kovacevich, M
;
Kowalski, M
;
Kozynets, T
;
Kruiswijk, K
;
Krupczak, E
;
Kumar, A
;
Kun, E
;
Kurahashi, N
;
Lad, N
;
Gualda, C Lagunas
;
Lamoureux, M
;
Larson, MJ
;
Lauber, F
;
Lazar, JP
;
Lee, JW
;
DeHolton, K Leonard
;
Leszczyńska, A
;
Lincetto, M
;
Liu, QR
;
Liubarska, M
;
Lohfink, E
;
Love, C
;
Mariscal, CJ Lozano
;
Lu, L
;
Lucarelli, F
;
Ludwig, A
;
Luszczak, W
;
Lyu, Y
;
Ma, WY
;
Madsen, J
;
Mahn, KBM
;
Makino, Y
;
Mancina, S
;
Sainte, W Marie
;
Mariş, IC
;
Marka, S
;
Marka, Z
;
Marsee, M
;
Martinez-Soler, I
;
Maruyama, R
;
Mayhew, F
;
McElroy, T
;
McNally, F
;
Mead, JV
;
Meagher, K
;
Mechbal, S
;
Medina, A
;
Meier, M
;
Meighen-Berger, S
;
Merckx, Y
;
Merten, L
;
Meures, T
;
Micallef, J
;
Mockler, D
;
Montaruli, T
;
Moore, RW
;
Morii, Y
;
Morse, R
;
Moulai, M
;
Mukherjee, T
;
Naab, R
;
Nagai, R
;
Naumann, U
;
Nayerhoda, A
;
Necker, J
;
Neumann, M
;
Niederhausen, H
;
Nisa, MU
;
Noell, A
;
Nowicki, SC
;
Pollmann, A Obertacke
;
Oehler, M
;
Oeyen, B
;
Olivas, A
;
Orsoe, R
;
Osborn, J
;
O'Sullivan, E
;
Pandya, H
;
Pankova, DV
;
Park, N
;
Parker, GK
;
Paudel, EN
;
Paul, L
;
de los Heros, C Pérez
;
Peterson, J
;
Philippen, S
;
Pieper, S
;
Pizzuto, A
;
Plum, M
;
Popovych, Y
;
Rodriguez, M Prado
;
Pries, B
;
Procter-Murphy, R
;
Przybylski, GT
;
Raab, C
;
Rack-Helleis, J
;
Rawlins, K
;
Rechav, Z
;
Rehman, A
;
Reichherzer, P
;
Renzi, G
;
Resconi, E
;
Reusch, S
;
Rhode, W
;
Richman, M
;
Riedel, B
;
Roberts, EJ
;
Robertson, S
;
Rodan, S
;
Roellinghoff, G
;
Rongen, M
;
Rott, C
;
Ruhe, T
;
Ruohan, L
;
Ryckbosch, D
;
Cantu, D Rysewyk
;
Athanasiadou, S
;
Safa, I
;
Saffer, J
;
Salazar-Gallegos, D
;
Sampathkumar, P
;
Herrera, SE Sanchez
;
Sandrock, A
;
Sandstrom, P
;
Santander, M
;
Sarkar, S
;
Sarkar, S
;
Savelberg, J
;
Savina, P
;
Schaufel, M
;
Schieler, H
;
Schindler, S
;
Schlüter, B
;
Schmidt, T
;
Schneider, J
;
Schröder, FG
;
Schumacher, L
;
Schwefer, G
;
Sclafani, S
;
Seckel, D
;
Seunarine, S
;
Sharma, A
;
Shefali, S
;
Shimizu, N
;
Shimizu, S
;
Silva, M
;
Skrzypek, B
;
Smithers, B
;
Snihur, R
;
Soedingrekso, J
;
Søgaard, A
;
Soldin, D
;
Spannfellner, C
;
Spiczak, GM
;
Spiering, C
;
Stamatikos, M
;
Stanev, T
;
Stein, R
;
Stezelberger, T
;
Stürwald, T
;
Stuttard, T
;
Sulanke, KH
;
Sullivan, GW
;
Taboada, I
;
Ter-Antonyan, S
;
Thompson, WG
;
Thwaites, J
;
Tilav, S
;
Tollefson, K
;
Tönnis, C
;
Toscano, S
;
Tosi, D
;
Trettin, A
;
Tung, CF
;
Turcotte, R
;
Twagirayezu, JP
;
Ty, B
;
Elorrieta, MA Unland
;
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
;
Watson, TB
;
Weaver, C
;
Weber, J
;
Weigel, P
;
Weindl, A
;
Weldert, J
;
Wendt, C
;
Werthebach, J
;
Weyrauch, M
;
Whitehorn, N
;
Wiebusch, CH
;
Willey, N
;
Williams, DR
;
Wisher, I
;
Wolf, M
;
Wrede, G
;
Wulff, J
;
Xu, XW
;
Yanez, JP
;
Yildizci, E
;
Yoshida, S
;
Yu, S
;
Yuan, T
;
Zhang, Z
;
Zhelnin, P
;
Collaboration, The IceCube
UC Berkeley Previously Published Works
(2023)
The D-Egg, an acronym for "Dual optical sensors in an Ellipsoid Glass for Gen2,"is one of the optical modules designed for future extensions of the IceCube experiment at the South Pole. The D-Egg has an elongated-sphere shape to maximize the photon-sensitive effective area while maintaining a narrow diameter to reduce the cost and the time needed for drilling of the deployment holes in the glacial ice for the optical modules at depths up to 2700 m. The D-Egg design is utilized for the IceCube Upgrade, the next stage of the IceCube project also known as IceCube-Gen2 Phase 1, where nearly half of the optical sensors to be deployed are D-Eggs. With two 8-inch high-quantum efficiency photomultiplier tubes (PMTs) per module, D-Eggs offer an increased effective area while retaining the successful design of the IceCube digital optical module (DOM). The convolution of the wavelength-dependent effective area and the Cherenkov emission spectrum provides an effective photodetection sensitivity that is 2.8 times larger than that of IceCube DOMs. The signal of each of the two PMTs is digitized using ultra-low-power 14-bit analog-to-digital converters with a sampling frequency of 240 MSPS, enabling a flexible event triggering, as well as seamless and lossless event recording of single-photon signals to multi-photons exceeding 200 photoelectrons within 10 ns. Mass production of D-Eggs has been completed, with 277 out of the 310 D-Eggs produced to be used in the IceCube Upgrade. In this paper, we report the design of the D-Eggs, as well as the sensitivity and the single to multi-photon detection performance of mass-produced D-Eggs measured in a laboratory using the built-in data acquisition system in each D-Egg optical sensor module.
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