6 research outputs found
Hybrid cosmic ray measurements using the IceAct telescopes in coincidence with the IceCube and IceTop detectors
- Author
- Abbasi Rasha
- Ackermann Markus
- Adams Jenni
- Aguilar Juanan
- Ahlers M.
- Ahrens Maryon
- Alispach Cyril Martin
- Alves Junior Antonio Augusto
- Amin Najia Moureen Binte
- An Rui
- Andeen Karen
- Anderson Tyler
- Anton Gisela
- Arguelles Carlos
- Ashida Yosuke
- Axani Spencer
- Bai Xinhua
- Balagopal V. Aswathi
- Barbano Anastasia Maria
- Barwick S. W.
- Bastian Benjamin
- Basu Vedant
- Baur Sebastian
- Bay R. C.
- Beatty J. J.
- Becker Tjus Julia
- Becker K.-H.
- Bellenghi Chiara
- BenZvi Segev
- Berley D.
- Bernardini Elisa
- Besson D. Z.
- Binder Gary
- Bindig Daniel
- Blaufuss E.
- Blot Summer
- Boddenberg Matthias
- Bontempo Federico
- Borowka Jurgen
- Boser S.
- Botner Olga
- Bottcher Jakob
- Bourbeau Etienne
- Bradascio Federica
- Braun J.
- Bretz Thomas
- Bron Stephanie
- Brostean-Kaiser Jannes
- Browne Sally-Ann
- Burgman Alexander
- Burley Ryan
- Busse Raffaela
- Campana Michael
- Carnie-Bronca Erin
- Chen Chujie
- Chirkin Dmitry
- Choi Koun
- Clark Brian
- Clark Kenneth
- Classen Lew
- Coleman Alan
- Collin Gabriel
- Conrad J. M.
- Coppin Paul
- Correa Pablo
- Cowen D. F.
- Cross R.
- Dappen Christian
- Dave Pranav
- DE CLERCQ Catherine
- De Ridder Sam
- De With Meike
- DeLaunay James
- Dembinski Hans
- Deoskar Kunal
- Desai Abhishek
- Desiati Paolo
- DeYoung Tyce
- Dharani Sukeerthi
- Diaz Alejandro
- Diaz-Velez Juan Carlos
- Dittmer Markus
- Do Giang
- Dujmovic Hrvoje
- Dunkman Matt
- DuVernois Michael
- Dvorak Emily
- Ehrhardt Thomas
- Eijndhoven Nick van
- Eller Philipp
- Engel Ralph
- Erpenbeck Hannah
- Evans John
- Evenson P. A.
- Fan Kwok Lung
- Fazely A. R.
- Fiedlschuster Sebastian
- Fienberg Aaron
- Filimonov Kirill
- Finley Chad
- Fischer Leander
- Fox Derek B.
- Franckowiak Anna
- Friedman Elizabeth
- Fritz Alexander
- Furst Philipp
- Gaisser T. K.
- Gallagher Jay
- Ganster Erik
- Garcia Alfonso
- Garrappa Simone
- Gerhardt L.
- Ghadimi Ava
- Glaser Christian
- Glauch Theo
- Glusenkamp Thorsten
- Goldschmidt A.
- Gonzalez Javier
- Goswami Sreetama
- Grant Darren
- Griswold Spencer
- Grégoire Timothée
- Gunduz Mehmet
- GĂŒnther Christoph
- Ha Minh Martin
- Haack Christian
- Hallgren Allan
- Halliday R.
- Halve L.
- Halzen F.
- Hanson Kael
- Hardin John
- Harnisch Alexander A.
- Haungs Andreas
- Hauser Simon
- Hebecker Dustin
- Helbing K.
- Henningsen Felix
- Hettinger Emma C.
- Hewitt John
- Hickford Stephanie
- Hignight Joshua
- Hill Colton
- Hill G. C.
- Hoffman Kara
- Hoffmann Ruth
- Hoinka Tobias
- Hokanson-Fasig Benjamin
- Hoshina K.
- Huang Feifei
- Huber Matthias
- Huber Thomas
- Hultqvist Klas
- Hunnefeld Mirco
- Hussain Raamis
- IceCube Collaboration
- In Seongjin
- Iovine NadĂšge
- Ishihara Aya
- Jansson Matti
- Japaridze George
- Jeong Minjin
- Jones Ben
- Kang Donghwa
- Kang Woosik
- Kang Xinyue
- Kappes Alexander
- Kappesser David
- Karg Timo
- Karl Martina
- Karle A.
- Katz U.
- Kauer M.
- Kellermann Moritz
- Kelley J. L.
- Kheirandish Ali
- Kin Ken\u27ichi
- Kintscher Thomas
- Kiryluk Joanna
- Klein Spencer
- Koirala Ramesh
- Kolanoski Hermann
- Kontrimas Tomas
- Kopke Lutz
- Kopper Claudio
- Kopper Sandro
- Koskinen D. J.
- Koundal Paras
- Kovacevich Michael
- Kowalski Marek
- Kozynets Tetiana
- Kun Emma
- Kurahashi Naoko
- Lad Neha
- Lagunas Gualda Cristina
- Lanfranchi Justin
- Larson M. J.
- Lauber Frederik Hermann
- Lazar Jeffrey
- Lee Jiwoong
- Leonard Kayla
- LeszczyĆska Agnieszka
- Li Yijia
- Lincetto Massimiliano
- Liu Qinrui
- Liubarska Maria
- Lohfink Elisa
- Lozano Mariscal Cristian Jesus
- Lu Lu
- Lucarelli Francesco
- Ludwig Andrew
- Luszczak William
- Lyu Yang
- Ma Wing Yan
- Madsen James
- Mahn Kendall
- Makino Yuya
- Mancina Sarah
- Maris Ioana Codrina
- Maruyama Reina H.
- Mase K.
- Maslowski Frank
- McElroy Thomas
- McNally Frank
- Mead James Vincent
- Meagher K.
- Medina Andres
- Meier Maximilian
- Meighen-Berger Stephan
- Micallef Jessie
- Mockler Daniela
- Montaruli Teresa
- Moore Roger
- Morse R.
- Moulai Marjon
- Naab Richard
- Nagai Ryo
- Naumann Uwe
- Necker Jannis
- Nguyen Le Viet
- Niederhausen Hans
- Nisa Mehr
- Nowicki Sarah
- Nygren Dave
- O\u27Sullivan Erin
- Obertacke Pollmann Anna
- Oehler Marie
- Olivas A.
- Pandya Hershal
- Pankova Daria
- Park Nahee
- Parker Grant
- Paudel Ek Narayan
- Paul Larissa
- Perez de los Heros Carlos
- Peters Lilly
- Peterson Josh
- Philippen Saskia
- Pieloth Damian
- Pieper Sarah
- Pittermann Martin
- Pizzuto A.
- Plum M.
- Popovych Yuiry
- Porcelli Alessio
- Prado Rodriguez Maria
- Price P. Buford
- Pries Brandom
- Przybylski Gerald
- Raab Christoph
- Raissi Amirreza
- Rameez Mohamed
- Rawlins K.
- Rea Immacolata Carmen
- Rehbein Florian
- Rehman Abdul
- Reichherzer Patrick
- Reimann René
- Renzi Giovanni
- Resconi Elisa
- Reusch Simeon
- Rhode Wolfgang
- Richman Mike
- Riedel Benedikt
- Roberts Ella
- Robertson Sally
- Roellinghoff Gerrit
- Rongen Martin
- Rott Carsten
- Ruhe Tim
- Ryckbosch Dirk
- Rysewyk Cantu Devyn
- Safa Ibrahim
- Saffer Julian
- Sanchez Herrera Sebastian
- Sandrock Alexander
- Sandroos Joakim
- Santander Marcos
- Santen Jakob van
- Sarkar Sourav
- Sarkar Subir
- Satalecka Konstancja
- Scharf Maximilian Karl
- Schaufel Merlin
- Schieler Harald
- Schindler Sebastian
- Schlunder P.
- Schmidt Torsten
- Schneider Austin
- Schneider Judith
- Schröder Frank G.
- Schumacher Lisa Johanna
- Schwefer Georg
- SchÀfer Johannes
- Sclafani Steve
- Seckel D.
- Seunarine Surujhdeo
- Sharma Ankur
- Shefali Shefali
- Silva Manuel
- Skrzypek Barbara
- Smithers Ben
- Snihur Robert
- Soedingrekso Jan
- Soldin Dennis
- Spannfellner Christian
- Spiczak Glenn
- Spiering Christian
- Stachurska Juliana
- Stamatikos Michael
- Stanev T.
- Stein Robert
- Stettner Joeran
- Steuer A.
- Stezelberger T.
- Sturwald Timo
- Stuttard Thomas
- Sullivan G. W.
- Taboada I.
- Tenholt Frederik
- Ter-Antonyan Samvel
- Tilav S.
- Tischbein Franziska
- Tollefson Kirsten
- Tomankova Lenka
- Toscano Simona
- Tosi Delia
- Trettin Alexander
- Tselengidou Maria
- Tung Chunfai
- Turcati Andrea
- Turcotte Roxanne
- Turley Colin
- Twagirayezu Jean Pierre
- Ty Bunheng
- Tönnis Christoph
- Unland Elorrieta Martin
- Valtonen-Mattila Nora
- Vandenbroucke Justin
- Vannerom David
- Verpoest Stef
- Vraeghe Matthias
- Vries Krijn de
- Walck C.
- Wasseige Gwenhaël de
- Watson Timothyblake
- Weaver Chris
- Weigel Philip
- Weindl Andreas
- Weiss Matthew
- Weldert Jan
- Wendt Chris
- Werthebach Johannes
- Weyrauch Mark
- Whitehorn Nathan
- Wiebusch C. H.
- Williams Dawn
- Wolf Martin
- Woschnagg Kurt
- Wrede Gerrit
- Wulff Johan
- Xu Xianwu
- Xu Yiqian
- Yanez Juan Pablo
- Yoshida S.
- Yu Shiqi
- Yuan Tianlu
- Zhang Zelong
- Zink Adrian
- Publication venue
- Scuola Internazionale Superiore di Studi Avanzati
- Publication date
- 04/10/2021
- Field of study
IceAct is a proposed surface array of compact (50 cm diameter) and cost-effective Imaging Air Cherenkov Telescopes installed at the site of the IceCube Neutrino Observatory at the geographic South Pole. Since January 2019, two IceAct telescope demonstrators, featuring 61 silicon photomultiplier (SiPM) pixels have been taking data in the center of the IceTop surface array during the austral winter. We present the first analysis of hybrid cosmic ray events detected by the IceAct imaging air-Cherenkov telescopes in coincidence with the IceCube Neutrino Observatory, including the IceTop surface array and the IceCube in-ice array. By featuring an energy threshold of about 10 TeV and a wide field-of-view, the IceAct telescopes show promising capabilities of improving current cosmic ray composition studies: measuring the Cherenkov light emissions in the atmosphere adds new information about the shower development not accessible with the current detectors, enabling significantly better primary particle type discrimination on a statistical basis. The hybrid measurement also allows for detailed feasibility studies of detector cross-calibration and of cosmic ray veto capabilities for neutrino analyses. We present the performance of the telescopes, the results from the analysis of two years of data, and an outlook of a hybrid simulation for a future telescope array
Three-year performance of the IceAct telescopes at the IceCube Neutrino Observatory
- Author
- Abbasi Rasha
- Ackermann Markus
- Adams Jenni
- Agarwalla Sanjib
- Aguilar Juanan
- Ahlers Markus
- Alameddine Jean-Marco
- Amin Najia Moureen Binte
- Andeen Karen
- Anton Gisela
- ArgĂŒelles Carlos
- Ashida Yosuke
- Athanasiadou Sofia
- Axani Spencer
- Bai Xinhua
- Balagopal V Aswathi
- Baricevic Moreno
- Barwick Steve
- Basu Vedant
- Bay Ryan
- Beatty James
- Becker Tjus Julia
- Beise Jakob
- Bellenghi Chiara
- Benning Charlotte
- BenZvi Segev
- Berley David
- Bernardini Elisa
- Besson Dave
- Blaufuss Erik
- Blot Summer
- Bontempo Federico
- Book Julia
- Boscolo Meneguolo Caterina
- Boser Sebastian
- Botner Olga
- Bottcher Jakob
- Bourbeau Etienne
- Braun Jim
- Bretz Thomas
- Brinson Bennett
- Brostean-Kaiser Jannes
- Burley Ryan T.
- Busse Raffaela
- Butterfield Delaney
- Campana Michael
- Carloni Kiara
- Carnie-Bronca Erin
- Chattopadhyay Sharmistha
- Chau Thien Nhan
- Chen Chujie
- Chen Zheyang
- Chirkin Dmitry
- Choi Seowon
- Clark Brian
- Classen Lew
- Clercq Catherine De
- Coleman Alan
- Collin Gabriel
- Connolly Amy
- Conrad Janet
- Coppin Paul
- Correa Pablo
- Cowen Doug
- Dave Pranav
- DeLaunay James
- Delgado Lopez Diyaselis
- Deng Shuyang
- Deoskar Kunal
- Desai Abhishek
- Desiati Paolo
- DeYoung Tyce
- Diaz Alejandro
- Diaz-Velez Juan Carlos
- Dittmer Markus
- Domi Alba
- Dujmovic Hrvoje
- DuVernois Michael
- Ehrhardt Thomas
- Eijndhoven Nick Van
- Eller Philipp
- Ellinger Enrico
- ElsÀsser Dominik
- Engel Ralph
- Erpenbeck Hannah
- Evans John
- Evenson Paul
- Fan Kwok Lung
- Fang Ke
- Farrag Kareem Ramadan
- Fazely Ali
- Fedynitch Anatoli
- Feigl Nora
- Fiedlschuster Sebastian
- Finley Chad
- Fischer Leander
- Fox Derek B.
- Franckowiak Anna
- Fritz Alexander
- Furst Philipp
- Gallagher Jay
- Ganster Erik
- Garcia Alfonso
- Gerhardt Lisa
- Ghadimi Ava
- Glaser Christian
- Glauch Theo
- Glusenkamp Thorsten
- Goehlke Noah
- Gonzalez Javier
- Goswami Sreetama
- Grant Darren
- Gray Shannon
- Gries Oliver
- Griffin Sean
- Griswold Spencer
- Groth Kathrine Morch
- Gutjahr Pascal
- GĂŒnther Christoph
- Ha Minh Martin
- Haack Christian
- Hallgren Allan
- Halliday Robert
- Halve Lasse
- Halzen Francis
- Hamdaoui Hassane
- Hanson Kael
- Hardin John
- Harnisch Alexander
- Hatch Patrick
- Haungs Andreas
- Helbing Klaus
- Hellrung Jonas
- Henningsen Felix
- Heuermann Lars Philipp
- Hewitt John W.
- Heyer Nils
- Hickford Stephanie
- Hidvegi Attila
- Hill Colton
- Hill Gary
- Hoffman Kara
- Hori Sam
- Hoshina Kotoyo
- Hou Wenjie
- Huber Thomas
- Hultqvist Klas
- Hunnefeld Mirco
- Hussain Raamis
- Hymon Karolin
- IceCube
- In Seongjin
- Ishihara Aya
- Jacquart Marc
- Janik Oliver
- Jansson Matti
- Japaridze George
- Jayakumar Krishnamoorthi
- Jeong Minjin
- Jin Miaochen
- Jones Ben
- Kang Donghwa
- Kang Woosik
- Kang Xinyue
- Kappes Alexander
- Kappesser David
- Kardum Leonora
- Karg Timo
- Karl Martina
- Karle Albrecht
- Katz UlĂŹ
- Kauer Matt
- Kelley John
- Khatee Zathul Arifa
- Kheirandish Ali
- Kiryluk Joanna
- Klein Spencer
- Kochocki Alina
- Koirala Ramesh
- Kolanoski Hermann
- Kontrimas Tomas
- Kopke Lutz
- Kopper Claudio
- Koskinen Jason
- Koundal Paras
- Kovacevich Michael
- Kowalski Marek
- Kozynets Tetiana
- Kruiswijk Karlijn
- Krupczak Emmett
- Kumar Anil
- Kun Emma
- Lad Neha Navnitkumar
- Lagunas Gualda Cristina
- Lamoureux Mathieu
- Larson Michael J.
- Latseva Silvia
- Lauber Frederik Hermann
- Lazar Jeffrey
- Lee Jiwoong
- Leonard DeHolton Kayla
- Leszczynska Agnieszka
- Lincetto Massimiliano
- Liu Qinrui
- Liubarska Maria
- Lohfink Elisa
- Love Christina
- Lozano Mariscal Cristian Jesus
- Lu Lu
- Lucarelli Francesco
- Luszczak William
- Lyu Yang
- Madsen Jim
- Mahn Kendall
- Makino Yuya
- Manao Elena
- Mancina Sarah
- Marie Sainte Wenceslas
- Maris Ioana Codrina
- Marka Szabolcs
- Marka Zsuzsa
- Marsee Matthew
- Martinez-Soler Ivan
- Maruyama Reina H.
- Mayhew Finn
- McElroy Thomas
- McNally Frank
- Mead James Vincent
- Meagher Kevin
- Mechbal Sarah
- Medina Andres
- Meier Maximilian
- Mentawi Sharif El
- Merckx Yarno
- Merten Lukas
- Micallef Jessie
- Mitchell Justin
- Montaruli Teresa
- Moore Roger
- Morii Yasutsugu
- Morse Bob
- Moulai Marjon
- Mukherjee Tista
- Naab Richard
- Nagai Ryo
- Nakos Maxwell
- Naumann Uwe
- Necker Jannis
- Negi Akshima
- Neilson Naoko Kurahashi
- Neumann Miriam
- Niederhausen Hans
- Nisa Mehr
- Noell Andreas
- Novikov Alexander
- Nowicki Sarah
- O\u27Dell Vivian
- O\u27Sullivan Erin
- Oehler Marie
- Oeyen Bob
- Olivas Alex
- Orsoe Rasmus
- Osborn Jesse
- Pandya Hershal
- Park Nahee
- Parker Grant
- Paudel Ek Narayan
- Paul Larissa
- Peterson Josh
- Philippen Saskia
- Pizzuto Alex
- Plum Matthias
- Pollmann Anna
- Ponten Axel
- Popovych Yuriy
- Prado Rodriguez Maria
- Pries Brandon
- Procter-Murphy Rachel
- Przybylski Gerald
- PĂ©rez de los Heros Carlos
- Raab Christoph
- Rack-Helleis John
- Rawlins Katherine
- Rechav Zoe
- Rehman Abdul
- Reichherzer Patrick
- Renzi Giovanni
- Resconi Elisa
- Reusch Simeon
- Rhode Wolfgang
- Riedel Benedikt
- Rifaie Adam
- Roberts Ella
- Robertson Sally
- Rodan Steven T.
- Roellinghoff Gerrit
- Rongen Martin
- Rott Carsten
- Ruhe Tim
- Ruohan Li
- Ryckbosch Dirk
- Safa Ibrahim
- Saffer Julian
- Salazar-Gallegos Daniel
- Sampathkumar Pranav
- Sanchez Herrera Sebastian
- Sandrock Alexander
- Santander Marcos
- Santen Jakob Van
- Sarkar Sourav
- Sarkar Subir
- Savelberg Joelle
- Savina Pierpaolo
- Schaufel Merlin
- Schieler Harald
- Schindler Sebastian
- Schlickmann Lea
- SchlĂŒter Berit
- SchlĂŒter Felix
- Schmeisser Nick
- Schmidt Torsten
- Schneider Judith
- Schröder Frank G.
- Schumacher Lisa Johanna
- Schwefer Georg
- Sclafani Steve
- Seckel David
- Seikh Mohammad Ful Hossain
- Seunarine Suruj
- Shah Riya
- Sharma Ankur
- Shefali S.
- Shimizu Nobuhiro
- Silva Manuel
- Skrzypek Barbara
- Smithers Ben
- Snihur Robert
- Soedingrekso Jan
- Sogaard Andreas
- Soldin Dennis
- Soldin Philipp
- Sommani Giacomo
- Spannfellner Christian
- Spiczak Glenn
- Spiering Christian
- Stamatikos Michael
- Stanev Todor
- Stezelberger Thorsten
- Sturwald Timo
- Stuttard Thomas
- Sullivan Greg
- Taboada Ignacio
- Ter-Antonyan Samvel
- Thiesmeyer Matthias
- Thompson Will
- Thwaites Jessie
- Tilav Serap
- Tollefson Kirsten
- Toscano Simona
- Tosi Delia
- Trettin Alexander
- Tung Chun Fai
- Turcotte Roxanne
- Twagirayezu Jean Pierre
- Ty Bunheng
- Tönnis Christoph
- Unland Elorrieta Martin
- Upadhyay Anuj Kumar
- Upshaw Karriem
- Valtonen-Mattila Nora
- Vandenbroucke Justin
- Vannerom David
- Vara Javi
- Veitch-Michaelis Joshua
- Venugopal Megha
- Vereecken Matthias
- Verpoest Stef
- Veske DoÄa
- Vijai Aishwarya
- Vries Krijn De
- Walck Christian
- Wasseige Gwenhaël De
- Weaver Chris
- Weigel Philip
- Weindl Andreas
- Weldert Jan
- Wendt Chris
- Werthebach Johannes
- Weyrauch Mark
- Whitehorn Nathan
- Wiebusch Christopher
- Willey Nathan
- Williams Dawn
- Witthaus Lucas
- Wolf Annika
- Wolf Martin
- Wrede Gerrit
- Xu Xianwu
- Yanez Juan Pablo
- Yildizci Emre Burak
- Yoshida Shigeru
- Young Robert
- Yu Felix J.
- Yu Shiqi
- Yuan Tianlu
- Zhang Zelong
- Zhelnin Pavel
- Zimmerman Melany
- Zink Adrian
- Publication venue
- Scuola Internazionale Superiore di Studi Avanzati
- Publication date
- 24/10/2023
- Field of study
IceAct is an array of compact Imaging Air Cherenkov Telescopes at the ice surface as part of the IceCube Neutrino Observatory. The telescopes, featuring a camera of 61 silicon photomultipliers and fresnel-lens-based optics, are optimized to be operated in harsh environmental conditions, such as at the South Pole. Since 2019, the first two telescopes have been operating in a stereoscopic configuration in the center of IceCube\u27s surface detector IceTop. With an energy threshold of about 10 TeV and a wide field-of-view, the IceAct telescopes show promising capabilities of improving current cosmic-ray composition studies: measuring the Cherenkov light emissions in the atmosphere adds new information about the shower development not accessible with the current detectors. First simulations indicate that the added information of a single telescope leads, e.g., to an improved discrimination between flux contributions from different primary particle species in the sensitive energy range.
We review the performance and detector operations of the telescopes during the past 3 years (2020-2022) and give an outlook on the future of IceAct
Search for Spatial Correlations of Neutrinos with Ultra-high-energy Cosmic Rays
- Author
- A. M.
- Abbasi R.
- Abreu P.
- Abu-Zayyad T.
- Ackermann M.
- Adams J.
- Aglietta M.
- Aguilar J. A.
- Ahlers M.
- Ahrens M.
- Alameddine J. M.
- Albert A.
- Albury J. M.
- Alispach C.
- Allekotte I.
- Allen M.
- Almeida R. M. de
- Almela A.
- Alvarez-Muñiz J.
- Alves Jr. A. A.
- Alves S.
- Amin N. M.
- Anastasi G. A.
- Anchordoqui L.
- Andeen K.
- Anderson T.
- Andrada B.
- Andringa S.
- André M.
- Anghinolfi M.
- Anjos R. C. dos
- Anton G.
- Arai Y.
- Aramo C.
- Arbeletche L. Bonneau
- Ardid S.
- ArgĂŒelles C.
- Arimura R.
- Armand J. Perez
- Arnone E.
- Ashida Y.
- Asorey H.
- Assis P.
- Aubert J.-J.
- Aublin J.
- Avila G.
- Axani S.
- Badescu A. M.
- Bai X.
- Bakalova A.
- Balaceanu A.
- Barbano A.
- Barbato F.
- Barcikowski E.
- Baret B.
- Barwick S. W.
- Basa S.
- Bastian B.
- Basu V.
- Batista R. Alves
- Baur S.
- Bay R.
- Beatty J. J.
- Becker K.-H.
- Belhorma B.
- Bellenghi C.
- Bellido J. A.
- Belz J. W.
- Bendahman M.
- BenZvi S.
- Berat C.
- Bergman D. R.
- Berisso M. GĂłmez
- Berley D.
- Bernardini E.
- Bertaina M. E.
- Bertin V.
- Bertolli C. PĂ©rez
- Bertou X.
- Besson D. Z.
- Bhatta G.
- Biagi S.
- Biermann P. L.
- Binder G.
- Bindig D.
- Binet V.
- Bismark K.
- Bissinger M.
- Bister T.
- Biteau J.
- Blake S. A.
- Blaufuss E.
- Blazek J.
- Bleve C.
- Blot S.
- BlĂŒmer J.
- Boddenberg M.
- BohĂĄÄovĂĄ M.
- Boncioli D.
- Bonifazi C.
- Bontempo F.
- Borodai N.
- Borowka J.
- Botner O.
- Botti A. M.
- Boumaaza J.
- Bourbeau E.
- Bouta M.
- Bouwhuis M. C.
- Brack J.
- Bradascio F.
- Braun J.
- Breton R. Le
- Bretz T.
- Briechle F. L.
- Brinson B.
- Bron S.
- Brostean-Kaiser J.
- Browne S.
- Bruijn R.
- Brunner J.
- BrĂąnzaĆ H.
- Buchholz P.
- Buckland I.
- Bueno A.
- Buitink S.
- Burgman A.
- Burley R. T.
- Buscemi M.
- Busse R. S.
- Busto J.
- Böser S.
- Böttcher J.
- BĂŒsken M.
- Caballero-Mora K. S.
- Caccianiga L.
- Cady R.
- Caiffi B.
- Calvo D.
- Campana M. A.
- Canfora F.
- Cantu D. Rysewyk
- Capone A.
- Caracas I.
- Caramete L.
- Carnie-Bronca E. G.
- Carr J.
- Carretero V.
- Caruso R.
- Castellina A.
- Catalani F.
- Cataldi G.
- Cazon L.
- Celli S.
- Cerda M.
- Cerutti A. C. Cobos
- Chabab M.
- Chau T. N.
- Cheminant K. Almeida
- Chen C.
- Chen Z.
- Cheon B. G.
- Chiarusi T.
- Chiba J.
- Chikawa M.
- Chinellato J. A.
- Chirkin D.
- Choi K.
- Chudoba J.
- Chytka L.
- Circella M.
- Clark B. A.
- Clark K.
- Classen L.
- Clay R. W.
- Clercq C. De
- Colalillo R.
- Coleiro A.
- Coleman A.
- Collin G. H.
- Coluccia M. R.
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- Zundel Z.
- ZĂșñiga J.
- Ć mĂda R.
- Publication venue
- Institute of Physics Publishing Ltd
- Publication date
- 24/09/2022
- Field of study
For several decades, the origin of ultra-high-energy cosmic rays (UHECRs) has been an unsolved question of high-energy astrophysics. One approach for solving this puzzle is to correlate UHECRs with high-energy neutrinos, since neutrinos are a direct probe of hadronic interactions of cosmic rays and are not deflected by magnetic fields. In this paper, we present three different approaches for correlating the arrival directions of neutrinos with the arrival directions of UHECRs. The neutrino data are provided by the IceCube Neutrino Observatory and ANTARES, while the UHECR data with energies above âŒ50 EeV are provided by the Pierre Auger Observatory and the Telescope Array. All experiments provide increased statistics and improved reconstructions with respect to our previous results reported in 2015. The first analysis uses a high-statistics neutrino sample optimized for point-source searches to search for excesses of neutrino clustering in the vicinity of UHECR directions. The second analysis searches for an excess of UHECRs in the direction of the highest-energy neutrinos. The third analysis searches for an excess of pairs of UHECRs and highest-energy neutrinos on different angular scales. None of the analyses have found a significant excess, and previously reported overfluctuations are reduced in significance. Based on these results, we further constrain the neutrino flux spatially correlated with UHECRs
Calibration of the logarithmic-periodic dipole antenna (LPDA) radio stations at the Pierre Auger Observatory using an octocopter
- Author
- Aab Alexander
- Abreu Pedro
- Aglietta Marco
- Al Samarai Imen
- Albuquerque Ivone
- Allekotte Ingomar
- Almela Alejandro
- Alvarez Castillo Jesus
- Alvarez-Muñiz Jaime
- Anastasi Gioacchino Alex
- Anchordoqui Luis
- Andrada Belén
- Andringa Sofia
- Aramo Carla
- Arqueros Fernando
- Arsene Nicusor
- Asorey HernĂĄn Gonzalo
- Assis Pedro
- Aublin Julien
- Avila Gualberto
- Badescu Alina Mihaela
- Balaceanu Alexandru
- Barbato Felicia
- Barreira Luz Ricardo Jorge
- Beatty Jim
- Becker Karl-Heinz
- Bellido Jose A.
- Berat Corinne
- Bertaina Mario Edoardo
- Bertou Xavier
- Biermann Peter
- Billoir Pierre
- Biteau Jonathan
- Blaess Simon G.
- Blanco Alberto
- Blazek Jiri
- Bleve Carla
- BohĂĄÄovĂĄ Martina
- Boncioli Denise
- Bonifazi Carla
- Borodai Nataliia
- Botti Ana Martina
- Brack Jeffrey
- Brancus Iliana
- Bretz Thomas GĂŒnther
- Bridgeman Ariel
- Briechle Florian
- Buchholz Peter
- Bueno Antonio
- Buitink Stijn
- Buscemi Mario
- Caballero-Mora Karen S.
- Caccianiga Lorenzo
- Cancio Ăngel
- Canfora Fabrizia
- Caramete Laurentiu
- Caruso Rossella
- Castellina Antonella
- Cataldi Gabriella
- Cazon Lorenzo
- Chavez Alan G.
- Chinellato Jose Augusto
- Chudoba Jiri
- Clay Roger W.
- Cobos AgustĂn
- Colalillo Roberta
- Coleman Alan
- Collica Laura
- Coluccia Maria Rita
- Conceição Ruben
- Consolati Giovanni
- Contreras Fernando
- Cooper Mathew J.
- Coutu Stephane
- Covault Corbin
- Cronin James
- D'Amico Stefano
- D'Olivo Juan Carlos
- Daniel Bruno
- Dasso Sergio
- Daumiller Kai
- Dawson Bruce R.
- de Almeida Rogerio M.
- de Jong Sijbrand J.
- De Mauro Giuseppe
- de Mello Neto Joao
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- Todero Peixoto Carlos J.
- Tomankova Lenka
- Tomé Bernardo
- Torralba Elipe Guillermo
- Travnicek Petr
- Trini Marta
- Ulrich Ralf
- Unger Michael
- Urban Martin
- Valdés Galicia Jose F.
- Valiño Ines
- Valore Laura
- van Aar Guus
- van Bodegom Patrick
- van den Berg Ad M.
- van Vliet Arjen
- Varela Enrique
- Vargas CĂĄrdenas Bernardo
- Varner Gary
- VeberiÄ Darko
- Vergara Quispe Indira D.
- Verzi Valerio
- Vicha Jakub
- Villaseñor Luis
- Vorobiov Serguei
- VĂĄzquez Ricardo
- Wahlberg Hernan
- Wainberg Oscar
- Walz David Simon
- Watson Alan
- Weber Marc
- Weindl Andreas
- Wiencke Lawrence
- WilczyĆski Henryk
- Winchen Tobias
- Wirtz Marcus
- Wittkowski David
- Wundheiler Brian
- Yang Lili
- Yelos Diana
- Yushkov Alexey
- Zas Enrique
- Zavrtanik Danilo
- Zavrtanik Marko
- Zepeda Arnulfo
- Zimmermann Benedikt
- Ziolkowski Michael
- Zong Zizhao
- Zuccarello Francesca
- ĆmiaĆkowski Andrzej
- Ć mĂda Radomir
- Publication venue
- 'IOP Publishing'
- Publication date
- 01/01/2017
- Field of study
International audienceAn in-situ calibration of a logarithmic periodic dipole antenna with a frequency coverage of 30 MHz to 80 MHz is performed. Such antennas are part of a radio station system used for detection of cosmic ray induced air showers at the Engineering Radio Array of the Pierre Auger Observatory, the so-called Auger Engineering Radio Array (AERA) . The directional and frequency characteristics of the broadband antenna are investigated using a remotely piloted aircraft carrying a small transmitting antenna. The antenna sensitivity is described by the vector effective length relating the measured voltage with the electric-field components perpendicular to the incoming signal direction. The horizontal and meridional components are determined with an overall uncertainty of 7.4(+0.9)(â)(0.3)% and 10.3(+2.8)(â)(1.7)% respectively. The measurement is used to correct a simulated response of the frequency and directional response of the antenna. In addition, the influence of the ground conductivity and permittivity on the antenna response is simulated. Both have a negligible influence given the ground conditions measured at the detector site. The overall uncertainties of the vector effective length components result in an uncertainty of 8.8(+2.1)(â)(1.3)% in the square root of the energy fluence for incoming signal directions with zenith angles smaller than 60°
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- Wormell
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- Wyse
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- Wörle
- Wörrle
- Wörrle
- Wörrle
- WĂŒst
- WĂŒst
- WĂŒst
- WĂŒst
- Yailenko
- Yailenko
- Yailenko
- Yailenko
- Yakovenko
- Yon
- Yon
- Yon
- Yon
- Yourukova
- Yourukova
- Yoyotte
- Zadok
- Zadok
- Zadok
- Zadok
- Zadok
- Zadok
- Zadok
- Zadok
- Zadok
- Zahrnt
- Zauzich
- Zauzich
- Zedgenidze
- Zedgenidze
- Zervos
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- Zograf
- Zograf
- Zolotaryov
- Zolotaryov
- Publication venue
- 'Cambridge University Press (CUP)'
- Publication date
- 01/01/1994
- Field of study
Search for Spatial Correlations of Neutrinos with Ultra-high-energy Cosmic Rays
- Author
- A. Diaz A. Diaz.
- Abbasi R.
- Abreu P.
- Abu-Zayyad T.
- Ackermann M.
- Adams J.
- Aglietta M.
- Aguilar J. A.
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- Vivolo D.
- Vorobiov S.
- VĂĄsquez-RamĂrez A.
- Wahlberg H.
- Walck C.
- Warren D.
- Watanabe C.
- Watson A. A.
- 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.
- Wiencke L.
- WilczyĆski H.
- Williams D. R.
- Wilms J.
- Wirtz M.
- Wittkowski D.
- Wolf M.
- Wong T.
- Woschnagg K.
- Wrede G.
- Wulff J.
- Wundheiler B.
- Xu X. W.
- Yamamoto M.
- Yamazaki K.
- Yanez J. P.
- Yashiro K.
- Yoshida F.
- Yoshida S.
- Yoshioka Y.
- Yu S.
- Yuan T.
- Yushkov A.
- Zapparrata O.
- Zas E.
- Zavatarelli S.
- Zavrtanik D.
- Zavrtanik M.
- Zegarelli A.
- Zehrer L.
- Zhang Z.
- Zhelnin P.
- Zhezher Y.
- Zornoza J. D.
- Zundel Z.
- ZĂșñiga J.
- Ć mĂda R.
- Publication venue
- 'American Astronomical Society'
- Publication date
- 01/01/2022
- Field of study
International audienceFor several decades, the origin of ultra-high-energy cosmic rays (UHECRs) has been an unsolved question of high-energy astrophysics. One approach for solving this puzzle is to correlate UHECRs with high-energy neutrinos, since neutrinos are a direct probe of hadronic interactions of cosmic rays and are not deflected by magnetic fields. In this paper, we present three different approaches for correlating the arrival directions of neutrinos with the arrival directions of UHECRs. The neutrino data are provided by the IceCube Neutrino Observatory and ANTARES, while the UHECR data with energies above âŒ50 EeV are provided by the Pierre Auger Observatory and the Telescope Array. All experiments provide increased statistics and improved reconstructions with respect to our previous results reported in 2015. The first analysis uses a high-statistics neutrino sample optimized for point-source searches to search for excesses of neutrino clustering in the vicinity of UHECR directions. The second analysis searches for an excess of UHECRs in the direction of the highest-energy neutrinos. The third analysis searches for an excess of pairs of UHECRs and highest-energy neutrinos on different angular scales. None of the analyses have found a significant excess, and previously reported overfluctuations are reduced in significance. Based on these results, we further constrain the neutrino flux spatially correlated with UHECRs