IceCube-Gen2 - The Next Generation Neutrino Observatory at the South  Pole: Contributions to ICRC 2015

Collaboration TI-G; Aartsen MG; Abraham K; Ackermann M; Adams J; Aguilar JA; Ahlers M; Ahrens M; Altmann D; Anderson T; Ansseau I; Anton G; Archinger M; Arguelles C; Arlen TC; Auffenberg J; Axani S; Bai X; Bartos I; Barwick SW; Baum V; Bay R; Beatty JJ; Tjus JB; Becker K-H; Beiser E; BenZvi S; Berghaus P; Berley D; Bernardini E; Bernhard A; Besson DZ; Binder G; Bindig D; Bissok M; Blaufuss E; Blumenthal J; Boersma DJ; Bohm C; Börner M; Bos F; Bose D; Böser S; Botner O; Braun J; Brayeur L; Bretz H-P; Buzinsky N; Casey J; Casier M; Cheung E; Chirkin D; Christov A; Clark K; Classen L; Coenders S; Collin GH; Conrad JM; Cowen DF; Silva AHC; Daughhetee J; Davis JC; Day M; André JPAMD; Clercq CD; Rosendo EDP; Dembinski H; Ridder SD; Desiati P; Vries KDD; Wasseige GD; With MD; DeYoung T; Diaz-Vélez JC; Lorenzo VD; Dumm JP; Dunkman M; Eagan R; Eberhardt B; Ehrhardt T; Eichmann B; Euler S; Evans JJ; Evenson PA; Fadiran O; Fahey S; Fazely AR; Fedynitch A; Feintzeig J; Felde J; Filimonov K; Finley C; Fischer-Wasels T; Flis S; Fösig C-C; Fuchs T; Gaisser TK; Gaior R; Gallagher J; Gerhardt L; Ghorbani K; Gier D; Gladstone L; Glagla M; Glüsenkamp T; Goldschmidt A; Golup G; Gonzalez JG; Góra D; Grant D; Groh JC; Groß A; Ha C; Haack C; Ismail AH; Hallgren A; Halzen F; Hansmann B; Hanson K; Haugen J; Hebecker D; Heereman D; Helbing K; Hellauer R; Hellwig D; Hickford S; Hignight J; Hill GC; Hoffman KD; Hoffmann R; Holzapfel K; Homeier A; Hoshina K; Huang F; Huber M; Huelsnitz W; Hulth PO; Hultqvist K; In S; Ishihara A; Jacobi E; Japaridze GS; Jero K; Jones BJP; Jurkovic M; Kalekin O; Kaminsky B; Kappes A; Karg T; Karle A; Katori T; Katz U; Kauer M; Keivani A; Kelley JL; Kemp J; Kheirandish A; Kiryluk J; Kläs J; Klein SR; Kohnen G; Koirala R; Kolanoski H; Konietz R; Koob A; Köpke L; Kopper C; Kopper S; Koskinen DJ; Kowalski M; Krauss CB; Krings K; Kroll G; Kroll M; Kunnen J; Kurahashi N; Kuwabara T; Labare M; Lanfranchi JL; Larson MJ; Lesiak-Bzdak M; Leuermann M; Leuner J; LoSecco J; Lu L; Lünemann J; Madsen J; Maggi G; Mahn KBM; Marka S; Marka Z; Maruyama R; Mase K; Matis HS; Maunu R; McNally F; Meagher K; Medici M; Meli A; Menne T; Merino G; Meures T; Miarecki S; Middell E; Middlemas E; Mohrmann L; Montaruli T; Moore RW; Morse R; Nahnhauer R; Naumann U; Neer G; Niederhausen H; Nowicki SC; Nygren DR; Obertacke A; Olivas A; Omairat A; O'Murchadha A; Palazzo A; Palczewski T; Pandya H; Paul L; Pepper JA; Heros CPDL; Petersen TC; Pfendner C; Pieloth D; Pinat E; Pinfold JL; Posselt J; Price PB; Przybylski GT; Pütz J; Quinnan M; Raab C; Rädel L; Rameez M; Rawlins K; Reimann R; Relich M; Resconi E; Rhode W; Richman M; Richter S; Riedel B; Robertson S; Rongen M; Rott C; Ruhe T; Ryckbosch D; Saba SM; Sabbatini L; Sander H-G; Sandrock A; Sandroos J; Sandstrom P; Sarkar S; Schatto K; Scheriau F; Schimp M; Schmidt T; Schmitz M; Schoenen S; Schöneberg S; Schönwald A; Schulte L; Seckel D; Seunarine S; Shaevitz MH; Shanidze R; Smith MWE; Soldin D; Söldner-Rembold S; Song M; Spiczak GM; Spiering C; Stahlberg M; Stamatikos M; Stanev T; Stanisha NA; Stasik A; Stezelberger T; Stokstad RG; Stößl A; Ström R; Strotjohann NL; Sullivan GW; Sutherland M; Taavola H; Taboada I; Taketa A; Tanaka HKM; Ter-Antonyan S; Terliuk A; Tešić G; Tilav S; Toale PA; Tobin MN; Toscano S; Tosi D; Tselengidou M; Turcati A; Unger E; Usner M; Vallecorsa S; Vandenbroucke J; Eijndhoven NV; Vanheule S; Santen JV; Veenkamp J; Vehring M; Voge M; Vraeghe M; Walck C; Wallace A; Wallraff M; Wandkowsky N; Weaver C; Wendt C; Westerhoff S; Whelan BJ; Whitehorn N; Wichary C; Wiebe K; Wiebusch CH; Wille L; Williams DR; Wissing H; Wolf M; Wood TR; Woschnagg K; Wren S; Xu DL; Xu XW; Xu Y; Yanez JP; Yodh G; Yoshida S; Zoll M

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Author

Collaboration TI-G

Aartsen MG

Abraham K

Ackermann M

Adams J

Aguilar JA

Ahlers M

Ahrens M

Altmann D

Anderson T

Ansseau I

Anton G

Archinger M

Arguelles C

Arlen TC

Auffenberg J

Axani S

Bai X

Bartos I

Barwick SW

Baum V

Bay R

Beatty JJ

Tjus JB

Becker K-H

Beiser E

BenZvi S

Berghaus P

Berley D

Bernardini E

Bernhard A

Besson DZ

Binder G

Bindig D

Bissok M

Blaufuss E

Blumenthal J

Boersma DJ

Bohm C

Börner M

Bos F

Bose D

Böser S

Botner O

Braun J

Brayeur L

Bretz H-P

Buzinsky N

Casey J

Casier M

Cheung E

Chirkin D

Christov A

Clark K

Classen L

Coenders S

Collin GH

Conrad JM

Cowen DF

Silva AHC

Daughhetee J

Davis JC

Day M

André JPAMD

Clercq CD

Rosendo EDP

Dembinski H

Ridder SD

Desiati P

Vries KDD

Wasseige GD

With MD

DeYoung T

Diaz-Vélez JC

Lorenzo VD

Dumm JP

Dunkman M

Eagan R

Eberhardt B

Ehrhardt T

Eichmann B

Euler S

Evans JJ

Evenson PA

Fadiran O

Fahey S

Fazely AR

Fedynitch A

Feintzeig J

Felde J

Filimonov K

Finley C

Fischer-Wasels T

Flis S

Fösig C-C

Fuchs T

Gaisser TK

Gaior R

Gallagher J

Gerhardt L

Ghorbani K

Gier D

Gladstone L

Glagla M

Glüsenkamp T

Goldschmidt A

Golup G

Gonzalez JG

Góra D

Grant D

Groh JC

Groß A

Ha C

Haack C

Ismail AH

Hallgren A

Halzen F

Hansmann B

Hanson K

Haugen J

Hebecker D

Heereman D

Helbing K

Hellauer R

Hellwig D

Hickford S

Hignight J

Hill GC

Hoffman KD

Hoffmann R

Holzapfel K

Homeier A

Hoshina K

Huang F

Huber M

Huelsnitz W

Hulth PO

Hultqvist K

In S

Ishihara A

Jacobi E

Japaridze GS

Jero K

Jones BJP

Jurkovic M

Kalekin O

Kaminsky B

Kappes A

Karg T

Karle A

Katori T

Katz U

Kauer M

Keivani A

Kelley JL

Kemp J

Kheirandish A

Kiryluk J

Kläs J

Klein SR

Kohnen G

Koirala R

Kolanoski H

Konietz R

Koob A

Köpke L

Kopper C

Kopper S

Koskinen DJ

Kowalski M

Krauss CB

Krings K

Kroll G

Kroll M

Kunnen J

Kurahashi N

Kuwabara T

Labare M

Lanfranchi JL

Larson MJ

Lesiak-Bzdak M

Leuermann M

Leuner J

LoSecco J

Lu L

Lünemann J

Madsen J

Maggi G

Mahn KBM

Marka S

Marka Z

Maruyama R

Mase K

Matis HS

Maunu R

McNally F

Meagher K

Medici M

Meli A

Menne T

Merino G

Meures T

Miarecki S

Middell E

Middlemas E

Mohrmann L

Montaruli T

Moore RW

Morse R

Nahnhauer R

Naumann U

Neer G

Niederhausen H

Nowicki SC

Nygren DR

Obertacke A

Olivas A

Omairat A

O'Murchadha A

Palazzo A

Palczewski T

Pandya H

Paul L

Pepper JA

Heros CPDL

Petersen TC

Pfendner C

Pieloth D

Pinat E

Pinfold JL

Posselt J

Price PB

Przybylski GT

Pütz J

Quinnan M

Raab C

Rädel L

Rameez M

Rawlins K

Reimann R

Relich M

Resconi E

Rhode W

Richman M

Richter S

Riedel B

Robertson S

Rongen M

Rott C

Ruhe T

Ryckbosch D

Saba SM

Sabbatini L

Sander H-G

Sandrock A

Sandroos J

Sandstrom P

Sarkar S

Schatto K

Scheriau F

Schimp M

Schmidt T

Schmitz M

Schoenen S

Schöneberg S

Schönwald A

Schulte L

Seckel D

Seunarine S

Shaevitz MH

Shanidze R

Smith MWE

Soldin D

Söldner-Rembold S

Song M

Spiczak GM

Spiering C

Stahlberg M

Stamatikos M

Stanev T

Stanisha NA

Stasik A

Stezelberger T

Stokstad RG

Stößl A

Ström R

Strotjohann NL

Sullivan GW

Sutherland M

Taavola H

Taboada I

Taketa A

Tanaka HKM

Ter-Antonyan S

Terliuk A

Tešić G

Tilav S

Toale PA

Tobin MN

Toscano S

Tosi D

Tselengidou M

Turcati A

Unger E

Usner M

Vallecorsa S

Vandenbroucke J

Eijndhoven NV

Vanheule S

Santen JV

Veenkamp J

Vehring M

Voge M

Vraeghe M

Walck C

Wallace A

Wallraff M

Wandkowsky N

Weaver C

Wendt C

Westerhoff S

Whelan BJ

Whitehorn N

Wichary C

Wiebe K

Wiebusch CH

Wille L

Williams DR

Wissing H

Wolf M

Wood TR

Woschnagg K

Wren S

Xu DL

Xu XW

Xu Y

Yanez JP

Yodh G

Yoshida S

Zoll M

Date

2015

Permanent Link

http://hdl.handle.net/10092/16232

Papers submitted to the 34th International Cosmic Ray Conference (ICRC 2015, The Hague) by the IceCube-Gen2 Collaboration. IceTop is the 1 km2 surface array of the IceCube Neutrino Observatory. Measurements of ground level particles by IceTop have been used for high resolution measurements of the cosmic ray spectrum for energies of 2-500 PeV. Composition has been studied by considering coincident measurements of TeV muon bundles in the 2 km deep IceCube neutrino detector. Including IceTop data for GeV muons may reduce uncertainties inherent to hadronic interaction models; however, all three parts of this program are somewhat limited by the size of IceTop. We explore the potential for IceCube-Gen2 with surface components (IceTop-2, "veto") to improve the cosmic ray science program. The increased area would permit a factor of ∼ 3 increase in energy range for the spectral measurement, a factor of 50 increase in coincident data, and enable lateral and production depth muon measurements for every event.

Subjects

astro-ph.IM

astro-ph.HE

physics.ins-det

Field of Research::02 - Physical Sciences::0201 - Astronomical and Space Sciences::020106 - High Energy Astrophysics; Cosmic Rays

Field of Research::02 - Physical Sciences::0201 - Astronomical and Space Sciences::020102 - Astronomical and Space Instrumentation

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