Search for High-energy Neutrinos from Ultraluminous Infrared Galaxies with IceCube
Ultraluminous infrared galaxies (ULIRGs) have infrared luminosities LIR � 1012Le, making them the most luminous objects in the infrared sky. These dusty objects are generally powered by starbursts with star formation rates that exceed 100 Me yr?1 , possibly combined with a contribution from an activ...
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ftatlantaucrada:oai:radar.auctr.edu:cau.ir_2021_japaridze_george_abbasi_etal_2 2023-07-02T03:33:44+02:00 Search for High-energy Neutrinos from Ultraluminous Infrared Galaxies with IceCube Japaridze, George, Clark Atlanta University (Author) IceCube collaboration (Author) 2020-2029 application/pdf https://hdl.handle.net/20.500.12322/cau.ir:2021_japaridze_george_abbasi_etal_2 https://radar.auctr.edu/islandora/object/cau.ir%3A2021_japaridze_george_abbasi_etal_2/datastream/TN/view/Search%20for%20High-energy%20Neutrinos%20from%20Ultraluminous%20Infrared%20Galaxies%20with%20IceCube.jpg eng eng http://rightsstatements.org/vocab/InC-EDU/1.0/ The Astrophysical Journal Clark Atlanta University Text ftatlantaucrada https://doi.org/20.500.12322/cau.ir:2021_japaridze_george_abbasi_etal_2 2023-06-13T18:53:12Z Ultraluminous infrared galaxies (ULIRGs) have infrared luminosities LIR � 1012Le, making them the most luminous objects in the infrared sky. These dusty objects are generally powered by starbursts with star formation rates that exceed 100 Me yr?1 , possibly combined with a contribution from an active galactic nucleus. Such environments make ULIRGs plausible sources of astrophysical high-energy neutrinos, which can be observed by the IceCube Neutrino Observatory at the South Pole. We present a stacking search for high-energy neutrinos from a representative sample of 75 ULIRGs with redshift z � 0.13 using 7.5 yr of IceCube data. The results are consistent with a background-only observation, yielding upper limits on the neutrino flux from these 75 ULIRGs. For an unbroken E?2.5 power-law spectrum, we report an upper limit on the stacked flux ( ) � 3.24 10 TeV cm s 10 TeV E F= � 90% 14 1 2 1 2.5 n n + - - -- - m m at 90% confidence level. In addition, we constrain the contribution of the ULIRG source population to the observed diffuse astrophysical neutrino flux as well as model predictions. Text South pole RADAR - Repository of AUC Digital collections, Archives, and Research (Atlanta University Center, Robert W. Woodruff Library) South Pole |
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RADAR - Repository of AUC Digital collections, Archives, and Research (Atlanta University Center, Robert W. Woodruff Library) |
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English |
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Clark Atlanta University |
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Clark Atlanta University Search for High-energy Neutrinos from Ultraluminous Infrared Galaxies with IceCube |
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Clark Atlanta University |
description |
Ultraluminous infrared galaxies (ULIRGs) have infrared luminosities LIR � 1012Le, making them the most luminous objects in the infrared sky. These dusty objects are generally powered by starbursts with star formation rates that exceed 100 Me yr?1 , possibly combined with a contribution from an active galactic nucleus. Such environments make ULIRGs plausible sources of astrophysical high-energy neutrinos, which can be observed by the IceCube Neutrino Observatory at the South Pole. We present a stacking search for high-energy neutrinos from a representative sample of 75 ULIRGs with redshift z � 0.13 using 7.5 yr of IceCube data. The results are consistent with a background-only observation, yielding upper limits on the neutrino flux from these 75 ULIRGs. For an unbroken E?2.5 power-law spectrum, we report an upper limit on the stacked flux ( ) � 3.24 10 TeV cm s 10 TeV E F= � 90% 14 1 2 1 2.5 n n + - - -- - m m at 90% confidence level. In addition, we constrain the contribution of the ULIRG source population to the observed diffuse astrophysical neutrino flux as well as model predictions. |
author2 |
Japaridze, George, Clark Atlanta University (Author) IceCube collaboration (Author) |
format |
Text |
title |
Search for High-energy Neutrinos from Ultraluminous Infrared Galaxies with IceCube |
title_short |
Search for High-energy Neutrinos from Ultraluminous Infrared Galaxies with IceCube |
title_full |
Search for High-energy Neutrinos from Ultraluminous Infrared Galaxies with IceCube |
title_fullStr |
Search for High-energy Neutrinos from Ultraluminous Infrared Galaxies with IceCube |
title_full_unstemmed |
Search for High-energy Neutrinos from Ultraluminous Infrared Galaxies with IceCube |
title_sort |
search for high-energy neutrinos from ultraluminous infrared galaxies with icecube |
url |
https://hdl.handle.net/20.500.12322/cau.ir:2021_japaridze_george_abbasi_etal_2 https://radar.auctr.edu/islandora/object/cau.ir%3A2021_japaridze_george_abbasi_etal_2/datastream/TN/view/Search%20for%20High-energy%20Neutrinos%20from%20Ultraluminous%20Infrared%20Galaxies%20with%20IceCube.jpg |
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2020-2029 |
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South Pole |
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South Pole |
genre |
South pole |
genre_facet |
South pole |
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The Astrophysical Journal |
op_rights |
http://rightsstatements.org/vocab/InC-EDU/1.0/ |
op_doi |
https://doi.org/20.500.12322/cau.ir:2021_japaridze_george_abbasi_etal_2 |
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1770273803915493376 |