Testing high energy neutrino emission from the Fermi Gamma-ray Space Telescope Large Area Telescope (4LAC) sources
The detection of the high-energy neutrino IC-170922A in spatial (within the error region) and temporal flare activity correlation with the blazar TXS 0506+056 allowed these objects to be considered as progenitor sources of neutrinos. Besides this, no more detection of this kind was reported. Some ot...
Gespeichert in:
Hauptverfasser: | , , , , , |
---|---|
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext bestellen |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | |
---|---|
container_issue | |
container_start_page | |
container_title | |
container_volume | |
creator | Galván, Antonio Fraija, Nissim Aguilar-Ruiz, Edilberto Joshi, Jagdish C Onsurbe, Jose Antonio de Diego Marinelli, Antonio |
description | The detection of the high-energy neutrino IC-170922A in spatial (within the
error region) and temporal flare activity correlation with the blazar TXS
0506+056 allowed these objects to be considered as progenitor sources of
neutrinos. Besides this, no more detection of this kind was reported. Some
other neutrinos detected by IceCube show a spatial correlation (within the
error region) from other Fermi-LAT detected sources. However, these objects did
not show a flare activity like TXS 0506+056. Assuming a lepto-hadronic scenario
through p$\gamma$ interactions, this work describes the SED in some objects
from the fourth catalog of active galactic nuclei (AGNs) detected by the Fermi
Gamma-ray Space Telescope Large Area Telescope (4LAC) sources, which are in
spatial correlation with neutrinos detected by IceCube. Additionally, we
estimate the corresponding neutrino flux counterpart from these sources. |
doi_str_mv | 10.48550/arxiv.2109.04088 |
format | Article |
fullrecord | <record><control><sourceid>arxiv_GOX</sourceid><recordid>TN_cdi_arxiv_primary_2109_04088</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2109_04088</sourcerecordid><originalsourceid>FETCH-LOGICAL-a678-4e78b6b1da4495125df9842ba50e140bf255d4fb29a123f7f314880fd98a7a53</originalsourceid><addsrcrecordid>eNpNzzFPhDAYxnEWB3P6AZx8Rx3AtrRHGQnxThMSh2MnL_AWmlyBtJyRb288HZye5D88yS-KHjhLpFaKvaD_sp-J4CxPmGRa30a-prDaaYDRDiPQRH7YYKLL6u00Azkbgp0nMH52sI4EB_LOwhGdw9jjBqcFO4KazhS6eSGo0A8EhSf8F59kVZTPEOaL7yjcRTcGz4Hu_3YXnQ6vdfkWVx_H97KoYtxnOpaU6Xbf8h6lzBUXqje5lqJFxYhL1hqhVC9NK3LkIjWZSbnUmpk-15ihSnfR4-_r1dws3jr0W_Njb6729Bukd1Rl</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Testing high energy neutrino emission from the Fermi Gamma-ray Space Telescope Large Area Telescope (4LAC) sources</title><source>arXiv.org</source><creator>Galván, Antonio ; Fraija, Nissim ; Aguilar-Ruiz, Edilberto ; Joshi, Jagdish C ; Onsurbe, Jose Antonio de Diego ; Marinelli, Antonio</creator><creatorcontrib>Galván, Antonio ; Fraija, Nissim ; Aguilar-Ruiz, Edilberto ; Joshi, Jagdish C ; Onsurbe, Jose Antonio de Diego ; Marinelli, Antonio</creatorcontrib><description>The detection of the high-energy neutrino IC-170922A in spatial (within the
error region) and temporal flare activity correlation with the blazar TXS
0506+056 allowed these objects to be considered as progenitor sources of
neutrinos. Besides this, no more detection of this kind was reported. Some
other neutrinos detected by IceCube show a spatial correlation (within the
error region) from other Fermi-LAT detected sources. However, these objects did
not show a flare activity like TXS 0506+056. Assuming a lepto-hadronic scenario
through p$\gamma$ interactions, this work describes the SED in some objects
from the fourth catalog of active galactic nuclei (AGNs) detected by the Fermi
Gamma-ray Space Telescope Large Area Telescope (4LAC) sources, which are in
spatial correlation with neutrinos detected by IceCube. Additionally, we
estimate the corresponding neutrino flux counterpart from these sources.</description><identifier>DOI: 10.48550/arxiv.2109.04088</identifier><language>eng</language><subject>Physics - High Energy Astrophysical Phenomena</subject><creationdate>2021-09</creationdate><rights>http://creativecommons.org/licenses/by/4.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,776,881</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/2109.04088$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.2109.04088$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Galván, Antonio</creatorcontrib><creatorcontrib>Fraija, Nissim</creatorcontrib><creatorcontrib>Aguilar-Ruiz, Edilberto</creatorcontrib><creatorcontrib>Joshi, Jagdish C</creatorcontrib><creatorcontrib>Onsurbe, Jose Antonio de Diego</creatorcontrib><creatorcontrib>Marinelli, Antonio</creatorcontrib><title>Testing high energy neutrino emission from the Fermi Gamma-ray Space Telescope Large Area Telescope (4LAC) sources</title><description>The detection of the high-energy neutrino IC-170922A in spatial (within the
error region) and temporal flare activity correlation with the blazar TXS
0506+056 allowed these objects to be considered as progenitor sources of
neutrinos. Besides this, no more detection of this kind was reported. Some
other neutrinos detected by IceCube show a spatial correlation (within the
error region) from other Fermi-LAT detected sources. However, these objects did
not show a flare activity like TXS 0506+056. Assuming a lepto-hadronic scenario
through p$\gamma$ interactions, this work describes the SED in some objects
from the fourth catalog of active galactic nuclei (AGNs) detected by the Fermi
Gamma-ray Space Telescope Large Area Telescope (4LAC) sources, which are in
spatial correlation with neutrinos detected by IceCube. Additionally, we
estimate the corresponding neutrino flux counterpart from these sources.</description><subject>Physics - High Energy Astrophysical Phenomena</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2021</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNpNzzFPhDAYxnEWB3P6AZx8Rx3AtrRHGQnxThMSh2MnL_AWmlyBtJyRb288HZye5D88yS-KHjhLpFaKvaD_sp-J4CxPmGRa30a-prDaaYDRDiPQRH7YYKLL6u00Azkbgp0nMH52sI4EB_LOwhGdw9jjBqcFO4KazhS6eSGo0A8EhSf8F59kVZTPEOaL7yjcRTcGz4Hu_3YXnQ6vdfkWVx_H97KoYtxnOpaU6Xbf8h6lzBUXqje5lqJFxYhL1hqhVC9NK3LkIjWZSbnUmpk-15ihSnfR4-_r1dws3jr0W_Njb6729Bukd1Rl</recordid><startdate>20210909</startdate><enddate>20210909</enddate><creator>Galván, Antonio</creator><creator>Fraija, Nissim</creator><creator>Aguilar-Ruiz, Edilberto</creator><creator>Joshi, Jagdish C</creator><creator>Onsurbe, Jose Antonio de Diego</creator><creator>Marinelli, Antonio</creator><scope>GOX</scope></search><sort><creationdate>20210909</creationdate><title>Testing high energy neutrino emission from the Fermi Gamma-ray Space Telescope Large Area Telescope (4LAC) sources</title><author>Galván, Antonio ; Fraija, Nissim ; Aguilar-Ruiz, Edilberto ; Joshi, Jagdish C ; Onsurbe, Jose Antonio de Diego ; Marinelli, Antonio</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a678-4e78b6b1da4495125df9842ba50e140bf255d4fb29a123f7f314880fd98a7a53</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2021</creationdate><topic>Physics - High Energy Astrophysical Phenomena</topic><toplevel>online_resources</toplevel><creatorcontrib>Galván, Antonio</creatorcontrib><creatorcontrib>Fraija, Nissim</creatorcontrib><creatorcontrib>Aguilar-Ruiz, Edilberto</creatorcontrib><creatorcontrib>Joshi, Jagdish C</creatorcontrib><creatorcontrib>Onsurbe, Jose Antonio de Diego</creatorcontrib><creatorcontrib>Marinelli, Antonio</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Galván, Antonio</au><au>Fraija, Nissim</au><au>Aguilar-Ruiz, Edilberto</au><au>Joshi, Jagdish C</au><au>Onsurbe, Jose Antonio de Diego</au><au>Marinelli, Antonio</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Testing high energy neutrino emission from the Fermi Gamma-ray Space Telescope Large Area Telescope (4LAC) sources</atitle><date>2021-09-09</date><risdate>2021</risdate><abstract>The detection of the high-energy neutrino IC-170922A in spatial (within the
error region) and temporal flare activity correlation with the blazar TXS
0506+056 allowed these objects to be considered as progenitor sources of
neutrinos. Besides this, no more detection of this kind was reported. Some
other neutrinos detected by IceCube show a spatial correlation (within the
error region) from other Fermi-LAT detected sources. However, these objects did
not show a flare activity like TXS 0506+056. Assuming a lepto-hadronic scenario
through p$\gamma$ interactions, this work describes the SED in some objects
from the fourth catalog of active galactic nuclei (AGNs) detected by the Fermi
Gamma-ray Space Telescope Large Area Telescope (4LAC) sources, which are in
spatial correlation with neutrinos detected by IceCube. Additionally, we
estimate the corresponding neutrino flux counterpart from these sources.</abstract><doi>10.48550/arxiv.2109.04088</doi><oa>free_for_read</oa></addata></record> |
fulltext | fulltext_linktorsrc |
identifier | DOI: 10.48550/arxiv.2109.04088 |
ispartof | |
issn | |
language | eng |
recordid | cdi_arxiv_primary_2109_04088 |
source | arXiv.org |
subjects | Physics - High Energy Astrophysical Phenomena |
title | Testing high energy neutrino emission from the Fermi Gamma-ray Space Telescope Large Area Telescope (4LAC) sources |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-28T02%3A25%3A40IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-arxiv_GOX&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Testing%20high%20energy%20neutrino%20emission%20from%20the%20Fermi%20Gamma-ray%20Space%20Telescope%20Large%20Area%20Telescope%20(4LAC)%20sources&rft.au=Galv%C3%A1n,%20Antonio&rft.date=2021-09-09&rft_id=info:doi/10.48550/arxiv.2109.04088&rft_dat=%3Carxiv_GOX%3E2109_04088%3C/arxiv_GOX%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true |