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001 | 601583 | ||
005 | 20250715170943.0 | ||
024 | 7 | _ | |a arXiv:2401.06666 |2 arXiv |
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088 | _ | _ | |a arXiv:2401.06666 |2 arXiv |
100 | 1 | _ | |a Garrappa, S. |0 P:(DE-HGF)0 |b 0 |e Corresponding author |
245 | _ | _ | |a $Fermi$-LAT follow-up observations in seven years of realtime high-energy neutrino alerts |
260 | _ | _ | |a Les Ulis |c 2024 |b EDP Sciences |
336 | 7 | _ | |a article |2 DRIVER |
336 | 7 | _ | |a Output Types/Journal article |2 DataCite |
336 | 7 | _ | |a Journal Article |b journal |m journal |0 PUB:(DE-HGF)16 |s 1730207373_2816131 |2 PUB:(DE-HGF) |
336 | 7 | _ | |a ARTICLE |2 BibTeX |
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500 | _ | _ | |a A&A 687, A59 (2024). Published on A&A |
520 | _ | _ | |a The realtime program for high-energy neutrino track events detected by the IceCube South Pole Neutrino Observatory releases alerts to the astronomical community with the goal of identifying electromagnetic counterparts to astrophysical neutrinos. Gamma-ray observations from the $Fermi$-Large Area Telescope (LAT) enabled the identification of the flaring gamma-ray blazar TXS 0506+056 as a likely counterpart to the neutrino event IC-170922A. By continuously monitoring the gamma-ray sky, $Fermi$-LAT plays a key role in the identification of candidate counterparts to realtime neutrino alerts. In this paper, we present the $Fermi$-LAT strategy for following up high-energy neutrino alerts applied to seven years of IceCube data. Right after receiving an alert, a search is performed in order to identify gamma-ray activity from known and newly-detected sources that are positionally consistent with the neutrino localization. In this work, we study the population of blazars found in coincidence with high-energy neutrinos and compare them to the full population of gamma-ray blazars detected by $Fermi$-LAT. We also evaluate the relationship between the neutrino and gamma-ray luminosities, finding different trends between the two blazar classes BL Lacs and flat-spectrum radio quasars. |
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700 | 1 | _ | |a Franckowiak, A. |0 P:(DE-HGF)0 |b 3 |
700 | 1 | _ | |a Liodakis, I. |0 P:(DE-HGF)0 |b 4 |
700 | 1 | _ | |a Bartolini, C. |0 P:(DE-HGF)0 |b 5 |
700 | 1 | _ | |a Giroletti, M. |0 P:(DE-HGF)0 |b 6 |
700 | 1 | _ | |a Nanci, C. |0 P:(DE-HGF)0 |b 7 |
700 | 1 | _ | |a Principe, G. |0 P:(DE-HGF)0 |b 8 |
700 | 1 | _ | |a Venters, T. M. |0 P:(DE-HGF)0 |b 9 |
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773 | _ | _ | |a 10.1051/0004-6361/202449221 |g Vol. 687, p. A59 - |0 PERI:(DE-600)1458466-9 |p A59 |t Astronomy and astrophysics |v 687 |y 2024 |x 0004-6361 |
787 | 0 | _ | |a Garrappa, Simone et.al. |d Les Ulis, 2024 |i IsParent |0 PUBDB-2024-06559 |r arXiv:2401.06666 |t Fermi-LAT follow-up observations in seven years of real-time high-energy neutrino alerts |
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