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@ARTICLE{Kherlakian:482415,
author = {Kherlakian, Maria Carolina},
collaboration = {{VERITAS Collaboration}},
title = {{G}amma-ray {F}ollow-up {O}bservations of {D}warf {N}ova
{AT}2021afpi as a {P}ossible {N}eutrino {C}ounterpart with
the {VERITAS} {I}nstrument},
journal = {Acta physica Polonica / B / Proceedings supplement},
volume = {15},
number = {3},
issn = {1899-2358},
address = {Cracow},
publisher = {Inst. of Physics, Jagellonian Univ.},
reportid = {PUBDB-2022-04764},
pages = {A26.1 - A26.6},
year = {2022},
abstract = {AT2021afpi was a 10 mag outburst seen by the MASTER-Tavrida
autodetection system in temporal coincidence with the
astrophysical neutrino candidate IC211125A. The object was
observed as an optical bright transient, initially
classified as a classical nova. Follow-up observations by
the VERITAS instrument at gamma-ray energies > 100 GeV on
the nova location resulted in no detection for an exposure
of 5.5 hours. Further spectroscopic reports reclassified
AT2021afpi as a dwarf nova of the type WZ Sge-Type, which
are not expected to be neutrino emitters. A possible blazar
detected by Fermi-LAT, 4FGL J0248.0+2232, which lies within
the $90\%$ localisation region of IC211125A, was observed in
a flaring radio state four days after the neutrino alert. A
further combined analysis with 1 hour of exposure time on
4FGL J0248.0+2232 at the position of AT2021afpi still
resulted in no detection.},
month = {Jan},
date = {2022-01-10},
organization = {28th Cracow EPIPHANY Conference on
Recent Advances in Astroparticle
Physics, Cracow (Poland), 10 Jan 2022 -
14 Jan 2022},
keywords = {gamma ray (INSPIRE) / VERITAS (INSPIRE)},
cin = {ZEU-CTA},
ddc = {530},
cid = {I:(DE-H253)ZEU-CTA-20120731},
pnm = {613 - Matter and Radiation from the Universe (POF4-613)},
pid = {G:(DE-HGF)POF4-613},
experiment = {EXP:(DE-H253)CTA-20150101},
typ = {PUB:(DE-HGF)8 / PUB:(DE-HGF)16},
doi = {10.5506/APhysPolBSupp.15.3-A26},
url = {https://bib-pubdb1.desy.de/record/482415},
}