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@ARTICLE{Acharyya:490354,
author = {Acharyya, A. and Archer, A. and Bangale, P. and Bartkoske,
J. T. and Batista, P. and Baumgart, M. and Benbow, W. and
Buckley, J. H. and Falcone, A. and Feng, Q. and Finley, J.
P. and Foote, G. M. and Fortson, L. and Furniss, A. and
Gallagher, G. and Hanlon, W. F. and Hervet, O. and Hoang, J.
and Holder, J. and Humensky, T. B. and Jin, W. and Kaaret,
P. and Kertzman, M. and Kherlakian, M. and Kieda, D. and
Kleiner, Tobias Kai and Korzoun, N. and Krennrich, F. and
Lang, M. J. and Lundy, M. and Maier, G. and McGrath, C. E.
and Moriarty, P. and O'Brien, S. and Ong, R. A. and Pfrang,
Konstantin Johannes and Pohl, M. and Pueschel, E. and Quinn,
J. and Ragan, K. and Reynolds, P. T. and Roache, E. and
Rodd, N. L. and Ryan, J. L. and Sadeh, I. and Saha, L. and
Santander, M. and Sembroski, G. H. and Shang, R. and
Splettstoesser, M. and Tak, Donggeun and Tucci, J. V. and
Vassiliev, V. V. and Williams, D. A.},
title = {{S}earch for {U}ltraheavy {D}ark {M}atter from
{O}bservations of {D}warf {S}pheroidal {G}alaxies with
{VERITAS}},
journal = {The astrophysical journal / 1},
volume = {945},
number = {2},
issn = {0004-637X},
address = {London},
publisher = {Institute of Physics Publ.},
reportid = {PUBDB-2022-07671, arXiv:2302.08784},
pages = {101},
year = {2023},
note = {10 pages, 7 figures},
abstract = {Dark matter is a key piece of the current cosmological
scenario, with weakly interacting massive particles (WIMPs)
a leading dark matter candidate. WIMPs have not been
detected in their conventional parameter space (100 GeV ≲M
$_{χ}$ ≲ 100 TeV), a mass range accessible with current
Imaging Atmospheric Cherenkov Telescopes. As ultraheavy dark
matter (UHDM; M $_{χ}$ ≳ 100 TeV) has been suggested as
an underexplored alternative to the WIMP paradigm, we search
for an indirect dark matter annihilation signal in a higher
mass range (up to 30 PeV) with the VERITAS γ-ray
observatory. With 216 hr of observations of four dwarf
spheroidal galaxies, we perform an unbinned likelihood
analysis. We find no evidence of a γ-ray signal from UHDM
annihilation above the background fluctuation for any
individual dwarf galaxy nor for a joint-fit analysis, and
consequently constrain the velocity-weighted annihilation
cross section of UHDM for dark matter particle masses
between 1 TeV and 30 PeV. We additionally set constraints on
the allowed radius of a composite UHDM particle.},
keywords = {dark matter: annihilation (INSPIRE) / dark matter: mass
(INSPIRE) / background: fluctuation (INSPIRE) / WIMP
(INSPIRE) / galaxy (INSPIRE) / TeV (INSPIRE) / VERITAS
(INSPIRE) / observatory (INSPIRE) / GeV (INSPIRE) /
composite (INSPIRE) / Cherenkov counter (INSPIRE) / imaging
(INSPIRE) / gamma ray: VHE (INSPIRE)},
cin = {$Z_VER$},
ddc = {520},
cid = {$I:(DE-H253)Z_VER-20210408$},
pnm = {613 - Matter and Radiation from the Universe (POF4-613)},
pid = {G:(DE-HGF)POF4-613},
experiment = {EXP:(DE-H253)VERITAS-20170101},
typ = {PUB:(DE-HGF)16},
eprint = {2302.08784},
howpublished = {arXiv:2302.08784},
archivePrefix = {arXiv},
SLACcitation = {$\%\%CITATION$ = $arXiv:2302.08784;\%\%$},
UT = {WOS:000950838900001},
doi = {10.3847/1538-4357/acbc7b},
url = {https://bib-pubdb1.desy.de/record/490354},
}