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000626526 005__ 20250427135835.0
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000626526 0247_ $$2arXiv$$aarXiv:2407.16518
000626526 0247_ $$2altmetric$$aaltmetric:165612337
000626526 037__ $$aPUBDB-2025-01478
000626526 041__ $$aEnglish
000626526 088__ $$2arXiv$$aarXiv:2407.16518
000626526 082__ $$a530
000626526 1001_ $$aAcharyya, A.$$b0
000626526 245__ $$aIndirect search for dark matter with a combined analysis of dwarf spheroidal galaxies from VERITAS
000626526 260__ $$c2024
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000626526 500__ $$a18 pages, 7 figures, 3 tables, accepted in PRD
000626526 520__ $$aUnderstanding the nature and identity of dark matter is a key goal in the physics community. In the case that TeV-scale dark matter particles decay or annihilate into Standard Model particles, very-high-energy (VHE) gamma rays (greater than 100 GeV) will be present in the final state. The Very Energetic Radiation Imaging Telescope Array System (VERITAS) is an imaging atmospheric Cherenkov telescope array that can indirectly detect VHE gamma rays in an energy range of 100 GeV to >30 TeV. Dwarf spheroidal galaxies (dSphs) are ideal candidates in the search for dark matter due to their high dark matter content, high mass-to-light ratios, and their low gamma-ray fluxes from astrophysical processes. This study uses a legacy dataset of 638 h collected on 17 dSphs, built over 11 years with an observing strategy optimized according to the dark matter content of the targets. The study addresses a broad dark matter particle mass range, extending from 200 GeV to 30 PeV. In the absence of a detection, we set the upper limits on the dark matter velocity-weighted annihilation cross section.
000626526 536__ $$0G:(DE-HGF)POF4-613$$a613 - Matter and Radiation from the Universe (POF4-613)$$cPOF4-613$$fPOF IV$$x0
000626526 588__ $$aDataset connected to CrossRef, INSPIRE, Journals: bib-pubdb1.desy.de
000626526 693__ $$0EXP:(DE-H253)VERITAS-20170101$$5EXP:(DE-H253)VERITAS-20170101$$eVery Energetic Radiation Imaging Telescope Array System$$x0
000626526 7001_ $$aAdams, C. B.$$b1
000626526 7001_ $$aBangale, P.$$b2
000626526 7001_ $$aBartkoske, J. T.$$b3
000626526 7001_ $$0P:(DE-HGF)0$$aBatista, P.$$b4
000626526 7001_ $$aBenbow, W.$$b5
000626526 7001_ $$aChristiansen, J. L.$$b6
000626526 7001_ $$aChromey, A. J.$$b7
000626526 7001_ $$aDuerr, A.$$b8
000626526 7001_ $$aErrando, M.$$b9
000626526 7001_ $$aFalcone, A.$$b10
000626526 7001_ $$aFeng, Q.$$b11
000626526 7001_ $$aFoote, G. M.$$b12
000626526 7001_ $$aFortson, L.$$b13
000626526 7001_ $$aFurniss, A.$$b14
000626526 7001_ $$aHanlon, W.$$b15
000626526 7001_ $$aHanna, D.$$b16
000626526 7001_ $$aHervet, O.$$b17
000626526 7001_ $$aHinrichs, C. E.$$b18
000626526 7001_ $$aHolder, J.$$b19
000626526 7001_ $$aHumensky, T. B.$$b20
000626526 7001_ $$aJin, W.$$b21
000626526 7001_ $$aJohnson, M. N.$$b22
000626526 7001_ $$aKaaret, P.$$b23
000626526 7001_ $$aKertzman, M.$$b24
000626526 7001_ $$aKieda, D.$$b25
000626526 7001_ $$0P:(DE-H253)PIP1093214$$aKleiner, T. K.$$b26$$udesy
000626526 7001_ $$0P:(DE-H253)PIP1104085$$aKorzoun, N.$$b27
000626526 7001_ $$aKumar, S.$$b28
000626526 7001_ $$aLang, M. J.$$b29
000626526 7001_ $$aLundy, M.$$b30
000626526 7001_ $$aMaier, G.$$b31
000626526 7001_ $$00000-0003-4427-6490$$aMcGrath, Conor E.$$b32$$eCorresponding author
000626526 7001_ $$aMillard, M. J.$$b33
000626526 7001_ $$aMooney, C. L.$$b34
000626526 7001_ $$aMoriarty, P.$$b35
000626526 7001_ $$aMukherjee, R.$$b36
000626526 7001_ $$aNing, W.$$b37
000626526 7001_ $$aO'Brien, S.$$b38
000626526 7001_ $$aOng, R. A.$$b39
000626526 7001_ $$aPark, N.$$b40
000626526 7001_ $$aPohl, M.$$b41
000626526 7001_ $$aPueschel, E.$$b42
000626526 7001_ $$aQuinn, J.$$b43
000626526 7001_ $$aRabinowitz, P. L.$$b44
000626526 7001_ $$aRagan, K.$$b45
000626526 7001_ $$aReynolds, P. T.$$b46
000626526 7001_ $$aRibeiro, D.$$b47
000626526 7001_ $$aRoache, E.$$b48
000626526 7001_ $$aRyan, J. L.$$b49
000626526 7001_ $$aSadeh, I.$$b50
000626526 7001_ $$aSaha, L.$$b51
000626526 7001_ $$aSembroski, G. H.$$b52
000626526 7001_ $$aShang, R.$$b53
000626526 7001_ $$aSplettstoesser, M.$$b54
000626526 7001_ $$aTak, Donggeun$$b55
000626526 7001_ $$aTalluri, A. K.$$b56
000626526 7001_ $$aTucci, J. V.$$b57
000626526 7001_ $$aVassiliev, V. V.$$b58
000626526 7001_ $$aWeinstein, A.$$b59
000626526 7001_ $$aWilliams, D. A.$$b60
000626526 7001_ $$aWong, S. L.$$b61
000626526 7001_ $$0P:(DE-HGF)0$$aVERITAS Collaboration$$b62$$eCollaboration author
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000626526 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1104085$$aExternal Institute$$b27$$kExtern
000626526 9131_ $$0G:(DE-HGF)POF4-613$$1G:(DE-HGF)POF4-610$$2G:(DE-HGF)POF4-600$$3G:(DE-HGF)POF4$$4G:(DE-HGF)POF$$aDE-HGF$$bForschungsbereich Materie$$lMatter and the Universe$$vMatter and Radiation from the Universe$$x0
000626526 9141_ $$y2024
000626526 915__ $$0StatID:(DE-HGF)0580$$2StatID$$aPublished
000626526 9201_ $$0I:(DE-H253)Z_CTA-20210408$$kZ_CTA$$lCherenkov Telescope Array$$x0
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