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000625890 088__ $$2arXiv$$aarXiv:2407.16518
000625890 1001_ $$aAcharyya, A.$$b0
000625890 245__ $$aIndirect search for dark matter with a combined analysis of dwarf spheroidal galaxies from VERITAS
000625890 260__ $$aRidge, NY$$bAmerican Physical Society$$c2024
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000625890 520__ $$aUnderstanding the nature and identity of dark matter is a key goal in the physics community. In the case that TeV-scale dark matter particles decay or annihilate into Standard Model particles, very-high-energy (VHE) gamma rays (greater than 100 GeV) will be present in the final state. The Very Energetic Radiation Imaging Telescope Array System (VERITAS) is an imaging atmospheric Cherenkov telescope array that can indirectly detect VHE gamma rays in an energy range of 100 GeV to >30 TeV. Dwarf spheroidal galaxies (dSphs) are ideal candidates in the search for dark matter due to their high dark matter content, high mass-to-light ratios, and their low gamma-ray fluxes from astrophysical processes. This study uses a legacy dataset of 638 h collected on 17 dSphs, built over 11 years with an observing strategy optimized according to the dark matter content of the targets. The study addresses a broad dark matter particle mass range, extending from 200 GeV to 30 PeV. In the absence of a detection, we set the upper limits on the dark matter velocity-weighted annihilation cross section.
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000625890 693__ $$0EXP:(DE-H253)VERITAS-20170101$$5EXP:(DE-H253)VERITAS-20170101$$eVery Energetic Radiation Imaging Telescope Array System$$x0
000625890 7001_ $$aAdams, C. B.$$b1
000625890 7001_ $$aBangale, P.$$b2
000625890 7001_ $$aBartkoske, J. T.$$b3
000625890 7001_ $$aBatista, P.$$b4
000625890 7001_ $$aBenbow, W.$$b5
000625890 7001_ $$aChristiansen, J. L.$$b6
000625890 7001_ $$aChromey, A. J.$$b7
000625890 7001_ $$aDuerr, A.$$b8
000625890 7001_ $$aErrando, M.$$b9
000625890 7001_ $$aFalcone, A.$$b10
000625890 7001_ $$aFeng, Q.$$b11
000625890 7001_ $$aFoote, G. M.$$b12
000625890 7001_ $$aFortson, L.$$b13
000625890 7001_ $$aFurniss, A.$$b14
000625890 7001_ $$aHanlon, W.$$b15
000625890 7001_ $$aHanna, D.$$b16
000625890 7001_ $$aHervet, O.$$b17
000625890 7001_ $$aHinrichs, C. E.$$b18
000625890 7001_ $$aHolder, J.$$b19
000625890 7001_ $$aHumensky, T. B.$$b20
000625890 7001_ $$aJin, W.$$b21
000625890 7001_ $$aJohnson, M. N.$$b22
000625890 7001_ $$aKaaret, P.$$b23
000625890 7001_ $$aKertzman, M.$$b24
000625890 7001_ $$aKieda, D.$$b25
000625890 7001_ $$0P:(DE-H253)PIP1093214$$aKleiner, Tobias Kai$$b26
000625890 7001_ $$0P:(DE-H253)PIP1104085$$aKorzoun, N.$$b27
000625890 7001_ $$aKumar, S.$$b28
000625890 7001_ $$aLang, M. J.$$b29
000625890 7001_ $$aLundy, M.$$b30
000625890 7001_ $$aMaier, G.$$b31
000625890 7001_ $$00000-0003-4427-6490$$aMcGrath, C. E.$$b32$$eCorresponding author
000625890 7001_ $$aMillard, M. J.$$b33
000625890 7001_ $$aMooney, C. L.$$b34
000625890 7001_ $$aMoriarty, P.$$b35
000625890 7001_ $$aMukherjee, R.$$b36
000625890 7001_ $$aNing, W.$$b37
000625890 7001_ $$aO’Brien, S.$$b38
000625890 7001_ $$aOng, R. A.$$b39
000625890 7001_ $$aPark, N.$$b40
000625890 7001_ $$aPohl, M.$$b41
000625890 7001_ $$aPueschel, E.$$b42
000625890 7001_ $$aQuinn, J.$$b43
000625890 7001_ $$aRabinowitz, P. L.$$b44
000625890 7001_ $$aRagan, K.$$b45
000625890 7001_ $$aReynolds, P. T.$$b46
000625890 7001_ $$aRibeiro, D.$$b47
000625890 7001_ $$aRoache, E.$$b48
000625890 7001_ $$aRyan, J. L.$$b49
000625890 7001_ $$0P:(DE-H253)PIP1006066$$aSadeh, I.$$b50$$udesy
000625890 7001_ $$aSaha, L.$$b51
000625890 7001_ $$aSembroski, G. H.$$b52
000625890 7001_ $$aShang, R.$$b53
000625890 7001_ $$aSplettstoesser, M.$$b54
000625890 7001_ $$aTak, D.$$b55
000625890 7001_ $$aTalluri, A. K.$$b56
000625890 7001_ $$aTucci, J. V.$$b57
000625890 7001_ $$aVassiliev, V. V.$$b58
000625890 7001_ $$aWeinstein, A.$$b59
000625890 7001_ $$aWilliams, D. A.$$b60
000625890 7001_ $$aWong, S. L.$$b61
000625890 773__ $$0PERI:(DE-600)2844732-3$$a10.1103/PhysRevD.110.063034$$gVol. 110, no. 6, p. 063034$$n6$$p063034$$tPhysical review / D$$v110$$x2470-0010$$y2024
000625890 7870_ $$0PUBDB-2025-01478$$aAcharyya, A. et.al.$$d2024$$iIsParent$$rarXiv:2407.16518$$tIndirect search for dark matter with a combined analysis of dwarf spheroidal galaxies from VERITAS
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