TY - JOUR
T1 - Search for Dark Matter Annihilation Signals in the H.E.S.S. Inner Galaxy Survey
AU - (H.E.S.S. Collaboration)
AU - Abdalla, H.
AU - Aharonian, F.
AU - Benkhali, F. Ait
AU - Angüner, E. O.
AU - Armand, C.
AU - Ashkar, H.
AU - Backes, M.
AU - Baghmanyan, V.
AU - Martins, V. Barbosa
AU - Batzofin, R.
AU - Becherini, Y.
AU - Berge, D.
AU - Bernlöhr, K.
AU - Bi, B.
AU - Böttcher, M.
AU - Bolmont, J.
AU - De Lavergne, M. De Bony
AU - Brose, R.
AU - Brun, F.
AU - Cangemi, F.
AU - Caroff, S.
AU - Cerruti, M.
AU - Chand, T.
AU - Chen, A.
AU - Cotter, G.
AU - Mbarubucyeye, J. Damascene
AU - Devin, J.
AU - Djannati-Ataï, A.
AU - Dmytriiev, A.
AU - Doroshenko, V.
AU - Egberts, K.
AU - Fiasson, A.
AU - De Clairfontaine, G. Fichet
AU - Fontaine, G.
AU - Funk, S.
AU - Gabici, S.
AU - Giavitto, G.
AU - Glawion, D.
AU - Glicenstein, J. F.
AU - Grondin, M. H.
AU - Hinton, J. A.
AU - Hofmann, W.
AU - Holch, T. L.
AU - Holler, M.
AU - Horns, D.
AU - Huang, Zhiqiu
AU - Jamrozy, M.
AU - Jankowsky, F.
AU - Kasai, E.
AU - Katarzyński, K.
N1 - Publisher Copyright:
©. Assuming Einasto and Navarro-Frenk-White (NFW) DM density profiles at the GC, these constraints are the strongest obtained so far in the TeV DM mass range. For the Einasto profile, the constraints reach ?σv?
PY - 2022/9/9
Y1 - 2022/9/9
N2 - The central region of the Milky Way is one of the foremost locations to look for dark matter (DM) signatures. We report the first results on a search for DM particle annihilation signals using new observations from an unprecedented γ-ray survey of the Galactic Center (GC) region, i.e., the Inner Galaxy Survey, at very high energies (?100 GeV) performed with the H.E.S.S. array of five ground-based Cherenkov telescopes.
AB - The central region of the Milky Way is one of the foremost locations to look for dark matter (DM) signatures. We report the first results on a search for DM particle annihilation signals using new observations from an unprecedented γ-ray survey of the Galactic Center (GC) region, i.e., the Inner Galaxy Survey, at very high energies (?100 GeV) performed with the H.E.S.S. array of five ground-based Cherenkov telescopes.
U2 - 10.1103/PhysRevLett.129.111101
DO - 10.1103/PhysRevLett.129.111101
M3 - Article
C2 - 36154418
AN - SCOPUS:85138290208
SN - 0031-9007
VL - 129
JO - Physical Review Letters
JF - Physical Review Letters
IS - 11
M1 - 111101
ER -