2023
DOI: 10.1103/physrevd.107.043028
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Toward the ultimate reach of current imaging atmospheric Cherenkov telescopes and their sensitivity to TeV dark matter

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Cited by 9 publications
(4 citation statements)
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“…We will make use of the SA100 (R12) model as a model for the GDE predictions with GALPROP extracted from ref. [61]. A detailed study of the GDE impact on the sensitivities to sub-GeV DM is out of the scope of the present paper, however, we will show how much the sensitivity can be improved when the GDE is subtracted from the measured residual background for the H.E.S.S.-like and CTA observations.…”
Section: Jcap07(2024)012mentioning
confidence: 83%
See 1 more Smart Citation
“…We will make use of the SA100 (R12) model as a model for the GDE predictions with GALPROP extracted from ref. [61]. A detailed study of the GDE impact on the sensitivities to sub-GeV DM is out of the scope of the present paper, however, we will show how much the sensitivity can be improved when the GDE is subtracted from the measured residual background for the H.E.S.S.-like and CTA observations.…”
Section: Jcap07(2024)012mentioning
confidence: 83%
“…We warmly thank Alessandro Montanari for providing GDE emission fits data of figures 3 and 4 of ref. [61] for the SA10 (R12) model. This work was conducted in the context of the CTA Consortium 2 and the SWGO Collaboration.…”
Section: Acknowledgmentsmentioning
confidence: 99%
“…To perform the fits, the expected annihilation gamma-ray signal dN/dE given by [63,64] is convoluted to a Gaussian distribution (with σ/E = 0.10) to take into account the energy resolution of the H.E.S.S. telescope [49]. VIR.…”
Section: Methodsmentioning
confidence: 99%
“…Despite the benchmark approach in DM indirect searches, which aims to set constraints on the DM annihilation cross-section by selecting a couple of possible (typically, one core and one cusp) DM density distribution profiles (see e.g. [49,50]), our main focus is to set constraints on the DM density profile within in a radius of 450 pc from the GC, by assuming a thermal DM candidate which could explain the gamma-ray spectra detected by H.E.S.S. in the inner 15 pc of the Galaxy [17,18].…”
Section: Introductionmentioning
confidence: 99%