Sensitivity of the Cherenkov Telescope Array to dark subhalos

Coronado-Blázquez, Javier; Doro, M.; Aguirre-Santaella, Alejandra

doi:10.22323/1.395.0544

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Pos(icrc2021)0471

Prospects For Future Gamma-ray Detectors1

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2021

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“…In fact, the hierarchical formation scenario of the cosmological structures, predicts that a population of dark subhalos should be present in DM halos like that one that hosts our galaxy. At ICRC 2021, the properties and relevance of these substructures for DM searches have been discussed in [4][5][6][7][8][9]. Ref.…”

Section: Pos(icrc2021)047mentioning

confidence: 99%

“…It will cover a wide energy range, from about 20 GeV up to 300 GeV, with an excellent angular resolution, down to arcminute scales. At ICRC 2021, prospects for DM searches with CTA have been discussed focussing on the galactic center region [25], the Perseus cluster of galaxies [26], and DM subhalos [4]. The analysis of [25] assumes a survey of the galactic center region with about 500 hours of observations, and it is based on a template fitting approach, where a series of signal and backgrounds templates are fitted to the (simulated in this case) data.…”

Section: Prospects For Future Gamma-ray Detectorsmentioning

confidence: 99%

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