2021
DOI: 10.1088/1475-7516/2021/01/057
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Abstract: A deep survey of the Large Magellanic Cloud at ∼ 0.1−100 TeV photon energies with the Cherenkov Telescope Array is planned. We assess the detection prospects based on a model for the emission of the galaxy, comprising the four known TeV emitters, mock populations of sources, and interstellar emission on galactic scales. We also assess the detectability of 30 Doradus and SN 1987A, and the constraints that can be derived on the nature of dark matter. The survey will allow for fine spectral studies of N 157B, N 1… Show more

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Cited by 90 publications
(134 citation statements)
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References 373 publications
(523 reference statements)
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“…In the future, the Cherenkov Telescope Array (CTA) observatory will start probing thermal dark matter in the TeV mass range through observations of the Galactic Center. Assuming an Einasto dark matter profile, the expected sensitivity [77] for thermal dark matter candidates is in the range 400 GeV m 1 10 TeV. CTA will thus be able to probe a large part of the parameter space relevant for the dark matter models presented in this work.…”
Section: Jhep02(2021)091mentioning
confidence: 97%
See 1 more Smart Citation
“…In the future, the Cherenkov Telescope Array (CTA) observatory will start probing thermal dark matter in the TeV mass range through observations of the Galactic Center. Assuming an Einasto dark matter profile, the expected sensitivity [77] for thermal dark matter candidates is in the range 400 GeV m 1 10 TeV. CTA will thus be able to probe a large part of the parameter space relevant for the dark matter models presented in this work.…”
Section: Jhep02(2021)091mentioning
confidence: 97%
“…The dashed blue curves in the plots show the expected reach of a proton-proton FCC operating at a 100 TeV center-of-mass energy with 20 ab −1 of integrated luminosity, and have been obtained by performing a naive rescaling of the expected LHC exclusions with the Collider Reach β tool [97]. Similarly, the yellow dashed lines show the projected sensitivity of the CTA observatory from the observation of the Galactic Center [77]. Although points with the highest values of m 3 and an inverted hierarchy will remain inaccessible, most of the parameter space can be probed both by a 100 TeV collider and by future observations of the Galactic Center by CTA.…”
Section: Jhep02(2021)091mentioning
confidence: 99%
“…In both panels we show the constraints from the CMB measurements by the Planck collaboration [1], recasted using [55], the limits from the joint analysis of the gammaray flux from dwarf spheroidal galaxies (dSphs) performed by Fermi-LAT and MAGIC collaborations [52] and the prospects for CTA [53]. All these limits need to be taken as The results of the scan showing the points that correspond to Ωh 2 = 0.12 ± 0.012 with the superimposed indirect detection limits.…”
Section: Jhep06(2021)026mentioning
confidence: 99%
“…figure 4 while the empty ones are beyond these prospects. The existing limits from Planck measurements of the CMB [1] (light brown) and Fermi-LAT+MAGIC combined analysis of the gamma-ray observations of dSphs [52] (orange) are shown as shaded regions, while the dashed red line gives the projected sensitivity of the CTA for the bb channel [53]. Left: points with dominant semi-annihilation σv χχ→χφ > σv χχ→ φφ projected onto the (m χ , σv χχ→χφ ) plane.…”
Section: Jhep06(2021)026mentioning
confidence: 99%
“…We will use data from the current Fermi-LAT [13], H.E.S.S. [14] experiments, and also the prospects for the Southern telescopes CTA [15] and SWGO [16]. This proceeding is structured as follows: in Section 2, we will discuss the secluded setup, in Section 3, we will explore how to compute gamma-ray flux for DM particles in a secluded sector.…”
Section: Introductionmentioning
confidence: 99%