2022
DOI: 10.1103/physrevlett.129.111101
|View full text |Cite
|
Sign up to set email alerts
|

Search for Dark Matter Annihilation Signals in the H.E.S.S. Inner Galaxy Survey

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1
1

Citation Types

0
31
0

Year Published

2022
2022
2024
2024

Publication Types

Select...
5
4

Relationship

1
8

Authors

Journals

citations
Cited by 43 publications
(31 citation statements)
references
References 36 publications
0
31
0
Order By: Relevance
“…ID" label), where we combine different limits of indirect detection of DM, such as MAGIC and Fermi-LAT observations [182], and H.E.S.S. [183]. We also included bounds from the analysis derived from CMB observations [184], and antiproton AMS-02 data [185].…”
Section: Dark Matter Genesismentioning
confidence: 99%
“…ID" label), where we combine different limits of indirect detection of DM, such as MAGIC and Fermi-LAT observations [182], and H.E.S.S. [183]. We also included bounds from the analysis derived from CMB observations [184], and antiproton AMS-02 data [185].…”
Section: Dark Matter Genesismentioning
confidence: 99%
“…The scaled velocity-weighted cross section can be seen in figure 5. The Fermi-LAT limits from dwarfspheroidal galaxies [70], HESS limits from the Galactic centre [78], and the IceCube and ANTARES [29,30] limits on the resulting neutrino spectra are implemented, and for specific annihilation channels indicated by the solid blue lines in figure 5. In order to be conservative, we do not include the limits on the velocity-weighted annihilation cross section arising from antiproton limits due to large inherent hadronization and propagation uncertainties [19][20][21][22][23][24][25][26][27].…”
Section: Indirect-detection Limitsmentioning
confidence: 99%
“…In this work, we will derive constraints on σv at 95% confidence level which corresponds to a criterion value TS = 2.71, in the case of a one-sided test and following previous γ-ray telescope analyses such as [24,25,42,43]. The total likelihood function L is the product of a Poisson likelihood L P i on the events of all energy bins i with a log-normal distribution L J of the J-factor, which reads…”
Section: Jcap11(2022)055mentioning
confidence: 99%