C Farnier
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Explore the profile of C Farnier including associated specialties, affiliations and a list of published articles.
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26
Citations
182
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Recent Articles
1.
Abdallah H, Abramowski A, Aharonian F, Benkhali F, Anguner E, Arakawa M, et al.
Phys Rev Lett
. 2018 Jun;
120(20):201101.
PMID: 29864326
Spectral lines are among the most powerful signatures for dark matter (DM) annihilation searches in very-high-energy γ rays. The central region of the Milky Way halo is one of the...
2.
Abdalla H, Abramowski A, Aharonian F, Benkhali F, Akhperjanian A, Andersson T, et al.
Phys Rev Lett
. 2016 Oct;
117(15):151302.
PMID: 27768338
Results: No significant excess associated with dark matter annihilations was found in the energy range of 100 GeV to 2 TeV and upper limits on the gamma-ray flux and the...
3.
Abdallah H, Abramowski A, Aharonian F, Benkhali F, Akhperjanian A, Anguner E, et al.
Phys Rev Lett
. 2016 Sep;
117(11):111301.
PMID: 27661677
The inner region of the Milky Way halo harbors a large amount of dark matter (DM). Given its proximity, it is one of the most promising targets to look for...
4.
Abramowski A, Aharonian F, Benkhali F, Akhperjanian A, Anguner E, Backes M, et al.
Phys Rev Lett
. 2015 Mar;
114(8):081301.
PMID: 25768750
An annihilation signal of dark matter is searched for from the central region of the Milky Way. Data acquired in dedicated on-off observations of the Galactic center region with H.E.S.S....
5.
Abramowski A, Acero F, Aharonian F, Akhperjanian A, Anton G, Balenderan S, et al.
Phys Rev Lett
. 2014 Aug;
110(4):041301.
PMID: 25166149
Gamma-ray line signatures can be expected in the very-high-energy (E(γ)>100 GeV) domain due to self-annihilation or decay of dark matter (DM) particles in space. Such a signal would be readily...
6.
Abramowski A, Acero F, Aharonian F, Akhperjanian A, Anton G, Barnacka A, et al.
Phys Rev Lett
. 2011 May;
106(16):161301.
PMID: 21599352
A search for a very-high-energy (VHE; ≥100 GeV) γ-ray signal from self-annihilating particle dark matter (DM) is performed towards a region of projected distance r∼45-150 pc from the Galactic center....
7.
Abdo A, Ackermann M, Ajello M, Atwood W, Baldini L, Ballet J, et al.
Phys Rev Lett
. 2010 Apr;
104(9):091302.
PMID: 20366979
Dark matter (DM) particle annihilation or decay can produce monochromatic gamma rays readily distinguishable from astrophysical sources. gamma-ray line limits from 30 to 200 GeV obtained from 11 months of...
8.
Abdo A, Ackermann M, Ajello M, Atwood W, Baldini L, Ballet J, et al.
Phys Rev Lett
. 2010 Apr;
104(10):101101.
PMID: 20366411
We report on the first Fermi Large Area Telescope (LAT) measurements of the so-called "extragalactic" diffuse gamma-ray emission (EGB). This component of the diffuse gamma-ray emission is generally considered to...
9.
Abdo A, Ackermann M, Ajello M, Anderson B, Atwood W, Axelsson M, et al.
Phys Rev Lett
. 2010 Apr;
103(25):251101.
PMID: 20366246
The diffuse galactic gamma-ray emission is produced by cosmic rays (CRs) interacting with the interstellar gas and radiation field. Measurements by the Energetic Gamma-Ray Experiment Telescope (EGRET) instrument on the...
10.
Abdo A, Ackermann M, Ajello M, Atwood W, Baldini L, Ballet J, et al.
Science
. 2010 Apr;
328(5979):725-9.
PMID: 20360067
The Fermi Gamma-ray Space Telescope has detected the gamma-ray glow emanating from the giant radio lobes of the radio galaxy Centaurus A. The resolved gamma-ray image shows the lobes clearly...