OBSERVATIONS OF MILKY WAY DWARF SPHEROIDAL GALAXIES WITH THE FERMI-LARGE AREA TELESCOPE DETECTOR AND CONSTRAINTS ON DARK MATTER MODELS

By A. Abdo, M. Ackermann, M. Ajello, W. Atwood, L. Baldini, J. Ballet, G. Barbiellini, D. Bastieri, K. Bechtol, R. Bellazzini and 152 more. 2010

178 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/381e0471e85eb2c8636a74ccd4f55f46597a2d72

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Citations in the corpus

Too big to fail? The puzzling darkness of massive Milky Way subhaloes (2011, background): “…steradians (a cir- c© 2011 RAS, MNRAS 000, 1–6 cular region with radius 0.5 degrees) of the center of each massive dark subhalo relative to the predicted flux within the same angular radius originating from Draco, one of the most promising targets among the MW dwarfs for Fermi (Abdo et al. 2010).”
THE VELOCITY WIDTH FUNCTION OF GALAXIES FROM THE 40% ALFALFA SURVEY: SHEDDING LIGHT ON THE COLD DARK MATTER OVERABUNDANCE PROBLEM (2011, background): “…of dark energy and the lack of a direct or indirect detection of the dark matter (DM) particle (Ahmed et al. 2009; Angle et al. 2008a,b; Abdo et al. 2010a,b; Adriani et al. 2009), it is important to test in detail the astrophysical implications of the established cosmological paradigm.”
SEARCHING FOR DARK MATTER ANNIHILATION IN RECENTLY DISCOVERED MILKY WAY SATELLITES WITH FERMI-LAT (2016, methodology): “…dSphs using LAT data and have reported constraints on DM annihilation that are competitive with other DM targets such as the Galactic center (e.g., Abdo et al. 2010; Ackermann et al. 2011; Geringer-Sameth & Koushiappas 2011; Mazziotta et al. 2012; Ackermann et al. 2014; Geringer-Sameth et al.…”
SEARCH FOR DARK MATTER SATELLITES USING FERMI-LAT (2012, unknown): “However, since Sourcelike fits each energy bin indepen dently, we expected to find source candidates that were excluded from the 1FGL, either because they had non-power-Iaw spectra or they had hard spectra with too few photons to pass the 1FGL spectral analysis.”
SEARCH FOR GAMMA-RAY EMISSION FROM DES DWARF SPHEROIDAL GALAXY CANDIDATES WITH FERMI-LAT DATA (2015, methodology): “Several searches for gamma-ray emission from known dSphs have been performed using LAT data, none of which has resulted in a positive detection (e.g., Abdo et al. 2010; Ackermann et al. 2011, 2014, 2015a; GeringerSameth & Koushiappas 2011; Mazziotta et al. 2012; GeringerSameth et al. 2015b).”