Fermi LAT Search for Photon Lines from 30 to 200 GeV

By A. Abdo, M. Ackermann, M. Ajello, U. Stanford, W. Atwood, S. Uc, L. Baldini, Pisa Infn, J. Ballet, Saclay Dapnia and 52 more. 2010

142 citations recorded by the source corpus.

Subfields: Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/42365a03ab8c9ef7bfad235f96dae0c105087b44

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Nuclear and High Energy Physics

1. E. Orlando
2. L. Strigari
3. A. Reimer
4. I. Grenier
5. G. Jóhannesson
6. J. Scargle
7. Igor V. Moskalenko
8. S. Funk

Citations in the corpus

• 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.”
• THE FERMI LARGE AREA TELESCOPE ON ORBIT: EVENT CLASSIFICATION, INSTRUMENT RESPONSE FUNCTIONS, AND CALIBRATION (2012, methodology): “For comparison the intensity of the extragalactic diffuse γ-ray emission measured by the LAT (Abdo et al. 2010f) is overlaid to demonstrate the many orders of background suppression necessary to distinguish it from particle background.”
• 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.”
• Galactic Searches for Dark Matter (2012, methodology): “So considering that other dSphs have negligible star formation, it is very likely that any gamma-rays observed from these objects arise from dark matter annihilation (Note that it is possible that several more star forming galaxies could appear as Fermi-LAT sources before the end of the mission, wit”
• Search for gamma-ray spectral lines with the Fermi Large Area Telescope and dark matter implications (2013, unknown): “Following the approach used in previous line searches published by the LAT Collaboration, we use a sum of Gaussians to parametrize the energy dispersion at any given energy, averaging over the LAT FOV and combining front- and back-converting events [14].”