Dissecting the inner Galaxy with gamma-ray pixel count statistics
Journal of Physics Conference Series, vol. 2156, pp. 012093
Abstract
Abstract The nature of the GeV gamma-ray Galactic center excess (GCE) in the data of Fermi-LAT is still under investigation. Different techniques, such as template fitting and photon-count statistical methods, have been applied in the past few years in order to disentangle between a GCE coming from sub-threshold point sources or rather from diffuse emissions, such as the dark matter annihilation in the Galactic halo. A major limit to all these studies is the modeling of the Galactic diffuse foreground, and the impact of residual mis-modeled emission on the results’ robustness. We combine for the first time adaptive template fitting and pixel count statistical methods in order to assess the role of sub-threshold point sources to the GCE, while minimizing the mis-modelling of diffuse emission components. We reconstruct the flux distribution of point sources in the inner Galaxy well below the Fermi-LAT detection threshold, and measure their radial and longitudinal profiles. We find that point sources and diffuse emission from the Galactic bulge each contributes about 10% of the total emission therein, disclosing a potential sub-threshold point-source contribution to the GCE.
Authors 3
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Affiliation as printed
Speaker, Institut fur Theoretische Teilchenphysik und Kosmologie, RWTH Aachen University, Germany
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Centre National de la Recherche Scientifique · Université Grenoble Alpes · Laboratoire d'Annecy de Physique Théorique
Affiliation as printed
Univ. Grenoble Alpes, USMB, CNRS, LAPTh, F-74940 Annecy, France
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Istituto Nazionale di Fisica Nucleare, Sezione di Torino
Affiliation as printed
Dipartimento di Fisica, Universita di Torino and Istituto Nazionale di Fisica Nucleare, Sezione di Torino, via P. Giuria, 1, I-10125 Torino, Italy
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