Unidentified EGRET sources and their possible Fermi counterparts

International Conference on Particle Physics and Astrophysics

物理学;天文学

Lyapin, A.R.^1 ; Arkhangelskaja, I.V.^2 ; Larin, D.S.^2

Moscow Institute of Physics and Technology (State University), Institutskiy pereulok 9, Dolgoprudny, Moscow Region

141701, Russia^1

National Research Nuclear University MEPhI, Moscow Engineering Physics Institute, Kashirskoe Highway 31, Moscow

115409, Russia^2

关键词: Backsplash;    Count rates;    Counts-as;    Gamma quanta;    Latitudinal profiles;    Particles identification;    Trigger systems;   

Others  :  https://iopscience.iop.org/article/10.1088/1742-6596/798/1/012005/pdf
DOI  :  10.1088/1742-6596/798/1/012005

学科分类：天文学(综合)

来源: IOP

【 摘 要 】

Unidentified EGRET sources from 3EG catalog have been analyzed. Preliminary data analysis has shown at least 23 of these sources coincide with those in 3FGL Fermi catalogue within 1, 2 and 3 sigma error intervals of the coordinates and fluxes. Their properties are discussed in the presented work. Even 3-sigma difference allows supposing sources similarity because of more than 3-sigma distinctions in values of fluxes between identified EGRET sources and their Fermi counterparts. For instance, the coincidence between 3EG J1255-0549 and 3FGL J1256.1-0547 was reported in Fermi catalogues 1FGL, 2FGL, 3FGL. However, these sources fluxes (in units of 10-8photons × cm-2× s-1) in the energy band E > 100 MeV were 179.7 ± 6.7 (3EG), 44.711 ± 0.724 (3FGL), 53.611 ± 0.997 (2FGL) and 67.939 ± 1.861 (1FGL). Such effect was observed for sufficient portion of identified EGRET sources. It could cause by troubles of particles identification by Fermi/LAT trigger system. Very often charged particles recognized as gamma-quanta because of wrong backsplash analysis. Nevertheless, gammas counts as charged particles due analogous reason and rejected during ground data processing. For example, it appears as geomagnetic modulation presence on gamma-quanta count rate latitudinal profiles in energy band E > 20 MeV.