TeV sources analysis with AGILE
F. Longo, A. Rappoldi, F. Lucarelli, C. Pittori, F. Verrecchia, A., Bulgarelli, M. Tavani (for the AGILE Collaboration)

TL;DR
This paper analyzes three years of AGILE gamma-ray data to identify or constrain GeV and sub-GeV counterparts of TeV sources, aiding in the identification of high-energy astrophysical objects.
Contribution
It provides a systematic study linking TeV sources with GeV and sub-GeV observations using AGILE data, highlighting the need for multi-energy observations.
Findings
Detection of GeV/sub-GeV counterparts for some TeV sources.
Upper limits set for sources without clear counterparts.
Identification prospects for unidentified TeV sources improved.
Abstract
AGILE (Astrorivelatore Gamma a Immagini LEggero) is an Italian Space Agency (ASI) mission launched on April 23rd, 2007. The AGILE-GRID instrument onboard of the AGILE satellite is devoted to gamma-ray astrophysics in the 30 MeV - 50 GeV energy range. This paper presents the results of a systematic study performed on the first three years of AGILE-GRID data to search for GeV and sub-GeV counterparts (or derive flux upper limits) of sources detected at very high-energy by TeV experiments. Many of the TeV sources are still unidentified and deep observations at lower energies are needed to identify their possible counterparts.
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Taxonomy
TopicsParticle Detector Development and Performance · Dark Matter and Cosmic Phenomena · Nuclear Physics and Applications
