Bulgarelli, A.A.BulgarelliTavani, M.M.TavaniCaraveo, P.P.CaraveoGiommi, PaoloPaoloGiommiPittori, CarlottaCarlottaPittoriVerrecchia, FrancescoFrancescoVerrecchiaSantolamazza, P.P.SantolamazzaGasparrini, DarioDarioGasparriniCutini, SaraSaraCutiniColafrancesco, SergioSergioColafrancesco2020-09-172020-09-172008-10-01https://hdl.handle.net/20.500.13025/978Astronomy and Astrophysics, Volume 489, Issue 2, 2008, pp.L17-L20Context We present the AGILE gamma-ray observations of the field containing the puzzling gamma-ray source 3EG J1835+5918. This source is one of the most remarkable unidentified EGRET sources. <BR />Aims An unprecedentedly long AGILE monitoring of this source yields important information on the positional error box, flux evolution, and spectrum. <BR />Methods 3EG J1835+5918 has been in the AGILE field of view several times in 2007 and 2008 for a total observing time of 138 days from 2007 Sep. 04 to 2008 June 30 encompassing several weeks of continuous coverage. <BR />Results With an exposure time approximately twice that of EGRET, AGILE confirms the existence of a prominent gamma-ray source (AGL J1836+5926) at a position consistent with that of EGRET, although with a remarkably lower average flux value for photon energies greater than 100 MeV. A 5-day bin temporal analysis of the whole data set of AGL J1836+5926 shows some evidence for variability of the gamma-ray flux. The source spectrum between 100 MeV and 1 GeV can be fitted with a power law with photon index in the range 1.6-1.7, fully consistent with the EGRET value. <BR />Conclusions The faint X-ray source RX J1836.2+5925 that has been proposed as a possible counterpart of 3EG J1835+5918 is well within the AGILE error box. Future continuous monitoring (both by AGILE and GLAST) is needed to confirm the gamma-ray flux variability and to unveil the source origin, a subject that is currently being pursued through a multiwavelength search for counterparts.gamma rays observations10.1051/0004-6361 200810711http://adsabs.harvard.edu/abs/2008A&A...489L..17B2008A&A...489L..17B