Ackermann, M.M.AckermannAjello, M.M.AjelloAllafort, A.A.AllafortCavazzuti, ElisabettaElisabettaCavazzutiCiprini, StefanoStefanoCipriniCutini, SaraSaraCutiniGasparrini, DarioDarioGasparriniGiommi, PaoloPaoloGiommi2020-09-172020-09-172014-01-01https://hdl.handle.net/20.500.13025/3980VizieR On-line Data Catalog J/ApJS/209/34. Originally published in 2013ApJS..209...34AThe time interval analyzed here is from the beginning of Fermi LAT science operations, 2008 August 4 (MET 239557447) to 2011 August 1 (MET 333849586), covering very nearly 3 yr. In this work we analyze gamma rays with energies in the range 10-500 GeV. To limit the contamination from gamma rays produced by cosmic-ray interactions in the upper atmosphere, gamma rays with zenith angles greater than 105 were excluded. To further reduce the residual gamma rays from the upper atmosphere only data for time periods when the spacecraft rocking angle was less than 52 were considered. See section 2 for further explanations. (2 data files).Gamma raysRedshifts Comment table3.dat 514x165 LAT catalog of sources above 10GeV; table7.dat 393x113 Characteristics of the 1FHL sources with; AGN associationson-line data cataloghttp://adsabs.harvard.edu/abs/2014yCat..22090034A2014yCat..22090034A