Senturk, G.D.Böttcher, M.Errando, M.Mukherjee, R.2015-04-082015-04-082013Senturk, G.D. et al. 2013. Gamma-ray observational properties of TeV-detected blazars. Astrophysical journal, 764(2): Article no 119. [https://doi.org/10.1088/0004-637X/764/2/119]0004-637X1538-4357 (Online)http://hdl.handle.net/10394/13660https://doi.org/10.1088/0004-637X/764/2/119The synergy between the Fermi-LAT and ground-based Cherenkov telescope arrays gives us the opportunity for the first time to characterize the high-energy emission from blazars over 5 decades in energy, from 100 MeV to 10 TeV. In this study, we perform a Fermi-LAT spectral analysis for TeV-detected blazars and combine it with archival TeV data. We examine the observational properties in the γ-ray band of our sample of TeV-detected blazars and compare the results with X-ray and GeV-selected populations. The spectral energy distributions (SEDs) that result from combining Fermi-LAT and ground-based spectra are studied in detail. Simple parameterizations such as a power-law function do not always reproduce the high-energy SEDs, where spectral features that could indicate intrinsic absorption are observed.enGalaxies: activegalaxies: nucleigamma rays: generalArticle