%0 Journal Article
%A Olmo García, Amanda
%A Paliya, Vaidehi S.
%A Álvarez Crespo, Nuria
%A Kumar, Brajesh
%A Domínguez Díaz, Alberto
%A Gil De Paz, Armando
%A Sánchez Blázquez, Patricia
%T Optical spectroscopic characterization of Fermi blazar candidates of uncertain type with TNG and DOT: first results
%D 2022
%@ 0035-8711
%U https://hdl.handle.net/20.500.14352/72720
%X The classification of gamma-ray-detected blazar candidates of uncertain type (BCU) is a relevant problem in extragalactic gamma-ray astronomy. Here we report the optical spectroscopic characterization, using two 3-4 m class telescopes, Telescopio Nazionale Galileo and Devasthal Optical Telescope, of 27 BCUs detected with the Fermi Large Area Telescope. Since the identification of emission lines is easier in broad-line blazars, which usually exhibit low frequency peaked (synchrotron peak frequency </=10^(14) Hz) spectral energy distribution, we primarily target such BCUs. We found that 8 out of 27 sources exhibit broad emission lines in their optical spectra, 3 of them have redshifts >1 and the farthest one is at z=2.55. The optical spectra of 2 of the 19 remaining objects are dominated by the absorption spectra of the host galaxy, and there is a tentative detection of the Lyman-alfa absorption feature in one source. The spectra of the remaining 16 objetcts, on the other hand, are found to be featureless.
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