Farina, E. P.E. P.FarinaFumagalli, M.M.FumagalliDECARLI, ROBERTOROBERTODECARLIFanidakis, N.N.Fanidakis2020-06-292020-06-2920160035-8711http://hdl.handle.net/20.500.12386/26244PKS 2155-304 is one of the brightest extragalactic source in the X-ray and EUV bands, and is a prototype for the BL Lac class of objects. In this paper, we investigate the large-scale environment of this source using new multi-object as well as long-slit spectroscopy, together with archival spectra and optical images. We find clear evidence of a modest overdensity of galaxies at z = 0.116 10 ± 0.000 06, consistent with previous determinations of the BL Lac redshift. The galaxy group has a radial velocity dispersion of 250^{+80}_{-40} km s<SUP>-1</SUP> and a virial radius of 0.22 Mpc, yielding a role-of-thumb estimate of the virial mass of M<SUB>vir</SUB> ∼ 1.5 × 10<SUP>13</SUP> M<SUB>☉</SUB>, I.e. one order of magnitude less than that observed in similar objects. This result hints towards a relatively wide diversity in the environmental properties of BL Lac objects.STAMPAenArticle10.1093/mnras/stv22772-s2.0-84958260867000368005900073https://academic.oup.com/mnras/article/455/1/618/9843062016MNRAS.455..618FFIS/05 - ASTRONOMIA E ASTROFISICA