XMM-Newton observations of the BL Lac MS 0205.7+3509: A dense, low-metallicity absorber

The high-frequency-peaked BL Lac, MS 0205.7+3509 was observed twice with XMM-Newton. Both X-ray spectra are synchrotron-dominated, with mean 0.2-10 keV fluxes of 2.80 ± 0.01 and 3.34 ± 0.02 × 10 −12 erg cm −2 s −1 . The X-ray spectra are well fit by a power-law with absorption above the Galactic value, however no absorption edges are detected, implying a low metallicity absorber (Z� = 0.04 +0.03 −0.01 ) or an absorber with redshift above one (best-fit z = 2.1 for an absorber with solar abundances). In either case the absorbing column density must be ∼9 × 10 21 cm −2 . A new optical spectrum is presented, with a Mg  absorption doublet detected at z = 0.351, but no other significant features. The optical spectrum shows little reddening, implying a low dust to gas ratio in the absorber. MS 0205.7+3509 must therefore be viewed through a high column density, low-metallicity gas cloud, probably at z = 0.351 and associated with the galaxy that has been shown to be within ∼2 �� of the BL Lac.