摘要：Context.FermiJ1544–0639/ASASSN-17gs/AT2017egv was identified as a gamma-ray/optical transient on May 15, 2017. Subsequent multiwavelength observations suggest that this source may belong to the new class of radio-weak BL Lacs.Aims. We studied the X-ray spectral properties and short-term variability ofFermiJ1544–0639 to constrain the X-ray continuum emission mechanism of this peculiar source.Methods. We present the analysis of anXMM-Newtonobservation, 56 ks in length, performed on February 21, 2018.Results. The source exhibits strong X-ray variability, both in flux and spectral shape, on timescales of ∼10 ks, with a harder-when-brighter behaviour typical of BL Lacs. The X-ray spectrum is nicely described by a variable broken power law, with a break energy of around 2.7 keV consistent with radiative cooling due to Comptonization of broad-line region photons. We find evidence for a “soft excess”, nicely described by a blackbody with a temperature of ∼0.2 keV, consistent with being produced by bulk Comptonization along the jet.
