FERMI transient J1544-0649: a flaring radio-weak BL Lac
G. Bruni, F. Panessa, G. Ghisellini, V. Chavushyan, H. A., Pe\~na-Herazo, L. Hern\'andez-Garc\'ia, A. Bazzano, P. Ubertini, A. Kraus

TL;DR
This paper reports the discovery and multi-wavelength follow-up of a transient gamma-ray source, J1544-0649, identified as a potential radio-weak BL Lac object with a gamma-ray flare, expanding the understanding of such rare sources.
Contribution
It presents the first detailed multi-wavelength analysis of a gamma-ray transient identified as a radio-weak BL Lac, highlighting its unique properties and potential classification.
Findings
Confirmed flat radio spectrum indicating jet alignment
Radio loudness near the boundary between radio-loud and quiet AGN
Spectral energy distribution consistent with low-power BL Lac
Abstract
On May 15th, 2017, the \emph{FERMI}/LAT gamma-ray telescope observed a transient source not present in any previous high-energy catalogue: J1544-0649. It was visible for two consecutive weeks, with a flux peak on May 21st. Subsequently observed by a \emph{Swift}/XRT follow-up starting on May 26, the X-ray counterpart position was coincident with the optical transient ASASSN-17gs = AT2017egv, detected on May 25, with a potential host galaxy at =0.171. We conducted a 4-months follow-up in radio (Effelsberg-100m) and optical (San Pedro M\'artir, 2.1m) bands, in order to build the overall Spectral Energy Distribution (SED) of this object. The radio data from 5 to 15 GHz confirmed the flat spectrum of the source, favoring a line of sight close to jet axis, not showing significant variability in the explored post-burst time-window. The Rx ratio, common indicator of radio loudness, gives a…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
