Multi-band radio emission enhancement of the flat spectrum radio quasar OP 313
Published: 05/2025
The RATAN-600 light curves of OP 313
Yu. V. Sotnikova, T. V. Mufakharov, A. K. Erkenov, T. A. Semenova, R.Yu. Udovitskij (SAO RAS), Yu. A. Kovalev (ASC Lebedev), A.V. Popkov (MIPT, ASC Lebedev)
The significant brightening of the flat spectrum radio quasar OP 313 (BZU J1310+3220, 4FGL J1310.5+3221) was recently been reported in gamma-ray (
ATel #17167), near-infrared (
ATel #17179) and optical bands (
ATel #17173,
#17184,
#17185) over the past two weeks. This source is included in the RATAN-600 long-term monitoring program, and it has exhibited a consistent upward trend in radio flux density since January 2017.
On 2025 May 8, we measured its flux densities at five frequencies using the RATAN-600 telescope, obtaining the following values (in Jy):
- 4.37 ± 0.6 at 22.3 GHz
- 4.22 ± 0.4 at 14.4 GHz
- 3.93 ± 0.4 at 11.2 GHz
- 3.85 ± 0.3 at 8.2 GHz
- 2.71 ± 0.2 at 4.7 GHz
These measurements indicate that OP 313 is currently in its highest radio emission state observed over the past decade, based on our monitoring data.