A Strong Optical Flare from Blazar S4 1849+67 Detected by ASAS-SN
ATel #7205; K. Z. Stanek, T. W.-S. Holoien, C. S. Kochanek, A. B. Danilet, G. Simonian, U. Basu, N. Goss, J. F. Beacom, T. A. Thompson (Ohio State), B. J. Shappee (Hubble Fellow, Carnegie Observatories), J. L. Prieto (Diego Portales; MAS), D. Bersier (LJMU), J. Brimacombe (Coral Towers Observatory), Subo Dong (KIAA-PKU), E. Falco (CfA), P. R. Wozniak (LANL), D. Szczygiel, G. Pojmanski (Warsaw University Observatory)
on 11 Mar 2015; 18:16 UT
Distributed as an Instant Email Notice Transients
Credential Certification: Krzysztof Stanek (stanek.32@osu.edu)
Subjects: Optical, Blazar
Flaring blazar
S4 1849+67 (e.g., ATel #3478) is in a field regularly observed by
ASAS-SN quadruple "Brutus" telescope. Two images obtained on UT
2015-03-10.60 reveal a strong (delta V~2 mag) V-band flare of that
object, see this
figure for last 30 days of ASAS-SN V-band photometry. In particular, the
last four ASAS-SN epochs had the following V-band photometry:
UT Date V
2015-02-15.64 16.40
2015-02-24.58 16.80
2015-03-02.58 >16.20
2015-03-10.60 15.15
We thank LCOGT and its staff for their continued support of
ASAS-SN. ASAS-SN is supported in part by Mt. Cuba Astronomical
Foundation. For more information about the ASAS-SN project, see the
ASAS-SN
Homepage.