MASTER-OAFA: XMM source's bright optical outburst discovery
ATel #9814; V. Shumkov, V. Lipunov (Lomonosov MSU), R. Podesta(OAFA), H. Levato (ICATE), D. Buckley(SAAO), C. Lopez, F. Podesta (OAFA),C. Saffe(ICATE), E. Gorbovskoy, P. Balanutsa, N. Tiurina, A. Kuznetsov, V. Kornilov, V. Vladimirov, A. Krylov, I. Gorbunov, V. Chazov, O. Gress, K. Ivanov (Lomonosov MSU), A. Gabovich (BSPU), T. Pogrosheva
on 1 Dec 2016; 12:08 UT
Credential Certification: Nataly Tyurina (firstname.lastname@example.org)
Subjects: Optical, Request for Observations, AGN, Transient, Variables
MASTER OT J111326.87-763146.0 discovery - XMM source's (AGN?) optical outburst discovery, ampl>5.2m
MASTER-OAFA (located in Argentina) auto-detection system
( Lipunov et al., "MASTER Global Robotic Net",
Advances in Astronomy, 2010, 30L ) discovered OT source at (RA, Dec) = 11h 13m 26.87s -76d 31m 46.0s on 2016-11-30.33949 UT.List of Optical Transients discovered by MASTER
The OT unfiltered magnitude is 16.8m (limit 19.3m).
The OT is seen in 3 images. We have reference image without OT on 2016-08-07.04407 UT with unfiltered magnitude mlim=19.7m.
There is GALEX and XMM source, also known as AGN (Lin et al., 2012).
22mag POSS limit gives more then 5.2m amplitude of current optical outburst
Spectral observations are required.
MASTER Global Robotic Net