MASTER: bright PSN in PGC212862
ATel #8262; V. Shumkov, V. Lipunov, E. Gorbovskoy (Lomonosov MU), D. Buckley (SAAO), V. Kornilov, N. Tiurina, P. Balanutsa, A. Kuznetsov, I. Gorbunov, D. Vlasenko, V. Vladimirov, E. Popova (M. V.Lomonosov Moscow State University, Sternberg Astronomical Institute), S. Potter, A. Knyazev, M. Kotze (South African Astronomical Observatory)
on 9 Nov 2015; 09:15 UT
Credential Certification: Nataly Tyurina (email@example.com)
Subjects: Optical, Request for Observations, Cataclysmic Variable, Supernovae, Transient, Variables
MASTER OT J015539.85+485955.6 discovery - bright PSN in PGC212862
MASTER-IAC auto-detection system ( Lipunov et al., Advances in Astronomy, MASTER Global Robotic Net, 2010 ) discovered OT source at (RA, Dec) = 01h 55m 39.85s +48d 59m 55.6s on 2015-11-07.99775 UT.
The OT unfiltered magnitude is 15.2m (limit 19.1m). The OT is seen in 5 images.
We have reference image without OT on 2015-08-02.08168 UT with unfiltered magnitude limit 18.4m.
This PSN is in 9.4"E,7.9"N from the center of PGC212862 galaxy with Btot=17.5m.
The discovery and reference images are available at: http://master.sai.msu.ru/static/OT/015539.85485955.6.png
There is a possibility for the second scenario with the USNO B1 star in 0.5" with B2=19.98(20.5 GSC2.3.2) R2=19.25(19.6 GSC2.3.2). In this case there is a dwarf nova outburst with Ampl>4.6m
List of Optical Transients discovered by MASTER
Spectral observations are required.
MASTER Global Robotic Net