MASTER: bright PSN in UGC00402
ATel #8112; O. Gress, V. Lipunov, E. Gorbovskoy (Lomonosov MSU), R. Rebolo, M. Serra-Ricart, N. Lodieu, G. Israelian (The Instituto de Astrofisica de Canarias), V. Kornilov, N. Tiurina, P. Balanutsa, V. Vladimirov, A. Kuznetsov, E. Popova, I. Gorbunov, D. Vlasenko, V. Chazov (M. V. Lomonosov MSU, SAI), A. Tlatov, V. Senik, D. Dormidontov (Kislovodsk Solar Station of the Pulkovo Observatory),N. Budnev, K. Ivanov (Irkutsk State University, Applied Physics Institute), D. Buckley, S. Potter, M. Kotze (South African Astronomical Observatory), V. Krushinskiy (Ural Federal University), Yu. Sergienko, A. Gabovich, V. Yurkov (Blagoveschensk Educational State University)
on 1 Oct 2015; 21:53 UT
Credential Certification: Nataly Tyurina (firstname.lastname@example.org)
Subjects: Optical, Supernovae, Transient
MASTER-IAC auto-detection system ( Lipunov et al., Advances in Astronomy, MASTER Global Robotic Net, 2010 ) discovered OT source at (RA, Dec) = 00h 39m 18.04s +03d 56m 59.6s on 2015-10-01.15811 UT.
List of Optical Transients discovered by MASTER
The OT unfiltered magnitude is 15.2m (limit 19.3m).
This OT is seen in 6 images. There is no minor planet at this place. We have reference image without OT on 2015-09-13.12723 UT with unfiltered magnitude limit 20.7m.
This PSN is in 8.5"W and 9.2"S from the UGC00402
Spectral observations are required.
The discovery and reference images are available at http://observ.pereplet.ru/images/MASTER003918.04+035659.6.png
MASTER Global Robotic Net