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ATEL # 2878; V.Shumkov, E.Gorbovskoy, P.Balanutsa,V.Lipunov, V.Kornilov, A.Belinski, N.Shatskiy, N.Tyurina, D.Kuvshinov, V.Chazov, A.Kuznetsov, D.Zimnukhov, M. Kornilov (SAI, Moscow), A. Tlatov, A.V. Parhomenko, D. Dormidontov (Kislovodsk solar station of the Pulkovo observatory RAS), V.Yurkov, Yu.Sergienko, D.Varda (Blagoveshchensk Educational University), V.Krushinski, I.Zalozhnih, T.Kopytova, A. Popov (Ural State University), K.Ivanov, S.Yazev, N.Budnev, E.Konstantinov, V.Lenok, O.Chuvalaev, V.Poleschuk, O.Gres,(Irkutsk State University)
on 28 Sep 2010; 15:38 UT
Distributed as an Instant Email Notice (Request for Observations)
Password Certification: Vladimir Lipunov (email@example.com)
Subjects: Optical, Request for Observations, Nova, Supernova, Transients
Referred to by ATEL #: 2883
The MASTER auto-detection system at Kislovodsk detected a new transient source as the SN candidate at the position (R.A., Dec) = 07h 19m 48.91s , +40d 53m 32s.3, (J2000) with a typical uncertainty of 0.5" ( offset 10.6W 9.1N from SDSSJ071949.80+405322.9 galaxy) at 2010-09-27 23:52:32 (UT). The OT was seen at next image after ~45 min (2010-09-28 00:39:08 UT). There is now minor planet and any object brighter 21 mag in DSS at this place. We have a number images this field without OT. The last one was made at 2010-02-27 18:39:23 and have the limit 17.8 (5 hours before detection).
The unfiltered magnitude is about 16.7 +-0.1 ( exposition 180s, mlim = 18.6 ).
The OT as the SN-candidate is relatively far and more brighter than posible host galaxy (m~18.55).
The spectral observations are needed.
The discovery image is available at http://observ.pereplet.ru/images/MASTER071948.9+405332/MASTER071948.jpg
MASTER Robotic Net