MASTER SN candidate in PGC1539979 discovery
ATel #3240; D. Cheryasov, 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, I. Kudelina ,Yu. Sergienko, D. Varda (Blagoveshchensk Educational University), V. Krushinski, I. Zalozhnih, A. Popov (Ural State University), K. Ivanov, S. Yazev, N. Budnev, E. Konstantinov, O. Chuvalaev, V. Poleschuk, O. Gres,(Irkutsk State University) , V. Shumkov, S. Shurpakov (MASTER team member)
on 28 Mar 2011; 09:43 UT
Credential Certification: Vladimir Lipunov (email@example.com)
Subjects: Optical, Supernovae, Transient
The MASTER auto-detection system at Kislovodsk detected a new transient source as the SN candidate at the position (R.A., Dec) = 08h 39m 18.37s, +17d 43m 15s.9, (J2000) with a typical uncertainty of 0.5" (offset is 20.7E 11.4S from PGC1539979 galaxy) at 2011-03-26.76 (UT). The OT is seen at 3 images.
There is no minor planet and any object brighter 21 mag in DSS at this place.
The unfiltered magnitude is about 18.90+-0.4 ( exposition 180s, mag limit =20.0).
The spectral observations are needed.
The discovery image is available at http://observ.pereplet.ru/images/SN110328/sn.jpg
MASTER Robotic Net