Central Bureau for Astronomical Telegrams

Central Bureau for Astronomical Telegrams -- Image credits

CBAT "Transient Object Followup Reports"

PSN J13224838+3330207

PSN J13224838+3330207   2013 11 28.8872*  13 22 48.38 +33 30 20.7  16.5 U    7E  11S  P2033541  9 9       9 9



2013 11 28.8872

Vladimir Lipunov reports the discovery by Sergey Shurpakov of a possible supernova (mag 16.5) on 3 unfiltered CCD images (limiting mag 18.2) obtained with the auto-detection system of the MASTER II 40-cm telescope (+ Apogee Alta U16m camera; field-of-view 2x4 square degrees) at the MASTER-Amur observatory (see website URL http://observ.pereplet.ru) on 2013-11-28.88726 UT. The new object is located at R.A. = 13h22m48s.38, Decl. = +33d30'20".7 (equinox 2000.0), which is 7" east and 11" south of the center of PGC 2033541.




2013 11 29.4754

L. Elenin (Lyubertsy, Russia) and I. Molotov (Moscow, Russia) confirm an apparent supernova PSN J13224838+3330207. Object visible on 3x150sec images remotely taken at ISON-NM Observatory (Mayhill, NM, USA) with 0.4-m f/3 telescope + CCD (KAF09000) on Nov. 29.4754, 2013. Object located at 13h 22m 48s.36 +/- 0".12, 33d 30' 21".4 +/- 0".16 (UCAC-4) with magnitude 17.1R (mag. limit ~19.4m). Nothing is visible at this position on the POSS and POSSII images. Image of PSN J13224838+3330207 available at http://spaceobs.org/images/TOCP/PSNJ13224838+3330207-20131129.png




2013 12 01.1734

This object was observed by Federica Luppi and Luca Buzzi from Schiaparelli Observatory, Varese, Italy. In a stack of images totalling 4 minutes of unfiltered exposure time, the object has position end figures 48s.36, 21".4 and magnitude 17.2. Image posted at URL http://www.astrogeo.va.it/pub/TOCP/PSN_P2033541.jpg




2013 12 05.124

This transient was observed on 2013 12 05.124 by Gianluca Masi, Francesca Nocentini and Patrick Schmeer, remotely using the 17"-f/6.8 robotic unit part of the Virtual Telescope Project facility in Ceccano, Italy. 120-seconds exposures, unfiltered, show the source at mag. 17.3 (R mags for the reference stars from UCAC-4). We also performed astrometry, getting the following end figures: 48.35s; 21.6" (J2000.0, mean residuals of 0.2" on both axes).



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