Central Bureau for Astronomical Telegrams

Central Bureau for Astronomical Telegrams -- Image credits

CBAT "Transient Object Followup Reports"

PSN J11355080+3417027

PSN J11355080+3417027   2013 05 01.787 *  11 35 50.80 +34 17 02.7  17.3 U    4W   7N  PGC35860  9 9



2013 05 01.787

Discovered by P. Balanutsa on two unfiltered images (60-sec exposures) obtained with MASTER-Kislovodsk telescope (double 0.40-m f/2.5 reflector + 4Kx4K CCD) on 2013 May 01.753 and 01.787 UT. The prediscovery images from the same telescope were then found by D. Denisenko. Photometry (unfiltered with the red zero point; data by MASTER-Kislovodsk except for Feb. 23): 2013 Feb. 11.896, <19.2; Feb. 23.642, <17.5 (the latest non-detection by MASTER-Amur); Mar. 06.921 UT, 16.74; 06.952, 16.66; Mar. 30.893, 17.05; May 01.754, 17.23. Discovery and reference images are available at http://master.sai.msu.ru/static/OT/113550.80341702.7.png with more details in ATel #5044, http://www.astronomerstelegram.org/?read=5044




2013 05 05.1722

This PSN detected at coordinates 11 35 50.79 +34 17 01.9 (UCAC3). Magnitude 18.3 U +/- 0.2 . Limiting magnitude 20.6 . Sum of 6 x 240-sec images. Nothing visible other than galaxy background at these coordinates on DSS. Observer: R. A. Koff, Antelope Hills Observatory, Bennett, Colorado USA (H09). Image posted at: http://antelopehillsobservatory.org/SNpictures/PSNJ11355080+3417027final.jpg




2013 05 05.304

This possible supernova in PGC 35860 was detected with 43 x 0.75 min images using a luminance filter Astrometry: RA 11 35 50.87 Dec +34 17 01.9 Photometry: 17.17 +/- 0.28 L (V as ref) These data were collected remotely by Joseph Brimacombe, Cairns, Australia. Link to image and further information: http://www.flickr.com/photos/43846774@N02/8712437390/




2013 05 04.888

This PSN detected at RA=11 35 50.83, Dec=+34 17 02.5 (2000.0). Magnitude 17.5 R +/- 0.1. 8 x 60 sec images with the 0.40-m Lendulet-reflector at Konkoly Observatoy, Piszkesteto, Hungary. Observer: K. Sarneczky, Konkoly Observatory, Hungary.



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