IAU Central Bureau for Astronomical Telegrams

Central Bureau for Astronomical Telegrams -- Image credits

CBAT "Transient Object Followup Reports"

PSN J06280368+7418338

PSN J06280368+7418338   2015 09 02.1000*  06 28 03.68 +74 18 33.8  18.3 U   18E  28N  U3460     7 0



2015 09 02.1000

Paolo Campaner report the discovery of PSN (unfiltered magnitude = 18.3) on three images (limiting magnitude 20.0) obtained on September 02.1000 UT with a 0,4m reflector F/5.5 + CCD and exposure 3x75sec. at Ponte di Piave - Italy, in the course of the Italian Supernovae Search Project.




2015 09 03.01

This transient was observed on 2015 09 03.00675 by M.Caimmi from C92 - Valdicerro Observatory in the course of the Italian Supernovae Search Project (ISSP) using 0.24-m f/6.5 SCT - CCD Atik 314L. Stack of 15 unfiltered b1x1 frames x 240sec guiding exposures, show the source at 18.2 Mag. End figures for astrometry were AR. 03,74s DEC. 34,1" position measured from reference stars UCAC-4 catalogue. The image of this observation is available http://www.oav.name/public/PSN_J06280368+7418338_20150903.jpg




2015 09 04.1243

This transient was observed by Paolo Campaner (unfiltered magnitude = 18.1) on several images (limiting magnitude 20.0) obtained on September 04.1243 UT with a 0,4m reflector F/5.5 + CCD and exposure 10x75sec. at Ponte di Piave - Italy, in the course of the Italian Supernovae Search Project




2015 09 07.382

This possible supernova in UGC 3460 was detected with 21 x 5 min images using a clear filter Photometry: Mag 17.63 +/- 0.27 C (V for ref; USNOA2) Astrometry: RA 06 28 03.61 Dec +74 18 34.2 These data were collected remotely by Joseph Brimacombe, Coral Towers Observatory, Cairns, Australia. Link to image and further information: https://www.flickr.com/photos/43846774@N02/21082868068/




2015 09 12.90366

This transient was observed on 2015 09 12.90366 by G. Masi, remotely using the 17"-f/6.8 robotic unit part of the Virtual Telescope Project facility, at Bellatrix Astronomical Observatory in Ceccano, Italy. 120-seconds exposures, unfiltered, show the source at mag. 17.0 (R mags for the reference stars from UCAC-4). We also performed astrometry, getting the following end figures: 03.57; 34.0 (J2000.0, mean residuals of 0.2" on both axes).




2015 09 18.90243

This transient was observed on 2015 09 18.90243 UT by Zhijian Xu and Xing Gao, using an unfiltered CCD ( + Celestron C14 Schmidt-Cassegrain telescope D=356-mm @f/6.9 ), in Xingming Observation Sky Survey(C42). 60-seconds exposures, show the source at mag. 17.7 U (reference stars from UCAC-4), with position end figures 03s.56, 34".3. Image can be seen: http://njzhijian.lamost.org/Supernova/PSN_J06280368+7418338_0918.jpg



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