Central Bureau for Astronomical Telegrams

Central Bureau for Astronomical Telegrams -- Image credits

CBAT "Transient Object Followup Reports"

TCP J02332248+0051018

TCP J02332248+0051018   2019 09 24.7493*  02 33 22.48 +00 51 01.8  13.3 U             Cet       9 0



2019 09 09.9747

Superoutburst (since Sept. 9, peak magnitude g= 12.1) of the WZ Sge-type dwarf nova candidate HP Cet. Recent ASAS-SN Sky Patrol (Shappee et al. 2014ApJ...788...48S and Kochanek et al. 2017PASP..129j4502K) data and light curve: https://asas-sn.osu.edu/light_curves/5ca91d4b-8ce6-4014-b289-e4bcb0456474. Time-resolved photometry is strongly recommended. --- Patrick Schmeer (Saarbr├╝cken-Bischmisheim, Germany)




2019 09 24.749

Discovered by T. Kojima, Tsumagoi,Gunma-ken, Japan, on three frames (limiting mag.= 14.3) taken by Canon EOS 6D + 200-mm f/3.2 lens.




2019 09 25.686

2019 09 25.686 02 33 22.61 +00 50 59.7 Mag.=13.8 0.6-m F/5.7 reflector + CCD (KAF-1001) Image : http://k-itagaki.jp/images/TCP-Cet.jpg




2019 09 25.534

F. Watanabe (Nayoro Observatory, Nayoro, Japan) performed a follow-up observation for this transient using a 0.4-m f/10 Meili telescope (Meade Schmidt-Cassegrain telescope) + R-filtered CCD (SBIG STL-1001E) on Sep. 25.534 UT. The magnitude is measured to be R = 14.1 +/- 0.1 (reference stars from UCAC4 Rmag). The position end figures are given as 22s.63, 59".6.



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