SIMBAD references

2012CBET.3089....1K - Central Bureau Electronic Telegrams, 3089, 1 (2012/April-0)

Nova Sagittarii 2012 = PNV J17452791-2305213.

KOROTKIY S., SOKOLOVSKY K., BROWN N.J., GAO R.J., SEACH J., KIYTOTA S., GUIDO E., HOWES N., SOSTERO G., ELENIN L., MOLOTOV I., KOFF R.A., NISSINEN M., NISHIYAMA K., KABASHIMA F., KOBERGER H., VOLLMANN W. and GERKE V.

Abstract (from CDS):

Stanislav Korotkiy, Ka-Dar Observatory; and Kirill Sokolovsky, Astro Space Center, Lebedev Physical Institute, and Sternberg Astronomical Institute, Moscow State University, report the discovery of a possible nova (magnitude 9.6) on three 30-s unfiltered CCD images (limiting magnitude about 14.0) obtained on Apr. 21.011 UT with a wide-field survey camera (+ 135-mm-f.l. f/2 telephoto lens + ST8300M camera) at Ka-Dar Observatory's TAU Station near Nizhny Arkhyz, Russia. The new object is located at R.A. = 17:45:28.03, Decl. = -23:05:22.8 (equinox 2000.0; UCAC2 reference stars; uncertainty 1"), noting that a red USNO-B1.0-catalogued star (magnitudes R1 = 16.21, B2=18.61) lies just 0".6 away from the variable's position. Their discovery images are posted at URL http://www.astroalert.su/files/pnv_j17452791-2305213.jpg. The variable was designated PSN J17452791-2305213 when it was posted at the Central Bureau's TOCP webpage.

Additional magnitudes for PSN J17452791-2305213 (from unfiltered CCD images unless noted otherwise): Apr. 17.99, [14.0 (Korotkiy and Sokolovsky); 19.73, [12.0 (N. J. Brown, Two Rocks, W. Australia; TMax 400 film + 135-mm-f.l. f/2.0 camera lens); 20.84, 10.2 (R. J. Gao, Xingming Observatory, China; V-band suggested; position end figures 28s.02, 23".3; USNO-A2.0 reference stars; no instrumentation details given); 21.654, 8.8 (John Seach, Chatsworth Island, NSW, Australia; digital camera + 50-mm-f.l. f/1.0 lens); 22.353, V = 9.58, B = 10.30, I_c = 7.70 (Seiichiro Kiytota, Tsukuba, Japan; remotely with 25-cm reflector + ST-10XME camera near Mayhill, NM, USA; position end figures 28s.03, 22".9); 22.4, 9.1 (Ernesto Guido, Nick Howes, and Giovanni Sostero; 0.25-m f/3.4 reflector, remotely from Mayhill; position end figures 28s.02, 23".2; reference stars from UCAC-3 catalogue; they also note the USNO-B1.0 star only 0".2 away; they have posted a comparison between their confirmation image and an archival red 1996 plate from the Digitized Sky Survey at website URL http://bit.ly/IIV8oN); 22.415, 9.0 (L. Elenin, Lyubertsy, Russia; and I. Molotov, Moscow, Russia; remotely with a 0.45-m f/2.8 telescope at the ISON-NM Observatory near Mayhill, NM, USA; position end figures 28s.02, 23".1; NOMAD reference stars; limiting mag about 17.8); 22.454, V = 9.06 ± 0.10 (R. A. Koff, Bennett, CO, USA; Meade 0.25-m f/10 reflector + Apogee AP-47p camera; limiting magnitude 15.3; position end figures 28s.02, 22".9; UCAC3 reference stars); 22.462, 9.4 (Markku Nissinen, Varkaus, Finland; remotely with a 15- cm f/7.3 refractor + color CCD camera of "itelescope.net" near Mayhill; position end figures 28s.02, 23".0; corrected GSC 1.1 catalogue stars; limiting magnitude 17.2; nothing brighter than mag 18 on a red Palomar Sky Survey F plate at this position); 22.718, 9.6 (Koichi Nishiyama, Kurume, Japan; and Fujio Kabashima, Miyaki, Japan; limiting magnitude 17.6; Meade 200R 0.40-m f/9.8 reflector + SBIG STL1001E camera; position end figures 28s.05, 23".2); 22.979, 9.7 (Korotkiy and Sokolovsky); 23.217, 10.0 (Hermann Koberger; 0.6-m reflector at Vilaflor, Tenerife; green magnitude from a digital SLR camera; a low-resolution spectrum at 100 lines per mm from Apr. 23.243 showed H_alpha emission for the object; communicated by Wolfgang Vollmann); 23.976, 10.0 (Korotkiy and Sokolovsky); 23.993, 10.0 (Korotkiy and Sokolovsky; 40-cm telescope; position end figures 28s.03, 22".7, uncertainty 0".3; measured by Korotkiy and V. Gerke); Kiytota's image is posted at website URL http://meineko.sakura.ne.jp/ccd/PNV_J17452791-2305213-120422.jpg.


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