Bright Transient in Sgr (PNV J18142514-2554343)

Exoplanet occultation, asteroid occultation,
solar research, comet observation, astrometry, etc.
回覆文章
PTS
夸克星
文章: 17313
註冊時間: 週日 28 10月, 2007 08:50
來自: HK

Bright Transient in Sgr (PNV J18142514-2554343)

文章 PTS » 週一 16 2月, 2015 08:32

Patrick Schmeer (SPK, Bischmisheim, Germany) reports the announcement on the CBAT Transient Object Confirmation Page (TOCP) of the discovery of a bright transient in Sgr on 2015 February 12.852 at an unfiltered magnitude of
10.9 by K. Nishiyama, using a 105-mm f/4 camera lens with an SBIG STL6303E CCD camera. Nishiyama notes nothing is present on a previous image from
2015 February 02.887. The transient has been independently confirmed with two pre-discovery images: by H. Nishimura (Shizuoka-ken, Japan) at magnitude
11.2 on 2015 February 12.840, and by T. Kojima (Gunma-ken, Japan) at magnitude 10.5 on 2015 February 11.841.

The object was designated PNV J18142514-2554343 on the TOCP website. More information about the discovery and prediscovery images may be found at the following URL:

http://www.cbat.eps.harvard.edu/unconf/ ... 54343.html

Photometry and spectroscopy are all strongly encouraged. Spectroscopy is needed urgently to determine whether the object is a nova or some other type of transient. A sequence is currently in preparation. Observers should note that the field is extremely crowded.

The J2000 coordinates for this transient are as follows:

RA: 18 14 25.24 , Dec: -25 54 32.6

Please promptly report all observations to the AAVSO International Database using the name PNV J18142514-2554343.

This AAVSO Special Notice was prepared by M. Templeton.

回覆文章

回到「業餘天文研究專區 Amateur Astronomers' Research Area」

誰在線上

正在瀏覽這個版面的使用者:沒有註冊會員 和 21 位訪客