2006CBET..352....1B

Query : 2006CBET..352....1B

2006CBET..352....1B - Central Bureau Electronic Telegrams, 352, 1 (2006/January-0)

Supernova 2005nb in NGC 7753.

BOLES T., LI W. and ROGERS G.

Abstract (from CDS):

T. Boles, Coddenham, England, reports the discovery of an apparent supernova (mag 18.1) on an unfiltered CCD image taken on Jan. 2.856 UT with a 0.35-m reflector. The new object is located at R.A. = 23h47m03s.78, Decl. = +29o28'55".7, which is approximately 13".6 west and 5".1 south of the center of NGC 7753. A confirmation image was acquired via KAIT (Lick Observatory) by W. Li on Jan. 5.108; Boles provides the following position end figures for 2005nb from Li's image: 03s.81, 55".6. Traces of 2005nb are also visible on an unfiltered CCD image taken by G. Rogers (Long Crendon, England, 0.40-m reflector) on Jan. 4.794. Nothing is visible at the location of 2005nb on Boles' images from 2005 Oct. 10 and Sept. 24 (limiting mag 19.5) or on Digitized Sky Survey images from 1991 (limiting red mag 21.0) and 1993 (limiting blue mag 20.5).

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Journal keyword(s):

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 SN 2005A SN* 02 30 43.25 -02 56 19.8     17.1     SNIa 60 1

Query : 2006CBET..352....1B

Basic data :
SN 2005A -- SuperNova
Other object types: otypes_help 		SN* (2012MNRAS,SN), smm (JCMTSE,JCMTSF)
ICRS coord. (ep=J2000) : 		02 30 43.25 -02 56 19.8 (Optical) [ ] C 2015ApJS..220....9F
FK4 coord. (ep=B1950 eq=1950) : 		02 28 11.66 -03 09 36.4 [ ]
Gal coord. (ep=J2000) : 		171.67920 -56.10817 [ ]
Radial velocity / Redshift / cz : 		V(km/s) 4404 [~] / z(spectroscopic) 0.0148 [~] / cz 4437 [~]
   (Opt) D 2012MNRAS.425.1789S
Spectral type: 		SNIa C 2015ApJS..220....9F
Fluxes (1) :
V 17.1 [~] D 2008yCat.2283....0B
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Hierarchy : number of linked objects
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Identifiers (3) :
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SN 2005A JCMTSE J023043.0-025614 JCMTSF J023043.0-025614

References (60 between 1850 and 2026) (Total 60)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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