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[vsnet-j 410] Possible Nova in Pup: astrometry update
- Date: Wed, 3 Jan 2001 18:17:13 +0900 (JST)
- To: vsnet-alert, vsnet-campaign-nova
- From: Taichi Kato <tkato>
- Subject: [vsnet-j 410] Possible Nova in Pup: astrometry update
- Cc: CBAT@CFA.HARVARD.EDU, GREEN@CFA.HARVARD.EDU, kazuyoshi.kanatsu@nifty.ne.jp, vsnet-j
- Sender: owner-vsnet-j@kusastro.kyoto-u.ac.jp
Possible Nova in Pup: astrometry update
R.A. (J2000) Decl.
07 37 56.91 -25 56 59.7 H. Abe, GSC-ACT (vsnet-alert 5492)
07 37 56.91 -25 56 59.0 G. Masi, Kyoto image, USNO A2.0 (vsnet-alert 5494)
07 37 56.880 -25 56 58.89 K. Kadota, GSC-ACT (vsnet-alert 5497)
07 37 56.88 -25 56 58.8 A. Henden, UCAC1 (vsnet-chat 3932)
Arne Henden wrote in [vsnet-chat 3932] as follows:
As I promised, I've updated the astrometry
in this field using UCAC1. The field photometry file at
http://ftp.nofs.navy.mil/pub/outgoing/aah/sequence/npup00.dat
now has improved astrometry (the photometry remains the same).
In particular, the nova candidate can be found at:
RA (J2000) DEC RA DEC V B-V V-R R-I
114.487000 -25.949680 07:37:56.88 -25:56:58.8 9.090 0.564 0.475 0.758
There is a UCAC1 star at:
RA (J2000) DEC mag
07 37 56.882 -25 56 58.85 13.60
So the nova candidate and this star are identical within error
(less than 100mas). This is a *very* small magnitude range for
a nova.
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