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[vsnet-obs 30226] [FWD] SN observation (APO)
- Date: Wed, 11 Oct 2000 10:31:55 +0900 (JST)
- To: vsnet-obs@kusastro.kyoto-u.ac.jp
- From: Hitoshi YAMAOKA <yamaoka@rc.kyushu-u.ac.jp>
- Subject: [vsnet-obs 30226] [FWD] SN observation (APO)
- Sender: owner-vsnet-obs@kusastro.kyoto-u.ac.jp
>Date: Tue, 10 Oct 2000 11:39:41 -0400
From: David Bishop <dbishop@vhdl.org>
Subject: [Fwd: 2000dk]
>From: Kevin Krisciunas <kevin@lensing.astro.washington.edu>
Subject: 2000dk
Yesterday I ran the data of Sept 20th through this program Dophot,
which gives point spread function (PSF) raw magnitudes. That's to
counter the plate scale of the 30-inch and the proximity of this
SN wrt the core of NGC 382. The calibration of the field stars from
aperture photometry is OK as is, b/c they are all nicely isolated.
As expected, the result for the SN via PSF mags comes out differently.
You might update on your website that V = 15.87, B-V = 0.08, with
uncertainties of +/- 0.03.
On Oct 5.26 UT I found V = 16.02, B-V = 0.54 (uncertainties +/- 0.02)
from two images obtained with the APO 3.5-m.
Kevin
------
Reformatted:
SN2000dk 20000920.20 15.87V APO (MRO)
SN2000dk 20000920.20 15.95B APO (MRO)
SN2000dk 20001005.26 16.02V APO
SN2000dk 20001005.26 16.56B APO
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