Date: Tue, 04 Aug 1998 19:28:08 -0500 To: vsnet-chat@kusastro.kyoto-u.ac.jp From: Larry <lrobinsn@ix.netcom.com> Cc: rhaler@lymax.com Precedence: list X-Distribute: distribute [version 2.1 (Alpha) patchlevel=24] X-Sequence: vsnet-chat 0 Subject: [vsnet-chat 0] Re: [vsnet 1499] Larry Robinson's SN1998dh image Errors-To: owner-vsnet-chat@kusastro.kyoto-u.ac.jp Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp >Date: Tue, 04 Aug 1998 19:26:23 -0500 >To: Yamaoka Hitoshi <yamaoka@rc.kyushu-u.ac.jp> >From: Larry <lrobinsn@ix.netcom.com> >Subject: Re: [vsnet 1499] Larry Robinson's SN1998dh image I redid my measurements using Astrometrica and my 60 sec image and the following data is recorded using different reference stars in the image than before: OBJECT RA DEC D MAG DMAG SA 0900.3310336 23 14 32.65 +04 35 30.8 +1.1 13.69 -0.11 SA 0900.3311229 23 14 59.02 +04 33 48.1 -0.5 13.88 -0.32 SA 0900.3308707 23 13 48.10 +04 36 18.9 -0.4 12.71 +0.11 SA 0900.3310824 23 14 47.47 +04 38 14.3 -0.3 14.26 +0.46 Object 23 14 43.72 +04 32 06.7 13.20 MEAN RESIDUALS: DRA = 7.54 DDEC=0.56 DMAG=0.25MAG So what am I doing wrong. I get the same answer. Any suggestions from this data? Any knowledgeable comment is welcome. I am still learning. Please help me. Larry >At 01:16 PM 8/3/98 +0900, you wrote: >>Dear SN watchers, >> >>Larry Robinson wrote: >> >>> Object Date U.T. R.A. (2000.0) Decl. Mag. Observer >>>SN1998dh 1998 08 02.26876 23 14 37.23 +04 32 19.5 13.2 V Sunflower >>>Observ >> >>This magnitude is quite brighter than other estimates. He wrote he >>have used Astrometrica and USNO-SA as reference stars, but it is >>uncertain which stars are choosed as a photometry reference. >> >>I have seen the image >>(http://ftp.kusastro.kyoto-u.ac.jp/pub/vsnet/SNe/sn1998dh/robinson.jpg) >>which seems to me that SN 1998dh was about 14.0 mag or so, comparing >>with 1306 and 1456 stars (USNO-A1.0). >> >>Is this a problem of reference stars or of a software? >> >>Sincerely Yours, >>Hitoshi Yamaoka, Kyushu Univ., Japan >>yamaoka@rc.kyushu-u.ac.jp >> >> >