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1998di の検査結果
To: vsnet@kusastro.kyoto-u.ac.jp Date: Sun, 06 Sep 1998 03:15:10 +0900 From: Seiichi Yoshida <seiichi@muraoka.info.waseda.ac.jp> Subject: [vsnet 1596] sn1998di.fts Dear VSNET members, Hello. I am Seiichi Yoshida working on the MISAO Project. Now I introduce you the examination result of the image of (SN)1998di, sn1998di.fts taken by Dr. Schwartz. These data are automatically measured by the PIXY system, an automatic image examination software, of the MISAO Project. Reference catalog is USNO-A1.0 (V) [V=R+0.375(B-R)]. False data removal and identification verification have been done by hand after all. For more information about the project and the system, please see the URL: http://www.info.waseda.ac.jp/muraoka/members/seiichi/misao/ The output view of the PIXY system is available at: http://www.info.waseda.ac.jp/muraoka/members/seiichi/misao/tmp/vsnet/sn1998di.gif The data of 1998di is: 19 24 38.22 +59 41 47.2 mag=16.5 x= 71.15 y= 268.48 1998di 19h24m38s.19 +59o41'46".7 16.8 mag type:(dn) Aug. 2 M. Schwartz The positional difference from IAUC data is 0.6 arcsec. Unfortunately, the arm of a galaxy MCG+10-27-012 was detected, as a red star plotted in "Detected Stars" chart (sn1998di.gif). This faint object is an anonymous galaxy. 19 24 19.33 +59 38 09.3 mag=17.2 x= 188.84 y= 441.75 USNO1425.09788959 19 24 19.28 +59 38 08.9 16.1 R 17.2 B (16.51V) USNO1425.09788999 19 24 19.46 +59 38 09.4 17.0 R 18.0 B (17.38V) The three stars which are not in USNO are all near by another star. So the data in USNO are probably blending. Image Information **************************************************** Image size: 512 x 512 Center: 19 24 07.80 +59 41 59.1 Field of view: 10.62 x 10.62 arcmin Pixel size: 1.24" / pixel P.A.: 359.05 deg Limiting mag: 18.4 mag Faintest mag: 19.6 mag Position error: 0.28" 0.40" Mag error: 0.51 mag The following stars are not recorded in the catalog. ***************** 19 24 38.22 +59 41 47.2 mag=16.5 x= 71.15 y= 268.48 1998di 19h24m38s.19 +59o41'46".7 16.8 mag type:(dn) Aug. 2 M. Schwartz 19 23 59.13 +59 38 54.6 mag=16.9 x= 311.32 y= 403.47 19 23 50.14 +59 38 57.5 mag=17.5 x= 366.08 y= 400.23 19 23 27.45 +59 40 21.2 mag=18.1 x= 502.98 y= 330.35 The following stars may be variable. ********************************* 19 24 29.05 +59 42 01.5 mag=14.7 x= 126.78 y= 256.06 USNO1425.09790911 19 24 29.00 +59 42 01.0 10.3 R 11.3 B (10.68V) MCG+10-27-012 R.A.=19 24.4 Decl.=+59 42 15 mag 19 24 37.51 +59 41 43.1 mag=15.3 x= 75.54 y= 271.67 USNO1425.09792613 19 24 37.56 +59 41 43.9 11.4 R 12.8 B (11.93V) IRAS 19238+5933 R.A.=19 24 39.71 Decl.=+59 39 31.3 (17 x 8", p.a.=147) flux(12)=0.66 flux(25)=0.17 flux(60)=<0.40 flux(100)=<1.22 10% variable 19 24 39.34 +59 39 29.0 mag= 9.8 x= 65.97 y= 379.66 USNO1425.09792944 19 24 39.33 +59 39 28.7 11.1 R 13.1 B (11.85V) IRAS 19238+5933 R.A.=19 24 39.71 Decl.=+59 39 31.3 (17 x 8", p.a.=147) flux(12)=0.66 flux(25)=0.17 flux(60)=<0.40 flux(100)=<1.22 10% variable 19 24 41.47 +59 39 48.9 mag=17.6 x= 52.75 y= 363.86 USNO1425.09793404 19 24 41.51 +59 39 47.8 18.7 R 20.0 B (19.19V) The following stars may be moving by proper motion. ****************** 19 24 41.05 +59 39 38.5 mag=18.3 x= 55.47 y= 372.13 USNO1425.09793290 19 24 40.93 +59 39 38.6 17.7 R 20.3 B (18.68V) 19 24 39.10 +59 41 58.1 mag=19.4 x= 65.72 y= 259.74 USNO1425.09792925 19 24 39.27 +59 41 58.8 18.8 R 20.0 B (19.25V) 19 24 00.36 +59 42 06.1 mag=12.7 x= 301.20 y= 249.63 USNO1425.09785142 19 24 00.47 +59 42 07.8 12.2 R 13.5 B (12.69V) 19 24 08.53 +59 43 35.3 mag=13.7 x= 250.32 y= 178.74 USNO1425.09786758 19 24 08.40 +59 43 33.8 13.5 R 14.3 B (13.80V) 19 24 45.87 +59 46 11.5 mag=15.4 x= 21.72 y= 56.85 USNO1425.09794276 19 24 45.79 +59 46 09.8 15.1 R 16.2 B (15.51V) Photometric data ***************************************************** 1998di 16.5 IRAS 19238+5933 9.8 = USNO1425.09792944 MCG+10-27-012 14.7 = USNO1425.09790911 J192327.45+594021.2 18.1 J192350.14+593857.5 17.5 J192359.13+593854.6 16.9 USNO1425.09778067 17.7 USNO1425.09778224 18.2 USNO1425.09778248 19.2 USNO1425.09778298 17.4 USNO1425.09778341 15.6: : 以下、個々の恒星の光度測定値が続く。 |