[vsnet-j 390] Possible Nova Pup 2000: extended sequence

[Taichi Kato <tkato>]

Possible Nova Pup 2000: extended sequence

　以下の拡張比較星が発表されています。暗くなった場合は（精密なCCD等級が発表
　されていなければ）これをお使いください。

From: Brian Skiff <bas@lowell.edu>
Subject: [vsnet-alert 5481] Sequence near Nova Puppis

     These stars extracted from my photometric reference file should help
extend the calibration near the nova to fainter limits for wide-field images
and allow local zero-point adjustment of GSC and USNO-Ax.x magnitudes closer
to the object.  I note that GSC magnitudes are a few tenths fainter than V in
this area.

\Brian


Name             RA   (2000)   Dec        GSC       V     B-V
LF12  39       7 39 42.8   -26 28 03   6547-2012  10.37   1.13
LF12  26       7 37 57.2   -25 33 41   6543-2074  10.39   0.28
LF12   7       7 35 04.6   -26 15 10   6547-0059  10.65   0.10
LF12  53       7 41 44.0   -26 15 14   6548-2407  10.86   1.04
LF12  43       7 40 13.2   -26 35 57   6547-2182  11.45   0.08
LF12  19       7 37 17.0   -24 22 17   6539-3128  11.53   1.15
LF12  54       7 41 46.8   -25 34 36   6544-0950  11.54   1.10
Loden 2 3      7 41 02.4   -24 09 04   6540-4412  11.60   0.02
LF12  44       7 40 32.4   -26 53 41   6548-3449  11.67   1.18
Loden 2 4      7 41 04.7   -24 09 06   6540-3880  11.80   1.07
LF12  12       7 36 38.4   -26 05 11   6543-3321  12.19   0.45
LF12  13       7 36 50.1   -26 07 40   6543-3227  12.26   0.11
Loden 2 12     7 40 53.6   -24 17 12   6540-4155  12.38   0.16
Loden 2 11     7 40 59.4   -24 16 21   6540-2650  12.67   0.34
Loden 2 10     7 41 05.9   -24 14 58   6540-3952  12.98   0.55
Loden 2 14     7 40 43.6   -24 14 37   6540-4295  13.52   0.17

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