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[vsnet-chat 4675] UBVRI sequence for WZ Sge
- Date: Thu, 2 Aug 2001 17:11:22 +1000
- To: <vsnet-sequence@kusastro.kyoto-u.ac.jp>, <vsnet-chat@kusastro.kyoto-u.ac.jp>
- From: "Bruce Sumner" <b.sumner@bom.gov.au>
- Subject: [vsnet-chat 4675] UBVRI sequence for WZ Sge
- Importance: Normal
- In-Reply-To: <3B5AD654.3D130801@astro.uio.no>
- Reply-To: <b.sumner@bom.gov.au>
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
UBVRI sequence for WZ Sge
For those observers performing differential photometry during this
current outburst here is a UBRVI sequence to assist you in reducing
your instrumental photometry to the UBVRI Standard System.
This sequence has been derived from Arne Henden's single night bright
star field photometry, and errors are estimated to be in the order of
+/-0.02 magnitudes.
All stars in this list, except #5, are shown on Reinder Bouma's recent
charts. In addition the AAVSO/RASNZ charts show all the comparison
stars except #7, #11 and #12.
Bruce Sumner
No RA (J2000) DEC X Y nobs V B-V U-B V-R R-I
1 20 07 33.7 +17 40 01 -39 -134 1 8.719 0.174 0.146 0.044 0.089
2 20 08 01.5 +17 40 12 357 -123 1 9.675 1.031 0.850 0.507 0.499
3 20 08 00.9 +17 38 00 349 -255 1 10.843 0.679 0.191 0.351 0.362
4 20 07 33.6 +17 39 16 -42 -179 1 11.760 0.197 0.153 0.049 0.108
5 20 07 45.1 +17 42 38 123 23 1 12.568 0.507 0.116 0.259 0.321
6 20 07 53.3 +17 42 03 240 -12 1 12.782 0.968 0.864 0.531 0.482
7 20 07 38.1 +17 37 05 23 -311 1 13.022 0.731 0.255 0.369 0.370
8 20 07 45.8 +17 40 01 133 -134 1 13.087 0.589 0.110 0.305 0.342
9 20 07 29.5 +17 43 36 -100 81 1 13.214 0.810 0.386 0.376 0.383
10 20 07 35.6 +17 45 10 -13 175 1 13.343 0.660 0.210 0.364 0.381
11 20 07 48.1 +17 38 55 166 -200 1 13.582 0.617 0.167 0.329 0.364
12 20 07 48.5 +17 42 18 172 3 1 13.678 0.705 0.342 0.368 0.358
13 20 07 36.2 +17 44 50 -4 155 1 13.897 0.443 0.284 0.268 0.312
14 20 07 38.5 +17 42 30 28 15 1 14.104 1.334 1.938 0.722 0.636
Notes:
1. Krzeminski and Kraft (ApJ 140, 921, 1964), have three comparison
stars in common with this sequence. Note that Henden's B-V and U-B colours
match well for those three stars, but V differs by roughly 0.04 magnitude
for all three, in the sense that Henden's values are brighter.
No V B-V U-B
1 9.70 1.11 Tycho-2 transformed
9.68 1.03 0.85 Henden 1 night
9.72 1.03 0.76 Krzeminski 2 nights
2 11.77 0.43 0.19 Henden 1 night
11.84 0.39 0.22 Krzeminski 2 nights
4 8.76 0.15 Tycho-2 transformed
8.72 0.17 0.15 Henden 1 night
8.76 0.16 0.13 Krzeminski 6 nights
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