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[vsnet-chart 193] BVRI sequence near Nova SMC 1999-2
- Date: Wed, 18 Aug 1999 01:40:20 -0700
- To: vsnet-alert@kusastro.kyoto-u.ac.jp, vsnet-chart@kusastro.kyoto-u.ac.jp
- From: bas@lowell.Lowell.Edu (Brian Skiff)
- Subject: [vsnet-chart 193] BVRI sequence near Nova SMC 1999-2
- Sender: owner-vsnet-chart@kusastro.kyoto-u.ac.jp
Observers who have archive patrol images of the SMC that include the
recent nova may find the following BVRI data useful for calibration. These
stars fall within about a degree of the nova location, and will be far more
reliable than the USNO-A values. Remember that in these extremely crowded
fields the Schmidt plate scans utterly break down, and at least half the USNO-A
detections are spurious, plus the magnitudes themselves are totally bogus in
both A1.0 and A2.0.
Column 's' is the source of the positions: A = USNO-A2.0, G = GSC-ACT
(by Bill Gray), S = SkyView position from DSS image. Most of the data here
are from a paper by Vigneau & Azzopardi (1982 A&AS 50,119), where finder charts
can be found. The list extends down past V = 15, and for anything fainter
you'll need quite a large telescope (and accompanying image scale) to overcome
the crowding problems. The list below is extracted from (and is in the format
of) my large file at:
http://ftp.lowell.edu/pub/bas/starcats/loneos.phot.gz
\Brian
Name RA (2000) Dec s GSC V B-V V-R V-I
[HKS77] SMC 1-12 0 48 51.3 -71 26 30 A 14.97 -0.10
[HKS77] SMC 1-14 0 49 31.7 -71 21 54 A 9138-1741 13.21 0.64
[VA82] I-10 0 49 32.0 -73 01 37 A 14.87 0.37 0.17 0.44
[VA82] I-11 0 49 51.3 -72 55 45 A 9141-7595 11.16 0.00 0.05 0.08
[VA82] I-12 0 49 55.6 -73 00 09 A 14.63 -0.11 -0.00
[VA82] I-13 0 50 06.9 -73 00 10 G 9141-7577 12.55 0.97 0.52 0.95
[VA82] I-14 0 50 33.2 -72 57 44 S 13.17 0.19 0.14 0.32
[VA82] II-1 0 55 47.5 -72 39 30 A 13.27 0.01 0.06 0.17
[VA82] II-2 0 55 55.1 -72 40 31 A 9141-7723 12.02 1.40 0.68 1.27
[VA82] II-3 0 56 58.3 -72 31 18 A 9141-7686 13.42 0.16 0.13 0.27
[VA82] II-4 0 57 00.1 -72 30 10 A 14.90 -0.15 -0.03 -0.04
[VA82] II-5 0 57 23.5 -72 39 56 S 12.83 0.42 0.25 0.50
[VA82] II-6 0 57 27.0 -72 33 14 A 13.98 -0.20 -0.08 -0.15
[VA82] II-7 0 57 29.6 -72 32 24 S 14.64 0.14 0.25 -0.09
[VA82] II-8 0 57 58.2 -72 35 22 A 15.41 -0.20 -0.00
[VA82] II-9 0 58 01.6 -72 41 59 A 14.20 -0.05 -0.03 -0.09
[VA82] II-10 0 58 17.0 -72 30 47 A 15.15 0.08 0.13 0.19
[VA82] II-11 0 58 28.8 -72 31 55 A 15.62 -0.07 0.06
[VA82] II-12 0 58 29.7 -72 41 09 A 14.62 -0.04 0.01 0.07
[VA82] II-13 0 58 32.4 -72 33 28 A 9141-7816 13.64 1.85 0.92 1.72
[VA82] II-14 0 58 38.3 -72 41 42 S 15.26 -0.16 -0.02
[VA82] II-15 0 58 49.2 -72 32 54 A 14.27 1.51 0.75 1.46
[VA82] II-16 0 58 52.0 -72 38 54 A 15.55 -0.14 -0.08 -0.05
[VA82] II-17 0 58 53.5 -72 40 39 A 9141-7845 11.81 1.61 0.85 1.72
[VA82] II-18 0 58 55.7 -72 32 08 A 12.77 -0.11 -0.03 -0.09
[VA82] II-19 0 58 59.3 -72 44 34 A 14.20 -0.16 -0.04 -0.06
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