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[vsnet-j 1591] AS 270 sequence



From owner-vsnet-sequence@kusastro.kyoto-u.ac.jp Thu Sep  6 09:19 JST 2001
From: "Bruce Sumner" <b.sumner@bom.gov.au>
To: <vsnet-chat@kusastro.kyoto-u.ac.jp>,
        <vsnet-sequence@kusastro.kyoto-u.ac.jp>
Cc: <aah@nofs.navy.mil>
Date: Thu, 6 Sep 2001 10:11:08 +1000
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Subject: [vsnet-sequence 102] AS270 sequence
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I have made a single night sequence for this symbiotic
variable from Arne's recent field photometry. As Arne
mentioned the zeropoint error will be in the 0.02mag 
range.
Bruce
-------------------------
231  AS270 (SAGITTARII)  (ZAND)   Range: 11.5-
     Position:   18 05 22.73  -20 20 38.1 (J2000, from .dat file)
     Magnitude:  V=11.544  B-V=1.103      (from .dat file)

ID     RA (2000)    DEC       X    Y   N    V      ERR     B-V    ERR     

a) Comparison star sequence

1    18 05 57.3  -20 16 27   333  251  1  11.419          1.435          
2    18 05 39.9  -20 24 45    87 -247  1  12.264          1.511          
3    18 05 15.4  -20 23 03  -257 -145  1  12.549          0.778          
4    18 05 28.9  -20 21 39   -68  -61  1  13.147          1.402          
5    18 05 46.0  -20 25 57   172 -319  1  13.413          0.770          
6    18 05 44.2  -20 24 02   147 -204  1  13.915          0.790          
7    18 05 39.8  -20 17 30    86  188  1  14.237          0.752          
8    18 05 36.4  -20 21 02    37  -24  1  14.393          0.779          
9    18 05 44.6  -20 21 25   154  -47  1  14.639          0.680          
10   18 05 18.1  -20 24 17  -220 -219  1  14.963          1.085          
11   18 05 35.3  -20 19 30    22   69  1  15.308          1.053          
12   18 05 26.2  -20 19 50  -106   48  1  15.926          1.145          

b) Wide-colour extension for CCD calibration

     18 05 13.0  -20 19 00  -292   98  1  13.191          0.455          
     18 05 24.2  -20 24 22  -134 -224  1  13.424          2.019          
     18 05 54.8  -20 16 27   297  251  1  12.187          2.715 

Notes:

1. This single night sequence is expected to have errors of about 
+/-0.02 mag.

2. Most of the bright stars in this field are quite red, which explains 
why the brighter sequence stars are redder than I would normally choose.

Bruce Sumner
6 September 2001


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