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[vsnet-newvar 1826] Re: GSC 6248:1255 Variability
- Date: Sun, 9 Feb 2003 11:47:58 +0100
- To: <vsnet-newvar@ooruri.kusastro.kyoto-u.ac.jp>
- From: "Ondrej Pejcha" <opejcha@volny.cz>
- Subject: [vsnet-newvar 1826] Re: GSC 6248:1255 Variability
- Delivered-To: vsnet-newvar-archive@ooruri.kusastro.kyoto-u.ac.jp
- Delivered-To: vsnet-newvar@ooruri.kusastro.kyoto-u.ac.jp
- References: <15f.1b7221c1.2b769fdf@aol.com>
- Sender: owner-vsnet-newvar@ooruri.kusastro.kyoto-u.ac.jp
> The star GSC 6248:1255 (in the field of V2540 Oph) appears
to be variable. I
> used GSC 6248:1364 (V=11.05, Rc=10.66) and SAO 160704
(V=9.97, Rc=9.72) as
> comparison stars. For reference, the Tycho 2 position
(J2000) is 17 37
> 22.694 -16 21 11.09 and photometry Bt = 13.160 and Vt =
11.422. This is a
> red star (M type). I did not find the star listed in the
GCVS. My CCD
> measurements are:
>
> 20020213.584 11.76V WJD
> 20020819.115 11.35V WJD
> 20020819.101 9.27Rc WJD
> 20020907.091 11.21V WJD
>
> Assume an error of +/- 0.1 magnitude to account for lack
of color correction.
The field of V2540 Oph was observed at Brno observatory in
VRI during 2002 mostly by me, some observations also with
Petr Sobotka and Jan Skalicky. The star Doug mentions is
overexposed on I band frames, but can be well measured on R
and V frames. Here is a list of nightly averages of
differential magnitudes with respect to GSC 6248 1364 (V-C):
R band:
2452413.484744 -2.0581 0.0082 5
2452461.486586 -1.8167 0.0069 3
2452478.395457 -1.7443 0.0033 3
2452483.363241 -1.7603 0.0059 3
2452506.308848 -1.8347 0.0012 3
2452517.288041 -1.9262 0.0076 5
2452520.276873 -1.8321 0.0179 3
2452574.209109 -1.6174 0.0213 3
V band:
2452461.487938 0.3520 0.0164 3
2452478.397049 0.3800 0.0053 3
2452483.366422 0.4163 0.0043 3
2452484.325555 0.3703 0.0128 13
2452506.310779 0.4957 0.0173 3
2452517.290398 0.4278 0.0169 5
2452520.278407 0.4020 0.0114 3
2452574.207490 0.6024 0.0212 3
Column 1: JD
Column 2: Averaged magnitude, weighted according to
photometric errors
Column 3: rms scatter of averaged magnitudes
Column 4: number of observations
The last measurement should be taken with care as it was
obtained at very high airmass (~20 degs above the horizon).
The star is probably some kind of low amplitude semiregular
pulsator.
Best regards,
Ondrej Pejcha
P.S: I have searched my I band photometry of this field with
code similar to that of Pojmanski (Astro-ph/0005236). There
does not seem to be any other variable stars except for
V2540 Oph and GSC 6248 1255.
> Regards,
> Doug West
> http://hometown.aol.com/dwest61506/index.html
>
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