[Aavso-photometry] W Aur Comp Stars
Richard Huziak
huziak at sedsystems.ca
Fri Dec 9 10:50:58 EST 2005
On Oct 11, JJI questioned the seequence for W Aur. Arne responded with
the same answer most would give who have looked in detail at the
sequences off of old charts - that the sequences are sometimes good and
sometimes poor, based on photographic plates that may fall off at the
lower end. Often sequences also come from different sources and are
mixed, so inconsistent. But that is life until all stars in the sky are
measured precisely on the same scale. For visual observers, this may
or may not be an issue depending on how truly bad the sequence is, but
since all visual observers are using the same charts, at least their
data is consistent within itself (mostly). For CCD people, as Jim
pointed out, the choice of the comp star will produce different results
for the measured stars and will introduce a zero-point offset (which is
easily correctible if the comp star chosen is reported). This may look
poor on the LCG at times, but that is raw data, and anyone using it
needs to understand the zero-point offset issues. However, I ramble.....
After yacking with Jim on the AAVSO discussion group last eve, I
remembered I promised him I'd post a sequence for W Aur, since it is a
Suspect Field which I hit regularly. This is a 1-night sequence
linearly extended from the 9.5 comp star defined as 9.500. Stars not
measured are not in the frame, with the exception of the 131 and 132
which are close together, and I didn't bother at this time to readjust
the annulus to do these separately. Differences in JJI and HUZ derived
mags are due to different comp stars used.
At any rate - take it for what it is worth - it confirms Jim's result
that some stars are out by a fair bit at the lower end, but you will
find this on the majority of charts that did not get PEP or CCD
sequences, and this currently just is life. :-) An as a result, it
may take several tries to find an ensemble set of comp stars that 'makes
sense'. I could write a book about this and associated issues!
Column 1 - AAVSO chart value, Column 2 CCDV rounded value (based on 9.5
comp), Column 3 CCD value not rounded. Column 4 - error (stdev of 5
consecutive frames on 1 night). Sorry for the alignment.
rick (HUZ)
W Aur PRELIM SEQUENCE
Chart 050223 (Original HCO sequence 1944)
Single star photometry based on 95 = 9.500
One night, 5 frames, 4 Oct 2005
Instumental mags - not all-sky
AAVSO CCDV CCDV Err (stdev)
X.X X.XXX
9.0 not measured
9.3 not measured
9.5 9.5 9.500 Ref star defined as 9.500
9.6 not measured
9.9 not measured
10.0 9.9 9.869 0.007
10.5 10.4 10.374 0.007
10.7 not measured
10.9 10.9 10.887 0.005
11.4 11.3 11.325 0.006
11.6E 11.3 11.338 0.008
11.6SW 11.3 11.271 0.010
12.0 12.0 12.011 0.013
12.1 12.0 12.049 0.010
12.3 12.7 12.666 0.140
12.6 12.7 12.748 0.022
12.8 12.9 12.919 0.038
13.1 not measured
13.2 not measured
13.7 14.0 14.037 0.129
14.0 14.6 14.641 0.110
14.1 14.3 14.332 0.060
14.5 15.0 15.009 0.209
Nothing is known about variability in this field
I have 7 nights on this field if a better reduction is wanted.
Rick Huziak (HUZ)
Jim Jones wrote:
> I have two nights of V data from W Aur that is driving me crazy. The
> measured magnitude will vary by several tenths of a magnitude
> depending on which comp stars I use. I finally concluded that 13.2,
> 14.0, and 14.1 are in error (F chart dated 12/70). Using 13.1, 11.4,
> 12.1 in an ensemble, I measured as follows:
>
> 13.2 13.57 +/- 0.007
> 14.0 14.56 +/- 0.01
> 14.1 14.29 +/-0.01
>
> Both nights data are consistent. I figured that such a thing isn't
> likely so I must be doing something wrong. But the new values result
> in consistent measurements of the variable.
>
> So is anyone else having problems with W Aur?
>
> Thanks
>
> Jim Jones, JJI
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--
* * * * * * * * * * * * *
Richard Huziak
Manufacturing Engineering
SED Systems
Saskatoon, SK, Canada
tel. (306) 933-1676
<huziak at SEDSystems.ca>
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