Preview of Coming Attractions

["Tom Droege" <droege@snapmail.us>]

Finally there was a break in the weather and I got a short run where
everything worked.  I am still adjusting parameters for the coming run. 
This will probably take a couple of months.

In the run there was some change in the number of stars detected.  Mostly
at the beginning and end of the run which could be an atmospheric effect.

The first two plots are mag vs mag sigma.  I am now fairly confident that
this is what typical runs will look like.

I ran the result through WS and plotted the stars with WS over 10.  Note
that I am not yet using Michael's new software which might make WS more
effective.

This turned up one known variable, WY Hya, and a number of candidates of
which the last plot is typical.  Nothing found in Vizier for the last
plot.  Note to the critics and ghouls.  I am not claiming that this last
star is variable.  It just shows a trend that I find difficult to explain.
 It is not in all stars in the set, so I can see no reason that it is not
a real trend.

Tom Droege

i_sigma.png

v_sigma.png

J081410.9+002944.png

J081843.4+002851.png