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Re: Last Night's Run
tom
i believe it is recommended that one take bias and dark frames at
different temperatures so that one knows what the system is like
. . maybe a few at each temp just to make certain it is within a decent
sigma :]]]]] better confidence level this way :]]]
keep with it, you are heading in the right direction, it is just a long
row to hoe
best
jamie
On Mon, 14 May 2001, Tom Droege wrote:
> Jure and all,
>
> The plan is to take one bias frame at the start of each run. This would
> normally be done after the temperature had stabilized. By starting with a
> bias and a dark, the present program can use dusk time that is otherwise
> useless. The bias frame now includes a temperature. The bias level will
> wander around with the ambient temperature though the sigma should be
> pretty constant. The bias level shift will be of order the noise level, I
> think. When I get enough of this data I will encourage someone to plot the
> bias level vs the available temperatures. I expect to see about 6 ADU
> counts per C ambient shift. This is just 100 parts per million resistor
> change and the 16 bit ADC.
>
> Tom Droege
>
> At 08:25 PM 5/14/01 +0200, you wrote:
> >Tom
> >
> >I think it can be very useful to have this bias frame. But, since it is not
> >really necessary to make bias frames at night, you may just make a
> >collection of
> >biases (and darks, for that matter) before or after you start imaging of the
> >sky. For the statistical reasons, it is better to have a
> >larger collection of
> >these files and then make some sort of average. Maybe one CDROM dedicated to
> >calibration images (bias and dark) would be in place, unless you have wildly
> >unstable cooling and read-out electronics.
> >
> > regards
> > Jure Skvarc
> >
> >Tom Droege wrote:
> > >
> > > Last night I got another run to add to disk set 18. Jure, you will be glad
> > > to know that this one has a bias run at the beginning. I will now keep
> > > running with this format.
> > >
>
>