One basic step in calibrating raw science images is debiassing. Every exposure by the camera contains a non-zero ``bias'' level, introduced by the AD converter on the FIERA. Because the bias is literally added by the instrument it needs to be subtracted from every exposure. A bias image is a zero-second exposure and typically for each night multiple bias images (5-10) are averaged to create a ``master'' bias image, which is subtracted from the science images. By using a bias image to correct for bias, any structure in the bias is corrected for, especially also any structure orthogonal to the CCD readout direction. A disadvantage of using bias images is that there may be a significant time difference between the determination of the bias and the (science) images that you want to correct. Therefore a different method (overscan correction) is often used when the bias level of a camera is variable on relatively short timescales.
In AWE the bias image used to correct raw science images is called
the BiasFrame.
Creating bias images is not the only way to correct images for bias. Pre-
and overscan regions can be used for this purpose as well. These regions
are strips of 1#1
In AWE, bias images are assumed to be available for your data. Bias
images are always required. However, it is possible to use a number of
different overscan correction methods. When running tasks, the method of
overscan correction can be specified with the option ``overscan''. Possible
values are:
To derive a master bias image, it is necessary to derive ReadNoise objects
first (if they are not already present). See the ReadNoise
/portal/howtos/man_howto_readnoise/man_howto_readnoise.shtmlHOW-TO
for more information.
Now derive the master bias as follows:
Or using short options:
where "oc", or "overscan" is one of the values described in the previous
section.
1.1.3 AWE: combining both methods
In AWE, both methods can be used together. It is possible to subtract the
overscan values from the bias images themselves, and then create a master
bias image. This master bias image will have an average level of 0,
approximately. If you then use the overscan regions in the science images
as well as the master bias image, you will correct for both structure in x
direction, as well as variations in the bias level. Obviously, if the bias
changes in level as well as structure on short time scales, there is
little that can be done.
1.1.4 Syntax, examples
awe> dpu.run('Bias', instrument='OMEGACAM', date='2014-04-28', overscan=6, commit=1)
awe> dpu.run('Bias', i='OMEGACAM', d='2014-04-28', oc=6, C=1)