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SUSI2
Fast Photometry
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It is possible to define sequences of many windowed frames in order to
sample the lightcurve of a rapidly varying object.
For example, the window presented above has a size of 100 x 400
pixels. The mean dead time between two images is 13 seconds, with an
exposure time of 10 seconds in the 3x3 mode, so a sampling time of
23 seconds. To use this mode, use the following procedure:
- acquisition template: SUSI_img_acq_Preset
(blind acquisition)
- a test exposure with full frame and 1x1 binning, SUSI_img_obs_Jitter,
with an offset to move the object of interest out of the
gap.
- Once this image is displayed, measure the position of the
object of interest (x,y in pixels on the RTD), and define the
read out window in a SUSI_img_obs_Jitter
template: (i.e.)
- Number of exposures = 1
- CCD Windowing Flag = TRUE
- First column of window = 50
- First row of window = 50
- Number of columns = 400
- Number of rows = 100
- excute the OB, and check that the object is well
centered. Adjust the window parameters as needed and
retest.
- modify the Number of Exposures to the number required (eg
500), and restart the OB.
Additionally, another template SUSI_img_obs_DoubleW, has
been introduced to perform fast photometry of two objects at the same
time (e.g. a variable star and a reference star) using two
non-overlapping windows. You follow the same procedure outlined above
to define the two sub-windows. To decrease the read-out-time between
two exposures you can use 2x2 bining or even better 3x3 binning.
Usually if you are looking for quick photometric variations, you are
not really interested in resolution. More important is to minimize
the dead time. The following is an example of a light curve obtained
with this method:

Seconds
Send comments to : ls-susi
Last modified: Wed Nov 5 2003 |
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