Quick Start
- Run MAlign and analyze the images in the default (spectroscopic) mode. Send
the moves.
- Press the Load button on coma.tcl.
- After setting up on a field (in particular, make sure you are at the right
physical rotator angle, if you are doing imaging), click on the appropriate
mode button (Spectr. or Imaging).
- Start guiding once the DCS has corrected pointing for the new secondary
tilts.
- When imaging for a long time, you may want to update the secondary tilts
by clicking Imaging again in between exposures. PAUSE GUIDING when you do
this, and wait for DCS pointing to compensate before resuming.
Note: If you are in spectroscopic mode you do not need to update secondary
tilts for different rotator angles. All rotator angles use the same tilts.
Description of the Tool
The Coma Control Tool is shown below:

In operation, the main title
should show the relevant instrument (e.g. "ESI Coma Control Tool" as shown here).
The two top blue buttons, labeled "Spectr" and
"Imaging", are used to select one of the two modes. In spectroscopic
mode the secondary tilts are independent of physical rotator angle (ROTPPOSN),
and are optimized to eliminate coma in the telescope focal plane. In
imaging mode the secondary is tilted to the position which will eliminate coma
at the instrument's detector. The tool will minimize coma for imaging only at
the current physical rotator angle, ROTPPOSN. It will not actively "cone"
the secondary as is done on the high-precision f/25 secondary use with LWS.
Hence if you are in imaging mode you may want to tweak up the secondary tilt
in between exposures to keep image quality good.
Note that thebutton for the currently selected mode has a border
around it. The current mode is also shown in the following line of text.
Below the mode buttons are three informational lines. The first
line shows the mode, and in the case of imaging mode it shows you the value
of ROTPPOSN at which you last selected imaging mode. The second line contains
the current rotator angle and tilts. The third line contains an estimate of
the coma error in imaging mode. (In spectroscopic mode or after clicking "Reload"
this value is not relevant.) This value is calculated from the difference between
the current value of ROTPPOSN and the value when you last clicked "Reload".
This can be used as an indicator of when you should update the tilts if you
have changed rotator physical angle significantly since last updating them.
The "Reload" button is used after running MAlign, analyzing
images in the default (spectroscopic) mode, and sending the tilts. The coma
control tool will read the current tilts and assume that these are the tilts
relevant to spectroscopic mode.
WARNING: if you click "Reload" while
you are in Imaging mode you will incorrectly reload the current, imaging tilts
as the spectroscopic tilts. Unfortunately the only way you can recover is to
either reset to the spectroscopic tilts by hand and clicking "Reload"
again, or by rerunning MAlign.
At bottom left is a Help button which briefly describes the use
of the tool, and on bottom right a Quit button.
WARNING: it is generally not
a bad idea to click the "Spectr" button before quitting, if you are
in Imaging mode.
A Wish List
Some other modifications could be made to the way we handle coma control.
A number of DCS keywords could be implemented:
- Two keywords for the current "base offsets" appropriate for spectroscopy.
- A keyword for the value of ROTPPOSN at which the secondary tilts were
last set.
- A "mode" keyword.
Also, it would be better if the MAlign analysis software measured the tilt
offsets (as it now does), and then applies them to the secondary tilts stored
in the image headers. Currently it adds the tilt corrections to the current
values of (secthetx, secthety). Now if you were to send the corrections again
(e.g. if you wer unsure as to whether they took effect the first time), you
would overcorrect. If, instead, you were correcting the values stored
in the FITS headers of the images, you would always be sending the secondary
to the same absolute tilt.
Also, if a problem occurs and you lose track of what
tilts should be set, reanalyzing the latest MAlign data set will set to the
exact same tilts as it did before.
This would require that instrument headers start carrying the secthetx and
secthety keywords. The MAlign analysis software would look for these, and
if it does not find them it would read the current values as it does now.