PNS MANUAL: Focussing the Spectrograph
Focussing the spectrograph
The PN.S has a mask which can be flipped into the focal plane. It consists of a regular
grid of holes, with a small slit in the center of the field. By illuminating the mask with an arc lamp, focus exposures can be taken so that each arm may be focussed onto the mask. Later on, at night, the telescope is also focussed onto this same focal plane.
Focus adjustments are made with three capstans on the mount of each CCD. The procedure described below first finds a focus in the center of the field, and then corrects for tilt
of the CCD with respect to the image plane.
Usually the CCDs will be close to focus after being put
on the PNS by the ING team.
Focussing probably has to be re-done after any filter change!
For a list of focus offsets between filters, see here.
It is simplest to focus one arm at a time. It may take several hours to complete this task!
Once the focus and tilt are properly corrected, lock down the dewars.
This is done by winding back the locking nuts, then gently
winding down the screws with finger pressure only until they contact the
black flange (visually check this). Then wind down the
locking nuts to eliminate the possibility of the screws loosening.
- Window the CCDs. Fast readout speed may be used for focussing.
- Make sure image viewer (ximtool or whatever) is viewing the whole
chip: set stdimage=imt4096
- Note the initial positions of the capstans
(they are gradated, but it is not possible to get
an absolute reading from them as their full range is more than one turn).
- Loosen the locking screws if required
- For initial starting point, manually set the capstans to positions
such that the mount is evenly spaced away from the instrument.
A poor starting position can result in an inability to focus the spectrograph
(because of finding local minima?)
- Put in the mask and open the shutter:
issue CALIB command on PNS console.
- Issue AGCOMP on the A&G console.
- Take an arc exposure (ca. 3 minutes): issue
ARC PNSL (or PNSR) 180 on DAS console, then switch on lamps
(COMPLAMPS CUAR+CUNE on A&G console). Switch them off (COMPLAMPS OFF) before end of exposure.
- Now do a focus sequence: turn all capstans by the same amount and take new exposures.
Measure the fwhm of a bright arc line in the images
(using the "j" key in imexam).
Avoid the corners, where the image quality degrades a bit. Best measure the spectra from spots diagonally inwards from the corners (3 in x, 3 in y) and near the center. As holes in the mask may have different sizes, be consistent about which holes to measure. Record the measured fwhms and corresponding capstan turns. Typical
focus steps are 0.1 - 0.2 turns.
Note it may be desirable to adapt this procedure to using the tungsten
lamp since the exposure time would be much shorter.
- Once the best average focus has been found, look for systematic changes in focus that may indicate tilt. Tilt causes a systematic degradation of focus away from a line through the center of the field. Decide which direction to correct.
Typical steps for tilt corrections are 0.3 turns.
- A tilt about a vertical (i.e. spatial direction) line can be corrected by turning capstan 1 and 2 clockwise, and 3 twice as far counterclockwise.
- A tilt about the horizontal (dispersion) axis can be corrected for by turning 1 and 2 equal amounts in opposite directions, and leaving 3 alone.
- Perform a sequence of measurements at different tilts, until the focus is as uniform as possible.
- Finally it is a good idea to tweak the focus again, without changing the tilt.
FWHM should be close to 2.5 pixels over most of the field when the focus is good.
- Now repeat for the other arm!
It seems that filter changes affect the focussing. Here are the offsets
determined for the A -> B change, i.e. the changes required if the spectrograph
was in focus with A and you change to B.
All turns counter-clockwise
L1 0.925 -> 0.45
L2 0.875 -> 0.40
L3 0.475 -> 0.00
R1 0.15 -> 0.725
R2 0.85 -> 0.425
R3 0.75 -> 0.32
On 23/04/2012 we used the following offsets to change from AB0 to A0
Offsets (- is counter-clockwise):
AB0 applied A0
(absolute) offset (absolute)
L1 0.10 -0.10 0.00
L2 0.05 -0.10 0.95
L3 0.25 -0.10 0.15
R1 0.80 -0.10 0.70
R2 0.80 -0.10 0.70
R3 0.70 -0.10 0.60
PSF is about ~2.9 pixels (a-imexam, moffat profile)
Here are the offsets for the AB -> B change
0.5 turn counter-clockwise
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Last updated 28-03-2006
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