Bruce Truax
May 23, 2008
Arlin Crotts (Columbia University) and Gerald Cecil (University of North Carolina) have developed a lunar observing program for Calypso called Lucky Imaging. This program uses a high speed CCD camera from Andor Corporation mounted in the position of the WFCam guide camera. A variety of color filters are used for the observations with each filter cell containing the appropriate color filter plus a selected ND filter in order to allow exposure times in of approximately 0.1s. These exposure times are fast enough to freeze the atmostpheric turbulence. The observer then instructs the camera controller to acquire 5 to 8 sets of 1,000 images on each target. Once the data is aquired it is shipped (on a hard disk) to Gerald who then runs it through software which selects the sharpest images and aligns and stacks those images to form a final, high resolution, low noise image. The name Lucky Imaging comes from the fact that only the best images with almost perfect seeing (the lucky ones) are selected for analysis.
Calypso can be switched from normal observing to Lucky Imaging in less than 1 hour. The switch involves removing the normal guide camera and installing the Andor camera + filter, lugging the Andor camera control computer up to the observing level and connecting it to the camera and the network and testing the camera function. Switching back is also about 1 hour of work.
Observing the moon does require some special software to generate the pointing and tracking information. Russell Owen provided Calypso with a Python script which generates the required TCC commands to point and track objects on the moon based on their lunar longitude and latitude. These commands need to be given directly to the TCC, bypassing the TOI. This is a relatively simple operation involving multiple windows and cutting and pasting operations but once you get proficient at the procedure it is quite efficient.
This document provides instructions on how to change over the telescope for Lucky Imaging, how to connect to the Andor camera computer and how to tell Calypso to track objects on the lunar surface.




In the best Bentley service manual tradition - Removal is the reverse of the installation procedure. Actually there is one exception, the Focus Reference label needs to be re-installed on the lens tube. Print a new Focus Reference label using the label printer which is located in the library on the top of the bookshelves. Position the label so that its bottom edge is located at the same position recorded in step 5 above. When you slide the lens tube back into the mount on the WFCam position it so that the bottom of the label just touches the mount.

SET INSTRUMENT=ANDOR


/Shared Items/Calypso Documents/Lunar Observing Program/lunar_pointer 2/./moon_pos_calypso.py FEATURE_NAME where FEATURE_NAME is the name of the feature you wish to observe (i.e. TYCHO)tcc track 283.333820, -26.291222/distance=0.00268635 geo /keep=bore
tcc offset arc 0.0, 0.0, 0.000136923, 0.000021975, 4718274959.00 /computed
Ignore the TCC and copy the rest of the first line. Open the TCC command window in the TOI and paste the command into the text field and press send. 
We have tried using offset commands to nudge the pointing direction while performing lunar tracking and found that none of the offset commands work properly. It does not seem to be possible to offset and maintain the proper drift rate. If it is necessary to offset the telescope you are advised to compute the new coordinates on the moon and enter a new feature with those coordinates in the "features.dat" file located in the directory with the Python script.
Rather than pasting the track and offset commands into the TCC Command dialog window I found it much quicker to issue the commands directly to the TCC. To do this, open another XTERM window and log into charon as user TCC. Once logged in start a TCC session using the command TELRUN. Once you have this separate session running it is possible to paste the track and offset commands directly into this window. It saves a few mouse clicks.