Starting with fast photometry



To get started with fast CCD photometry photometry, first start the tcpcom program by executing the fastphot_start script, and use it to obtain a frame of the field that the telescope is (currently) pointing to. Use the DS9 region feature to mark the target and reference windows in the CCD image displayed by DS9, and create a list of target coordinates. Next, convert the DS9 region output list to a format that the tcpcom program can understand, using the photcnv program. Transmit this list to the CCD controller from tcpcom and start a sequence of integrations. Windowed CCD integrations are then obtained and stored in cycles down to a few seconds. The CCD data can be processed and the resulting light curves displayed in real time with the rtp program.

How to start the tcpcom program.


A detailed description on how to set up windowed mode photometry is given in the tcpcom guide.
For a description on how to run the Real Time Photometry program, rtp, see the rtp guide.


How to exit the tcpcom program.

Before you exit tcpcom, make sure to put the transfer mode back to 'full frame transfer mode', using keystroke 't'. If you forget this, the standard ALFOSC CCD control program BIAS will hang once you make an exposure.

An alternative solution is to reset the CCD controller (staff only).


Last updated: 9/6 2006, Jacob Clasen.