Introduction
This page will provide information of interest to the observer preparing SITELLE observations. Like Megacam, WIRCam, and ESPaDOnS, SITELLE is operated in Queued Service Observing mode. Classical observing is not offered to observers. Observers will receive their SITELLE data after pre-processing (and astrometric and photometric calibration) by the CFHT ORBS analysis system, though they may request raw data if necessary.
Observing Constraints
Hereafter we list some of the constraints that PIs should keep in mind when writing a proposal for SITELLE, and when entering their PH2. The critical idea here is to keep OGs as short as what is allowed by the scientific goals of your proposal.
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