Lessons
	Instrumental sensitivity Calculation of how much exposure time is needed for a given observation.
	Calibration and reduction of images Removing artifacts and imperfections, alignment, averaging, and tesselation of images.
	Deconvolution of images How to make images a sharper than the seeing allows, and the price one pays for doing so.
	Basics of observing Quick start for learning to operate telescope and caemera
	Spectral-line imaging Challenges in the use of narrow-band spectral-line filters in imaging. See also the H II region long form, below.
	Crowded-field stellar photometry How to decompose the image of a dense stellar cluster into its component stellar images.
	Observation of periodically-variable objects Observing cadence, light curves, and periodograms.
	Uncertainties in astronomical observations How to propagate uncertainties through the calibration and reduction process
	Pretty astronomical pictures With 4 hours and a few tricks in Photoshop, one can make extremely respectable pictures at Mees. With 40-80 hours, APOD quality.
Other resources
	Astronomy 203 Lectures 18 (first three sections) and 19-24 pertain to lesson 1.
	H II regions: the long form Elaboration on the short form presented in the lesson on spectral-line imaging.