Astronomical observations can be divided into two fundamental types: direct imaging and spectroscopy. Astronomy Camp provides the opportunity to explore both observational modes in a stimulating 'hands on' environment. The Astronomy Camp spectrograph is adaptable to both the 40" and 60" telescopes on Mt. Lemmon and can be used to explore the properties of a variety of astronomical objects.
Download a IRAF-ready HgNe linelist for wavelength calibration, labeled spectra of Hg and Ne lines , and FIVEL, a Fortran code that will compute physical conditions in photoionized nebulae.
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|visitors since Feb. 4, 1997.||Authored by Craig Kulesa Last modified: Wed Sep 27 16:22:02 MST 2000|