Spectral line identification exampleSpectrograph ManualOpening Procedure for the SBO spectrometer:
PICKING YOUR SLITAny slit will do for stellar spectroscopy. The tradeoffs are resolution and exposure time. A wider slit allows more light to pass through it, and therefore requires less time. A narrower slit will reduce the blurring caused by overlapping spectra - think about slitless spectroscopy: if you spread a continuum over a detector, if there is an image at each wavelength the images will overlap. So a narrower slit limits that overlap to the width of the slitCOMP LAMPSThere are TWO comp lamps: Neon and HeAr. The Neon lamp appears orange, the HeAr lamp appears pink. If both are on, it will be pinkish-orange. You can turn the Neon lamp off by unplugging it. The HeAr lamp has a power switch on its power cordData from the SBO 24" telescope spectrometerTo transfer data from the 24" telescope to your home directory, use the program "WinSCP". Login to cosmos.colorado.edu with your normal username and password.The software at SBO saves the fits files generated as .fit files. Josh Walawender's solution also changes the stored variable type to signed (+/-) integer. You can also use my FIT to fits script Created 10/8/07 by Adam Ginsburg (adam.ginsburg@colorado.edu) |