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Virtual Telescope predicts the signal-to-noise and other parameters of imaging and/or spectroscopic observations as a function of telescope size, detector noise, and other factors for the Next-Generation Space Telescope.
ericsteinbring/virtual_telescope
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Virtual Telescope Download the tarfile called virtual_telescope.tar, and unpack it. Running the code will generate any required sub-directories and populate them with subsequent files. Copy entire contents of: /net/polaris/u/steinb/virtual_telescope including the sub-directories and their contents to a directory with more than 100 Mb free disk space. You will need IDL along with the astro-lib programs in order to run the code. Go to the directory and run IDL. >idl Compile as. >.run virtual_telescope.pro Then run it. >virtual_telescope The text-size is machine dependent. If the text on your display is too small contact the author on how to fix this. All questions and comments can be addressed to the author: Eric Steinbring Department of Astronomy and Astrophysics University of California at Santa Cruz Santa Cruz, CA, 95064 Office: (831) 459-5804 Fax: (831) 459-5717 E-mail: [email protected] WWW: www.ucolick.org/~steinb 1 November 2000
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Virtual Telescope predicts the signal-to-noise and other parameters of imaging and/or spectroscopic observations as a function of telescope size, detector noise, and other factors for the Next-Generation Space Telescope.
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