Difference between revisions of "Astronomical Spectroscopy"
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The overall goal of the Astronomical Spectroscopy Project is to be able to collect and reduce data gathered from astronomical objects. This is being done using a Celestron CPC 800 GPS (XLT) telescope and a fiber-fed Ocean Optics USB2000+ spectrometer. | The overall goal of the Astronomical Spectroscopy Project is to be able to collect and reduce data gathered from astronomical objects. This is being done using a Celestron CPC 800 GPS (XLT) telescope and a fiber-fed Ocean Optics USB2000+ spectrometer. | ||
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[[File:TelescopeSystem.png]] [[File:TAdapter.png]] | [[File:TelescopeSystem.png]] [[File:TAdapter.png]] | ||
Revision as of 14:56, 7 December 2013
The overall goal of the Astronomical Spectroscopy Project is to be able to collect and reduce data gathered from astronomical objects. This is being done using a Celestron CPC 800 GPS (XLT) telescope and a fiber-fed Ocean Optics USB2000+ spectrometer.
Presentations:
Links:
