I know that some instruments suffer from a lack of stability which can lead to a shift in the position of the reference spectrum relative the the CCD pixel positions...hence the concept of taking a reference before and after an observation.
My question is - has anyone actually analysed the problem and determined the variables which should be addressed??
Accepting it is one thing - finding and fixing the root cause is another.....
Shift in Reference spectrum with instrument orientation
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Shift in Reference spectrum with instrument orientation
"Astronomical Spectroscopy - The Final Frontier" - to boldly go where few amateurs have gone before....
"Imaging Sunlight - Using a digital Spectroheliograph" - Springer
http://www.astronomicalspectroscopy.com
"Imaging Sunlight - Using a digital Spectroheliograph" - Springer
http://www.astronomicalspectroscopy.com
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- Posts: 197
- Joined: Thu Oct 25, 2012 5:45 am
- Location: St Leonards, Australia
- Contact:
Re: Shift in Reference spectrum with instrument orientation
I have adopted a f7 transfer lens for the reference lamp in the latest batch of Spectra-L200.
This uses a 4mm aperture in the housing, which allows all/ any reference lamp to be used ie Neon, Relco, Flouro, Filly etc.
Testing so far has shown good repeatability - as long as the lamp illuminates the aperture the position of the wavelength/pixel doesn't change.
Onwards and upwards.
This uses a 4mm aperture in the housing, which allows all/ any reference lamp to be used ie Neon, Relco, Flouro, Filly etc.
Testing so far has shown good repeatability - as long as the lamp illuminates the aperture the position of the wavelength/pixel doesn't change.
Onwards and upwards.
"Astronomical Spectroscopy - The Final Frontier" - to boldly go where few amateurs have gone before....
"Imaging Sunlight - Using a digital Spectroheliograph" - Springer
http://www.astronomicalspectroscopy.com
"Imaging Sunlight - Using a digital Spectroheliograph" - Springer
http://www.astronomicalspectroscopy.com