Signal to noise ratio of the image of the star Capella with respect to the CCD temperature / Rafidah Sarnin

This study focused on signal to noise ratio of the image of the star Capella with respect to CCD temperature. In this research we used Meade 8" LX200 GPS Telescope, SBIG ST-8XME CCD Camera and computer to link the telescope and CCD camera. We also used the computer software such as AIP Software...

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Bibliographic Details
Main Author: Sarnin, Rafidah
Format: Student Project
Language:English
Published: 2007
Subjects:
Online Access:https://ir.uitm.edu.my/id/eprint/46678/1/46678.pdf
https://ir.uitm.edu.my/id/eprint/46678/
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