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...
Saved in:
Main Author: | |
---|---|
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/ |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|