Characterizing a CCD detector for astronomical purposes: OAUNI Project
DOI:
https://doi.org/10.21754/tecnia.v26i2.54Keywords:
Charge-coupled devices, Linearity, Gain, Readout noiseAbstract
This work verifies the instrumental characteristics of the CCD detector which is part of the UNI astronomical observatory. We measured the linearity of the CCD detector of the SBIG STXL6303E camera, along with the associated gain and readout noise. The linear response to the incident light of the detector is extremely linear (R2 =99.99%), its effective gain is 1.65 ± 0.01 e-/ADU and its readout noise is 12.2 e-. These values are in agreement with the manufacturer. We confirm that this detector is extremely precise to make measurements for astronomical purposes.
Downloads
References
} [1] Pereyra A, Cori W, Meza E, et al. "OA-UNI: an astronomical observatory at UNI". REVCIUNI. 2012; 15(1): 209.
[2] Ford WK. "Digital Imaging Techiques", Ann. Rev. Astron. Astrophys. 1979; 17: 189-212
[3] Holst, G. C., "CCD Arrays, Cameras and Displays", 1998, SPIE Optical Engineering Press.
[4] Janesick, J. R., "Scientific Charge-Coupled Devices", 2001, SPIE Press
[6] Performance Specification KAF-6303E, Revision 2, October 15, 2001
[7] http://www.sonnensystem.at/ccd-atik383-linearity-readout-noise-again
[8] http://spiff.rit.edu/classes/phys445/lectures/gain/gain.html
Published
How to Cite
Issue
Section
License
Copyright (c) 2016 TECNIA
This work is licensed under a Creative Commons Attribution 4.0 International License.