Translator Disclaimer
15 May 2000 CCD detector performance for NOAO's wide-field MOSAIC cameras
Author Affiliations +
In July of 1998 the National Optical Astronomy Observatories (NOAO) successfully upgraded MOSAIC 1, an 8192 by 8192 pixel array using eight Scientific Imaging Technologies, Inc. (SITe) St-002A thinned backside 2k by 4k charge coupled devices (CCDs). In July of 1999 MOSAIC II, a clone of MOSAIC I was commissioned also using eight SITe ST-002A CCDs. Additionally in December of 1998 NOAO implemented Mini- MOSAIC a 4096 by 4096 pixel array using two SITe ST-002A thinned CCDs. This report will discuss the performance, characterization and capabilities of the three wide field imagers now in operation at NOAO's Kitt Peak Observatory, Cerro Tololo Inter-American Observatory and at the WIYN Consortium 3.5-Meter telescope on Kitt Peak.
© (2000) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Thomas Wolfe, Taft Armandroff, Morley M. Blouke, Travis Rector, Richard Reed, Abhijit Saha, Robert Schommer, Chris Smith, Roger M. Smith, and Alistair R. Walker "CCD detector performance for NOAO's wide-field MOSAIC cameras", Proc. SPIE 3965, Sensors and Camera Systems for Scientific, Industrial, and Digital Photography Applications, (15 May 2000);


Mosaic3 a red sensitive upgrade for the prime focus...
Proceedings of SPIE (August 09 2016)
PS2 managing the next step in the Pan STARRS...
Proceedings of SPIE (September 25 2012)
Instrumentation at the W. M. Keck Observatory
Proceedings of SPIE (July 09 2008)
Large-area CCD mosaic for astronomical imaging
Proceedings of SPIE (August 12 1992)

Back to Top