Published July 10, 2008
| Published
Book Section - Chapter
Open
Using All Sky Cameras to determine cloud statistics for the Thirty Meter Telescope candidate sites
Chicago
An error occurred while generating the citation.
Abstract
All Sky Cameras were deployed at all Thirty Meter Telescope (TMT) candidate sites. The images gathered by these cameras were used to assess the cloud statistics for each site. We describe two methods that were developed to do this, a manual method based on inspection of blue and red movies, and an automated method based on photometric analysis of the images.
Additional Information
© 2008 Society of Photo-Optical Instrumentation Engineers (SPIE). The authors acknowledge the contributions of the late Hugo Schwarz to the development, construction and deployment of the ASCA units and his assistance during the interpretation of the ASCA images. The authors gratefully acknowledge the support of the TMT partner institutions. They are the Association of Canadian Universities for Research in Astronomy (ACURA), the California Institute of Technology and the University of California. This work was supported as well by the Gordon and Betty Moore Foundation, the Canada Foundation for Innovation, the Ontario Ministry of Research and Innovation, the National Research Council of Canada, the Natural Sciences and Engineering Research Council of Canada, the British Columbia Knowledge Development Fund, the Association of Universities for Research in Astronomy (AURA) and the U.S. National Science Foundation. The San Pedro Mártir ASCA system is owned and operated by the LSST project and data is made available to TMT as part of a data sharing agreement. The LSST design and development activity is supported by the National Science Foundation under Scientific Program Order No. 9 (AST-0551161) through Cooperative Agreement AST-0132798, and at NOAO under AST-0244680. Additional funding comes from private donations, in-kind support at Department of Energy laboratories and other LSSTC Institutional Members.Attached Files
Published - 701224.pdf
Files
701224.pdf
Files
(339.1 kB)
| Name | Size | Download all |
|---|---|---|
|
md5:efa5bcf76daaf63cd6198e5c2777cf52
|
339.1 kB | Preview Download |
Additional details
- Eprint ID
- 88543
- Resolver ID
- CaltechAUTHORS:20180802-154731093
- Association of Canadian Universities for Research in Astronomy (ACURA)
- Caltech
- University of California
- Gordon and Betty Moore Foundation
- Canada Foundation for Innovation
- Ontario Ministry of Research and Innovation
- National Research Council of Canada
- Natural Sciences and Engineering Research Council of Canada (NSERC)
- British Columbia Knowledge Development Fund
- Association of Universities for Research in Astronomy (AURA)
- NSF
- AST-0551161
- NSF
- AST-0132798
- NSF
- AST-0244680
- Department of Energy (DOE)
- Created
-
2018-08-03Created from EPrint's datestamp field
- Updated
-
2021-11-16Created from EPrint's last_modified field
- Caltech groups
- Thirty Meter Telescope
- Series Name
- Proceedings of SPIE
- Series Volume or Issue Number
- 7012