Submillimeter (λ < 1 mm) Continuum Imaging at CSO: A Retrospective
Abstract
This contribution is submitted on behalf of all students, postdocs, and staff inspired and supported by Tom Phillips to build an instrument and then wait for low precipitable water vapor. Over the 20+ years of its existence, the Caltech Submillimeter Observatory (CSO) has seen a succession of ever more powerful detectors to measure continuum emission in the shortest submillimeter bands available from Mauna Kea. These instruments have been trained on the nearest solar systems, the most distant galaxies, and objects in between. I show several images collected over the 5+ year history of the SHARC II camera and anecdotal comparison with past work.
Additional Information
© 2009 Astronomical Society of the Pacific. I thank the following people for supplying material for the conference poster and this paper: Dominic Benford, Ed Bufil, Sunil Golwala, Darek Lis, and John Vaillancourt. Part of the research described in this paper was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration.Attached Files
Published - Dowell2009p11356Submillimeter_Astrophysics_And_Technology_A_Symposium_Honoring_Thomas_G._Phillips.pdf
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Additional details
- Eprint ID
- 19924
- Resolver ID
- CaltechAUTHORS:20100914-081828183
- NASA
- Created
-
2010-09-16Created from EPrint's datestamp field
- Updated
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2019-10-03Created from EPrint's last_modified field
- Series Name
- ASP Conference Series
- Series Volume or Issue Number
- 417