Submillimeter (λ < 1 mm) Continuum Imaging at CSO: A Retrospective

Details Submillimeter (λ < 1 mm) Continuum Imaging at CSO: A Retrospective Submillimeter (λ < 1 mm) Continuum Imaging at CSO: A Retrospective

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..417..143d&link_type=abstract

Submillimeter Astrophysics and Technology: a Symposium Honoring Thomas G. Phillips ASP Conference Series, Vol. 417, proceedings

Astronomy and Astrophysics

Astrophysics

Scientific paper

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.

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