SUMMARY AASTOWG (formerly AAOWG) Meeting May 23, 1994 Boulder, CO ******************************************************************* Attendees _______ NAME INSTITUTION AASTOWG John Bally CARA, Univ. of CO * Frank Bartko CASA, Univ. of CO Pierre Bely STSCI Jousef Billawala Univ. of CO Richard Chamberlin CARA, Boston Univ. Mike Dopita JACARA, Mt. Stomolo * Dave Fischer Antarctic Support Associates Ed Friedman Ball Aerospace Jeff Peterson CARA, Carnegie Mellon Univ. * Simon Radford NRAO Tony Stark CARA, CFA * David Theil CASA, Univ. of CO Jay Tilley Ball Aerospace ******************************************************************* AGENDA Monday, May 23 Morning 9:00 - 9:30 Intro and Review of the Lockheed AGO capabilities. - J. Bally 9:30 - 10:00 Review of the Australian Antarctic Initiative - M. Dopita 10:00 - 10:30 Review of POST - P. Bely break 10:45 - 11:00 NRAO MMA site selection strategies - S. Radford 11:00 - 11:15 SMA site selection and testing - A. A. Stark 11:15 - 11:30 South Pole Tipper Results - R. Chamberlin 11:30 - 11:45 Isoplanameters, scintilometers - J. Tilley 11:45 - 12:00 Bolometric tippers - J. Peterson 12:00 - 12:15 DIMMs - M. Dopita lunch 1:30 - 3:00 Open Discussion: break 3:10 - 5:00 Continue Open Discussion: During the morning, presentations were made in which plans for CARA, JACARA, and POST were discussed. After break, we heard presentations on recent site testing results in Antarctica and other observatory sites, and discussed a variety of site testing strategies covering optical, infrared, sub-mm, and radio wavelengths. The afternoon was devoted to discussions of strategies and implementation. The AASTOWG agreed on the following resolutions: RESOLUTIONS 1. The name of the Automated Astronomical Observatory Working Group (AAOWG) shall be changed to: Automated Astronomical Site Testing Observatory Working Group (AASTOWG) 2. Having considered the proposed JACARA plans for the deployment of an Automated Astronomical Site Testing Observatory, the AASTOWG strongly endorses this proposal, and additionally recommends that NSF be responsible for the deployment, operations, and logistics support tasks, that CARA be responsible for the development of the sub-mm sky brightness monitor, and further recommends consideration of the following provisional suite of instruments for deployment in a Lockheed AGO module: * Differential Image Motion Monitor (DIMM) * Sub-millimeter sky brightness monitor * Isoplanameter/scintilometer * Near-IR and mid-IR spectrometer * Wide-field-of-view optical imaging spectrometer * Acoustic sounder * Microthermal sensor array John Bally Co-chair AASTOWG