[mmaimcal] ImCal Meeting WEDS 22 Feb

Al Wootten awootten at nrao.edu
Tue Feb 21 15:40:56 EST 2006


Folks,

Recall that collisions of our usual time with a PSI meeting and with the
ASAC telecon have prompted us to move our meeting to tomorrow, which some of us
will remember as Washington's REAL birthday.

Date: 22 February 2006
Time: 4:00 pm EST (6:00 pm Santiago; 2:00 pm Socorro, 2:00 pm Tucson)
Phone: Phone: (434)296-7082 (CV SoundStation Premier Conference phone 3rd floor). No Video planned.
Past minutes, etc on MMA Imaging and Calibration Division Page

News
The AOS TB Shell Arises The AOS TB Shell Arises: 15 Feb

    * Science Requirements -- The revised document is located in the Science area.
          o Subarrays:
    * Characterization -- Move to Ops?
          o 19 applications for 2nd ALMA postdoc. Status report.
          o Science IPT Q3 Q4 2005 Quarterly Report

Topics

    * SRR Topics
          o Date, venue of followup
          o AI #18 from your report of the July 2005 SRR says:18 OPEN Sci, SE -> FE DS 2006-02-17 70 "Check need for requirement on -3dB freqs.
          o QUESTION: How big a frequency change of ANY of the local oscillators will we ever want, where we want to refer the interferometric phase of the new frequency to that of the original frequency? An equivalent question is how big a frequency change will we ever want, without having to recalibrate the phase?
                + Should our spec be "we want the phase to be reproducible within 0.5 degrees (??) for any frequency change of any LO, but we want the phase change to be computable without further calibration, to the same tolerance, for any frequency change up to [X] GHz."

Please think about the Question up for discussion.  Peter, Dick and Clint may
join the discussion.

Clear skies,
Al



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