MMA Imaging and Calibration Group

Agenda/Minutes for meeting Monday, 31 Mar 2003 at 11:30am EDT.

Date: 31 Mar 2003

Time: 11:30 am EDT (9:30 am Socorro, 9:30 am Tucson)

Daylight Saving Time (DST) starts in North America on April 6th, 2003. Daylight Saving Time (DST) starts in Europe and ends in Australia on March 30th 2003.

Phone: (434)972-7268 (CV SoundStation Premier Conference phone 2nd floor).

Past minutes, etc on MMA Imaging and Calibration Division Page
 
 

Agenda

Notes from the meeting are in this font!
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Science IPT News - Wootten

News from my point of view.
Action Items from 11 March Science IPT Meeting.
Discussion of impressions of the Software PDR, AMAC and ANASAC meetings.
The ANATAC has requested advice on a number of items; please see Darrel's inquiry.
 
 
  • Project News - 
  • ASAC Agenda 2-3 April
  •  Software IPT Preliminary Design Review
  • was held in Tucson 18-20 March 2003.

  • AMAC Meeting 24-25 March Socorro
  • ASAC Face-to-face Meeting 2-3 April 2003 in Grenoble, France at IRAM. A tentative agenda is available above.
  •  May 26/27 ALMA Board face-to-face (Europe)
  • ALMA Week 2-6 June Victoria
  • November 3/4 ALMA Board face-to-face (S.A. groundbreaking?)

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    Proposed correlator upgrade -- Wootten


    There is a chart from Webber comparing correlator capabilities.

    Also see second generation correlator system requirements and specifications.  
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    Polarization Widget -- Wootten

     
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    After much discussion, it was decided that the polarization widget, perhaps a quarter wave plate, will be inserted at Band 7.
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    Scientific Benefits of a Single Antenna Design -- Wootten


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    Al summarized scientific reasons favoring a single antenna design. At its first meeting, in item
    (21), The Board endorsed the goal of the JAO to procure the production antennas to a single design which has been prototyped and evaluated.
    Note that it is a goal. Also, please see the ANATAC Report.
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    Illumination Offsets -- Holdaway


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     See Mark's report on illumination offsets tests and milestones. Recall that in ALMA Memo No. 402, Mark showed that offsets in the illumination of the dishes by the feeds would result in a phase graident in voltage patterns, a serious problem for high dynamic range mosaicing. Mark notes that a simple correction algorithm can remove essentially the entire effect of the voltage pattern phase gradient. In the report, he explores how to measure the offsets and to apply corrections to the (u,v) coordinates.
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    Calibration - Butler



     
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    AIPS++ - Myers

     
    The Skeptical Review occurred.

    - phase I final report (Lucas)

    - phase II+III progress reports (Lucas)

    The report written by J. Pety with all the testers is available at: http://iram.fr/~lucas/almassr/aips++reuse-phase2.pdf

    A report for Phase I is also available. The Audit is also available.  The current statusof Phase III is available.


     
     
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    Configuration - Holdaway

     

    Large Configuration: Progress Report.

      Version D of the configuration document (ALMA-90.02.00.00-001-D-SPE) the distance between pads is set to a distance of 15.15m. Last chance for comments!!!
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    Site Characterization - Radford


    Plans for Visit to the Site.


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    Other


    Reading Materials:
    ALMA Project Plan v1.0
    ALMA Bilateral Agreement

    most recent quarterly report  (No. 2)
    even more recent quarterly report (No. 3 dated 2003-Mar-31)



     
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     SMA News...
     
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    Upcoming Meetings - Wootten

    JUN 22-27, 2003 2003 IEEE AP-S INTERNATIONAL SYMPOSIUM AND USNC/CNC/URSI NATIONAL RADIO SCIENCE MEETING

    JUL 13-26, 2003 Twenty-Fifth General Assembly of the IAU Abstracts due NOW.

    JUL 22/25, 2003 IAU Symposium (221): Star Formation at High Angular Resolution, Sydney, Australia. Tyler Bourke is a co-chair of the scientific organizing committee. Good opportunity to show ALMA capabilities.

    SEP 22-26, 2003 4th Cologne-Bonn-Zermatt-Symposium on The Dense Interstellar Medium in Galaxies

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    Travel

     Oh, always

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