ALMA Science Advisory Committee

Draft Agenda for ASAC Telecon November 13, 2000

Conference Date: December 11-2000 (Monday)

Here's the dial-in information for the telecon (last of the millenium):

Conference Date: Dec-11-2000 (Monday)

Conference Time: 10:15 AM EASTERN TIME=15:15 UT

Conference Duration: 1 hr

Service Level: STANDARD

Call Type: MEET ME/DIALOUT

USA Toll Free Number: 1-888-391-6586

Non-USA Number: +1-415-228-4734

PASSCODE: ALMA

Conference Leader: Mr Al Wootten

Agenda items so far include:

Old Business

(1) Please approve the minutes of the November Meeting.

New Business

(1) The Proposal for the Feb 23-24 Proposed Face-to-Face ASAC Meeting. -- Walmsley, Local Organizing Committee

Please make your Reservation. December 16 is too late!

Other dates during the timeframe:

Feb 19-20 receiver PDR in Tucson

Feb 25-26 Configuration PDR in Grenoble

Mar 5-11th Meeting on Cosmic Masers (Rio de Janeiro)

April 5-6 ACC meeting in Tokyo

Nominations have been received for the Japanese members of the ALMA Science Advisory Committee:

ASAC Members from Japan:

  • Yasuo Fukui (Nagoya U.)
  • Tetsuo Hasegawa (NAOJ)
  • Hiroshi Matsuo (NAOJ)
  • Naomasa Nakai (NAOJ)
  • Seiichi Sakamoto (NAOJ)
  • Ken'ichi Tatematsu (NAOJ)
  • Masato Tsuboi (Ibaraki U.)
  • Satoshi Yamamoto (U. of Tokyo)
  • Ryohei Kawabe, who was an active observer, is to be deleted from the list.

    (2) Report on the Antenna CDR - Welch

    (3) Project Book, Polarization - Crutcher

    For the first time in the joint project, there is an entry for all chapters in the project book. Please see The Project Book and comment. Chapter 5, on receivers, front end and WVR is of special interest.

    Dick will discuss his concerns: 'I'm concerned that polarization seems to be getting shorted. I don't know of a single design decision that has been made to insure good polarization characteristics. Darrell's bandpass calibration method may be an exception, but even that does not seem to have high priority. Things seem to me to be going the way the usually do with radio telescope design. One discovers that to make polarization work well will compromise other things, so polarization is not given sufficient priority and polarization science is compromised. Examples of adverse decisions include not having a prime polarization receiver on axis, not having the ability to rotate the receiver package so linears at 45 degrees can be received, refusal to have a circular polarized feed system, etc.. The ASAC job is of course to make the science case, not to dictate how the science specs will be met. I have seen nothing reporting how the hardware and software groups are going to guarantee that polarization science can be done at the required levels.'

    (4)ACA Issues - Baars, Guilloteau

    Please read NEW ALMA Memo No. 339. Koh-Ichiro Morita has made a summary of my recent imaging simulations for ACA. The summary may be seen at this URL. Any comments or questions are welcome.

    Brief summary:

  • 1. Imaging simulations show that it is hard to obtain significant improvement by simple adding of ACA data with ALMA data.
  • 2. I have proposed the modified method (method-2) to use smoothed total power data instead of raw total power data from 12 m antennas. Improvements of imaging quality have been obtained by this method.
  • 3. Imaging simulation using the method-2 shows that ACA with 6 m antennas would provide better performance on wide field imagings than that of with that with 8 m antennas.

    Please read Advance of Alma simulation at IRAM by F. Gueth, S. Guilloteau, R. Moreno and J. Pety considering the performance of ALMA with the ACA.

    (5) Fringe Tracking Centres -- Emerson

    The LO, systems & software groups have decided that for OTF interferometry, the fringe tracking center position will be kept constant for the duration of one scan. This has implications for the realtime software (a great simplification), for the analysis software (a similar simplification), for potential maximum data rates (possibly higher), for the maximum OTF field size that can be covered in one scan, and for how OTF interferometry observing is carried out.

    Please read ALMA Memo 331. The SSR group has also discussed this, and the relevant emails may be found here.

    (6) Site Issues - Booth, Kurz, Ishiguro

    Report from the IAU Meeting on Site Characterization in Morocco.

    (7) Next Teleconference - Monday, December 15, 2001 at 15:15 UT?

    ---New time? On Mondays Christine Wilson is unavailable from 10:30-11:30 EST and 1:30-2:30 EST. Suggestions: Move telecon 45 minutes earlier? According to one calculation, the time zones relevant are now (1515 UT):

  • 0715 am PST
  • 1015 am EST
  • 1115 am Chilean time
  • 1515 am UT
  • 1615 am CET
  • 2415 am Japan

    so this change would affect our three west coast members most severely. Other possibilities include different days.