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