[mmaimcal] FYI: 24 Apr 06 BIWEEKLY CALENDAR OF THE ALMA PROJECT at NRAO
Al Wootten
awootten at nrao.edu
Mon Apr 24 18:31:40 EDT 2006
Folks,
Comments, corrections, criticisms?
Al
BIWEEKLY CALENDAR OF THE ALMA PROJECT at NRAO
24 April 2006 - 8 May 2006
******************************** THIS FORTNIGHT****************************
Pursuant to Article 12.9 of the ALMA Agreement, Board Members have
officially designated Annelia Sargent as ALMA Board Chairperson
effective immediately and expiring at the end of the current term,
December 31, 2006.
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Near 11:20 hours on 2006 April 18 the Láscar volcano erupted,
generating a column of smoke of about 3,000 meters (10,000 feet) in
height. The eruption was observed from hundreds of
kilometers the distance and the ash-gray column throws particular material
and ash. Eruptions occurred near noon on the two subsequent days. On
20 April the ash plume passed over the ALMA site. Photos are collected at:
https://wikio.nrao.edu/bin/view/ALMA/LascarStirs06
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Past issues of this Calendar may be viewed at
http://www.cv.nrao.edu/~awootten/mmaimcal/ALMACalendars.html
See also the JAO ALMA Calendar overview at:
http://www.alma.cl/alma_project
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General Happenings
OSF (Ops Support Facility, 9600ft altitude): Approximately 64 people
are working on the ALMA site.
Santiago: Early discussions on Santiago ALMA Offices at Vitacura continue.
AOS (Array Ops Site, 16000ft altitude): Lascar erupted; see above.
The AOS Technical Building Foundation and Shell construction is
substantially complete.
Picture: http://www.cv.nrao.edu/~awootten/mmaimcal/AOSTB06Ap18.jpg
TUC: Emerson chaired Computing System Requirements Review, held via
multicon.
AOC: PSI testing has successfully spectrally cross-correlated a common signal
in the lab. The test involved sending the same analogue noise signal into two
different digitizers and through different channels of the same antenna
rack, into the correlator and producing a cross-spectrum. In a followup
test to occur shortly the same will be done using two different antenna racks.
The final report of the 4th offline user test, of CASA
- Common Astronomy Software Applications - is available at:
http://tinyurl.com/syqfc . CASA is a python binding of the
C++ functionality that was in AIPS++. This initial version of CASA had
pythony commands that had a one-to-one correspondence with AIPS++ Glish
commands.
The ALMA software continues to work end-to-end. Previous user testing
had identified 13 top priority items that needed to be addressed.
A user test 'spot check' of the ALMA integrated software report is complete.
See http://tinyurl.com/lmwx7
ATF (ALMA Test Facility, VLA site): Optical Pointing Test report available.
AEM personnel are on the AEC antenna working on metrology and drive systems.
NTC: Finished measuring all 8 Band 3 OMTs.
The final design review before procuring the production Master Laser and
Laser Synthesizer is scheduled tentatively for Charlottesville on 13 June.
NAASC (North American ALMA Science Center: Gallery of ALMA photos at:
http://www.alma.nrao.edu/almanews/almagallery/index.html
Mangum engaged in further discussion of calibration and source catalogue
issues with Ed Fomalont and John Benson. ALMA Science IPT telecon was
held.
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DAILY CALENDAR (Times EDT ) see
https://wikio.nrao.edu/bin/view/ALMA/AlmaCalendar
Mon 24 Apr
Tue 25 Apr
6:02 AM: Launch of CloudSat/CALIPSO is planned for 25 April 2006
(third attempt) at 3:02 AM PDT (1002 UTC). Live coverage on
NASA TV begins at 1:00 AM PDT.
10:30 AM-11:30 AM: JAO IPT Telecon
4:00 PM-5:00 PM: NAScienceIPT teleconference (open to all interested
parties) (434)296-7082
Wed 26 Apr
Thu 27 Apr New Moon
11:30 AM-12:30 PM: Management IPT Telecon
Fri 28 Apr
Sat 29 Apr
Sun 30 Apr
Mon 1 May Chile, Europe
Tue 2 May
10:30 AM-11:30 AM: JAO IPT Telecon
Wed 3 May
Thu 4 May
Fri 5 May
Sat 6 May
Sun 7 May
Mon 8 May Complex Molecules in Space: Present status and prospects with
ALMA 8th thru 11th May 2006, Fuglsøcentret, Denmark
EVLA Advisory Committee, Socorro
Mon 15 May Registration Deadline, IAU XXVI General Assy
Events of ALMA interest compiled at:
http://www.cv.nrao.edu/~awootten/mmaimcal/IAUALMA.txt
****************************** UPCOMING EVENTS ****************************
April 24-25 All day SRR followup meeting Garching
April 27 ALMA Board Telecon
April 28 1900 UT ANASAC Telecon
May 3 1500UT ASAC Telecon
May 3 1700UT NAASC Telecon
May 25 ALMA Board Telecon
June 13-14 all day ALMA Board Meeting Santiago
Jun 19-20 (tent)all day AIVCSV Meeting Santiago
Aug 1 Move of PSI to ATF
Sept 22-23 evening Dave Matthews Band CV JPJ Arena opening
November 9-10 all day ALMA Board Meeting Madrid TBD
Nov 13-16 all day Science with ALMA: a new era for Astrophysics Madrid
******************************* TECHNICAL NEWS ****************************
EVLA Memo #101 "Multi Frequency Synthesis Imaging for the EVLA : An initial
investigation"
Authors : Urvashi R.V., NRAO & New Mexico Tech; T.J.Cornwell, ATNF;
S.T.Myers, NRAO
April 12, 2006
Abstract: This document presents an analysis and comparison of existing multi
frequency synthesis algorithms along with some hybrids, from the point
of view of (E)VLA wide-band imaging requirements of 1 microJy rms
noise and >10^6 dynamic range from an 8 hour observation
over a bandwidth of 1GHz at L Band. Tests on simulated wide-band data
with power law (and non power-law) spectra show the following.
(i) Single channel deconvolution techniques are inadequate due to the
limiting single channel sensitivity and the varying spatial resolution
across channels.
(ii) Bandwidth synthesis along with double deconvolution techniques
that model the spectral variation as a power law work well for sources
with pure power law spectra.
For non power-law spectra, especially with large scale weak emission,
inaccuracies in the estimation of the actual spectral signature of the
sources lead to deconvolution artifacts at the 10 microJy level.
(iii) Hybrid techniques that combine single channel imaging and
bandwidth synthesis using a power law model for spectral flux variation,
work well when only bright and compact sources have significant spectral
flux variation.
Therefore, alternate algorithms (or variants) must be devised to
extend the modeling of the spectral flux variation beyond that of a
pure power law and simultaneously account for the accurate
deconvolution of extended emission.
View a ps or pdf version of EVLA Memo #100 at:
http://www.aoc.nrao.edu/evla/memolist.shtml
******************************ALSO OF INTEREST*****************************
ALMA presentations from the Inaugural Japan-Taiwan ALMA Science Workshop
Dec. 15 -16, 2005 are available on line through links at
http://alma.asiaa.sinica.edu.tw/activities/workshop2005/program_frame.php
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The Caltech Submillimeter Observatory (CSO) encourages observing
participation by astronomers from both U.S. and non-U.S. institutions.
Lodging, subsistence and transportation on the mountain are provided free
by the CSO, for two observers per program. A limited amount of travel
money may also be available.
Proposals for observing time should include the CSO cover form (please
use the latest version available at
http://www.submm.caltech.edu/cso/cso-call.html . The proposals will be
reviewed by an external peer group committee and should be sent by 31
May for the observing period 1 September through 31 January.
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2nd pan-ALMA Conference : 2nd Announcement
Dear Colleague,
The 2nd pan-ALMA conference on "Science with ALMA: a new era for
Astrophysics" will be held 13-16 November 2006 in Madrid, Spain. The
venue will be the campus of the CSIC (Consejo Superior de
Investigaciones Cientificas), in the centre of town.
Information on the 2nd pan-ALMA meeting is available via
http://www.oan.es/alma2006/ (final slash is mandatory)
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Post Doctoral Research Associate Studies of high-mass star formation
Salary up to £26,401 per annum (Ref: EPS/108/06)
THE UNIVERSITY OF MANCHESTER FACULTY OF ENGINEERING AND PHYSICAL SCIENCES
SCHOOL OF PHYSICS AND ASTRONOMY JODRELL BANK OBSERVATORY
A postdoctoral position is available to work on a new VLA high resolution
radio continuum survey of the Galactic Plane. This Large VLA Project has
been awarded ~400 hours of observing time and will begin in June 2006; it
will cover the same area as the northern GLIMPSE survey made by the
SPITZER satellite. The postdoctoral fellow will take charge of the
observations, reduction and exploitation of the survey, aimed principally
at the study of high-mass star formation. Collaboration with other members
of the international team is envisaged.
The position is available immediately for a period of two years in the
first instance, with the possibility of extension beyond this date. The
appointment will be as a Research Associate, with a starting salary in the
range of £24,886 to £26,401 per annum.
Application forms and further particulars are available at
http://www.manchester.ac.uk/vacancies or from EPS HR Office, The
University of Manchester, Sackville Street Building, Manchester M60 1QD,
Tel: 0161 275 8837; Fax: 0161 306 5037 or email: eps-hr at manchester.ac.uk.
Quote ref: EPS/108/06
Closing date: Monday 1 May 2006
Informal inquiries may be made to Philip Diamond, tel: 01477 571321,
email pdiamond at jb.man.ac.uk
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Anne Dutrey informs us of a CNRS post-doctoral position at the Observatory of
Bordeaux. The position is opened for two years and will start on september
2006 at the Observatory of Bordeaux. The application deadline is June 2006.
The position is dedicated to the modelling of chemistry in proto-planetary
disks in order to interpret observational data obtained with the IRAM array.
Interested people can read the dedicated CNRS web page
http://www.k-projects.com/cnrs_postdocs/public/departement_details.php?IdDpt=9&Dep=SDU&NumOffre=2&Langue=en
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