- Group Communications
In order to get everyone "on the same page" regarding calibration
issues, Mangum suggested that:
- We hold this telecon at least monthly. Suggestions for a
different frequency?
- The consensus opinion was that once-per-month was an
acceptable rate for this telecon. Irregular telecons can be scheduled
as necessary. Given the need to make progress on the Calibration
Plan, the next telecon will be one of these "irregularities" (in
two weeks).
- A calibration web page be developed which can serve as a starting
point for those wishing to find information on ALMA calibration
issues. See http://www.cv.nrao.edu/~jmangum/ALMA/Calibration/ for a
first-cut at this page.
- The consensus option was that a calibration web page was a good
central point-of-contact for ALMA Calibration issues.
- If the Wiki is found to be an efficient communications tool (see
below), then the Wiki should incorporate the information on the
calibration web page.
- A calibration wiki, which is a more efficient way to hold
"discussions" on calibration topics than email or web pages.
- The consensus opinion was that it was worth giving the Wiki a
try.
- ACTION: Mangum works with NRAO Computing to implement an
externally-accessible Wiki. If this option will not develop within
the next month or so, explore use of the existing ESO Wiki. Richer
suggests building Calibration Wiki within an ALMA Science IPT Wiki.
- Calibration Plan
The Calibration
Plan needs to be finished. In order to accomplish this, it will
be necessary to have small groups concentrate on specific sections of
the plan. Mangum suggested the following breakdown for group
concentration (I also list some possible "volunteers" for review and
update of each section, with a suggested "lead volunteer" denoted in
bold):
- Amplitude and Flux Calibration (Welch, Butler, Carter,
Gibson, Holdaway, Mangum, Martin-Pintado, Kawabe)
- Phase Calibration (Hills, Holdaway, Mundy, Richer,
Stirling, Wootten)
- Bandpass Calibration (Guilloteau, Bacmann)
- Polarization Calibration (Myers, Holdaway, Laing)
- Pointing Calibration (Mangum, Lucas, Holdaway)
- Antenna Location Calibration (Conway, Wright)
- Antenna and Electronic Delay Calibration (Lucas)
- Optics Calibration (Butler, Kawabe, Saito)
- Total Power Calibration (Holdaway, Mangum, Mundy, Kawabe)
- Archiving and Accessing Calibration Quantities (Lucas, Mangum)
Please be prepared to volunteer to work on one or more of these
sections.
- A proposal by D'Addario suggested a different structure to the
Calibration
Plan and the organization of the group discussions as a
whole which emphasized an operational approach to calibration. The
group consensus was that, although this is a reasonable structure, it
isn't necessarily a better structure. Wright commented that D'Addario's
suggested structure is tied to an ALMA operational model which might
change.
- The structure of the current Calibration
Plan, listed above, was
felt to be the correct structure for this Plan and for further group
discussions.
- Further "volunteering" resulted in the additional names added to
each calibration category in the list above.
- Via email Kawabe brought up the issue of how we incorporate
ACA-specific calibration in the Calibration
Plan and in our future discussions.
- Wright and Richer suggested that the ACA-specific calibration
issues be incorporated into the existing calibration category
structure.
- Mundy cautioned that our procedure for dealing with ACA
calibration is dependent upon how the ACA will be operated within
ALMA (separate array or integrated with ALMA).
- ACTION: Mangum will seek guidance from ALMA Management on the
question of ACA operation. In the meantime, group discussions
should consider ACA-related issues within the context of specific
calibration categories.
- The content of the Calibration
Plan was discussed.
- Richer and Butler pointed out that the current Plan is lacking
recipes for how calibration is implemented within a given type of
observation. For example, how long will a certain type of
calibration measurement take, and how often will it need to be
done.
- Holdaway suggested that there should be an appendix which
contains example calibration sequences and durations for typical
kinds of observations.
- The need for Total Power and/or Primary Beam calibration sections?
- Via email, Holdaway suggested that Primary Beam calibration
should be its own calibration category and section in the
Calibration
Plan. Mangum agrees. Please comment.
- Via email, Mangum pointed out that the current content of the
"Total Power" section in the Calibration
Plan is composed of
calibration categories which exist on their own elsewhere (like
pointing, amplitude, focus, etc.). Therefore, perhaps the issues
pertinent to "Total Power" calibration should be incorporated into
other calibration categories. Please comment.
- ACTION: All will consider:
- whether "Total Power" calibration can be incorporated within
other calibration categories (use the current content of the
Calibration
Plan as a guide), and
- whether "Primary Beam" calibration should be added to the
list of calibration categories and Calibration
Plan sections.
- ACTION: All will review/update Calibration
Plan sections.
Updates will be discussed at next telecon (in two weeks). Changes
should be distributed to the group no later than 2004-07-27.
- Calibration Category Issues
The following is a suggested list of "calibration categories" which
Mangum suggests we should discuss on a regular basis (note the
similarity to the Calibration
Plan sections). Please suggest
additions/deletions to the following list. Also, if you have issues
to discuss for the next telecon, please let me know and I can add
them.
- Amplitude and Flux Calibration
- Phase Calibration
- Bandpass Calibration
- Polarization Calibration
- Pointing Calibration
- Antenna Location Calibration
- Antenna and Electronic Delay Calibration
- Optics Calibration
- Total Power Calibration (may be subsumed into other
calibration categories)
- Primary Beam Calibration
- Archiving and Accessing Calibration Quantities
Mangum's proposal is to discuss a few of these categories at each
telecon. Once we all get our arms around how each of these categories
function, we can then discuss how they interconnect.
All agreed that this was a reasonable approach.
- Amplitude Calibration Subsystem Development Reports
- Berkeley Absolute Flux Calibration System (Welch)
- Icarus paper on 28.5 GHz work (Gibson and Welch) weaving its way
through the referee process.
- ACTION: Welch will send preprint of Icarus paper to the
group.
- Currently installing equipment on BIMA for 3mm experiment.
- Measurements must be done by the end of July (BIMA moving to CARMA).
- This 3mm experiment will make measurements in a similar way to
how the 28.5 GHz measurements were done, with a few exceptions:
- Standard horn will be used to make tipping curve measurements.
- Standard horn will be used as a separate interferometer
element.
- Implementation of this system for ALMA will require mounting a
system of calibration horns on a separate antenna mount.
- This system will allow for amplitude calibration and monitoring
of phase calibration sources (secondary calibrators).
- Semi-Transparent Vane (STV) Calibration System
(Martin-Pintado/Wilson): No report.
- Date of next phone meeting
The next ALMA Calibration Group telecon will be
2004, July 30th 15:00 UT (NOTE UNUSUAL DATE).