- Gemini Home
- Telescopes and Sites
- Science Visitors at Gemini
- Observing With Gemini
- Future Instrumentation
- Queue and Schedules
- Data and Results
- Image Library
Change page style:
Special Instructions 2007A
Instructions for Completion of Phase II/OT Science Programs: Semester 2007A
This page provides instructions for completing Phase II Science Programs for all Gemini North and Gemini South instruments. It includes submission details and procedural changes. Please read this page carefully!
Note: As in the previous semester the Phase II deadlines are hard deadlines for queue programs (see details below). Programs that have not completed their Phase II definitions by the deadlines will be dropped from the queue.
Distribution of Phase II Skeletons
All observations must be defined using the Observing Tool (OT) software. Gemini staff have translated approved Phase I proposals into the Phase II format for loading into the OT. In this process, the observations and other details entered in Phase I are used to construct a ("skeleton") framework of your Science Program.
Instructions on skeleton retrieval were sent to PIs during the week of December 11. As in previous semesters, the Phase II skeletons are downloaded/uploaded directly from/to the Gemini telescope databases to enable more efficient and rapid processing. See more information on using the Observing Database.
A new release of the OT ("avispa") is available to support Semester 2007A Phase II preparation (as well as on-going 2006A and 2006B programs); do not use the previous "abeja" public release. There are OT installation instructions available. If you are unfamiliar with the OT, there is an OT tutorial that provides a useful introduction. In addition, each instrument also has several web pages that provide guidance on observing strategies and how to describe these in the OT.
Relaxation of Observing Condition Constraints and Other Observation Changes
For semester 2007A the queue was constructed by filling the expected observing conditions (and overfilling the poorer than average conditions) but limited to the total available queue time (i.e. the total science time less scheduled classical nights and estimated Band 1 rollover programs). Band 3 programs, which occupy the lowest half of the queue, are unlikely to be executed, and very unlikely to be completed, if they request conditions that are better than average (especially in cloud cover and image quality).
As in the previous semester we encourage PIs of Band 3 programs, in particular, to think carefully about relaxing the observation constraints within the context of their overall time allocation and approved science goals (e.g. by observing fewer targets). One useful analogy is to consider "how would I attempt this program if it were classically scheduled and the conditions were sub-optimal?".In semester 2007A we are continuing the "poor weather queue". This is a program to fill telescope time under very poor, but usable, conditions. Time spent on these programs will not be charged to the PI or the partner countries. These are queue programs only but are distinct from the "regular" band 1 to band 3 queue. They will be executed only when nothing in the regular queue is observable. In all other respects (Phase II deadlines, NGO and contact scientist support, science archive data distribution) they are identical to other Gemini programs.
If your program is in the poor weather queue, it will be designated as "Band 4" above (and in the Phase II definition); it will also be identified as such in the ITAC comments.
Acceptable observing condition constraints for poor weather programs are:
- CC=70%, 90% or "Any" and IQ="Any" and WV="Any" (no restriction on SB)
- CC=90% or "Any" and WV="Any" (no restriction on IQ and SB)
The Observing Conditions component now also makes it possible to add airmass or hour angle constraints. While needed for some programs, use of these constraints is equivalent to a change to better conditions constraints than approved by the ITAC. Therefore, any use of the airmass or hour angle constraints requires approval via the change request procedure.
If during detailed definition you find that the approved observations need to be modified, please follow the change request procedure.
The National Gemini Offices are responsible for Phase II support for the "established" facility and visiting instruments as mandated by the Gemini Board. Phase II support for the other instruments remains with the Gemini Observatory staff. In outline, the Phase II process for the established instruments is as follows:
- PIs interact with NGO support staff to complete Phase II using the OT for all observations with NIRI (including Altair), Phoenix, both GMOSs (including MOS mask design), T-ReCS, GNIRS and Michelle.
- All Phase II Science Programs are checked by NGO staff prior to being forwarded to the Gemini Contact Scientist. (Note that Gemini CSs will return any Phase II programs that are received directly from PIs, with instructions to contact their NGO).
- Gemini Contact Scientist checks Phase II Science Programs; if there is any problem the Science Program will be returned to the NGO support staff. The NGO staff will then iterate further with the PI.
- Only when the Gemini Contact Scientist agrees that the Science Program is ready will it be activated in the queue for execution. The PI will be notified that their program is in the active queue and that the Gemini CS is now the primary contact point.
If you wish to change the primary contact for this program, e.g. to a co-I, please e-mail both Sybil Adams (sadamsgemini.edu) with a copy to both Gemini Heads of Science Operations (ijorgensengemini.edu, mwestgemini.edu) and a copy to your National Gemini office.
To help us in tracking and resolving user problems, questions and suggestions, and thereby improving the software and web pages, please use the Gemini HelpDesk. This allows us to ensure that no queries are missed and help us improve the software and documentation. A streamlined interface is available for Phase II queries, keyed to your Gemini Program ID (e.g. GS-2006B-Q-12). As with the regular HelpDesk interface, your query will be directed to the specific NGO or Gemini support staff. Support assignments do change occasionally and you can verify the contact names from the "interactive snapshot" of the Observing Database, accessed from the contents list on the schedules web page. (The NGO and Gemini support staff email addresses are listed on the support staff web page).
The mechanism for submitting your completed Phase II Science Program is by using the Store command in the Observing Tool and is the same for all instruments. See the Observing Database information for more details.
Dates for submission of completed Phase II information are (all 6pm local time):
|Phase II deadlines for all instruments|
|10 January||Early submission, recommended for any programs and especially advantageous for observations that can be executed early in the semester|
|31 January||Mandatory deadline for all queue programs.|
|various||Deadlines for GMOS mask design and MOS updates (several dates, synchronized with lunar phase)|
These deadlines apply to all queue programs including templates for Quick Response / ToO observations. (In addition there are periodic deadlines during the semester for GMOS mask design and corresponding MOS observation updates only).
PIs of all classical programs must also submit Phase II observation definitions. The deadline for these is three weeks prior to the first scheduled night.
Programs that have not completed their Phase II definitions by the deadlines noted above will be dropped from the queue or schedule. In exceptional cases an exemption may be requested by emailing both Heads of Science Operations (ijorgensengemini.edu and mwestgemini.edu)
In some cases GMOS PIs may be contacted directly and asked to submit their Phase II early to provide sufficient observations for pre-imaging and MOS spectroscopy at the very start of the semester. All MOS pre-imaging observation descriptions must be submitted by the regular deadlines (see table above).
OT and Other Late-Breaking Changes for 2007A
The principal changes to the OT software are listed on the OT Release Notes page. There are also several new policy changes. Here we summarise how they affect Phase II observation definition and point the user to further details.
GMOS mask designs without GMOS pre-imagingWe are implementing the capability for the design of GMOS MOS masks from any available imaging with good astrometry. This has the potential to save observing time since pre-imaging with GMOS will no longer be required. In 2007A this may be offered on an "at risk" basis after a new version of the Gemini IRAF package is released in early 2007. PIs who are interested in utilizing this should inform their contact scientists.
Major new OT capabilities and procedure changes
- Improved non-sidereal support in the target component
- Name lookup for non-sidereal objects
- Remove redundant orbital elements formats from target component
- Current position button for non-sidereal targets
- Improvements and additions to guide star query algorithms
Notification of Data Taken and Electronic Distribution
The "Notify PI" checkbox in the OT observation component is
not yet active. Nonetheless, raw data are available "immediately"
(usually within minutes) from the Gemini Science Archive using your OT
(observing database) key for secure access to proprietary data. PIs
will be notified by email once their data have been quality assessed
and ingested into the archive and are available as a package along
with other metadata (observing logs, calibrations etc). See more
information about data retrieval
Status of Submitted Programs and Observations
The queue summary and "interactive database snapshot" pages show the current execution status of all queue programs and indicates when data have been taken. (For the next level of detail, click on the "execution status" link under each program to see the status of each observation or on the execution log links in the contents list to see which observations were executed each night).
Last update December 4, 2006; Bryan Miller