- Gemini Home
- Telescopes and Sites
- Science Visitors at Gemini
- Observing With Gemini
- Future Instrumentation
- Queue and Schedules
- Data and Results
Change page style:
Special Instructions 2008B
Instructions for Completion of Phase II/OT Science Programs: Semester 2008B
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!
As in the previous semester the Phase II deadline is a hard deadline for queue programs. Programs that have not completed their Phase II definitions by the deadline will be dropped from the queue.
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|
|14 July 2008||Mandatory deadline for all queue programs.|
|1st and 15th of each month||Deadlines for GMOS mask design and MOS updates|
|4 August 2008
3 September 2008
26 September 2008
3 November 2008
1 December 2008
15 January 2009
|Dates of preparation of LGS targets lists by Gemini staff for approval by Space Command. Change requests for target additions and alterations must be made well in advance of these dates for the target to be included in the next LGS run, and observations set to "ready" at least two days prior. (These restrictions do not apply to LGS programs granted ToO status.)|
The mandatory deadline applies to all queue programs including templates for Quick Response / ToO observations. The mask design deadlines are more flexible but we encourage PIs to submit their mask designs and final MOS observations as early as possible. The LGS target list preparation dates are subject to change if LGS runs are rescheduled.
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 deadline noted above will be dropped from the queue or schedule. In exceptional cases an exemption may be requested by emailing the Heads of Science Operations (ijorgensengemini.edu, brodgersgemini.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 deadline (see table above).
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 June 9. 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 is available to support Semester 2008B Phase II preparation (as well as on-going 2007B and 2008A programs); do not use the previous "tabano" 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. OT libraries with example observations and configurations for each instrument can also be fetched.
Relaxation of Observing Condition Constraints and Other Observation Changes
For semester 2008B 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).
Programs in Band 3 will be expected to use the relaxed Band 3 conditions that were specified during Phase I. It is always acceptable to relax the conditions even more since more relaxed conditions leads to a higher probability of execution (see Advice for Band 3 PIs). 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 2008B we are continuing the "poor weather queue" to fill telescope time under very poor, but usable, conditions. Poor weather proposals can be submitted at any time using the PIT.
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 Rosemary Pike (rpikegemini.edu) with a copy to the Gemini Heads of Science Operations (ijorgensengemini.edu, brodgersgemini.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,
the Gemini HelpDesk. This allows us to ensure that no queries are missed and
help us improve the software and documentation. A streamlined
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).
OT and Other Late-Breaking Changes for 2008B
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 have implemented 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 2008B is offered on an "at risk" basis. PIs who are interested in utilizing this should inform their contact scientists.
Updated GMOS GCAL exposure tablesThe exposure tables for GMOS arcs and flats using GCAL have been updated. The new table includes images of example calibration spectra. The GMOS OT libraries have been updated accordingly.
Major new OT capabilities and procedure changes
- Target duplication feature
- In Review observation status. NGO staff will use this status to prevent observations from being edited while they are being reviewed. In order to avoid the unexpected loss of any work, PIs should always fetch their program before making changes and should not make any changes to observations stored with status For Review until the NGO contact as set the status back to Phase 2. Exporting a program to a XML file before storing is also recommended.
- NICI offset iterator and other NICI instrument componet change
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 from GSA.
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 June 12, 2008; Bryan Miller