- Gemini Home
- Telescopes and Sites
- Science Visitors at Gemini
- Observing With Gemini
- Partner Subscription
- Proposal Routes and Observing Modes
- Observing Overheads
- Proposal Submission
- 2016B Call for Proposals
- Nightlog GN
- Nightlog GS
- Phase II and S/W Tools
- Observing Tool
- Finding Charts
- ToO Activation
- Changing Approved Programs
- Advice for Band 3 Programs
- What to expect
- Telescope Time Charging
- Future Instrumentation & Current Development
- Queue and Schedules
- Data and Results
- Gemini Research Staff
Change page style:
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!
The Phase II deadline of July 15, 2011 is a hard deadline for both queue and classical programs. Note that failure to submit a defined program by the Phase II deadline will result in the progam being canceled. Extensions are granted only in exceptional circumstances and only if requested prior to the deadline.
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.
|Phase II deadlines for all instruments|
|15 July 2011||Mandatory deadline for all queue and classical programs.|
|MOS Mask Cut Deadlines||
MOS Masks are cut at Gemini South for both telescopes. Masks are cut twice a week. Allow an extra week for delivery to Gemini North.
The mask design and corresponding Phase II updates are submitted via the OT and then checked by the NGO contact before being forwarded to the observatory for cutting. The time between mask design submission and when the mask can be available at the telescope is approximately 2 weeks for Gemini South and 3 weeks for Gemini North (due to mask shipping time). We strongly encourage all MOS PIs to submit their mask designs as early as possible (either at the start of the semester if not using GMOS pre-imaging or immediately after the pre-imaging is taken) in order to increase the chance that the MOS observations will be completed. Gemini reserves the right to not cut masks for queue programs submitted within 6 weeks of the end of the semester if the queue coordinators determine that the MOS observations cannot be scheduled.
Be sure to use the latest version of the mask design software.
Classical program PIs must submit their mask designs at least two weeks prior to their arrival at Gemini South and three weeks prior to their arrival at Gemini North.
Note that all MOS observations must be defined by the phase II deadline. Observations without masks will be reviewed and set to "On Hold" until the masks become available, at which time the PI will have a chance to make modifications if necessary.
3 August 2011
30 August 2011
27 September 2011
23 November 2011
18 January 2012
|Dates of preparation of Gemini-North 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 and classical 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 (see the table above). The LGS target list preparation dates are subject to change if LGS runs are rescheduled.
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. In all cases it benefits programs with early targets to get their Phase II ready early, as some 2011B programs will most likely be observed at the end of 2011A to help fill 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 of 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. NGO staff may have also copied relevant observation templates from the OT example libraries into selected programs. Please use any templates as the starting point for completing the Phase II observations.
Instructions on skeleton retrieval were sent to PIs on June 16, 2011. 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 2011B Phase II preparation (as well as on-going 2010A, 2010B, and 2011A programs); do not use the previous "2011A" 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 must be fetched and used for your observations, as these contain updated calibration observations as well as templates.
Relaxation of Observing Condition Constraints and Other Observation Changes
By default observations must use the observing conditions constraints approved by the ITAC during the Phase I process. Band 3 programs must use the approved Band 3 conditions. It is always acceptable to relax the conditions since more relaxed conditions lead to a higher probability of execution.
To change to better observing conditions than approved by the ITAC, or to add airmass or hour angle constraints, requires approval via the change request procedure. Target changes and other significant modifications to the original proposed observations also require approval, see the change request procedure for more information.
The National Gemini Offices are responsible for Phase II support for the established facility and visiting instruments. In outline, the Phase II process is as follows:
- PIs develop their Phase II using the OT library examples and interacting with NGO support staff as needed for assistance;
- Phase II Science Programs are checked by NGO staff who iterate with PI if needed, before setting observations to "For Activation";
- Once set for activation, the Gemini Contact Scientist will perform a final check before setting observations "Ready" to observe. If there is any problem the observation status will be returned to "For Review" for further iteration between the NGO and the PI.
- As observation status changes in the OT, the PI, NGO contact and Gemini contact receive emails. The PI must always fetch the program to ensure he/she has the latest version before making changes and storing again.
OT and Other Late-Breaking Changes for 2011B
The principal changes to the OT software are listed on the OT Release Notes page. There are also several new policy changes. Here we summarize how they affect Phase II observation definition and point the user to further details.
Changes to program time accounting
Starting in Semester 11B, no time accounting corrections will be applied if these are less than one hour. Statistics from four previous semesters show that the effect on the partner imbalances is minimal as the corrections are approximately distributed as the nominal partner shares. To avoid stopping executions of programs prematurely, NGO support and Contact scientists must ensure that each program contains a top level note with the title “PhaseII-filling” that states how the program time was filled, following specified templates. The PI and NGO for a program can request a review of the time accounting for a given program, and the Head of Science Operations and core-QCs will respond to such requests within one week. More information is available on the queue planning and execution page.
There are many changes to the OT libraries, especially for GNIRS. Fetch the new libraries by selecting "Fetch Libraries..." from the File menu of the OT Science Program Editor.
NGO staff may have added relevant template observations from the OT libraries to selected programs in order to improve the Phase II process. Please use these templates as the starting point for the final Phase II observation definitions. Contact your NGO contact scientist if you have any questions.
Many instrument libraries now include "Standardized Notes" which should be used if possible to efficiently convey important information to the nighttime observers.
Major new OT capabilities and procedure changes
- Introduction of the 80 percentile cloud cover constraint. CC90 is now obsolete.
- Label GMOS CCDs in Position Editor
- Update GSAOI overheads based on commissioning data.
GMOS-N CCDs should be E2V
All GMOS-N observations should use the E2V CCDs. See the GMOS Status page for news on the GMOS-North detector upgrade.
Minimizing the effects of atmospheric refraction in GMOS data
The GMOS instrument web pages have been updated to give information about some of the consequences that can result from the fact the GMOSs do not have atmospheric dispersion correctors. Advice is given on how to limit the effects on data.
Phase II Deadline for Classical Programs
The Phase II deadline for classical programs is the same as the queue deadline, in this case July 15, 2011. For classical programs, backup observations to use poorer conditions, if appropriate, must have been specified and approved by this date.
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).