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Poor Weather Queue Summary : Semester 2014B GN |
The queues shown in the tables below summarise the programs that constitute the "Poor Weather Queue" on GN. The Poor Weather Queue is a pilot program introduced in 2006B to fill telescope time under very poor, but usable, conditions. These programs are distinct from other queue programs in three important ways: 1) time spent on poor weather programs will not be charged to the PIs or the partner countries; 2) poor weather programs can exist in queue only, and must meet the observing condition constraints shown below; and 3) poor weather programs are lower priority than the "regular" queue (bands 1 to 3) and have no explicit or implicit guarantee of being observed. They will be executed only when nothing in the regular queue is observable.
In all other respects — NGO and Gemini contact scientist support, Phase II definitions, Gemini Science Archive data distribution — programs in the Poor Weather Queue are similar to all other Gemini queue programs. In the Observing Tool, poor weather queue programs are designated as Band 4, to distinguish them from the rest of the queue.
Observing condition constraints for poor weather programs must meet one of the following:
This report is generated daily (see the bottom of the page for the current timestamp). The pages linked via Completion Status are updated approximately every 4 hours. Note that the completion fraction may change as the time accounting is adjusted during the quality assessment process.
The assigned support staff (Gemini Contact Scientists and National Office staff) for each Gemini North ODB and Gemini South ODB program are listed in the interactive 'snapshots' of the Observing Database (ODB).
GN Poor Weather Queue | ||||||
Ref # | PI | Partner | Title | Instrument | Hours allocated |
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GN-2014B-Q-102 | Beers | BR | Missing metal-poor stars from the HK and Hamburg/ESO Surveys (North) | GMOS | 30.00 | |
Execution Status: complete | Dates Taken: 20140712 20141031 20141104 20141106 20141108 20141120 20141122 20141129 20141204 20141205 20141206 20141211 20141214 20141217 20141220 20141222 20150107 20150113 |
Completion Status:
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GN-2014B-Q-105 | FLAGEY | UH | To Be or nor to B[e] a LBV | GNIRS | 10.00 | |
Execution Status: | Dates Taken: |
Completion Status:
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GN-2014B-Q-106 | Maille | GS | Spectroscopy of Very High Redshift Blazars | GNIRS+Altair | 0.60 | |
Execution Status: | Dates Taken: |
Completion Status:
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GN-2014B-Q-107 | Hillwig | GS | A Spectroscopic Search for Companions to Planetary Nebula Central Stars | GMOS | 18.50 | |
Execution Status: | Dates Taken: 20141111 20141122 20141129 20141206 20141214 20141219 20150107 20150125 20150130 |
Completion Status:
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GN-2014B-Q-108 | Shih | GS | Extended Outflows From Low-Excitation AGNs? | GMOS | 16.00 | |
Execution Status: | Dates Taken: 20141122 20141216 20141217 20141220 20150112 20150113 20150125 |
Completion Status:
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GN-2014B-Q-109 | Chené | GS | Twinkle little star, how I wonder where you are. | GNIRS+Altair / NIRI+Altair | 0.34 | |
Execution Status: complete | Dates Taken: 20141204 20141211 |
Completion Status:
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GN-2014B-Q-110 | Arias | AR | Be stars: circumstellar environment variability through hydrogen emission lines in the near IR | GNIRS | 1.40 | |
Execution Status: | Dates Taken: |
Completion Status:
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Last updated on: 24 Jul 2020 17:21:52 GMT