![]() |
Poor Weather Queue Summary : Semester 2013A GS |
The queues shown in the tables below summarise the programs that constitute the "Poor Weather Queue" on GS. 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).
GS Poor Weather Queue | ||||||
Ref # | PI | Partner | Title | Instrument | Hours allocated |
|
GS-2013A-Q-95 | Beers | BR | Missing metal-poor stars from the HK and Hamburg/ESO Surveys (South) | GMOS-S | 10.90 | |
Execution Status: complete | Dates Taken: 20130120 20130124 20130302 20130306 20130509 20130510 20130514 20130515 20130516 20130517 20130520 20130521 20130522 20130614 20130618 20130619 20130723 |
Completion Status:
|
||||
GS-2013A-Q-96 | Tisserand | AU | What is the nature of OGLE-2012-BLG-0577 source star ? | GMOS-S | 0.90 | |
Execution Status: | Dates Taken: |
Completion Status:
|
||||
GS-2013A-Q-97 | Gamen | AR | Searching for very massive binary systems among faint galactic WN stars | GMOS-S | 54.60 | |
Execution Status: complete | Dates Taken: 20130526 20130531 20130601 20130602 20130604 20130610 20130611 20130614 20130615 20130617 20130618 20130619 20130701 20130702 20130703 20130704 20130707 20130708 20130723 20130729 20130731 20130803 20130811 20130812 20140129 20140218 20140315 20140427 |
Completion Status:
|
||||
GS-2013A-Q-98 | Weidmann | AR | Confirmation of very reddenig planetary nebulae | GMOS-S | 3.50 | |
Execution Status: complete | Dates Taken: 20130525 20130526 20130528 20130604 20130619 |
Completion Status:
|
||||
GS-2013A-Q-99 | Titov | AU | Testing the cosmological model with Very Long Baseline Interferometry | GMOS-S | 31.40 | |
Execution Status: complete | Dates Taken: 20130531 20130601 20130602 20130604 20130608 20130609 20130611 20130616 20130618 20130619 20130629 20130701 20130702 20130704 20130707 20130708 20130709 20130723 20130731 20130801 20130802 |
Completion Status:
|
Last updated on: 24 Jul 2020 12:22:55 GMT