![]() | Poor Weather Queue Summary : Semester 2020A 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-2020A-Q-401 | Retamales González | CL | B-type supergiant eclipsing binaries as a key to understand evolution of massive stars | GMOS-S | 36.36 | |
Execution Status: | Dates Taken: | Completion Status: | ||||
GS-2020A-Q-402 | Oviedo | AR | New templates of subsolar metallicity | GMOS-S | 5.00 | |
Execution Status: | Dates Taken: 20200119 20200306 20200314 20200315 20200316 | Completion Status: | ||||
GS-2020A-Q-403 | Kalari | GS | The Galactic O-Star Spectroscopic Survey (GOSSS): the faint southern sample | GMOS-S | 19.40 | |
Execution Status: | Dates Taken: | Completion Status: | ||||
GS-2020A-Q-404 | Lubar | US | The Stellar Population of TWA and Beta Pictoris | Visitor | 10.00 | |
Execution Status: | Dates Taken: | Completion Status: | ||||
GS-2020A-Q-405 | Sneden | GS | High Resolution Infrared Spectroscopy of Barium and S Stars | Visitor | 4.30 | |
Execution Status: | Dates Taken: | Completion Status: | ||||
GS-2020A-Q-406 | Weidmann | AR | Central Stars of Planetary Nebulae: Survey for Spectral Classification | GMOS-S | 16.10 | |
Execution Status: | Dates Taken: 20200214 20200310 20200316 | Completion Status: | ||||
GS-2020A-Q-407 | Seccull | US | A Search for Faint Solar Calibrators | GMOS / GMOS-S | 28.50 | |
Execution Status: | Dates Taken: 20200228 20200229 20200307 20200310 20200311 20200314 | Completion Status: | ||||
GS-2020A-Q-408 | Maille | US | High Redshift Blazar Candidates in Optical | GMOS-S | 1.30 | |
Execution Status: | Dates Taken: | Completion Status: | ||||
GS-2020A-Q-409 | Xu | GS | The Gaia View of Dust Disks around White Dwarfs | Flamingos2 / NIRI | 7.20 | |
Execution Status: | Dates Taken: | Completion Status: | ||||
GS-2020A-Q-410 | Chené | GS | What is Wolf-Rayet Stars Favorite Dance? | GMOS / GMOS-S | 27.00 | |
Execution Status: | Dates Taken: 20200306 20200310 20200311 | Completion Status: | ||||
GS-2020A-Q-411 | Dennihy | US | Mapping the emitting line region of post-main-sequence planetary disks - GS | GMOS-S | 16.30 | |
Execution Status: | Dates Taken: 20200310 20200311 | Completion Status: | ||||
GS-2020A-Q-412 | Hinkle | US | The Neutron Star Symbiotic Binary IGR J16194-2810 | Visitor | 3.00 | |
Execution Status: | Dates Taken: | Completion Status: |
Last updated on: 7 Jun 2021 12:23:18 GMT