Poor Weather Queue Summary : Semester 2019B 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 |
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GS-2019B-Q-401 | Ahumada | AR | New templates of subsolar metallicity | GMOS-S | 3.70 | |
Execution Status: complete | Dates Taken: 20190718 20190724 20190731 20190803 20190808 20190913 |
Completion Status:
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GS-2019B-Q-402 | Caso | AR | Revealing the mass profiles of satellite galaxies in dense environments | GMOS-S | 9.80 | |
Execution Status: complete | Dates Taken: 20190808 20190920 20190921 20190925 20190927 20190929 |
Completion Status:
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GS-2019B-Q-403 | Scaringi | US | The Gemini Galactic Spectroscopic H-alpha Emitter Large Legacy Survey (G-SHELLS) | GMOS-S | 22.00 | |
Execution Status: complete | Dates Taken: 20190706 20190710 20190711 20190712 20190718 20190723 20190724 20190901 20190904 20190913 20190919 20190922 20190923 20190924 20190925 20191001 20191009 20191019 20191020 20191029 20191102 20191114 20191122 20191125 20191221 20191228 20200111 20200118 20200121 |
Completion Status:
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GS-2019B-Q-404 | Chené | US | What is Wolf-Rayet Stars Favorite Dance? | GMOS / GMOS-S | 27.00 | |
Execution Status: | Dates Taken: 20190710 20190811 |
Completion Status:
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GS-2019B-Q-405 | Nitta | US | Determination of White-Dwarf Mass in Peculiar Dwarf Nova with a Bright Donor Star, V364 Lib, by Optical Spectroscopy in Outburst | GMOS-S | 2.70 | |
Execution Status: | Dates Taken: 20190808 20191114 |
Completion Status:
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GS-2019B-Q-406 | Caso | AR | Revealing the mass profiles of satellite galaxies in dense environments | GMOS-S | 20.40 | |
Execution Status: complete | Dates Taken: 20190802 20190808 20190809 20190812 20190829 20190919 20190921 20190922 20190923 20190924 20190929 |
Completion Status:
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GS-2019B-Q-407 | weidmann | AR | Central Stars of Planetary Nebulae: Survey for Spectral Classification | GMOS-S | 15.80 | |
Execution Status: complete | Dates Taken: 20190811 20190812 20190913 20190914 20190920 20191019 20191020 20191029 20191030 20191102 20191122 20191126 20191204 20191205 20191216 20191228 20200107 20200111 20200115 20200116 20200128 |
Completion Status:
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GS-2019B-Q-408 | Xu | US | The Gaia View of Dust Disks around White Dwarfs | Flamingos2 / NIRI | 30.00 | |
Execution Status: | Dates Taken: 20191030 20191109 20191112 20191114 20191115 20191116 20191122 20191216 20191217 20191228 20200107 20200109 20200110 20200113 20200118 |
Completion Status:
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GS-2019B-Q-409 | Maille | US | High Redshift Blazar Candidates in Optical | GMOS-S | 0.70 | |
Execution Status: | Dates Taken: |
Completion Status:
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GS-2019B-Q-410 | Rivera Sandoval | US | Spectroscopic identification of UV variables with large radial velocities | GMOS-S | 16.00 | |
Execution Status: complete | Dates Taken: 20190918 20190919 20190922 20190925 20190926 20190930 20191001 20191019 20191030 20200311 |
Completion Status:
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GS-2019B-Q-411 | Kalari | US | Characterising new faint massive star candidates in the SMC | GMOS-S | 24.30 | |
Execution Status: | Dates Taken: 20190930 20191008 20191028 20191030 20191112 20191116 20191122 20191125 20191205 20200118 |
Completion Status:
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GS-2019B-Q-412 | Dennihy | US | Mapping the emitting line region of post-main-sequence planetary disks - GS | GMOS-S | 8.70 | |
Execution Status: | Dates Taken: 20191007 20191019 20191020 20191030 20191123 20200131 20200201 |
Completion Status:
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GS-2019B-Q-413 | Peterson | US | Testing the interferometric broad-line region radius of 3C 273 with near-IR reverberation | Flamingos2 / GNIRS | 60.00 | |
Execution Status: | Dates Taken: |
Completion Status:
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GS-2019B-Q-414 | Gallo | CA | Consequences of the gamma-ray flare on the BLR of PKS2004-447 | GMOS-S | 1.00 | |
Execution Status: | Dates Taken: 20200109 20200110 20200117 |
Completion Status:
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Last updated on: 7 Jun 2021 12:23:18 GMT