Semester 2024B - GS FT Programs
The table below summarizes the Gemini queue programs and their execution status. This page is updated once per day.
The columns in the table are:
Ref # Gemini reference number (note that this is different from any internal National TAC reference number). Click on it to see the proposal abstract (when available).
PI Name of Principal Investigator. (If a joint proposal, the name of the primary contact for the entire program is listed).
Partner Participant (AR, BR, CA, CL, KR, UH, US) to which time will be charged. If a joint proposal, all contributors are shown.
Title The title of the science program.
Instrument Name of the instrument(s) required.
Hours Allocated Time allocated to the program (if a joint proposal, this is the total time for the program). Semesters shown in square brackets e.g. [] indicate that the program can be carried over to the specified semester.
Execution Status Click on this hyperlink to see the current status of each observation in the program.
Data Taken The UT date(s) on which data were taken.
Completion Status This shows an estimate of the fraction of allocated time that has been used. Note that this is a preliminary estimate and is only an indication of the completion state of the program. The completion state may not reflect the formal time accounting. Also note that some programs may be completed in less than the allocated time (e.g. if conditions were better than requested or if the request was overestimated).
The assigned support staff (Gemini Contact Scientists and National Office staff) for each program are listed in the interactive 'snapshots' of the Observing Database (ODB).
GS Fast Turnaround Time Queue Band 1 | ||||||
Ref # | PI | Partner | Title | Instrument | Hours allocated |
|
GS-2024B-FT-101 | Biswas | CA | Optical follow-up of the misaligned DDRG LEDA 884893: a binary AGN candidate | GHOST | 1.40 | |
Execution Status: |
Dates Taken: 20240901 |
Completion Status:
97%
|
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GS-2024B-FT-102 | Mo | US | Uncovering SN Ia progenitors from an overlooked population of CSM interactors | GMOS-S | 1.64 | |
Execution Status: |
Dates Taken: 20240825 20240826 20241012 |
Completion Status:
0%
|
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GS-2024B-FT-103 | Smith | US | Singing in the (iron) rain: Interrogating the Hypothesis of Fe Condsensation on an Ultra Hot Jupiter | GHOST | 8.00 | |
Execution Status: |
Dates Taken: 20240929 |
Completion Status:
48%
|
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GS-2024B-FT-104 | Chené | US | What happened to NGC300 ULX-1? | Flamingos2 / GMOS-S | 0.97 | |
Execution Status: complete |
Dates Taken: 20240905 |
Completion Status:
100%
|
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GS-2024B-FT-105 | Woodward | US | IR Spectroscopy of V745Sco - Catching A Recurrent Nova Between Eruptions | Flamingos2 | 1.23 | |
Execution Status: |
Dates Taken: 20240826 20241012 |
Completion Status:
52%
|
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GS-2024B-FT-106 | Breuval | US | Cepheid Light Curves in Nearby Galaxies: Gemini and HST jointly test the Hubble Tension | GMOS-S | 2.00 | |
Execution Status: |
Dates Taken: 20240928 20241011 |
Completion Status:
76%
|
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GS-2024B-FT-107 | Lacy | US | Connecting the dots - spectroscopy of a radio-loud little red dot analog | GMOS-S | 2.00 | |
Execution Status: complete |
Dates Taken: 20241001 20241002 20241004 |
Completion Status:
100%
|
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GS-2024B-FT-108 | LeBaron | US | Ultra-Late (>800d) NIR Photometry of a Peculiar Type Ic Supernova with Signatures of Dust Reprocessing | Flamingos2 | 1.88 | |
Execution Status: |
Dates Taken: |
Completion Status:
0%
|
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GS Fast Turnaround Time Queue Band 2 | ||||||
Ref # | PI | Partner | Title | Instrument | Hours allocated |
|
GS-2024B-FT-201 | Muller | US | Constraining metallicity in the lowest luminosity FRB host galaxy discovered to date | GMOS-S | 2.60 | |
Execution Status: |
Dates Taken: |
Completion Status:
0%
|
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GS-2024B-FT-202 | Venn | CA | The C-19 Stellar Stream | GHOST | 2.36 | |
Execution Status: complete |
Dates Taken: 20240901 20240907 20240908 20240923 20240927 |
Completion Status:
100%
|
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GS-2024B-FT-203 | Hartman | US | To be a Binary or Not to be a Binary: Confirming the Multiplicity Status of Potential HWO Targets | Visitor | 0.66 | |
Execution Status: |
Dates Taken: |
Completion Status:
0%
|
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GS-2024B-FT-204 | Medoff | US | Confirmation of two new dwarf galaxy satellites of NGC 55, discovered with the Dark Energy Camera | GMOS-S | 3.30 | |
Execution Status: |
Dates Taken: 20241004 |
Completion Status:
41%
|
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GS-2024B-FT-205 | Petryk | CA | Measuring the ionization state in the ambient medium of the extraordinary supernova remnant RCW 86 | GMOS-S | 2.24 | |
Execution Status: |
Dates Taken: 20240913 |
Completion Status:
0%
|
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GS-2024B-FT-206 | Cerny | US | Confirming a New Magellanic Satellite Candidate Identified Through Machine Learning | GMOS-S | 2.88 | |
Execution Status: |
Dates Taken: |
Completion Status:
0%
|
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GS-2024B-FT-207 | Boutsia | US | Testing the Big Bang Nucleosynthesis | GHOST | 3.00 | |
Execution Status: |
Dates Taken: 20240901 |
Completion Status:
89%
|
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GS-2024B-FT-208 | Jones | US | Faint Local Volume Dwarfs Across All Environments | GMOS-S | 3.52 | |
Execution Status: |
Dates Taken: |
Completion Status:
0%
|
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GS-2024B-FT-209 | Kim | US | Photoevaporating Protoplanetary Disks in Orion's NGC 1977 in the Most Common UV Environment | GMOS-S | 3.48 | |
Execution Status: |
Dates Taken: |
Completion Status:
0%
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GS-2024B-FT-210 | Saffe | AR | Discovery of lambda Boo stars in open clusters | GHOST | 3.49 | |
Execution Status: |
Dates Taken: 20241004 20241005 |
Completion Status:
13%
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