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Queue Summary : Semester 2001B Gemini North and South |
The queues shown in the tables below summarise the programs that have been awarded time on Gemini North and South. As a reminder, all capabilities are made available on a shared-risks basis. Jump directly to the queue for:
The queue is constructed by the International TAC from the ranked list of proposals of each National TAC using the merging sequence and is divided into four scientific ranking bands (SRBs). Several proposals have multiple occurrences as they were sub-divided by the relevant NTAC. Only the first three bands are shown in the table. Within each band, all proposals are assumed to have equal scientific merit and have been sorted by PI name for convenience. The choice of which observation within which program to execute next depends on the match to current observing conditions, the balance of each partner's usage and other factors such as future accessibility, whether a program has been started etc. (see a detailed discussion in Puxley 1997; Gemini Preprint #19). The aim is to exhaust band 1 (highest ranked) programs before moving onto band 2 and so on. An observation in band 1 that does not require the best conditions will nevertheless be executed in preference to a band 2 observation even if the latter is a better match. Thus the likelihood of execution decreases from band 1 through to band 4. Bands 1 through 3 aim to fill the nominal time available (excluding weather loss). Programs in band 4 overfill the queue and provide further flexibility with respect to weather conditions and foreseen or unforeseen problems.
Each program has been assigned a Gemini Contact Scientist (CS) who is the point of contact between the Observatory and the Principal Investigator (PI) after the detailed observations are defined by the PI in Phase II. (Prior to submission of Phase II programs, each National Office provides the first point of contact). The Contact Scientist is responsible for overseeing data quality. During this (shared-risks) phase of early science use the observing and data processing are largely manual activities and therefore the SRBs are also used to prioritise program preparation and user support.
In routine operation the intent is to update this page nightly. During shared-risks science use, this queue status page may only be updated after each observing block with a given instrument. Please check back from time to time.
Note that individual SRBs
will not be in detailed balance with respect to partner shares. Aggregating over two or
more bands generally provides an equitable distribution of queue loading (in hours, not in
the number of proposals). Additional flexibility is available when executing observations
to balance the partner usage of time. The intent is to achieve balance over 2 or 3
semesters, not a single semester.
The columns in the table for Gemini
North 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.
PI: name of Principal Investigator.
Partner: partner or country to which time will be charged (US, UK, CA=Canada,
AU=Australia, AR=Argentina, BR=Brazil, UH=University of Hawaii (host), GS=Gemini staff).
Title: the title of the program.
Instrument: name of the instrument
Hours: time allocated to the program (if a joint or duplicate proposal, this is is the time allocated
to this part of the program only)
Status: the execution status of the program: blank field = not yet in preparation,
"in prep" = Phase II preparation of detailed observation descriptions
done;
"started" = executed one or more observations; "continued" =
additional data taken for a started program; "completed" = all
requested data taken; "data in QA" = data undergoing
pre-ship quality assessment; "data sent" = data for one or more observations and
calibrations sent to PI; "done" = program complete. Recent changes
are highlighted in bold font.
Update: the date when the status information was last updated.
GN Scientific Ranking Band 1 | |||||||
Ref # | PI | Partner | Title | Instrument | Hours | Status | Updated |
GN-2001B-Q-1 | Cid Fernandes | BR | A Near-IR study of optically ambiguous Seyfert 2's: Implications for the Starburst-AGN connection | NIRI | 3.5 | in prep | 19Oct01 |
GN-2001B-Q-2 | Crampton | CA | Probing the high redshift Universe via quasars with z > 5 [joint proposal with GN-2001B-Q-60] | GMOS | 10 | data sent | 11Mar02 |
GN-2001B-Q-3 | de Carvalho | BR | Fundamental Properties of Elliptical Galaxies and Their Evolution | NIRI | 2 | in prep | 19Oct01 |
GN-2001B-Q-4 | Dunlop | UK | The dust-enshrouded formation of massive elliptical galaxies | NIRI | 20 | in prep | 19Oct01 |
GN-2001B-Q-5 | Forte | AR | K-band Imaging of Globular Clusters in Young and Old Ellipticals [joint proposal with GN-2001B-Q-58] | NIRI | 1.25 | in prep | 19Oct01 |
GN-2001B-Q-6 | Gladders | CA | Multi-Filter High-Resolution Imaging Observations of a Unique Sample of Strong-Lensing Clusters | GMOS | 3.85 | data sent | 11Mar02 |
GN-2001B-Q-7 | Gladders | CA | Multi-Filter High-Resolution Imaging Observations of a Unique Sample of Strong-Lensing Clusters | NIRI | 8.6 | in prep | 19Oct01 |
GN-2001B-Q-8 | Gómez | AR | Search for Protoplanetary Disks and Giant Extrasolar Planets Around Extremely Low Mass Young Objects | NIRI | 6.5 | in prep | 19Oct01 |
GN-2001B-Q-9 | Graham | US | Near-IR Imaging of Super Star Clusters in the Antennae | NIRI | 5 | in prep | 19Oct01 |
GN-2001B-C-1 | Jayawardhana | US | A Search for Disks around Young Brown Dwarfs and Very-Low-Mass Stars [moved from classical sched] | NIRI | 10 | in prep | 19Oct01 |
GN-2001B-Q-10 | Jorgensen | GS | Galaxy Evolution During Half the Age of the Universe | GMOS | 39 | data sent | 11Mar02 |
GN-2001B-Q-11 | Lada | US | Constraining the Lifetimes of Circumstellar Disks:L band Observations of NGC 2362 | NIRI | 5 | in prep | 19Oct01 |
GN-2001B-Q-12 | Malkan | US | Direct Comparison of Optical and Infrared Searches for High-Redshift Galaxies: How Much of the Young | NIRI | 20 | in prep | 19Oct01 |
GN-2001B-Q-13 | Roche | UK | Classification of young brown dwarfs and planetary mass objects in Orion | GMOS | 12 | data sent | 10Apr02 |
GN-2001B-Q-14 | Schmidt | AU | Measuring the Universe to z=1.2 with SN Ia [joint proposal with GN-2001B-Q-16 & Q-17] | NIRI | 21 | data sent | 04Feb02 |
GN-2001B-Q-15 | Sodre | BR | Search for Gravitational Arcs in X-Ray Luminous clusters | GMOS | 4 | data sent | 11Mar02 |
GN-2001B-Q-16 | Suntzeff | US | Type Ia Supernovae in the Epoch of Deceleration [joint proposal with GN-2001B-Q-14 & Q-17] | NIRI | 40 | data sent | 04Feb02 |
GN-2001B-Q-17 | Tonry | UH | Measuring the Universe to z=1.2 with SN Ia [joint proposal with GN-2001B-Q-14 & Q-16] | NIRI | 14 | data sent | 04Feb02 |
GN Scientific Ranking Band 2 | |||||||
Ref # | PI | Partner | Title | Instrument | Hours | Status | Updated |
GN-2001B-Q-18 | Barbá | AR | Massive stars in NGC 604: where is the next generation? | NIRI | 2.5 | in prep | 19Oct01 |
GN-2001B-Q-19 | Burleigh | UK | Imaging extra-solar planets | NIRI | 20 | in prep | 19Oct01 |
GN-2001B-Q-20 | Crowther | UK | Quantitative analysis of the peculiar Wolf-Rayet population in the starburst galaxy IC 10 [joint proposal with GN-2001B-Q-23] | GMOS | 7 | data sent | 11Mar02 |
GN-2001B-Q-21 | Da Costa | AU | The Extended Star Formation Histories of the M81 Group dwarf Ellipticals F8D1 and BK 5N | NIRI | 6.83 | in prep | 19Oct01 |
GN-2001B-Q-22 | Dietrich | US | Probing the Star Formation History at z >= 5 | NIRI | 11 | in prep | 19Oct01 |
GN-2001B-Q-23 | Drissen | CA | Quantitative analysis of the peculiar Wolf-Rayet population in the starburst galaxy IC 10 [joint proposal with GN-2001B-Q-20] | GMOS | 6.7 | data sent | 11Mar02 |
GN-2001B-Q-24 | Lada | US | Circumstellar Disks around Brown Dwarfs in the Trapezium Cluster | NIRI | 10 | in prep | 19Oct01 |
GN-2001B-Q-25 | Lilly | CA | Metallicities of 0.5 < z < 1.0 galaxies | NIRI | 8.75 | in prep | 19Oct01 |
GN-2001B-Q-26 | Liu | UH | A Methane-Break Imaging Survey in Orion | NIRI | 20 | in prep | 19Oct01 |
GN-2001B-C-8 | Luhman | US | Searching for the Bottom of the Initial Mass Function [moved from classical sched] | NIRI | 20 | in prep | 19Oct01 |
GN-2001B-Q-27 | Rhoads | US | A Census of z > 4 Galaxies | GMOS | 20 | data sent | 11Mar02 |
GN-2001B-Q-28 | Richer | CA | Testing White Dwarf Cosmochronology in M67 | GMOS | 18.25 | in prep | 19Oct01 |
GN-2001B-Q-29 | Tolstoy | UK | Using the Ca II triplet to disentangle age, metallicity and dynamical properties of Leo I | GMOS | 10 | data sent | 11Mar02 |
GN-2001B-Q-30 | Tolstoy | UK | HI Selected Dwarfs: A New Class of Galaxy -or- Unreliable Distances? | GMOS | 16 | in prep | 19Oct01 |
GN-2001B-C-7 | Trager | US | Surface Brightness Fluctutations in the Near Infrared: A Unique Tool for Stellar Population Studies [moved from classical sched] | NIRI | 10 | in prep | 19Oct01 |
GN-2001B-Q-31 | van Zee | CA | Stellar Rotation Curves of Starbursting Dwarf Galaxies | GMOS | 8.5 | in prep | 19Oct01 |
GN Scientific Ranking Band 3 | |||||||
Ref # | PI | Partner | Title | Instrument | Hours | Status | Updated |
GN-2001B-Q-32 | Bosch | AR | The youngest and most luminous Giant HII regions: a link with HII galaxies | NIRI | 2.3 | ||
GN-2001B-Q-33 | Carranza | AR | Circumnuclear Structures in the Interacting Seyfert Galaxy NGC 1241. II.- Spectroscopy. | NIRI | 4.5 | ||
GN-2001B-Q-34 | Crampton | CA | The first galaxies in the Universe | NIRI | 12 | ||
GN-2001B-Q-35 | Figueredo | BR | Spectroscopy of OB Stars in the Giant HII Region W49A | NIRI | 3.9 | ||
GN-2001B-Q-36 | Gallagher | US | Near-IR characterization of the intermediate age clusters of NGC 1275. | NIRI | 15 | ||
GN-2001B-Q-37 | Geballe | GS | CO in T-type (CH4-dominated) brown dwarfs | NIRI | 23 | ||
GN-2001B-Q-38 | Gil de Paz | US | Star Formation History of IZw18 & SBS0335--052E | GMOS | 10 | data sent | 11Mar02 |
GN-2001B-Q-39 | Kukula | UK | The evolution of high-redshift quasar host galaxies | NIRI | 12 | ||
GN-2001B-Q-40 | Macri | US | A Study of the Metallicity Dependence of the Cepheid Period-Luminosity Relation in M33 | NIRI | 6 | ||
GN-2001B-Q-41 | Martin | CA | The Chemistry of the Extreme Outer Disks of Nearby Spiral Galaxies | GMOS | 8.5 | data sent | 11Mar02 |
GN-2001B-Q-42 | Postman | US | Clustering of Galaxy Clusters at Intermediate Redshifts | GMOS | 50 | ||
GN-2001B-Q-43 | Rawlings | UK | Redshift, velocity structure and starburst activity of a forming ultramassive cluster | GMOS | 8 | ||
GN-2001B-Q-44 | Sharples | UK | The Formation History of NGC 3115 | GMOS | 6 | data sent | 11Mar02 |
GN-2001B-Q-45 | Storchi Bergmann | BR | The nature of distant radio galaxies | NIRI | 5 | ||
GN-2001B-Q-46 | Webb | CA | A GEMINI investigation of the history of energy production in the universe [joint proposal with GN-2001B-Q-57] | NIRI | 12 | ||
GN-2001B-Q-47 | Webster | AU | Microarcsecond Imaging of a Gravitationally Lensed QSO: 2237+0305 | NIRI | 4.7 | ||
GN-2001B-Q-48 | Williams | UK | Imaging the evolving dust cloud from WR140 | NIRI | 3 |
The columns in the table for Gemini
South 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.
PI: name of Principal Investigator.
Partner: partner or country to which time will be charged (US, UK, CA=Canada,
AU=Australia, CH=Chile (host), AR=Argentina, BR=Brazil, GS=Gemini staff).
Title: the title of the program.
Instrument: name of the instrument
Hours: time allocated to the program (if a joint or duplicate proposal, this is is the time allocated
to this part of the program only)
Status: the execution status of the program: blank field = not yet in preparation,
"in prep" = Phase II preparation of detailed observation descriptions
done;
"started" = executed one or more observations; "continued" =
additional data taken for a started program; "completed" = all
requested data taken; "data in QA" = data undergoing
pre-ship quality assessment; "data sent" = data for one or more observations and
calibrations sent to PI; "done" = program complete. Recent changes
are highlighted in bold font.
Update: the date when the status information was last updated.
GS Scientific Ranking Band 1 | |||||||
Ref # | PI | Partner | Title | Instrument | Hours | Status | Updated |
GS-2001B-Q-1 | Barbosa | BR | Massive YSOs in NGC 3576 | OSCIR | 2.8 | data sent | 02Jan02 |
GS-2001B-Q-2 | Bronfman | CH | The Stellar Density Around Massive Young Stars: A Test of Collisional Models of High Mass Star Formation | Flamingos-I | 8 | in prep | 24Aug01 |
GS-2001B-Q-3 | Crabtree | CA | Spatial Variations in the PAH Features of the Red Rectangle | OSCIR | 4.75 | in prep | 06Nov01 |
GS-2001B-Q-4 | Da Costa | AU | The Extended Star Formation Histories of the Sculptor Group Dwarf Galaxies ESO540-032 and ESO294-010 | Flamingos-I | 3.91 | data sent | 22Nov01 |
GS-2001B-Q-5 | Davidge | CA | The Star-Forming History of Nearby Isolated Dwarf Spheroidal Galaxies | Flamingos-I | 13.1 | data sent | 14Nov01 |
GS-2001B-Q-6 | Francis | AU | Extremely Red Galaxies in the Early Universe | Flamingos-I | 5 | in prep | 24Aug01 |
GS-2001B-Q-7 | Fruchter | US | Quick Response to GRBs: the early burst and the late-time decay [joint proposal with GS-2001B-Q-35] | Acquisition Cam | 5 | in prep | 02Oct01 |
GS-2001B-Q-8 | Halpern | US | Search for Small-Scale Structure in Gamma-ray Burst Afterglows | Acquisition Cam | 5 | in prep | 02Oct01 |
GS-2001B-Q-9 | Hayward | GS | Ten Micron Imaging of the Beta Pictoris Dust Disk | OSCIR | 8 | ||
GS-2001B-Q-10 | Hayward | GS | Ten Micron Imaging and Spectroscopy of Orion Nebula Silhouette Disks | OSCIR | 10 | data sent | 08Dec01 |
GS-2001B-Q-11 | Lucas | UK | How Low can the IMF go ? (Mk II) | Flamingos-I | 20 | data sent | 14Nov01 |
GS-2001B-Q-12 | Marleau | CA | Molecular hydrogen spectroscopy of cooling-flow galaxies | Flamingos-I | 8.6 | in prep | 02Oct01 |
GS-2001B-Q-13 | Morrell | AR | G353.2+0.9: A laboratory for theories of star formation. | Flamingos-I | 3 | data sent | 10Nov01 |
GS-2001B-Q-14 | Oppenheimer | US | Temperatures and Composition of Halo White Dwarfs | Flamingos-I | 13 | data sent | 19Nov01 |
GS-2001B-Q-15 | Suntzeff | US | Type Ia Supernovae in the Epoch of Deceleration | Acquisition Cam | 10 | data sent | 12Feb02 |
GS-2001B-Q-16 | Tothill | CA | Early stages of star formation in NGC 2068 | OSCIR | 6 | data sent | 02Jan02 |
GS-2001B-Q-17 | von Hippel | GS | Studying a Proto-planetary disk at 75 km resolution | Acquisition Cam | 4.25 | data sent | 12Feb01 |
GS-2001B-Q-18 | Willis | CH | The star-formation history of field and cluster galaxies at z = 3.09 | Flamingos-I | 16.5 | data sent | 10Nov01 |
GS Scientific Ranking Band 2 | |||||||
Ref # | PI | Partner | Title | Instrument | Hours | Status | Updated |
GS-2001B-Q-19 | Aspin | GS | Multiplicity and Circumstellar Structure of Deeply Embedded Herbig-Haro Energy Sources [joint proposal with GS-2001B-Q-44] | OSCIR | 10 | data sent | 02Jan02 |
GS-2001B-Q-20 | Barba | AR | Study of Low End of the Initiall Mass Function in Large Magellanic Cloud Star Forming Regions: N159 [joint proposal with GS-2001B-Q-32] | Flamingos-I | 6 | in prep | 24Aug01 |
GS-2001B-Q-21 | Bonatto | BR | The hosts and environment of distant radio galaxies | Flamingos-I | 5.3 | in prep | 24Aug01 |
GS-2001B-Q-22 | Calvet | US | Protoplanetary Disk Evolution in the Orion OB1 Association | OSCIR | 20 | data sent | 02Jan02 |
GS-2001B-Q-23 | Drinkwater | AU | The origin of ultra-compact dwarf galaxies | Flamingos-I | 10.8 | data sent | 16Nov01 |
GS-2001B-Q-24 | Gaidos | US | Ten-micron imaging and spectroscopy of dust around young solar analogs | OSCIR | 5 | data sent | 02Jan02 |
GS-2001B-Q-25 | Hynes | UK | Reverberation Mapping of Black Hole X-ray Transients | Acquisition Cam | 12 | in prep | 02Oct01 |
GS-2001B-Q-26 | Ledlow | GS | A Very Unusual, Highly Obscured AGN and Jet-Source in a Spiral Galaxy | Flamingos-I | 4.6 | in prep | 24Aug01 |
GS-2001B-Q-27 | Mallen-Ornelas | CH | Number Counts of Extremely Red Galaxies to Extremely Faint Magnitudes | Flamingos-I | 5.5 | in prep | 24Aug01 |
GS-2001B-Q-28 | Mason | UK | Spatially-resolved mid-infrared spectra of the obscuring dust in NGC1068 | OSCIR | 8 | ||
GS-2001B-Q-29 | Plante | CA | The impact of the youngest Super Star-Clusters on the insterstellar medium in He 2-10 | OSCIR | 3.5 | ||
GS-2001B-Q-30 | Plante | CA | Very Young Super Star Cluster in SBS 0335-052 | OSCIR | 3.5 | in prep | 06Nov01 |
GS-2001B-Q-31 | Robert | CA | Very Young Stellar Populations in Starburst Galaxies: The Process of Star Formation | OSCIR | 11 | data sent | 02Jan02 |
GS-2001B-Q-32 | Rubio | CH | Study of the Initial Mass Function in Large Magellanic Cloud Star Forming Regions [joint proposal with GS-2001B-Q-20] | Flamingos-I | 5 | in prep | 24Aug01 |
GS-2001B-Q-33 | Serabyn | US | Mid-Infrared Probes of Brown Dwarfs | OSCIR | 10 | data sent | 02Jan02 |
GS-2001B-Q-34 | Sharples | UK | Globular Cluster Systems of Elliptical Galaxies in Low Density Environments | Flamingos-I | 12 | in prep | 24Aug01 |
GS-2001B-Q-35 | Tanvir | UK | Quick Response to GRBs: the early burst and the late-time decay [joint proposal with GS-2001B-Q-7] | Acquisition Cam | 8 | in prep | 02Oct01 |
GS Scientific Ranking Band 3 | |||||||
Ref # | PI | Partner | Title | Instrument | Hours | Status | Updated |
GS-2001B-Q-36 | Campusano | CH | The Morphology of Low-luminosity High-z Galaxies Magnified by the Massive Cluster Lens Abell AC114 (z=0.312) | Flamingos-I | 13.5 | ||
GS-2001B-Q-37 | Casassus | CH | OSCIR imaging of the LINER in the heavily interacting Virgo Galaxy NGC4438 | OSCIR | 1 | ||
GS-2001B-Q-38 | Casassus | CH | Dust in Halo and Magellanic Cloud PNe | OSCIR | 10 | ||
GS-2001B-Q-39 | Colbert | US | Nuclear Starbursts in Seyfert 1 Galaxies | Flamingos-I | 10 | ||
GS-2001B-Q-40 | Gallagher | US | Mid-IR Spectra of Ultradense HII Regions | OSCIR | 3 | ||
GS-2001B-Q-41 | Gregorio-Hetem | BR | The nature of unidentified X-ray sources in CMa star formation region | Acquisition Cam | 1.3 | data sent | 23Nov01 |
GS-2001B-Q-42 | Hoare | UK | The circumstellar matter distribution around massive young stellar objects | OSCIR | 4 | ||
GS-2001B-Q-43 | Jones | UK | Dusty dwarfs | OSCIR | 8 | ||
GS-2001B-Q-44 | Reipurth | US | Multiplicity and Circumstellar Structure of Deeply Embedded Herbig-Haro Energy Sources [joint proposal with GS-2001B-Q-19] | OSCIR | 10 | ||
GS-2001B-Q-45 | Ruiz | UK | Testing Dusty torus models in AGN | OSCIR | 22 | ||
GS-2001B-Q-46 | Shanks | UK | The Nature of Narrow-Line, FIR-Luminous, X-ray Galaxies | OSCIR | 9 | ||
GS-2001B-Q-47 | Weinberger | US | A Search for Disks around Nearby Young Stars | OSCIR | 30 | ||
GS-2001B-Q-48 | Whiting | AU | Mid-infrared spectra of Parkes Quasars | OSCIR | 3.7 | ||
GS-2001B-Q-49 | Wood | AU | Bolometric luminosities of post-AGB stars in the LMC | OSCIR | 2 | ||
GS-2001B-Q-50 | Woodward | US | OSCIR Spectroscopy of Comet C/2000 WM1 (LINEAR) | OSCIR | 6 | ||
GS Scientific Ranking Band 4 | |||||||
Ref # | PI | Partner | Title | Instrument | Hours | Status | Updated |
GS-2001B-Q-51 | Charles | UK | Ultra-Short-Period X-Ray Binaries in Globular Clusters | Acquisition Cam | 9 | data sent | 23Nov01 |
GS-2001B-Q-52 | Hynes | UK | The Nature of Optical Flaring in Quiescent Black Holes and Neutron Stars | Acquisition Cam | 16 | in prep | 02Oct01 |
GS-2001B-Q-53 | Moth | US | A Near-IR Study of the Properties of Lyman Break Galaxies | Flamingos-I | 30 | ||
GS-2001B-Q-54 | Ueta | US | High-Resolution Mid-IR Imaging of Southern Proto-Planetary Nebula Candidates | OSCIR | 10 | ||
GS-2001B-Q-55 | Yan | US | Gemini JHK imaging of z~6 candidates in the HDF-S: Pregalactic objects forming around young weak AGN | Flamingos-I | 5 |
Last update April 10, 2002; Phil Puxley