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Queue Summary : Semester 2000QS (QuickStart) |
The 2000QS queue shown in the table below summarises the programs that have been awarded time on Gemini North for QuickStart service observing. The blocked observing schedule indicates the likely blocks for QuickStart observations. As a reminder, all capabilities are made available on a shared-risks basis.
The queue is constructed from the ranked list of proposals of each National TAC using the merging sequence and is divided into four scientific ranking bands (SRBs; jump directly to band 1, band 2 or band 3). 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 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 and is responsible for defining the detailed configuration and observing sequences and for overseeing data quality assessment. During this phase of early science use these are largely manual processes and therefore the SRBs are also used to prioritise program preparation and user support. Initially only programs in the top two SRBs will be prepared for observation.
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 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.
Partner: partner or country to which time will be charged (US, UK, CA=Canada,
AU=Australia, CH=Chile, AR=Argentina, BR=Brazil, UH=University of Hawaii (host), GS=Gemini
staff).
Title: the title of the program.
Instrument: Hokupa'a/QUIRC or OSCIR for 2000QS.
Status: the execution status of the program (blank field = not yet in preparation,
"in prep" = Phase II preparation of detailed observation desciptions underway;
"started" = executed one or more observations; "continued" =
additional data taken for a started program; "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).
Update: the date when the status information was last updated.
Scientific Ranking Band 1 | ||||||
Ref # | PI | Partner | Title | Instrument | Status | Update |
GN-2000QS-Q-1 | Allen | US | Revealing the youngest protostars in the nearest young cluster | OSCIR | in prep | 13-Aug-00 |
GN-2000QS-Q-2 | Baker | UK | The Nature of Damped Lyman alpha Absorbers, and Quasar Environments | Hokupa'a | data sent | 19-Mar-01 |
GN-2000QS-Q-3 | Barba | AR | Massive stars in NGC 604: where is the next generation? [joint proposal with GN-2000QS-Q-57] | Hokupa'a | in prep | 13-Aug-00 |
GN-2000QS-Q-4 | Chun | GS | Imaging of Low Redshift QSO Damped Lyman-alpha Absorption Line Systems | Hokupa'a | data sent | 19-Mar-01 |
GN-2000QS-Q-5 | Croom | AU | Typical AGN host galaxies at the epoch of galaxy formation | Hokupa'a | data sent | 19-Mar-01 |
GN-2000QS-Q-6 | Dottori | BR | Circumnuclear Structures in the Interacting Seyfert Galaxy NGC1241 [joint proposal with GN-2000QS-Q-40] | Hokupa'a | data sent | 1-Nov-00 |
GN-2000QS-Q-7 | Feldman | CA | Mid-Infrared Observations of Bright SCUBA Sources in MSX Infrared-Dark Clouds | OSCIR | data sent | 19-Mar-01 |
GN-2000QS-Q-8 | Frogel | US | The Stellar Content of M33's Bulge Revealed with Deep IR Imaging | Hokupa'a | data sent | 19-Mar-01 |
GN-2000QS-Q-9 | Jensen | GS | Measuring Infrared Surface Brightness Fluctuations with Hokupaa | Hokupa'a | data sent | 1-Nov-00 |
GN-2000QS-Q-10 | Jewitt | UH | AO Imaging of Circumstellar Disks | Hokupa'a | data sent | 19-Mar-01 |
GN-2000QS-Q-11 | Kavelaars | CA | Hot dust as a probe of planetary disks, observations of Epsilon Eridani | OSCIR | data sent | 19-Mar-01 |
GN-2000QS-Q-12 | Kochanek | US | Astrometry of the PKS1830-211 Gravitational Lens [duplicate of GN-2000QS-Q-24] | Hokupa'a | data sent | 1-Nov-00 |
GN-2000QS-Q-13 | Kwok | CA | High-Resolution Mid-IR Imaging of Emission Features in Carbon-Rich Proto-Planetary Nebulae | OSCIR | data sent | 19-Mar-01 |
GN-2000QS-Q-14 | Lopez | CH | Identifying the CIV absorbers in the lines of sight to the double QSO HS 1216+5032 | Hokupa'a | data sent | 19-Mar-01 |
GN-2000QS-Q-15 | Luhman | US | A Search for Newborn Planets | Hokupa'a | data sent | 19-Mar-01 |
GN-2000QS-Q-16 | Mendes de Oliveira | BR | Tidal Dwarf Galaxy Candidates in Stephan's Quintet | Hokupa'a | data sent | 1-Nov-00 |
GN-2000QS-Q-17 | Mirabel | AR | Gamma-ray Bursts as a Cosmic Window for Star Formation and Galaxy Evolution | Hokupa'a | data sent | 19-Mar-01 |
GN-2000QS-Q-18 | Pastoriza | BR | Near IR imaging of the nuclear region of NGC 7626 [joint proposal with GN-2000QS-Q-43] | Hokupa'a | data sent | 19-Mar-01 |
GN-2000QS-Q-19 | Roche | UK | The bottom of the IMF: a pencil beam search for Planetary Mass Objects in Orion | Hokupa'a | data sent | 19-Mar-01 |
GN-2000QS-Q-20 | Still | US | High resolution imaging of magnetically-propelled ejecta from the accreting binary star AE Aquarii | Hokupa'a | data sent | 1-Nov-00 |
GN-2000QS-Q-21 | Storchi-Bergmann | BR | The Nature of the Mid-IR Emission in Radio-Galaxies: Cygnus A, a Test Case | OSCIR | in prep | 13-Aug-00 |
Scientific Ranking Band 2 | ||||||
Ref # | PI | Partner | Title | Instrument | Status | Update |
GN-2000QS-Q-22 | Abraham | CA | Deep IR Imaging of Extremely Red Objects in the LCIR Survey | Hokupa'a | in prep | 13-Aug-00 |
GN-2000QS-Q-23 | Boroson | US | QSO Host Galaxies: The Link to Nuclear Properties | Hokupa'a | data sent | 19-Mar-01 |
GN-2000QS-Q-24 | Courbin | CH | A sharp look at the obscured Einstein ring PKS 1830-211 [duplicate of GN-2000QS-Q-12] | Hokupa'a | data sent | 1-Nov-00 |
GN-2000QS-Q-25 | Fajardo-Acosta | US | Probing Newly Discovered Exozodiacal Vega-type Dust | OSCIR | data sent | 19-Mar-01 |
GN-2000QS-Q-26 | Garnavich | US | Host Galaxies of High Redshift Supernovae | Hokupa'a | in prep | 13-Aug-00 |
GN-2000QS-Q-27 | Hartmann | US | Probing dusty protostellar binaries in the mid-IR | OSCIR | data sent | 19-Mar-01 |
GN-2000QS-Q-28 | Jameson | UK | A search for planets and brown dwarfs in the Pleiades | Hokupa'a | data sent | 19-Mar-01 |
GN-2000QS-Q-29 | Jorgensen | GS | Stellar populations of the E+A galaxy in Abell 665 | Hokupa'a | data sent | 19-Mar-01 |
GN-2000QS-Q-30 | Mardones | CH | Mid-Infrared Observation of Northern Hot Molecular Cores | OSCIR | data sent | 19-Mar-01 |
GN-2000QS-Q-31 | Plante | CA | Very Young Super Star Cluster in SBS 0335-052 | OSCIR | data sent | 19-Mar-01 |
GN-2000QS-Q-32 | Puxley | GS | Mid-IR imaging of dusty super star clusters and their bolometric luminosities | OSCIR | data sent | 19-Mar-01 |
GN-2000QS-Q-33 | Reipurth | US | Multiplicity and Circumstellar Structure of Deeply Embedded Herbig-Haro Energy Sources | OSCIR | data sent | 19-Mar-01 |
GN-2000QS-Q-34 | Serjeant | UK | Mid-infrared photometry of the prototypical hyperluminous galaxy IRAS F10214+4724 | OSCIR | data sent | 15-Dec-00 |
GN-2000QS-Q-35 | Stockton | UH | Adaptive Optics Imaging of the Radio Galaxy 3C68.2 | Hokupa'a | data sent | 1-Nov-00 |
GN-2000QS-Q-36 | Tully | UH | Tip of the Red Giant Branch at Kp in External Galaxies | Hokupa'a | in prep | 13-Aug-00 |
GN-2000QS-Q-37 | Tully | UH | Tip of the Red Giant Branch at Kp in External Galaxies | Hokupa'a | in prep | 13-Aug-00 |
Scientific Ranking Band 3 | ||||||
Ref # | PI | Partner | Title | Instrument | Status | Update |
GN-2000QS-Q-38 | Balick | US | Evolution & Expansion Parallax of Planetary Nebulae | Hokupa'a | data sent | 19-Mar-01 |
GN-2000QS-Q-39 | Barbá | AR | The Stellar and Interstellar Environment of Soft Gamma-Ray Repeaters | Hokupa'a | ||
GN-2000QS-Q-40 | Carranza | AR | Circumnuclear Structures in the Interacting Seyfert Galaxy NGC 1241 [joint proposal with GN-2000QS-Q-6] | Hokupa'a | data sent | 1-Nov-00 |
GN-2000QS-Q-41 | Courbin | CH | High resolution imaging at 2.2 microns of the nuclear structure of NGC1068 [joint proposal with GN-2000QS-Q-61] | Hokupa'a | ||
GN-2000QS-Q-42 | Diaz | BR | The Structure of Nova Shells | Hokupa'a | data sent | 1-Nov-00 |
GN-2000QS-Q-43 | Donzelli | AR | Near IR imaging of the nuclear region of NGC 7626 [joint proposal with GN-2000QS-Q-18] | Hokupa'a | data sent | 1-Nov-00 |
GN-2000QS-Q-44 | Efstathiou | UK | A search for dust features in the mid-infrared spectra of PG quasars | OSCIR | ||
GN-2000QS-Q-45 | Geballe | GS | Spatially resolved mid-infrared spectra of the nucleus of NGC1068 | OSCIR | ||
GN-2000QS-Q-46 | Gledhill | UK | Imaging Superwind Shells in Proto-Planetary Nebulae at 10 and 18 microns | OSCIR | ||
GN-2000QS-Q-47 | Jorgensen | GS | Deep IR study of the candidate galaxy cluster around Q0835+580 at z=1.5 | Hokupa'a | ||
GN-2000QS-Q-48 | Lipari | AR | Galaxies/QSOs with Extreme IR and FeII Emission (IR Imaging) | Hokupa'a | ||
GN-2000QS-Q-49 | Lucas | UK | Adaptive Optics imaging of embedded Young Stellar objects | Hokupa'a | ||
GN-2000QS-Q-50 | Marleau | UK | Stellar Populations in the Dwarf Elliptical Galaxy M32 Resolved with AO | Hokupa'a | ||
GN-2000QS-Q-51 | Minniti | CH | AO near-IR observations of 4C41.17 at z=3.8: a massive galaxy in formation ? | Hokupa'a | ||
GN-2000QS-Q-52 | Moffat | CA | Resolving Cool Dust Ejecta Around Carbon-Rich Wolf-Rayet Stars | OSCIR | ||
GN-2000QS-Q-53 | Morris | CA | Mid IR Observations of High Star Formation Rate Galaxies | OSCIR | ||
GN-2000QS-Q-54 | Pellerin | CA | Young Stellar Populations in Barred Spiral Galaxies: the Starburst-AGN Connection | OSCIR | ||
GN-2000QS-Q-55 | Puxley | GS | Reddening of young blue star clusters in NGC1275 | Hokupa'a | ||
GN-2000QS-Q-56 | Rodrigues | BR | Mid-IR spectroscopy of the proto-planetary nebula Hen 3-1475 | OSCIR | ||
GN-2000QS-Q-57 | Rubio | CH | Massive stars in NGC 604: where is the next generation? [joint proposal with GN-2000QS-Q-3] | Hokupa'a | ||
GN-2000QS-Q-58 | Sanders | UH | Identification of the Far-IR Extragalactic Background Population | Hokupa'a | ||
GN-2000QS-Q-59 | Takamiya | GS | Ages of sub-kiloparsec structures of galaxies at 0.3<z<1 | Hokupa'a | ||
GN-2000QS-Q-60 | Tully | UH | Tip of the Red Giant Branch at Kp in External Galaxies | Hokupa'a | ||
GN-2000QS-Q-61 | Veran | CA | High resolution imaging at 2.2 microns of the nuclear structure of NGC1068 [joint proposal with GN-2000QS-Q-41] | Hokupa'a | ||
GN-2000QS-Q-62 | Woodward | US | Origins of Disks & Protoplanetesimals Using Silicate Mineralogy | OSCIR | ||
GN-2000QS-Q-63 | Woodward | US | Origins of Disks & Protoplanetesimals Using Silicate Mineralogy | OSCIR |
Last update March 19, 2001; Phil Puxley