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Queue Summary : Semester 2002A 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. 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.
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 (when
available).
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-2002A-Q-1 | Bechtold | US | The Lyman Alpha Forest and the Galaxy Distribution towards PG 1634+706 | GMOS | 1 | done | 19Aug02 |
GN-2002A-Q-2 | Bechtold | US | The Lyman Alpha Forest and the Galaxy Distribution towards PG 1634+706 | GMOS | 4.5 | done | 19Aug02 |
GN-2002A-Q-3 | Benvenuto | AR | Very Cool White Dwarf Stars: Constraints to the Chemical Evolution Models and Theories of Non-Ideal Gases | NIRI | 3 | data sent | 12Aug02 |
GN-2002A-Q-4 | Blum | US | A Near Infrared Investigation of Optically Obscured Galactic Giant HII Regions | NIRI | 10 | data sent | 12Aug02 |
GN-2002A-Q-5 | Cid Fernandes | BR | A Near-IR study of optically ambiguous Seyferts: Implications for the Starburst-AGN connection | NIRI | 5.33 | data sent | 12Aug02 |
GN-2002A-Q-6 | Close | US | Direct imaging of very low mass companions and binary brown dwarfs | Hokupa'a + QUIRC | 20 | data sent | 26jun02 |
GN-2002A-Q-7 | Close | US | Direct imaging of very low mass companions and binary brown dwarfs | Hokupa'a + QUIRC | 5 | ||
GN-2002A-Q-8 | Cote | CA | SC24: the lowest metallicity star-forming galaxy in the Universe? | GMOS | 1.5 | done | 19Aug02 |
GN-2002A-Q-9 | Crampton | CA | Probing the high redshift Universe via quasars with z>5 [joint proposal with Q-75] | GMOS | 7.33 | done | 19Aug02 |
GN-2002A-Q-10 | Da Costa | AU | The Extended Star Formation Histories of the M81 Group dwarf Ellipticals F8D1 and BK 5N | NIRI | 6.83 | data sent | 12Aug02 |
GN-2002A-Q-11 | Diaz | BR | The structure of nova shells | GMOS | 2.81 | done | 19Aug02 |
GN-2002A-Q-12 | Dunlop | UK | The dust-enshrouded formation of massive elliptical galaxies | NIRI | 20 | data sent | 12Aug02 |
GN-2002A-Q-13 | Forte | AR | Multi-Object Spectroscopy of the GC Systems of Luminous Ellipticals [joint proposal with Q-21, Q-29, Q-64] | GMOS | 2.8 | data sent | 9Aug02 |
GN-2002A-Q-14 | Geballe | GS | CO in T-type (methane-dominated) brown dwarfs | NIRI | 15 | data sent | 12Aug02 |
GN-2002A-Q-15 | Ledlow | GS | Galaxy Evolution and the Micro-Jy Radio Population [joint proposal with Q-22] | GMOS | 22 | data sent | 26Jun02 |
GN-2002A-Q-16 | Melatos | AU | Rapid Variability of Subarcsecond Wisps and Knots in the Crab Nebula | Hokupa'a + QUIRC | 7.85 | data sent | 26Jun02 |
GN-2002A-Q-17 | Miller | GS | The Ages, Metallicities, and Velocities of Globular Clusters in Virgo Dwarf Elliptical Galaxies | GMOS | 18 | done | 19Aug02 |
GN-2002A-Q-18 | Perlmutter | US | Cosmology with High-Redshift Type Ia Supernovae [joint proposal with Q-30] | GMOS | 24 | done | 19Aug02 |
GN-2002A-Q-19 | Postman | US | Clustering of Galaxy Clusters at Intermediate Redshifts | GMOS | 20 | data sent | 14May02 |
GN-2002A-Q-20 | Pritchet | CA | A search for evidence of early star formation in galaxies around the highest known redshift QSOs at z~6 | GMOS | 14 | data sent | 9Aug02 |
GN-2002A-Q-21 | Sharples | UK | Multi-Object Spectroscopy of the GC Systems of Luminous Ellipticals [joint proposal with Q-13, Q-29, Q-64] | GMOS | 18.5 | data sent | 9Aug02 |
GN-2002A-Q-22 | Smail | UK | Galaxy Evolution and the Micro-Jy Radio Population [joint proposal with Q-15] | GMOS | 10.9 | data sent | 26Jun02 |
GN Scientific Ranking Band 2 | |||||||
Ref # | PI | Partner | Title | Instrument | Hours | Status | Updated |
GN-2002A-Q-23 | Bosch | AR | The youngest and most luminous Giant HII regions: a link with HII galaxies | NIRI | 2 | ||
GN-2002A-Q-24 | Burleigh | UK | Imaging extra-solar planets | NIRI | 10 | data sent | 12Aug02 |
GN-2002A-Q-25 | Couch | AU | Distant cluster galaxy evolution: spectroscopic dissection of E+A galaxies. | GMOS | 7.33 | ||
GN-2002A-Q-26 | Dickinson | US | A galaxy census at z~1 in the GOODS/HDF-N region [joint proposal with Q-88] | GMOS | 20 | data sent | 10Apr02 |
GN-2002A-Q-27 | Doyon | CA | A Multi-Wavelength Study of the Circumnuclear Starburst Regions of M83 | NIRI | 5.8 | data sent | 12Aug02 |
GN-2002A-Q-28 | Feinstein | AR | Ionization cones and filaments in Active Galaxy Nuclei | GMOS | 2 | ||
GN-2002A-Q-29 | Hanes | CA | Multi-Object Spectroscopy of the GC Systems of Luminous Ellipticals [joint proposal with Q-13, Q-21, Q-64] | GMOS | 7.8 | data sent | 9Aug02 |
GN-2002A-Q-30 | Hook | UK | Cosmology with High-Redshift Type Ia Supernovae [joint proposal with Q-18] | GMOS | 12 | done | 19Aug02 |
GN-2002A-Q-31 | Hook | UK | Cosmology with High-Redshift Type Ia Supernovae [joint proposal with Q-37] | NIRI | 12 | data sent | 12Aug02 |
GN-2002A-Q-32 | Hutchings | CA | Line imaging of highest redshift QSOs | NIRI | 12 | data sent | 12Aug02 |
GN-2002A-Q-33 | Jayawardhana | US | A Search for Disks around Young Brown Dwarfs and Very-Low-Mass Stars | NIRI | 10 | data sent | 12Aug02 |
GN-2002A-Q-34 | Jorgensen | GS | Galaxy Evolution During Half the Age of the Universe | GMOS | 20 | done | 19Aug02 |
GN-2002A-Q-35 | Kukula | UK | The evolution of high-redshift quasar host galaxies | NIRI | 12 | ||
GN-2002A-Q-36 | Lada | US | Constraining the Lifetimes of Circumstellar Disks:L band Observations of NGC 2362 | NIRI | 5 | ||
GN-2002A-Q-37 | Perlmutter | US | Cosmology with High-Redshift Type Ia Supernovae [joint proposal with Q-31] | NIRI | 24 | data sent | 12Jul02 |
GN-2002A-Q-38 | Tholen | UH | The Eccentricity of Charon's Orbit | Hokupa'a + QUIRC | 5 | ||
GN-2002A-Q-39 | Tonry | UH | Cosmology from High Redshift Supernovae | NIRI | 10 | ||
GN-2002A-Q-40 | Wayth | AU | Imaging the BLR of the Gravitationally Lensed QSO 2237+0305 | GMOS | 3.5 | done | 19Aug02 |
GN-2002A-Q-41 | Weiner | US | Probing the assembly and evolution of z~1 galaxies with spatially resolved IFU kinematics | GMOS | 27.5 | ||
GN-2002A-Q-42 | Yee | CA | Rich Optically-Selected Galaxy Clusters at z~1 from the RCS Survey | GMOS | 10.17 | data sent | 19Aug02 |
GN Scientific Ranking Band 3 | |||||||
Ref # | PI | Partner | Title | Instrument | Hours | Status | Updated |
GN-2002A-Q-43 | Croom | UK | The evolution of typical AGN host galaxies | Hokupa'a + QUIRC | 19 | ||
GN-2002A-Q-44 | Davies | UK | The lifecycle of cluster galaxies: GMOS age-dating of K-band selected samples at z=0.4-0.6 | GMOS | 40 | data sent | 19Aug02 |
GN-2002A-Q-45 | Figueredo | BR | The Stellar Content of the Giant HII Region W51 | NIRI | 4.12 | data sent | 12Aug02 |
GN-2002A-Q-46 | Garnavich | US | SN~Ia: The Collision of Theory and Observation | NIRI | 9 | ||
GN-2002A-Q-47 | Garnavich | US | SN~Ia: The Collision of Theory and Observation | NIRI | 9 | ||
GN-2002A-Q-48 | Gebhardt | US | Black Holes in Brightest Cluster Galaxies | NIRI | 20 | ||
GN-2002A-Q-49 | Hodapp | UH | A Search for Planetary-Mass Young Objects in the Serpens SVS2 Cluster | NIRI | 20 | ||
GN-2002A-Q-50 | Idiart | BR | The enigma of Terzan 1 globular cluster | GMOS | 3.4 | done | 19Aug02 |
GN-2002A-Q-51 | Maria Victoria | AR | The star formation history of the galactic bulge | Hokupa'a + QUIRC | 4.5 | ||
GN-2002A-Q-52 | Martin | CA | The Chemistry of the Extreme Outer Disks of Nearby Spiral Galaxies [joint proposal with Q-87] | GMOS | 6 | data sent | 24May02 |
GN-2002A-Q-53 | Mendes de Oliveira | BR | Multi-object Spectroscopy of Tidal Dwarfs in the Stephan's Quintet | GMOS | 2.58 | done | 19Aug02 |
GN-2002A-Q-54 | Merline | US | Search for Asteroidal Satellites using Adaptive Optics | Hokupa'a + QUIRC | 20 | data sent | 26Jun02 |
GN-2002A-Q-55 | Mirabel | AR | Are the hosts of Gamma-Ray Bursts luminous starbursts or normal galaxies? | NIRI | 3.6 | ||
GN-2002A-Q-56 | Noll | US | 3-4um Spectra of L and T Dwarfs | NIRI | 10 | ||
GN-2002A-Q-57 | Poole | CA | Spectroscopic Confirmation of z=4.4 Galaxies | GMOS | 8 | data sent | 10Apr02 |
GN-2002A-Q-58 | Rhoads | US | A Census of z > 4 Galaxies | GMOS | 20 | data sent | 24May02 |
GN-2002A-Q-59 | Robertson | AU | What are the Damped Lyman Alpha 'protogalaxies'? | GMOS | 4.55 | ||
GN-2002A-Q-60 | Sawicki | CA | At the Epoch of Reionization | GMOS | 8 | ||
GN-2002A-Q-61 | Sodre | BR | Near Infra-Red Imaging of Tidal Dwarf Galaxy Candidates in Stephan's Quintet | NIRI | 1 | ||
GN Scientific Ranking Band 4 | |||||||
Ref # | PI | Partner | Title | Instrument | Hours | Status | Updated |
GN-2002A-Q-62 | Aussel | UH | Characterization of the sources contributing to the cosmic infrared background | GMOS | 10 | data sent | 10Apr02 |
GN-2002A-Q-63 | Balogh | UK | The Galaxy Group Environment at z=1 | GMOS | 17 | ||
GN-2002A-Q-64 | Beasley | AU | Multi-Object Spectroscopy of the GC Systems of Luminous Ellipticals [joint proposal with Q-13, Q-21, Q-29] | GMOS | 2.4 | data sent | 9Aug02 |
GN-2002A-Q-65 | Blundell | UK | What triggers radio galaxies? | GMOS | 2.5 | done | 20May02 |
GN-2002A-Q-66 | Bower | UK | The Enigma of "E+A" galaxies | GMOS | 7 | ||
GN-2002A-Q-67 | Couch | AU | DORIS: A Deep Redshift Survey with Gemini North [joint proposal with Q-68] | GMOS | 8 | ||
GN-2002A-Q-68 | Crampton | CA | DORIS: A Deep Redshift Survey with Gemini North [joint proposal with Q-67] | GMOS | 8 | ||
GN-2002A-Q-69 | Davidge | CA | Comparing the Stellar and Gas Phase Metallicities in Nearby Dwarf Irregular Galaxies | NIRI | 8 | ||
GN-2002A-Q-70 | Donahue | US | Harvesting the High Redshift Cluster Candidates from the ROX Survey | NIRI | 10 | ||
GN-2002A-Q-71 | Ebeling | UH | A multi-wavelength study of the two most massive galaxy clusters known at z~1 | GMOS | 10 | data sent | 24May02 |
GN-2002A-Q-72 | Ferrarese | US | Understanding Supermassive Black Holes and Their Host Galaxies | GMOS | 20 | ||
GN-2002A-Q-73 | Garnavich | US | SNIa: The Collision of Theory and Observation | NIRI | 9 | ||
GN-2002A-Q-74 | Gomez | AR | The VLA 1623 Molecular Hydrogen Outflow: Tracing the Impact Zone of a High Velocity Stellar Flow | NIRI | 1 | ||
GN-2002A-Q-75 | Hook | UK | Probing the high redshift Universe via quasars with z>5 [joint proposal with Q-9] | GMOS | 6.5 | done | 19Aug02 |
GN-2002A-Q-76 | Hutchings | CA | The galaxy environment of z=2 QSOs | GMOS | 3 | data sent | 10Apr02 |
GN-2002A-Q-77 | Jayawardhana | US | Direct Detection of Giant Planets Around the Nearest Young Stars | Hokupa'a + QUIRC | 20 | ||
GN-2002A-Q-78 | Jensen | GS | Using IR Surface Brightness Fluctuations to Measure the Star Formation History of Galaxies in the Coma Cluster | NIRI | 10 | ||
GN-2002A-Q-79 | Malhotra | US | Confirming and Characterizing Young Lyman(alpha) Galaxies at z=4.5 | NIRI | 4 | ||
GN-2002A-Q-80 | Malhotra | US | Confirming and Characterizing Young Lyman(alpha) Galaxies at z=4.5 | NIRI | 15 | ||
GN-2002A-Q-81 | Maloney | US | Buried AGN in LINER-type Ultraluminous Infrared Galaxies | NIRI | 20 | ||
GN-2002A-Q-82 | McCall | CA | The ABCs of BCDs | NIRI | 12 | ||
GN-2002A-Q-83 | Najita | US | Brown Dwarfs in the NOAO Deep Wide-Field Survey and the Substellar Mass Function | GMOS | 20 | ||
GN-2002A-Q-84 | Peacock | UK | Sub-mm EROs, photometric redshifts, and the cluster gravitational lens A2218 | NIRI | 14 | ||
GN-2002A-Q-85 | Richer | CA | Extremely Red Objects in the Direction of the Globular Cluster M4: A Globular Cluster Deep Field | NIRI | 9.1 | ||
GN-2002A-Q-86 | Roth | GS | Characterizing Galaxies Around Damped Lyman-Alpha QSO Absorbers | GMOS | 6 | data sent | 10Apr02 |
GN-2002A-Q-87 | Roy | GS | The Chemistry of the Extreme Outer Disks of Nearby Spiral Galaxies [joint proposal with Q-52] | GMOS | 7.5 | data sent | 13May02 |
GN-2002A-Q-88 | Takamiya | GS | A galaxy census at z~1 in the GOODS/HDF-N region [joint proposal with Q-26] | GMOS | 10 | data sent | 10Apr02 |
GN-2002A-Q-89 | Jorgensen | GS | A GMOS survey of the Coma cluster | GMOS | 10 | data sent | 13Mar02 |
GN-2002A-Q-90 | Richer | CA | Canadian High School Student Programs | GMOS | 2 | done | 26Jun02 |
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 (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 (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-2002A-Q-1 | Barbuy | BR | Oxygen abundance of the metal-rich bulge globular cluster NGC 6553 | Phoenix | 5.33 | done | 1Jul02 |
GS-2002A-Q-2 | Barrientos | CH | Homogeneity of Cluster Elliptical Galaxies at z~1 | Flamingos-I | 17 | data sent | 28Aug02 |
GS-2002A-Q-3 | Bernath | CA | High Resolution Infrared Spectroscopy of L Dwarfs [joint proposal with Q-16] | Phoenix | 10 | data sent | 1Jul02 |
GS-2002A-Q-4 | Burleigh | UK | Imaging extra-solar planets | Flamingos-I | 30 | data sent | 10Sep02 |
GS-2002A-Q-5 | Halpern | US | Search for Small-Scale Structure in Gamma-ray Burst Afterglows [joint proposal with Q-9] | Acquisition Camera | 7 | ||
GS-2002A-Q-6 | Matthews | CA | Imaging the heart of Centaurus A - the nature of the AGN | T-ReCS | 6.2 | ||
GS-2002A-Q-7 | Mirabel | AR | Are the hosts of Gamma-Ray Bursts luminous starbursts or normal galaxies? | Flamingos-I | 6 | data sent | 20Aug02 |
GS-2002A-Q-8 | Najita | US | The Gas Dissipation Timescale in Protoplanetary Disks | Phoenix | 30 | data sent | 1Jul02 |
GS-2002A-Q-9 | Price | AU | Search for Small-Scale Structure in Gamma-Ray Burst Afterglows [joint proposal with Q-5] | Acquisition Camera | 6 | ||
GS-2002A-Q-10 | Rodgers | GS | Structure of inner disks of young stars from fundamental CO emission | Phoenix | 18.3 | data sent | 1Jul02 |
GS Scientific Ranking Band 2 | |||||||
Ref # | PI | Partner | Title | Instrument | Hours | Status | Updated |
GS-2002A-Q-11 | Balachandran | US | The 16O/17O Ratio in Halo Giants | Phoenix | 13 | data sent | 12Apr02 |
GS-2002A-Q-12 | Bremer | AU | Probing the forming cores of galaxy clusters [joint proposal with Q-23, Q-35] | Flamingos-I | 3.6 | data sent | 4Sep02 |
GS-2002A-Q-13 | Bronfman | CH | The Stellar Density Around Massive Young Stars: A Test of Collisional Models of High Mass Star Formation | Flamingos-I | 9 | data sent | 13Sep02 |
GS-2002A-Q-14 | Davidge | CA | Probing the Halos of Late-type Spiral Galaxies in the Sculptor Group | Flamingos-I | 8.42 | ||
GS-2002A-Q-15 | Fisher | GS | Mid-Infrared Imaging of Disks of Transitional Herbig Ae/Be Stars [joint proposal with Q-20] | T-ReCS | 17 | ||
GS-2002A-Q-16 | Hinkle | US | High Resolution Infrared Spectroscopy of L Dwarfs [joint proposal with Q-3] | Phoenix | 20 | data sent | 1Jul02 |
GS-2002A-Q-17 | Kulesa | US | Direct Measurement of Cold H_2 and CO in the Rho-Ophiuchus Star Forming Region | Phoenix | 20 | ||
GS-2002A-Q-18 | Kwok | CA | Imaging of the Dust Torus in Proto-Planetary Nebulae | T-ReCS | 5.83 | ||
GS-2002A-Q-19 | Tanvir | UK | Quick Response to GRBs: the early burst and the late-time decay | Acquisition Camera | 20 | ||
GS-2002A-Q-20 | Telesco | US | Mid-Infrared Imaging of Disks of Transitional Herbig Ae/Be Stars [joint proposal with Q-15] | T-ReCS | 15 | ||
GS-2002A-Q-21 | Wood | AU | Winds in post-AGB stars: shaping planetary nebulae | Phoenix | 4.8 | data sent | 1Jul02 |
GS Scientific Ranking Band 3 | |||||||
Ref # | PI | Partner | Title | Instrument | Hours | Status | Updated |
GS-2002A-Q-22 | Aspin | GS | Multiplicity and Circumstellar Structure of Deeply Embedded Herbig-Haro Energy Sources | T-ReCS | 10 | ||
GS-2002A-Q-23 | Athreya | CH | Probing the forming cores of galaxy clusters [joint proposal with Q-12, Q-35] | Flamingos-I | 12 | data sent | 19Aug02 |
GS-2002A-Q-24 | Barbosa | BR | Massive YSOs in W31 | T-ReCS | 4.98 | ||
GS-2002A-Q-25 | Brittain | US | Circumstellar H_2 and H3+ Line Emission in HD 141569 | Phoenix | 20 | ||
GS-2002A-Q-26 | Burton | AU | Towards an Evolutionary Sequence for Massive Star Formation | T-ReCS | 7 | ||
GS-2002A-Q-27 | Davidge | CA | The Star-Forming History of Isolated Dwarf Spheroidal Galaxies | Flamingos-I | 13 | data sent | 20Aug02 |
GS-2002A-Q-28 | De Buizer | US | Mid-Infrared Imaging of the G29.96-0.02 Hot Core | T-ReCS | 5 | ||
GS-2002A-Q-29 | De Buizer | US | High-Resolution Imaging of Circumstellar Disks in Massive Star Forming Regions using T-ReCS | T-ReCS | 30 | ||
GS-2002A-Q-30 | Feldman | CA | Mid-Infrared Observations of Bright SCUBA Sources in MSX Infrared-Dark Clouds | T-ReCS | 5.1 | ||
GS-2002A-Q-31 | Gledhill | UK | A mid-IR imaging survey of proto-planetary nebulae | T-ReCS | 18 | ||
GS-2002A-Q-32 | Gomez | AR | Young Brown Dwarfs: Exploring the Formation Process and Physical Properties | Flamingos-I | 3 | ||
GS-2002A-Q-33 | Mallen-Ornelas | CH | Number Counts of Extremely Red Galaxies to Extremely Faint Magnitudes | Flamingos-I | 5.5 | data sent | 10Sep02 |
GS-2002A-Q-34 | Morrell | AR | G353.2+0.9: A laboratory for theories of star formation. | Flamingos-I | 1.2 | data sent | 4Sep02 |
GS Scientific Ranking Band 4 | |||||||
Ref # | PI | Partner | Title | Instrument | Hours | Status | Updated |
GS-2002A-Q-35 | Bremer | UK | Probing the forming cores of galaxy clusters [joint proposal with Q-12, Q-23] | Flamingos-I | 16 | data sent | 19Aug02 |
GS-2002A-Q-36 | Casassus | CH | Isotopic ratios and physical conditions from the hyperfine structure and broadening of IR coronal lines in PN NGC6302 | Phoenix | 12 | ||
GS-2002A-Q-37 | Croom | UK | Post-starburst QSOs: spatially resolving the missing link. | Flamingos-I | 13 | ||
GS-2002A-Q-38 | Hynes | UK | Reverberation Mapping of Black Hole X-ray Transients | Acquisition Camera | 12 | ||
GS-2002A-Q-39 | Kalirai | CA | White Dwarf Seismology in M4 | Acquisition Camera | 2.25 | data sent | 12Apr02 |
GS-2002A-Q-40 | Kwok | CA | Mid-infrared Imaging of Southern Bipolar Reflection Nebulae | T-ReCS | 5 | ||
GS-2002A-Q-41 | Luhman | US | Searching for the Bottom of the Initial Mass Function | Flamingos-I | 24 | ||
GS-2002A-Q-42 | Moffat | CA | Survey of the Circumstellar Environments of Prolific Wolf-Rayet Dust Makers with T-ReCS Survey of the Circumstellar Environments of Prolific Wolf-Rayet Dust Makers with T-ReCS | T-ReCS | 4 | ||
GS-2002A-Q-43 | Plante | CA | Hidden Star-Formation in Low-Metallicity Galaxies | T-ReCS | 5 | ||
GS-2002A-Q-44 | Ryde | US | A CO Resonance Scattering Map of alpha Ori's Circumstellar Shell | Phoenix | 10 | ||
GS-2002A-Q-45 | Simon | US | IR Detection of Low-Mass Secondaries in PMS Spectroscopic Binaries | Phoenix | 10 | data sent | 12Apr02 |
GS-2002A-Q-46 | Simon | US | IR Detection of Low-Mass Secondaries in PMS Spectroscopic Binaries | Phoenix | 10 | ||
GS-2002A-Q-47 | Stallard | UK | Detection and Measurement of Ions Winds on Uranus | Phoenix | 12 | ||
GS-2002A-Q-48 | Volk | CA | Mapping the Dust and UIR emisison in Planetary Nebulae | T-ReCS | 5 | ||
GS-2002A-Q-49 | Wood | AU | Nucleosynthesis in Massive AGB Stars | Phoenix | 4.07 | data sent | 12Apr02 |
GS-2002A-Q-50 | Woodward | US | TRECS Imagery of Circumstellar Disks: Herbig Ae Stars | T-ReCS | 20 |
Last update September 12, 2002; Phil Puxley