| RUNID | PI name | Prg Type | I-time (hrs) |
Grade | Title |
| 10AC10 | Puzia | Regular | 23 | A | The
Next Generation Virgo Survey -- Infrared: Ks-Band Observations of the
Central 4 deg square |
| 10AC30 | Croll | Regular | 25 | B | Multi-wavelength
near-infrared thermal emission from the hottest of the hot
Jupiters |
| 10AC98 | Yee | Regular | 22 | B | Galaxy
Evolution in Rich Clusters at z > 1 |
| 10AC34 | Webb | Regular | 16.1 | C
| Understanding Galaxy Evolution in Dense Cluster Environments |
| 10AF05 | Lehnert | Regular | 21 | A | Massive
Galaxies at High Redshift: Deep H-band Imaging of the SERVS
fields |
| 10AO02 | Hopwood | Regular | 1.4 | B | Deep
JHKs-band imaging of the gravitational lensing cluster Abell
2218 |
| 10AF03 | Lancon | Regular | 23 | B | The
Next Generation Virgo Survey -- Infrared: Ks-Band Observations of the
Central 4 deg square |
| 10AF12 | Forveille | Regular | 15 | B | Searching
for ultracool brown dwarfs - a WIRCam extension to the Canada-France Brown Dwarfs Survey |
| 10AF15 | Nesvadba | Regular | 15 | B | Two
birds with one stone: Identifying two galaxy overdensities surrounding
two submillimeter galaxies at z~2.3 with one observation |
| 10AF14 | Soucail | Regular | 17 | C
| Probing the dark matter distribution and the mass-to-light
ratio of galaxy groups with the CFHTLS Strong Lensing Legacy Survey
(SL2S) |
| 10AT04 | Lin | Regular | 12 | A | WIRCAM Imaging in Extended GOODS-N: Searching for the Most Luminous Galaxies at z > 7 |
| 10AT03 | Wang | Regular | 5 | B | Deep J-Band Imaging of the Strong Lensing Cluster A2390 |
| 10AT19 | Hsieh | Regular | 4.5 | B |
|
| 10AT07 | Chiang | Snapshot | 1 | S | Identication of T Dwarfs with Methane Imaging |
| 10AH31 | Dupuy | Regular | 13.8 | A | Dynamical masses of brown dwarfs and low mass stars |
| 10AH33 | Liu | Regular | 20 | A | |
| 10AH10 | Goto | Regular | 24 | B | CFHT/WIRCam imaging of the AKARI NEP deep field |
| 10AH23 | Cowie | Regular | 20 | B | Searching for Z>>4 ultraluminous dusty galaxies |
| 10AH99 | Liu | Regular | 7.4 | B | |