Approved Programs
16 projects in 2005
Project Status [Authentication required]
|
ID |
PI |
Obs Type |
Instrument |
Title |
Time Allocated |
Time Observed |
05AT01 |
Lin, Li-Hwai |
QSO |
MegaCam |
MegaCam i and z survey of DEEP2 fields |
10.0 hours |
10.0 hours |
05AT02 |
Kawasaki, Wataru |
QSO |
MegaCam |
Dwarf galaxies in the Hercules cluster |
2.0 hours |
2.0 hours |
05AT04 |
Lim, Jeremy |
Classical |
CFHTIR |
Combined Near-IR Stellar and Atomic Hydrogen (HI) Gas Imagining of QSO Host Galaxies |
1.0 night |
|
05AT05 |
Kwok, Sun |
Classical |
CFHTIR |
Imaging of Planetary Nebulae at Molecular Hydrogen Emission |
1.0 night |
|
05AT06 |
Chiueh, Tzi-Hong |
QSO |
MegaCam |
Galaxy Clusters as a Dark Energy Probe |
10.0 hours |
4.2 hours |
05AT07 |
Lyo, A-Ran |
Classical |
CFHTIR |
Low-mass population studies in the Ursa Major Group and the Coma Berenices |
1.0 night |
|
05BT01 |
Chiueh, Tzi-Hong |
QSO |
MegaCam |
Galaxy Clusters as a Dark Energy Probe |
20.0 hours |
20.0 hours |
05BT02 |
Phan, Bao-Ngoc |
Classical |
EsPADOnS |
High resolution spectropolarimetric observation of nearby ultracool and brown dwarfs |
1.0 night |
1.0 night |
05BT03 |
Lyo, A-Ran |
QSO |
MegaCam |
Search for a nearby young cluster in the Northern Hemisphere (WIRCam) |
1.3 hours |
1.3 hours |
05BT04 |
Lyo, A-Ran |
QSO |
WIRCam |
Search for a nearby young cluster in the Northern Hemisphere (WIRCam) |
2.7 hours |
1.8 hours |
05BT05 |
Su, Yu-Nung |
QSO |
MegaCam |
Outflows from Luminous Young Stellar Objects II |
4.5 hours |
4.5 hours |
05BT06 |
Su, Yu-Nung |
QSO |
WIRCam |
Outflows from Luminous Young Stellar Objects I |
2.0 hours |
2.0 hours |
05BT07 |
Chen, Huei-Ru |
QSO |
WIRCam |
Searching Embedded Stellar Content in a High Density Layer with Triggered Star Formation |
4.7 hours |
1.0 hour |
05BT08 |
Lim, Jeremy |
QSO |
WIRCam |
First Maps of Nearby Galaxies in Molecular Hydrogen Gas |
15.9 hours |
3.3 hours |
05BT09 |
Huang, Li-Jin |
QSO |
MegaCam |
What is the nature of the X-ray Flashes ? |
0.0 hour |
0.0 hour |
05BT10 |
Dinh, Van-Trung |
Classical |
MegaCam |
High resolution spectro-polarimetry of post-AGB stars |
1.0 night |
|
Acknowledgement of Publications with CFHT Data
Publications based on data taken with and through Taiwan's access to
the CFHT from Jan 1 2011 should contain the following acknowledgement:
Access to the CFHT was made possible by the Institute of Astronomy and
Astrophysics, Academia Sinica.