TMT NSCU: The facility science calibration system for the adaptive optics and infrared instruments of the Thirty Meter Telescope (PI: Dae-Sik Moon; Expected first light whenever TMT is built.) |
WIFIS (Wide Integral-Field Infrared Spectrograph): A near-infared integral-field spectrograph with 6" x 12" field on a 10-m telescope (or 15" x 30" on a 4-m telescope) and R = 5000 spectral resolving power. The (potential) host telescopes include Palomar 5-m, IRTF 3-m and 10.4-m Gran Telescopio Canarias (in collaboration with the University of Florida). (PI: Dae-Sik Moon; Expected first light in 2012.) |
NIRES (Near-Infrared Echelle Spectrograph): The facility near-infrared spectrograph of the 10-m Keck II telescope. (PI: Keith Matthews at Caltech, Co-Is: Dae-Sik Moon and B. Tom Soifer; Almost ready and expected first light in 2011.) |
TripleSpecs: (General, Performance) are the facility near-infrared spectrographs for the 5-m Palomar telescope and 3.5-m Apache Point Observatory telescope. They share the same basic optical design, mechanical design, and electronics with the NIRES of the 10-m Keck I telescope (see above). I was the co-I of the TripleSpecs. |
Automation of the Palomar 1.5-m Telescope: I was the hardware leader of the automation project of the Palomar 1.5-m telescope for observations of optical transients. |
EISSPM: I developed an infrared photon-counting photometer based on the Edge-illuminated Solid-state Photomultiplier. |
Multi-channel Data Acqusition System: I developed the next-generation high-speed multi-channel data acquisition system for infrared and optical photometry. |