The Keck Planet Finder (KPF) is a fiber-fed, high-resolution, high-stability spectrometer in development at the UC Berkeley Space Sciences Laboratory for the W.M. Keck Observatory. KPF is designed to characterize exoplanets via Doppler spectroscopy with a goal of a single measurement precision of 0.3 m s-1 or better, however its resolution and stability will enable a wide variety of astrophysical pursuits. Here we provide post-preliminary design review design updates for several subsystems, including: the main spectrometer, the fabrication of the Zerodur optical bench; the data reduction pipeline; fiber agitator; fiber cable design; fiber scrambler; VPH testing results and the exposure meter
We present the design and test results of a double-scrambler and fiber agitator system for the Keck ...
The Keck Cosmic Web Imager (KCWI) is a new facility instrument being developed for the W. M. Keck Ob...
The recent site testing pointed out the potential of Dome C for Next Generation Optical Interferomet...
The Keck Planet Finder (KPF) is a fiber-fed, high-resolution, high-stability spectrometer in develop...
KPF is a fiber-fed, high-resolution, high-stability spectrometer in development at the UC Berkeley S...
The Keck Planet Finder (KPF) is a fiber-fed, high-resolution, high-stability spectrometer in develop...
The Keck Planet Imager and Characterizer (KPIC) is an upgrade to the Keck II adaptive optics system ...
Here we report on the status of the The Keck Planet Imager and Characterizer (KPIC), which is an on-...
Coupling a high-contrast imaging instrument to a high-resolution spectrograph has the potential to e...
Coupling a high-contrast imaging instrument to a high-resolution spectrograph has the potential to e...
The Keck Planet Imager and Characterizer (KPIC) is an upgrade to the Keck II adaptive optics system ...
The Keck Planet Imager and Characterizer (KPIC) is a cost-effective upgrade path to the W.M. Keck ob...
The Keck Planet Imager and Characterizer (KPIC) is a cost-effective upgrade path to the W.M. Keck ob...
The Keck Planet Imager and Characterizer (KPIC) is a purpose-built instrument to demonstrate new tec...
The Keck Planet Imager and Characterizer comprises of a series of upgrades to the Keck II adaptive o...
We present the design and test results of a double-scrambler and fiber agitator system for the Keck ...
The Keck Cosmic Web Imager (KCWI) is a new facility instrument being developed for the W. M. Keck Ob...
The recent site testing pointed out the potential of Dome C for Next Generation Optical Interferomet...
The Keck Planet Finder (KPF) is a fiber-fed, high-resolution, high-stability spectrometer in develop...
KPF is a fiber-fed, high-resolution, high-stability spectrometer in development at the UC Berkeley S...
The Keck Planet Finder (KPF) is a fiber-fed, high-resolution, high-stability spectrometer in develop...
The Keck Planet Imager and Characterizer (KPIC) is an upgrade to the Keck II adaptive optics system ...
Here we report on the status of the The Keck Planet Imager and Characterizer (KPIC), which is an on-...
Coupling a high-contrast imaging instrument to a high-resolution spectrograph has the potential to e...
Coupling a high-contrast imaging instrument to a high-resolution spectrograph has the potential to e...
The Keck Planet Imager and Characterizer (KPIC) is an upgrade to the Keck II adaptive optics system ...
The Keck Planet Imager and Characterizer (KPIC) is a cost-effective upgrade path to the W.M. Keck ob...
The Keck Planet Imager and Characterizer (KPIC) is a cost-effective upgrade path to the W.M. Keck ob...
The Keck Planet Imager and Characterizer (KPIC) is a purpose-built instrument to demonstrate new tec...
The Keck Planet Imager and Characterizer comprises of a series of upgrades to the Keck II adaptive o...
We present the design and test results of a double-scrambler and fiber agitator system for the Keck ...
The Keck Cosmic Web Imager (KCWI) is a new facility instrument being developed for the W. M. Keck Ob...
The recent site testing pointed out the potential of Dome C for Next Generation Optical Interferomet...