The Keck Interferometer (KI) combines the two 10m diameter Keck telescopes providing milliarcsecond angular resolution. KI has unique observing capabilities such as sensitive K-band V^2, L-band V^2 and N-band nulling modes. The instrument improvements and status of the Keck Interferometer since the 2010 SPIE meeting are summarized. We discuss the current capabilities of the KI, operational improvements, and the science from the KI during the past two years. We will conclude with a brief note on the closure of the KI facility. Details of dual field phase referencing developments and nulling science results are presented elsewhere at this conference
In this paper we describe both recently completed instrumentation projects and our current developme...
The visibility science mode of the Keck Interferometer fully transitioned into operations with the s...
The W. M. Keck Observatory continues to develop new capabilities in support of our science driven st...
The Keck Interferometer (KI) combines the two 10m diameter Keck telescopes providing milliarcsecond ...
The Keck Interferometer combines the two 10m diameter Keck telescopes for near-infrared fringe visib...
We summarize the status of the Keck Interferometer in V^2 mode, and science results recently obtaine...
The Keck Interferometer combines the two 10 m Keck telescopes as a long baseline interferometer, fun...
The addition of new observational capabilities and continued sensitivity improvements have allowed o...
Keck Interferometer is a NASA-funded project to combine the two 10 m Keck telescopes for high sensit...
The Keck Interferometer (KI) combined the two 10 m W. M. Keck Observatory telescopes on Mauna Kea, H...
The Keck Interferometer is a NASA funded project developed by the Jet Propulsion Laboratory, the Wil...
The nulling mode of the Keck Interferometer is being commissioned at the Mauna Kea summit. The nulle...
The Keck Interferometer is entering a regular limited observational phase. A restricted number of ob...
The Keck Interferometer Nuller (KIN) is one of the major scientific and technical precursors to the ...
The Keck Interferometer combines the two 10 m Keck telescopes as a long baseline interferometer. It ...
In this paper we describe both recently completed instrumentation projects and our current developme...
The visibility science mode of the Keck Interferometer fully transitioned into operations with the s...
The W. M. Keck Observatory continues to develop new capabilities in support of our science driven st...
The Keck Interferometer (KI) combines the two 10m diameter Keck telescopes providing milliarcsecond ...
The Keck Interferometer combines the two 10m diameter Keck telescopes for near-infrared fringe visib...
We summarize the status of the Keck Interferometer in V^2 mode, and science results recently obtaine...
The Keck Interferometer combines the two 10 m Keck telescopes as a long baseline interferometer, fun...
The addition of new observational capabilities and continued sensitivity improvements have allowed o...
Keck Interferometer is a NASA-funded project to combine the two 10 m Keck telescopes for high sensit...
The Keck Interferometer (KI) combined the two 10 m W. M. Keck Observatory telescopes on Mauna Kea, H...
The Keck Interferometer is a NASA funded project developed by the Jet Propulsion Laboratory, the Wil...
The nulling mode of the Keck Interferometer is being commissioned at the Mauna Kea summit. The nulle...
The Keck Interferometer is entering a regular limited observational phase. A restricted number of ob...
The Keck Interferometer Nuller (KIN) is one of the major scientific and technical precursors to the ...
The Keck Interferometer combines the two 10 m Keck telescopes as a long baseline interferometer. It ...
In this paper we describe both recently completed instrumentation projects and our current developme...
The visibility science mode of the Keck Interferometer fully transitioned into operations with the s...
The W. M. Keck Observatory continues to develop new capabilities in support of our science driven st...