Add to ORKGASTRA (ASTrometric and phase-Referencing Astronomy) is an upgrade to the existing Keck Interferometer which aims at providing new self-phase referencing (high spectral resolution observation of YSOs), dual-field phase referencing (sensitive AGN observations), and astrometric (known exoplanetary systems characterization and galactic center general relativity in strong field regime) capabilities. With the first high spectral resolution mode now offered to the community, this contribution focuses on the progress of the dual field and astrometric modes
A cross-dispersed spectrophotometer with CCD detector and its automated 0.5-m telescope at the Fairb...
We summarize the status of the Keck Interferometer in V^2 mode, and science results recently obtaine...
The Keck Planet Imager and Characterizer (KPIC) is an upgrade to the Keck II adaptive optics system ...
ASTRA (ASTrometric and phase-Referencing Astronomy) is an upgrade to the existing Keck Interferomete...
The ASTrometric and phase-Referenced Astronomy (ASTRA) project will provide phase referencing and as...
ASTRA (ASTrometric and phase-Referencing Astronomy) is an upgrade to the existing Keck Interferomete...
As part of the astrometric and phase-referenced astronomy (ASTRA) project, three new science modes a...
The sensitivity and astrometry upgrade ASTRA of the Keck Interferometer is in-troduced. After a brie...
Recently, the Keck interferometer was upgraded to do self-phase-referencing (SPR) assisted K-band sp...
Ground-based long baseline interferometers have long been limited in sensitivity by the short integr...
The Keck Interferometer combines the two 10m diameter Keck telescopes for near-infrared fringe visib...
The addition of new observational capabilities and continued sensitivity improvements have allowed o...
The Keck Interferometer combines the two 10 m Keck telescopes as a long baseline interferometer, fun...
Keck Interferometer is a NASA-funded project to combine the two 10 m Keck telescopes for high sensit...
The Keck Interferometer (KI) combines the two 10m diameter Keck telescopes providing milliarcsecond ...
A cross-dispersed spectrophotometer with CCD detector and its automated 0.5-m telescope at the Fairb...
We summarize the status of the Keck Interferometer in V^2 mode, and science results recently obtaine...
The Keck Planet Imager and Characterizer (KPIC) is an upgrade to the Keck II adaptive optics system ...
ASTRA (ASTrometric and phase-Referencing Astronomy) is an upgrade to the existing Keck Interferomete...
The ASTrometric and phase-Referenced Astronomy (ASTRA) project will provide phase referencing and as...
ASTRA (ASTrometric and phase-Referencing Astronomy) is an upgrade to the existing Keck Interferomete...
As part of the astrometric and phase-referenced astronomy (ASTRA) project, three new science modes a...
The sensitivity and astrometry upgrade ASTRA of the Keck Interferometer is in-troduced. After a brie...
Recently, the Keck interferometer was upgraded to do self-phase-referencing (SPR) assisted K-band sp...
Ground-based long baseline interferometers have long been limited in sensitivity by the short integr...
The Keck Interferometer combines the two 10m diameter Keck telescopes for near-infrared fringe visib...
The addition of new observational capabilities and continued sensitivity improvements have allowed o...
The Keck Interferometer combines the two 10 m Keck telescopes as a long baseline interferometer, fun...
Keck Interferometer is a NASA-funded project to combine the two 10 m Keck telescopes for high sensit...
The Keck Interferometer (KI) combines the two 10m diameter Keck telescopes providing milliarcsecond ...
A cross-dispersed spectrophotometer with CCD detector and its automated 0.5-m telescope at the Fairb...
We summarize the status of the Keck Interferometer in V^2 mode, and science results recently obtaine...
The Keck Planet Imager and Characterizer (KPIC) is an upgrade to the Keck II adaptive optics system ...