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Resource Record Summary

Organization:
W. M. Keck Observatory

Short name: Keck
IVOA Identifier: ivo://KeckObs/KeckObsPublisher: W. M. Keck Observatory, CARA
More Info: http://www.keckobservatory.org/
VO Compliance: Level 2: This is a VO-compliant resource.
Status: active
Registered: 2008 Apr 04 16:43:32Z
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Description


The Keck Observatory's instruments are the twin Keck Telescopes, the world's largest optical and infrared telescopes. Each stands eight stories tall and weighs 300 tons, yet operates with nanometer precision. At the heart of each Keck Telescope is a revolutionary primary mirror. Ten meters in diameter, the mirror is composed of 36 hexagonal segments that work in concert as a single piece of reflective glass.

More About this Resource

About the Resource Providers

This section describes who is responsible for this resource

Publisher: W. M. Keck Observatory, CARA

STScI Archivearchive@stsci.edu

Contact Information:
X Shui Hung Kwok
Email: skwok at keck.hawaii.edu

Status of This Resource

This section provides some status information: the resource version, availability, and relevant dates.

Version: n/a
Availability: This is an active resource.

This resource was registered on: 2008 Apr 04 16:43:32Z
This resource description was last updated on: 2008 Apr 04 16:43:32Z

What This Resource is About

This section describes what the resource is, what it contains, and how it might be relevant.

Resource Class: Organisation
This resource represents an organization, institute, or academic departmentthat provides and/or uses VO data, services, or applications.
Resource type keywords:
  • Organisation
Subject keywords:
  • optical astronomy
  • optical interferometry
Associated observatories/telescopes/instruments:
  • facility: Keck Telescopes
Intended audience or use:
  • General: This resource provides information appropriate for all users.
  • Research: This resource provides information appropriate for supporting scientific research.
More Info: http://www.keckobservatory.org/



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under Cooperative Agreement AST0122449 with the Johns Hopkins University
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