Interferometry Science Center
leftnav_space1
Palmar Testbed KECK Interferometer
KECK Interferometer
Space Interferometry Mission
Terrestrial Planet Finder
Other
leftnav_space2
Support Services
Events
Science by NExScI Personnel
NASA
Caltech
Caltech
 
Last Updated: 
  27 May 2005
spacer

On July 4 (UT), the Deep Impact spacecraft intercepted comet Tempel 1. Director's time at the W. M. Keck Observatory was allocated in order to observe the comet with the High Resolution Echelle Spectrograph (HIRES) on Keck 1, as well as the Near Infrared Spectrometer (NIRSPEC) on Keck 2.

These data comprise the first public release of data from the Keck Observatory Archive (KOA), which will begin publicly serving non-proprietary HIRES data in February 2006.

The data are also available from the W. M. Keck Observatory's Deep Impact Observations site.

For help downloading HIRES and NIRSPEC Deep Impact observations, please see the download user's guide, or contact the KOA Helpdesk.

HIRES Data NIRSPEC Data Weather Data

HIRES Data:
User-selected Download Packaging:
HIRES Level 0 (uncalibrated) FITS data, as well as JPEG "Quicklook" images, are available for browsing and user-selected download packaging:
Pre-packaged TAR Files:
HIRES data are also available for bulk download as gzipped TAR files, including text logs and guide images:

July 4, 2005 (UT) - impact observations

May 30, 2005 (UT) - pre-impact observations


NIRSPEC Data:

The NIRSPEC data from observation of the impact are available as a gzipped TAR file:

July 4, 2005 (UT) - impact observations:


Weather Data:

Weather data includes archived CONCAM webpages and images (when available), as well as WMKO-generated weather plots:

The Keck Observatory Archive has been made possible by funding provided by the National Aeronautics and Space Administration to Caltech and the W. M. Keck Observatory. The W. M. Keck Observatory Director Fred Chaffee is thanked for donating his director's time for the HIRES observations of Tempel 1 and for providing the data to the public. Thanks also to Dr. Mike Bolte for making part of his observing time available for the pre-impact observations.

Please contact koaadmin@ipac.caltech.edu with questions or problems.