text-only page produced automatically by LIFT Text Transcoder Skip all navigation and go to page contentSkip top navigation and go to directorate navigationSkip top navigation and go to page navigation
National Science Foundation
Search  
Awards
design element
Search Awards
Recent Awards
Presidential and Honorary Awards
About Awards
Grant Policy Manual
Grant General Conditions
Cooperative Agreement Conditions
Special Conditions
Federal Demonstration Partnership
Policy Office Website


Award Abstract #0079523
Acquisition of a new Infrared Detector for Astronomical Research


NSF Org: AST
Division of Astronomical Sciences
divider line
divider line
Initial Amendment Date: July 14, 2000
divider line
Latest Amendment Date: July 14, 2000
divider line
Award Number: 0079523
divider line
Award Instrument: Standard Grant
divider line
Program Manager: Andrew Clegg
AST Division of Astronomical Sciences
MPS Directorate for Mathematical & Physical Sciences
divider line
Start Date: July 15, 2000
divider line
Expires: June 30, 2003 (Estimated)
divider line
Awarded Amount to Date: $208174
divider line
Investigator(s): Gary Wegner gaw@bellz.dartmouth.edu (Principal Investigator)
Robert Fesen (Co-Principal Investigator)
John Thorstensen (Co-Principal Investigator)
Brian Chaboyer (Co-Principal Investigator)
divider line
Sponsor: Dartmouth College
OFFICE OF SPONSORED PROJECTS
HANOVER, NH 03755 603/646-3007
divider line
NSF Program(s): MAJOR RESEARCH INSTRUMENTATION
divider line
Field Application(s):
divider line
Program Reference Code(s): OTHR, 0000
divider line
Program Element Code(s): 1189

ABSTRACT

Wegner

MRI0079523

Abstract

An upgrade of the infrared detector for the Ohio State University-NOAO infrared imaging spectrometer (ONIS) at the 2.4-meter telescope at Kitt Peak National Observatory will be implemented. This has been a very productive instrument for astronomical research. The MDM Consortium, Inc operates the telescope, which is a consortium of Dartmouth College (1/3) and Ohio State University, Columbia University and the University of Michigan. In addition to doubling the field of view and wavelength coverage of the instrument, this upgrade eliminates serious cosmetic effect errors in the current system that causes calibration errors. The current detector will be replaced by an improved 1024x1024 pixel large format Raytheon InSb focal plane for use in the 1 to 3 micrometer wavelength region.

The scientific research areas planned are wide-field surveys for extremely red objects (ERO's), infrared studies of globular cluster ages and infrared studies of supernovae.

***

 

Please report errors in award information by writing to: awardsearch@nsf.gov.

 

 

Print this page
Back to Top of page
  Web Policies and Important Links | Privacy | FOIA | Help | Contact NSF | Contact Web Master | SiteMap  
National Science Foundation
The National Science Foundation, 4201 Wilson Boulevard, Arlington, Virginia 22230, USA
Tel: (703) 292-5111, FIRS: (800) 877-8339 | TDD: (800) 281-8749
Last Updated:
April 2, 2007
Text Only


Last Updated:April 2, 2007