Award Abstract #0079523
Acquisition of a new Infrared Detector for Astronomical Research
![](common/images/greenline.jpg)
NSF Org: |
AST
Division of Astronomical Sciences
|
![divider line](common/images/x.gif) |
![divider line](common/images/x.gif) |
Initial Amendment Date: |
July 14, 2000 |
![divider line](common/images/x.gif) |
Latest Amendment Date: |
July 14, 2000 |
![divider line](common/images/x.gif) |
Award Number: |
0079523 |
![divider line](common/images/x.gif) |
Award Instrument: |
Standard Grant |
![divider line](common/images/x.gif) |
Program Manager: |
Andrew Clegg
AST Division of Astronomical Sciences
MPS Directorate for Mathematical & Physical Sciences
|
![divider line](common/images/x.gif) |
Start Date: |
July 15, 2000 |
![divider line](common/images/x.gif) |
Expires: |
June 30, 2003 (Estimated) |
![divider line](common/images/x.gif) |
Awarded Amount to Date: |
$208174 |
![divider line](common/images/x.gif) |
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](common/images/x.gif) |
Sponsor: |
Dartmouth College
OFFICE OF SPONSORED PROJECTS
HANOVER, NH 03755 603/646-3007
|
![divider line](common/images/x.gif) |
NSF Program(s): |
MAJOR RESEARCH INSTRUMENTATION
|
![divider line](common/images/x.gif) |
Field Application(s): |
|
![divider line](common/images/x.gif) |
Program Reference Code(s): |
OTHR, 0000
|
![divider line](common/images/x.gif) |
Program Element Code(s): |
1189
|
ABSTRACT
![](common/images/bluefade.jpg)
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.
|