Published February 21, 2003
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Low-resolution spectrograph for the IOTA interferometer
- Other:
- Traub, Wesley A.
Abstract
The design and scientific objectives of a near infrared channeled spectrometer planned at the IOTA interferometer are discussed. The spectrometer has the flexibility to reconfigure easily for conventional broadband operations in addition to multi-channel mode. This instrument makes use of the existing PICNIC camera at the IOTA in order to be cost efficient. The spectrometer has been designed specifically for studying Mira stars. However, it will find its application in other areas of astrophysical interests such as studies of circumstellar disks around young stars and binary stars.
Additional Information
© 2003 Society of Photo-optical Instrumentation Engineers (SPIE). This work was performed in part under contract with the Jet Propulsion Laboratory (JPL) through the Michelson Fellowship program funded by NASA as an element of the planet finder program. JPL is managed for NASA by the California Institute of Technology.Attached Files
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Additional details
- Eprint ID
- 90847
- Resolver ID
- CaltechAUTHORS:20181112-113919758
- NASA/JPL/Caltech
- NASA Michelson Fellowship
- Created
-
2018-11-13Created from EPrint's datestamp field
- Updated
-
2021-11-16Created from EPrint's last_modified field
- Series Name
- Proceedings of SPIE
- Series Volume or Issue Number
- 4838