A Low-resolution spectrograph for the IOTA interferometer

S. Ragland, W.~A. Traub, R. Millan-Gabet, N.~P. Carleton, E. Pedretti

Research output: Chapter in Book/Report/Conference proceedingConference contribution

5 Citations (Scopus)

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.
Original languageUndefined/Unknown
Title of host publicationInterferometry for Optical Astronomy II
EditorsW.~A. Traub
Pages1225-1233
Number of pages9
Volume4838
DOIs
Publication statusPublished - 24 Feb 2003

Publication series

NameSociety of Photo-Optical Instrumentation Engineers (SPIE) Conference Series

Cite this

Ragland, S., Traub, W. A., Millan-Gabet, R., Carleton, N. P., & Pedretti, E. (2003). A Low-resolution spectrograph for the IOTA interferometer. In W. A. Traub (Ed.), Interferometry for Optical Astronomy II (Vol. 4838, pp. 1225-1233). (Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series). https://doi.org/10.1117/12.459321