A Low-resolution spectrograph for the IOTA interferometer

Sam Ragland; Wesley A. Traub; Rafael Millan-Gabet; Nathaniel P. Carleton; Ettore Pedretti

A Low-resolution spectrograph for the IOTA interferometer

Sam Ragland
, Wesley A. Traub
, Rafael Millan-Gabet
, Nathaniel P. Carleton
, Ettore Pedretti

SAMS UHI

科研成果: Article › 同行评审

摘要

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.

源语言	English
页（从-至）	1225-1233
期刊	Interferometry for Optical Astronomy II
卷	4838
出版状态	Published - 1 2月 2003

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http://adsabs.harvard.edu/abs/2003SPIE.4838.1225R

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title = "A Low-resolution spectrograph for the IOTA interferometer",

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.",

author = "Sam Ragland and Traub, \{Wesley A.\} and Rafael Millan-Gabet and Carleton, \{Nathaniel P.\} and Ettore Pedretti",

year = "2003",

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T1 - A Low-resolution spectrograph for the IOTA interferometer

AU - Ragland, Sam

AU - Traub, Wesley A.

AU - Millan-Gabet, Rafael

AU - Carleton, Nathaniel P.

AU - Pedretti, Ettore

PY - 2003/2/1

Y1 - 2003/2/1

N2 - 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.

AB - 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.

M3 - Article

VL - 4838

SP - 1225

EP - 1233

JO - Interferometry for Optical Astronomy II

JF - Interferometry for Optical Astronomy II

ER -

A Low-resolution spectrograph for the IOTA interferometer

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