ARIES: Arizona infrared imager and echelle spectrograph

Donald W. McCarthy; James H. Burge; James Roger P. Angel; Jian Ge; Roland J. Sarlot; Bruce C. Fitz-Patrick; Joannah L. Hinz

doi:10.1117/12.317340

ARIES: Arizona infrared imager and echelle spectrograph

Donald W. McCarthy, James H. Burge, James Roger P. Angel, Jian Ge, Roland J. Sarlot, Bruce C. Fitz-Patrick, Joannah L. Hinz

Research output: Contribution to journal › Conference article

31 Scopus citations

Abstract

ARIES, a new 1-5 μm camera/spectrograph, is designed to capitalize on the exceptionally low thermal background and high optical throughput offered by the f/15 adaptive secondary system being built for the upgraded 6.5m MMT. With two state-of-the-art IR arrays, ARIES will provide diffraction-limited imaging in the JHKLM atmospheric windows and also echelle, long-slit spectroscopy at resolutions of 2,000 and 30,000. ARIES will also supply global wavefront tip/tilt information to the adaptive system using cryogenic pick-off mirrors to access field stars over a 50 arcsec diameter field at wavelengths from 1-2 μm.

Original language	English (US)
Pages (from-to)	750-754
Number of pages	5
Journal	Proceedings of SPIE - The International Society for Optical Engineering
Volume	3354
DOIs	https://doi.org/10.1117/12.317340
State	Published - Dec 1 1998
Event	Infrared Astronomical Instrumentation - Kona, HI, United States Duration: Mar 23 1998 → Mar 23 1998

Keywords

Adaptive optics
High resolution imaging
Infrared
Spectroscopy

ASJC Scopus subject areas

Electronic, Optical and Magnetic Materials
Condensed Matter Physics
Computer Science Applications
Applied Mathematics
Electrical and Electronic Engineering

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McCarthy, D. W., Burge, J. H., Angel, J. R. P., Ge, J., Sarlot, R. J., Fitz-Patrick, B. C., & Hinz, J. L. (1998). ARIES: Arizona infrared imager and echelle spectrograph. Proceedings of SPIE - The International Society for Optical Engineering, 3354, 750-754. https://doi.org/10.1117/12.317340

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title = "ARIES: Arizona infrared imager and echelle spectrograph",

abstract = "ARIES, a new 1-5 μm camera/spectrograph, is designed to capitalize on the exceptionally low thermal background and high optical throughput offered by the f/15 adaptive secondary system being built for the upgraded 6.5m MMT. With two state-of-the-art IR arrays, ARIES will provide diffraction-limited imaging in the JHKLM atmospheric windows and also echelle, long-slit spectroscopy at resolutions of 2,000 and 30,000. ARIES will also supply global wavefront tip/tilt information to the adaptive system using cryogenic pick-off mirrors to access field stars over a 50 arcsec diameter field at wavelengths from 1-2 μm.",

keywords = "Adaptive optics, High resolution imaging, Infrared, Spectroscopy",

author = "McCarthy, {Donald W.} and Burge, {James H.} and Angel, {James Roger P.} and Jian Ge and Sarlot, {Roland J.} and Fitz-Patrick, {Bruce C.} and Hinz, {Joannah L.}",

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doi = "10.1117/12.317340",

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journal = "Proceedings of SPIE - The International Society for Optical Engineering",

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note = "Infrared Astronomical Instrumentation ; Conference date: 23-03-1998 Through 23-03-1998",

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TY - JOUR

T1 - ARIES

T2 - Infrared Astronomical Instrumentation

AU - McCarthy, Donald W.

AU - Burge, James H.

AU - Angel, James Roger P.

AU - Ge, Jian

AU - Sarlot, Roland J.

AU - Fitz-Patrick, Bruce C.

AU - Hinz, Joannah L.

PY - 1998/12/1

Y1 - 1998/12/1

N2 - ARIES, a new 1-5 μm camera/spectrograph, is designed to capitalize on the exceptionally low thermal background and high optical throughput offered by the f/15 adaptive secondary system being built for the upgraded 6.5m MMT. With two state-of-the-art IR arrays, ARIES will provide diffraction-limited imaging in the JHKLM atmospheric windows and also echelle, long-slit spectroscopy at resolutions of 2,000 and 30,000. ARIES will also supply global wavefront tip/tilt information to the adaptive system using cryogenic pick-off mirrors to access field stars over a 50 arcsec diameter field at wavelengths from 1-2 μm.

AB - ARIES, a new 1-5 μm camera/spectrograph, is designed to capitalize on the exceptionally low thermal background and high optical throughput offered by the f/15 adaptive secondary system being built for the upgraded 6.5m MMT. With two state-of-the-art IR arrays, ARIES will provide diffraction-limited imaging in the JHKLM atmospheric windows and also echelle, long-slit spectroscopy at resolutions of 2,000 and 30,000. ARIES will also supply global wavefront tip/tilt information to the adaptive system using cryogenic pick-off mirrors to access field stars over a 50 arcsec diameter field at wavelengths from 1-2 μm.

KW - Adaptive optics

KW - High resolution imaging

KW - Infrared

KW - Spectroscopy

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JO - Proceedings of SPIE - The International Society for Optical Engineering

JF - Proceedings of SPIE - The International Society for Optical Engineering

SN - 0277-786X

Y2 - 23 March 1998 through 23 March 1998

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