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On-sky Performance and Results of the Recently Upgraded ALES Integral Field Spectrograph
Author
Stone, J.M.Skemer, A.
Hinz, P.
Ertel, S.
Briesemeister, Z.
Leisenring, J.
Durney, O.
Montoya, M.
Woodward, C.
Skrutskie, M.
Barman, T.
Affiliation
University of Arizona, Steward ObservatoryUniversity of Arizona, Lunar and Planetary Laboratory
Issue Date
2022-08-29
Metadata
Show full item recordPublisher
SPIECitation
Jordan M. Stone, Andrew Skemer, Phil Hinz, Steve Ertel, Zackery Briesemeister, Jarron Leisenring, Olivier Durney, Manny Montoya, Charles Woodward, Michael Skrutskie, Travis Barman, "On-sky performance and results of the recently upgraded ALES integral field spectrograph," Proc. SPIE 12184, Ground-based and Airborne Instrumentation for Astronomy IX, 1218442 (29 August 2022); https://doi.org/10.1117/12.2630308Rights
© 2022 SPIE. (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE).Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
The Arizona Lenslets for Exoplanet Spectroscopy (ALES) is an integral field spectrograph implemented with a modular design comprising magnifiers, a lenslet array, and direct-vision prisms all installed in filterwheels within the LBTI/LMIRCam instrument. ALES is unique among high-contrast instruments for providing spatially resolved spectroscopy out to 5 microns. ALES has been operating with an upgraded lenslet array and prism assembly since late 2018. The new lenslet array includes larger lenslets to reduce diffraction losses and spatial crosstalk in the data. The lenslet array is fabricated with a unique sag surface for each lenslet, correcting for rotating off-axis astigmatism in the magnified intermediate focal plane. The result is tighter lenslet spots and better data. The new prism assembly provides increased spectral resolution in the 2.9 to 4.2 micron wavelength range. Here we characterize the performance of upgraded ALES, and report initial results probing the atmospheres of high-contrast companions to nearby stars. A calibration and data pre-processing strategy unique to the upgraded instrument is discussed. We also report laboratory tests of additional future upgrades including prism and blocking filter pairs for added bandpasses and magnification modes to facilitate Fizeau interferometry with LMIRCam and ALES. © 2022 SPIE.Note
Immediate accessISSN
0277-786XISBN
978-151065349-8Version
Final Published Versionae974a485f413a2113503eed53cd6c53
10.1117/12.2630308