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dc.contributor.authorStone, J.M.
dc.contributor.authorSkemer, A.
dc.contributor.authorHinz, P.
dc.contributor.authorErtel, S.
dc.contributor.authorBriesemeister, Z.
dc.contributor.authorLeisenring, J.
dc.contributor.authorDurney, O.
dc.contributor.authorMontoya, M.
dc.contributor.authorWoodward, C.
dc.contributor.authorSkrutskie, M.
dc.contributor.authorBarman, T.
dc.date.accessioned2024-03-22T02:57:05Z
dc.date.available2024-03-22T02:57:05Z
dc.date.issued2022-08-29
dc.identifier.citationJordan 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/10.1117/12.2630308
dc.identifier.isbn978-151065349-8
dc.identifier.issn0277-786X
dc.identifier.doi10.1117/12.2630308
dc.identifier.urihttp://hdl.handle.net/10150/671620
dc.description.abstractThe 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.
dc.language.isoen
dc.publisherSPIE
dc.rights© 2022 SPIE. (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE).
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/
dc.subjectAdaptive Optics
dc.subjectExoplanets
dc.subjectIntegral Field Spectroscopy
dc.subjectThermal-Infrared
dc.titleOn-sky Performance and Results of the Recently Upgraded ALES Integral Field Spectrograph
dc.typeProceedings
dc.typetext
dc.contributor.departmentUniversity of Arizona, Steward Observatory
dc.contributor.departmentUniversity of Arizona, Lunar and Planetary Laboratory
dc.identifier.journalProceedings of SPIE - The International Society for Optical Engineering
dc.description.noteImmediate access
dc.description.collectioninformationThis 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.
dc.eprint.versionFinal Published Version
dc.source.journaltitleProceedings of SPIE - The International Society for Optical Engineering
refterms.dateFOA2024-03-22T02:57:05Z


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