Design and testing of a low-resolution NIR spectrograph for the EXoplanet Climate Infrared TElescope

dc.contributor.authorBernard, Lee
dc.contributor.authorJensen, Logan
dc.contributor.authorGamaunt, John
dc.contributor.authorButler, Nat
dc.contributor.authorHelson, Kyle
dc.contributor.authoret al
dc.date.accessioned2023-02-20T19:23:53Z
dc.date.available2023-02-20T19:23:53Z
dc.date.issued2022-08-29
dc.descriptionAuthors: Lee Bernard, Logan Jensen, John Gamaunt, Nat Butler, Andrea Bocchieri, Quentin Changeat, Azzurra D'Alessandro, Billy Edwards, Qian Gong, John Hartley, Kyle Helson, Dan Kelly, Kanchita Klangboonkrong, Annalies Kleyheeg, Nikole Lewis, Steven Li, Michael Line, Stephen Maher, Ryan McClelland, Laddawan Miko, Lorenzo Mugnai, Peter Nagler, Barth Netterfield, Vivien Parmentier, Enzo Pascale, Jennifer Patience, Tim Rehm, Javier Romualdez, Subhajit Sarkar, Paul Scowen, Gregory S. Tucker, Augustyn Waczynski, Ingo Waldmanen_US
dc.description.abstractThe EXoplanet Climate Infrared TElescope (EXCITE) experiment is a balloon-borne, purpose-designed mission to measure spectroscopic phase curves of short-period extrasolar giant planets (EGPs, or “hot Jupiters”). Here, we present EXCITE’s principal science instrument: a high-throughput, single-object spectrograph operating in the 0.8-2.5 µm and 2.5-4.0 µm bands with R≥50. Our compact design achieves diffraction-limited, on-axis performance with just three powered optics: two off-axis parabolic mirrors and a CaF2 prism. We discuss the optical and mechanical design, the expected optical performance of the spectrograph, and summarize the tolerances needed to achieve that performance. We also discuss plans for establishing alignment of the optics and verifying the optical performance.en_US
dc.description.sponsorshipThis work is supported by NASA award 18-APRA18-0075 selected under NASA Research Announcement NNH18ZDA001N, Research Opportunities in Space Science – 2018 (ROSES-2018). Work by Kyle Helson is supported by NASA under award number 80GSFC17M0002.en_US
dc.description.urihttps://www.spiedigitallibrary.org/conference-proceedings-of-spie/12184/1218429/Design-and-testing-of-a-low-resolution-NIR-spectrograph-for/10.1117/12.2629717.fullen_US
dc.format.extent11 pagesen_US
dc.genreconference papers and proceedingsen_US
dc.identifierdoi:10.13016/m2cqhv-t7wu
dc.identifier.citationLee Bernard, Logan Jensen, John Gamaunt, Nat Butler, Andrea Bocchieri, Quentin Changeat, Azzurra D'Alessandro, Billy Edwards, Qian Gong, John Hartley, Kyle Helson, Dan Kelly, Kanchita Klangboonkrong, Annalies Kleyheeg, Nikole Lewis, Steven Li, Michael Line, Stephen Maher, Ryan McClelland, Laddawan Miko, Lorenzo Mugnai, Peter Nagler, Barth Netterfield, Vivien Parmentier, Enzo Pascale, Jennifer Patience, Tim Rehm, Javier Romualdez, Subhajit Sarkar, Paul Scowen, Gregory S. Tucker, Augustyn Waczynski, and Ingo Waldman "Design and testing of a low-resolution NIR spectrograph for the EXoplanet Climate Infrared TElescope", Proc. SPIE 12184, Ground-based and Airborne Instrumentation for Astronomy IX, 1218429 (29 August 2022); https://doi.org/10.1117/12.2629717en_US
dc.identifier.urihttps://doi.org/10.1117/12.2629717
dc.identifier.urihttp://hdl.handle.net/11603/26839
dc.language.isoen_USen_US
dc.publisherSPIEen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Center for Space Sciences and Technology
dc.relation.ispartofUMBC Faculty Collection
dc.rightsThis work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law.en_US
dc.rightsPublic Domain Mark 1.0*
dc.rights.urihttp://creativecommons.org/publicdomain/mark/1.0/*
dc.titleDesign and testing of a low-resolution NIR spectrograph for the EXoplanet Climate Infrared TElescopeen_US
dc.typeTexten_US
dcterms.creatorhttps://orcid.org/0000-0001-9238-4918en_US

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