Diamond-loaded polyimide aerogel scattering filters and their applications in astrophysical and planetary science observations

dc.contributor.authorHelson, Kyle
dc.contributor.authorChan, Carol Yan Yan
dc.contributor.authorArseneau, Stefan
dc.contributor.authorBarlis, Alyssa
dc.contributor.authorBennett, Charles L.
dc.contributor.authorEssinger-Hileman, Thomas M.
dc.contributor.authorGuo, Haiquan
dc.contributor.authorMarriage, Tobias
dc.contributor.authorQuijada, Manuel A.
dc.contributor.authorTokarz, Ariel E.
dc.contributor.authorVivod, Stephanie L.
dc.contributor.authorWollack, Edward J.
dc.date.accessioned2026-02-12T16:44:32Z
dc.date.issued2025-08-28
dc.description.abstractInfrared-blocking, aerogel-based scattering filters have a broad range of potential applications in astrophysics and planetary science instruments in the far-infrared, sub-millimeter, and microwave regimes. This paper demonstrates the ability of conductively-loaded, polyimide aerogel filters to meet the mechanical and science instrument requirements for several experiments, including the Cosmology Large Angular Scale Surveyor (CLASS), the Experiment for Cryogenic Large-Aperture Intensity Mapping (EXCLAIM), and the Sub-millimeter Solar Observation Lunar Volatiles Experiment (SSOLVE). Thermal multi-physics simulations of the filters predict their performance when integrated into a cryogenic receiver. Prototype filters have survived cryogenic cycling to 4\,K with no degradation in mechanical properties. Measurement of total hemispherical reflectance and transmittance, as well as cryogenic tests of the aerogel filters in a full receiver context, allow estimates of the integrated infrared emissivity of the filters. Knowledge of the emissivity will help instrument designers incorporate the filters into future experiments in planetary science, astrophysics, and cosmology.
dc.description.sponsorshipThis work was supported by the National Aeronautics and Space Administration under grant numbers NNX14AB76A and NNH18ZDA001N-18-APRA18-0008, as well as the National Science Foundation Division of Astronomical Sciences for their support of this work under Grant Numbers 0959349, 1429236, 1636634, and 1654494. K.R.H. acknowledges that the material is based upon work supported by NASA under award number 80GSFC24M0006. We also gratefully acknowledge support under the Goddard Internal Research and Development (IRAD) program. Portions of this work were presented at the SPIE conference on Astronomical Telescopes + Instrumentation in 2022, under papers titled “Characterization of aerogel scattering filters for astronomical telescopes” and “Novel infrared-blocking aerogel scattering filters and their applications in astrophysical and planetary science observations.
dc.description.urihttp://arxiv.org/abs/2508.20406
dc.format.extent16 pages
dc.genrejournal articles
dc.genrepreprints
dc.identifierdoi:10.13016/m2zxei-egen
dc.identifier.urihttps://doi.org/10.48550/arXiv.2508.20406
dc.identifier.urihttp://hdl.handle.net/11603/41916
dc.language.isoen
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Center for Space Sciences and Technology (CSST) / Center for Research and Exploration in Space Sciences & Technology II (CRSST II)
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.
dc.rightsPublic Domain
dc.rights.urihttps://creativecommons.org/publicdomain/mark/1.0/
dc.subjectAstrophysics - Instrumentation and Methods for Astrophysics
dc.subjectCondensed Matter - Materials Science
dc.subjectPhysics - Optics
dc.titleDiamond-loaded polyimide aerogel scattering filters and their applications in astrophysical and planetary science observations
dc.typeText
dcterms.creatorhttps://orcid.org/0000-0001-9238-4918

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