Development of x-ray microcalorimeter imaging spectrometers for the X-ray Surveyor mission concept

dc.contributor.authorBandler, Simon R.
dc.contributor.authorAdams, Joseph S.
dc.contributor.authorChervenak, James A.
dc.contributor.authorDatesman, Aaron M.
dc.contributor.authorMiniussi, Antoine
dc.contributor.authorPorter, Frederick S.
dc.contributor.authorSadleir, John E.
dc.contributor.authorSakai, Kazuhiro
dc.contributor.authorSmith, Stephen J.
dc.contributor.authorWakeham, Nicholas
dc.contributor.authoret al
dc.date.accessioned2022-01-20T16:12:39Z
dc.date.available2022-01-20T16:12:39Z
dc.date.issued2016-07-19
dc.descriptionSimon R. Bandler, Joseph S. Adams, James A. Chervenak, Aaron M. Datesman, Megan E. Eckart, Fred M. Finkbeiner, Richard L. Kelley, Caroline A. Kilbourne, Gabriele Betancourt-Martinez, Antoine Miniussi, Frederick S. Porter, John E. Sadleir, Kazuhiro Sakai, Stephen J. Smith, Thomas R. Stevenson, Nicholas Wakeham, Edward J. Wassell, Wonsik Yoon, Dan Becker, Douglas Bennett, William B. Doriese, Joseph W. Fowler, Johnathan D. Gard, Gene C. Hilton, Benjamin Mates, Kelsey M. Morgan, Carl D. Reintsema, Daniel Swetz, Joel N. Ullom, Saptarshi Chaudhuri, Kent D. Irwin, Sang-Jun Lee, Alexey Vikhlininen_US
dc.description.abstractFour astrophysics missions are currently being studied by NASA as candidate large missions to be chosen in the 2020 astrophysics decadal survey.1 One of these missions is the “X-Ray Surveyor” (XRS), and possible configurations of this mission are currently under study by a science and technology definition team (STDT). One of the key instruments under study is an X-ray microcalorimeter, and the requirements for such an instrument are currently under discussion. In this paper we review some different detector options that exist for this instrument, and discuss what array formats might be possible. We have developed one design option that utilizes either transition-edge sensor (TES) or magnetically coupled calorimeters (MCC) in pixel array-sizes approaching 100 kilo-pixels. To reduce the number of sensors read out to a plausible scale, we have assumed detector geometries in which a thermal sensor such a TES or MCC can read out a sub-array of 20-25 individual 1” pixels. In this paper we describe the development status of these detectors, and also discuss the different options that exist for reading out the very large number of pixels.en_US
dc.description.urihttps://www.spiedigitallibrary.org/conference-proceedings-of-spie/9905/99050Q/Development-of-x-ray-microcalorimeter-imaging-spectrometers-for-the-X/10.1117/12.2232156.fullen_US
dc.format.extent13 pagesen_US
dc.genrejournal articlesen_US
dc.identifierdoi:10.13016/m2ay6g-eyy4
dc.identifier.citationSimon R. Bandler, Joseph S. Adams, James A. Chervenak, Aaron M. Datesman, Megan E. Eckart, Fred M. Finkbeiner, Richard L. Kelley, Caroline A. Kilbourne, Gabriele Betancourt-Martinez, Antoine R. Miniussi, Frederick S. Porter, John E. Sadleir, Kazuhiro Sakai, Stephen J. Smith, Thomas R. Stevenson, Nicholas A. Wakeham, Edward J. Wassell, Wonsik Yoon, Dan Becker, Douglas Bennett, William B. Doriese, Joseph W. Fowler, Johnathan D. Gard, Gene C. Hilton, Benjamin Mates, Kelsey M. Morgan, Carl D. Reintsema, Daniel Swetz, Joel N. Ullom, Saptarshi Chaudhuri, Kent D. Irwin, Sang-Jun Lee, Alexey Vikhlinin, "Development of x-ray microcalorimeter imaging spectrometers for the X-ray Surveyor mission concept," Proc. SPIE 9905, Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray, 99050Q (19 July 2016); https://doi.org/10.1117/12.2232156en_US
dc.identifier.urihttps://doi.org/10.1117/12.2232156
dc.identifier.urihttp://hdl.handle.net/11603/24029
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 Physics Department
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.titleDevelopment of x-ray microcalorimeter imaging spectrometers for the X-ray Surveyor mission concepten_US
dc.typeTexten_US
dcterms.creatorhttps://orcid.org/0000-0003-0622-5174en_US
dcterms.creatorhttps://orcid.org/0000-0003-4096-4675en_US
dcterms.creatorhttps://orcid.org/0000-0002-9247-3010en_US
dcterms.creatorhttps://orcid.org/0000-0001-8397-9338en_US

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