Kristin K. Madsen,1 James Corsetti,1 Steven Kenyon,1 Takashi Okajima,1 Scott Rohrback,1 Keisuke Tamura,1 William W. Zhang,1 Danielle N. Gurgew,2 Finn Erland Christensen,3 Desiree Della Monica Ferreira,3 Nis Christian Gellert,3 Sonny Massahi,3 Stefano Basso,4 Giovanni Pareschi,4 Alberto Moretti,4 Daniele Spigahttps://orcid.org/0000-0003-1163-7843,4 Giuseppe Valsecchi,5 Dervis Vernani,5 Daniel K. Stern6
1NASA Goddard Space Flight Ctr. (United States) 2NASA Marshall Space Flight Ctr. (United States) 3DTU Space, Technical Univ. of Denmark (Denmark) 4INAF, Osservatorio Astronomico di Brera (Italy) 5Media Lario S.r.L. (Italy) 6Jet Propulsion Lab., California Institute of Technology (United States)
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The High Energy X-ray Probe (HEX-P) is a probe-class mission concept that combines high spatial resolution x-ray imaging and broad spectral coverage to enable revolutionary new insights into the important astrophysical questions of the next decade. HEX-P will fly a complement of two Hard Energy Mirror Assemblies (HEMA) and one Low Energy Mirror Assembly (LEMA), all of which will have a focal length of 20 meter. Ir/C has been chosen as the baseline coating for the LEMA, and a combination of Pt/C and W/Si multilayers for the HEMA. We present here the mirror design, optimization of coating recipes, and estimated performance.
(2023) Published by SPIE. Downloading of the abstract is permitted for personal use only.
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Kristin K. Madsen, James Corsetti, Steven Kenyon, Takashi Okajima, Scott Rohrback, Keisuke Tamura, William W. Zhang, Danielle N. Gurgew, Finn Erland Christensen, Desiree Della Monica Ferreira, Nis Christian Gellert, Sonny Massahi, Stefano Basso, Giovanni Pareschi, Alberto Moretti, Daniele Spiga, Giuseppe Valsecchi, Dervis Vernani, Daniel K. Stern, "Mirror design for the high-energy x-ray probe (HEX-P)," Proc. SPIE 12679, Optics for EUV, X-Ray, and Gamma-Ray Astronomy XI, 126791E (5 October 2023); https://doi.org/10.1117/12.2677554