NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Press Enter or click the Search button to begin your search.

Back to Results
The HEROIX Broadband X-Ray Space Telescope Mission ConceptThe High EneRgy Observatory for Imaging X-rays (HEROIX) Medium-Class Mission concept envisions a next-generation broadband X-ray observatory designed to meet the astrophysics community’s need for high-angular-resolution studies of the Cosmic X-ray Background. Building on the science legacy of NASA’s NuSTAR mission and more than 30 years of advances in replicated NiCo shell technology at NASA Marshall, HEROIX proposes a space observatory comprising four co-aligned telescopes achieving 5 arcsecond half-power diameter (HPD) angular resolution. This capability, approached by the resolution demonstrated in the FOXSI-4 sounding rocket mission and under development through the SuperHERO balloon mission, will be extended to energies up to 80 keV through multilayer coatings. Marshall’s inhouse precision optics manufacturing enables an integrated effective area of 380 cm² at 30 keV, which, combined with high-resolution optics, opens new windows into extreme astrophysical non-thermal processes.
Document ID
20260005967
Acquisition Source
Marshall Space Flight Center
Document Type
Presentation
Authors
Nick Thomas
(Marshall Space Flight Center Redstone Arsenal, United States)
Chien-Ting Chen
(Universities Space Research Association Columbia, United States)
Mike Baysinger
(Marshall Space Flight Center Redstone Arsenal, United States)
Steve Bongiorno
(Marshall Space Flight Center Redstone Arsenal, United States)
Thomas E Brooks
(Marshall Space Flight Center Redstone Arsenal, United States)
Patrick Champey
(Marshall Space Flight Center Redstone Arsenal, United States)
Casey DeRoo
(University of Iowa Iowa City, United States)
James David
(Amentum Chantilly, Virginia, United States)
Ben Diedrich
(Amentum Chantilly, Virginia, United States)
Kirtan Dixit
(Marshall Space Flight Center Redstone Arsenal, United States)
Steve Ehlert
(Marshall Space Flight Center Redstone Arsenal, United States)
Leo Fabisinski
(Amentum Chantilly, Virginia, United States)
Rebekah Frederick
(Marshall Space Flight Center Redstone Arsenal, United States)
Jay Garcia
(Amentum Chantilly, Virginia, United States)
Danielle Gurgew
(Universities Space Research Association Columbia, United States)
Kouichi Hagino
(The University of Tokyo)
Mark Ibekwe
(Marshall Space Flight Center Redstone Arsenal, United States)
John Inness
(Marshall Space Flight Center Redstone Arsenal, United States)
Phil Kaaret
(Marshall Space Flight Center Redstone Arsenal, United States)
Ravi Kannan
(Amentum Chantilly, Virginia, United States)
W Peter Maksym
(Marshall Space Flight Center Redstone Arsenal, United States)
Hironori Matsumoto
(The University of Osaka Osaka, Japan)
John Morley
(Marshall Space Flight Center Redstone Arsenal, United States)
Koji Mori
(University of Miyazaki Miyazaki, Japan)
Kazuhiro Nakazawa
(NAGOYA U.)
Panini Singam
(Universities Space Research Association Huntsville, AL, United States)
David Smith
(Marshall Space Flight Center Redstone Arsenal, United States)
Benjamin H Stolz
(Marshall Space Flight Center Redstone Arsenal, United States)
Doug Swartz
(Universities Space Research Association Columbia, United States)
Tadayuki Takahashi
(Kavli Institute for the Physics and Mathematics of the Universe Kashiwa, Japan)
Shin'ichiro Takeda
(Fukushima Institute for Research, Education and Innovation Namie, Japan)
Dan Thomas
(Marshall Space Flight Center Redstone Arsenal, United States)
Sarah Triana
(Marshall Space Flight Center Redstone Arsenal, United States)
Takeshi G Tsuru
(Kyoto University)
Yoshihiro Ueda
(Kyoto University)
Shin Watanabe
(Japan Aerospace Exploration Agency Tokyo, Japan)
Date Acquired
July 2, 2026
Subject Category
Space Sciences (General)
Meeting Information
Meeting: SPIE Astronomical Telescopes + Instrumentation
Location: Copenhagen
Country: DK
Start Date: July 5, 2026
End Date: July 10, 2026
Sponsors: International Society for Optics and Photonics
Funding Number(s)
WBS: 399131.02.01.06.05
Distribution Limits
Public
Copyright
Public Use Permitted.
No Preview Available