Observations of cosmic X-rays.
Eight discrete cosmic X-ray sources observed by rocket techniques
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Eight discrete cosmic X-ray sources observed by rocket techniques
Cosmic X-ray sources in Scorpius and Sagittarius detected by rocket flights
Three cosmic X-ray source locations determined, using rocket mounted Geiger counters
Galactic origins of cosmic x-rays and gamma rays inferred from the relations between these rays
Spectral composition of X-ray source in Scorpius and in vicinity of Galactic centre, using rocket mounted NaI detector
Cosmic X-ray and IR wavelengths as tools for exploring large scale structure of universe
The High EneRgy Observatory for Imaging X-rays (HEROIX) is a next-generation broadband X-ray space telescope concept under development as a Medium-Class Explorer mission. Building on more than three decades of replicated NiCo shell technology at NASA’s Marshall Space Flight Center, HEROIX will deliver 5 arcsecond half-power-diameter imaging resolution in the hard X-ray band. The observatory will incorporate four co-aligned telescopes with advanced multilayer coatings, extending the bandpass into the hard X-ray regime and providing an integrated effective area of 380 cm² at 30 keV. A suite of focal plane detectors will enable imaging capability throughout its 1–80 keV bandpass. This combination of angular resolution and high-energy coverage will open new windows into non-thermal processes in extreme astrophysical environments. HEROIXwill deliver transformative science, advancing the astrophysics community’s understanding of supernova physics, the X-ray binary population of the Galactic Center, accretion-driven galaxy evolution, and the origin of the Cosmic X-ray Background.
The 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.
High energy gamma and X-ray photons and neutrinos from cosmic sources - galactic radiation
Balloon flight experiment to search for celestial sources of X-rays in energy range 20 to 58 kev
Nuclear emulsion, scintillation photodosimeter, and x-ray film for measurement of cosmic radiation dose in vostok iii and iv spacecraft
Angular diameters of X-ray source regions in Scorpio and Sagittarius constellations by rocket measurement with collimator
Mechanism for production of X-rays and gamma rays in galaxies noting photon and electron spectrum
Mechanism for production of X-rays and gamma rays in galaxies, noting photon and electron spectrum
Explosive limb flare of November 20, 1960 shown to coincide with beginning of radio and X-ray emission
Neutron stars considered as origin of X-ray emission from Scorpius and Crab Nebula
Interstellar X-ray absorption edges due to K- shell photoionization of oxygen and neon, using element abundances and atomic photoelectric cross section data