High-energy X-rays from the Crab Nebula
Balloon measurement of high energy X-ray spectrum from Crab Nebula
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Balloon measurement of high energy X-ray spectrum from Crab Nebula
High energy X rays from Cygnus XR-1, Cassiopeia A and SN 1572 measured by balloon- borne scintillation counter
High energy X ray flux increase from Cygnus XR-1
Balloon flight observations of high energy X ray source in Centaurus, Norma and Lupus
Weak X ray sources at 20-100 Kev photon energies observed during balloon flight, finding hard rays from Ara XR-1 and Nor XR-1
High energy X ray observational data for Sagittarius sources scanned by active telescope during February 1968 balloon flight
Balloon observations of Cen XR-2 X ray emission decrease
Balloonborne X ray telescopic observations of two point sources in Crux
Balloonborne X ray telescopic observation of point source in Crux
High energy X ray flux from source in Centaurus Crux detected by balloon sounding
Rapid fluctuations in high energy X ray flux from source in Centaurus Crux from balloon sounding
High-energy X-ray observations have transformed our understanding of astrophysical systems where non-thermal processes dominate, from shock-accelerated particles in supernova remnants to relativistic jets and hot coronae in active galactic nuclei. NuSTAR’s pioneering focusing images of the hard X-ray sky have demonstrated the immense scientific potential of this band, while also highlighting how limited angular resolution constrains our ability to fully characterize complex physical processes in faint extended sources and resolving faint sources in crowded sky regions. In this presentation, I will discuss a pathway to overcome these challenges through NASA Marshall Space Flight Center’s replicated NiCo full-shell X-ray mirror technology. Specifically, I will discuss the SuperHERO hard X-ray telescope to achieve better than 10-arcsecond half-power diameter (HPD) angular resolution on a balloon flight observing the Crab Nebula, and the High EneRgy Observatory for Imaging X-rays (HEROIX) Medium-Class Mission concept to achieve an integrated effective area of 570 cm2 at 30 keV with 5 arcsec HPD angular resolution.
OGO III spectrometric determination time history and differential intensity of solar X-rays
Northern sky survey of high energy cosmic X rays and sources spectra in Crab Nebula and Cygnus using balloon-borne detector
X ray survey of northern sky in 20-100 kev energy range, giving spectra for Cyg X-1, Tau X-1 and Crab nebula
Scorpius X-1 high energy X ray flux variations from balloon-borne scanner data
Sources of X-rays and high-energy gamma rays, including inverse Compton effect, synchrotron radiation, brehmsstrahlung from hot plasma, and decay of neutral pions
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.