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Document Type: Journal Article Author: Daniel Stern (3266) Production Date: 2023

1 to 9 of 9 Results

The High Energy X-ray Probe (HEX-P): Probing the physics of the X-ray corona in active galactic nucleiEmbargoed Dec 18, 2023 Daniel Stern, 2023, "The High Energy X-ray Probe (HEX-P): Probing the physics of the X-ray corona in active galactic nuclei", https://doi.org/10.48577/jpl.UVNCMJ, Frontiers of Astronomy and Space Sciences, JPL Open Repository The hard, non-thermal X-ray emission in active galactic nuclei (AGN) and black hole X-ray binaries (BHXRBs) is traditionally thought to be produced by a hot cloud of electrons referred to as the corona, which resides in close vicinity to the central black hole. This emission is c...
The High Energy X-ray Probe (HEX-P): Magnetars and Other Isolated Neutron StarsEmbargoed Dec 7, 2023 Daniel Stern, 2023, "The High Energy X-ray Probe (HEX-P): Magnetars and Other Isolated Neutron Stars", https://doi.org/10.48577/jpl.BBLHOG, Frontiers in Astronomy and Space Sciences, JPL Open Repository The hard X-ray emission from magnetars and other isolated neutron stars remains under- explored. An instrument with higher sensitivity to hard X-rays is critical to understanding the physics of neutron star magnetospheres and also the relationship between magnetars and Fast Radio...
The High Energy X-ray Probe (HEX-P): resolving the nature of Sgr A* flares, compact object binaries, ultra-relativistic cosmic-rays and particle accelerators in the Galactic CenterEmbargoed Dec 6, 2023 Daniel Stern, 2023, "The High Energy X-ray Probe (HEX-P): resolving the nature of Sgr A* flares, compact object binaries, ultra-relativistic cosmic-rays and particle accelerators in the Galactic Center", https://doi.org/10.48577/jpl.BCST9N, Frontiers in Astronomy and Space Sciences, JPL Open Repository HEX-P is a probe-class mission concept that will combine high spatial resolution X-ray imaging (< 10′′ FWHM) and broad spectral coverage (0.2–80 keV) with a sensitivity far superior to current facilities (including XMM-Newton and NuSTAR). These capabilities will enable revolution...
The High Energy X-ray Probe (HEX-P): Galactic PeVatrons, star clusters, superbubbles, microquasar jets, and gamma-ray binariesEmbargoed Dec 4, 2023 Daniel Stern, 2023, "The High Energy X-ray Probe (HEX-P): Galactic PeVatrons, star clusters, superbubbles, microquasar jets, and gamma-ray binaries", https://doi.org/10.48577/jpl.SRHTEW, Frontiers in Astronomy and Space Sciences, JPL Open Repository HEX-P is a probe-class mission concept that will combine high spatial resolution X-ray imaging and broad spectral coverage (0.2-80 keV) with a sensitivity far superior to current facilities (including XMM-Newton and NuSTAR) to enable revolutionary new insights into a variety of i...
The High Energy X-ray Probe (HEX-P): Supernova remnants, pulsar wind nebulae, and nuclear astrophysics Nov 27, 2023 Daniel Stern, 2023, "The High Energy X-ray Probe (HEX-P): Supernova remnants, pulsar wind nebulae, and nuclear astrophysics", https://doi.org/10.48577/jpl.GMU5IV, Frontiers of Astronomy and Space Sciences, JPL Open Repository HEX-P is a probe-class mission concept that will combine high spatial resolution X-ray imaging and broad spectral coverage (0.2--80 keV) with a sensitivity area far superior to current facilities (including XMM-Newton and NuSTAR) to enable revolutionary new insights into a variet...
The High Energy X-ray Probe (HEX-P): Supernova remnants, pulsar wind nebulae, and nuclear astrophysicsEmbargoed Nov 27, 2023 Daniel Stern, 2023, "The High Energy X-ray Probe (HEX-P): Supernova remnants, pulsar wind nebulae, and nuclear astrophysics", https://doi.org/10.48577/jpl.Q2LZA6, Frontiers of Astronomy and Space Sciences, JPL Open Repository HEX-P is a probe-class mission concept that will combine high spatial resolution X-ray imaging and broad spectral coverage (0.2--80 keV) with a sensitivity area far superior to current facilities (including XMM-Newton and NuSTAR) to enable revolutionary new insights into a variet...
The High Energy X-ray Probe (HEX-P): Probing Accretion onto Stellar Mass Black HolesEmbargoed Nov 22, 2023 Daniel Stern, 2023, "The High Energy X-ray Probe (HEX-P): Probing Accretion onto Stellar Mass Black Holes", https://doi.org/10.48577/jpl.BJHZU1, Frontiers in Astronomy and Space Sciences, JPL Open Repository Accretion is a universal astrophysical process that plays a key role in cosmic history, from the epoch of reionization to galaxy and stellar formation and evolution. Accreting stellar-mass black holes in X-ray binaries are one of the best laboratories to study the accretion proce...
The High Energy X-ray Probe: Resolved X-ray Populations in Extragalactic EnvironmentsEmbargoed Oct 30, 2023 Daniel Stern, 2023, "The High Energy X-ray Probe: Resolved X-ray Populations in Extragalactic Environments", https://doi.org/10.48577/jpl.ASQKCD, Frontiers in Astronomy and Space Sciences, JPL Open Repository The High Energy X-ray Probe (HEX-P) is a probe-class mission concept that will combine high spatial resolution X-ray imaging (<20 arcsec FWHM) and broad spectral coverage (0.2–80 keV) with a sensitivity superior to current facilities (including XMM-Newton and NuSTAR). HEX-P will...
The High Energy X-ray Probe (HEX-P): Studying Extreme Accretion with Ultraluminous X-ray SourcesEmbargoed Oct 30, 2023 Daniel Stern, 2023, "The High Energy X-ray Probe (HEX-P): Studying Extreme Accretion with Ultraluminous X-ray Sources", https://doi.org/10.48577/jpl.3AYAGF, Frontiers in Astronomy and Space Sciences, JPL Open Repository Ultraluminous X-ray sources (ULXs) represent an extreme class of accreting compact objects: from the identification of some of the accretors as neutron stars to the detection of powerful winds travelling at 0.1-0.2 c, the increasing evidence points towards ULXs harbouring stellar...

The High Energy X-ray Probe (HEX-P): Probing the physics of the X-ray corona in active galactic nucleiEmbargoed

Dec 18, 2023

Daniel Stern, 2023, "The High Energy X-ray Probe (HEX-P): Probing the physics of the X-ray corona in active galactic nuclei", https://doi.org/10.48577/jpl.UVNCMJ, Frontiers of Astronomy and Space Sciences, JPL Open Repository

The hard, non-thermal X-ray emission in active galactic nuclei (AGN) and black hole X-ray binaries (BHXRBs) is traditionally thought to be produced by a hot cloud of electrons referred to as the corona, which resides in close vicinity to the central black hole. This emission is c...

The High Energy X-ray Probe (HEX-P): Magnetars and Other Isolated Neutron StarsEmbargoed

Dec 7, 2023

Daniel Stern, 2023, "The High Energy X-ray Probe (HEX-P): Magnetars and Other Isolated Neutron Stars", https://doi.org/10.48577/jpl.BBLHOG, Frontiers in Astronomy and Space Sciences, JPL Open Repository

The hard X-ray emission from magnetars and other isolated neutron stars remains under- explored. An instrument with higher sensitivity to hard X-rays is critical to understanding the physics of neutron star magnetospheres and also the relationship between magnetars and Fast Radio...

The High Energy X-ray Probe (HEX-P): resolving the nature of Sgr A* flares, compact object binaries, ultra-relativistic cosmic-rays and particle accelerators in the Galactic CenterEmbargoed

Dec 6, 2023

Daniel Stern, 2023, "The High Energy X-ray Probe (HEX-P): resolving the nature of Sgr A* flares, compact object binaries, ultra-relativistic cosmic-rays and particle accelerators in the Galactic Center", https://doi.org/10.48577/jpl.BCST9N, Frontiers in Astronomy and Space Sciences, JPL Open Repository

HEX-P is a probe-class mission concept that will combine high spatial resolution X-ray imaging (< 10′′ FWHM) and broad spectral coverage (0.2–80 keV) with a sensitivity far superior to current facilities (including XMM-Newton and NuSTAR). These capabilities will enable revolution...

The High Energy X-ray Probe (HEX-P): Galactic PeVatrons, star clusters, superbubbles, microquasar jets, and gamma-ray binariesEmbargoed

Dec 4, 2023

Daniel Stern, 2023, "The High Energy X-ray Probe (HEX-P): Galactic PeVatrons, star clusters, superbubbles, microquasar jets, and gamma-ray binaries", https://doi.org/10.48577/jpl.SRHTEW, Frontiers in Astronomy and Space Sciences, JPL Open Repository

HEX-P is a probe-class mission concept that will combine high spatial resolution X-ray imaging and broad spectral coverage (0.2-80 keV) with a sensitivity far superior to current facilities (including XMM-Newton and NuSTAR) to enable revolutionary new insights into a variety of i...

The High Energy X-ray Probe (HEX-P): Supernova remnants, pulsar wind nebulae, and nuclear astrophysics

Nov 27, 2023

Daniel Stern, 2023, "The High Energy X-ray Probe (HEX-P): Supernova remnants, pulsar wind nebulae, and nuclear astrophysics", https://doi.org/10.48577/jpl.GMU5IV, Frontiers of Astronomy and Space Sciences, JPL Open Repository

HEX-P is a probe-class mission concept that will combine high spatial resolution X-ray imaging and broad spectral coverage (0.2--80 keV) with a sensitivity area far superior to current facilities (including XMM-Newton and NuSTAR) to enable revolutionary new insights into a variet...

The High Energy X-ray Probe (HEX-P): Supernova remnants, pulsar wind nebulae, and nuclear astrophysicsEmbargoed

Nov 27, 2023

Daniel Stern, 2023, "The High Energy X-ray Probe (HEX-P): Supernova remnants, pulsar wind nebulae, and nuclear astrophysics", https://doi.org/10.48577/jpl.Q2LZA6, Frontiers of Astronomy and Space Sciences, JPL Open Repository

The High Energy X-ray Probe (HEX-P): Probing Accretion onto Stellar Mass Black HolesEmbargoed

Nov 22, 2023

Daniel Stern, 2023, "The High Energy X-ray Probe (HEX-P): Probing Accretion onto Stellar Mass Black Holes", https://doi.org/10.48577/jpl.BJHZU1, Frontiers in Astronomy and Space Sciences, JPL Open Repository

Accretion is a universal astrophysical process that plays a key role in cosmic history, from the epoch of reionization to galaxy and stellar formation and evolution. Accreting stellar-mass black holes in X-ray binaries are one of the best laboratories to study the accretion proce...

The High Energy X-ray Probe: Resolved X-ray Populations in Extragalactic EnvironmentsEmbargoed

Oct 30, 2023

Daniel Stern, 2023, "The High Energy X-ray Probe: Resolved X-ray Populations in Extragalactic Environments", https://doi.org/10.48577/jpl.ASQKCD, Frontiers in Astronomy and Space Sciences, JPL Open Repository

The High Energy X-ray Probe (HEX-P) is a probe-class mission concept that will combine high spatial resolution X-ray imaging (<20 arcsec FWHM) and broad spectral coverage (0.2–80 keV) with a sensitivity superior to current facilities (including XMM-Newton and NuSTAR). HEX-P will...

The High Energy X-ray Probe (HEX-P): Studying Extreme Accretion with Ultraluminous X-ray SourcesEmbargoed

Oct 30, 2023

Daniel Stern, 2023, "The High Energy X-ray Probe (HEX-P): Studying Extreme Accretion with Ultraluminous X-ray Sources", https://doi.org/10.48577/jpl.3AYAGF, Frontiers in Astronomy and Space Sciences, JPL Open Repository

Ultraluminous X-ray sources (ULXs) represent an extreme class of accreting compact objects: from the identification of some of the accretors as neutron stars to the detection of powerful winds travelling at 0.1-0.2 c, the increasing evidence points towards ULXs harbouring stellar...

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