HEX-P Publications

Frontiers HEX-P Webpage:

https://www.frontiersin.org/research-topics/59532/high-energy-astrophysics-research-enabled-by-the-probe-class-mission-concept-hex-p

The High Energy X-ray Probe (HEX–P): The Future of Hard X-ray Dual AGN Science, Ryan W, Pfiefle et al.

The High Energy X-ray Probe (HEX–P): Supernova remnants, pulsar wind nebulae, and nuclear astrophysics, Stephen Reynolds et al.

The High Energy X-ray Probe (HEX–P): The Circum-nuclear Environment of Growing Supermassive Black Holes, P. G. Boorman et al.

The High Energy X-ray Probe (HEX–P): Sensitive broadband X-ray observations of transient phenomena in the 2030s, Murray Brightman et al.

The High Energy X-ray Probe (HEX–P): resolving the nature of Sgr A* flares, compact object binaries and diffuse X-ray emission in the Galactic Center and beyond, Kaya Mori et al.

The High Energy X-ray Probe (HEX–P): Galactic PeVatrons, star clusters, superbubbles, microquasar jets, and gamma-ray binaries, Kaya Mori et al.

The High Energy X-ray Probe (HEX–P): Bringing the Cosmic X-ray Background into Focus, Francesco Civano et al.

The High Energy X-ray Probe (HEX–P): the most powerful jets through the lens of a superb X-ray eye, Lea Marcotulli

The High Energy X-ray Probe (HEX–P): Probing Accretion onto Stellar Mass Black Holes, Riley Conners et al.

The High Energy X-ray Probe (HEX–P): Constraining Supermassive Black Hole Growth with Population Spin Measurements, J. M. Piotrowska et al.

The High Energy X-ray Probe (HEX–P): Magnetars and Other Isolated Neutron Stars, J. A. J. Alford et al.

The High Energy X-ray Probe: Resolved X-ray Populations in Extragalactic Environments, Bret D. Lehmer et al.

The High Energy X-ray Probe (HEX–P): Studying Extreme Accretion with Ultraluminous X-ray Sources, Matteo Bachetti et al.

The High Energy X-ray Probe (HEX–P): A New Window into Neutron Star Accretion, R. M. Ludlam et al.

The High Energy X-ray Probe (HEX–P): Probing the physics of the X-ray corona in active galactic nuclei, E. Kammoun et al.