HEX-P: The High-Energy X-ray Probe

Date

2019

Department

Program

Citation of Original Publication

Madsen, K. K., Hickox, R., Bachetti, M., Stern, D., Gellert, N. C., García, J., Kara, E., Brandt, N. W., Krawczynski, H., Lohfink, A., Brenneman, L., Christensen, F., Middleton, M., Hornstrup, A., Matt, G., Jaodand, A., Lansbury, G., Ricci, C., Fuerst, F., ... Craig, W. (2019). HEX-P: The High-Energy X-ray Probe. American Astronomical Society. Bulletin (Online), 51(7). https://baas.aas.org/pub/2020n7i166

Rights

This work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law.
Public Domain Mark 1.0

Subjects

Abstract

The High-Energy X-ray Probe (HEX-P) is a next-generation high-energy X-ray observatory with broadband (2-200 keV) response that has 40 times the sensitivity of any previous mission in the 10-80 keV band and > 100 times the sensitivity of any previous mission in the 80-200 keV band. With this leap in observational capability, HEX-P will address a broad range of science objectives beyond any planned mission in the hard X-ray bandpass. HEX-P will probe the extreme environments around black holes and neutron stars, map the growth of supermassive black holes, and quantify the effect they have on their environments. HEX-P will resolve the hard X-ray emission from dense regions of our Galaxy to understand the highenergy source populations and investigate dark matter candidate particles through their decay channel signatures. If developed and launched on a timescale similar to Athena, the complementary abilities of the two missions will greatly enhance the Community’s ability to address the important science questions of the hot universe. HEX-P addresses science that is not planned by any flagship-class missions, and is beyond the capability of an Explorer-class mission.