556 citations
- Goddard Space Flight CenterUS60 papers
- Oak Ridge National LaboratoryUS30 papers
- University of Maryland, College ParkUS18 papers
- Fermi National Accelerator LaboratoryUS16 papers
- Space Telescope Science InstituteUS12 papers
- Center for Astrophysics Harvard & SmithsonianUS11 papers
- Johns Hopkins UniversityUS11 papers
- Los Alamos National LaboratoryUS11 papers
- General Atomics (United States)US10 papers
- Ames Research CenterUS9 papers
- Argonne National LaboratoryUS9 papers
- California Institute of TechnologyUS9 papers
11 papers · 1 filter
Science of High Resolution X-ray Imaging
H. L. Marshall, K. Weaver, M. Schattenburg +34
This report summarizes potential studies of the Hi-ReX Science Analysis Group for an Ultra-High Angular Resolution X-ray Observatory. Many potential science cases are presented, sp…
An Intermediate Mass Black Hole Hidden Behind Thick Obscuration
Peter G. Boorman, Daniel Stern, Roberto J. Assef +12
Recent models suggest approximately half of all accreting supermassive black holes (SMBHs; 10 M) are expected to undergo intense growth phase…
The High Energy X-ray Probe (HEX-P): The Future of Hard X-ray Dual AGN Science
Ryan W. Pfeifle, Peter G. Boorman, Kimberly A. Weaver +15
A fundamental goal of modern-day astrophysics is to understand the connection between supermassive black hole (SMBH) growth and galaxy evolution. Merging galaxies offer one of the…
The Properties of the Progenitor Supernova, Pulsar Wind, and Neutron Star inside PWN G54.1+0.3
Joseph D. Gelfand, Patrick O. Slane, Tea Temim
The evolution of a pulsar wind nebula (PWN) inside a supernova remnant (SNR) is sensitive to properties of the central neutron star, pulsar wind, progenitor supernova, and interste…
High-Energy Emission from the Composite Supernova Remnant MSH 15-56
Tea Temim, Patrick Slane, Daniel Castro +3
MSH 15-56 (G326.3-1.8) is a composite supernova remnant (SNR) that consists of an SNR shell and a displaced pulsar wind nebula (PWN) in the radio. We present XMM-Newton and Chandra…
Techniques for targeted Fermi-GBM follow-up of gravitational-wave events
Lindy Blackburn, Michael S. Briggs, Jordan Camp +4
The Advanced LIGO and Advanced Virgo ground-based gravitational-wave detectors are projected to come online 2015-2016, reaching a final sensitivity sufficient to observe dozens of…