activity
20142023
most citedThe distribution of radioactive Ti in Cassiopeia A

134 citations · 508 across the 12 of their papers we have counts for

collaborators

13 papers

astro-ph.IM2024

Curved detectors for future X-ray astrophysics missions

Eric D. Miller, James A. Gregory, Marshall W. Bautz +17

Future X-ray astrophysics missions will survey large areas of the sky with unparalleled sensitivity, enabled by lightweight, high-resolution optics. These optics inherently produce…

astro-ph.IM202377 cited

Overview of the Advanced X-ray Imaging Satellite (AXIS)

Christopher S. Reynolds, Erin A. Kara, Richard F. Mushotzky +40

The Advanced X-ray Imaging Satellite (AXIS) is a Probe-class concept that will build on the legacy of the Chandra X-ray Observatory by providing low-background, arcsecond-resolutio…

astro-ph.HE20238 cited

A broadband X-ray imaging spectroscopy in the 2030s: the FORCE mission

Koji Mori, Takeshi G. Tsuru, Kazuhiro Nakazawa +49

In this multi-messenger astronomy era, all the observational probes are improving their sensitivities and overall performance. The Focusing on Relativistic universe and Cosmic Evol…

astro-ph.IM2021

A Comprehensive Line-Spread Function Error Budget for the Off-Plane Grating Rocket Experiment

Benjamin D. Donovan, Randall L. McEntaffer, James H. Tutt +13

The Off-plane Grating Rocket Experiment (OGRE) is a soft X-ray grating spectrometer to be flown on a suborbital rocket. The payload is designed to obtain the highest-resolution sof…

astro-ph.HE2016134 cited

The distribution of radioactive Ti in Cassiopeia A

Brian W. Grefenstette, Chris L. Fryer, Fiona A. Harrison +28

The distribution of elements produced in the inner-most layers of a supernova explosion is a key diagnostic for studying the collapse of massive stars. Here we present the results…

astro-ph.HE201428 cited

The Hard X-Ray View of the Young Supernova Remnant G1.9+0.3

Andreas Zoglauer, Stephen P. Reynolds, Hongjun An +12

NuSTAR observed G1.9+0.3, the youngest known supernova remnant in the Milky Way, for 350 ks and detected emission up to 30 keV. The remnant's X-ray morphology does not change…