activity
20072021
most citedDetailed Design of the Science Operations for the XRISM mission

23 citations · 37 across the 2 of their papers we have counts for

collaborators

7 papers

astro-ph.IM202123 cited

Detailed Design of the Science Operations for the XRISM mission

Yukikatsu Terada, Matt Holland, Michael Loewenstein +36

XRISM is an X-ray astronomical mission by the JAXA, NASA, ESA and other international participants, that is planned for launch in 2022 (Japanese fiscal year), to quickly restore hi…

astro-ph.IM2019

A concept for the X-ray telescope system with an angular-resolution booster

Yoshitomo Maeda, Ryo Iizuka, Takayuki Hayashi +7

We present a concept of the X-ray imaging system with high angular-resolution and moderate sensitivity. In this concept, a two-dimensional detector, i.e., imager, is put at a sligh…

astro-ph.HE2018

Detection of polarized gamma-ray emission from the Crab nebula with Hitomi Soft Gamma-ray Detector

Hitomi Collaboration, Felix Aharonian, Hiroki Akamatsu +191

We present the results from the Hitomi Soft Gamma-ray Detector (SGD) observation of the Crab nebula. The main part of SGD is a Compton camera, which in addition to being a spectrom…

astro-ph.IM2018

In-flight performance of the Canadian Astro-H Metrology System

Luigi C. Gallo, Alexander Koujelev, Stephane Gagnon +11

The Canadian Astro-H Metrology System (CAMS) on the Hitomi X-ray satellite is a laser alignment system that measures the lateral displacement (X/Y) of the extensible optical bench…

astro-ph.IM2018

Inorbit Performance of the Hard X-ray Telescope (HXT) on board the Hitomi (ASTRO-H) satellite

H. Matsumoto, H. Awaki, M. Ishida +16

Hitomi (ASTRO-H) carries two Hard X-ray Telescopes (HXTs) that can focus X-rays up to 80 keV. Combined with the Hard X-ray Imagers (HXIs) that detect the focused X-rays, imaging sp…

astro-ph.HE2018

Hitomi X-ray Observation of the Pulsar Wind Nebula G21.50.9

Hitomi Collaboration, Felix Aharonian, Hiroki Akamatsu +194

We present results from the Hitomi X-ray observation of a young composite-type supernova remnant (SNR) G21.50.9, whose emission is dominated by the pulsar wind nebula (PWN) cont…