activity
20092025
most citedDiscovery of Strong Radiative Recombination Continua from The Supernova Remnant IC 443 with Suzaku

110 citations · 123 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2025

In-orbit Performance of the Soft X-ray Imaging Telescope Xtend aboard XRISM

Hiroyuki Uchida, Koji Mori, Hiroshi Tomida +62

We present a summary of the in-orbit performance of the soft X-ray imaging telescope Xtend onboard the XRISM mission, based on in-flight observation data, including first-light cel…

astro-ph.IM2025

Soft X-ray Imager of the Xtend system onboard XRISM

Hirofumi Noda, Koji Mori, Hiroshi Tomida +57

The Soft X-ray Imager (SXI) is the X-ray charge-coupled device (CCD) camera for the soft X-ray imaging telescope Xtend installed on the X-ray Imaging and Spectroscopy Mission (XRIS…

astro-ph.HE2014★ 3 cited

ASTRO-H White Paper - Young Supernova Remnants

J. P. Hughes, S. Safi-Harb, A. Bamba +23

Thanks to the unprecedented spectral resolution and sensitivity of the Soft X-ray Spectrometer (SXS) to soft thermal X-ray emission, ASTRO-H will open a new discovery window for un…

astro-ph.HE2014★ 1 cited

ASTRO-H White Paper - Older Supernova Remnants and Pulsar Wind Nebulae

K. S. Long, A. Bamba, F. Aharonian +20

Most supernova remnants (SNRs) are old, in the sense that their structure has been profoundly modified by their interaction with the surrounding interstellar medium (ISM). Old SNRs…

astro-ph.HE2012★ 9 cited

Limits on Large Extra Dimensions Based on Observations of Neutron Stars with the Fermi-LAT

Bijan Berenji, Elliott Bloom, Johann Cohen-Tanugi

We present limits for the compactification scale in the theory of Large Extra Dimensions (LED) proposed by Arkani-Hamed, Dimopoulos, and Dvali. We use 11 months of data from the Fe…

astro-ph.HE2009★ 110 cited

Discovery of Strong Radiative Recombination Continua from The Supernova Remnant IC 443 with Suzaku

Hiroya Yamaguchi, Midori Ozawa, Katsuji Koyama +4

We present the Suzaku spectroscopic study of the Galactic middle-aged supernova remnant (SNR) IC 443. The X-ray spectrum in the 1.75-6.0 keV band is described by an optically-thin…