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researcher

K. Matsushita

10 papers hereh-index 3206 citations9 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author10

Across the 10 of 10 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA4
  • astro-ph.HE4
  • astro-ph2
same name
  • K. Matsushita — 68 papers, h 43
  • K. Matsushita — 15 papers, h 9
  • K. Matsushita — 13 papers, h 12
  • K. Matsushita — 5 papers, h 9
  • K. Matsushita — 1 paper, h 2
  • K. Matsushita — 1 paper, h 3

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20022026
collaborators
Showing astro-ph.GAShow all

4 papers · 1 filter

astro-ph.GA2026

Probing the All-sky Distribution of Soft X-ray Emission Associated with the Milky Way

Kazuki Ampuku, Ikuyuki Mitsuishi, Philip Kaaret +5

We present an all-sky analysis of soft X-ray emission associated with the Milky Way using HaloSat and ROSAT data, extending our previous study of five Galactic-plane regions to 330…

astro-ph.GA2026

Diagnosing the Fe line complex of the intracluster medium by XRISM high-resolution spectroscopy

K. Fukushima, L. Hirata, N. Y. Yamasaki +17

We aim to test the validity of the CIE framework in the ICM by performing line diagnostics based mainly on resolved Fe-K emission lines. Methods. We analyse Resolve full-array spec…

astro-ph.GA2026

XRISM Reveals a Kinematically Coherent Core System of the Nearby Cool-Core Cluster Abell 2199

Kazunori Suda, Kyoko Matsushita, Kosuke Sato +14

We present the results of a deep 251 ks XRISM/Resolve observation of the cool core of the galaxy cluster Abell 2199. From the integrated spectrum of the central 3′×3′ Reso…

astro-ph.GA2026

Kinematics of the Weak Cool-Core Cluster A3571 Observed with XRISM: Low Cooling Rate Balanced by Low Heating Rate?

Hannah McCall, Irina Zhuravleva, Kyoko Matsushita +10

Most XRISM galaxy cluster observations to date have focused on AGN feedback or actively merging systems. The weak cool-core cluster A3571 was observed in four XRISM Cycle 1 pointin…

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