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Marie Kondo

3 papers here

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

author position
  • middle author2
  • last author1

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA2
  • astro-ph.HE1
ORCID 0009-0005-5685-1562

identity via Semantic Scholar / OpenAlex

most citedXRISM Observation of the Ophiuchus Galaxy Cluster: Quiescent Velocity Structure in the Dynamically Disturbed Core

15 citations · 15 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.GA2025

Suzaku observations of outskirts of nearby clusters and groups: I. electron density and gas fraction to the virial radius

Kyoko Matsushita, Marie Kondo, Kosuke Sato +3

We present an analysis of Suzaku observations of 14 nearby galaxy clusters and groups (z < 0.06), extending radial coverage out to the virial radius (approximately r200). The sampl…

astro-ph.HE2025★ 15 cited

XRISM Observation of the Ophiuchus Galaxy Cluster: Quiescent Velocity Structure in the Dynamically Disturbed Core

Yutaka Fujita, Kotaro Fukushima, Kosuke Sato +2

We present the high-resolution X-rayspectroscopic observations of the Ophiuchus galaxy cluster core using the XRISM satellite. Despite previous observations revealing multiple cold…

astro-ph.GA2024

AGN properties of ~1 million member galaxies of galaxy groups and clusters at z < 1.4 based on the Subaru Hyper Suprime-Cam survey

Yoshiki Toba, Aoi Hashiguchi, Naomi Ota +17

Herein, we present the statistical properties of active galactic nuclei (AGNs) for approximately 1 million member galaxies of galaxy groups and clusters, with 0.1 < cluster redsh…

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