activity
20072026
most citedRobust Quantification of Galaxy Cluster Morphology Using Asymmetry and Central Concentration

52 citations · 163 across the 13 of their papers we have counts for

collaborators

14 papers

astro-ph.GA2026

Reigniting the FUSE II: O VI Emission in Massive Elliptical Galaxies

Michael Reefe, Michael McDonald, Greg L. Bryan +6

This is the second paper in a series where we examine archival far-ultraviolet spectroscopy of 29 massive elliptical galaxies from the Far Ultraviolet Spectroscopic Explorer (FUSE)…

astro-ph.HE2026

XRISM reveals sloshing-driven gas motions in the core of Abell 2029

Yuusuke Uchida, Yuna Saito, Naomi Ota +13

We investigate the velocity structure of the intracluster medium (ICM) in the core of the relaxed cool-core cluster Abell 2029 using XRISM Resolve spectroscopy. We analyze combined…

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 Reso…

astro-ph.HE2026★ 1 cited

Accurate Determination of Chemical Abundances near a Supermassive Black Hole

The XRISM collaboration

The metal abundances in galactic nuclei carry key information on the history of star formation and mass transfer in central regions of galaxies. X-ray fluorescence analysis is a un…

astro-ph.HE2025

Cross Calibration of Galaxy Cluster Temperatures Measured with NuSTAR, XMM-Newton, and Chandra

Fiona Lopez, Daniel R. Wik, Cicely Potter +10

The use of galaxy clusters to constrain cosmology is limited in part due to uncertainties in derived cluster masses, which often depend on the gas temperature. Unfortunately, there…

astro-ph.GA2025★ 1 cited

The intracluster light analysis of the most evolved systems of galaxies: fossil groups

Nícolas O. L. de Oliveira, Yolanda Jiménez-Teja, Renato A. Dupke +7

We present the analysis of the intracluster light (ICL) in three fossil groups (FG), RXJ085640.72+055347.36, RX J1136+0713, and RX J1410+4145, at z ~ 0.1. We used two optical broad…

astro-ph.GA2025

Constraints on Non-Thermal Pressure at galaxy cluster outskirts from a Joint SPT and XMM-Newton Analysis

Arnab Sarkar, Michael McDonald, Lindsey Bleem +11

We present joint South Pole Telescope (SPT) and XMM-Newton observations of 8 massive galaxy clusters (0.8--1.710 M) spanning a redshift range of 0.16 to 0.…

astro-ph.GA2024★ 2 cited

Unveiling the Cosmic Chemistry II: "Direct" -based metallicity of galaxies at 3 10 with JWST/NIRSpec

Priyanka Chakraborty, Arnab Sarkar, Randall Smith +10

We report the detection of the [O III] auroral line in 42 galaxies within the redshift range of . These galaxies were selected from publicly available JWST data release…

astro-ph.GA2024

Unveiling the Cosmic Chemistry: Revisiting the Mass-Metallicity Relation with JWST/NIRSpec at 4 < z < 10

Arnab Sarkar, Priyanka Chakraborty, Mark Vogelsberger +12

We present star formation rates (SFR), the mass-metallicity relation (MZR), and the SFR-dependent MZR across redshifts 4 to 10 using 81 star-forming galaxies observed by the JWST N…

astro-ph.HE2017★ 43 cited

Temperature Structure in the Perseus Cluster Core Observed with Hitomi

Hitomi Collaboration, Felix Aharonian, Hiroki Akamatsu +192

The present paper investigates the temperature structure of the X-ray emitting plasma in the core of the Perseus cluster using the 1.8--20.0 keV data obtained with the Soft X-ray S…

astro-ph.HE2015★ 31 cited

Simulating Astro-H Observations of Sloshing Gas Motions in the Cores of Galaxy Clusters

J. ZuHone, E. Miller, A. Simionescu +1

Astro-H will be the first X-ray observatory to employ a high-resolution microcalorimeter, capable of measuring the shift and width of individual spectral lines to the precision nec…

astro-ph.HE2014★ 23 cited

ASTRO-H White Paper - Clusters of Galaxies and Related Science

T. Kitayama, M. Bautz, M. Markevitch +22

The next generation X-ray observatory ASTRO-H will open up a new dimension in the study of galaxy clusters by achieving for the first time the spectral resolution required to measu…

astro-ph.CO2013★ 52 cited

Robust Quantification of Galaxy Cluster Morphology Using Asymmetry and Central Concentration

D. Nurgaliev, M. McDonald, B. A. Benson +3

We present a novel quantitative scheme of cluster classification based on the morphological properties that are manifested in X-ray images. We use a conventional radial surface bri…

astro-ph2007★ 10 cited

Detection of a Rare Supersoft Outburst Event during a Suzaku Observation of 1E0102.2-7219

D. Takei, M. Tsujimoto, S. Kitamoto +4

We report the detection of a transient X-ray source toward the Small Magellanic Cloud (SMC) using the X-ray Imaging Spectrometer (XIS) onboard the Suzaku telescope. The source was…