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researcher

R. Morris

4 papers hereh-index 283.2k citations70 works total

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

author position
  • middle author4

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO3
  • astro-ph.IM1
same name
  • R. Morris — 1 paper, h 2
  • R. Morris — 1 paper, h 15
  • R. Morris — 1 paper, h 2
  • R. Morris — 1 paper, h 6
  • R. Morris — 1 paper, h 4
  • R. Morris — 1 paper, h 31

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

collaborators

4 papers

astro-ph.IM2026

Ruminations Upon the Modeling of X-ray Foregrounds, Backgrounds and Faint Sources

Adam B. Mantz, Anthony M. Flores, Taweewat Somboonpanyakul +4

With the goal of extracting as much information as possible from Chandra and XMM-Newton observations of faint, diffuse sources such as galaxy clusters, as well as those of future X…

astro-ph.CO2026

SPT-CL J0417-4748: A Deep Chandra Study of a Relaxed Galaxy Cluster Without Central Star Formation

Taweewat Somboonpanyakul, Adam B. Mantz, Steven W. Allen +7

We present an in-depth Chandra X-ray analysis of the galaxy cluster SPT-CL J0417−4748 (hereafter SPT J0417), at z = 0.58, with a focus on its thermodynamic properties and the app…

astro-ph.CO2026

Multiwavelength Characterization of a Dynamically Relaxed Cool Core Galaxy Cluster at z=1.5

Anthony M. Flores, Adam B. Mantz, Steven W. Allen +5

We present imaging and spectroscopic analyses of Chandra and XMM-Newton observations of ACT-CL J0123.5−0428, one of the most massive, highest redshift galaxy clusters detected wi…

astro-ph.CO2026

Deep Chandra Observations of the z = 1.16 Relaxed, Cool-core Galaxy Cluster SPT-CL J2215-3537

Haley R. Stueber, Adam B. Mantz, Steven W. Allen +10

Galaxy clusters serve as a unique and valuable laboratory for probing cosmological models and understanding astrophysics at the high-mass limit of structure formation. Clusters tha…

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