Publication data of Hallman, Eric J.:
Link to Inspire
Created with Highcharts 9.0.1
Citations
Citations
w/o self-citaion
self-citaion
2010
2020
2005
2015
2025
0
250
500
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1750
Created with Highcharts 9.0.1
Publications
publications per year
Publications
Publications per year
Cumulative publications
2010
2020
2005
2015
2025
0
8
16
24
32
40
0
1
2
3
4
5
Created with Highcharts 9.0.1
h-index
h-index
h-index
h-index w/o self-citaion
2002
2004
2006
2008
2010
2012
2014
2016
2018
2020
2022
2024
0
5
10
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20
Created with Highcharts 9.0.1
Citations
Breakdown of Most Cited Papers
rest
On the Origin of Cool Core Galaxy Clusters: Comparing X-Ray Observations with Numerical Simulations
On the Origin of Cool Core Galaxy Clusters: Comparing X-Ray Observations wit…
Structure and Turbulence in Simulated Galaxy Clusters and the Implications for the Formation of Radio Halos
Structure and Turbulence in Simulated Galaxy Clusters and the Implications f…
Probing the Curious Case of a Galaxy Cluster Merger in Abell 115 with High Fidelity Chandra X-ray Temperature and Radio Maps
Probing the Curious Case of a Galaxy Cluster Merger in Abell 115 with High Fi…
How Much can we Learn From a Merging Cold Front Cluster? Insights From X-ray Temperature and Radio Maps of A3667
How Much can we Learn From a Merging Cold Front Cluster? Insights From X-…
Simulating X-ray Observations with Python
X-ray Point Sources and Radio Galaxies in Clusters of Galaxies
Challenges for Precision Cosmology with X-ray and Sunyaev-Zeldovich Effect Gas Mass Measurements of Galaxy Clusters
Challenges for Precision Cosmology with X-ray and Sunyaev-Zeldovich Effect …
How well do cosmological simulations reproduce individual-halo properties?
The Beta-Model Problem: The Incompatibility of X-ray and Sunyaev-Zeldovich Effect Model Fitting for Galaxy Clusters
The Beta-Model Problem: The Incompatibility of X-ray and Sunyaev-Zeldovich …
Chandra observation of the merging cluster A168: A Late stage in the evolution of a cold front
Chandra observation of the merging cluster A168: A Late stage in the evoluti…
Galaxy Cluster Radio Relics in Adaptive Mesh Refinement Cosmological Simulations: Relic Properties and Scaling Relationships
Galaxy Cluster Radio Relics in Adaptive Mesh Refinement Cosmological Simula…
The Santa Fe Light Cone Simulation Project: I. Confusion and the WHIM in Upcoming Sunyaev-Zel'dovich Effect Surveys
The Santa Fe Light Cone Simulation Project: I. Confusion and the WHIM in Up…
Cluster Structure in Cosmological Simulations I: Correlation to Observables, Mass Estimates, and Evolution
Cluster Structure in Cosmological Simulations I: Correlation to Observables, M…
The Nature of the Warm/Hot Intergalactic Medium I. Numerical Methods, Convergence, and OVI Absorption
The Nature of the Warm/Hot Intergalactic Medium I. Numerical Methods, Con…
Cosmological MHD Simulations of Galaxy Cluster Radio Relics: Insights and Warnings for Observations
Cosmological MHD Simulations of Galaxy Cluster Radio Relics: Insights and W…
Why Do Only Some Galaxy Clusters Have Cool Cores?
Cosmological Shocks in Adaptive Mesh Refinement Simulations and the Acceleration of Cosmic Rays
Cosmological Shocks in Adaptive Mesh Refinement Simulations and the Accel…
The Integrated Sunyaev-Zeldovich effect as the superior method for measuring the mass of clusters of galaxies
The Integrated Sunyaev-Zeldovich effect as the superior method for measuri…
Cosmological shock waves and their role in the large scale structure of the universe
Cosmological shock waves and their role in the large scale structure of the u…
2010
2020
2005
2015
2025
0
250
500
750
1000
1250
1500
1750
Created with Highcharts 9.0.1
Fraction [%]
Breakdown of Most Cited Papers (Fraction)
On the Origin of Cool Core Galaxy Clusters: Comparing X-Ray Observations with Numerical Simulations
On the Origin of Cool Core Galaxy Clusters: Comparing X-Ray Observations wit…
Structure and Turbulence in Simulated Galaxy Clusters and the Implications for the Formation of Radio Halos
Structure and Turbulence in Simulated Galaxy Clusters and the Implications f…
Probing the Curious Case of a Galaxy Cluster Merger in Abell 115 with High Fidelity Chandra X-ray Temperature and Radio Maps
Probing the Curious Case of a Galaxy Cluster Merger in Abell 115 with High Fi…
How Much can we Learn From a Merging Cold Front Cluster? Insights From X-ray Temperature and Radio Maps of A3667
How Much can we Learn From a Merging Cold Front Cluster? Insights From X-…
Simulating X-ray Observations with Python
X-ray Point Sources and Radio Galaxies in Clusters of Galaxies
Challenges for Precision Cosmology with X-ray and Sunyaev-Zeldovich Effect Gas Mass Measurements of Galaxy Clusters
Challenges for Precision Cosmology with X-ray and Sunyaev-Zeldovich Effect …
How well do cosmological simulations reproduce individual-halo properties?
The Beta-Model Problem: The Incompatibility of X-ray and Sunyaev-Zeldovich Effect Model Fitting for Galaxy Clusters
The Beta-Model Problem: The Incompatibility of X-ray and Sunyaev-Zeldovich …
Chandra observation of the merging cluster A168: A Late stage in the evolution of a cold front
Chandra observation of the merging cluster A168: A Late stage in the evoluti…
Galaxy Cluster Radio Relics in Adaptive Mesh Refinement Cosmological Simulations: Relic Properties and Scaling Relationships
Galaxy Cluster Radio Relics in Adaptive Mesh Refinement Cosmological Simula…
The Santa Fe Light Cone Simulation Project: I. Confusion and the WHIM in Upcoming Sunyaev-Zel'dovich Effect Surveys
The Santa Fe Light Cone Simulation Project: I. Confusion and the WHIM in Up…
Cluster Structure in Cosmological Simulations I: Correlation to Observables, Mass Estimates, and Evolution
Cluster Structure in Cosmological Simulations I: Correlation to Observables, M…
The Nature of the Warm/Hot Intergalactic Medium I. Numerical Methods, Convergence, and OVI Absorption
The Nature of the Warm/Hot Intergalactic Medium I. Numerical Methods, Con…
Cosmological MHD Simulations of Galaxy Cluster Radio Relics: Insights and Warnings for Observations
Cosmological MHD Simulations of Galaxy Cluster Radio Relics: Insights and W…
Why Do Only Some Galaxy Clusters Have Cool Cores?
Cosmological Shocks in Adaptive Mesh Refinement Simulations and the Acceleration of Cosmic Rays
Cosmological Shocks in Adaptive Mesh Refinement Simulations and the Accel…
The Integrated Sunyaev-Zeldovich effect as the superior method for measuring the mass of clusters of galaxies
The Integrated Sunyaev-Zeldovich effect as the superior method for measuri…
Cosmological shock waves and their role in the large scale structure of the universe
Cosmological shock waves and their role in the large scale structure of the u…
2002
2004
2006
2008
2010
2012
2014
2016
2018
2020
2022
2024
0
25
50
75
100
Created with Highcharts 9.0.1
Citations/1 Year
Citations/Period
Citations / 1 Year
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