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H. Eckmiller

3 papers hereh-index 3144 citations3 works total

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

author position
  • first author1
  • middle author1
  • last author1

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

fields
  • astro-ph.CO3

identity via Semantic Scholar / OpenAlex

most citedTesting the Low-Mass End of X-Ray Scaling Relations with a Sample of Chandra Galaxy Groups

132 citations · 192 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.CO2014★ 29 cited

Extending the LX​−T relation from clusters to groups-Impact of cool core nature, AGN feedback, and selection effects

V. Bharadwaj, T. H. Reiprich, L. Lovisari +1

We aim to investigate the bolometric LX​−T relation for galaxy groups, and study the impact of gas cooling, feedback from supermassive black holes, and selection effec…

astro-ph.CO2014★ 31 cited

ICM cooling, AGN feedback and BCG properties of galaxy groups-Five properties where groups differ from clusters

V. Bharadwaj, T. H. Reiprich, G. Schellenberger +3

Using Chandra data for a sample of 26 galaxy groups, we constrained the central cooling times (CCTs) of the ICM and classified the groups as strong cool-core (SCC), weak cool-core…

astro-ph.CO2011★ 132 cited

Testing the Low-Mass End of X-Ray Scaling Relations with a Sample of Chandra Galaxy Groups

H. J. Eckmiller, D. S. Hudson, T. H. Reiprich

Well-determined scaling relations between X-ray observables and cluster mass are essential for using large cluster samples for cosmology. Cluster relations such as the Lx-T, M-T, L…

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