Pith. sign in

REVIEW 1 cited by

Mass profiles of Galaxy Clusters from X-ray analysis

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1303.3530 v2 pith:IVJ2KX7U submitted 2013-03-14 astro-ph.CO

S. Ettori , A. Donnarumma , E. Pointecouteau , T.H. Reiprich , S. Giodini , L. Lovisari , R.W. Schmidt This is my paper
classification astro-ph.CO
keywords massprofilesclustersgalaxyx-rayadoptedaffectinganalysis
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

We review the methods adopted to reconstruct the mass profiles in X-ray luminous galaxy clusters. We discuss the limitations and the biases affecting these measurements and how these mass profiles can be used as cosmological proxies.

Discussion (0). Sign in to comment.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Exploring the physics of ram pressure stripping with radio continuum observations in the SKA era

    astro-ph.GA 2026-06 unverdicted novelty 2.0 of 10

    Perspective on using SKA-Low and SKA-Mid radio continuum to extend ram pressure stripping studies to southern clusters and z~0.5.

Pith tools