Pith. sign in

REVIEW 1 cited by

Ten Billion Years of Brightest Cluster Galaxy Alignments

Not yet reviewed by Pith; the record is open.

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 1706.03798 v1 pith:IVAGTKRG submitted 2017-06-12 astro-ph.GA

classification astro-ph.GA
keywords galaxiesgalaxyclustersalignmentsbrightestorientationspaceyears
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

A galaxy's orientation is one of its most basic observable properties. Astronomers once assumed that galaxies are randomly oriented in space, however it is now clear that some have preferred orientations with respect to their surroundings. Chief among these are giant elliptical galaxies found in the centers of rich galaxy clusters. Numerous studies have shown that the major axes of these galaxies often share the same orientation as the surrounding matter distribution on larger scales. Using Hubble Space Telescope observations of 65 distant galaxy clusters, we show for the first time that similar alignments are seen at earlier epochs when the universe was only one-third its current age. These results suggest that the brightest galaxies in clusters are the product of a special formation history, one influenced by development of the cosmic web over billions of years.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 43 citations worldwide. Full citation record

  1. S-PLUS Clusters And Large-scale Environments (SCALE): I. A catalog of known clusters and groups in DR5 and a pilot study of Abell 4038

    astro-ph.CO 2026-07 conditional novelty 5.0 of 10

    SCALE delivers dynamical properties for 83 known z≤0.1 systems and uses S-PLUS photo-zs plus RPM to map Abell 4038 substructure and mass-dependent color-concentration trends.

Pith tools