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Observing positive and negative AGN feedback

3 Pith papers cite this work, alongside 77 external citations. Polarity classification is still indexing.

3 Pith papers citing it
77 external citations · OpenAlex

citation-role summary

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citation-polarity summary

years

2026 2 2019 1

verdicts

UNVERDICTED 3

roles

background 1

polarities

background 1

representative citing papers

Extragalactic astrophysics with next-generation CMB experiments

astro-ph.GA · 2019-07-11 · unverdicted · novelty 3.0

Next-generation CMB experiments are expected to detect thousands of strongly lensed galaxies to z~6 and proto-clusters, plus tens of thousands of local dusty galaxies and radio sources, enabling new studies of galaxy formation.

The Large-Scale Structure of the Universe through the SKA lenses

astro-ph.CO · 2026-06-30 · unverdicted · novelty 1.0

This review chapter summarizes the cosmic web's theoretical framework, recent radio observations of diffuse gas, and the expected impact of the SKA on detecting baryons in filaments and cluster outskirts.

citing papers explorer

Showing 3 of 3 citing papers.

  • Kinematic Stratification in Extremely Red Quasars Revealed by JWST astro-ph.GA · 2026-05-06 · unverdicted · none · ref 95

    JWST observations of ERQs show stratified gas kinematics via deblended optical emission lines, with UV lines dominated by scattered light and optical lines mixing scattered and obscured emission.

  • Extragalactic astrophysics with next-generation CMB experiments astro-ph.GA · 2019-07-11 · unverdicted · none · ref 54

    Next-generation CMB experiments are expected to detect thousands of strongly lensed galaxies to z~6 and proto-clusters, plus tens of thousands of local dusty galaxies and radio sources, enabling new studies of galaxy formation.

  • The Large-Scale Structure of the Universe through the SKA lenses astro-ph.CO · 2026-06-30 · unverdicted · none · ref 54

    This review chapter summarizes the cosmic web's theoretical framework, recent radio observations of diffuse gas, and the expected impact of the SKA on detecting baryons in filaments and cluster outskirts.