Paper Citation Record · LEDGER

Half-mass radii for ~7,000 galaxies at 1.0 < z < 2.5: most of the evolution in the mass-size relation is due to color gradients

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1904.10992.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
1904.10992 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T14:56:46.589654Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-07-01T05:45:26.435236Z

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation f15c5712-539e-47fb-b158-1613d26558ab · inbound

Evidence for Inside-Out Galaxy Growth and Quenching of a z~2 Compact Galaxy from High-Resolution Molecular Gas Imaging cites this paper.

Evidence for Inside-Out Galaxy Growth and Quenching of a z~2 Compact Galaxy from High-Resolution Molecular Gas Imaging Half-mass radii for ~7,000 galaxies at 1.0 < z < 2.5: most of the evolution in the mass-size relation is due to color gradients

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-14T14:56:46.589654Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8cb02a16-2012-4b57-939e-0cd9fa18c8b4 · inbound

Witnessing the rapid growth of disk galaxies over cosmic time using JWST and HST cites this paper.

Witnessing the rapid growth of disk galaxies over cosmic time using JWST and HST Half-mass radii for ~7,000 galaxies at 1.0 < z < 2.5: most of the evolution in the mass-size relation is due to color gradients

Reference 152

Resolution: verified exact; local_arxiv, observed 2026-05-19T15:27:38.428079Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 46115b74-64a6-4853-9943-4b5314bcf73e · inbound

Morphology, sizes, and scatter in a large sample of distant quiescent galaxies cites this paper.

Morphology, sizes, and scatter in a large sample of distant quiescent galaxies Half-mass radii for ~7,000 galaxies at 1.0 < z < 2.5: most of the evolution in the mass-size relation is due to color gradients

Reference 125

Resolution: metadata mismatch; local_arxiv, observed 2026-06-27T13:50:57.851939Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 0c6cef98-7cc8-4081-aa09-d2609dc71775 · inbound

A big step forward with SHARP: spatially resolved stellar population properties in passive galaxies at z > 1.5 cites this paper.

A big step forward with SHARP: spatially resolved stellar population properties in passive galaxies at z > 1.5 Half-mass radii for ~7,000 galaxies at 1.0 < z < 2.5: most of the evolution in the mass-size relation is due to color gradients

Reference 22

Resolution: verified exact; local_arxiv, observed 2026-07-01T05:45:26.437121Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.