Paper Citation Record · LEDGER

Galaxy And Mass Assembly (GAMA): mass-size relations of z$<$0.1 galaxies subdivided by S\'ersic index, colour and morphology

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1411.6355.

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

pith.paper-citation-record.v1
1411.6355 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 2026-08-13T06:32:02.005865+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T00:51:08.109116Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-19T15:27:38.076163Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 9dec4b33-ba19-49d6-a3b9-61a98cf6fdbd · inbound

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations cites this paper.

Accuracy of analytic potentials for orbits of satellites around a Milky Way-like galaxy: comparison with $N$-body simulations Galaxy And Mass Assembly (GAMA): mass-size relations of z$<$0.1 galaxies subdivided by S\'ersic index, colour and morphology

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-07T00:51:08.109116Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 43820f26-0c55-4856-9f1a-21cf37ed28e8 · inbound

Empirical estimates of how massive galaxies can be in {\Lambda}CDM cites this paper.

Empirical estimates of how massive galaxies can be in {\Lambda}CDM Galaxy And Mass Assembly (GAMA): mass-size relations of z$<$0.1 galaxies subdivided by S\'ersic index, colour and morphology

Reference 186

Resolution: verified exact; local_arxiv, observed 2026-05-14T21:09:28.298489Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 1743413f-3df2-4ec5-8451-496d2dd28ce2 · 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 Galaxy And Mass Assembly (GAMA): mass-size relations of z$<$0.1 galaxies subdivided by S\'ersic index, colour and morphology

Reference 146

Resolution: verified exact; local_arxiv, observed 2026-05-19T15:27:38.079998Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation e8aeee9b-e05b-4f12-b125-6a42ac6e0dad · inbound

RABBITS IV: Stellar feedback and SMBH merging time-scales in the sub-Milky Way mass regime cites this paper.

RABBITS IV: Stellar feedback and SMBH merging time-scales in the sub-Milky Way mass regime Galaxy And Mass Assembly (GAMA): mass-size relations of z$<$0.1 galaxies subdivided by S\'ersic index, colour and morphology

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-02T03:50:08.521607Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.