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Paper Citation Record · LEDGER

The sizes, masses and specific star-formation rates of massive galaxies at 1.3<z<1.5: strong evidence in favour of evolution via minor mergers

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1205.4058.

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

pith.paper-citation-record.v1
1205.4058 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T15:07:32.078548Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-27T06:40:38.488987Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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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 82786121-df9c-4608-83ec-403cb09b3382 · inbound

Galaxy clusters in the VIDEO fields: detection and characterisation in the context of MOONRISE cites this paper.

Galaxy clusters in the VIDEO fields: detection and characterisation in the context of MOONRISE The sizes, masses and specific star-formation rates of massive galaxies at 1.3<z<1.5: strong evidence in favour of evolution via minor mergers

Reference 19

Resolution
verified exact
local_arxiv, observed 2026-06-27T06:40:38.490411Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:83ec798f2b3cc24735dbca43d1e740e0f8220c88949f256d297f17be9e4911f0

Observation 922f4e12-9b60-4e8d-af20-6bca5b322419 · inbound

No hidden monsters: Probing recently-quenched galaxies for obscured AGN with JWST-PRIMER MIRI and NIRCam cites this paper.

No hidden monsters: Probing recently-quenched galaxies for obscured AGN with JWST-PRIMER MIRI and NIRCam The sizes, masses and specific star-formation rates of massive galaxies at 1.3<z<1.5: strong evidence in favour of evolution via minor mergers

Reference 57

Resolution
verified exact
local_arxiv, observed 2026-06-26T16:39:35.510429Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:cb366c242794a990ed89207967029c93d97013af437a773a4f840b1b9d5cc6ef

Observation a926ad8b-b4fa-41dc-a525-ad55174aa1d0 · inbound

Weak-lensing Shear-Selected Galaxy Clusters from the Hyper Suprime-Cam Subaru Strategic Program: III. A precision cosmological sample enabled by optical confirmation cites this paper.

Weak-lensing Shear-Selected Galaxy Clusters from the Hyper Suprime-Cam Subaru Strategic Program: III. A precision cosmological sample enabled by optical confirmation The sizes, masses and specific star-formation rates of massive galaxies at 1.3<z<1.5: strong evidence in favour of evolution via minor mergers

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-15T15:07:32.078548Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:07:32.078548Z digest=sha256:67f938f29bc8e2cd909513c08dd35a06f3cf0ca313bf57db35d2d8e41563a802