Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Galaxy evolution in the post-merger regime I -- Most merger-induced in-situ stellar mass growth happens post-coalescence
As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2410.06356.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-09T18:33:39.734780Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-10T05:30:23.456663Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
0
pith, observed 2026-08-10T05:30:23.456663Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 931e6255-235c-4d55-96f3-8bb752098e5b · inbound
Unions with UNIONS: Using galaxy-galaxy lensing to probe galaxy mergers cites this paper.
Unions with UNIONS: Using galaxy-galaxy lensing to probe galaxy mergers Galaxy evolution in the post-merger regime I -- Most merger-induced in-situ stellar mass growth happens post-coalescence
Reference 23
- Resolution
- unresolved
- no resolver link, observed 2026-08-09T18:33:39.734780Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c80c90e3-834e-44b8-b6af-1de40ab6fe5d · inbound
The connection between galaxy mergers, star formation and AGN activity in the HSC-SSP cites this paper.
The connection between galaxy mergers, star formation and AGN activity in the HSC-SSP Galaxy evolution in the post-merger regime I -- Most merger-induced in-situ stellar mass growth happens post-coalescence
Reference 50
- Resolution
- verified exact
- local_arxiv, observed 2026-08-07T05:19:18.243599Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation ff5ef6a9-1109-4fbd-a683-86ed292290ed · inbound
Beyond the Brightest: A Deep Learning Approach to Identifying Major and Minor Galaxy Mergers in CANDELS at $z \sim 1$ cites this paper.
Beyond the Brightest: A Deep Learning Approach to Identifying Major and Minor Galaxy Mergers in CANDELS at $z \sim 1$ Galaxy evolution in the post-merger regime I -- Most merger-induced in-situ stellar mass growth happens post-coalescence
Reference 31
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T10:03:47.754344Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.