Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-05-08T02:26:08.629982Z
Paper Citation Record · LEDGER
The evolution of the baryonic content and mass profiles of satellite galaxies in the MTNG simulations
As of 4 August 2026, this Paper Citation Record lists 2 of 2 outbound references and 1 inbound Pith citation observation for arXiv:2604.24837.
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 2026-08-04T06:34:03.388597+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-31T23:49:19.641308Z
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
2 of 2 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier1
- metadata mismatch1
External citation measurements
No source-named external measurement is stored.
Outbound references
Observation 7c369a9e-2c47-46d9-9e07-b55976a48630 · outbound
This paper cites The tidal evolution of satellite galaxies in cosmological simulations: insights from COLIBRE.
The evolution of the baryonic content and mass profiles of satellite galaxies in the MTNG simulations The tidal evolution of satellite galaxies in cosmological simulations: insights from COLIBRE
Reference 1
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-05-11T22:46:13.227641Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation b4bc0f4b-7d27-40c3-a46a-26b8bce8e537 · outbound
This paper cites We find that, by using the same pa- rameterisation as forv max/vinfall, we can recover the evolution of most properties almost perfectly.
The evolution of the baryonic content and mass profiles of satellite galaxies in the MTNG simulations We find that, by using the same pa- rameterisation as forv max/vinfall, we can recover the evolution of most properties almost perfectly
Reference 2
- Resolution
- malformed identifier
- raw_fallback, observed 2026-05-26T23:08:11.881303Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Pith citing papers
Observation 8210df7f-6d1d-4a4b-8f6e-25a9499e39d3 · inbound
Interpreting the stacked kinetic SZ effect I: velocity reconstruction and non-linear velocity effects cites this paper.
Interpreting the stacked kinetic SZ effect I: velocity reconstruction and non-linear velocity effects The evolution of the baryonic content and mass profiles of satellite galaxies in the MTNG simulations
Reference 34
- Resolution
- unresolved
- no resolver link, observed 2026-07-31T23:49:19.641308Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.