Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Introducing the NewHorizon simulation: Galaxy properties with resolved internal dynamics across cosmic time
As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2009.10578.
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 2026-08-05T06:32:48.257954+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-04T22:14:26.146015Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-04T22:14:34.286970Z
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 2ab6ed86-4695-47a1-8d3c-ab924b822c7d · inbound
Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps cites this paper.
Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Introducing the NewHorizon simulation: Galaxy properties with resolved internal dynamics across cosmic time
Reference 50
- Resolution
- verified exact
- local_arxiv, observed 2026-08-04T22:14:34.308141Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.
Observation e2098a52-fc33-4ca3-ac59-e64c5064c18c · inbound
Outflows in super-Eddington quasars drive clumpy circumgalactic medium and extended H$\alpha$ nebulae at $z \gtrsim 6$ cites this paper.
Outflows in super-Eddington quasars drive clumpy circumgalactic medium and extended H$\alpha$ nebulae at $z \gtrsim 6$ Introducing the NewHorizon simulation: Galaxy properties with resolved internal dynamics across cosmic time
Reference 53
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T06:58:37.766881Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.