Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The stellar mass assembly of galaxies in the Illustris simulation: growth by mergers and the spatial distribution of accreted stars
As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1511.08804.
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 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T16:49:18.371306Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-27T16:11:01.860383Z
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 3a426fb0-e6ca-4d72-9628-fce3fe86f88a · inbound
Satellite compaction pathways: environmental drivers shaping dwarf galaxy corpulence in the TNG50 simulation cites this paper.
Satellite compaction pathways: environmental drivers shaping dwarf galaxy corpulence in the TNG50 simulation The stellar mass assembly of galaxies in the Illustris simulation: growth by mergers and the spatial distribution of accreted stars
Reference 185
- Resolution
- verified exact
- local_arxiv, observed 2026-06-27T16:11:01.861710Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation a3d4ce8f-9728-4a0e-a9d4-b47ac476e90a · inbound
How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy cites this paper.
How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy The stellar mass assembly of galaxies in the Illustris simulation: growth by mergers and the spatial distribution of accreted stars
Reference 18
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T23:42:32.818073Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 33a69da0-a008-4da3-816d-6beaa085c242 · inbound
Inflow-driven galaxy evolution - I. Revealing the physics of the fundamental metallicity relation cites this paper.
Inflow-driven galaxy evolution - I. Revealing the physics of the fundamental metallicity relation The stellar mass assembly of galaxies in the Illustris simulation: growth by mergers and the spatial distribution of accreted stars
Reference 225
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T16:49:18.371306Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.