Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The Size Evolution of Star-forming and Quenched Galaxies in the IllustrisTNG simulation
As of 24 July 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1707.05327.
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 2026-07-24T06:31:00.690269+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-09T11:06:11.034967Z
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 e500fc1f-f9ea-46e8-ada2-3852c65ff34f · inbound
Probing the faint end of simulated galaxy counts at z>3 cites this paper.
Probing the faint end of simulated galaxy counts at z>3 The Size Evolution of Star-forming and Quenched Galaxies in the IllustrisTNG simulation
Reference 115
- Resolution
- verified exact
- local_arxiv, observed 2026-05-20T18:48:52.905311Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-07-24T06:31:00.690269+00:00.
Observation 6d432d6e-d05d-48a5-8a2b-051aff8c64b8 · 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 Size Evolution of Star-forming and Quenched Galaxies in the IllustrisTNG simulation
Reference 101
- Resolution
- verified exact
- local_arxiv, observed 2026-06-27T16:11:02.237404Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-07-24T06:31:00.690269+00:00.
Observation 9a696849-c7c9-4d44-9c03-8cdec42712e4 · inbound
The MASSIVE SURVEY XXI: Local Variations in the Stellar Initial Mass Function of MASSIVE Early-Type Galaxies cites this paper.
The MASSIVE SURVEY XXI: Local Variations in the Stellar Initial Mass Function of MASSIVE Early-Type Galaxies The Size Evolution of Star-forming and Quenched Galaxies in the IllustrisTNG simulation
Reference 178
- Resolution
- verified exact
- local_arxiv, observed 2026-06-26T00:28:43.489746Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-07-24T06:31:00.690269+00:00.
Observation 5113e971-37f9-48c2-a36f-94321acbe2c9 · inbound
Columba: isolated dwarf galaxy populations in diverse cosmological environments simulated with a cold interstellar medium cites this paper.
Columba: isolated dwarf galaxy populations in diverse cosmological environments simulated with a cold interstellar medium The Size Evolution of Star-forming and Quenched Galaxies in the IllustrisTNG simulation
Reference 148
- Resolution
- verified exact
- local_arxiv, observed 2026-06-27T01:00:20.889493Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-07-24T06:31:00.690269+00:00.
Observation f8d9de0d-0009-4839-a4f0-7c196649a112 · inbound
A machine learning approach to estimating HI deficiency in galaxies cites this paper.
A machine learning approach to estimating HI deficiency in galaxies The Size Evolution of Star-forming and Quenched Galaxies in the IllustrisTNG simulation
Reference 78
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T11:06:11.036207Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-07-24T06:31:00.690269+00:00.