Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-11T22:20:40.065029Z
Paper Citation Record · LEDGER
The Growth of Galaxy Stellar Haloes Over $0.2 \leq z \leq 1.1$
As of 14 August 2026, this Paper Citation Record lists 2 of 2 outbound references and 1 inbound Pith citation observation for arXiv:2412.03662.
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 2026-08-05T05:22:21.386491Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-10T05:30:23.456663Z
Reference resolution
2 of 2 outbound references displayed
- verified exact1
- verified fuzzy0
- unresolved1
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
0
pith, observed 2026-08-10T05:30:23.456663Z
Outbound references
Observation 50b54c08-7c7b-46ae-a33f-a3e7a477e947 · outbound
This paper cites 2018, PASJ, 70, S4, doi: 10.1093/pasj/psx066 Aihara, H., AlSayyad, Y ., Ando, M., et al.
The Growth of Galaxy Stellar Haloes Over $0.2 \leq z \leq 1.1$ 2018, PASJ, 70, S4, doi: 10.1093/pasj/psx066 Aihara, H., AlSayyad, Y ., Ando, M., et al
Reference 1
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T22:20:40.059267Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6163e0bb-10d2-40a1-8ce2-fc8898dc45bd · outbound
This paper cites Data points are placed in the center of our four redshift ranges (Table 2).
The Growth of Galaxy Stellar Haloes Over $0.2 \leq z \leq 1.1$ Data points are placed in the center of our four redshift ranges (Table 2)
Reference 17
- Resolution
- verified exact
- arxiv_id_nonexistent, observed 2026-08-11T22:20:40.150119Z
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.
Pith citing papers
Observation c1e2e3ad-996c-4ffd-b701-cc754afe2f91 · inbound
Evolution of the Physical Properties of the Most Massive Galaxies in Clusters and their Protohalos cites this paper.
Evolution of the Physical Properties of the Most Massive Galaxies in Clusters and their Protohalos The Growth of Galaxy Stellar Haloes Over $0.2 \leq z \leq 1.1$
Reference 82
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-08-05T05:22:21.924162Z
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.