Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Predicting dark matter halo masses from simulated galaxy images and environments
As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2407.13735.
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 2026-08-08T06:32:00.761636+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T10:27:43.212921Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
0
arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 5b3d9d53-f17b-4da3-8eca-72ec5c5e518e · inbound
Learning Intrinsic Alignments from Local Galaxy Environments cites this paper.
Learning Intrinsic Alignments from Local Galaxy Environments Predicting dark matter halo masses from simulated galaxy images and environments
Reference 43
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T10:27:43.212921Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 34138d5e-ff91-4461-9bf1-592838f3b907 · inbound
Estimating the triaxiality of massive clusters from 2D observables in MillenniumTNG with machine learning cites this paper.
Estimating the triaxiality of massive clusters from 2D observables in MillenniumTNG with machine learning Predicting dark matter halo masses from simulated galaxy images and environments
Reference 31
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T04:31:31.229755Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation 1a44d538-f20d-41d1-af9c-7a478678f911 · inbound
Cluster Mass Inference from Galaxy Kinematics cites this paper.
Cluster Mass Inference from Galaxy Kinematics Predicting dark matter halo masses from simulated galaxy images and environments
Reference 2
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-06-27T07:30:41.956246Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.