Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
IGM damping wing constraints on the tail end of reionisation from the enlarged XQR-30 sample
As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2404.12585.
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 2026-08-06T06:34:29.942622+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-05T20:39:34.135099Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-09T05:26:01.333352Z
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 1f68c4ef-eb02-4e39-a50a-b6b01cc2cbd0 · inbound
Risk-based framework to determine climate-informed design storms for road drainage infrastructure cites this paper.
Risk-based framework to determine climate-informed design storms for road drainage infrastructure IGM damping wing constraints on the tail end of reionisation from the enlarged XQR-30 sample
Reference 63
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T20:39:34.135099Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 44cdca23-b9e3-4bf2-87ff-6c585f803699 · inbound
Into the Gompverse: A robust Gompertzian reionization model for CMB analyses cites this paper.
Into the Gompverse: A robust Gompertzian reionization model for CMB analyses IGM damping wing constraints on the tail end of reionisation from the enlarged XQR-30 sample
Reference 56
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T11:36:03.456728Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation fd555427-423b-4489-8e2e-0b5d7ab0154e · inbound
JWST Constraints on Primordial Magnetic Fields cites this paper.
JWST Constraints on Primordial Magnetic Fields IGM damping wing constraints on the tail end of reionisation from the enlarged XQR-30 sample
Reference 77
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T23:11:17.225008Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 9b7ccb3c-f204-4999-b7a6-aa68071d8800 · inbound
A self-consistent analytical model for both the photoionization rate and reionization history cites this paper.
A self-consistent analytical model for both the photoionization rate and reionization history IGM damping wing constraints on the tail end of reionisation from the enlarged XQR-30 sample
Reference 16
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T02:29:23.557653Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation d4671434-452b-40ba-9c5e-10e48fd0be9a · inbound
Gamma-ray bursts reveal the history and faint contributors of cosmic reionization cites this paper.
Gamma-ray bursts reveal the history and faint contributors of cosmic reionization IGM damping wing constraints on the tail end of reionisation from the enlarged XQR-30 sample
Reference 130
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-07-09T05:26:01.336619Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 777472b9-c1a2-43aa-bae6-b4da22c61547 · inbound
No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization cites this paper.
No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization IGM damping wing constraints on the tail end of reionisation from the enlarged XQR-30 sample
Reference 33
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T17:17:52.898047Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a3d28855-2aab-432e-9406-2053d1564eb3 · inbound
No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization cites this paper.
No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization IGM damping wing constraints on the tail end of reionisation from the enlarged XQR-30 sample
Reference 33
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T03:21:45.484754Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.