Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The disc instability model of dwarf-novae and low-mass X-ray binary transients
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:astro-ph/0102072.
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 2026-07-12T03:29:42.101488Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-03T23:59:05.570644Z
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 8f4a611d-3205-4936-a6eb-f2c23b61cc95 · inbound
Pulse profile modelling of the 2024 outburst of the accreting millisecond pulsar SRGA J144459.2-604207 cites this paper.
Pulse profile modelling of the 2024 outburst of the accreting millisecond pulsar SRGA J144459.2-604207 The disc instability model of dwarf-novae and low-mass X-ray binary transients
Reference 5
- Resolution
- verified exact
- local_arxiv, observed 2026-05-20T08:58:09.683987Z
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 15ffef8f-7fa6-454f-adf7-a944bee6b4b5 · inbound
On the origin of anomalous dissipation in simulations of tidal disruption events cites this paper.
On the origin of anomalous dissipation in simulations of tidal disruption events The disc instability model of dwarf-novae and low-mass X-ray binary transients
Reference 154
- Resolution
- verified exact
- local_arxiv, observed 2026-05-21T01:23:53.771793Z
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 41fa5a3e-e6fd-4cbb-a202-1d9d917d51f0 · inbound
A micronova burst in the intermediate polar IGR J17014-4306 cites this paper.
A micronova burst in the intermediate polar IGR J17014-4306 The disc instability model of dwarf-novae and low-mass X-ray binary transients
Reference 300
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T00:31:26.455901Z
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 6e4bde75-6506-4669-b775-c0ac680ba174 · inbound
Balmer decrements as a new diagnostic for period-bounce Cataclysmic Variable stars cites this paper.
Balmer decrements as a new diagnostic for period-bounce Cataclysmic Variable stars The disc instability model of dwarf-novae and low-mass X-ray binary transients
Reference 21
- Resolution
- verified exact
- local_arxiv, observed 2026-06-27T15:00:59.340069Z
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 08b0a9a3-2816-43cd-be7c-e078eb62b053 · inbound
Discovery of EP J175257.3-351923 as a Candidate Black Hole Low-Mass X-ray Binary cites this paper.
Discovery of EP J175257.3-351923 as a Candidate Black Hole Low-Mass X-ray Binary The disc instability model of dwarf-novae and low-mass X-ray binary transients
Reference 4
- Resolution
- verified exact
- local_arxiv, observed 2026-06-27T13:30:57.337849Z
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 47a43269-1ca6-4257-bfb4-8daa65b449ad · inbound
Discovery of EP J175257.3-351923 as a Candidate Black Hole Low-Mass X-ray Binary cites this paper.
Discovery of EP J175257.3-351923 as a Candidate Black Hole Low-Mass X-ray Binary The disc instability model of dwarf-novae and low-mass X-ray binary transients
Reference 4
- Resolution
- verified exact
- local_arxiv, observed 2026-07-03T23:59:05.572643Z
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 1a76a6a6-0c87-4df8-baa4-203eaf2d86d3 · inbound
Physically motivated AGN emissivity profiles and their effects on quasar microlensing signatures. 1. Multi-epoch accretion disc size inference cites this paper.
Physically motivated AGN emissivity profiles and their effects on quasar microlensing signatures. 1. Multi-epoch accretion disc size inference The disc instability model of dwarf-novae and low-mass X-ray binary transients
Reference 295
- Resolution
- unresolved
- no resolver link, observed 2026-07-12T03:29:42.101488Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.