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Paper Citation Record · LEDGER

The origin of optical emission lines in the soft state of X-ray binary outbursts: the case of MAXI J1820+070

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2303.09242.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2303.09242 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T16:32:32.104274Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-08-06T18:25:20.819311Z

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 614a0862-0a5d-49cc-b8b4-e66857082639 · inbound

XMM-Newton follow-up of two eROSITA X-ray binary candidates cites this paper.

XMM-Newton follow-up of two eROSITA X-ray binary candidates The origin of optical emission lines in the soft state of X-ray binary outbursts: the case of MAXI J1820+070

Reference 90

Resolution
verified exact
local_arxiv, observed 2026-08-06T18:25:20.822586Z

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.

source=pdf_text observed=2026-08-06T18:24:55.933463Z digest=sha256:de393d3b57874899a9de6a2d2ce7ecd2f6c87b264b9cb179037d0c5549144cc3

Observation 7d3eb68b-6b32-4d8f-97c2-581056194f7b · inbound

A Galactic intermediate-mass stripped star with a Wolf-Rayet-like wind cites this paper.

A Galactic intermediate-mass stripped star with a Wolf-Rayet-like wind The origin of optical emission lines in the soft state of X-ray binary outbursts: the case of MAXI J1820+070

Reference 196

Resolution
unresolved
no resolver link, observed 2026-08-08T16:32:32.104274Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T16:32:32.104274Z digest=sha256:9cb8e9a5e21e64ab6cfa66277460c3144eaf54e7495f81d22949f23d7207ffde