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Paper Citation Record · LEDGER

XMM-Newton X-ray and UV observations of the fast nova V2491 Cyg during the supersoft source phase

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1103.4543.

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

pith.paper-citation-record.v1
1103.4543 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 2026-08-11T06:34:44.6726+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T23:47:56.840950Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-22T05:31:07.436899Z

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 3ffdeb13-3d77-4d3e-be70-c64b3b997103 · inbound

The powerful shocks in RS Oph: NuSTAR X-ray data and a complete review cites this paper.

The powerful shocks in RS Oph: NuSTAR X-ray data and a complete review XMM-Newton X-ray and UV observations of the fast nova V2491 Cyg during the supersoft source phase

Reference 233

Resolution
verified exact
local_arxiv, observed 2026-05-22T05:31:07.439823Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:bf116c18b0c9182c6cfb52d80230ceec7ea9d18b49da85a6fe56733b667959f1

Observation a5142d82-369a-45af-9e17-eeb96cb7e72f · inbound

When will T Coronae Borealis next erupt as a nova? Constraints from recurrence, orbital phase, and accretion-state evolution cites this paper.

When will T Coronae Borealis next erupt as a nova? Constraints from recurrence, orbital phase, and accretion-state evolution XMM-Newton X-ray and UV observations of the fast nova V2491 Cyg during the supersoft source phase

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-01T23:47:56.840950Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T23:47:56.840950Z digest=sha256:8b45d141c6eb52f535b3f620db7f35c05fb921810f14a833180d5fc4a6b8bf6d