Pith. sign in

Paper Citation Record · LEDGER

A Light Curve Analysis of 32 Recent Galactic Novae --- Distances and White Dwarf Masses

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1905.10655.

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

pith.paper-citation-record.v1
1905.10655 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 2026-08-23T06:30:58.430688+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T05:40:13.808690Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T05:40:16.172431Z

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 f245cdc4-d843-4fc8-8445-2a6e9b14834b · inbound

Identification of recurrent novae from parametric modeling of the optical light curve cites this paper.

Identification of recurrent novae from parametric modeling of the optical light curve A Light Curve Analysis of 32 Recent Galactic Novae --- Distances and White Dwarf Masses

Reference 18

Resolution
malformed identifier
local_arxiv, observed 2026-08-05T05:40:16.293649Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-08-05T05:40:13.808690Z digest=sha256:3337aed97222a58ab281f6bdffb135abd8ddffb51a3d63872f9e3f10a56a40df

Observation cd14e4f7-6204-4b78-bafb-865896328e5b · 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 A Light Curve Analysis of 32 Recent Galactic Novae --- Distances and White Dwarf Masses

Reference 104

Resolution
unresolved
no resolver link, observed 2026-08-01T23:48:02.675967Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T23:48:02.675967Z digest=sha256:1df77a11cc8327623ee8dd382ec225a54bd698bbcd262d9ed925509c2bb1d94d