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Paper Citation Record · LEDGER

A helium-burning white dwarf binary as a supersoft X-ray source

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2303.13338.

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

pith.paper-citation-record.v1
2303.13338 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 2026-08-07T13:46:15.934747Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-07T13:46:24.694422Z

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 5185131b-5998-40e6-b000-e9cf7fbc0dab · inbound

What triggers type Ia supernovae: Prompt detonations from primordial black holes or companion stars? cites this paper.

What triggers type Ia supernovae: Prompt detonations from primordial black holes or companion stars? A helium-burning white dwarf binary as a supersoft X-ray source

Reference 7

Resolution
verified exact
local_arxiv, observed 2026-08-07T13:46:24.756723Z

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=2026-08-07T13:46:15.934747Z digest=sha256:321e740270e7b6a9d0f9b4870324d247d3055ae5c79357311097ab01ff05c5a7

Observation 1243e070-f10e-4e88-aac2-c598835bd275 · inbound

eRASSU J043115.8-711730 :the first pulsating symbiotic super-soft X-ray source in the Magellanic Bridge cites this paper.

eRASSU J043115.8-711730 :the first pulsating symbiotic super-soft X-ray source in the Magellanic Bridge A helium-burning white dwarf binary as a supersoft X-ray source

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-01T02:32:27.492735Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T02:32:27.492735Z digest=sha256:ff5b7c66e8d3ac4bf687b9122336cde0b2499bc9140a740f8e90660d50e443bb