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Paper Citation Record · LEDGER

Formation and Destiny of White Dwarf and Be Star Binaries

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2304.02615.

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

pith.paper-citation-record.v1
2304.02615 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 2026-08-21T06:32:19.484+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T15:20:03.376602Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-08T17:55:20.667682Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • malformed identifier0
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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 c791a1de-0863-41f5-b15e-48866f457032 · inbound

A Possible Triple Formation Scenario of Binary Black Hole Merge With One In Pair-instability Supernova Mass Gap cites this paper.

A Possible Triple Formation Scenario of Binary Black Hole Merge With One In Pair-instability Supernova Mass Gap Formation and Destiny of White Dwarf and Be Star Binaries

Reference 70

Resolution
verified exact
local_arxiv, observed 2026-07-08T17:55:20.669025Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-07-08T17:53:06.845093Z digest=sha256:487d62736531d0b2d281d28068d07bfc8f6409846162025e191672c28235d75c

Observation 61cbc2ff-74e9-442b-986f-ef7ff86d7352 · inbound

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs cites this paper.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Formation and Destiny of White Dwarf and Be Star Binaries

Reference 293

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:03.376602Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:03.376602Z digest=sha256:390ce09e7c02afebd6884046afe1c075afc25aef1ae188eccdfee0e16c5a866d