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Paper Citation Record · LEDGER

Formation of heavy double neutron stars I: Eddington-limited accretion for a 1.4 $M_{\odot}$ neutron star at solar metallicity

As of 7 August 2026, this Paper Citation Record lists 2 of 2 outbound references and 1 inbound Pith citation observation for arXiv:2508.15624.

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

pith.paper-citation-record.v1
2508.15624 v1

Coverage vector

measured 2 of 2 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-05T17:53:06.869276Z

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T19:06:37.234962Z

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

2 of 2 outbound references displayed

  • verified exact1
  • verified fuzzy1
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 7b2fd76b-3c8a-4d32-ae69-f636e7751a59 · outbound

This paper cites P., et al., 2017a, Phys.

Formation of heavy double neutron stars I: Eddington-limited accretion for a 1.4 $M_{\odot}$ neutron star at solar metallicity P., et al., 2017a, Phys

Reference 1

Resolution
verified fuzzy
raw_fallback, observed 2026-08-05T17:53:07.503356Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-08-05T17:53:06.766552Z digest=sha256:045028045256a09839abbfe07ec569bc3ab9c64ca886661094c45c4155c31743

Observation 13dae428-2d7c-4b13-acdd-e28dc5baf86f · outbound

This paper cites The landscape of binary core-collapse supernova progenitors and the late emergence of Wolf-Rayet winds.

Formation of heavy double neutron stars I: Eddington-limited accretion for a 1.4 $M_{\odot}$ neutron star at solar metallicity The landscape of binary core-collapse supernova progenitors and the late emergence of Wolf-Rayet winds

Reference 2

Resolution
verified exact
local_arxiv, observed 2026-08-05T17:53:07.220522Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-08-05T17:53:06.869276Z digest=sha256:5915df94b3a0e6d7ce9f5efd454b92db8d5e16e317d04f8160288abd4f07e8a5

Pith citing papers

Observation 54884522-3178-492d-83ce-a2bf12e2bd89 · inbound

Probing the redshift evolution and sub-populations of binary neutron stars with the Einstein Telescope cites this paper.

Probing the redshift evolution and sub-populations of binary neutron stars with the Einstein Telescope Formation of heavy double neutron stars I: Eddington-limited accretion for a 1.4 $M_{\odot}$ neutron star at solar metallicity

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-03T19:06:37.234962Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-03T19:06:37.234962Z digest=sha256:f808a697b012a06a8bcbd180d6231f9a7ab6afa5e39404b4c115134c00552beb