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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 15 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 2026-08-15T06:32:42.880941+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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-05T17:53:06.766552Z digest=sha256:b86f418f1bfc37e24cb6a00f4a1fc79d505f03c85a9b2f13db186abc194ed2c1

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-05T17:53:06.869276Z digest=sha256:1fda208b2787dfc92697b333884067bd4b29a7c81c2a6b8b91c4b4f4ba582136

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:b8406f27072605242cd2a5624f3084d50834760b7e5fa2abd741fa8eab48e698