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Paper Citation Record · LEDGER

Total r-process Yields of Milky Way Neutron Star Mergers

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2310.03847.

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

pith.paper-citation-record.v1
2310.03847 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 2026-08-10T06:31:04.303077+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-09T12:19:43.103423Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-10T05:30:23.456663Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

0
pith, observed 2026-08-10T05:30:23.456663Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 3c293b1b-7146-4fcb-b034-7a0303547368 · inbound

Mixing neutron star material into the jets in the common envelope jets supernova r-process scenario cites this paper.

Mixing neutron star material into the jets in the common envelope jets supernova r-process scenario Total r-process Yields of Milky Way Neutron Star Mergers

Reference 22

Resolution
unresolved
no resolver link, observed 2026-08-09T12:19:43.103423Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T12:19:43.103423Z digest=sha256:1bcbb4f4f0f002c58f57cb2778a7d9a07fbfdcf40e3ceb4573b272bec890d294

Observation 22e8f734-ea2a-44f7-a7aa-a8f7dd8fe8d0 · inbound

Forming Double Neutron Stars using Detailed Binary Evolution Models with POSYDON: Comparison to the Galactic Systems cites this paper.

Forming Double Neutron Stars using Detailed Binary Evolution Models with POSYDON: Comparison to the Galactic Systems Total r-process Yields of Milky Way Neutron Star Mergers

Reference 77

Resolution
verified exact
local_arxiv, observed 2026-08-06T10:28:55.249128Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-08-06T10:25:57.246705Z digest=sha256:12e1fdaeb3387966d013d77f2c4df5c04b56d7df503261a099c854bb91e7db19