Pith. sign in

Paper Citation Record · LEDGER

A Turbulent Interstellar Medium Origin of the Binary Period Distribution

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0303280.

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

pith.paper-citation-record.v1
astro-ph/0303280 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 2026-08-14T06:32:32.682623+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T04:44:36.756378Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-25T20:58:21.386891Z

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 77de65e5-9b27-4a3e-b15b-16e67b11ba32 · inbound

Formation of a Protostellar Multiple System via Rotational Fragmentation cites this paper.

Formation of a Protostellar Multiple System via Rotational Fragmentation A Turbulent Interstellar Medium Origin of the Binary Period Distribution

Reference 30

Resolution
verified exact
local_arxiv, observed 2026-06-25T20:58:21.388151Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:ffdec92f993d366c5cd98a5b45c5361b1085d4b13b3070a40a399839913f2dcd

Observation 908d269a-dc54-42e2-a7a6-ecedc6974814 · inbound

The ALMA carbon monoxide supernova (ACOS) survey II. Turbulent giant molecular clouds at the positions of core-collapse supernovae cites this paper.

The ALMA carbon monoxide supernova (ACOS) survey II. Turbulent giant molecular clouds at the positions of core-collapse supernovae A Turbulent Interstellar Medium Origin of the Binary Period Distribution

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-14T04:44:36.756378Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:44:36.756378Z digest=sha256:b77a59ef30663d97085556e1cc4caae4cc2f82d64789067934495c69ce3f02be