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Paper Citation Record · LEDGER

Continuous stellar mass-loss in N-body models of galaxies

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0107160.

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

pith.paper-citation-record.v1
astro-ph/0107160 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 2026-08-08T06:32:00.761636+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T13:44:38.170387Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-14T20:52:56.959064Z

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 ca39b150-2309-4cfe-8a97-8fb21f12b886 · inbound

Dark-matter-induced transients over cosmic time: The role of star formation history profiles cites this paper.

Dark-matter-induced transients over cosmic time: The role of star formation history profiles Continuous stellar mass-loss in N-body models of galaxies

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-07T13:44:38.170387Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T13:44:38.170387Z digest=sha256:76e8dc871d8b3af572f27267bfdd01a8a7c7d4b412468b082d368994b8a331ff

Observation 5618ae85-20f2-45ce-88c3-5fcff6eda105 · inbound

Strong Progenitor Age Bias in Supernova Cosmology. III. Progenitor Age as the Physical Origin of the Type Ia Supernova Magnitude Steps with Host Properties cites this paper.

Strong Progenitor Age Bias in Supernova Cosmology. III. Progenitor Age as the Physical Origin of the Type Ia Supernova Magnitude Steps with Host Properties Continuous stellar mass-loss in N-body models of galaxies

Reference 46

Resolution
verified exact
local_arxiv, observed 2026-05-14T20:52:56.962763Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:942e1b895194179ac8777a5bec8b9ad127f3d42c973f484af9d05c1bdcc1f097