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Paper Citation Record · LEDGER

The empirical metallicity dependence of the mass-loss rate of O- and early B-type stars

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:0708.2042.

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

pith.paper-citation-record.v1
0708.2042 v1

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measured 0 of 0 reference resolution

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Source: paper_references, paper_reference_links

measured 3 of 3 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 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z

measured 0 of 1 external citation measurements

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Source: pith, observed 2026-07-01T01:05:12.137743Z

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0 of 0 outbound references displayed

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Outbound references

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Pith citing papers

Observation 835a2a45-a530-4eca-a96b-e7e78040993a · inbound

Massquerade: Impacts of Mass Ratio Reversals on Binary Black Hole Merger Rates and Mass Distributions cites this paper.

Massquerade: Impacts of Mass Ratio Reversals on Binary Black Hole Merger Rates and Mass Distributions The empirical metallicity dependence of the mass-loss rate of O- and early B-type stars

Reference 274

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verified exact
local_arxiv, observed 2026-05-22T09:31:21.748620Z

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=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:f9ee9fc8d7eb08c0ce452dee128e30cc1933c1268820d2322c4a1efec0773d65

Observation 7e950257-06bf-497c-a94b-89f73e8f0496 · inbound

Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI cites this paper.

Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI The empirical metallicity dependence of the mass-loss rate of O- and early B-type stars

Reference 139

Resolution
verified exact
local_arxiv, observed 2026-06-26T18:09:41.335487Z

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=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:b121c9ce5be324b72a541976df419d4a72cc8e32d8d5907ab6682e543613e3e0

Observation 40c638a2-44c0-49e0-a48b-0e79c66aa7f9 · inbound

SN 2023rve: A Type II Supernova with No Nebular Oxygen cites this paper.

SN 2023rve: A Type II Supernova with No Nebular Oxygen The empirical metallicity dependence of the mass-loss rate of O- and early B-type stars

Reference 193

Resolution
verified exact
local_arxiv, observed 2026-07-01T01:05:12.139175Z

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=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:8a0241957ea1663ed29500e41695ec89c49f4fa6d488ded1474cc878163899eb