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Paper Citation Record · LEDGER

First grids of low-mass stellar models and isochrones with self-consistent treatment of rotation : From 0.2 to 1.5 M_\odot at 7 metallicities from PMS to TAMS

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1905.08516.

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

pith.paper-citation-record.v1
1905.08516 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

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 2026-08-06T06:34:29.942622+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T02:40:35.438952Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-14T09:00:21.986370Z

Reference resolution

0 of 0 outbound references displayed

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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 49f7c847-5e59-4e78-acaa-5a5a72d69b84 · inbound

Asteroseismic forward modelling of 36 $\beta$ Cep pulsators and inferences on their internal differential rotation cites this paper.

Asteroseismic forward modelling of 36 $\beta$ Cep pulsators and inferences on their internal differential rotation First grids of low-mass stellar models and isochrones with self-consistent treatment of rotation : From 0.2 to 1.5 M_\odot at 7 metallicities from PMS to TAMS

Reference 14

Resolution
verified exact
local_arxiv, observed 2026-07-14T09:00:21.993050Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=arxiv_source observed=2026-07-14T08:55:08.442634Z digest=sha256:bd91fa6e24d66fc4311854676205e75f2d3e418e5f2ba80be4d22e2c2ee0ccb8

Reference 16

Resolution
unresolved
no resolver link, observed 2026-08-01T04:54:20.243350Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T04:54:20.243350Z digest=sha256:6f38bd2403a5d00f61c1f7f713a4ed0fc322addece950ae6238fb204f817ffcb

Observation 0eb89f25-63ad-4bd0-ac42-c2509057a1b2 · inbound

The IACOB project XIX. Revisiting massive-star evolution with empirical TAMS constraints: updated models, overshoot calibration, and the population of blue supergiants cites this paper.

The IACOB project XIX. Revisiting massive-star evolution with empirical TAMS constraints: updated models, overshoot calibration, and the population of blue supergiants First grids of low-mass stellar models and isochrones with self-consistent treatment of rotation : From 0.2 to 1.5 M_\odot at 7 metallicities from PMS to TAMS

Reference 9

Resolution
unresolved
no resolver link, observed 2026-08-03T02:40:35.438952Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-03T02:40:35.438952Z digest=sha256:5fbc10afd7684cfa6852e78a097fa092242a896c36a8d07dfff01847db36854a