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Paper Citation Record · LEDGER

Evolutionary tracks and isochrones for low- and intermediate-mass stars: from 0.15 to 7 M_sun, and from Z=0.0004 to 0.03

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 14 inbound Pith citation observations for arXiv:astro-ph/9910164.

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

pith.paper-citation-record.v1
astro-ph/9910164 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 14 of 14 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 14 of 14 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T00:30:25.676434Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-07-02T18:17:16.563089Z

Reference resolution

0 of 0 outbound references displayed

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External citation measurements

1986
pith, observed 2026-07-02T18:17:16.563089Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 051fa6c3-0d0e-4d96-9820-6ce0b99f81eb · inbound

The heart of NGC 5253 as seen with MUSE-NFM: nitrogen enrichment through stellar chemical feedback at parsec scales cites this paper.

The heart of NGC 5253 as seen with MUSE-NFM: nitrogen enrichment through stellar chemical feedback at parsec scales Evolutionary tracks and isochrones for low- and intermediate-mass stars: from 0.15 to 7 M_sun, and from Z=0.0004 to 0.03

Reference 43

Resolution
verified exact
doi, observed 2026-05-21T21:50:41.127040Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation eaea5535-1ad4-4662-be06-b1586db861c9 · inbound

IZ Tel and UW Vir: Southern oscillating eclipsing Algol systems with active mass transfer cites this paper.

IZ Tel and UW Vir: Southern oscillating eclipsing Algol systems with active mass transfer Evolutionary tracks and isochrones for low- and intermediate-mass stars: from 0.15 to 7 M_sun, and from Z=0.0004 to 0.03

Reference 110

Resolution
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doi, observed 2026-05-10T02:27:37.293676Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=arxiv_source observed=2026-05-10T02:11:58.893710Z digest=sha256:d4766369b6f12ff5c23bd47afe57244c93ed874ec1ed55d5a603267c7e0a8095

Observation bd9f7049-c45d-4e9b-9f68-74ba16e2b074 · inbound

Asteroseismic analysis of RY Leporis: the post-main sequence HADS in a binary system cites this paper.

Asteroseismic analysis of RY Leporis: the post-main sequence HADS in a binary system Evolutionary tracks and isochrones for low- and intermediate-mass stars: from 0.15 to 7 M_sun, and from Z=0.0004 to 0.03

Reference 36

Resolution
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doi, observed 2026-05-09T02:34:42.603048Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-05-07T15:12:16.443826Z digest=sha256:e4ea05068fee816909e4b471ec8408cab6a3f2479a0613ad9a895bbbf5279fff

Observation d768b508-a718-4755-85c5-c08a3c96fe86 · inbound

Morphological and Star Formation Properties of Cosmic Noon Massive Quiescent Galaxies cites this paper.

Morphological and Star Formation Properties of Cosmic Noon Massive Quiescent Galaxies Evolutionary tracks and isochrones for low- and intermediate-mass stars: from 0.15 to 7 M_sun, and from Z=0.0004 to 0.03

Reference 45

Resolution
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doi, observed 2026-05-08T19:04:02.323872Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 7e0c2a11-a240-4a3c-a5a6-ceada2c25d4d · inbound

A CNN--Transformer Denoiser for low-$S/N$ Galaxy Spectra: Stellar Population Recovery in Synthetic Tests cites this paper.

A CNN--Transformer Denoiser for low-$S/N$ Galaxy Spectra: Stellar Population Recovery in Synthetic Tests Evolutionary tracks and isochrones for low- and intermediate-mass stars: from 0.15 to 7 M_sun, and from Z=0.0004 to 0.03

Reference 11

Resolution
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doi, observed 2026-05-08T18:08:53.020518Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation c7b30d28-df9a-432a-b1ec-a5dedf566f6a · inbound

Witnessing the rapid growth of disk galaxies over cosmic time using JWST and HST cites this paper.

Witnessing the rapid growth of disk galaxies over cosmic time using JWST and HST Evolutionary tracks and isochrones for low- and intermediate-mass stars: from 0.15 to 7 M_sun, and from Z=0.0004 to 0.03

Reference 139

Resolution
verified exact
local_arxiv, observed 2026-05-19T15:27:38.113332Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:79da7e45af2b0f42999a4194694ee492286b804d7b65500fafb87c4ef9541a95

Observation d3950b0d-bb4b-48bf-9bc6-40ca9a5fe27a · inbound

MEGA and SMILES Find Fewer Dusty Galaxies than Expected at Cosmic Noon cites this paper.

MEGA and SMILES Find Fewer Dusty Galaxies than Expected at Cosmic Noon Evolutionary tracks and isochrones for low- and intermediate-mass stars: from 0.15 to 7 M_sun, and from Z=0.0004 to 0.03

Reference 138

Resolution
verified exact
doi, observed 2026-06-27T03:30:27.246018Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 75d551fd-2954-4b98-b599-66e3ea01607b · inbound

Chemical hints of Population III stars from silicon abundances in massive galaxies cites this paper.

Chemical hints of Population III stars from silicon abundances in massive galaxies Evolutionary tracks and isochrones for low- and intermediate-mass stars: from 0.15 to 7 M_sun, and from Z=0.0004 to 0.03

Reference 148

Resolution
verified exact
local_arxiv, observed 2026-06-27T03:10:24.535800Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 0721a0fe-3546-4154-9e13-c21524966b13 · inbound

Global trends in morphology from massive to dwarf galaxies cites this paper.

Global trends in morphology from massive to dwarf galaxies Evolutionary tracks and isochrones for low- and intermediate-mass stars: from 0.15 to 7 M_sun, and from Z=0.0004 to 0.03

Reference 104

Resolution
verified exact
doi, observed 2026-07-01T02:45:17.999346Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 7fcb5d06-ad45-44f5-a944-4247c6256234 · inbound

AGN radiative feedback as the main regulator of [O III] outflow activity and obscuration in X-ray AGN cites this paper.

AGN radiative feedback as the main regulator of [O III] outflow activity and obscuration in X-ray AGN Evolutionary tracks and isochrones for low- and intermediate-mass stars: from 0.15 to 7 M_sun, and from Z=0.0004 to 0.03

Reference 100

Resolution
verified exact
local_arxiv, observed 2026-07-02T18:17:16.564546Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Observation 5b6cd6ca-be01-4a3d-8829-e8a8414f80db · inbound

AGN radiative feedback as the main regulator of [O III] outflow activity and obscuration in X-ray AGN cites this paper.

AGN radiative feedback as the main regulator of [O III] outflow activity and obscuration in X-ray AGN Evolutionary tracks and isochrones for low- and intermediate-mass stars: from 0.15 to 7 M_sun, and from Z=0.0004 to 0.03

Reference 102

Resolution
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no resolver link, observed 2026-07-12T09:44:28.146054Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-12T09:44:28.146054Z digest=sha256:ff553b9a8d9c8080dcb1e2b06fad897869d1b7de60243a5d588f881497a4fe5d

Observation d3ca6e44-b372-4c6a-b92f-61f1b362b657 · inbound

OCCAM X. Neutron Capture Abundances with Keck/HIRES & Magellan/MIKE cites this paper.

OCCAM X. Neutron Capture Abundances with Keck/HIRES & Magellan/MIKE Evolutionary tracks and isochrones for low- and intermediate-mass stars: from 0.15 to 7 M_sun, and from Z=0.0004 to 0.03

Reference 250

Resolution
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doi, observed 2026-07-02T09:56:50.900183Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=arxiv_source observed=2026-07-02T09:53:37.236656Z digest=sha256:62a31b9dd27c9c916eb1298147a79dd6a93416d6a2a28b06dc068f1326e3aa06

Observation 5abab5c8-b30f-4f13-9d00-9d4154bc77a7 · inbound

The potential broader complex linked to the key Cepheid SV Vul cites this paper.

The potential broader complex linked to the key Cepheid SV Vul Evolutionary tracks and isochrones for low- and intermediate-mass stars: from 0.15 to 7 M_sun, and from Z=0.0004 to 0.03

Reference 38

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.098983Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.098983Z digest=sha256:14f797f2e916cf1257f80c1a6e02e9a32aa556adf844706b453d3cf092879df1

Observation 28947f96-097c-4d2a-8963-3459c2364cef · inbound

First Light and Assembly of GalaxieS (FLAGS) I: The JWST/NIRCam Number Counts and IGL as Constraints on Galaxy Formation Models cites this paper.

First Light and Assembly of GalaxieS (FLAGS) I: The JWST/NIRCam Number Counts and IGL as Constraints on Galaxy Formation Models Evolutionary tracks and isochrones for low- and intermediate-mass stars: from 0.15 to 7 M_sun, and from Z=0.0004 to 0.03

Reference 77

Resolution
unresolved
no resolver link, observed 2026-08-11T00:30:25.676434Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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