Pith. sign in

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 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 15 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 15 of 15 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-21T06:32:19.484+00:00

measured 15 of 15 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T15:06:11.541049Z

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

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

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 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-05-21T21:48:20.183638Z digest=sha256:0fcc1ebc88c76c116a888b24bbb4de5c2eed95fe71fb105bbe063712049a70e8

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
metadata mismatch
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 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-05-10T02:11:58.893710Z digest=sha256:ce04e826dd88e9514677f95f5938d43bb48960ab49b7f47d7cc158e0c4bcff87

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
metadata mismatch
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 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-05-07T15:12:16.443826Z digest=sha256:a21fc9d1c0e0066912bdd9de0a21dd6725ac55f258fb41fac8809a06d8345ce0

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
metadata mismatch
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 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-05-08T19:01:57.066359Z digest=sha256:89d0b616ef0613f556f28f4214ca37ea87f92ee0c834f73183eda54bf84bfcb0

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
metadata mismatch
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 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-05-08T18:08:46.151992Z digest=sha256:f54f3d60fb613b959b1d557c74da5ebb6ce24d5b34e93532904affa56e811b6e

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 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:b02764784a69295ccde9f94f3f552556573c33989826d5da11b1e1742e91981b

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 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-06-27T03:22:47.800684Z digest=sha256:ccde43d1901ca0e45ab76b2c41a5c4b84865d641346d9c9db3229225232682af

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 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:6d46b9a748228ace5fc9ecfb1725e0071ba1f934625f878f78b835b0dc15f010

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 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-01T02:06:55.056595Z digest=sha256:5e91dd8e10d799c68ddb3333284f9cc2ac33a55c3d1205f27274639dd8399cd5

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 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:d15d8c6a0786f4a17d52b22d9ccd795f1c2a6d6914a47bf5e95ec6c6c0c8b8d0

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
unresolved
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=sha256:9de7b0b1d4ec416445a0619ffad867361ddba9a80987b3a4acc53b4fb7beffbc

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
metadata mismatch
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 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-02T09:53:37.236656Z digest=sha256:f8121289081164606958a3c32b37b4b8005a39005069676bc69137c12900f37b

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=sha256:20153100274acb879a90d96cd8069d339ecdc20cb94edf14ec3abd238c95f55f

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.

source=arxiv_source observed=2026-08-11T00:30:25.676434Z digest=sha256:9cf6ff5b283827edd3fd9e176d291f660ab9b85581ba040152ef1453d0c2e107

Observation f3c4f009-6a44-4c77-9722-87a3ce66b894 · inbound

Cosmography with DESI-DR1 Cosmic Chronometers: Direct H(z) measurements from Luminous Red Galaxy ages cites this paper.

Cosmography with DESI-DR1 Cosmic Chronometers: Direct H(z) measurements from Luminous Red Galaxy ages 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 146

Resolution
unresolved
no resolver link, observed 2026-08-15T15:06:11.541049Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:06:11.541049Z digest=sha256:3e3360cfe87351edba736b78a03ef1190d61cd3c722fc49b43ab3da94c597a55