Paper Citation Record · LEDGER

The IACOB project: XVII. Nitrogen abundances in Galactic O-type stars: further hints for separating binary-interaction products from effectively single stars

As of 9 August 2026, this Paper Citation Record lists 6 of 6 outbound references and 2 inbound Pith citation observations for arXiv:2604.26606.

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

pith.paper-citation-record.v1
2604.26606 v2

Coverage vector

measured 6 of 6 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-05-07T12:50:12.561146Z

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T20:32:24.838655Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

6 of 6 outbound references displayed

verified exact0
verified fuzzy4
unresolved1
parse uncertain0
malformed identifier1
metadata mismatch0

External citation measurements

0
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

Observation 89d8a7b1-b05c-4346-b9af-e9a585ee26d5 · outbound

This paper cites M., Holgado G., Mart \' nez-Sebasti \'a n C., Sim \'o n-D \' az S., 2025, @doi [arXiv e-prints] 10.48550/arXiv.2510.21577 , https://ui.adsabs.harvard.edu/abs/2025arXiv251021577C p.

The IACOB project: XVII. Nitrogen abundances in Galactic O-type stars: further hints for separating binary-interaction products from effectively single stars M., Holgado G., Mart \' nez-Sebasti \'a n C., Sim \'o n-D \' az S., 2025, @doi [arXiv e-prints] 10.48550/arXiv.2510.21577 , https://ui.adsabs.harvard.edu/abs/2025arXiv251021577C p

Reference 1

Resolution: malformed identifier; arxiv_id, observed 2026-05-12T09:06:26.621222Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation b3339930-708c-42ef-83fa-afa2777dc946 · outbound

This paper cites The results of both analyses, together with the original model parameters, are summarized in Table C.1.

The IACOB project: XVII. Nitrogen abundances in Galactic O-type stars: further hints for separating binary-interaction products from effectively single stars The results of both analyses, together with the original model parameters, are summarized in Table C.1

Reference 2

Resolution: verified fuzzy; raw_fallback, observed 2026-05-27T06:23:40.974625Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 5fe745f7-c2a3-4bc9-9712-d2b6e03130a9 · outbound

This paper cites To assess this effect, we performed a consistency check by reanalyzing our sample with IACOB-GBAT (Simón-Díaz et al.

The IACOB project: XVII. Nitrogen abundances in Galactic O-type stars: further hints for separating binary-interaction products from effectively single stars To assess this effect, we performed a consistency check by reanalyzing our sample with IACOB-GBAT (Simón-Díaz et al

Reference 3

Resolution: verified fuzzy; raw_fallback, observed 2026-05-27T06:23:40.968097Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 892cddac-69f5-4238-bf28-44df4adbdbb3 · outbound

This paper cites We find that the differences between groups 0.05 0.1 0.15 0.2 0.05 0.1 0.15 0.2 0.17 0.29 0.37 0.44 Y (ξHe) 0.17 0.29 0.37 0.44 Y (ξN) YHe(ξHe) YHe(ξN) Fig.

The IACOB project: XVII. Nitrogen abundances in Galactic O-type stars: further hints for separating binary-interaction products from effectively single stars We find that the differences between groups 0.05 0.1 0.15 0.2 0.05 0.1 0.15 0.2 0.17 0.29 0.37 0.44 Y (ξHe) 0.17 0.29 0.37 0.44 Y (ξN) YHe(ξHe) YHe(ξN) Fig

Reference 4

Resolution: verified fuzzy; raw_fallback, observed 2026-05-27T06:23:40.965030Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 495991f9-fa3a-466b-9655-8cb9fdf582c6 · outbound

This paper cites an unresolved cited work.

The IACOB project: XVII. Nitrogen abundances in Galactic O-type stars: further hints for separating binary-interaction products from effectively single stars Unresolved cited work

Reference 5

Resolution: unresolved; raw_fallback, observed 2026-05-27T06:23:40.971216Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation eb141627-d61a-4c29-a68e-25d543a8d92d · outbound

This paper cites C.5.Results of the analysis of synthetic spectra from FASTWIND models.

The IACOB project: XVII. Nitrogen abundances in Galactic O-type stars: further hints for separating binary-interaction products from effectively single stars C.5.Results of the analysis of synthetic spectra from FASTWIND models

Reference 6

Resolution: verified fuzzy; raw_fallback, observed 2026-05-27T06:23:40.961338Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Pith citing papers

Observation 4bc04ea9-273c-45de-90d5-572d86f1fdfd · 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 The IACOB project: XVII. Nitrogen abundances in Galactic O-type stars: further hints for separating binary-interaction products from effectively single stars

Reference 200

Resolution: verified exact; local_arxiv, observed 2026-08-03T02:43:27.632387Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation eb57cd1b-5974-463c-97c2-50a01a282786 · inbound

Unravelling Mass Transfer in Algols from Surface Abundances. I. Z Vulpeculae cites this paper.

Unravelling Mass Transfer in Algols from Surface Abundances. I. Z Vulpeculae The IACOB project: XVII. Nitrogen abundances in Galactic O-type stars: further hints for separating binary-interaction products from effectively single stars

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-05T20:32:24.838655Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.