Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-05-07T12:50:12.561146Z
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 7 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.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-06T06:34:29.942622+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-05T20:32:24.838655Z
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 2026-08-06T06:34:29.942622+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 2026-08-06T06:34:29.942622+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 2026-08-06T06:34:29.942622+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 2026-08-06T06:34:29.942622+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 2026-08-06T06:34:29.942622+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 2026-08-06T06:34:29.942622+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 2026-08-06T06:34:29.942622+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.