Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Constraining mixing in massive stars in the Small Magellanic Cloud
As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1903.10423.
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 2026-08-04T06:34:03.388597+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-28T13:02:10.762760Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
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 d1fd6cd7-fc52-43a2-904a-1d15500a9918 · inbound
Binarity at LOw Metallicity (BLOeM): massive star variability revealed using a novel software tool for point-spread function fitting of TESS images cites this paper.
Binarity at LOw Metallicity (BLOeM): massive star variability revealed using a novel software tool for point-spread function fitting of TESS images Constraining mixing in massive stars in the Small Magellanic Cloud
Reference 108
- Resolution
- verified exact
- local_arxiv, observed 2026-05-19T19:42:43.823292Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation 57227ebe-fb9e-40af-ad09-1bf95897604f · inbound
Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models cites this paper.
Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Constraining mixing in massive stars in the Small Magellanic Cloud
Reference 19
- Resolution
- verified exact
- local_arxiv, observed 2026-05-21T02:13:55.252697Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation eefc048f-d29c-4b6a-9f17-af0bc9b285ac · inbound
Can current models predict the local black hole merger rate? cites this paper.
Can current models predict the local black hole merger rate? Constraining mixing in massive stars in the Small Magellanic Cloud
Reference 238
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T13:02:10.764057Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation a279eecf-0f06-447d-8aa0-d30afbafcb8e · inbound
The effect of near-core mixing on rejuvenation and the asteroseismic properties of massive accretors cites this paper.
The effect of near-core mixing on rejuvenation and the asteroseismic properties of massive accretors Constraining mixing in massive stars in the Small Magellanic Cloud
Reference 245
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-27T05:40:36.179201Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation bb6638ab-187c-473c-86a2-86c3e77bb31a · inbound
Comparative Study of Two Luminous Red Novae I. Progenitor Modeling and Dust Formation cites this paper.
Comparative Study of Two Luminous Red Novae I. Progenitor Modeling and Dust Formation Constraining mixing in massive stars in the Small Magellanic Cloud
Reference 106
- Resolution
- verified exact
- local_arxiv, observed 2026-06-26T09:59:18.181016Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.