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Paper Citation Record · LEDGER

Binarity at LOw Metallicity (BLOeM): Enhanced multiplicity of early B-type dwarfs and giants at $Z=0.2\,{\rm Z}_\odot$

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2503.21936.

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

pith.paper-citation-record.v1
2503.21936 v4

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T16:40:19.201189Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T20:04:33.616554Z

Reference resolution

0 of 0 outbound references displayed

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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 d3422906-cd7d-4683-9018-5516fdf2e127 · inbound

Diversity in Hydrogen-rich Envelope Mass of Type II Supernovae. (III). The mass-loss and evolutionary pathways of the red supergiant progenitors cites this paper.

Diversity in Hydrogen-rich Envelope Mass of Type II Supernovae. (III). The mass-loss and evolutionary pathways of the red supergiant progenitors Binarity at LOw Metallicity (BLOeM): Enhanced multiplicity of early B-type dwarfs and giants at $Z=0.2\,{\rm Z}_\odot$

Reference 155

Resolution
unresolved
no resolver link, observed 2026-08-06T15:56:38.084894Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T15:56:38.084894Z digest=sha256:54c087b153f7756c05f27c2d329f90dfa03c20cc20f924e91c42dad9b64c61b1

Observation c6491b71-ccc7-4adf-817e-0cffbfab830b · inbound

Impact of Uncertainties in Spectral Energy Distribution Modelling on Inferred Galaxy Properties cites this paper.

Impact of Uncertainties in Spectral Energy Distribution Modelling on Inferred Galaxy Properties Binarity at LOw Metallicity (BLOeM): Enhanced multiplicity of early B-type dwarfs and giants at $Z=0.2\,{\rm Z}_\odot$

Reference 189

Resolution
unresolved
no resolver link, observed 2026-08-15T16:40:19.201189Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T16:40:19.201189Z digest=sha256:9cc595c79825174d825313403c9c150708dd76c8df1c93826cbec3438db57f72

Observation 88c89668-2665-4431-b6f7-1dc641ff0e35 · inbound

The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry cites this paper.

The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry Binarity at LOw Metallicity (BLOeM): Enhanced multiplicity of early B-type dwarfs and giants at $Z=0.2\,{\rm Z}_\odot$

Reference 185

Resolution
verified exact
local_arxiv, observed 2026-08-05T20:04:33.636704Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-05T20:04:30.459993Z digest=sha256:f05f5bcdde27c9216441bbab67463b4b1e4c7c3f2a4a0b5a25ca288e189d8a7a

Observation fb227b6b-5d90-4e46-9737-f9c90321f783 · inbound

The ALMA carbon monoxide supernova (ACOS) survey II. Turbulent giant molecular clouds at the positions of core-collapse supernovae cites this paper.

The ALMA carbon monoxide supernova (ACOS) survey II. Turbulent giant molecular clouds at the positions of core-collapse supernovae Binarity at LOw Metallicity (BLOeM): Enhanced multiplicity of early B-type dwarfs and giants at $Z=0.2\,{\rm Z}_\odot$

Reference 213

Resolution
unresolved
no resolver link, observed 2026-08-14T04:44:37.603907Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:44:37.603907Z digest=sha256:6e82b91c4e5757c7af9665fa467391d217ff7bb38165cab1f1d9a283b38c082d