Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Are LGRBs biased tracers of star formation? Clues from the host galaxies of the $Swift$/BAT6 complete sample of bright LGRBs III: Stellar masses, star formation rates and metallicities at $z>1$
As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1901.02457.
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 2026-08-05T16:33:53.171352Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-28T05:41:40.834693Z
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 6d247c18-cfa0-47e8-a789-d64b1c6386a2 · inbound
Earliest simultaneous multi-color optical observations of GRB 230328B: from 41 seconds to the host-galaxy identification cites this paper.
Earliest simultaneous multi-color optical observations of GRB 230328B: from 41 seconds to the host-galaxy identification Are LGRBs biased tracers of star formation? Clues from the host galaxies of the $Swift$/BAT6 complete sample of bright LGRBs III: Stellar masses, star formation rates and metallicities at $z>1$
Reference 26
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T05:41:40.836221Z
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 92e754e8-2292-4881-9d94-659b0bd30a9c · inbound
Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster cites this paper.
Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Are LGRBs biased tracers of star formation? Clues from the host galaxies of the $Swift$/BAT6 complete sample of bright LGRBs III: Stellar masses, star formation rates and metallicities at $z>1$
Reference 241
- Resolution
- unresolved
- no resolver link, observed 2026-07-14T05:32:07.775931Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4c0ac235-632f-44e7-9ce7-02fc39e12a17 · inbound
A JWST redshift for the host galaxy of EP250207b of z=3.2: a collapsar origin is viable cites this paper.
A JWST redshift for the host galaxy of EP250207b of z=3.2: a collapsar origin is viable Are LGRBs biased tracers of star formation? Clues from the host galaxies of the $Swift$/BAT6 complete sample of bright LGRBs III: Stellar masses, star formation rates and metallicities at $z>1$
Reference 27
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T16:33:53.171352Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.