Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The Relation Between [OIII]/H$\beta$ and Specific Star Formation Rate in Galaxies at $z \sim 2$
As of 19 July 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1606.01259.
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 2026-07-19T06:30:13.599613+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 2026-07-10T06:15:00.866473Z
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 a370e81a-eac2-41b6-9311-4a34866f2a79 · inbound
Inferring the role of binary neutron star mergers in r-process nucleosynthesis with multi-messenger observations using Cosmic Explorer and Einstein Telescope cites this paper.
Inferring the role of binary neutron star mergers in r-process nucleosynthesis with multi-messenger observations using Cosmic Explorer and Einstein Telescope The Relation Between [OIII]/H$\beta$ and Specific Star Formation Rate in Galaxies at $z \sim 2$
Reference 52
- Resolution
- verified exact
- local_arxiv, observed 2026-05-25T03:55:18.698923Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-07-19T06:30:13.599613+00:00.
Observation 6bf17477-ac17-4f9d-8325-4b851b017a8e · inbound
MEGA and SMILES Find Fewer Dusty Galaxies than Expected at Cosmic Noon cites this paper.
MEGA and SMILES Find Fewer Dusty Galaxies than Expected at Cosmic Noon The Relation Between [OIII]/H$\beta$ and Specific Star Formation Rate in Galaxies at $z \sim 2$
Reference 97
- Resolution
- verified exact
- local_arxiv, observed 2026-06-27T03:30:27.488068Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-07-19T06:30:13.599613+00:00.