Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1412.4153.
A citation records a reference. It does not transfer a finding from one paper to another.
Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-05T06:32:48.257954+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-01T20:35:53.173771Z
A source-named dated measurement, never combined with another source.
Source: cited_works
0 of 0 outbound references displayed
External citation measurements
No source-named external measurement is stored.
No outbound reference observations are available for this paper version.
Observation 6da129af-f8e9-4920-b990-eb2db1350a7f · inbound
Effective temperatures estimation of low-mass stars and identification of T Tauri stars in LAMOST DR10 using machine learning The Gaia-ESO Survey: Chromospheric Emission, Accretion Properties, and Rotation in $\gamma$ Velorum and Chamaeleon I
Reference 9
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation daaf6d54-7d16-4627-b941-c04d4f544e17 · inbound
LBT-MODS spectroscopy of young stellar objects in the distant metal-poor star forming region Sh2-284: Stellar and accretion properties The Gaia-ESO Survey: Chromospheric Emission, Accretion Properties, and Rotation in $\gamma$ Velorum and Chamaeleon I
Reference 68
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4ff401bd-3ee3-4a1b-8346-7c8f0d3ed02a · inbound
Exploring the radial velocity variations of RY Lup with VLT/ESPRESSO: Binary versus spot hypotheses The Gaia-ESO Survey: Chromospheric Emission, Accretion Properties, and Rotation in $\gamma$ Velorum and Chamaeleon I
Reference 4
Source-reported events for the cited work
Unavailable: canonical work link unavailable.