Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2412.01155.
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 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T00:15:14.190351Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z
0 of 0 outbound references displayed
External citation measurements
0
arxiv_reference, observed 2026-08-05T02:28:24.338817Z
No outbound reference observations are available for this paper version.
Observation 3005f83e-fa3b-4224-a219-cc61488d2294 · inbound
Reproducing morphological features in the supernova remnant G11.2-0.3 by simulating jittering jets Long-time 3D supernova simulations of non-rotating progenitors with magnetic fields
Reference 163
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 0c0a40b2-9327-401d-9727-a1526a9e59e7 · inbound
Stellar black hole binaries from two common envelope evolution phases in triple stellar systems Long-time 3D supernova simulations of non-rotating progenitors with magnetic fields
Reference 167
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 5f48032f-111d-4a0d-87df-75746cd9dd3f · inbound
A "Neutrino Fog" For Gravitational Waves: The Stochastic Gravitational Wave Background from Supernova Neutrino Memory Long-time 3D supernova simulations of non-rotating progenitors with magnetic fields
Reference 68
Source-reported events for the cited work
Unavailable: canonical work link unavailable.