Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-07T12:45:57.276875Z
Paper Citation Record · LEDGER
As of 8 August 2026, this Paper Citation Record lists 10 of 10 outbound references and 0 inbound Pith citation observations for arXiv:2505.23544.
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, observed 2026-08-07T12:45:57.276875Z
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links
A source-named dated measurement, never combined with another source.
Source: cited_works
10 of 10 outbound references displayed
External citation measurements
No source-named external measurement is stored.
Observation 8f33f0c3-67d9-4c07-b1ae-6d7cc5108384 · outbound
Metagalactic Ultraviolet Background Tables for Calculating Diffuse Astrophysical Plasma Properties , " * write output.state after.block = add.period write newline
Reference 1
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e73d68a1-b034-416d-a831-4460d494cf8b · outbound
Metagalactic Ultraviolet Background Tables for Calculating Diffuse Astrophysical Plasma Properties write newline
Reference 2
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c5ed543e-fe23-4cc7-b937-bbc72c6d54b8 · outbound
Metagalactic Ultraviolet Background Tables for Calculating Diffuse Astrophysical Plasma Properties c D ) @ S <@ yL 1
Reference 3
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation defcaab5-c1ee-4d2b-926e-46382422c571 · outbound
Metagalactic Ultraviolet Background Tables for Calculating Diffuse Astrophysical Plasma Properties 2020, , 493, 1614, 10.1093/mnras/staa302
Reference 4
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b689a401-860b-43aa-90d1-b62596f27968 · outbound
Metagalactic Ultraviolet Background Tables for Calculating Diffuse Astrophysical Plasma Properties 2009, , 703, 1416, 10.1088/0004-637X/703/2/1416
Reference 5
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 18e92291-0b11-4f87-b1ce-d1d3d8b8a1b5 · outbound
Metagalactic Ultraviolet Background Tables for Calculating Diffuse Astrophysical Plasma Properties The 2013 Release of Cloudy
Reference 6
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d92b06d5-1b5c-4cfb-8e69-32ed7d1bb435 · outbound
Metagalactic Ultraviolet Background Tables for Calculating Diffuse Astrophysical Plasma Properties 2012, , 746, 125, 10.1088/0004-637X/746/2/125
Reference 7
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 84ae382c-dc1b-43d4-9936-f1f225625068 · outbound
Metagalactic Ultraviolet Background Tables for Calculating Diffuse Astrophysical Plasma Properties B., Smith , B
Reference 8
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a32607eb-fd7c-47fb-ae0e-8de2ea2a4d5b · outbound
Metagalactic Ultraviolet Background Tables for Calculating Diffuse Astrophysical Plasma Properties G., & Madau, P
Reference 9
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ee1eeff1-d148-4139-8ba4-f9cb3725d8a6 · outbound
Metagalactic Ultraviolet Background Tables for Calculating Diffuse Astrophysical Plasma Properties 2025, tairaeli/Metagalactic\_Ultraviolet\_Background\_Data\_ Tables: Ultraviolet Background Data Table Reformat, v1.0.0, Zenodo, 10.5281/zenodo.15367103
Reference 10
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
No inbound Pith citation observations are available.