Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2408.00848.
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 2026-08-15T06:32:42.880941+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-12T12:34:30.167694Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-10T05:30:23.456663Z
0 of 0 outbound references displayed
External citation measurements
2
pith, observed 2026-08-10T05:30:23.456663Z
No outbound reference observations are available for this paper version.
Observation bedbe6b7-4b21-4088-b0af-b24cd3bba7fe · inbound
Secret of Longevity: Protoplanetary Disks as a Source of Gas in Debris Disks Photoevaporation of protoplanetary discs with PLUTO+PRIZMO I. Lower X-ray-driven mass-loss rates due to enhanced cooling
Reference 81
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1c2cabfb-094d-445f-b71d-d4e20bb43089 · inbound
A possible trail of dust from a young, highly-extincted brown dwarf in the outskirts of the Trapezium Cluster Photoevaporation of protoplanetary discs with PLUTO+PRIZMO I. Lower X-ray-driven mass-loss rates due to enhanced cooling
Reference 80
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 44b47133-42d1-47f9-a6ae-1ddc4ea4437b · inbound
The ALMA Survey of Gas Evolution of PROtoplanetary Disks (AGE-PRO): VII. Testing accretion mechanisms from disk population synthesis Photoevaporation of protoplanetary discs with PLUTO+PRIZMO I. Lower X-ray-driven mass-loss rates due to enhanced cooling
Reference 100
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.