Pith. sign in

Paper Citation Record · LEDGER

A simple model for magnetic reconnection heated corona

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0205257.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
astro-ph/0205257 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-07-03T08:27:48.247046Z

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 fb326502-ca3e-4ace-86f0-3a058a6693cd · inbound

Neutrino and pair creation in reconnection-powered coronae of accreting black holes cites this paper.

Neutrino and pair creation in reconnection-powered coronae of accreting black holes A simple model for magnetic reconnection heated corona

Reference 5

Resolution
verified exact
local_arxiv, observed 2026-05-23T19:15:47.451904Z

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.

source=pdf_text observed=2026-05-23T19:09:50.863935Z digest=sha256:8434e950be836c0c4485ad68e12406401d065df78d91e30be665352fe144f551

Observation 5e2f2989-dcc1-44c7-8378-f7d6f0f5de6d · inbound

Bolometric correction factor and radiative efficiency for the super-Eddington accretion flow in tidal disruption events cites this paper.

Bolometric correction factor and radiative efficiency for the super-Eddington accretion flow in tidal disruption events A simple model for magnetic reconnection heated corona

Reference 92

Resolution
verified exact
local_arxiv, observed 2026-07-03T08:27:48.248205Z

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.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:48f4250595ad54b44a7d6337eb2eb60f671daabb13743736970d112436e2d911