Pith. sign in

Paper Citation Record · LEDGER

Black Hole Mass Accretion Rates and Efficiency Factors for over 750 AGN and Multiple GBH

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2010.06908.

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

pith.paper-citation-record.v1
2010.06908 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 2026-08-16T06:30:59.297886+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T18:38:08.008178Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-15T18:38:08.063993Z

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 3b21e683-5acd-4d00-bc90-7b0437669a81 · inbound

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots cites this paper.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Black Hole Mass Accretion Rates and Efficiency Factors for over 750 AGN and Multiple GBH

Reference 70

Resolution
verified exact
local_arxiv, observed 2026-08-15T18:38:08.070692Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

source=pdf_text observed=2026-08-15T18:38:08.008178Z digest=sha256:fe9d575e66dbd2782b94461e2d6fc09c1a40f601e185b63880343a51979b1ed2

Observation b8b40eb0-ff33-4a7b-b274-4e85196903c0 · inbound

Comprehensive X-ray Study of Giant Radio Galaxies with XMM-Newton and Chandra cites this paper.

Comprehensive X-ray Study of Giant Radio Galaxies with XMM-Newton and Chandra Black Hole Mass Accretion Rates and Efficiency Factors for over 750 AGN and Multiple GBH

Reference 104

Resolution
unresolved
no resolver link, observed 2026-08-01T01:57:42.836568Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T01:57:42.836568Z digest=sha256:9b82d0ce05145bbd19770591b92987ac2dc5945b3b4f03d6958d13a518b30f20