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Paper Citation Record · LEDGER

Reinterpreting Low Frequency LIGO/Virgo Events as Magnified Stellar-Mass Black Holes at Cosmological Distances

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:1802.05273.

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

pith.paper-citation-record.v1
1802.05273 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T17:35:01.587093Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

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External citation measurements

26
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation e3b5553d-bdf7-4faf-b1a5-02fae018bf55 · inbound

GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs cites this paper.

GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs Reinterpreting Low Frequency LIGO/Virgo Events as Magnified Stellar-Mass Black Holes at Cosmological Distances

Reference 185

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verified exact
arxiv_id, observed 2026-05-12T14:08:36.743702Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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Observation 1d5b5485-6310-4f1b-b574-759dd976d004 · inbound

Retrieving the True Masses of Gravitational-wave Sources cites this paper.

Retrieving the True Masses of Gravitational-wave Sources Reinterpreting Low Frequency LIGO/Virgo Events as Magnified Stellar-Mass Black Holes at Cosmological Distances

Reference 13

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verified exact
local_arxiv, observed 2026-05-25T15:15:58.881490Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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Observation 418c6155-b149-4f89-aed3-317a9a240162 · inbound

Using time series to identify strongly-lensed gravitational waves with deep learning cites this paper.

Using time series to identify strongly-lensed gravitational waves with deep learning Reinterpreting Low Frequency LIGO/Virgo Events as Magnified Stellar-Mass Black Holes at Cosmological Distances

Reference 17

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unresolved
no resolver link, observed 2026-08-12T17:35:01.587093Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation e5794517-9f8d-4a03-8d18-6a909fcc2c63 · inbound

Spin Precession Signatures as an Indicator of Microlensing in Strongly Lensed Gravitational Waves cites this paper.

Spin Precession Signatures as an Indicator of Microlensing in Strongly Lensed Gravitational Waves Reinterpreting Low Frequency LIGO/Virgo Events as Magnified Stellar-Mass Black Holes at Cosmological Distances

Reference 17

Resolution
unresolved
no resolver link, observed 2026-08-05T14:31:12.907860Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 12bbe226-7996-4bf5-900c-c04c3ab6b8a8 · inbound

Can Eccentric Binary Black Hole Signals Mimic Gravitational-Wave Microlensing? cites this paper.

Can Eccentric Binary Black Hole Signals Mimic Gravitational-Wave Microlensing? Reinterpreting Low Frequency LIGO/Virgo Events as Magnified Stellar-Mass Black Holes at Cosmological Distances

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-03T18:57:02.389218Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T18:57:02.389218Z digest=sha256:3f8f2d9c0f617b3062cac5f3e03f7d367893781643dac5090bb8233a41b24ad5

Observation 3a788534-d7ce-4bab-ba79-b394435a567f · inbound

Across the Universe: GW231123 as a magnified and diffracted black hole merger cites this paper.

Across the Universe: GW231123 as a magnified and diffracted black hole merger Reinterpreting Low Frequency LIGO/Virgo Events as Magnified Stellar-Mass Black Holes at Cosmological Distances

Reference 18

Resolution
unresolved
no resolver link, observed 2026-08-03T15:22:16.006047Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 374c7c4b-bac2-4bbb-a485-d99440492ae2 · inbound

Mapping the star formation peak with LIGO A# and Next-Generation detectors cites this paper.

Mapping the star formation peak with LIGO A# and Next-Generation detectors Reinterpreting Low Frequency LIGO/Virgo Events as Magnified Stellar-Mass Black Holes at Cosmological Distances

Reference 227

Resolution
metadata mismatch
local_arxiv, observed 2026-06-28T05:11:39.697402Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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Observation 9653ca99-389c-419f-a3b2-4fdcb57e3ee5 · inbound

Joint population and strong-lensing inference for resolved gravitational-wave events probes the black-hole merger rate beyond the peak of star formation cites this paper.

Joint population and strong-lensing inference for resolved gravitational-wave events probes the black-hole merger rate beyond the peak of star formation Reinterpreting Low Frequency LIGO/Virgo Events as Magnified Stellar-Mass Black Holes at Cosmological Distances

Reference 127

Resolution
verified exact
local_arxiv, observed 2026-06-30T14:34:45.941340Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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