Pith. sign in

Paper Citation Record · LEDGER

Who Ordered That? Unequal-Mass Binary Black Hole Mergers Have Larger Effective Spins

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2106.00521.

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

pith.paper-citation-record.v1
2106.00521 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 9 of 9 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 9 of 9 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T15:36:23.129557Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T06:59:38.018894Z

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 52438c4c-4f8f-45d2-a613-5c2f9cfb901b · inbound

Waveform Modelling for the Laser Interferometer Space Antenna cites this paper.

Waveform Modelling for the Laser Interferometer Space Antenna Who Ordered That? Unequal-Mass Binary Black Hole Mergers Have Larger Effective Spins

Reference 201

Resolution
verified exact
arxiv_id, observed 2026-05-24T05:23:57.848294Z

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.

source=pdf_text observed=2026-05-24T05:21:16.199631Z digest=sha256:bc544cfb33a340d6524cada7ee225d6085659cf55b5061965f208df1593d55cf

Observation 5c2a6288-f8ee-49a7-847c-f32ad09a9961 · inbound

The Long Road to Alignment: Measuring Black Hole Spin Orientation with Expanding Gravitational-Wave Datasets cites this paper.

The Long Road to Alignment: Measuring Black Hole Spin Orientation with Expanding Gravitational-Wave Datasets Who Ordered That? Unequal-Mass Binary Black Hole Mergers Have Larger Effective Spins

Reference 40

Resolution
unresolved
no resolver link, observed 2026-08-07T15:36:23.129557Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T15:36:23.129557Z digest=sha256:1bb2361a7318183baa97ed23be3493aa2f529a2760f085c4876a9cc0fd2424f4

Observation ff15c954-99b6-4aba-9dcd-70cb3d154f70 · inbound

Inferring the pair-instability mass gap from gravitational wave data cites this paper.

Inferring the pair-instability mass gap from gravitational wave data Who Ordered That? Unequal-Mass Binary Black Hole Mergers Have Larger Effective Spins

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-07T05:02:01.032530Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T05:02:01.032530Z digest=sha256:ebbb4da26b6b76c88a932169839cb6cf23d46be24f6de3e2cef8b7e0f1d9152d

Observation d37c289a-cf4d-419b-b6f6-15972461fe33 · inbound

Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop cites this paper.

Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Who Ordered That? Unequal-Mass Binary Black Hole Mergers Have Larger Effective Spins

Reference 105

Resolution
unresolved
no resolver link, observed 2026-08-06T22:52:12.369033Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T22:52:12.369033Z digest=sha256:08355382d339a9fd8414bfd9edb9883f39df09df60f9e22993b827b4bfb453d1

Observation d9bf48da-5ba6-4845-b39b-b71378b03bde · inbound

Comparing astrophysical models to gravitational-wave data in the observable space cites this paper.

Comparing astrophysical models to gravitational-wave data in the observable space Who Ordered That? Unequal-Mass Binary Black Hole Mergers Have Larger Effective Spins

Reference 21

Resolution
verified exact
arxiv_id, observed 2026-05-19T04:37:03.835914Z

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.

source=pdf_text observed=2026-05-19T04:36:12.661648Z digest=sha256:d0387efdc2e406b5a18a4549b087fabfa361782a6d72d01a7467e1e847340e09

Observation cc71f3d9-3e65-4354-af31-41f48f9ed889 · inbound

Posterior Predictive Checks for Gravitational-wave Populations: Limitations and Improvements cites this paper.

Posterior Predictive Checks for Gravitational-wave Populations: Limitations and Improvements Who Ordered That? Unequal-Mass Binary Black Hole Mergers Have Larger Effective Spins

Reference 49

Resolution
verified exact
arxiv_id, observed 2026-05-10T23:25:49.912395Z

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.

source=pdf_text observed=2026-05-10T19:10:35.351205Z digest=sha256:01e6e5ecad14fede495854bf16ad4160be89aee929096074d53b8a36ed85de1f

Observation ba3c28c9-4a0b-4da8-b7ac-056cd6a4ae62 · inbound

Emergent structure in the binary black hole mass distribution and implications for population-based cosmology cites this paper.

Emergent structure in the binary black hole mass distribution and implications for population-based cosmology Who Ordered That? Unequal-Mass Binary Black Hole Mergers Have Larger Effective Spins

Reference 62

Resolution
verified exact
arxiv_id, observed 2026-05-11T11:51:01.539656Z

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.

source=pdf_text observed=2026-05-10T12:31:50.358428Z digest=sha256:268913587bbbeb6fb54fd4d3d48d75aae6048cf0a10d01297b6ef9e869b3e193

Observation 35e945c9-3e3a-42a7-8a0e-6ced95adc424 · inbound

Population-level correlations in Bayesian statistics: an illustrative model for gravitational-wave astronomy cites this paper.

Population-level correlations in Bayesian statistics: an illustrative model for gravitational-wave astronomy Who Ordered That? Unequal-Mass Binary Black Hole Mergers Have Larger Effective Spins

Reference 24

Resolution
verified exact
arxiv_id, observed 2026-07-04T06:59:38.020493Z

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.

source=pdf_text observed=2026-06-26T13:59:14.326070Z digest=sha256:95d89cd91fd8d6d9b3a618701b9e83756301cb70855c284508a5a6c07651259f

Observation b6ffea3a-a2e7-4c5d-8407-1f3a66eaecd8 · 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 Who Ordered That? Unequal-Mass Binary Black Hole Mergers Have Larger Effective Spins

Reference 117

Resolution
verified exact
arxiv_id, observed 2026-06-30T14:34:45.613557Z

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.

source=pdf_text observed=2026-06-30T05:24:03.103599Z digest=sha256:7740e490873e06f7c5ad02c22a76b3e8af80abff1e17973ddc3b8705b98eeae2