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Paper Citation Record · LEDGER

Accounting for Source Uncertainties in Analyses of Astronomical Survey Data

As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 14 inbound Pith citation observations for arXiv:astro-ph/0409387.

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

pith.paper-citation-record.v1
astro-ph/0409387 v1

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Source: paper_references, paper_reference_links

measured 14 of 14 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00

measured 14 of 14 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T10:19:04.544885Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-30T14:34:46.067687Z

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 23e54de5-3996-4827-8068-2e90276874f5 · inbound

Tests of General Relativity with Binary Black Holes from the second LIGO-Virgo Gravitational-Wave Transient Catalog cites this paper.

Tests of General Relativity with Binary Black Holes from the second LIGO-Virgo Gravitational-Wave Transient Catalog Accounting for Source Uncertainties in Analyses of Astronomical Survey Data

Reference 88

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local_arxiv, observed 2026-05-15T03:47:46.302677Z

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Constraining Population III stellar demographics with next-generation gravitational-wave observatories cites this paper.

Constraining Population III stellar demographics with next-generation gravitational-wave observatories Accounting for Source Uncertainties in Analyses of Astronomical Survey Data

Reference 155

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A fast deep-learning approach to probing primordial black hole populations in gravitational wave events cites this paper.

A fast deep-learning approach to probing primordial black hole populations in gravitational wave events Accounting for Source Uncertainties in Analyses of Astronomical Survey Data

Reference 57

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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 Accounting for Source Uncertainties in Analyses of Astronomical Survey Data

Reference 136

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Observation 6ac0c494-6d13-4a33-880d-0a76c4d55f51 · inbound

Disentangling spinning and nonspinning binary black hole populations with spin sorting cites this paper.

Disentangling spinning and nonspinning binary black hole populations with spin sorting Accounting for Source Uncertainties in Analyses of Astronomical Survey Data

Reference 73

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local_arxiv, observed 2026-05-19T02:22:56.273988Z

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Observation c83ac349-ee54-4f04-98b1-fe64c1b39bbb · inbound

Population Properties of Binary Black Holes with Eccentricity cites this paper.

Population Properties of Binary Black Holes with Eccentricity Accounting for Source Uncertainties in Analyses of Astronomical Survey Data

Reference 94

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Observation bf70fcc9-94f6-4dd2-b151-96208c113fb6 · inbound

Gravitational-wave astronomy requires population-informed parameter estimation cites this paper.

Gravitational-wave astronomy requires population-informed parameter estimation Accounting for Source Uncertainties in Analyses of Astronomical Survey Data

Reference 12

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arxiv_id, observed 2026-05-10T08:22:37.312941Z

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Observation b307f936-ceea-4327-b230-6e6a31607fcf · inbound

Gravitational-wave astronomy requires population-informed parameter estimation cites this paper.

Gravitational-wave astronomy requires population-informed parameter estimation Accounting for Source Uncertainties in Analyses of Astronomical Survey Data

Reference 12

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Observation 852a0ef7-eb27-437e-8a21-85d287669a83 · inbound

Radio sirens: inferring $H_0$ with binary black holes and neutral hydrogen in the era of the Einstein Telescope and the SKA Observatory cites this paper.

Radio sirens: inferring $H_0$ with binary black holes and neutral hydrogen in the era of the Einstein Telescope and the SKA Observatory Accounting for Source Uncertainties in Analyses of Astronomical Survey Data

Reference 68

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local_arxiv, observed 2026-05-14T20:37:57.714396Z

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Observation adeb9685-ebcb-45f9-b6ec-de44565ca91d · 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 Accounting for Source Uncertainties in Analyses of Astronomical Survey Data

Reference 39

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local_arxiv, observed 2026-06-28T05:11:39.700421Z

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Observation 0f1df25e-4b02-4aec-9b16-97f92314a9f2 · inbound

When the black holes align: a subpopulation of aligned massive binary black holes observed via gravitational waves cites this paper.

When the black holes align: a subpopulation of aligned massive binary black holes observed via gravitational waves Accounting for Source Uncertainties in Analyses of Astronomical Survey Data

Reference 57

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local_arxiv, observed 2026-06-26T07:39:07.587036Z

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Observation c8f72b32-ee59-4860-9f15-343cb8c32b02 · 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 Accounting for Source Uncertainties in Analyses of Astronomical Survey Data

Reference 48

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local_arxiv, observed 2026-06-30T14:34:46.069036Z

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Observation a220c7aa-23c5-4d5c-a43e-df5716451369 · inbound

Uncovering Hierarchical Sub-Population of Binary Black Holes cites this paper.

Uncovering Hierarchical Sub-Population of Binary Black Holes Accounting for Source Uncertainties in Analyses of Astronomical Survey Data

Reference 78

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Assessing the waveform systematics from parameter estimation to population inference with eccentricity cites this paper.

Assessing the waveform systematics from parameter estimation to population inference with eccentricity Accounting for Source Uncertainties in Analyses of Astronomical Survey Data

Reference 88

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