Paper Citation Record · LEDGER

LISA data analysis: Source identification and subtraction

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:astro-ph/0301548.

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

pith.paper-citation-record.v1
astro-ph/0301548 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T22:29:59.795255Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-16T23:11:20.883840Z

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 1470e348-3750-4266-9c93-7114e38a5300 · inbound

Detectability and Parameter Estimation for Einstein Telescope Configurations with GWJulia cites this paper.

Detectability and Parameter Estimation for Einstein Telescope Configurations with GWJulia LISA data analysis: Source identification and subtraction

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-06T22:29:59.795255Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b052da56-663f-429c-83b3-cc21ee78a404 · inbound

A Multimessenger Strategy for Downselecting the Orientations of Galactic Close White Dwarf Binaries cites this paper.

A Multimessenger Strategy for Downselecting the Orientations of Galactic Close White Dwarf Binaries LISA data analysis: Source identification and subtraction

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-06T21:11:17.400626Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9b9eb8ea-75b0-4ec6-9b49-618c798280cd · inbound

Gravitational-wave parameter estimation to the Moon and back: massive binaries and the case of GW231123 cites this paper.

Gravitational-wave parameter estimation to the Moon and back: massive binaries and the case of GW231123 LISA data analysis: Source identification and subtraction

Reference 69

Resolution: verified exact; local_arxiv, observed 2026-05-16T23:11:20.885624Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 0834f760-62c2-4fa5-8408-4a4645eb8843 · inbound

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals cites this paper.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals LISA data analysis: Source identification and subtraction

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:34.726687Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 145308ac-16a1-4e64-89b0-7cd3d80b4674 · inbound

Probing the Orientation Distribution of Nearby Double White Dwarfs through Gravitational Waves with LISA cites this paper.

Probing the Orientation Distribution of Nearby Double White Dwarfs through Gravitational Waves with LISA LISA data analysis: Source identification and subtraction

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-02T05:33:16.801474Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2200e731-ade4-4141-bdfc-8e923f4912ee · inbound

Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy cites this paper.

Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy LISA data analysis: Source identification and subtraction

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-01T02:48:49.228374Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.