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Paper Citation Record · LEDGER

How would GW150914 look with future GW detector networks?

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1703.08988.

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

pith.paper-citation-record.v1
1703.08988 v2

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 2026-08-10T06:31:04.303077+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T10:46:06.121690Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-06T20:31:48.477073Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • 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 23161443-b750-48a9-8a47-45b67abd2927 · inbound

Statistical biases in parametrized searches for gravitational-wave polarizations cites this paper.

Statistical biases in parametrized searches for gravitational-wave polarizations How would GW150914 look with future GW detector networks?

Reference 64

Resolution
unresolved
no resolver link, observed 2026-08-10T10:46:06.121690Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T10:46:06.121690Z digest=sha256:9aa25a20ee1b7b516ae7c99bd3d3e7a7ced1eee7843ec0da7d294c23fafbb4a1

Observation 069ad70d-27a5-4ee9-8376-effc85896a99 · inbound

PhenomXPNR: An improved gravitational wave model linking precessing inspirals and NR-calibrated merger-ringdown cites this paper.

PhenomXPNR: An improved gravitational wave model linking precessing inspirals and NR-calibrated merger-ringdown How would GW150914 look with future GW detector networks?

Reference 65

Resolution
verified exact
local_arxiv, observed 2026-08-06T20:31:48.480184Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-08-06T20:31:47.977664Z digest=sha256:b64f1c4c0f25a34b5c446b23833834ae6a6ecd5a02f2a3c0a7e5d9cfec31b401