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Paper Citation Record · LEDGER

Using gravitational wave dark sirens to choose between host galaxy weighting models

As of 12 August 2026, this Paper Citation Record lists 2 of 2 outbound references and 1 inbound Pith citation observation for arXiv:2508.15574.

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

pith.paper-citation-record.v1
2508.15574 v1

Coverage vector

measured 2 of 2 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-05T17:53:12.910662Z

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T23:05:14.699329Z

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

2 of 2 outbound references displayed

  • verified exact1
  • verified fuzzy1
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation a9e1e50e-d579-49ab-a827-3ff1638ae787 · outbound

This paper cites *Corresponding author(s).

Using gravitational wave dark sirens to choose between host galaxy weighting models *Corresponding author(s)

Reference 1

Resolution
verified exact
raw_fallback, observed 2026-08-05T17:53:13.256447Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-08-05T17:53:12.826844Z digest=sha256:ac4a305ec48a166400a1e9c92d60c92a97afdaa9116d239c5258955b671a6ea3

Observation bd7916f9-c7fd-4f6a-977d-a4338bafb91f · outbound

This paper cites For the same number of iterations the model built using the LFaB scheme results in an MAE of about 1.5 kcal/mol.

Using gravitational wave dark sirens to choose between host galaxy weighting models For the same number of iterations the model built using the LFaB scheme results in an MAE of about 1.5 kcal/mol

Reference 4

Resolution
verified fuzzy
raw_fallback, observed 2026-08-05T17:53:13.474575Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-08-05T17:53:12.910662Z digest=sha256:63ab73e4afc57a727505dbf2545cfba7e9362dcaf19fe7d2d600dd90cae1ec83

Pith citing papers

Observation b328c250-f7e0-4e36-a1f4-478a4aeef78c · inbound

The impact of precession and higher-order multipoles for gravitational wave cosmological inference cites this paper.

The impact of precession and higher-order multipoles for gravitational wave cosmological inference Using gravitational wave dark sirens to choose between host galaxy weighting models

Reference 38

Resolution
unresolved
no resolver link, observed 2026-08-03T23:05:14.699329Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T23:05:14.699329Z digest=sha256:d62e4d6b8ddd14d115fd80e4666596e8be3d2b0243dc78ca07567437973b4710