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Paper Citation Record · LEDGER

A Precise Distance to the Host Galaxy of the Binary Neutron Star Merger GW170817 Using Surface Brightness Fluctuations

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1801.06080.

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

pith.paper-citation-record.v1
1801.06080 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-04T06:34:03.388597+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T00:40:14.150525Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-18T21:55:02.284490Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
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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 57ff7ef6-97a8-4d1d-8b61-855530230cbc · inbound

Bayesian inference for compact binary coalescences with BILBY: Validation and application to the first LIGO--Virgo gravitational-wave transient catalogue cites this paper.

Bayesian inference for compact binary coalescences with BILBY: Validation and application to the first LIGO--Virgo gravitational-wave transient catalogue A Precise Distance to the Host Galaxy of the Binary Neutron Star Merger GW170817 Using Surface Brightness Fluctuations

Reference 240

Resolution
verified exact
local_arxiv, observed 2026-05-18T21:55:02.290530Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:67b20ac57b5051764b4f88184888afd19bfde150d78def814b657f5739a5daf3

Observation c9aeea1f-02cf-4470-999b-0a8a0b1203f4 · inbound

Constraining Hamiltonians from chiral effective field theory with neutron-star data cites this paper.

Constraining Hamiltonians from chiral effective field theory with neutron-star data A Precise Distance to the Host Galaxy of the Binary Neutron Star Merger GW170817 Using Surface Brightness Fluctuations

Reference 77

Resolution
unresolved
no resolver link, observed 2026-08-04T00:40:14.150525Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T00:40:14.150525Z digest=sha256:8fd6ff29df50e609ebf0fc073f0ecb6bb3c19dc09cc901be2fa2e6b2017a252a

Observation f51c7d05-a9f0-464c-b5e7-8a1bdb40fed0 · inbound

Modernising Reinforcement Learning-Based Navigation for Embodied Semantic Scene Graph Generation cites this paper.

Modernising Reinforcement Learning-Based Navigation for Embodied Semantic Scene Graph Generation A Precise Distance to the Host Galaxy of the Binary Neutron Star Merger GW170817 Using Surface Brightness Fluctuations

Reference 17

Resolution
unresolved
no resolver link, observed 2026-07-13T18:17:13.161529Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-13T18:17:13.161529Z digest=sha256:ab35ad2f25a7c7a0e608523f1e7a0fb7018bdf3a41d8b59f7556d657f68783e6

Observation 96bd8119-2b82-4f80-9bd3-c722c47155bf · inbound

Black hole-neutron star binaries with high spins and large mass asymmetries: III. Properties of the ejected material and its electromagnetic signatures cites this paper.

Black hole-neutron star binaries with high spins and large mass asymmetries: III. Properties of the ejected material and its electromagnetic signatures A Precise Distance to the Host Galaxy of the Binary Neutron Star Merger GW170817 Using Surface Brightness Fluctuations

Reference 171

Resolution
unresolved
no resolver link, observed 2026-08-01T09:55:52.308338Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T09:55:52.308338Z digest=sha256:4111a8474846ea54a55426e38e780854e5c282c17a4ec80732b819545e3fb391