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Paper Citation Record · LEDGER

The influence of diffuse scattered light I. The PSF and its role to observations of the edge-on galaxy NGC 5907

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1406.5508.

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

pith.paper-citation-record.v1
1406.5508 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 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 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T23:42:37.538619Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-20T08:58:09.920224Z

Reference resolution

0 of 0 outbound references displayed

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External citation measurements

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 8d00eb6c-e33e-4902-81ba-18578b0a1708 · inbound

Witnessing the rapid growth of disk galaxies over cosmic time using JWST and HST cites this paper.

Witnessing the rapid growth of disk galaxies over cosmic time using JWST and HST The influence of diffuse scattered light I. The PSF and its role to observations of the edge-on galaxy NGC 5907

Reference 201

Resolution
verified exact
local_arxiv, observed 2026-05-19T15:27:38.192339Z

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=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:a6a38513021d0b7f1ef12702c28f4459e5ed4d6c4fcbfc3f4b7987b0e35adbc2

Observation d8ae7dbb-d237-4417-9ff6-29b6cbaa3fc3 · inbound

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies cites this paper.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies The influence of diffuse scattered light I. The PSF and its role to observations of the edge-on galaxy NGC 5907

Reference 12

Resolution
verified exact
local_arxiv, observed 2026-05-20T08:58:09.921650Z

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=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:dec70c439438bf34cc2b11881a67e3752e4310774102ea98bc341356cbf1c869

Observation ec3f321b-bb20-4c15-a22c-e338f52da9db · inbound

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy cites this paper.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy The influence of diffuse scattered light I. The PSF and its role to observations of the edge-on galaxy NGC 5907

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-01T23:42:37.538619Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T23:42:37.538619Z digest=sha256:595b9ea790b40e6ae0e1bf4af9bd0979ca48d8dea46eb7a07b88fd99a9e800b2