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Paper Citation Record · LEDGER

Color Profiles of Spiral Galaxies: Clues on Outer-Disk Formation Scenarios

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:0807.2776.

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

pith.paper-citation-record.v1
0807.2776 v2

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 2026-08-05T06:32:48.257954+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T23:42:37.846423Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

195
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 660fe102-b707-44cc-8c55-ef7b9e48f35c · 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 Color Profiles of Spiral Galaxies: Clues on Outer-Disk Formation Scenarios

Reference 65

Resolution
verified exact
local_arxiv, observed 2026-05-20T08:58:09.821516Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:05c098ede31f00af566bc19a4ee34e4fbfa43900abc76be93985866c4a42fd82

Observation 2d052ba4-9e91-403f-ba58-86bca0069470 · inbound

Projection-Enhanced Disk Breaks: Evidence from Deep Photometric Decomposition cites this paper.

Projection-Enhanced Disk Breaks: Evidence from Deep Photometric Decomposition Color Profiles of Spiral Galaxies: Clues on Outer-Disk Formation Scenarios

Reference 32

Resolution
verified exact
local_arxiv, observed 2026-07-02T08:56:49.038727Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=pdf_text observed=2026-07-11T11:50:26.030339Z digest=sha256:dee78367f6af7c47f95a8603aa5bd9884ea543cb43debe99b1076323d777e342

Observation 7a005135-79fc-4ce0-a057-3a3726352d6c · 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 Color Profiles of Spiral Galaxies: Clues on Outer-Disk Formation Scenarios

Reference 62

Resolution
unresolved
no resolver link, observed 2026-08-01T23:42:37.846423Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T23:42:37.846423Z digest=sha256:c2560329374e271575927ed28237da003e0fc3bb64807373fd03cb1f495516db