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Paper Citation Record · LEDGER

Clumpy Galaxies in CANDELS. II. Physical Properties of UV-bright Clumps at $0.5\leq z<3$

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1712.01858.

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

pith.paper-citation-record.v1
1712.01858 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 2026-08-07T06:34:17.273281+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-29T04:13:05.779645Z

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 8f6da9a4-7df6-42d1-a7af-ecb021194582 · inbound

Investigating black hole accretion and feedback self-regulation in Seyfert galaxies using the FIRE-3 cosmological hydrodynamic simulations cites this paper.

Investigating black hole accretion and feedback self-regulation in Seyfert galaxies using the FIRE-3 cosmological hydrodynamic simulations Clumpy Galaxies in CANDELS. II. Physical Properties of UV-bright Clumps at $0.5\leq z<3$

Reference 124

Resolution
verified exact
local_arxiv, observed 2026-06-25T23:48:42.858402Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:4fcd54c24a9ea3100c785a0615a97d6ec94e9844c608da14413c466dbd07d577

Observation 01f6115b-a137-41de-a09d-bdb775a00319 · inbound

Quantifying the inside-out formation of disk galaxies at $1.5 \le z \le 3.0$ cites this paper.

Quantifying the inside-out formation of disk galaxies at $1.5 \le z \le 3.0$ Clumpy Galaxies in CANDELS. II. Physical Properties of UV-bright Clumps at $0.5\leq z<3$

Reference 47

Resolution
verified exact
local_arxiv, observed 2026-06-26T01:38:50.975972Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:de6b2d7afdcf068c779deda7fe2648a5154b0dfb92a7c7b61001df63c7dac38b

Observation 409e8a11-d0f9-47e8-834c-02209d2c2487 · inbound

MSA-3D: Rotation Curves and Dark Matter Fractions at z~0.5-1.7 with JWST/NIRSpec cites this paper.

MSA-3D: Rotation Curves and Dark Matter Fractions at z~0.5-1.7 with JWST/NIRSpec Clumpy Galaxies in CANDELS. II. Physical Properties of UV-bright Clumps at $0.5\leq z<3$

Reference 193

Resolution
verified exact
local_arxiv, observed 2026-06-29T04:13:05.780874Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:8d3fdb8a91b6668a13ac742223e215bf954856510ffb7371d434b23a332f69e4