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Paper Citation Record · LEDGER

Possible environmental quenching in an interacting little red dot pair at $z\sim7$

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2501.17925.

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

pith.paper-citation-record.v1
2501.17925 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 2026-08-10T06:31:04.303077+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T16:36:20.816775Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-06T22:27:12.364887Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • 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 f6e731f6-751d-48ec-ae67-806b2c9c9adc · inbound

CANUCS/Technicolor Data Release 1: Imaging, Photometry, Slit Spectroscopy, and Stellar Population Parameters cites this paper.

CANUCS/Technicolor Data Release 1: Imaging, Photometry, Slit Spectroscopy, and Stellar Population Parameters Possible environmental quenching in an interacting little red dot pair at $z\sim7$

Reference 12

Resolution
metadata mismatch
local_arxiv, observed 2026-08-06T22:27:12.438513Z

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=pdf_text observed=2026-08-06T22:27:11.895122Z digest=sha256:4424dd46978aa5de943f81c9bf83fb2f3c1397bb4beda25d7b072e62eb708d63

Observation 85aced76-19db-4744-96af-4b1b9da1428c · inbound

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs cites this paper.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Possible environmental quenching in an interacting little red dot pair at $z\sim7$

Reference 98

Resolution
unresolved
no resolver link, observed 2026-08-01T00:25:36.497655Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T00:25:36.497655Z digest=sha256:7f36b120771f163bf3855f83329c33a48f6cedc5af9d70e7e5d60afa795abe65

Observation 90d69796-eb04-4b40-a547-9fd4aef873a5 · inbound

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ cites this paper.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Possible environmental quenching in an interacting little red dot pair at $z\sim7$

Reference 126

Resolution
unresolved
no resolver link, observed 2026-08-08T16:36:20.816775Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T16:36:20.816775Z digest=sha256:3df872fa6b876a3bfffd4d6fec46623c029b263c67cded2746b0edb9e80bb0b6