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Paper Citation Record · LEDGER

A massive interacting galaxy 510 million years after the Big Bang

As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2303.00306.

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

pith.paper-citation-record.v1
2303.00306 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-20T06:33:59.587034+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T04:26:10.414488Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-11T10:19:03.912444Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • malformed identifier0
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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 d0e3ef4e-ab76-45ce-bda4-a9ad150087ae · inbound

High-z stellar masses can be recovered robustly with JWST photometry cites this paper.

High-z stellar masses can be recovered robustly with JWST photometry A massive interacting galaxy 510 million years after the Big Bang

Reference 2023

Resolution
unresolved
no resolver link, observed 2026-08-11T23:20:51.959779Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T23:20:51.959779Z digest=sha256:a6aa3ec8e5a5ca5fd59cc3d9b2286f778716e292c948d2b99105683a3394fb2e

Observation fa387a31-5060-4e33-82f4-c642c1178ad4 · inbound

Evolution of Size, Mass, and Density of Galaxies Since Cosmic Dawn cites this paper.

Evolution of Size, Mass, and Density of Galaxies Since Cosmic Dawn A massive interacting galaxy 510 million years after the Big Bang

Reference 28

Resolution
unresolved
no resolver link, observed 2026-08-04T10:26:46.699516Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T10:26:46.699516Z digest=sha256:374de797e74d9b0e578ef6dc37e9151f1864e0c6977543687aa7a7377d51ef5e

Observation fe8a3592-d6a9-4f65-a369-0ec7b4abca90 · inbound

A Massive Galaxy at the Edge of Feedback-Free Efficiency cites this paper.

A Massive Galaxy at the Edge of Feedback-Free Efficiency A massive interacting galaxy 510 million years after the Big Bang

Reference 9

Resolution
unresolved
no resolver link, observed 2026-08-03T04:05:16.774052Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-03T04:05:16.774052Z digest=sha256:b22bda3e4b27163c734729c6182a735e68e4efa19165d5e02e0ae2f195f4744f

Observation 58aed349-ed80-4444-9b66-8584c9b2ffb9 · inbound

An emerging baryon cycle in a galaxy 500 million years after the Big Bang cites this paper.

An emerging baryon cycle in a galaxy 500 million years after the Big Bang A massive interacting galaxy 510 million years after the Big Bang

Reference 4

Resolution
metadata mismatch
local_arxiv, observed 2026-08-11T10:19:03.916334Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-08-11T10:19:02.215081Z digest=sha256:16c20aadab9d97dfcbd375cc3bc560fdd214d4ccaf9421e1e8f0382dab7e73ce

Observation 793fc451-a90f-4cef-a18e-7e5d62794fbb · inbound

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics cites this paper.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics A massive interacting galaxy 510 million years after the Big Bang

Reference 285

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:18.888399Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:18.888399Z digest=sha256:afd2b180aca0212515a2878b00211b07edbd1a3a761c7b689cca25485b36168f

Observation 2045e9c0-7259-4746-beb6-3854b50eef2d · inbound

SPURS: Massive Stars, Dense Gas, and Ly$\alpha$ Escape in GN-z11 at $z = 10.6$ cites this paper.

SPURS: Massive Stars, Dense Gas, and Ly$\alpha$ Escape in GN-z11 at $z = 10.6$ A massive interacting galaxy 510 million years after the Big Bang

Reference 210

Resolution
unresolved
no resolver link, observed 2026-08-16T04:26:10.414488Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T04:26:10.414488Z digest=sha256:76e5fd7e425193d497577d59d38e6856390a0f5c60e99d180f3ef1def8858182