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Paper Citation Record · LEDGER

Extremely red galaxies at $z=5-9$ with MIRI and NIRSpec: dusty galaxies or obscured AGNs?

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2305.14418.

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

pith.paper-citation-record.v1
2305.14418 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 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 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T18:47:40.755015Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, 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

8
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 7a729765-3246-47a4-8e6f-8f41eb59b4db · inbound

Discovery of Multiply Ionized Iron Emission Powered by an Active Galactic Nucleus in a z~7 Little Red Dot cites this paper.

Discovery of Multiply Ionized Iron Emission Powered by an Active Galactic Nucleus in a z~7 Little Red Dot Extremely red galaxies at $z=5-9$ with MIRI and NIRSpec: dusty galaxies or obscured AGNs?

Reference 15

Resolution
unresolved
no resolver link, observed 2026-08-04T18:47:40.755015Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T18:47:40.755015Z digest=sha256:4a482a02a0f3d7bb236982686745429e877f51b07dbea89313e77c8c5d67124f

Observation 5e479e3e-cb5e-4d9e-ae42-7bae4237612f · inbound

Gravitational Waves from the Cosmic Dawn: Tracing Cosmic Black Hole Binaries with ET, LGWA and LISA cites this paper.

Gravitational Waves from the Cosmic Dawn: Tracing Cosmic Black Hole Binaries with ET, LGWA and LISA Extremely red galaxies at $z=5-9$ with MIRI and NIRSpec: dusty galaxies or obscured AGNs?

Reference 51

Resolution
metadata mismatch
arxiv_id, observed 2026-05-10T05:00:36.924938Z

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=2026-05-10T04:58:18.085345Z digest=sha256:7d611d1f9d7cdf488bb0617fdefcd8fd3e9f6d40fdbffe6737d4dfe98517a276

Observation 299ea48e-5fa6-44db-a5ba-733468e32914 · inbound

Origins of Extreme Emission-Line Ratios in z > 3 Galaxies: Insights from the Lumen Model cites this paper.

Origins of Extreme Emission-Line Ratios in z > 3 Galaxies: Insights from the Lumen Model Extremely red galaxies at $z=5-9$ with MIRI and NIRSpec: dusty galaxies or obscured AGNs?

Reference 212

Resolution
verified exact
arxiv_id, observed 2026-05-11T01:30:51.643092Z

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=2026-05-11T00:53:14.584468Z digest=sha256:1fbedcd489ebd783125788dd04cb70b25ed2a1d33d9fbd4ee7d204fa6a763a31

Observation 7df6f61c-66f7-4cd7-ae67-3ed983af9a74 · inbound

The role of major mergers in triggering super-Eddington accretion cites this paper.

The role of major mergers in triggering super-Eddington accretion Extremely red galaxies at $z=5-9$ with MIRI and NIRSpec: dusty galaxies or obscured AGNs?

Reference 1

Resolution
metadata mismatch
arxiv_id, observed 2026-06-28T09:01:48.747691Z

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=2026-06-28T08:58:09.556687Z digest=sha256:03d19cbc8ebca0890079a7a73564e0e749a54fbd384f7ec678ea1bad98f1dcc5

Observation c31cdea9-90a0-43ae-939e-1e531a8cc16c · inbound

Little red dots as a cosmological probe: constraining $H_0$ with quasi-periodic pulsations cites this paper.

Little red dots as a cosmological probe: constraining $H_0$ with quasi-periodic pulsations Extremely red galaxies at $z=5-9$ with MIRI and NIRSpec: dusty galaxies or obscured AGNs?

Reference 5

Resolution
verified exact
arxiv_id, observed 2026-07-02T10:06:51.568125Z

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=2026-06-28T05:20:29.507384Z digest=sha256:5f2763e833a199da5cbc94015e18ab3ff6b5c6ca6e0f62abd0eed4d2b2267fd3

Observation 4d70044c-11f7-4283-90b0-2822614fa079 · inbound

Little Red Dots at z~2 in EIGER reveal a gentle decline with respect to their peak number density at z~5 cites this paper.

Little Red Dots at z~2 in EIGER reveal a gentle decline with respect to their peak number density at z~5 Extremely red galaxies at $z=5-9$ with MIRI and NIRSpec: dusty galaxies or obscured AGNs?

Reference 85

Resolution
metadata mismatch
arxiv_id, observed 2026-07-02T18:27:16.080001Z

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=2026-07-02T18:25:22.489682Z digest=sha256:3f42b84450ee9f343c58b4cd633f679e3d9e6440b5859f58592b7d58a6fa57ff

Observation 02cec2bc-b82c-46d8-a3de-85ddfe97f220 · inbound

Star-forming clump detection in nearby galaxies using Faster R-CNN and $ugrizy$ imaging data from CLAUDS and HSC-SSP cites this paper.

Star-forming clump detection in nearby galaxies using Faster R-CNN and $ugrizy$ imaging data from CLAUDS and HSC-SSP Extremely red galaxies at $z=5-9$ with MIRI and NIRSpec: dusty galaxies or obscured AGNs?

Reference 177

Resolution
unresolved
no resolver link, observed 2026-07-11T21:10:16.126324Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T21:10:16.126324Z digest=sha256:814ec78afff0287ca8b649432cea5881ca13c76e281a7c57bc3600067444bf6c

Observation 818c9f96-d6a3-41d1-a86d-83494846a0af · inbound

Star-forming clump detection in nearby galaxies using Faster R-CNN and $ugrizy$ imaging data from CLAUDS and HSC-SSP cites this paper.

Star-forming clump detection in nearby galaxies using Faster R-CNN and $ugrizy$ imaging data from CLAUDS and HSC-SSP Extremely red galaxies at $z=5-9$ with MIRI and NIRSpec: dusty galaxies or obscured AGNs?

Reference 177

Resolution
unresolved
no resolver link, observed 2026-08-02T08:46:56.683272Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T08:46:56.683272Z digest=sha256:d7d9e424377acda73860666f563fe39d592d3c8b864dbf8657b9ea4796eda910