Paper Citation Record · LEDGER

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

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 13 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 13 of 13 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 13 of 13 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T04:19:00.607583Z

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

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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 2142d191-4165-44f9-811b-92fac5d3a7e7 · 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 Extremely red galaxies at $z=5-9$ with MIRI and NIRSpec: dusty galaxies or obscured AGNs?

Reference 128

Resolution: unresolved; no resolver link, observed 2026-08-11T23:20:51.951904Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 70d3f6aa-fb95-4c73-bf58-bfd76eae460e · inbound

Red, hot, and very metal poor: extreme properties of a massive accreting black hole in the first 500 Myr cites this paper.

Red, hot, and very metal poor: extreme properties of a massive accreting black hole in the first 500 Myr Extremely red galaxies at $z=5-9$ with MIRI and NIRSpec: dusty galaxies or obscured AGNs?

Reference 160

Resolution: unresolved; no resolver link, observed 2026-08-11T21:08:52.461993Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 851fa07f-9897-4750-8383-dfc728da3b82 · inbound

Episodic super-Eddington accretion as a clue to Overmassive Black Holes in the early Universe cites this paper.

Episodic super-Eddington accretion as a clue to Overmassive Black Holes in the early Universe Extremely red galaxies at $z=5-9$ with MIRI and NIRSpec: dusty galaxies or obscured AGNs?

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-11T12:29:56.581815Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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.

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 2026-08-14T06:32:32.682623+00:00.

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 2026-08-14T06:32:32.682623+00:00.

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 2026-08-14T06:32:32.682623+00:00.

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 2026-08-14T06:32:32.682623+00:00.

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 2026-08-14T06:32:32.682623+00:00.

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.

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.

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.

Observation 424e0438-c4ad-455a-a746-ae7bf564ae83 · 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 $z < 0.35$ Extremely red galaxies at $z=5-9$ with MIRI and NIRSpec: dusty galaxies or obscured AGNs?

Reference 101

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.649011Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7b5111dc-2661-4f5e-9706-a7dc5f9398c0 · inbound

A cosmic collision in the making: JWST/NIRISS reveals a merging and maturing protocluster core at z~3 around a red quasar cites this paper.

A cosmic collision in the making: JWST/NIRISS reveals a merging and maturing protocluster core at z~3 around a red quasar Extremely red galaxies at $z=5-9$ with MIRI and NIRSpec: dusty galaxies or obscured AGNs?

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-14T04:19:00.607583Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.