Paper Citation Record · LEDGER

Counting Little Red Dots at $z<4$ with Ground-based Surveys and Spectroscopic Follow-up

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 22 inbound Pith citation observations for arXiv:2504.08032.

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

pith.paper-citation-record.v1
2504.08032 v1

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measured 0 of 0 reference resolution

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measured 22 of 22 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 22 of 22 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T16:36:20.787343Z

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

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External citation measurements

2
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 53811fbb-e67f-45af-bd43-00e2be9b6ba1 · inbound

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots cites this paper.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots Counting Little Red Dots at $z<4$ with Ground-based Surveys and Spectroscopic Follow-up

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:02.911582Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2962330b-29cd-4554-ab61-b6b3c75fb147 · inbound

NEXUS: A Spectroscopic Census of Broad-line AGNs and Little Red Dots at $3\lesssim z\lesssim 6$ cites this paper.

NEXUS: A Spectroscopic Census of Broad-line AGNs and Little Red Dots at $3\lesssim z\lesssim 6$ Counting Little Red Dots at $z<4$ with Ground-based Surveys and Spectroscopic Follow-up

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-07T14:03:30.126796Z

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Unavailable: canonical work link unavailable.

Observation 60f40ae2-67db-463f-b66d-cbae373bf9c1 · inbound

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots cites this paper.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots Counting Little Red Dots at $z<4$ with Ground-based Surveys and Spectroscopic Follow-up

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:02.913411Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation eaea0f4e-af3f-454d-9e04-4f95f46df7a9 · inbound

JWST IFU observations uncover host galaxy continua in extremely red and obscured quasars cites this paper.

JWST IFU observations uncover host galaxy continua in extremely red and obscured quasars Counting Little Red Dots at $z<4$ with Ground-based Surveys and Spectroscopic Follow-up

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-07T01:05:07.815735Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d75c6670-692c-40a7-a8e1-5f42b3ffde60 · inbound

Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XXIV. 54 New Quasars and Candidate Obscured Quasars at $5.71 \le z \le 7.02$ cites this paper.

Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XXIV. 54 New Quasars and Candidate Obscured Quasars at $5.71 \le z \le 7.02$ Counting Little Red Dots at $z<4$ with Ground-based Surveys and Spectroscopic Follow-up

Reference 116

Resolution: unresolved; no resolver link, observed 2026-08-05T14:33:57.331308Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b4038b8e-459a-4ee9-a42e-f96c2bc4a3e0 · inbound

How similar are narrow-line Seyfert 1 galaxies and high-z type 1 AGN? cites this paper.

Reference 167

Resolution: unresolved; no resolver link, observed 2026-08-05T10:54:34.976558Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 245603b8-432a-4d8a-9ba7-acb5eb7221bc · inbound

Characterizing the roles of transitory obscured phases and inner torus in shaping the fractions of obscured AGN at cosmic noon cites this paper.

Characterizing the roles of transitory obscured phases and inner torus in shaping the fractions of obscured AGN at cosmic noon Counting Little Red Dots at $z<4$ with Ground-based Surveys and Spectroscopic Follow-up

Reference 106

Resolution: unresolved; no resolver link, observed 2026-08-05T06:04:42.724846Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 994dafe2-0c7f-4a45-a0a0-4d3253bade88 · inbound

Spectral Uniformity of Little Red Dots: A Natural Outcome of Coevolving Seed Black Holes and Nascent Starbursts cites this paper.

Spectral Uniformity of Little Red Dots: A Natural Outcome of Coevolving Seed Black Holes and Nascent Starbursts Counting Little Red Dots at $z<4$ with Ground-based Surveys and Spectroscopic Follow-up

Reference 91

Resolution: verified exact; arxiv_id, observed 2026-05-18T14:41:29.387767Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation fed3dd3b-19b7-43cc-9787-1e208b1771d2 · inbound

Connecting the Dots: UV-Bright Companions of Little Red Dots as Lyman-Werner Sources Enabling Direct Collapse Black Hole Formation cites this paper.

Connecting the Dots: UV-Bright Companions of Little Red Dots as Lyman-Werner Sources Enabling Direct Collapse Black Hole Formation Counting Little Red Dots at $z<4$ with Ground-based Surveys and Spectroscopic Follow-up

Reference 72

Resolution: verified exact; arxiv_id, observed 2026-05-16T08:00:44.427740Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 9e7e42cc-7707-4e3f-9fb8-511b9bdef50d · inbound

Local Analogs of Little Red Dots: Optical Variability and Evidence for an Active Galatic Nucleus Origin cites this paper.

Local Analogs of Little Red Dots: Optical Variability and Evidence for an Active Galatic Nucleus Origin Counting Little Red Dots at $z<4$ with Ground-based Surveys and Spectroscopic Follow-up

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-02T19:41:38.383544Z

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Unavailable: canonical work link unavailable.

Observation 633506df-17f0-4878-b120-f763773f1300 · inbound

Blackbody Quasar and Radio Source (BBQSORS): A Candidate of Transitional Little Red Dots with a $T\sim10^4\ K$ Blackbody Spectrum cites this paper.

Blackbody Quasar and Radio Source (BBQSORS): A Candidate of Transitional Little Red Dots with a $T\sim10^4\ K$ Blackbody Spectrum Counting Little Red Dots at $z<4$ with Ground-based Surveys and Spectroscopic Follow-up

Reference 41

Resolution: verified exact; arxiv_id, observed 2026-05-15T12:19:59.867465Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 98568b9b-68cf-4b7d-88d7-5f12f79edc8e · inbound

Compact, AGN-hosting Dwarf Galaxies with "Little Red Dots"-like SEDs in the Local Universe cites this paper.

Compact, AGN-hosting Dwarf Galaxies with "Little Red Dots"-like SEDs in the Local Universe Counting Little Red Dots at $z<4$ with Ground-based Surveys and Spectroscopic Follow-up

Reference 58

Resolution: verified exact; arxiv_id, observed 2026-05-08T19:59:08.277903Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 391a54b0-1479-428d-9693-616f7c344cd5 · inbound

A new sample of Little Red Dots at $z<0.45$ in DESI DR1: Broad Balmer lines, low ionization spectrum and no variability cites this paper.

A new sample of Little Red Dots at $z<0.45$ in DESI DR1: Broad Balmer lines, low ionization spectrum and no variability Counting Little Red Dots at $z<4$ with Ground-based Surveys and Spectroscopic Follow-up

Reference 50

Resolution: verified exact; arxiv_id, observed 2026-05-15T02:48:33.341937Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 83f90e15-e0f8-4a29-9170-5baa9b355b24 · inbound

(LRDs)$^2$: The Low-ReDshift Little Red Dots Survey. II. DESI DR1 Sample cites this paper.

(LRDs)$^2$: The Low-ReDshift Little Red Dots Survey. II. DESI DR1 Sample Counting Little Red Dots at $z<4$ with Ground-based Surveys and Spectroscopic Follow-up

Reference 85

Resolution: verified exact; arxiv_id, observed 2026-05-22T09:46:22.183115Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation ccbfc099-0d9c-4dde-a1e0-3e48ce4cf8b0 · inbound

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution cites this paper.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Counting Little Red Dots at $z<4$ with Ground-based Surveys and Spectroscopic Follow-up

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:28.201015Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 51cfe250-4694-4dcc-8e4e-b76488d2068d · inbound

NEXUS: Abundance, Environments, and Spectral Diversity of Little Red Dots from the NIRSpec MSA Sample cites this paper.

NEXUS: Abundance, Environments, and Spectral Diversity of Little Red Dots from the NIRSpec MSA Sample Counting Little Red Dots at $z<4$ with Ground-based Surveys and Spectroscopic Follow-up

Reference 48

Resolution: verified exact; arxiv_id, observed 2026-06-27T16:21:01.453257Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 017421ed-32ba-4a0e-aa44-39d2b5aad123 · inbound

No evolution in the number density of little red dots from cosmic dawn to cosmic noon cites this paper.

No evolution in the number density of little red dots from cosmic dawn to cosmic noon Counting Little Red Dots at $z<4$ with Ground-based Surveys and Spectroscopic Follow-up

Reference 44

Resolution: verified exact; arxiv_id, observed 2026-06-30T04:54:16.184954Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation f73c3b46-e94e-4a69-84b4-26e181f6bf17 · inbound

Little Red Dots as Intermediate Mass, Super-Eddington Engines: Insights from Type IIn Supernovae and The 1837-1856 Great Eruption of $\eta$ Carinae cites this paper.

Little Red Dots as Intermediate Mass, Super-Eddington Engines: Insights from Type IIn Supernovae and The 1837-1856 Great Eruption of $\eta$ Carinae Counting Little Red Dots at $z<4$ with Ground-based Surveys and Spectroscopic Follow-up

Reference 125

Resolution: verified exact; arxiv_id, observed 2026-07-01T12:15:43.902494Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 767ad224-d5dd-4e1b-98df-8bc963f75381 · 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 Counting Little Red Dots at $z<4$ with Ground-based Surveys and Spectroscopic Follow-up

Reference 32

Resolution: metadata mismatch; arxiv_id, observed 2026-07-02T18:27:16.557368Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 77469a5d-e69e-47ff-b170-442257247b69 · inbound

BlackTHUNDER Reveals a Massive Filament around a Compact AGN at $z\simeq5.23$ cites this paper.

BlackTHUNDER Reveals a Massive Filament around a Compact AGN at $z\simeq5.23$ Counting Little Red Dots at $z<4$ with Ground-based Surveys and Spectroscopic Follow-up

Reference 22

Resolution: unresolved; no resolver link, observed 2026-07-11T06:23:06.110361Z

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Unavailable: canonical work link unavailable.

Observation 1601824b-f74c-4f39-b863-12432b94457f · inbound

Outflows in super-Eddington quasars drive clumpy circumgalactic medium and extended H$\alpha$ nebulae at $z \gtrsim 6$ cites this paper.

Outflows in super-Eddington quasars drive clumpy circumgalactic medium and extended H$\alpha$ nebulae at $z \gtrsim 6$ Counting Little Red Dots at $z<4$ with Ground-based Surveys and Spectroscopic Follow-up

Reference 293

Resolution: unresolved; no resolver link, observed 2026-08-01T06:59:01.989819Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f258e818-7ae1-44d6-8c4e-9a749fd2689c · 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 $z < 0.35$ Counting Little Red Dots at $z<4$ with Ground-based Surveys and Spectroscopic Follow-up

Reference 122

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.787343Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.