Paper Citation Record · LEDGER

No [CII] or dust detection in two Little Red Dots at z$_{\rm spec}$ > 7

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 12 inbound Pith citation observations for arXiv:2503.01945.

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

pith.paper-citation-record.v1
2503.01945 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 12 of 12 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 12 of 12 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T16:36:20.582722Z

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

1
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 b94c77f4-3870-4e37-952b-5753324f87a7 · inbound

A "Black Hole Star" Reveals the Remarkable Gas-Enshrouded Hearts of the Little Red Dots cites this paper.

A "Black Hole Star" Reveals the Remarkable Gas-Enshrouded Hearts of the Little Red Dots No [CII] or dust detection in two Little Red Dots at z$_{\rm spec}$ > 7

Reference 60

Resolution: verified exact; arxiv_id, observed 2026-05-16T08:53:14.816468Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation f58cddc4-59c1-44c7-8552-596144a4b1b0 · 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 No [CII] or dust detection in two Little Red Dots at z$_{\rm spec}$ > 7

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:04.706464Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation eb897892-9e5f-4584-94e0-fa813f1ac49f · inbound

Beneath the Surface: >85% of z>5.9 QSOs in Massive Host Galaxies are UV-Faint cites this paper.

Beneath the Surface: >85% of z>5.9 QSOs in Massive Host Galaxies are UV-Faint No [CII] or dust detection in two Little Red Dots at z$_{\rm spec}$ > 7

Reference 109

Resolution: unresolved; no resolver link, observed 2026-08-06T21:45:25.899300Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 90e1302c-b3c3-4ba6-bf9b-f5372546eec3 · inbound

Little Red reionization factories cites this paper.

Little Red reionization factories No [CII] or dust detection in two Little Red Dots at z$_{\rm spec}$ > 7

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-05T19:03:20.333201Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3625c1a4-2f77-4572-9562-5aa93a25b18a · inbound

Investigating Little Red Dots with UV Excess: Are They the High-Redshift Siblings of Blue Hot DOGs? cites this paper.

Investigating Little Red Dots with UV Excess: Are They the High-Redshift Siblings of Blue Hot DOGs? No [CII] or dust detection in two Little Red Dots at z$_{\rm spec}$ > 7

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-05T14:09:01.511428Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2474a039-777c-4d92-b18a-76373d9edd0d · inbound

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots cites this paper.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots No [CII] or dust detection in two Little Red Dots at z$_{\rm spec}$ > 7

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:30.269648Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4ac6b1f2-96b6-45d5-a504-35347fa6712d · inbound

Little Red Dots as Hidden Neutrino Sources cites this paper.

Little Red Dots as Hidden Neutrino Sources No [CII] or dust detection in two Little Red Dots at z$_{\rm spec}$ > 7

Reference 99

Resolution: verified exact; arxiv_id, observed 2026-05-16T13:42:56.268674Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 6088f6e1-1882-47d2-bdcf-2e100e243a9e · 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 No [CII] or dust detection in two Little Red Dots at z$_{\rm spec}$ > 7

Reference 89

Resolution: verified exact; arxiv_id, observed 2026-05-08T19:59:08.638862Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 4f7e88c8-8bde-415c-8ddd-46b37dcb2770 · 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 No [CII] or dust detection in two Little Red Dots at z$_{\rm spec}$ > 7

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:26.666046Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 16ca1bcf-18a6-49bc-b04d-967bb5a1f4f1 · inbound

Learning the Universe at High Redshifts: Impact of Accretion Modeling on Early Black Hole Growth cites this paper.

Learning the Universe at High Redshifts: Impact of Accretion Modeling on Early Black Hole Growth No [CII] or dust detection in two Little Red Dots at z$_{\rm spec}$ > 7

Reference 99

Resolution: verified exact; arxiv_id, observed 2026-06-27T17:21:07.125384Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 710d4f7f-db7f-450e-a307-5bd5f4fa79a5 · inbound

Dust in the Average Galaxy: Attenuation, Emission, and Opacity from 0<z<7 cites this paper.

Dust in the Average Galaxy: Attenuation, Emission, and Opacity from 0<z<7 No [CII] or dust detection in two Little Red Dots at z$_{\rm spec}$ > 7

Reference 168

Resolution: verified exact; arxiv_id, observed 2026-06-27T02:30:23.021785Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation cf63eff9-be07-4697-abb6-2e171c4aad37 · 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 $z < 0.35$ No [CII] or dust detection in two Little Red Dots at z$_{\rm spec}$ > 7

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.582722Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.