Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
No [CII] or dust detection in two Little Red Dots at z$_{\rm spec}$ > 7
As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 13 inbound Pith citation observations for arXiv:2503.01945.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T16:42:07.856844Z
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 2026-08-22T06:32:14.747728+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 93bad0b3-d32e-4083-a4b3-3234c1530f68 · inbound
No Luminous Little Red Dots: A Sharp Cutoff in Their Luminosity Function cites this paper.
No Luminous Little Red Dots: A Sharp Cutoff in Their Luminosity Function No [CII] or dust detection in two Little Red Dots at z$_{\rm spec}$ > 7
Reference 78
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T16:42:07.856844Z
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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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.