Paper Citation Record · LEDGER

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

As of 14 August 2026, this Paper Citation Record lists 34 of 34 outbound references and 10 inbound Pith citation observations for arXiv:2505.18873.

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2505.18873 v1

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measured 34 of 34 reference resolution

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Source: paper_references, paper_reference_links, observed 2026-08-07T14:31:04.706464Z

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measured 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T16:36:20.954909Z

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

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

Outbound references

Observation cab316ce-84ca-4ce7-a6a8-e8dfc732d781 · outbound

This paper cites COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:00.396647Z

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Observation b5ebca32-2f2d-47e0-b220-f57db37125a7 · outbound

This paper cites Tentative detection of neutral gas in a Little Red Dot at $z=4.46$.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots Tentative detection of neutral gas in a Little Red Dot at $z=4.46$

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:00.488537Z

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Observation bfb687d4-7410-4711-b2de-a8b83beac04e · outbound

This paper cites The Small Sizes and High Implied Densities of `Little Red Dots' with Balmer Breaks Could Explain Their Broad Emission Lines Without an AGN.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots The Small Sizes and High Implied Densities of `Little Red Dots' with Balmer Breaks Could Explain Their Broad Emission Lines Without an AGN

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:00.577535Z

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Observation 74e69c9e-17b0-48a7-874c-5e112decfb5e · outbound

This paper cites 2025, arXiv e-prints, arXiv:2503.15323, doi: 10.48550/arXiv.2503.15323.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots 2025, arXiv e-prints, arXiv:2503.15323, doi: 10.48550/arXiv.2503.15323

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:00.720094Z

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Observation 197c8cd9-1db0-4cc6-bdb6-c668fd604721 · outbound

This paper cites M., Akins, H.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots M., Akins, H

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:00.827035Z

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Observation 31c31330-7a93-4983-9ef4-cde2754ee007 · outbound

This paper cites M., Zavala, J.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots M., Zavala, J

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:00.922736Z

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Observation ec4a989a-6df9-44ea-8be5-9b34785f133a · outbound

This paper cites M., Kartaltepe, J.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots M., Kartaltepe, J

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:01.012747Z

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Observation 24f5937e-95bc-4145-81ef-e4ae90556832 · outbound

This paper cites A remarkable Ruby: Absorption in dense gas, rather than evolved stars, drives the extreme Balmer break of a Little Red Dot at $z=3.5$.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots A remarkable Ruby: Absorption in dense gas, rather than evolved stars, drives the extreme Balmer break of a Little Red Dot at $z=3.5$

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:01.148934Z

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Observation 814a95a0-4ade-4fa2-b5ae-35f61479e347 · outbound

This paper cites UNCOVER spectroscopy confirms a surprising ubiquity of AGN in red galaxies at $z>5$.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots UNCOVER spectroscopy confirms a surprising ubiquity of AGN in red galaxies at $z>5$

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:01.273472Z

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Observation 5094d875-565c-4d07-a46b-b30b37422ad2 · outbound

This paper cites Extremely Dense Gas around Little Red Dots and High-redshift Active Galactic Nuclei: A Non-stellar Origin of the Balmer Break and Absorption Features.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots Extremely Dense Gas around Little Red Dots and High-redshift Active Galactic Nuclei: A Non-stellar Origin of the Balmer Break and Absorption Features

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:01.405183Z

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Observation 31932d66-03b2-452f-ba9d-e3a2b94b1d23 · outbound

This paper cites 2025, arXiv e-prints, arXiv:2501.13082, doi: 10.48550/arXiv.2501.13082.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots 2025, arXiv e-prints, arXiv:2501.13082, doi: 10.48550/arXiv.2501.13082

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:01.534660Z

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Observation 797f635f-8a6d-4228-bd54-81e33f1bd315 · outbound

This paper cites The Rise of Faint, Red AGN at $z>4$: A Sample of Little Red Dots in the JWST Extragalactic Legacy Fields.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots The Rise of Faint, Red AGN at $z>4$: A Sample of Little Red Dots in the JWST Extragalactic Legacy Fields

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:01.692355Z

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Observation 88e41822-4af8-4ed9-aea8-4ceafe28407c · outbound

This paper cites A Census of Photometrically Selected Little Red Dots at 4 < z < 9 in JWST Blank Fields.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots A Census of Photometrically Selected Little Red Dots at 4 < z < 9 in JWST Blank Fields

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:01.807995Z

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Observation 32383220-bff1-47eb-808e-37bf4aa1e8f6 · outbound

This paper cites A population of red candidate massive galaxies ~600 Myr after the Big Bang.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots A population of red candidate massive galaxies ~600 Myr after the Big Bang

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:01.912168Z

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Observation c54517ff-da4d-4696-9ee9-7152bdfc3fe0 · outbound

This paper cites UNCOVER: Candidate Red Active Galactic Nuclei at 3<z<7 with JWST and ALMA.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots UNCOVER: Candidate Red Active Galactic Nuclei at 3<z<7 with JWST and ALMA

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:02.024270Z

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Observation 3ccb5810-dd6b-443d-9b29-4781a562b900 · outbound

This paper cites S., et al.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots S., et al

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:02.195337Z

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Observation c9730866-3825-491e-aeef-15aec5b7ad89 · outbound

This paper cites 2001, ApJ, 554, 778, doi: 10.1086/323147.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots 2001, ApJ, 554, 778, doi: 10.1086/323147

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:02.344868Z

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Observation 32f552de-f0e4-4cc1-a51b-040b87770e9b · outbound

This paper cites Little Red Dots: Rapidly Growing Black Holes Reddened by Extended Dusty Flows.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots Little Red Dots: Rapidly Growing Black Holes Reddened by Extended Dusty Flows

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:02.451241Z

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Observation 1668b94f-a06d-4271-b839-e1d5f25908a1 · outbound

This paper cites 2025a, ApJL, 980, L34, doi: 10.3847/2041-8213/adaaf1.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots 2025a, ApJL, 980, L34, doi: 10.3847/2041-8213/adaaf1

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:02.627452Z

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Observation 8a2ae8d7-5731-4979-9163-22c86cd0f09e · outbound

This paper cites 2025b, arXiv e-prints, arXiv:2504.08039, doi: 10.48550/arXiv.2504.08039.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots 2025b, arXiv e-prints, arXiv:2504.08039, doi: 10.48550/arXiv.2504.08039

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:02.771209Z

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Observation 53811fbb-e67f-45af-bd43-00e2be9b6ba1 · outbound

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

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

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Observation f1309684-1438-4102-95a7-6dd92a55df07 · outbound

This paper cites 2025, arXiv e-prints, arXiv:2501.09854, doi: 10.48550/arXiv.2501.09854.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots 2025, arXiv e-prints, arXiv:2501.09854, doi: 10.48550/arXiv.2501.09854

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:03.072619Z

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Observation 1916ddd0-10a6-496d-af18-4bb7f002dcfe · outbound

This paper cites P., Brammer, G., et al.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots P., Brammer, G., et al

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:03.204916Z

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Observation 9590156a-84fd-4be2-8fb1-38ea34c3bc6a · outbound

This paper cites C., Rosenthal, L.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots C., Rosenthal, L

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:03.355485Z

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Observation 73219710-0b9b-4a93-b70f-5bcc17dd2ae7 · outbound

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

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots A "Black Hole Star" Reveals the Remarkable Gas-Enshrouded Hearts of the Little Red Dots

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:03.516049Z

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Observation 71ee3fa2-7e25-42f7-bb8d-185739e6b1ed · outbound

This paper cites B., & Gunn, J.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots B., & Gunn, J

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:03.692121Z

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Observation 75c7a8d2-e01d-4434-ae0a-e6b989e5a7fd · outbound

This paper cites 2025, arXiv e-prints, arXiv:2505.05556, doi: 10.48550/arXiv.2505.05556.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots 2025, arXiv e-prints, arXiv:2505.05556, doi: 10.48550/arXiv.2505.05556

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:03.838945Z

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Observation c2419bc9-22e2-4fd0-8209-715ecef4bba8 · outbound

This paper cites P., et al.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots P., et al

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:03.977943Z

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Observation 55f8bccd-98e4-42ca-a995-5e22ce26ee03 · outbound

This paper cites A confirmed deficit of hot and cold dust emission in the most luminous Little Red Dots.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots A confirmed deficit of hot and cold dust emission in the most luminous Little Red Dots

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:04.155899Z

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Observation 94a81be2-4dbc-4b3f-861c-9870db706ee4 · outbound

This paper cites Broad-Line AGN at 3.5<z<6: The Black Hole Mass Function and a Connection with Little Red Dots.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots Broad-Line AGN at 3.5<z<6: The Black Hole Mass Function and a Connection with Little Red Dots

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:04.270737Z

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Observation e88c5e99-0354-49f0-9b5e-26c5eaaaccd2 · outbound

This paper cites CAPERS-LRD-z9: A Gas Enshrouded Little Red Dot Hosting a Broad-line AGN at z=9.288.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots CAPERS-LRD-z9: A Gas Enshrouded Little Red Dot Hosting a Broad-line AGN at z=9.288

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:04.414538Z

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Observation 464e3f67-ef3d-4f2d-9432-2187ac28481e · outbound

This paper cites RUBIES: JWST/NIRSpec Confirmation of an Infrared-luminous, Broad-line Little Red Dot with an Ionized Outflow.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots RUBIES: JWST/NIRSpec Confirmation of an Infrared-luminous, Broad-line Little Red Dot with an Ionized Outflow

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:04.492167Z

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Observation 379fe6dc-b995-4d34-b613-88c54de1cc59 · outbound

This paper cites The galaxies missed by Hubble and ALMA: the contribution of extremely red galaxies to the cosmic census at 3<z<8.

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots The galaxies missed by Hubble and ALMA: the contribution of extremely red galaxies to the cosmic census at 3<z<8

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:04.612690Z

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Observation f58cddc4-59c1-44c7-8552-596144a4b1b0 · outbound

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

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

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Pith citing papers

Observation cc38e9cb-1b57-45eb-b9d1-94cb19381f76 · inbound

Lonely Little Red Dots: Challenges to the AGN-nature of little red dots through their clustering and spectral energy distributions cites this paper.

Lonely Little Red Dots: Challenges to the AGN-nature of little red dots through their clustering and spectral energy distributions An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-07T10:56:02.543597Z

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Observation af7273d4-9dda-4ea5-a9eb-b3ac4218ef3a · 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 An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-06T21:45:14.279219Z

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Observation 9c41bb75-740d-4707-8c04-4c29cf51d0a7 · inbound

MEGA: Spectrophotometric SED Fitting of Little Red Dots Detected in JWST MIRI cites this paper.

MEGA: Spectrophotometric SED Fitting of Little Red Dots Detected in JWST MIRI An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-05T15:21:40.779679Z

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Observation 93fbc81d-ce24-4cc2-b6a6-7c9eac7b8813 · 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? An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-05T14:08:54.031165Z

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Observation b0558b33-bdac-4cf9-ba66-c548e1e08cf8 · 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 An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:29.871885Z

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Observation 9203a622-0cbe-426f-bd73-e19207021d60 · 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 An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots

Reference 13

Resolution: verified exact; arxiv_id, observed 2026-05-18T14:41:29.781749Z

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Observation 0a0f22fc-71b4-4a91-9b78-1213df1110db · 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 An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots

Reference 17

Resolution: verified exact; arxiv_id, observed 2026-05-08T19:59:08.677776Z

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 ac3feaa0-c0c4-4667-bf71-af4402008821 · 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 An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots

Reference 27

Resolution: verified exact; arxiv_id, observed 2026-05-22T09:46:21.917668Z

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 e94fd796-8658-4f1c-b078-22e77d309828 · inbound

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs cites this paper.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:25.223604Z

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Observation 675b593a-dfbb-45cc-9c6d-7e5faadfbfb7 · 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 $z < 0.35$ An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots

Reference 152

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.954909Z

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