Paper Citation Record · LEDGER

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

As of 17 August 2026, this Paper Citation Record lists 58 of 58 outbound references and 5 inbound Pith citation observations for arXiv:2506.03244.

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

pith.paper-citation-record.v1
2506.03244 v2

Coverage vector

measured 58 of 58 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-07T11:16:06.163660Z

measured 63 of 63 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T18:38:08.003854Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: arxiv_reference, observed 2026-05-16T13:42:56.275990Z

Reference resolution

58 of 58 outbound references displayed

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External citation measurements

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Outbound references

Observation f44b6cb5-f328-4bed-85e4-568c0a1ffce9 · outbound

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

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the 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 2026-08-07T11:15:59.607138Z

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Observation deb3161b-1181-4162-8a10-3cc301fd18b3 · outbound

This paper cites T., Bogd´ an,´A., Kov´ acs, O.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots T., Bogd´ an,´A., Kov´ acs, O

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-07T11:15:59.659533Z

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Observation 25daeebf-a0b0-4fbf-9686-7e697fa11fa9 · outbound

This paper cites 2008, ApJ, 682, 1195, doi: 10.1086/589278.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots 2008, ApJ, 682, 1195, doi: 10.1086/589278

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-07T11:15:59.749733Z

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Observation f1a0cc58-34c0-46b7-9022-bd3d7f4541db · outbound

This paper cites an unresolved cited work.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots Unresolved cited work

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-07T11:15:59.812145Z

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Observation 46f48de1-1b67-4854-a240-a2e528a3f2c2 · outbound

This paper cites an unresolved cited work.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots Unresolved cited work

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-07T11:15:59.898396Z

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Observation 33baf6fa-86b6-44e0-bdd9-b9535bfd11a5 · outbound

This paper cites 2001, PhR, 349, 125, doi: 10.1016/S0370-1573(01)00019-9.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots 2001, PhR, 349, 125, doi: 10.1016/S0370-1573(01)00019-9

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-07T11:15:59.964521Z

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Observation 9e6c6003-2f73-4c01-b01d-2a5726674b18 · outbound

This paper cites S., Wechsler, R.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots S., Wechsler, R

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:00.060056Z

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Observation de707ca2-8d3d-4b85-9c29-548ed8834f53 · outbound

This paper cites 2022, MNRAS, 512, 3703, doi: 10.1093/mnras/stac648.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots 2022, MNRAS, 512, 3703, doi: 10.1093/mnras/stac648

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:00.110169Z

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Observation 8149b1cb-7eaa-4817-a2c4-90498a066eb6 · outbound

This paper cites J., Oesch, P.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots J., Oesch, P

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:00.179686Z

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Observation 6581b00d-991c-4df6-9925-a16bd48d750f · outbound

This paper cites 2024, Nature, 633, 318, doi: 10.1038/s41586-024-07860-9.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots 2024, Nature, 633, 318, doi: 10.1038/s41586-024-07860-9

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:00.301749Z

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Observation d21a4262-ab1a-412f-b2af-5e63f5169fe5 · outbound

This paper cites 1996, MNRAS, 281, 716, doi: 10.1093/mnras/281.2.716.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots 1996, MNRAS, 281, 716, doi: 10.1093/mnras/281.2.716

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:00.376343Z

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Observation 06e4e226-ad14-4a58-bcd6-de8a7c254121 · outbound

This paper cites an unresolved cited work.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots Unresolved cited work

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:00.432879Z

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Observation 6e444acd-2b34-4185-bf08-bc96dc01a1e3 · outbound

This paper cites 2007, ApJ, 654, 27, doi: 10.1086/509314 11.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots 2007, ApJ, 654, 27, doi: 10.1086/509314 11

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:00.497769Z

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Observation 49080460-7437-4f25-91f0-88cca123d422 · outbound

This paper cites J., & Loeb, A.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots J., & Loeb, A

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:00.634724Z

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Observation 1b90a075-1e83-4041-9bad-77e33c311211 · outbound

This paper cites G., & Struck, C.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots G., & Struck, C

Reference 15

Resolution: verified exact; doi, observed 2026-08-07T11:16:06.756662Z

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Observation bfe193f3-95dc-4145-a891-42b4fbcd6ce7 · outbound

This paper cites L., Bagley, M.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots L., Bagley, M

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:00.860903Z

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Observation 5f8fac07-05a9-435a-aedf-cd41c3c9a802 · outbound

This paper cites S., Wang, L., Tanikawa, A., Hirai, Y., & Saitoh, T.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots S., Wang, L., Tanikawa, A., Hirai, Y., & Saitoh, T

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:00.969858Z

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Observation 28f3d162-c093-471a-9cf6-5c3d27b6be0c · outbound

This paper cites J., Zitrin, A., Plat, A., et al.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots J., Zitrin, A., Plat, A., et al

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:01.075247Z

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Observation d38c41be-3482-4435-80b1-8cd59297fa11 · outbound

This paper cites E., Labbe, I., Goulding, A.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots E., Labbe, I., Goulding, A

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:01.231101Z

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Observation dd6cbc4e-ee20-4a74-8d17-59a161703d99 · outbound

This paper cites A., Pacucci, F., & Kocevski, D.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots A., Pacucci, F., & Kocevski, D

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:01.320095Z

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Observation 8f50d5b8-776f-4729-8112-0eef2d1760f8 · outbound

This paper cites 2023, ApJ, 959, 39, doi: 10.3847/1538-4357/ad029e.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots 2023, ApJ, 959, 39, doi: 10.3847/1538-4357/ad029e

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:01.577481Z

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Observation 6101ff09-cf6c-44eb-ba1f-14d0dca268b4 · outbound

This paper cites 1958, Physics and Philosophy: The Revolution in Modern Science (New York: Harper & Row).

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots 1958, Physics and Philosophy: The Revolution in Modern Science (New York: Harper & Row)

Reference 22

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T11:16:07.117865Z

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Observation 424cefda-ccc0-4d1f-9beb-afa2f4c867e7 · outbound

This paper cites F., Murray, N., Quataert, E., & Thompson, T.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots F., Murray, N., Quataert, E., & Thompson, T

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:01.847000Z

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Observation 635d889c-5976-4cca-afd3-9b85f1291539 · outbound

This paper cites 2024, ApJL, 973, L49, doi: 10.3847/2041-8213/ad74e2.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots 2024, ApJL, 973, L49, doi: 10.3847/2041-8213/ad74e2

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:02.003934Z

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Observation d98b3be9-e41c-42f4-8884-98aa9f1eb73c · outbound

This paper cites 2025, ApJL, 980, L27, doi: 10.3847/2041-8213/adaebd.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots 2025, ApJL, 980, L27, doi: 10.3847/2041-8213/adaebd

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:02.128549Z

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Observation 1f95f1d4-1d35-488f-93d0-12ba7aada420 · outbound

This paper cites D., Onoue, M., Inayoshi, K., et al.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots D., Onoue, M., Inayoshi, K., et al

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:02.256835Z

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Observation d699c65d-465d-476e-ac34-17eda821b639 · outbound

This paper cites D., Finkelstein, S.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots D., Finkelstein, S

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:02.383758Z

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Observation fc7164fb-ee86-48b8-bdc0-8faf35d33814 · outbound

This paper cites 2023, ApJL, 957, L7, doi: 10.3847/2041-8213/ad037a.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots 2023, ApJL, 957, L7, doi: 10.3847/2041-8213/ad037a

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:02.478620Z

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Observation 092c1a24-ee14-43cf-9b0c-03fbd57fbd0c · outbound

This paper cites I., Greene, J.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots I., Greene, J

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:02.556024Z

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Observation 0071fca6-250a-409d-bebb-1e0b49a04322 · outbound

This paper cites an unresolved cited work.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots Unresolved cited work

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:02.643724Z

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Observation 58d65428-7406-44f8-af1b-ec337e8818f0 · outbound

This paper cites The case for super-Eddington accretion in JWST broad-line AGN during the first billion years.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots The case for super-Eddington accretion in JWST broad-line AGN during the first billion years

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:02.733756Z

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Observation cb33e75e-2778-4461-885d-c0b41a62fdb3 · outbound

This paper cites 2024, Research Notes of the American Astronomical Society, 8, 182, doi: 10.3847/2515-5172/ad614c.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots 2024, Research Notes of the American Astronomical Society, 8, 182, doi: 10.3847/2515-5172/ad614c

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:02.824294Z

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

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

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

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Observation 025286a3-46e9-478e-b305-4ad1b0776661 · outbound

This paper cites 2024, ApJL, 976, L24, doi: 10.3847/2041-8213/ad90e1.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots 2024, ApJL, 976, L24, doi: 10.3847/2041-8213/ad90e1

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:03.060021Z

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Observation a880fbc8-608f-48f4-9079-cbcb11e7803f · outbound

This paper cites 2024, A&A, 691, A145, doi: 10.1051/0004-6361/202347640.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots 2024, A&A, 691, A145, doi: 10.1051/0004-6361/202347640

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:03.219034Z

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Observation f47a3fa2-7e70-4782-8fcc-26988130adea · outbound

This paper cites 2025, MNRAS, 538, 1921, doi: 10.1093/mnras/staf359.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots 2025, MNRAS, 538, 1921, doi: 10.1093/mnras/staf359

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:03.348350Z

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Observation 9168a5cf-30e5-4c23-ba8e-1e8b671e6969 · outbound

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

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots P., Brammer, G., et al

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:03.497175Z

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Observation 2b069b2a-cb21-4ec3-a026-ecf3b3a8cd97 · outbound

This paper cites J., Mao, S., & White, S.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots J., Mao, S., & White, S

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:03.623481Z

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Observation 2d04b44b-bab4-4ccf-beb6-bb14f5bf4abc · outbound

This paper cites P., Naab, T., & White, S.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots P., Naab, T., & White, S

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:03.783370Z

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Observation 555c8dd9-8434-4309-9e1e-53b0baf9ec81 · outbound

This paper cites F., Frenk, C.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots F., Frenk, C

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:03.976016Z

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Observation b4bebb86-2bb9-472b-9180-c7c7735a51d1 · outbound

This paper cites 2022, MNRAS, 513, 670, doi: 10.1093/mnras/stac351.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots 2022, MNRAS, 513, 670, doi: 10.1093/mnras/stac351

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:04.129185Z

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Observation c81e8760-5b5d-4692-aa0a-2ad6e9cf9f71 · outbound

This paper cites 2020, ApJ, 904, 89, doi: 10.3847/1538-4357/abbe11.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots 2020, ApJ, 904, 89, doi: 10.3847/1538-4357/abbe11

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:04.259608Z

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Observation e20f5db1-1054-4316-bee1-5ea15c82cecf · outbound

This paper cites 2024, ApJ, 964, 154, doi: 10.3847/1538-4357/ad3044.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots 2024, ApJ, 964, 154, doi: 10.3847/1538-4357/ad3044

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:04.379855Z

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Observation 7de4b16a-cc90-4a01-867c-bff3dfdc9c22 · outbound

This paper cites 2024, ApJ, 976, 96, doi: 10.3847/1538-4357/ad84f7.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots 2024, ApJ, 976, 96, doi: 10.3847/1538-4357/ad84f7

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:04.535211Z

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Observation 1b1e76b4-e569-49b1-80f9-bb75f3d2ce95 · outbound

This paper cites 2023, ApJL, 957, L3, doi: 10.3847/2041-8213/ad0158 Planck Collaboration, Aghanim, N., Akrami, Y., et al.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots 2023, ApJL, 957, L3, doi: 10.3847/2041-8213/ad0158 Planck Collaboration, Aghanim, N., Akrami, Y., et al

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:04.727158Z

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Observation 26845f0a-63b3-4d33-bf56-ceda94d28757 · outbound

This paper cites J., Kelly, D.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots J., Kelly, D

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:04.851143Z

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Observation c75c32ee-58c9-4168-8f89-2ec2c9c4dd80 · outbound

This paper cites B., Agertz, O., & Renaud, F.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots B., Agertz, O., & Renaud, F

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:04.992739Z

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Observation 46416ba9-7dc2-4924-9ea7-b04113479b6f · outbound

This paper cites B., Agertz, O., & Renaud, F.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots B., Agertz, O., & Renaud, F

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:05.136183Z

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Observation a865b05e-ddaa-4e61-9ecc-d65ae0dafd2d · outbound

This paper cites Little Red Dots at an Inflection Point: Ubiquitous "V-Shaped" Turnover Consistently Occurs at the Balmer Limit.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots Little Red Dots at an Inflection Point: Ubiquitous "V-Shaped" Turnover Consistently Occurs at the Balmer Limit

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:05.243962Z

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Observation a24f6ebd-f670-4f09-85ca-887c367ed80e · outbound

This paper cites 1995, MNRAS, 272, 570, doi: 10.1093/mnras/272.3.570.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots 1995, MNRAS, 272, 570, doi: 10.1093/mnras/272.3.570

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:05.347906Z

Source-reported events for the cited work

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Observation 122d2bf7-c159-46ba-ba8d-991f893f61b4 · outbound

This paper cites M., et al.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots M., et al

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:05.535474Z

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Observation 370a246d-8962-48b4-b960-02d3bef2635d · outbound

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

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots Broad-Line AGN at 3.5<z<6: The Black Hole Mass Function and a Connection with Little Red Dots

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:05.653950Z

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Observation 9c1b36ec-e4f7-4cff-9978-ceec66eeb221 · outbound

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

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots CAPERS-LRD-z9: A Gas Enshrouded Little Red Dot Hosting a Broad-line AGN at z=9.288

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:05.738484Z

Source-reported events for the cited work

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Observation 4b3e6544-91b1-44cc-8e42-c4948bcacf65 · outbound

This paper cites C., Askar, A., Kamlah, A.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots C., Askar, A., Kamlah, A

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:05.822927Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 34c0972b-5065-49f6-a454-4800ef4255fa · outbound

This paper cites S., Quinn, P.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots S., Quinn, P

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:05.916829Z

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Unavailable: canonical work link unavailable.

Observation bb57a08f-e006-413c-a1cc-64e17cea65c7 · outbound

This paper cites T., et al.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots T., et al

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:06.006934Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e172b3d9-2740-441a-ab55-ea806de13e28 · outbound

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

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots NEXUS: A Spectroscopic Census of Broad-line AGNs and Little Red Dots at $3\lesssim z\lesssim 6$

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:06.087797Z

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Observation ef7b7c3d-9c46-43cf-a858-55de789a3fef · outbound

This paper cites 2015, MNRAS, 450, 2327, doi: 10.1093/mnras/stv740.

Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots 2015, MNRAS, 450, 2327, doi: 10.1093/mnras/stv740

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:06.163660Z

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Pith citing papers

Observation 509f7925-8d4a-47da-a536-cdb52ed34f78 · inbound

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots cites this paper.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:08.003854Z

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Observation e4969bc1-d591-4d28-9e34-e78eaee78446 · inbound

Little Red Dots as Hidden Neutrino Sources cites this paper.

Little Red Dots as Hidden Neutrino Sources Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots

Reference 96

Resolution: verified exact; arxiv_id, observed 2026-05-16T13:42:56.277765Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation b726bf6f-1c41-4ee9-accb-5a9ac21e1e78 · inbound

The Way We Tally Becomes the Tale: the Impact of Selection Strategies on the Inferred Evolution of Little Red Dots Across Cosmic Time cites this paper.

The Way We Tally Becomes the Tale: the Impact of Selection Strategies on the Inferred Evolution of Little Red Dots Across Cosmic Time Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots

Reference 5

Resolution: metadata mismatch; arxiv_id, observed 2026-05-11T00:00:55.356393Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 63adb6e9-9463-4539-a1df-6438cabab260 · 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 Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:30.703845Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bc207340-f1ab-4d90-941f-3ee191061333 · 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 $z < 0.35$ Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.194849Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.