Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution | Paper Citation Record

Observation 8215789e-84d6-411b-bc50-c808428e295c · outbound

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

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution A population of red candidate massive galaxies ~600 Myr after the Big Bang

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:25.379687Z

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Observation 1179cd19-9ea4-4551-bf09-8a6596964a9f · outbound

This paper cites A JWST/NIRSpec First Census of Broad-Line AGNs at z=4-7: Detection of 10 Faint AGNs with M_BH~10^6-10^8 M_sun and Their Host Galaxy Properties.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution A JWST/NIRSpec First Census of Broad-Line AGNs at z=4-7: Detection of 10 Faint AGNs with M_BH~10^6-10^8 M_sun and Their Host Galaxy Properties

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:25.423206Z

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Observation 40c24e1b-dbc7-4e4e-9c04-b9d032267f20 · outbound

This paper cites A high black hole to host mass ratio in a lensed AGN in the early Universe.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution A high black hole to host mass ratio in a lensed AGN in the early Universe

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:25.507284Z

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Observation 09287fcb-3e57-4eba-aabe-41c46fcec631 · outbound

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

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution UNCOVER spectroscopy confirms a surprising ubiquity of AGN in red galaxies at $z>5$

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:25.564771Z

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Observation db7b5f76-b5e7-4a68-bf4a-d0c0d56652e5 · outbound

This paper cites Little Red Dots: an abundant population of faint AGN at z~5 revealed by the EIGER and FRESCO JWST surveys.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Little Red Dots: an abundant population of faint AGN at z~5 revealed by the EIGER and FRESCO JWST surveys

Reference 5

Resolution: malformed identifier; no resolver link, observed 2026-08-02T12:34:25.645180Z

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Observation 375c081a-598f-44a0-be79-a6dbe5c85a17 · outbound

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

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution A Census of Photometrically Selected Little Red Dots at 4 < z < 9 in JWST Blank Fields

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:25.696911Z

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Observation 9787dd95-1828-4285-beb9-9dc56c8fe5d2 · outbound

This paper cites an unresolved cited work.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Unresolved cited work

Reference 7

Resolution: malformed identifier; no resolver link, observed 2026-08-02T12:34:25.777195Z

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Observation f3bb519d-6188-4ff4-9702-a2d924e305b2 · outbound

This paper cites an unresolved cited work.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Unresolved cited work

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:25.859281Z

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Observation ba33f0f5-a06b-4e3a-ac31-7c2449fbe23a · outbound

This paper cites RUBIES: Evolved Stellar Populations with Extended Formation Histories at $z \sim 7-8$ in Candidate Massive Galaxies Identified with JWST/NIRSpec.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution RUBIES: Evolved Stellar Populations with Extended Formation Histories at $z \sim 7-8$ in Candidate Massive Galaxies Identified with JWST/NIRSpec

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:25.914675Z

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Observation 0c689920-09a2-473c-9120-c335d188953a · outbound

This paper cites BlackTHUNDER strikes twice: rest-frame Balmer-line absorption and high Eddington accretion rate in a Little Red Dot at $z=7.04$.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution BlackTHUNDER strikes twice: rest-frame Balmer-line absorption and high Eddington accretion rate in a Little Red Dot at $z=7.04$

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:25.997241Z

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Observation 807f55fe-f77e-455e-9dfa-115f18783c34 · outbound

This paper cites X-ray View of Little Red Dots: Do They Host Supermassive Black Holes?.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution X-ray View of Little Red Dots: Do They Host Supermassive Black Holes?

Reference 11

Resolution: malformed identifier; no resolver link, observed 2026-08-02T12:34:26.057994Z

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Observation d24af936-3bf9-43b4-9975-8273e5f9d8b3 · outbound

This paper cites Stacking X-ray Observations of "Little Red Dots": Implications for their AGN Properties.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Stacking X-ray Observations of "Little Red Dots": Implications for their AGN Properties

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:26.115822Z

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Observation 81b8ac2d-ef98-4c01-b678-f099c2046085 · 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.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution 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 13

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:26.198483Z

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Observation e0e2bc83-6f40-4e60-9179-40ebc81e9f06 · outbound

This paper cites an unresolved cited work.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Unresolved cited work

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:26.288962Z

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Observation ea38481b-47c9-4fcf-9702-499f03ea3db1 · outbound

This paper cites an unresolved cited work.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Unresolved cited work

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:26.350402Z

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Observation c29410e5-6974-499f-afb6-ca15ae7a135e · outbound

This paper cites an unresolved cited work.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Unresolved cited work

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:26.433564Z

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Observation 04465dac-1e0e-4be5-bb9c-ddb135c0b779 · outbound

This paper cites little red dots.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution little red dots

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:26.493330Z

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Observation 99b70cc4-78d1-4537-9ccd-6c6e413354b3 · outbound

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

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Little Red Dots: Rapidly Growing Black Holes Reddened by Extended Dusty Flows

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:26.575272Z

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Observation 4f7e88c8-8bde-415c-8ddd-46b37dcb2770 · outbound

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

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

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Observation d2e54572-96b1-4b85-a383-fe88420103aa · outbound

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

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution A confirmed deficit of hot and cold dust emission in the most luminous Little Red Dots

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:26.762937Z

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Observation e241cbe3-5e37-4eb2-8302-0ad2330ed7cf · outbound

This paper cites an unresolved cited work.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Unresolved cited work

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:26.825878Z

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Observation 0d5d81a6-e3bb-4a58-9765-7ab68c63d145 · outbound

This paper cites & Mayer, L.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution & Mayer, L

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:26.866570Z

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Observation 35b26106-eaf8-4ae6-8d26-34c482cafc45 · outbound

This paper cites Spectral Appearance of Self-gravitating Disks Powered by Stellar Objects: Universal Effective Temperature in the Optical Continuum and Application to Little Red Dots.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Spectral Appearance of Self-gravitating Disks Powered by Stellar Objects: Universal Effective Temperature in the Optical Continuum and Application to Little Red Dots

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:26.933650Z

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Observation ff66e43f-e292-4899-a774-226be9a171d6 · 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.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution The Rise of Faint, Red AGN at $z>4$: A Sample of Little Red Dots in the JWST Extragalactic Legacy Fields

Reference 24

Resolution: malformed identifier; no resolver link, observed 2026-08-02T12:34:26.961125Z

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Observation fdd3359b-6b7e-430c-a7bf-50e962a0a59e · outbound

This paper cites Red, hot, and very metal poor: extreme properties of a massive accreting black hole in the first 500 Myr.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Red, hot, and very metal poor: extreme properties of a massive accreting black hole in the first 500 Myr

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:27.066041Z

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Observation a1249dcb-91c1-4e24-8178-b87455e2ff51 · outbound

This paper cites an unresolved cited work.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Unresolved cited work

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:27.131012Z

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Observation 1716e842-dcc2-4b21-b5af-1023f907a299 · outbound

This paper cites The Host Galaxy (If Any) of the Little Red Dots.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution The Host Galaxy (If Any) of the Little Red Dots

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:27.224618Z

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Observation 26e9c61c-12f1-448d-a176-edd28a4573cd · outbound

This paper cites A direct black hole mass measurement in a Little Red Dot at the Epoch of Reionization.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution A direct black hole mass measurement in a Little Red Dot at the Epoch of Reionization

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:27.295834Z

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Observation aadb6193-c23b-4d08-8856-eaa4830532bf · outbound

This paper cites an unresolved cited work.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Unresolved cited work

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:27.366456Z

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Observation be199f96-dfb9-4056-97f1-ad213d5d04b0 · outbound

This paper cites UNCOVER: 404 Error -- Models Not Found for the Triply Imaged Little Red Dot A2744-QSO1.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution UNCOVER: 404 Error -- Models Not Found for the Triply Imaged Little Red Dot A2744-QSO1

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:27.410627Z

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Observation 7a84db79-f71e-4c9b-b40d-0ef46498055a · outbound

This paper cites an unresolved cited work.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Unresolved cited work

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:27.448338Z

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Observation 31e0bb21-6991-4d36-82f8-d2f65ed3fb69 · outbound

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

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 32

Resolution: malformed identifier; no resolver link, observed 2026-08-02T12:34:27.480144Z

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Observation 581ad3ae-a956-48e8-a949-a90449d22c4e · outbound

This paper cites The z=5 Quasar Luminosity Function from SDSS Stripe 82.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution The z=5 Quasar Luminosity Function from SDSS Stripe 82

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:27.516548Z

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Observation 5e11e123-6254-4c18-b6f2-389ef26cb0b0 · outbound

This paper cites The Faint End of the z=5 Quasar Luminosity Function from the CFHTLS.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution The Faint End of the z=5 Quasar Luminosity Function from the CFHTLS

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:27.567938Z

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Observation 43f46d81-74cd-4509-a588-ec5341a17eed · outbound

This paper cites A survey of luminous high-redshift quasars with SDSS and WISE II. the bright end of the quasar luminosity function at z ~ 5.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution A survey of luminous high-redshift quasars with SDSS and WISE II. the bright end of the quasar luminosity function at z ~ 5

Reference 35

Resolution: malformed identifier; no resolver link, observed 2026-08-02T12:34:27.650078Z

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Observation e2cf5ce7-11d6-4092-9cff-64bbb393a4c5 · outbound

This paper cites The Final SDSS High-Redshift Quasar Sample of 52 Quasars at z>5.7.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution The Final SDSS High-Redshift Quasar Sample of 52 Quasars at z>5.7

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:27.714186Z

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Observation d92ccecd-5492-41b2-92b5-a918fecd7978 · outbound

This paper cites Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). X. Discovery of 35 Quasars and Luminous Galaxies at 5.7 $\le$ z $\le$ 7.0.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). X. Discovery of 35 Quasars and Luminous Galaxies at 5.7 $\le$ z $\le$ 7.0

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:27.768384Z

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Observation b58a13da-3a26-4950-a2b1-160f12b62334 · outbound

This paper cites The Pan-STARRS1 $\mathbf{z>5.6}$ Quasar Survey: III. The $\mathbf{z\approx6}$ Quasar Luminosity Function.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution The Pan-STARRS1 $\mathbf{z>5.6}$ Quasar Survey: III. The $\mathbf{z\approx6}$ Quasar Luminosity Function

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:27.846233Z

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Observation bd2b3de3-e315-4773-b8a8-9f10fe313853 · outbound

This paper cites Exploring Reionization-Era Quasars III: Discovery of 16 Quasars at $6.4\lesssim z \lesssim 6.9$ with DESI Legacy Imaging Surveys and UKIRT Hemisphere Survey and Quasar Luminosity Function at $z\sim6.7$.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Exploring Reionization-Era Quasars III: Discovery of 16 Quasars at $6.4\lesssim z \lesssim 6.9$ with DESI Legacy Imaging Surveys and UKIRT Hemisphere Survey and Quasar Luminosity Function at $z\sim6.7$

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:27.902214Z

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Observation 812cd59d-759e-42ee-875c-ddb1958db862 · outbound

This paper cites Quasar Luminosity Function at z = 7.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Quasar Luminosity Function at z = 7

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:27.983922Z

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Observation f52527c1-8f6d-4f7f-afac-94271a81dfdc · outbound

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

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Lonely Little Red Dots: Challenges to the AGN-nature of little red dots through their clustering and spectral energy distributions

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:28.082153Z

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

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

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

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Observation 5c349bf0-883b-4a2e-b1c0-545c3cdbe8d5 · outbound

This paper cites Little Red Dots as the Very First Activity of Black Hole Growth.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Little Red Dots as the Very First Activity of Black Hole Growth

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:28.289290Z

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Observation 92e5eba4-e087-4b01-8c14-5843aeb9d020 · outbound

This paper cites an unresolved cited work.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Unresolved cited work

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:28.391699Z

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Observation 0f47e8f7-9c3c-4898-ad55-7400d5976ee4 · outbound

This paper cites an unresolved cited work.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Unresolved cited work

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:28.521583Z

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Observation c2f181c4-12ce-460e-970a-fbffd8c25f84 · outbound

This paper cites Estimating Black Hole Masses in Active Galaxies Using the Halpha Emission Line.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Estimating Black Hole Masses in Active Galaxies Using the Halpha Emission Line

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:28.675966Z

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Observation b8859b5d-8438-4511-8843-a37ce56b4544 · outbound

This paper cites an unresolved cited work.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Unresolved cited work

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:28.852115Z

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Observation c282eb8b-013f-40db-be49-14ef6cb499a9 · outbound

This paper cites an unresolved cited work.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Unresolved cited work

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:28.974086Z

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Observation 7e849438-b163-4174-9dd0-ebc021aba32c · outbound

This paper cites an unresolved cited work.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Unresolved cited work

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:29.153557Z

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Observation 1e8832e2-90f6-430f-9fe8-4f24d3ab01a7 · outbound

This paper cites an unresolved cited work.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Unresolved cited work

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:29.314034Z

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Observation 2f2016b9-1461-484f-b97e-491d8ba1ca7c · outbound

This paper cites an unresolved cited work.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Unresolved cited work

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:29.434868Z

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Observation c6777e27-6c35-4fe7-ba23-06d945594259 · outbound

This paper cites Clustering of High Redshift ($z\ge 2.9$) Quasars from the Sloan Digital Sky Survey.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Clustering of High Redshift ($z\ge 2.9$) Quasars from the Sloan Digital Sky Survey

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:29.499468Z

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Observation dd714fd9-5a1c-46e9-b0d3-c8a7e6d73f21 · outbound

This paper cites Clustering of Low-Redshift (z <= 2.2) Quasars from the Sloan Digital Sky Survey.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Clustering of Low-Redshift (z <= 2.2) Quasars from the Sloan Digital Sky Survey

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:29.586906Z

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Observation 261d2471-cfc8-477b-bb41-dd97deadc581 · outbound

This paper cites an unresolved cited work.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Unresolved cited work

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:29.653114Z

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Observation ea806575-5c16-4c39-b466-3473224c77d1 · outbound

This paper cites The Clustering of High-Redshift (2.9 $\leq$ z $\leq$ 5.1) Quasars in SDSS Stripe 82.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution The Clustering of High-Redshift (2.9 $\leq$ z $\leq$ 5.1) Quasars in SDSS Stripe 82

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:29.701685Z

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Observation 27a0ad77-f875-4a25-b590-4af62104c3af · outbound

This paper cites Clustering of quasars in a wide luminosity range at redshift 4 with Subaru Hyper Suprime-Cam wide field imaging.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Clustering of quasars in a wide luminosity range at redshift 4 with Subaru Hyper Suprime-Cam wide field imaging

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:29.770832Z

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Observation b54b19ec-9d5c-4ff1-9f07-a013c5c6794d · outbound

This paper cites Subaru High-$z$ Exploration of Low-Luminosity Quasars (SHELLQs). XVIII. The Dark Matter Halo Mass of Quasars at $z\sim6$.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Subaru High-$z$ Exploration of Low-Luminosity Quasars (SHELLQs). XVIII. The Dark Matter Halo Mass of Quasars at $z\sim6$

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:29.872685Z

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Unavailable: canonical work link unavailable.

Observation 9209fe3e-9186-4506-bc05-a53b512eed9b · outbound

This paper cites EIGER VI. The Correlation Function, Host Halo Mass and Duty Cycle of Luminous Quasars at $z\gtrsim6$.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution EIGER VI. The Correlation Function, Host Halo Mass and Duty Cycle of Luminous Quasars at $z\gtrsim6$

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:29.988431Z

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Observation 8553afac-b28b-4a24-81a3-4590553d2b20 · outbound

This paper cites Probing Dark Matter Halos of High-redshift Quasars via Wide-Field Clustering.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Probing Dark Matter Halos of High-redshift Quasars via Wide-Field Clustering

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:30.103866Z

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Observation 155ceaa6-d1af-434f-a43c-22ab48bbfc3f · outbound

This paper cites The nature of low-luminosity AGNs discovered by JWST based on clustering analysis: progenitors of low-$z$ quasars?.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution The nature of low-luminosity AGNs discovered by JWST based on clustering analysis: progenitors of low-$z$ quasars?

Reference 60

Resolution: malformed identifier; no resolver link, observed 2026-08-02T12:34:30.192369Z

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Observation 219be0de-b6fc-4c46-a62c-024532389076 · outbound

This paper cites Constraints on the early Universe star formation efficiency from galaxy clustering and halo modeling of H$\alpha$ and [O III] emitters.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Constraints on the early Universe star formation efficiency from galaxy clustering and halo modeling of H$\alpha$ and [O III] emitters

Reference 61

Resolution: malformed identifier; no resolver link, observed 2026-08-02T12:34:30.232268Z

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Observation a4b76ae4-a85b-4dc2-9045-fb813eae8269 · outbound

This paper cites UniverseMachine: The Correlation between Galaxy Growth and Dark Matter Halo Assembly from z=0-10.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution UniverseMachine: The Correlation between Galaxy Growth and Dark Matter Halo Assembly from z=0-10

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:30.293332Z

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Observation bb80cafd-0fd2-46ff-b935-c8b94fb8a5a3 · outbound

This paper cites Beyond the Bulge: a Fundamental Relation Between Supermassive Black Holes and Dark Matter Halos.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Beyond the Bulge: a Fundamental Relation Between Supermassive Black Holes and Dark Matter Halos

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:30.370110Z

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Observation a9c88a01-7580-45c3-84d7-922c78e3d2b5 · outbound

This paper cites Tully-Fisher Distances and Dynamical Mass Constraints for 24 Host Galaxies of Reverberation-Mapped AGN.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Tully-Fisher Distances and Dynamical Mass Constraints for 24 Host Galaxies of Reverberation-Mapped AGN

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:30.404957Z

Source-reported events for the cited work

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Observation d7780c45-cf7e-4a11-bd76-1687fe1b5676 · outbound

This paper cites Black-Hole-to-Halo Mass Relation From UNIONS Weak Lensing.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Black-Hole-to-Halo Mass Relation From UNIONS Weak Lensing

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:30.479985Z

Source-reported events for the cited work

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Observation 101c0a1a-9ef5-4cd2-8874-cabe9f66472b · outbound

This paper cites Evolutionary Paths of Active Galactic Nuclei and Their Host Galaxies.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Evolutionary Paths of Active Galactic Nuclei and Their Host Galaxies

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:30.519954Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation dfaa9399-6ccf-44d9-9040-0c532ec54f48 · outbound

This paper cites an unresolved cited work.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Unresolved cited work

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:30.568551Z

Source-reported events for the cited work

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Observation 5dde3fd0-8d5a-4f42-a29b-836c5983c136 · outbound

This paper cites an unresolved cited work.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Unresolved cited work

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:30.649009Z

Source-reported events for the cited work

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Observation 63adb6e9-9463-4539-a1df-6438cabab260 · outbound

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

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 18fedc0c-7928-4190-ac36-eb4586ff45cf · outbound

This paper cites & Haehnelt, M.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution & Haehnelt, M

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:30.811896Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5d1b855d-2aad-4afe-b9b9-c90c2584d855 · outbound

This paper cites Evolution of the Size-Mass Relation of Star-forming Galaxies Since $z=5.5$ Revealed by CEERS.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Evolution of the Size-Mass Relation of Star-forming Galaxies Since $z=5.5$ Revealed by CEERS

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:30.889655Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1f0d3da1-afac-498d-a32c-8b3c2c7d45a7 · outbound

This paper cites COSMOS-Web: Unraveling the Evolution of Galaxy Size and Related Properties at $2<z<10$.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution COSMOS-Web: Unraveling the Evolution of Galaxy Size and Related Properties at $2<z<10$

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:30.980363Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c7128e0f-c7c4-4f66-9553-2cee0816433a · outbound

This paper cites an unresolved cited work.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Unresolved cited work

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:31.066527Z

Source-reported events for the cited work

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Observation 41942b05-168e-4c4d-994a-05c3fe453ad4 · outbound

This paper cites The JWST UNCOVER Treasury survey: Ultradeep NIRSpec and NIRCam ObserVations before the Epoch of Reionization.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution The JWST UNCOVER Treasury survey: Ultradeep NIRSpec and NIRCam ObserVations before the Epoch of Reionization

Reference 74

Resolution: malformed identifier; no resolver link, observed 2026-08-02T12:34:31.139367Z

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Observation dcd6497b-6aaf-444f-bbf0-43fd5fa670f0 · outbound

This paper cites A Long Time Ago in a Galaxy Far, Far Away: A Candidate z ~ 12 Galaxy in Early JWST CEERS Imaging.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution A Long Time Ago in a Galaxy Far, Far Away: A Candidate z ~ 12 Galaxy in Early JWST CEERS Imaging

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:31.216312Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 597495bd-ddd0-43b1-bb10-35a0148e409e · outbound

This paper cites Overview of the JWST Advanced Deep Extragalactic Survey (JADES).

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Overview of the JWST Advanced Deep Extragalactic Survey (JADES)

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:31.305322Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cd57d077-4d7c-4382-8ff5-44d65b168893 · outbound

This paper cites an unresolved cited work.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Unresolved cited work

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:31.426107Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 37779bc3-7cb2-4477-9d9d-39e185954498 · outbound

This paper cites An Atlas of Color-selected Quiescent Galaxies at $z>3$ in Public $JWST$ Fields.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution An Atlas of Color-selected Quiescent Galaxies at $z>3$ in Public $JWST$ Fields

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:31.501317Z

Source-reported events for the cited work

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Observation 8c5a63f8-e7db-40e7-812d-6c75408e7ea7 · outbound

This paper cites grizli (2023).

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution grizli (2023)

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:31.657843Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bb61125e-9da4-45b7-a8c8-ca963d99758b · outbound

This paper cites msaexp: Nirspec analysis tools (2023).

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution msaexp: Nirspec analysis tools (2023)

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:31.785260Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1be971cc-845e-4964-956e-38e2bcbc7184 · outbound

This paper cites EAZY: A Fast, Public Photometric Redshift Code.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution EAZY: A Fast, Public Photometric Redshift Code

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:31.939342Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f2fde659-a3bd-4fc7-b0ea-4dc4e8f6a1f0 · outbound

This paper cites UNCOVERing the extended strong lensing structures of Abell 2744 with the deepest JWST imaging.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution UNCOVERing the extended strong lensing structures of Abell 2744 with the deepest JWST imaging

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:32.100585Z

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Unavailable: canonical work link unavailable.

Observation eabf78fc-020d-4aba-8a77-24a2f1efd014 · outbound

This paper cites The UNCOVER Survey: First Release of Ultradeep JWST/NIRSpec PRISM spectra for ~700 galaxies from z~0.3-13 in Abell 2744.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution The UNCOVER Survey: First Release of Ultradeep JWST/NIRSpec PRISM spectra for ~700 galaxies from z~0.3-13 in Abell 2744

Reference 83

Resolution: malformed identifier; no resolver link, observed 2026-08-02T12:34:32.253108Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f0124887-83df-474d-a432-8a4c406d6252 · outbound

This paper cites Machine Learning-based Search of High-redshift Quasars.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Machine Learning-based Search of High-redshift Quasars

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:32.414567Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c6fa92c6-9bdc-4353-9086-84b4d0aeb9ff · outbound

This paper cites ASTRODEEP-JWST: NIRCam-HST multiband photometry and redshifts for half a million sources in six extragalactic deep fields.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution ASTRODEEP-JWST: NIRCam-HST multiband photometry and redshifts for half a million sources in six extragalactic deep fields

Reference 85

Resolution: malformed identifier; no resolver link, observed 2026-08-02T12:34:32.561925Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6dfa5ed9-7790-411c-9029-d7f9079a4676 · outbound

This paper cites The DESI Experiment Part I: Science,Targeting, and Survey Design.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution The DESI Experiment Part I: Science,Targeting, and Survey Design

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:32.730683Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5fa0aca8-230d-4817-9252-5efdbd304276 · outbound

This paper cites The DESI Experiment Part II: Instrument Design.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution The DESI Experiment Part II: Instrument Design

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:32.862533Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f161cd7b-a3dc-4090-bba4-56c4a56ab268 · outbound

This paper cites Data Release 1 of the Dark Energy Spectroscopic Instrument.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Data Release 1 of the Dark Energy Spectroscopic Instrument

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:32.999857Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 82e10a8c-6f1a-4426-9983-867fdde39317 · outbound

This paper cites The Construction of Large-scale Structure Catalogs for the Dark Energy Spectroscopic Instrument.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution The Construction of Large-scale Structure Catalogs for the Dark Energy Spectroscopic Instrument

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:33.161816Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ffc8540c-dddb-4b8b-a27e-e1e2e390bf8d · outbound

This paper cites DESI 2024 II: Sample Definitions, Characteristics, and Two-point Clustering Statistics.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution DESI 2024 II: Sample Definitions, Characteristics, and Two-point Clustering Statistics

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:33.391346Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 201f92ed-a50c-4210-827a-d7c407a09dc6 · outbound

This paper cites Overview of the DESI Legacy Imaging Surveys.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Overview of the DESI Legacy Imaging Surveys

Reference 91

Resolution: malformed identifier; no resolver link, observed 2026-08-02T12:34:33.530396Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a6f49c77-6e4f-4087-b3ae-b44416ed9da9 · outbound

This paper cites DESI luminous red galaxy samples for cross-correlations.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution DESI luminous red galaxy samples for cross-correlations

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:33.609378Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 501b5791-bb5d-4886-b6c3-a0819a107d27 · outbound

This paper cites The Clustering of DESI-like Luminous Red Galaxies Using Photometric Redshifts.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution The Clustering of DESI-like Luminous Red Galaxies Using Photometric Redshifts

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:33.741670Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8bf89658-8cc6-4c2f-819e-c5d6e66df77f · outbound

This paper cites an unresolved cited work.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Unresolved cited work

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:33.862909Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 01b31740-404a-4d3a-bb7f-4247966f28f8 · outbound

This paper cites & Peebles, P.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution & Peebles, P

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:33.989855Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 84f2eabc-da1a-467c-ba8d-f4cd385565c4 · outbound

This paper cites HMFcalc: An Online Tool for Calculating Dark Matter Halo Mass Functions.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution HMFcalc: An Online Tool for Calculating Dark Matter Halo Mass Functions

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:34.101785Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 276080b3-d897-48f1-9929-8038cac54aec · outbound

This paper cites an unresolved cited work.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Unresolved cited work

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:34.202741Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8056be6a-9266-4afc-a516-85582c0934c8 · outbound

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Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:34.361410Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b681c4f2-887d-4bbf-b4da-48dd91024e34 · outbound

This paper cites Efficient Computation of CMB anisotropies in closed FRW models.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Efficient Computation of CMB anisotropies in closed FRW models

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:34.497483Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3d750da5-6838-4bbd-8d5f-98c03e7f27d6 · outbound

This paper cites The Cosmological Constant.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution The Cosmological Constant

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:34.642987Z

Source-reported events for the cited work

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