Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ | Paper Citation Record

Observation c3b6bb39-bd88-4acc-bcc3-78e1d5d704a4 · outbound

This paper cites A comprehensive and uniform sample of broad-line active galactic nuclei from the SDSS DR7.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ A comprehensive and uniform sample of broad-line active galactic nuclei from the SDSS DR7

Reference 1

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Observation 784b6f2b-dda4-4078-820e-d7768f3eff42 · outbound

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

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Estimating Black Hole Masses in Active Galaxies Using the Halpha Emission Line

Reference 2

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Observation a1cbd697-8765-49a5-9637-462f8b0e26dc · outbound

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

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 3

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Observation 035a78f2-7f60-46df-986b-ca2e3920eef6 · outbound

This paper cites arXiv e-prints , keywords =.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ arXiv e-prints , keywords =

Reference 4

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Observation 00b488ea-6e37-42d0-92b9-99aa227c1fb3 · outbound

This paper cites What drives the growth of black holes: a decade of progress.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ What drives the growth of black holes: a decade of progress

Reference 5

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Observation 3be649d3-3d60-4cba-bd55-bdd83bfc8345 · outbound

This paper cites The Dust Content and Opacity of Actively Star-Forming Galaxies.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ The Dust Content and Opacity of Actively Star-Forming Galaxies

Reference 6

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Observation 05fc4dda-03a8-4e5a-8c00-bcdc0887b3f1 · outbound

This paper cites arXiv e-prints , keywords =.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ arXiv e-prints , keywords =

Reference 7

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Observation f215f871-a40a-460a-82db-fb0c7f6d8a2a · outbound

This paper cites Overview of the DESI Legacy Imaging Surveys.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Overview of the DESI Legacy Imaging Surveys

Reference 8

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Observation e9b5ff56-6433-47fd-b4e0-ad2a6955c7ba · outbound

This paper cites an unresolved cited work.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Unresolved cited work

Reference 9

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Observation 7d35ab9f-4c8e-4abf-8a9a-3fde31cfc64c · 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.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ The galaxies missed by Hubble and ALMA: the contribution of extremely red galaxies to the cosmic census at 3<z<8

Reference 10

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Observation 4e99ea94-7c17-4ebb-8987-cfe0b77be411 · 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 $z=3.5$.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ 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 11

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Observation 07250cc5-a24f-41cf-858a-5f25ad1d2bdb · outbound

This paper cites RUBIES: a complete census of the bright and red distant Universe with JWST/NIRSpec.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ RUBIES: a complete census of the bright and red distant Universe with JWST/NIRSpec

Reference 12

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Observation a7d2d520-2305-4790-a2e6-8ef5099594fb · outbound

This paper cites arXiv e-prints , keywords =.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ arXiv e-prints , keywords =

Reference 13

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Observation 47fa9188-c1ff-4429-995a-6e05d3d36cab · outbound

This paper cites , keywords =.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ , keywords =

Reference 14

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Observation c4012663-304d-4ebd-ae97-25c4397489d9 · outbound

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

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ A "Black Hole Star" Reveals the Remarkable Gas-Enshrouded Hearts of the Little Red Dots

Reference 15

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Observation 8dba1549-8ed6-4f44-8756-efb7b2ff0cbf · outbound

This paper cites Investigating photometric and spectroscopic variability in the multiply-imaged Little Red Dot A2744-QSO1.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Investigating photometric and spectroscopic variability in the multiply-imaged Little Red Dot A2744-QSO1

Reference 16

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Observation 3bf7ce63-3533-4816-b54d-8038b16cb13f · outbound

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

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ A high black hole to host mass ratio in a lensed AGN in the early Universe

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.125432Z

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Observation 6328dc48-b9b8-4a85-8fd7-6089af590bdb · outbound

This paper cites UNCOVER: A NIRSpec Identification of a Broad Line AGN at z = 8.50.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ UNCOVER: A NIRSpec Identification of a Broad Line AGN at z = 8.50

Reference 18

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Observation cc5a46da-5ea6-4269-96b2-7d95e20f4a21 · outbound

This paper cites Nature Astronomy , keywords =.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Nature Astronomy , keywords =

Reference 19

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Observation 8a73db9c-edd7-499a-af3c-f203f308e554 · outbound

This paper cites arXiv e-prints , keywords =.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ arXiv e-prints , keywords =

Reference 20

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Observation 7e077961-5716-4e32-a54d-3f3ef1415244 · outbound

This paper cites , keywords =.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ , keywords =

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.155013Z

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Observation f5c9425a-d22b-41b8-b78e-50a41f9dba7f · outbound

This paper cites arXiv e-prints , keywords =.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ arXiv e-prints , keywords =

Reference 22

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Observation a6b8a335-0a91-41db-b949-5abbfa9bceba · outbound

This paper cites Dark Bondi Accretion Aided by Baryons and the Origin of JWST Little Red Dots.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Dark Bondi Accretion Aided by Baryons and the Origin of JWST Little Red Dots

Reference 23

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Observation 02d70706-8ac1-4ac1-85de-dc1e00f25403 · outbound

This paper cites arXiv e-prints , keywords =.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ arXiv e-prints , keywords =

Reference 24

Resolution: verified exact; doi, observed 2026-08-08T16:36:23.798073Z

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Observation bb50fb9e-8d16-40eb-9af7-7ab623e5a536 · outbound

This paper cites arXiv e-prints , keywords =.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ arXiv e-prints , keywords =

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.182605Z

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Observation 60ebba20-2d5c-4d93-bf7f-c625e21d97e1 · outbound

This paper cites , keywords =.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ , keywords =

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.188830Z

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Observation bc207340-f1ab-4d90-941f-3ee191061333 · outbound

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

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

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Observation 6a551fe3-4b75-45ea-b709-aae726a457db · outbound

This paper cites Little Red Dots from Small-Scale Primordial Black Hole Clustering.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Little Red Dots from Small-Scale Primordial Black Hole Clustering

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.201834Z

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Observation 1dc44153-e94e-4bc8-8eca-c04c5c42cddd · outbound

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

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ UNCOVER spectroscopy confirms a surprising ubiquity of AGN in red galaxies at $z>5$

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.212110Z

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Observation 34f960cf-59f4-490c-9747-bb1c5876c06f · outbound

This paper cites , keywords =.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ , keywords =

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.220475Z

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Observation 746dddf7-1de6-407a-b330-364cf9c2de03 · 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.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ The Rise of Faint, Red AGN at $z>4$: A Sample of Little Red Dots in the JWST Extragalactic Legacy Fields

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.229239Z

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Observation 5de05f23-66d1-4354-a9c8-25109d3cc40c · outbound

This paper cites Dust extinction from Balmer decrements of star-forming galaxies at 0.75<z<1.5 with HST/WFC3 spectroscopy from the WISP survey.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Dust extinction from Balmer decrements of star-forming galaxies at 0.75<z<1.5 with HST/WFC3 spectroscopy from the WISP survey

Reference 32

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Observation b0896666-8dd2-453c-a2bb-3dc781c3ce74 · outbound

This paper cites Correcting for the Effects of Interstellar Extinction.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Correcting for the Effects of Interstellar Extinction

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.245221Z

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Observation 16f88e8b-16b7-4596-acc7-4bd696eae385 · outbound

This paper cites Now You See It, Now You Don't: The Disappearing Central Engine of the Quasar J1011+5442.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Now You See It, Now You Don't: The Disappearing Central Engine of the Quasar J1011+5442

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.252775Z

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Observation 5a950340-d3c8-48cc-b061-01a3aab91cbf · outbound

This paper cites Measuring Reddening with SDSS Stellar Spectra and Recalibrating SFD.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Measuring Reddening with SDSS Stellar Spectra and Recalibrating SFD

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.259743Z

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Observation 4cac6cf0-e839-49d4-8c19-9de263449034 · outbound

This paper cites Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.266770Z

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Observation efa65a42-843d-4523-98c4-e9aaad9f7044 · outbound

This paper cites A Catalog of Quasar Properties from SDSS DR7.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ A Catalog of Quasar Properties from SDSS DR7

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.273427Z

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Observation 30cb8714-762e-4861-bdcc-c33444b81f18 · outbound

This paper cites Empirical extinction coefficients for the GALEX, SDSS, 2MASS and WISE passbands.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Empirical extinction coefficients for the GALEX, SDSS, 2MASS and WISE passbands

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.279146Z

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Observation f0b09865-19c3-4f3d-93fa-5dafe7d5e07c · outbound

This paper cites an unresolved cited work.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Unresolved cited work

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.285023Z

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Observation 675a4d3a-a430-4a63-a907-97808c002b4c · outbound

This paper cites , keywords =.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ , keywords =

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.290429Z

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Observation 7982ba20-bffc-46e5-b4af-b2aed3357a8e · outbound

This paper cites Beyond the Dot: an LRD-like nucleus at the Heart of an IR-Bright Galaxy and its implications for high-redshift LRDs.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Beyond the Dot: an LRD-like nucleus at the Heart of an IR-Bright Galaxy and its implications for high-redshift LRDs

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.296383Z

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Observation a3da72d6-a014-4534-b38a-aed3ff806120 · outbound

This paper cites Exploring Changing-look Active Galactic Nuclei with the Sloan Digital Sky Survey V: First Year Results.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Exploring Changing-look Active Galactic Nuclei with the Sloan Digital Sky Survey V: First Year Results

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.301891Z

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Observation a9578ee8-2acf-40ee-b589-f7feb5898819 · outbound

This paper cites , keywords =.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ , keywords =

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.307507Z

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Observation 74132454-e595-45ea-988e-d8d02de28745 · outbound

This paper cites , keywords =.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ , keywords =

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.313745Z

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Observation d964f283-1ccf-4558-a4ca-3d0969b0f518 · outbound

This paper cites , keywords =.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ , keywords =

Reference 45

Resolution: verified exact; doi, observed 2026-08-08T16:36:23.612424Z

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No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 2bfe2d47-9397-4b25-bc0d-71e26a9f268a · outbound

This paper cites The nature of massive black hole binary candidates: I. Spectral properties and evolution.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ The nature of massive black hole binary candidates: I. Spectral properties and evolution

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.326266Z

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Observation f485cec7-0954-4477-ba22-9770583a4327 · outbound

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

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Little Red Dots at an Inflection Point: Ubiquitous "V-Shaped" Turnover Consistently Occurs at the Balmer Limit

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.332427Z

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Observation a9799de3-3255-4b3d-acf6-0fcc67ed4d7a · outbound

This paper cites The Ninth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Baryon Oscillation Spectroscopic Survey.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ The Ninth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Baryon Oscillation Spectroscopic Survey

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.339580Z

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Observation bf1b6ac2-ae53-4ddf-82b1-cdf30d037460 · outbound

This paper cites The Zwicky Transient Facility: Data Processing, Products, and Archive.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ The Zwicky Transient Facility: Data Processing, Products, and Archive

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.345460Z

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Observation 5861d1ce-b48d-421f-b0e1-a46937a9384d · outbound

This paper cites Little Red reionization factories.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Little Red reionization factories

Reference 50

Resolution: metadata mismatch; local_arxiv, observed 2026-08-08T16:36:23.595812Z

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No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 4a25d15b-9090-4f29-b555-2c8cfc6b583d · outbound

This paper cites , year = 2025, month = aug, doi =.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ , year = 2025, month = aug, doi =

Reference 51

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Observation 704c2cd1-39bc-4c7c-b2aa-0ebbfc04b5b8 · outbound

This paper cites arXiv e-prints , keywords =.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ arXiv e-prints , keywords =

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.359496Z

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Observation 91a56ba5-b85b-47d4-9dbb-cd36bc51939f · outbound

This paper cites , keywords =.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ , keywords =

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.363628Z

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Observation b83ef83b-510d-4c35-b227-722d29390bdd · outbound

This paper cites What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events?.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events?

Reference 54

Resolution: metadata mismatch; local_arxiv, observed 2026-08-08T16:36:23.573402Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation cd0a60b3-cf05-4aeb-9e96-6b8e0812a840 · outbound

This paper cites , keywords =.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ , keywords =

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.382594Z

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Observation 5edfceab-f0d5-40c6-91d5-35b07fa0882c · outbound

This paper cites Do Little Red Dots Vary?.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Do Little Red Dots Vary?

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.388684Z

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Observation 6e8ee37b-a43d-4397-bc44-82e05f9e288b · outbound

This paper cites , keywords =.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ , keywords =

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.396149Z

Source-reported events for the cited work

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Observation fc5ab5b6-168c-48c2-8686-6a275ffd2194 · outbound

This paper cites Changing-look Active Galactic Nuclei.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Changing-look Active Galactic Nuclei

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.403403Z

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Observation 75387646-dc19-4cf0-bd34-569c1c60d3d7 · outbound

This paper cites , keywords =.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ , keywords =

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.410324Z

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Observation e79d6198-190d-4f47-8f2a-f379a9f8220b · 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.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ 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 60

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.416163Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6acae579-de89-4201-98bd-31a308e73f46 · outbound

This paper cites , keywords =.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ , keywords =

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.423161Z

Source-reported events for the cited work

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Observation 5c167476-54be-4925-9e04-a540522d808f · outbound

This paper cites The Seventh Data Release of the Sloan Digital Sky Survey.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ The Seventh Data Release of the Sloan Digital Sky Survey

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.428755Z

Source-reported events for the cited work

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Observation e41f3e4e-9ce1-4b56-af3c-ada6a20117f7 · outbound

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

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ A confirmed deficit of hot and cold dust emission in the most luminous Little Red Dots

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.434406Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation caed1286-bbe5-4ddf-8941-da60f2903d8a · outbound

This paper cites Planck 2018 results. VI. Cosmological parameters.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Planck 2018 results. VI. Cosmological parameters

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.439674Z

Source-reported events for the cited work

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Observation aea576bc-85ac-4a81-b4e4-867e1312da5d · outbound

This paper cites Understanding extreme quasar optical variability with CRTS: II. Changing-state quasars.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Understanding extreme quasar optical variability with CRTS: II. Changing-state quasars

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.445320Z

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Observation 29d9f8a9-f4e8-4846-a184-43101882615e · outbound

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

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ A population of red candidate massive galaxies ~600 Myr after the Big Bang

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.450726Z

Source-reported events for the cited work

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Observation f950b25a-656d-4d1d-92bc-55d9eeeb240e · outbound

This paper cites What is the nature of Little Red Dots and what is not, MIRI SMILES edition.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ What is the nature of Little Red Dots and what is not, MIRI SMILES edition

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.455883Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 44aadc94-efb9-4942-9e9f-583924e5695f · outbound

This paper cites doi:10.5281/zenodo.8370018 , version =.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ doi:10.5281/zenodo.8370018 , version =

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.461559Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5639ed2e-2a07-4cd1-92a6-1cf654b08dff · outbound

This paper cites Research in Astronomy and Astrophysics , year = 2012, month = sep, volume =.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Research in Astronomy and Astrophysics , year = 2012, month = sep, volume =

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.466767Z

Source-reported events for the cited work

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Observation 0eae7b52-c3a9-4677-9830-c5fe74248def · outbound

This paper cites The Wide-field Infrared Survey Explorer (WISE): Mission Description and Initial On-orbit Performance.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ The Wide-field Infrared Survey Explorer (WISE): Mission Description and Initial On-orbit Performance

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.472481Z

Source-reported events for the cited work

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Observation 160d1daf-310e-4a69-9453-b0990a18f8e0 · outbound

This paper cites , keywords =.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ , keywords =

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.477578Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6fcd268c-cf01-4929-99da-2b7564406862 · outbound

This paper cites The Galaxy Evolution Explorer: A Space Ultraviolet Survey Mission.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ The Galaxy Evolution Explorer: A Space Ultraviolet Survey Mission

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.482622Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7116e183-249d-4d67-97f2-c608c768c5ae · outbound

This paper cites The Pan-STARRS1 Surveys.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ The Pan-STARRS1 Surveys

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.488252Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9d6055e9-8300-4104-a17a-a6354b517969 · outbound

This paper cites The Gaia mission.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ The Gaia mission

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.493668Z

Source-reported events for the cited work

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Observation 2a60c1c7-8008-4b63-a150-9dd079904cf6 · outbound

This paper cites SDSS-III: Massive Spectroscopic Surveys of the Distant Universe, the Milky Way Galaxy, and Extra-Solar Planetary Systems.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ SDSS-III: Massive Spectroscopic Surveys of the Distant Universe, the Milky Way Galaxy, and Extra-Solar Planetary Systems

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.498742Z

Source-reported events for the cited work

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Observation e8d5f7ea-eeac-4628-aa7e-b41c9e532292 · outbound

This paper cites , keywords =.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ , keywords =

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.503551Z

Source-reported events for the cited work

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Observation bab8f308-753f-4026-8dc5-7264743bf528 · outbound

This paper cites , keywords =.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ , keywords =

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.509210Z

Source-reported events for the cited work

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Observation a17abc3c-fc1a-461d-8b8e-0e3e00d92f36 · outbound

This paper cites Detailed Structural Decomposition of Galaxy Images.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Detailed Structural Decomposition of Galaxy Images

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.513634Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 904a3fdd-add1-4fcb-81a7-2c3eb2b4c781 · outbound

This paper cites an unresolved cited work.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Unresolved cited work

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.519051Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4ec6134d-26e3-4119-8ab1-7978ae181c46 · outbound

This paper cites , keywords =.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ , keywords =

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.523466Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation db571dbb-9bbd-48b1-a499-7288decd77f7 · outbound

This paper cites arXiv e-prints , keywords =.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ arXiv e-prints , keywords =

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.527813Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c44e5c46-b063-40d2-bb3d-fdd30a6972ff · outbound

This paper cites ATLAS: A High-Cadence All-Sky Survey System.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ ATLAS: A High-Cadence All-Sky Survey System

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.532874Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation efdaaa33-3165-49dc-826f-7de4b970c2e4 · outbound

This paper cites First Results from the Catalina Real-time Transient Survey.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ First Results from the Catalina Real-time Transient Survey

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.538197Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6bad4f7d-3875-40ab-b901-89d460cdd747 · outbound

This paper cites Cosmology with the SPHEREX All-Sky Spectral Survey.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Cosmology with the SPHEREX All-Sky Spectral Survey

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.543456Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fad242ca-e6b9-47e1-a7ae-b459b9eb282c · outbound

This paper cites The James Webb Space Telescope.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ The James Webb Space Telescope

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.550045Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 95e380ff-9194-407f-8aaa-e9ee2715125e · 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.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ 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

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Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.555338Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c6a7200f-e242-46a6-a606-5e8c80776445 · outbound

This paper cites JWST UNCOVER: Extremely red and compact object at$z_{\mathrm{phot}}\simeq7.6$ triply imaged by Abell 2744.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ JWST UNCOVER: Extremely red and compact object at$z_{\mathrm{phot}}\simeq7.6$ triply imaged by Abell 2744

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.560858Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9e051070-3043-4a5b-bb05-9644ff20435e · outbound

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

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ X-ray View of Little Red Dots: Do They Host Supermassive Black Holes?

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.565941Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c7aa9a05-8b02-480f-ba68-ccf248faa9d1 · outbound

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

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Stacking X-ray Observations of "Little Red Dots": Implications for their AGN Properties

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.571883Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1031cf61-8401-4565-995e-bc1c202cf2e2 · outbound

This paper cites Dust in Little Red Dots.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Dust in Little Red Dots

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.577681Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cf63eff9-be07-4697-abb6-2e171c4aad37 · outbound

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

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ No [CII] or dust detection in two Little Red Dots at z$_{\rm spec}$ > 7

Reference 91

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 54d88d20-31ac-4e31-9faa-f2b3b213b45c · outbound

This paper cites , keywords =.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ , keywords =

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.588463Z

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Unavailable: canonical work link unavailable.

Observation 70191494-1b69-4e7c-bfa4-d349e9894e12 · outbound

This paper cites The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Overview and Early Data.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Overview and Early Data

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.593534Z

Source-reported events for the cited work

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Observation 1477b766-20d8-4019-896c-4c4c65549f5b · outbound

This paper cites Inferring the star-formation histories of massive quiescent galaxies with BAGPIPES: Evidence for multiple quenching mechanisms.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Inferring the star-formation histories of massive quiescent galaxies with BAGPIPES: Evidence for multiple quenching mechanisms

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.599060Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9d80d404-c717-42be-b537-948b797a0621 · outbound

This paper cites doi:10.1007/978-3-642-54083-7 , adsurl =.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ doi:10.1007/978-3-642-54083-7 , adsurl =

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.604995Z

Source-reported events for the cited work

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Observation 23e791de-5127-4031-a457-f3457b3f9034 · outbound

This paper cites pysersic: A Python package for determining galaxy structural properties via Bayesian inference, accelerated with jax.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ pysersic: A Python package for determining galaxy structural properties via Bayesian inference, accelerated with jax

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.611565Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4c9efa05-b11c-425c-ab17-e3f8cfd341ac · outbound

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

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ Little Red Dots: an abundant population of faint AGN at z~5 revealed by the EIGER and FRESCO JWST surveys

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.619553Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 35845820-f166-4e72-b195-7a0e2e0b89e4 · outbound

This paper cites EIGER I. a large sample of [OIII]-emitting galaxies at $5.3 < z < 6.9$ and direct evidence for local reionization by galaxies.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ EIGER I. a large sample of [OIII]-emitting galaxies at $5.3 < z < 6.9$ and direct evidence for local reionization by galaxies

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.624990Z

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Unavailable: canonical work link unavailable.

Observation 10a83c75-81d2-4d03-854e-c8ebf77d7681 · outbound

This paper cites The JWST FRESCO Survey: Legacy NIRCam/Grism Spectroscopy and Imaging in the two GOODS Fields.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ The JWST FRESCO Survey: Legacy NIRCam/Grism Spectroscopy and Imaging in the two GOODS Fields

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.635832Z

Source-reported events for the cited work

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Observation af2c5379-404c-43cd-8e9c-980b16ca424d · outbound

This paper cites CEERS Key Paper I: An Early Look into the First 500 Myr of Galaxy Formation with JWST.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ CEERS Key Paper I: An Early Look into the First 500 Myr of Galaxy Formation with JWST

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.643076Z

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