COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly | Paper Citation Record

Observation 1639acb9-dedc-4f90-9bd7-b865fa4a661d · inbound

Impact of primordial black holes on the formation of the first stars and galaxies cites this paper.

Impact of primordial black holes on the formation of the first stars and galaxies COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 105

Resolution: verified exact; arxiv_id, observed 2026-05-24T04:56:00.895289Z

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Exploring the Nature of Little Red Dots: Constraints on AGN and Stellar Contributions from PRIMER MIRI Imaging COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-12T18:08:35.129806Z

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Indefinitely flat rotation curves from Mpc sized charged cocoons COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

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Resolution: unresolved; no resolver link, observed 2026-08-12T11:39:40.817965Z

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Observation 3f2e0016-07ab-4f87-bb49-3d4d83dff7c1 · inbound

Signatures of black hole seeding in the local Universe: Predictions from the BRAHMA cosmological simulations cites this paper.

Signatures of black hole seeding in the local Universe: Predictions from the BRAHMA cosmological simulations 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 3db02ff2-98b3-4bb6-8b9f-c45dce5cc91d · inbound

Deep silence: radio properties of little red dots cites this paper.

Deep silence: radio properties of little red dots COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-12T10:12:04.052478Z

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A Comprehensive Photometric Selection of `Little Red Dots' in MIRI Fields: An IR-Bright LRD at $z=3.1386$ with Warm Dust Emission COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-12T00:57:55.837047Z

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Environmental Evidence for Overly Massive Black Holes in Low Mass Galaxies and a Black Hole - Halo Mass Relation at $z \sim 5$ COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-11T23:10:37.595818Z

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Observation 306f8e4e-bb6e-4b47-8866-b1d9f5137f28 · inbound

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Weakness of X-rays and Variability in High-redshift AGNs with Super-Eddington Accretion COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-11T22:20:27.161351Z

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An unambiguous AGN and a Balmer break in an Ultraluminous Little Red Dot at z=4.47 from Ultradeep UNCOVER and All the Little Things Spectroscopy cites this paper.

An unambiguous AGN and a Balmer break in an Ultraluminous Little Red Dot at z=4.47 from Ultradeep UNCOVER and All the Little Things Spectroscopy COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-11T21:29:42.382109Z

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Evaluating the Predictive Capacity of FLARES Simulations for High Redshift "Little Red Dots" cites this paper.

Evaluating the Predictive Capacity of FLARES Simulations for High Redshift "Little Red Dots" 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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Episodic super-Eddington accretion as a clue to Overmassive Black Holes in the early Universe COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-11T12:29:56.564889Z

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EPOCHS XI: The Structure and Morphology of Galaxies in the Epoch of Reionization to z ~ 12.5 COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

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Resolution: unresolved; no resolver link, observed 2026-08-11T11:49:29.272483Z

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Observation 372f3688-b77c-447e-b48c-160ea7b453c5 · inbound

Little Red Dots are Tidal Disruption Events in Runaway-Collapsing Clusters cites this paper.

Little Red Dots are Tidal Disruption Events in Runaway-Collapsing Clusters COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-10T22:03:27.685903Z

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Observation 36a1d52a-0766-4f87-bb31-4b51df700117 · inbound

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Another piece to the puzzle: radio detection of a JWST detected AGN candidate COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-10T21:27:30.398044Z

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Luminous Mid-IR Selected Type-2 Quasars at Cosmic Noon in SDSS Stripe82 I: Selection, Composite Photometry, and Spectral Energy Distributions COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 1

Resolution: malformed identifier; no resolver link, observed 2026-08-10T15:36:25.819231Z

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Observation bd3c30e3-54fb-42ae-a4bb-ac0bd371155c · inbound

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Radio emission from little red dots may reveal their true nature COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-09T01:00:39.268829Z

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Investigating photometric and spectroscopic variability in the multiply-imaged Little Red Dot A2744-QSO1 COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-08T11:37:36.167229Z

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A "Black Hole Star" Reveals the Remarkable Gas-Enshrouded Hearts of the Little Red Dots COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 22

Resolution: verified exact; arxiv_id, observed 2026-05-16T08:53:14.716903Z

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No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Dust-obscured Galaxies with Broken Power-law Spectral Energy Distributions Discovered by UNIONS COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-16T11:38:32.419701Z

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Observation 89b5c1a9-e8e8-4c74-a193-c710b0f3b6a9 · inbound

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The Physical Nature of the Off-centered Extended Emission Associated with the Little Red Dots COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-16T00:03:10.748671Z

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Observation f45443e7-754f-4d77-8f53-c236cdbb918b · inbound

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CAPERS-LRD-z9: A Gas Enshrouded Little Red Dot Hosting a Broad-line AGN at z=9.288 COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-15T23:32:33.417234Z

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First Light and Reionization Epoch Simulations (FLARES) -- XVIII: the ionising emissivities and hydrogen recombination line properties of early AGN COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-15T23:15:25.705877Z

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The Lyman-$\alpha$ emitter bispectrum as a probe of reionization morphology COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-07T14:55:35.325214Z

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

Reference 1

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

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Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-07T11:15:59.607138Z

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COSMOS-Web: Comprehensive Data Reduction for Wide-Area JWST NIRCam Imaging COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-07T11:14:20.578993Z

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COSMOS-Web: MIRI Data Reduction and Number Counts at 7.7$\mu$m using JWST COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-07T11:16:02.613911Z

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Lonely Little Red Dots: Challenges to the AGN-nature of little red dots through their clustering and spectral energy distributions COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-07T10:56:02.325061Z

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Primordial black holes in cosmological simulations: growth prospects for supermassive black holes COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-07T04:19:16.417871Z

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Signatures of BH seeding on the $\mathrm{M_{\displaystyle \bullet}}-\sigma$ relation: Predictions from the BRAHMA simulations COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-15T19:14:52.288560Z

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Beneath the Surface: >85% of z>5.9 QSOs in Massive Host Galaxies are UV-Faint COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-06T21:45:13.900918Z

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Little Red Dots from Small-Scale Primordial Black Hole Clustering COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-06T19:01:56.099692Z

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Observation 2518f9e0-85ed-4834-bb92-7c92ba041e4b · inbound

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Beyond the Dot: an LRD-like nucleus at the Heart of an IR-Bright Galaxy and its implications for high-redshift LRDs COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-06T14:44:22.891465Z

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Observation 15586e7c-5b9f-440f-86b1-7eaee75f44a6 · inbound

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Luminous Mid-IR Selected Obscured Quasars at Cosmic Noon in SDSS Stripe82 II: Spectroscopic Diversity and Broad H$\alpha$ Emissions COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-15T17:43:45.654867Z

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Observation 312de477-9e49-4c13-ad9d-1b5c8186bd67 · inbound

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Physical properties of galaxies and the UV Luminosity Function from $z\sim6$ to $z\sim14$ in COSMOS-Web COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-05T23:52:33.219091Z

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Observation fcc3f3ed-2136-4148-8bd2-7bb01667eaa0 · inbound

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Little Red reionization factories COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-05T19:03:20.316297Z

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Observation efd4e0b6-17ac-480e-8e9d-1698dc179942 · inbound

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Little Red Dots as Direct-collapse Black Hole Nurseries COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-05T18:19:59.146373Z

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Glimmers in the Cosmic Dawn. III. On the Photometrically Determined Black Hole Mass to Stellar Mass Relation Across Cosmic Time COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-05T17:45:09.320231Z

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Observation a9665731-8484-4f9d-863a-c4b2fcc8649a · inbound

On the Variability Features of Active Galactic Nuclei in Little Red Dots cites this paper.

On the Variability Features of Active Galactic Nuclei in Little Red Dots COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-05T17:14:43.497601Z

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Observation d8382a2e-200e-480a-859b-8191e680e905 · inbound

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MEGA: Spectrophotometric SED Fitting of Little Red Dots Detected in JWST MIRI COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-05T15:21:40.712523Z

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Observation ad227e08-4306-4d04-98f9-33e19bf580c2 · inbound

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Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XXIV. 54 New Quasars and Candidate Obscured Quasars at $5.71 \le z \le 7.02$ COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-05T14:33:51.926291Z

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Observation 9af8c509-3fbb-4ad9-8867-86e7724d8be5 · inbound

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Investigating Little Red Dots with UV Excess: Are They the High-Redshift Siblings of Blue Hot DOGs? COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-05T14:08:52.891463Z

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Observation 7387c8e3-1b89-4859-9bfa-d75efc4ad985 · inbound

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Understanding the Evolution of Black Hole Accretion and Dust out to z=4 with a Deep Imaging Extragalactic Survey with PRIMA COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-05T12:23:24.204896Z

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Observation 90d16ea7-63fa-4e85-b9a3-dbcba41b13d2 · inbound

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No Luminous Little Red Dots: A Sharp Cutoff in Their Luminosity Function COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-15T16:42:07.477554Z

Source-reported events for the cited work

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Observation 8de52128-c1fc-47ac-8445-decfa8a73c33 · inbound

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A two-phase model of galaxy formation: IV. Seeding and growing supermassive black holes in dark matter halos COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 1

Resolution: verified exact; arxiv_id, observed 2026-05-18T19:46:48.626349Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 9fb6c966-c9dc-4932-b9cb-d3000ddd7cb4 · inbound

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What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.242466Z

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Observation 96b68473-9461-44c1-8ae2-d42ce0790033 · inbound

Do Little Red Dots Vary? cites this paper.

Do Little Red Dots Vary? COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-05T10:54:52.965633Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c92665fb-03c0-46b8-a008-2066fef31281 · inbound

Characterizing the roles of transitory obscured phases and inner torus in shaping the fractions of obscured AGN at cosmic noon cites this paper.

Characterizing the roles of transitory obscured phases and inner torus in shaping the fractions of obscured AGN at cosmic noon COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-05T06:04:29.968512Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0fc565e8-8360-4996-a506-05acccca3447 · inbound

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots cites this paper.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:29.827497Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e4d3076f-182e-4ece-b3ec-e3177af1c04a · inbound

Balmer Absorption in Iron Low-Ionization Broad Absorption Line Quasars cites this paper.

Balmer Absorption in Iron Low-Ionization Broad Absorption Line Quasars COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-04T22:02:47.728633Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 96b5d8c4-e481-47fa-8e4e-005887b52960 · inbound

Discovery of Multiply Ionized Iron Emission Powered by an Active Galactic Nucleus in a z~7 Little Red Dot cites this paper.

Discovery of Multiply Ionized Iron Emission Powered by an Active Galactic Nucleus in a z~7 Little Red Dot COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-04T18:47:40.748123Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e764f734-bfae-45bd-a696-d478360d920f · inbound

Spectral Uniformity of Little Red Dots: A Natural Outcome of Coevolving Seed Black Holes and Nascent Starbursts cites this paper.

Spectral Uniformity of Little Red Dots: A Natural Outcome of Coevolving Seed Black Holes and Nascent Starbursts COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 1

Resolution: verified exact; arxiv_id, observed 2026-05-18T14:41:30.001688Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation b2390cea-6fa5-4a90-be2e-25981182b229 · inbound

The Cosmic Rush Hour: Rapid Formation of Bright, Massive, Disky, Star-Forming Galaxies as Signatures of Early-Universe Physics cites this paper.

The Cosmic Rush Hour: Rapid Formation of Bright, Massive, Disky, Star-Forming Galaxies as Signatures of Early-Universe Physics COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-04T15:37:57.035834Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 07fe3c45-946a-477e-8c24-3187e7d3598d · inbound

Evidence of violation of Case B recombination in Little Red Dots cites this paper.

Evidence of violation of Case B recombination in Little Red Dots COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-04T11:17:02.339089Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0a76835f-ce9e-40c7-95bc-dffa1fee6fc3 · inbound

Evolution of Size, Mass, and Density of Galaxies Since Cosmic Dawn cites this paper.

Evolution of Size, Mass, and Density of Galaxies Since Cosmic Dawn COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 166

Resolution: unresolved; no resolver link, observed 2026-08-04T10:27:03.396481Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0ded335b-4148-4f58-9a68-f83c084d0e92 · inbound

VENUS: When Red meets Blue -- A multiply imaged Little Red Dot with an apparent blue companion behind the galaxy cluster Abell 383 cites this paper.

VENUS: When Red meets Blue -- A multiply imaged Little Red Dot with an apparent blue companion behind the galaxy cluster Abell 383 COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-03T19:07:25.631012Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7bf28ff6-ad37-418b-8888-c6a6bdaa82d9 · inbound

(Re)solving the Complex Multiscale Morphology and V-shaped Spectral Energy Distribution of a Newly Discovered Strongly Lensed Little Red Dot in A383 cites this paper.

(Re)solving the Complex Multiscale Morphology and V-shaped Spectral Energy Distribution of a Newly Discovered Strongly Lensed Little Red Dot in A383 COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-03T18:55:20.242927Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 002127ee-5469-40bb-b68f-fef8769806e4 · inbound

Little Red Dots as Hidden Neutrino Sources cites this paper.

Little Red Dots as Hidden Neutrino Sources COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 6

Resolution: verified exact; arxiv_id, observed 2026-05-16T13:42:56.318061Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 2149e8e7-2a00-4640-95f6-346200e626ee · inbound

Smoluchowski Coagulation Equation and the Evolution of Primordial Black Hole Clusters cites this paper.

Smoluchowski Coagulation Equation and the Evolution of Primordial Black Hole Clusters COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 72

Resolution: verified exact; arxiv_id, observed 2026-05-13T21:23:17.482693Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 1fc6becb-da24-4506-83df-3316ea896ceb · inbound

Gravitational Waves from the Cosmic Dawn: Tracing Cosmic Black Hole Binaries with ET, LGWA and LISA cites this paper.

Gravitational Waves from the Cosmic Dawn: Tracing Cosmic Black Hole Binaries with ET, LGWA and LISA COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 28

Resolution: metadata mismatch; arxiv_id, observed 2026-05-10T05:00:36.818448Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation a4690201-358d-4069-a125-80ec2958414b · inbound

Light, heavy, primordial: exploring the diversity of black hole seeding and growth mechanisms in the JWST era cites this paper.

Light, heavy, primordial: exploring the diversity of black hole seeding and growth mechanisms in the JWST era COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 14

Resolution: verified exact; arxiv_id, observed 2026-05-09T23:24:43.021665Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation c4e9190f-3048-493d-ae6b-202f1711a938 · inbound

The GlimmIr: Spectroscopic Variability in a z~7 LRD Indicates Rapid Changes in Both the Narrow and Broad Line Regions cites this paper.

The GlimmIr: Spectroscopic Variability in a z~7 LRD Indicates Rapid Changes in Both the Narrow and Broad Line Regions COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 1

Resolution: verified exact; arxiv_id, observed 2026-05-09T02:29:40.798116Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation d07fbcf8-f0c8-475e-a771-ca0542139b70 · inbound

Hidden Monsters with SPHEREx I: A goldmine for heavily reddened quasars at cosmic noon cites this paper.

Hidden Monsters with SPHEREx I: A goldmine for heavily reddened quasars at cosmic noon COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 54

Resolution: metadata mismatch; arxiv_id, observed 2026-05-11T01:10:52.469049Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 1d1fa9a3-9872-4155-b608-992ed5adfe3c · inbound

Quenching of X-ray emission in little red dots by both Compton-thick gas and high accretion rates cites this paper.

Quenching of X-ray emission in little red dots by both Compton-thick gas and high accretion rates COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 54

Resolution: metadata mismatch; arxiv_id, observed 2026-05-19T16:17:39.588163Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation c26fdc4f-26ca-41a0-823d-5b0546c8cf42 · inbound

(LRDs)$^2$: The Low-ReDshift Little Red Dots Survey. II. DESI DR1 Sample cites this paper.

(LRDs)$^2$: The Low-ReDshift Little Red Dots Survey. II. DESI DR1 Sample COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 3

Resolution: verified exact; arxiv_id, observed 2026-05-22T09:46:22.288471Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation eccd24fc-728d-41e8-aa73-a17e08b5b1ff · inbound

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution cites this paper.

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

Reference 32

Resolution: malformed identifier; arxiv_id, observed 2026-07-02T00:36:24.458335Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution cites this paper.

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5f3ef51c-17d7-44f8-872a-0ada112193c4 · inbound

Little Red Dot progenitors from Compact Starbursts: A Natural Path to Early AGN Formation cites this paper.

Little Red Dot progenitors from Compact Starbursts: A Natural Path to Early AGN Formation COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 1

Resolution: verified exact; arxiv_id, observed 2026-06-28T09:31:48.996037Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation fbee67ff-4e36-4289-8811-3fd8dc6319d0 · inbound

Little red dots as a cosmological probe: constraining $H_0$ with quasi-periodic pulsations cites this paper.

Little red dots as a cosmological probe: constraining $H_0$ with quasi-periodic pulsations COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 4

Resolution: verified exact; arxiv_id, observed 2026-07-02T10:06:51.607898Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 65da3229-ca4c-4161-a40e-a0525887c037 · inbound

NEXUS: Abundance, Environments, and Spectral Diversity of Little Red Dots from the NIRSpec MSA Sample cites this paper.

NEXUS: Abundance, Environments, and Spectral Diversity of Little Red Dots from the NIRSpec MSA Sample COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 2

Resolution: verified exact; arxiv_id, observed 2026-06-27T16:21:01.422882Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 80b6a59a-2b62-4fdd-92ae-8fda29655bc4 · inbound

SEEDZ: Rapid Galaxy Assembly as a Pathway to Supermassive Stars, Dense Stellar Environments and Massive Black Hole Seeds cites this paper.

SEEDZ: Rapid Galaxy Assembly as a Pathway to Supermassive Stars, Dense Stellar Environments and Massive Black Hole Seeds COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 1

Resolution: verified exact; arxiv_id, observed 2026-06-29T05:13:07.319541Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation ffc13aaa-0c7c-4319-9b75-736a68ccd570 · inbound

The metallicities of little red dot host galaxies: LRDs are metal poor, but not pristine cites this paper.

The metallicities of little red dot host galaxies: LRDs are metal poor, but not pristine COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 194

Resolution: metadata mismatch; arxiv_id, observed 2026-07-01T05:05:24.196739Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 36f4197c-b1c0-4127-b44d-87a5c6554218 · inbound

Little Red Dots at z~2 in EIGER reveal a gentle decline with respect to their peak number density at z~5 cites this paper.

Little Red Dots at z~2 in EIGER reveal a gentle decline with respect to their peak number density at z~5 COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 243

Resolution: metadata mismatch; arxiv_id, observed 2026-07-02T18:27:16.320831Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 2b735a2c-26cb-4954-af32-15d6d6237a83 · inbound

Spatial decomposition of Little Red Dots with JWST/NIRSpec IFU into broad-line red cores and narrow-line blue host galaxies cites this paper.

Spatial decomposition of Little Red Dots with JWST/NIRSpec IFU into broad-line red cores and narrow-line blue host galaxies COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 7

Resolution: unresolved; no resolver link, observed 2026-07-13T01:29:44.810998Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d3db8356-5357-4f5e-854a-1aed9c2674a8 · inbound

Outflows in super-Eddington quasars drive clumpy circumgalactic medium and extended H$\alpha$ nebulae at $z \gtrsim 6$ cites this paper.

Outflows in super-Eddington quasars drive clumpy circumgalactic medium and extended H$\alpha$ nebulae at $z \gtrsim 6$ COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 290

Resolution: unresolved; no resolver link, observed 2026-08-01T06:59:01.647977Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0ec5a531-4dfe-4481-8e71-6f40de0fc6f3 · inbound

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

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 123

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:39.404480Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f0f637ad-694d-48c1-a33b-bca62d621e8a · inbound

Misaligned or chaotic? A strong break of axial symmetry in the local LRD J1025 revealed with VLT/FORS2 spectropolarimetry cites this paper.

Misaligned or chaotic? A strong break of axial symmetry in the local LRD J1025 revealed with VLT/FORS2 spectropolarimetry COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-03T00:41:18.865648Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

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

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

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.008907Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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