What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? | Paper Citation Record

Observation 04e58e1d-bdcf-4745-9c72-dba16e4fa378 · outbound

This paper cites JWST UNCOVER: Extremely Red and Compact Object at z phot = 7.6 Triply Imaged by A2744.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? JWST UNCOVER: Extremely Red and Compact Object at z phot = 7.6 Triply Imaged by A2744

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.149838Z

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Observation 8404efc1-3c57-46a2-a2ae-87cb278b7b3e · outbound

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

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? A population of red candidate massive galaxies 600 Myr after the Big Bang

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.155995Z

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Observation 01cf9980-870a-4c8b-abc3-eea7e2049b8d · outbound

This paper cites Extremely Red Galaxies at z = 5–9 with MIRI and NIRSpec: Dusty Galaxies or Obscured Active Galactic Nuclei? Astrophys.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Extremely Red Galaxies at z = 5–9 with MIRI and NIRSpec: Dusty Galaxies or Obscured Active Galactic Nuclei? Astrophys

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.161551Z

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Observation 4b1ca7cc-abf0-4dfe-bcb7-984d148a67f9 · outbound

This paper cites UNCOVER Spectroscopy Confirms the Surprising Ubiquity of Active Galactic Nuclei in Red Sources at z > 5.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? UNCOVER Spectroscopy Confirms the Surprising Ubiquity of Active Galactic Nuclei in Red Sources at z > 5

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.167238Z

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Observation 85865348-9105-434a-b928-376416f047df · outbound

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

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? The Rise of Faint, Red Active Galactic Nuclei at z > 4: A Sample of Little Red Dots in the JWST Extragalactic Legacy Fields

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.172864Z

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Observation 95a619c4-2ffa-4b68-9be0-ec2ed443b75c · outbound

This paper cites Little Red Dots: An Abundant Population of Faint Active Galactic Nuclei at z ∼ 5 Revealed by the EIGER and FRESCO JWST Surveys.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Little Red Dots: An Abundant Population of Faint Active Galactic Nuclei at z ∼ 5 Revealed by the EIGER and FRESCO JWST Surveys

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.178543Z

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Observation c552bb27-7b51-490f-a46a-63a4dd203099 · outbound

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

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? UNCOVER: Candidate Red Active Galactic Nuclei at 3 < z < 7 with JWST and ALMA

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.184747Z

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Observation 1ec2668c-a46c-42b0-89bd-2c4ffb39af63 · outbound

This paper cites Hidden Little Monsters: Spectroscopic Identification of Low-mass, Broad-line AGNs at z > 5 with CEERS.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Hidden Little Monsters: Spectroscopic Identification of Low-mass, Broad-line AGNs at z > 5 with CEERS

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.189819Z

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Observation 47c123d7-e239-43ed-a909-e749fd67b931 · outbound

This paper cites Exploring the Active Galactic Nucleus Fraction of a Sample of JWST’s Little Red Dots at 4 < z < 8: Overmassive Black Holes Are Strongly Favored.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Exploring the Active Galactic Nucleus Fraction of a Sample of JWST’s Little Red Dots at 4 < z < 8: Overmassive Black Holes Are Strongly Favored

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.195747Z

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Observation 9d700975-e5f8-4046-8ebc-658883c93068 · outbound

This paper cites Little Red Dots.

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

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.200986Z

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Observation 3c931f66-68ef-432c-9fa7-036eaf9f13cf · outbound

This paper cites What Is the Nature of Little Red Dots and what Is Not, MIRI SMILES Edition.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? What Is the Nature of Little Red Dots and what Is Not, MIRI SMILES Edition

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.206695Z

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Observation 8a10fff0-c2a8-436b-b520-8c215c4e9904 · 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.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? The Galaxies Missed by Hubble and ALMA: The Contribution of Extremely Red Galaxies to the Cosmic Census at 3 < z < 8

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.211627Z

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Observation a0dc0f62-3537-41eb-a3d5-79f59772a983 · outbound

This paper cites Quiescent or dusty? Unveiling the nature of extremely red galaxies at z > 3.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Quiescent or dusty? Unveiling the nature of extremely red galaxies at z > 3

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.216894Z

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Observation 2de14e6a-e0c2-4d82-bdea-1f72775e136b · outbound

This paper cites CEERS Key Paper.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? CEERS Key Paper

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.222123Z

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Observation 1e95c0f3-8f02-4097-85aa-7f2523c960c4 · outbound

This paper cites Silencing the Giant: Evidence of Active Galactic Nucleus Feedback and Quenching in a Little Red Dot at z = 4.13.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Silencing the Giant: Evidence of Active Galactic Nucleus Feedback and Quenching in a Little Red Dot at z = 4.13

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.227029Z

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Observation 2487063e-7c58-4068-883d-35a7d74e18c4 · outbound

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

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? X-Ray View of Little Red Dots: Do They Host Supermassive Black Holes? Astrophys

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.232394Z

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Observation 6153cd75-d375-49f4-8643-51f7fb58c835 · outbound

This paper cites Little Red Dots.

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

Reference 17

Resolution: malformed identifier; no resolver link, observed 2026-08-15T16:36:25.237577Z

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

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

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 d047d461-7c94-428a-b646-891d6c2845b8 · outbound

This paper cites Deep silence: Radio properties of little red dots.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Deep silence: Radio properties of little red dots

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.247657Z

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Observation 1559163a-d362-48ae-94c1-446a7ba0755d · outbound

This paper cites The radio properties of the JWST-discovered AGN.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? The radio properties of the JWST-discovered AGN

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.252442Z

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Observation dd5783ad-aa8e-4e67-aeed-65e2928370c0 · outbound

This paper cites Another Piece to the Puzzle: Radio Detection of a JWST-detected Active Galactic Nucleus Candidate.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Another Piece to the Puzzle: Radio Detection of a JWST-detected Active Galactic Nucleus Candidate

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.257263Z

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Observation dabbed8f-5fa0-4cbe-9c09-9f93ed8a5cd7 · outbound

This paper cites Radio emission from little red dots may reveal their true nature.Astron.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Radio emission from little red dots may reveal their true nature.Astron

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.261758Z

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Observation 14a23b75-75da-49ff-be3b-4b5d9efc2f4f · outbound

This paper cites JWST meets Chandra: A large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? JWST meets Chandra: A large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.266736Z

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Observation 8b5d3032-4f51-4532-81bf-512580585b6b · outbound

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

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? RUBIES: JWST/NIRSpec Confirmation of an Infrared-luminous, Broad-line Little Red Dot with an Ionized Outflow

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.271549Z

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Observation 20fd020c-9831-4969-8461-463db9340518 · outbound

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

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? A Census of Photometrically Selected Little Red Dots at 4 < z < 9 in JWST Blank Fields

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.276585Z

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Observation 219694f0-4c3f-4b0b-9b85-fb62d3434998 · outbound

This paper cites JWST Insights into Narrow-line Little Red Dots.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? JWST Insights into Narrow-line Little Red Dots

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.281228Z

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Observation 39b93867-d9ba-4321-a9da-3d4495723bab · outbound

This paper cites ’Little red dots’ cannot reside in the same dark matter haloes as comparably luminous unobscured quasars.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? ’Little red dots’ cannot reside in the same dark matter haloes as comparably luminous unobscured quasars

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.286187Z

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Observation d066dfc5-1e4b-4231-842e-7314c47c95bd · outbound

This paper cites Dust in Little Red Dots.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Dust in Little Red Dots

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.291438Z

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Observation 0c72fc2e-416c-4e55-a15c-8f5026504c0e · outbound

This paper cites Challenging the AGN scenario for JWST/NIRSpec broad H α emitters/Little Red Dots in light of non-detection of NIRCam photometric variability and X-ray.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Challenging the AGN scenario for JWST/NIRSpec broad H α emitters/Little Red Dots in light of non-detection of NIRCam photometric variability and X-ray

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.296395Z

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Observation e7cec8e7-db8b-4fb9-9f26-f606ba160bd6 · outbound

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

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Lonely Little Red Dots: Challenges to the AGN-nature of little red dots through their clustering and spectral energy distributions

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.301482Z

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Observation da2e6c2b-2f64-4252-8a12-b23e8a35b2ab · outbound

This paper cites Little Red Dots Are Tidal Disruption Events in Runaway-collapsing Clusters.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Little Red Dots Are Tidal Disruption Events in Runaway-collapsing Clusters

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.306865Z

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Observation b401f639-5818-45d7-a744-ed9cbaa68d3c · outbound

This paper cites Black hole masses of tidal disruption event host galaxies.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Black hole masses of tidal disruption event host galaxies

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.312205Z

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Observation 76143792-08f0-4114-b38c-0781ad722dd9 · outbound

This paper cites Measuring stellar and black hole masses of tidal disruption events.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Measuring stellar and black hole masses of tidal disruption events

Reference 33

Resolution: verified exact; local_arxiv, observed 2026-08-15T16:36:26.981288Z

Source-reported events for the cited work

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

Observation ada909c5-9d58-4296-8ddc-8d373f808389 · outbound

This paper cites A Census of Archival X-Ray Spectra for Modeling Tidal Disruption Events.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? A Census of Archival X-Ray Spectra for Modeling Tidal Disruption Events

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.322476Z

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Observation e4b7af9f-a232-481a-88d6-add00a73e1ab · outbound

This paper cites Radio Properties of Tidal Disruption Events.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Radio Properties of Tidal Disruption Events

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.327934Z

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Observation 97f750e1-d3fa-4dc7-9815-6e988fe66c4a · outbound

This paper cites A Systematic Analysis of the Radio Properties of 22 X-Ray-selected Tidal Disruption Event Candidates with the Australia Telescope Compact Array.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? A Systematic Analysis of the Radio Properties of 22 X-Ray-selected Tidal Disruption Event Candidates with the Australia Telescope Compact Array

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.333040Z

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Observation ef97396d-2b8e-4dba-bc78-970292fbadd9 · outbound

This paper cites Radio Afterglows from Tidal Disruption Events: An Unbiased Sample from ASKAP RACS.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Radio Afterglows from Tidal Disruption Events: An Unbiased Sample from ASKAP RACS

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.338271Z

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Observation 519f497a-bc52-4d57-a3fd-c7d9a0bf540a · outbound

This paper cites Ubiquitous Late Radio Emission from Tidal Disruption Events.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Ubiquitous Late Radio Emission from Tidal Disruption Events

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.343115Z

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Observation 45a80e5e-033a-4960-ad22-d23869224d79 · outbound

This paper cites Are Delayed Radio Flares Common in Tidal Disruption Events? The Case of the TDE iPTF 16fnl.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Are Delayed Radio Flares Common in Tidal Disruption Events? The Case of the TDE iPTF 16fnl

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.348323Z

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Observation 6ce41360-90f2-422f-9149-fb4e28f88a14 · outbound

This paper cites Relativistic jet activity from the tidal disruption of a star by a massive black hole.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Relativistic jet activity from the tidal disruption of a star by a massive black hole

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.353197Z

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Observation 958fb80f-1c99-4ca4-878f-fb030d63c8c2 · outbound

This paper cites Discovery of Transient Infrared Emission from Dust Heated by Stellar Tidal Disruption Flares.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Discovery of Transient Infrared Emission from Dust Heated by Stellar Tidal Disruption Flares

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.357973Z

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Observation a3a3f85c-6fef-447f-ad53-c77535dac7b9 · outbound

This paper cites Discovery of an Outflow from Radio Observations of the Tidal Disruption Event ASASSN-14li.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Discovery of an Outflow from Radio Observations of the Tidal Disruption Event ASASSN-14li

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.362983Z

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Observation 84c359ec-17f9-4755-904a-818b506b9781 · outbound

This paper cites A radio-emitting outflow produced by the tidal disruption event AT2020vwl.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? A radio-emitting outflow produced by the tidal disruption event AT2020vwl

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.368155Z

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Observation 0e30ab30-01e5-4b4c-856a-411bc1cce125 · outbound

This paper cites Discovery of a Time Lag between the Soft X-Ray and Radio Emission of the Tidal Disruption Flare ASASSN-14li: Evidence for Linear Disk-Jet Coupling.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Discovery of a Time Lag between the Soft X-Ray and Radio Emission of the Tidal Disruption Flare ASASSN-14li: Evidence for Linear Disk-Jet Coupling

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.373219Z

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Observation 624867fa-60e1-4d9e-b24d-e193feb426ae · outbound

This paper cites A Late-time Radio Flare Following a Possible Transition in Accretion State in the Tidal Disruption Event AT 2019azh.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? A Late-time Radio Flare Following a Possible Transition in Accretion State in the Tidal Disruption Event AT 2019azh

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.378178Z

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Observation bdfe61bd-8291-4c05-9a51-782ff47d013f · outbound

This paper cites ASASSN-14li: A Model Tidal Disruption Event.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? ASASSN-14li: A Model Tidal Disruption Event

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.382806Z

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Observation ff7cc527-cf84-4cf4-a457-e2d66d4c9d1e · outbound

This paper cites Radio emission from the unbound debris of tidal disruption events.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Radio emission from the unbound debris of tidal disruption events

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.387356Z

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Observation f0321432-480a-42af-8eb5-8a8ab9efe069 · outbound

This paper cites A dust-enshrouded tidal disruption event with a resolved radio jet in a galaxy merger.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? A dust-enshrouded tidal disruption event with a resolved radio jet in a galaxy merger

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.391575Z

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Observation e86cccaf-6b27-41cf-af68-b8caedbb1bcd · outbound

This paper cites FIRST J153350.8+272729: The Radio Afterglow of a Decades-old Tidal Disruption Event.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? FIRST J153350.8+272729: The Radio Afterglow of a Decades-old Tidal Disruption Event

Reference 49

Resolution: malformed identifier; no resolver link, observed 2026-08-15T16:36:25.396191Z

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Observation c87cc160-8019-471c-b88e-0d0eae58a41a · outbound

This paper cites iPTF16fnl: A Faint and Fast Tidal Disruption Event in an E+A Galaxy.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? iPTF16fnl: A Faint and Fast Tidal Disruption Event in an E+A Galaxy

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.400790Z

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Observation a9547775-1463-4be4-a855-797ebd87cbf9 · outbound

This paper cites Tidal Disruption Events.

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

Reference 51

Resolution: verified exact; doi, observed 2026-08-15T16:36:25.928189Z

Source-reported events for the cited work

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

Observation f780710a-cd73-40b8-8e22-3ab7bfcda673 · outbound

This paper cites X-Ray Properties of TDEs.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? X-Ray Properties of TDEs

Reference 52

Resolution: malformed identifier; no resolver link, observed 2026-08-15T16:36:25.410299Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d773bd9d-a42a-4489-851b-6a12a894110e · outbound

This paper cites Optical-Ultraviolet Tidal Disruption Events.Space Sci.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Optical-Ultraviolet Tidal Disruption Events.Space Sci

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.415381Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6355a490-129c-4dea-8081-ec0c39c5855e · outbound

This paper cites Luminous Thermal Flares from Quiescent Supermassive Black Holes.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Luminous Thermal Flares from Quiescent Supermassive Black Holes

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.420087Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4fb8669f-0875-4c4a-9dd1-579442628f20 · outbound

This paper cites Swift J1112.2-8238: A candidate relativistic tidal disruption flare.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Swift J1112.2-8238: A candidate relativistic tidal disruption flare

Reference 55

Resolution: verified exact; doi, observed 2026-08-15T16:36:25.891094Z

Source-reported events for the cited work

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

Observation 44c5438d-7423-4843-a173-4ccd93d8d93e · outbound

This paper cites Rates of stellar tidal disruption as probes of the supermassive black hole mass function.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Rates of stellar tidal disruption as probes of the supermassive black hole mass function

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.430021Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8ab50395-b8d1-438e-bc4e-de1cd23ae40e · outbound

This paper cites On the Mass and Luminosity Functions of Tidal Disruption Flares: Rate Suppression due to Black Hole Event Horizons.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? On the Mass and Luminosity Functions of Tidal Disruption Flares: Rate Suppression due to Black Hole Event Horizons

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.435248Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fb27a0bb-4b91-48ea-8d6c-9ea437c26d43 · outbound

This paper cites A Catalog of Very Large Array Sky Survey Epoch 1 Quick Look Components, Sources, and Host Identifications.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? A Catalog of Very Large Array Sky Survey Epoch 1 Quick Look Components, Sources, and Host Identifications

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.440410Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5cbe2ccb-43b1-4e33-a6a5-1348c0518ab2 · outbound

This paper cites A Quick Look at the 3 GHz Radio Sky.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? A Quick Look at the 3 GHz Radio Sky

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.445404Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1f8726ff-60d2-440d-ae74-4e860548e9e1 · outbound

This paper cites Delayed radio flares from a tidal disruption event.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Delayed radio flares from a tidal disruption event

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.450317Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ab001552-6904-45ba-ba3b-ec380e2bf7d6 · outbound

This paper cites The radio detection and accretion properties of the peculiar nuclear transient AT 2019avd.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? The radio detection and accretion properties of the peculiar nuclear transient AT 2019avd

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.455350Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a6fa34a5-35b5-44b6-a5b6-32fdd2878359 · outbound

This paper cites An Untargeted Search for Radio-emitting Tidal Disruption Events in the VAST Pilot Survey.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? An Untargeted Search for Radio-emitting Tidal Disruption Events in the VAST Pilot Survey

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.460295Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ba12ed13-567e-44b0-a818-44c202688c1d · outbound

This paper cites Eight Years of Light from ASASSN-15oi: Toward Understanding the Late-time Evolution of TDEs.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Eight Years of Light from ASASSN-15oi: Toward Understanding the Late-time Evolution of TDEs

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.465562Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 85909cd6-67c3-48af-b4cc-ac4115787a0c · outbound

This paper cites Extragalactic High-energy Transients: Event Rate Densities and Luminosity Functions.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Extragalactic High-energy Transients: Event Rate Densities and Luminosity Functions

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.470190Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 40c3e8fa-4131-46bb-8c71-71139ebf32c2 · outbound

This paper cites The Star Ingesting Luminosity of Intermediate-Mass Black Holes in Globular Clusters.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? The Star Ingesting Luminosity of Intermediate-Mass Black Holes in Globular Clusters

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.475131Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b57e01d6-80e5-48e1-8204-a0688eef592f · outbound

This paper cites Star Formation at z ~6: The Hubble Ultra Deep Parallel Fields.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Star Formation at z ~6: The Hubble Ultra Deep Parallel Fields

Reference 66

Resolution: verified exact; doi, observed 2026-08-15T16:36:25.763965Z

Source-reported events for the cited work

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

Observation 27367f17-7ad9-403f-87ac-c15c83ddbfc9 · outbound

This paper cites A tidal disruption event coincident with a high-energy neutrino.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? A tidal disruption event coincident with a high-energy neutrino

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.485708Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 81b5d023-5a29-4dca-92b0-304a42038b8d · outbound

This paper cites High-resolution VLBI Observations of and Modeling the Radio Emission from the Tidal Disruption Event AT2019dsg.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? High-resolution VLBI Observations of and Modeling the Radio Emission from the Tidal Disruption Event AT2019dsg

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.490300Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 37760228-a52e-44c2-8e07-5e3ad8c2f9b0 · outbound

This paper cites Confronting predictions of the galaxy stellar mass function with observations at high redshift.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Confronting predictions of the galaxy stellar mass function with observations at high redshift

Reference 69

Resolution: malformed identifier; no resolver link, observed 2026-08-15T16:36:25.495206Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3651beb4-ff49-476a-807a-be7f0db624a5 · outbound

This paper cites UV Luminosity Functions at Redshifts z ∼ 4 to z ∼ 10: 10,000 Galaxies from HST Legacy Fields.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? UV Luminosity Functions at Redshifts z ∼ 4 to z ∼ 10: 10,000 Galaxies from HST Legacy Fields

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.500192Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b675c403-ba66-48ec-a6d0-1c7f117899ec · outbound

This paper cites A lack of evolution in the very bright end of the galaxy luminosity function from z = 8 to 10.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? A lack of evolution in the very bright end of the galaxy luminosity function from z = 8 to 10

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.504829Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c4536f05-475a-4f89-b619-ae7205a17a60 · outbound

This paper cites JWST high-redshift galaxy constraints on warm and cold dark matter models.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? JWST high-redshift galaxy constraints on warm and cold dark matter models

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.509714Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 99a45282-5dad-4a87-bcda-8f15c0f1c818 · outbound

This paper cites Introducing cosmosTNG: Simulating galaxy formation with constrained realizations of the COSMOS field.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Introducing cosmosTNG: Simulating galaxy formation with constrained realizations of the COSMOS field

Reference 73

Resolution: verified exact; doi, observed 2026-08-15T16:36:25.693728Z

Source-reported events for the cited work

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

Observation 7446eef6-89b3-4b43-b7ce-434113c2289d · outbound

This paper cites an unresolved cited work.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Unresolved cited work

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.518719Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5d5f1b07-3e07-4893-b7c1-f9cd6fca8db4 · outbound

This paper cites The BoRG-JWST Survey: Abundance and Mass-to-light Ratio of Luminous z = 7–9 Galaxies from Independent Sight Lines with NIRSpec.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? The BoRG-JWST Survey: Abundance and Mass-to-light Ratio of Luminous z = 7–9 Galaxies from Independent Sight Lines with NIRSpec

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.522755Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3cfee02c-7e71-4ef5-a65c-2b9d8687f543 · outbound

This paper cites Using photometric redshift data to improve the detection of galactic filaments with the Bisous model.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Using photometric redshift data to improve the detection of galactic filaments with the Bisous model

Reference 76

Resolution: verified exact; doi, observed 2026-08-15T16:36:25.655276Z

Source-reported events for the cited work

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

Observation 78f1f888-ebb7-4479-9aca-8cfc88b90889 · outbound

This paper cites The star formation rate of the Universe at z~6 from the Hubble Ultra-Deep Field.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? The star formation rate of the Universe at z~6 from the Hubble Ultra-Deep Field

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.531443Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 831f1053-1dc2-4e71-9ef6-9d5d1bba4c11 · outbound

This paper cites an unresolved cited work.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Unresolved cited work

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.535756Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 97072e45-a0cf-4706-8bfc-fdd7bef950c2 · outbound

This paper cites The evolution of galaxies at constant number density: A less biased view of star formation, quenching, and structural formation.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? The evolution of galaxies at constant number density: A less biased view of star formation, quenching, and structural formation

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.540054Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bf3c29bc-2f0f-4852-aae2-fb285398a313 · outbound

This paper cites Measuring Galaxy Abundance and Clustering at High Redshift from Incomplete Spectroscopic Data: Tests on Mock Catalogs.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Measuring Galaxy Abundance and Clustering at High Redshift from Incomplete Spectroscopic Data: Tests on Mock Catalogs

Reference 80

Resolution: verified exact; doi, observed 2026-08-15T16:36:25.617898Z

Source-reported events for the cited work

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

Observation 793d8f07-aedf-4a23-aa88-f451be411681 · outbound

This paper cites The Complete CEERS Early Universe Galaxy Sample: A Surprisingly Slow Evolution of the Space Density of Bright Galaxies at z ∼ 8.5–14.5.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? The Complete CEERS Early Universe Galaxy Sample: A Surprisingly Slow Evolution of the Space Density of Bright Galaxies at z ∼ 8.5–14.5

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.548542Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7f707fb5-cf9a-48ac-b99d-fe1137e189d9 · outbound

This paper cites Unveiling the Distant Universe: Characterizing z ≥ 9 Galaxies in the First Epoch of COSMOS-Web.

What Do Radio Emission Constraints Tell Us About Little Red Dots as Tidal Disruption Events? Unveiling the Distant Universe: Characterizing z ≥ 9 Galaxies in the First Epoch of COSMOS-Web

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-15T16:36:25.553170Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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