Paper Citation Record · LEDGER

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

As of 20 August 2026, this Paper Citation Record lists 70 of 70 outbound references and 2 inbound Pith citation observations for arXiv:2506.19589.

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

pith.paper-citation-record.v1
2506.19589 v1

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Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T03:35:56.530119Z

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

Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Reference resolution

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arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

Observation e3bfc0ea-8568-41cf-94dd-251766c244f2 · outbound

This paper cites an unresolved cited work.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Unresolved cited work

Reference 1

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Observation 4c7a63a8-ce5b-4f8c-a5a3-3a698f7284f1 · outbound

This paper cites Measurements of Omega and Lambda from 42 High-Redshift Supernovae.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Measurements of Omega and Lambda from 42 High-Redshift Supernovae

Reference 2

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Observation 8771f683-adcb-4f55-ad5c-fcf20a029a0b · outbound

This paper cites Dark Energy and the Accelerating Universe.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Dark Energy and the Accelerating Universe

Reference 3

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Observation 5d8018c1-5761-43be-8eb4-acd35dd3a837 · outbound

This paper cites Dark Energy.

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

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.747125Z

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Observation dfe4fc70-f39e-43f3-bd94-c0ef722ebf75 · outbound

This paper cites Cosmological Imprint of an Energy Component with General Equation of State.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Cosmological Imprint of an Energy Component with General Equation of State

Reference 5

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Observation 24c50dfa-c508-43f2-ac1e-8f09f415f53a · outbound

This paper cites Cosmology with a Primordial Scaling Field.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Cosmology with a Primordial Scaling Field

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.755222Z

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Observation c51066a4-e58e-4b4c-9230-c7d4b15976f6 · outbound

This paper cites The Limits of Quintessence.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots The Limits of Quintessence

Reference 7

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Observation 580b9d8f-09cf-4448-9c5f-0f5b40259665 · outbound

This paper cites Quintessence: A Review.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Quintessence: A Review

Reference 8

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Observation a6037156-3995-425e-90fe-398dae0437f4 · outbound

This paper cites Phantom Energy and Cosmic Doomsday.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Phantom Energy and Cosmic Doomsday

Reference 9

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Observation a11e79ee-86cb-43e7-b4e9-8892d6b33724 · outbound

This paper cites Quintom Cosmology: Theoretical implications and observations.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Quintom Cosmology: Theoretical implications and observations

Reference 10

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Observation 38c7a3ae-4d4b-45ed-bef9-8390b2ab1746 · outbound

This paper cites Theoretical Aspects of Quintom Models.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Theoretical Aspects of Quintom Models

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.774468Z

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Observation 44e7c3a4-74f9-456e-bf04-6f415418ddf7 · outbound

This paper cites f(T) teleparallel gravity and cosmology.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots f(T) teleparallel gravity and cosmology

Reference 12

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Observation 5f100786-1ce5-4fc2-8963-c237f87660ad · outbound

This paper cites Amendola, C.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Amendola, C

Reference 13

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Observation 0c549ad4-be6c-4f1e-a36e-378fbd73b765 · outbound

This paper cites Tracking and coupled dark energy as seen by WMAP.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Tracking and coupled dark energy as seen by WMAP

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.785270Z

Source-reported events for the cited work

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Observation 7b401012-dbea-41b3-9d49-5604f6f54607 · outbound

This paper cites Implications of Symmetry and Pressure in Friedmann Cosmology. II. Stellar Remnant Black Hole Mass Function.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Implications of Symmetry and Pressure in Friedmann Cosmology. II. Stellar Remnant Black Hole Mass Function

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.789297Z

Source-reported events for the cited work

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Observation 8a8f76a2-f468-4d62-a788-839a0c55aafc · outbound

This paper cites A Preferential Growth Channel for Supermassive Black Holes in Elliptical Galaxies at z<2.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots A Preferential Growth Channel for Supermassive Black Holes in Elliptical Galaxies at z<2

Reference 16

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Observation 57e03ce2-bd45-4d67-9b32-4c4bd2d362cc · outbound

This paper cites The dashed contours in black, blue and red show our simulated LRDs redshiftz∼6,z∼1.61 and z∼0.85.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots The dashed contours in black, blue and red show our simulated LRDs redshiftz∼6,z∼1.61 and z∼0.85

Reference 17

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Observation d5848c48-acc6-4728-b5bc-a4424797edd3 · outbound

This paper cites Observational evidence for cosmological coupling of black holes and its implications for an astrophysical source of dark energy.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Observational evidence for cosmological coupling of black holes and its implications for an astrophysical source of dark energy

Reference 18

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Source-reported events for the cited work

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Observation 8e6d52a6-7aa1-40a8-b1f9-864821f1439b · outbound

This paper cites Black hole event horizons are cosmologically coupled.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Black hole event horizons are cosmologically coupled

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.800584Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0ae5650d-2db7-4afb-bd69-0a7b0860c699 · outbound

This paper cites Quasi-local masses and cosmological coupling of black holes and mimickers.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Quasi-local masses and cosmological coupling of black holes and mimickers

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.804180Z

Source-reported events for the cited work

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Observation bdb53a8d-aa4f-4f0b-813b-5342744e2803 · outbound

This paper cites Disforming scalar-tensor cosmology.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Disforming scalar-tensor cosmology

Reference 21

Resolution: verified exact; local_arxiv, observed 2026-08-15T18:38:08.858893Z

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Observation 8e681003-b8a0-46c1-b7be-4fb6e7727991 · outbound

This paper cites Apparent horizons in cosmologically-embedded black holes.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Apparent horizons in cosmologically-embedded black holes

Reference 22

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Source-reported events for the cited work

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Observation d4b8c344-85dd-4ce0-b808-f91739853616 · outbound

This paper cites Interaction of a black hole with scalar field in cosmology background.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Interaction of a black hole with scalar field in cosmology background

Reference 23

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Observation f51588f5-047d-41b2-8899-97d015085155 · outbound

This paper cites Can gravitational vacuum condensate stars be a dark energy source?.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Can gravitational vacuum condensate stars be a dark energy source?

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.819286Z

Source-reported events for the cited work

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Observation 74389f2d-eeab-4de9-b4ca-46c043774901 · outbound

This paper cites Comment on "Observational Evidence for Cosmological Coupling of Black Holes and its Implications for an Astrophysical Source of Dark Energy".

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Comment on "Observational Evidence for Cosmological Coupling of Black Holes and its Implications for an Astrophysical Source of Dark Energy"

Reference 25

Resolution: verified exact; local_arxiv, observed 2026-08-15T18:38:08.806154Z

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Observation 98838a8f-90d4-41bd-8855-a2962aa1c543 · outbound

This paper cites Black holes embedded in FLRW cosmologies.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Black holes embedded in FLRW cosmologies

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.826920Z

Source-reported events for the cited work

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Observation 68258fce-2da8-4ef7-b38c-c84adbbf2b2d · outbound

This paper cites Models of cosmological black holes.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Models of cosmological black holes

Reference 27

Resolution: verified exact; local_arxiv, observed 2026-08-15T18:38:08.779799Z

Source-reported events for the cited work

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Observation 491113ab-3d1c-4acf-af94-a1f990202212 · outbound

This paper cites Can cosmologically-coupled mass growth of black holes solve the mass gap problem?.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Can cosmologically-coupled mass growth of black holes solve the mass gap problem?

Reference 28

Resolution: verified exact; local_arxiv, observed 2026-08-15T18:38:08.763098Z

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Observation 72c6e742-7f70-494b-ad8e-85ef655a9e92 · outbound

This paper cites DESI Dark Energy Time Evolution is Recovered by Cosmologically Coupled Black Holes.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots DESI Dark Energy Time Evolution is Recovered by Cosmologically Coupled Black Holes

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.838755Z

Source-reported events for the cited work

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Observation ccfe0528-85fe-473e-a70f-475a63200975 · outbound

This paper cites Positive neutrino masses with DESI DR2 via matter conversion to dark energy.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Positive neutrino masses with DESI DR2 via matter conversion to dark energy

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.842319Z

Source-reported events for the cited work

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Observation b4a9ec5d-3ac9-4641-bd17-626655d643d6 · outbound

This paper cites Gravastars and Black Holes of Anisotropic Dark Energy.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Gravastars and Black Holes of Anisotropic Dark Energy

Reference 31

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Source-reported events for the cited work

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Observation 4a282c91-f880-4a4f-b537-3126ec3cf18f · outbound

This paper cites Dark Energy on Astrophysical Scales and Its Detection in the Milky Way.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Dark Energy on Astrophysical Scales and Its Detection in the Milky Way

Reference 32

Resolution: verified exact; local_arxiv, observed 2026-08-15T18:38:08.713558Z

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Observation 597d4140-4440-4926-9156-02ed9d492b53 · outbound

This paper cites Anisotropic Distance Ladder in Pantheon+ Supernovae.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Anisotropic Distance Ladder in Pantheon+ Supernovae

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.852457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a6c72413-8597-4089-adf6-8de4f3c31db0 · outbound

This paper cites Cosmological coupling of nonsingular black holes.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Cosmological coupling of nonsingular black holes

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.855839Z

Source-reported events for the cited work

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Observation e646756d-ba3d-410c-b04d-663ccf4111e2 · outbound

This paper cites Constraints on cosmological coupling from the accretion history of supermassive black holes.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Constraints on cosmological coupling from the accretion history of supermassive black holes

Reference 35

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Source-reported events for the cited work

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Observation e7335774-9d42-48f7-a7ac-3293291cba3d · outbound

This paper cites Implications of cosmologically coupled black holes for pulsar timing arrays.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Implications of cosmologically coupled black holes for pulsar timing arrays

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.865346Z

Source-reported events for the cited work

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Observation c8def5da-8fea-48fd-ac0d-0be636b775ec · outbound

This paper cites Constraints on the cosmological coupling of black holes from Gaia.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Constraints on the cosmological coupling of black holes from Gaia

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.869791Z

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Observation 6e585d0f-3b9b-4d1e-aa54-92c38dce9b8c · outbound

This paper cites Black holes as the source of dark energy: a stringent test with high-redshift JWST AGNs.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Black holes as the source of dark energy: a stringent test with high-redshift JWST AGNs

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.874261Z

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Unavailable: canonical work link unavailable.

Observation 1be32e5b-2460-476f-aae9-3ee98ae92b3c · outbound

This paper cites Constraints on cosmologically coupled black holes from gravitational wave observations and minimal formation mass.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Constraints on cosmologically coupled black holes from gravitational wave observations and minimal formation mass

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.878695Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 353f24aa-0ddb-472b-9247-6219be383af3 · outbound

This paper cites Determining cosmological growth parameter for stellar-mass black holes.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Determining cosmological growth parameter for stellar-mass black holes

Reference 40

Resolution: verified exact; local_arxiv, observed 2026-08-15T18:38:08.620559Z

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 f4e7c2ce-40d6-4929-8aec-ceb85d8e7302 · outbound

This paper cites Constraints on the Cosmological Coupling of Black Holes from the Globular Cluster NGC 3201.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Constraints on the Cosmological Coupling of Black Holes from the Globular Cluster NGC 3201

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.887457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4d8afb43-5271-4257-9cb1-7ba3741400f8 · outbound

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

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Planck 2018 results. VI. Cosmological parameters

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.891545Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b12d5e73-a982-41c7-bbc9-72b96c4ced48 · outbound

This paper cites Modeling the JWST high-redshift galaxies with a general formation scenario and the consistency with the $\Lambda$CDM model.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Modeling the JWST high-redshift galaxies with a general formation scenario and the consistency with the $\Lambda$CDM model

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.895586Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3f43684e-a6e7-45fc-84a1-2073a8ef0311 · outbound

This paper cites Hunting Dark Matter Lines in the Infrared Background with the James Webb Space Telescope.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Hunting Dark Matter Lines in the Infrared Background with the James Webb Space Telescope

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.899430Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 684c4800-b787-4e71-aab6-d8c4a5648d5a · outbound

This paper cites Sensitivity of JWST to eV-Scale Decaying Axion Dark Matter.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Sensitivity of JWST to eV-Scale Decaying Axion Dark Matter

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.904964Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fbb94ee6-d1e2-4644-aa20-496ce19e2582 · outbound

This paper cites Can Dark Stars account for the star formation efficiency excess at very high redshifts?.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Can Dark Stars account for the star formation efficiency excess at very high redshifts?

Reference 46

Resolution: verified exact; local_arxiv, observed 2026-08-15T18:38:08.552624Z

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 83ee4966-5b30-43e1-a20a-0ef783d775b3 · outbound

This paper cites JWST observations constrain the time evolution of fine structure constants and dark energy - electromagnetic coupling.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots JWST observations constrain the time evolution of fine structure constants and dark energy - electromagnetic coupling

Reference 47

Resolution: verified exact; local_arxiv, observed 2026-08-15T18:38:08.536088Z

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 0d8a15f3-6352-4c0d-8dd8-b05df11e1c42 · outbound

This paper cites Detection of stellar light from quasar host galaxies at redshifts above 6.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Detection of stellar light from quasar host galaxies at redshifts above 6

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.917165Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0e14a84d-2ebe-460d-b65d-0cd951b10363 · outbound

This paper cites Zhang, E.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Zhang, E

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.921908Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 404a1c90-a87a-4449-90fd-317270be9c43 · outbound

This paper cites Juod ˇzbalis, R.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Juod ˇzbalis, R

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.925766Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 16256801-5411-464d-9ea8-9f5d6e71976d · outbound

This paper cites an unresolved cited work.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Unresolved cited work

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.929284Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 64b7374f-ae27-4f2b-ac1c-80135c84b942 · outbound

This paper cites EIGER V. Characterizing the Host Galaxies of Luminous Quasars at $z\gtrsim6$.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots EIGER V. Characterizing the Host Galaxies of Luminous Quasars at $z\gtrsim6$

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.933906Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 036d8a6d-158c-41e3-95e6-5d91f86b8ae5 · outbound

This paper cites JADES. The diverse population of infant Black Holes at 4<z<11: merging, tiny, poor, but mighty.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots JADES. The diverse population of infant Black Holes at 4<z<11: merging, tiny, poor, but mighty

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.938974Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 82c5cfc8-5a48-4867-8f87-83549ff20024 · 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.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots A JWST/NIRSpec First Census of Broad-Line AGNs at z=4-7: Detection of 10 Faint AGNs with M_BH~10^6-10^8 M_sun and Their Host Galaxy Properties

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.943743Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c84b4e01-be87-4e4e-b414-3a6107c5d7ab · outbound

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

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Silencing the Giant: Evidence of AGN Feedback and Quenching in a Little Red Dot at z = 4.13

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.948519Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f8167bb7-4304-4621-b667-cb529c52d424 · outbound

This paper cites A Highly Consistent Framework for the Evolution of the Star-Forming "Main Sequence" from z~0-6.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots A Highly Consistent Framework for the Evolution of the Star-Forming "Main Sequence" from z~0-6

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.952801Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0775f601-b811-4da0-9399-d671d05db6f8 · outbound

This paper cites Dilution of chemical enrichment in galaxies 600 Myr after the Big Bang.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Dilution of chemical enrichment in galaxies 600 Myr after the Big Bang

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.957502Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 02bce967-8da0-4d22-9140-e71192a6a7a6 · outbound

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

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Little Red Dots: an abundant population of faint AGN at z~5 revealed by the EIGER and FRESCO JWST surveys

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.960760Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 905b3b29-671e-42fa-8644-19d321975eb3 · outbound

This paper cites A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): A First Look at the Rest-frame Optical Spectra of $z > 6.5$ Quasars Using JWST.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): A First Look at the Rest-frame Optical Spectra of $z > 6.5$ Quasars Using JWST

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.963778Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 220a2c4e-ac45-4b8d-a75f-f47a503da183 · outbound

This paper cites an unresolved cited work.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Unresolved cited work

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.967066Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ad228109-bcf1-43c4-b398-0ecb0511bf13 · outbound

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

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots UNCOVER: Candidate Red Active Galactic Nuclei at 3<z<7 with JWST and ALMA

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.970693Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation dc6de5b8-835e-4c61-bcda-bedc98704eaf · outbound

This paper cites SMBH Seeds: Model Discrimination with High Energy Emission Based on Scaling Relation Evolution.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots SMBH Seeds: Model Discrimination with High Energy Emission Based on Scaling Relation Evolution

Reference 62

Resolution: verified exact; local_arxiv, observed 2026-08-15T18:38:08.177629Z

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 70161d82-b2d4-4baf-90c4-f596331d9480 · outbound

This paper cites Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.978431Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4db4e019-26e4-4ad2-8ec8-94f7b3ca0f37 · outbound

This paper cites Relations Between Central Black Hole Mass and Total Galaxy Stellar Mass in the Local Universe.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Relations Between Central Black Hole Mass and Total Galaxy Stellar Mass in the Local Universe

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.982289Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 288fa845-9b68-4dcd-88bb-80cd78064a21 · outbound

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

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Evolutionary Paths of Active Galactic Nuclei and Their Host Galaxies

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.986513Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6ba57e1e-6094-40e2-aa50-66daf66f1282 · outbound

This paper cites Two massive, compact, and dust-obscured candidate $z\sim 8$ galaxies discovered by JWST.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Two massive, compact, and dust-obscured candidate $z\sim 8$ galaxies discovered by JWST

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.990401Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c2fb999d-fe00-44bd-9391-24826c3fc2d9 · outbound

This paper cites Chandra Rules Out Super-Eddington Accretion Models For Little Red Dots.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Chandra Rules Out Super-Eddington Accretion Models For Little Red Dots

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.994604Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6614ea3f-9c11-40da-a1ac-d5a2da2bbb2d · outbound

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

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Counting Little Red Dots at $z<4$ with Ground-based Surveys and Spectroscopic Follow-up

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-15T18:38:07.998739Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

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

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

Reference 69

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3b21e683-5acd-4d00-bc90-7b0437669a81 · outbound

This paper cites Black Hole Mass Accretion Rates and Efficiency Factors for over 750 AGN and Multiple GBH.

Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots Black Hole Mass Accretion Rates and Efficiency Factors for over 750 AGN and Multiple GBH

Reference 70

Resolution: verified exact; local_arxiv, observed 2026-08-15T18:38:08.070692Z

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.

Pith citing papers

Observation 15be0b4d-3271-4a2c-9803-295930b39cb1 · inbound

How do the LIGO-Virgo-KAGRA's Heavy Black Holes Form? No evidence for core-collapse Intermediate-mass black holes in GWTC-4 cites this paper.

How do the LIGO-Virgo-KAGRA's Heavy Black Holes Form? No evidence for core-collapse Intermediate-mass black holes in GWTC-4 Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots

Reference 62

Resolution: verified exact; arxiv_id, observed 2026-05-08T23:14:23.528428Z

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 b276bc33-f4c0-4da9-b305-1440c1c73e35 · inbound

Evaporating cosmologically coupled black holes cites this paper.

Evaporating cosmologically coupled black holes Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remanants of Little Red Dots

Reference 101

Resolution: unresolved; no resolver link, observed 2026-08-02T03:35:56.530119Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.