The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 | Paper Citation Record

Observation b49dab5c-38c7-4251-af5d-a4511d4aee57 · outbound

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The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 , keywords =

Reference 1

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Observation 29355c1b-521a-4643-92cc-2c27c36fec51 · outbound

This paper cites NuSTAR hard X-ray spectra of radio galaxies.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 NuSTAR hard X-ray spectra of radio galaxies

Reference 2

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Observation 5c0eb90e-8f3a-42cb-9e8f-1528b2272b67 · outbound

This paper cites The $L_\mathrm{x}$-$L_\mathrm{uv}$-$L_\mathrm{radio}$ relation and corona-disk-jet connection in optically selected radio-loud quasars.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 The $L_\mathrm{x}$-$L_\mathrm{uv}$-$L_\mathrm{radio}$ relation and corona-disk-jet connection in optically selected radio-loud quasars

Reference 3

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Observation 1d450b27-f5c8-4df1-907a-2e12b462d216 · outbound

This paper cites The composite X-ray spectrum of 3CRR Quasars.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 The composite X-ray spectrum of 3CRR Quasars

Reference 4

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Observation dec14a92-b6d2-4085-beac-fee6ef3ba8df · outbound

This paper cites Comparison of SEDs of very massive radio-loud and radio-quiet AGN.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Comparison of SEDs of very massive radio-loud and radio-quiet AGN

Reference 5

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Observation 25ef55e6-f8d4-49bb-953c-86b3288dff2f · outbound

This paper cites A nearby luminous AGN sample optically selected from Hubble Space Telescope (HST).

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 A nearby luminous AGN sample optically selected from Hubble Space Telescope (HST)

Reference 6

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Observation 1cc2a322-376f-469e-90d3-9890dafd6a82 · outbound

This paper cites Black Hole Fundamental Plane in Low-Excitation Radio Galaxies.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Black Hole Fundamental Plane in Low-Excitation Radio Galaxies

Reference 7

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Observation 4de32b5f-9286-4c7d-89c5-b253cb91adf6 · outbound

This paper cites Comparison of hard X-ray spectra of luminous radio galaxies and their radio-quiet counterparts.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Comparison of hard X-ray spectra of luminous radio galaxies and their radio-quiet counterparts

Reference 8

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Observation 5d01d684-da4a-4c9a-8bb7-ea78e792a212 · outbound

This paper cites A systematic study of the condensation of the corona and the application for $\Gamma_{\rm 2-10keV}-L_{\rm bol}/L_{\rm Edd}$ correlation in luminous active galactic nuclei.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 A systematic study of the condensation of the corona and the application for $\Gamma_{\rm 2-10keV}-L_{\rm bol}/L_{\rm Edd}$ correlation in luminous active galactic nuclei

Reference 9

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Observation 3f943b0f-46d8-467b-84e9-01e113d2d92b · outbound

This paper cites Quasars as standard candles I: The physical relation between disc and coronal emission.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Quasars as standard candles I: The physical relation between disc and coronal emission

Reference 10

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Observation 29e403bc-11b2-4636-97a9-977195faa0ab · outbound

This paper cites Revisiting the structure and spectrum of the magnetic-reconnection-heated corona in luminous AGNs.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Revisiting the structure and spectrum of the magnetic-reconnection-heated corona in luminous AGNs

Reference 11

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Observation aafaf478-09bd-482b-8a56-b27e8fe1cfda · outbound

This paper cites Research in Astronomy and Astrophysics , year = 2016, month = sep, volume =.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Research in Astronomy and Astrophysics , year = 2016, month = sep, volume =

Reference 12

Resolution: verified exact; doi, observed 2026-08-15T15:15:06.485881Z

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Observation 973c0684-db06-4c33-982a-68e4dec0a636 · outbound

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The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Accretion disc dynamo activity in local simulations spanning weak-to-strong net vertical magnetic flux regimes

Reference 13

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Observation 6153bd6a-f886-4d2c-b3ca-a5ca7364089a · outbound

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The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Revisit the fundamental plane of black-hole activity from sub-Eddington to quiescent state

Reference 14

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Observation 7c0c0980-2fa3-46c6-99aa-6992ee57a6ac · outbound

This paper cites Revisiting the relationship between 6 {\mu}m and 2-10 keV continuum luminosities of AGN.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Revisiting the relationship between 6 {\mu}m and 2-10 keV continuum luminosities of AGN

Reference 15

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Observation 7e020187-d721-464b-ad3f-3113adb398a2 · outbound

This paper cites Cosmic X-ray Surveys of Distant Active Galaxies: The Demographics, Physics, and Ecology of Growing Supermassive Black Holes.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Cosmic X-ray Surveys of Distant Active Galaxies: The Demographics, Physics, and Ecology of Growing Supermassive Black Holes

Reference 16

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Observation 032db204-3a89-4acf-b022-bb6a06623ac4 · outbound

This paper cites Hot Accretion Flows Around Black Holes.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Hot Accretion Flows Around Black Holes

Reference 17

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Observation 1776a8fa-e1af-457f-a921-7f5e0d89c58a · outbound

This paper cites On the role of initial and boundary conditions in numerical simulations of accretion flows.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 On the role of initial and boundary conditions in numerical simulations of accretion flows

Reference 18

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Observation 028c7bc2-11ef-43a1-8e9e-ca49a0a81536 · outbound

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The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Revealing the heavily obscured AGN population of High Redshift 3CRR Sources with Chandra X-ray Observations

Reference 19

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Observation 219e3eb6-a97a-481d-8d62-cde226830dae · outbound

This paper cites Local Study of Accretion Disks with a Strong Vertical Magnetic Field: Magnetorotational Instability and Disk Outflow.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Local Study of Accretion Disks with a Strong Vertical Magnetic Field: Magnetorotational Instability and Disk Outflow

Reference 20

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Observation b448e93c-09b8-4834-b9fd-70bec4a1478c · outbound

This paper cites The large scale magnetic fields of thin accretion disks.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 The large scale magnetic fields of thin accretion disks

Reference 21

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Observation 575efa63-b61f-46c4-84d7-082b36430957 · outbound

This paper cites An X-ray and Multiwavelength Survey of Highly Radio-Loud Quasars at z > 4: Jet-Linked Emission in the Brightest Radio Beacons of the Early Universe.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 An X-ray and Multiwavelength Survey of Highly Radio-Loud Quasars at z > 4: Jet-Linked Emission in the Brightest Radio Beacons of the Early Universe

Reference 22

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Observation 91b19ff3-f2f4-4ae3-ae9f-c6636aedfa20 · outbound

This paper cites The Swift BAT-detected Seyfert 1 Galaxies: X-ray Broadband Properties and Warm Absorbers.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 The Swift BAT-detected Seyfert 1 Galaxies: X-ray Broadband Properties and Warm Absorbers

Reference 26

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Observation 61ec3e50-fc2b-4d63-8e94-948c9ccfe353 · outbound

This paper cites The New Generation Atlas of Quasar Spectral Energy Distributions from Radio to X-rays.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 The New Generation Atlas of Quasar Spectral Energy Distributions from Radio to X-rays

Reference 27

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Observation 9d0c4531-dd7e-471b-b7aa-cb2ae9c257b9 · outbound

This paper cites The Suzaku view of 3C 382.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 The Suzaku view of 3C 382

Reference 28

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Observation 3d8c6690-4aa0-421e-900a-844bc8f05b3e · outbound

This paper cites Chandra Observations of 3C Radio Sources with z<0.3: Nuclei, Diffuse Emission, Jets and Hotspots.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Chandra Observations of 3C Radio Sources with z<0.3: Nuclei, Diffuse Emission, Jets and Hotspots

Reference 29

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Observation 01d46d84-52d9-4a26-a18e-e63fe9814ed4 · outbound

This paper cites The X-ray to optical-UV luminosity ratio of X-ray selected Type 1 AGN in XMM-COSMOS.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 The X-ray to optical-UV luminosity ratio of X-ray selected Type 1 AGN in XMM-COSMOS

Reference 30

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Observation 8a3f04bb-f0c2-410f-9574-83ee76595d6b · outbound

This paper cites An optical spectroscopic survey of the 3CR sample of radio galaxies with z<0.3. II. Spectroscopic classes and accretion modes in radio-loud AGN.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 An optical spectroscopic survey of the 3CR sample of radio galaxies with z<0.3. II. Spectroscopic classes and accretion modes in radio-loud AGN

Reference 31

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Observation 084e8321-292b-4487-ae87-bf6bd38d0880 · outbound

This paper cites The SDSS/XMM-Newton Quasar Survey: Correlation between X-ray spectral slope and Eddington ratio.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 The SDSS/XMM-Newton Quasar Survey: Correlation between X-ray spectral slope and Eddington ratio

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.695280Z

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Observation afab89f0-721f-423f-a778-783df405e241 · outbound

This paper cites 3C 33: another case of photoionized soft X-ray emission in radio galaxies.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 3C 33: another case of photoionized soft X-ray emission in radio galaxies

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.699755Z

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Observation 76534663-e521-4c5d-bcc8-fca0190c6030 · outbound

This paper cites Periodic subvarieties of semiabelian varieties and annihilators of irreducible representations.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Periodic subvarieties of semiabelian varieties and annihilators of irreducible representations

Reference 34

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Observation 5f43b020-28be-46d4-bebb-b9e8d63d1a9e · outbound

This paper cites Heavy absorption and soft X-ray emission lines in the XMM-Newton spectrum of the Type 2 radio-loud quasar 3C 234.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Heavy absorption and soft X-ray emission lines in the XMM-Newton spectrum of the Type 2 radio-loud quasar 3C 234

Reference 35

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Observation 8e9cf7e5-0f0a-4b57-8449-815642c9ab5e · outbound

This paper cites Deep Chandra and multicolor HST observations of the jets of 3C 371 and PKS 2201+044.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Deep Chandra and multicolor HST observations of the jets of 3C 371 and PKS 2201+044

Reference 36

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Observation e1078755-33a8-4e6f-8197-d4febd365455 · outbound

This paper cites Spitzer Observations of 3C Quasars and Radio Galaxies: Mid-Infrared Properties of Powerful Radio Sources.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Spitzer Observations of 3C Quasars and Radio Galaxies: Mid-Infrared Properties of Powerful Radio Sources

Reference 37

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Observation bd4bddde-e0bc-4562-9791-237f14978cb9 · outbound

This paper cites Spectral Energy Distributions and Multiwavelength Selection of Type 1 Quasars.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Spectral Energy Distributions and Multiwavelength Selection of Type 1 Quasars

Reference 39

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Observation 87b912f6-6b25-4ac4-bdc1-53034a35058a · outbound

This paper cites Spitzer Reveals Hidden Quasar Nuclei in Some Powerful FR II Radio Galaxies.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Spitzer Reveals Hidden Quasar Nuclei in Some Powerful FR II Radio Galaxies

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.731464Z

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Observation fb9ec3d6-d75a-4065-a85a-3306964e4e8a · outbound

This paper cites Chandra Observations of the Highest Redshift Quasars from the Sloan Digital Sky Survey.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Chandra Observations of the Highest Redshift Quasars from the Sloan Digital Sky Survey

Reference 42

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Observation eaed4d8a-ac4d-48ea-9f47-aea806a32ec5 · outbound

This paper cites Chandra and XMM-Newton Observations of a Sample of Low-Redshift FRI and FRII Radio-Galaxy Nuclei.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Chandra and XMM-Newton Observations of a Sample of Low-Redshift FRI and FRII Radio-Galaxy Nuclei

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.746837Z

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Observation dfaf22be-de8d-4e0b-86fd-aa84d5d0286c · outbound

This paper cites , keywords =.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 , keywords =

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.752353Z

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Observation aa150b41-fc8e-4632-a02e-a32899af92b6 · outbound

This paper cites , keywords =.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 , keywords =

Reference 45

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Observation f98cea04-b0f5-4c66-be8d-0ca7bc2a0ff2 · outbound

This paper cites Far Infrared Observations of Radio Quasars and FR II Radio Galaxies.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Far Infrared Observations of Radio Quasars and FR II Radio Galaxies

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.761295Z

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Observation 846d5944-f64c-4720-94c9-e3a4ebc35a81 · outbound

This paper cites A Scheme to Unify Low-Power Accreting Black Holes - Jet-Dominated Accretion Flows and the Radio/X-Ray Correlation.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 A Scheme to Unify Low-Power Accreting Black Holes - Jet-Dominated Accretion Flows and the Radio/X-Ray Correlation

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.765185Z

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Observation c002d239-0a23-4c5b-a042-7bad21f451ac · outbound

This paper cites , keywords =.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 , keywords =

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.768884Z

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Observation 232543a6-df2a-4c1a-bcb1-5d74c5f3dec5 · outbound

This paper cites , keywords =.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 , keywords =

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.772342Z

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This paper cites , keywords =.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 , keywords =

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.775823Z

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Observation 44bf90d0-f046-4c9c-9ef3-2f0321aa1fed · outbound

This paper cites an unresolved cited work.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Unresolved cited work

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.779215Z

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This paper cites , keywords =.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 , keywords =

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.782787Z

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Observation cd03af7c-1cff-47d1-b045-c1c76a7ffb5f · outbound

This paper cites an unresolved cited work.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Unresolved cited work

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.788077Z

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This paper cites , keywords =.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 , keywords =

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.801076Z

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Observation dd0fab80-099e-4237-aa2f-c47f4ed3e2de · outbound

This paper cites , keywords =.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 , keywords =

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.805365Z

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Observation 7adfceca-5fe0-4211-b720-60a2c2ba4d27 · outbound

This paper cites Global simulations of axisymmetric radiative black hole accretion disks in general relativity with a sub-grid magnetic dynamo.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Global simulations of axisymmetric radiative black hole accretion disks in general relativity with a sub-grid magnetic dynamo

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.813909Z

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Observation 865c5444-1522-4489-baa0-bc06be976b00 · outbound

This paper cites Relativistic Jets in Active Galactic Nuclei.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Relativistic Jets in Active Galactic Nuclei

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.818375Z

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Observation f37c836b-f3a4-4d19-91f2-09d28b0fed37 · outbound

This paper cites Black holes in binary systems.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Black holes in binary systems

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.822812Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e4d49d05-7fc5-4ee1-937c-7da0bb7d3bcf · outbound

This paper cites The large scale magnetic fields of advection dominated accretion flows.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 The large scale magnetic fields of advection dominated accretion flows

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.827572Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7bef27a4-9d22-4796-9dd5-c5a1e1803c9d · outbound

This paper cites Thermal stability of thin disk with magnetically driven winds.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Thermal stability of thin disk with magnetically driven winds

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.832630Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3b5ef982-f7d2-4c7b-916e-011e0f30db0c · outbound

This paper cites Magnetically Arrested Disk: An Energetically Efficient Accretion Flow.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Magnetically Arrested Disk: An Energetically Efficient Accretion Flow

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.837378Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4793ec22-9d77-494e-aec7-fc65fe1e468f · outbound

This paper cites Angular Momentum Transport in Thin Magnetically Arrested Disks.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Angular Momentum Transport in Thin Magnetically Arrested Disks

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.841768Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c9cd67f4-a2ad-4c6d-aa63-af624d78163b · outbound

This paper cites General Relativistic Radiation Magnetohydrodynamic Simulations of Thin Magnetically Arrested Disks.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 General Relativistic Radiation Magnetohydrodynamic Simulations of Thin Magnetically Arrested Disks

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.846190Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9dde1b83-35aa-45f2-b7b2-6c23579f7354 · outbound

This paper cites A Resolution Study of Magnetically Arrested Disks.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 A Resolution Study of Magnetically Arrested Disks

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.850620Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3368fadf-68ef-4260-bcda-6bfda255de15 · outbound

This paper cites The Rest-Frame Extreme Ultraviolet Spectral Properties of QSOs.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 The Rest-Frame Extreme Ultraviolet Spectral Properties of QSOs

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.855605Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7c369c6c-70fa-4323-9f47-034f688bc749 · outbound

This paper cites The Extreme Ultraviolet Deficit and Magnetically Arrested Accretion in Radio Loud Quasars.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 The Extreme Ultraviolet Deficit and Magnetically Arrested Accretion in Radio Loud Quasars

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.860502Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 561155eb-2aab-428b-bbc8-685ccc31e709 · outbound

This paper cites Evidence of the Dynamics of Relativistic Jet Launching in Quasars.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Evidence of the Dynamics of Relativistic Jet Launching in Quasars

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.864303Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 84ae539a-a8f7-484c-be4d-d067f5ece246 · outbound

This paper cites X-ray reverberation around accreting black holes.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 X-ray reverberation around accreting black holes

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.868583Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ac4e0f06-8ccb-4e93-a181-541f10574526 · outbound

This paper cites Radiative Properties of Magnetically-Arrested Disks.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Radiative Properties of Magnetically-Arrested Disks

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.872178Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b8716657-16da-493b-9832-7dbeacd27f70 · outbound

This paper cites HST-COS Observations of AGN. II. Extended Survey of Ultraviolet Composite Spectra from 159 Active Galactic Nuclei.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 HST-COS Observations of AGN. II. Extended Survey of Ultraviolet Composite Spectra from 159 Active Galactic Nuclei

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.876487Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 018d5a3b-6e02-4653-8a27-089cd47343dd · outbound

This paper cites A Hybrid Two Component Accretion Flow Surrounding Supermassive Black Holes in AGN.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 A Hybrid Two Component Accretion Flow Surrounding Supermassive Black Holes in AGN

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.881105Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 59c28c60-f188-45f2-a6bf-3fa1f93e2fad · outbound

This paper cites Magnetic flux captured by an accretion disk.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Magnetic flux captured by an accretion disk

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.885521Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 25eb3ce8-e072-4f1a-a88f-4254178d5dda · outbound

This paper cites , keywords =.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 , keywords =

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.889919Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3ce69239-b23b-4fb8-9cd0-d024c1337bd3 · outbound

This paper cites The black hole fundamental plane: revisit with a larger sample of radio and X-ray emitting broad-line AGNs.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 The black hole fundamental plane: revisit with a larger sample of radio and X-ray emitting broad-line AGNs

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.894351Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f5374b09-440c-435f-983d-35c160c464b3 · outbound

This paper cites Reverberation Measurements for 17 Quasars and the Size-Mass-Luminosity Relations in Active Galactic Nuclei.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Reverberation Measurements for 17 Quasars and the Size-Mass-Luminosity Relations in Active Galactic Nuclei

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.904256Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 338e8942-bd0c-4ee2-8847-26d1a62b5cc8 · outbound

This paper cites The Simultaneous Optical-to-X-ray Spectral Energy Distribution of Soft X-ray Selected AGN observed by Swift.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 The Simultaneous Optical-to-X-ray Spectral Energy Distribution of Soft X-ray Selected AGN observed by Swift

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.908812Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1332f6ec-7f6b-4f24-89a3-09051df61244 · outbound

This paper cites Star formation in z>1 3CR host galaxies as seen by Herschel.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Star formation in z>1 3CR host galaxies as seen by Herschel

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.913280Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 03a0ec8d-8498-4d5b-aa02-4277b2194181 · outbound

This paper cites Revista Mexicana de Astronomia y Astrofisica Conference Series , year = 2008, series =.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Revista Mexicana de Astronomia y Astrofisica Conference Series , year = 2008, series =

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.917677Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3199edd8-a43f-48ac-91e0-24b175bd6a11 · outbound

This paper cites , keywords =.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 , keywords =

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.922111Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f0aa30d9-b0dd-4433-805e-4629373c8db5 · outbound

This paper cites , keywords =.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 , keywords =

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.926189Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9cf3cbc0-dec0-427a-987e-d5a6fa896034 · outbound

This paper cites On the nature of optical nuclei in FR I radio-galaxies from ACS/HST imaging polarimetry.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 On the nature of optical nuclei in FR I radio-galaxies from ACS/HST imaging polarimetry

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.930171Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation df678e85-eb52-4b59-ba4f-763a4533a473 · outbound

This paper cites On the origin of X-ray emission in some FR Is: ADAF or jet?.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 On the origin of X-ray emission in some FR Is: ADAF or jet?

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.934024Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 235509b2-f11a-43a8-9c39-61e02b502c23 · outbound

This paper cites , keywords =.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 , keywords =

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.938506Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d3d813df-85a3-4d0c-8cf2-e070694b805f · outbound

This paper cites The Spitzer view of FR-I radio galaxies: on the origin of the nuclear mid-infrared continuum.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 The Spitzer view of FR-I radio galaxies: on the origin of the nuclear mid-infrared continuum

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.942534Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b29152d7-3135-4444-b04d-469b14322f79 · outbound

This paper cites The 1.6 micron near infrared nuclei of 3C radio galaxies: Jets, thermal emission or scattered light?.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 The 1.6 micron near infrared nuclei of 3C radio galaxies: Jets, thermal emission or scattered light?

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.947172Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6aff9895-ffeb-4853-8177-ddefd5d5356f · outbound

This paper cites Astronomical and Astrophysical Transactions , keywords =.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Astronomical and Astrophysical Transactions , keywords =

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.951784Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 432b02cb-93d6-4fce-8d6d-919c4036e2c2 · outbound

This paper cites , keywords =.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 , keywords =

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.956398Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9e317063-c3f5-4702-b827-5bea8f7449dd · outbound

This paper cites The Origin of the X-ray Emission in Two Well-Aligned Extragalactic Jets: The Case for IC/CMB.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 The Origin of the X-ray Emission in Two Well-Aligned Extragalactic Jets: The Case for IC/CMB

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.960693Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8cc5d4ef-83dd-4bd1-86b8-4bf4df22681b · outbound

This paper cites High-resolution x-ray telescopes.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 High-resolution x-ray telescopes

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.965324Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5236858c-701d-4c8d-b396-c60dbb113c02 · outbound

This paper cites A Composite HST Spectrum of Quasars.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 A Composite HST Spectrum of Quasars

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.969652Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 74df80f4-28fe-4ef5-adc8-43caf3597336 · outbound

This paper cites The origin of X-ray emission in 3CRR sources: hints from mid-infrared Spitzer observations.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 The origin of X-ray emission in 3CRR sources: hints from mid-infrared Spitzer observations

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.974295Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a8aacddc-830e-44e2-96e8-558f84f4aef0 · outbound

This paper cites BAT AGN Spectroscopic Survey -- XII. The relation between coronal properties of Active Galactic Nuclei and the Eddington ratio.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 BAT AGN Spectroscopic Survey -- XII. The relation between coronal properties of Active Galactic Nuclei and the Eddington ratio

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.978579Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0660eedc-cde9-48a2-bf25-c2138d86cf8f · outbound

This paper cites The composite X-ray spectra of radio-loud and radio-quiet SDSS quasars.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 The composite X-ray spectra of radio-loud and radio-quiet SDSS quasars

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.982760Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3c9fbd44-4757-4ffd-ac07-733fbce5c636 · outbound

This paper cites Interpreting the radio/X-ray correlation of black hole sources based on the accretion-jet model.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Interpreting the radio/X-ray correlation of black hole sources based on the accretion-jet model

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.987032Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 897fd7c0-5945-4ab5-bf67-5f39e01dbac3 · outbound

This paper cites Radio / X-ray correlation in the low/hard state of GX 339--4.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Radio / X-ray correlation in the low/hard state of GX 339--4

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.990689Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 89781600-d987-47da-bf79-e2e383dd71aa · outbound

This paper cites The Soft X-Ray Properties of a Complete Sample of Optically Selected Quasars II. Final Results.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 The Soft X-Ray Properties of a Complete Sample of Optically Selected Quasars II. Final Results

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.994541Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 07777f54-4553-4336-8b4a-ee7e5bf7f119 · outbound

This paper cites , keywords =.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 , keywords =

Reference 101

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:04.998176Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 046f827d-6cf7-4b73-b127-8d30f59f3e5b · outbound

This paper cites Going with the flow: can the base of jets subsume the role of compact accretion disk coronae?.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Going with the flow: can the base of jets subsume the role of compact accretion disk coronae?

Reference 102

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:05.001978Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 29a8b3e9-e4b7-4a3c-a1ca-4e8938865b5e · outbound

This paper cites The X-ray spectral and variability properties of typical radio-loud quasars.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 The X-ray spectral and variability properties of typical radio-loud quasars

Reference 103

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:05.006428Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 60beda4d-d8a9-4f18-ac1c-58068bf522b6 · outbound

This paper cites an unresolved cited work.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Unresolved cited work

Reference 104

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:05.010700Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6febb46c-fbff-44d3-ac7a-4d97107f624f · outbound

This paper cites Flux eruption events drive angular momentum transport in magnetically arrested accretion flows.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Flux eruption events drive angular momentum transport in magnetically arrested accretion flows

Reference 105

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:05.015008Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ad2b69d7-c2d9-4c46-9c8b-c6d62467752d · outbound

This paper cites The Accretion flow in M87 is really MAD.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 The Accretion flow in M87 is really MAD

Reference 106

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:05.020350Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation da238e52-0f6d-4e0c-99e0-50e8c7e0956f · outbound

This paper cites Magnetic support, wind-driven accretion, coronal heating, and fast outflows in a thin magnetically arrested disc.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Magnetic support, wind-driven accretion, coronal heating, and fast outflows in a thin magnetically arrested disc

Reference 107

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:05.024749Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0693796e-490a-4869-ae5f-b22ef82c6d6f · outbound

This paper cites , year = 2014, month = jun, volume =.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 , year = 2014, month = jun, volume =

Reference 108

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:05.029187Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 14514186-df28-4144-bc34-bd9baa60aaab · outbound

This paper cites The power of relativistic jets is larger than the luminosity of their accretion disks.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 The power of relativistic jets is larger than the luminosity of their accretion disks

Reference 109

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:05.033573Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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