Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region | Paper Citation Record

Observation e73e2e4b-e003-426c-956a-37a920a3d921 · outbound

This paper cites The LOFAR-eFEDS survey: The incidence of radio and X-ray AGN and the disk-jet connection.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The LOFAR-eFEDS survey: The incidence of radio and X-ray AGN and the disk-jet connection

Reference 1

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Observation e346d4dd-e519-4b23-8f50-313572e6e67a · outbound

This paper cites The LOFAR Two-metre Sky Survey (LoTSS) III. First Data Release: optical/IR identifications and value-added catalogue.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The LOFAR Two-metre Sky Survey (LoTSS) III. First Data Release: optical/IR identifications and value-added catalogue

Reference 2

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Observation 9757293a-afe8-43a6-b678-69c376cd1c1c · outbound

This paper cites , keywords =.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region , keywords =

Reference 3

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Observation afeedbcb-cdec-4088-aea1-2dfe3a072718 · outbound

This paper cites The LOFAR Two-Metre Sky Survey (LoTSS): VI. Optical identifications for the second data release.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The LOFAR Two-Metre Sky Survey (LoTSS): VI. Optical identifications for the second data release

Reference 4

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Observation dcabe4ad-d188-4d15-9c3d-76c087fd71e5 · outbound

This paper cites Research in Astronomy and Astrophysics , keywords =.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Research in Astronomy and Astrophysics , keywords =

Reference 5

Resolution: verified exact; doi, observed 2026-08-01T00:16:17.894605Z

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Observation 10966a54-cb92-476e-a478-baa70f423de9 · outbound

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

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Periodic subvarieties of semiabelian varieties and annihilators of irreducible representations

Reference 6

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Observation 0e5a38fb-e2ed-4f1d-b1d3-55b29bbe5694 · outbound

This paper cites The Astrophysical Journal , keywords =.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The Astrophysical Journal , keywords =

Reference 7

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Observation a386b8d2-33c8-4a5e-8b49-3f38fff44f7d · outbound

This paper cites Monthly Notices of the Royal Astronomical Society , keywords =.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Monthly Notices of the Royal Astronomical Society , keywords =

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:47.293642Z

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Observation 98ed9e64-11eb-48e9-95b7-da17b191f759 · outbound

This paper cites The Co-Evolution of Galaxies and Supermassive Black Holes: Insights from Surveys of the Contemporary Universe.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The Co-Evolution of Galaxies and Supermassive Black Holes: Insights from Surveys of the Contemporary Universe

Reference 9

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Observation f1589a39-cd7b-4664-baf3-16bf86bc1433 · outbound

This paper cites Quasar feedback and the origin of radio emission in radio-quiet quasars.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Quasar feedback and the origin of radio emission in radio-quiet quasars

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:47.538196Z

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Observation 5b2198cf-dd15-452a-8329-90303498fc79 · outbound

This paper cites Outflow-related radio emission in radio-quiet quasars.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Outflow-related radio emission in radio-quiet quasars

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:47.664597Z

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Observation 551537b8-f1ea-4ae5-af65-b80b0213e56a · outbound

This paper cites A universal average spectral energy distribution for quasars from optical to extreme ultraviolet.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region A universal average spectral energy distribution for quasars from optical to extreme ultraviolet

Reference 12

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Observation f697b110-96b2-43c1-b72d-28c667ebfa65 · outbound

This paper cites Annual Review of Astronomy and Astrophysics , keywords =.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Annual Review of Astronomy and Astrophysics , keywords =

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:47.787483Z

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Observation d185db91-3d87-47ae-a5a2-74b2dc7b524e · outbound

This paper cites The fundamental plane of black hole activity for low-luminosity radio active galactic nuclei across 1 < z < 4.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The fundamental plane of black hole activity for low-luminosity radio active galactic nuclei across 1 < z < 4

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:47.910205Z

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Observation 12d25ce3-f580-4f22-a147-6d55339d7cb8 · outbound

This paper cites Relation between winds and jets in radio-loud AGN.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Relation between winds and jets in radio-loud AGN

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:47.991077Z

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Observation 16b160a8-377c-4ae9-8897-d958103cdf1e · outbound

This paper cites an unresolved cited work.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Unresolved cited work

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:48.093181Z

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Observation 76bcad9d-bb6f-4f6f-9d03-c0bdbde89d0f · outbound

This paper cites an unresolved cited work.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Unresolved cited work

Reference 17

Resolution: verified exact; arxiv_id, observed 2026-08-01T00:16:17.814103Z

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Observation 670dc0be-5748-42d1-a2b3-d08ec4e65aad · outbound

This paper cites The X-ray and Radio Connection in Low-luminosity Active Nuclei.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The X-ray and Radio Connection in Low-luminosity Active Nuclei

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:48.330194Z

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Observation 0dcbc734-526b-45f7-9bed-bc893cb3c1fc · outbound

This paper cites On the Relationship Between Radio Emission and Black Hole Mass in Galactic Nuclei.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region On the Relationship Between Radio Emission and Black Hole Mass in Galactic Nuclei

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:48.433635Z

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Observation 0c5c9fe4-7b58-46ae-9ef0-c8866f711b4f · outbound

This paper cites Astronomische Nachrichten , keywords =.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Astronomische Nachrichten , keywords =

Reference 20

Resolution: verified exact; doi, observed 2026-08-01T00:16:17.754078Z

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Observation 31d99ca1-908e-40ca-8e0c-74cd282adfd9 · outbound

This paper cites Ionised gas outflows over the radio AGN life cycle.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Ionised gas outflows over the radio AGN life cycle

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:48.576731Z

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Observation c045dffb-9504-4a18-ae8e-ec5c236ebe9d · outbound

This paper cites The Origin of Radio Emission from Radio-Quiet AGN.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The Origin of Radio Emission from Radio-Quiet AGN

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:48.640590Z

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Observation f3eb07a4-e9ca-42a5-8c4d-db8ab1ea6e33 · outbound

This paper cites Relativistic Jets in Active Galactic Nuclei.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Relativistic Jets in Active Galactic Nuclei

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:48.686498Z

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Observation 3c54b2f8-0113-4d3f-986a-7eb91fe180b9 · outbound

This paper cites Quasars and Cosmology , year = 1999, editor =.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Quasars and Cosmology , year = 1999, editor =

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:48.765163Z

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Observation 71aed5d0-5d50-4283-8127-6e40b5420512 · outbound

This paper cites The Astrophysical Journal , keywords =.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The Astrophysical Journal , keywords =

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:48.964697Z

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Observation 3e31633f-c871-4ec7-a693-b311737e15b8 · outbound

This paper cites The Astrophysical Journal , keywords =.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The Astrophysical Journal , keywords =

Reference 27

Resolution: verified exact; doi, observed 2026-08-01T00:16:17.642630Z

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Observation 09ea5453-6ed5-4197-b6fc-bde1577bc243 · outbound

This paper cites Monthly Notices of the Royal Astronomical Society , keywords =.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Monthly Notices of the Royal Astronomical Society , keywords =

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:49.158504Z

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Observation f891c9b3-5bae-475e-bc0a-a24cbd57a06e · outbound

This paper cites A Relation Between Supermassive Black Hole Mass and Quasar Metallicity?.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region A Relation Between Supermassive Black Hole Mass and Quasar Metallicity?

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:49.235563Z

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Observation f6924051-e7c4-4119-8f42-439806e47efc · outbound

This paper cites Average UV Quasar Spectra in the Context of Eigenvector 1: A Baldwin Effect Governed by Eddington Ratio?.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Average UV Quasar Spectra in the Context of Eigenvector 1: A Baldwin Effect Governed by Eddington Ratio?

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:49.338957Z

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Observation cf33833c-3a3d-47fd-894b-d7c1546597d7 · outbound

This paper cites Eddington ratio governs the equivalent width of MgII emission line in active galactic nuclei.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Eddington ratio governs the equivalent width of MgII emission line in active galactic nuclei

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:49.501847Z

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Observation 6b954df2-d68b-4ccb-be05-0b074a634c33 · outbound

This paper cites An extensive study of blazar broad emission line: Changing-look blazars and Baldwin effect.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region An extensive study of blazar broad emission line: Changing-look blazars and Baldwin effect

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:49.584684Z

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Observation eefbdbc7-e817-47c0-b309-5ec676313543 · outbound

This paper cites Emission Line-Ultraviolet to X-Ray Continuum Correlations: Constraints on the Anisotropy of the Ionizing Continuum in Active Galactic Nuclei.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Emission Line-Ultraviolet to X-Ray Continuum Correlations: Constraints on the Anisotropy of the Ionizing Continuum in Active Galactic Nuclei

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:49.631627Z

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Observation b84abd73-de17-4f52-b3da-0261cddcf322 · outbound

This paper cites The Astrophysical Journal , keywords =.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The Astrophysical Journal , keywords =

Reference 34

Resolution: verified exact; doi, observed 2026-08-01T00:16:17.566437Z

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No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation c9c3e2a0-defc-47b0-b328-5c80a21b3b35 · outbound

This paper cites Quasars as Cosmological Probes: The Ionizing Continuum, Gas Metallicity and the EW-L Relation.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Quasars as Cosmological Probes: The Ionizing Continuum, Gas Metallicity and the EW-L Relation

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:49.736370Z

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Observation 4a14f7f1-889a-4739-abe5-1a94c691f4a7 · outbound

This paper cites A Composite Extreme Ultraviolet QSO Spectrum from the Far Ultraviolet Spectroscopic Explorer.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region A Composite Extreme Ultraviolet QSO Spectrum from the Far Ultraviolet Spectroscopic Explorer

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:49.803658Z

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Observation de72d1d7-6952-4bfa-be47-5ad9a3efcc0b · outbound

This paper cites The intrinsic Baldwin effect in broad Balmer lines of six long-term monitored AGNs.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The intrinsic Baldwin effect in broad Balmer lines of six long-term monitored AGNs

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:49.934595Z

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Observation 371516e1-81c9-45fa-a8f0-0a9e4d6bdc6d · outbound

This paper cites The Astronomical Journal , keywords =.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The Astronomical Journal , keywords =

Reference 39

Resolution: verified exact; doi, observed 2026-08-01T00:16:17.512998Z

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No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 5b79e875-b40a-4534-b107-08233280c8b0 · outbound

This paper cites The Astrophysical Journal , keywords =.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The Astrophysical Journal , keywords =

Reference 40

Resolution: verified exact; doi, observed 2026-08-01T00:16:17.371694Z

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No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation fe7d8aad-a537-4085-a8d4-b2013ae5660a · outbound

This paper cites The Baldwin effect in the narrow emission lines of AGNs.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The Baldwin effect in the narrow emission lines of AGNs

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:50.157783Z

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Observation 6e28f9c5-db7c-4379-ba93-dae27dd52c53 · outbound

This paper cites The Correlation of Narrow Line Emission and X-ray Luminosity in Active Galactic Nuclei.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The Correlation of Narrow Line Emission and X-ray Luminosity in Active Galactic Nuclei

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:50.216286Z

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Observation a9e449f4-e839-42e2-9922-5328a2212a28 · outbound

This paper cites Narrow Iron K$\alpha$ Lines in Active Galactic Nuclei: Evolving Populations?.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Narrow Iron K$\alpha$ Lines in Active Galactic Nuclei: Evolving Populations?

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:50.274524Z

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Observation 31665d18-0c5e-435b-a6de-69f35b20b4ee · outbound

This paper cites Active Galactic Nuclei Emission-Line Properties Versus Eddington Ratio.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Active Galactic Nuclei Emission-Line Properties Versus Eddington Ratio

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:50.343586Z

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Observation e2c3f181-060f-46ff-8fc2-be33cbcb149b · outbound

This paper cites Monthly Notices of the Royal Astronomical Society , keywords =.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Monthly Notices of the Royal Astronomical Society , keywords =

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:50.508680Z

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Observation 2d89e7c5-3439-483c-bddd-5a5d940cd9cc · outbound

This paper cites Monthly Notices of the Royal Astronomical Society , keywords =.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Monthly Notices of the Royal Astronomical Society , keywords =

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:50.580774Z

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Observation f6763567-5607-44f5-ae1b-206e327d46b0 · outbound

This paper cites On the dependence of the iron K-line profiles with luminosity in Active Galactic Nuclei.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region On the dependence of the iron K-line profiles with luminosity in Active Galactic Nuclei

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:50.661129Z

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Observation 2606d735-15f7-4518-837f-b43e8410e360 · outbound

This paper cites The Relationship Between the High Energy Continuum and Emission Lines in QSOs: A Low-Redshift Sample.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The Relationship Between the High Energy Continuum and Emission Lines in QSOs: A Low-Redshift Sample

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:50.692647Z

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Observation dcb499b4-b91a-4a83-a1c4-ac2e690ff58f · outbound

This paper cites The Astrophysical Journal Supplement Series , keywords =.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The Astrophysical Journal Supplement Series , keywords =

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:50.755157Z

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Observation 5ac6c3c6-9d7a-4417-8005-b143cbdaec41 · outbound

This paper cites Monthly Notices of the Royal Astronomical Society , keywords =.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Monthly Notices of the Royal Astronomical Society , keywords =

Reference 51

Resolution: verified exact; doi, observed 2026-08-01T00:16:17.273259Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation e6d0e112-47de-4ef3-ac67-2fd6ba852659 · outbound

This paper cites The Astrophysical Journal Letters , keywords =.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The Astrophysical Journal Letters , keywords =

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:50.887682Z

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Observation 63da93df-5ca1-4bb1-89db-376a60d1a433 · outbound

This paper cites III - Line and continuum correlations.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region III - Line and continuum correlations

Reference 53

Resolution: verified exact; doi, observed 2026-08-01T00:16:17.194930Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 3a81d29c-4df2-427b-a802-aded764cc63c · outbound

This paper cites The Astrophysical Journal Supplement Series , keywords =.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The Astrophysical Journal Supplement Series , keywords =

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:51.012308Z

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Observation 524d31d5-5e6d-4252-9774-8a9b12c21730 · outbound

This paper cites The Astrophysical Journal , keywords =.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The Astrophysical Journal , keywords =

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:51.083682Z

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Observation 0f398138-8456-47f4-a420-1011f9c70761 · outbound

This paper cites The Astrophysical Journal , keywords =.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The Astrophysical Journal , keywords =

Reference 56

Resolution: verified exact; doi, observed 2026-08-01T00:16:16.973169Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 6d73a374-1f89-4eb1-9bbc-0250e0b6909c · outbound

This paper cites Emission-Line versus Continuum Correlations in Active Galactic Nuclei.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Emission-Line versus Continuum Correlations in Active Galactic Nuclei

Reference 57

Resolution: verified exact; local_arxiv, observed 2026-08-01T00:16:16.825720Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 7909a3b9-3a47-42e3-adab-4fe59a7c6d5f · outbound

This paper cites Continuum and Emission Line Strength Relations for a large Active Galactic Nuclei Sample.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Continuum and Emission Line Strength Relations for a large Active Galactic Nuclei Sample

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:51.354661Z

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Observation 289f5182-f9b5-480e-aa74-46dd9d678aed · outbound

This paper cites The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package

Reference 59

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This paper cites The Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:51.538864Z

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This paper cites Astropy: A Community Python Package for Astronomy.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Astropy: A Community Python Package for Astronomy

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:51.626414Z

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This paper cites Monthly Notices of the Royal Astronomical Society , year = 1978, month = nov, volume =.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Monthly Notices of the Royal Astronomical Society , year = 1978, month = nov, volume =

Reference 62

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This paper cites The Astrophysical Journal , year = 1977, month = jun, volume =.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The Astrophysical Journal , year = 1977, month = jun, volume =

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:51.815581Z

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Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region 2023 , month =

Reference 64

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This paper cites Frontiers in Astronomy and Space Sciences , keywords =.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Frontiers in Astronomy and Space Sciences , keywords =

Reference 65

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Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Radio-Loudness of Active Galactic Nuclei: Observational Facts and Theoretical Implications

Reference 66

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Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Disclosing the Radio Loudness Distribution Dichotomy in Quasars: An Unbiased Monte Carlo Approach Applied to the SDSS-FIRST Quasar Sample

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:52.083406Z

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Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The Astronomical Journal , keywords =

Reference 68

Resolution: verified exact; doi, observed 2026-08-01T00:16:16.396300Z

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Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Unresolved cited work

Reference 69

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Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Unresolved cited work

Reference 70

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Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Unresolved cited work

Reference 71

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This paper cites 2022 , month =.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region 2022 , month =

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:52.408890Z

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Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The Astrophysical Journal Supplement Series , year=

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:52.478559Z

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This paper cites The Baryon Oscillation Spectroscopic Survey of SDSS-III.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The Baryon Oscillation Spectroscopic Survey of SDSS-III

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:52.549828Z

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Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Overview and Early Data

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:52.649717Z

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This paper cites The Multi-Object, Fiber-Fed Spectrographs for SDSS and the Baryon Oscillation Spectroscopic Survey.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The Multi-Object, Fiber-Fed Spectrographs for SDSS and the Baryon Oscillation Spectroscopic Survey

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:52.725754Z

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Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The Seventh Data Release of the Sloan Digital Sky Survey

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:52.896730Z

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Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The 2025 Release of Cloudy

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:53.041671Z

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This paper cites Broad-band SED properties.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Broad-band SED properties

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:53.221086Z

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This paper cites The Astrophysical Journal , keywords =.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The Astrophysical Journal , keywords =

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:53.399034Z

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This paper cites Locally Optimally Emitting Clouds and the Origin of Quasar Emission Lines.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Locally Optimally Emitting Clouds and the Origin of Quasar Emission Lines

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:53.505858Z

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This paper cites Monthly Notices of the Royal Astronomical Society , volume =.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Monthly Notices of the Royal Astronomical Society , volume =

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:53.643825Z

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This paper cites Annual Review of Astronomy and Astrophysics , year =.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region Annual Review of Astronomy and Astrophysics , year =

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:53.843117Z

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Observation 3e87d4f9-5d57-4e0a-9e72-e6805e475ee1 · outbound

This paper cites and Siegmund, Walter A.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region and Siegmund, Walter A

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-01T00:11:53.971923Z

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