ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs | Paper Citation Record

Observation 82d15d9e-93df-4b3b-b5b6-ab2570167642 · outbound

This paper cites Little Red Dot $-$ Host Galaxy $=$ Black Hole Star: A Gas-Enshrouded Heart at the Center of Every Little Red Dot.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Little Red Dot $-$ Host Galaxy $=$ Black Hole Star: A Gas-Enshrouded Heart at the Center of Every Little Red Dot

Reference 1

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Observation 1db52bb9-dbfc-49e1-b572-f43caddcb4e1 · outbound

This paper cites arXiv e-prints , keywords =.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs arXiv e-prints , keywords =

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:23.368534Z

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Observation 16b6c9b1-e08c-4200-962f-060b4d94430d · outbound

This paper cites A comprehensive and uniform sample of broad-line active galactic nuclei from the SDSS DR7.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs A comprehensive and uniform sample of broad-line active galactic nuclei from the SDSS DR7

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:23.553852Z

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Observation ea8ada2f-fd89-46ed-a59d-d5d0ef907b94 · outbound

This paper cites Discovery of strong Balmer line absorption in two luminous LoBAL quasars at z~1.5.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Discovery of strong Balmer line absorption in two luminous LoBAL quasars at z~1.5

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:23.785820Z

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Observation 7d30e343-2201-4245-bb38-11f0cf9c8f91 · outbound

This paper cites Discovery of Balmer Broad Absorption Lines in the Quasar LBQS 1206+1052.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Discovery of Balmer Broad Absorption Lines in the Quasar LBQS 1206+1052

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:23.943508Z

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Observation aa3389b3-b48b-4f10-9be9-e5ab174154c7 · outbound

This paper cites A Balmer-line Broad Absorption Line Quasar.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs A Balmer-line Broad Absorption Line Quasar

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:24.057466Z

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Observation 23bde1d9-d0b0-4662-a74f-dddbde8eb216 · outbound

This paper cites Discovery of H alpha absorption in the unusual broad absorption line quasar SDSS J083942.11+380526.3.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Discovery of H alpha absorption in the unusual broad absorption line quasar SDSS J083942.11+380526.3

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:24.208645Z

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Observation 30038c2e-b794-4cdc-a456-33bdf45a51f0 · outbound

This paper cites ABCD: The Nuclear Structure of the Little Red Dots Revealted through Absorption, Break, Continuum, and Decrement.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs ABCD: The Nuclear Structure of the Little Red Dots Revealted through Absorption, Break, Continuum, and Decrement

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:24.389931Z

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Observation adb85a01-60ef-484e-9e77-5743ba267e95 · outbound

This paper cites The case for super-Eddington accretion in JWST broad-line AGN during the first billion years.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs The case for super-Eddington accretion in JWST broad-line AGN during the first billion years

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:24.558059Z

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Observation 45671e26-af7f-438a-b539-d5290e25425f · outbound

This paper cites , keywords =.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs , keywords =

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:24.728222Z

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Observation 32b74a4a-0d99-4b91-a74d-99ad1514c610 · outbound

This paper cites Little Red Dots at an Inflection Point: Ubiquitous "V-Shaped" Turnover Consistently Occurs at the Balmer Limit.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Little Red Dots at an Inflection Point: Ubiquitous "V-Shaped" Turnover Consistently Occurs at the Balmer Limit

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:24.903096Z

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Observation a5a71b5c-eb18-4e66-8121-0bbd8dee9a07 · outbound

This paper cites , keywords =.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs , keywords =

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:24.991722Z

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Observation 2cd8fdf2-58e5-4aec-99b4-b78d59a0fc59 · outbound

This paper cites A Comprehensive Photometric Selection of `Little Red Dots' in MIRI Fields: An IR-Bright LRD at $z=3.1386$ with Warm Dust Emission.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs A Comprehensive Photometric Selection of `Little Red Dots' in MIRI Fields: An IR-Bright LRD at $z=3.1386$ with Warm Dust Emission

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:25.105909Z

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Observation e94fd796-8658-4f1c-b078-22e77d309828 · outbound

This paper cites An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:25.223604Z

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Observation 6314793f-a463-40fe-b305-bb8cf7bd1da9 · outbound

This paper cites , keywords =.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs , keywords =

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:25.384536Z

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Observation 86eaf3a1-6a31-4bb1-b2af-dfd9ace033b0 · outbound

This paper cites arXiv e-prints , keywords =.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs arXiv e-prints , keywords =

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:25.559268Z

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Observation 33aca6c0-3073-417a-b9a8-4e81ebab2c2e · outbound

This paper cites A Scaling Relation of LRDs between Broad H$\alpha$ and Bolometric Luminosities: Enhanced Broad H$\alpha$ Emission Relative to Low-$z$ Type 1 AGN.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs A Scaling Relation of LRDs between Broad H$\alpha$ and Bolometric Luminosities: Enhanced Broad H$\alpha$ Emission Relative to Low-$z$ Type 1 AGN

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:25.799798Z

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Observation 56ff119d-1262-4b8c-b9c2-93fc2bbc6e32 · outbound

This paper cites OCEANS of Absorption: High-resolution NIRSpec Spectroscopy Reveals Diverse Balmer-line Absorption in Little Red Dots.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs OCEANS of Absorption: High-resolution NIRSpec Spectroscopy Reveals Diverse Balmer-line Absorption in Little Red Dots

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:26.029473Z

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Observation b83090d8-605c-4e7a-87c1-838258d0eb33 · outbound

This paper cites The Extreme Rarity and Physical Properties of Low-redshift AGNs with Balmer Absorption.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs The Extreme Rarity and Physical Properties of Low-redshift AGNs with Balmer Absorption

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:26.111640Z

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Observation 7cac8f60-d0b1-40e6-9ae4-a73afc259cd7 · outbound

This paper cites , keywords =.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs , keywords =

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:26.203817Z

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Observation 2c750dd9-e4e9-4354-87bc-b92d6899cc6b · outbound

This paper cites Comparing Single-Epoch Virial Black Hole Mass Estimators for Luminous Quasars.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Comparing Single-Epoch Virial Black Hole Mass Estimators for Luminous Quasars

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:26.279262Z

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Observation f2b3e2cb-8f0d-49fc-8e19-2ae30f098bb2 · outbound

This paper cites The Low-Luminosity End of the Radius-Luminosity Relationship for Active Galactic Nuclei.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs The Low-Luminosity End of the Radius-Luminosity Relationship for Active Galactic Nuclei

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:26.333838Z

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Observation fc0afb3f-3caf-44c5-a3de-cda8f5f5e77e · outbound

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

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Reverberation Measurements for 17 Quasars and the Size-Mass-Luminosity Relations in Active Galactic Nuclei

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:26.420176Z

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Observation f65cc2dc-8c72-4b60-b5ce-4aece5779611 · outbound

This paper cites Central Masses and Broad-Line Region Sizes of Active Galactic Nuclei. II. A Homogeneous Analysis of a Large Reverberation-Mapping Database.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Central Masses and Broad-Line Region Sizes of Active Galactic Nuclei. II. A Homogeneous Analysis of a Large Reverberation-Mapping Database

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:26.604312Z

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Observation e2bb1bbd-c49e-4aef-a7ad-42d6d56cb073 · outbound

This paper cites an unresolved cited work.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Unresolved cited work

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:26.805251Z

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Observation 3d38c23a-7086-4dec-b6c4-903c3584e114 · outbound

This paper cites , keywords =.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs , keywords =

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:26.952400Z

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Observation 127b6e9f-84a4-4c90-ac63-2cd9fabc2296 · outbound

This paper cites Reports on Progress in Physics , year = 1991, month = apr, volume =.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Reports on Progress in Physics , year = 1991, month = apr, volume =

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:27.140549Z

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Observation 03ca3217-fc28-4c43-943a-3f99142f86f9 · outbound

This paper cites , keywords =.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs , keywords =

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:27.275900Z

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Observation f237ece4-dd8f-4ebd-9b8b-5a3d71ceddb4 · outbound

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

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Chandra Rules Out Super-Eddington Accretion Models For Little Red Dots

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:27.407459Z

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Observation 360f546d-734c-4d00-9eeb-13a72079e9b8 · outbound

This paper cites arXiv e-prints , keywords =.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs arXiv e-prints , keywords =

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:27.541314Z

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Observation d4d03c9e-8808-41af-a995-0f21c394b142 · outbound

This paper cites The Way We Tally Becomes the Tale: the Impact of Selection Strategies on the Inferred Evolution of Little Red Dots Across Cosmic Time.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs The Way We Tally Becomes the Tale: the Impact of Selection Strategies on the Inferred Evolution of Little Red Dots Across Cosmic Time

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:27.679092Z

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Observation e6c67275-e01c-4757-8571-f277c76bef16 · outbound

This paper cites Physics of Active Galactic Nuclei at all Scales , year = 2006, editor =.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Physics of Active Galactic Nuclei at all Scales , year = 2006, editor =

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:27.764374Z

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Observation 51dfad10-6bdc-45cf-937e-64fbb8b71320 · outbound

This paper cites How I Wonder What You Are -- JWST's Little Red Dots do not TWINKLE.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs How I Wonder What You Are -- JWST's Little Red Dots do not TWINKLE

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:27.838242Z

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Observation b5eaada4-7eca-4552-a4e9-103d4ffc5a4d · outbound

This paper cites Do Little Red Dots Vary?.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Do Little Red Dots Vary?

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:27.895354Z

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Observation f5872165-9156-4c22-bf1a-8700382ea011 · outbound

This paper cites Reviews of Modern Physics , year = 1979, month = oct, volume =.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Reviews of Modern Physics , year = 1979, month = oct, volume =

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:27.986548Z

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Observation d396e88e-aa15-4e59-8e2c-acdf49201a6c · outbound

This paper cites An Atlas of Computed Equivalent Widths of Quasar Broad Emission Lines.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs An Atlas of Computed Equivalent Widths of Quasar Broad Emission Lines

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:28.051465Z

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Observation 771850b4-8013-431b-872c-f1a324adae4a · outbound

This paper cites Paschen Jumps in Little Red Dots: Evidence for Nebular Continua.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Paschen Jumps in Little Red Dots: Evidence for Nebular Continua

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:28.119607Z

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Observation 32a3cfe1-035d-4d54-895d-959678a930c5 · outbound

This paper cites arXiv e-prints , keywords =.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs arXiv e-prints , keywords =

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:28.197753Z

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Observation 88b32673-b87a-42f8-9d65-ee8c265923d5 · outbound

This paper cites , keywords =.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs , keywords =

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:28.297720Z

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Observation 17b92361-6569-47fe-a5f8-6b71303024a9 · outbound

This paper cites , keywords =.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs , keywords =

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:28.367339Z

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Observation b79dd106-b770-4640-9ad8-f4d8d8723fad · outbound

This paper cites The Structure and Evolution of LRDs: Insights from JWST NIRSpec Medium and High Resolution Spectroscopy at $z\sim4$.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs The Structure and Evolution of LRDs: Insights from JWST NIRSpec Medium and High Resolution Spectroscopy at $z\sim4$

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:28.444891Z

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Observation 6b9e8955-3b0c-4375-a256-0da6ea717d2e · outbound

This paper cites arXiv e-prints , keywords =.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs arXiv e-prints , keywords =

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:28.541303Z

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Observation d90b03d0-57d5-4d68-a70a-f9af620bf022 · outbound

This paper cites , keywords =.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs , keywords =

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:28.644309Z

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Observation a2b406ee-2caf-431b-a0fd-0e8068ebfe76 · outbound

This paper cites An Atlas of Color-selected Quiescent Galaxies at $z>3$ in Public $JWST$ Fields.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs An Atlas of Color-selected Quiescent Galaxies at $z>3$ in Public $JWST$ Fields

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:28.721252Z

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Observation 71fe8afe-b332-4260-87a8-7fc7ea09b9ac · outbound

This paper cites The UNCOVER Survey: A first-look HST+JWST catalog of 60,000 galaxies near Abell 2744 and beyond.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs The UNCOVER Survey: A first-look HST+JWST catalog of 60,000 galaxies near Abell 2744 and beyond

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:28.789638Z

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Observation 25cc8b64-c8ac-4774-991f-142080a100ba · outbound

This paper cites Medium Bands, Mega Science: a JWST/NIRCam Medium-Band Imaging Survey of Abell 2744.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Medium Bands, Mega Science: a JWST/NIRCam Medium-Band Imaging Survey of Abell 2744

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:28.860140Z

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Observation f8f85714-d31a-48bd-894f-7ecd55f2cb51 · outbound

This paper cites The UNCOVER Survey: First Release of Ultradeep JWST/NIRSpec PRISM spectra for ~700 galaxies from z~0.3-13 in Abell 2744.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs The UNCOVER Survey: First Release of Ultradeep JWST/NIRSpec PRISM spectra for ~700 galaxies from z~0.3-13 in Abell 2744

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:28.925201Z

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Observation 7f74ee36-0921-4d65-90bb-82e8b95d76e6 · outbound

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

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:29.002598Z

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Observation a03568ab-1c96-4e44-960b-0278760ffc4b · outbound

This paper cites , keywords =.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs , keywords =

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:29.089795Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0ae333f6-8e18-4a9f-9a13-78848def521e · outbound

This paper cites A Massive Protocluster Anchored by a Luminous Quasar at $z=6.63$.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs A Massive Protocluster Anchored by a Luminous Quasar at $z=6.63$

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:29.261932Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation de89aaad-0e01-4daa-8b00-b45a2ba79a01 · outbound

This paper cites A Catalog of Quasar Properties from Sloan Digital Sky Survey Data Release 16.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs A Catalog of Quasar Properties from Sloan Digital Sky Survey Data Release 16

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:29.427863Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation abeb0a2d-97a8-43f7-9e5b-94a82cbba052 · outbound

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

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs (LRDs)$^2$: The Low-ReDshift Little Red Dots Survey. II. DESI DR1 Sample

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:29.593871Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e70f880f-5077-43ce-b329-708cf9e3caeb · outbound

This paper cites A new sample of Little Red Dots at $z<0.45$ in DESI DR1: Broad Balmer lines, low ionization spectrum and no variability.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs A new sample of Little Red Dots at $z<0.45$ in DESI DR1: Broad Balmer lines, low ionization spectrum and no variability

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:29.716510Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 49a0bc55-0352-4179-b1bd-10a551e99c96 · outbound

This paper cites an unresolved cited work.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Unresolved cited work

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:29.871913Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 32e20405-3f69-436d-beb6-48937e48926c · outbound

This paper cites Estimating Black Hole Masses in Active Galaxies Using the Halpha Emission Line.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Estimating Black Hole Masses in Active Galaxies Using the Halpha Emission Line

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:30.003899Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 52a9e234-d273-42d7-a74b-609409a78f76 · outbound

This paper cites A confirmed deficit of hot and cold dust emission in the most luminous Little Red Dots.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs A confirmed deficit of hot and cold dust emission in the most luminous Little Red Dots

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:30.130342Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a746215d-f691-4bdc-8a0c-38a9f2901eb8 · outbound

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

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs An unambiguous AGN and a Balmer break in an Ultraluminous Little Red Dot at z=4.47 from Ultradeep UNCOVER and All the Little Things Spectroscopy

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:30.258026Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 08f5c82f-7601-4bc9-aa8a-3db696b60f3b · outbound

This paper cites Redshift Evolution of the Electron Density in the ISM at $z\sim 0-9$ Uncovered with JWST/NIRSpec Spectra and Line-Spread Function Determinations.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Redshift Evolution of the Electron Density in the ISM at $z\sim 0-9$ Uncovered with JWST/NIRSpec Spectra and Line-Spread Function Determinations

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:30.417725Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 07758e62-1ea1-4017-a4f7-a3c2d79654f8 · outbound

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

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Locally Optimally Emitting Clouds and the Origin of Quasar Emission Lines

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:30.579810Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 28c99c8e-6554-4fc6-8b76-3b5c0f8fad73 · outbound

This paper cites What the Optical Recombination Lines Can Tell Us About the Broad Line Regions of Active Galactic Nuclei.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs What the Optical Recombination Lines Can Tell Us About the Broad Line Regions of Active Galactic Nuclei

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:30.762716Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 03d10c4b-17e5-4124-8c87-0c90e937c51c · outbound

This paper cites emcee: The MCMC Hammer.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs emcee: The MCMC Hammer

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:30.907957Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 44a1e1e8-fe71-460d-8eab-ad7d475188c7 · outbound

This paper cites Gas outflows in two recently quenched galaxies at z = 4 and 7.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Gas outflows in two recently quenched galaxies at z = 4 and 7

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:31.076102Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a7c47d76-b670-4dc1-a81a-8182c9a4f387 · outbound

This paper cites Extreme damped Lyman-$\alpha$ absorption in young star-forming galaxies at $z=9-11$.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Extreme damped Lyman-$\alpha$ absorption in young star-forming galaxies at $z=9-11$

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:31.191826Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a1ab42cc-6734-4508-a77e-65c95e2da544 · outbound

This paper cites RUBIES: a complete census of the bright and red distant Universe with JWST/NIRSpec.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs RUBIES: a complete census of the bright and red distant Universe with JWST/NIRSpec

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:31.369376Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9f6dfbd8-c0aa-4d38-b618-90e37cb06ed0 · outbound

This paper cites arXiv e-prints , keywords =.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs arXiv e-prints , keywords =

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:31.570366Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6eb0140c-4642-48f9-b73e-d0104b2fed6b · outbound

This paper cites arXiv e-prints , keywords =.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs arXiv e-prints , keywords =

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:31.680225Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d94526e1-540b-40b8-bd0e-01690466c9e0 · outbound

This paper cites MEGA: Spectrophotometric SED Fitting of Little Red Dots Detected in JWST MIRI.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs MEGA: Spectrophotometric SED Fitting of Little Red Dots Detected in JWST MIRI

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:31.772010Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5a18e3f4-4c23-44bb-a186-70245f6b08e2 · outbound

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

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs What you see is what you get: empirically measured bolometric luminosities of Little Red Dots

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:31.840857Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 333b1662-f403-4f81-b82c-7e4bf5c29287 · outbound

This paper cites Analysis of Multi-epoch JWST Images of $\sim 300$ Little Red Dots: Tentative Detection of Variability in a Minority of Sources.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Analysis of Multi-epoch JWST Images of $\sim 300$ Little Red Dots: Tentative Detection of Variability in a Minority of Sources

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:31.932734Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 132e77ab-b20e-4d2d-a884-17e452d6b0da · outbound

This paper cites NEXUS: A Search for Nuclear Variability with the First Two JWST NIRCam Epochs.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs NEXUS: A Search for Nuclear Variability with the First Two JWST NIRCam Epochs

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:32.002188Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 912649a8-60ba-44bb-9118-870df3944fb0 · outbound

This paper cites Lack of Rest-frame UV Variability in Little Red Dots Based on HST and JWST Observations.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Lack of Rest-frame UV Variability in Little Red Dots Based on HST and JWST Observations

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:32.135109Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d95d9fe1-1161-463a-9a41-373b2e988193 · outbound

This paper cites arXiv e-prints , keywords =.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs arXiv e-prints , keywords =

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:32.238064Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 82e22550-d95b-4298-8c9c-1d90ad5d0b35 · outbound

This paper cites arXiv e-prints , keywords =.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs arXiv e-prints , keywords =

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:32.298199Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 42f8daf8-176a-4508-a879-113319b004fd · outbound

This paper cites A high black hole to host mass ratio in a lensed AGN in the early Universe.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs A high black hole to host mass ratio in a lensed AGN in the early Universe

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:32.484866Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7b6b1c1f-5524-412f-ba6c-07823aa3a798 · outbound

This paper cites JWST UNCOVER: Extremely red and compact object at$z_{\mathrm{phot}}\simeq7.6$ triply imaged by Abell 2744.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs JWST UNCOVER: Extremely red and compact object at$z_{\mathrm{phot}}\simeq7.6$ triply imaged by Abell 2744

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:32.646223Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cd15fcd2-90b5-4766-9fb9-c29a2fb2ae45 · outbound

This paper cites Active galactic nuclei in four metal-poor dwarf emission-line galaxies.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Active galactic nuclei in four metal-poor dwarf emission-line galaxies

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:32.783568Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2ab1a915-efa9-4a73-9e0f-21c259d3b47c · outbound

This paper cites , keywords =.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs , keywords =

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:32.986914Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cbb87f56-f8f8-4062-af7e-0abd0dbe6bcf · outbound

This paper cites Another piece to the puzzle: radio detection of a JWST detected AGN candidate.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Another piece to the puzzle: radio detection of a JWST detected AGN candidate

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:33.177749Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9db6cddb-f30a-4106-b693-21c4d45f3d57 · outbound

This paper cites , keywords =.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs , keywords =

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:33.358734Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0617888d-aabd-4a73-8175-d8a68e75c885 · outbound

This paper cites A Novel Formation Channel for Supermassive Black Hole Binaries in the Early Universe via Primordial Black Holes.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs A Novel Formation Channel for Supermassive Black Hole Binaries in the Early Universe via Primordial Black Holes

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:33.537719Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5856b697-e0f3-431c-8051-184ba76669f9 · outbound

This paper cites The Reionization Lensing Cluster Survey (RELICS) and the Brightest High-z Galaxies.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs The Reionization Lensing Cluster Survey (RELICS) and the Brightest High-z Galaxies

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:33.756418Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1a41e145-be19-4191-88cc-64dcc1dd7c92 · outbound

This paper cites Complex diffuse emission in the $z=0.52$ cluster PLCK~G004.5-19.5.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Complex diffuse emission in the $z=0.52$ cluster PLCK~G004.5-19.5

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:33.940503Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cc234222-4ceb-44fb-a8b7-3e3950f71873 · outbound

This paper cites Strong Lensing Analysis of PLCK G004.5$-$19.5, a Planck-Discovered Cluster Hosting a Radio Relic at $z=0.52$.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Strong Lensing Analysis of PLCK G004.5$-$19.5, a Planck-Discovered Cluster Hosting a Radio Relic at $z=0.52$

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:34.082382Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 190c70ff-2888-423a-b4b7-9168d4242362 · outbound

This paper cites ComPRASS: a Combined Planck-RASS catalogue of X-ray-SZ clusters.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs ComPRASS: a Combined Planck-RASS catalogue of X-ray-SZ clusters

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:34.217248Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 47ca1bdd-0fbc-4b6a-b309-b6e85d196c4c · outbound

This paper cites an unresolved cited work.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Unresolved cited work

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:34.335193Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 33e320ba-de26-4f03-ae48-e720010beda2 · outbound

This paper cites Formation of Intermediate-Mass Black Holes through Runaway Collisions in the First Star Clusters.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Formation of Intermediate-Mass Black Holes through Runaway Collisions in the First Star Clusters

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:34.505008Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d6499ec1-753e-4685-82ee-18c7ed979840 · outbound

This paper cites The runaway growth of intermediate-mass black holes in dense star clusters.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs The runaway growth of intermediate-mass black holes in dense star clusters

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:34.661338Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a278f56a-e215-4a96-88c5-baaa1e73115a · outbound

This paper cites The formation of massive black holes through collision runaway in dense young star clusters.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs The formation of massive black holes through collision runaway in dense young star clusters

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:34.812797Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 37e635c8-5e4a-479a-ae0b-a2e7729f7a50 · outbound

This paper cites Growth of Massive Black-Holes in FFB Galaxies at Cosmic Dawn.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Growth of Massive Black-Holes in FFB Galaxies at Cosmic Dawn

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:34.981883Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8f2e262c-6b98-4b12-8042-f082906c61c0 · outbound

This paper cites , keywords =.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs , keywords =

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:35.121550Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3cac0961-b40a-4fac-8f45-9b256617c3cc · outbound

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

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Planck 2018 results. VI. Cosmological parameters

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:35.274987Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7e53d37e-0ba2-4bf6-81c6-8fe243f8b174 · outbound

This paper cites Intermediate-Mass Black Holes.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Intermediate-Mass Black Holes

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:35.462204Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e32711d5-1b55-403f-ab0f-871a836c4bbe · outbound

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

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:35.627174Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1f61cef6-94cd-4ac8-918f-87f3ae27ab16 · outbound

This paper cites BlackTHUNDER: Evidence of three massive black holes in a z~5 galaxy.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs BlackTHUNDER: Evidence of three massive black holes in a z~5 galaxy

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:35.804453Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 71ee1356-2607-403b-b024-097b0470a289 · outbound

This paper cites A Long Time Ago in a Galaxy Far, Far Away: A Candidate z ~ 12 Galaxy in Early JWST CEERS Imaging.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs A Long Time Ago in a Galaxy Far, Far Away: A Candidate z ~ 12 Galaxy in Early JWST CEERS Imaging

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:35.946485Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 839ebd4a-6a68-43d5-9aee-4e1f8c479747 · outbound

This paper cites The Star-Forming Main Sequence in JADES and CEERS at $z>1.4$: Investigating the Burstiness of Star Formation.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs The Star-Forming Main Sequence in JADES and CEERS at $z>1.4$: Investigating the Burstiness of Star Formation

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:36.136105Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 538c1c8a-ac8a-4ff2-88a6-0bf1f8bcb6d1 · outbound

This paper cites arXiv e-prints , keywords =.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs arXiv e-prints , keywords =

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:36.289364Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 85aced76-19db-4744-96af-4b1b9da1428c · outbound

This paper cites Possible environmental quenching in an interacting little red dot pair at $z\sim7$.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Possible environmental quenching in an interacting little red dot pair at $z\sim7$

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:36.497655Z

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Observation 14e79b0a-be5b-408f-8342-0b39f3aa18a5 · outbound

This paper cites The Assembly and Merging History of Supermassive Black Holes in Hierarchical Models of Galaxy Formation.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs The Assembly and Merging History of Supermassive Black Holes in Hierarchical Models of Galaxy Formation

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:36.650628Z

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Observation 0a5306ad-48aa-4e46-9569-f2d602affd75 · outbound

This paper cites Little Red Dots as the Very First Activity of Black Hole Growth.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Little Red Dots as the Very First Activity of Black Hole Growth

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:36.794829Z

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