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Paper Citation Record · LEDGER

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

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 27 inbound Pith citation observations for arXiv:2405.00504.

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

pith.paper-citation-record.v1
2405.00504 v2

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Source: paper_references, paper_reference_links

measured 27 of 27 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 27 of 27 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-09T01:00:39.406158Z

measured 1 of 1 external citation measurements

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

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

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External citation measurements

9
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation f1bcf551-0ac4-469d-985b-0f4bc0b73a8a · inbound

Hidden in Pixels I: Discovery of dual "little red dots" indicates excess clustering on kilo-parsec scales cites this paper.

Hidden in Pixels I: Discovery of dual "little red dots" indicates excess clustering on kilo-parsec scales JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe

Reference 25

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arxiv_id, observed 2026-05-23T06:37:39.067083Z

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Observation 7c9ba7a3-64ad-4add-adb0-ed4c6db26c88 · inbound

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

Radio emission from little red dots may reveal their true nature JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe

Reference 22

Resolution
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Observation cc625ca9-80d6-417a-a70a-378952563b40 · inbound

A "Black Hole Star" Reveals the Remarkable Gas-Enshrouded Hearts of the Little Red Dots cites this paper.

A "Black Hole Star" Reveals the Remarkable Gas-Enshrouded Hearts of the Little Red Dots JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe

Reference 69

Resolution
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arxiv_id, observed 2026-05-16T08:53:14.846743Z

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Observation 87b7360d-8719-45ee-9573-ed8f243326f7 · inbound

Discovery and characterization of 25 new quasars at 4.6 < z < 6.9 from wide-field multi-band surveys cites this paper.

Discovery and characterization of 25 new quasars at 4.6 < z < 6.9 from wide-field multi-band surveys JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe

Reference 106

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Observation 3ebf87a3-a990-4819-90f3-53cd156b8aeb · inbound

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

Lonely Little Red Dots: Challenges to the AGN-nature of little red dots through their clustering and spectral energy distributions JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe

Reference 90

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Observation 12d464a8-bee2-44a6-8572-2daefe86f018 · inbound

Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XXIV. 54 New Quasars and Candidate Obscured Quasars at $5.71 \le z \le 7.02$ cites this paper.

Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XXIV. 54 New Quasars and Candidate Obscured Quasars at $5.71 \le z \le 7.02$ JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe

Reference 117

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Observation 1e261314-83a0-4c88-a67e-b7da63391ccb · inbound

Investigating Little Red Dots with UV Excess: Are They the High-Redshift Siblings of Blue Hot DOGs? cites this paper.

Investigating Little Red Dots with UV Excess: Are They the High-Redshift Siblings of Blue Hot DOGs? JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe

Reference 45

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Observation b1dac9ff-6238-4c51-9406-2cbb0481be0c · inbound

A direct black hole mass measurement in a Little Red Dot at the Epoch of Reionization cites this paper.

A direct black hole mass measurement in a Little Red Dot at the Epoch of Reionization JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe

Reference 6

Resolution
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Observation 27603b8b-b753-4bd5-8e2e-3de781a73c81 · inbound

Characterizing the roles of transitory obscured phases and inner torus in shaping the fractions of obscured AGN at cosmic noon cites this paper.

Characterizing the roles of transitory obscured phases and inner torus in shaping the fractions of obscured AGN at cosmic noon JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe

Reference 109

Resolution
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Observation 8749bdbe-362d-4340-a1df-7d25927ef08f · inbound

Discovery of Multiply Ionized Iron Emission Powered by an Active Galactic Nucleus in a z~7 Little Red Dot cites this paper.

Discovery of Multiply Ionized Iron Emission Powered by an Active Galactic Nucleus in a z~7 Little Red Dot JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe

Reference 26

Resolution
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Observation c87ac646-2576-4656-bb87-6552c1d7384f · inbound

Little Red Dots as Hidden Neutrino Sources cites this paper.

Little Red Dots as Hidden Neutrino Sources JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe

Reference 76

Resolution
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arxiv_id, observed 2026-05-16T13:42:56.226180Z

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Observation c5123502-bdb2-4531-bdf7-8d1328983fdd · inbound

The Two Orbital, Interacting Hatano-Nelson Model cites this paper.

The Two Orbital, Interacting Hatano-Nelson Model JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe

Reference 28

Resolution
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Observation ae6598ee-882e-497a-b9b0-a58c8c3eef1f · inbound

Ultrahigh-energy cosmogenic neutrino emissions in the high-redshift universe cites this paper.

Ultrahigh-energy cosmogenic neutrino emissions in the high-redshift universe JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe

Reference 28

Resolution
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arxiv_id, observed 2026-05-10T11:10:09.316943Z

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Observation 669338fc-c2b6-4a4b-80da-1a1f1b72e99d · inbound

Ultrahigh-energy cosmogenic neutrino emissions in the high-redshift universe cites this paper.

Ultrahigh-energy cosmogenic neutrino emissions in the high-redshift universe JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe

Reference 28

Resolution
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Observation eb23ae29-9803-4122-82b1-5fc9315994af · inbound

Gravitational Waves from the Cosmic Dawn: Tracing Cosmic Black Hole Binaries with ET, LGWA and LISA cites this paper.

Gravitational Waves from the Cosmic Dawn: Tracing Cosmic Black Hole Binaries with ET, LGWA and LISA JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe

Reference 16

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arxiv_id, observed 2026-05-10T05:00:36.573483Z

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Observation e312ec09-84e7-4944-9c84-45b575ec3cdb · inbound

Compact, AGN-hosting Dwarf Galaxies with "Little Red Dots"-like SEDs in the Local Universe cites this paper.

Compact, AGN-hosting Dwarf Galaxies with "Little Red Dots"-like SEDs in the Local Universe JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe

Reference 59

Resolution
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arxiv_id, observed 2026-05-08T19:59:08.282915Z

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Observation e8f38d88-66cb-423c-bdd0-573dec04abe6 · inbound

Quenching of X-ray emission in little red dots by both Compton-thick gas and high accretion rates cites this paper.

Quenching of X-ray emission in little red dots by both Compton-thick gas and high accretion rates JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe

Reference 37

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Observation b3e7164e-3d99-4809-b133-dd91df9b9b56 · inbound

Exploring biases in derived stellar parameters and the ionizing photon production efficiency cites this paper.

Exploring biases in derived stellar parameters and the ionizing photon production efficiency JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe

Reference 73

Resolution
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arxiv_id, observed 2026-06-29T23:54:03.440674Z

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Observation 1cf30c0c-f808-45e3-aefa-a7242ea2203a · inbound

Little red dots as a cosmological probe: constraining $H_0$ with quasi-periodic pulsations cites this paper.

Little red dots as a cosmological probe: constraining $H_0$ with quasi-periodic pulsations JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe

Reference 14

Resolution
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arxiv_id, observed 2026-07-02T10:06:51.626133Z

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Observation 83d9833b-60a3-4c0c-9437-af0d09983de1 · inbound

TBD LBD: The nature of `little blue dots' cites this paper.

TBD LBD: The nature of `little blue dots' JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe

Reference 18

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arxiv_id, observed 2026-07-03T11:58:05.840416Z

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Observation f155586d-c7eb-4b9f-9924-eda7f2f40899 · inbound

Memoirs of the curvaton: non-perturbative non-Gaussianity and supermassive primordial black holes cites this paper.

Memoirs of the curvaton: non-perturbative non-Gaussianity and supermassive primordial black holes JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe

Reference 213

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arxiv_id, observed 2026-07-01T18:15:57.872539Z

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Observation 83d17218-ea97-4a96-a9fc-c7a9b52de212 · inbound

Unveil the nature of JWST-AGN and Little Red Dots with SKAO continuum surveys cites this paper.

Unveil the nature of JWST-AGN and Little Red Dots with SKAO continuum surveys JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe

Reference 190

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arxiv_id, observed 2026-07-01T06:25:28.109160Z

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Observation 6030a298-f9d3-48ca-9ebf-ed83a2a15788 · inbound

Two Peas in a Pod: The First Confirmed Dual Active Galactic Nucleus within a Green Pea Galaxy System cites this paper.

Two Peas in a Pod: The First Confirmed Dual Active Galactic Nucleus within a Green Pea Galaxy System JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe

Reference 109

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Observation cb9125b9-85c6-4ce2-8d0f-bc193c84d071 · inbound

An (in)complete NIRSpec census of Balmer absorption in Type 1 AGN -- radiation-driven outflows in little red dots, quasars and variable stars cites this paper.

An (in)complete NIRSpec census of Balmer absorption in Type 1 AGN -- radiation-driven outflows in little red dots, quasars and variable stars JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe

Reference 135

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Observation 0c953cdf-1ba3-4bd0-b21f-c52f5f0d451b · inbound

Outflows in super-Eddington quasars drive clumpy circumgalactic medium and extended H$\alpha$ nebulae at $z \gtrsim 6$ cites this paper.

Outflows in super-Eddington quasars drive clumpy circumgalactic medium and extended H$\alpha$ nebulae at $z \gtrsim 6$ JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe

Reference 294

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Source-reported events for the cited work

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Observation e4312d3f-8fde-4214-802e-666e5b76bbce · inbound

A quasar hatching from a buried red phase at z = 3.7 cites this paper.

A quasar hatching from a buried red phase at z = 3.7 JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe

Reference 52

Resolution
unresolved
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Observation 7f74ee36-0921-4d65-90bb-82e8b95d76e6 · inbound

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs cites this paper.

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
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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