Paper Citation Record · LEDGER

A remarkable Ruby: Absorption in dense gas, rather than evolved stars, drives the extreme Balmer break of a Little Red Dot at $z=3.5$

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 23 inbound Pith citation observations for arXiv:2503.16600.

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pith.paper-citation-record.v1
2503.16600 v2

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measured 0 of 0 reference resolution

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measured 23 of 23 standing notices

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

measured 23 of 23 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T16:36:20.070821Z

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

2
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

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Pith citing papers

Observation 98224954-3859-4f04-b175-ce7fdc857630 · inbound

Investigating photometric and spectroscopic variability in the multiply-imaged Little Red Dot A2744-QSO1 cites this paper.

Investigating photometric and spectroscopic variability in the multiply-imaged Little Red Dot A2744-QSO1 A remarkable Ruby: Absorption in dense gas, rather than evolved stars, drives the extreme Balmer break of a Little Red Dot at $z=3.5$

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-08T11:37:36.253365Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 24f5937e-95bc-4145-81ef-e4ae90556832 · inbound

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

An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots A remarkable Ruby: Absorption in dense gas, rather than evolved stars, drives the extreme Balmer break of a Little Red Dot at $z=3.5$

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-07T14:31:01.148934Z

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Unavailable: canonical work link unavailable.

Observation a860270c-7158-4eb3-ad66-0bcbed32b991 · inbound

NEXUS: A Spectroscopic Census of Broad-line AGNs and Little Red Dots at $3\lesssim z\lesssim 6$ cites this paper.

NEXUS: A Spectroscopic Census of Broad-line AGNs and Little Red Dots at $3\lesssim z\lesssim 6$ A remarkable Ruby: Absorption in dense gas, rather than evolved stars, drives the extreme Balmer break of a Little Red Dot at $z=3.5$

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-07T14:03:25.678036Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6f8cf89c-0195-46bb-8676-19198ee589d7 · 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 A remarkable Ruby: Absorption in dense gas, rather than evolved stars, drives the extreme Balmer break of a Little Red Dot at $z=3.5$

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-07T10:56:02.628170Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c71abd63-798f-497f-82bc-2f6e11762615 · inbound

On the ages of the stellar populations of galaxies at $z=0.1$-7 cites this paper.

On the ages of the stellar populations of galaxies at $z=0.1$-7 A remarkable Ruby: Absorption in dense gas, rather than evolved stars, drives the extreme Balmer break of a Little Red Dot at $z=3.5$

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-06T20:24:22.424885Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7d358604-a7fa-4330-98c0-126e7a58a141 · inbound

BASS. XLIX. Characterization of highly luminous and obscured AGNs: local X-ray and [NeV]$\lambda$3426 emission in comparison with the high-redshift Universe cites this paper.

BASS. XLIX. Characterization of highly luminous and obscured AGNs: local X-ray and [NeV]$\lambda$3426 emission in comparison with the high-redshift Universe A remarkable Ruby: Absorption in dense gas, rather than evolved stars, drives the extreme Balmer break of a Little Red Dot at $z=3.5$

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-06T17:36:50.438710Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 53020cf6-accf-49f1-8f86-ed42b6a702f3 · inbound

Little Red reionization factories cites this paper.

Little Red reionization factories A remarkable Ruby: Absorption in dense gas, rather than evolved stars, drives the extreme Balmer break of a Little Red Dot at $z=3.5$

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-05T19:03:20.293736Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7e6bbf59-ee85-4bd3-88bb-e751a5de0a4e · inbound

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

MEGA: Spectrophotometric SED Fitting of Little Red Dots Detected in JWST MIRI A remarkable Ruby: Absorption in dense gas, rather than evolved stars, drives the extreme Balmer break of a Little Red Dot at $z=3.5$

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-05T15:21:40.809990Z

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Unavailable: canonical work link unavailable.

Observation 7feb60ea-78eb-400f-93fa-9a8dab2b3ef7 · inbound

How similar are narrow-line Seyfert 1 galaxies and high-z type 1 AGN? cites this paper.

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-05T10:54:34.684195Z

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Observation f8675fa7-5e18-4217-ae84-3d9c479c9be0 · inbound

Another view into JWST-discovered X-ray weak AGNs via radiative dusty feedback cites this paper.

Another view into JWST-discovered X-ray weak AGNs via radiative dusty feedback A remarkable Ruby: Absorption in dense gas, rather than evolved stars, drives the extreme Balmer break of a Little Red Dot at $z=3.5$

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-05T05:32:42.288643Z

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Unavailable: canonical work link unavailable.

Observation 5bb2a2e8-56f8-46ad-a02b-73eb7a35b55a · 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 A remarkable Ruby: Absorption in dense gas, rather than evolved stars, drives the extreme Balmer break of a Little Red Dot at $z=3.5$

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-04T18:47:40.816971Z

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Unavailable: canonical work link unavailable.

Observation e7d95fc8-64d8-44dc-8221-3bacca5458c2 · inbound

(Re)solving the Complex Multiscale Morphology and V-shaped Spectral Energy Distribution of a Newly Discovered Strongly Lensed Little Red Dot in A383 cites this paper.

(Re)solving the Complex Multiscale Morphology and V-shaped Spectral Energy Distribution of a Newly Discovered Strongly Lensed Little Red Dot in A383 A remarkable Ruby: Absorption in dense gas, rather than evolved stars, drives the extreme Balmer break of a Little Red Dot at $z=3.5$

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-03T18:55:21.584941Z

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Unavailable: canonical work link unavailable.

Observation b12d0460-01bf-478f-8e58-882be104a95d · inbound

The X-ray weakness of Little Red Dots and JWST-selected AGN: comparison with local AGN in different accretion regimes cites this paper.

The X-ray weakness of Little Red Dots and JWST-selected AGN: comparison with local AGN in different accretion regimes A remarkable Ruby: Absorption in dense gas, rather than evolved stars, drives the extreme Balmer break of a Little Red Dot at $z=3.5$

Reference 18

Resolution: verified exact; arxiv_id, observed 2026-05-15T12:45:37.228261Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 4281f3fe-cc22-4130-859d-66cb5291a8c8 · inbound

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

Paschen Jumps in Little Red Dots: Evidence for Nebular Continua A remarkable Ruby: Absorption in dense gas, rather than evolved stars, drives the extreme Balmer break of a Little Red Dot at $z=3.5$

Reference 57

Resolution: verified exact; arxiv_id, observed 2026-05-11T07:45:59.092141Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation f7f9a023-a971-4abf-8e94-91bc531dd8bd · inbound

Hidden Monsters with SPHEREx I: A goldmine for heavily reddened quasars at cosmic noon cites this paper.

Hidden Monsters with SPHEREx I: A goldmine for heavily reddened quasars at cosmic noon A remarkable Ruby: Absorption in dense gas, rather than evolved stars, drives the extreme Balmer break of a Little Red Dot at $z=3.5$

Reference 44

Resolution: metadata mismatch; arxiv_id, observed 2026-05-11T01:10:52.200441Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 3b94244f-5525-44a3-8e4c-5252019b5ae9 · 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 A remarkable Ruby: Absorption in dense gas, rather than evolved stars, drives the extreme Balmer break of a Little Red Dot at $z=3.5$

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-02T13:59:30.351233Z

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Unavailable: canonical work link unavailable.

Observation 289f71ad-12e7-450f-9b61-20c8271adfcb · inbound

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

(LRDs)$^2$: The Low-ReDshift Little Red Dots Survey. II. DESI DR1 Sample A remarkable Ruby: Absorption in dense gas, rather than evolved stars, drives the extreme Balmer break of a Little Red Dot at $z=3.5$

Reference 35

Resolution: verified exact; arxiv_id, observed 2026-05-22T09:46:22.261018Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 8053ca1f-c4cc-4307-8fd3-ed363c1b8268 · inbound

JWST's Little Red Dots as collapsed Supermassive Dark Stars cites this paper.

JWST's Little Red Dots as collapsed Supermassive Dark Stars A remarkable Ruby: Absorption in dense gas, rather than evolved stars, drives the extreme Balmer break of a Little Red Dot at $z=3.5$

Reference 5

Resolution: verified exact; arxiv_id, observed 2026-07-02T00:56:25.361542Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 9c20574f-4b03-4241-8bee-117a86b60b23 · inbound

No evolution in the number density of little red dots from cosmic dawn to cosmic noon cites this paper.

No evolution in the number density of little red dots from cosmic dawn to cosmic noon A remarkable Ruby: Absorption in dense gas, rather than evolved stars, drives the extreme Balmer break of a Little Red Dot at $z=3.5$

Reference 11

Resolution: metadata mismatch; arxiv_id, observed 2026-06-30T04:54:16.230860Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation a38d2498-3782-4601-8c48-4b9bb85fc7f9 · inbound

Spatial decomposition of Little Red Dots with JWST/NIRSpec IFU into broad-line red cores and narrow-line blue host galaxies cites this paper.

Spatial decomposition of Little Red Dots with JWST/NIRSpec IFU into broad-line red cores and narrow-line blue host galaxies A remarkable Ruby: Absorption in dense gas, rather than evolved stars, drives the extreme Balmer break of a Little Red Dot at $z=3.5$

Reference 133

Resolution: unresolved; no resolver link, observed 2026-07-13T01:29:44.810998Z

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Unavailable: canonical work link unavailable.

Observation b18c69e7-9f7f-48ba-a4e2-e090033b6aa1 · 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 A remarkable Ruby: Absorption in dense gas, rather than evolved stars, drives the extreme Balmer break of a Little Red Dot at $z=3.5$

Reference 105

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:37.520621Z

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Unavailable: canonical work link unavailable.

Observation 0fa72a21-30aa-4772-b7dd-227e311f12c1 · inbound

Misaligned or chaotic? A strong break of axial symmetry in the local LRD J1025 revealed with VLT/FORS2 spectropolarimetry cites this paper.

Misaligned or chaotic? A strong break of axial symmetry in the local LRD J1025 revealed with VLT/FORS2 spectropolarimetry A remarkable Ruby: Absorption in dense gas, rather than evolved stars, drives the extreme Balmer break of a Little Red Dot at $z=3.5$

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-03T00:41:21.899284Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4e99ea94-7c17-4ebb-8987-cfe0b77be411 · inbound

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ cites this paper.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ A remarkable Ruby: Absorption in dense gas, rather than evolved stars, drives the extreme Balmer break of a Little Red Dot at $z=3.5$

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.070821Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.