Paper Citation Record · LEDGER

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension

As of 3 August 2026, this Paper Citation Record lists 41 of 41 outbound references and 1 inbound Pith citation observation for arXiv:2511.13708.

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

pith.paper-citation-record.v1
2511.13708 v3

Coverage vector

measured 41 of 41 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-05-17T21:42:40.737453Z

measured 42 of 42 standing notices

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measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T02:52:20.210937Z

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

41 of 41 outbound references displayed

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verified fuzzy1
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External citation measurements

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Outbound references

Observation 74352149-ed79-4adb-9af6-0e4e92cac6f6 · outbound

This paper cites Stress Testing $\Lambda$CDM with High-redshift Galaxy Candidates.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension Stress Testing $\Lambda$CDM with High-redshift Galaxy Candidates

Reference 1

Resolution: verified exact; arxiv_id, observed 2026-05-17T21:45:18.357995Z

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Observation a17fc06c-0751-48bd-aedd-431ecc74fa25 · outbound

This paper cites Are the ultra-high-redshift galaxies at z > 10 surprising in the context of standard galaxy formation models?.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension Are the ultra-high-redshift galaxies at z > 10 surprising in the context of standard galaxy formation models?

Reference 2

Resolution: verified exact; arxiv_id, observed 2026-05-17T21:45:18.241214Z

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Observation b27cfa70-4139-44f6-a230-5f2f7817fc4f · outbound

This paper cites arXiv preprint arXiv:2504.18618 , year=.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension arXiv preprint arXiv:2504.18618 , year=

Reference 3

Resolution: verified exact; arxiv_id, observed 2026-05-17T21:45:18.291150Z

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Observation 6be297fa-fb56-40e2-badf-1e0b199aa2f6 · outbound

This paper cites Early Galaxies and Early Dark Energy: A Unified Solution to the Hubble Tension and Puzzles of Massive Bright Galaxies revealed by JWST.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension Early Galaxies and Early Dark Energy: A Unified Solution to the Hubble Tension and Puzzles of Massive Bright Galaxies revealed by JWST

Reference 4

Resolution: verified exact; arxiv_id, observed 2026-05-17T21:45:18.284638Z

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Observation b8140e75-ea75-452f-99c5-9ce33b9a2e93 · outbound

This paper cites Evidence for a Shallow Evolution in the Volume Densities of Massive Galaxies at $z=4$ to $8$ from CEERS.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension Evidence for a Shallow Evolution in the Volume Densities of Massive Galaxies at $z=4$ to $8$ from CEERS

Reference 5

Resolution: verified exact; arxiv_id, observed 2026-05-17T21:45:18.269458Z

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Observation 7142fd36-ec5d-44cb-8f8b-8747d98f24c3 · outbound

This paper cites Efficient Formation of Massive Galaxies at Cosmic Dawn by Feedback-Free Starbursts.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension Efficient Formation of Massive Galaxies at Cosmic Dawn by Feedback-Free Starbursts

Reference 6

Resolution: verified exact; arxiv_id, observed 2026-05-17T21:45:18.258921Z

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Observation 7a9f37e3-454e-4414-9049-53d77d6b993c · outbound

This paper cites Can Cosmological Simulations Reproduce the Spectroscopically Confirmed Galaxies Seen at $z\geq 10$?.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension Can Cosmological Simulations Reproduce the Spectroscopically Confirmed Galaxies Seen at $z\geq 10$?

Reference 7

Resolution: verified exact; arxiv_id, observed 2026-05-17T21:45:18.255325Z

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Observation 2a072ccf-cda6-4086-8ddb-023971430a29 · outbound

This paper cites McCaffrey, S.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension McCaffrey, S

Reference 8

Resolution: verified exact; arxiv_id, observed 2026-05-17T21:45:18.262248Z

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Observation 1708d5cd-764d-4f3b-a0ab-e2d875112386 · outbound

This paper cites E., Tacchella, S., Johnson, B.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension E., Tacchella, S., Johnson, B

Reference 9

Resolution: verified exact; arxiv_id, observed 2026-05-17T21:45:18.309181Z

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Observation 52bef194-6a50-4cc3-afa0-27b6d2421030 · outbound

This paper cites The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics

Reference 10

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Observation 995b590c-2b5b-4938-89cd-989266a8ee37 · outbound

This paper cites Accelerating early massive galaxy formation with primordial black holes.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension Accelerating early massive galaxy formation with primordial black holes

Reference 11

Resolution: verified exact; arxiv_id, observed 2026-05-17T21:45:18.280955Z

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Observation 8afeea5e-19ef-45f8-b822-9a53b07dc7e9 · outbound

This paper cites High-redshift JWST Observations and Primordial Non-Gaussianity.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension High-redshift JWST Observations and Primordial Non-Gaussianity

Reference 12

Resolution: verified exact; arxiv_id, observed 2026-05-17T21:45:18.319977Z

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Observation d9e94888-e2e0-43b3-bd82-a8ef325058d8 · outbound

This paper cites Did JWST observe imprints of axion miniclusters or primordial black holes?.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension Did JWST observe imprints of axion miniclusters or primordial black holes?

Reference 13

Resolution: verified exact; arxiv_id, observed 2026-05-17T21:45:18.230753Z

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Observation a2b2fc04-d61e-4aef-bafa-c27a0e4da45d · outbound

This paper cites Structure Formation Paradigm and Axion Quark Nugget dark matter model.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension Structure Formation Paradigm and Axion Quark Nugget dark matter model

Reference 14

Resolution: verified exact; arxiv_id, observed 2026-05-17T21:45:18.294670Z

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Observation 7cc0dc9d-073b-4dac-afbc-5b5daa2a0d90 · outbound

This paper cites Footprints of Axion-Like Particle in Pulsar Timing Array Data and James Webb Space Telescope Observations.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension Footprints of Axion-Like Particle in Pulsar Timing Array Data and James Webb Space Telescope Observations

Reference 15

Resolution: verified exact; arxiv_id, observed 2026-05-17T21:45:18.287939Z

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Observation 1cdb5073-3be2-4b38-9904-373a46dbe22c · outbound

This paper cites Enhanced Early Galaxy Formation in JWST from Axion Dark Matter?.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension Enhanced Early Galaxy Formation in JWST from Axion Dark Matter?

Reference 16

Resolution: verified exact; arxiv_id, observed 2026-05-17T21:45:18.237775Z

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Observation 1c3b3e1b-1741-4fc6-b090-5cf735d3b98c · outbound

This paper cites Dark energy in light of the early JWST observations: case for a negative cosmological constant?.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension Dark energy in light of the early JWST observations: case for a negative cosmological constant?

Reference 17

Resolution: verified exact; arxiv_id, observed 2026-05-17T21:45:18.302230Z

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Observation fe3d1553-dea9-46d1-bae1-1a6079f389a8 · outbound

This paper cites Self-Calibration of Cluster Dark Energy Studies: Observable-Mass Distribution.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension Self-Calibration of Cluster Dark Energy Studies: Observable-Mass Distribution

Reference 18

Resolution: verified exact; local_arxiv, observed 2026-05-17T21:45:18.265907Z

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Observation 4e95f079-1d27-4ff0-b7f8-1b715e7997f5 · outbound

This paper cites Extreme Value Statistics of the Halo and Stellar Mass Distributions at High Redshift: are JWST Results in Tension with {\Lambda}CDM?.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension Extreme Value Statistics of the Halo and Stellar Mass Distributions at High Redshift: are JWST Results in Tension with {\Lambda}CDM?

Reference 19

Resolution: verified exact; arxiv_id, observed 2026-05-17T21:45:18.298599Z

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Observation b6439c68-0f5a-4c9d-bebb-fee8dea11f32 · outbound

This paper cites an unresolved cited work.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension Unresolved cited work

Reference 20

Resolution: unresolved; raw_fallback, observed 2026-05-17T21:45:18.725672Z

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Observation 56385a1d-8d6e-4aa0-9ee9-a5eaee3da822 · outbound

This paper cites Eddington-Malmquist bias in a cosmological context.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension Eddington-Malmquist bias in a cosmological context

Reference 21

Resolution: verified exact; local_arxiv, observed 2026-05-17T21:45:18.248640Z

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Observation 2095a578-d337-4d69-bf4e-a98d4136b4d5 · outbound

This paper cites A population of red candidate massive galaxies ~600 Myr after the Big Bang.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension A population of red candidate massive galaxies ~600 Myr after the Big Bang

Reference 22

Resolution: metadata mismatch; arxiv_id, observed 2026-05-17T21:45:18.227086Z

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Observation b3d3a607-2c6a-4861-b5a4-2a8882c2f598 · outbound

This paper cites Spectroscopic Confirmation of CEERS NIRCam-selected Galaxies at $\boldsymbol{z \simeq 8-10}$.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension Spectroscopic Confirmation of CEERS NIRCam-selected Galaxies at $\boldsymbol{z \simeq 8-10}$

Reference 23

Resolution: verified exact; arxiv_id, observed 2026-05-17T21:45:18.316387Z

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Observation 5b8ae3f9-c3af-40b5-a61c-0add7e15c2f1 · outbound

This paper cites JADES NIRSpec Spectroscopy of GN-z11: Lyman-$\alpha$ emission and possible enhanced nitrogen abundance in a $z=10.60$ luminous galaxy.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension JADES NIRSpec Spectroscopy of GN-z11: Lyman-$\alpha$ emission and possible enhanced nitrogen abundance in a $z=10.60$ luminous galaxy

Reference 24

Resolution: verified exact; arxiv_id, observed 2026-05-17T21:45:18.353888Z

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Observation aa5dd005-c5a6-409b-92e5-6e62be7c4211 · outbound

This paper cites JWST NIRSpec Spectroscopy of the Remarkable Bright Galaxy GHZ2/GLASS-z12 at Redshift 12.34.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension JWST NIRSpec Spectroscopy of the Remarkable Bright Galaxy GHZ2/GLASS-z12 at Redshift 12.34

Reference 25

Resolution: metadata mismatch; arxiv_id, observed 2026-05-17T21:45:18.350595Z

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Observation 88845145-4726-4048-905f-184839ecc944 · outbound

This paper cites Spectroscopic confirmation of two luminous galaxies at $z\sim14$.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension Spectroscopic confirmation of two luminous galaxies at $z\sim14$

Reference 26

Resolution: metadata mismatch; arxiv_id, observed 2026-05-17T21:45:18.347172Z

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Observation e51adfe9-7381-41ed-af28-2682f323bc6c · outbound

This paper cites P., Oesch, P.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension P., Oesch, P

Reference 27

Resolution: verified exact; arxiv_id, observed 2026-05-17T21:45:18.338797Z

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Observation b21c0f60-f5ee-430c-bc2c-59f60b3b6418 · outbound

This paper cites arXiv e-prints , keywords =.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension arXiv e-prints , keywords =

Reference 28

Resolution: verified exact; arxiv_id, observed 2026-05-17T21:45:18.343121Z

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Observation ad929c06-2c80-4ebf-9590-a64440bf73ea · outbound

This paper cites Halo Models of Large Scale Structure.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension Halo Models of Large Scale Structure

Reference 29

Resolution: verified exact; local_arxiv, observed 2026-05-17T21:45:18.334915Z

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Observation 450ac843-7f0f-4960-9738-8bd1d94159c6 · outbound

This paper cites The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes

Reference 30

Resolution: verified exact; local_arxiv, observed 2026-05-17T21:45:18.331276Z

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Observation 41956b66-0591-4131-87b7-f763f55975b3 · outbound

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

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension Planck 2018 results. VI. Cosmological parameters

Reference 31

Resolution: metadata mismatch; local_arxiv, observed 2026-05-17T21:45:18.323563Z

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Observation b2e43be1-0615-44fb-ab13-ee66d8a773da · outbound

This paper cites the scatter of the many out- weighs the scatter of the few: Systematic error asymmetry in steeply-falling mass functions for high- redshift jwst galaxies.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension the scatter of the many out- weighs the scatter of the few: Systematic error asymmetry in steeply-falling mass functions for high- redshift jwst galaxies

Reference 32

Resolution: verified fuzzy; raw_fallback, observed 2026-05-17T21:45:18.734770Z

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Observation c115280c-2a8c-4ec5-bdd9-527eb54e70f1 · outbound

This paper cites Toward a halo mass function for precision cosmology: the limits of universality.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension Toward a halo mass function for precision cosmology: the limits of universality

Reference 33

Resolution: verified exact; local_arxiv, observed 2026-05-17T21:45:18.312945Z

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Observation 2483f964-4f2e-4945-ac47-2cd888fa578b · outbound

This paper cites Large scale bias and the peak background split.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension Large scale bias and the peak background split

Reference 34

Resolution: verified exact; local_arxiv, observed 2026-05-17T21:45:18.244832Z

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Observation 17afc46c-9117-4dbf-94e6-fd7703d77c9f · outbound

This paper cites Precision Determination of the Mass Function of Dark Matter Halos.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension Precision Determination of the Mass Function of Dark Matter Halos

Reference 35

Resolution: verified exact; local_arxiv, observed 2026-05-17T21:45:18.252085Z

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Observation a867a2da-d9fc-456a-a769-c50d9d0c971d · outbound

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Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension Unresolved cited work

Reference 36

Resolution: verified exact; arxiv_id, observed 2026-05-17T21:45:18.305777Z

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Observation 9913ba47-8ce0-4460-9793-4583e068e93c · outbound

This paper cites EPOCHS I. The Discovery and Star Forming Properties of Galaxies in the Epoch of Reionization at $6.5 < z < 18$ with PEARLS and Public JWST data.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension EPOCHS I. The Discovery and Star Forming Properties of Galaxies in the Epoch of Reionization at $6.5 < z < 18$ with PEARLS and Public JWST data

Reference 37

Resolution: verified exact; arxiv_id, observed 2026-05-17T21:45:18.277135Z

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Observation 30be0819-9ea7-4ed4-a6ca-75c7a5a70ea1 · outbound

This paper cites Sample Variance Considerations for Cluster Surveys.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension Sample Variance Considerations for Cluster Surveys

Reference 38

Resolution: verified exact; local_arxiv, observed 2026-05-17T21:45:18.327535Z

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Observation e6f846d5-75ba-45e9-adf5-99f36a6221c0 · outbound

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Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension Unresolved cited work

Reference 39

Resolution: unresolved; raw_fallback, observed 2026-05-17T21:45:18.731120Z

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Observation 6a052227-2e05-4ba4-8788-d4b1e5ea7159 · outbound

This paper cites an unresolved cited work.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension Unresolved cited work

Reference 40

Resolution: unresolved; raw_fallback, observed 2026-05-17T21:45:18.728162Z

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Observation 1ad0984f-f926-4ed9-b89b-03c25a7bde70 · outbound

This paper cites The Effect of Surface Brightness Dimming in the Selection of High-z Galaxies.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension The Effect of Surface Brightness Dimming in the Selection of High-z Galaxies

Reference 41

Resolution: malformed identifier; local_arxiv, observed 2026-05-17T21:45:18.272835Z

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Pith citing papers

Observation 9bfb56f6-3c9e-473b-9a17-ae7efc18c3ba · inbound

Non-Primordial Contribution to the Cosmic Microwave Background cites this paper.

Non-Primordial Contribution to the Cosmic Microwave Background Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-02T02:52:20.210937Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.