Paper Citation Record · LEDGER

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters

As of 21 August 2026, this Paper Citation Record lists 40 of 40 outbound references and 0 inbound Pith citation observations for arXiv:2607.15339.

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pith.paper-citation-record.v1
2607.15339 v1

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measured 40 of 40 reference resolution

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Outbound references

Observation cdad05f7-b9fc-49e8-8e49-0d93074c61f7 · outbound

This paper cites The Structure of Cold Dark Matter Halos.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters The Structure of Cold Dark Matter Halos

Reference 1

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Observation 66827c18-1721-4f3a-8534-a8e96b60467c · outbound

This paper cites A Universal Density Profile from Hierarchical Clustering.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters A Universal Density Profile from Hierarchical Clustering

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:54.233865Z

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Observation 09cc33eb-96f1-4321-97cf-e91f29061b8c · outbound

This paper cites The distribution of dark matter in galaxies.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters The distribution of dark matter in galaxies

Reference 3

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Observation 31e104a6-9afb-4a29-8e94-67b00172a3a3 · outbound

This paper cites Galaxy Groups.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters Galaxy Groups

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:54.472285Z

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Observation 8519640f-b2cd-4792-8827-edcd8689cab3 · outbound

This paper cites Stellar mass-to-light ratios and the Tully-Fisher relation.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters Stellar mass-to-light ratios and the Tully-Fisher relation

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:54.583238Z

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Observation d51685d3-7a1a-4d41-bf12-fce51136ea20 · outbound

This paper cites an unresolved cited work.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters Unresolved cited work

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:54.682803Z

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Observation 6a815c92-eede-463c-a929-24a091d38765 · outbound

This paper cites Heisler, S.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters Heisler, S

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:54.791776Z

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Observation feaba217-aa0d-4080-91f9-e149fac7de32 · outbound

This paper cites The Masses of the Milky Way and Andromeda galaxies.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters The Masses of the Milky Way and Andromeda galaxies

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:54.979472Z

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Observation 4483eae6-7181-4fd2-b319-74012e71afdf · outbound

This paper cites The frozen outskirts: a cold Hubble flow and the mass of the Local Group.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters The frozen outskirts: a cold Hubble flow and the mass of the Local Group

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:55.179376Z

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Observation 4ef96b82-8296-42fa-8c5d-a6eb857fc890 · outbound

This paper cites Applying scale-free mass estimators to the Local Group in Constrained Local Universe Simulations.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters Applying scale-free mass estimators to the Local Group in Constrained Local Universe Simulations

Reference 11

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Observation 7b51be3c-0632-4150-8112-41a3b6ebbd9e · outbound

This paper cites First Results from the TNG50 Simulation: The evolution of stellar and gaseous disks across cosmic time.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters First Results from the TNG50 Simulation: The evolution of stellar and gaseous disks across cosmic time

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:55.787920Z

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Observation 298bdf8b-4a78-41ae-9955-e1aae7e14e83 · outbound

This paper cites Prediction of galaxy halo masses in SDSS DR7 via a machine learning approach.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters Prediction of galaxy halo masses in SDSS DR7 via a machine learning approach

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:55.943017Z

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Observation 4dcdf6ae-f5cf-485c-b1d9-b0a7cd711702 · outbound

This paper cites The mass of the Milky Way from satellite dynamics.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters The mass of the Milky Way from satellite dynamics

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:56.100845Z

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Observation eaabf89b-eda7-48bc-aa5d-8d1b2ba255b0 · outbound

This paper cites Line-of-sight mass estimator and the masses of the Milky Way and Andromeda Galaxy.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters Line-of-sight mass estimator and the masses of the Milky Way and Andromeda Galaxy

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:56.255781Z

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Observation afbb9e3b-f93e-40fc-82df-fbc6377144a7 · outbound

This paper cites Properties of galaxies reproduced by a hydrodynamic simulation.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters Properties of galaxies reproduced by a hydrodynamic simulation

Reference 16

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Observation 6b2ac3fa-729e-42b8-9c66-78767599b19b · outbound

This paper cites The Illustris Simulation: Public Data Release.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters The Illustris Simulation: Public Data Release

Reference 17

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Observation 431ee8ea-6dd1-486d-a031-fd15470fb052 · outbound

This paper cites First Results from the TNG50 Simulation: Galactic outflows driven by supernovae and black hole feedback.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters First Results from the TNG50 Simulation: Galactic outflows driven by supernovae and black hole feedback

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:56.670944Z

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Observation b9ffbe56-17dd-4955-93d5-327248ab41dc · outbound

This paper cites Populating a cluster of galaxies - I. Results at z=0.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters Populating a cluster of galaxies - I. Results at z=0

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:56.847048Z

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Observation c6afce7a-c9de-4c10-887c-56d29d1c5d1e · outbound

This paper cites Sandage, Astrophys.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters Sandage, Astrophys

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:56.999112Z

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Observation 48cddf82-a7ff-4fa2-b29c-edfc175c99b9 · outbound

This paper cites The Orbital Ellipticity of Satellite Galaxies and the Mass of the Milky Way.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters The Orbital Ellipticity of Satellite Galaxies and the Mass of the Milky Way

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:57.175254Z

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Observation f44496d5-9b18-4c6c-bcc9-1234371c4f9f · outbound

This paper cites an unresolved cited work.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters Unresolved cited work

Reference 22

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Observation f21c9eb3-a68b-4d3a-b578-6c987d8cbd10 · outbound

This paper cites Goodfellow, Y.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters Goodfellow, Y

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:57.419804Z

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Observation de8ba6ab-8c63-4190-8991-7efa08f93a18 · outbound

This paper cites Using X-Ray Morphological Parameters to Strengthen Galaxy Cluster Mass Estimates via Machine Learning.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters Using X-Ray Morphological Parameters to Strengthen Galaxy Cluster Mass Estimates via Machine Learning

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:57.600085Z

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Observation 42e1f43b-a09f-467f-8db8-2dad2a60cfa4 · outbound

This paper cites an unresolved cited work.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters Unresolved cited work

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:57.740042Z

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Observation 3db0d424-f3e7-4a03-94f2-550469a638cf · outbound

This paper cites Adam: A Method for Stochastic Optimization.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters Adam: A Method for Stochastic Optimization

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:57.852996Z

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Observation a2a4b941-2e5b-40d1-bd76-8b45379a51aa · outbound

This paper cites A Comprehensive Analysis of Uncertainties Affecting the Stellar Mass - Halo Mass Relation for 0<z<4.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters A Comprehensive Analysis of Uncertainties Affecting the Stellar Mass - Halo Mass Relation for 0<z<4

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:57.970064Z

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Observation 3912d99a-97fe-4eb9-8891-f841602a0d7a · outbound

This paper cites The EAGLE project: Simulating the evolution and assembly of galaxies and their environments.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters The EAGLE project: Simulating the evolution and assembly of galaxies and their environments

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:58.080876Z

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Observation ee3273b7-b4f2-401a-9f44-424365bf88d7 · outbound

This paper cites Simulating Galaxy Formation with the IllustrisTNG Model.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters Simulating Galaxy Formation with the IllustrisTNG Model

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:58.201598Z

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Observation d3a5c739-d851-42b4-9fb4-9d4d700bfca9 · outbound

This paper cites Green Valley Galaxies.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters Green Valley Galaxies

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:58.316773Z

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Observation 11c6ba01-e306-41c1-8dec-45caf458712b · outbound

This paper cites Snake in the Clouds: A new nearby dwarf galaxy in the Magellanic bridge.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters Snake in the Clouds: A new nearby dwarf galaxy in the Magellanic bridge

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:58.449239Z

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Observation e3ebd8d6-7311-419d-a0b0-d48389b5de46 · outbound

This paper cites Wagner, D.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters Wagner, D

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:58.650391Z

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Observation 5f6d2986-bc3f-449d-92b3-b38483759a68 · outbound

This paper cites Antoine, A.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters Antoine, A

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:58.808059Z

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Observation 3be6132d-99ad-4ad2-8e38-eaf875ef3b27 · outbound

This paper cites Stellar and dark matter density in the Local Universe.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters Stellar and dark matter density in the Local Universe

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:58.958773Z

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Observation 92090e23-67b6-4546-b2e7-e19288cef8e2 · outbound

This paper cites Tracing the Local Volume galaxy halo-to-stellar mass ratio with satellite kinematics.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters Tracing the Local Volume galaxy halo-to-stellar mass ratio with satellite kinematics

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:59.142676Z

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Observation 724857b2-b509-4143-9b11-c58e033fef13 · outbound

This paper cites Chandra and XMM-Newton Detection of Large-scale Diffuse X-ray Emission from the Sombrero Galaxy.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters Chandra and XMM-Newton Detection of Large-scale Diffuse X-ray Emission from the Sombrero Galaxy

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:59.342922Z

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Observation c963a2c8-d4d6-4899-9754-ea2ce4498244 · outbound

This paper cites NGC 5128: The Giant Beneath.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters NGC 5128: The Giant Beneath

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:59.515137Z

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Observation 878a5fa5-3f5d-4392-a381-0c42fec050c4 · outbound

This paper cites Mass and shape of the Milky Way's dark matter halo with globular clusters from Gaia and Hubble.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters Mass and shape of the Milky Way's dark matter halo with globular clusters from Gaia and Hubble

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:59.578732Z

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Observation c34d8e15-54a3-4236-8966-537c7fc649d7 · outbound

This paper cites No Routing Needed Between Capsules.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters No Routing Needed Between Capsules

Reference 39

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Observation 5099af4c-28fa-4f3d-9db9-974b19d91e49 · outbound

This paper cites The Milky Way's plane of satellites: consistent with $\Lambda$CDM.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters The Milky Way's plane of satellites: consistent with $\Lambda$CDM

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:59.759754Z

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Observation d334f90a-f5da-4f70-b71d-390dcdad0125 · outbound

This paper cites The Local Group Mass in the light of Gaia.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters The Local Group Mass in the light of Gaia

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:59.820037Z

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