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Paper Citation Record · LEDGER

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps

As of 15 August 2026, this Paper Citation Record lists 100 of 111 outbound references and 0 inbound Pith citation observations for arXiv:2509.07470.

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

pith.paper-citation-record.v1
2509.07470 v1

Coverage vector

measured 100 of 111 reference resolution

Typed states for the displayed outbound observations.

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measured 100 of 100 standing notices

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Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links

measured 0 of 1 external citation measurements

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Source: cited_works

Reference resolution

100 of 111 outbound references displayed

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External citation measurements

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Outbound references

Observation 03b74d13-2f99-43b7-bf21-fc9f5ef149fa · outbound

This paper cites an unresolved cited work.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Unresolved cited work

Reference 1

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Reference 2

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Reference 3

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Reference 4

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Reference 5

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Observation a52ed224-9226-49c5-8096-caef38512302 · outbound

This paper cites Symfind: Addressing the Fragility of Subhalo Finders and Revealing the Durability of Subhalos.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Symfind: Addressing the Fragility of Subhalo Finders and Revealing the Durability of Subhalos

Reference 6

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Observation 68624a0d-2bb2-453f-86fd-43d391d817fa · outbound

This paper cites Survivors and Zombies: The Quenching and Disruption of Satellites around Milky Way Analogs.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Survivors and Zombies: The Quenching and Disruption of Satellites around Milky Way Analogs

Reference 7

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Observation fc8986d1-9ecf-407b-9183-cd52cd8ae5ac · outbound

This paper cites Too big to fail? The puzzling darkness of massive Milky Way subhaloes.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Too big to fail? The puzzling darkness of massive Milky Way subhaloes

Reference 8

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Reference 9

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Observation fe04f7a7-65d7-490e-abe7-26b4027495a1 · outbound

This paper cites The central slope of dark matter cores in dwarf galaxies: Simulations vs. THINGS.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps The central slope of dark matter cores in dwarf galaxies: Simulations vs. THINGS

Reference 10

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Observation cb2bc591-b2ce-404f-85d6-8e7379a7e6e2 · outbound

This paper cites Moore, Evidence against dissipation-less dark matter from observations of galaxy haloes, Nature370(1994) 629.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Moore, Evidence against dissipation-less dark matter from observations of galaxy haloes, Nature370(1994) 629

Reference 11

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Observation ae7cd930-7137-45ed-8d17-c3dae928bc75 · outbound

This paper cites Observational and Theoretical Constraints on Singular Dark Matter Halos.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Observational and Theoretical Constraints on Singular Dark Matter Halos

Reference 12

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Observation 89b872a5-589f-403f-8d29-09bf92b3d1cb · outbound

This paper cites Review of solutions to the Cusp-core problem of the $\Lambda$CDM Model.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Review of solutions to the Cusp-core problem of the $\Lambda$CDM Model

Reference 13

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Reference 14

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Observation 1eb5c3c3-5a40-4be1-8634-95e97c5fed72 · outbound

This paper cites Baryons Matter: Why Luminous Satellite Galaxies Have Reduced Central Masses.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Baryons Matter: Why Luminous Satellite Galaxies Have Reduced Central Masses

Reference 15

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Observation cba7e913-65dd-41be-b66f-9610fd1b732c · outbound

This paper cites A unified solution to the small scale problems of the $\Lambda$CDM model.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps A unified solution to the small scale problems of the $\Lambda$CDM model

Reference 16

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Observation a3a546e4-55bd-4db7-a201-fe71eab4c0a1 · outbound

This paper cites Cosmological puzzle resolved by stellar feedback in high redshift galaxies.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Cosmological puzzle resolved by stellar feedback in high redshift galaxies

Reference 17

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Reference 18

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Observation b665a9e1-c774-430e-a704-4ca876d28313 · outbound

This paper cites The impact of dark matter cusps and cores on the satellite galaxy population around spiral galaxies.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps The impact of dark matter cusps and cores on the satellite galaxy population around spiral galaxies

Reference 19

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Observation d636b2aa-456a-4c35-b190-9a981090ff21 · outbound

This paper cites Dark matter halo cores and the tidal survival of Milky Way satellites.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Dark matter halo cores and the tidal survival of Milky Way satellites

Reference 20

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Reference 21

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Observation 75400ff7-3b22-4994-b6f4-38160d11ec47 · outbound

This paper cites Formation of Disk Galaxies: Warm Dark Matter and the Angular Momentum problem.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Formation of Disk Galaxies: Warm Dark Matter and the Angular Momentum problem

Reference 22

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Observation ca817071-4076-4345-8796-a36510fcbe3d · outbound

This paper cites Milgrom,A modification of the Newtonian dynamics - Implications for galaxies., Astrophys.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Milgrom,A modification of the Newtonian dynamics - Implications for galaxies., Astrophys

Reference 30

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Observation a6824610-1e56-4b82-9f71-ff08f5502b60 · outbound

This paper cites Milgrom, A modification of the Newtonian dynamics as a possible alternative to the hidden mass hypothesis., Astrophys.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Milgrom, A modification of the Newtonian dynamics as a possible alternative to the hidden mass hypothesis., Astrophys

Reference 31

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Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Unresolved cited work

Reference 32

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Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Unresolved cited work

Reference 33

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Reference 34

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Observation f1976d3b-c1c7-4a2c-815c-033717b4fa94 · outbound

This paper cites f(T) gravity mimicking dynamical dark energy. Background and perturbation analysis.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps f(T) gravity mimicking dynamical dark energy. Background and perturbation analysis

Reference 35

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Reference 36

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Observation bbed94c7-fc65-4b16-81ca-2ad7cbaa0eb1 · outbound

This paper cites Simulating Observations of Dark Matter Dominated Galaxies: Towards the Optimal Halo Profile.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Simulating Observations of Dark Matter Dominated Galaxies: Towards the Optimal Halo Profile

Reference 37

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Observation 7cb44542-01f3-4fd9-8ace-16f32cee3a8b · outbound

This paper cites The Inner Structure of LambdaCDM Halos I: A Numerical Convergence Study.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps The Inner Structure of LambdaCDM Halos I: A Numerical Convergence Study

Reference 38

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Observation 621b7e36-76a6-4943-aee0-34f5c9a23239 · outbound

This paper cites The dependence of dark matter profiles on the stellar to halo mass ratio: a prediction for cusps vs cores.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps The dependence of dark matter profiles on the stellar to halo mass ratio: a prediction for cusps vs cores

Reference 39

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Observation de6d4c86-fd25-49b8-9f01-15fa576ac21d · outbound

This paper cites NIHAO IV: Core creation and destruction in dark matter density profiles across cosmic time.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps NIHAO IV: Core creation and destruction in dark matter density profiles across cosmic time

Reference 40

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Observation 5cb0de0c-0d2e-4f1f-924d-4c00a9d0b3d5 · outbound

This paper cites The Impact of Baryonic Physics on the Structure of Dark Matter Halos: the View from the FIRE Cosmological Simulations.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps The Impact of Baryonic Physics on the Structure of Dark Matter Halos: the View from the FIRE Cosmological Simulations

Reference 41

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Observation 4a26859c-969f-46f0-80be-83c6b9d7eadb · outbound

This paper cites The formation of cores in galaxies across cosmic time -- the existence of cores is not in tension with the LCDM paradigm.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps The formation of cores in galaxies across cosmic time -- the existence of cores is not in tension with the LCDM paradigm

Reference 42

Resolution
verified exact
local_arxiv, observed 2026-08-04T22:14:34.798807Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

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Reference 43

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T22:14:25.688607Z digest=sha256:d85923320269f16dfc985fbda0ad0af81157d08c647bfc677904db5ac0bb50f0

Observation a0d5adfd-f79d-417c-80db-d110d5261681 · outbound

This paper cites No cores in dark matter-dominated dwarf galaxies with bursty star formation histories.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps No cores in dark matter-dominated dwarf galaxies with bursty star formation histories

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-04T22:14:25.783154Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Reference 45

Resolution
verified exact
local_arxiv, observed 2026-08-04T22:14:34.615127Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-04T22:14:25.828427Z digest=sha256:cb035d93b70eceb258d94f865b46c2fb4a77bb61111a7364e02c10fc05f18b67

Observation 2258ce61-a2c8-4970-a48b-92c77fef6a17 · outbound

This paper cites Cosmological simulations of the same spiral galaxy: the impact of baryonic physics.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Cosmological simulations of the same spiral galaxy: the impact of baryonic physics

Reference 46

Resolution
verified exact
local_arxiv, observed 2026-08-04T22:14:34.506778Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-04T22:14:25.888776Z digest=sha256:c79df977938497e3f577995ce4cd60d614b0c80a2e5f8e7731c6c3774a6a0782

Observation 4f7052ff-28dc-47ce-8440-a2a182c8e9a7 · outbound

This paper cites Hundreds of Milky Way Satellites? Luminosity Bias in the Satellite Luminosity Function.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Hundreds of Milky Way Satellites? Luminosity Bias in the Satellite Luminosity Function

Reference 47

Resolution
verified exact
local_arxiv, observed 2026-08-04T22:14:34.389406Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-04T22:14:25.957391Z digest=sha256:fc64efa21ebf598030cf02935a1c3b3279074dc5761e83b920bb1a6bdc0dbbcc

Observation d8fe9d9c-5280-413f-9c85-5b7e7cc52331 · outbound

This paper cites The observed properties of dwarf galaxies in and around the Local Group.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps The observed properties of dwarf galaxies in and around the Local Group

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-04T22:14:26.030796Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T22:14:26.030796Z digest=sha256:0b60cef3268c212eb640d26799ac599f8e34d3baedbff88a9c5d9f793f81391b

Observation 69ebc8bf-8f2a-4925-813d-acda47bd23d9 · outbound

This paper cites The cold dark matter content of Galactic dwarf spheroidals: no cores, no failures, no problem.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps The cold dark matter content of Galactic dwarf spheroidals: no cores, no failures, no problem

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-04T22:14:26.109625Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T22:14:26.109625Z digest=sha256:a0890eb3eb1f44cb792914ac0f5e2a40bfd0718c39f7e87d0a45d651f355aebf

Observation 2ab6ed86-4695-47a1-8d3c-ab924b822c7d · outbound

This paper cites Introducing the NewHorizon simulation: Galaxy properties with resolved internal dynamics across cosmic time.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Introducing the NewHorizon simulation: Galaxy properties with resolved internal dynamics across cosmic time

Reference 50

Resolution
verified exact
local_arxiv, observed 2026-08-04T22:14:34.308141Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

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Observation 4a0f07db-fecf-4662-8707-ce37971de69b · outbound

This paper cites The Auriga Project: the properties and formation mechanisms of disc galaxies across cosmic time.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps The Auriga Project: the properties and formation mechanisms of disc galaxies across cosmic time

Reference 51

Resolution
unresolved
no resolver link, observed 2026-08-04T22:14:26.214376Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T22:14:26.214376Z digest=sha256:16c9d9e58de5458ac0b62d0f655706048f296f8e44507c1eddbd7fdb55303a32

Observation fc813ea5-7017-47e3-bcd1-606e9329f4e3 · outbound

This paper cites Cosmological simulations of the same spiral galaxy: connecting the dark matter distribution of the host halo with the subgrid baryonic physics.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Cosmological simulations of the same spiral galaxy: connecting the dark matter distribution of the host halo with the subgrid baryonic physics

Reference 52

Resolution
verified exact
local_arxiv, observed 2026-08-04T22:14:34.232846Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-04T22:14:26.284339Z digest=sha256:39b45ce4e5ab1660e0fcf4681a05bd7be43d7aab9ec86cce3e88069ee137d600

Observation 2ae33934-bbfb-4034-bfaf-3c75236570ce · outbound

This paper cites Reconciling dwarf galaxies with LCDM cosmology: Simulating a realistic population of satellites around a Milky Way-mass galaxy.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Reconciling dwarf galaxies with LCDM cosmology: Simulating a realistic population of satellites around a Milky Way-mass galaxy

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-04T22:14:26.335029Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T22:14:26.335029Z digest=sha256:be9b7d375db69d91012fc24db7f9eda9b0e8cd8e17eefeda663a9e1ce5dd4680

Observation c61627ae-b7ee-4a1d-945e-9882ae53e971 · outbound

This paper cites Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-04T22:14:26.376812Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T22:14:26.376812Z digest=sha256:a7e6049208ab67ff9621aaf0dd8ee1c5e43f8249755cfa325436df70b8b93667

Observation 642a7e18-cae7-44ea-a4c6-93ab08e0548e · outbound

This paper cites MUSIC: MUlti-Scale Initial Conditions.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps MUSIC: MUlti-Scale Initial Conditions

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-04T22:14:26.449232Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T22:14:26.449232Z digest=sha256:d7ce189c6a02105f2d9f4b238c88a713d237e04430cb8b44a65f34eac140c95c

Observation de14d708-2ad6-4e7d-bbc3-5f4aff2ee1ff · outbound

This paper cites Baryonic and dark matter distribution in cosmological simulations of spiral galaxies.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Baryonic and dark matter distribution in cosmological simulations of spiral galaxies

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-04T22:14:26.484332Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T22:14:26.484332Z digest=sha256:7b87398db2d55fe5a6aabdebb07e6dec3ed45d50555e8c69217007f6ca2fcb2b

Observation a2d81ae1-b8d3-449e-893b-8b044c735afc · outbound

This paper cites The formation of disc galaxies in high resolution moving-mesh cosmological simulations.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps The formation of disc galaxies in high resolution moving-mesh cosmological simulations

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-04T22:14:26.547975Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T22:14:26.547975Z digest=sha256:d02fd60957627a6a323e677cb491656c5a9451d7b8dd95af992693552cbef3c4

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-04T22:14:26.618389Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T22:14:26.618389Z digest=sha256:02939ecbebfafbe0f06d7161a63e3db1450476b7bd03ae5160fc936dd038c3f1

Observation 000fd476-5fb0-40a0-ba6c-20656acc7678 · outbound

This paper cites Cusp-core transformations in dwarf galaxies: observational predictions.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Cusp-core transformations in dwarf galaxies: observational predictions

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-04T22:14:26.681388Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T22:14:26.681388Z digest=sha256:7774583b33b415911385cef6cdce1ea585a4950623a4a34ea1b616d2ae3d7455

Observation 2774d003-0ee6-484b-a7e9-e43e8f5985f2 · outbound

This paper cites The Star Formation Rate of Turbulent Magnetized Clouds: Comparing Theory, Simulations, and Observations.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps The Star Formation Rate of Turbulent Magnetized Clouds: Comparing Theory, Simulations, and Observations

Reference 60

Resolution
unresolved
no resolver link, observed 2026-08-04T22:14:26.766341Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T22:14:26.766341Z digest=sha256:2aa4fc4ef308485cc5d522ec992d0685023199d33d4f445e0477e8ed41ea7b4e

Observation 53bb8b88-bd3c-4351-a985-d8f0de4a373d · outbound

This paper cites A General Theory of Turbulence-Regulated Star Formation, From Spirals to ULIRGs.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps A General Theory of Turbulence-Regulated Star Formation, From Spirals to ULIRGs

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-04T22:14:26.832649Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T22:14:26.832649Z digest=sha256:44b2d552f60935c3f40f3cba87ddec36e5390e0cdac6df5a3c2a8e2f9906c857

Observation 7415da3b-8413-4cb3-a50b-288e63f9190a · outbound

This paper cites Towards simulating star formation in turbulent high-z galaxies with mechanical supernova feedback.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Towards simulating star formation in turbulent high-z galaxies with mechanical supernova feedback

Reference 62

Resolution
verified exact
local_arxiv, observed 2026-08-04T22:14:34.055757Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

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Observation cc52009b-d7da-414a-9c9c-d319cd851751 · outbound

This paper cites SKIRT: an Advanced Dust Radiative Transfer Code with a User-Friendly Architecture.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps SKIRT: an Advanced Dust Radiative Transfer Code with a User-Friendly Architecture

Reference 63

Resolution
unresolved
no resolver link, observed 2026-08-04T22:14:26.969024Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T22:14:26.969024Z digest=sha256:3a540e08673a03547df9e070c9d01eaaa541f97817fb634df469a8be65bc0271

Reference 64

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no resolver link, observed 2026-08-04T22:14:27.033314Z

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source=pdf_text observed=2026-08-04T22:14:27.033314Z digest=sha256:ff5a4e6642c0d7718e8604eb745fa382cb78105b3a6318babca4f0c3a375e0c2

Observation 58151c09-1ad0-418a-84b3-2edb3a977ce6 · outbound

This paper cites Binney and S.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Binney and S

Reference 65

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unresolved
no resolver link, observed 2026-08-04T22:14:27.144679Z

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Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T22:14:27.144679Z digest=sha256:bf07ef7b3fa1159dbce4dae2a05553466f44099fbe6c126b0f19c5ca995b0f0b

Observation 81bed3bd-68af-46bc-9469-37216a9fafd7 · outbound

This paper cites an unresolved cited work.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Unresolved cited work

Reference 66

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unresolved
no resolver link, observed 2026-08-04T22:14:27.180562Z

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Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T22:14:27.180562Z digest=sha256:0c921081ecb60f634a47135f1219840a40d458cc274b9e38b17ba08f473baa00

Reference 67

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unresolved
no resolver link, observed 2026-08-04T22:14:27.251065Z

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Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T22:14:27.251065Z digest=sha256:d61082a55cb5895a15dfcc2eae5a0fea2779f4aef49ba48eea231947925dba11

Reference 68

Resolution
verified exact
local_arxiv, observed 2026-08-04T22:14:33.946678Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-04T22:14:27.319497Z digest=sha256:af53ea417ba1f86216afbdfcbf466d2e29b171e2babdcb5734c7451230ec49ff

Observation 00edd97e-8028-4936-99af-3031492107e2 · outbound

This paper cites Rockstar: Phase-space halo finder.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Rockstar: Phase-space halo finder

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-04T22:14:27.385338Z

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source=pdf_text observed=2026-08-04T22:14:27.385338Z digest=sha256:6e2ff3e50702af772926a76116e24ff5f4135b446055dc6ed456b2e9f4d3c677

Reference 70

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verified exact
arxiv_id, observed 2026-08-04T22:14:33.820945Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

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Reference 71

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unresolved
no resolver link, observed 2026-08-04T22:14:27.518794Z

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source=pdf_text observed=2026-08-04T22:14:27.518794Z digest=sha256:de9a23be2604927eed5ab3f002a885b8021a6f8b1d141a2eba02347f6d6267e8

Reference 72

Resolution
verified exact
local_arxiv, observed 2026-08-04T22:14:33.727896Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-04T22:14:27.603294Z digest=sha256:eb227ac068740b7f87a6d907c8a0a7de32b0fef352a21c28ee6a9186319bd26c

Observation 2c2caa32-2ce2-4b32-a99a-99a97af7379a · outbound

This paper cites Systematics in virial mass estimators for pressure-supported systems.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Systematics in virial mass estimators for pressure-supported systems

Reference 73

Resolution
unresolved
no resolver link, observed 2026-08-04T22:14:27.678621Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T22:14:27.678621Z digest=sha256:6f0a35d3eb20cf535aceef23f079d80caa0f4bd21f6fa58191d16598b23891ca

Observation 1a9f96b8-e0cd-4460-81bd-95fda80059f3 · outbound

This paper cites Milky Way Satellite Census. II. Galaxy--Halo Connection Constraints Including the Impact of the Large Magellanic Cloud.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Milky Way Satellite Census. II. Galaxy--Halo Connection Constraints Including the Impact of the Large Magellanic Cloud

Reference 74

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unresolved
no resolver link, observed 2026-08-04T22:14:27.721044Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T22:14:27.721044Z digest=sha256:b7b0fb9bcbd4cb0aec45ebc29128e4ad0c5a2e86a461a57f1746abd2f540ed58

Observation e6b3d842-3b63-4e8f-afa9-e78cbd4dcff0 · outbound

This paper cites The Average Star Formation Histories of Galaxies in Dark Matter Halos from z=0-8.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps The Average Star Formation Histories of Galaxies in Dark Matter Halos from z=0-8

Reference 75

Resolution
unresolved
no resolver link, observed 2026-08-04T22:14:27.835363Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T22:14:27.835363Z digest=sha256:227270403cf9c09cfc62844471d4ba66759dbcb4e47fa7ab2833d010fadccfa5

Observation 332795c8-b2f5-4436-972d-ca8d07520403 · outbound

This paper cites Constraints on the relationship between stellar mass and halo mass at low and high redshift.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Constraints on the relationship between stellar mass and halo mass at low and high redshift

Reference 76

Resolution
unresolved
no resolver link, observed 2026-08-04T22:14:27.870335Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T22:14:27.870335Z digest=sha256:b686301b96d81f866a0bb69b3d742c92ace045e013764814fb53a42ab0742f3a

Observation f412e671-912f-44e4-a155-4a0a85261459 · outbound

This paper cites ELVES IV: The Satellite Stellar-to-Halo Mass Relation Beyond the Milky-Way.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps ELVES IV: The Satellite Stellar-to-Halo Mass Relation Beyond the Milky-Way

Reference 77

Resolution
verified exact
local_arxiv, observed 2026-08-04T22:14:33.588452Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-04T22:14:27.953938Z digest=sha256:270075f9564648e92199a257b301fc71c3758a041ac2a0f3333de0a9f523c726

Reference 78

Resolution
verified exact
local_arxiv, observed 2026-08-04T22:14:33.470874Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-04T22:14:28.009081Z digest=sha256:0dd8dc3d4f083f2bfef44fadd35b1e6577aa86c2f80269c82a3a7df9be967d64

Observation d378c763-36c1-4336-b25f-6c6cd6877d2e · outbound

This paper cites Ultra-faint dwarfs in a Milky Way context: Introducing the Mint Condition DC Justice League Simulations.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Ultra-faint dwarfs in a Milky Way context: Introducing the Mint Condition DC Justice League Simulations

Reference 79

Resolution
verified exact
local_arxiv, observed 2026-08-04T22:14:33.327792Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-04T22:14:28.069243Z digest=sha256:bc262ee01117edf8cb982e67fdd4542e7336c2aee0db6e3a8e954423193c6c20

Observation 903362c7-3df9-445c-890d-a646e3c67864 · outbound

This paper cites Formation and evolution of galaxy dark matter halos and their substructure.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Formation and evolution of galaxy dark matter halos and their substructure

Reference 80

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Observation 413931b7-e8da-444e-a267-a01c8c738e8b · outbound

This paper cites an unresolved cited work.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Unresolved cited work

Reference 81

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Observation a8c9c723-171f-454b-80f8-8e18377e1938 · outbound

This paper cites an unresolved cited work.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Unresolved cited work

Reference 82

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Observation e2befb3f-88e0-496d-9cd3-612adaf2503e · outbound

This paper cites an unresolved cited work.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Unresolved cited work

Reference 83

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Reference 84

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Reference 85

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Observation 08a16614-81da-48e4-8ca6-b8845ea614a0 · outbound

This paper cites The Excursion Set Theory of Halo Mass Functions, Halo Clustering, and Halo Growth.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps The Excursion Set Theory of Halo Mass Functions, Halo Clustering, and Halo Growth

Reference 86

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Reference 87

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verified exact
local_arxiv, observed 2026-08-04T22:14:33.202674Z

Source-reported events for the cited work

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Reference 88

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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

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Observation f3486b0d-d68c-426c-9568-e46aa41ae6c3 · outbound

This paper cites At the heart of the matter: the origin of bulgeless dwarf galaxies and Dark Matter cores.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps At the heart of the matter: the origin of bulgeless dwarf galaxies and Dark Matter cores

Reference 89

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Reference 90

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Reference 91

Resolution
verified exact
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No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

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Observation f2e56460-4cf3-4b43-bb7a-a5369916bb31 · outbound

This paper cites A model for core formation in dark matter haloes and ultra diffuse galaxies by outflow episodes.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps A model for core formation in dark matter haloes and ultra diffuse galaxies by outflow episodes

Reference 92

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verified exact
local_arxiv, observed 2026-08-04T22:14:32.765825Z

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No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

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Reference 93

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local_arxiv, observed 2026-08-04T22:14:32.598484Z

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No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

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Reference 94

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unresolved
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Reference 95

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Reference 96

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Observation bca63428-90e5-4838-99cd-cbff47fda05f · outbound

This paper cites Core Formation in High-z Massive Haloes: Heating by Post Compaction Satellites and Response to AGN Outflows.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Core Formation in High-z Massive Haloes: Heating by Post Compaction Satellites and Response to AGN Outflows

Reference 97

Resolution
verified exact
local_arxiv, observed 2026-08-04T22:14:32.376027Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

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Reference 98

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verified exact
local_arxiv, observed 2026-08-04T22:14:32.209249Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

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Observation a5db569e-ba68-4a4f-a12c-24d7aa0988d9 · outbound

This paper cites The Star Formation Histories of Local Group Dwarf Galaxies I. Hubble Space Telescope / Wide Field Planetary Camera 2 Observations.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps The Star Formation Histories of Local Group Dwarf Galaxies I. Hubble Space Telescope / Wide Field Planetary Camera 2 Observations

Reference 99

Resolution
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Source-reported events for the cited work

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Observation b62a2dda-a56c-4d7a-88b7-19198612d987 · outbound

This paper cites Formation of ultra-diffuse galaxies in the field and in galaxy groups.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Formation of ultra-diffuse galaxies in the field and in galaxy groups

Reference 100

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Pith citing papers

No inbound Pith citation observations are available.