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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 20 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

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measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

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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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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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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 2026-08-20T06:33:59.587034+00:00.

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Reference 43

Resolution
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no resolver link, observed 2026-08-04T22:14:25.688607Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T22:14:25.688607Z digest=sha256:96562295ff19c13f0d3b36122037e37cfe75202f8b6a836029b12c89fe9255c6

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

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source=pdf_text observed=2026-08-04T22:14:25.783154Z digest=sha256:2328b19c9052cd5333965e7c2a588805891b85967b0d4b7e008f4051c402634d

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 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-08-04T22:14:25.828427Z digest=sha256:0ea4a5088641970efc680b6dcd2fe1d03f3f00a96a7fc06b8a7a774e912cfd44

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 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-08-04T22:14:25.888776Z digest=sha256:cae574b100536f3691965217bf26c19e45dadd00fdf2e00c7634f66d1ee24b9a

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 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-08-04T22:14:25.957391Z digest=sha256:8ec18fb86c094e74b45bdabd6f0914dcbc1f8ca16fa0366006bb93bfa28e1db3

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:cde91a23da5b8b03e687e80cf17fc12e53da6fd729da019cc6aa64b39de93208

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:db0a9b2aeca5bbe097a2e210e7b59ac996d86bb67e05e1907616283f28d20b38

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 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-08-04T22:14:26.146015Z digest=sha256:a14d1de62f45bd26e13b3f1e74263a1364fc22ace29dbf2a93781af199598527

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=sha256:20129afbb702a23d1f66c1f649b867e82b3d7edf5d3b49de9ae0b6ff61f7b741

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 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-08-04T22:14:26.284339Z digest=sha256:9468ea66392a1fa6b588c7ae0b4eb52480e8a3d9491c0307b213b39b40611ead

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:fc5b267aa04f5535deba6611be190ea6cb7baae5d0863f6973dc9d8f2adf5341

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:d0ae72fce710303f233de289591048a4f81b42746ade663baa52dd7a5cdab375

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

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source=pdf_text observed=2026-08-04T22:14:26.449232Z digest=sha256:c55a679fc22f636f9b716c3ce8dc7496d1ec5b964e0af085bf0a08cbb848c115

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=sha256:2925b6d14f98265a5adeda64695abaa18eea0d8a9aeb3fef7dffb9abeab7de9c

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=sha256:119c70f4edcfaa9c23ed35bd73d315c2b458dd3bee9bef646a6eb1e971439ffc

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:fceed8ec437803d2073461032b583d99ce3dd8340e2e3b5d23545cd6cfff230b

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:d00f65ca4af9c5abc46212c8b9355a483db16050cc79ed70330f0d2ad3f22ef5

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=sha256:9a429b60a74ff415b3904732fad994cc535effffcb540c259e591eeae4f3ba45

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=sha256:32f60e5a5d4c3e2aca4a04aa67f5efa5107844dc3fe1d38df0254e251c73b221

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 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-08-04T22:14:26.905956Z digest=sha256:e955d75ddfa82ed2fd8400922f294dcd7c73382b9af1d2c527e81b23205432dc

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

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Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T22:14:26.969024Z digest=sha256:6f189f83dd259c82354d11e4a4aaaaa90a46188b73a926f2f117aec39fe74fae

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=sha256:0cf82baa15a71267f6cb45c8645a36b2cefbd83d35408fe99a80f889d6989c2e

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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source=pdf_text observed=2026-08-04T22:14:27.144679Z digest=sha256:b51c6bd1ab9b3f098f63712d5a527e160aa857bf78a550c398b60c08239cd825

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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source=pdf_text observed=2026-08-04T22:14:27.180562Z digest=sha256:ff018b4acb1904d1d4e17c861ea6b192224f2ff2541fba1491ca3c7ab2c83c51

Reference 67

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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:a8f4aaaeec43e4361f9fbd3bb797b87b46f968348091a3e56ea4b1934486574a

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 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-08-04T22:14:27.319497Z digest=sha256:20f27bc21e6fa5eda8fdb3b5e63000d702dec39a2eb12cc2b0a3805354cd6685

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=sha256:11fcd3b888a732f0bd97c2dd971e20ef24eb58b01b500c21ea1053d7e96c6c88

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 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-08-04T22:14:27.459771Z digest=sha256:6b05bba22da7d412970cbff0afe69e0849efa6873fc69e56cb52de647a9bfe8f

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:e424721f857a2b8ac600e78d54ce82664908effa4a525a186187542d19393731

Reference 72

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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 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-08-04T22:14:27.603294Z digest=sha256:b528fe14a4a3c2ce3a6995d52b458530eb31d4999ecd1102cd10776f6b00fede

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:a3f90fa279320a2ea2c708d340261d52b794550885e02632fe1552a37582126f

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

Resolution
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:ee04ffac14667ca8442a8a5aaab47bfc8ca34d160b2daeb3d20214a3dd035314

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:f27746252e3355c5641681aa607a67d839923292f9f75633803e567881a7cc42

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:be586f9d71436532c3e552a459b7e18d6c5c22de9a27f638e4b088369911672f

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 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-08-04T22:14:27.953938Z digest=sha256:0956e7e2642020389d92bcbab67d1269872bd4bfa7801d047a02640e5c2ef8e2

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 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-08-04T22:14:28.009081Z digest=sha256:944a08d8ff7b1e81b7200200c6bd8c87907a9655504648ed0e6af1fd43df1a1c

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 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-08-04T22:14:28.069243Z digest=sha256:606e7a41ba78f7a183c2e3e441af39e86a9ac848eb40c3e24d86f2f5b8ee42f2

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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unresolved
no resolver link, observed 2026-08-04T22:14:28.072325Z

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Unavailable: canonical work link unavailable.

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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 81

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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 82

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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

Resolution
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Reference 87

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No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Reference 88

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No event found in the named queried sources as of 2026-08-20T06:33:59.587034+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

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verified exact
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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

Resolution
verified exact
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No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Reference 93

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verified exact
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No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Reference 94

Resolution
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Source-reported events for the cited work

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Reference 95

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Reference 96

Resolution
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Source-reported events for the cited work

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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
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Reference 98

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Source-reported events for the cited work

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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

Unavailable: canonical work link unavailable.

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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.