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Paper Citation Record · LEDGER

Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 57 inbound Pith citation observations for arXiv:astro-ph/9710107.

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pith.paper-citation-record.v1
astro-ph/9710107 v1

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Pith citing papers itemized under the disclosed page cap.

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Source: pith, observed 2026-07-04T14:19:54.112724Z

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External citation measurements

2000
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Pith citing papers

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Imprints of energy injection by compact dark stars in the 21-cm signal cites this paper.

Imprints of energy injection by compact dark stars in the 21-cm signal Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 71

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SHAPE: cosmology with cluster halo intrinsic alignments from subhalo distributions cites this paper.

SHAPE: cosmology with cluster halo intrinsic alignments from subhalo distributions Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 69

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Cosmology with Galaxy Clusters cites this paper.

Cosmology with Galaxy Clusters Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 23

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CSST Cosmological Emulator II: Generalized Accurate Halo Mass Function Emulation cites this paper.

CSST Cosmological Emulator II: Generalized Accurate Halo Mass Function Emulation Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 82

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Differentiable Halo Mass Prediction and the Cosmology-Dependence of Halo Mass Functions cites this paper.

Differentiable Halo Mass Prediction and the Cosmology-Dependence of Halo Mass Functions Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 27

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Missing baryons recovered: a measurement of the gas fraction in galaxies and groups with the kinematic Sunyaev-Zel'dovich effect and CMB lensing cites this paper.

Missing baryons recovered: a measurement of the gas fraction in galaxies and groups with the kinematic Sunyaev-Zel'dovich effect and CMB lensing Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 47

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Where does non-Universality in Assembly Bias come from? cites this paper.

Where does non-Universality in Assembly Bias come from? Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 70

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Observation b6b818a8-d3be-417c-ae18-5856aa028ce9 · inbound

COLIBRE: calibrating subgrid feedback in cosmological simulations that include a cold gas phase cites this paper.

COLIBRE: calibrating subgrid feedback in cosmological simulations that include a cold gas phase Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 24

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Constraining Gas Mass Fractions in Galaxy Groups and Clusters with the First CHIME/FRB Outrigger cites this paper.

Constraining Gas Mass Fractions in Galaxy Groups and Clusters with the First CHIME/FRB Outrigger Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 18

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The evolution of the galaxy stellar mass function and star formation rates in the COLIBRE simulations from redshift 17 to 0 cites this paper.

The evolution of the galaxy stellar mass function and star formation rates in the COLIBRE simulations from redshift 17 to 0 Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 25

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Spectral Uniformity of Little Red Dots: A Natural Outcome of Coevolving Seed Black Holes and Nascent Starbursts cites this paper.

Spectral Uniformity of Little Red Dots: A Natural Outcome of Coevolving Seed Black Holes and Nascent Starbursts Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 10

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Impact of projection-induced optical selection bias on the weak lensing mass calibration of galaxy clusters cites this paper.

Impact of projection-induced optical selection bias on the weak lensing mass calibration of galaxy clusters Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 65

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Strong-lensing Perturber Signatures in Self-interacting Dark Matter Simulations cites this paper.

Strong-lensing Perturber Signatures in Self-interacting Dark Matter Simulations Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 68

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FOGGIE: Figuring Out Gas & Galaxies In Enzo XII. The Formation and Evolution of Extended HI Galactic Disks and Warps with a Dynamic Circumgalactic medium cites this paper.

FOGGIE: Figuring Out Gas & Galaxies In Enzo XII. The Formation and Evolution of Extended HI Galactic Disks and Warps with a Dynamic Circumgalactic medium Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 9

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The Broken Similarity: Sinking and Merging of Dark Matter Subhalos Across Hierarchical Levels cites this paper.

The Broken Similarity: Sinking and Merging of Dark Matter Subhalos Across Hierarchical Levels Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 48

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Inferring Halo Mass and Scale Radius of Galaxy Clusters Using Convolutional Neural Networks and Uchuu-UniverseMachine Catalogs cites this paper.

Inferring Halo Mass and Scale Radius of Galaxy Clusters Using Convolutional Neural Networks and Uchuu-UniverseMachine Catalogs Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 11

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Measuring neutrino mass and asymmetry through galaxy pairwise peculiar velocity cites this paper.

Measuring neutrino mass and asymmetry through galaxy pairwise peculiar velocity Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 45

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The Thermodynamic and Kinematic Evolution of Circumgalactic Gas around $z=1$ in the IllustrisTNG model cites this paper.

The Thermodynamic and Kinematic Evolution of Circumgalactic Gas around $z=1$ in the IllustrisTNG model Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

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Beyond Cloud-9: The case for discovering more HI-rich failed halos cites this paper.

Beyond Cloud-9: The case for discovering more HI-rich failed halos Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 9

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Anisotropy of Cosmic Background Photons from Annihilating/Decaying Dark Matter cites this paper.

Anisotropy of Cosmic Background Photons from Annihilating/Decaying Dark Matter Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 60

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NEFERTITI: Linking early galaxy formation to the assembly of the Milky Way cites this paper.

NEFERTITI: Linking early galaxy formation to the assembly of the Milky Way Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 170

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Non-Equilibrium Ionisation in Photoionised Haloes: Implications for Shock Stability and Absorption-Line Signatures cites this paper.

Non-Equilibrium Ionisation in Photoionised Haloes: Implications for Shock Stability and Absorption-Line Signatures Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

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Euclid preparation. CosmoPostProcess: A simulation calibrated framework for weak lensing selection bias in richness-selected galaxy clusters cites this paper.

Euclid preparation. CosmoPostProcess: A simulation calibrated framework for weak lensing selection bias in richness-selected galaxy clusters Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

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A statistical look on kinematic planes of satellite galaxies II: The physics behind their early formation in TNG50 MW/M31-like galaxies cites this paper.

A statistical look on kinematic planes of satellite galaxies II: The physics behind their early formation in TNG50 MW/M31-like galaxies Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 220

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An Inverse-Compton-Boosted Cool Core Unifies Perseus's Radio and X-ray Halos cites this paper.

An Inverse-Compton-Boosted Cool Core Unifies Perseus's Radio and X-ray Halos Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 39

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The Simulated Oxygen Shortage (SOS): Mapping the Missing OVI in Simulated Dwarf Galaxies to Subgrid Physics cites this paper.

The Simulated Oxygen Shortage (SOS): Mapping the Missing OVI in Simulated Dwarf Galaxies to Subgrid Physics Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 94

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Bulgeless Evolution And the Rise of Discs (BEARD) III. A numerical simulation view of satellites around Milky-Way analogues cites this paper.

Bulgeless Evolution And the Rise of Discs (BEARD) III. A numerical simulation view of satellites around Milky-Way analogues Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

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How High-Specific-Energy Winds Regulate the Circumgalactic Medium of Dwarf Galaxies cites this paper.

How High-Specific-Energy Winds Regulate the Circumgalactic Medium of Dwarf Galaxies Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 13

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The Splashback Mass Function of Galaxy Clusters from Photometric Data cites this paper.

The Splashback Mass Function of Galaxy Clusters from Photometric Data Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 10

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The AGORA High-resolution Galaxy Simulations Comparison Project. XI: Solving the Non-Spherical Morphology and Evolution of Dark Matter Halos with Haskap Pie cites this paper.

The AGORA High-resolution Galaxy Simulations Comparison Project. XI: Solving the Non-Spherical Morphology and Evolution of Dark Matter Halos with Haskap Pie Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 10

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Hierarchical assembly in action: a galaxy tail from a disrupting group in the Virgo cluster outskirts cites this paper.

Hierarchical assembly in action: a galaxy tail from a disrupting group in the Virgo cluster outskirts Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 229

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The impact of source and survey modelling on the connection between [O III] emitters and Ly $\alpha$ forest transmission at z ~ 6 cites this paper.

The impact of source and survey modelling on the connection between [O III] emitters and Ly $\alpha$ forest transmission at z ~ 6 Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 92

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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.

source=arxiv_source observed=2026-06-28T08:30:12.037696Z digest=sha256:b46c85245d953cf73a640d8d693c42f24d231089276350566cf73d62d56ec8ba

Observation 88147a94-15dc-4b90-b089-5d9d49c8cd8d · inbound

Cooler Phases of the Circumgalactic Medium Are More Centrally Concentrated: Constraints from Multiphase Absorption Lines cites this paper.

Cooler Phases of the Circumgalactic Medium Are More Centrally Concentrated: Constraints from Multiphase Absorption Lines Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 8

Resolution
verified exact
doi, observed 2026-06-28T05:51:41.044046Z

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=2026-06-28T05:32:29.165988Z digest=sha256:4bad83ebdfa4fbf017e68822d976b3553a8b0e6bdcb52a5bbc75a242876bfdfd

Observation 6ba4ca3b-bcfb-4b12-b1d5-6c25ac091e99 · inbound

Cooler Phases of the Circumgalactic Medium Are More Centrally Concentrated: Constraints from Multiphase Absorption Lines cites this paper.

Cooler Phases of the Circumgalactic Medium Are More Centrally Concentrated: Constraints from Multiphase Absorption Lines Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 8

Resolution
verified exact
doi, observed 2026-07-04T00:29:14.572615Z

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=2026-07-04T00:21:33.171988Z digest=sha256:f86fb4c36d7863f7fe89461820dcb33b9870d8945333a1fc883466f3375d351f

Observation 6c01a961-28f7-4a27-93d4-d445df5214a7 · inbound

Learning the Universe with cosmological rescaling of merger trees and semi-analytic galaxy formation models cites this paper.

Learning the Universe with cosmological rescaling of merger trees and semi-analytic galaxy formation models Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 20

Resolution
verified exact
local_arxiv, observed 2026-06-27T15:20:59.737733Z

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=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:5656b6c20b235730d1849703f3c59a3e48193fb3ba66f3f5efbc9a218ced5bcb

Observation 2d5ade5d-9127-49f7-a5aa-92a16f0d2071 · inbound

Learning the Universe: Constrained simulations of the Coma galaxy cluster -- I. Radial X-ray and Compton-y signatures cites this paper.

Learning the Universe: Constrained simulations of the Coma galaxy cluster -- I. Radial X-ray and Compton-y signatures Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 139

Resolution
verified exact
local_arxiv, observed 2026-06-27T15:21:00.509856Z

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=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:66e1441644f64274464b234a99a14a62e254d135992482f919855a96c0bac2a8

Observation 117a39da-6afc-4934-b453-289e96299dfc · inbound

Galaxy formation in modified gravity -- II. galaxy halo connection and assembly bias cites this paper.

Galaxy formation in modified gravity -- II. galaxy halo connection and assembly bias Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 98

Resolution
metadata mismatch
local_arxiv, observed 2026-07-03T13:18:12.406194Z

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=arxiv_source observed=2026-06-27T08:22:48.704788Z digest=sha256:9be90eec7025e6c987ece001bb268c05b07cacce407f80315a30c01ffa5445d7

Observation fceb7e39-f2c8-451d-95d0-1704bf00f522 · inbound

TNG SAM: Bridging Hydrodynamical Complexity and Semi-Analytic Efficiency to Model Galaxy Formation cites this paper.

TNG SAM: Bridging Hydrodynamical Complexity and Semi-Analytic Efficiency to Model Galaxy Formation Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 111

Resolution
metadata mismatch
doi, observed 2026-06-27T00:30:16.981310Z

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=arxiv_source observed=2026-06-26T23:41:20.418211Z digest=sha256:ed2fd16af41c3bd37dc6ab0fcb618182112386f63ef7e3290dc907cd89524d8b

Observation 8d6dca19-fa69-4f53-9999-cd0c474cc7c0 · inbound

PHANTOM: A MATLAB and Octave Toolbox Connecting Linear Field Statistics to Dark Matter Halo Observables cites this paper.

PHANTOM: A MATLAB and Octave Toolbox Connecting Linear Field Statistics to Dark Matter Halo Observables Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 11

Resolution
verified exact
doi, observed 2026-06-26T19:49:50.402589Z

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=2026-06-26T19:45:14.793850Z digest=sha256:654a46ae1e14d48d089c14ee425982347a1a95557648dc422040ed68d77b67f9

Observation b3c083ba-d162-4481-9b29-dbe74fa9b366 · inbound

The MASSIVE SURVEY XXI: Local Variations in the Stellar Initial Mass Function of MASSIVE Early-Type Galaxies cites this paper.

The MASSIVE SURVEY XXI: Local Variations in the Stellar Initial Mass Function of MASSIVE Early-Type Galaxies Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 50

Resolution
metadata mismatch
doi, observed 2026-06-26T00:28:43.574369Z

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=arxiv_source observed=2026-06-26T00:18:54.011715Z digest=sha256:1357c79dac4e9b567b557321b6f4084e520b6c53b9ff6ec9203052f5897ab8cd

Observation 67337034-4e50-4924-bde4-b52375804a48 · inbound

Universal Fitting Formulae for the Peak Concentration of Dark Matter Halos cites this paper.

Universal Fitting Formulae for the Peak Concentration of Dark Matter Halos Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 8

Resolution
verified exact
doi, observed 2026-06-25T23:58:42.868763Z

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=2026-06-25T23:52:21.029726Z digest=sha256:19c28045e6beaf1815a2622acdde6a38feb9d8894a023da312ba1a25ed4eb882

Observation bcaaa85c-a890-472f-bba3-76703e8d7a44 · inbound

Exploring the physics of ram pressure stripping with radio continuum observations in the SKA era cites this paper.

Exploring the physics of ram pressure stripping with radio continuum observations in the SKA era Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 100

Resolution
verified exact
local_arxiv, observed 2026-06-25T21:28:28.573229Z

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=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:1e1a0a3eea12261efeca7cf88d72fd1b7b70f76480eac6e6a85ec0d38b4f2cac

Observation c205f2be-1339-4d2b-acd8-f053f19d28aa · inbound

Columba: isolated dwarf galaxy populations in diverse cosmological environments simulated with a cold interstellar medium cites this paper.

Columba: isolated dwarf galaxy populations in diverse cosmological environments simulated with a cold interstellar medium Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 3

Resolution
verified exact
local_arxiv, observed 2026-06-27T01:00:20.899998Z

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=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:8ede46c94dbff5f15ffde56f0b544e480a78d3120632b0a98b7b7cfb0f32194b

Observation 8cad13e3-b136-461d-906f-076e6767c8fc · inbound

Spherical Collapse and Halo Formation in a Cosmology with Decaying Dark Matter and a Semi-Cosmographic Dark Energy cites this paper.

Spherical Collapse and Halo Formation in a Cosmology with Decaying Dark Matter and a Semi-Cosmographic Dark Energy Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 39

Resolution
verified exact
local_arxiv, observed 2026-07-04T14:19:54.114133Z

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=2026-06-26T04:08:17.208050Z digest=sha256:006e6fb5c70790d5fa41a35a3c097cc417981937c2c529d11d68d4abe26ed377

Observation ba70495f-df62-40c2-a3dd-b9decaedc1f5 · inbound

COSMOS-Web: does halo mass alone shape the clustering of star-forming and quiescent galaxies? cites this paper.

COSMOS-Web: does halo mass alone shape the clustering of star-forming and quiescent galaxies? Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 213

Resolution
verified exact
local_arxiv, observed 2026-07-01T04:05:20.633631Z

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=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:586d3ca00947e8e6f935907a587757fdab8d9d65eea4fdeaca2c70111954fd5e

Observation 1c0b9478-58e9-4913-9280-972536e94330 · inbound

Hot or Cold? Radial Redistribution of Stars in FIRE Simulations of Milky Way-Mass Galaxies and the Asymmetry of Inward versus Outward Migrators cites this paper.

Hot or Cold? Radial Redistribution of Stars in FIRE Simulations of Milky Way-Mass Galaxies and the Asymmetry of Inward versus Outward Migrators Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 167

Resolution
verified exact
doi, observed 2026-07-02T18:47:16.743192Z

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=arxiv_source observed=2026-07-02T18:37:30.526056Z digest=sha256:7d86ad28514f470c0d5c336a6fd55fa2bf4d7e807df5be5dc689b92a8ad7f70d

Observation fdc37b19-285f-447e-bc58-487f6e8b8a21 · inbound

The youth of the intracluster medium. I. A non-parametric characterisation of the gas and electron number density profiles of $z \simeq 2$ protoclusters cites this paper.

The youth of the intracluster medium. I. A non-parametric characterisation of the gas and electron number density profiles of $z \simeq 2$ protoclusters Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 14

Resolution
unresolved
no resolver link, observed 2026-07-12T07:56:00.734481Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-12T07:56:00.734481Z digest=sha256:23a79f91d74d28b7923ac430d269b39c6fa4a011195608df16aecdeab55f2166

Observation 11cedf4a-ef78-4fbc-82da-2ad40830dcc4 · inbound

The dark matter halo mass function in the $\Lambda\mathrm{CDM}$ cosmology at all times and over all scales -- from planetary to galaxy cluster masses cites this paper.

The dark matter halo mass function in the $\Lambda\mathrm{CDM}$ cosmology at all times and over all scales -- from planetary to galaxy cluster masses Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 28

Resolution
unresolved
no resolver link, observed 2026-07-11T06:41:50.562143Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T06:41:50.562143Z digest=sha256:d1c84b2802e6cbbe9fb8c05abd1cd899d14600226d7d90b05b798e64fac18bdf

Observation ed3e88fa-9083-4701-94f8-eba62029a688 · inbound

Dark matter density profiles of the Milky Way satellite population: reconciling simulations and observations cites this paper.

Dark matter density profiles of the Milky Way satellite population: reconciling simulations and observations Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 37

Resolution
unresolved
no resolver link, observed 2026-07-13T06:28:17.325404Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-13T06:28:17.325404Z digest=sha256:ea15f6812c557d40bdade0a38b4bda97049477ed4525f935fe6841ad97210bdf

Observation 35af7fc9-4348-4fa7-b441-3c5a9742473a · inbound

mitigating the overcooling problem with sink-based bursty star formation in a high-z dwarf galaxy cites this paper.

mitigating the overcooling problem with sink-based bursty star formation in a high-z dwarf galaxy Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 13

Resolution
unresolved
no resolver link, observed 2026-07-13T06:20:04.707661Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-13T06:20:04.707661Z digest=sha256:20a87acc00f85f0ed8170ad3aef78d28b800d6ba72d91e17c8a87fac1ef4f264

Observation 946c4f66-9c56-4e37-aed4-81d46a38c13b · inbound

RABBITS IV: Stellar feedback and SMBH merging time-scales in the sub-Milky Way mass regime cites this paper.

RABBITS IV: Stellar feedback and SMBH merging time-scales in the sub-Milky Way mass regime Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 101

Resolution
unresolved
no resolver link, observed 2026-08-02T03:50:11.033162Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:50:11.033162Z digest=sha256:fe03c12f2dbe995595727487f895fd97411badf49c833d1361a07962b0106ad6

Observation de0b0922-53c0-4f71-a241-e58ee6113ac3 · inbound

The chemodynamical signature of coherent metal-poor inflow and enriched recycled accretion in the cool circumgalactic medium cites this paper.

The chemodynamical signature of coherent metal-poor inflow and enriched recycled accretion in the cool circumgalactic medium Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-02T02:22:43.402971Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T02:22:43.402971Z digest=sha256:25cdb14ee4a9db15a90a2a45ba9fb130e3b6f71ad0719c879372b09b7e1fe1e3

Observation c7fcfbee-4c08-45cd-b136-21fe647a25b5 · inbound

Enabling Cosmic Web Analysis at Gigaparsec Scales: A Multi Block Approach for DisPerSE cites this paper.

Enabling Cosmic Web Analysis at Gigaparsec Scales: A Multi Block Approach for DisPerSE Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 67

Resolution
unresolved
no resolver link, observed 2026-08-02T01:08:00.558682Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T01:08:00.558682Z digest=sha256:ad9fe1557dd85a8990cbd87ba760b5d8a5b64c73b73d6a7945f25a487d4e1cc2

Observation 053dc520-8666-4725-9f2a-e0a53b4d203c · inbound

Outflows in super-Eddington quasars drive clumpy circumgalactic medium and extended H$\alpha$ nebulae at $z \gtrsim 6$ cites this paper.

Outflows in super-Eddington quasars drive clumpy circumgalactic medium and extended H$\alpha$ nebulae at $z \gtrsim 6$ Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 229

Resolution
unresolved
no resolver link, observed 2026-08-01T06:58:55.743193Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T06:58:55.743193Z digest=sha256:61e5837870ca71cc8e51040f2d884904c55b159739a3c73d951b3cf0df3f8e5e

Observation 85af80c8-c9c9-4afb-805d-a9b19ff42012 · inbound

Anisotropic Secondary Bias of Dark Matter Haloes in a $\Lambda$CDM Universe cites this paper.

Anisotropic Secondary Bias of Dark Matter Haloes in a $\Lambda$CDM Universe Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 177

Resolution
unresolved
no resolver link, observed 2026-08-01T00:56:20.935428Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T00:56:20.935428Z digest=sha256:36fa8a59dd8efd8104790ffaafa55aecc40cc72f8c5dc6a14693c92162d625ef

Observation ac5fa3fd-45a7-48d0-951f-86c540c6e9f2 · inbound

The mass-dependent interplay of active galacitc nuclei and supernova feedback in shaping the $L_{\rm X}$--$T$ relation of early-type galaxies cites this paper.

The mass-dependent interplay of active galacitc nuclei and supernova feedback in shaping the $L_{\rm X}$--$T$ relation of early-type galaxies Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 26

Resolution
unresolved
no resolver link, observed 2026-08-06T00:06:24.809189Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T00:06:24.809189Z digest=sha256:697f64aa6f36e528154abee9df2d245f5ed28d1c277597ffd022ad65022b99e3

Observation d5f108dd-a1f6-4acf-9b45-908bca518b50 · inbound

An emerging baryon cycle in a galaxy 500 million years after the Big Bang cites this paper.

An emerging baryon cycle in a galaxy 500 million years after the Big Bang Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-11T10:19:02.414797Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T10:19:02.414797Z digest=sha256:81183082c4182113f4c19b423455f5486d1cf333e361fc42d97ae374120f794f