Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data | Paper Citation Record

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Unresolved cited work

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Constraints on Cosmological Parameters from Future Galaxy Cluster Surveys

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Chandra Cluster Cosmology Project III: Cosmological Parameter Constraints

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This paper cites Cluster Cosmology Constraints from the 2500 deg$^2$ SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space Telescope.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Cluster Cosmology Constraints from the 2500 deg$^2$ SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space Telescope

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This paper cites SPT Clusters with DES and HST Weak Lensing. II. Cosmological Constraints from the Abundance of Massive Halos.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data SPT Clusters with DES and HST Weak Lensing. II. Cosmological Constraints from the Abundance of Massive Halos

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This paper cites The SRG/eROSITA all-sky survey: Cosmology constraints from cluster abundances in the western Galactic hemisphere.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data The SRG/eROSITA all-sky survey: Cosmology constraints from cluster abundances in the western Galactic hemisphere

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

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Planck 2018 results. VI. Cosmological parameters

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This paper cites The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample

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This paper cites SDSS-III Baryon Oscillation Spectroscopic Survey Data Release 12: galaxy target selection and large scale structure catalogues.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data SDSS-III Baryon Oscillation Spectroscopic Survey Data Release 12: galaxy target selection and large scale structure catalogues

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This paper cites The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory

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This paper cites KiDS-1000 Cosmology: Multi-probe weak gravitational lensing and spectroscopic galaxy clustering constraints.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data KiDS-1000 Cosmology: Multi-probe weak gravitational lensing and spectroscopic galaxy clustering constraints

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This paper cites Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data DES Y3 + KiDS-1000: Consistent cosmology combining cosmic shear surveys

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Euclid Definition Study Report

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Cosmology and fundamental physics with the Euclid satellite

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This paper cites Euclid preparation: I. The Euclid Wide Survey.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Euclid preparation: I. The Euclid Wide Survey

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This paper cites CMB-S4 Science Book, First Edition.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data CMB-S4 Science Book, First Edition

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data CMB-S4 Science Case, Reference Design, and Project Plan

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data LSST: from Science Drivers to Reference Design and Anticipated Data Products

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Lesgourgues et al

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This paper cites Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data

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This paper cites Cosmological Constraints from Galaxy Clusters and Groups in the eROSITA Final Equatorial Depth Survey.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Cosmological Constraints from Galaxy Clusters and Groups in the eROSITA Final Equatorial Depth Survey

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data The one-dimensional power spectrum from the SDSS DR14 Ly$\alpha$ forests

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Dark Matter Self-interactions and Small Scale Structure

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Small-Scale Challenges to the $\Lambda$CDM Paradigm

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data The Cosmological Evolution of Self-interacting Dark Matter

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data From 100 kpc to 10 Gpc: Dark Matter self-interactions before and after DESI

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Constraining decaying dark matter with BOSS data and the effective field theory of large-scale structures

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Decaying Dark Matter and Lyman-$\alpha$ forest constraints

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Constraining dark matter decays with cosmic microwave background and weak lensing shear observations

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Is dark matter with long-range interactions a solution to all small-scale problems of \Lambda CDM cosmology?

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Non-Abelian dark matter and dark radiation

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Evidence for dark matter interactions in cosmological precision data?

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data ETHOS - An Effective Theory of Structure Formation: From dark particle physics to the matter distribution of the Universe

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data ETHOS - An Effective Theory of Structure Formation: Dark matter physics as a possible explanation of the small-scale CDM problems

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data A Hidden Dark Matter Sector, Dark Radiation, and the CMB

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Partially Acoustic Dark Matter, Interacting Dark Radiation, and Large Scale Structure

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Partially Acoustic Dark Matter Cosmology and Cosmological Constraints

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Interacting Dark Sector and Precision Cosmology

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This paper cites Linear scale bounds on dark matter--dark radiation interactions and connection with the small scale crisis of cold dark matter.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Linear scale bounds on dark matter--dark radiation interactions and connection with the small scale crisis of cold dark matter

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Searching for Signatures of Dark matter-Dark Radiation Interaction in Observations of Large-scale Structure

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This paper cites Constraining Dark Matter -- Dark Radiation interactions with CMB, BAO, and Lyman-$\alpha$.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Constraining Dark Matter -- Dark Radiation interactions with CMB, BAO, and Lyman-$\alpha$

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Cosmological constraints on multi-interacting dark matter

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Full-shape BOSS constraints on dark matter interacting with dark radiation and lifting the $S_8$ tension

Reference 44

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data One likelihood to bind them all: Lyman-$\alpha$ constraints on non-standard dark matter

Reference 45

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This paper cites Probing interacting dark sector models with future weak lensing-informed galaxy cluster abundance constraints from SPT-3G and CMB-S4.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Probing interacting dark sector models with future weak lensing-informed galaxy cluster abundance constraints from SPT-3G and CMB-S4

Reference 46

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Probing Dark Relativistic Species and Their Interactions with Dark Matter through CMB and 21cm surveys

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Unresolved cited work

Reference 48

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data A Multi-component Matched Filter Cluster Confirmation Tool for eROSITA: Initial Application to the RASS and DES-SV Datasets

Reference 49

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data A New RASS Galaxy Cluster Catalog with Low Contamination Extending to $z\sim1$ in the DES Overlap Region

Reference 50

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Observation 579b00e8-efd9-4599-a8fb-0cbcabf819ae · outbound

This paper cites Flaugher, H.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Flaugher, H

Reference 51

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Observation 46e66ac8-07e2-4467-8f36-19f71877f0b1 · outbound

This paper cites The Dark Energy Survey: more than dark energy - an overview.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data The Dark Energy Survey: more than dark energy - an overview

Reference 52

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This paper cites The Dark Energy Survey Data Release 1.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data The Dark Energy Survey Data Release 1

Reference 53

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Observation 76bcfde4-0ba1-47ad-83b6-e36e83c8b110 · outbound

This paper cites Mass calibration of distant SPT galaxy clusters through expanded weak lensing follow-up observations with HST, VLT & Gemini-South.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Mass calibration of distant SPT galaxy clusters through expanded weak lensing follow-up observations with HST, VLT & Gemini-South

Reference 54

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Observation 180d5ab3-012d-44b1-abf9-0c819e251e1d · outbound

This paper cites Galaxy Clusters Discovered via the Sunyaev-Zel'dovich Effect in the 2500-square-degree SPT-SZ survey.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Galaxy Clusters Discovered via the Sunyaev-Zel'dovich Effect in the 2500-square-degree SPT-SZ survey

Reference 55

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Observation 78d31cb7-e82d-4d7d-ab12-d13e1d684916 · outbound

This paper cites The SPTpol Extended Cluster Survey.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data The SPTpol Extended Cluster Survey

Reference 56

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This paper cites Make Dark Matter Charged Again.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Make Dark Matter Charged Again

Reference 59

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Observation 3a9b8d01-55c3-4f9d-871d-06dadcff7d1d · outbound

This paper cites SPT Clusters with DES and HST Weak Lensing. I. Cluster Lensing and Bayesian Population Modeling of Multi-Wavelength Cluster Datasets.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data SPT Clusters with DES and HST Weak Lensing. I. Cluster Lensing and Bayesian Population Modeling of Multi-Wavelength Cluster Datasets

Reference 60

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Observation 1e901b5c-731b-4cbf-af63-4a7ce1d172bb · outbound

This paper cites SPT-SZ MCMF: An extension of the SPT-SZ catalog over the DES region.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data SPT-SZ MCMF: An extension of the SPT-SZ catalog over the DES region

Reference 61

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Observation d198ed5d-657e-42ce-8893-e7373418b59e · outbound

This paper cites RASS-MCMF: A full-sky X-ray selected galaxy cluster catalog.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data RASS-MCMF: A full-sky X-ray selected galaxy cluster catalog

Reference 62

Resolution: verified exact; local_arxiv, observed 2026-08-12T05:47:35.895161Z

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Observation 6e68a53a-cbbe-4fba-bace-fab579d4307c · outbound

This paper cites The PSZ-MCMF catalogue of Planck clusters over the DES region.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data The PSZ-MCMF catalogue of Planck clusters over the DES region

Reference 63

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This paper cites The ACT-DR5 MCMF Galaxy Cluster Catalog.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data The ACT-DR5 MCMF Galaxy Cluster Catalog

Reference 64

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Observation 5f87a3ef-9843-4f24-b2f8-940eafcb5761 · outbound

This paper cites Galaxy Clusters Discovered via the Thermal Sunyaev-Zel'dovich Effect in the 500-square-degree SPTpol Survey.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Galaxy Clusters Discovered via the Thermal Sunyaev-Zel'dovich Effect in the 500-square-degree SPTpol Survey

Reference 65

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Unresolved cited work

Reference 66

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This paper cites Stalder, A.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Stalder, A

Reference 67

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This paper cites Metacalibration: Direct Self-Calibration of Biases in Shear Measurement.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Metacalibration: Direct Self-Calibration of Biases in Shear Measurement

Reference 68

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Observation 43e5aef0-4a3c-4d9c-b1d2-8e8ac8429064 · outbound

This paper cites Practical Weak Lensing Shear Measurement with Metacalibration.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Practical Weak Lensing Shear Measurement with Metacalibration

Reference 69

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Observation a1ade88b-b9ea-4bd5-939e-fa2df5d324b9 · outbound

This paper cites gravity-only mass.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data gravity-only mass

Reference 70

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Observation 628d0a67-ca3c-446c-bc06-62caf81d46ff · outbound

This paper cites Dark Energy Survey Year 3 Results: Point-Spread Function Modeling.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Dark Energy Survey Year 3 Results: Point-Spread Function Modeling

Reference 71

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This paper cites Sevilla-Noarbe et al.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Sevilla-Noarbe et al

Reference 72

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Observation ba22d0eb-bcbf-45a8-a940-b4a8bbd7e38c · outbound

This paper cites Everett et al.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Everett et al

Reference 73

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This paper cites DES Y3 results: Blending shear and redshift biases in image simulations.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data DES Y3 results: Blending shear and redshift biases in image simulations

Reference 74

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Observation fbaf380e-f571-474f-a1bf-a90b1376646b · outbound

This paper cites Cluster Mass Calibration at High Redshift: HST Weak Lensing Analysis of 13 Distant Galaxy Clusters from the South Pole Telescope Sunyaev-Zel'dovich Survey.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Cluster Mass Calibration at High Redshift: HST Weak Lensing Analysis of 13 Distant Galaxy Clusters from the South Pole Telescope Sunyaev-Zel'dovich Survey

Reference 75

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Observation 1e38c35f-b501-4f94-a0a7-273044331b6e · outbound

This paper cites Dark Energy Survey Year 3 Results: Redshift Calibration of the Weak Lensing Source Galaxies.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Dark Energy Survey Year 3 Results: Redshift Calibration of the Weak Lensing Source Galaxies

Reference 76

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Observation 808b46fc-4f57-4633-81e4-df2c590b4cc2 · outbound

This paper cites Constraining the masses of high-redshift clusters with weak lensing: Revised shape calibration testing for the impact of stronger shears and increased blending.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Constraining the masses of high-redshift clusters with weak lensing: Revised shape calibration testing for the impact of stronger shears and increased blending

Reference 77

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Observation 448fc9b7-265e-44cd-bc75-5d9752f4df75 · outbound

This paper cites Testing the accuracy of 3D-HST photometric redshift estimates as reference samples for deep weak lensing studies.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Testing the accuracy of 3D-HST photometric redshift estimates as reference samples for deep weak lensing studies

Reference 78

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Observation 00a341c1-5b7f-4657-aaf7-f5cb75c97865 · outbound

This paper cites Vanderlinde et al.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Vanderlinde et al

Reference 79

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This paper cites Extending empirical constraints on the SZ-mass scaling relation to higher redshifts via HST weak lensing measurements of nine clusters from the SPT-SZ survey at $z\gtrsim1$.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Extending empirical constraints on the SZ-mass scaling relation to higher redshifts via HST weak lensing measurements of nine clusters from the SPT-SZ survey at $z\gtrsim1$

Reference 80

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Observation 4697fe9d-2510-481c-9161-4e9fca60099b · outbound

This paper cites On the Accuracy of Weak Lensing Cluster Mass Reconstructions.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data On the Accuracy of Weak Lensing Cluster Mass Reconstructions

Reference 81

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This paper cites A Universal Density Profile from Hierarchical Clustering.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data A Universal Density Profile from Hierarchical Clustering

Reference 82

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Observation f87daff8-2352-4e85-8aa3-b2f1c8c2d985 · outbound

This paper cites Calibration of bias and scatter involved in cluster mass measurements using optical weak gravitational lensing.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Calibration of bias and scatter involved in cluster mass measurements using optical weak gravitational lensing

Reference 83

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Observation 0622aba1-773e-431e-870d-182beb664e96 · outbound

This paper cites Sunyaev-Zel'dovich Effect and X-ray Scaling Relations from Weak-Lensing Mass Calibration of 32 SPT Selected Galaxy Clusters.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Sunyaev-Zel'dovich Effect and X-ray Scaling Relations from Weak-Lensing Mass Calibration of 32 SPT Selected Galaxy Clusters

Reference 84

Resolution: verified exact; local_arxiv, observed 2026-08-12T05:47:35.366710Z

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Observation 45bf515c-cdcf-4c8a-b649-915fe1c0ae5b · outbound

This paper cites The Aemulus Project II: Emulating the Halo Mass Function.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data The Aemulus Project II: Emulating the Halo Mass Function

Reference 85

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Observation 4144538c-7b05-43a3-abb2-16ec5c08c73d · outbound

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Toward a halo mass function for precision cosmology: the limits of universality

Reference 86

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Observation 1a91bc08-5d69-4e18-a0bb-356862a02ab0 · outbound

This paper cites The Mira-Titan Universe. III. Emulation of the Halo Mass Function.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data The Mira-Titan Universe. III. Emulation of the Halo Mass Function

Reference 87

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This paper cites Dark Quest. I. Fast and Accurate Emulation of Halo Clustering Statistics and Its Application to Galaxy Clustering.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Dark Quest. I. Fast and Accurate Emulation of Halo Clustering Statistics and Its Application to Galaxy Clustering

Reference 88

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Unresolved cited work

Reference 89

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Cosmological simulations of black hole growth: AGN luminosities and downsizing

Reference 90

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This paper cites Distribution and Evolution of Metals in the Magneticum simulations.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Distribution and Evolution of Metals in the Magneticum simulations

Reference 91

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This paper cites An improved SPH scheme for cosmological simulations.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data An improved SPH scheme for cosmological simulations

Reference 92

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This paper cites First results from the IllustrisTNG simulations: radio haloes and magnetic fields.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 93

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 94

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data First results from the IllustrisTNG simulations: the galaxy color bimodality

Reference 95

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This paper cites First results from the IllustrisTNG simulations: matter and galaxy clustering.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data First results from the IllustrisTNG simulations: matter and galaxy clustering

Reference 96

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data The IllustrisTNG Simulations: Public Data Release

Reference 97

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Unresolved cited work

Reference 98

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Weak lensing mass bias and the alignment of center proxies

Reference 99

Resolution: verified exact; local_arxiv, observed 2026-08-12T05:47:34.953676Z

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Observation c2dcfd39-67df-4f22-a7ac-440da178f20e · outbound

This paper cites Weak lensing mass modeling bias and the impact of miscentring.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data Weak lensing mass modeling bias and the impact of miscentring

Reference 100

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data The Cosmic Linear Anisotropy Solving System (CLASS) I: Overview

Reference 101

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Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data CosmoSIS: modular cosmological parameter estimation

Reference 102

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