ERD

Characterising filaments in the SDSS volume from the galaxy distribution

Project: ByoPiC

Updated at: 27-04-2024

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Project acronym ByoPiC

A search for warm/hot gas filaments between pairs of SDSS Luminous Red Galaxies

Project: ByoPiC

Updated at: 27-04-2024

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Project acronym ByoPiC

Star formation rates and stellar masses from machine learning

Project: ByoPiC

Updated at: 27-04-2024

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Project acronym ByoPiC

PACT. I. Combining ACT and Planck data for optimal detection of tSZ signal

Project: ByoPiC

Updated at: 27-04-2024

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Project acronym ByoPiC

On the Tension between Large Scale Structures and Cosmic Microwave Background

Project: ByoPiC

Updated at: 27-04-2024

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Project acronym ByoPiC

Questioning Planck-selected star-forming high-redshift galaxy protoclusters and their fate

Project: ByoPiC

Updated at: 27-04-2024

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Project acronym ByoPiC

Relative distribution of dark matter, gas, and stars around cosmic filaments in the IllustrisTNG simulation

Project: ByoPiC

Updated at: 27-04-2024

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Project acronym ByoPiC

On the slow quenching of ℳ* galaxies: heavily obscured AGNs clarify the picture

Project: ByoPiC

Updated at: 27-04-2024

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Project acronym ByoPiC

T-ReX: a graph-based filament detection method

Project: ByoPiC

Updated at: 27-04-2024

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Project acronym ByoPiC

Filament profiles from WISExSCOS galaxies as probes of the impact of environmental effects

Project: ByoPiC

Updated at: 27-04-2024

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Project acronym ByoPiC

Populations of filaments from the distribution of galaxies in numerical simulations

Project: ByoPiC

Updated at: 27-04-2024

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Project acronym ByoPiC

Direct detection of the kinetic Sunyaev-Zel’dovich effect in galaxy clusters

Project: ByoPiC

Updated at: 27-04-2024

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Project acronym ByoPiC

Imprint of baryons and massive neutrinos on velocity statistics

Project: ByoPiC

Updated at: 27-04-2024

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Project acronym ByoPiC

Encoding large scale cosmological structure with Generative Adversarial Networks

Project: ByoPiC

Updated at: 27-04-2024

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Project acronym ByoPiC

Cosmology with the kinetic Sunyaev-Zeldovich effect: Independent of the optical depth and $\sigma_8$

Project: ByoPiC

Updated at: 27-04-2024

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Project acronym ByoPiC

Cosmology with cosmic web environments. II. Redshift-space auto and cross-power spectra

Project: ByoPiC

Updated at: 27-04-2024

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Project acronym ByoPiC

How Do Galaxies Trace a Large-scale Structure? A Case Study around a Massive Protocluster at Z = 3.13

Project: ByoPiC

Updated at: 27-04-2024

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Project acronym ByoPiC

Probing galaxy cluster and intra-cluster gas with luminous red galaxies

Project: ByoPiC

Updated at: 27-04-2024

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Project acronym ByoPiC

Fast and easy super-sample covariance of large-scale structure observables

Project: ByoPiC

Updated at: 27-04-2024

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Project acronym ByoPiC

Mass bias evolution in tSZ cluster cosmology

Project: ByoPiC

Updated at: 27-04-2024

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Project acronym ByoPiC

Secondary CMB anisotropies from magnetized haloes

Project: ByoPiC

Updated at: 27-04-2024

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Project acronym ByoPiC

Probing hot gas around luminous red galaxies through the Sunyaev-Zel'dovich effect

Project: ByoPiC

Updated at: 27-04-2024

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Project acronym ByoPiC

On the slow quenching of M* galaxies: heavily-obscured AGNs clarify the picture

Project: ByoPiC

Updated at: 27-04-2024

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Project acronym ByoPiC

Characterising filaments in the SDSS volume from the galaxy distribution

Project: ByoPiC

Updated at: 27-04-2024

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Project acronym ByoPiC

Probing the azimuthal environment of galaxies around clusters. From cluster core to cosmic filaments

Project: ByoPiC

Updated at: 27-04-2024

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Project acronym ByoPiC

Simulating the LOcal Web (SLOW): I. Anomalies in the local density field

Project: ByoPiC

Updated at: 27-04-2024

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Project acronym ByoPiC

Constraints from thermal Sunyaev-Zel’dovich cluster counts and power spectrum combined with CMB

Project: ByoPiC

Updated at: 27-04-2024

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Project acronym ByoPiC

Detection of intercluster gas in superclusters using the thermal Sunyaev–Zel’dovich effect

Project: ByoPiC

Updated at: 27-04-2024

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Project acronym ByoPiC

Gas and galaxies in filaments between clusters of galaxies

Project: ByoPiC

Updated at: 27-04-2024

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Project acronym ByoPiC

Analytic growth rate of gravitational instability in self-gravitating planar polytropes

Project: ByoPiC

Updated at: 27-04-2024

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Project acronym ByoPiC

Resources

Selected filters:

Characterising filaments in the SDSS volume from the galaxy distribution

A search for warm/hot gas filaments between pairs of SDSS Luminous Red Galaxies

Star formation rates and stellar masses from machine learning

PACT. I. Combining ACT and Planck data for optimal detection of tSZ signal

On the Tension between Large Scale Structures and Cosmic Microwave Background

Questioning Planck-selected star-forming high-redshift galaxy protoclusters and their fate

Relative distribution of dark matter, gas, and stars around cosmic filaments in the IllustrisTNG simulation

On the slow quenching of ℳ* galaxies: heavily obscured AGNs clarify the picture

T-ReX: a graph-based filament detection method

Filament profiles from WISExSCOS galaxies as probes of the impact of environmental effects

Populations of filaments from the distribution of galaxies in numerical simulations

Direct detection of the kinetic Sunyaev-Zel’dovich effect in galaxy clusters

Imprint of baryons and massive neutrinos on velocity statistics

Encoding large scale cosmological structure with Generative Adversarial Networks

Cosmology with the kinetic Sunyaev-Zeldovich effect: Independent of the optical depth and $\sigma_8$

Cosmology with cosmic web environments. II. Redshift-space auto and cross-power spectra

How Do Galaxies Trace a Large-scale Structure? A Case Study around a Massive Protocluster at Z = 3.13

Probing galaxy cluster and intra-cluster gas with luminous red galaxies

Fast and easy super-sample covariance of large-scale structure observables

Mass bias evolution in tSZ cluster cosmology

Secondary CMB anisotropies from magnetized haloes

Probing hot gas around luminous red galaxies through the Sunyaev-Zel'dovich effect

On the slow quenching of M* galaxies: heavily-obscured AGNs clarify the picture

Characterising filaments in the SDSS volume from the galaxy distribution

Probing the azimuthal environment of galaxies around clusters. From cluster core to cosmic filaments

Simulating the LOcal Web (SLOW): I. Anomalies in the local density field

Constraints from thermal Sunyaev-Zel’dovich cluster counts and power spectrum combined with CMB

Detection of intercluster gas in superclusters using the thermal Sunyaev–Zel’dovich effect

Gas and galaxies in filaments between clusters of galaxies

Analytic growth rate of gravitational instability in self-gravitating planar polytropes