ERD

The ALFALFA H i velocity width function

Project: DMIDAS

Updated at: 30-06-2024

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Project acronym DMIDAS

A forward-modelling method to infer the dark matter particle mass from strong gravitational lenses

Project: DMIDAS

Updated at: 30-06-2024

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Project acronym DMIDAS

The Santiago–Harvard–Edinburgh–Durham void comparison II: unveiling the Vainshtein screening using weak lensing

Project: DMIDAS

Updated at: 27-04-2024

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Project acronym DMIDAS

The Ophiuchus stream progenitor: a new type of globular cluster and its possible Sagittarius connection

Project: DMIDAS

Updated at: 27-04-2024

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Project acronym DMIDAS

Measuring the baryon acoustic oscillation peak position with different galaxy selections

Project: DMIDAS

Updated at: 27-04-2024

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Project acronym DMIDAS

The H i velocity function: a test of cosmology or baryon physics?

Project: DMIDAS

Updated at: 27-04-2024

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Project acronym DMIDAS

Abundance and group coalescence time-scales of compact groups of galaxies in the EAGLE simulation

Project: DMIDAS

Updated at: 27-04-2024

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Project acronym DMIDAS

Screening maps of the local Universe I – Methodology

Project: DMIDAS

Updated at: 27-04-2024

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Project acronym DMIDAS

Cosmological test of gravity using weak lensing voids

Project: DMIDAS

Updated at: 27-04-2024

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Project acronym DMIDAS

Robust H i kinematics of gas-rich ultra-diffuse galaxies: hints of a weak-feedback formation scenario

Project: DMIDAS

Updated at: 27-04-2024

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Project acronym DMIDAS

The mass of our Milky Way

Project: DMIDAS

Updated at: 27-04-2024

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Project acronym DMIDAS

A comparison between semi-analytical gas cooling models and cosmological hydrodynamical simulations

Project: DMIDAS

Updated at: 27-04-2024

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Project acronym DMIDAS

Correcting for fibre assignment incompleteness in the DESI Bright Galaxy Survey

Project: DMIDAS

Updated at: 27-04-2024

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Project acronym DMIDAS

The signal of decaying dark matter with hydrodynamical simulations

Project: DMIDAS

Updated at: 27-04-2024

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Project acronym DMIDAS

Halo concentrations from extended Press–Schechter merger histories

Project: DMIDAS

Updated at: 27-04-2024

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Project acronym DMIDAS

To β or not to β: can higher order Jeans analysis break the mass–anisotropy degeneracy in simulated dwarfs?

Project: DMIDAS

Updated at: 27-04-2024

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Project acronym DMIDAS

Radiative cooling rates, ion fractions, molecule abundances, and line emissivities including self-shielding and both loc...

Project: DMIDAS

Updated at: 27-04-2024

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Project acronym DMIDAS

The origin of X-ray coronae around simulated disc galaxies

Project: DMIDAS

Updated at: 27-04-2024

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Project acronym DMIDAS

The edge of the Galaxy

Project: DMIDAS

Updated at: 27-04-2024

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Project acronym DMIDAS

Constraining the inner density slope of massive galaxy clusters

Project: DMIDAS

Updated at: 27-04-2024

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Project acronym DMIDAS

Reconstructing the baryon acoustic oscillations using biased tracers

Project: DMIDAS

Updated at: 27-04-2024

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Project acronym DMIDAS

The self-similarity of weak lensing peaks

Project: DMIDAS

Updated at: 27-04-2024

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Project acronym DMIDAS

The milky way total mass profile as inferred from Gaia DR2

Project: DMIDAS

Updated at: 27-04-2024

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Project acronym DMIDAS

The Cosmic Ballet: spin and shape alignments of haloes in the cosmic web

Project: DMIDAS

Updated at: 27-04-2024

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Project acronym DMIDAS

The star formation rate and stellar content contributions of morphological components in the EAGLE simulations

Project: DMIDAS

Updated at: 27-04-2024

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Project acronym DMIDAS

Non-circular motions and the diversity of dwarf galaxy rotation curves

Project: DMIDAS

Updated at: 27-04-2024

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Project acronym DMIDAS

Cusp or core? Revisiting the globular cluster timing problem in Fornax

Project: DMIDAS

Updated at: 27-04-2024

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Project acronym DMIDAS

Baryon-induced dark matter cores in the eagle simulations

Project: DMIDAS

Updated at: 27-04-2024

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Project acronym DMIDAS

The chemical imprint of the bursty nature of Milky Way’s progenitors

Project: DMIDAS

Updated at: 27-04-2024

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Project acronym DMIDAS

Coming of age of the standard model

Project: DMIDAS

Updated at: 27-04-2024

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Project acronym DMIDAS

Resources

Selected filters:

The ALFALFA H i velocity width function

A forward-modelling method to infer the dark matter particle mass from strong gravitational lenses

The Santiago–Harvard–Edinburgh–Durham void comparison II: unveiling the Vainshtein screening using weak lensing

The Ophiuchus stream progenitor: a new type of globular cluster and its possible Sagittarius connection

Measuring the baryon acoustic oscillation peak position with different galaxy selections

The H i velocity function: a test of cosmology or baryon physics?

Abundance and group coalescence time-scales of compact groups of galaxies in the EAGLE simulation

Screening maps of the local Universe I – Methodology

Cosmological test of gravity using weak lensing voids

Robust H i kinematics of gas-rich ultra-diffuse galaxies: hints of a weak-feedback formation scenario

The mass of our Milky Way

A comparison between semi-analytical gas cooling models and cosmological hydrodynamical simulations

Correcting for fibre assignment incompleteness in the DESI Bright Galaxy Survey

The signal of decaying dark matter with hydrodynamical simulations

Halo concentrations from extended Press–Schechter merger histories

To β or not to β: can higher order Jeans analysis break the mass–anisotropy degeneracy in simulated dwarfs?

Radiative cooling rates, ion fractions, molecule abundances, and line emissivities including self-shielding and both loc...

The origin of X-ray coronae around simulated disc galaxies

The edge of the Galaxy

Constraining the inner density slope of massive galaxy clusters

Reconstructing the baryon acoustic oscillations using biased tracers

The self-similarity of weak lensing peaks

The milky way total mass profile as inferred from Gaia DR2

The Cosmic Ballet: spin and shape alignments of haloes in the cosmic web

The star formation rate and stellar content contributions of morphological components in the EAGLE simulations

Non-circular motions and the diversity of dwarf galaxy rotation curves

Cusp or core? Revisiting the globular cluster timing problem in Fornax

Baryon-induced dark matter cores in the eagle simulations

The chemical imprint of the bursty nature of Milky Way’s progenitors

Coming of age of the standard model