Presentations

3 March 2019 — scipresentation0283

Not all galaxies’ dust content is the same

3 March 2019 — scipresentation0282

A3COSMOS: Systematic Biases and New Measurements of the Gas Evolution in Galaxies out to z~6

3 March 2019 — scipresentation0281

Beyond the Milky Way: Resolved Dust Observations and CO X Factor Measurements of Individual Giant Molecular Clouds in the Andromeda Galaxy M31

3 March 2019 — scipresentation0280

Dust, Gas and Star Formation in Andromeda

3 March 2019 — scipresentation0278

PAH Fraction in the Magellanic Clouds

3 March 2019 — scipresentation0279

Metals and dust content across the discs of nearby galaxies

3 March 2019 — scipresentation0277

Gas, Dust, and Metals in the ISM of Galaxies

3 March 2019 — scipresentation0276

Why does dust distribution matter to galaxies?

3 March 2019 — scipresentation0273

Investigating Interstellar Dust in Local Group Galaxies with New UV Extinction Curves

3 March 2019 — scipresentation0271

Review: Empirical Results on Attenuation Curves

3 March 2019 — scipresentation0272

Which dust attenuation curve(s) for star forming galaxies?

3 March 2019 — scipresentation0274

Spatially Resolved UV Attenuation Curves with SOLV: Swift Observations of the Local Volume

3 March 2019 — scipresentation0275

Infrared Extinction Law & Very Large Dust Grains

3 March 2019 — scipresentation0270

What do we want to learn, and why?

3 March 2019 — scipresentation0269

Transfer of ionizing radiation through gas and dust

3 March 2019 — scipresentation0268

Modelling the dust content of galaxies over cosmic time

3 March 2019 — scipresentation0266

DUSTY GALAXIES AT HIGH REDSHIFT

3 March 2019 — scipresentation0267

Models for Dust-to-Gas Ratios and Grain Size Distributions in Galaxies

3 March 2019 — scipresentation0265

A Two-Parameter Dust Model for Galaxies and AGN

3 March 2019 — scipresentation0264