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Geometry effects on dust attenuation curves with different grain sources at high redshift
Yen-Hsing Lin, Hiroyuki Hirashita, Peter Camps +1
Dust has been detected in high-redshift () galaxies but its origin is still being debated. Dust production in high-redshift galaxies could be dominated by stellar production o…
The structure of the Milky Way based on unWISE 3.4m integrated photometry
Aleksandr V. Mosenkov, Sergey S. Savchenko, Anton A. Smirnov +1
We present a detailed analysis of the Galaxy structure using an unWISE wide-field image at m. We perform a 3D photometric decomposition of the Milky Way taking into account i…
First Light And Reionisation Epoch Simulations (FLARES) III: The properties of massive dusty galaxies at cosmic dawn
Aswin P. Vijayan, Stephen M. Wilkins, Christopher C. Lovell +6
Using the First Light And Reionisation Epoch Simulations (\textsc{Flares}) we explore the dust driven properties of massive high-redshift galaxies at . By post-processi…
High-resolution synthetic UV-submm images for simulated Milky Way-type galaxies from the Auriga project
Anand Utsav Kapoor, Peter Camps, Maarten Baes +6
We present redshift-zero synthetic observational data considering dust attenuation and dust emission for the thirty galaxies of the Auriga project, calculated with the SKIRT radiat…
Polarised emission from aligned dust grains in nearby galaxies: predictions from the Auriga simulations
Bert Vandenbroucke, Maarten Baes, Peter Camps +3
(Aims) In this work, we predict the far-infrared polarisation signal emitted by non-spherical dust grains in nearby galaxies. We determine the angular resolution and sensitivity re…
Effects of Spatial Discretization in Lyman-alpha Line Radiation Transfer Simulations
Peter Camps, Christoph Behrens, Maarten Baes +2
We describe the addition of Lyman-alpha resonant line transfer to our dust continuum radiation transfer code SKIRT, verifying our implementation with published results for spherica…