The Origin and Fate of Dust in Our Universe

Research Project, 2020 – 2026

Participants

Collaborations

Funding

Related Areas of Advance and Infrastructure

Onsala Space Observatory

Infrastructure

Publications

Probing infrared eXcess to investigate early-Universe dust (PIXIEDust)

An empirical view of the extended atmosphere and inner envelope of the asymptotic giant branch star R Doradus II. Constraining the dust properties with radiative transfer modelling

The dust doesn’t settle in merger galaxy II Zw 096

Compact Ionized Gas Region Surrounded by Porous Neutral Gas in a Dusty Lyman Break Galaxy at Redshift z = 8.312

Kinematics of synthetically observed high-z rotating discs: reliability and biases of 3D fitting tools

An accreting dwarf star orbiting the S-type giant star π1 Gru

A warm ultraluminous infrared galaxy just 600 million years after the big bang

ALMA Lensing Cluster Survey: Dust mass measurements as a function of redshift, stellar mass, and star formation rate from z = 1 to z = 5

HerS-3: An Exceptional Einstein Cross Reveals a Massive Dark Matter Halo

Behind the dust veil: A panchromatic view of an optically dark galaxy at z = 4.82

A dusty protocluster surrounding the binary galaxy HerBS-70 at z = 2.3

An empirical view of the extended atmosphere and inner envelope of the asymptotic giant branch star R Doradus I. Physical model based on CO lines

Accurate sticking coefficient calculation for carbonaceous dust growth through accretion and desorption in astrophysical environments

A novel high-z submm galaxy efficient line survey in ALMA Bands 3 through 8-an ANGELS pilot

ALMA Lensing Cluster Survey: Deep 1.2 mm Number Counts and Infrared Luminosity Functions at z ≃ 1-8

Modeling Dust Production, Growth, and Destruction in Reionization-era Galaxies with the CROC Simulations. II. Predicting the Dust Content of High-redshift Galaxies

More information

Project Web Page

https://cosmic-dust.se/

Latest update