Using Galaxy Halos to Study Baryonic Feedback in FLAMINGO
Today’s authors use FLAMINGO simulations to probe the tension between different observational methods of estimating cosmological parameters.
Today’s authors use FLAMINGO simulations to probe the tension between different observational methods of estimating cosmological parameters.
Turns out there’s more than one way to “plate” a planet!
Today’s authors consider the way AGN jet shape changes our measurements of blazar polarization.
When we don’t have spectra, we can estimate the distance to a quasar by calculating its photometric redshift. Today’s authors present a new way to use the ‘flickering’ of quasars to improve these distance estimates.
Planets should form aligned with their host protoplanetary discs. So why does this star have a planet and disc that aren’t at all in line?
Today’s bite explores planets made of dark matter and how we might find them.