
Spotting close-in giant planets with spectroscopy
Today’s authors have a way to find giant planets using spectroscopy!
Today’s authors have a way to find giant planets using spectroscopy!
Today’s paper explores a novel method to use intermediate-age AGB stars to probe the metallicity and age othe Triangulum galaxy M33.
Today’s authors take a look at clustering-based redshift estimation!
Journey to the distant universe with today’s paper, as we discover what the X-ray emission from high-redshift quasars can tell us about their formation and accretion physics!
The authors of today’s paper study the distribution of cold gas in a group of galaxies and use that to understand how AGNs are powered.
Cosmological simulations are supposed to recreate the observed Universe, but they don’t always match up. Today’s paper shows what we can learn when part of a simulation doesn’t reflect reality.