How will the Universe’s cosmic clumps impact future gravitational wave measurements of H0?
Today’s paper explores the impact of clumpy matter on gravitational lensing and measurements of the Hubble Constant.
Today’s paper explores the impact of clumpy matter on gravitational lensing and measurements of the Hubble Constant.
Today’s authors come up with a new way to account for foreground and background galaxies in galaxy cluster measurements.
Read on to learn how radio observations are uncovering hidden AGNs and what this means for our understanding of protocluster evolution.
Nearby in the Milky Way, the Radcliffe Wave hosts a dense concentration of dust, gas, and star clusters. And in the past few million years, the Sun might have passed right through it! But what effect did that have on our own Earth?
Today’s paper explores the possibility of impacts delivering organics to the ocean worlds in our solar system.
Where do Hot Sub-Neptunes Come From?!