Less than meets the eye: measuring the bias in galaxy cluster observations
Today’s authors come up with a new way to account for foreground and background galaxies in galaxy cluster measurements.
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.
This study by the LHAASO Collaboration presents the first measurement of diffuse gamma-ray emissions in the 1–25 TeV range, revealing excess flux beyond theoretical predictions. The findings suggest hidden gamma-ray sources, such as pulsar wind nebulae or massive star clusters, and indicate spectral variations across the Galactic plane. These results challenge existing cosmic-ray transport models and highlight the need for further observations and refined theoretical frameworks.
In the latest of our #UndergradResearch series, discover how Vidit Bhandari determined the physical conditions and chemical composition of galaxy Q2343-D40 using JWST.
Today’s paper explores how JWST was able to observe 44 individual stars in a galaxy eight and a half billion light years away!
The BH-galaxy relations are crucial in our understanding of how they co-evolve. In today’s paper find out a new method to explore this relation.