Astronomers are hearing a new type of radio transient, but no one knows where they come from and how they are created. This paper suggests one of the six documented Fast Radio Bursts detected so far originated close to home, within our own galaxy.
The link between a pile of data and a physical explanation is the fun part. Astronomers spend countless hours gathering data, and countless more thinking up physical models for different pieces of the Universe. But reconciling these two things—finding a model that not only agrees with observations, but is the sole likely explanation—isn’t easy.
Part two of our recap of the “Modern Statistical and Computational Methods for Analysis of Kepler Data” workshop in North Carolina, featuring both astronomers and statisticians!
A recap of the “Modern Statistical and Computational Methods for Analysis of Kepler Data” workshop in North Carolina, featuring both astronomers and statisticians!
There’s a new space telescope on the block, which just might find as many new planet candidates as the Kepler mission.
Highlights from the International Astronomical Union Symposium on “Exploring the Formation and Evolution of Planetary Systems”.
Our simple formula for predicting the probability that an exoplanet will transit might miss something important.
The census of planets for smaller stars—M dwarfs—is now basically complete. In this paper, Courtney Dressing and Dave Charbonneau use this M dwarf advantage to determine the occurrence rate of small planets around M dwarfs.
Witzel et. al examine the statistical properties of the photometric variability of our Galaxy’s central black hole.
Title: Handedness asymmetry of spiral galaxies with z<0.3 shows cosmic parity violation and a dipole axis Authors: L. Shamir First Author’s Institution: Lawrence Technological University A cherished principle of cosmology is isotropy—that things look the same whatever direction you look. The cosmic microwave background, radiation left over from 300,000 years after the Big Bang, is […]