The final parsec problem is an astronomical puzzle involving the dynamical evolution of supermassive black holes (SMBHs) at the centres of most galaxies.

Astronomers around the globe are preparing to catch a once-in-a-lifetime event, where a nova explosion located 3000 light years from us will illuminate the night sky.

I like to look at the Telescope Live gallery nearly every day to see what others are working on, and sometimes seeing what others have posted inspires me to take a crack at what they posted.

A team at Penn State have discovered a transiting exoplanet with the most eccentric orbit found.

Join us for an in-depth exploration of gradient correction in astrophotography with Warren Keller, an award-winning astrophotographer and the esteemed author of “Inside PixInsight”.

Observations of black holes in the universe reveal that they exhibit a wide range of masses. However, there is a significant gap in our understanding between the lightest and heaviest black holes.

In cosmology, the prevailing model that describes the universe is the Lambda Cold Dark Matter (ΛCDM) model.

A new study led by an international team involving scientists from NCCR PlanetS, the University of Geneva and the University of Bern have demonstrated the existence of two distinguishable populations of sub-Neptunes based

Classical Cepheid variables are a special class of stars that exhibit period variation in their observed brightness. These are typically young population III stars with high masses, usually 3 – 30 solar masses.

I occasionally try out different software to see if anything can make my workflows better for astrophotography processing, and I decided to try out the Starnet++ standalone app for Windows computers since it has a GUI and

In December 2019, researchers at the Zwicky Transient Facility (ZTF) identified unusual nuclear variability in an early-type galaxy, SDSS J133519.91+072807.4 (hereafter SDSS1335).

Settings considerations in the Image Solver script when drizzle integration is applied.