The Very Large Array Sky Survey (VLASS) map updates in real-time!
We know that there are over 41,253 square degrees in the sky, and of that, the VLA Sky Survey can observe 33,885 square degrees from its position in New Mexico. Observing the sky in terms of its vast area means that we have to break down the area into smaller components shown here as tiles, with each tile representing an area of 10 x 4 degrees. To give you an idea of the scale of that area, let’s look at our closest celestial neighbor, the Moon. The Moon is only a half degree wide, corresponding to an area of only .2 square degrees. So, with one of our 10 x 4 tiles, we could fit up to 200 Moons — a lot of radio data are packed into these tiles! We expect to observe approximately 10 million radio sources three times, over 7 years, providing one of the largest radio catalogs ever assembled.
Make sure to check back regularly as we continue to scan the sky in three distinct epochs over the next 7 years.
Note: The radio data tiles highlighted in blue is overlaid upon the latest optical data from the Digitized Sky Survey (DSS).