
Galaxies of the last 10 billion years observed in the 3D-DASH program, created using 3D-DASH/F160W and ACS-COSMOS/F814W imagery. 1 credit
There is a part of the sky known as the COSMOS field, a region rich in galaxies, which has been chosen for the Cosmic Evolution Survey (COSMOS) project. For the first time, a complete near-infrared survey of the entire COSMOS field, imaged by the[{” attribute=””>Hubble Space Telescope, is being provided to researchers via 3D-DASH.
Although Hubble launched in 1990, a series of five servicing missions have kept it on the cutting edge of technology for the last 30 years. 3D-DASH will allow scientists to find rare objects that the brand new Webb Space Telescope can target for close-up study.
An international team of scientists recently released the largest near-infrared image ever taken by
A patch of sky imaged by 3D-DASH, showing the brightest and rarest objects of the universe such as monster galaxies. Credit: Image by Gabe Brammer
“Since its launch more than 30 years ago, the Hubble Space Telescope has led a renaissance in the study of how galaxies have changed in the last 10 billion years of the universe,” says Lamiya Mowla, Dunlap Fellow at the Faculty of Arts & Science’s Dunlap Institute for Astronomy & Astrophysics at the University of Toronto and lead author of the study.
“The 3D-DASH program extends Hubble’s legacy in wide-area imaging so we can begin to unravel the mysteries of the galaxies beyond our own.”
The Hubble Space Telescope captured the entire COSMOS field by stitching together multiple images into one master image, a process called mosaicing. Credit: Ivelina Momcheva
For the first time, 3D-DASH provides researchers with a complete near-infrared survey of the entire COSMOS field, one of the richest data fields for extragalactic studies beyond the
Astronomers also need to search a vast area of the sky to find rare objects in the universe. Until now, such a large image was only available from the ground and suffered from poor resolution, which limited what could be observed. 3D-DASH will help to identify unique phenomena like the universe’s most massive galaxies, highly active black holes, and galaxies on the brink of colliding and merging into one.

Zoomed-in panels on the 3D-DASH depth map reveal the wealth of bright objects that can be studied. Credit: Mowla et al. 2022
“I am curious about monster galaxies, which are the most massive ones in the universe formed by the mergers of other galaxies. How did their structures grow, and what drove the changes in their form?” says Mowla, who began working on the project in 2015 as a graduate student at
Lamiya Mowla, Dunlap Fellow at the Faculty of Arts & Science’s Dunlap Institute for Astronomy & Astrophysics at the University of Toronto and lead author of the study. Credit: Courtesy of Lamiya Mowla