Radio telescopes are good probes of star formation. But
until now, they haven’t been sensitive enough to see radio waves coming from
the vast majority of galaxies
that produced stars during the peak of star production, an epoch roughly 10
billion years ago known as cosmic noon (SN: 6/20/14).
Now, a new image from the MeerKAT observatory in South
Africa has lifted the radio veil on those unsung galaxies. In that image, more
than 17,000 pinpoints of radio energy — nearly every one a star-forming galaxy —
fill a patch of sky that, as seen from Earth, could be covered by about five
full moons.
Using about 10,000 well-studied nearby galaxies as a
template, James Condon and his colleagues calculated how luminous and how far
away all those points of light must be. To match the observations, the radio
waves must come from star-forming galaxies at cosmic noon churning out stars at
about 10 times the rate of modern galaxies, says Condon, an astrophysicist at
the National Radio Astronomy Observatory in Charlottesville, Va.
What’s more, he says, there are a little less than twice as
many of these sources as expected, suggesting that star formation was much
higher around cosmic noon than predicted by calculations based on infrared,
optical and ultraviolet data. These preliminary results appear December 15 at
arXiv.org.