by Editorial Team

12 April 2023

from Astron Website
 

 

 



Telescopes

WSRT-APERTIF

 



After upgrading the radio telescope array at Westerbork, The Netherlands, astronomers have found five new Fast Radio Bursts.

 

The telescope images, much sharper than previously possible, revealed that multiple bursts had pierced our neighboring Triangulum Galaxy.

 

This allowed the astronomers to determine the maximum number of otherwise invisible atoms in this galaxy for the first time. The results will be published on April 12th.
 

Fast Radio Bursts, FRBs, are among the brightest explosions in the universe.

 

The bursts mainly emit radio waves. The flashes are so powerful that radio telescopes can detect them even from over four billion (!) light years away. That continued visibility over such vast distances means the bursts contain immense amounts of energy.

 

When it goes off, a single FRB contains ten trillion (ten million times a million) times the annual energy consumption of the entire world population.

This gigantic energy generation makes FRBs highly interesting. Many astronomers think they are emitted by neutron stars.

 

The density and magnetic field strength of those extremely compact stars are unique in the universe. By investigating the flashes, astronomers aim to better understand the fundamental properties of the matter that makes up the universe.

 

But studying these flashes is difficult. No one knows where in the sky the next burst will go off. And an FRB lasts only a millisecond: if you blink, you will miss it.

Powered by new receivers and a new supercomputer (the Apertif Radio Transient System, ARTS), Westerbork has now discovered five new FRBs.

 

It also immediately pinpointed them, says principal investigator Joeri van Leeuwen (ASTRON):

"We now have an instrument with both a very wide field of view and very sharp vision. And all this live. That is new and exciting."

 


Three new Fast Radio Bursts discovered by the Westerbork telescope

were shown to have pierced the halo of our neighboring Triangulum Galaxy.

Invisible electrons in that galaxy deform the FRBs.

From sharp, new, live images, astronomers could estimate

the maximum number of invisible atoms in the Triangulum Galaxy

for the first time.

(Credit: ASTRON/Futselaar/van Leeuwen)
 


Previously, radio telescopes such as Westerbork detected FRBs as with the compound eyes of a fly.

 

Flies can see in all directions, but blurred. The Westerbork upgrade is like cross breeding the eyes of a fly with that of an eagle.

 

The ARTS supercomputer continuously combines the images from twelve Westerbork dishes to create a sharp picture over a massive field of view.

"One cannot just go buy the complex electronics you need for this," says system architect Eric Kooistra (ASTRON).

 

"We designed most of the system ourselves, with a large team. That resulted in a state-of-the-art machine, one of the most powerful in the world."

 

 


Skewering galaxies

Astronomers want to understand how and why FRBs get to be so bright.

 

But the flashes are also interesting because on their way to Earth they pierce other galaxies. Electrons in those galaxies, normally mostly invisible, distort the flashes.

 

Tracking down invisible electrons, and their accompanying atoms, is important because most of the matter in the universe is dark and we still know little about it.

 

Previously, radio telescopes could only roughly indicate where an FRB occurred.

 

The ARTS supercomputer now enables Westerbork to indicate the exact location of an FRB very accurately.

 

Van Leeuwen:

"We demonstrated that three of the FRBs we discovered had skewered our neighbor, the Triangulum Galaxy! We were thus able to count how many invisible electrons that galaxy contains at most, for the first time.

 

A fantastic result."

 



Paper

The Apertif Radio Transient System (ARTS): Design, commissioning, data release, and detection of the first five fast radio bursts - Joeri van Leeuwen, Eric Kooistra and the ARTS + Apertif Team - Astronomy & Astrophysics, 12 April 2023, Open Access.