The LOFAR-EoR experiment: Searching for a needle in a haystack
by
Vibor Jelic(ASTRON, The Netherlands)
→
Europe/Brussels
E/3rd floor-E.349 - Seminar room (E.349) (Marc de Hemptinne (chemin du Cyclotron, 2, Louvain-la-Neuve))
E/3rd floor-E.349 - Seminar room (E.349)
Marc de Hemptinne (chemin du Cyclotron, 2, Louvain-la-Neuve)
30
Description
About four hundred million years after the birth of our Universe the first objects were formed,
which then started to ionize the surrounding gas with their strong radiation. Six hundred million
years later, the all-pervasive gas was transformed from a neutral to an ionized state. This pivotal
period in the history of the Universe is called the Epoch of Reionization (EoR). It holds the key to
structure formation and evolution, but also represents a missing piece of the puzzle in our current
knowledge of the Universe. Currently, this is changing with the completion of a new generation of
radio telescopes, which are capable of directly probing the EoR. LOFAR is the first telescope of this kind,
and will use an array of simple radio antennas to hunt for the radiation emitted by the neutral hydrogen
during the EoR. The wavelength of this radiation is 21 cm, but on its way to us it is stretched by the
Universe's expansion to the radio wavelengths of 1-2 m. However, its detection will be quite a challenge
due to a number of complicating factors. For example, the desired signal is so weak that it is like a needle
in a haystack, overwhelmed by the prominent foreground emission of our own Galaxy and other
extragalactic radio sources. During this talk I will give an overview of the LOFAR-EoR experiment,
discuss how the foregrounds influence the extraction of the cosmological signal, and present present first
(commissioning) deep images obtained by LOFAR.