World's most complex radio telescope begins its first low frequency survey of the sky, as it prepares to open its doors to the international astronomy community this year.
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Part of the ongoing commissioning effort for LOFAR is determining good
models for the bright A-team sources that dominate the radio sky at
low-frequencies.
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The photograph shows that LOFAR is not the first and only
radiotelescope in Nançay, but each instrument operates in a different
frequency range and has its unique capabilites.
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To take some of the the pressure on the central storage, observation
data is regularly transferred to the Petabyte BiG Grid storage at SARA
since January 2011.
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The image shows two of the very first polarisation profiles of pulsars
observed with the LOFAR HBAs, those of PSR B0329+54 and PSR J2219+475.
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Adding the LOFAR station beams in phase, or "coherently", is vital to
achieving the maximum possible raw sensitivity for beam-formed
observations of e.g. pulsars, planets, and cosmic rays.
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ASTRON initiated LOFAR as a new and innovative effort to force a breakthrough in sensitivity for astronomical observations at radio-frequencies below 250 MHz.