ann14069 — Announcement
ALMA Extends Its Arms
Longest ALMA baseline yet achieved
24 September 2014
The Atacama Large Millimeter/submillimeter Array (ALMA) has successfully tested an antenna in the most extended configuration of the array yet, producing the longest baseline ever achieved by ALMA. This advance became possible once the first of ALMA's three extended arms was successfully powered up for the first time, and opens up the possibility of greatly extending ALMA’s capabilities. With longer baselines, the ability of a radio telescope to see fine detail increases, allowing astronomers to uncover much more information about objects observed in the Universe.
Lore, one of ALMA’s two tailor-made antenna transporters, made its first journey along the Pampa la Bola arm and for the first time relocated an antenna to a position seven kilometers away from its furthest neighbour. This marks a major new technical achievement in the Atacama Desert in Chile, at more than 5000 metres above sea level. This new baseline is more than four times longer than is currently available to the ALMA scientific community, and tests of even longer baselines are in progress.
Catherine Vlahakis, Lead Program Scientist for the ALMA Long Baseline Campaign says that: "successfully powering up an antenna for the first time over these long distances marks an important technical step towards increasing ALMA's ability to see objects in the Universe in fine detail".
Ed Fomalont, Lead Scientist for the ALMA Long Baseline Campaign, explains that "the combination of the signals from the antennas produces patterns called fringes. The fringes measured from the antenna seven kilometres away were as pure and strong as will be needed to obtain high quality images when additional antennas are moved to these long baselines."
Catherine Vlahakis, adds that "this is the first step in a process of moving several antennas out to these longer distances. Once the rest of the antennas are also in place we will be able to begin test observations of astronomical objects at higher angular resolution, and therefore in more exquisite detail, than ALMA has yet achieved."
Observations that will further test extended configurations of the array will continue over the next two months. If all goes as intended, this process will provide astronomers with the knowledge needed to offer long-baseline observations to the scientific community.
Lars Lindberg Christensen
Head of ESO ePOD
Garching bei München, Germany
Tel: +49 89 3200 6761
Cell: +49 173 3872 621
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