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How does SKA1 compare with the world’s biggest ?

SKA1 LOW SKA1 MID Lovell Effelsberg Germany 2 2 UK 419,000m 33,000m 4,500m2 7,800m2 ~130,000 antennas ~200 dishes 76m dish 100m dish

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FAST ALMA JVLA NRT Five Hundred Meter Aperture Arecibo Atacama Large Millimeter/ Karl G. , USA Nancay , France Spherical Telescope, China Puerto Rico , Chile n e s s A 2 , 2 2 2 2 to Fo 42,000m - 13,200m 7,000m 71,000m 6,500m op T o: ot Ph 27 dishes 300m x 35m 500m dish 305m dish 66 dishes antenna

C red it: NA OC ARRAYS SINGLE DISHES At 110 MHz Pho to: H . Sc R hw F eik I er -T /W A I R oastronomi YN C adi e d N e r e N a : d a nd to n n o io ca N h t y O P ta A S O : / o A t U o R LOW MID h HIGH A P NON-STEERABLE / N S FREQUENCIES FREQUENCIES F FREQUENCIES

The (SKA) will be the world's largest radio A telescope's capacity to receive faint signals - called sensitivity - depends on its The collecting area is just one aspect of a telescope’s capability though. Arrays telescope, revolutionising our understanding of the . The SKA will be collecting area, the bigger the better. But just like you can't compare radio like the SKA have an advantage over single dish telescopes: by being spread built in two phases - SKA1 and SKA2 - starting in 2018, with SKA1 telescopes and optical telescopes, comparison only works between telescopes over long distances, they simulate a virtual dish the size of that distance and so representing a fraction of the full SKA. SKA1 will include two instruments - working in similar frequencies, hence the different categories above. can see smaller details in the sky, this is called resolution. SKA1 MID and SKA1 LOW - observing the Universe at different frequencies.