{"id":28285,"date":"2019-11-01T12:00:09","date_gmt":"2019-11-01T01:00:09","guid":{"rendered":"http:\/\/astro3d.org.au\/?p=28285"},"modified":"2021-05-06T13:29:41","modified_gmt":"2021-05-06T03:29:41","slug":"observing-with-the-engineering-development-array","status":"publish","type":"post","link":"https:\/\/astro3d.org.au\/observing-with-the-engineering-development-array\/","title":{"rendered":"Observing with the Engineering Development Array"},"content":{"rendered":"
November 2019\u2019s Monthly Media was of nearly 2 days of observing with the\u00a0Engineering Development Array 2<\/a><\/span>\u00a0(EDA2) at the Murchison Radio Observatory (MRO), from Associate Professor\u00a0Randall Wayth<\/a><\/span>.<\/p>\n<\/div> The Milky Way, the Sun, the nearby galaxy Centaurus A and other space objects as they pass overhead.<\/span> <\/i><\/p>\n<\/div> This above GIF shows snapshots of the radio sky above the Murchison Radio Observatory taken at 64 second intervals at a frequency of 230 MHz, covering roughly 1.75 days of continuous data. The colour bar at the bottom shows radio intensity (brightness) in the commonly-used astronomer units of Jy\/beam (Jansky per beam). The celestial coordinate system (CCS) is also overlaid on the image to aid the eye (the gridded circle), and the apparent low-level radio emission outside the CCS is an artefact of the imaging process and is not real.<\/p>\n The EDA2 tests the proposed antenna layout of the\u00a0SKA-LOW<\/a><\/span>\u00a0using the current technology of the\u00a0Murchison Widefield Array<\/a><\/span>\u00a0(MWA) dipoles.<\/p>\n<\/div><\/span><\/div><\/div><\/div>