| 1. |
- Olofsson, Henrik, 1972, et al.
(författare)
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Profiling the EMBRACE tile beam using GPS satellite carriers
- 2009
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Ingår i: Proceedings of Science. - 1824-8039. ; 132, s. 253-257
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Konferensbidrag (refereegranskat)abstract
- All rights reserved. The L2C carriers of multiple GPS satellites have been used to trace out a nearly complete beam pattern out to 45 away from the main lobe centre for a horizontally mounted single EMBRACE tile. The beam was formed along its bore-sight direction, i.e., staring at the local sky zenith. The result is very close to design specifications although there is evidence for at least one side lobe rising above the achieved noise level. We have also used the older L2 carrier to estimate the system temperature, although an exact figure in addition requires knowledge of the aperture efficiency. © 2018 Sissa Medialab Srl.
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| 2. |
- Torchinsky, S. A., et al.
(författare)
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Characterization of a dense aperture array for radio astronomy
- 2016
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Ingår i: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 589, s. Art. no. A77-
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Tidskriftsartikel (refereegranskat)abstract
- EMBRACE@Nancay is a prototype instrument consisting of an array of 4608 densely packed antenna elements creating a fully sampled, unblocked aperture. This technology is proposed for the Square Kilometre Array and has the potential of providing an extremely large field of view making it the ideal survey instrument. We describe the system, calibration procedures, and results from the prototype.
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| 3. |
- Torchinsky, S. A., et al.
(författare)
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EMBRACE@Nançay: An ultra wide field of view prototype for the SKA
- 2015
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Ingår i: Journal of Instrumentation. - 1748-0221. ; 10:7
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Tidskriftsartikel (refereegranskat)abstract
- A revolution in radio receiving technology is underway with the development of densely packed phased arrays for radio astronomy. This technology can provide an exceptionally large field of view, while at the same time sampling the sky with high angular resolution. Such an instrument, with a field of view of over 100 square degrees, is ideal for performing fast, all-sky, surveys, such as the ''intensity mapping'' experiment to measure the signature of Baryonic Acoustic Oscillations in the HI mass distribution at cosmological redshifts. The SKA, built with this technology, will be able to do a billion galaxy survey. I will present a very brief introduction to radio interferometry, as well as an overview of the Square Kilometre Array project. This will be followed by a description of the EMBRACE prototype and a discussion of results and future plans.
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