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21-22 September 2020
Max Planck Institute for Radio Astronomy
Europe/Berlin timezone
Session 3
Place
Location: Max Planck Institute for Radio Astronomy
Address: Auf dem Huegel 69
53123 Bonn
GERMANY
Room: Lecture Hall 0.02
Date:
22 Sep 09:00 - 10:40
Description
Data handling and timing.
Chair: Dr. Alan Roy
Timetable | Contribution List
Displaying 4
contributions
out of
4
Session:
Session 3
A 19 feed 33-50GHz receiver under construction for the SRT antenna will be presented. The key modules will be described as well as their measurements in the laboratory.
Presented by Dr. Alessandro ORFEI
on
22/9/2020
at
8:15
Session:
Session 3
In the 20th century high end correlators were built with ASICs (VLA, Westerbork, Australia Telescope). As we entered the 21st century FPGAs came to the fore (eVLA, CABB, etc.) but due to the huge data flows they needed massive dedicated data transport systems. The CASPER group followed a different path and used network switches for data transport but this imposed a significant extra cost and for
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Presented by Dr. Grant HAMPSON
on
22/9/2020
at
7:00
Session:
Session 3
Bluering is the CSIRO name given to a new generation of radio astronomy array receivers based on Xilinx’s Radio Frequency System on Chip (RFSOC) technology. Bluering was initially designed for low frequency radio astronomy applications (such as the MWA telescope), but has grown to be a receiver also capable of L-band radio astronomy (such as Phased Array Feeds). Bluering is not only an array re
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Presented by Dr. Grant HAMPSON
on
22/9/2020
at
7:25
Session:
Session 3
The Hydrogen maser is required equipment for any VLBI station, and so is a formatter such as a DBBC(1,2 or 3) or DBE. Together, these ensure that the received spectrum gets digitized, timestamped with sufficient stability, and provided with headers to allow playback at a correlator. These necessities however don't come cheap.
White Rabbit is an open standard for time and frequency distribution
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Presented by Mr. Paul BOVEN
on
22/9/2020
at
7:50