The primary goal of CASPER is to streamline and simplify the design flow of radio astronomy instrumentation by promoting design reuse through the development of platform-independent, open-source hardware and software.
Our aim is to couple the real-time streaming performance of application-specific hardware with the design simplicity of general-purpose software. By employing reconfigurable, modular hardware building blocks and parameterized, platform-independent “gateware” libraries, many low-level implementation details can be abstracted, allowing instruments to be rapidly designed and deployed.
CASPER is currently focusing on porting our existing libraries and designs to the newest version of our toolflow for eventual use with our newest processing board, the Reconfigurable Open Architecture Computing Hardware (ROACH) board.
At the same time, we are building demo instruments, both to validate our library blocks and to provide reference designs for end users. Most notably, we continue to improve our packetized correlator design.
We plan to offer training courses in the use of our toolflow to interested scientists and engineers.
If you are a CASPER collaborator, or you're just interested in what we're
up to, feel free to join our mailing list:
To subscribe, go to
http://lists.berkeley.edu.
Presentation
June 11, 2009
CASPER Case Study: Pulsar and Transient Instrumentation (JPL Workshop 2009)
Workshop Announcement
May 28, 2009
CASPER workshop 2009 signup sheet now online
New Memo
April 22, 2009
IBOB PROM burning procedure in iMPACT 10.1
Workshop 2009 announced!
April 08, 2009
The 2009 CASPER workshop will take place from 28 Sept to 2 Oct in Cape Town, South Africa.
New Presentation
March 20, 2009
The CASPER Instrument System - MCCT/SKADS - Oxford, UK 2009
New Presentation
March 18, 2009
Using the CASPER Tool Flow - MCCT/SKADS - Oxford, UK 2009
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