Hi Louis,
You can grab the report from the terminal, but it's also at the top of
the map report file, at
compile-directory/XPS_ROACH_base/implementation/system_map.mrp
Cheers,
Jack
On 29 October 2014 03:31, Louis Dartez louisdar...@gmail.com wrote:
Hi Dan,
I cut the number of frequency
That's exactly what I needed, Thank you!
Jay
Date: Wed, 29 Oct 2014 06:33:18 +0200
Subject: Re: [casper] more chipscope troubles
From: he...@ska.ac.za
To: jay_br...@live.com
CC: casper@lists.berkeley.edu
Hi Jay
Attached is a chipscope project file for ROACH2. You can open it and it will
Hi Jack, Dan, et al,
I’ve linked to two .mrp files in this message. The first is here
https://drive.google.com/file/d/0BwvomAqfDQ2DNFZJOEZnS2NUZHd0QV9GamN4S3F6dkl6MXpj/view?usp=sharing
and contains the utilization report for the spectrometer logic on a SX95T
chip. The second, this one
Hey guys,
The CASPER community has been a great help to me in the past few years.
People have asked for my libraries and due to JPL policy, I've always had
to turn them away. Thanks to help from Bob Jarnot, Jonathon Kocz and
others, I'm now free to open-source some of my designs/libraries.
For
Hey Ryan,
This sounds great. I've just got a 312mhz design for a project in Cambridge
to meet timing (broadly similar to what you're describing, but 10 single
pol antennas and only 4k channels over 5ghz bw).
Whilst I don't have any particular requests, I would be very interested in
hearing about
Hi Ryan,
That does look cool! You don’t mention which ADC you plan to use. Is it this
one?
https://casper.berkeley.edu/wiki/ADC1x5000-8
Just to mention in case it proves useful that our group at Submillimeter Array
(SMA) and Event Horizon Telescope (EHT) has been working on a correlator /
Hi Jonathan! Reply is inline (in blue)
Hi Ryan,
That does look cool! You don’t mention which ADC you plan to use. Is it
this one?
https://casper.berkeley.edu/wiki/ADC1x5000-8
That's the one.
Just to mention in case it proves useful that our group at Submillimeter
Array (SMA) and Event
Hi Ryan,
Thanks for the response.
To answer your question we use 2^15 = 32 k FFTs operating on 8 bit real time
samples, to channelize our visibility spectrum to 2^14 = 16k complex points.
There is a pair of these 2^15 point PFBs on each Virtex 6, one for each 5 Gsps
ADC input.
We’d
They're not released yet, I'm going to deal with that once I've gotten the
design up and running :-)
Thanks for all your help as well!
On Wed, Oct 29, 2014 at 6:21 PM, Jonathan Weintroub
jweintr...@cfa.harvard.edu wrote:
Hi Ryan,
Thanks for the response.
To answer your question we use
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