Dear Morag,

At CHIME <https://chime-experiment.ca/en>, we have used Roach1 with a two-dish system as a proof of concept back in 2010. Then later, we developed our own customized F-engine hardware with the same FPGA and ADC chips as Roach1. We use CASPER ADC/FFT/PFB blocks into an AXI-Streaming interface wrapper, which is the standard used for our signal processing pipeline. We inherit core concepts of the signal processing chain implemented in the CASPER spectrometer, mainly the notion of 4b/4b re/imag output going to the X-engine.

The current CHIME F-engine provides additional functionality, uses different packet assembly and shuffle code, and offers a multi-board synchronization scheme in order to scale up to 2048 channels, all of which, is designed and developed outside of the CASPER framework.

The FFT is a critical element in the quality of the science data and in addition to being fast and resource-efficient, we know that we can trust it for it has been vetted by the community.

Mandana for the CHIME team

On 9/3/2022 1:25 AM, 'Jonathan Weintroub' via [email protected] wrote:
[*CAUTION:* Non-UBC Email]

Ciao Morag,

It is not a full CASPER instrument, so maybe a marginal case: the ALMA Phasing System <https://iopscience.iop.org/article/10.1088/1538-3873/aa9c3d/pdf> (APS) is a retrofit of a VLBI beam forming capability to the non-VLBI capable ALMA Correlator, <https://www.aanda.org/articles/aa/pdf/2007/05/aa4519-05.pdf> which was designed a non CASPER proprietary ASIC-FPGA instrument.  The APS used CASPER ROACH2 boards (and non-CASPER flow HDL firmware) as the hardware platform for the “Phasing Interface Cards” or PICs, of which there are eight in the system.  The PICs are shown in figure 2 and also in figure 7 of the first linked reference.

While it’s not a holistically CASPER instrument, the APS is a very significant facility instrument at a very important radio telescope. I’d be interested to hear whether CASPERites feel it warrants inclusion in your list, and how it should be described.

Best wishes,
Jonathan


On Aug 31, 2022, at 12:53 PM, Morag Brown <[email protected]> wrote:

Ciao dalla Sardegna, collaborati!

I'm hoping to put together a more up-to-date list of instruments that have been built using CASPER hardware and tools. The most current list was compiled in 2016 for the "A Decade of Developing Radio-Astronomy Instrumentation using CASPER Open-Source Technology" paper by Jack et al, so it could probably use updating.

The list is currently as follows:

*Spectrometers and packetizers -*
Fly’s Eye
GUPPY
CASPER
BPSR
GAVRT
SERENDIP V.v
HiTREKS
NUPPI
Skynet
RATTY
cycSpec
C-BASS
HIPSTER
KuPol
VEGAS
ALMA Phasing Project
Leuschner
R2DBE
DSN Transient Observatory
VGOS
AVN-Ghana
COMAP

*MKID readout systems -*
Columbia MKID
Mustang2
DARKNESS
MEC
BLAST-TNG
HOLMES
*
*
*Correlators and beamformers -*
KAT7
PAPER
ATA
LEDA
ARI
MAD
pocketcorr
Medicina FFTT
GMRT
Meteor
AMI
MeerKAT AR-1
FLAG
BIRALES
Starburst
AMiBA
EOVSA
SWARM
MeerKAT
HERA

If you are not (or know of any instruments that are not) on this list, please reach out to me for it to be added?

Grazie!
Morag




--
You received this message because you are subscribed to the Google Groups "[email protected]" group. To unsubscribe from this group and stop receiving emails from it, send an email to [email protected]. To view this discussion on the web visit https://groups.google.com/a/lists.berkeley.edu/d/msgid/casper/CAGH-0TcON2s8K2JqXe0OAWWMeUeuKrnGSzhfRJS%2BWym%2BZiiE_A%40mail.gmail.com <https://www.google.com/url?q=https://groups.google.com/a/lists.berkeley.edu/d/msgid/casper/CAGH-0TcON2s8K2JqXe0OAWWMeUeuKrnGSzhfRJS%252BWym%252BZiiE_A%2540mail.gmail.com?utm_medium%3Demail%26utm_source%3Dfooter&source=gmail-imap&ust=1662547996000000&usg=AOvVaw3c06Y03UGNP25sWPeQhWqj>.

--
You received this message because you are subscribed to the Google Groups "[email protected]" group. To unsubscribe from this group and stop receiving emails from it, send an email to [email protected]. To view this discussion on the web visit https://groups.google.com/a/lists.berkeley.edu/d/msgid/casper/3D804AB2-5ACD-448C-B3DB-F381D3551BE8%40cfa.harvard.edu <https://groups.google.com/a/lists.berkeley.edu/d/msgid/casper/3D804AB2-5ACD-448C-B3DB-F381D3551BE8%40cfa.harvard.edu?utm_medium=email&utm_source=footer>.

--
    Mandana Amiri
    Department of Physics & Astronomy
    University of British Columbia
    204-Hennings, 6224 Agricultural Rd.
    Vancouver, BC V6T 1Z1, Canada
    +1 778 788 4431
    skype id: mandana.amiri2

--
You received this message because you are subscribed to the Google Groups 
"[email protected]" group.
To unsubscribe from this group and stop receiving emails from it, send an email 
to [email protected].
To view this discussion on the web visit 
https://groups.google.com/a/lists.berkeley.edu/d/msgid/casper/276bf2e4-c9b3-fe11-a53e-62ed4c838828%40phas.ubc.ca.

Reply via email to