Re: [casper] Dealing with extreme RFI

2017-12-08 Thread Gerald Harp
Hi Xavier I understand your problem -- we face similar impulsive RFI at the ATA. You are trying to "observe through" the periods of RFI, hence need a lot of bits. A method we sometimes use is to "blank" the spectrometer output if the input signal exceeds a certain threshold. When the RFI is

Re: [casper] ROACH-2 power requirements

2017-12-08 Thread Jason Ray
John, We use these picoPSU modules exclusively for powering our roach2 systems.  They have 120W capacity and are powered from +12VDC. http://www.mini-box.com/s.nl/it.A/id.417/.f So far they've been great. Good luck! Jason On 12/8/2017 1:18 PM, John D. Sahr wrote: I have an application

[casper] ROACH-2 power requirements

2017-12-08 Thread John D. Sahr
I have an application for a ROACH-2 which will be powered from 12V rather than 120 VAC, and I need to find some appropriate DC-DC converters. I can see what the TC-1U20FX2 power supply module is capable of, but I'm trying to find out what the ROACH2 actually needs. (*) I haven't been able to

RE: [casper] Dealing with extreme RFI

2017-12-08 Thread Richard Prestage
Hi All - Van Vleck corrections definitely apply to spectrometers. We used them for the 3 and 9 level GBT spectrometers, before VEGAS, which uses the ASIAA 5 Gsps ADCs. Fred Schwab did most of the work on this, which strangely seems to be best documented on Jeff Hagen's web page:

Re: [casper] Dealing with extreme RFI

2017-12-08 Thread Ryan Monroe
On 12/08/2017 01:04 AM, Jean Borsenberger wrote: I knew that correlators could operate using only the sign bit trough the van-vleck correction and total-power denormalization, but I did not know that this also applies to spectrometers. I will look into it. "To the extent of my (imperfect)

Re: [casper] Dealing with extreme RFI

2017-12-08 Thread Jean Borsenberger
    Hello,     In Nançay, we deal with such high RFI, with a 8bits ADC. We experienced no problem. It is to be noticed anyhow that we work with analog filters that almost completely cut low frequencies, and have a usually a smoother edge for hi freq. For some observations, we have