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Testing of the TriP chip at DAB J. Estrada, C. Garcia, B. Hoeneisen, P. Rubinov

Testing of the TriP chip at DAB J. Estrada, C. Garcia, B. Hoeneisen, P. Rubinov. First VLPC spectrum with the TriP chip Z measurement using the TriP chip Conclusion and plans. …in case you do not know.

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Testing of the TriP chip at DAB J. Estrada, C. Garcia, B. Hoeneisen, P. Rubinov

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  1. Testing of the TriP chip at DABJ. Estrada, C. Garcia, B. Hoeneisen, P. Rubinov First VLPC spectrum with the TriP chip Z measurement using the TriP chip Conclusion and plans

  2. …in case you do not know • Two summers ago the design of AFEII started. AFEI does not work at 132 nsec (at that point 132nsec was still alive). • A new front end chip (TriP: Trigger and Pipeline) was designed to replace the SIFT+SVX combination. The new system uses a commercial ADC for the charge readout. • MCMII was designed for the TriP chip, MCMII mounts on the existing AFE. We have been using MCMII for 1.5 years, three existing versions. • Last summer we received the TriP chips, they were mounted on MCMII and readout using the existing AFE (SASeq). Extensive tests of 8 chips were done in the bench (see DØNote 004009 and DØNote 4076), high yield ~90%. We have enough TriP chips for the full AFE replacement. • This summer we have the 4-cassette cryostat to look at real signals from the VLPC.

  3. Why do we still bother with AFEII?(132nsec is not a possibility anymore) • The situation is as follows: • we have the TriP chip, we have enough of them. • we have seen that it works, and maybe it solves many of the issues with AFEI (split pedestals, tick to tick variations). • After some discussion with DØ management we agreed to: • build a real AFEII and populate it with 8 MCMII (J. Anderson) • at the end of the year, with the information from our tests and our knowledge of the performance of AFEI, we will make a decision on the possible replacement of the CFT electronics.

  4. VLPC spectrum We have a high gain cassette (~55K in Don’s units), from our spares. Without seriously optimizing the parameters for the operation of the TriP in these conditions, we got a nice sprectrum. Notice the very little spread between channels and the uniformity in the gain. Same channels as seen by the stereo board, after very hard work to reduce the noise.

  5. Fits to the spectra Mysterious deformation around 128 counts • We measure a gain of around 21 counts/p.e., from our previous studies of the chip we believe this means that the VLPC are running at ~75K, a bit higher than what we were expecting… • Other typical parameters: pedestal width=0.18 p.e., gain dispersion=0.17 p.e., pedestal spread (RMS-16 channels)= 0.05 p.e.

  6. The TriP seems to be working, we will keep testing it to have the information to make the correct decision in December. One idea: a minor modification to the TriP that would allow us to measure the time when the discriminators fired with respect to the crossing clock , (see DØNote 004009) . This will give a measurement of the Z position of the hit along the fiber, could help for tracking (tracking algorithm experts need to evaluate how useful this will be). We are now measuring the resolution that we can achieve for this z measurement using the current version of the TriP (we can only look at ½ the channels of the TriP and we needed to implement an external readout for the timing). Z measurement

  7. Cosmic Muon Trigger  AFEII-prototype VLPC ethernet scope timing information bit3 SASeq ADC information

  8. Our events DISCR. from TriP CROSSING(132nsec) SCINT.1 SCINT.2 This is how me measure timing of the discriminator, with respect to the muon trigger. The green line is the OR of 16 channels.

  9. Our signal We do no seem to be getting a lot of light, but we get some.

  10. Results Combining the results of 32 channels (2 TriPs), we see that we can only have a timing measurement when the total (direct+replected pulse) number of photoelectrons is above ~5. Our threshold is here is around 1.5 p.e.

  11. Results, with a cut at 5 p.e. The width of the peak is about 4 nsec wide, and there is a tail that makes the RMS 6.2 nsec. This could come from muons at large angle that have a different Z

  12. Results as a function of the cut in the ADC we start to get a measurement only above 5 p.e., and seems like for the large signal pulses we get about RMS=4.5 nsec.

  13. Changing the TriP operating parameters (programmable registers). 3.5 nsec x 16.6 cm/nsec = 58.1cm We changed the TriP operating parameters to see if we could improve our resolution. Things got a little bit better, improving by 1nsec for large number of photoelectrons. Did not re-calibrate the VLPC with this new parameters.

  14. Conclusion and Plans • The TriP still looks good. The noise and the channel to channel differences look ok (so far we looked at a small number of channels). It is amazing how easy it is to operate this chip compared to SVX+TriP . • For the moment we get σ=58cm for the Z measurement of the hit in the fiber. Things are a not as good as we where hoping for, we will continue trying to understand if this is the best we can do (part of this resolution could come from cosmic muons at large angle, that actually have a different Z). • When Paul gets back we will move to 396 nsec, the performance of the TriP has not been studied in detail with this timing…

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