09:31:13 From  Mary Bishai  to  Everyone:
	https://indico.bnl.gov/event/10495/
09:52:43 From  Hallsie Reno  to  Everyone:
	At leading order with massless quarks, F4=0
10:17:34 From  Mary Bishai  to  Everyone:
	The DUNE high energy beam is actually peaked between 6-10 GeV  and is around 30% QE.
10:19:42 From  Mauricio Bustamante  to  Everyone:
	@Ty: I might show preliminary results about measuring the UHE nu-nucleon in the radio array of Gen2 tomorrow. 
        We assumed 2° of resolution for those results, but we plan to study how much the angular resolution affects our results.
10:21:20 From  Ty DeYoung  to  Everyone:
	great, thanks Mauricio!
11:34:51 From  Ty DeYoung  to  Everyone:
	at GHz you are hitting the PMT TTS
11:35:10 From  Ty DeYoung  to  Everyone:
	although at high PE rates maybe you can get down under that limit
11:35:29 From  Juliana Stachurska  to  Everyone:
	one square is 100ns (not one bin) on the plot
11:36:11 From  Milind Diwan  to  Everyone:
	thanks
12:32:18 From  Christian Glaser  to  Everyone:
	@John: We did this optimisation study for the in-ice detector ARIANNA where we checked which bandwidth gives us the 
        most neutrino effective volume: https://arxiv.org/abs/2011.12997 
        It turned out that 80-200MHz is the optimum. But for reconstruction, a larger bandwidth is of course better, 
        so we only trigger on the small bandwidth but then record the signal at higher bandwidth
12:33:17 From  John Krizmanic  to  Everyone:
	Hi Christian ... thanks!
12:43:12 From  Stephanie Wissel  to  Everyone:
	It’s a little confusing, John. Because the polarity is not the same payload to payload.
12:43:49 From  FRANCIS L HALZEN  to  Everyone:
	What about the paper by Prohira and deVries? They claim that the events are due to the reflection of transition radiation of 
        cosmic ray showers hitting the surface.
12:43:50 From  Stephanie Wissel  to  Everyone:
	*absolute
12:45:39 From  Stephanie Wissel  to  Everyone:
	@Francis I think that’s what Enrique was referring to as a possible standard model explanation
12:49:08 From  zas  to  Everyone:
	Yes, I think that is a possible explanation, not necessarily reflected though, it can just be transition radiation, 
        but there is not a detailed simulation made yet. 
	12:50:44 From  FRANCIS L HALZEN  to  Everyone:
	But they cannot come through the Earth.
12:51:43 From  zas  to  Everyone:
	Ok, it is semantic, i mean from the interface
12:51:56 From  FRANCIS L HALZEN  to  Everyone:
	OK
13:45:59 From  Mary Bishai  to  Everyone:
	I just uploaded Dario's slides to indico - please refresh if you want to access them.
15:13:23 From  Thomas Guillaume Kosc  to  Everyone:
	Hey team :). Can we move to reco. session to be with Juliana and Carlos ?
15:22:53 From  Thomas Guillaume Kosc  to  Everyone:
	I’m leaving the meeting now, thanks everyone for the discussion, I enjoyed. See you tomorrow :)
15:32:52 From  Mary Bishai  to  Everyone:
	I am going to set out for a little bit.