From e6eafe34b6901456123a114014acd24ed9147680 Mon Sep 17 00:00:00 2001
From: Eric Teunis de Boone <ericteunis@gmail.com>
Date: Mon, 17 Feb 2020 17:30:43 +0100
Subject: [PATCH] Worked on an outline

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 presentation/outline.txt | 87 ++++++++++++++++++++++++++++++++++++++++
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+Multi-Messenger Astrophysics
+
+
+Instruments and Observations
+Neutrino
+	IceCube
+		place, size
+
+	Interactions
+		- CC
+		- NC
+
+	Properties of this neutrino
+		cc -> muon
+		129TeV
+
+	Followup of Antares
+
+
+High Energy gamma ray
+	Instruments
+		Satellites(Fermi-LAT / AGILE)
+
+	Observations
+		Pinning to TXS 0506+056
+			0.1 grad from best-fitting direction
+			is blazar BL Lac
+			redshift measured from a study triggered by this neutrion observation
+
+		Elevated gamma emission
+		automated processing showed flare (usual)
+		
+
+VHE gamma
+	Instruments
+		IACT (HESS / MAGIC / VERITAS )
+		HAWC
+
+	Observations
+		Upper limits  on gamma-flux
+		flux(E>175GeV) < 1e-11 1/cm/s
+
+		MAGIC 2: signal 374 +- 62 photons
+		probability constant flux: <0.0135
+		
+		Further observations prevented by full moon
+
+		HAWC: no signal
+
+		upper limits on redshift by attenuation of extragalactic background light
+		z_upp = 0.6 to 1 depending on EBL model
+
+Radio
+	Instruments
+		VLA / OVRO
+	Observations
+		gradual increase over 18 months prior
+
+Optical
+	Instruments
+
+	redshift measure by Gran Telescopio Canarias
+
+X-ray
+	Instruments
+		Satellites
+
+	Observations
+	Spectrum fitting gives
+		
+
+Total Spectrum
+	
+Interpretations
+
+	IceCube archival data -> neutrino in 2014
+	Coincidence probability
+		associate \nu with \gamma
+		chance disfavored at 3\sigma
+	Science to be extracted
+	
+
+	
+		
+		
+		
+