1. Analysis
  A B C D E F G H I J K L M N O P Q R S T U V W X Y Z AA AB AC AD AE AF AG AH AI AJ AK AL AM AN AO AP AQ AR AS AT AU AV AW
1                                                                                                
2 Analysis Elements / Institutions









 		                                                                                              
3 Low Energy/Neutrino Oscillations WG  
4 Atmospheric Mixing Parameters X X X X X  
5 Tau Neutrino Appearance/PMNS Unitarity X X X  
6 Neutrino Mass Ordering X  
7 Neutrino Cross-section Measurements  
8 Atmospheric Neutrino Flux Measurements (GeV) X X X  
9 Sterile Neutrino Searches (TeV) X X X  
10 Sterile Neutrino Searches (GeV) X  
11 Non-Standard Neutrino Interactions X X  
12 Lorentz Violation/Quantum Gravity Searches X  
13 Diffuse/Atmospheric neutrino WG  
14 Astrophysical Neutrino Flux Measurement X X X X X  
15 Astrophysical Neutrino Flavor Ratio Analysis X X X  
16 Atmospheric Neutrino Flux Measurements (TeV) X X X X X  
17 Atmospheric Neutrino Flavor Ratio measurement X X  
18 High-Energy/Cosmogenic Neutrino Searches X  
19 High-Energy Event Energy Estimators X X X X  
20 Measurement of High-Energy Neutrino Cross Section X X  
21 Contained Event Inelasticity Distribution Measurements X  
22 Earth Core Neutrino Tomography X  
23 Point Source WG  
24 All-sky point source searches X X  
25 Point source searches with contained events X X X X X  
26 Source Catalog/Stacking PS searches X X X X X  
27 UHECR motivated PS searches X X X  
28 Diffuse and Point source combination fits X X  
29 Multi-source/anisotropy PS searches X X X X X  
30 Galactic Plane PS searches X X X  
31 Extended source PS searches X X  
32 Time Dependent/Realtime PS searches X X X X X  
33 Transients/GRB WG  
34 Prompt Neutrinos from GRBs X  
35 Realtime GRB neutrino searches X  
36 Neutrinos from Fast Radio Bursts X  
37 Searches for Low Energy Transients X  
38 Realtime followup of neutrino multiplets X X  
39 Realtime Astrophysical (HESE/EHE) neutrino alerts X X X  
40 Realtime Alert Response X  
41 GRB Precursor/Afterglow Neutrino searches  
42 Beyond the Standard Model WG  
43 WIMP signal from Sun X X X X X  
44 WIMP signal from Earth X  
45 Boosted Dark Matter searches X  
46 Decaying Dark Matter searches X X X X  
47 Dark Matter Annihilation in Galaxy Halo/Center X X  
48 Solar Atmospheric Neutrinos X  
49 SUSY Model parameter limits X  
50 Neutrino decay, Lorentz/CPT invariance tests X  
51 Magnetic monopole searches X X X X  
52 Direct BSM particle detection X X  
53 Searches for Strangelets, Q-balls  
54 Searches for TeV scale extra dimensions  
55 Dark Photons  
56 Supernova WG  
57 MeV Supernova Neutrino Burst searches X X  
58 Galactic Supernova Axion Searches X  
59 Neutrino from Solar Bursts X  
60 Low Energy neutrinos from Fast Radio Bursts X  
61 Searches for hidden Galactic Supernova X  
62 Cosmic Rays WG  
63 Primary Cosmic Ray Spectrum and Composition X X X X  
64 Anisotropy in Cosmic Rays X  
65 Atmospheric Muon Spectrum X X  
66 Prompt Muons in High Energy Showers X X X  
67 Low Energy (GeV) Surface Muons X X  
68 High-pT and ultra-forward muons X X  
69 Cosmic ray Vetoing for High Energy Neutrino Searches X X X  
70 IceTop Neutron searches X  
71 IceTop PeV Photon searches X X  
72 Solar and Heliospheric Physics X  
73 Sun shadow in Cosmic Rays X  
74 Cascade/Tau neutrino WG  
75 Contained Low Energy Cascades X  
76 Contained High Energy Cascades X X  
77 Tau Neutrino - Double Bang searches/algorithms X X X  
78 Tau Neutrinos - Double pulse analyses X X X  
79 Tau Neutrinos - Muon decay searches X  
80 Cherenkov light yield studies for Cascades X  
81 Muon/Tracks WG  
82 Muon Energy resolution improvements X X X X  
83 Track Identifications and Reconstructions Improvements X X  
84 TOTALS 3 1 0 5 4 2 0 0 6 1 3 5 3 1 2 2 1 0 5 0 19 0 0 12 3 8 2 0 4 10 5 1 5 3 1 6 1 4 2 0 4 3 0 6 3 2 4  
85                                                                                                  
86 Current locations of WG Chairs and Co-Chairs (nominal 2-yr terms)

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