Store PV covariance matrix; store jet SV variables.
Set pvcxx = pvcxy = pvcxz = pvcyy = pvcyz = pvczz = 0.
Store and plot PV covariance matrix and SV jet variables.
version = 'v19'
ANA_HASH, PUBLISH_USER, ANA_VERSION.
MFVNtupleV19 SampleFiles for mfv_neutralino_tau1000um_M0400, ttbarhadronic, qcdht1000.
Plot jet vertex positions w.r.t. beamspot; plot y vs. x and z vs. rho; plot dphi, dxy, dz, d3d between jet vertices for events with exactly two jets that have vertices.
Plot distance, error, significance to the closest jet vertex; count the number of our vertices that are within 5 sigma to a jet vertex; plot closest and next closest deltaphi between vertex position and bjet momentum.
For each vertex, plot jet momentum phi vs. vertex position phi.
For each of our vertices, plot absdeltaphi to the closest jet vertex, both by distance and by absdeltaphi.
V19.
Plot globalCosmicMuons tracks, and angles between tracks for events with two tracks.
Plot relative pT error, dxy and dz w.r.t. primary vertex; require trigger; make sets of plots with different parameters; run over mfv_signal_samples.
Plot vy vs. vx of cosmic tracks; pt, eta, phi, dxy, dz of generated muons; for each cosmic track, scatter plot fraction of hits shared with a general track vs. number of general tracks sharing that fraction.
Merge branch 'master' into ntuplev19

Conflicts:
	MFVNeutralino/plugins/CosmicMuons.cc
	MFVNeutralino/plugins/EventHistos.cc
	MFVNeutralino/plugins/VertexHistos.cc
	MFVNeutralino/test/cosmic_muons.py
	MFVNeutralino/test/histos.py
	Tools/python/Samples.py
Merge branch 'master' into ntuplev19
Invert tobtecfakesfilter like it should be.
Calojets in ntuple (not working in PAT sequences yet).
Part of inverting tobtecfakesfilter.
Get rid of junk we don't use any more.