The Chandra COSMOS Legacy Survey: The z>3 Sample

The host star peak intensity (blue line), the companion intensity (green line), the inverse of the averaged intensity in an area surrounding the central peak (red line) and

The dashed line represents the yields for a charged Higgs boson with a mass of 1 TeV (500 GeV) for the single lepton (dilepton) final state and a product of the cross section

Distributions of the fit to simulated background SM multijet events (solid red line) and a 500 GeV top squark (dashed blue line), normalized to a factor of ten times its cross

(a) Angular velocity as a function of the applied laser power and power density for a bare upconverting NaYF 4 :Er 3+ ,Yb 3+ microspinner (black line and hexagons) and for a

The graph on the right gives the maximum bias bounds (`(), solid line; u() dotted-dashed line) for an MM-estimate based on biweight loss functions with 50% breakdown point and

Results are shown for the KB3G effective interaction (black circles, solid line), the collective Hamiltonian H coll (red circles, dashed line), H coll without the isoscalar pairing

Relationship between the total cluster stellar mass and the photometric blue fraction for the ALHAMBRA cluster and group sample stacked into different redshift bins. The galaxy

Figures 3(a) and 3(b) show PDFs of the achieved correlation coe fficients, with histograms for the sample selection results, and solid lines for the directly generated data.. The