Critical surface density — where it appears
Named by 2 essays across one field — each of them below, with the objects they name alongside it.
Weighed by the light that bends past it
Every other mass in this collection is measured from something orbiting, which requires the system to have settled down. A gravitational lens weighs whatever is in the way with no such assumption — the light does not care whether the mass is in equilibrium.
A one-per-cent distortion, and a million galaxies to see it
A galaxy's own shape is unknown and scatters with a dispersion of about 0.3, so a coherent one-per-cent shear is thirty times smaller than the noise on any single measurement. Nothing is ever measured about one object; the estimator is an average, and the whole design of a survey follows from 0.3 over the square root of N.
Named alongside it
The objects these essays reach for when they reach for this one.
ConvergenceThe mass-sheet degeneracyCosmic shearThe cross componentDark matterDeflection angleEinstein radiusExcess surface densityGravitational lensingImage multiplicityMagnificationPhotometric redshift