To derive
statistically robust estimates of ΔT 2x we therefore approximate the inferred relationship between ΔT 2x and LGM SST cooling by a linear regression (Fig. 6, solid red curve).
Not exact matches
Weak lensing cosmology will be challenging: in addition to highly accurate galaxy shape measurements,
statistically robust and accurate photometric redshift (photo - z)
estimates for billions of faint galaxies will... ▽ More A key goal of the Stage IV dark energy experiments Euclid, LSST and WFIRST is to measure the growth of structure with cosmic time from weak lensing analysis over large regions of the sky.
This curve is
statistically speaking a «random walk», with no
robust statistical correlation with atmospheric CO2, which has seen no cycles but has increased at a fairly constant CAGR of around 0.4 % per year since measurements started at Mauna Loa in 1958 and at an
estimated somewhat slower rate before this, based on ice core data.