We also compare our data with the observations at 15 GHz conducted by the Ryle telescope.
In order to compare our data with previously published sequences28, we amplified and sequenced the mitochondrial control region.
When we compare our data to that collected by normal absence recording tools in the NHS for example, we find a discrepancy.
To check this prediction, we compare our data with the XMM-Newton observations of similar quality that are available for two other magnetic β Cep-type stars, β Cen (B1III) and β Cep (B2V 25,55,59,60,62.
The best agreement is found when we compare our data to the modeled hemispheric reflectance, corrected by an adjustable factor that shows a small wavelength dependence.
We attribute the change in spin relaxation type in part with the inclusion of WS2 as a substrate to proximity induced spin-orbit coupling due to the adjacent WS2 layer, and we compare our data to the literature.
To delve further, compare our data on each fund.
And being able to compare our data to what others were doing in related fields could have yielded results that we would never have aimed for.
Then, we compare our data with simulation data of CO2 adsorptivity on CS1000A and also Filtrasorb F400.
As the population-based data concerning the relation between TTH and menopause was very limited, it was difficult to compare our data with other studies.
Consequently, we did not compare our data to pulse pressure variation (PPV) or stroke volume variation (SVV) because we set the tidal volume under 8 ml/kg.
