Sentence examples for limits of about from inspiring English sources

In this case, detection limits of about 0.5 ng mL−1 for both targeted analytes permitted the application of the designed strategy to evaluate the effect of cisplatin on the changes of the methylation index among epithelial ovarian cancer cell lines sensitive (A2780) and resistant (A2780CIS) to this drug after exposition to cisplatin.

"If you are someone who knows they are going to own a car for 10 years and you are driving all over the country, you are not the type of person who should be leasing," said Alec Gutierrez, a senior market analyst of automotive insights at Kelley Blue Book, referring to the mileage limits of about 12,000 a year on leased vehicles.

For Co detection limits of about 300 fg determined by a single element standard have been achieved.

The linear correlation is very good, and the fitted slope is identical to one within the given error limits of about 5% (Table 2).

The procedure was applied to analyzing easily bought PCPs, providing detection limits of about 8 ng g−1, with precisions lower than 11% in terms of relative standard deviation.

While in the case of the photoinduced absorptive variations, it is within the limits of about 20%to30%0%, the photoinduced refractive response showed much higher sensitivity to the crystal composition due to the R e(χ (3)) rise/reduction by about 3 to 10 times.

There is now a limit of about 15,000 controllers, but the union says the agency needs to hire more now to prepare replacements for the thousands expected to retire in four years, when 5,000 controllers qualify for retirement.

EDS compositional analysis reveals that only Au was observed, indicating that the residual Ag is below the detection limit of about 0.5% (Figure 1C).

The 3F3/3B3 primer pair was finally chosen with a good specificity and high efficiency of amplification, with a detection limit of about 10 copies of recombinant plasmid containing AbSV genes in a 20-μL reaction mixture.

When the mass of the inert core exceeds the Chandrasekhar limit of about, electron degeneracy alone is no longer sufficient to counter gravity and maintain stellar equilibrium.

When the core's mass exceeds the Chandrasekhar limit of about, degeneracy pressure can no longer support it, and catastrophic collapse ensues.