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The number density of quasars increases dramatically with redshift, which translates through Hubble's law to more quasars at larger distances.
At earlier ages, the number density of quasars decreases sharply, corresponding to an era when the quasar population was still building up.
The most conspicuous variations occur in the z direction, above and below the plane of the Galaxy, where the number density falls off rapidly.
This formula holds true if the number density of free oxygen molecules outside water is large compared to the number density of dissolved molecules (N(O_2)).
The number density and height of such pattern increase with voltage increment.
Finally, the number density evolution of a whole simulated experiment is observed at different sampling rates.
The external driving force magnitude does not affect the number density distribution.
The number density is assumed to be constant and volume fraction of dust particles is neglected.
The number density of the solar flare tracks was estimated to be <1 × 109 tracks/cm2.
The number density of particles is estimated to be 9.0 × 1018 ± 1.0 × 1018 cm-3.
However, the number density of islands without NWs exceeds that of those hosting NWs.
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Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com