However, late frost abundance was not investigated in that study.
Increasing biofilm coverage of the habitat was associated with increasing anopheline late instars abundance (Table 4).
Similar to early anopheline instars, late instars abundance significantly decreased with increasing water surface area of the habitat and increasing water flow (Table 4).
Emergent plant cover, filamentous algae and the presence of both fish and culicines were no longer significantly associated with late instars abundance in the multivariate analysis.
We thank the referees for the suggestion to examine the late Golgi abundance distributions.
Finally, the two common species made up 31 and 45%% of the early and late aboveground abundance but only 8%% of the seed bank.
Their distribution and late season abundance overlap with distribution of human cases, and they will feed opportunistically on avian and mammalian hosts.
As shown below, we see exactly this with the experimentally measured late Golgi abundance distribution excellently matched by the Poisson distribution calculated using the experimentally measured late Golgi copy number, thus using no fitting parameters.
Thus, as in the case of the Anp1-mRFP labeled Golgi apparatus, we would expect that the Sec7-GFP labeled late Golgi abundance distribution would closely follow Poisson statistics with a Fano factor of 1.
Confirmed and putative stress related genes such as aquaporin, dehydrin, ABC (ATP-binding cassette subfamily G, ABCG or Eibi), ERD (Early Response to Dehydration stresses), LEA (Late Embryogenesis Abundance), HSP (Heat Shock Protein) in barley, wheat, sorghum, maize, rice and Arabidopsis were searched in the literature and downloaded from the Uniprot and NCBI databases.
