A molecular shielding strategy to convert “protein‐sticky” and “non‐tumor specific” clinical ICG dye, into a “low protein binding” and “tumor‐targeting” dye with prolonged blood circulation and renal clearance is described. These shielded ICGs demonstrate strong tumor accumulation and optimal tissue clearance, resulting in high tumor‐to‐background ...
Li Xiang +9 more
wiley +1 more source
Lytic viruses drive the decrease in polyphosphate-accumulating and phosphate-solubilizing potential of microbial communities with increasing reservoir age. [PDF]
Wu Q +7 more
europepmc +1 more source
Effect of Aeration Rate Redistribution on Nitrogen Removal Performance of a Novel Multi-Compartment Fixed-Biofilm Cyclic Activated Sludge System. [PDF]
Yan Z, Fan S, Yan W, Ma H, Zhao T.
europepmc +1 more source
Spatial and temporal variation in bacterial-archaeal community and niche differentiation of denitrifying anaerobic methane-oxidizing microbes in grass carp (<i>Ctenopharyngodon idellus</i>) aquaculture ponds of Northern China. [PDF]
Chen Y, Pan Z, Wu Z, Tian Z.
europepmc +1 more source
Spatiotemporal dynamics in airborne fungi and allergenic fungal taxa across the United States. [PDF]
Gering SM +3 more
europepmc +1 more source
Dissolved Organic Matter in the Coastal Ocean Is Structurally More Diverse Than in Terrestrial Systems, as Shown in an Amazonian Mangrove Estuary. [PDF]
Mitschke N, Dittmar T, Seidel M.
europepmc +1 more source
On the influence of the environment on galactic chemical abundances [PDF]
We examine the influence of the environment on the chemical abundances of late-type galaxies with masses of 10(9.1)-10(11) M-circle dot using data from the Sloan Digital Sky Survey. We find that the environmental influence on galactic chemical abundances
L S Pilyugin +2 more
exaly +3 more sources
Chemical abundances in the nuclear region of nearby galaxies from the Palomar Survey
We estimate chemical abundances and ionization parameters in the nuclear region of a sample of 143 galaxies from the Palomar Spectroscopic Survey, composed by star-forming galaxies (87), Seyferts 2 (16), and LINERs (40) using the HII-CHI-MISTRY code.
B Pérez-Díaz, J Masegosa, I Marquez
exaly +2 more sources

