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Antiparasitic Drugs<br />

40<br />

■■<br />

Introduction to Antiparasitic Drugs<br />

There is a tremendously unequal variation in the<br />

human burden of parasitic disease, based on geography,<br />

industrialization/hygiene, and immune status.<br />

It is estimated that up to half of the world’s<br />

population is chronically infected with parasites.<br />

The extent of parasite-related morbidity and mortality<br />

depends on parasite burden, preexisting<br />

immunity, and patient comorbidities. We focus on<br />

parasitic diseases primarily affecting inhabitants<br />

of industrialized nations. Parasites causing human<br />

disease can be broadly grouped into two main categories,<br />

the unicellular protozoa and the multicellular<br />

helminthes ( Table 40–1 ). The protozoa have<br />

many subgroups, but we present them as primarily<br />

intestinal or primarily extraintestinal pathogens.<br />

The helminthes are subdivided into nematodes<br />

(roundworms), trematodes (flukes), and cestodes<br />

(tapeworms). Examples of common pathogens<br />

for each group are given along with some of the<br />

agents used in their treatment. Although not technically<br />

considered parasites, two other organisms<br />

that are susceptible to antiparasitic drugs also<br />

are addressed: Pneumocystis jirovecii (technically<br />

a fungus) and Sarcoptes scabei (the scabies mite,<br />

technically an Arachnid).

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