  We present ALMA observations of organic molecules towards five low-mass Class
0/I protostellar disk candidates in the Serpens cluster. Three sources (Ser-emb
1, Ser-emb 8, and Ser-emb 17) present emission of CH3OH as well as CH3OCH3,
CH3OCHO, and CH2CO, while NH2CHO is detected in just Ser-emb 8 and Ser-emb 17.
Detecting hot corino-type chemistry in three of five sources represents a high
occurrence rate given the relative sparsity of these sources in the literature,
and this suggests a possible link between protostellar disk formation and hot
corino formation. For sources with CH3OH detections, we derive column densities
of 10^{17}-10^{18} cm^{-2} and rotational temperatures of ~200-250 K. The
CH3OH-normalized column density ratios of large, oxygen-bearing COMs in the
Serpens sources and other hot corinos span two orders of magnitude,
demonstrating a high degree of chemical diversity at the hot corino stage.
Resolved observations of a larger sample of objects are needed to understand
the origins of chemical diversity in hot corinos, and the relationship between
different protostellar structural elements on disk-forming scales.
