  We have used Chandra observations of eight bulge-less disk galaxies to
identify new ultraluminous X-ray source (ULX) candidates, study their high mass
X-ray binary (HMXB) population, and search for low-luminosity active galactic
nuclei (AGN). We report the discovery of 16 new ULX candidates in our sample of
galaxies. Eight of these are found in the star forming galaxy NGC 337, none of
which are expected to be background contaminants. The HMXB luminosity function
of NGC 337 implies a star formation rate (SFR) of 6.8$^{+4.4}_{-3.5}$ \msun\
yr$^{-1}$, consistent at 1.5$\sigma$ with a recent state of the art SFR
determination. We also report the discovery of a bright ULX candidate (X-1) in
ESO 501-23. X-1's spectrum is well fit by an absorbed power law with $\Gamma =
1.18^{+0.19}_{-0.11}$ and N$\rm{_H}$ = 1.13$^{+7.07}_{-1.13} \times 10^{20}$
cm$^{-2}$, implying a 0.3-8 keV flux of $1.08^{+0.05}_{-0.07} \times 10^{-12}$
\esc. Its X-ray luminosity (L$_X$) is poorly constrained due to uncertainties
in the host galaxy's distance, but we argue that its spectrum implies L$_X >
10^{40}$ \es. An optical counterpart to this object may be present in HST
imaging. We also identify ULX candidates in IC 1291, PGC 3853, NGC 5964 and NGC
2805. We find no evidence of nuclear activity in the galaxies in our sample,
placing a flux upper limit of $4 \times 10^{-15}$ \esc\ on putative AGN.
Additionally, the type II-P supernova SN 2011DQ in NGC 337, which exploded 2
months before our X-ray observation, is undetected.
