  We present resolved images of IRAS 23077+6707 ("Dracula's Chivito") in 1.3
mm/225 GHz thermal dust and CO gas emission with the Submillimeter Array (SMA)
and optical (0.5-$0.8\,\mu\mathrm{m}$) scattered light with the Panoramic
Survey Telescope and Rapid Response System (Pan-STARRS). The Pan-STARRS data
show a bipolar distribution of optically scattering dust that is characteristic
for disks observed at high inclinations. Its scattered light emission spans
${\sim}14''$, with two highly asymmetric filaments extending along the upper
bounds of each nebula by ${\sim}9''$. The SMA data measure 1.3 mm continuum
dust as well as $^{12}$CO, $^{13}$CO and C$^{18}$O $J$=2$-$1 line emission over
$12''$-$14''$ extents, with the gas presenting the typical morphology of a disk
in Keplerian rotation, in both position-velocity space and in each CO line
spectrum. IRAS 23077+6707 has no reported distance estimate, but if it is
located in the Cepheus star-forming region (180-800 pc), it would have a radius
spanning thousands of au. Taken together, we infer IRAS 23077+6707 to be a
giant and gas-rich edge-on protoplanetary disk, which to our knowledge is the
largest in extent so far discovered.
