  We present the BoRG-JWST survey, a combination of two JWST Cycle 1 programs
aimed at obtaining NIRSpec spectroscopy of representative, UV-bright $7<z<10$
galaxy candidates across 22 independent sight lines selected from Hubble/WFC3
pure-parallel observations. We confirm the high-$z$ nature of 10 out of 19
observed primary targets through low-resolution prism observations, with the
rest revealing themselves unsurprisingly to be $z\sim1-3$ interlopers, brown
dwarfs, or yielding inconclusive results. From the MSA observations, we confirm
an additional 9 filler sources at $z>5$, highlighting the large abundance of
high-redshift galaxies even in individual WFC3 pointings. The primary sample
span an absolute magnitude range $-20.4<M_{\rm UV}<-22.4$ mag and harbour UV
continuum slopes of $\beta\simeq-2.5$ to $-2.0$, representing some of the most
luminous $z>7$ sources currently known and comparable to the brightest sources
at $z>10$. Prominent [O III]+H$\beta$ lines are found across the full sample,
while a stack of sources reveals a plethora of other rest-optical lines and
additional rest-UV C III]1909 \r{A} emission. Despite their luminosities, none
of the low-resolution spectra display evidence for Type 1 AGN activity based on
a search for broad-line emission. Lastly, we present a spectroscopic data
release of 188 confirmed $0.5\lesssim z\lesssim5.0$ sources from filler MSA
observations, highlighting the legacy value of the survey and a representative
benchmark for comparisons to deep field observations.
