  The ANtarctic Impulsive Transient Antenna (ANITA) long-duration balloon
payload searches for Askaryan radio emission from ultra-high-energy ($>10^{18}$
eV) neutrinos interacting in Antarctic ice. ANITA is also sensitive to
geomagnetic radio emission from extensive air showers (EAS). This talk
summarizes recently released results from the third flight of ANITA, which flew
during the 2014-2015 Austral summer. The most sensitive search from ANITA-III
identified one neutrino candidate with an a priori background estimate of
0.7$^{+0.5}_{-0.3}$. When combined with previous flights, ANITA sets the best
limits on diffuse neutrino flux at energies above $\sim10^{19.5}$ eV.
Additionally, ANITA-III searches identified nearly 30 EAS candidates. One
unusual event appears to correspond to an upward-going air shower, similar to
an event from ANITA-I.
