  An unprecedented array of new observational capabilities are starting to
yield key constraints on models of the epoch of first light in the Universe. In
this Letter we discuss the implications of the UV radiation background at
cosmic dawn inferred by recent JWST observations for radio experiments aimed at
detecting the redshifted 21-cm hyperfine transition of diffuse neutral
hydrogen. Under the basic assumption that the 21-cm signal is activated by the
Ly$\alpha$ photon field produced by metal-poor stellar systems, we show that a
detection at the low frequencies of the EDGES and SARAS3 experiments may be
expected from a simple extrapolation of the declining UV luminosity density
inferred at $z\lesssim 14$ from JWST early galaxy data. Accounting for an early
radiation excess above the CMB suggests a shallower or flat evolution to
simultaneously reproduce low and high-$z$ current UV luminosity density
constraints, which cannot be entirely ruled out, given the large uncertainties
from cosmic variance and the faint-end slope of the galaxy luminosity function
at cosmic dawn. Our findings raise the intriguing possibility that a high star
formation efficiency at early times may trigger the onset of intense Ly$\alpha$
emission at redshift $z\lesssim 20$ and produce a cosmic 21-cm absorption
signal 200 Myr after the Big Bang.
