On 1998 May 9-11,BeppoSAX observed the low-luminosity Seyfert 1 galaxy NGC
4051 in an ultra-dim X-ray state. The 2-10 keV flux (1.26 x 10-(12) erg cm(
-2) s(-1)) was about 20 times fainter than its historical average value, an
d remained steady along the whole observation (similar to 2.3 d). The obser
ved flat spectrum (Gamma similar or equal to 0.8) and intense iron line (EW
similar or equal to 600 eV) are best explained by assuming that the active
nucleus has switched off, leaving only a residual reflection component vis
ible.