  In an ongoing effort to search for X-ray transients on diverse time scales in
the data archive of the BeppoSAX Wide Field Cameras we have identified four
GRBs that are long (between 540 and at least 2550 s) and faint (with 3 events
having peak fluxes below 7X10^-9 erg/s/cm2 in 2-10 keV). Three of the events
were covered and detected by BATSE, suggesting that there may be a substantial
number of bursts still hidden in the BATSE database. A spectral analysis of the
three events shows that, although soft, they are not typical X-ray flashes. The
fourth event (not covered by BATSE) is within 3' coincident with a double-lobed
radio galaxy. The chance probability is estimated at 0.001. If real, the
association would be remarkable.
