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We have searched for gamma-ray bursts (GRB) in the BATSE DISCLA data coveringthe period TJD 8365-10528. We employ an algorithm that uses the background bothbefore and after the onset of the burst, and that requires an excess of atleast 5 sigma over background in the energy range 50-300 keV. For the initialset of 7536 triggers, we find strong concentrations at given geographiclocations of the satellite. After excluding these geographic areas, we are leftwith 4485 triggers. We exclude triggers close in position to solar flares,CygX-1, and Nova Persei 1992 when active, as well as soft bursts close to thesun. We accept 1018 triggers that occur within 230 sec of a GRB listed in theBATSE catalog, and upon visual inspection classify 881 triggers asmagnetospheric events and 404 as GRBs. The final sample of 1422 GRBs representseffectively 2.0 years of isotropic exposure, for an annual rate of 710 GRBs peryear.Comment: 4 pages, 3 figures, Astronomy & Astrophysics Suppl. Ser. in press,  proceedings of the Workshop "Gamma Ray Bursts in the Afterglow Era" held in  Rome, November 199

Gamma-ray bursts detected from BATSE DISCLA data