TITLE: GCN CIRCULAR NUMBER: 20580 SUBJECT: GRB 170202A: Zadko observatory - Gingin optical observations DATE: 17/02/02 22:55:17 GMT FROM: Alain Klotz at IRAP-CNRS-OMP A. Klotz, D. Turpin (IRAP-CNRS-OMP), D. Macpherson (UWA/ICRAR), D. Coward (UWA), M. Boer, R. Laugier (UNS-CNRS-OCA), Gendre B. (UVI - Etelman Obs.), A. Williams (PO-UWA), R. Martin (PO-UWA) report: We imaged the field of GRB 170202A detected by SWIFT (trigger 736407) with the Zadko robotic telescope (D=100cm) located at the observatory - Gingin, Australia. The observations started 58s after the GRB trigger (42s after the notice). The elevation of the field decreased from 51 degrees above horizon and weather conditions were very good. The first image is trailed with a duration of 60.0s (see the description in Klotz et al., 2006, A&A 451, L39). We detect the optical transcient described by Racusin et al. (GCNC 20575), Xin et al. (GCNC 20576) and Lipunov et al. (GCNC 20578). We calibrated magnitudes using the same reference star than Xin et al. (GCNC 20576). The afterglow increases slowly and continuously from 73s (i.e. the limiting magnitude R~19) until 400s (R=16.5). After 550s the flux start to decrease with a standard temporal decay alpha=-1 until 5000s (R=19). Extrapolation with this rate gives R=22.3 at t0+1day. So we encourage to perform spectrometry. N.B. Zadko Magnitudes are not corrected for galactic dust extinction.