TITLE: GCN CIRCULAR NUMBER: 32789 SUBJECT: AGILE detection of short X-ray flaring activity contemporary to SGR J1935+2154 reported bursts DATE: 22/10/18 12:18:39 GMT FROM: Francesco Verrecchia at SSDC,INAF-OAR C. Casentini (INAF/IAPS), F. Verrecchia (SSDC, and INAF/OAR), M. Tavani (INAF/IAPS, and Univ. Roma Tor Vergata), M. Pilia (INAF/OA-Cagliari), � A. Ursi, A. Argan, M. Cardillo, L. Foffano, Y. Evangelista, E. Menegoni, G. Piano (INAF/IAPS), A. Bulgarelli, A. Di Piano, V. Fioretti, G. Panebianco, N. Parmiggiani (INAF/OAS-Bologna), F. Lucarelli, C. Pittori(SSDC, and INAF/OAR), M. Romani (INAF/OA-Brera), M. Marisaldi (INAF/OAS-Bologna, and Bergen University), A. Trois (INAF/OA-Cagliari), I. Donnarumma (ASI), A. Giuliani (INAF/IASF-Mi), F. Longo (Univ. Trieste and INFN Trieste), and P. Tempesta (TeleSpazio), report on behalf of the AGILE Team: The AGILE Anti-Coincidence system (AC Top; 50-200 keV), is detecting short X-ray flaring activity from October 12nd 2022, at times within the X-ray burst forest reported by INTEGRAL (GCN #32706), Fermi/GBM (GCN #32708, #32737, ATel #15672), Swift (ATel #15667), and NICER (ATel #15674). The time of the radio burst (2022-10-14 19:21:47) detected by CHIME/FRB (Atel #15681) and the associated X-ray burst detected by GECAM and HEBS (Atel #15682) and Konus-Wind (GCN #2770) falls within a SAA passage. Moreover AGILE AC is also detecting activity related to the bursts reported by Konus-Wind  (GCN #32768) and Fermi/GBM (GCN #32764). We selected significant AC Top events occurring when SGR J1935+2154 was within the AGILE field-of-view at off-axis angles <= 70 degrees. We report the following 33 X-ray bursts at times within 2hrs from the Swift, Fermi/GBM, and Konus-Wind bursts:     Date (UT)         Counts    Significance  2022-10-01 21:57:59  3970.43    11.69 sigma ; +1h  from Fermi/GBM trigger  2022-10-02 10:24:05  3944.53    13.33 sigma ; -1h  from Fermi/GBM trigger  2022-10-02 11:45:31  4022.77    14.72 sigma ; +12m from Fermi/GBM trigger  2022-10-02 11:54:18  3899.73    12.54 sigma ; +21m from Fermi/GBM trigger  2022-10-05 15:46:44  4367.29    18.83 sigma ; +11m from Fermi/GBM trigger  2022-10-05 21:06:08  4031.74    15.32 sigma ; -44m from Fermi/GBM trigger  2022-10-05 21:54:00  3747.75    10.27 sigma ; +4m  from Fermi/GBM trigger  2022-10-10 01:35:58  3902.83    14.00 sigma ; -4m  from Swift trigger  2022-10-10 09:05:40  3891.70    10.29 sigma ; -10m from Swift trigger  2022-10-10 14:00:03  3886.20    10.44 sigma ; -12m from Swift trigger  2022-10-10 20:53:32  3714.24    10.88 sigma ; -30m from Swift trigger  2022-10-10 21:40:42  3786.05    12.17 sigma ; +12m from Swift trigger  2022-10-10 23:19:25  3673.79    10.16 sigma ; +1h50m from Swift trigger  2022-10-11 10:27:56  4061.66    14.66 sigma ; -14m from Fermi/GBM trigger  2022-10-11 10:44:26  4156.55    16.33 sigma ; +3m  from Fermi/GBM trigger  2022-10-11 13:56:18  4089.80    11.43 sigma ; -15m from Fermi/GBM trigger  2022-10-12 12:47:10  3771.73    7.33  sigma ; +6s from Fermi/GBM trigger  2022-10-12 14:23:18  3977.49    10.88 sigma ; +30s from Fermi/GBM trigger  2022-10-12 14:44:45  4361.14    17.14 sigma ; +22m from Fermi/GBM trigger  2022-10-12 15:51:41  3959.15    10.21 sigma ; +11m from Fermi/GBM trigger  2022-10-12 16:21:38  4143.65    13.39 sigma ; +11m from Fermi/GBM trigger  2022-10-12 17:08:20  4335.50    16.19 sigma ; +8m  from Fermi/GBM trigger  2022-10-13 22:47:40  3704.51   10.49 sigma ; +6m  from trigger KW  2022-10-14 06:55:27  3932.92   11.37 sigma ; -17m from trigger KW  2022-10-14 07:12:35  3720.07   7.65  sigma ; +6s from trigger KW, +7s from trigger FERMI/GBM  2022-10-14 07:24:52  3728.30   7.80  sigma ; +10s from trigger FERMI/GBM  2022-10-14 08:25:59  4016.67   12.83 sigma ; +1h13m from KW trigger  2022-10-14 08:33:00  3890.61   10.63 sigma ; +1h21m from KW trigger  2022-10-14 08:38:24  4502.51   21.31 sigma ; +1h26m from KW trigger  2022-10-14 11:40:42  3782.95   7.32  sigma ; -1'10s from Fermi/GBM trigger  2022-10-14 13:20:48  3801.83   8.37  sigma ; +17s from Fermi/GBM trigger  2022-10-14 13:29:21  3917.88   10.39 sigma ; +9m   from Fermi/GBM trigger  2022-10-14 14:29:38  4317.47   17.32 sigma ; +25m  from Fermi/GBM trigger where the typical burst duration is one second (single bin). An AGILE AC ratemeters light curve can be found at https://tools.ssdc.asi.it/ImgView/Agile/AGILE-AC-RM_SGR_burst_14_10_2253 Additional analysis of AGILE data is in progress.