Title: 17 Years of Magnetar Bursts Observed with the Fermi {Gamma}-ray Burst Monitor Authors: Godwin M., Keskin O., Demirer M., Yi Y.-J., Lin L., Roberts O.J., Gogus E., Kaneko Y., Briggs M., Baring M.G., Burns E., Palmer D.M., Hristov B.A., Mailyan B., Malacaria C., Palafox E., Kouveliotou C., van der Horst A.J., Veres P., Younes G. Table: 1254 magnetar bursts observed with Fermi GBM ================================================================================ Columns Units Explanations -------------------------------------------------------------------------------- 01 EventMET s Event Burst start time in Fermi MET (1)(2) 02 EventUTC --- Event Burst start date/time in UTC (YYMMDD HH:MM:SS) 03 BurstName --- Burst Name (3) 04 BB_Dur ms Bayesian block duration 05 DET --- NaI detectors (4) 06 RAdeg deg Right Ascension, decimal degrees (J2000) 07 DEdeg deg Declination, decimal degrees (J2000) 08 PosErr deg Positional error (5) 09 MPS --- Most Probable Source 10 Other --- Other Detection (6) 11 Binned ???? --- g=Burst lies within a 64-ms long time bin of the triggered data -------------------------------------------------------------------------------- Note (1): Fermi Mission Elapsed Time is the number of seconds elapsed since 00:00:00 UTC on January 1, 2001. Note (2): * = Saturated events; The saturated parts of these events were excluded from the spectral analysis. Note (3): Burst name from the Fermi-GBM Trigger Catalog. If this space is blank, the event was untriggered. Note (4): Brightest detectors used in spectral analysis and with detector-to-source angle less than 60â—¦and not partially or fully blocked by the spacecraft itself (ordered by brightness). Note (5): Radius of a circle with equivalent area to the 1 sigma error contour. 0 degree error means that an untriggered event was assigned the known location of its confirmed source. Note (6): y = Event was also detected by Swift BAT