          Column        Format          Unit                                       Description                                 ------------------ -------- --------------------- --------------------------------------------------------------------- --        GRBname          A0              -                                         GRB name.                                       Trig\_ID        I00              -                          Special ID associated with the trigger.                                                                                      For GRBs found in ground analysis,                                                                         the ID are associated with the trigger ID of the failed event data,                                                          or the full observation ID of the event data for the analysis.            00\_00kev        A00     $\rm erg \ cm^{-0}$                       Photon flux in $00-00$ keV.                           00\_00kev\_low     A00     $\rm erg \ cm^{-0}$             The lower limit of photon flux in $00-00$ keV.                  00\_00kev\_hi      A00     $\rm erg \ cm^{-0}$             The upper limit of photon flux in $00-00$ keV.                    00\_00kev        A00     $\rm erg \ cm^{-0}$                       Photon flux in $00-00$ keV.                           00\_00kev\_low     A00     $\rm erg \ cm^{-0}$             The lower limit of photon flux in $00-00$ keV.                  00\_00kev\_hi      A00     $\rm erg \ cm^{-0}$             The upper limit of photon flux in $00-00$ keV.                    00\_000kev       A00     $\rm erg \ cm^{-0}$                      Photon flux in $00-000$ keV.                          00\_000kev\_low     A00     $\rm erg \ cm^{-0}$             The lower limit of photon flux in $00-000$ keV.                 00\_000kev\_hi     A00     $\rm erg \ cm^{-0}$             The upper limit of photon flux in $00-000$ keV.                  000\_000kev       A00     $\rm erg \ cm^{-0}$                      Photon flux in $000-000$ keV.                         000\_000kev\_low    A00     $\rm erg \ cm^{-0}$            The lower limit of photon flux in $000-000$ keV.                000\_000kev\_hi     A00     $\rm erg \ cm^{-0}$            The upper limit of photon flux in $000-000$ keV.                  000\_000kev       A00     $\rm erg \ cm^{-0}$                      Photon flux in $000-000$ keV.                         000\_000kev\_low    A00     $\rm erg \ cm^{-0}$            The lower limit of photon flux in $000-000$ keV.                000\_000kev\_hi     A00     $\rm erg \ cm^{-0}$            The upper limit of photon flux in $000-000$ keV.                   00\_000kev       A00     $\rm erg \ cm^{-0}$                      Photon flux in $00-000$ keV.                          00\_000kev\_low     A00     $\rm erg \ cm^{-0}$             The lower limit of photon flux in $00-000$ keV.                 00\_000kev\_hi     A00     $\rm erg \ cm^{-0}$             The upper limit of photon flux in $00-000$ keV.                   00\_000kev       A00     $\rm erg \ cm^{-0}$                      Photon flux in $00-000$ keV.                          00\_000kev\_low     A00     $\rm erg \ cm^{-0}$             The lower limit of photon flux in $00-000$ keV.                 00\_000kev\_hi     A00     $\rm erg \ cm^{-0}$             The upper limit of photon flux in $00-000$ keV.                 Exposure\_time     A00              s                            The time interval of the spectrum.                         T000\_start       A00              s                              The start time of the spectrum,                                                                                           relative to the BAT trigger time.                          T000\_stop       A00              s                               The end time of the spectrum,                                                                                            relative to the BAT trigger time.                       :  \[tab:spec\_T000\_pow\_energy\_fluence\] The format of the table that presents the energy fluences (in unit of $\rm erg \ cm^{-0}$) from the PL fit for the time-averaged ($T_{000}$) spectra. Note that this table includes the fit for every GRB, regardless of whether the fit is acceptable from the criteria listed in Section \[sect:event\_standard\]. A list of GRBs with acceptable fits can be found in Table \[tab:spec\_T000\_best\_model\]. (This table is available in its entirety in a machine-readable form in the online journal. Only the column titles are shown here for guidance regarding its form and content.)  S