s peak spectrum for each burst. (This table is available in its entirety in a machine-readable form in the online journal. Only the column formats are shown here for guidance regarding its form and content.)         Column       Format                    Unit                                                  Description   ---------------- -------- ---------------------------------------- --------------------------------------------------------------------------       GRBname         A0                       -                                                     GRB name.       Trig\_ID       I00                       -                                     Special ID associated with each triggers.                                                                                          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.        alpha         A00                       -                                   $\alpha^{\rm PL}$ as defined in Eq. \[eq:PL\].      alpha\_low      A00                       -                                       The lower limit of $\alpha^{\rm PL}$.      alpha\_hi       A00                       -                                       The upper limit of $\alpha^{\rm PL}$.         norm         A00     $\rm ph \ cm^{-0} \ s^{-0} \ keV^{-0}$   The normalization factor $K^{\rm PL}_{00}$, as defined in Eq. \[eq:PL\].      norm\_low       A00     $\rm ph \ cm^{-0} \ s^{-0} \ keV^{-0}$                    The lower limit of $K^{\rm PL}_{00}$.       norm\_hi       A00     $\rm ph \ cm^{-0} \ s^{-0} \ keV^{-0}$                    The upper limit of $K^{\rm PL}_{00}$.         chi0         F0.0                      -                                   $\chi^0$ from the fitting, reported by XSPEC.         dof           I0                       -                               degree of freedom from the fitting, reported by XSPEC.    reduced\_chi0     F0.0                      -                        reduced $\chi^0$ (i.e., $\chi^0$ divided by the degree of freedom),                                                                                                  reported by XSPEC.      null\_prob      A00                       -                               The null probability of the model, reported by XSPEC.        enorm         F0.0                     KeV                          The normalization energy, which is set to 00 keV in our fits,                                                                                              as shown in Eq. \[eq:PL\].    Exposure\_time     A0                       s                                         The time interval of the spectrum.     Peak\_start      A00                       s                                          The start time of the spectrum,                                                                                          relative to the BAT trigger time.      Peak\_stop      A00                       s                                           The end time of the spectrum,                                                                                          relative to the BAT trigger time.    :  \[tab:spec\_00mspeak\_pow\_parameter\] The format of the table that presents the parameters from the PL fit for the 00-ms peak 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 \[tab:spec\_00mspeak\_best\_model\]. (This table is available in its entirety in a machine-readable form in the online journal. Only the column formats are shown here for guidance regarding its form and content.)          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     $\rm ph \ cm^{-0} \ s^{-0}$                       Photon flux in $00-00$ keV.     00\_00kev\_low     A00     $\rm ph \ cm^{-0} \ s^{-0}$             The lower limit of photon flux in $00-00$ keV.     00\_00kev\_hi      A00     $\rm ph \ cm^{-0} \ s^{-0}$             The upper limit of photon flux in $00-00$ keV.       00\_00kev        A00     $\rm ph \ cm^{-0} \ s^{-0}$                       Photon flux in $00-00$ keV.     00\_00kev\_low     A00     $\rm ph \ cm^{-0} \ s^{-0}$             The lower limit of photon flux in $00-00$ keV.     00\_00kev\_hi      A00     $\rm ph \ cm^{-0} \ s^{-0}$             The upper limit of photon flux in $00-00$ keV.       00\_000kev       A00     $\rm ph \ cm^{-0} \ s^{-0}$                      Photon flux in $00-000$ keV.    00\_000kev\_low     A00     $\rm ph \ cm^{-0} \ s^{-0}$             The lower limit of photon flux in $00-000$ keV.     00\_000kev\_hi     A00     $\rm ph \ cm^{-0} \ s^{-0}$             The upper limit of photon flux in $00-000$ keV.      000\_000kev       A00     $\rm ph \ cm^{-0} \ s^{-0}$                      Photon flux in $000-000$ keV.    000\_000kev\_low    A00     $\rm ph \ cm^{-0} \ s^{-0}$            The lower limit of photon flux in $000-000$ keV.    000\_000kev\_hi     A00     $\rm ph \ cm^{-0} \ s^{-0}$            The upper limit of photon flux in $000-000$ keV.      000\_000kev       A00     $\rm ph \ cm^{-0} \ s^{-0}$                      Photon flux in $000-000$ keV.    000\_000kev\_low    A00     $\rm ph \ cm^{-0} \ s^{-0}$            The lower limit of photon flux in $000-000$ keV.    000\_000kev\_hi     A00     $\rm ph \ cm^{-0} \ s^{-0}$            The upper limit of photon flux in $000-000$ keV.       00\_000kev       A00     $\rm ph \ cm^{-0} \ s^{-0}$                      Photon flux in $00-000$ keV.    00\_000kev\_low     A00     $\rm ph \ cm^{-0} \ s^{-0}$             The lower limit of photon flux in $00-000$ keV.     00\_000kev\_hi     A00     $\rm ph \ cm^{-0} \ s^{-0}$             The upper limit of photon flux in $00-000$ keV.       00\_000kev       A00     $\rm ph \ cm^{-0} \ s^{-0}$                      Photon flux in $00-000$ keV.    00\_000kev\_low     A00     $\rm ph \ cm^{-0} \ s^{-0}$             The lower limit of photon flux in $00-000$ keV.     00\_000kev\_hi     A00     $\rm ph \ cm^{-0} \ s^{-0}$             The upper limit of photon flux in $00-000$ keV.     Exposure\_time     A00                  s                                The time interval of the spectrum.      Peak\_start       A00                  s                                  The start time of the spectrum,                                                                               relative to the BAT trigger time.       Peak\_stop       A00                  s                                   The end time of the spectrum,                                                                               relative to the BAT trigger time.    :  \[tab:spec\_00mspeak\_pow\_photon\_flux\] The format of the table that presents the photon flux (in unit of $\rm ph \ cm^{-0} \ s^{-0}$) from the PL fit for the 00-ms peak 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 \[tab:spec\_00mspeak\_best\_model\]. (This table is available in its entirety in a machine-readable form in the online journal. Only the column formats are shown here for guidance regarding its form and content.)          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     $\rm erg \ cm^{-0} \ s^{-0}$                       Photon flux in $00-00$ keV.                           00\_00kev\_low     A00     $\rm erg \ cm^{-0} \ s^{-0}$             The lower limit of photon flux in $00-00$ keV.                  00\_00kev\_hi      A00     $\rm erg \ cm^{-0} \ s^{-0}$             The upper limit of photon flux in $00-00$ keV.                    00\_00kev        A00     $\rm erg \ cm^{-0} \ s^{-0}$                       Photon flux in $00-00$ keV.                           00\_00kev\_low     A00     $\rm erg \ cm^{-0} \ s^{-0}$             The lower limit of photon flux in $00-00$ keV.                  00\_00kev\_hi      A00     $\rm erg \ cm^{-0} \ s^{-0}$             The upper limit of photon flux in $00-00$ keV.                    00\_000kev       A00     $\rm erg \ cm^{-0} \ s^{-0}$                      Photon flux in $00-000$ keV.                          00\_000kev\_low     A00     $\rm erg \ cm^{-0} \ s^{-0}$             The lower limit of photon flux in $00-000$ keV.                 00\_000kev\_hi     A00     $\rm erg \ cm^{-0} \ s^{-0}$             The upper limit of photon flux in $00-000$ keV.                  000\_000kev       A00     $\rm erg \ cm^{-0} \ s^{-0}$                      Photon flux in $000-000$ keV.                         000\_000kev\_low    A00     $\rm erg \ cm^{-0} \ s^{-0}$            The lower limit of photon flux in $000-000$ keV.                000\_000kev\_hi     A00     $\rm erg \ cm^{-0} \ s^{-0}$            The upper limit of photon flux in $000-000$ keV.                  000\_000kev       A00     $\rm erg \ cm^{-0} \ s^{-0}$                      Photon flux in $000-000$ keV.                         000\_000kev\_low    A00     $\rm erg \ cm^{-0} \ s^{-0}$            The lower limit of photon flux in $000-000$ keV.                000\_000kev\_hi     A00     $\rm erg \ cm^{-0} \ s^{-0}$            The upper limit of photon flux in $000-000$ keV.                   00\_000kev       A00     $\rm erg \ cm^{-0} \ s^{-0}$                      Photon flux in $00-000$ keV.                          00\_000kev\_low     A00     $\rm erg \ cm^{-0} \ s^{-0}$             The lower limit of photon flux in $00-000$ keV.                 00\_000kev\_hi     A00     $\rm erg \ cm^{-0} \ s^{-0}$             The upper limit of photon flux in $00-000$ keV.                   00\_000kev       A00     $\rm erg \ cm^{-0} \ s^{-0}$                      Photon flux in $00-000$ keV.                          00\_000kev\_low     A00     $\rm erg \ cm^{-0} \ s^{-0}$             The lower limit of photon flux in $00-000$ keV.                 00\_000kev\_hi     A00     $\rm erg \ cm^{-0} \ s^{-0}$             The upper limit of photon flux in $00-000$ keV.                 Exposure\_time     A00                  s                                 The time interval of the spectrum.                         Peak\_start       A00                  s                                   The start time of the spectrum,                                                                                                    relative to the BAT trigger time.                          Peak\_stop       A00                  s                                    The end time of the spectrum,                                                                                                     relative to the BAT trigger time.                       :  \[tab:spec\_00mspeak\_pow\_energy\_flux\] The format of the table that presents the energy flux (in unit of $\rm erg \ s^{-0} \ cm^{-0}$) from the PL fit for the 00-ms peak 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 \[tab:spec\_00mspeak\_best\_model\]. (This table is available in its entirety in a machine-readable form in the online journal. Only the column formats are shown here for guidance regarding its form and content.)          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.                         Peak\_start       A00              s                              The start time of the spectrum,                                                                                           relative to the BAT trigger time.                          Peak\_stop       A00              s                               The end time of the spectrum,                                                                                            relative to the BAT trigger time.                       :  \[tab:spec\_00mspeak\_pow\_energy\_fluence\] The format of the table that presents the energy fluences (in unit of $\rm erg \ cm^{-0}$) from the PL fit for the 00-ms peak 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 \[tab:spec\_00mspeak\_best\_model\]. (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.)         Column       Format                    Unit                                                   Description                                     ---------------- -------- ---------------------------------------- ---------------------------------------------------------------------------- --       GRBname         A0                       -                                                      GRB name.                                          Trig\_ID       I00                       -                                      Special ID associated with each triggers.                                                                                                              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.                alpha         A00                       -                                   $\alpha^{\rm CPL}$ as defined in Eq. \[eq:CPL\].                     alpha\_low      A00                       -                                        The lower limit of $\alpha^{\rm CPL}$.                          alpha\_hi       A00                       -                                        The upper limit of $\alpha^{\rm CPL}$.                            Epeak         A00                      keV                                    $E_{\rm peak}$ as defined in Eq. \[eq:CPL\].                       Epeak\_low      A00                      keV                                         The lowe limit of $E_{\rm peak}$.                             Epeak\_hi       A00                      keV                                         The upper limit of $E_{\rm peak}$.                               norm         A00     $\rm ph \ cm^{-0} \ s^{-0} \ keV^{-0}$   The normalization factor $K^{\rm CPL}_{00}$, as defined in Eq. \[eq:CPL\].        norm\_low       A00     $\rm ph \ cm^{-0} \ s^{-0} \ keV^{-0}$                     The lower limit of $K^{\rm CPL}_{00}$.                           norm\_hi       A00     $\rm ph \ cm^{-0} \ s^{-0} \ keV^{-0}$                     The upper limit of $K^{\rm CPL}_{00}$.                             chi0         F0.0                      -                                    $\chi^0$ from the fitting, reported by XSPEC.                          dof           I0                       -                                degree of freedom from the fitting, reported by XSPEC.                reduced\_chi0     F0.0                      -                         reduced $\chi^0$ (i.e., $\chi^0$ divided by the degree of freedom),                                                                                                         reported by XSPEC.                                    null\_prob      A00                       -                                The null probability of the model, reported by XSPEC.                     enorm         F0.0                     KeV                           The normalization energy, which is set to 00 keV in our fits,                                                                                                        as shown in Eq. \[eq:PL\].                              Exposure\_time     A0                       s                                          The time interval of the spectrum.                           Peak\_start      A00                       s                                           The start time of the spectrum,                                                                                                                   relative to the BAT trigger time.                             Peak\_stop      A00                       s                                            The end time of the spectrum,                                                                                                                    relative to the BAT trigger time.                           :  \[tab:spec\_00mspeak\_cutpow\_parameter\] The format of the table that presents the parameters from the CPL fit for the 00-ms peak 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 \[tab:spec\_00mspeak\_best\_model\]. (This table is available in its entirety in a machine-readable form in the online journal. Only the column formats are shown here for guidance regarding its form and content.)          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     $\rm ph \ cm^{-0} \ s^{-0}$                       Photon flux in $00-00$ keV.                           00\_00kev\_low     A00     $\rm ph \ cm^{-0} \ s^{-0}$             The lower limit of photon flux in $00-00$ keV.                  00\_00kev\_hi      A00     $\rm ph \ cm^{-0} \ s^{-0}$             The upper limit of photon flux in $00-00$ keV.                    00\_00kev        A00     $\rm ph \ cm^{-0} \ s^{-0}$                       Photon flux in $00-00$ keV.                           00\_00kev\_low     A00     $\rm ph \ cm^{-0} \ s^{-0}$             The lower limit of photon flux in $00-00$ keV.                  00\_00kev\_hi      A00     $\rm ph \ cm^{-0} \ s^{-0}$             The upper limit of photon flux in $00-00$ keV.                    00\_000kev       A00     $\rm ph \ cm^{-0} \ s^{-0}$                      Photon flux in $00-000$ keV.                          00\_000kev\_low     A00     $\rm ph \ cm^{-0} \ s^{-0}$             The lower limit of photon flux in $00-000$ keV.                 00\_000kev\_hi     A00     $\rm ph \ cm^{-0} \ s^{-0}$             The upper limit of photon flux in $00-000$ keV.                  000\_000kev       A00     $\rm ph \ cm^{-0} \ s^{-0}$                      Photon flux in $000-000$ keV.                         000\_000kev\_low    A00     $\rm ph \ cm^{-0} \ s^{-0}$            The lower limit of photon flux in $000-000$ keV.                000\_000kev\_hi     A00     $\rm ph \ cm^{-0} \ s^{-0}$            The upper limit of photon flux in $000-000$ keV.                  000\_000kev       A00     $\rm ph \ cm^{-0} \ s^{-0}$                      Photon flux in $000-000$ keV.                         000\_000kev\_low    A00     $\rm ph \ cm^{-0} \ s^{-0}$            The lower limit of photon flux in $000-000$ keV.                000\_000kev\_hi     A00     $\rm ph \ cm^{-0} \ s^{-0}$            The upper limit of photon flux in $000-000$ keV.                   00\_000kev       A00     $\rm ph \ cm^{-0} \ s^{-0}$                      Photon flux in $00-000$ keV.                          00\_000kev\_low     A00     $\rm ph \ cm^{-0} \ s^{-0}$             The lower limit of photon flux in $00-000$ keV.                 00\_000kev\_hi     A00     $\rm ph \ cm^{-0} \ s^{-0}$             The upper limit of photon flux in $00-000$ keV.                   00\_000kev       A00     $\rm ph \ cm^{-0} \ s^{-0}$                      Photon flux in $00-000$ keV.                          00\_000kev\_low     A00     $\rm ph \ cm^{-0} \ s^{-0}$             The lower limit of photon flux in $00-000$ keV.                 00\_000kev\_hi     A00     $\rm ph \ cm^{-0} \ s^{-0}$             The upper limit of photon flux in $00-000$ keV.                 Exposure\_time     A00                  s                                The time interval of the spectrum.                         Peak\_start       A00                  s                                  The start time of the spectrum,                                                                                                   relative to the BAT trigger time.                          Peak\_stop       A00                  s                                   The end time of the spectrum,                                                                                                    relative to the BAT trigger time.                       :  \[tab:spec\_00mspeak\_cutpow\_photon\_flux\] The format of the table that presents the photon flux (in unit of $\rm ph \ s^{-0} \ cm^{-0}$) from the CPL fit for the 00-ms peak 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 \[tab:spec\_00mspeak\_best\_model\]. (This table is available in its entirety in a machine-readable form in the online journal. Only the column formats are shown here for guidance regarding its form and content.)          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     $\rm erg \ cm^{-0} \ s^{-0}$                       Photon flux in $00-00$ keV.                           00\_00kev\_low     A00     $\rm erg \ cm^{-0} \ s^{-0}$             The lower limit of photon flux in $00-00$ keV.                  00\_00kev\_hi      A00     $\rm erg \ cm^{-0} \ s^{-0}$             The upper limit of photon flux in $00-00$ keV.                    00\_00kev        A00     $\rm erg \ cm^{-0} \ s^{-0}$                       Photon flux in $00-00$ keV.                           00\_00kev\_low     A00     $\rm erg \ cm^{-0} \ s^{-0}$             The lower limit of photon flux in $00-00$ keV.                  00\_00kev\_hi      A00     $\rm erg \ cm^{-0} \ s^{-0}$             The upper limit of photon flux in $00-00$ keV.                    00\_000kev       A00     $\rm erg \ cm^{-0} \ s^{-0}$                      Photon flux in $00-000$ keV.                          00\_000kev\_low     A00     $\rm erg \ cm^{-0} \ s^{-0}$             The lower limit of photon flux in $00-000$ keV.                 00\_000kev\_hi     A00     $\rm erg \ cm^{-0} \ s^{-0}$             The upper limit of photon flux in $00-000$ keV.                  000\_000kev       A00     $\rm erg \ cm^{-0} \ s^{-0}$                      Photon flux in $000-000$ keV.                         000\_000kev\_low    A00     $\rm erg \ cm^{-0} \ s^{-0}$            The lower limit of photon flux in $000-000$ keV.                000\_000kev\_hi     A00     $\rm erg \ cm^{-0} \ s^{-0}$            The upper limit of photon flux in $000-000$ keV.                  000\_000kev       A00     $\rm erg \ cm^{-0} \ s^{-0}$                      Photon flux in $000-000$ keV.                         000\_000kev\_low    A00     $\rm erg \ cm^{-0} \ s^{-0}$            The lower limit of photon flux in $000-000$ keV.                000\_000kev\_hi     A00     $\rm erg \ cm^{-0} \ s^{-0}$            The upper limit of photon flux in $000-000$ keV.                   00\_000kev       A00     $\rm erg \ cm^{-0} \ s^{-0}$                      Photon flux in $00-000$ keV.                          00\_000kev\_low     A00     $\rm erg \ cm^{-0} \ s^{-0}$             The lower limit of photon flux in $00-000$ keV.                 00\_000kev\_hi     A00     $\rm erg \ cm^{-0} \ s^{-0}$             The upper limit of photon flux in $00-000$ keV.                   00\_000kev       A00     $\rm erg \ cm^{-0} \ s^{-0}$                      Photon flux in $00-000$ keV.                          00\_000kev\_low     A00     $\rm erg \ cm^{-0} \ s^{-0}$             The lower limit of photon flux in $00-000$ keV.                 00\_000kev\_hi     A00     $\rm erg \ cm^{-0} \ s^{-0}$             The upper limit of photon flux in $00-000$ keV.                 Exposure\_time     A00                  s                                 The time interval of the spectrum.                         Peak\_start       A00                  s                                   The start time of the spectrum,                                                                                                    relative to the BAT trigger time.                          Peak\_stop       A00                  s                                    The end time of the spectrum,                                                                                                     relative to the BAT trigger time.                       :  \[tab:spec\_00mspeak\_cutpow\_energy\_flux\] The format of the table that presents the energy flux (in unit of $\rm erg \ s^{-0} \ cm^{-0}$) from the CPL fit for the 00-ms peak 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 \[tab:spec\_00mspeak\_best\_model\]. (This table is available in its entirety in a machine-readable form in the online journal. Only the column formats are shown here for guidance regarding its form and content.)          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.                         Peak\_start       A00              s                              The start time of the spectrum,                                                                                           relative to the BAT trigger time.                          Peak\_stop       A00              s                               The end time of the spectrum,                                                                                            relative to the BAT trigger time.                       :  \[tab:spec\_00mspeak\_cutpow\_energy\_fluence\] The format of the table that presents the energy fluence in unit of $\rm erg \ s^{-0}$ from the CPL fit for the 00-ms peak 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 \[tab:spec\_00mspeak\_best\_model\]. (This table is available in its entirety in a machine-readable form in the online journal. Only the column formats are shown here for guidance regarding its form and content.)  A list of GRBs with bright X-ray sources in the same field of view ------------------------------------------------------------------     