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## BAT5BGRBSP - CGRO/BATSE 5B Gamma-Ray Burst Spectral Catalog |
HEASARC Archive |

This table lists all of the spectroscopy results of gamma-ray bursts observed by a subset of the 8 BATSE Large Area Detectors. BATSE consisted, in part, of an array of 8 sodium iodide Large Area Detectors (LADs) which covered the energy range from ~20 keV - 2 MeV. The LAD detectors were placed at each of the eight corners of the CGRO spacecraft with an outward orientation such that the entire sky not occulted by the Eartt was observed. The spectrum files ("scat" files) available as FITS-format data products associated with this catalog provide parameter values and goodness-of-fit measures for different types of spectral fits and models. These fits are performed using 14-channel data, usually 2-second resolution CONT data. There are currently two spectrum categories:

* Peak flux ('pflx') - a single spectrum over a 2.05-second time range at the peak flux of the burst * Fluence ('flnc') - a single spectrum over the entire burst durationThe quoted fluxes and fluences are for the 20 keV - 2 MeV energy range, notice. The scat files have two extensions. The first extension gives detector-specific information, including photon fluxes and fluences for each detector, which are provided for each energy channel. The second extension provides derived quantities such as flux, fluence and model parameters for the joint fit of all included detectors. The scat files and their energy-resolved quantities contained in these two extensions will be available soon in the HEASARC data archive. Quantities derived from these spectral fits are available in the present table, as described below and in the Goldstein et al. (2013) reference paper.

The spectra are fit with a number of models, with the signal-to-noise ratio of the spectrum often determining whether a more complex model is statistically favored. The current set is:

* Power law ('plaw'), * Comptonized (exponentially attenuated power law; 'comp') * Band ('band') * Smoothly broken power law ('sbpl') * Log_10 Gaussian ('glog')The full details of these models are presented in Section 4 of the reference paper.

The type of spectrum and spectral model are coded into the parameter names
(and the associated file names) using the acronyms given above. Thus for
example, the parameters with names beginning with 'flnc_glog' contain the
results from fits to the fluence spectra using Log_{10} Gaussian models. The
corresponding spectrum file for the burst with trigger number 105 with the
results from a fit to the fluence spectrum using a Log_{10} Gaussian model is
named scat_0105_flnc_glog_v00.fit.

Please note that this table lists the raw results of each spectral fit to each GRB. In cases where the spectral fit failed, the values reported are those that initialized the spectral fit. If the uncertainty on the spectral parameters is reported as zero (no uncertainty), then the fit failed. In a few cases throughout this table, the uncertainties for certain spectral parameters may be reported as '9999.99' which indicates that the uncertainty on that parameter is completely unconstrained. An example of this is when the spectral data from a burst is fitted with a BAND function but is unable to constrain the high-energy index. In this case, the best fit centroid value of the high-energy index parameter is reported, and the '9999.99' value is reported for the uncertainty.

The BATSE 5B Gamma-Ray Burst Spectral Catalog. Goldstein A., Preece R. D., Mallozzi R. S., Briggs M. S., Fishman G. J., Kouveliotou C., Paciesas W. S., Burgess J. M. <Astrophys. J. Suppl. 208, 21 (2013)> =2013ApJS..208...21G (SIMBAD/NED BibCode)

**Trigger_Num**

The BATSE trigger designation that is assigned for each new
trigger detected. The naming scheme used is an incrementing trigger number,
where 105 is the minimum and 8121 is the maximum trigger number in this table.

**Name**

The BATSE burst name. This was not present in the reference paper
tables but was added by the HEASARC using the relevant information in the
BATSEGRB table (see http://heasarc.gsfc.nasa.gov/W3Browse/cgro/batsegrb.html
for more information). Each burst has a unique catalog name. These names may
have a prefix of either "4B" or "GRB". The "4B" prefix means that the burst is
listed in BATSE 4B Catalog, while the "GRB" prefix means that the burst is
listed in the BATSE Current Gamma-Ray Burst Catalog. The prefix is followed by
the "yymmdd" (date) of the burst, where "yymmdd" is the two digit year, two
digit month, and two digit day. An ending hyphen is added when this name is
not unique, i.e., when there were two or more bursts on a particular day.

**RA**

The Right Ascension of the object that triggered the BATSE instrument in
the selected equinox. This was not present in the reference paper
tables but was added by the HEASARC using the relevant information in the
BATSEGRB table (see http://heasarc.gsfc.nasa.gov/W3Browse/cgro/batsegrb.html
for more information).

**Dec**

The Declination of the object that triggered the BATSE instrument in
the selected equinox. This was not present in the reference paper
tables but was added by the HEASARC using the relevant information in the
BATSEGRB table (see http://heasarc.gsfc.nasa.gov/W3Browse/cgro/batsegrb.html
for more information).

**LII**

The Galactic Longitude of the object that triggered the BATSE
instrument.

**BII**

The Galactic Latitude of the object that triggered the BATSE instrument.

**Trigger_Time**

The burst trigger time defined as the end of the interval
(64, 256 or 1024 ms) in which the burst triggered the detector. The time
system for the values is UT. This was not present in the reference paper
tables but was added by the HEASARC using the relevant information in the
BATSEGRB table (see http://heasarc.gsfc.nasa.gov/W3Browse/cgro/batsegrb.html
for more information).

**Seconds_Trigger**

The burst trigger time, in decimal seconds of the day (UT)
on which it occurred. The burst trigger time is the end of the interval (64,
256 or 1024 ms) in which the burst triggered the detector. This was not
present in the reference paper
tables but was added by the HEASARC using the relevant information in the
BATSEGRB table (see http://heasarc.gsfc.nasa.gov/W3Browse/cgro/batsegrb.html
for more information).

**T90**

The 90% duration of the burst in seconds. T90 measures the duration of
the time interval during which 90% of the total observed counts in the burst
have been detected. The start of the T90 interval is defined by the time at
which 5% of the total counts have been detected, and the end of the T90
interval is defined by the time at which 95% of the total counts have been
detected. This was not present in the reference paper
tables but was added by the HEASARC using the relevant information in the
BATSEGRB table (see http://heasarc.gsfc.nasa.gov/W3Browse/cgro/batsegrb.html
for more information).

**T90_Error**

The uncertainty in the T90 duration, in seconds. This was not
present in the reference paper
tables but was added by the HEASARC using the relevant information in the
BATSEGRB table (see http://heasarc.gsfc.nasa.gov/W3Browse/cgro/batsegrb.html
for more information).

**Lad_Numbers**

The LAD detectors which detected the burst. There were 8
detector modules on CGRO each of which contained a LAD
(numbered 0 through 7). A GRB could illuminate up to 4 detectors

**Lad_Data_Type**

The LAD data type, 'CONT' or 'MER'. The primary data type
used in this catalog is the 2.048 s resolution CONT data, which provided
semi-continuous count rate and 16 channel spectral coverage during the entire
BATSE lifetime. When CONT data were not available (usually due to data
corruption), the associated MER data were used if possible. The native time
resolution of MER data was 16 ms but only started at trigger time and extended
to less than 200 s after trigger. The energy resolution is the same as CONT
data, so the count rates were binned to 2.048 s in order to be compatible with
CONT data. MER data were used only if a background model could be fit to the
post-burst background and extrapolated through the duration of the burst. MER
data were used for only 15 GRBs in this catalog.

**Pflx_Band_Ampl**

The amplitude of a Band function fit to a single spectrum
over the time range of the peak flux of the burst, in photon/cm^{2}/s/keV.

**Pflx_Band_Ampl_Error**

The 1-sigma statistical error of the Band function
amplitude for the peak flux spectrum, in photon/cm^{2}/s/keV. An error value
of 0.0 implies a fixed parameter

**Pflx_Band_Alpha**

The low-energy power law index, alpha, of a Band function
fit to a single spectrum over the time range of the peak flux of the burst

**Pflx_Band_Alpha_Error**

The 1-sigma statistical error of the Band function
power law, alpha, for the
peak flux spectrum. An error of 0.0 implies a fixed parameter.

**Pflx_Band_Beta**

The high-energy power law index, beta, of a Band function
fit to a single spectrum over the time range of the peak flux of the burst.

**Pflx_Band_Beta_Error**

The 1-sigma statistical error of the Band function
power law, beta, for the
peak flux spectrum. An error of 0.0 implies a fixed parameter.

**Pflx_Band_Epeak**

The peak energy of a Band function fit to a single
nu*F_{nu} spectrum over the time range of the peak flux of the burst, in keV

**Pflx_Band_Epeak_Error**

The 1-sigma statistical error of the Band function
peak energy for the peak flux spectrum, in keV. An error of 0.0 implies a
fixed parameter.

**Pflx_Band_Phtflux**

The photon flux, in photon/cm^{2}/s, for a Band function
fit to a single spectrum over the time range of the peak flux of the burst.

**Pflx_Band_Phtflux_Error**

The 1-sigma statistical error in the photon flux,
in photon/cm^{2}/s, for the Band function peak flux spectrum.

**Pflx_Band_Phtflnc**

The photon fluence, in photon/cm^{2}, for a Band function
fit to a single spectrum over the time range of the peak flux of the burst.

**Pflx_Band_Phtflnc_Error**

The 1-sigma statistical error in the photon fluence,
in photon/cm^{2}, for the Band function peak flux spectrum.

**Pflx_Band_Flux**

The energy flux, in erg/cm^{2}/s, for a Band function fit to
a single spectrum over the time range of the peak flux of the burst.

**Pflx_Band_Flux_Error**

The 1-sigma statistical error on the energy flux, in
erg/cm^{2}/s, for the Band function peak flux spectrum.

**Pflx_Band_Flnc**

The energy fluence, in erg/cm^{2}, for a Band function fit to
a single spectrum over the time range of the peak flux of the burst.

**Pflx_Band_Flnc_Error**

The 1-sigma statistical error in the energy fluence,
in erg/cm^{2}, for the Band function peak flux spectrum.

**Pflx_Band_Chisq**

The chi-squared goodness of fit statistic for the Band
function fit to the peak flux spectrum.

**Pflx_Band_DoF**

The degrees of freedom for the Band function fit to the peak
flux spectrum.

**Pflx_Comp_Ampl**

The amplitude of a Comptonized (exponentially attenuated
power law) model fit to a single spectrum
over the time range of the peak flux of the burst, in photon/cm^{2}/s/keV.

**Pflx_Comp_Ampl_Error**

The 1-sigma statistical error of the Comptonized model
amplitude for the peak flux spectrum, in photon/cm^{2}/s/keV.
An error of 0.0 implies a fixed parameter.

**Pflx_Comp_Index**

The power law index of a Comptonized model fit to a single
spectrum over the time range of the peak flux of the burst.

**Pflx_Comp_Index_Error**

The 1-sigma statistical error of the Comptonized
model power law index for the
peak flux spectrum. An error of 0.0 implies a fixed parameter.

**Pflx_Comp_Epeak**

The peak energy of a Comptonized model fit to a single
nu*F_{nu} spectrum over the time range of the peak flux of the burst, in keV.

**Pflx_Comp_Epeak_Error**

The 1-sigma statistical error of the Comptonized
model peak energy for the peak
flux spectrum, in keV. An error of 0.0 implies a fixed parameter.

**Pflx_Comp_Phtflux**

The photon flux, in photon/cm^{2}/s, for a Comptonized
model fit to a single
spectrum over the time range of the peak flux of the burst.

**Pflx_Comp_Phtflux_Error**

The 1-sigma statistical error on the photon flux,
in photon/cm^{2}/s, for the Comptonized model peak flux spectrum.

**Pflx_Comp_Phtflnc**

The photon fluence in photon/cm^{2} for a Comptonized model
fit to a single
spectrum over the time range of the peak flux of the burst.

**Pflx_Comp_Phtflnc_Error**

The 1-sigma statistical error in the photon fluence,
in photon/cm^{2}, for the Comptonized model peak flux spectrum.

**Pflx_Comp_Flux**

The energy flux, in erg/cm^{2}/s, for a Comptonized model fit
to a single spectrum over the time range of the peak flux of the burst.

**Pflx_Comp_Flux_Error**

The 1-sigma statistical error on the energy flux, in
erg/cm^{2}/s, for the Comptonized model peak flux spectrum.

**Pflx_Comp_Flnc**

The energy fluence, in erg/cm^{2}, for a Comptonized model
fit to a single spectrum over the time range of the peak flux of the burst.

**Pflx_Comp_Flnc_Error**

The 1-sigma statistical error in the energy fluence,
in erg/cm^{2}, for the Comptonized model peak flux spectrum.

**Pflx_Comp_Chisq**

The chi-squared goodness of fit statistic for the
Comptonized model fit to the peak flux spectrum.

**Pflx_Comp_DoF**

The degrees of freedom for the Comptonized model fit to the
peak flux spectrum.

**Pflx_Glog_Ampl**

The amplitude of a Log_{10} Gaussian model fit to a single
spectrum over the
time range of the peak flux of the burst, in photon/cm^{2}/s/keV.

**Pflx_Glog_Ampl_Error**

The 1-sigma statistical error of the Log_{10} Gaussian
model amplitude for the peak flux spectrum, in photon/cm^{2}/s/keV. An error of
0.0 implies a fixed parameter.

**Pflx_Glog_FWHM**

The full width at half maximum of a Log_{10} Gaussian model
fit to a single spectrum over the time range of the peak flux of the burst, in
log_10(keV).

**Pflx_Glog_FWHM_Error**

The 1-sigma statistical error of the Log_{10} Gaussian
model full width at half maximum for the peak flux spectrum, in log_{10} (keV).
An error of 0.0 implies a fixed parameter.

**Pflx_Glog_Ecent**

The log_{10} of the centroid energy E_{cen} of a Log_{10}
Gaussian model fit to a single spectrum over the
time range of the peak flux of the burst, in keV.

**Pflx_Glog_Ecent_Error**

The 1-sigma statistical error of the Log_10 Gaussian
model log_{10} (E_{cen}) for the
peak flux spectrum, in keV. An error of 0.0 implies a fixed parameter.

**Pflx_Glog_Epeak**

The peak energy of a model fit to a single Log_{10}
Gaussian model nu*F_{nu} spectrum over the time range of the peak flux of
the burst, in keV.

**Pflx_Glog_Epeak_Error**

The 1-sigma statistical error of the
Log_{10} Gaussian model model peak energy for the peak
flux spectrum, in keV. An error of 0.0 implies a fixed parameter.

**Pflx_Glog_Phtflux**

The average photon flux, in photon/cm^{2}/s, for a Log_{10}
Gaussian model fit to a
single spectrum over the time range of the peak flux of the burst.

**Pflx_Glog_Phtflux_Error**

The 1-sigma statistical error of the average photon
flux, in photon/cm^{2}/s,
for the Log_10 Gaussian model peak flux spectrum.

**Pflx_Glog_Phtflnc**

The photon fluence, in photon/cm^{2}, for a Log_{10}
Gaussian model fit to a single
spectrum over the time range of the peak flux of the burst.

**Pflx_Glog_Phtflnc_Error**

The 1-sigma statistical error in the photon fluence,
in photon/cm^{2}, for the
Log_{10} Gaussian peak flux spectrum.

**Pflx_Glog_Flux**

The average energy flux, in erg/cm^{2}/s, for a Log_{10}
Gaussian model fit to a
single spectrum over the time range of the peak flux of the burst.

**Pflx_Glog_Flux_Error**

The 1-sigma statistical error on the average energy
flux, in erg/cm^{2}/s, for
the Log_{10} Gaussian model peak flux spectrum.

**Pflx_Glog_Flnc**

The energy fluence, in erg/cm^{2}, for a Log_{10} Gaussian
model fit to a single spectrum over the time range of the peak flux of the
burst.

**Pflx_Glog_Flnc_Error**

The 1-sigma statistical error in the energy fluence,
in erg/cm^{2}, for the Log_{10} Gaussian peak flux spectrum.

**Pflx_Glog_Chisq**

The chi-squared goodness of fit statistic for the
Log_{10} Gaussian model fit to the peak flux spectrum.

**Pflx_Glog_DoF**

The degrees of freedom for the Log_{10} Gaussian model fit to
the peak flux spectrum.

**Pflx_Plaw_Ampl**

The amplitude of a power law fit to a single spectrum over
the time range of the peak flux of the burst, in photon/cm^{2}/s/keV.

**Pflx_Plaw_Ampl_Error**

The 1-sigma statistical error of the power law fit
amplitude for the peak flux
spectrum, in photon/cm^{2}/s/keV. An error of 0.0 implies a fixed parameter.

**Pflx_Plaw_Index**

The power law index of a power law fit to a single spectrum
over the time range of the peak flux of the burst.

**Pflx_Plaw_Index_Error**

The 1-sigma statistical error in the power law index
of a power law fit for the peak
flux spectrum. An error of 0.0 implies a fixed parameter.

**Pflx_Plaw_Phtflux**

The photon flux, in photon/cm^{2}/s, for a power law fit
to a single spectrum over the time range of the peak flux of the burst.

**Pflx_Plaw_Phtflux_Error**

The 1-sigma statistical error on the photon flux,
in photon/cm^{2}/s, for the power law peak flux spectrum.

**Pflx_Plaw_Phtflnc**

The photon fluence, in photon/cm^{2}, for a power law fit
to a single spectrum over the time range of the peak flux of the burst.

**Pflx_Plaw_Phtflnc_Error**

The 1-sigma statistical error in the photon fluence,
in photon/cm^{2}, for the power law peak flux spectrum.

**Pflx_Plaw_Flux**

The energy flux, in erg/cm^{2}/s, for a power law fit to a
single spectrum over the time range of the peak flux of the burst.

**Pflx_Plaw_Flux_Error**

The 1-sigma statistical error on the energy flux, in
erg/cm^{2}/s, for the power law peak flux spectrum

**Pflx_Plaw_Flnc**

The energy fluence, in erg/cm^{2}, for a power law fit to a
single spectrum over the time range of the peak flux of the burst.

**Pflx_Plaw_Flnc_Error**

The 1-sigma statistical error in the energy fluence,
in erg/cm^{2}, for the power law peak flux spectrum.

**Pflx_Plaw_Chisq**

The chi-squared goodness of fit statistic for the
power law fit to the peak flux spectrum.

**Pflx_Plaw_DoF**

The degrees of freedom for the power law fit to
the peak flux spectrum.

**Pflx_SBPL_Ampl**

The amplitude of a smoothly broken power law fit to a single
spectrum over the time range of the peak flux of the burst, in
photon/cm^{2}/s/keV.

**Pflx_SBPL_Ampl_Error**

The 1-sigma statistical error of the smoothly broken
power law amplitude for the peak flux spectrum, in photon/cm^{2}/s/keV.
An error of 0.0 implies a fixed parameter.

**Pflx_SBPL_Indx1**

The low-energy power law index, lambda_{1}, of a smoothly
broken power law fit to a single spectrum over the time range of the peak flux
of the burst.

**Pflx_SBPL_Indx1_Error**

The 1-sigma statistical error of the smoothly broken
power low-energy power law index
for the peak flux spectrum. An error of 0.0 implies a fixed parameter.

**Pflx_SBPL_Indx2**

The high-energy power law index, lambda_{2}, of a smoothly
broken power law fit to a single spectrum over the time range of the peak flux
of the burst.

**Pflx_SBPL_Indx2_Error**

The 1-sigma statistical error of the smoothly broken
power high-energy power law index
for the peak flux spectrum. An error of 0.0 implies a fixed parameter.

**Pflx_SBPL_Brken**

The break energy, E_{b}, of a smoothly broken power law fit
to a single spectrum over
the time range of the peak flux of the burst, in keV.

**Pflx_SBPL_Brken_Error**

The 1-sigma statistical error of the smoothly broken
power law break energy for
the peak flux spectrum, in keV. An error of 0.0 implies a fixed parameter.

**Pflx_SBPL_Epeak**

The peak energy of a model fit to a smoothly broken
power law model nu*F_{nu} spectrum over the time range of the peak flux of
the burst, in keV.

**Pflx_SBPL_Epeak_Error**

The 1-sigma statistical error of the
smoothly broken power law model peak energy for the peak
flux spectrum, in keV. An error of 0.0 implies a fixed parameter.

**Pflx_SBPL_Phtflux**

The photon flux, in photon/cm^{2}/s, for a smoothly broken
power law fit to a
single spectrum over the time range of the peak flux of the burst.

**Pflx_SBPL_Phtflux_Error**

The 1-sigma statistical error in the photon flux,
in photon/cm^{2}/s, for the
smoothly broken power law peak flux spectrum.

**Pflx_SBPL_Phtflnc**

The photon fluence in photon/cm^{2} for a smoothly broken
power law fit to a single spectrum over the time range of the peak flux of
the burst.

**Pflx_SBPL_Phtflnc_Error**

The 1-sigma statistical error in the photon fluence,
in photon/cm^{2}, for the smoothly broken power law peak flux spectrum.

**Pflx_SBPL_Flux**

The energy flux, in erg/cm^{2}/s, for a smoothly broken power
law fit to a single spectrum over the time range of the peak flux of the burst.

**Pflx_SBPL_Flux_Error**

The 1-sigma statistical error on the energy flux,
in erg/cm^{2}/s, for the smoothly broken power law peak flux spectrum.

**Pflx_SBPL_Flnc**

The energy fluence, in erg/cm^{2}, for a smoothly broken power
law fit to a single spectrum over the time range of the peak flux of the burst.

**Pflx_SBPL_Flnc_Error**

The 1-sigma statistical error in the energy fluence,
in erg/cm^{2}, for the smoothly broken power law peak flux spectrum.

**Pflx_SBPL_Chisq**

The chi-squared goodness of fit statistic for the
smoothly broken power law model fit to the peak flux spectrum.

**Pflx_SBPL_DoF**

The degrees of freedom for the smoothly broken power law
fit to the peak flux spectrum.

**Flnc_Integration_Time**

The total time, in seconds, over which the fluence
was calculated. The time-integrated fluence distributions are estimated over
the duration of the observed emission, where the observed emission is defined
as 3.5 sigma over the estimated background in the 20-2000 keV energy range.

**Flnc_Band_Ampl**

The amplitude of a Band function fit to a single spectrum
over the duration of the burst, in photon/cm^{2}/s/keV.

**Flnc_Band_Ampl_Error**

The 1-sigma statistical error of the Band function
amplitude for the fluence spectrum, in photon/cm^{2}/s/keV. An error value
of 0.0 implies a fixed parameter

**Flnc_Band_Alpha**

The low-energy power law index, alpha, of a Band function
fit to a single spectrum over the duration of the burst

**Flnc_Band_Alpha_Error**

The 1-sigma statistical error of the Band function
power law, alpha, for the
fluence spectrum. An error of 0.0 implies a fixed parameter.

**Flnc_Band_Beta**

The high-energy power law index, beta, of a Band function
fit to a single spectrum over the duration of the burst.

**Flnc_Band_Beta_Error**

The 1-sigma statistical error of the Band function
power law, beta, for the
fluence spectrum. An error of 0.0 implies a fixed parameter.

**Flnc_Band_Epeak**

The peak energy of a Band function fit to a single
nu*F_{nu} spectrum over the time range of the fluence of the burst, in keV

**Flnc_Band_Epeak_Error**

The 1-sigma statistical error of the Band function
peak energy for the fluence spectrum, in keV. An error of 0.0 implies a
fixed parameter.

**Flnc_Band_Phtflux**

The photon flux, in photon/cm^{2}/s, for a Band function
fit to a single spectrum over the duration of the burst.

**Flnc_Band_Phtflux_Error**

The 1-sigma statistical error in the photon flux,
in photon/cm^{2}/s, for the Band function fluence spectrum.

**Flnc_Band_Phtflnc**

The photon fluence, in photon/cm^{2}, for a Band function
fit to a single spectrum over the duration of the burst.

**Flnc_Band_Phtflnc_Error**

The 1-sigma statistical error in the photon fluence,
in photon/cm^{2}, for the Band function fluence spectrum.

**Flnc_Band_Flux**

The energy flux, in erg/cm^{2}/s, for a Band function fit to
a single spectrum over the duration of the burst.

**Flnc_Band_Flux_Error**

The 1-sigma statistical error on the energy flux, in
erg/cm^{2}/s, for the Band function fluence spectrum.

**Flnc_Band_Flnc**

The energy fluence, in erg/cm^{2}, for a Band function fit to
a single spectrum over the duration of the burst.

**Flnc_Band_Flnc_Error**

The 1-sigma statistical error in the energy fluence,
in erg/cm^{2}, for the Band function fluence spectrum.

**Flnc_Band_Chisq**

The chi-squared goodness of fit statistic for the Band
function fit to the fluence spectrum.

**Flnc_Band_DoF**

The degrees of freedom for the Band function fit to the peak
flux spectrum.

**Flnc_Comp_Ampl**

The amplitude of a Comptonized (exponentially attenuated
power law) model fit to a single spectrum
over the duration of the burst, in photon/cm^{2}/s/keV.

**Flnc_Comp_Ampl_Error**

The 1-sigma statistical error of the Comptonized model
amplitude for the fluence spectrum, in photon/cm^{2}/s/keV.
An error of 0.0 implies a fixed parameter.

**Flnc_Comp_Index**

The power law index of a Comptonized model fit to a single
spectrum over the duration of the burst.

**Flnc_Comp_Index_Error**

The 1-sigma statistical error of the Comptonized
model power law index for the
fluence spectrum. An error of 0.0 implies a fixed parameter.

**Flnc_Comp_Epeak**

The peak energy of a Comptonized model fit to a single
nu*F_{nu} spectrum over the duration of the burst, in keV.

**Flnc_Comp_Epeak_Error**

The 1-sigma statistical error of the Comptonized
model peak energy for the peak
flux spectrum, in keV. An error of 0.0 implies a fixed parameter.

**Flnc_Comp_Phtflux**

The photon flux, in photon/cm^{2}/s, for a Comptonized
model fit to a single
spectrum over the duration of the burst.

**Flnc_Comp_Phtflux_Error**

The 1-sigma statistical error on the photon flux,
in photon/cm^{2}/s, for the Comptonized model fluence spectrum.

**Flnc_Comp_Phtflnc**

The photon fluence in photon/cm^{2} for a Comptonized model
fit to a single
spectrum over the duration of the burst.

**Flnc_Comp_Phtflnc_Error**

The 1-sigma statistical error in the photon fluence,
in photon/cm^{2}, for the Comptonized model fluence spectrum.

**Flnc_Comp_Flux**

The energy flux, in erg/cm^{2}/s, for a Comptonized model fit
to a single spectrum over the duration of the burst.

**Flnc_Comp_Flux_Error**

The 1-sigma statistical error on the energy flux, in
erg/cm^{2}/s, for the Comptonized model fluence spectrum.

**Flnc_Comp_Flnc**

The energy fluence, in erg/cm^{2}, for a Comptonized model
fit to a single spectrum over the duration of the burst.

**Flnc_Comp_Flnc_Error**

The 1-sigma statistical error in the energy fluence,
in erg/cm^{2}, for the Comptonized model fluence spectrum.

**Flnc_Comp_Chisq**

The chi-squared goodness of fit statistic for the
Comptonized model fit to the fluence spectrum.

**Flnc_Comp_DoF**

The degrees of freedom for the Comptonized model fit to the
fluence spectrum.

**Flnc_Glog_Ampl**

The amplitude of a Log_{10} Gaussian model fit to a single
spectrum over the
duration of the burst, in photon/cm^{2}/s/keV.

**Flnc_Glog_Ampl_Error**

The 1-sigma statistical error of the Log_{10} Gaussian
model amplitude for the fluence spectrum, in photon/cm^{2}/s/keV. An error of
0.0 implies a fixed parameter.

**Flnc_Glog_FWHM**

The full width at half maximum of a Log_{10} Gaussian model
fit to a single spectrum over the duration of the burst, in
log_10(keV).

**Flnc_Glog_FWHM_Error**

The 1-sigma statistical error of the Log_{10} Gaussian
model full width at half maximum for the fluence spectrum, in log_{10} (keV).
An error of 0.0 implies a fixed parameter.

**Flnc_Glog_Ecent**

The log_{10} of the centroid energy E_{cen} of a Log_{10}
Gaussian model fit to a single spectrum over the
duration of the burst, in keV.

**Flnc_Glog_Ecent_Error**

The 1-sigma statistical error of the Log_10 Gaussian
model log_{10} (E_{cen}) for the
fluence spectrum, in keV. An error of 0.0 implies a fixed parameter.

**Flnc_Glog_Epeak**

The peak energy of a model fit to a single Log_{10}
Gaussian model nu*F_{nu} spectrum over the duration of
the burst, in keV.

**Flnc_Glog_Epeak_Error**

The 1-sigma statistical error of the
Log_{10} Gaussian model model peak energy for the peak
flux spectrum, in keV. An error of 0.0 implies a fixed parameter.

**Flnc_Glog_Phtflux**

The average photon flux, in photon/cm^{2}/s, for a Log_{10}
Gaussian model fit to a
single spectrum over the duration of the burst.

**Flnc_Glog_Phtflux_Error**

The 1-sigma statistical error of the average photon
flux, in photon/cm^{2}/s,
for the Log_10 Gaussian model fluence spectrum.

**Flnc_Glog_Phtflnc**

The photon fluence, in photon/cm^{2}, for a Log_{10}
Gaussian model fit to a single
spectrum over the duration of the burst.

**Flnc_Glog_Phtflnc_Error**

The 1-sigma statistical error in the photon fluence,
in photon/cm^{2}, for the
Log_{10} Gaussian fluence spectrum.

**Flnc_Glog_Flux**

The average energy flux, in erg/cm^{2}/s, for a Log_{10}
Gaussian model fit to a
single spectrum over the duration of the burst.

**Flnc_Glog_Flux_Error**

The 1-sigma statistical error on the average energy
flux, in erg/cm^{2}/s, for
the Log_{10} Gaussian model fluence spectrum.

**Flnc_Glog_Flnc**

The energy fluence, in erg/cm^{2}, for a Log_{10} Gaussian
model fit to a single spectrum over the duration of the
burst.

**Flnc_Glog_Flnc_Error**

The 1-sigma statistical error in the energy fluence,
in erg/cm^{2}, for the Log_{10} Gaussian fluence spectrum.

**Flnc_Glog_Chisq**

The chi-squared goodness of fit statistic for the
Log_{10} Gaussian model fit to the fluence spectrum.

**Flnc_Glog_DoF**

The degrees of freedom for the Log_{10} Gaussian model fit to
the fluence spectrum.

**Flnc_Plaw_Ampl**

The amplitude of a power law fit to a single spectrum over
the duration of the burst, in photon/cm^{2}/s/keV.

**Flnc_Plaw_Ampl_Error**

The 1-sigma statistical error of the power law fit
amplitude for the fluence
spectrum, in photon/cm^{2}/s/keV. An error of 0.0 implies a fixed parameter.

**Flnc_Plaw_Index**

The power law index of a power law fit to a single spectrum
over the duration of the burst.

**Flnc_Plaw_Index_Error**

The 1-sigma statistical error in the power law index
of a power law fit for the peak
flux spectrum. An error of 0.0 implies a fixed parameter.

**Flnc_Plaw_Phtflux**

The photon flux, in photon/cm^{2}/s, for a power law fit
to a single spectrum over the duration of the burst.

**Flnc_Plaw_Phtflux_Error**

The 1-sigma statistical error on the photon flux,
in photon/cm^{2}/s, for the power law fluence spectrum.

**Flnc_Plaw_Phtflnc**

The photon fluence, in photon/cm^{2}, for a power law fit
to a single spectrum over the duration of the burst.

**Flnc_Plaw_Phtflnc_Error**

The 1-sigma statistical error in the photon fluence,
in photon/cm^{2}, for the power law fluence spectrum.

**Flnc_Plaw_Flux**

The energy flux, in erg/cm^{2}/s, for a power law fit to a
single spectrum over the duration of the burst.

**Flnc_Plaw_Flux_Error**

The 1-sigma statistical error on the energy flux, in
erg/cm^{2}/s, for the power law fluence spectrum

**Flnc_Plaw_Flnc**

The energy fluence, in erg/cm^{2}, for a power law fit to a
single spectrum over the duration of the burst.

**Flnc_Plaw_Flnc_Error**

The 1-sigma statistical error in the energy fluence,
in erg/cm^{2}, for the power law fluence spectrum.

**Flnc_Plaw_Chisq**

The chi-squared goodness of fit statistic for the
power law fit to the fluence spectrum.

**Flnc_Plaw_DoF**

The degrees of freedom for the power law fit to
the fluence spectrum.

**Flnc_SBPL_Ampl**

The amplitude of a smoothly broken power law fit to a single
spectrum over the duration of the burst, in
photon/cm^{2}/s/keV.

**Flnc_SBPL_Ampl_Error**

The 1-sigma statistical error of the smoothly broken
power law amplitude for the fluence spectrum, in photon/cm^{2}/s/keV.
An error of 0.0 implies a fixed parameter.

**Flnc_SBPL_Indx1**

The low-energy power law index, lambda_{1}, of a smoothly
broken power law fit to a single spectrum over the duration
of the burst.

**Flnc_SBPL_Indx1_Error**

The 1-sigma statistical error of the smoothly broken
power low-energy power law index
for the fluence spectrum. An error of 0.0 implies a fixed parameter.

**Flnc_SBPL_Indx2**

The high-energy power law index, lambda_{2}, of a smoothly
broken power law fit to a single spectrum over the duration
of the burst.

**Flnc_SBPL_Indx2_Error**

The 1-sigma statistical error of the smoothly broken
power high-energy power law index
for the fluence spectrum. An error of 0.0 implies a fixed parameter.

**Flnc_SBPL_Brken**

The break energy, E_{b}, of a smoothly broken power law fit
to a single spectrum over
the duration of the burst, in keV.

**Flnc_SBPL_Brken_Error**

The 1-sigma statistical error of the smoothly broken
power law break energy for
the fluence spectrum, in keV. An error of 0.0 implies a fixed parameter.

**Flnc_SBPL_Epeak**

The peak energy of a model fit to a smoothly broken
power law model nu*F_{nu} spectrum over the duration of
the burst, in keV.

**Flnc_SBPL_Epeak_Error**

The 1-sigma statistical error of the
smoothly broken power law model peak energy for the peak
flux spectrum, in keV. An error of 0.0 implies a fixed parameter.

**Flnc_SBPL_Phtflux**

The photon flux, in photon/cm^{2}/s, for a smoothly broken
power law fit to a
single spectrum over the duration of the burst.

**Flnc_SBPL_Phtflux_Error**

The 1-sigma statistical error in the photon flux,
in photon/cm^{2}/s, for the
smoothly broken power law fluence spectrum.

**Flnc_SBPL_Phtflnc**

The photon fluence in photon/cm^{2} for a smoothly broken
power law fit to a single spectrum over the duration of
the burst.

**Flnc_SBPL_Phtflnc_Error**

The 1-sigma statistical error in the photon fluence,
in photon/cm^{2}, for the smoothly broken power law fluence spectrum.

**Flnc_SBPL_Flux**

The energy flux, in erg/cm^{2}/s, for a smoothly broken power
law fit to a single spectrum over the duration of the burst.

**Flnc_SBPL_Flux_Error**

The 1-sigma statistical error on the energy flux,
in erg/cm^{2}/s, for the smoothly broken power law fluence spectrum.

**Flnc_SBPL_Flnc**

The energy fluence, in erg/cm^{2}, for a smoothly broken power
law fit to a single spectrum over the duration of the burst.

**Flnc_SBPL_Flnc_Error**

The 1-sigma statistical error in the energy fluence,
in erg/cm^{2}, for the smoothly broken power law fluence spectrum.

**Flnc_SBPL_Chisq**

The chi-squared goodness of fit statistic for the
smoothly broken power law model fit to the fluence spectrum.

**Flnc_SBPL_DoF**

The degrees of freedom for the smoothly broken power law
fit to the fluence spectrum.