batgrbproduct analysis for trigger=324744

batgrbproduct Analysis for Trigger=324744

Analysis Summary

Notes:

1) No attempt has been made to eliminate the non-significant decimal places.
2) This batgrbproduct analysis is done using the HEASARC data.
3) This batgrbproduct analysis is using the flight position for the mask-weighting calculation.

======================================================================
                  BAT GRB EVENT DATA PROCESSING REPORT
    Process Script Ver: batgrbproduct v2.46
    Process Start Time (local time): Sun Jan 19 22:45:44 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger324744
======================================================================

  Trigger: 00324744      Segment: 000

  BAT Trigger Time: 243129773.056   [s; MET]
      Trigger Stop: 243129777.152   [s; MET]
               UTC: 2008-09-15T00:02:49.957760    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 18.0040672407145   Dec: -76.0144041971717  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    7.13
     Image Trigger?:     NO
     Rate S/N Ratio:     8.18535277187245  [ if not an image trigger ]
     Image S/N Ratio:    7.13

  Flight Position:   [ source = BAT ]
    RA: 18.0040672407145   Dec: -76.0144041971717  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 17.8853408690745   Dec: -76.0443829252976  [deg; J2000]  
        { 01h 11m 32.5s , -76d 02' 39.8" }
         +/- 2.43155402306048 [arcmin] (estimated 90% radius based on SNR)
         +/- 1.52620369750692 [arcmin] (formal 1-sigma fit error)
    SNR: 8.54782520983947
 
  Angular difference between Flight and Ground position is 2.488600 arcmin
 
  Partial Coding Fraction: 0.890625    [ including projection effects ]

  Duration
     T90: 26.2879999577999 +/- 3.89810207565097
        Measured from: -0.815999984741211
                   to: 25.4719999730587     [s; relative to TRIGTIME]
     T50: 10.6079999804497 +/- 9.8563247074382
        Measured from: 3.12000000476837
                   to: 13.727999985218     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 3.04399999976158     
                   to: 4.04399999976158     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -2.67199999094009     
                   to: 26.7199999988079     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.146887   0.201004   0.097420   0.021154
           0.028435   0.029328   0.026237   0.024173 [error]
 Peak      0.019211   0.015941   0.016887  -0.000338
           0.005280   0.005457   0.004887   0.004639 [error]

     [ fluence units of on-axis counts / fully illuminated detector ] 

======================================================================
 
=== Fluence/Peak Flux Summary ===
 
              Model    Band1    Band2    Band3    Band4    Band5    Total      
                       15-25    25-50   50-100  100-350   15-150   15-350   keV
Fluence   Power-law 4.28e-08 7.48e-08 1.00e-07 2.74e-07 2.91e-07 4.91e-07   erg/cm2
              Error 1.18e-08 1.32e-08 2.52e-08 1.45e-07 6.02e-08 1.67e-07   erg/cm2
Peak flux Power-law 1.51e-01 1.53e-01 1.09e-01 1.24e-01 4.62e-01 5.38e-01   ph/cm2/s
              Error 7.41e-02 4.52e-02 4.18e-02 1.04e-01 1.29e-01 1.55e-01   ph/cm2/s
 
Fluence   Cutoff-PL 4.20e-08 7.79e-08 9.94e-08 1.55e-07 2.80e-07 3.71e-07   erg/cm2
              Error 1.26e-08 1.95e-08 2.40e-08 2.18e-07 7.89e-08 2.36e-07   erg/cm2
Peak flux Cutoff-PL 1.55e-01 1.54e-01 1.07e-01 1.18e-01 4.63e-01 5.36e-01   ph/cm2/s
              Error 5.81e-02 4.68e-02 4.21e-02 1.27e-01 1.29e-01 1.63e-01   ph/cm2/s
 
Fluence        Band -------- -------- -------- -------- -------- --------   erg/cm2
              Error -------- -------- -------- -------- -------- --------   erg/cm2
Peak flux      Band -------- -------- -------- -------- -------- --------   ph/cm2/s
              Error -------- -------- -------- -------- -------- --------   ph/cm2/s

 
=== Time-averaged spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.582    0.309    -      -           1.06e-03 2.00e-04   52.620 57
CPL   1.268    1.502      98.6    0.0      1.61e-03 2.26e-02   52.500 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.488    0.553    -      -           3.72e-03 1.10e-03   55.670 57
CPL   2.055    0.000      21.3    0.0      1.73e-03 0.00e+00   55.100 56
 
Model      : spectral model: simple power-law (PL) and cutoff power-law (CPL)
Ph_index   : photon index: E^-{Ph_index} (minus sign is not included in the index)
Ph_90err   : 90% error of the photon index
Epeak      : Epeak in keV
Epeak_90err: 90% error of Epeak
Norm       : normalization at 50 keV in PL model and at 1 keV in CPL model
Nomr_90err : 90% error of the normalization
chi2       : Chi-Squared
dof        : degree of freedom

 
=== T90/T50 calculation in the 50-300 keV band (BATSE band) using 64 ms lc ===
 
T90 in the 50-300 keV band: 0.000000 sec.
T50 in the 50-300 keV band: 0.000000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   29.392   -2.672   26.720
T90    26.288   -0.816   25.472
T50    10.608    3.120   13.728
Peak    1.000    3.044    4.044

Click here for the BAT GCN circular template

Special notes of this burst

Image

Pre-slew 15.0-350.0 keV image (Event data)

#   RAcent    DECcent   POSerr    Theta     Phi              Peak Cts       SNR   Name
   17.8853   -76.0444   0.0224    27.3669  -170.2244         0.4767006      8.548 TRIG_00324744                 
 
Foreground time interval of the image:
 -2.672  26.720 (delta_t =  29.392 [sec])
Background time interval of the image:
-239.056  -2.672 (delta_t = 236.384 [sec])

Lightcurves

Notes:

1) The mask-weighted light curves are using the flight position.
2) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
3) For all the mask-weighted lightcurves, the y-axis units are counts/sec/det where a det is 0.4 x 0.4 = 0.16 sq cm.
4) The verticle lines correspond to following: green dotted lines are T50 interval, black dotted lines are T90 interval, blue solid line(s) is a spacecraft slew start time, and orange solid line(s) is a spacecraft slew end time.
5) Time of each bin is in the middle of the bin.

1 s binning

From T0-310 s to T0+310 s

From T100_start - 20 s to T100_end + 30 s

Full time interval

64 ms binning

Full time interval

From T100_start to T100_end

From T0-5 sec to T0+5 sec

16 ms binning

From T100_start-5 s to T100_start+5 s

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000

8 ms binning

From T100_start-3 s to T100_start+3 s

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000

2 ms binning

From T100_start-1 s to T100_start+1 s

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000

SN=5 or 10 sec. binning (whichever binning is satisfied first)

SN=5 or 10 sec. binning (T < 200 sec)

Quad-rate summed light curves (from T0-300s to T0+1000s)

Spectral Evolution

Spectra

Notes:

1) The fitting includes the systematic errors.
2) When the burst includes telescope slew time periods, the fitting uses an average response file made from multiple 5-s response files through out the slew time plus single time preiod for the non-slew times, and weighted by the total counts in the corresponding time period using addrmf. An average response file is needed becuase a spectral fit using the pre-slew DRM will introduce some errors in both a spectral shape and a normalization if the PHA file contains a lot of the slew/post-slew time interval.
3) For fits to more complicated models (e.g. a power-law over a cutoff power-law), the BAT team has decided to require a chi-square improvement of more than 6 for each extra dof.

Time averaged spectrum fit using the average DRM

Power-law model

Time interval is from   -2.672 sec. to   26.720 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.58218     ( -0.306052   0.311857 )
Norm@50keV  : 1.05660E-03    ( -0.000202089   0.000198044 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.62 using 59 PHA bins.
# Reduced chi-squared =         0.9231 for     57 degrees of freedom 
# Null hypothesis probability =   6.400448e-01
 
Photon flux (15-150 keV)    in 29.39 sec: 0.135039 ( -0.0236994  0.0237145 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.91072e-07 ( -5.93446e-08  6.10768e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -2.672 sec. to   26.720 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.26818     ( -2.40219   0.602578 )
Epeak [keV] : 98.5862      ( -103.225 -103.225 )
Norm@50keV  : 1.60551E-03    ( -0.00155061   0.0436275 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.50 using 59 PHA bins.
# Reduced chi-squared =         0.9376 for     56 degrees of freedom 
# Null hypothesis probability =   6.079573e-01
 
Photon flux (15-150 keV)    in 29.39 sec: 0.133512 ( -0.013055  0.024684 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.79915e-07 ( -8.72263e-08  7.04755e-08 ) ergs/cm2

Band function

Time interval is from   -2.672 sec. to   26.720 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.64979   ( -5.96529   -4.64979 )
beta        : -1.92558    ( -0.561322   0.43677 )
Epeak [keV] : 29.1711      ( -7.38847 7.3 )
Norm@50keV   : 29.3473    ( -5.03959   1219.43 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.74 using 59 PHA bins.
# Reduced chi-squared =         0.9044 for     55 degrees of freedom 
# Null hypothesis probability =   6.751827e-01
 
Photon flux (15-150 keV)    in 29.39 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 0 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 10.9709  (-1.92473  2.58567)
R^2/D10^2   : 4.65623E-02  (-0.0253977   0.0487601)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.01 using 59 PHA bins.
# Reduced chi-squared =         0.9827 for     57 degrees of freedom 
# Null hypothesis probability =   5.121887e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.440e-08   1.340e-08
25- 50  9.693e-08   2.685e-08
50-150  6.577e-08   2.893e-08
15-150  1.971e-07   5.940e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 159.740       (-89.1221      -161.198)
Norm        : 0.556295       (-0.102427     0.138996)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.43 using 59 PHA bins.
# Reduced chi-squared =         0.9199 for     57 degrees of freedom 
# Null hypothesis probability =   6.467737e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.175e-08   2.347e-08
25- 50  7.809e-08   4.295e-08
50-150  1.581e-07   9.449e-08
15-150  2.779e-07   1.546e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 9.11759        (-1.58656      1.85589)
R1^2/D10^2  : 8.22439E-02        (-0.0426355      0.0882885)
kT2 [keV]   : 198.619        (-130.776      -198.744)
R2^2/D10^2  : 1.73220E-05    (-8.53431e-06   0.000628721)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.34 using 59 PHA bins.
# Reduced chi-squared =         0.8426 for     55 degrees of freedom 
# Null hypothesis probability =   7.907076e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.003e-08   1.881e-08
25- 50  9.092e-08   4.636e-08
50-150  1.680e-07   3.743e-08
15-150  2.990e-07   1.061e-07

Peak spectrum fit

Power-law model

Time interval is from    3.044 sec. to    4.044 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.48762     ( -0.539899   0.566544 )
Norm@50keV  : 3.71588E-03    ( -0.00112055   0.00106972 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.67 using 59 PHA bins.
# Reduced chi-squared =         0.9766 for     57 degrees of freedom 
# Null hypothesis probability =   5.252393e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.462360 ( -0.128798  0.129268 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.53232e-08 ( -1.14538e-08  1.18476e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    3.044 sec. to    4.044 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.05480     (     )
Epeak [keV] : 21.2741      (   )
Norm@50keV  : 1.72992E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.10 using 59 PHA bins.
# Reduced chi-squared =         0.9839 for     56 degrees of freedom 
# Null hypothesis probability =   5.089090e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.463271 ( -0.130233  0.128239 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.5411e-08 ( -1.1642e-08  1.15994e-08 ) ergs/cm2

Band function

Time interval is from    3.044 sec. to    4.044 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.21214   ( 1.21214   1.21214 )
beta        : -1.48755    ( 1.48758   0.540262 )
Epeak [keV] : 32.0157      ( -31.9954 -31.9954 )
Norm@50keV   : 7.39119E-03    ( -0.00469876   0.188157 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.67 using 59 PHA bins.
# Reduced chi-squared =          1.012 for     55 degrees of freedom 
# Null hypothesis probability =   4.495458e-01
 
Photon flux (15-150 keV)    in 1 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 0 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 16.0294  (-5.53182  9.51608)
R^2/D10^2   : 4.03843E-02  (-0.0401286   0.133891)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.44 using 59 PHA bins.
# Reduced chi-squared =          1.060 for     57 degrees of freedom 
# Null hypothesis probability =   3.525448e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.145e-09   1.355e-09
25- 50  9.039e-09   5.440e-09
50-150  1.624e-08   1.075e-08
15-150  2.743e-08   1.753e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.361       (-199.363      -199.363)
Norm        : 1.88028       (-0.520884     0.521399)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.05 using 59 PHA bins.
# Reduced chi-squared =         0.9833 for     57 degrees of freedom 
# Null hypothesis probability =   5.108815e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.682e-09   2.879e-09
25- 50  9.007e-09   5.525e-09
50-150  1.975e-08   1.201e-08
15-150  3.344e-08   2.030e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 2.77950        (-1.59156      4.92705)
R1^2/D10^2  : 33.5684        (-33.4239      36003.1)
kT2 [keV]   : 21.0712        (-7.69956      54.1119)
R2^2/D10^2  : 1.48760E-02    (-0.0125664   0.0547703)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.81 using 59 PHA bins.
# Reduced chi-squared =         0.9965 for     55 degrees of freedom 
# Null hypothesis probability =   4.820331e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.090e-09   2.843e-09
25- 50  6.844e-09   4.059e-09
50-150  2.125e-08   1.292e-08
15-150  3.318e-08   1.907e-08

Pre-slew spectrum (Pre-slew PHA with pre-slew DRM)

Power-law model

 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.58218     ( -0.306052   0.311857 )
Norm@50keV  : 1.05660E-03    ( -0.000202089   0.000198044 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.62 using 59 PHA bins.
# Reduced chi-squared =         0.9231 for     57 degrees of freedom 
# Null hypothesis probability =   6.400448e-01
 
Photon flux (15-150 keV)    in 29.39 sec: 0.135039 ( -0.0236994  0.0237145 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.91072e-07 ( -5.93446e-08  6.10768e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.26818     ( -2.40219   0.602578 )
Epeak [keV] : 98.5862      ( -103.225 -103.225 )
Norm@50keV  : 1.60551E-03    ( -0.00155061   0.0436275 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.50 using 59 PHA bins.
# Reduced chi-squared =         0.9376 for     56 degrees of freedom 
# Null hypothesis probability =   6.079573e-01
 
Photon flux (15-150 keV)    in 29.39 sec: 0.133512 ( -0.013055  0.024684 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.79915e-07 ( -8.72263e-08  7.04755e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.64979   ( -13.2207   -4.64979 )
beta        : -1.92558    ( -0.561322   0.43677 )
Epeak [keV] : 29.1711      ( -7.38847 7.3 )
Norm@50keV   : 29.3473    ( -5.03959   1219.43 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.74 using 59 PHA bins.
# Reduced chi-squared =         0.9044 for     55 degrees of freedom 
# Null hypothesis probability =   6.751827e-01
 
Photon flux (15-150 keV)    in 29.39 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 0 ( 0  0 ) ergs/cm2

S(25-50 keV) vs. S(50-100 keV) plot

S(25-50 keV)  = 7.48e-08
S(50-100 keV) = 1.00e-07

T90 vs. Hardness ratio plot

T90                                   = 26.2879999577999 sec.
Hardness ratio (energy fluence ratio) = 1.3369

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.36843
Count Ratio (50-100 keV) / (15-25 keV) = 0.663231

Mask shadow pattern

IMX = -5.101016289983309E-01, IMY = 8.788627582560590E-02

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000

Spacecraft aspect plot

Bright source in the pre-burst/pre-slew/post-slew images

Pre-burst image of 15-350 keV band

Time interval of the image:
-239.056000 -2.672000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
256.0552 -37.8700    5.8  37.0  -29.5   0.5644   2.0    3.6	4U 1700-377                   
256.4260 -36.4160   26.7  38.0  -27.8   0.1273   0.4    0.6	GX 349+2                      
263.1257 -24.7301    4.3  45.7  -11.9   0.9522   2.7    6.4	GX 1+4                        
264.6800 -44.3862    6.0  27.9  -26.4   0.3978   1.9    4.7	4U 1735-44                    
270.3978 -25.0392    5.2  42.9   -3.3   0.7618   2.2    6.6	GX 5-1                        
270.2549 -25.6356    3.9  42.4   -3.8   0.9489   2.9    6.9	GRS 1758-258                  
273.9867 -14.0274   12.5  52.4    5.6   0.5683   0.9    1.2	GX 17+2                       
275.9099 -30.3855    4.3  36.2    1.0   0.7152   2.7    1.4	H1820-303                     
284.9284 -24.8028    9.1  39.4   16.0  -0.4066  -1.3    9.2	HT1900.1-2455                 
262.9855 -33.8376    2.2  37.6  -18.1   1.3515   5.3    0.3	GX 354-0                      
292.1667 -18.6176    2.7  44.5   27.4   2.0414   4.2 ------	UNKNOWN                       
281.0967 -12.1761    2.0  52.5   14.7   4.6759   5.9 ------	UNKNOWN                       
273.2337 -10.0276    2.5  56.4    6.1   5.4369   4.6 ------	UNKNOWN

Pre-slew background subtracted image of 15-350 keV band

Time interval of the image:
-2.672000 26.720000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
256.0197 -37.7130    4.7  37.1  -29.3   0.1892   2.5    8.0	4U 1700-377                   
256.4524 -36.4558   15.0  38.0  -27.8   0.0628   0.8    2.1	GX 349+2                      
262.9011 -24.8311    7.6  45.7  -12.2  -0.1439  -1.5    7.8	GX 1+4                        
264.8858 -44.2766    4.1  27.9  -26.0  -0.1717  -2.8   12.1	4U 1735-44                    
270.1353 -24.9905    6.6  43.1   -3.6  -0.1564  -1.7    9.7	GX 5-1                        
270.3931 -25.6236   13.2  42.4   -3.6  -0.0755  -0.9    8.7	GRS 1758-258                  
273.8806 -13.9932    7.7  52.4    5.5   0.2810   1.5    7.7	GX 17+2                       
276.0659 -30.3460    7.8  36.2    1.2  -0.1066  -1.5    7.4	H1820-303                     
285.0963 -24.7853   18.3  39.4   16.3   0.0556   0.6    8.8	HT1900.1-2455                 
262.9986 -33.6872    4.1  37.7  -17.9  -0.2082  -2.8    8.9	GX 354-0                      
341.0981 -31.8111    2.4  39.6   98.1   1.0078   4.9 ------	UNKNOWN                       
 17.8850 -76.0444    1.3  27.4 -170.2   0.4774   8.6 ------	UNKNOWN                       
215.8261 -55.8768    1.9  41.1  -81.3   1.2473   6.1 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:

Plot creation:
Sun May 31 06:26:32 EDT 2015