batgrbproduct analysis for trigger=534015

batgrbproduct Analysis for Trigger=534015

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): Mon Jan 13 00:37:36 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger534015
======================================================================

  Trigger: 00534015      Segment: 000

  BAT Trigger Time: 369659780.288   [s; MET]
      Trigger Stop: 369659781.312   [s; MET]
               UTC: 2012-09-18T11:16:10.624900    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 181.053946302635   Dec: -32.7576526591057  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    12.04
     Image Trigger?:     NO
     Rate S/N Ratio:     21.51743479135  [ if not an image trigger ]
     Image S/N Ratio:    12.04

  Flight Position:   [ source = BAT ]
    RA: 181.053946302635   Dec: -32.7576526591057  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 181.042274021015   Dec: -32.7623104417412  [deg; J2000]  
        { 12h 04m 10.1s , -32d 45' 44.3" }
         +/- 1.13833367413494 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.454785526709033 [arcmin] (formal 1-sigma fit error)
    SNR: 25.2774500554093
 
  Angular difference between Flight and Ground position is 0.651888 arcmin
 
  Partial Coding Fraction: 0.15625    [ including projection effects ]

  Duration
     T90: 25.095999956131 +/- 2.46916989103431
        Measured from: -1.85199999809265
                   to: 23.2439999580383     [s; relative to TRIGTIME]
     T50: 8.09599995613098 +/- 0.799622431797607
        Measured from: 0.752000033855438
                   to: 8.84799998998642     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: -0.283999979496002     
                   to: 0.716000020503998     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -2.86000001430511     
                   to: 23.9160000085831     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     1.295331   1.873860   1.415511   0.250458
           0.083614   0.086800   0.075870   0.061607 [error]
 Peak      0.113173   0.211930   0.173875   0.053659
           0.018298   0.019650   0.018480   0.013297 [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 4.62e-07 8.01e-07 1.06e-06 2.85e-06 3.09e-06 5.17e-06   erg/cm2
              Error 4.24e-08 4.50e-08 7.27e-08 4.17e-07 1.77e-07 4.72e-07   erg/cm2
Peak flux Power-law 1.34e+00 1.46e+00 1.14e+00 1.46e+00 4.49e+00 5.40e+00   ph/cm2/s
              Error 2.49e-01 1.72e-01 1.40e-01 3.59e-01 4.86e-01 5.77e-01   ph/cm2/s
 
Fluence   Cutoff-PL 4.14e-07 8.46e-07 1.10e-06 1.32e-06 2.98e-06 3.69e-06   erg/cm2
              Error 5.12e-08 5.41e-08 8.18e-08 6.21e-07 1.91e-07 6.38e-07   erg/cm2
Peak flux Cutoff-PL 1.12e+00 1.56e+00 1.25e+00 7.09e-01 4.37e+00 4.64e+00   ph/cm2/s
              Error 3.07e-01 2.02e-01 1.76e-01 4.75e-01 5.00e-01 5.37e-01   ph/cm2/s
 
Fluence        Band 4.12e-07 8.41e-07 1.10e-06 1.36e-06 2.99e-06 3.78e-06   erg/cm2
              Error 3.57e-08 -------- 7.73e-08 -------- -------- --------   erg/cm2
Peak flux      Band 1.15e+00 1.54e+00 1.24e+00 8.14e-01 4.40e+00 4.76e+00   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    1.598    0.092    -      -           1.23e-02 6.65e-04   62.760 57
CPL   1.002    0.392      85.9   37.0      2.43e-02 1.11e-02   55.010 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.362    0.170    -      -           3.72e-02 3.90e-03   72.060 57
CPL   0.525    0.801      95.5  125.8      9.28e-02 9.53e-02   68.120 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: 27.136000 sec.
T50 in the 50-300 keV band: 8.832000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   26.776   -2.860   23.916
T90    25.096   -1.852   23.244
T50     8.096    0.752    8.848
Peak    1.000   -0.284    0.716

Click here for the BAT GCN circular template

Image

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

#   RAcent    DECcent   POSerr    Theta     Phi              Peak Cts       SNR   Name
  181.0423   -32.7623   0.0076    37.6305   -91.2288         5.0286099     25.277 TRIG_00534015                 
 
Foreground time interval of the image:
 -2.860  23.916 (delta_t =  26.776 [sec])
Background time interval of the image:
-239.288  -2.860 (delta_t = 236.428 [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 1.024000

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 1.024000

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 1.024000

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   -2.860 sec. to   23.916 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.59755     ( -0.0912048   0.0918006 )
Norm@50keV  : 1.23415E-02    ( -0.000665764   0.000664469 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          62.76 using 59 PHA bins.
# Reduced chi-squared =          1.101 for     57 degrees of freedom 
# Null hypothesis probability =   2.795382e-01
 
Photon flux (15-150 keV)    in 26.78 sec: 1.58474 ( -0.0879658  0.0881452 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.09186e-06 ( -1.76565e-07  1.77155e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from   -2.860 sec. to   23.916 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.00182     ( -0.409768   0.374442 )
Epeak [keV] : 85.9200      ( -16.7641 57.3206 )
Norm@50keV  : 2.42761E-02    ( -0.00823624   0.01392 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.01 using 59 PHA bins.
# Reduced chi-squared =         0.9823 for     56 degrees of freedom 
# Null hypothesis probability =   5.124232e-01
 
Photon flux (15-150 keV)    in 26.78 sec: 1.53810 ( -0.09235  0.09247 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.98158e-06 ( -1.91316e-07  1.91182e-07 ) ergs/cm2

Band function

Time interval is from   -2.860 sec. to   23.916 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.00177   ( -0.337744   0.461566 )
beta        : -10.0000    ( 10   7.10543e-15 )
Epeak [keV] : 85.9031      ( -14.5218 57.2829 )
Norm@50keV   : 2.42755E-02    ( -0.00823106   0.0139303 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.01 using 59 PHA bins.
# Reduced chi-squared =          1.000 for     55 degrees of freedom 
# Null hypothesis probability =   4.743233e-01
 
Photon flux (15-150 keV)    in 26.78 sec: 1.53962 ( 5.46038  -0.09332 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.98929e-06 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 14.8622  (  )
R^2/D10^2   : 0.182240  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         118.45 using 59 PHA bins.
# Reduced chi-squared =         2.0781 for     57 degrees of freedom 
# Null hypothesis probability =   3.343761e-06
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.260e-07   2.240e-08
25- 50  8.904e-07   6.641e-08
50-150  1.333e-06   1.446e-07
15-150  2.449e-06   1.453e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 177.897       (-40.948      -177.527)
Norm        : 6.48053       (-0.378801     0.413198)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.35 using 59 PHA bins.
# Reduced chi-squared =         0.9886 for     57 degrees of freedom 
# Null hypothesis probability =   4.994346e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.382e-07   3.441e-08
25- 50  8.314e-07   1.086e-07
50-150  1.753e-06   6.651e-07
15-150  3.023e-06   7.755e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 7.17336        (-1.47049      1.59063)
R1^2/D10^2  : 1.42808        (-0.664532      1.69559)
kT2 [keV]   : 23.7408        (-3.6332      5.82279)
R2^2/D10^2  : 2.61616E-02    (-0.0150505   0.0249795)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.07 using 59 PHA bins.
# Reduced chi-squared =          1.020 for     55 degrees of freedom 
# Null hypothesis probability =   4.343550e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.945e-07   8.046e-08
25- 50  8.541e-07   1.482e-07
50-150  1.719e-06   4.211e-07
15-150  2.967e-06   6.206e-07

Peak spectrum fit

Power-law model

Time interval is from   -0.284 sec. to    0.716 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.36179     ( -0.169487   0.170043 )
Norm@50keV  : 3.71907E-02    ( -0.00390636   0.0039022 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          72.06 using 59 PHA bins.
# Reduced chi-squared =          1.264 for     57 degrees of freedom 
# Null hypothesis probability =   8.632037e-02
 
Photon flux (15-150 keV)    in 1 sec: 4.49142 ( -0.485758  0.486723 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.62283e-07 ( -4.11464e-08  4.13425e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.284 sec. to    0.716 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.524525     ( -0.875136   0.726441 )
Epeak [keV] : 95.5322      ( -25.0691 226.555 )
Norm@50keV  : 9.27822E-02    ( -0.0500116   0.140619 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.12 using 59 PHA bins.
# Reduced chi-squared =          1.216 for     56 degrees of freedom 
# Null hypothesis probability =   1.284571e-01
 
Photon flux (15-150 keV)    in 1 sec: 4.36724 ( -0.49972  0.49955 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.50901e-07 ( -4.3476e-08  4.3312e-08 ) ergs/cm2

Band function

Time interval is from   -0.284 sec. to    0.716 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.524469   ( -0.468473   0.866265 )
beta        : -10.0000    ( 10   3.55271e-15 )
Epeak [keV] : 95.5151      ( -35.6672 201.18 )
Norm@50keV   : 9.27880E-02    ( -0.0500415   0.140731 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.12 using 59 PHA bins.
# Reduced chi-squared =          1.239 for     55 degrees of freedom 
# Null hypothesis probability =   1.101263e-01
 
Photon flux (15-150 keV)    in 1 sec: 4.40119 (    ) 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]    : 17.2216  (-2.0112  2.32462)
R^2/D10^2   : 0.341564  (-0.121072   0.181606)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          79.07 using 59 PHA bins.
# Reduced chi-squared =          1.387 for     57 degrees of freedom 
# Null hypothesis probability =   2.817800e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.056e-08   4.480e-09
25- 50  9.189e-08   1.242e-08
50-150  1.954e-07   3.680e-08
15-150  3.078e-07   4.340e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (      )
Norm        : 18.7678       (-1.97126     1.97115)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          73.75 using 59 PHA bins.
# Reduced chi-squared =          1.294 for     57 degrees of freedom 
# Null hypothesis probability =   6.707911e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.673e-08   6.015e-09
25- 50  8.989e-08   3.560e-08
50-150  1.971e-07   1.027e-07
15-150  3.338e-07   1.732e-07

Double BB

R1^2/D10^2  : 1.41505        (      )
kT2 [keV]   : 27.8384        (-10.2794      50.0883)
R2^2/D10^2  : 4.69951E-02    (-0.0451066   0.263867)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          70.64 using 59 PHA bins.
#Fit statistic : Chi-Squared =          68.82 using 59 PHA bins.
#Fit statistic : Chi-Squared =          68.80 using 59 PHA bins.
# Reduced chi-squared =          1.284 for     55 degrees of freedom 
# Reduced chi-squared =          1.251 for     55 degrees of freedom 
# Reduced chi-squared =          1.251 for     55 degrees of freedom 
# Null hypothesis probability =   7.606907e-02
# Null hypothesis probability =   9.968895e-02
# Null hypothesis probability =   9.992245e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.655e-08   1.466e-08
25- 50  8.216e-08   1.802e-08
50-150  2.138e-07   4.990e-08
15-150  3.326e-07   6.510e-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: 1.59755     ( -0.0912048   0.0918006 )
Norm@50keV  : 1.23415E-02    ( -0.000665764   0.000664469 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          62.76 using 59 PHA bins.
# Reduced chi-squared =          1.101 for     57 degrees of freedom 
# Null hypothesis probability =   2.795382e-01
 
Photon flux (15-150 keV)    in 26.78 sec: 1.58474 ( -0.0879658  0.0881452 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.09186e-06 ( -1.76565e-07  1.77155e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.00182     ( -0.409768   0.374442 )
Epeak [keV] : 85.9200      ( -16.7641 57.3206 )
Norm@50keV  : 2.42761E-02    ( -0.00823624   0.01392 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.01 using 59 PHA bins.
# Reduced chi-squared =         0.9823 for     56 degrees of freedom 
# Null hypothesis probability =   5.124232e-01
 
Photon flux (15-150 keV)    in 26.78 sec: 1.53810 ( -0.09235  0.09247 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.98158e-06 ( -1.91316e-07  1.91182e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.00177   ( -0.337744   0.461566 )
beta        : -10.0000    ( 10   1.77636e-15 )
Epeak [keV] : 85.9031      ( -14.5218 57.2829 )
Norm@50keV   : 2.42755E-02    ( -0.00823106   0.0139303 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.01 using 59 PHA bins.
# Reduced chi-squared =          1.000 for     55 degrees of freedom 
# Null hypothesis probability =   4.743233e-01
 
Photon flux (15-150 keV)    in 26.78 sec: 1.53962 ( 5.46038  -0.09332 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.98929e-06 ( 0  0 ) ergs/cm2

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

S(25-50 keV)  = 8.01e-07
S(50-100 keV) = 1.06e-06

T90 vs. Hardness ratio plot

T90                                   = 25.095999956131 sec.
Hardness ratio (energy fluence ratio) = 1.32335

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.44663
Count Ratio (50-100 keV) / (15-25 keV) = 1.09278

Mask shadow pattern

IMX = -1.653280851973350E-02, IMY = 7.707761230919873E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000

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:
-239.288000 -2.860000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.5876 -40.5466    4.4  51.1 -141.6   2.8354   2.6    2.7	Vela X-1                      
170.0159 -60.5637    8.6  22.1 -142.7   0.2947   1.3    9.5	Cen X-3                       
186.6944 -62.7753    1.3  13.9 -140.8   1.9511   9.0    1.1	GX 301-2                      
244.9788 -15.6360    1.2  50.9   -1.4   5.0796   9.3    0.3	Sco X-1                       
256.1448 -37.8588  365.6  34.1   25.3  -0.0095  -0.0    7.5	4U 1700-377                   
256.4903 -36.5133    4.1  35.4   24.5   0.8533   2.8    6.0	GX 349+2                      
263.1407 -24.8172    6.3  48.4   23.8  -1.3197  -1.8    8.4	GX 1+4                        
264.9595 -44.5952    6.8  32.4   42.2   0.5073   1.7   12.7	4U 1735-44                    
270.2796 -24.9406    4.8  51.3   31.4  -2.7337  -2.4    8.3	GX 5-1                        
270.4499 -25.7937   12.3  50.6   32.1   1.0133   0.9    8.5	GRS 1758-258                  
263.1255 -33.9906  501.5  40.3   30.0   0.0094   0.0   11.6	GX 354-0                      
292.3724 -50.5981    2.6  40.4   72.3   3.9325   4.5 ------	UNKNOWN                       
266.3020 -26.3842    1.2  48.3   28.2   7.2315   9.7 ------	UNKNOWN                       
 43.0478 -74.2108    2.3  43.1  145.7   2.5350   5.0 ------	UNKNOWN                       
 75.8079 -71.1585    3.3  43.6  160.4   1.5710   3.6 ------	UNKNOWN                       
256.7743 -32.5251    2.3  39.0   21.6   1.7811   5.0 ------	UNKNOWN                       
254.1125 -73.8043    2.2  17.1  108.9   1.1665   5.2 ------	UNKNOWN                       
248.5211 -47.4085    0.9  23.1   26.7   2.6260  12.6 ------	UNKNOWN                       
113.9624 -42.2415    3.8  58.8 -159.2   5.7527   3.1 ------	UNKNOWN                       
226.4991  -4.3088    3.0  58.7  -25.9   5.2017   3.8 ------	UNKNOWN                       
174.1178 -31.8594    5.9  41.1  -98.8   3.0609   2.5 ------	UNKNOWN                       
	UNKNOWN

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

Time interval of the image:
-2.860000 23.916000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.4810 -40.5258   19.2  51.2 -141.7  -0.1865  -0.6    2.8	Vela X-1                      
170.2065 -60.4886    5.3  22.0 -142.4  -0.1471  -2.2    8.7	Cen X-3                       
186.5032 -62.9706    0.0  14.0 -141.6  -0.1307  -2.1   12.7	GX 301-2                      
244.8810 -15.6252  113.0  50.8   -1.6  -0.0142  -0.1    5.8	Sco X-1                       
255.8186 -37.9694    0.0  33.9   25.0   0.1554   1.8   10.9	4U 1700-377                   
256.5919 -36.5312    6.7  35.5   24.6  -0.1500  -1.7   10.0	GX 349+2                      
263.0275 -24.6534    6.1  48.5   23.6   0.3253   1.9    5.6	GX 1+4                        
264.5912 -44.3059   14.0  32.5   41.5   0.0739   0.8   10.8	4U 1735-44                    
270.3059 -25.1179    4.0  51.1   31.6  -0.9153  -2.9    2.6	GX 5-1                        
270.3569 -25.8866   24.3  50.5   32.1   0.1387   0.5    9.1	GRS 1758-258                  
262.8306 -33.7715    4.2  40.4   29.5  -0.3068  -2.8    8.8	GX 354-0                      
181.0423 -32.7623    0.5  37.6  -91.2   5.0272  25.3 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:

Plot creation:
Sat May 30 18:21:20 EDT 2015