batgrbproduct analysis for trigger=293707

batgrbproduct Analysis for Trigger=293707

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 20 06:44:27 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger293707
======================================================================

  Trigger: 00293707      Segment: 000

  BAT Trigger Time: 213680475.136   [s; MET]
      Trigger Stop: 213680479.232   [s; MET]
               UTC: 2007-10-10T03:41:12.855120    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 288.100630766172   Dec: -32.3786069237812  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    7.17
     Image Trigger?:     NO
     Rate S/N Ratio:     9.1104335791443  [ if not an image trigger ]
     Image S/N Ratio:    7.17

  Flight Position:   [ source = BAT ]
    RA: 288.100630766172   Dec: -32.3786069237812  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 288.042417503405   Dec: -32.3838763787873  [deg; J2000]  
        { 19h 12m 10.2s , -32d 23' 02.0" }
         +/- 2.50674241819008 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.956013726506567 [arcmin] (formal 1-sigma fit error)
    SNR: 8.18392519995838
 
  Angular difference between Flight and Ground position is 2.966574 arcmin
 
  Partial Coding Fraction: 0.4296875    [ including projection effects ]

  Duration
     T90: 6.32400000095367 +/- 1.86554119492639
        Measured from: -0.904000014066696
                   to: 5.41999998688698     [s; relative to TRIGTIME]
     T50: 2.70800000429153 +/- 1.57969618105291
        Measured from: 0.859999984502792
                   to: 3.56799998879433     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 0.803999990224838     
                   to: 1.80399999022484     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -1.14399999380112     
                   to: 5.8759999871254     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.143275   0.149767   0.071647  -0.016126
           0.023874   0.024170   0.021141   0.018948 [error]
 Peak      0.040175   0.026281   0.020976   0.004316
           0.009044   0.009223   0.008179   0.007286 [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 5.49e-08 6.46e-08 5.48e-08 7.87e-08 2.02e-07 2.53e-07   erg/cm2
              Error 1.29e-08 1.23e-08 1.85e-08 5.05e-08 4.42e-08 7.51e-08   erg/cm2
Peak flux Power-law 4.93e-01 2.76e-01 9.73e-02 4.49e-02 8.91e-01 9.12e-01   ph/cm2/s
              Error 1.84e-01 9.38e-02 6.76e-02 6.41e-02 2.52e-01 2.61e-01   ph/cm2/s
 
Fluence   Cutoff-PL 4.72e-08 7.83e-08 5.37e-08 1.20e-08 1.89e-07 1.91e-07   erg/cm2
              Error 1.52e-08 1.70e-08 2.24e-08 2.83e-08 4.21e-08 4.95e-08   erg/cm2
Peak flux Cutoff-PL 5.05e-01 2.71e-01 9.12e-02 3.90e-02 8.90e-01 9.10e-01   ph/cm2/s
              Error 1.86e-01 9.00e-02 -------- 6.40e-02 2.51e-01 2.58e-01   ph/cm2/s
 
Fluence        Band 4.67e-08 7.80e-08 5.36e-08 1.20e-08 1.89e-07 1.91e-07   erg/cm2
              Error -------- -------- -------- -------- 4.15e-08 --------   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    2.238    0.343    -      -           3.05e-03 7.67e-04   48.070 57
CPL   0.615    1.627      36.4    0.0      2.56e-02 0.00e+00   43.770 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    2.505    0.782    -      -           4.52e-03 3.41e-03   50.710 57
CPL   3.066    0.000     339.4    0.0      2.42e-03 3.33e-03   50.470 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    7.020   -1.144    5.876
T90     6.324   -0.904    5.420
T50     2.708    0.860    3.568
Peak    1.000    0.804    1.804

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
  288.0424   -32.3839   0.0235    45.2507  -167.6347         0.3727602      8.184 TRIG_00293707                 
 
Foreground time interval of the image:
 -1.144   5.876 (delta_t =   7.020 [sec])
Background time interval of the image:
-239.136  -1.144 (delta_t = 237.992 [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   -1.144 sec. to    5.876 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.23792     ( -0.319724   0.365738 )
Norm@50keV  : 3.04935E-03    ( -0.000777621   0.000755673 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.07 using 59 PHA bins.
# Reduced chi-squared =         0.8434 for     57 degrees of freedom 
# Null hypothesis probability =   7.941128e-01
 
Photon flux (15-150 keV)    in 7.02 sec: 0.515113 ( -0.0944965  0.0945223 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.02399e-07 ( -4.33482e-08  4.49615e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -1.144 sec. to    5.876 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.614526     ( -1.88346   1.37105 )
Epeak [keV] : 36.3976      (   )
Norm@50keV  : 2.56220E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          43.77 using 59 PHA bins.
# Reduced chi-squared =         0.7816 for     56 degrees of freedom 
# Null hypothesis probability =   8.825940e-01
 
Photon flux (15-150 keV)    in 7.02 sec: 0.496251 ( -0.09515  0.095089 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.89256e-07 ( -4.04808e-08  4.37683e-08 ) ergs/cm2

Band function

Time interval is from   -1.144 sec. to    5.876 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.201056   ( -0.861128   2.57853 )
beta        : -9.37167    ( 9.37167   19.3717 )
Epeak [keV] : 39.9673      ( -26.2642 13.9392 )
Norm@50keV   : 3.93407E-02    ( -0.0391242   0.320051 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.10 using 59 PHA bins.
# Reduced chi-squared =         0.8018 for     55 degrees of freedom 
# Null hypothesis probability =   8.536711e-01
 
Photon flux (15-150 keV)    in 7.02 sec: 0.500040 ( 6.49996  -0.090227 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.88857e-07 ( -1.88808e-07  -3.97557e-08 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 9.97166  (-1.8953  2.21124)
R^2/D10^2   : 0.248355  (-0.134628   0.313221)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.24 using 59 PHA bins.
# Reduced chi-squared =         0.8287 for     57 degrees of freedom 
# Null hypothesis probability =   8.184037e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.527e-08   1.222e-08
25- 50  8.734e-08   3.001e-08
50-150  4.521e-08   2.090e-08
15-150  1.678e-07   4.672e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 48.3716       (-16.5937      30.161)
Norm        : 3.03013       (-0.790408     1.13126)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.46 using 59 PHA bins.
# Reduced chi-squared =         0.7799 for     57 degrees of freedom 
# Null hypothesis probability =   8.869321e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.161e-08   1.151e-08
25- 50  7.323e-08   1.925e-08
50-150  6.889e-08   3.477e-08
15-150  1.937e-07   5.405e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 3.23143        (-1.98942      4.32288)
R1^2/D10^2  : 13.3821        (-12.9742      18308.7)
kT2 [keV]   : 12.2391        (-2.86653      5.81841)
R2^2/D10^2  : 9.74703E-02    (-0.0844701   0.198477)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          42.50 using 59 PHA bins.
# Reduced chi-squared =         0.7727 for     55 degrees of freedom 
# Null hypothesis probability =   8.909464e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.917e-08   2.650e-08
25- 50  7.506e-08   4.184e-08
50-150  6.380e-08   4.054e-08
15-150  1.880e-07   9.986e-08

Peak spectrum fit

Power-law model

Time interval is from    0.804 sec. to    1.804 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.50512     ( -0.629267   0.933876 )
Norm@50keV  : 4.52192E-03    ( -0.00452143   0.00229276 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.71 using 59 PHA bins.
# Reduced chi-squared =         0.8896 for     57 degrees of freedom 
# Null hypothesis probability =   7.086226e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.891101 ( -0.251521  0.251564 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.52776e-08 ( -1.66784e-08  1.79669e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.804 sec. to    1.804 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 3.06643     ( -1.98995   -1.98995 )
Epeak [keV] : 339.354      (   )
Norm@50keV  : 2.41749E-03    ( -0.00239518   0.00426235 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.47 using 59 PHA bins.
# Reduced chi-squared =         0.9013 for     56 degrees of freedom 
# Null hypothesis probability =   6.833063e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.889730 ( -0.251716  0.25052 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.49629e-08 ( -1.63716e-08  1.80177e-08 ) ergs/cm2

Band function

Time interval is from    0.804 sec. to    1.804 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.108021   ( -1.88164   0.107959 )
beta        : -2.50562    ( -0.935099   0.628179 )
Epeak [keV] : 3.11031      ( -3.10998 -3.10998 )
Norm@50keV   : 21.9652    ( -21.9591   4.87517e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.71 using 59 PHA bins.
# Reduced chi-squared =         0.9220 for     55 degrees of freedom 
# Null hypothesis probability =   6.391902e-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]    : 5.67065  (-2.20432  5.62398)
R^2/D10^2   : 3.75290  (-3.64978   35.2877)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.80 using 59 PHA bins.
# Reduced chi-squared =         0.9965 for     57 degrees of freedom 
# Null hypothesis probability =   4.825252e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.472e-08   8.885e-09
25- 50  1.295e-08   8.480e-09
50-150  9.353e-10   8.100e-10
15-150  2.860e-08   1.782e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 38.7658       (-24.7796      72.5787)
Norm        : 5.76083       (-2.63267     10.3511)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.23 using 59 PHA bins.
# Reduced chi-squared =         0.9164 for     57 degrees of freedom 
# Null hypothesis probability =   6.541584e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.309e-08   6.000e-09
25- 50  1.698e-08   8.785e-09
50-150  1.269e-08   9.487e-09
15-150  4.276e-08   2.283e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 3.30175        (-2.22487      2.43284)
R1^2/D10^2  : 40.8382        (-38.0323      86719.5)
kT2 [keV]   : 16.8401        (-4.89353      18.1238)
R2^2/D10^2  : 3.83090E-02    (-0.0351822   0.466651)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.55 using 59 PHA bins.
# Reduced chi-squared =         0.9010 for     55 degrees of freedom 
# Null hypothesis probability =   6.820054e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.574e-08   8.635e-09
25- 50  1.246e-08   7.155e-09
50-150  1.967e-08   1.376e-08
15-150  4.787e-08   2.636e-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: 2.23792     ( -0.319724   0.365738 )
Norm@50keV  : 3.04935E-03    ( -0.000777621   0.000755673 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.07 using 59 PHA bins.
# Reduced chi-squared =         0.8434 for     57 degrees of freedom 
# Null hypothesis probability =   7.941128e-01
 
Photon flux (15-150 keV)    in 7.02 sec: 0.515113 ( -0.0944965  0.0945223 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.02399e-07 ( -4.33482e-08  4.49615e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.614526     ( -1.88346   1.37105 )
Epeak [keV] : 36.3976      (   )
Norm@50keV  : 2.56220E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          43.77 using 59 PHA bins.
# Reduced chi-squared =         0.7816 for     56 degrees of freedom 
# Null hypothesis probability =   8.825940e-01
 
Photon flux (15-150 keV)    in 7.02 sec: 0.496251 ( -0.09515  0.095089 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.89256e-07 ( -4.04808e-08  4.37683e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.201056   ( -0.861128   2.57853 )
beta        : -9.37167    ( 9.37167   19.3717 )
Epeak [keV] : 39.9673      ( -28.2491 13.9373 )
Norm@50keV   : 3.93407E-02    ( -0.0391242   0.320051 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.10 using 59 PHA bins.
# Reduced chi-squared =         0.8018 for     55 degrees of freedom 
# Null hypothesis probability =   8.536711e-01
 
Photon flux (15-150 keV)    in 7.02 sec: 0.500040 ( 6.49996  -0.090227 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.88857e-07 ( -1.88808e-07  -3.97557e-08 ) ergs/cm2

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

S(25-50 keV)  = 6.46e-08
S(50-100 keV) = 5.48e-08

T90 vs. Hardness ratio plot

T90                                   = 6.32400000095367 sec.
Hardness ratio (energy fluence ratio) = 0.848297

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.04531
Count Ratio (50-100 keV) / (15-25 keV) = 0.500066

Mask shadow pattern

IMX = -9.853890630636623E-01, IMY = 2.160253970975944E-01

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:
-239.136000 -1.144000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
268.3569  -1.4160    7.1  35.5 -112.4   0.6374   1.6    2.3	SW J1753.5-0127               
270.3663 -25.0940   12.5  47.3 -144.1   0.4450   0.9    4.6	GX 5-1                        
270.4444 -25.9213    7.4  47.9 -144.9  -0.7519  -1.6   13.2	GRS 1758-258                  
274.0465 -14.0266    3.6  37.2 -135.6   1.0382   3.2    2.4	GX 17+2                       
275.8663 -30.4929   29.7  48.4 -153.8  -0.1744  -0.4    8.1	H1820-303                     
284.9065 -24.7494    0.0  39.3 -159.4  -0.3103  -1.0   12.5	HT1900.1-2455                 
288.7947  10.9411    1.2  12.9  -92.7   1.8939   9.7    0.3	GRS 1915+105                  
299.5868  35.2050    0.2  24.4   -8.7   9.9637  46.6    0.3	Cyg X-1                       
308.1666  40.9439    1.2  30.6    5.2   2.0985   9.7    2.6	Cyg X-3                       
326.1445  38.3161   19.8  35.0   30.1   0.1659   0.6    1.3	Cyg X-2                       
308.0793  37.6213    0.9  27.3    6.6   2.7204  13.3 ------	UNKNOWN                       
277.6361  58.2679    2.1  50.8  -20.3   2.5887   5.6 ------	UNKNOWN                       
257.9729  36.6173    3.3  47.1  -53.6   3.4566   3.5 ------	UNKNOWN

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

Time interval of the image:
-1.144000 5.876000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
268.3289  -1.5247    8.9  35.6 -112.5  -0.0694  -1.3    4.9	SW J1753.5-0127               
270.3487 -24.9942    7.5  47.3 -144.0   0.0978   1.5    6.2	GX 5-1                        
270.1683 -25.7184    6.0  47.9 -144.5  -0.1258  -1.9    7.4	GRS 1758-258                  
273.9862 -14.1713   23.4  37.3 -135.7  -0.0194  -0.5    8.2	GX 17+2                       
275.8672 -30.2561    7.9  48.2 -153.6  -0.0872  -1.5    7.3	H1820-303                     
285.0308 -25.0528    6.9  39.5 -159.8  -0.0595  -1.7    7.9	HT1900.1-2455                 
288.6415  10.8040    0.0  13.0  -93.3   0.0529   2.0   12.5	GRS 1915+105                  
299.4941  35.0552    9.1  24.3   -8.9   0.0320   1.3   10.0	Cyg X-1                       
308.2697  40.8640    5.3  30.5    5.4  -0.0676  -2.2    9.0	Cyg X-3                       
326.3614  38.4214    0.0  35.2   30.2   0.0457   1.1   10.7	Cyg X-2                       
308.1339 -44.8613    2.8  56.0  170.5   0.6081   4.0 ------	UNKNOWN                       
303.7701  32.2887    2.3  21.5    0.2   0.1343   5.0 ------	UNKNOWN                       
288.0424 -32.3839    1.4  45.3 -167.6   0.3728   8.2 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:

Plot creation:
Sun May 31 09:05:24 EDT 2015