batgrbproduct analysis for trigger=156434

batgrbproduct Analysis for Trigger=156434

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): Wed Jan 22 20:07:52 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger156434
======================================================================

  Trigger: 00156434      Segment: 000

  BAT Trigger Time: 149094120   [s; MET]
      Trigger Stop: 149094288   [s; MET]
               UTC: 2005-09-22T15:02:00.257060    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 5.79986495504588   Dec: -5.59886385721478  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    8.66
     Image Trigger?:     YES
     Rate S/N Ratio:     0  [ if not an image trigger ]
     Image S/N Ratio:    8.66

  Flight Position:   [ source = BAT ]
    RA: 5.79986495504588   Dec: -5.59886385721478  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 5.78404911530879   Dec: -5.6210218655456  [deg; J2000]  
        { 00h 23m 08.2s , -05d 37' 15.7" }
         +/- 2.54520874396333 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.937023975116539 [arcmin] (formal 1-sigma fit error)
    SNR: 8.00780545120976
 
  Angular difference between Flight and Ground position is 1.630773 arcmin
 
  Partial Coding Fraction: 0.1152344    [ including projection effects ]

  Duration
     T90: 157.02399995923 +/- 94.4868116047978
        Measured from: 27.3840000033379
                   to: 184.407999962568     [s; relative to TRIGTIME]
     T50: 15.3759999573231 +/- 187.397459802878
        Measured from: 39.7680000066757
                   to: 55.1439999639988     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 98.636000007391     
                   to: 99.636000007391     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: 24.4239999949932     
                   to: 273.624000012875     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     1.644715   1.671852   0.869463   0.065991
           0.188739   0.194448   0.172683   0.159015 [error]
 Peak      0.026084   0.048330   0.054775  -0.001340
           0.014706   0.014705   0.013228   0.012127 [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 5.81e-07 7.36e-07 6.80e-07 1.10e-06 2.37e-06 3.10e-06   erg/cm2
              Error 9.95e-08 9.43e-08 1.62e-07 5.15e-07 3.68e-07 7.04e-07   erg/cm2
Peak flux Power-law 3.11e-01 3.53e-01 2.86e-01 3.86e-01 1.09e+00 1.34e+00   ph/cm2/s
              Error 1.80e-01 1.28e-01 9.56e-02 2.70e-01 3.52e-01 4.06e-01   ph/cm2/s
 
Fluence   Cutoff-PL 5.69e-07 7.64e-07 6.68e-07 6.22e-07 2.30e-06 2.62e-06   erg/cm2
              Error 1.08e-07 1.23e-07 1.80e-07 5.82e-07 4.20e-07 9.31e-07   erg/cm2
Peak flux Cutoff-PL 2.44e-01 3.63e-01 3.18e-01 2.09e-01 1.05e+00 1.13e+00   ph/cm2/s
              Error 2.20e-01 1.49e-01 1.25e-01 2.47e-01 3.68e-01 4.93e-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    2.114    0.252    -      -           1.02e-03 1.76e-04   51.460 57
CPL   1.816    0.701      25.0   -0.5      1.53e-03 3.14e-03   51.170 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.303    0.520    -      -           9.14e-03 2.77e-03   54.040 57
CPL   0.458    2.631     108.4    0.0      2.11e-02 1.57e-01   53.480 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  249.200   24.424  273.624
T90   157.024   27.384  184.408
T50    15.376   39.768   55.144
Peak    1.000   98.636   99.636

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
    5.7840    -5.6210   0.0240    37.5967    98.3201         3.4534263      8.008 TRIG_00156434                 
 
Foreground time interval of the image:
 24.424 177.701 (delta_t = 153.277 [sec])
Background time interval of the image:
-299.000  24.424 (delta_t = 323.424 [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 168.000000

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 168.000000

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 168.000000

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   24.424 sec. to  273.624 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.11410     ( -0.241773   0.262904 )
Norm@50keV  : 1.02293E-03    ( -0.000178983   0.000173412 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.46 using 59 PHA bins.
# Reduced chi-squared =         0.9028 for     57 degrees of freedom 
# Null hypothesis probability =   6.821570e-01
 
Photon flux (15-150 keV)    in 249.2 sec: 0.162062 ( -0.0200982  0.0200997 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.37177e-06 ( -3.62539e-07  3.73556e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from   24.424 sec. to  273.624 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.81639     ( -1.12351   0.278479 )
Epeak [keV] : 25.0496      ( -23.9617 -25.0489 )
Norm@50keV  : 1.53249E-03    ( -0.000709   0.00556913 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.17 using 59 PHA bins.
# Reduced chi-squared =         0.9138 for     56 degrees of freedom 
# Null hypothesis probability =   6.578694e-01
 
Photon flux (15-150 keV)    in 249.2 sec: 0.160240 ( -0.020837  0.020655 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.29776e-06 ( -4.1362e-07  4.26947e-07 ) ergs/cm2

Band function

Time interval is from   24.424 sec. to  273.624 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.80128   ( 1.76412   1.76412 )
beta        : -2.52659    ( 2.51128   0.625508 )
Epeak [keV] : 25.5155      ( -25.5113 -25.5113 )
Norm@50keV   : 1.56710E-03    ( -0.00058991   0.102194 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.15 using 59 PHA bins.
# Reduced chi-squared =         0.9301 for     55 degrees of freedom 
# Null hypothesis probability =   6.223382e-01
 
Photon flux (15-150 keV)    in 249.2 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]    : 9.14535  (-1.42102  1.66156)
R^2/D10^2   : 0.103316  (-0.0490915   0.0966809)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          66.59 using 59 PHA bins.
# Reduced chi-squared =          1.168 for     57 degrees of freedom 
# Null hypothesis probability =   1.803283e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.226e-07   8.722e-08
25- 50  9.209e-07   1.566e-07
50-150  3.689e-07   1.388e-07
15-150  1.712e-06   3.189e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 55.4166       (-17.3423      30.2492)
Norm        : 0.876513       (-0.178493     0.229171)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.79 using 59 PHA bins.
# Reduced chi-squared =         0.9086 for     57 degrees of freedom 
# Null hypothesis probability =   6.702085e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.413e-07   8.971e-08
25- 50  8.033e-07   1.220e-07
50-150  8.540e-07   2.994e-07
15-150  2.199e-06   3.905e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 4.52892        (-1.60322      1.98981)
R1^2/D10^2  : 1.14371        (-0.829164      7.38503)
kT2 [keV]   : 15.6977        (-4.22036      9.49183)
R2^2/D10^2  : 9.53329E-03    (-0.00805051   0.0258457)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.17 using 59 PHA bins.
# Reduced chi-squared =         0.9304 for     55 degrees of freedom 
# Null hypothesis probability =   6.217501e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.801e-07   3.096e-07
25- 50  7.358e-07   3.863e-07
50-150  8.657e-07   5.043e-07
15-150  2.182e-06   1.120e-06

Peak spectrum fit

Power-law model

Time interval is from   98.636 sec. to   99.636 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.30268     ( -0.527472   0.512311 )
Norm@50keV  : 9.14166E-03    ( -0.00276712   0.00276312 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.04 using 59 PHA bins.
# Reduced chi-squared =         0.9481 for     57 degrees of freedom 
# Null hypothesis probability =   5.867747e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.09118 ( -0.349132  0.354924 ) ph/cm2/s
Energy fluence (15-150 keV)             : 9.02772e-08 ( -2.84148e-08  2.86873e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   98.636 sec. to   99.636 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.457668     ( -3.34663   1.91574 )
Epeak [keV] : 108.361      ( -108.451 -108.451 )
Norm@50keV  : 2.11034E-02    ( -0.0210779   0.293702 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.48 using 59 PHA bins.
# Reduced chi-squared =         0.9550 for     56 degrees of freedom 
# Null hypothesis probability =   5.707949e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.04582 ( -0.367557  0.36938 ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.83496e-08 ( -2.91376e-08  2.92894e-08 ) ergs/cm2

Band function

Time interval is from   98.636 sec. to   99.636 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.563361   ( -2.78072   4.57482 )
beta        : -9.37167    ( 9.37131   19.3713 )
Epeak [keV] : 117.728      ( -59.7249 354.993 )
Norm@50keV   : 1.87788E-02    ( -0.0187775   206.835 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.49 using 59 PHA bins.
# Reduced chi-squared =         0.9726 for     55 degrees of freedom 
# Null hypothesis probability =   5.324228e-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]    : 20.9114  (-6.32655  9.48292)
R^2/D10^2   : 4.34101E-02  (-0.0434101   0.10055)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.63 using 59 PHA bins.
# Reduced chi-squared =         0.9584 for     57 degrees of freedom 
# Null hypothesis probability =   5.645213e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.593e-09   2.275e-09
25- 50  1.842e-08   1.123e-08
50-150  6.001e-08   4.081e-08
15-150  8.202e-08   5.315e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.363       (-111.611      -199.363)
Norm        : 4.63655       (-1.4108     1.41084)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.56 using 59 PHA bins.
# Reduced chi-squared =         0.9572 for     57 degrees of freedom 
# Null hypothesis probability =   5.670404e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.155e-08   7.060e-09
25- 50  2.221e-08   1.342e-08
50-150  4.871e-08   2.915e-08
15-150  8.246e-08   5.085e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.53375        (-5.50876      194.415)
R1^2/D10^2  : 2.04774        (-2.07135      -2.07135)
kT2 [keV]   : 24.9646        (-8.37299      -24.9539)
R2^2/D10^2  : 2.16981E-02    (-0.0217315   0.0680892)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.54 using 59 PHA bins.
# Reduced chi-squared =         0.9553 for     55 degrees of freedom 
# Null hypothesis probability =   5.690469e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  9.699e-09   6.165e-09
25- 50  1.944e-08   1.061e-08
50-150  6.200e-08   3.955e-08
15-150  9.114e-08   5.190e-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: 2.02150     ( -0.245563   0.265558 )
Norm@50keV  : 1.52781E-03    ( -0.000262237   0.000253207 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.46 using 59 PHA bins.
# Reduced chi-squared =         0.8677 for     57 degrees of freedom 
# Null hypothesis probability =   7.507459e-01
 
Photon flux (15-150 keV)    in 153.3 sec: 0.231468 ( -0.0299095  0.0299185 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.16256e-06 ( -3.38506e-07  3.4737e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.79905     ( -1.06624   0.337302 )
Epeak [keV] : 38.7492      (   )
Norm@50keV  : 2.04578E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.29 using 59 PHA bins.
# Reduced chi-squared =         0.8802 for     56 degrees of freedom 
# Null hypothesis probability =   7.249897e-01
 
Photon flux (15-150 keV)    in 153.3 sec: 0.229481 ( -0.030959  0.015469 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.11795e-06 ( -3.76413e-07  3.80935e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.79896   ( -2.33819   1.00752 )
beta        : -10.0000    ( 10   3.55271e-15 )
Epeak [keV] : 38.7194      ( -22.1122 -38.7196 )
Norm@50keV   : 2.04584E-03    ( -0.000553656   0.00612734 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.29 using 59 PHA bins.
# Reduced chi-squared =         0.8962 for     55 degrees of freedom 
# Null hypothesis probability =   6.916161e-01
 
Photon flux (15-150 keV)    in 153.3 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.11697e-06 ( 0  0 ) ergs/cm2

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

S(25-50 keV)  = 7.36e-07
S(50-100 keV) = 6.80e-07

T90 vs. Hardness ratio plot

T90                                   = 157.02399995923 sec.
Hardness ratio (energy fluence ratio) = 0.923913

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.0165
Count Ratio (50-100 keV) / (15-25 keV) = 0.528641

Mask shadow pattern

IMX = -1.114227923780043E-01, IMY = -7.619069414942475E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 168.000000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 168.000000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 168.000000

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:
-299.000000 24.424000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
299.5862  35.2026    0.5  36.8  -87.8  11.4816  21.8    0.2	Cyg X-1                       
308.1217  40.9378    1.0  32.8  -73.9   3.7257  11.0    1.0	Cyg X-3                       
326.1069  38.2233    3.6  21.1  -56.3   0.6629   3.2    6.6	Cyg X-2                       
 14.7746  14.2269    3.1  36.1   61.7   1.6430   3.7 ------	UNKNOWN                       
338.3435 -29.7706    3.5  49.4  148.0   2.9460   3.3 ------	UNKNOWN                       
 32.0772  42.9002    2.7  51.1   19.2   3.0963   4.3 ------	UNKNOWN                       
347.5982  26.4752    2.4  11.6   20.8   0.8205   4.7 ------	UNKNOWN                       
358.4001  54.2854    3.5  38.2  -11.2   0.8016   3.3 ------	UNKNOWN                       
311.9930  58.5244    2.9  43.1  -50.1   2.0279   4.0 ------	UNKNOWN

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

Time interval of the image:
24.424000 177.700610
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
299.7762  35.1921    6.6  36.6  -87.8  -0.5776  -1.7    9.1	Cyg X-1                       
308.1897  40.8372    4.8  32.7  -74.0  -0.5376  -2.4    7.8	Cyg X-3                       
326.3730  38.3074    8.7  21.0  -55.7   0.1924   1.3    9.5	Cyg X-2                       
  5.7840  -5.6211    1.4  37.6   98.3   3.4531   8.0  483.5	UNKNOWN                       
318.5965 -15.9858    1.8  40.1  177.9   1.2657   6.3 ------	UNKNOWN                       
312.6483  17.7768    2.4  23.5 -121.2   0.6627   4.9 ------	UNKNOWN                       
304.4057   6.3190    2.5  34.7 -138.9   0.8697   4.7 ------	UNKNOWN                       
289.8006   2.2547    2.1  49.6 -135.2   3.3861   5.4 ------	UNKNOWN                       
289.1587   3.3656    2.2  49.8 -133.6   3.3744   5.3 ------	UNKNOWN                       
293.0344  28.3709    2.2  41.3  -99.9   2.8967   5.3 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:

Plot creation:
Sun May 31 15:34:23 EDT 2015