batgrbproduct analysis for trigger=375246

batgrbproduct Analysis for Trigger=375246

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 12:56:25 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger375246
======================================================================

  Trigger: 00375246      Segment: 000

  BAT Trigger Time: 279435468.608   [s; MET]
      Trigger Stop: 279435484.992   [s; MET]
               UTC: 2009-11-09T04:57:43.363760    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 309.264961145751   Dec: -44.1765036048656  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    7.64
     Image Trigger?:     NO
     Rate S/N Ratio:     13.5277492584687  [ if not an image trigger ]
     Image S/N Ratio:    7.64

  Flight Position:   [ source = BAT ]
    RA: 309.264961145751   Dec: -44.1765036048656  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 309.252520677822   Dec: -44.1774300469834  [deg; J2000]  
        { 20h 37m 00.6s , -44d 10' 38.7" }
         +/- 2.09299540506235 [arcmin] (estimated 90% radius based on SNR)
         +/- 1.09865328435654 [arcmin] (formal 1-sigma fit error)
    SNR: 10.5895617528812
 
  Angular difference between Flight and Ground position is 0.538210 arcmin
 
  Partial Coding Fraction: 0.1972656    [ including projection effects ]

  Duration
     T90: 48.0320000648499 +/- 16.9502235222856
        Measured from: 0.407999992370605
                   to: 48.4400000572205     [s; relative to TRIGTIME]
     T50: 15.1520000696182 +/- 8.93454955460532
        Measured from: 7.87999999523163
                   to: 23.0320000648499     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 8.2039999961853     
                   to: 9.2039999961853     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -0.839999973773956     
                   to: 51.7520000338554     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.557170   0.779658   0.692264   0.325297
           0.104882   0.104663   0.088659   0.075500 [error]
 Peak      0.021632   0.058814   0.046209   0.028349
           0.014465   0.014648   0.012649   0.010496 [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 1.77e-07 3.66e-07 5.92e-07 2.15e-06 1.64e-06 3.28e-06   erg/cm2
              Error 5.03e-08 6.04e-08 8.67e-08 7.60e-07 2.19e-07 7.89e-07   erg/cm2
Peak flux Power-law 3.65e-01 4.00e-01 3.12e-01 4.00e-01 1.23e+00 1.48e+00   ph/cm2/s
              Error 2.16e-01 1.45e-01 1.01e-01 2.85e-01 3.94e-01 4.30e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.77e-07 3.67e-07 5.92e-07 2.12e-06 1.64e-06 3.26e-06   erg/cm2
              Error 5.00e-08 5.96e-08 8.67e-08 7.90e-07 2.15e-07 8.66e-07   erg/cm2
Peak flux Cutoff-PL 3.67e-01 4.00e-01 3.11e-01 3.94e-01 1.23e+00 1.47e+00   ph/cm2/s
              Error 2.33e-01 1.14e-01 1.13e-01 -------- 3.95e-01 4.33e-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    1.306    0.250    -      -           3.16e-03 4.15e-04   60.550 57
CPL   2.172    0.000      63.7    0.0      9.19e-04 0.00e+00   59.870 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.358    0.541    -      -           1.02e-02 2.98e-03   60.540 57
CPL   3.183    0.000     326.9    0.0      9.15e-04 0.00e+00   60.120 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: 20.928000 sec.
T50 in the 50-300 keV band: 10.112000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   52.592   -0.840   51.752
T90    48.032    0.408   48.440
T50    15.152    7.880   23.032
Peak    1.000    8.204    9.204

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
  309.2525   -44.1774   0.0182    47.4042   162.8163         2.3124980     10.590 TRIG_00375246                 
 
Foreground time interval of the image:
 -0.840  51.752 (delta_t =  52.592 [sec])
Background time interval of the image:
-239.608  -0.840 (delta_t = 238.768 [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 16.384000

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 16.384000

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 16.384000

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   -0.840 sec. to   51.752 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.30624     ( -0.254288   0.245172 )
Norm@50keV  : 3.16003E-03    ( -0.000415803   0.000413227 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.55 using 59 PHA bins.
# Reduced chi-squared =          1.062 for     57 degrees of freedom 
# Null hypothesis probability =   3.489874e-01
 
Photon flux (15-150 keV)    in 52.59 sec: 0.377434 ( -0.0550933  0.0555345 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.63972e-06 ( -2.19003e-07  2.19798e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.840 sec. to   51.752 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.17212     (     )
Epeak [keV] : 63.7133      (   )
Norm@50keV  : 9.18811E-04    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.87 using 59 PHA bins.
# Reduced chi-squared =          1.069 for     56 degrees of freedom 
# Null hypothesis probability =   3.370438e-01
 
Photon flux (15-150 keV)    in 52.59 sec: 0.381405 ( -0.059527  0.052057 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.63917e-06 ( -2.18433e-07  2.12416e-07 ) ergs/cm2

Band function

Time interval is from   -0.840 sec. to   51.752 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.03587   ( 1.03588   1.03588 )
beta        : -1.30620    ( 1.30622   0.255018 )
Epeak [keV] : 42.5635      ( -42.5544 -42.5544 )
Norm@50keV   : 6.09942E-03    ( -0.00334845   0.479556 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.55 using 59 PHA bins.
# Reduced chi-squared =          1.101 for     55 degrees of freedom 
# Null hypothesis probability =   2.824734e-01
 
Photon flux (15-150 keV)    in 52.59 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]    : 22.4180  (-4.43355  6.00928)
R^2/D10^2   : 1.08889E-02  (-0.0108392   0.0119929)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          85.30 using 59 PHA bins.
# Reduced chi-squared =          1.497 for     57 degrees of freedom 
# Null hypothesis probability =   8.960713e-03
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.280e-08   1.595e-08
25- 50  2.823e-07   7.620e-08
50-150  1.060e-06   2.409e-07
15-150  1.395e-06   3.087e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (      )
Norm        : 1.60894       (-0.211293     0.211209)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          66.20 using 59 PHA bins.
# Reduced chi-squared =          1.161 for     57 degrees of freedom 
# Null hypothesis probability =   1.892730e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.107e-07   1.194e-07
25- 50  4.054e-07   2.245e-07
50-150  8.890e-07   4.899e-07
15-150  1.505e-06   8.183e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 7.06964        (-2.10593      2.72506)
R1^2/D10^2  : 0.428331        (-0.298161      1.31377)
kT2 [keV]   : 42.5836        (-13.6225      53.1157)
R2^2/D10^2  : 1.32424E-03    (-0.00111652   0.00187838)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.97 using 59 PHA bins.
# Reduced chi-squared =          1.054 for     55 degrees of freedom 
# Null hypothesis probability =   3.662814e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.983e-07   1.113e-07
25- 50  3.632e-07   1.739e-07
50-150  1.157e-06   6.123e-07
15-150  1.719e-06   8.082e-07

Peak spectrum fit

Power-law model

Time interval is from    8.204 sec. to    9.204 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.35843     ( -0.558068   0.524517 )
Norm@50keV  : 1.01567E-02    ( -0.00298279   0.00296745 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.54 using 59 PHA bins.
# Reduced chi-squared =          1.062 for     57 degrees of freedom 
# Null hypothesis probability =   3.494930e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.22572 ( -0.390403  0.397278 ) ph/cm2/s
Energy fluence (15-150 keV)             : 9.90125e-08 ( -2.98731e-08  3.00976e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    8.204 sec. to    9.204 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 3.18313     (     )
Epeak [keV] : 326.852      (   )
Norm@50keV  : 9.14874E-04    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.12 using 59 PHA bins.
# Reduced chi-squared =          1.074 for     56 degrees of freedom 
# Null hypothesis probability =   3.288485e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.22678 ( -0.394555  0.3955 ) ph/cm2/s
Energy fluence (15-150 keV)             : 9.89389e-08 ( -3.05463e-08  3.00911e-08 ) ergs/cm2

Band function

Time interval is from    8.204 sec. to    9.204 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.637794   ( 0.842581   0.842581 )
beta        : -1.43113    ( 1.4218   0.614979 )
Epeak [keV] : 69.7126      ( -68.1926 648.186 )
Norm@50keV   : 2.73091E-02    ( -0.0290725   1.02532e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.47 using 59 PHA bins.
# Reduced chi-squared =          1.099 for     55 degrees of freedom 
# Null hypothesis probability =   2.849220e-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]    : 18.6410  (-7.20373  13.4696)
R^2/D10^2   : 6.59330E-02  (-0.0651311   0.298939)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          64.43 using 59 PHA bins.
# Reduced chi-squared =          1.130 for     57 degrees of freedom 
# Null hypothesis probability =   2.328795e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.534e-09   2.975e-09
25- 50  2.151e-08   1.304e-08
50-150  5.472e-08   3.556e-08
15-150  8.077e-08   5.180e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.363       (-115.113      -199.363)
Norm        : 5.19227       (-1.52606     1.52614)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.15 using 59 PHA bins.
# Reduced chi-squared =          1.073 for     57 degrees of freedom 
# Null hypothesis probability =   3.293512e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.293e-08   7.880e-09
25- 50  2.487e-08   1.496e-08
50-150  5.455e-08   3.267e-08
15-150  9.235e-08   5.470e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 8.75289        (-5.55049      7.8717)
R1^2/D10^2  : 0.639922        (-0.540608      17.1571)
kT2 [keV]   : 40.7048        (-40.7874      -44.366)
R2^2/D10^2  : 3.90266E-03    (-0.00319438   0.0507667)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.02 using 59 PHA bins.
# Reduced chi-squared =          1.091 for     55 degrees of freedom 
# Null hypothesis probability =   2.988491e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.023e-08   7.070e-09
25- 50  2.477e-08   1.489e-08
50-150  6.185e-08   3.762e-08
15-150  9.685e-08   5.195e-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: 1.30624     ( -0.254288   0.245172 )
Norm@50keV  : 3.16003E-03    ( -0.000415803   0.000413227 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.55 using 59 PHA bins.
# Reduced chi-squared =          1.062 for     57 degrees of freedom 
# Null hypothesis probability =   3.489874e-01
 
Photon flux (15-150 keV)    in 52.59 sec: 0.377434 ( -0.0550933  0.0555345 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.63972e-06 ( -2.19003e-07  2.19798e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.17212     (     )
Epeak [keV] : 63.7133      (   )
Norm@50keV  : 9.18811E-04    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.87 using 59 PHA bins.
# Reduced chi-squared =          1.069 for     56 degrees of freedom 
# Null hypothesis probability =   3.370438e-01
 
Photon flux (15-150 keV)    in 52.59 sec: 0.381405 ( -0.059527  0.052057 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.63917e-06 ( -2.18433e-07  2.12416e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.03587   ( 1.03588   1.03588 )
beta        : -1.30620    ( 1.30622   0.255018 )
Epeak [keV] : 42.5635      ( -42.5544 -42.5544 )
Norm@50keV   : 6.09942E-03    ( -0.00334845   0.479556 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.55 using 59 PHA bins.
# Reduced chi-squared =          1.101 for     55 degrees of freedom 
# Null hypothesis probability =   2.824734e-01
 
Photon flux (15-150 keV)    in 52.59 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)  = 3.66e-07
S(50-100 keV) = 5.92e-07

T90 vs. Hardness ratio plot

T90                                   = 48.0320000648499 sec.
Hardness ratio (energy fluence ratio) = 1.61749

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.39932
Count Ratio (50-100 keV) / (15-25 keV) = 1.24246

Mask shadow pattern

IMX = -1.039103341736319E+00, IMY = -3.213317189307310E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 16.384000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 16.384000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 16.384000

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:
-239.608000 -0.840000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9770 -15.6503    0.7  37.4 -100.8   8.3701  15.6    0.6	Sco X-1                       
254.5019  35.3677    2.2  46.4  -20.1   2.3577   5.3    2.6	Her X-1                       
256.0620 -37.7879    8.0  41.0 -139.2   0.5264   1.4    4.9	4U 1700-377                   
256.2874 -36.5046    5.5  39.9 -138.1  -0.7222  -2.1    8.7	GX 349+2                      
262.9731 -24.7435    1.8  27.3 -131.8   1.6844   6.4    2.0	GX 1+4                        
264.9519 -44.5922   17.0  43.2 -153.0  -0.2398  -0.7   12.4	4U 1735-44                    
268.4083  -1.4099    3.0  12.9  -69.5   0.7722   3.9    3.5	SW J1753.5-0127               
270.2870 -25.0634    2.7  23.7 -144.8   0.9035   4.3    1.0	GX 5-1                        
270.3622 -25.7898    3.1  24.3 -145.8   0.7790   3.8    4.3	GRS 1758-258                  
273.9395 -14.0026    2.9  12.4 -135.7   0.7416   4.0    4.4	GX 17+2                       
276.0548 -30.2307    4.5  26.9 -160.2   0.5563   2.6   10.6	H1820-303                     
284.9754 -24.8595    4.3  21.4 -179.5   0.5661   2.7    4.9	HT1900.1-2455                 
288.7942  10.9415    0.5  16.6   37.6   4.9533  23.1    0.3	GRS 1915+105                  
299.6065  35.1927    0.8  42.7   32.7   6.6648  15.1    1.0	Cyg X-1                       
262.8460 -33.8992   13.0  34.6 -142.6  -0.2245  -0.9    8.1	GX 354-0                      
314.0305 -43.3670    2.4  49.2  158.7   3.2621   4.9 ------	UNKNOWN                       
277.4410 -54.2648    3.6  50.6 -167.0   1.4865   3.2 ------	UNKNOWN                       
268.0519 -22.3357    0.5  22.4 -136.7   4.5234  21.9 ------	UNKNOWN

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

Time interval of the image:
-0.840000 51.752000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9728 -15.5200    7.8  37.4 -100.6   0.3071   1.5    7.2	Sco X-1                       
254.3820  35.3024    8.9  46.4  -20.2   0.2273   1.3    4.4	Her X-1                       
255.9370 -37.9758   21.5  41.2 -139.2   0.0809   0.5    8.2	4U 1700-377                   
256.3212 -36.5497    3.8  39.9 -138.2   0.4306   3.0    9.4	GX 349+2                      
262.9257 -24.7539    3.6  27.3 -131.7  -0.3187  -3.2    4.6	GX 1+4                        
264.7509 -44.4845  370.1  43.2 -152.7  -0.0047  -0.0    2.1	4U 1735-44                    
268.2174  -1.4579    4.8  13.1  -69.9   0.2019   2.4    9.0	SW J1753.5-0127               
270.4428 -25.0781    9.0  23.6 -145.1   0.1159   1.3    8.6	GX 5-1                        
270.4570 -25.7195    6.1  24.2 -145.9  -0.1709  -1.9    8.5	GRS 1758-258                  
273.8731 -14.1624   49.4  12.6 -135.8  -0.0186  -0.2   10.8	GX 17+2                       
276.0913 -30.4996   10.6  27.1 -160.3   0.0975   1.1   11.7	H1820-303                     
284.8921 -24.9802   11.3  21.5 -179.2   0.0836   1.0    8.6	HT1900.1-2455                 
288.9140  10.8133   84.2  16.5   38.2  -0.0124  -0.1   10.5	GRS 1915+105                  
299.5851  35.2816   11.3  42.7   32.6   0.1962   1.0    4.8	Cyg X-1                       
263.1316 -33.7305    6.5  34.3 -142.7   0.1915   1.8    9.5	GX 354-0                      
309.2525 -44.1774    1.1  47.4  162.8   2.3119  10.6 ------	UNKNOWN                       
304.4269 -48.0941    2.0  48.6  169.5   1.2366   5.7 ------	UNKNOWN                       
281.7239 -32.6978    2.0  28.9 -170.9   0.4902   5.7 ------	UNKNOWN                       
273.7324 -27.0091    2.3  24.3 -153.7   0.4050   4.9 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
134.692600 790.392600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
256.1101 -37.7655    9.1  39.9  -90.8   2.0286   1.3    7.5	4U 1700-377                   
256.2038 -36.4581    0.0  40.5  -88.9   0.0331   0.0   11.4	GX 349+2                      
263.0722 -24.6383    5.7  42.1  -69.0   3.4209   2.0    7.3	GX 1+4                        
264.8221 -44.4876   12.2  31.4  -97.5   0.5495   0.9    4.1	4U 1735-44                    
270.2760 -25.0966    2.4  36.8  -62.9   3.3948   4.8    1.1	GX 5-1                        
270.4512 -25.7989    5.8  36.3  -63.6   1.3906   2.0    8.7	GRS 1758-258                  
274.0915 -14.1676    9.2  42.3  -47.0   0.9979   1.3    9.3	GX 17+2                       
275.9619 -30.3830    4.0  29.6  -64.6   1.4073   2.9    2.1	H1820-303                     
285.1955 -24.9111   13.2  27.4  -44.4   0.3351   0.9    8.7	HT1900.1-2455                 
288.8070  10.9631    2.2  58.2  -14.8   9.7691   5.4    1.2	GRS 1915+105                  
263.0949 -33.9910  515.1  36.7  -81.1  -0.0198  -0.0   10.8	GX 354-0                      
336.3924  -4.3431    2.8  46.4   47.9   7.1733   4.1 ------	UNKNOWN                       
331.3216  -7.0601    3.3  41.8   43.0   3.2766   3.5 ------	UNKNOWN                       
 49.2903 -68.6957    3.6  52.9  162.4   5.7250   3.2 ------	UNKNOWN                       
123.3098 -77.1804    3.0  58.6 -172.5  10.1577   3.8 ------	UNKNOWN                       
268.0691 -22.3326    0.9  40.2  -61.8  11.4487  12.5 ------	UNKNOWN                       
253.8675 -38.8564    2.5  41.0  -93.5   7.2186   4.5 ------	UNKNOWN

Plot creation:
Sun May 31 02:38:20 EDT 2015