batgrbproduct analysis for trigger=292004

batgrbproduct Analysis for Trigger=292004

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 May 27 00:49:36 EDT 2015
             Host Name: bat1
   Current Working Dir: /local/data/bat1/alien/Swift_3rdBATcatalog/event/batevent_reproc/trigger292004
======================================================================

  Trigger: 00292004      Segment: 000

  BAT Trigger Time: 212267725.932   [s; MET]
      Trigger Stop: 212267725.964   [s; MET]
               UTC: 2007-09-23T19:15:23.687760    [includes UTCF correction] 
       Where From?: (*SHORT BURST*) TDRSS scaled map message

  BAT 
    RA: 184.626373075231   Dec: -38.2677479658261  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    9.29
     Image Trigger?:     NO
     Rate S/N Ratio:     45.9673797382448  [ if not an image trigger ]
     Image S/N Ratio:    9.29

  Flight Position:   [ source = BAT ]
    RA: 184.626373075231   Dec: -38.2677479658261  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 184.641151554106   Dec: -38.2812519038051  [deg; J2000]  
        { 12h 18m 33.9s , -38d 16' 52.5" }
         +/- 1.89578307350786 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.795585009024764 [arcmin] (formal 1-sigma fit error)
    SNR: 12.1976864063386
 
  Angular difference between Flight and Ground position is 1.068202 arcmin
 
  Partial Coding Fraction: 0.765625    [ including projection effects ]

  Duration
     T90: 0.0399999916553497 +/- 0.00894429003608426
        Measured from: -0.00400000810623169
                   to: 0.035999983549118     [s; relative to TRIGTIME]
     T50: 0.0200000107288361 +/- 0.00565686571343518
        Measured from: 0.0039999783039093
                   to: 0.0239999890327454     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: -0.480000019073486     
                   to: 0.519999980926514     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -0.00400000810623169     
                   to: 0.0399999916553497     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.008743   0.013901   0.022007   0.011381
           0.001865   0.002368   0.002808   0.002375 [error]
 Peak      0.017267   0.015897   0.030256   0.011187
           0.006284   0.006544   0.006151   0.005599 [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 2.05e-09 6.00e-09 1.43e-08 9.32e-08 3.86e-08 1.16e-07   erg/cm2
              Error 6.49e-10 1.11e-09 2.38e-09 3.78e-08 6.62e-09 3.89e-08   erg/cm2
Peak flux Power-law 1.16e-01 1.61e-01 1.65e-01 3.10e-01 5.40e-01 7.51e-01   ph/cm2/s
              Error 7.23e-02 5.87e-02 4.93e-02 2.31e-01 1.51e-01 2.39e-01   ph/cm2/s
 
Fluence   Cutoff-PL 2.08e-09 6.04e-09 1.42e-08 9.08e-08 3.84e-08 1.13e-07   erg/cm2
              Error 6.78e-10 1.11e-09 2.55e-09 5.11e-08 8.22e-09 4.96e-08   erg/cm2
Peak flux Cutoff-PL 1.20e-01 1.63e-01 1.64e-01 2.97e-01 5.42e-01 7.46e-01   ph/cm2/s
              Error 7.71e-02 5.89e-02 5.14e-02 2.99e-01 -------- 5.03e-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    0.750    0.275    -      -           7.34e-02 1.11e-02   53.550 57
CPL   0.743    0.591    10000.0    0.0      7.39e-02 0.00e+00   53.570 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    0.962    0.566    -      -           4.70e-03 1.30e-03   65.750 57
CPL   0.967    0.571    9999.3    0.0      4.73e-03 8.93e-03   65.760 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: 0.064000 sec.
T50 in the 50-300 keV band: 0.064000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100    0.044   -0.004    0.040
T90     0.040   -0.004    0.036
T50     0.020    0.004    0.024
Peak    1.000   -0.480    0.520

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
  184.6412   -38.2813   0.0158    20.1521   -92.3035         0.0561092     12.198 TRIG_00292004                 
 
Foreground time interval of the image:
 -0.004   0.040 (delta_t =   0.044 [sec])
Background time interval of the image:
-239.932  -0.004 (delta_t = 239.928 [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 0.032000

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 0.032000

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 0.032000

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   -0.004 sec. to    0.040 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.750084     ( -0.28065   0.26986 )
Norm@50keV  : 7.33989E-02    ( -0.0111179   0.0110269 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.55 using 59 PHA bins.
# Reduced chi-squared =         0.9395 for     57 degrees of freedom 
# Null hypothesis probability =   6.052387e-01
 
Photon flux (15-150 keV)    in 0.044 sec: 8.45539 ( -1.2537  1.25432 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.85552e-08 ( -6.59098e-09  6.64796e-09 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.004 sec. to    0.040 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.742575     ( -0.835962   0.346429 )
Epeak [keV] : 1.00000E+04      (   )
Norm@50keV  : 7.39459E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.57 using 59 PHA bins.
# Reduced chi-squared =         0.9565 for     56 degrees of freedom 
# Null hypothesis probability =   5.675645e-01
 
Photon flux (15-150 keV)    in 0.044 sec: 8.45450 ( -1.25244  1.25279 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.83841e-08 ( -6.41898e-09  1.00203e-08 ) ergs/cm2

Band function

Time interval is from   -0.004 sec. to    0.040 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.912139   ( 0.912139   0.912139 )
beta        : -0.750088    ( -0.269856   0.280647 )
Epeak [keV] : 15.5788      ( -15.5788 -15.5788 )
Norm@50keV   : 0.103432    ( -0.0409428   0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.55 using 59 PHA bins.
# Reduced chi-squared =         0.9737 for     55 degrees of freedom 
# Null hypothesis probability =   5.301264e-01
 
Photon flux (15-150 keV)    in 0.044 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]    : 26.7624  (-5.24303  7.53015)
R^2/D10^2   : 0.178954  (-0.0891929   0.15602)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.63 using 59 PHA bins.
# Reduced chi-squared =          1.081 for     57 degrees of freedom 
# Null hypothesis probability =   3.141652e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  9.438e-10   3.069e-10
25- 50  5.537e-09   1.432e-09
50-150  2.903e-08   8.292e-09
15-150  3.551e-08   9.255e-09

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (      )
Norm        : 30.4999       (-4.92943     4.92943)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          75.30 using 59 PHA bins.
# Reduced chi-squared =          1.321 for     57 degrees of freedom 
# Null hypothesis probability =   5.262808e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.322e-09   1.888e-09
25- 50  6.390e-09   3.650e-09
50-150  1.401e-08   8.089e-09
15-150  2.373e-08   1.349e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 4.09406        (-2.18843      4.71705)
R1^2/D10^2  : 39.0447        (-36.9062      3274.26)
kT2 [keV]   : 32.5088        (-7.72654      17.4883)
R2^2/D10^2  : 9.79164E-02    (-0.0674698   0.081746)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.70 using 59 PHA bins.
# Reduced chi-squared =         0.9582 for     55 degrees of freedom 
# Null hypothesis probability =   5.628885e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.424e-09   1.206e-09
25- 50  4.984e-09   1.822e-09
50-150  3.106e-08   1.254e-08
15-150  3.847e-08   1.410e-08

Peak spectrum fit

Power-law model

Time interval is from   -0.480 sec. to    0.520 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.961571     ( -0.592194   0.540749 )
Norm@50keV  : 4.69875E-03    ( -0.00132249   0.00128231 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          65.75 using 59 PHA bins.
# Reduced chi-squared =          1.154 for     57 degrees of freedom 
# Null hypothesis probability =   1.996795e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.540026 ( -0.150358  0.151303 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.1529e-08 ( -1.53769e-08  1.5605e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.480 sec. to    0.520 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.966704     ( -0.608093   0.534241 )
Epeak [keV] : 9999.33      ( -9999.36 -9999.36 )
Norm@50keV  : 4.73252E-03    ( -0.00128727   0.0165685 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          65.76 using 59 PHA bins.
# Reduced chi-squared =          1.174 for     56 degrees of freedom 
# Null hypothesis probability =   1.747238e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.542066 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.15345e-08 ( -1.53615e-08  1.54012e-08 ) ergs/cm2

Band function

Time interval is from   -0.480 sec. to    0.520 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.861971   ( 0.861866   0.861866 )
beta        : -0.961526    ( 0.9615   0.592231 )
Epeak [keV] : 23.5354      ( -23.6769 -23.6769 )
Norm@50keV   : 7.13071E-03    ( -0.00368878   0.094068 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          65.75 using 59 PHA bins.
# Reduced chi-squared =          1.195 for     55 degrees of freedom 
# Null hypothesis probability =   1.520662e-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]    : 26.4611  (-8.65556  18.3268)
R^2/D10^2   : 1.08470E-02  (-0.0108458   0.0254178)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          69.02 using 59 PHA bins.
# Reduced chi-squared =          1.211 for     57 degrees of freedom 
# Null hypothesis probability =   1.320745e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.279e-09   8.125e-10
25- 50  7.463e-09   4.476e-09
50-150  3.835e-08   2.381e-08
15-150  4.710e-08   2.845e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (      )
Norm        : 2.19548       (-0.619814     0.619788)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          69.52 using 59 PHA bins.
# Reduced chi-squared =          1.220 for     57 degrees of freedom 
# Null hypothesis probability =   1.234298e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.469e-09   3.324e-09
25- 50  1.052e-08   6.445e-09
50-150  2.307e-08   1.422e-08
15-150  3.907e-08   2.327e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 4.13060        (-2.76543      4.81825)
R1^2/D10^2  : 4.07109        (-3.93466      6967.59)
kT2 [keV]   : 33.4045        (-12.2744      49.5616)
R2^2/D10^2  : 5.21124E-03    (-0.00459152   0.00805416)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.96 using 59 PHA bins.
# Reduced chi-squared =          1.163 for     55 degrees of freedom 
# Null hypothesis probability =   1.908111e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.166e-09   3.054e-09
25- 50  7.169e-09   3.788e-09
50-150  4.099e-08   2.503e-08
15-150  5.333e-08   2.897e-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: 0.750084     ( -0.28065   0.26986 )
Norm@50keV  : 7.33989E-02    ( -0.0111179   0.0110269 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.55 using 59 PHA bins.
# Reduced chi-squared =         0.9395 for     57 degrees of freedom 
# Null hypothesis probability =   6.052387e-01
 
Photon flux (15-150 keV)    in 0.044 sec: 8.45539 ( -1.2537  1.25432 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.85552e-08 ( -6.59098e-09  6.64796e-09 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.742575     ( -0.835962   0.346429 )
Epeak [keV] : 1.00000E+04      (   )
Norm@50keV  : 7.39459E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.57 using 59 PHA bins.
# Reduced chi-squared =         0.9565 for     56 degrees of freedom 
# Null hypothesis probability =   5.675645e-01
 
Photon flux (15-150 keV)    in 0.044 sec: 8.45450 ( -1.25244  1.25279 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.83841e-08 ( -6.41898e-09  1.00203e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.912139   ( 0.912139   0.912139 )
beta        : -0.750088    ( -0.269856   0.280647 )
Epeak [keV] : 15.5788      ( -15.5788 -15.5788 )
Norm@50keV   : 0.103432    ( -0.0409428   0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.55 using 59 PHA bins.
# Reduced chi-squared =         0.9737 for     55 degrees of freedom 
# Null hypothesis probability =   5.301264e-01
 
Photon flux (15-150 keV)    in 0.044 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)  = 6.00e-09
S(50-100 keV) = 1.43e-08

T90 vs. Hardness ratio plot

T90                                   = 0.0399999916553497 sec.
Hardness ratio (energy fluence ratio) = 2.38333

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.58996
Count Ratio (50-100 keV) / (15-25 keV) = 2.5171

Mask shadow pattern

IMX = -1.474964381518899E-02, IMY = 3.666820475980682E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.032000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.032000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.032000

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:
-239.932000 -0.004000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.5232 -40.5447    1.0  42.6 -156.4   2.2928  11.4    0.6	Vela X-1                      
169.9843 -60.4931    0.0  15.1 -178.0   0.1359   1.1   12.5	Cen X-3                       
186.3947 -62.7432    3.9   8.6  157.0   0.3225   3.0    7.4	GX 301-2                      
244.9706 -15.6419    1.1  54.0   -0.1   4.8682  10.1    0.5	Sco X-1                       
255.9559 -37.7911   11.6  42.1   28.5   0.2586   1.0    3.5	4U 1700-377                   
256.3895 -36.4185   12.3  43.3   27.4  -0.2852  -0.9    2.2	GX 349+2                      
264.5875 -44.3241    9.5  42.4   42.2   0.4246   1.2   10.1	4U 1735-44                    
262.9772 -33.8859    7.5  48.8   30.6   0.9205   1.5    3.1	GX 354-0                      
324.3382 -85.7918    2.5  36.2  113.5   1.2767   4.6 ------	UNKNOWN                       
258.3404 -35.7700    3.4  44.9   28.4   1.0500   3.4 ------	UNKNOWN

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

Time interval of the image:
-0.004000 0.040000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.5366 -40.4354    7.8  42.7 -156.2   0.0096   1.5    7.2	Vela X-1                      
170.4052 -60.7639 1013.0  14.9 -179.1   0.0000   0.0    8.9	Cen X-3                       
186.4171 -62.6512   18.5   8.5  157.5  -0.0024  -0.6    9.7	GX 301-2                      
245.0241 -15.6529   13.5  54.0   -0.1   0.0138   0.9    2.7	Sco X-1                       
255.9493 -37.8368    2.9  42.1   28.5   0.0324   4.0    1.8	4U 1700-377                   
256.5099 -36.4057    4.9  43.4   27.5   0.0210   2.3    3.7	GX 349+2                      
264.7434 -44.4847   12.6  42.3   42.5   0.0091   0.9    2.1	4U 1735-44                    
263.0294 -33.8957    4.7  48.9   30.6   0.0364   2.4    4.2	GX 354-0                      
113.2122 -61.3184    2.1  41.0  166.1   0.0360   5.4 ------	UNKNOWN                       
244.0632 -11.8923    2.5  56.8   -3.3   0.1028   4.6 ------	UNKNOWN                       
184.6412 -38.2812    0.9  20.2  -92.3   0.0561  12.2 ------	UNKNOWN                       
214.9528  -5.3493    2.7  52.8  -39.3   0.0855   4.3 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:

Plot creation:
Sun May 31 09:13:07 EDT 2015