batgrbproduct analysis for trigger=158855

batgrbproduct Analysis for Trigger=158855

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 19:54:41 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger158855
======================================================================

  Trigger: 00158855      Segment: 000

  BAT Trigger Time: 150482001.088   [s; MET]
      Trigger Stop: 150482002.112   [s; MET]
               UTC: 2005-10-08T16:33:21.316200    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 202.870241770763   Dec: 42.0905012677457  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    9.65
     Image Trigger?:     NO
     Rate S/N Ratio:     17.1464281994822  [ if not an image trigger ]
     Image S/N Ratio:    9.65

  Flight Position:   [ source = BAT ]
    RA: 202.870241770763   Dec: 42.0905012677457  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 202.865621510716   Dec: 42.0997094923151  [deg; J2000]  
        { 13h 31m 27.7s , +42d 05' 59.0" }
         +/- 0.722108342293613 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.212847548333887 [arcmin] (formal 1-sigma fit error)
    SNR: 48.4300597979343
 
  Angular difference between Flight and Ground position is 0.589545 arcmin
 
  Partial Coding Fraction: 0.375    [ including projection effects ]

  Duration
     T90: 12.4079999923706 +/- 1.35531546723488
        Measured from: -1.52399998903275
                   to: 10.8840000033379     [s; relative to TRIGTIME]
     T50: 4.75599998235703 +/- 0.395251826248921
        Measured from: 2.27200001478195
                   to: 7.02799999713898     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 2.87999999523163     
                   to: 3.87999999523163     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -24.9320000112057     
                   to: 13.3319999873638     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     1.144757   2.185086   2.502211   0.886195
           0.062574   0.059771   0.055731   0.046049 [error]
 Peak      0.119897   0.201092   0.245730   0.091403
           0.011762   0.012560   0.012948   0.010832 [error]

     [ fluence units of on-axis counts / fully illuminated detector ] 

======================================================================
 
=== Fluence/Peak Flux Summary ===
 
              Model    Band1    Band2    Band3    Band4    Band5    Total      
                       15-25    25-50   50-100  100-350   15-150   15-350   keV
Fluence   Power-law 4.42e-07 1.03e-06 1.89e-06 8.36e-06 5.14e-06 1.17e-05   erg/cm2
              Error 2.80e-08 3.86e-08 5.57e-08 5.81e-07 1.46e-07 5.96e-07   erg/cm2
Peak flux Power-law 1.26e+00 1.66e+00 1.61e+00 2.79e+00 5.46e+00 7.33e+00   ph/cm2/s
              Error 1.63e-01 1.30e-01 1.03e-01 3.94e-01 3.44e-01 4.67e-01   ph/cm2/s
 
Fluence   Cutoff-PL 3.93e-07 1.03e-06 1.98e-06 5.63e-06 5.08e-06 9.03e-06   erg/cm2
              Error 3.76e-08 4.04e-08 7.20e-08 1.23e-06 1.51e-07 1.22e-06   erg/cm2
Peak flux Cutoff-PL 1.19e+00 1.67e+00 1.65e+00 2.33e+00 5.41e+00 6.85e+00   ph/cm2/s
              Error 1.57e-01 1.34e-01 1.31e-01 6.92e-01 3.57e-01 6.23e-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    1.117    0.051    -      -           1.29e-02 3.78e-04   61.450 57
CPL   0.749    0.215     212.1  120.3      1.82e-02 3.56e-03   52.170 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.045    0.108    -      -           4.73e-02 2.88e-03   60.490 57
CPL   0.850    0.334     358.9    0.0      5.71e-02 1.97e-02   59.770 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: 16.448000 sec.
T50 in the 50-300 keV band: 5.312000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   38.264  -24.932   13.332
T90    12.408   -1.524   10.884
T50     4.756    2.272    7.028
Peak    1.000    2.880    3.880

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
  202.8656    42.0997   0.0040    44.0309   -28.6781         6.9821156     48.430 TRIG_00158855                 
 
Foreground time interval of the image:
-24.932  13.332 (delta_t =  38.264 [sec])
Background time interval of the image:
-299.088 -24.932 (delta_t = 274.156 [sec])

Lightcurves

Notes:

1) The mask-weighted light curves are using the flight position.
2) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
3) For all the mask-weighted lightcurves, the y-axis units are counts/sec/det where a det is 0.4 x 0.4 = 0.16 sq cm.
4) The verticle lines correspond to following: green dotted lines are T50 interval, black dotted lines are T90 interval, blue solid line(s) is a spacecraft slew start time, and orange solid line(s) is a spacecraft slew end time.
5) Time of each bin is in the middle of the bin.

1 s binning

From T0-310 s to T0+310 s

From T100_start - 20 s to T100_end + 30 s

Full time interval

64 ms binning

Full time interval

From T100_start to T100_end

From T0-5 sec to T0+5 sec

16 ms binning

From T100_start-5 s to T100_start+5 s

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

8 ms binning

From T100_start-3 s to T100_start+3 s

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

2 ms binning

From T100_start-1 s to T100_start+1 s

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

SN=5 or 10 sec. binning (whichever binning is satisfied first)

SN=5 or 10 sec. binning (T < 200 sec)

Quad-rate summed light curves (from T0-300s to T0+1000s)

Spectral Evolution

Spectra

Notes:

1) The fitting includes the systematic errors.
2) When the burst includes telescope slew time periods, the fitting uses an average response file made from multiple 5-s response files through out the slew time plus single time preiod for the non-slew times, and weighted by the total counts in the corresponding time period using addrmf. An average response file is needed becuase a spectral fit using the pre-slew DRM will introduce some errors in both a spectral shape and a normalization if the PHA file contains a lot of the slew/post-slew time interval.
3) For fits to more complicated models (e.g. a power-law over a cutoff power-law), the BAT team has decided to require a chi-square improvement of more than 6 for each extra dof.

Time averaged spectrum fit using the average DRM

Power-law model

Time interval is from  -24.932 sec. to   13.332 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.11750     ( -0.0514033   0.0509945 )
Norm@50keV  : 1.29197E-02    ( -0.000378374   0.000377305 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.45 using 59 PHA bins.
# Reduced chi-squared =          1.078 for     57 degrees of freedom 
# Null hypothesis probability =   3.196470e-01
 
Photon flux (15-150 keV)    in 38.26 sec: 1.50124 ( -0.0470437  0.0472011 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.13962e-06 ( -1.45976e-07  1.46034e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from  -24.932 sec. to   13.332 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.748953     ( -0.220239   0.209759 )
Epeak [keV] : 212.094      ( -55.7589 184.77 )
Norm@50keV  : 1.81892E-02    ( -0.00314466   0.0039716 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.17 using 59 PHA bins.
# Reduced chi-squared =         0.9315 for     56 degrees of freedom 
# Null hypothesis probability =   6.207718e-01
 
Photon flux (15-150 keV)    in 38.26 sec: 1.46637 ( -0.05033  0.05059 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.08185e-06 ( -1.51471e-07  1.51127e-07 ) ergs/cm2

Band function

Time interval is from  -24.932 sec. to   13.332 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.749058   ( -0.22646   0.194107 )
beta        : -10.0000    ( 10   1.77636e-15 )
Epeak [keV] : 212.115      ( -55.8291 184.651 )
Norm@50keV   : 1.81863E-02    ( -0.00314295   0.00397464 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.17 using 59 PHA bins.
# Reduced chi-squared =         0.9485 for     55 degrees of freedom 
# Null hypothesis probability =   5.836019e-01
 
Photon flux (15-150 keV)    in 38.26 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]    : 23.0118  (  )
R^2/D10^2   : 4.47376E-02  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         219.15 using 59 PHA bins.
# Reduced chi-squared =         3.8447 for     57 degrees of freedom 
# Null hypothesis probability =   7.412840e-21
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.642e-07   9.508e-09
25- 50  8.912e-07   3.749e-08
50-150  3.525e-06   1.429e-07
15-150  4.581e-06   1.435e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.363       (      )
Norm        : 6.58207       (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         288.81 using 59 PHA bins.
# Reduced chi-squared =         5.0669 for     57 degrees of freedom 
# Null hypothesis probability =   1.014095e-32
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.271e-07   1.970e-08
25- 50  1.206e-06   3.730e-08
50-150  2.646e-06   8.322e-08
15-150  4.479e-06   1.473e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 7.95842        (-0.970686      1.09661)
R1^2/D10^2  : 0.695723        (-0.239657      0.395922)
kT2 [keV]   : 31.8208        (-2.41418      3.10606)
R2^2/D10^2  : 1.38491E-02    (-0.00372449   0.00427941)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.99 using 59 PHA bins.
# Reduced chi-squared =         0.8180 for     55 degrees of freedom 
# Null hypothesis probability =   8.301718e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.846e-07   5.299e-08
25- 50  1.037e-06   8.207e-08
50-150  3.698e-06   2.242e-07
15-150  5.120e-06   3.023e-07

Peak spectrum fit

Power-law model

Time interval is from    2.880 sec. to    3.880 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.04472     ( -0.108227   0.10689 )
Norm@50keV  : 4.72949E-02    ( -0.00288214   0.00287359 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.49 using 59 PHA bins.
# Reduced chi-squared =          1.061 for     57 degrees of freedom 
# Null hypothesis probability =   3.510616e-01
 
Photon flux (15-150 keV)    in 1 sec: 5.46027 ( -0.343314  0.344259 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.0356e-07 ( -3.20887e-08  3.2159e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    2.880 sec. to    3.880 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.849989     ( -0.423304   0.244452 )
Epeak [keV] : 358.864      ( -358.862 -358.862 )
Norm@50keV  : 5.71162E-02    ( -0.0119632   0.0274724 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.77 using 59 PHA bins.
# Reduced chi-squared =          1.067 for     56 degrees of freedom 
# Null hypothesis probability =   3.405402e-01
 
Photon flux (15-150 keV)    in 1 sec: 5.40964 ( -0.3569  0.35798 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.0083e-07 ( -3.299e-08  3.2857e-08 ) ergs/cm2

Band function

Time interval is from    2.880 sec. to    3.880 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.862948   ( 0.154374   0.154374 )
beta        : -8.98260    ( 8.39239   18.3924 )
Epeak [keV] : 381.528      ( -226.015 -381.528 )
Norm@50keV   : 5.63719E-02    ( -0.00334662   0.0237605 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.77 using 59 PHA bins.
# Reduced chi-squared =          1.087 for     55 degrees of freedom 
# Null hypothesis probability =   3.065958e-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]    : 23.6383  (-1.93047  2.16276)
R^2/D10^2   : 0.153946  (-0.0366628   0.0472233)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         107.97 using 59 PHA bins.
# Reduced chi-squared =         1.8942 for     57 degrees of freedom 
# Null hypothesis probability =   5.346328e-05
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.538e-08   1.880e-09
25- 50  8.472e-08   8.690e-09
50-150  3.531e-07   3.020e-08
15-150  4.532e-07   3.530e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.359       (      )
Norm        : 22.8095       (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         124.29 using 59 PHA bins.
# Reduced chi-squared =         2.1805 for     57 degrees of freedom 
# Null hypothesis probability =   6.547005e-07
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.680e-08   3.975e-09
25- 50  1.093e-07   9.045e-09
50-150  2.396e-07   5.955e-08
15-150  4.057e-07   5.825e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 7.37741        (-1.44618      1.75933)
R1^2/D10^2  : 3.38586        (-1.73855      4.04931)
kT2 [keV]   : 33.6201        (-4.57487      6.84441)
R2^2/D10^2  : 4.57568E-02    (-0.0199135   0.0272512)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.23 using 59 PHA bins.
# Reduced chi-squared =         0.9860 for     55 degrees of freedom 
# Null hypothesis probability =   5.039126e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.868e-08   1.210e-08
25- 50  9.564e-08   2.198e-08
50-150  3.765e-07   8.890e-08
15-150  5.108e-07   8.730e-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: 1.11750     ( -0.0514033   0.0509945 )
Norm@50keV  : 1.29197E-02    ( -0.000378374   0.000377305 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.45 using 59 PHA bins.
# Reduced chi-squared =          1.078 for     57 degrees of freedom 
# Null hypothesis probability =   3.196470e-01
 
Photon flux (15-150 keV)    in 38.26 sec: 1.50124 ( -0.0470437  0.0472011 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.13962e-06 ( -1.45976e-07  1.46034e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.748953     ( -0.220239   0.209759 )
Epeak [keV] : 212.094      ( -55.7589 184.77 )
Norm@50keV  : 1.81892E-02    ( -0.00314466   0.0039716 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.17 using 59 PHA bins.
# Reduced chi-squared =         0.9315 for     56 degrees of freedom 
# Null hypothesis probability =   6.207718e-01
 
Photon flux (15-150 keV)    in 38.26 sec: 1.46637 ( -0.05033  0.05059 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.08185e-06 ( -1.51471e-07  1.51127e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.749058   ( -0.22646   0.194107 )
beta        : -10.0000    ( 10   3.55271e-15 )
Epeak [keV] : 212.115      ( -55.8291 184.651 )
Norm@50keV   : 1.81863E-02    ( -0.00314295   0.00397464 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.17 using 59 PHA bins.
# Reduced chi-squared =         0.9485 for     55 degrees of freedom 
# Null hypothesis probability =   5.836019e-01
 
Photon flux (15-150 keV)    in 38.26 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)  = 1.03e-06
S(50-100 keV) = 1.89e-06

T90 vs. Hardness ratio plot

T90                                   = 12.4079999923706 sec.
Hardness ratio (energy fluence ratio) = 1.83495

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.90878
Count Ratio (50-100 keV) / (15-25 keV) = 2.1858

Mask shadow pattern

IMX = 8.481412304303927E-01, IMY = 4.639230038776114E-01

TIME vs. PHA plot around the trigger time

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

TIME vs. DetID plot around the trigger time

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

100 us light curve (15-350 keV)

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

Spacecraft aspect plot

Bright source in the pre-burst/pre-slew/post-slew images

Pre-burst image of 15-350 keV band

Time interval of the image:
-299.088000 -24.932000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9802 -15.6392    0.1  27.5  177.5  25.1842  90.5    0.1	Sco X-1                       
254.4615  35.3184    3.2  27.9   38.1   1.1619   3.7    1.5	Her X-1                       
255.9042 -38.0112   12.1  51.7  173.2   0.7525   1.0   10.8	4U 1700-377                   
256.3464 -36.5752   66.0  50.5  172.1   0.1349   0.2   10.1	GX 349+2                      
263.1369 -24.7344    7.9  43.0  157.1   0.8986   1.5    7.0	GX 1+4                        
268.3958  -1.4438    7.2  31.9  121.8   0.7235   1.6    1.7	SW J1753.5-0127               
270.4191 -25.1791    0.0  47.6  150.4  -1.3832  -1.5    9.5	GX 5-1                        
270.2909 -25.8999    5.1  48.1  151.2  -2.0530  -2.2    9.4	GRS 1758-258                  
273.9245 -14.1036    4.6  43.0  135.5   2.2969   2.5    6.2	GX 17+2                       
263.1154 -33.8635    6.0  50.6  164.1  -1.7314  -1.9    6.5	GX 354-0                      
279.6357  18.4385    2.5  39.9   84.9   5.0200   4.7 ------	UNKNOWN                       
276.7239  47.6749    2.1  48.3   43.8   6.2973   5.4 ------	UNKNOWN                       
221.8263  63.6156    2.6  53.8    0.9   3.7604   4.4 ------	UNKNOWN                       
212.4550 -36.6079    3.6  53.9 -143.5   4.9684   3.2 ------	UNKNOWN                       
211.9246 -36.5224    4.2  54.1 -143.0   4.2603   2.8 ------	UNKNOWN

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

Time interval of the image:
-24.932000 13.332000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9546 -15.6544    1.1  27.5  177.6  -0.8737 -10.9    1.7	Sco X-1                       
254.5245  35.4865    8.1  28.1   38.0   0.1344   1.4    9.2	Her X-1                       
255.9854 -37.8458   28.4  51.6  173.0  -0.0908  -0.4    0.1	4U 1700-377                   
256.4372 -36.4246    7.7  50.4  171.9   0.3009   1.5    0.1	GX 349+2                      
263.1358 -24.7962   42.2  43.1  157.2   0.0415   0.3    7.5	GX 1+4                        
268.4735  -1.5144   21.1  32.0  121.8   0.0673   0.5    7.3	SW J1753.5-0127               
270.1491 -24.9791    0.0  47.3  150.5  -0.5339  -2.5    9.5	GX 5-1                        
270.4245 -25.6858   10.8  48.0  150.9   0.2441   1.1    7.4	GRS 1758-258                  
274.1416 -14.0478    7.9  43.1  135.3   0.3212   1.5    7.9	GX 17+2                       
263.0939 -33.7222    4.9  50.5  164.0  -0.5100  -2.3    8.5	GX 354-0                      
202.8656  42.0997    0.2  44.0  -28.7   6.9816  48.4 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:

Plot creation:
Sun May 31 15:24:51 EDT 2015