batgrbproduct analysis for trigger=191512

batgrbproduct Analysis for Trigger=191512

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 18:19:56 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger191512
======================================================================

  Trigger: 00191512      Segment: 000

  BAT Trigger Time: 162082086.144   [s; MET]
      Trigger Stop: 162082094.336   [s; MET]
               UTC: 2006-02-19T22:48:05.118160    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 241.806599596401   Dec: 32.3303789915981  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    7.2
     Image Trigger?:     NO
     Rate S/N Ratio:     8.24621125123532  [ if not an image trigger ]
     Image S/N Ratio:    7.2

  Flight Position:   [ source = BAT ]
    RA: 241.806599596401   Dec: 32.3303789915981  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 241.856308172933   Dec: 32.3078305910385  [deg; J2000]  
        { 16h 07m 25.5s , +32d 18' 28.2" }
         +/- 2.18678724966408 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.937476985655385 [arcmin] (formal 1-sigma fit error)
    SNR: 9.94673335124456
 
  Angular difference between Flight and Ground position is 2.860619 arcmin
 
  Partial Coding Fraction: 0.6796875    [ including projection effects ]

  Duration
     T90: 62.0439999997616 +/- 6.24681712150771
        Measured from: -55.0879999995232
                   to: 6.95600000023842     [s; relative to TRIGTIME]
     T50: 43.9560000002384 +/- 22.9842952657015
        Measured from: -40.6759999990463
                   to: 3.28000000119209     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 4.06000000238419     
                   to: 5.06000000238419     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -57.0679999887943     
                   to: 8.24000000953674     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.414854   0.413649   0.071703  -0.003578
           0.054226   0.048393   0.040634   0.034142 [error]
 Peak      0.031008   0.023438   0.005254   0.004351
           0.006982   0.006262   0.005036   0.004174 [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 1.48e-07 1.46e-07 1.01e-07 1.11e-07 4.40e-07 5.07e-07   erg/cm2
              Error 2.76e-08 2.45e-08 3.34e-08 6.87e-08 7.96e-08 1.18e-07   erg/cm2
Peak flux Power-law 3.38e-01 1.55e-01 4.27e-02 1.47e-02 5.44e-01 5.50e-01   ph/cm2/s
              Error 1.22e-01 6.23e-02 3.57e-02 2.50e-02 1.63e-01 1.66e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.36e-07 1.71e-07 8.05e-08 1.10e-08 3.97e-07 3.98e-07   erg/cm2
              Error 3.16e-08 3.40e-08 4.09e-08 4.59e-08 7.73e-08 9.09e-08   erg/cm2
Peak flux Cutoff-PL 3.38e-01 1.55e-01 4.26e-02 1.46e-02 5.43e-01 5.49e-01   ph/cm2/s
              Error -------- -------- -------- -------- -------- --------   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    2.529    0.322    -      -           6.69e-04 1.62e-04   64.300 57
CPL   0.970    1.409      24.1    0.0      6.24e-03 0.00e+00   60.970 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    2.857    0.890    -      -           2.19e-03 1.41e-03   49.120 57
CPL   1.876    0.000       4.4    0.0      9.24e-03 0.00e+00   49.470 56
 
Model      : spectral model: simple power-law (PL) and cutoff power-law (CPL)
Ph_index   : photon index: E^-{Ph_index} (minus sign is not included in the index)
Ph_90err   : 90% error of the photon index
Epeak      : Epeak in keV
Epeak_90err: 90% error of Epeak
Norm       : normalization at 50 keV in PL model and at 1 keV in CPL model
Nomr_90err : 90% error of the normalization
chi2       : Chi-Squared
dof        : degree of freedom

 
=== T90/T50 calculation in the 50-300 keV band (BATSE band) using 64 ms lc ===
 
T90 in the 50-300 keV band: 0.000000 sec.
T50 in the 50-300 keV band: 0.000000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   65.308  -57.068    8.240
T90    62.044  -55.088    6.956
T50    43.956  -40.676    3.280
Peak    1.000    4.060    5.060

Click here for the BAT GCN circular template

Image

Pre-slew 15.0-350.0 keV image (Event data)

#   RAcent    DECcent   POSerr    Theta     Phi              Peak Cts       SNR   Name
  241.8563    32.3078   0.0193    32.5885   167.5201         1.0165707      9.947 TRIG_00191512                 
 
Foreground time interval of the image:
-57.068   8.240 (delta_t =  65.308 [sec])
Background time interval of the image:
-299.144 -57.068 (delta_t = 242.076 [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 8.192000

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 8.192000

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 8.192000

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  -57.068 sec. to    8.240 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.52916     ( -0.302367   0.342262 )
Norm@50keV  : 6.68679E-04    ( -0.000162841   0.000161379 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          64.30 using 59 PHA bins.
# Reduced chi-squared =          1.128 for     57 degrees of freedom 
# Null hypothesis probability =   2.361666e-01
 
Photon flux (15-150 keV)    in 65.31 sec: 0.133741 ( -0.0199207  0.0199227 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.40205e-07 ( -7.79338e-08  8.1211e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from  -57.068 sec. to    8.240 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.969678     ( -1.78599   1.03206 )
Epeak [keV] : 24.1353      (   )
Norm@50keV  : 6.24248E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.97 using 59 PHA bins.
# Reduced chi-squared =          1.089 for     56 degrees of freedom 
# Null hypothesis probability =   3.018696e-01
 
Photon flux (15-150 keV)    in 65.31 sec: 0.128297 ( -0.020261  0.020368 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.97114e-07 ( -7.1374e-08  8.32487e-08 ) ergs/cm2

Band function

Time interval is from  -57.068 sec. to    8.240 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.06116   ( -0.896144   1.04081 )
beta        : -9.37167    ( 9.37167   19.3716 )
Epeak [keV] : 23.6509      ( -11.5343 10.3949 )
Norm@50keV   : 5.40548E-03    ( -0.00541345   0.0571076 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.98 using 59 PHA bins.
# Reduced chi-squared =          1.109 for     55 degrees of freedom 
# Null hypothesis probability =   2.695732e-01
 
Photon flux (15-150 keV)    in 65.31 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]    : 7.94220  (-1.21239  1.36005)
R^2/D10^2   : 0.149883  (-0.0718987   0.147602)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          65.30 using 59 PHA bins.
# Reduced chi-squared =          1.146 for     57 degrees of freedom 
# Null hypothesis probability =   2.106598e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.111e-07   3.110e-08
25- 50  1.919e-07   4.523e-08
50-150  4.920e-08   2.105e-08
15-150  3.522e-07   8.023e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 32.0801       (-9.08499      14.0087)
Norm        : 1.01871       (-0.27242     0.398957)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.14 using 59 PHA bins.
# Reduced chi-squared =          1.073 for     57 degrees of freedom 
# Null hypothesis probability =   3.295264e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.399e-07   2.870e-08
25- 50  1.657e-07   3.432e-08
50-150  9.893e-08   4.813e-08
15-150  4.046e-07   8.686e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 2.70560        (-1.59395      2.47555)
R1^2/D10^2  : 10.4157        (-9.99354      21339.6)
kT2 [keV]   : 9.59985        (-1.86652      3.23624)
R2^2/D10^2  : 5.94115E-02    (-0.0459013   0.0863642)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.13 using 59 PHA bins.
# Reduced chi-squared =          1.075 for     55 degrees of freedom 
# Null hypothesis probability =   3.272841e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.367e-07   7.014e-08
25- 50  1.746e-07   9.764e-08
50-150  7.788e-08   4.790e-08
15-150  3.892e-07   1.935e-07

Peak spectrum fit

Power-law model

Time interval is from    4.060 sec. to    5.060 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.85688     ( -0.709216   1.07122 )
Norm@50keV  : 2.18960E-03    ( -0.00138491   0.00143663 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.12 using 59 PHA bins.
# Reduced chi-squared =         0.8618 for     57 degrees of freedom 
# Null hypothesis probability =   7.616864e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.543742 ( -0.162833  0.16301 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.47205e-08 ( -9.28327e-09  1.03048e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    4.060 sec. to    5.060 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.87609     (     )
Epeak [keV] : 4.44053      (   )
Norm@50keV  : 9.23919E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.47 using 59 PHA bins.
# Reduced chi-squared =         0.8834 for     56 degrees of freedom 
# Null hypothesis probability =   7.186881e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.543499 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.45857e-08 ( -9.3638e-09  1.04561e-08 ) ergs/cm2

Band function

Time interval is from    4.060 sec. to    5.060 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -7.00335   ( 11.7286   7.00335 )
beta        : -2.85707    ( -1.07159   0.708559 )
Epeak [keV] : 39.4947      ( -39.4947 -39.4947 )
Norm@50keV   : 0.297558    ( -0.188204   0.195282 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.12 using 59 PHA bins.
# Reduced chi-squared =         0.8931 for     55 degrees of freedom 
# Null hypothesis probability =   6.976526e-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]    : 6.62799  (-2.53387  2.92323)
R^2/D10^2   : 1.24117  (-1.23513   9.66106)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.10 using 59 PHA bins.
# Reduced chi-squared =         0.9141 for     57 degrees of freedom 
# Null hypothesis probability =   6.588566e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.247e-09   5.080e-09
25- 50  1.014e-08   6.215e-09
50-150  1.373e-09   1.167e-09
15-150  1.976e-08   1.246e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 23.3425       (-12.6611      30.2891)
Norm        : 5.46941       (-2.92629     9.76961)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.77 using 59 PHA bins.
# Reduced chi-squared =         0.8731 for     57 degrees of freedom 
# Null hypothesis probability =   7.405679e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  9.562e-09   5.186e-09
25- 50  9.367e-09   5.801e-09
50-150  3.594e-09   3.044e-09
15-150  2.252e-08   1.364e-08

Double BB

------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 1.83962        (-1.74597      2.49467)
R1^2/D10^2  : 1067.84        (      )
kT2 [keV]   : 8.80616        (-3.11615      5.28586)
R2^2/D10^2  : 0.314229    (-0.287416   0.918204)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.72 using 59 PHA bins.
#Fit statistic : Chi-Squared =          47.63 using 59 PHA bins.
# Reduced chi-squared =         0.8676 for     55 degrees of freedom 
# Reduced chi-squared =         0.8661 for     55 degrees of freedom 
# Null hypothesis probability =   7.463990e-01
# Null hypothesis probability =   7.492405e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  9.567e-09   4.528e-09
25- 50  9.517e-09   5.925e-09
50-150  3.669e-09   2.813e-09
15-150  2.275e-08   1.260e-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: 2.52916     ( -0.302367   0.342262 )
Norm@50keV  : 6.68679E-04    ( -0.000162841   0.000161379 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          64.30 using 59 PHA bins.
# Reduced chi-squared =          1.128 for     57 degrees of freedom 
# Null hypothesis probability =   2.361666e-01
 
Photon flux (15-150 keV)    in 65.31 sec: 0.133741 ( -0.0199207  0.0199227 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.40205e-07 ( -7.79338e-08  8.1211e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.969678     ( -1.78599   1.03206 )
Epeak [keV] : 24.1353      (   )
Norm@50keV  : 6.24248E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.97 using 59 PHA bins.
# Reduced chi-squared =          1.089 for     56 degrees of freedom 
# Null hypothesis probability =   3.018696e-01
 
Photon flux (15-150 keV)    in 65.31 sec: 0.128297 ( -0.020261  0.020368 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.97114e-07 ( -7.1374e-08  8.32487e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.06116   ( -0.896144   1.04082 )
beta        : -9.37167    ( 9.37167   19.3716 )
Epeak [keV] : 23.6509      ( -11.5343 10.3949 )
Norm@50keV   : 5.40548E-03    ( -0.00541345   0.0571076 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.98 using 59 PHA bins.
# Reduced chi-squared =          1.109 for     55 degrees of freedom 
# Null hypothesis probability =   2.695732e-01
 
Photon flux (15-150 keV)    in 65.31 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)  = 1.46e-07
S(50-100 keV) = 1.01e-07

T90 vs. Hardness ratio plot

T90                                   = 62.0439999997616 sec.
Hardness ratio (energy fluence ratio) = 0.691781

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 0.997095
Count Ratio (50-100 keV) / (15-25 keV) = 0.172839

Mask shadow pattern

IMX = -6.241397423938010E-01, IMY = -1.381387024942553E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000

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:
-299.144000 -57.068000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9751 -15.6350    0.2  16.5  -36.8  13.9818  61.4    0.4	Sco X-1                       
254.5137  35.4047    3.4  38.4 -176.4   1.0940   3.4    4.6	Her X-1                       
255.8446 -37.9752    5.8  40.8  -37.0   0.7825   2.0   10.3	4U 1700-377                   
256.3724 -36.4235    4.4  39.6  -38.7   1.0194   2.6    3.0	GX 349+2                      
262.8904 -24.6000    0.0  33.5  -58.2   0.7455   2.1   10.9	GX 1+4                        
264.5043 -44.5969    9.3  49.8  -40.3   1.0481   1.2   13.5	4U 1735-44                    
268.3672  -1.4161    6.2  29.2 -104.1   0.6665   1.8    2.2	SW J1753.5-0127               
270.3189 -25.2046    7.8  39.1  -64.6   0.8042   1.5    7.8	GX 5-1                        
270.4300 -25.8724    0.0  39.6  -63.8  -0.5090  -0.9   10.4	GRS 1758-258                  
273.9190 -14.1428   11.2  37.1  -83.1   0.5519   1.0    8.1	GX 17+2                       
263.1412 -33.8839    5.9  40.5  -48.0   0.8392   1.9    8.1	GX 354-0                      
208.2455   8.1595    2.2  31.9   89.2   2.3956   5.4 ------	UNKNOWN

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

Time interval of the image:
-57.068000 8.240000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.7966 -15.7159    6.7  16.5  -36.2  -0.1452  -1.7   11.5	Sco X-1                       
254.4102  35.1962    7.4  38.1 -176.3   0.1805   1.6    9.1	Her X-1                       
255.8769 -37.7005    0.0  40.6  -37.2  -0.1634  -1.2   10.1	4U 1700-377                   
256.2913 -36.3596   35.6  39.5  -38.6  -0.0421  -0.3    7.9	GX 349+2                      
263.0592 -24.8822   77.3  33.8  -58.0   0.0197   0.1    8.6	GX 1+4                        
264.8687 -44.3945    4.9  49.8  -40.7  -0.8388  -2.3    6.3	4U 1735-44                    
268.2145  -1.5412    3.9  29.1 -103.9  -0.3650  -3.0   10.6	SW J1753.5-0127               
270.2534 -24.9539    6.5  39.0  -64.9   0.3713   1.8    7.7	GX 5-1                        
270.4120 -25.8715   63.6  39.6  -63.8   0.0409   0.2    9.7	GRS 1758-258                  
273.9853 -14.1449    7.3  37.2  -83.1   0.3324   1.6    6.6	GX 17+2                       
262.8946 -33.7630    3.9  40.3  -47.9  -0.5029  -3.0    6.4	GX 354-0                      
255.1045  55.0886    1.8  56.8  174.1   2.8705   6.2 ------	UNKNOWN                       
241.8563  32.3078    1.2  32.6  167.5   1.0166   9.9 ------	UNKNOWN                       
233.8601  -7.8402    2.2   9.3   17.7   0.4048   5.3 ------	UNKNOWN                       
236.0320 -44.0093    2.0  43.9  -13.5   0.7527   5.8 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
104.156600 302.928500
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9747 -15.6360    0.5  48.0  -12.7   8.5310  21.8    0.4	Sco X-1                       
254.5513  35.4743    4.6  11.0 -118.8   0.4162   2.5    9.1	Her X-1                       
268.4534  -1.5935    0.0  42.2  -50.4   0.8154   2.1    9.9	SW J1753.5-0127               
329.4647  68.2534    2.6  59.4 -163.1   4.9009   4.4 ------	UNKNOWN

Plot creation:
Sun May 31 14:08:36 EDT 2015