batgrbproduct analysis for trigger=702252

batgrbproduct Analysis for Trigger=702252

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): Fri Jul 15 14:13:48 EDT 2016
             Host Name: bat1
   Current Working Dir: /local/data/bat1/alien/Swift_3rdBATcatalog/event/batevent_reproc/trigger702252
======================================================================

  Trigger: 00702252      Segment: 000

  BAT Trigger Time: 488952266.432   [s; MET]
      Trigger Stop: 488952267.456   [s; MET]
               UTC: 2016-06-30T04:04:09.942380    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 198.239285438184   Dec: -56.0685035261327  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    7.82
     Image Trigger?:     NO
     Rate S/N Ratio:     17.8044938147649  [ if not an image trigger ]
     Image S/N Ratio:    7.82

  Flight Position:   [ source = BAT ]
    RA: 198.239285438184   Dec: -56.0685035261327  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 198.237918550575   Dec: -56.0283388415911  [deg; J2000]  
        { 13h 12m 57.1s , -56d 01' 42.0" }
         +/- 1.3771528524962 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.423329449685849 [arcmin] (formal 1-sigma fit error)
    SNR: 19.2562828759618
 
  Angular difference between Flight and Ground position is 2.410316 arcmin
 
  Partial Coding Fraction: 0.515625    [ including projection effects ]

  Duration
     T90: 29.5520000457764 +/- 5.60842792208861
        Measured from: -0.407999992370605
                   to: 29.1440000534058     [s; relative to TRIGTIME]
     T50: 10.7520000338554 +/- 2.28217440788382
        Measured from: 2.216000020504
                   to: 12.9680000543594     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: -0.419999957084656     
                   to: 0.580000042915344     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -1.41600000858307     
                   to: 34.8880000114441     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.481851   0.653517   0.587300   0.171749
           0.049268   0.048505   0.042284   0.035449 [error]
 Peak      0.041072   0.034511   0.066391   0.015881
           0.008741   0.009190   0.007965   0.006909 [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 1.38e-07 2.84e-07 4.54e-07 1.63e-06 1.26e-06 2.50e-06   erg/cm2
              Error 1.99e-08 2.40e-08 4.10e-08 3.34e-07 1.02e-07 3.58e-07   erg/cm2
Peak flux Power-law 2.56e-01 3.64e-01 3.86e-01 7.55e-01 1.24e+00 1.76e+00   ph/cm2/s
              Error 1.02e-01 8.54e-02 6.23e-02 3.03e-01 2.11e-01 3.05e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.34e-07 2.87e-07 4.61e-07 1.31e-06 1.25e-06 2.19e-06   erg/cm2
              Error 2.10e-08 2.66e-08 4.50e-08 5.27e-07 1.10e-07 5.88e-07   erg/cm2
Peak flux Cutoff-PL 2.56e-01 3.65e-01 3.86e-01 7.49e-01 1.24e+00 1.77e+00   ph/cm2/s
              Error -------- -------- -------- -------- 2.11e-01 3.55e-01   ph/cm2/s
 
Fluence        Band 1.36e-07 2.88e-07 4.61e-07 1.31e-06 1.25e-06 2.03e-06   erg/cm2
              Error 1.56e-08 2.29e-08 3.61e-08 8.43e-07 9.77e-08 3.63e-07   erg/cm2
Peak flux      Band 3.71e-01 3.64e-01 3.83e-01 3.38e-01 1.21e+00 1.14e+00   ph/cm2/s
              Error 1.02e-01 8.54e-02 6.38e-02 5.32e-02 2.44e-01 8.26e-01   ph/cm2/s

 
=== Time-averaged spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.319    0.135    -      -           3.53e-03 2.61e-04   68.420 57
CPL   1.167    0.416     297.3    0.0      4.16e-03 2.09e-03   68.170 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    0.918    0.327    -      -           1.08e-02 1.83e-03   61.330 57
CPL   0.927    0.331    9999.4    0.0      1.09e-02 4.90e-03   61.360 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: 14.784000 sec.
T50 in the 50-300 keV band: 7.040000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   36.304   -1.416   34.888
T90    29.552   -0.408   29.144
T50    10.752    2.216   12.968
Peak    1.000   -0.420    0.580

Click here for the BAT GCN circular template

Special notes of this burst

Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minute to calcaulte

Image

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

#   RAcent    DECcent   POSerr    Theta     Phi              Peak Cts       SNR   Name
  198.2379   -56.0283   0.0101    27.3095   -74.4054         1.5840673     19.256 TRIG_00702252                 
 
Foreground time interval of the image:
 -1.416  16.469 (delta_t =  17.885 [sec])
Background time interval of the image:
-35.331  -1.416 (delta_t =  33.915 [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

8 ms binning

From T100_start-3 s to T100_start+3 s

2 ms binning

From T100_start-1 s to T100_start+1 s

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   -1.416 sec. to   34.888 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.31863     ( -0.135318   0.134434 )
Norm@50keV  : 3.52764E-03    ( -0.000260726   0.000260709 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.42 using 59 PHA bins.
# Reduced chi-squared =          1.200 for     57 degrees of freedom 
# Null hypothesis probability =   1.429703e-01
 
Photon flux (15-150 keV)    in 36.3 sec: 0.422341 ( -0.032796  0.03293 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.2599e-06 ( -1.01772e-07  1.02412e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from   -1.416 sec. to   34.888 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.16662     ( -0.560424   0.271296 )
Epeak [keV] : 297.286      ( -297.537 -297.537 )
Norm@50keV  : 4.15804E-03    ( -0.000860317   0.00332007 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.17 using 59 PHA bins.
# Reduced chi-squared =          1.217 for     56 degrees of freedom 
# Null hypothesis probability =   1.276733e-01
 
Photon flux (15-150 keV)    in 36.3 sec: 0.418898 ( -0.034766  0.034652 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.24758e-06 ( -1.10822e-07  1.09601e-07 ) ergs/cm2

Band function

Time interval is from   -1.416 sec. to   34.888 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.00795   ( 1.02022   2.01536 )
beta        : -1.40680    ( 1.45267   0.262865 )
Epeak [keV] : 144.105      ( -204.649 -204.649 )
Norm@50keV   : 5.14162E-03    ( -0.00122473   0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.18 using 59 PHA bins.
# Reduced chi-squared =          1.240 for     55 degrees of freedom 
# Null hypothesis probability =   1.092325e-01
 
Photon flux (15-150 keV)    in 36.3 sec: 0.422341 ( -0.032796  0.03293 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.25045e-06 ( -9.46675e-08  1.0077e-07 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 17.8303  (-1.72627  1.97988)
R^2/D10^2   : 2.70992E-02  (-0.0081288   0.0112712)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         104.35 using 59 PHA bins.
# Reduced chi-squared =         1.8307 for     57 degrees of freedom 
# Null hypothesis probability =   1.320567e-04
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.280e-08   9.238e-09
25- 50  2.884e-07   3.519e-08
50-150  6.639e-07   8.512e-08
15-150  1.015e-06   9.765e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (-22.348      -200)
Norm        : 1.76239       (-0.131448     0.131448)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          77.47 using 59 PHA bins.
# Reduced chi-squared =          1.359 for     57 degrees of freedom 
# Null hypothesis probability =   3.693954e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.593e-07   1.394e-08
25- 50  3.064e-07   6.195e-08
50-150  6.720e-07   1.860e-07
15-150  1.138e-06   2.261e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 8.08051        (-2.80816      3.12886)
R1^2/D10^2  : 0.234906        (-0.141463      0.751652)
kT2 [keV]   : 31.0115        (-8.17298      25.9297)
R2^2/D10^2  : 3.47444E-03    (-0.00287065   0.00680808)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          71.22 using 59 PHA bins.
# Reduced chi-squared =          1.295 for     55 degrees of freedom 
# Null hypothesis probability =   6.963899e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.200e-07   3.712e-08
25- 50  2.968e-07   1.075e-07
50-150  8.277e-07   3.880e-07
15-150  1.245e-06   4.606e-07

Peak spectrum fit

Power-law model

Time interval is from   -0.420 sec. to    0.580 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.918237     ( -0.34003   0.314904 )
Norm@50keV  : 1.08137E-02    ( -0.00185958   0.0017929 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.33 using 59 PHA bins.
# Reduced chi-squared =          1.076 for     57 degrees of freedom 
# Null hypothesis probability =   3.235915e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.24145 ( -0.21027  0.21201 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.20523e-07 ( -1.98113e-08  1.98715e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.420 sec. to    0.580 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.926543     ( -0.357827   0.303382 )
Epeak [keV] : 9999.36      ( -9999.36 -9999.36 )
Norm@50keV  : 1.09137E-02    ( -0.00171353   0.00808589 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.36 using 59 PHA bins.
# Reduced chi-squared =          1.096 for     56 degrees of freedom 
# Null hypothesis probability =   2.899220e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.24121 ( -0.21053  0.21176 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.20454e-07 ( -1.9784e-08  1.98888e-08 ) ergs/cm2

Band function

Time interval is from   -0.420 sec. to    0.580 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -9.99999   ( 9.99999   9.99999 )
beta        : -0.918226    ( -0.314609   0.340027 )
Epeak [keV] : 13.6996      ( -13.6996 -13.6996 )
Norm@50keV   : 1.46974    ( -0.252757   0.243681 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.33 using 59 PHA bins.
# Reduced chi-squared =          1.115 for     55 degrees of freedom 
# Null hypothesis probability =   2.595515e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.20563 ( -0.18536  0.3022 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.19231e-28 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 29.5236  (-6.58309  10.4704)
R^2/D10^2   : 1.80649E-02  (-0.0102859   0.0204392)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          70.83 using 59 PHA bins.
# Reduced chi-squared =          1.243 for     57 degrees of freedom 
# Null hypothesis probability =   1.029981e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.488e-09   1.027e-09
25- 50  1.524e-08   4.970e-09
50-150  9.443e-08   3.219e-08
15-150  1.122e-07   3.875e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (-40.0567      -200)
Norm        : 5.25003       (-0.863565     0.863565)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          74.55 using 59 PHA bins.
# Reduced chi-squared =          1.308 for     57 degrees of freedom 
# Null hypothesis probability =   5.923113e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.307e-08   7.460e-09
25- 50  2.515e-08   1.435e-08
50-150  5.515e-08   3.175e-08
15-150  9.337e-08   5.200e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 3.67140        (-1.44742      2.3013)
R1^2/D10^2  : 18.5515        (-16.7974      358.099)
kT2 [keV]   : 36.2483        (-9.12432      17.7298)
R2^2/D10^2  : 9.68858E-03    (-0.00614404   0.0125029)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.66 using 59 PHA bins.
# Reduced chi-squared =          1.012 for     55 degrees of freedom 
# Null hypothesis probability =   4.499284e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.272e-08   7.030e-09
25- 50  1.472e-08   5.863e-09
50-150  9.801e-08   4.550e-08
15-150  1.255e-07   4.843e-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: 1.26822     ( -0.118552   0.117822 )
Norm@50keV  : 6.05884E-03    ( -0.000396583   0.00039654 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          70.73 using 59 PHA bins.
# Reduced chi-squared =          1.241 for     57 degrees of freedom 
# Null hypothesis probability =   1.045051e-01
 
Photon flux (15-150 keV)    in 17.88 sec: 0.718774 ( -0.0495378  0.0496759 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.07906e-06 ( -7.67642e-08  7.70803e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.909041     ( -0.521949   0.407702 )
Epeak [keV] : 170.285      ( -69.3822 -170.284 )
Norm@50keV  : 8.81491E-03    ( -0.00296243   0.00608082 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          69.02 using 59 PHA bins.
# Reduced chi-squared =          1.233 for     56 degrees of freedom 
# Null hypothesis probability =   1.134799e-01
 
Photon flux (15-150 keV)    in 17.88 sec: 0.704575 ( -0.05287  0.052819 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.05843e-06 ( -8.27111e-08  8.21961e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.909073   ( -0.165302   0.583914 )
beta        : -10.0000    ( 10   1.81188e-13 )
Epeak [keV] : 170.265      ( -48.9292 -170.265 )
Norm@50keV   : 8.81413E-03    ( -0.00295105   0.00608285 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          69.02 using 59 PHA bins.
# Reduced chi-squared =          1.255 for     55 degrees of freedom 
# Null hypothesis probability =   9.677248e-02
 
Photon flux (15-150 keV)    in 17.88 sec: 0.727553 ( -0.075633  0.033791 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.81856e-08 ( 0  0 ) ergs/cm2

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

S(25-50 keV)  = 2.84e-07
S(50-100 keV) = 4.54e-07

T90 vs. Hardness ratio plot

T90                                   = 29.5520000457764 sec.
Hardness ratio (energy fluence ratio) = 1.59859

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.35626
Count Ratio (50-100 keV) / (15-25 keV) = 1.21884

Mask shadow pattern

IMX = 1.388094637590144E-01, IMY = 4.973407424152088E-01

TIME vs. PHA plot around the trigger time

TIME vs. DetID plot around the trigger time

100 us light curve (15-350 keV)

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:
-35.331400 -1.416000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
169.9541 -60.6704    4.8  40.5  -89.1   0.8479   2.4   11.0	Cen X-3                       
186.5718 -62.7457    2.8  32.3  -89.3   0.4854   4.1    2.8	GX 301-2                      
244.9943 -15.6357    0.5  35.4   45.4   2.7577  21.6    0.9	Sco X-1                       
255.9913 -37.8856    5.8  15.5   81.0  -0.1443  -2.0    2.5	4U 1700-377                   
256.3673 -36.4243    2.0  17.0   79.5   0.4351   5.7    3.3	GX 349+2                      
262.9810 -24.5561    9.1  30.1   79.8  -0.1511  -1.3   11.5	GX 1+4                        
264.7055 -44.3752   11.9  15.2  116.3  -0.0728  -1.0    4.8	4U 1735-44                    
270.1865 -24.9785 2458.1  32.7   91.3   0.0005   0.0    8.0	GX 5-1                        
270.4503 -25.7297    5.3  32.2   92.4   0.2842   2.2    8.0	GRS 1758-258                  
275.9784 -30.4272    6.3  31.2  105.2   0.2286   1.8    4.5	H1820-303                     
285.1325 -25.0631    4.0  40.5  110.1   0.8237   2.8   10.0	HT1900.1-2455                 
263.0113 -33.8290   18.3  21.9   89.8  -0.0525  -0.6    1.2	GX 354-0                      
225.4841  -6.0795    2.3  47.6   18.5   0.8916   5.0 ------	UNKNOWN                       
217.4777 -36.7487    3.4  23.8  -19.3   0.2249   3.4 ------	UNKNOWN                       
 92.4434 -79.9372    3.6  48.0 -129.3   1.0185   3.2 ------	UNKNOWN

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

Time interval of the image:
-1.416000 16.468610
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
169.9657 -60.6550    4.3  40.5  -89.1  -0.7059  -2.7   10.5	Cen X-3                       
186.6416 -62.7682   74.3  32.3  -89.4   0.0172   0.2    0.4	GX 301-2                      
244.8399 -15.5865    3.4  35.4   45.2   0.3418   3.4    8.7	Sco X-1                       
256.1507 -37.7543    8.1  15.7   81.2   0.0896   1.4    9.5	4U 1700-377                   
256.4647 -36.6277    0.0  16.8   80.1  -0.0342  -0.5   12.4	GX 349+2                      
262.9832 -24.5534    0.0  30.1   79.8  -0.0789  -0.8   11.6	GX 1+4                        
264.9499 -44.3654    3.6  15.3  116.6   0.1896   3.2   10.2	4U 1735-44                    
270.4503 -25.0673    8.9  32.8   91.8   0.1454   1.3    9.1	GX 5-1                        
270.1850 -25.6885    8.9  32.1   92.0   0.1429   1.3    7.1	GRS 1758-258                  
276.0723 -30.3694    5.5  31.3  105.2  -0.2176  -2.1    7.6	H1820-303                     
284.8751 -25.0160    0.0  40.4  109.7   0.2075   0.9   10.5	HT1900.1-2455                 
262.7500 -33.8848    0.0  21.8   89.4  -0.1163  -1.6   12.3	GX 354-0                      
299.0427 -38.0661    2.4  40.1  137.4   0.5999   4.7 ------	UNKNOWN                       
274.8241 -31.0077    1.9  30.1  104.4   0.5386   6.1 ------	UNKNOWN                       
216.3253  -5.0195    2.4  51.6    7.7   0.8120   4.8 ------	UNKNOWN                       
287.1944 -81.4555    2.4  33.2 -146.4   0.3598   4.8 ------	UNKNOWN                       
198.2379 -56.0283    0.6  27.3  -74.4   1.5841  19.3 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
67.268590 962.624700
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.2039 -60.4182    0.0  15.3 -124.4   0.5927   1.1   12.7	Cen X-3                       
186.6858 -62.7827    0.5   8.9 -149.9  11.0040  22.5    1.1	GX 301-2                      
258.9884 -75.2187    3.6  29.3  146.7   2.6321   3.2 ------	UNKNOWN                       
178.5216 -61.1155    3.4  11.4 -130.7   1.6520   3.4 ------	UNKNOWN                       
 58.1440 -73.3030    2.6  47.8 -171.9   5.7968   4.5 ------	UNKNOWN                       
111.9466 -51.2395    2.4  48.0 -129.1  14.7854   4.9 ------	UNKNOWN

Plot creation:
Fri Jul 15 14:44:42 EDT 2016