batgrbproduct analysis for trigger=770528

batgrbproduct Analysis for Trigger=770528

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): Thu Sep 28 17:56:00 EDT 2017
             Host Name: bat1
   Current Working Dir: /local/data/bat1/alien/Swift_3rdBATcatalog/event/batevent_reproc/trigger770528
======================================================================

  Trigger: 00770528      Segment: 000

  BAT Trigger Time: 526135766.848   [s; MET]
      Trigger Stop: 526135767.872   [s; MET]
               UTC: 2017-09-03T12:49:07.219440    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 254.511712851535   Dec: 34.9835881466908  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    9.84
     Image Trigger?:     NO
     Rate S/N Ratio:     17.7763888346312  [ if not an image trigger ]
     Image S/N Ratio:    9.84

  Flight Position:   [ source = BAT ]
    RA: 254.511712851535   Dec: 34.9835881466908  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 254.523170046904   Dec: 34.9822900582206  [deg; J2000]  
        { 16h 58m 05.6s , +34d 58' 56.2" }
         +/- 1.22057722602866 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.444986574520974 [arcmin] (formal 1-sigma fit error)
    SNR: 22.8798787864337
 
  Angular difference between Flight and Ground position is 0.568588 arcmin
 
  Partial Coding Fraction: 0.3007812    [ including projection effects ]

  Duration
     T90: 27.7239999771118 +/- 4.50650779531548
        Measured from: -5.26800000667572
                   to: 22.4559999704361     [s; relative to TRIGTIME]
     T50: 10.3559999465942 +/- 1.76041018375818
        Measured from: 1.00400000810623
                   to: 11.3599999547005     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 0.579999983310699     
                   to: 1.5799999833107     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -9.99599999189377     
                   to: 25.7039999961853     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     1.230462   1.452451   0.838055   0.305940
           0.083683   0.081894   0.068563   0.055324 [error]
 Peak      0.126376   0.164330   0.102325   0.036224
           0.016225   0.017028   0.013970   0.010457 [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 5.00e-07 7.00e-07 7.21e-07 1.37e-06 2.36e-06 3.29e-06   erg/cm2
              Error 5.25e-08 4.54e-08 7.03e-08 2.77e-07 1.64e-07 3.40e-07   erg/cm2
Peak flux Power-law 1.60e+00 1.31e+00 7.29e-01 5.95e-01 3.91e+00 4.24e+00   ph/cm2/s
              Error 2.99e-01 1.57e-01 1.18e-01 1.90e-01 4.72e-01 4.93e-01   ph/cm2/s
 
Fluence   Cutoff-PL 5.03e-07 6.96e-07 7.28e-07 1.35e-06 2.37e-06 3.29e-06   erg/cm2
              Error -------- 4.60e-08 9.06e-08 4.07e-07 1.70e-07 3.44e-07   erg/cm2
Peak flux Cutoff-PL 1.60e+00 1.18e+00 5.99e-01 5.09e-01 3.58e+00 3.88e+00   ph/cm2/s
              Error 3.62e-01 2.70e-01 1.32e-01 1.06e-01 7.84e-01 2.66e+00   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    1.951    0.121    -      -           7.17e-03 5.12e-04   72.710 57
CPL   2.011    0.230       8.1    0.0      6.65e-03 0.00e+00   72.640 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.850    0.204    -      -           2.78e-02 3.53e-03   67.430 57
CPL   1.855    0.709    9999.4    0.0      2.78e-02 0.00e+00   67.430 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: 22.144000 sec.
T50 in the 50-300 keV band: 9.920000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   35.700   -9.996   25.704
T90    27.724   -5.268   22.456
T50    10.356    1.004   11.360
Peak    1.000    0.580    1.580

Click here for the BAT GCN circular template

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
  254.5232    34.9823   0.0084    46.7038   -29.2684         3.8462961     22.880 TRIG_00770528                 
 
Foreground time interval of the image:
 -9.996  25.704 (delta_t =  35.700 [sec])
Background time interval of the image:
-239.848  -9.996 (delta_t = 229.852 [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   -9.996 sec. to   25.704 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.95058     ( -0.119787   0.122369 )
Norm@50keV  : 7.16879E-03    ( -0.000514595   0.000508838 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          72.71 using 59 PHA bins.
# Reduced chi-squared =          1.276 for     57 degrees of freedom 
# Null hypothesis probability =   7.843826e-02
 
Photon flux (15-150 keV)    in 35.7 sec: 1.05168 ( -0.071412  0.07168 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.35564e-06 ( -1.63849e-07  1.64757e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from   -9.996 sec. to   25.704 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.01065     ( -0.446129   0.013823 )
Epeak [keV] : 8.12603      (   )
Norm@50keV  : 6.65484E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          72.64 using 59 PHA bins.
# Reduced chi-squared =          1.297 for     56 degrees of freedom 
# Null hypothesis probability =   6.676483e-02
 
Photon flux (15-150 keV)    in 35.7 sec: 1.03062 ( -0.133493  0.10102 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.36946e-06 ( -1.83818e-07  1.57155e-07 ) ergs/cm2

Band function

Time interval is from   -9.996 sec. to   25.704 sec.
 
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       :    (     )
beta        :     (     )
Epeak [keV] :       (   )
Norm@50keV   :     (     )
------------------------------------------------------------
 
Photon flux (15-150 keV)    in  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]    : 10.8008  (  )
R^2/D10^2   : 0.351252  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         145.46 using 59 PHA bins.
# Reduced chi-squared =         2.5520 for     57 degrees of freedom 
# Null hypothesis probability =   1.128413e-09
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.045e-07   3.857e-08
25- 50  8.407e-07   6.515e-08
50-150  5.462e-07   8.140e-08
15-150  1.691e-06   1.335e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 82.1585       (-16.3364      23.3772)
Norm        : 4.80002       (-0.505304     0.582645)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          78.67 using 59 PHA bins.
# Reduced chi-squared =          1.380 for     57 degrees of freedom 
# Null hypothesis probability =   3.014288e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.454e-07   4.409e-08
25- 50  7.378e-07   4.802e-08
50-150  1.060e-06   1.662e-07
15-150  2.243e-06   2.171e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 7.23568        (-1.01474      1.02781)
R1^2/D10^2  : 1.35596        (-0.522026      1.00789)
kT2 [keV]   : 33.5595        (-8.99683      19.401)
R2^2/D10^2  : 3.73236E-03    (-0.00273552   0.0073531)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          71.03 using 59 PHA bins.
# Reduced chi-squared =          1.291 for     55 degrees of freedom 
# Null hypothesis probability =   7.173133e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.427e-07   6.788e-08
25- 50  7.548e-07   1.119e-07
50-150  1.177e-06   5.299e-07
15-150  2.375e-06   6.251e-07

Peak spectrum fit

Power-law model

Time interval is from    0.580 sec. to    1.580 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.84979     ( -0.201656   0.207154 )
Norm@50keV  : 2.78208E-02    ( -0.00355849   0.00349897 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          67.43 using 59 PHA bins.
# Reduced chi-squared =          1.183 for     57 degrees of freedom 
# Null hypothesis probability =   1.625325e-01
 
Photon flux (15-150 keV)    in 1 sec: 3.91038 ( -0.47119  0.47223 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.55847e-07 ( -3.25669e-08  3.2782e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.580 sec. to    1.580 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.85523     ( -0.712774   0.705641 )
Epeak [keV] : 9999.36      (   )
Norm@50keV  : 2.77527E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          67.43 using 59 PHA bins.
# Reduced chi-squared =          1.204 for     56 degrees of freedom 
# Null hypothesis probability =   1.409466e-01
 
Photon flux (15-150 keV)    in 1 sec: 3.58162 ( -0.77133  0.79692 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.56478e-07 ( -3.32853e-08  2.65699e-08 ) ergs/cm2

Band function

Time interval is from    0.580 sec. to    1.580 sec.
 
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       :    (     )
beta        :     (     )
Epeak [keV] :       (   )
Norm@50keV   :     (     )
------------------------------------------------------------
 
Photon flux (15-150 keV)    in  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]    : 10.5041  (-1.40723  1.70064)
R^2/D10^2   : 1.53282  (-0.676758   1.14437)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          88.75 using 59 PHA bins.
# Reduced chi-squared =          1.557 for     57 degrees of freedom 
# Null hypothesis probability =   4.502741e-03
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.496e-08   6.565e-09
25- 50  9.303e-08   1.348e-08
50-150  5.589e-08   1.564e-08
15-150  1.839e-07   2.995e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 94.6785       (-31.6737      66.1057)
Norm        : 17.4459       (-2.92645     3.69747)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          69.19 using 59 PHA bins.
# Reduced chi-squared =          1.214 for     57 degrees of freedom 
# Null hypothesis probability =   1.290370e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.558e-08   8.060e-09
25- 50  7.793e-08   9.640e-09
50-150  1.223e-07   5.308e-08
15-150  2.458e-07   5.765e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 8.04695        (-1.63591      1.54601)
R1^2/D10^2  : 3.73015        (-1.11935      2.09058)
kT2 [keV]   : 60.8775        (-67.215      -99.3076)
R2^2/D10^2  : 2.74662E-03    (-0.000826788   0.00876225)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          62.08 using 59 PHA bins.
# Reduced chi-squared =          1.129 for     55 degrees of freedom 
# Null hypothesis probability =   2.383968e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.482e-08   1.561e-08
25- 50  8.470e-08   2.416e-08
50-150  1.245e-07   6.694e-08
15-150  2.541e-07   9.231e-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: 1.95058     ( -0.119787   0.122369 )
Norm@50keV  : 7.16879E-03    ( -0.000514595   0.000508838 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          72.71 using 59 PHA bins.
# Reduced chi-squared =          1.276 for     57 degrees of freedom 
# Null hypothesis probability =   7.843826e-02
 
Photon flux (15-150 keV)    in 35.7 sec: 1.05161 ( -0.071399  0.0716687 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.35524e-06 ( -1.64075e-07  1.64755e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.95061     ( -0.393084   0.530115 )
Epeak [keV] : 9982.91      (   )
Norm@50keV  : 7.18174E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          72.71 using 59 PHA bins.
# Reduced chi-squared =          1.298 for     56 degrees of freedom 
# Null hypothesis probability =   6.600019e-02
 
Photon flux (15-150 keV)    in 35.7 sec: 1.05196 ( -0.072196  0.0705 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.35458e-06 ( -1.70917e-07  1.63977e-07 ) ergs/cm2

Band function

 
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       :    (     )
beta        :     (     )
Epeak [keV] :       (   )
Norm@50keV   :     (     )
------------------------------------------------------------
 
Photon flux (15-150 keV)    in  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)  = 7.00e-07
S(50-100 keV) = 7.21e-07

T90 vs. Hardness ratio plot

T90                                   = 27.7239999771118 sec.
Hardness ratio (energy fluence ratio) = 1.03

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.18041
Count Ratio (50-100 keV) / (15-25 keV) = 0.68109

Mask shadow pattern

IMX = 9.258263296751151E-01, IMY = 5.188779791649856E-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:
-239.848000 -9.996000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9889 -15.6555    1.4  36.3 -109.8   4.2700   8.2    1.1	Sco X-1                       
254.3920  35.3379    5.4  47.1  -29.1  -0.9778  -2.1    3.2	Her X-1                       
255.9831 -37.8427   21.0  39.7 -149.3   0.2048   0.5    0.2	4U 1700-377                   
256.4417 -36.4386   16.2  38.4 -148.3   0.2383   0.7    1.0	GX 349+2                      
262.8540 -24.7629   17.4  26.0 -141.5   0.1613   0.7    8.5	GX 1+4                        
264.8394 -44.4167    4.7  41.7 -163.3   0.8184   2.4    4.6	4U 1735-44                    
268.3844  -1.4431  235.3  12.4  -74.0   0.0114   0.0    1.1	SW J1753.5-0127               
270.2696 -25.0106    2.3  22.3 -155.4   1.0705   4.9    4.2	GX 5-1                        
270.3234 -25.8476    6.0  23.0 -156.4   0.4159   1.9    6.4	GRS 1758-258                  
273.9570 -14.0578    3.2  11.1 -146.0   0.7713   3.6    3.1	GX 17+2                       
276.0808 -30.5219    0.0  25.9 -171.6   0.2890   1.2   12.3	H1820-303                     
285.1514 -24.7776    7.9  20.4  167.3   0.3149   1.5   10.6	HT1900.1-2455                 
288.8015  10.9563    1.1  18.0   28.1   2.2169  10.5    0.7	GRS 1915+105                  
299.6069  35.1925    1.2  44.0   22.9   4.1142   9.4    1.0	Cyg X-1                       
308.1104  40.9533   14.1  52.5   26.4   0.8617   0.8    0.0	Cyg X-3                       
263.0175 -33.8873    3.3  33.1 -153.1   0.9361   3.5    3.5	GX 354-0                      
266.5899   7.8399    3.5  18.7  -47.0   0.7433   3.3 ------	UNKNOWN                       
237.6865 -31.7089    2.8  48.0 -129.2   3.9312   4.1 ------	UNKNOWN

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

Time interval of the image:
-9.996000 25.704000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9678 -15.5669    3.0  36.3 -109.7  -0.6805  -3.8    4.5	Sco X-1                       
254.3053  35.1620    0.0  47.0  -29.3   0.0318   0.2   13.2	Her X-1                       
255.8217 -37.9552    0.0  39.8 -149.3  -0.2107  -1.7   10.3	4U 1700-377                   
256.5858 -36.5843   21.6  38.4 -148.6  -0.0673  -0.5   12.1	GX 349+2                      
263.0439 -24.6040   11.3  25.7 -141.6   0.0941   1.0    8.7	GX 1+4                        
264.6198 -44.3606    5.0  41.8 -163.1   0.2776   2.3    7.5	4U 1735-44                    
268.3372  -1.5992    6.0  12.4  -74.8  -0.1505  -1.9    9.0	SW J1753.5-0127               
270.1495 -25.1018   32.2  22.4 -155.2   0.0292   0.4    7.4	GX 5-1                        
270.1608 -25.7830    6.3  23.0 -156.0   0.1491   1.8    8.0	GRS 1758-258                  
274.1598 -13.8910    0.0  10.8 -146.4   0.1760   2.3   12.5	GX 17+2                       
276.0728 -30.4174    8.8  25.8 -171.6   0.1029   1.3    8.2	H1820-303                     
285.1928 -25.0651    0.0  20.7  167.4   0.0981   1.3   12.2	HT1900.1-2455                 
288.7193  11.0329    5.8  18.0   27.7  -0.1558  -2.0    7.0	GRS 1915+105                  
299.5720  35.2253    9.2  44.1   22.9  -0.1993  -1.3    1.7	Cyg X-1                       
308.0006  40.9514    5.3  52.4   26.3  -0.8067  -2.2    5.0	Cyg X-3                       
262.9515 -33.7456    5.3  33.0 -152.9  -0.2109  -2.2    5.7	GX 354-0                      
320.1092 -36.6359    2.8  48.3  136.5   1.4129   4.2 ------	UNKNOWN                       
254.5305  34.9781    0.6  46.7  -29.3   3.8879  23.1 ------	UNKNOWN                       
241.4875  27.5046    2.1  49.5  -46.9   1.8738   5.4 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
171.852610 962.248700
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
299.6166  35.2076    2.1  48.7  154.1  11.4289   5.5    1.3	Cyg X-1                       
308.0681  40.9823    2.5  40.2  150.7   6.3439   4.7    2.6	Cyg X-3                       
326.1872  38.3316   38.2  34.9  129.0   0.3495   0.3    0.9	Cyg X-2                       
 60.5139  21.6167    3.3  55.4    0.6   7.1431   3.5 ------	UNKNOWN                       
268.6834  45.4097    3.4  53.1 -173.4   6.0110   3.3 ------	UNKNOWN                       
 98.3637  56.5070    2.9  42.1  -57.6   8.6661   3.9 ------	UNKNOWN                       
106.4099  58.1563    3.3  43.6  -64.0  11.0438   3.5 ------	UNKNOWN

Plot creation:
Fri Sep 29 01:16:09 EDT 2017