batgrbproduct analysis for trigger=276212

batgrbproduct Analysis for Trigger=276212

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): Mon Jan 20 10:30:45 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger276212
======================================================================

  Trigger: 00276212      Segment: 000

  BAT Trigger Time: 198672247.872   [s; MET]
      Trigger Stop: 198672248.896   [s; MET]
               UTC: 2007-04-19T10:44:05.971820    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 315.718504424161   Dec: -31.2666947301328  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    7.02
     Image Trigger?:     NO
     Rate S/N Ratio:     17.4355957741627  [ if not an image trigger ]
     Image S/N Ratio:    7.02

  Flight Position:   [ source = BAT ]
    RA: 315.718504424161   Dec: -31.2666947301328  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 315.705474720509   Dec: -31.264742642361  [deg; J2000]  
        { 21h 02m 49.3s , -31d 15' 53.1" }
         +/- 0.767497907055403 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.292500640885236 [arcmin] (formal 1-sigma fit error)
    SNR: 44.3908855467132
 
  Angular difference between Flight and Ground position is 0.678430 arcmin
 
  Partial Coding Fraction: 0.6640625    [ including projection effects ]

  Duration
     T90: 238.008000016212 +/- 14.3393349777117
        Measured from: -3.53200000524521
                   to: 234.476000010967     [s; relative to TRIGTIME]
     T50: 69.8039999902248 +/- 4.18186559772703
        Measured from: 17.7960000038147
                   to: 87.5999999940395     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: -0.280000001192093     
                   to: 0.719999998807907     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -10.3440000116825     
                   to: 313.763999998569     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     3.991964   4.764220   3.259105   0.814429
           0.084496   0.087808   0.076904   0.065111 [error]
 Peak      0.045669   0.060110   0.048206   0.026747
           0.006275   0.006693   0.006102   0.005140 [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 1.18e-06 1.97e-06 2.51e-06 6.41e-06 7.44e-06 1.21e-05   erg/cm2
              Error 5.95e-08 5.57e-08 8.16e-08 4.83e-07 1.93e-07 5.24e-07   erg/cm2
Peak flux Power-law 3.75e-01 4.37e-01 3.66e-01 5.18e-01 1.36e+00 1.70e+00   ph/cm2/s
              Error 8.53e-02 5.86e-02 5.05e-02 1.57e-01 1.61e-01 2.05e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.18e-06 1.98e-06 2.51e-06 6.36e-06 7.44e-06 1.20e-05   erg/cm2
              Error 3.92e-08 5.71e-08 8.41e-08 9.71e-07 1.93e-07 8.79e-07   erg/cm2
Peak flux Cutoff-PL 3.82e-01 4.39e-01 3.63e-01 5.02e-01 1.37e+00 1.68e+00   ph/cm2/s
              Error 8.56e-02 5.80e-02 5.04e-02 1.96e-01 1.61e-01 2.22e-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    1.652    0.050    -      -           2.47e-03 6.15e-05   45.030 57
CPL   1.651    0.120    9999.4   -0.0      2.47e-03 2.99e-04   45.030 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.255    0.214    -      -           1.15e-02 1.32e-03   63.350 57
CPL   2.408    0.288     135.8    0.0      2.40e-03 0.00e+00   61.250 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: 103.680000 sec.
T50 in the 50-300 keV band: 55.680000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100  324.108  -10.344  313.764
T90   238.008   -3.532  234.476
T50    69.804   17.796   87.600
Peak    1.000   -0.280    0.720

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
  315.7055   -31.2647   0.0043    30.2865    20.1055         3.0959317     44.391 TRIG_00276212                 
 
Foreground time interval of the image:
-10.344  16.029 (delta_t =  26.373 [sec])
Background time interval of the image:
-239.872 -10.344 (delta_t = 229.528 [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  -10.344 sec. to  313.764 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.65210     ( -0.0499664   0.0500965 )
Norm@50keV  : 2.47008E-03    ( -6.14873e-05   6.14476e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.03 using 59 PHA bins.
# Reduced chi-squared =         0.7900 for     57 degrees of freedom 
# Null hypothesis probability =   8.743813e-01
 
Photon flux (15-150 keV)    in 324.1 sec: 0.322755 ( -0.00906665  0.00910569 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.44386e-06 ( -1.93077e-07  1.93525e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from  -10.344 sec. to  313.764 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.65052     ( -0.188953   0.0502183 )
Epeak [keV] : 9999.36      ( -9999.35 -9999.36 )
Norm@50keV  : 2.47457E-03    ( -6.16373e-05   0.000536211 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.03 using 59 PHA bins.
# Reduced chi-squared =         0.8041 for     56 degrees of freedom 
# Null hypothesis probability =   8.529418e-01
 
Photon flux (15-150 keV)    in 324.1 sec: 0.322649 ( -0.010376  0.008908 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.44403e-06 ( -1.95983e-07  1.90668e-07 ) ergs/cm2

Band function

Time interval is from  -10.344 sec. to  313.764 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.19541   ( 1.19357   1.19357 )
beta        : -1.65949    ( -0.130752   0.0552687 )
Epeak [keV] : 47.3212      ( -47.0148 -47.0148 )
Norm@50keV   : 5.21158E-03    ( -0.00285698   0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.80 using 59 PHA bins.
# Reduced chi-squared =         0.8145 for     55 degrees of freedom 
# Null hypothesis probability =   8.353539e-01
 
Photon flux (15-150 keV)    in 324.1 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]    : 15.3234  (  )
R^2/D10^2   : 3.05947E-02  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         437.48 using 59 PHA bins.
# Reduced chi-squared =         7.6750 for     57 degrees of freedom 
# Null hypothesis probability =   4.473131e-60
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.857e-07   2.625e-08
25- 50  1.968e-06   6.336e-08
50-150  3.173e-06   1.559e-07
15-150  5.627e-06   1.637e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 175.223       (-23.4581      -174.688)
Norm        : 1.28559       (-0.0388249     0.0218221)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.41 using 59 PHA bins.
# Reduced chi-squared =         0.9720 for     57 degrees of freedom 
# Null hypothesis probability =   5.350695e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.054e-06   5.477e-08
25- 50  1.996e-06   1.131e-07
50-150  4.184e-06   9.469e-07
15-150  7.234e-06   1.034e-06

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 6.99516        (-0.582688      0.615558)
R1^2/D10^2  : 0.361044        (-0.095278      0.13996)
kT2 [keV]   : 27.3730        (-2.31789      2.91663)
R2^2/D10^2  : 3.14840E-03    (-0.000948297   0.00119947)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.64 using 59 PHA bins.
# Reduced chi-squared =         0.9207 for     55 degrees of freedom 
# Null hypothesis probability =   6.418284e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.046e-06   8.021e-08
25- 50  2.006e-06   1.055e-07
50-150  4.292e-06   2.803e-07
15-150  7.343e-06   3.614e-07

Peak spectrum fit

Power-law model

Time interval is from   -0.280 sec. to    0.720 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.25473     ( -0.216061   0.212839 )
Norm@50keV  : 1.15179E-02    ( -0.00131769   0.00131662 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.35 using 59 PHA bins.
# Reduced chi-squared =          1.111 for     57 degrees of freedom 
# Null hypothesis probability =   2.624044e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.36331 ( -0.160391  0.160987 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.15128e-07 ( -1.48441e-08  1.49864e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.280 sec. to    0.720 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.40800     ( -0.36675   0.20876 )
Epeak [keV] : 135.816      ( -9999.36 -9999.36 )
Norm@50keV  : 2.40130E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.25 using 59 PHA bins.
# Reduced chi-squared =          1.094 for     56 degrees of freedom 
# Null hypothesis probability =   2.932484e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.36620 ( -0.16323  0.15795 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.15102e-07 ( -1.4738e-08  1.4506e-08 ) ergs/cm2

Band function

Time interval is from   -0.280 sec. to    0.720 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.947715   ( 0.949613   0.949613 )
beta        : -1.25325    ( 1.25418   0.215555 )
Epeak [keV] : 64.0114      ( -62.7115 -62.7115 )
Norm@50keV   : 2.11570E-02    ( -0.0110029   0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.35 using 59 PHA bins.
# Reduced chi-squared =          1.152 for     55 degrees of freedom 
# Null hypothesis probability =   2.056139e-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]    : 16.9432  (-3.01695  4.18122)
R^2/D10^2   : 0.102189  (-0.0524487   0.0963442)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          90.38 using 59 PHA bins.
# Reduced chi-squared =          1.586 for     57 degrees of freedom 
# Null hypothesis probability =   3.213038e-03
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.980e-09   1.440e-09
25- 50  2.639e-08   4.560e-09
50-150  5.403e-08   1.252e-08
15-150  8.640e-08   1.553e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (      )
Norm        : 5.62508       (-0.653289     0.653252)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          70.17 using 59 PHA bins.
# Reduced chi-squared =          1.231 for     57 degrees of freedom 
# Null hypothesis probability =   1.128949e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.401e-08   7.875e-09
25- 50  2.694e-08   1.496e-08
50-150  5.909e-08   3.252e-08
15-150  1.000e-07   5.550e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 9.07016        (-2.33991      2.52093)
R1^2/D10^2  : 0.634116        (-0.310562      0.92824)
kT2 [keV]   : 58.1353        (-40.6505      -77.4315)
R2^2/D10^2  : 2.02367E-03    (-0.000861545   0.00594275)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.85 using 59 PHA bins.
# Reduced chi-squared =          1.106 for     55 degrees of freedom 
# Null hypothesis probability =   2.735562e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.086e-08   5.848e-09
25- 50  2.688e-08   1.128e-08
50-150  7.773e-08   4.230e-08
15-150  1.155e-07   5.333e-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: 1.30224     ( -0.0642916   0.064025 )
Norm@50keV  : 7.77845E-03    ( -0.000264997   0.000264933 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.68 using 59 PHA bins.
# Reduced chi-squared =          1.012 for     57 degrees of freedom 
# Null hypothesis probability =   4.500717e-01
 
Photon flux (15-150 keV)    in 26.37 sec: 0.928373 ( -0.0340824  0.0342008 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.02583e-06 ( -7.40201e-08  7.42323e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.29834     ( -0.208193   0.0658739 )
Epeak [keV] : 1.00000E+04      (   )
Norm@50keV  : 7.81083E-03    ( -0.000265572   0.000265549 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.69 using 59 PHA bins.
# Reduced chi-squared =          1.030 for     56 degrees of freedom 
# Null hypothesis probability =   4.123978e-01
 
Photon flux (15-150 keV)    in 26.37 sec: 0.928439 ( -0.034541  0.03369 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.02559e-06 ( -7.11621e-08  7.40944e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -2.10377E-02   ( 0.840431   0.840431 )
beta        : -1.32990    ( -0.0942185   0.0738253 )
Epeak [keV] : 42.5370      ( -42.6038 96.3493 )
Norm@50keV   : 6.16696E-02    ( -0.0627203   454.26 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.43 using 59 PHA bins.
# Reduced chi-squared =          1.026 for     55 degrees of freedom 
# Null hypothesis probability =   4.213846e-01
 
Photon flux (15-150 keV)    in 26.37 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)  = 1.97e-06
S(50-100 keV) = 2.51e-06

T90 vs. Hardness ratio plot

T90                                   = 238.008000016212 sec.
Hardness ratio (energy fluence ratio) = 1.27411

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.19345
Count Ratio (50-100 keV) / (15-25 keV) = 0.816416

Mask shadow pattern

IMX = 5.484465900865042E-01, IMY = -2.007623712409803E-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:
-239.872000 -10.344000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
288.7748  10.9375    1.8  36.9  117.9   2.4443   6.4    1.5	GRS 1915+105                  
299.5896  35.1950    0.6  43.3  157.9   7.8748  19.6    0.4	Cyg X-1                       
308.2579  40.9334    6.2  45.0  170.4   0.6090   1.8    6.8	Cyg X-3                       
326.0222  38.3288  222.9  40.3 -170.2  -0.0122  -0.1    7.0	Cyg X-2                       
331.0812   8.9220    2.7  13.2 -138.5   0.6725   4.3 ------	UNKNOWN                       
329.3924  54.7546    2.6  56.9 -169.2   2.8126   4.5 ------	UNKNOWN                       
339.0527  56.0991    2.7  59.4 -163.2   4.7131   4.2 ------	UNKNOWN                       
  7.8822 -30.3529    3.1  50.7  -44.5   3.3923   3.7 ------	UNKNOWN                       
  2.9809  12.6850    3.0  41.8 -104.7   3.2605   3.9 ------	UNKNOWN                       
  1.2843  26.3889    2.5  46.1 -123.7   3.6642   4.7 ------	UNKNOWN

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

Time interval of the image:
-10.344000 16.028600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
288.7755  10.9592   76.0  36.9  117.9  -0.0210  -0.2    1.6	GRS 1915+105                  
299.5466  35.0929    5.4  43.3  157.7  -0.2330  -2.1    6.9	Cyg X-1                       
308.2054  40.8177   29.5  44.9  170.3   0.0417   0.4    9.2	Cyg X-3                       
326.0085  38.3914    7.5  40.4 -170.2  -0.1200  -1.5    8.7	Cyg X-2                       
315.7055 -31.2648    0.3  30.3   20.1   3.0956  44.4 ------	UNKNOWN                       
324.7055  -7.8112    2.7   6.0   -4.4   0.2043   4.2 ------	UNKNOWN                       
  1.8340  14.4079    2.9  41.3 -107.8   0.7743   3.9 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
69.628600 387.628580
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
270.4319 -25.1294    7.2  40.1  106.6  -1.2239  -1.6    8.6	GX 5-1                        
270.2829 -25.6257    6.2  40.1  105.8  -1.3692  -1.8    7.1	GRS 1758-258                  
273.9684 -14.1233    4.3  41.8  124.0   1.9905   2.7    5.7	GX 17+2                       
276.0698 -30.3530   12.2  33.9  100.5  -0.3711  -0.9    7.5	H1820-303                     
285.0290 -24.9241   36.2  27.7  115.0   0.0818   0.3    0.4	HT1900.1-2455                 
288.8032  10.9316    1.6  49.5  163.7   4.3156   7.2    0.9	GRS 1915+105                  
296.1246 -17.1235    3.5  22.7  143.4   0.6507   3.3 ------	UNKNOWN                       
315.6992 -31.2649    0.4   0.0  140.5   4.7358  27.0 ------	UNKNOWN                       
339.2061 -15.7555    3.2  26.4 -101.0   0.8747   3.6 ------	UNKNOWN                       
313.0878  28.0294    3.3  59.4 -163.2   4.8124   3.5 ------	UNKNOWN                       
 11.8940 -32.7143    4.0  47.1  -53.1   2.9117   2.8 ------	UNKNOWN

Plot creation:
Sun May 31 10:31:35 EDT 2015