batgrbproduct analysis for trigger=302888

batgrbproduct Analysis for Trigger=302888

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 04:34:11 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger302888
======================================================================

  Trigger: 00302888      Segment: 000

  BAT Trigger Time: 224322608   [s; MET]
      Trigger Stop: 224322688   [s; MET]
               UTC: 2008-02-10T07:50:05.435780    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 251.269750345052   Dec: 13.8302696590224  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    17.85
     Image Trigger?:     YES
     Rate S/N Ratio:     0  [ if not an image trigger ]
     Image S/N Ratio:    17.85

  Flight Position:   [ source = BAT ]
    RA: 251.269750345052   Dec: 13.8302696590224  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 251.260042347957   Dec: 13.8246798058874  [deg; J2000]  
        { 16h 45m 02.4s , +13d 49' 28.8" }
         +/- 1.04893127348964 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.384236052001109 [arcmin] (formal 1-sigma fit error)
    SNR: 28.4105577698154
 
  Angular difference between Flight and Ground position is 0.657564 arcmin
 
  Partial Coding Fraction: 0.734375    [ including projection effects ]

  Duration
     T90: 42.2639999985695 +/- 11.3673740317139
        Measured from: -9.96799999475479
                   to: 32.2960000038147     [s; relative to TRIGTIME]
     T50: 11.8039999902248 +/- 2.08513694431325
        Measured from: -0.0839999914169312
                   to: 11.7199999988079     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 4.50400000810623     
                   to: 5.50400000810623     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -14.2639999985695     
                   to: 46.0239999890327     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.946831   1.184332   0.731852   0.245239
           0.050404   0.053645   0.049398   0.049587 [error]
 Peak      0.045826   0.066274   0.066179   0.017083
           0.006916   0.007754   0.007278   0.006643 [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 3.05e-07 4.91e-07 5.98e-07 1.43e-06 1.80e-06 2.82e-06   erg/cm2
              Error 2.89e-08 2.75e-08 4.99e-08 2.57e-07 1.14e-07 2.96e-07   erg/cm2
Peak flux Power-law 4.43e-01 5.10e-01 4.21e-01 5.85e-01 1.59e+00 1.96e+00   ph/cm2/s
              Error 9.63e-02 6.66e-02 5.90e-02 1.76e-01 1.86e-01 2.39e-01   ph/cm2/s
 
Fluence   Cutoff-PL 3.06e-07 4.92e-07 5.96e-07 1.41e-06 1.80e-06 2.80e-06   erg/cm2
              Error 2.85e-08 2.73e-08 4.97e-08 3.23e-07 1.13e-07 3.80e-07   erg/cm2
Peak flux Cutoff-PL 4.43e-01 5.10e-01 4.21e-01 5.80e-01 1.59e+00 1.95e+00   ph/cm2/s
              Error 8.24e-02 6.95e-02 6.34e-02 2.59e-01 1.86e-01 3.12e-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    1.716    0.108    -      -           3.23e-03 1.94e-04   53.020 57
CPL   2.106    0.000      43.0    0.0      2.03e-03 0.00e+00   52.480 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.275    0.208    -      -           1.34e-02 1.54e-03   50.410 57
CPL   1.271    1.467    9996.7    0.0      1.34e-02 1.56e-02   50.410 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: 19.584000 sec.
T50 in the 50-300 keV band: 7.360000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   60.288  -14.264   46.024
T90    42.264   -9.968   32.296
T50    11.804   -0.084   11.720
Peak    1.000    4.504    5.504

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
  251.2600    13.8247   0.0068    32.6131    -5.2418         3.2025242     28.411 TRIG_00302888                 
 
Foreground time interval of the image:
-14.264  46.024 (delta_t =  60.288 [sec])
Background time interval of the image:
-365.799 -267.890 (delta_t =  97.909 [sec])
-239.000 -14.264 (delta_t = 224.736 [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 80.000000

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 80.000000

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 80.000000

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  -14.264 sec. to   46.024 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.71641     ( -0.107387   0.108812 )
Norm@50keV  : 3.23203E-03    ( -0.000194764   0.000193033 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.02 using 59 PHA bins.
# Reduced chi-squared =         0.9301 for     57 degrees of freedom 
# Null hypothesis probability =   6.252694e-01
 
Photon flux (15-150 keV)    in 60.29 sec: 0.431740 ( -0.0243852  0.0244399 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.80194e-06 ( -1.13944e-07  1.14938e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from  -14.264 sec. to   46.024 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.10635     (     )
Epeak [keV] : 42.9771      (   )
Norm@50keV  : 2.03008E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.48 using 59 PHA bins.
# Reduced chi-squared =         0.9371 for     56 degrees of freedom 
# Null hypothesis probability =   6.089126e-01
 
Photon flux (15-150 keV)    in 60.29 sec: 0.431671 ( -0.024412  0.024264 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.79932e-06 ( -1.1235e-07  1.14557e-07 ) ergs/cm2

Band function

Time interval is from  -14.264 sec. to   46.024 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.26996   ( 1.2804   6.0667 )
beta        : -1.75616    ( -0.188896   0.140984 )
Epeak [keV] : 51.4709      ( -52.1789 -52.1789 )
Norm@50keV   : 6.34721E-03    ( -0.00303257   0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.78 using 59 PHA bins.
# Reduced chi-squared =         0.9597 for     55 degrees of freedom 
# Null hypothesis probability =   5.598773e-01
 
Photon flux (15-150 keV)    in 60.29 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]    : 12.1187  (  )
R^2/D10^2   : 9.57427E-02  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         149.66 using 59 PHA bins.
# Reduced chi-squared =         2.6256 for     57 degrees of freedom 
# Null hypothesis probability =   2.980553e-10
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.794e-07   1.987e-08
25- 50  5.713e-07   3.708e-08
50-150  5.078e-07   7.102e-08
15-150  1.258e-06   8.320e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 136.777       (      )
Norm        : 1.77081       (-0.117361     0.154365)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.67 using 59 PHA bins.
# Reduced chi-squared =          1.029 for     57 degrees of freedom 
# Null hypothesis probability =   4.138571e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.737e-07   2.351e-08
25- 50  5.017e-07   4.850e-08
50-150  9.600e-07   3.055e-07
15-150  1.735e-06   3.515e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 7.21692        (-0.948565      1.00568)
R1^2/D10^2  : 0.503479        (-0.183265      0.326912)
kT2 [keV]   : 33.4716        (-7.7936      15.4424)
R2^2/D10^2  : 2.06858E-03    (-0.00135843   0.00286806)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.72 using 59 PHA bins.
# Reduced chi-squared =         0.9404 for     55 degrees of freedom 
# Null hypothesis probability =   6.007320e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.823e-07   4.272e-08
25- 50  5.114e-07   7.126e-08
50-150  1.057e-06   5.040e-07
15-150  1.851e-06   4.320e-07

Peak spectrum fit

Power-law model

Time interval is from    4.504 sec. to    5.504 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.27455     ( -0.208018   0.207388 )
Norm@50keV  : 1.33552E-02    ( -0.00153988   0.00153544 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.41 using 59 PHA bins.
# Reduced chi-squared =         0.8844 for     57 degrees of freedom 
# Null hypothesis probability =   7.188926e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.58609 ( -0.185517  0.185874 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.32813e-07 ( -1.72992e-08  1.7475e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    4.504 sec. to    5.504 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.27074     ( -0.811472   2.12279 )
Epeak [keV] : 9996.73      (   )
Norm@50keV  : 1.34136E-02    ( -0.0134136   0.01771 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.41 using 59 PHA bins.
# Reduced chi-squared =         0.9002 for     56 degrees of freedom 
# Null hypothesis probability =   6.855168e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.58575 ( -0.18564  0.18554 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.3282e-07 ( -1.8244e-08  1.7401e-08 ) ergs/cm2

Band function

Time interval is from    4.504 sec. to    5.504 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.01387   ( 1.01521   1.01521 )
beta        : -1.27452    ( 1.27453   0.208241 )
Epeak [keV] : 47.8153      ( -46.7168 -46.7168 )
Norm@50keV   : 2.48045E-02    ( -0.0130143   1.99922 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.41 using 59 PHA bins.
# Reduced chi-squared =         0.9166 for     55 degrees of freedom 
# Null hypothesis probability =   6.503617e-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]    : 18.7053  (-2.85797  3.48382)
R^2/D10^2   : 8.81074E-02  (-0.0376954   0.0644898)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          69.54 using 59 PHA bins.
# Reduced chi-squared =          1.220 for     57 degrees of freedom 
# Null hypothesis probability =   1.231985e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.093e-09   1.360e-09
25- 50  2.898e-08   5.895e-09
50-150  7.429e-08   1.703e-08
15-150  1.094e-07   2.018e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (      )
Norm        : 6.52220       (-0.757024     0.756958)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.89 using 59 PHA bins.
# Reduced chi-squared =         0.9805 for     57 degrees of freedom 
# Null hypothesis probability =   5.167943e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.624e-08   9.005e-09
25- 50  3.124e-08   1.721e-08
50-150  6.852e-08   3.789e-08
15-150  1.160e-07   6.360e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.70527        (-2.23137      3.10825)
R1^2/D10^2  : 2.90142        (-2.26151      21.4438)
kT2 [keV]   : 27.0435        (-6.12561      13.4217)
R2^2/D10^2  : 2.33417E-02    (-0.0169425   0.01834)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.15 using 59 PHA bins.
# Reduced chi-squared =         0.9119 for     55 degrees of freedom 
# Null hypothesis probability =   6.599707e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.447e-08   7.793e-09
25- 50  2.711e-08   1.061e-08
50-150  9.017e-08   4.025e-08
15-150  1.318e-07   5.422e-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: 1.71641     ( -0.107387   0.108812 )
Norm@50keV  : 3.23203E-03    ( -0.000194764   0.000193033 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.02 using 59 PHA bins.
# Reduced chi-squared =         0.9301 for     57 degrees of freedom 
# Null hypothesis probability =   6.252694e-01
 
Photon flux (15-150 keV)    in 60.29 sec: 0.431740 ( -0.0243852  0.0244399 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.80194e-06 ( -1.13944e-07  1.14938e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.10635     (     )
Epeak [keV] : 42.9771      (   )
Norm@50keV  : 2.03008E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.48 using 59 PHA bins.
# Reduced chi-squared =         0.9371 for     56 degrees of freedom 
# Null hypothesis probability =   6.089126e-01
 
Photon flux (15-150 keV)    in 60.29 sec: 0.431671 ( -0.024412  0.024264 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.79932e-06 ( -1.1235e-07  1.14557e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.26996   ( 1.2804   6.02619 )
beta        : -1.75616    ( -0.188896   0.140984 )
Epeak [keV] : 51.4709      ( -52.1789 -52.1789 )
Norm@50keV   : 6.34721E-03    ( -0.00303257   0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.78 using 59 PHA bins.
# Reduced chi-squared =         0.9597 for     55 degrees of freedom 
# Null hypothesis probability =   5.598773e-01
 
Photon flux (15-150 keV)    in 60.29 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)  = 4.91e-07
S(50-100 keV) = 5.98e-07

T90 vs. Hardness ratio plot

T90                                   = 42.2639999985695 sec.
Hardness ratio (energy fluence ratio) = 1.21792

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.25084
Count Ratio (50-100 keV) / (15-25 keV) = 0.772949

Mask shadow pattern

IMX = 6.371740446585199E-01, IMY = 5.845579753707202E-02

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 80.000000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 80.000000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 80.000000

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:
-365.799400 -267.890000
-239.000000 -14.264000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.2862  35.3895    8.4  10.9   -0.3   0.3328   1.4    8.8	Her X-1                       
268.4204  -1.3706    5.7  48.1  -31.7   1.1746   2.0    5.8	SW J1753.5-0127               
288.8578  10.9470    8.4  43.5  -64.5   1.7392   1.4    3.5	GRS 1915+105                  
299.5873  35.1938    0.7  32.7 -103.9   7.6596  17.6    0.5	Cyg X-1                       
308.0461  40.9443    2.2  35.8 -118.5   2.3876   5.4    2.9	Cyg X-3                       
274.6472  -4.5640    2.7  52.5  -38.8   4.9999   4.3 ------	UNKNOWN                       
333.8677  44.5533    4.1  51.1 -135.7   3.3928   2.8 ------	UNKNOWN

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

Time interval of the image:
-14.264000 46.024000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.3164  35.4782    6.7  10.8   -0.3   0.1528   1.7   10.7	Her X-1                       
268.2839  -1.4414    6.5  48.1  -31.5  -0.4166  -1.8    5.1	SW J1753.5-0127               
288.9531  11.0025   10.5  43.5  -64.6  -0.4255  -1.1    9.7	GRS 1915+105                  
299.6166  35.1802    8.4  32.7 -103.9  -0.2403  -1.4    1.8	Cyg X-1                       
308.0040  40.8370    6.0  35.8 -118.3  -0.3192  -1.9    8.4	Cyg X-3                       
212.3093  61.7270    2.5  30.6  119.7   0.7222   4.6 ------	UNKNOWN                       
 59.0384  78.4053    2.3  55.2  166.5   2.5357   5.1 ------	UNKNOWN                       
251.2601  13.8247    0.4  32.6   -5.2   3.2028  28.4 ------	UNKNOWN                       
279.3414  29.7284    2.2  23.0  -70.8   0.5804   5.2 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
141.300600 457.800630
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9726 -15.6331    0.2  30.1   -6.5  17.1614  55.7    0.6	Sco X-1                       
254.3279  35.4575   20.1  21.8  168.1   0.1652   0.6    9.4	Her X-1                       
256.0233 -37.8146    4.4  51.8  -23.5   1.9204   2.6    2.5	4U 1700-377                   
256.6072 -36.3920   23.2  50.5  -24.3  -0.3265  -0.5    8.5	GX 349+2                      
262.9454 -24.8763   16.0  40.3  -35.2  -0.3305  -0.7    8.6	GX 1+4                        
268.3083  -1.5801    7.3  22.9  -67.6   0.5238   1.6    8.4	SW J1753.5-0127               
270.2677 -25.1333   13.5  43.1  -44.2   0.5014   0.9    3.4	GX 5-1                        
270.2758 -25.8727    5.4  43.8  -43.7  -1.3523  -2.1    7.9	GRS 1758-258                  
273.9091 -13.9391    3.8  35.7  -58.5  -1.4584  -3.1    8.1	GX 17+2                       
288.6307  10.9366    6.5  36.6 -108.5   1.1461   1.8    9.9	GRS 1915+105                  
299.5960  35.1828    1.2  48.3 -143.8   7.3144  10.0    1.2	Cyg X-1                       
308.0129  40.8094   13.0  56.0 -148.9   1.4878   0.9    9.7	Cyg X-3                       
263.0379 -33.7207    5.3  48.8  -31.7   1.4294   2.2    7.3	GX 354-0                      
219.5242 -12.5133    3.0  41.0   32.8   2.2837   3.9 ------	UNKNOWN                       
227.3301  -8.2745    2.7  32.4   29.8   1.5153   4.3 ------	UNKNOWN                       
249.7029 -36.4435    2.6  50.3  -17.0   2.8227   4.5 ------	UNKNOWN                       
244.5319 -44.2417    3.2  58.4  -13.0   6.1972   3.5 ------	UNKNOWN                       
267.3143 -26.6511    2.0  43.4  -39.8   2.8520   5.7 ------	UNKNOWN

Plot creation:
Sun May 31 08:22:36 EDT 2015