Special notes of this burst
Image
Pre-slew 15.0-350.0 keV image (Event data with DETECTION mask)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
341.9162 -57.8724 0.0172 53.9158 147.9355 28.9170864 11.127 TRIG_00652847
Foreground time interval of the image:
21.096 161.301 (delta_t = 140.205 [sec])
Background time interval of the image:
-239.000 21.096 (delta_t = 260.096 [sec])
Lightcurves
Notes:
- 1) The mask-weighted lightcurves have units of either count/det or counts/sec/det, where a det is 0.4 x 0.4 = 0.16 sq cm.
- 2) 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 (for the best duration plot, slew times are marked by green arrows).
- 3) For lightcurves in unit of count rate, 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) For long bursts, a spectral fit of 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.
- 4) For short bursts (T90<1sec), the specrtum is also fit with Blackbody, OTTB, and Double Blackbody.
Time averaged spectrum fit using an average DRM
Power-law model
Time interval is from 174.240 sec. to 330.744 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.93097 ( -0.331814 0.35792 )
Norm@50keV : 5.86132E-04 ( -0.000144105 0.000141046 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.89 using 59 PHA bins.
# Reduced chi-squared = 1.103 for 57 degrees of freedom
# Null hypothesis probability = 2.758257e-01
Photon flux (15-150 keV) in 156.5 sec: 8.52515E-02 ( -0.0175126 0.0175255 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.43751e-07 ( -1.97763e-07 2.04594e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 174.240 sec. to 330.744 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.607063 ( -2.9492 1.89231 )
Epeak [keV] : 42.1053 ( -8.95597 14.1571 )
Norm@50keV : 1.68954E-02 ( -0.0179153 0.780932 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.83 using 59 PHA bins.
# Reduced chi-squared = 1.015 for 56 degrees of freedom
# Null hypothesis probability = 4.437534e-01
Photon flux (15-150 keV) in 156.5 sec: 7.95172E-02 ( -0.0177062 0.0177957 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.13025e-07 ( -1.67375e-07 1.98638e-07 ) ergs/cm2
Band function
Time interval is from 174.240 sec. to 330.744 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.546121 ( -1.80217 2.96291 )
beta : -9.37167 ( 9.37167 19.3713 )
Epeak [keV] : 42.5289 ( -9.38362 13.8096 )
Norm@50keV : 1.54815E-02 ( -0.0154839 0.202489 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.83 using 59 PHA bins.
# Reduced chi-squared = 1.033 for 55 degrees of freedom
# Null hypothesis probability = 4.065749e-01
Photon flux (15-150 keV) in 156.5 sec: 7.99337E-02 ( ) 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] : 10.7443 (-1.84756 2.25608)
R^2/D10^2 : 3.28642E-02 (-0.0172199 0.0346241)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.11 using 59 PHA bins.
# Reduced chi-squared = 1.002 for 57 degrees of freedom
# Null hypothesis probability = 4.708227e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.234e-07 4.564e-08
25- 50 3.385e-07 1.083e-07
50-150 2.167e-07 1.092e-07
15-150 6.786e-07 2.049e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 66.9686 (-27.1418 68.1895)
Norm : 0.437450 (-0.117817 0.157136)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.73 using 59 PHA bins.
# Reduced chi-squared = 1.048 for 57 degrees of freedom
# Null hypothesis probability = 3.768288e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.748e-07 5.209e-08
25- 50 2.747e-07 8.598e-08
50-150 3.412e-07 2.373e-07
15-150 7.907e-07 3.160e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.02930 (-4.11957 -4.11957)
R1^2/D10^2 : 0.320979 (-0.316765 2.52774)
kT2 [keV] : 11.7397 (-2.625 -11.757)
R2^2/D10^2 : 2.15322E-02 (-0.0214204 0.039711)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.43 using 59 PHA bins.
# Reduced chi-squared = 1.026 for 55 degrees of freedom
# Null hypothesis probability = 4.212617e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.453e-07 6.974e-08
25- 50 3.180e-07 1.849e-07
50-150 2.456e-07 1.534e-07
15-150 7.089e-07 4.099e-07
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 2.49e-07
S(50-100 keV) = 2.61e-07
T90 vs. Hardness ratio plot
T90 = 168.944000005722 sec.
Hardness ratio (energy fluence ratio) = 1.04819
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.23145
Count Ratio (50-100 keV) / (15-25 keV) = 0.482332
Mask shadow pattern (with DETECTION mask)
IMX = 0, IMY = 0
TIME vs. PHA plot around the beginning of event data (event_start to event_start+0.64s) with DETECTION mask
TIME vs. DetID plot around the beginning of event data (event_start to event_start+0.64s) with DETECTION mask
100 us light curve (15-350 keV; (event_start to event_start+0.64s)
Spacecraft aspect plot
Bright source in the event data image
Event data image of 15-350 keV band
Time interval of the image:
21.096000 161.300590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.4440 -60.7362 25.5 49.2 -131.2 -0.3134 -0.5 7.8 Cen X-3
186.7031 -62.7299 1.9 41.2 -131.6 -1.8543 -6.2 2.7 GX 301-2
244.8753 -15.6334 6.8 28.9 -5.9 0.3267 1.7 6.0 Sco X-1
256.0084 -37.8082 6.2 6.6 35.3 0.3091 1.9 2.4 4U 1700-377
256.6458 -36.5018 5.9 8.0 34.8 0.3334 2.0 11.2 GX 349+2
262.9936 -24.7777 281.2 20.9 37.2 0.0077 0.0 2.1 GX 1+4
264.8795 -44.2624 0.0 9.0 106.3 0.1671 0.9 12.7 4U 1735-44
268.3628 -1.5936 8.7 44.6 32.3 0.5358 1.3 8.5 SW J1753.5-0127
270.4447 -25.0513 63.7 23.9 53.2 0.0400 0.2 8.9 GX 5-1
270.3172 -25.7591 5.9 23.2 54.0 -0.4208 -2.0 1.2 GRS 1758-258
274.0826 -14.1529 132.4 35.0 47.9 0.0287 0.1 8.3 GX 17+2
275.9784 -30.4986 6.2 22.9 71.6 -0.4155 -1.9 8.4 H1820-303
284.9511 -25.0459 15.2 32.5 74.6 0.2762 0.8 8.8 HT1900.1-2455
262.9638 -33.6875 6.1 13.1 51.9 -0.3359 -1.9 8.9 GX 354-0
341.9163 -57.8724 1.0 53.9 147.9 28.9060 11.1 ------ UNKNOWN
275.7159 -68.9716 1.9 27.9 171.4 1.2468 6.0 ------ UNKNOWN
61.2211 -75.1454 2.7 60.8 -174.2 9.3411 4.3 ------ UNKNOWN
236.7988 7.3264 2.5 53.0 -10.3 1.9269 4.7 ------ UNKNOWN
203.6642 -23.6111 2.5 44.4 -70.2 4.0111 4.6 ------ UNKNOWN
Webpage updated on:
Mon Jan 11 18:19:16 EST 2016