Special notes of this burst
Image
15.0-350.0 keV image (Event data with DETECTION mask)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
219.8240 -25.2364 0.0094 41.3808 77.7865 28.5629485 20.633 TRIG_00745797
Foreground time interval of the image:
-27.104 50.605 (delta_t = 77.709 [sec])
Background time interval of the image:
-131.195 -27.104 (delta_t = 104.091 [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.
- 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 56.700 sec. to 242.496 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.51480 ( -0.118421 0.118727 )
Norm@50keV : 2.20437E-03 ( -0.000143329 0.000142976 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.35 using 59 PHA bins.
# Reduced chi-squared = 1.111 for 57 degrees of freedom
# Null hypothesis probability = 2.624303e-01
Photon flux (15-150 keV) in 185.8 sec: 0.276308 ( -0.018512 0.018569 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.87664e-06 ( -2.73299e-07 2.7496e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 56.700 sec. to 242.496 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.51618 ( -0.157876 0.116146 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 2.20664E-03 ( -0.000507137 0.000774694 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.37 using 59 PHA bins.
# Reduced chi-squared = 1.132 for 56 degrees of freedom
# Null hypothesis probability = 2.325820e-01
Photon flux (15-150 keV) in 185.8 sec: 0.277438 ( -0.023788 0.021511 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.9136e-06 ( -3.11581e-07 2.37047e-07 ) ergs/cm2
Band function
Time interval is from 56.700 sec. to 242.496 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.02757 ( 1.02913 1.02913 )
beta : -1.53310 ( -0.173372 0.133229 )
Epeak [keV] : 56.9407 ( -53.6627 -53.6627 )
Norm@50keV : 4.78800E-03 ( -0.00301462 255799 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.12 using 59 PHA bins.
# Reduced chi-squared = 1.148 for 55 degrees of freedom
# Null hypothesis probability = 2.111987e-01
Photon flux (15-150 keV) in 185.8 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] : 15.4139 ( )
R^2/D10^2 : 2.71644E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 145.60 using 59 PHA bins.
# Reduced chi-squared = 2.5544 for 57 degrees of freedom
# Null hypothesis probability = 1.080687e-09
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.499e-07 3.103e-08
25- 50 1.018e-06 9.392e-08
50-150 1.665e-06 2.067e-07
15-150 2.932e-06 2.397e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-37.8363 -200)
Norm : 1.12253 (-0.0720918 0.0720918)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.05 using 59 PHA bins.
# Reduced chi-squared = 1.176 for 57 degrees of freedom
# Null hypothesis probability = 1.704699e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.212e-07 3.874e-08
25- 50 1.003e-06 9.141e-08
50-150 2.199e-06 4.810e-07
15-150 3.723e-06 6.354e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.97273 (-1.11264 1.29837)
R1^2/D10^2 : 0.324599 (-0.145308 0.28888)
kT2 [keV] : 31.6654 (-6.06891 11.0321)
R2^2/D10^2 : 1.91091E-03 (-0.00114478 0.00199572)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.75 using 59 PHA bins.
# Reduced chi-squared = 1.123 for 55 degrees of freedom
# Null hypothesis probability = 2.474991e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.230e-07 1.231e-07
25- 50 9.770e-07 1.697e-07
50-150 2.453e-06 6.998e-07
15-150 3.953e-06 9.773e-07
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 9.66e-07
S(50-100 keV) = 1.35e-06
T90 vs. Hardness ratio plot
T90 = 165.31200003624 sec.
Hardness ratio (energy fluence ratio) = 1.39752
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.4405
Count Ratio (50-100 keV) / (15-25 keV) = 1.07452
Mask shadow pattern (with DETECTION mask)
IMX = 1.863853558528538E-01, IMY = -8.610831229835769E-01
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:
-27.104000 50.604600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
245.0193 -15.5905 4.4 23.8 113.6 -0.6572 -2.6 3.8 Sco X-1
256.1332 -38.0218 0.0 12.4 34.8 -0.1799 -1.1 12.7 4U 1700-377
256.2902 -36.2461 0.0 11.2 41.0 0.1280 0.7 12.7 GX 349+2
262.8677 -24.5779 0.0 5.4 137.5 -0.4946 -2.8 12.7 GX 1+4
264.5410 -44.4380 7.3 15.5 -1.0 -0.2661 -1.6 8.7 4U 1735-44
268.2219 -1.5752 23.6 27.5 177.9 -0.1003 -0.5 11.4 SW J1753.5-0127
270.1271 -25.0954 4.4 5.1 -144.8 -0.4512 -2.6 8.6 GX 5-1
270.2859 -25.7696 7.7 4.7 -138.2 0.2708 1.5 1.8 GRS 1758-258
274.0533 -14.0183 6.8 16.6 -159.1 -0.3009 -1.7 3.0 GX 17+2
275.8760 -30.2177 9.6 8.3 -85.2 -0.2052 -1.2 9.3 H1820-303
285.1141 -24.7743 3.2 17.2 -105.8 -0.5875 -3.6 9.7 HT1900.1-2455
288.8859 11.0761 8.4 45.6 -154.3 -0.3515 -1.4 9.4 GRS 1915+105
263.0403 -33.8545 81.6 5.7 23.8 -0.0239 -0.1 2.8 GX 354-0
224.0955 -16.1367 3.4 40.9 92.9 4.1724 3.4 ------ UNKNOWN
219.8240 -25.2364 0.6 41.4 77.8 28.5590 20.6 ------ UNKNOWN
283.2185 -26.1987 2.5 15.1 -102.6 0.7911 4.7 ------ UNKNOWN
Webpage updated on:
Wed Apr 26 16:41:20 EDT 2017