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Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
268.5649 -26.3115 0.0261 18.3 22.4 1.1940 7.4 TRIG_00449907
------------------------------------------
Foreground time interval of the image:
-42.008 71.101 (delta_t = 113.109 [sec])
Background time interval of the image:
-137.599 -42.008 (delta_t = 95.591 [sec])
Lightcurves
Notes:
- 1) All plots contain as much data as has been downloaded to date.
- 2) The mask-weighted light curves are using the flight position.
- 3) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
- 4) 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.
- 5) 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.
- 6) 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 64.000000
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 64.000000
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 64.000000
SN=5 or 10 sec. binning (whichever binning is satisfied first)
SN=5 or 10 sec. binning (T < 200 sec)
The mask-weighted light curves based on cleaned DPHs
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 the pre-slew DRM
Power-law model
Multiple GTIs in the spectrum
tstart tstop
-42.008000 113.135300
114.000000 664.508000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 4.25179 ( -0.235773 0.24746 )
Norm@50keV : 1.64676E-04 ( -3.14356e-05 3.48051e-05 )
------------------------------------------------------------
# Chi-Squared = 64.09 using 59 PHA bins.
# Reduced chi-squared = 1.124 for 57 degrees of freedom
# Null hypothesis probability = 2.419396e-01
Photon flux (15-150 keV) in 705.7 sec: 0.126935 ( -0.00936333 0.00942001 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.09238e-06 ( -2.12757e-07 2.12797e-07 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
-42.008000 113.135300
114.000000 664.508000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00000 ( )
Epeak [keV] : 50.0000 ( )
Norm@50keV : 1.15332E-03 ( )
------------------------------------------------------------
# Chi-Squared = 380.44 using 59 PHA bins.
# Reduced chi-squared = 6.7935 for 56 degrees of freedom
# Null hypothesis probability = 9.077256e-50
Photon flux (15-150 keV) in 705.7 sec: 0.126842 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.86248e-06 ( -2.307e-07 2.3492e-07 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
-42.008000 113.135300
114.000000 664.508000
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.41864 ( )
beta : -9.37167 ( )
Epeak [keV] : 35.9849 ( )
Norm@50keV : 9.46430E-04 ( )
------------------------------------------------------------
# Chi-Squared = 328.86 using 59 PHA bins.
# Reduced chi-squared = 5.9793 for 55 degrees of freedom
# Null hypothesis probability = 1.172262e-40
Photon flux (15-150 keV) in 705.7 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] : ( )
R^2/D10^2 : ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25
25- 50
50-150
15-150
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : ( )
Norm : ( )
------------------------------------------------------------
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25
25- 50
50-150
15-150
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : ( )
R1^2/D10^2 : ( )
kT2 [keV] : ( )
R2^2/D10^2 : ( )
------------------------------------------------------------
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25
25- 50
50-150
15-150
Peak spectrum fit
Power-law model
Time interval is from 44.052 sec. to 45.052 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.36389 ( -1.16971 0.97781 )
Norm@50keV : 2.58407E-03 ( -0.00109494 0.00102051 )
------------------------------------------------------------
# Chi-Squared = 44.77 using 59 PHA bins.
# Reduced chi-squared = 0.7855 for 57 degrees of freedom
# Null hypothesis probability = 8.801335e-01
Photon flux (15-150 keV) in 1 sec: 0.311988 ( -0.311991 0.131343 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.5179e-08 ( -1.1412e-08 1.17513e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 44.052 sec. to 45.052 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.36396 ( -1.37958 0.980441 )
Epeak [keV] : 9999.36 ( -9988.12 -9988.12 )
Norm@50keV : 2.59249E-03 ( -0.00110531 0.00813844 )
------------------------------------------------------------
# Chi-Squared = 44.78 using 59 PHA bins.
# Reduced chi-squared = 0.7996 for 56 degrees of freedom
# Null hypothesis probability = 8.591747e-01
Photon flux (15-150 keV) in 1 sec: 0.311810 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.51689e-08 ( -1.14156e-08 1.17597e-08 ) ergs/cm2
Band function
Time interval is from 44.052 sec. to 45.052 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.05842 ( 1.05662 1.05662 )
beta : -1.35440 ( 1.35989 1.16762 )
Epeak [keV] : 44.2947 ( -47.3311 -47.3311 )
Norm@50keV : 5.06559E-03 ( -0.00508505 8.43193 )
------------------------------------------------------------
# Chi-Squared = 44.77 using 59 PHA bins.
# Reduced chi-squared = 0.8140 for 55 degrees of freedom
# Null hypothesis probability = 8.361195e-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] : ( )
R^2/D10^2 : ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25
25- 50
50-150
15-150
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : ( )
Norm : ( )
------------------------------------------------------------
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25
25- 50
50-150
15-150
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : ( )
R1^2/D10^2 : ( )
kT2 [keV] : ( )
R2^2/D10^2 : ( )
------------------------------------------------------------
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25
25- 50
50-150
15-150
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: 3.63812 ( -0.326152 0.360037 )
Norm@50keV : 3.09445E-04 ( -8.78178e-05 9.95934e-05 )
------------------------------------------------------------
# Chi-Squared = 55.22 using 59 PHA bins.
# Reduced chi-squared = 0.9689 for 57 degrees of freedom
# Null hypothesis probability = 5.419595e-01
Photon flux (15-150 keV) in 113.1 sec: 0.140176 ( -0.0150213 0.0150216 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.008e-07 ( -7.35684e-08 7.62665e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00000 ( )
Epeak [keV] : 50.0000 ( )
Norm@50keV : 1.97345E-03 ( )
------------------------------------------------------------
# Chi-Squared = 160.77 using 59 PHA bins.
# Reduced chi-squared = 2.8708 for 56 degrees of freedom
# Null hypothesis probability = 4.639500e-12
Photon flux (15-150 keV) in 113.1 sec: 0.140100 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 5.4763e-07 ( -6.9259e-08 7.94527e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.32891 ( )
beta : -9.21312 ( )
Epeak [keV] : 46.1945 ( )
Norm@50keV : 1.48641E-03 ( )
------------------------------------------------------------
# Chi-Squared = 149.91 using 59 PHA bins.
# Reduced chi-squared = 2.7256 for 55 degrees of freedom
# Null hypothesis probability = 9.900788e-11
Photon flux (15-150 keV) in 113.1 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) = 7.77427e-07
S(50-100 keV) = 1.63106e-07
T90 vs. Hardness ratio plot
T90 = 613.887999951839 sec.
Hardness ratio (energy fluence ratio) = 0.209802
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.269069
Count Ratio (50-100 keV) / (15-25 keV) = 0.0142874
Mask shadow pattern
IMX = 3.052683427969461E-01, IMY = -1.260931387263530E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
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:
-137.599400 -42.008000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
245.0049 -15.6676 1.1 32.9 70.7 2.3288 10.2 2.2 Sco X-1
254.5974 35.4690 3.3 51.2 148.3 -2.0941 -3.5 10.2 Her X-1
256.1065 -37.7435 3.4 33.7 25.9 0.5311 3.4 8.3 4U 1700-377
256.3618 -36.2475 3.3 32.5 27.5 0.5223 3.5 11.1 GX 349+2
262.9146 -24.8759 3.7 20.5 37.0 0.3683 3.1 9.4 GX 1+4
264.7592 -44.3760 6.5 35.8 10.0 0.2783 1.8 4.5 4U 1735-44
268.4663 -1.4334 9.7 13.5 125.3 0.1351 1.2 6.0 SW J1753.5-0127
270.2839 -25.0796 2.7 16.4 20.1 0.5033 4.3 0.0 GX 5-1
270.2871 -25.7707 234.5 17.0 18.9 0.0059 0.0 1.9 GRS 1758-258
274.1089 -14.1644 5.8 5.5 42.2 0.2241 2.0 9.7 GX 17+2
276.0871 -30.2344 4.1 19.8 -0.9 0.3189 2.8 11.6 H1820-303
285.1293 -24.9327 3.1 15.7 -29.9 0.4143 3.8 5.1 HT1900.1-2455
288.7975 10.9391 1.0 23.9 -160.8 1.3769 11.6 0.4 GRS 1915+105
299.5508 35.3368 7.1 50.1 -164.2 0.4470 1.6 8.3 Cyg X-1
308.1049 40.9446 4.7 58.4 -160.7 1.9175 2.4 0.5 Cyg X-3
250.3410 -30.2159 2.7 32.7 42.1 0.7691 4.3 ------ UNKNOWN
298.9227 17.0899 2.4 34.3 -150.3 0.6566 4.9 ------ UNKNOWN
317.3953 30.0295 4.5 55.3 -145.3 1.9489 2.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-42.008000 71.100600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.8703 -15.6956 4.6 33.0 70.6 0.8386 2.5 7.1 Sco X-1
254.6254 35.5039 3.4 51.3 148.3 2.9239 3.4 12.7 Her X-1
255.9875 -37.8357 240.1 33.9 25.9 -0.0117 -0.0 0.5 4U 1700-377
256.3169 -36.2346 0.0 32.5 27.5 -0.4994 -2.1 12.7 GX 349+2
263.1910 -24.6338 0.0 20.2 37.0 0.1458 0.8 12.0 GX 1+4
264.5927 -44.3901 5.9 35.9 10.1 -0.4464 -2.0 7.4 4U 1735-44
268.3668 -1.4470 636.3 13.5 125.0 0.0029 0.0 0.3 SW J1753.5-0127
270.2031 -25.0163 609.2 16.4 20.4 0.0031 0.0 5.8 GX 5-1
270.1594 -25.6312 22.2 17.0 19.5 0.0899 0.5 10.2 GRS 1758-258
274.0030 -13.8850 10.1 5.4 45.2 0.1765 1.1 9.1 GX 17+2
275.7396 -30.4967 0.0 20.1 -0.1 0.1039 0.7 12.4 H1820-303
285.0336 -25.0693 13.3 15.8 -29.4 -0.1380 -0.9 8.9 HT1900.1-2455
288.8760 10.8890 2.7 23.9 -160.6 -0.6912 -4.2 5.7 GRS 1915+105
299.4565 35.0876 11.6 49.8 -164.2 0.3624 1.0 9.5 Cyg X-1
308.1432 40.9190 3.0 58.3 -160.7 -3.1212 -3.8 2.5 Cyg X-3
246.3558 -54.8873 2.2 51.0 16.3 2.9436 5.1 ------ UNKNOWN
268.5634 -26.3118 1.5 18.3 22.4 1.2144 7.5 ------ UNKNOWN
319.1691 15.8052 2.1 48.2 -129.4 3.4304 5.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
115.000600 963.073600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9745 -15.6437 0.3 24.5 110.5 24.8137 34.1 0.4 Sco X-1
255.8851 -37.8139 8.8 15.8 39.4 0.6827 1.3 5.1 4U 1700-377
256.4929 -36.4627 2.5 14.5 42.0 2.4026 4.6 3.7 GX 349+2
263.0211 -24.7485 2.0 5.3 105.3 3.1488 5.9 0.7 GX 1+4
264.8510 -44.4960 19.5 18.4 8.0 0.3037 0.6 5.4 4U 1735-44
268.3566 -1.4311 2.7 24.9 178.7 2.3797 4.3 1.5 SW J1753.5-0127
270.2626 -25.1052 1.9 1.9 -129.9 3.8560 6.2 2.0 GX 5-1
270.3200 -25.7246 7.4 1.6 -111.6 1.1097 1.8 1.5 GRS 1758-258
274.0424 -14.0548 2.6 13.3 -157.1 2.6911 4.4 2.4 GX 17+2
275.7990 -30.3612 24.9 7.5 -56.2 0.2560 0.5 6.5 H1820-303
285.1329 -24.7901 6.2 14.9 -92.8 1.0409 1.9 9.4 HT1900.1-2455
288.7968 10.9676 1.5 42.1 -150.3 7.9209 7.7 1.3 GRS 1915+105
241.0786 2.0084 2.5 38.9 131.9 6.0735 4.5 ------ UNKNOWN
247.2950 -63.6859 3.5 39.9 14.0 2.8639 3.4 ------ UNKNOWN
264.6589 8.8592 3.0 35.4 172.6 2.6788 3.9 ------ UNKNOWN
263.0337 -33.8436 2.2 9.0 30.8 2.8508 5.3 ------ UNKNOWN
268.6239 -26.3073 0.9 0.0 111.4 6.9912 12.3 ------ UNKNOWN
275.4379 30.5710 3.4 57.3 -173.6 8.5005 3.4 ------ UNKNOWN
284.1722 18.2898 4.0 47.1 -160.3 3.5062 2.9 ------ UNKNOWN
299.1551 20.3760 5.2 55.3 -145.2 10.7263 2.2 ------ UNKNOWN
325.6972 -48.4279 3.7 49.1 -48.1 10.9026 3.2 ------ UNKNOWN
Plot creation:
Thu Mar 24 14:48:04 EDT 2011