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Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
266.8238 -28.1834 0.0230 10.8 -48.9 1.3002 8.3 TRIG_00431582
------------------------------------------
Foreground time interval of the image:
-34.512 113.868 (delta_t = 148.380 [sec])
Background time interval of the image:
-198.499 -34.512 (delta_t = 163.987 [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
Time interval is from -34.512 sec. to 113.868 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 4.85130 ( -0.618804 0.611039 )
Norm@50keV : 6.85634E-05 ( -3.17523e-05 5.36722e-05 )
------------------------------------------------------------
# Chi-Squared = 51.96 using 59 PHA bins.
# Reduced chi-squared = 0.9116 for 57 degrees of freedom
# Null hypothesis probability = 6.640769e-01
Photon flux (15-150 keV) in 148.4 sec: 9.18959E-02 ( -0.0120145 0.0120151 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.43587e-07 ( -6.28149e-08 6.44682e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -34.512 sec. to 113.868 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00000 ( )
Epeak [keV] : 50.0000 ( )
Norm@50keV : 1.03193E-03 ( )
------------------------------------------------------------
# Chi-Squared = 149.88 using 59 PHA bins.
# Reduced chi-squared = 2.6765 for 56 degrees of freedom
# Null hypothesis probability = 1.672260e-10
Photon flux (15-150 keV) in 148.4 sec: 9.18179E-02 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 4.27147e-07 ( -6.14955e-08 7.41807e-08 ) ergs/cm2
Band function
Time interval is from -34.512 sec. to 113.868 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -2.02203 ( 2.02203 2.02203 )
beta : -4.81298 ( -0.646351 0.5806 )
Epeak [keV] : 0.160383 ( -0.160383 -0.160383 )
Norm@50keV : 3.64495 ( -3.64495 6.05717e+06 )
------------------------------------------------------------
# Chi-Squared = 51.95 using 59 PHA bins.
# Reduced chi-squared = 0.9446 for 55 degrees of freedom
# Null hypothesis probability = 5.918724e-01
Photon flux (15-150 keV) in 148.4 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 75.904 sec. to 76.904 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.03761 ( -0.858643 1.12617 )
Norm@50keV : 1.98754E-03 ( -0.00120354 0.00104173 )
------------------------------------------------------------
# Chi-Squared = 46.44 using 59 PHA bins.
# Reduced chi-squared = 0.8148 for 57 degrees of freedom
# Null hypothesis probability = 8.398662e-01
Photon flux (15-150 keV) in 1 sec: 0.303519 ( -0.117202 0.117204 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.8375e-08 ( -8.92825e-09 9.94354e-09 ) ergs/cm2
Cutoff power-law model
Time interval is from 75.904 sec. to 76.904 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.19443 ( )
Epeak [keV] : 79.7505 ( )
Norm@50keV : 1.54223E-03 ( )
------------------------------------------------------------
# Chi-Squared = 46.27 using 59 PHA bins.
# Reduced chi-squared = 0.8262 for 56 degrees of freedom
# Null hypothesis probability = 8.198599e-01
Photon flux (15-150 keV) in 1 sec: 0.303379 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.83898e-08 ( -8.91321e-09 9.9371e-09 ) ergs/cm2
Band function
Time interval is from 75.904 sec. to 76.904 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.98595 ( -137.886 -137.886 )
beta : -2.03039 ( -1.78064 0.84457 )
Epeak [keV] : 17.7060 ( -17.6408 12.4073 )
Norm@50keV : 3169.86 ( -3306.75 91557.5 )
------------------------------------------------------------
# Chi-Squared = 46.37 using 59 PHA bins.
# Reduced chi-squared = 0.8431 for 55 degrees of freedom
# Null hypothesis probability = 7.898136e-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: 4.85130 ( -0.618804 0.611039 )
Norm@50keV : 6.85634E-05 ( -3.17523e-05 5.36722e-05 )
------------------------------------------------------------
# Chi-Squared = 51.96 using 59 PHA bins.
# Reduced chi-squared = 0.9116 for 57 degrees of freedom
# Null hypothesis probability = 6.640769e-01
Photon flux (15-150 keV) in 148.4 sec: 9.18959E-02 ( -0.0120145 0.0120151 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.43587e-07 ( -6.28149e-08 6.44682e-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 : 1.03193E-03 ( )
------------------------------------------------------------
# Chi-Squared = 149.88 using 59 PHA bins.
# Reduced chi-squared = 2.6765 for 56 degrees of freedom
# Null hypothesis probability = 1.672260e-10
Photon flux (15-150 keV) in 148.4 sec: 9.18179E-02 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 4.27147e-07 ( -6.14955e-08 7.41807e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -2.02203 ( 2.02203 2.02203 )
beta : -4.81298 ( -0.646351 0.5806 )
Epeak [keV] : 0.160383 ( -0.160383 -0.160383 )
Norm@50keV : 3.64495 ( -3.64495 6.05698e+06 )
------------------------------------------------------------
# Chi-Squared = 51.95 using 59 PHA bins.
# Reduced chi-squared = 0.9446 for 55 degrees of freedom
# Null hypothesis probability = 5.918724e-01
Photon flux (15-150 keV) in 148.4 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) = 9.05561e-08
S(50-100 keV) = 1.28858e-08
T90 vs. Hardness ratio plot
T90 = 125.007999956608 sec.
Hardness ratio (energy fluence ratio) = 0.142296
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.164728
Count Ratio (50-100 keV) / (15-25 keV) = 0.0346484
Mask shadow pattern
IMX = 1.255214169728081E-01, IMY = 1.440236157690285E-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:
-198.499400 -34.512000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9796 -15.6400 0.4 34.6 -52.6 6.5776 29.8 0.0 Sco X-1
256.1267 -37.9248 4.6 18.1 -95.9 0.4016 2.5 8.2 4U 1700-377
256.2953 -36.3560 7.4 17.8 -90.9 0.2534 1.6 7.9 GX 349+2
262.9418 -24.8342 3.0 15.6 -45.6 0.5437 3.9 6.5 GX 1+4
264.7401 -44.5185 6.2 14.9 -127.0 0.2781 1.9 4.1 4U 1735-44
268.3726 -1.4681 2.8 33.3 -3.1 0.7823 4.2 1.0 SW J1753.5-0127
270.3195 -25.0709 1.5 10.7 -25.1 1.0822 7.8 2.0 GX 5-1
270.4936 -25.8620 0.0 9.9 -27.1 0.0402 0.3 12.6 GRS 1758-258
273.9523 -14.0404 4.5 19.8 3.3 0.3744 2.6 3.1 GX 17+2
275.8487 -30.4797 4.6 3.5 -14.3 0.3672 2.5 7.8 H1820-303
285.1160 -24.8484 5.8 10.8 52.5 0.2671 2.0 6.1 HT1900.1-2455
288.7243 10.9836 3.1 45.7 29.4 1.4789 3.8 4.9 GRS 1915+105
345.1860 -56.3084 2.6 50.4 152.6 2.9242 4.4 ------ UNKNOWN
266.5611 -32.1833 1.5 9.5 -70.6 1.0824 7.6 ------ UNKNOWN
259.2545 20.9697 2.5 57.3 -6.4 3.2451 4.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-34.512000 113.868000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9244 -15.5358 5.4 34.7 -52.5 -0.5035 -2.1 7.0 Sco X-1
255.7917 -37.7046 0.0 18.3 -95.1 0.3636 2.0 12.5 4U 1700-377
256.6243 -36.4734 10.4 17.5 -91.3 -0.2010 -1.1 9.6 GX 349+2
263.1276 -24.6975 4.8 15.5 -44.8 -0.3966 -2.4 7.1 GX 1+4
264.8369 -44.5397 3.6 14.9 -127.2 -0.5276 -3.1 6.7 4U 1735-44
268.3859 -1.2957 8.7 33.4 -3.0 0.2613 1.3 9.5 SW J1753.5-0127
270.3903 -24.9921 3.4 10.7 -24.6 -0.5024 -3.5 7.8 GX 5-1
270.3543 -25.6257 8.8 10.2 -26.8 0.1975 1.4 7.6 GRS 1758-258
274.0793 -13.8670 4.8 20.0 3.7 0.3955 2.4 11.0 GX 17+2
275.7236 -30.2815 4.9 3.7 -14.4 0.3781 2.3 11.6 H1820-303
285.2246 -25.0070 189.1 10.7 53.4 0.0091 0.1 11.5 HT1900.1-2455
288.6754 10.9254 17.2 45.7 29.3 -0.3048 -0.7 7.3 GRS 1915+105
327.3582 -57.1752 2.2 40.8 155.1 1.4546 5.2 ------ UNKNOWN
266.8238 -28.1834 1.4 10.8 -48.9 1.3002 8.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
378.100590 963.015400
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
12.5116 -4.0532 2.9 25.1 100.5 1.5031 3.9 ------ UNKNOWN
66.6452 8.9801 3.4 30.5 -80.1 1.4983 3.4 ------ UNKNOWN
Plot creation:
Sat Aug 14 11:01:56 EDT 2010