Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minutes to calcaulte
Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
298.8556 +36.9215 0.0128 0.5 94.1 6.3459 14.9 TRIG_01218417
------------------------------------------
Foreground time interval of the image:
-172.960 -102.340 (delta_t = 70.620 [sec])
-101.000 -16.450 (delta_t = 84.550 [sec])
-15.000 72.901 (delta_t = 87.901 [sec])
Background time interval of the image:
-229.199 -172.960 (delta_t = 56.239 [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)
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
-172.960000 -102.340000
-101.000000 -16.450000
-15.000000 120.740000
121.000000 128.660000
131.000000 131.890000
133.000000 257.920000
259.000000 266.676000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.86781 ( -0.0687868 0.0695499 )
Norm@50keV : 1.71968E-03 ( -6.63402e-05 6.60342e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.39 using 59 PHA bins.
# Reduced chi-squared = 1.095 for 57 degrees of freedom
# Null hypothesis probability = 2.905556e-01
Photon flux (15-150 keV) in 432.1 sec: 0.243489 ( -0.0092065 0.00923269 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.83128e-06 ( -2.63413e-07 2.64459e-07 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
-172.960000 -102.340000
-101.000000 -16.450000
-15.000000 120.740000
121.000000 128.660000
131.000000 131.890000
133.000000 257.920000
259.000000 266.676000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.33873 ( -0.309898 0.289939 )
Epeak [keV] : 59.8993 ( -7.95006 17.4942 )
Norm@50keV : 3.20708E-03 ( -0.000909466 0.00138474 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.19 using 59 PHA bins.
# Reduced chi-squared = 0.9319 for 56 degrees of freedom
# Null hypothesis probability = 6.199138e-01
Photon flux (15-150 keV) in 432.1 sec: 0.234350 ( -0.010305 0.010355 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.51131e-06 ( -3.11112e-07 3.1297e-07 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
-172.960000 -102.340000
-101.000000 -16.450000
-15.000000 120.740000
121.000000 128.660000
131.000000 131.890000
133.000000 257.920000
259.000000 266.676000
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.34961 ( -0.244789 0.263971 )
beta : -9.37144 ( 9.37163 19.3716 )
Epeak [keV] : 60.3237 ( -8.16422 17.0734 )
Norm@50keV : 3.16173E-03 ( -0.000836512 0.000333746 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.19 using 59 PHA bins.
# Reduced chi-squared = 0.9490 for 55 degrees of freedom
# Null hypothesis probability = 5.825106e-01
Photon flux (15-150 keV) in 432.1 sec: 0.234521 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 6.50596e-06 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 12.4905 ( )
R^2/D10^2 : 4.74605E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 189.26 using 59 PHA bins.
# Reduced chi-squared = 3.3203 for 57 degrees of freedom
# Null hypothesis probability = 4.287029e-16
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.783e-07 4.775e-08
25- 50 2.235e-06 9.096e-08
50-150 2.152e-06 1.761e-07
15-150 5.066e-06 1.923e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 93.4634 (-11.6131 14.4738)
Norm : 1.07245 (-0.0597231 0.0646161)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.210e-06 8.685e-08
25- 50 2.064e-06 8.296e-08
50-150 3.215e-06 8.275e-07
15-150 6.489e-06 8.188e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.54585 (-0.801992 0.918497)
R1^2/D10^2 : 0.614368 (-0.266687 0.545365)
kT2 [keV] : 18.5741 (-1.76866 2.37913)
R2^2/D10^2 : 8.59401E-03 (-0.00341224 0.00447168)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.214e-06 1.789e-07
25- 50 2.004e-06 1.992e-07
50-150 3.084e-06 2.886e-07
15-150 6.302e-06 5.920e-07
Peak spectrum fit
Power-law model
Time interval is from 77.704 sec. to 78.704 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.59518 ( -0.39823 0.419155 )
Norm@50keV : 5.01133E-03 ( -0.00124569 0.00119946 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.19 using 59 PHA bins.
# Reduced chi-squared = 0.9508 for 57 degrees of freedom
# Null hypothesis probability = 5.810489e-01
Photon flux (15-150 keV) in 1 sec: 0.643022 ( -0.143585 0.143683 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.68941e-08 ( -1.22643e-08 1.26253e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 77.704 sec. to 78.704 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.57154 ( -1.53161 1.17013 )
Epeak [keV] : 863.796 ( -831.581 -831.581 )
Norm@50keV : 5.15824E-03 ( -0.00142609 0.0308558 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.19 using 59 PHA bins.
# Reduced chi-squared = 0.9677 for 56 degrees of freedom
# Null hypothesis probability = 5.436140e-01
Photon flux (15-150 keV) in 1 sec: 0.642126 ( -0.144444 0.14421 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.65929e-08 ( -1.29466e-08 1.287e-08 ) ergs/cm2
Band function
Time interval is from 77.704 sec. to 78.704 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -2.94857 ( 3.28998 2.94857 )
beta : -1.59519 ( -0.419173 0.398234 )
Epeak [keV] : 86.8857 ( -86.8857 -86.8857 )
Norm@50keV : 0.681109 ( -0.169306 0.163029 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.19 using 59 PHA bins.
# Reduced chi-squared = 0.9853 for 55 degrees of freedom
# Null hypothesis probability = 5.054301e-01
Photon flux (15-150 keV) in 1 sec: 0.641939 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 4.64468e-08 ( 0 0 ) ergs/cm2
Single BB
XSPEC: quit
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 15.0284 (-4.077 5.48442)
R^2/D10^2 : 7.05770E-02 (-0.0468496 0.143954)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.336e-09 1.695e-09
25- 50 1.328e-08 6.401e-09
50-150 2.043e-08 1.254e-08
15-150 3.704e-08 1.817e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 180.777 (-117.8 -186.265)
Norm : 2.62005 (-0.588964 0.78862)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.604e-09 3.889e-09
25- 50 1.255e-08 7.115e-09
50-150 2.662e-08 1.585e-08
15-150 4.578e-08 2.614e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.57745 (-2.3481 3.41044)
R1^2/D10^2 : 3.56092 (-3.15653 151.442)
kT2 [keV] : 21.6925 (-6.83266 16.8287)
R2^2/D10^2 : 1.68137E-02 (-0.0142509 0.0277907)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.474e-09 4.279e-09
25- 50 1.086e-08 5.705e-09
50-150 2.724e-08 1.647e-08
15-150 4.557e-08 2.545e-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: 1.85534 ( -0.079379 0.080407 )
Norm@50keV : 1.87795E-03 ( -8.64803e-05 8.59395e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.07 using 59 PHA bins.
# Reduced chi-squared = 1.142 for 57 degrees of freedom
# Null hypothesis probability = 2.162130e-01
Photon flux (15-150 keV) in 243.1 sec: 0.264540 ( -0.0114852 0.0115086 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.19741e-06 ( -1.9374e-07 1.94794e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.43797 ( -0.345099 0.319745 )
Epeak [keV] : 62.6723 ( -11.4112 51.1261 )
Norm@50keV : 3.11593E-03 ( -0.0009808 0.00158723 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.00 using 59 PHA bins.
# Reduced chi-squared = 1.071 for 56 degrees of freedom
# Null hypothesis probability = 3.328601e-01
Photon flux (15-150 keV) in 243.1 sec: 0.257592 ( -0.012552 0.01257 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.03257e-06 ( -2.28781e-07 2.30362e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.41667 ( -0.334125 5.92832 )
beta : -2.31790 ( 2.34833 0.486574 )
Epeak [keV] : 61.2775 ( -42.1922 49.3769 )
Norm@50keV : 3.20520E-03 ( -0.00107369 0.0498745 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.90 using 59 PHA bins.
# Reduced chi-squared = 1.089 for 55 degrees of freedom
# Null hypothesis probability = 3.025130e-01
Photon flux (15-150 keV) in 243.1 sec: 0.257273 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 4.02897e-06 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 1.97e-06
S(50-100 keV) = 2.16e-06
T90 vs. Hardness ratio plot
T90 = 326.587999939919 sec.
Hardness ratio (energy fluence ratio) = 1.09645
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.1463
Count Ratio (50-100 keV) / (15-25 keV) = 0.688153
Mask shadow pattern
IMX = -6.159227398753745E-04, IMY = -8.517028254098689E-03
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:
-229.199400 -172.960000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4105 35.2215 8.7 36.1 65.5 -0.3660 -1.3 7.6 Her X-1
268.3599 -1.3242 4.7 47.6 8.1 0.5634 2.5 7.7 SW J1753.5-0127
274.1027 -14.0506 83.2 56.0 -6.1 -0.0603 -0.1 5.7 GX 17+2
288.9716 10.9599 5.5 27.3 -13.4 0.2626 2.1 10.2 GRS 1915+105
299.3339 35.1690 0.0 1.4 -36.4 0.2473 2.0 12.7 Cyg X-1
308.1102 40.9665 14.1 8.1 -161.2 -0.0914 -0.8 0.8 Cyg X-3
325.9504 38.3141 9.3 21.1 -138.8 -0.1674 -1.2 10.4 Cyg X-2
275.0183 54.7000 2.9 24.6 109.1 0.5711 4.0 ------ UNKNOWN
267.7490 4.2463 2.5 43.4 13.4 1.0011 4.5 ------ UNKNOWN
266.1544 -11.3173 2.6 57.2 3.6 2.7597 4.4 ------ UNKNOWN
299.1695 36.7026 0.6 0.2 91.8 2.1910 18.4 ------ UNKNOWN
322.7743 20.8541 2.5 25.8 -94.8 0.7024 4.5 ------ UNKNOWN
329.5423 8.1595 2.0 39.5 -87.6 2.6459 5.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-172.960000 -102.340000
-101.000000 -16.450000
-15.000000 72.900590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4729 35.2944 7.7 36.0 65.6 -1.2669 -1.5 3.0 Her X-1
268.3426 -1.3408 5.3 47.6 8.1 -1.9934 -2.2 6.9 SW J1753.5-0127
273.9159 -14.0128 6.1 56.0 -5.9 -3.4654 -1.9 5.4 GX 17+2
288.7636 11.1382 0.0 27.2 -12.9 -0.9170 -1.9 11.7 GRS 1915+105
299.3451 35.1623 7.4 1.4 -36.8 -0.7435 -1.6 12.3 Cyg X-1
308.2185 41.0805 21.7 8.2 -161.6 0.2273 0.5 9.1 Cyg X-3
326.3113 38.2250 4.9 21.4 -138.6 -1.1181 -2.3 8.8 Cyg X-2
268.0718 6.5123 2.4 41.5 15.1 3.5267 4.9 ------ UNKNOWN
319.3417 60.5801 2.1 27.1 165.6 2.6619 5.4 ------ UNKNOWN
275.4567 10.3610 2.5 34.0 9.4 2.4172 4.6 ------ UNKNOWN
298.8555 36.9208 0.8 0.5 94.1 6.4099 15.1 ------ UNKNOWN
279.7752 -12.0607 2.1 52.0 -11.5 6.2426 5.5 ------ UNKNOWN
301.5965 -9.2724 2.1 45.9 -39.2 5.4367 5.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
80.900590 120.740000
121.000000 128.660000
131.000000 131.890000
133.000000 257.920000
259.000000 362.999800
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5583 35.4536 4.7 35.5 65.6 -2.5284 -2.5 8.3 Her X-1
268.4758 -1.4588 7.1 47.6 7.5 -1.2881 -1.6 6.5 SW J1753.5-0127
274.1415 -13.9973 15.1 56.0 -6.4 1.0647 0.8 8.2 GX 17+2
288.5967 10.8880 0.0 27.6 -13.5 -0.5506 -1.1 12.4 GRS 1915+105
299.8469 35.2336 0.0 1.8 -61.3 -0.3322 -0.8 12.7 Cyg X-1
307.9091 40.9709 5.6 8.1 -158.9 0.7975 2.0 9.2 Cyg X-3
326.2090 38.5323 0.0 21.6 -138.6 -0.0808 -0.2 12.8 Cyg X-2
263.0432 29.5638 2.8 30.7 51.0 2.6827 4.2 ------ UNKNOWN
354.9666 65.3142 2.6 43.0 174.7 3.4035 4.4 ------ UNKNOWN
327.2001 60.0776 2.8 29.4 173.0 2.1180 4.1 ------ UNKNOWN
298.6373 37.0049 0.5 0.3 88.2 10.1525 24.4 ------ UNKNOWN
Plot creation:
Sun Mar 3 20:39:44 EST 2024