#XSPEC version: 12.11.0 #Build Date/Time: Mon Apr 13 12:38:19 2020 # !XSPEC12> show # #XSPEC version: 12.11.0 # #Mon Jun 1 00:27:10 2020 # Auto-saving is done after every command. # Fit statistic in use: Chi-Squared # Minimization technique: Levenberg-Marquardt # Convergence criterion = 0.01 # Parameter fit deltas: 0.01 * parValue #Using chain rule to calculate statistic derivatives (faster method). # Querying disabled - will not continue fitting. # Prefit-renorming enabled. # Solar abundance table: angr # Photoionization Cross-Section Table: # bcmc: Balucinska-Church and McCammon, 1998 # Cosmology in use: H0 = 70 q0 = 0 Lambda0 = 0.73 # Model data directory: /software/lheasoft/release/x86_64-pc-linux-gnu-libc2.12/../spectral/manager/../modelData/ # Plot settings: # Showing of individual additive components is OFF. # Showing of background spectra is OFF. # Effective area normalization is OFF. # Current unit settings: # Energy = keV # Wavelength = angstrom, with Y-Axis displayed per Hz # X-Axis data display mode: Channels # Spectra plots will be shifted to source frame by redshift value z: 0 # Device: /null # Plotting of line IDs is OFF. # Splashpage is ON. # xlog for data plots is ON. # ylog for data plots is OFF. # # Default plot rebin settings for all plot groups: # Min. Signif. Max. # Bins Error Type # 0.00000 1 quad # # Responses read: # ../sw00957271000b_preslew.rsp associated with spectrum 1 source 1 # energies: 204 channels: 80 # Distinct RMF files: # ../sw00957271000b_preslew.rsp # #1 file 1 spectrum #Spectrum 1 Spectral Data File: ../sw00957271000b_preslew.pha #Net count rate (cts/s) for Spectrum:1 1.792e-02 +/- 1.918e-03 # Assigned to Data Group 1 and Plot Group 1 # Noticed Channels: 4-62 # Telescope: SWIFT Instrument: BAT Channel Type: PI # Exposure Time: 31.1 sec # Using fit statistic: chi # Using Response (RMF) File ../sw00957271000b_preslew.rsp for Source 1 # # Spectral data counts: 0.557325 # Model predicted rate: 1.80138E-02 # # #Current model list: # #======================================================================== #Model npow<1> Source No.: 1 Active/On #Model Model Component Parameter Unit Value # par comp # 1 1 npow PhoIndex 1.25433 +/- 0.183368 # 2 1 npow enorm keV 50.0000 frozen # 3 1 npow norm 1.20606E-03 +/- 1.23283E-04 #________________________________________________________________________ # # Using energies from responses. # #Fit statistic : Chi-Squared 46.81 using 59 bins. # #Test statistic : Chi-Squared 46.81 using 59 bins. # Null hypothesis probability of 8.30e-01 with 57 degrees of freedom # !XSPEC12> flux 20.0 50.0 # Model Flux 0.062226 photons (3.2071e-09 ergs/cm^2/s) range (20.000 - 50.000 keV) # !XSPEC12> flux 50.0 150.0 # Model Flux 0.057799 photons (8.2191e-09 ergs/cm^2/s) range (50.000 - 150.00 keV) # !XSPEC12> error 1 # Parameter Confidence Range (2.706) # 1 0.942744 1.55559 (-0.311591,0.301252) # !XSPEC12> error 3 # Parameter Confidence Range (2.706) # 3 0.00100324 0.00140885 (-0.000202819,0.000202795) # !XSPEC12> flux 15.0 350.0 err 100 90 #Parameter distribution is derived from fit covariance matrix. # Model Flux 0.17751 photons (2.5007e-08 ergs/cm^2/s) range (15.000 - 350.00 keV) # Error range 0.1506 - 0.2182 (1.746e-08 - 3.572e-08) (90.00% confidence) # !XSPEC12> flux 15.0 150.0 err 100 90 #Parameter distribution is derived from fit covariance matrix. # Model Flux 0.14275 photons (1.2058e-08 ergs/cm^2/s) range (15.000 - 150.00 keV) # Error range 0.1211 - 0.1663 (1.005e-08 - 1.458e-08) (90.00% confidence) # !XSPEC12> flux 15.0 25.0 err 100 90 #Parameter distribution is derived from fit covariance matrix. # Model Flux 0.039238 photons (1.2239e-09 ergs/cm^2/s) range (15.000 - 25.000 keV) # Error range 0.02886 - 0.05249 (9.048e-10 - 1.630e-09) (90.00% confidence) # !XSPEC12> flux 25.0 50.0 err 100 90 #Parameter distribution is derived from fit covariance matrix. # Model Flux 0.045709 photons (2.6148e-09 ergs/cm^2/s) range (25.000 - 50.000 keV) # Error range 0.03646 - 0.05603 (2.094e-09 - 3.178e-09) (90.00% confidence) # !XSPEC12> flux 50.0 100.0 err 100 90 #Parameter distribution is derived from fit covariance matrix. # Model Flux 0.038322 photons (4.3844e-09 ergs/cm^2/s) range (50.000 - 100.00 keV) # Error range 0.03096 - 0.04514 (3.539e-09 - 5.199e-09) (90.00% confidence) # !XSPEC12> flux 100.0 150.0 err 100 90 #Parameter distribution is derived from fit covariance matrix. # Model Flux 0.019477 photons (3.8347e-09 ergs/cm^2/s) range (100.00 - 150.00 keV) # Error range 0.01393 - 0.02585 (2.730e-09 - 5.109e-09) (90.00% confidence) # !XSPEC12> flux 100.0 350.0 err 100 90 #Parameter distribution is derived from fit covariance matrix. # Model Flux 0.054237 photons (1.6784e-08 ergs/cm^2/s) range (100.00 - 350.00 keV) # Error range 0.03467 - 0.07527 (1.034e-08 - 2.405e-08) (90.00% confidence) # !XSPEC12> log none #