pm_batse::getLogPF53 Interface Reference

Generate and return the conversion of an input natural logarithm of a bolometric ( \([0.0001, 20000]\kev\)) energy flux/fluence in units of \(\ergs\) over a given time to the photon flux/fluence over the same time in the BATSE detection energy range \([50, 300]\kev\).
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Detailed Description

Generate and return the conversion of an input natural logarithm of a bolometric ( \([0.0001, 20000]\kev\)) energy flux/fluence in units of \(\ergs\) over a given time to the photon flux/fluence over the same time in the BATSE detection energy range \([50, 300]\kev\).

See the Eqn A4 of Shahmoradi and Nemiroff 2015, MNRAS, Short versus long gamma-ray bursts for more details.

Parameters

[in]	logEpk	: The input scalar, or array of the same rank as other input array-valued arguments, of the same type and kind as logPPF64, containing the natural logarithm of the spectral peak energy of the GRB in units of \(\ergs\).
[in]	logPbol	: The input scalar or array of the same rank as the input arguments of same type and kind as logPPF64, containing the natural logarithm of the bolometric ( \([0.0001, 20000]\kev\)) energy flux of the GRB event in units of \(\ergs\) over the same time interval.

Returns

logPF53 : The output scalar, or array of the same rank as other input array-valued arguments, of type real of kind any supported by the processor (e.g., RK, RK32, RK64, or RK128), containing the natural logarithm of the Photon Flux of an event in units of \([\ms{photons} / \ms{sec}]\).

Possible calling interfaces ⛓

use pm_batse, only: getLogPF53
 
logPF53 = getLogPF53(logEpk, logPbol)

Remarks

The procedures under discussion are pure.

The procedures under discussion are elemental.

See also

getLogPbol
getLogPF53
getLog10PF53
getLogEffPPF
setBandEnergy
setBandPhoton
getCorrectionLogEffPPF

Example usage ⛓

program example
 
    use pm_kind, only: SK, IK, LK
    use pm_kind, only: RKG => RKH ! all processor kinds are supported.
    use pm_io, only: display_type
    use pm_batse, only: getLogPF53
 
    implicit none
 
    integer(IK) :: info
    type(display_type) :: disp
    disp = display_type(file = "main.out.F90")
 
    block
 
        use pm_kind, only: RKG => RKD
 
        call disp%skip()
        call disp%show("getLogPF53(logEpk = 2._RKG, logPbol = 0._RKG)")
        call disp%show( getLogPF53(logEpk = 2._RKG, logPbol = 0._RKG) )
        call disp%skip()
 
    end block
 
    !%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
    ! Output an example array for visualization.
    !%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
 
    block
 
        use pm_arraySpace, only: setLinSpace
        use pm_distBand, only: getBandEbreak, setBandPhoton
        real(RKG) :: logEpk(1000), photon, alpha = -1.1, beta = -2.3
        integer :: fileUnit, i
 
        call setLinSpace(logEpk, log(1.e-3_RKG), log(1.e5_RKG))
        open(newunit = fileUnit, file = "getLogPF53.RK.txt")
        do i = 1, size(logEpk)
            call setBandPhoton(photon, 50._RKG, 300._RKG, 1._RKG, 0.001_RKG, 20000._RKG, alpha, beta, getBandEbreak(alpha, beta, exp(logEpk(i))), info)
            if (info < 0) error stop
            write(fileUnit, "(*(g0,:,' '))") exp(logEpk(i)), exp(getLogPF53(logEpk(i), log(1.e-6_RKG))), photon
        end do
        close(fileUnit)
 
    end block
 
end program example

Example Unix compile command via Intel ifort compiler ⛓

#!/usr/bin/env sh
rm main.exe
ifort -fpp -standard-semantics -O3 -Wl,-rpath,../../../lib -I../../../inc main.F90 ../../../lib/libparamonte* -o main.exe
./main.exe

Example Windows Batch compile command via Intel ifort compiler ⛓

del main.exe
set PATH=..\..\..\lib;%PATH%
ifort /fpp /standard-semantics /O3 /I:..\..\..\include main.F90 ..\..\..\lib\libparamonte*.lib /exe:main.exe
main.exe

Example Unix / MinGW compile command via GNU gfortran compiler ⛓

#!/usr/bin/env sh
rm main.exe
gfortran -cpp -ffree-line-length-none -O3 -Wl,-rpath,../../../lib -I../../../inc main.F90 ../../../lib/libparamonte* -o main.exe
./main.exe

Example output ⛓

 
getLogPF53(logEpk = 2._RKG, logPbol = 0._RKG)
+13.836739091145450
 
 

Postprocessing of the example output ⛓

#!/usr/bin/env python
 
import matplotlib.pyplot as plt
import pandas as pd
import numpy as np
import glob
import sys
 
fontsize = 17
 
kind = "RK"
 
pattern = "*." + kind + ".txt"
fileList = glob.glob(pattern)
if len(fileList) == 1:
 
    df = pd.read_csv(fileList[0], delimiter = " ")
 
    fig = plt.figure(figsize = 1.25 * np.array([6.4, 4.8]), dpi = 200)
    ax = plt.subplot()
 
    plt.plot( df.values[:, 1]
            , df.values[:, 0]
            , linewidth = 2
            )
 
    plt.plot( df.values[:,2]
            , df.values[:, 0]
            , linewidth = 2
            )
 
    plt.xticks(fontsize = fontsize - 2)
    plt.yticks(fontsize = fontsize - 2)
    ax.set_xlabel("Photon flux in 50-300 keV range", fontsize = fontsize)
    ax.set_ylabel("Epeak [ keV ]", fontsize = fontsize)
    ax.set_xscale("log")
    ax.set_yscale("log")
 
    plt.grid(visible = True, which = "both", axis = "both", color = "0.85", linestyle = "-")
    ax.tick_params(axis = "y", which = "minor")
    ax.tick_params(axis = "x", which = "minor")
 
    ax.legend   ( ["getLogPF53()", "setBandPhoton()"]
                , fontsize = fontsize
               #, loc = "center left"
               #, bbox_to_anchor = (1, 0.5)
                )
 
    plt.savefig(fileList[0].replace(".txt",".png"))
 
else:
 
    sys.exit("Ambiguous file list exists.")

Visualization of the example output ⛓

Test:

test_pm_batse

Final Remarks ⛓

---

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For details on the naming conventions, see this page.
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Copyright

Computational Data Science Lab

Author:

Amir Shahmoradi, Wednesday June 27, 2012, 7:15 PM, Institute for Fusion Studies, The University of Texas at Austin.

Definition at line 548 of file pm_batse.F90.

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The documentation for this interface was generated from the following file:

• src/fortran/main/pm_batse.F90