How to compute the Fourier transform of $e^{-2pi {mid x mid}}$?











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I want to compute the Fourier transform of $f(x)=e^{-2pi {mid x mid}}$ where $x$ is the vector in $mathbb{R}^n$. I know that the Fourier transform of a radial function is radial but cannot see how to use the fact to calculate the following integrate
begin{equation}
hat{f}(y)=int_{mathbb{R}^n} {e^{-2pi {mid x mid}}} e^{-2pi x cdot y } dx
end{equation}



Could anyone please help me?










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  • Use polar coordinates.
    – uniquesolution
    Nov 19 at 22:45










  • It is general n-dimensional. I cannot see how to use the polar coordinates.
    – Keith
    Nov 19 at 22:45










  • You can try writing $x=rphi$ with $rinmathbb R_+$ and $phiin S^{n-1}$.
    – Federico
    Nov 19 at 23:11










  • Look up the Hankel Transform and its relation to the Fourier Transform for cases of circular and spherical symmetry.
    – Andy Walls
    Nov 19 at 23:40










  • I just had a quick glance at the excellent lecture notes {see.stanford.edu/materials/lsoftaee261/chap8.pdf} but I didn't find an answer to your question.
    – Jean Marie
    Nov 20 at 0:22















up vote
0
down vote

favorite
1












I want to compute the Fourier transform of $f(x)=e^{-2pi {mid x mid}}$ where $x$ is the vector in $mathbb{R}^n$. I know that the Fourier transform of a radial function is radial but cannot see how to use the fact to calculate the following integrate
begin{equation}
hat{f}(y)=int_{mathbb{R}^n} {e^{-2pi {mid x mid}}} e^{-2pi x cdot y } dx
end{equation}



Could anyone please help me?










share|cite|improve this question
























  • Use polar coordinates.
    – uniquesolution
    Nov 19 at 22:45










  • It is general n-dimensional. I cannot see how to use the polar coordinates.
    – Keith
    Nov 19 at 22:45










  • You can try writing $x=rphi$ with $rinmathbb R_+$ and $phiin S^{n-1}$.
    – Federico
    Nov 19 at 23:11










  • Look up the Hankel Transform and its relation to the Fourier Transform for cases of circular and spherical symmetry.
    – Andy Walls
    Nov 19 at 23:40










  • I just had a quick glance at the excellent lecture notes {see.stanford.edu/materials/lsoftaee261/chap8.pdf} but I didn't find an answer to your question.
    – Jean Marie
    Nov 20 at 0:22













up vote
0
down vote

favorite
1









up vote
0
down vote

favorite
1






1





I want to compute the Fourier transform of $f(x)=e^{-2pi {mid x mid}}$ where $x$ is the vector in $mathbb{R}^n$. I know that the Fourier transform of a radial function is radial but cannot see how to use the fact to calculate the following integrate
begin{equation}
hat{f}(y)=int_{mathbb{R}^n} {e^{-2pi {mid x mid}}} e^{-2pi x cdot y } dx
end{equation}



Could anyone please help me?










share|cite|improve this question















I want to compute the Fourier transform of $f(x)=e^{-2pi {mid x mid}}$ where $x$ is the vector in $mathbb{R}^n$. I know that the Fourier transform of a radial function is radial but cannot see how to use the fact to calculate the following integrate
begin{equation}
hat{f}(y)=int_{mathbb{R}^n} {e^{-2pi {mid x mid}}} e^{-2pi x cdot y } dx
end{equation}



Could anyone please help me?







analysis fourier-analysis fourier-transform






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share|cite|improve this question













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edited Nov 19 at 23:05









Bernard

117k637109




117k637109










asked Nov 19 at 22:43









Keith

1,403920




1,403920












  • Use polar coordinates.
    – uniquesolution
    Nov 19 at 22:45










  • It is general n-dimensional. I cannot see how to use the polar coordinates.
    – Keith
    Nov 19 at 22:45










  • You can try writing $x=rphi$ with $rinmathbb R_+$ and $phiin S^{n-1}$.
    – Federico
    Nov 19 at 23:11










  • Look up the Hankel Transform and its relation to the Fourier Transform for cases of circular and spherical symmetry.
    – Andy Walls
    Nov 19 at 23:40










  • I just had a quick glance at the excellent lecture notes {see.stanford.edu/materials/lsoftaee261/chap8.pdf} but I didn't find an answer to your question.
    – Jean Marie
    Nov 20 at 0:22


















  • Use polar coordinates.
    – uniquesolution
    Nov 19 at 22:45










  • It is general n-dimensional. I cannot see how to use the polar coordinates.
    – Keith
    Nov 19 at 22:45










  • You can try writing $x=rphi$ with $rinmathbb R_+$ and $phiin S^{n-1}$.
    – Federico
    Nov 19 at 23:11










  • Look up the Hankel Transform and its relation to the Fourier Transform for cases of circular and spherical symmetry.
    – Andy Walls
    Nov 19 at 23:40










  • I just had a quick glance at the excellent lecture notes {see.stanford.edu/materials/lsoftaee261/chap8.pdf} but I didn't find an answer to your question.
    – Jean Marie
    Nov 20 at 0:22
















Use polar coordinates.
– uniquesolution
Nov 19 at 22:45




Use polar coordinates.
– uniquesolution
Nov 19 at 22:45












It is general n-dimensional. I cannot see how to use the polar coordinates.
– Keith
Nov 19 at 22:45




It is general n-dimensional. I cannot see how to use the polar coordinates.
– Keith
Nov 19 at 22:45












You can try writing $x=rphi$ with $rinmathbb R_+$ and $phiin S^{n-1}$.
– Federico
Nov 19 at 23:11




You can try writing $x=rphi$ with $rinmathbb R_+$ and $phiin S^{n-1}$.
– Federico
Nov 19 at 23:11












Look up the Hankel Transform and its relation to the Fourier Transform for cases of circular and spherical symmetry.
– Andy Walls
Nov 19 at 23:40




Look up the Hankel Transform and its relation to the Fourier Transform for cases of circular and spherical symmetry.
– Andy Walls
Nov 19 at 23:40












I just had a quick glance at the excellent lecture notes {see.stanford.edu/materials/lsoftaee261/chap8.pdf} but I didn't find an answer to your question.
– Jean Marie
Nov 20 at 0:22




I just had a quick glance at the excellent lecture notes {see.stanford.edu/materials/lsoftaee261/chap8.pdf} but I didn't find an answer to your question.
– Jean Marie
Nov 20 at 0:22










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From Bracewell, the n-dimensional Fourier Transform



$$F(s_1, dots, s_n) = int_{-infty}^{infty} dots int_{-infty}^{infty} f(x_1,dots, x_n) e^{-2pi i (x_1 s_1 + dots + x_n s_n)} space dx_1 dots dx_n $$



when there is n-dimensional symmetry, can be manipulated into



$$F(q) = dfrac{2pi}{q^{frac{1}{2}n-1}} int_{0}^{infty} f(r) J_{frac{1}{2}n-1}(2pi qr)space r^{frac{1}{2}n} space dr$$



Where $r$ and $q$ are the radii from the origin in the original domain and transform domain respectively.



So that the cases of $n=1$ and $n=3$ don't seem so foreign, it is probably worth noting that



$$J_{-frac{1}{2}}(x) = sqrt{dfrac{2}{pi x}}cos(x)$$
$$J_{frac{1}{2}}(x) = sqrt{dfrac{2}{pi x}}sin(x)$$



I'm not quite sure I know what you meant by $|x|$ in your original problem statement, but if you just meant the magnitude of $x$, then the specific transform you wanted to compute looks like



$$F(q) = dfrac{2pi}{q^{frac{1}{2}n-1}} int_{0}^{infty} e^{-2pi r} J_{frac{1}{2}n-1}(2pi qr)space r^{frac{1}{2}n} space dr$$



For $n=1$



$$begin{align*}F(q) &= 2pisqrt{q} int_{0}^{infty} e^{-2pi r} sqrt{dfrac{2}{pi(2pi qr)}}cos(2pi qr)space sqrt{r} space dr\
\
&= 2 int_{0}^{infty} e^{-2pi r} cos(2pi qr)space dr \
\
&=int_{0}^{infty} e^{-2pi r} left(e^{i2pi qr} + e^{-i2pi qr}right)space dr \
\
&= left[dfrac{e^{-2pi r}e^{i2pi qr}}{-2pi (1-iq)} + dfrac{e^{-2pi r}e^{-i2pi qr}}{-2pi (1+iq)}right]Biggr|_0^infty\
\
&= dfrac{1}{2pi}left[dfrac{1}{1-iq}+dfrac{1}{1+iq}right]\
\
&= dfrac{1}{2pi} dfrac{2}{1+q^2}
end{align*}$$



which is exactly what one would expect for the 1 dimensional Fourier Transform.



For $n=2$



$$begin{align*}F(q) &= 2pi int_{0}^{infty} e^{-2pi r} J_{0}(2pi qr)space r space dr\
\
&mbox{(Hankel Transform table lookup)}\
\
&= dfrac{2pi (2pi)}{left[(2pi q)^2 + (2pi)^2right]^{frac{3}{2}}}\
\
&= dfrac{1}{2pi} dfrac{1}{left(1+q^2right)^{frac{3}{2}}}
end{align*}$$



For $n =3$



$$begin{align*}F(q) &= dfrac{2pi}{sqrt{q}} int_{0}^{infty} e^{-2pi r} sqrt{dfrac{2}{pi(2pi qr)}}sin(2pi qr)space r^{frac{3}{2}} space dr \
\
&= dfrac{2}{q} int_{0}^{infty} e^{-2pi r} sin(2pi qr)space r space dr \
\
&mbox{(Wolfram Alpha invocation in lieu of integration by parts)}
\
&= dfrac{1}{(2pi)^2}dfrac{4}{(1+q^2)^2}\
end{align*}$$



And I suppose I'll let you keep on going until you see a pattern in terms of $n$ emerge.






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    From Bracewell, the n-dimensional Fourier Transform



    $$F(s_1, dots, s_n) = int_{-infty}^{infty} dots int_{-infty}^{infty} f(x_1,dots, x_n) e^{-2pi i (x_1 s_1 + dots + x_n s_n)} space dx_1 dots dx_n $$



    when there is n-dimensional symmetry, can be manipulated into



    $$F(q) = dfrac{2pi}{q^{frac{1}{2}n-1}} int_{0}^{infty} f(r) J_{frac{1}{2}n-1}(2pi qr)space r^{frac{1}{2}n} space dr$$



    Where $r$ and $q$ are the radii from the origin in the original domain and transform domain respectively.



    So that the cases of $n=1$ and $n=3$ don't seem so foreign, it is probably worth noting that



    $$J_{-frac{1}{2}}(x) = sqrt{dfrac{2}{pi x}}cos(x)$$
    $$J_{frac{1}{2}}(x) = sqrt{dfrac{2}{pi x}}sin(x)$$



    I'm not quite sure I know what you meant by $|x|$ in your original problem statement, but if you just meant the magnitude of $x$, then the specific transform you wanted to compute looks like



    $$F(q) = dfrac{2pi}{q^{frac{1}{2}n-1}} int_{0}^{infty} e^{-2pi r} J_{frac{1}{2}n-1}(2pi qr)space r^{frac{1}{2}n} space dr$$



    For $n=1$



    $$begin{align*}F(q) &= 2pisqrt{q} int_{0}^{infty} e^{-2pi r} sqrt{dfrac{2}{pi(2pi qr)}}cos(2pi qr)space sqrt{r} space dr\
    \
    &= 2 int_{0}^{infty} e^{-2pi r} cos(2pi qr)space dr \
    \
    &=int_{0}^{infty} e^{-2pi r} left(e^{i2pi qr} + e^{-i2pi qr}right)space dr \
    \
    &= left[dfrac{e^{-2pi r}e^{i2pi qr}}{-2pi (1-iq)} + dfrac{e^{-2pi r}e^{-i2pi qr}}{-2pi (1+iq)}right]Biggr|_0^infty\
    \
    &= dfrac{1}{2pi}left[dfrac{1}{1-iq}+dfrac{1}{1+iq}right]\
    \
    &= dfrac{1}{2pi} dfrac{2}{1+q^2}
    end{align*}$$



    which is exactly what one would expect for the 1 dimensional Fourier Transform.



    For $n=2$



    $$begin{align*}F(q) &= 2pi int_{0}^{infty} e^{-2pi r} J_{0}(2pi qr)space r space dr\
    \
    &mbox{(Hankel Transform table lookup)}\
    \
    &= dfrac{2pi (2pi)}{left[(2pi q)^2 + (2pi)^2right]^{frac{3}{2}}}\
    \
    &= dfrac{1}{2pi} dfrac{1}{left(1+q^2right)^{frac{3}{2}}}
    end{align*}$$



    For $n =3$



    $$begin{align*}F(q) &= dfrac{2pi}{sqrt{q}} int_{0}^{infty} e^{-2pi r} sqrt{dfrac{2}{pi(2pi qr)}}sin(2pi qr)space r^{frac{3}{2}} space dr \
    \
    &= dfrac{2}{q} int_{0}^{infty} e^{-2pi r} sin(2pi qr)space r space dr \
    \
    &mbox{(Wolfram Alpha invocation in lieu of integration by parts)}
    \
    &= dfrac{1}{(2pi)^2}dfrac{4}{(1+q^2)^2}\
    end{align*}$$



    And I suppose I'll let you keep on going until you see a pattern in terms of $n$ emerge.






    share|cite|improve this answer

























      up vote
      1
      down vote













      From Bracewell, the n-dimensional Fourier Transform



      $$F(s_1, dots, s_n) = int_{-infty}^{infty} dots int_{-infty}^{infty} f(x_1,dots, x_n) e^{-2pi i (x_1 s_1 + dots + x_n s_n)} space dx_1 dots dx_n $$



      when there is n-dimensional symmetry, can be manipulated into



      $$F(q) = dfrac{2pi}{q^{frac{1}{2}n-1}} int_{0}^{infty} f(r) J_{frac{1}{2}n-1}(2pi qr)space r^{frac{1}{2}n} space dr$$



      Where $r$ and $q$ are the radii from the origin in the original domain and transform domain respectively.



      So that the cases of $n=1$ and $n=3$ don't seem so foreign, it is probably worth noting that



      $$J_{-frac{1}{2}}(x) = sqrt{dfrac{2}{pi x}}cos(x)$$
      $$J_{frac{1}{2}}(x) = sqrt{dfrac{2}{pi x}}sin(x)$$



      I'm not quite sure I know what you meant by $|x|$ in your original problem statement, but if you just meant the magnitude of $x$, then the specific transform you wanted to compute looks like



      $$F(q) = dfrac{2pi}{q^{frac{1}{2}n-1}} int_{0}^{infty} e^{-2pi r} J_{frac{1}{2}n-1}(2pi qr)space r^{frac{1}{2}n} space dr$$



      For $n=1$



      $$begin{align*}F(q) &= 2pisqrt{q} int_{0}^{infty} e^{-2pi r} sqrt{dfrac{2}{pi(2pi qr)}}cos(2pi qr)space sqrt{r} space dr\
      \
      &= 2 int_{0}^{infty} e^{-2pi r} cos(2pi qr)space dr \
      \
      &=int_{0}^{infty} e^{-2pi r} left(e^{i2pi qr} + e^{-i2pi qr}right)space dr \
      \
      &= left[dfrac{e^{-2pi r}e^{i2pi qr}}{-2pi (1-iq)} + dfrac{e^{-2pi r}e^{-i2pi qr}}{-2pi (1+iq)}right]Biggr|_0^infty\
      \
      &= dfrac{1}{2pi}left[dfrac{1}{1-iq}+dfrac{1}{1+iq}right]\
      \
      &= dfrac{1}{2pi} dfrac{2}{1+q^2}
      end{align*}$$



      which is exactly what one would expect for the 1 dimensional Fourier Transform.



      For $n=2$



      $$begin{align*}F(q) &= 2pi int_{0}^{infty} e^{-2pi r} J_{0}(2pi qr)space r space dr\
      \
      &mbox{(Hankel Transform table lookup)}\
      \
      &= dfrac{2pi (2pi)}{left[(2pi q)^2 + (2pi)^2right]^{frac{3}{2}}}\
      \
      &= dfrac{1}{2pi} dfrac{1}{left(1+q^2right)^{frac{3}{2}}}
      end{align*}$$



      For $n =3$



      $$begin{align*}F(q) &= dfrac{2pi}{sqrt{q}} int_{0}^{infty} e^{-2pi r} sqrt{dfrac{2}{pi(2pi qr)}}sin(2pi qr)space r^{frac{3}{2}} space dr \
      \
      &= dfrac{2}{q} int_{0}^{infty} e^{-2pi r} sin(2pi qr)space r space dr \
      \
      &mbox{(Wolfram Alpha invocation in lieu of integration by parts)}
      \
      &= dfrac{1}{(2pi)^2}dfrac{4}{(1+q^2)^2}\
      end{align*}$$



      And I suppose I'll let you keep on going until you see a pattern in terms of $n$ emerge.






      share|cite|improve this answer























        up vote
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        From Bracewell, the n-dimensional Fourier Transform



        $$F(s_1, dots, s_n) = int_{-infty}^{infty} dots int_{-infty}^{infty} f(x_1,dots, x_n) e^{-2pi i (x_1 s_1 + dots + x_n s_n)} space dx_1 dots dx_n $$



        when there is n-dimensional symmetry, can be manipulated into



        $$F(q) = dfrac{2pi}{q^{frac{1}{2}n-1}} int_{0}^{infty} f(r) J_{frac{1}{2}n-1}(2pi qr)space r^{frac{1}{2}n} space dr$$



        Where $r$ and $q$ are the radii from the origin in the original domain and transform domain respectively.



        So that the cases of $n=1$ and $n=3$ don't seem so foreign, it is probably worth noting that



        $$J_{-frac{1}{2}}(x) = sqrt{dfrac{2}{pi x}}cos(x)$$
        $$J_{frac{1}{2}}(x) = sqrt{dfrac{2}{pi x}}sin(x)$$



        I'm not quite sure I know what you meant by $|x|$ in your original problem statement, but if you just meant the magnitude of $x$, then the specific transform you wanted to compute looks like



        $$F(q) = dfrac{2pi}{q^{frac{1}{2}n-1}} int_{0}^{infty} e^{-2pi r} J_{frac{1}{2}n-1}(2pi qr)space r^{frac{1}{2}n} space dr$$



        For $n=1$



        $$begin{align*}F(q) &= 2pisqrt{q} int_{0}^{infty} e^{-2pi r} sqrt{dfrac{2}{pi(2pi qr)}}cos(2pi qr)space sqrt{r} space dr\
        \
        &= 2 int_{0}^{infty} e^{-2pi r} cos(2pi qr)space dr \
        \
        &=int_{0}^{infty} e^{-2pi r} left(e^{i2pi qr} + e^{-i2pi qr}right)space dr \
        \
        &= left[dfrac{e^{-2pi r}e^{i2pi qr}}{-2pi (1-iq)} + dfrac{e^{-2pi r}e^{-i2pi qr}}{-2pi (1+iq)}right]Biggr|_0^infty\
        \
        &= dfrac{1}{2pi}left[dfrac{1}{1-iq}+dfrac{1}{1+iq}right]\
        \
        &= dfrac{1}{2pi} dfrac{2}{1+q^2}
        end{align*}$$



        which is exactly what one would expect for the 1 dimensional Fourier Transform.



        For $n=2$



        $$begin{align*}F(q) &= 2pi int_{0}^{infty} e^{-2pi r} J_{0}(2pi qr)space r space dr\
        \
        &mbox{(Hankel Transform table lookup)}\
        \
        &= dfrac{2pi (2pi)}{left[(2pi q)^2 + (2pi)^2right]^{frac{3}{2}}}\
        \
        &= dfrac{1}{2pi} dfrac{1}{left(1+q^2right)^{frac{3}{2}}}
        end{align*}$$



        For $n =3$



        $$begin{align*}F(q) &= dfrac{2pi}{sqrt{q}} int_{0}^{infty} e^{-2pi r} sqrt{dfrac{2}{pi(2pi qr)}}sin(2pi qr)space r^{frac{3}{2}} space dr \
        \
        &= dfrac{2}{q} int_{0}^{infty} e^{-2pi r} sin(2pi qr)space r space dr \
        \
        &mbox{(Wolfram Alpha invocation in lieu of integration by parts)}
        \
        &= dfrac{1}{(2pi)^2}dfrac{4}{(1+q^2)^2}\
        end{align*}$$



        And I suppose I'll let you keep on going until you see a pattern in terms of $n$ emerge.






        share|cite|improve this answer












        From Bracewell, the n-dimensional Fourier Transform



        $$F(s_1, dots, s_n) = int_{-infty}^{infty} dots int_{-infty}^{infty} f(x_1,dots, x_n) e^{-2pi i (x_1 s_1 + dots + x_n s_n)} space dx_1 dots dx_n $$



        when there is n-dimensional symmetry, can be manipulated into



        $$F(q) = dfrac{2pi}{q^{frac{1}{2}n-1}} int_{0}^{infty} f(r) J_{frac{1}{2}n-1}(2pi qr)space r^{frac{1}{2}n} space dr$$



        Where $r$ and $q$ are the radii from the origin in the original domain and transform domain respectively.



        So that the cases of $n=1$ and $n=3$ don't seem so foreign, it is probably worth noting that



        $$J_{-frac{1}{2}}(x) = sqrt{dfrac{2}{pi x}}cos(x)$$
        $$J_{frac{1}{2}}(x) = sqrt{dfrac{2}{pi x}}sin(x)$$



        I'm not quite sure I know what you meant by $|x|$ in your original problem statement, but if you just meant the magnitude of $x$, then the specific transform you wanted to compute looks like



        $$F(q) = dfrac{2pi}{q^{frac{1}{2}n-1}} int_{0}^{infty} e^{-2pi r} J_{frac{1}{2}n-1}(2pi qr)space r^{frac{1}{2}n} space dr$$



        For $n=1$



        $$begin{align*}F(q) &= 2pisqrt{q} int_{0}^{infty} e^{-2pi r} sqrt{dfrac{2}{pi(2pi qr)}}cos(2pi qr)space sqrt{r} space dr\
        \
        &= 2 int_{0}^{infty} e^{-2pi r} cos(2pi qr)space dr \
        \
        &=int_{0}^{infty} e^{-2pi r} left(e^{i2pi qr} + e^{-i2pi qr}right)space dr \
        \
        &= left[dfrac{e^{-2pi r}e^{i2pi qr}}{-2pi (1-iq)} + dfrac{e^{-2pi r}e^{-i2pi qr}}{-2pi (1+iq)}right]Biggr|_0^infty\
        \
        &= dfrac{1}{2pi}left[dfrac{1}{1-iq}+dfrac{1}{1+iq}right]\
        \
        &= dfrac{1}{2pi} dfrac{2}{1+q^2}
        end{align*}$$



        which is exactly what one would expect for the 1 dimensional Fourier Transform.



        For $n=2$



        $$begin{align*}F(q) &= 2pi int_{0}^{infty} e^{-2pi r} J_{0}(2pi qr)space r space dr\
        \
        &mbox{(Hankel Transform table lookup)}\
        \
        &= dfrac{2pi (2pi)}{left[(2pi q)^2 + (2pi)^2right]^{frac{3}{2}}}\
        \
        &= dfrac{1}{2pi} dfrac{1}{left(1+q^2right)^{frac{3}{2}}}
        end{align*}$$



        For $n =3$



        $$begin{align*}F(q) &= dfrac{2pi}{sqrt{q}} int_{0}^{infty} e^{-2pi r} sqrt{dfrac{2}{pi(2pi qr)}}sin(2pi qr)space r^{frac{3}{2}} space dr \
        \
        &= dfrac{2}{q} int_{0}^{infty} e^{-2pi r} sin(2pi qr)space r space dr \
        \
        &mbox{(Wolfram Alpha invocation in lieu of integration by parts)}
        \
        &= dfrac{1}{(2pi)^2}dfrac{4}{(1+q^2)^2}\
        end{align*}$$



        And I suppose I'll let you keep on going until you see a pattern in terms of $n$ emerge.







        share|cite|improve this answer












        share|cite|improve this answer



        share|cite|improve this answer










        answered Nov 21 at 0:05









        Andy Walls

        1,469127




        1,469127






























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