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fab13
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Hello,
I am working on Fisher's formalism in order to get constraints on cosmological parameters.
I am trying to do cross-correlation between 2 types of galaxy populations (LRG/ELG) into a total set of 3 types of population (BGS,LRG,ELG).
From the following article https://arxiv.org/pdf/0909.4544.pdf page 14, there is the following equation (63) :
As you can see, into eq(63), there is a sum on every pair of population types. In my case, I have 3 populations (BGS/LRG/ELG), so the term ##C^{-1}_{AB}## should have a size of 4x4 (with ##aa=BGS\quad##, ##bb=LRG\quad##, ##cc=ELG\quad## and ##bc=LRGxELG##) like this :
--------------------------------------------------------------------------------
##BGS\quad\quad\quad\quad 0\quad\quad\quad\quad 0\quad\quad\quad\quad 0##
##0\quad LRG\quad LRG/ELG\quad LRG/LRGxELG##
##0\quad LRG/ELG\quad ELG\quad ELG/LRGxELG##
##0\quad LRG/LRGxELG\quad ELG/LRGxELG\quad LRGxELG##
--------------------------------------------------------------------------------
But If I take eq(64), eq(65) and compare it with formula eq(63), I can't find the expression of the fourth element for power spectrum factor P_A, i.e when index A=4.
Indeed, If I follow what it is said in Paper, "where A,B label different pair of tracer populations"
I could identify ##P_{A}## to power spectrum for population ##A## and same for ##P_{B}## for population ##B##.
Finally, from your point of view, what's the size of ##C^{-1}_{AB}##, i.e 3x3 or 4x4 ?
and if this size is 4x4, how to sum on the A=B=4 with a power spectrum ##P_{A}## and ##P_{B}## ##(P_{\text{population}=4})## which is unknown since I have only 3 populations ?
On another hand, I think the non-diagonal terms on a covariance matrix 4x4 will transfer informations when I invert this one, and so I can only sum ##C^{-1}_{AB}## on 3 populations for the pair (A,B). I mean their contribution will remain after inversion.
I hope you will understand my issue on this sum. Regards
I am working on Fisher's formalism in order to get constraints on cosmological parameters.
I am trying to do cross-correlation between 2 types of galaxy populations (LRG/ELG) into a total set of 3 types of population (BGS,LRG,ELG).
From the following article https://arxiv.org/pdf/0909.4544.pdf page 14, there is the following equation (63) :
As you can see, into eq(63), there is a sum on every pair of population types. In my case, I have 3 populations (BGS/LRG/ELG), so the term ##C^{-1}_{AB}## should have a size of 4x4 (with ##aa=BGS\quad##, ##bb=LRG\quad##, ##cc=ELG\quad## and ##bc=LRGxELG##) like this :
--------------------------------------------------------------------------------
##BGS\quad\quad\quad\quad 0\quad\quad\quad\quad 0\quad\quad\quad\quad 0##
##0\quad LRG\quad LRG/ELG\quad LRG/LRGxELG##
##0\quad LRG/ELG\quad ELG\quad ELG/LRGxELG##
##0\quad LRG/LRGxELG\quad ELG/LRGxELG\quad LRGxELG##
--------------------------------------------------------------------------------
But If I take eq(64), eq(65) and compare it with formula eq(63), I can't find the expression of the fourth element for power spectrum factor P_A, i.e when index A=4.
Indeed, If I follow what it is said in Paper, "where A,B label different pair of tracer populations"
I could identify ##P_{A}## to power spectrum for population ##A## and same for ##P_{B}## for population ##B##.
Finally, from your point of view, what's the size of ##C^{-1}_{AB}##, i.e 3x3 or 4x4 ?
and if this size is 4x4, how to sum on the A=B=4 with a power spectrum ##P_{A}## and ##P_{B}## ##(P_{\text{population}=4})## which is unknown since I have only 3 populations ?
On another hand, I think the non-diagonal terms on a covariance matrix 4x4 will transfer informations when I invert this one, and so I can only sum ##C^{-1}_{AB}## on 3 populations for the pair (A,B). I mean their contribution will remain after inversion.
I hope you will understand my issue on this sum. Regards
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