what's the difference of the 'SubfindDMDensity' between PartType0,1,4
Di Yihuan
7 Jan '20
Hi TNG teams and other friends,
I wonder what's the difference of the 'SubfindDMDensity' between PartType0,1,4? if they are the same thing?
And does the Density and SubfindDensity in the PartType0 mean rho(x,y,z) (N,3)and rho(r)(N)?
if I try to picture a gas mean density profile with r, is it better to using SubfindDensity than Density?
Thanks in advance.
Yihuan
Dylan Nelson
13 Jan '20
Hello,
Yes SubfindDMDensity is the same measurement for all particle types. Note that this is a local estimate, so it is valid at the position of that gas/DM/star particle.
All such values, including Density and SubfindDensity, are estimates at the precise Coordinates value (x,y,z) of that cell or particle.
There is no rho(r) data, you would need to compute this by first computing r of cells/particles (from the halo center), then binning.
For gas density, you have two options: use average/median values of PartType0/Density at the r you are interested in, or else sum all PartType0/Masses in a bin, i.e. spherical shell, around r, and then normalize by the volume of that bin.
Di Yihuan
13 Jan '20
I got it. Thanks again.
Yun Wang
18 Aug '20
Are 'SubfindDMDensity' and 'SubfindDensity' the same thing?
Dylan Nelson
18 Aug '20
Hi Yun,
No exactly, the first is "dark matter density" and the second is "total density" (i.e., also including baryons).
But since DM dominates, they are going to be generally quite similar.
Yun Wang
18 Aug '20
Do you mean that "SubfindDensity' contains all kinds of particle types?
Dylan Nelson
18 Aug '20
That's correct, all particle types = DM + baryons.
Yun Wang
18 Aug '20
So, does that mean I can use "SubfindDensity" and "coordinates" to compute the power spectrum of all matter (DM + baryons) directly?
Dylan Nelson
18 Aug '20
Hello,
It depends what your goal is, I would read again the description of SubfindDensity carefully. This is a local mass density estimate, at the location of each Coordinates, which is based on an adaptive-size smoothing kernel.
Personally I would not have thought to use it to compute a power spectrum, but instead the combination of Masses and Coordinates which gives the (un-smoothed) mass distribution within the simulation volume.
Hi TNG teams and other friends,
I wonder what's the difference of the 'SubfindDMDensity' between PartType0,1,4? if they are the same thing?
And does the Density and SubfindDensity in the PartType0 mean rho(x,y,z) (N,3)and rho(r)(N)?
if I try to picture a gas mean density profile with r, is it better to using SubfindDensity than Density?
Thanks in advance.
Yihuan
Hello,
Yes
SubfindDMDensity
is the same measurement for all particle types. Note that this is a local estimate, so it is valid at the position of that gas/DM/star particle.All such values, including
Density
andSubfindDensity
, are estimates at the preciseCoordinates
value (x,y,z) of that cell or particle.There is no
rho(r)
data, you would need to compute this by first computingr
of cells/particles (from the halo center), then binning.For gas density, you have two options: use average/median values of
PartType0/Density
at ther
you are interested in, or else sum allPartType0/Masses
in a bin, i.e. spherical shell, aroundr
, and then normalize by the volume of that bin.I got it. Thanks again.
Are 'SubfindDMDensity' and 'SubfindDensity' the same thing?
Hi Yun,
No exactly, the first is "dark matter density" and the second is "total density" (i.e., also including baryons).
But since DM dominates, they are going to be generally quite similar.
Do you mean that "SubfindDensity' contains all kinds of particle types?
That's correct, all particle types = DM + baryons.
So, does that mean I can use "SubfindDensity" and "coordinates" to compute the power spectrum of all matter (DM + baryons) directly?
Hello,
It depends what your goal is, I would read again the description of
SubfindDensity
carefully. This is a local mass density estimate, at the location of eachCoordinates
, which is based on an adaptive-size smoothing kernel.Personally I would not have thought to use it to compute a power spectrum, but instead the combination of
Masses
andCoordinates
which gives the (un-smoothed) mass distribution within the simulation volume.Thank you for your clarification!