GalWeight Application: A publicly-available catalog of dynamical parameters of 1,870 galaxy clusters from SDSS-DR13, ($mathtt{GalWCat19}$). (arXiv:1907.05061v1 [astro-ph.CO])

GalWeight Application: A publicly-available catalog of dynamical parameters of 1,870 galaxy clusters from SDSS-DR13, ($mathtt{GalWCat19}$). (arXiv:1907.05061v1 [astro-ph.CO])
<a href="http://arxiv.org/find/astro-ph/1/au:+Abdullah_M/0/1/0/all/0/1">Mohamed H. Abdullah</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Wilson_G/0/1/0/all/0/1">Gillian Wilson</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Klypin_A/0/1/0/all/0/1">Anatoly Klypin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Old_L/0/1/0/all/0/1">Lyndsay Old</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Praton_E/0/1/0/all/0/1">Elizabeth Praton</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ali_G/0/1/0/all/0/1">Gamal Ali</a>

Utilizing the SDSS-DR13 spectroscopic dataset, we create a new
publicly-available catalog of 1,870 galaxy clusters (GalWeight cluster catalog,
$mathtt{GalWCat19}$) and a corresponding catalog of 38,536 identified member
galaxies. The clusters are identified from overdensities in redshift-phase
space. The GalWeight technique introduced in Abdullah, Wilson and Klypin
(AWK18) is then applied to identify cluster members. The completeness of the
cluster catalog ($mathtt{GalWCat19}$) and the procedure followed to determine
cluster mass are tested on the Bolshoi N-body simulations. The 1,870
$mathtt{GalWCat19}$ clusters range in redshift between $0.01 – 0.2$ and in
mass between $(0.4 – 14) times 10^{14}h^{-1}M_{odot}$. The cluster catalog
provides a large number of cluster parameters including sky position, redshift,
membership, velocity dispersion, and mass at overdensities $Delta = 500, 200,
100, 5.5$. The 38,536 member galaxies are identified within the radius at which
the density is 200 times the critical density of the Universe. The galaxy
catalog provides the coordinates of each galaxy and the ID of the cluster that
the galaxy belongs to. The cluster velocity dispersion scales with mass as
$log(sigma_{200})=log(933pm29~ mbox{km} ~ mbox{s}^{-1})
+(0.35pm0.04)logleft[h(z) ~ M_{200}/10^{15}M_odotright]$ with scatter of
$delta = 0.06$. The fundamental dynamical parameters of the cluster sample do
not show evolution in the redshift interval $0.0 < z < 0.2$. The catalogs are publicly available at the following websitefootnote{url{https://mohamed-elhashash-94.webself.net/}}.

Utilizing the SDSS-DR13 spectroscopic dataset, we create a new
publicly-available catalog of 1,870 galaxy clusters (GalWeight cluster catalog,
$mathtt{GalWCat19}$) and a corresponding catalog of 38,536 identified member
galaxies. The clusters are identified from overdensities in redshift-phase
space. The GalWeight technique introduced in Abdullah, Wilson and Klypin
(AWK18) is then applied to identify cluster members. The completeness of the
cluster catalog ($mathtt{GalWCat19}$) and the procedure followed to determine
cluster mass are tested on the Bolshoi N-body simulations. The 1,870
$mathtt{GalWCat19}$ clusters range in redshift between $0.01 – 0.2$ and in
mass between $(0.4 – 14) times 10^{14}h^{-1}M_{odot}$. The cluster catalog
provides a large number of cluster parameters including sky position, redshift,
membership, velocity dispersion, and mass at overdensities $Delta = 500, 200,
100, 5.5$. The 38,536 member galaxies are identified within the radius at which
the density is 200 times the critical density of the Universe. The galaxy
catalog provides the coordinates of each galaxy and the ID of the cluster that
the galaxy belongs to. The cluster velocity dispersion scales with mass as
$log(sigma_{200})=log(933pm29~ mbox{km} ~ mbox{s}^{-1})
+(0.35pm0.04)logleft[h(z) ~ M_{200}/10^{15}M_odotright]$ with scatter of
$delta = 0.06$. The fundamental dynamical parameters of the cluster sample do
not show evolution in the redshift interval $0.0 < z < 0.2$. The catalogs are
publicly available at the following
websitefootnote{url{https://mohamed-elhashash-94.webself.net/}}.

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