Re: Egal overdensity vs redshift offset from cluster

From: Saul Perlmutter (saul@lbl.gov)
Date: Fri Jan 13 2006 - 09:07:44 PST

  • Next message: Marc Postman: "color plot"

    Hi Marc,
        Nice plot! I think the number we care most about is -- for
    ellipticals -- the ratio of the integral under the cluster's spike
    compared to the integral under all the rest of the curve that is above
    z=1. I can't quite do that calculation exactly from the current plot,
    since there may be some below z=1 on the plot (for the z=1.1 cluster)
    and some missing above z=1 (for the z=1.24 and 1.27 clusters), but
    assuming that these average out it looks like the answer is: ~3.5
    times as many z>1 E+S0 in the cluster as in the field. (For Sa+, it
    looks like the ratio is more like ~0.75 in cluster to 1 in field.)
    Now I'm curious to know if each of these three clusters contributes
    simlarly to this overdensity of ellipticals.

       Can you make a version of this that shows all galaxies above z=1 and
    no galaxies below z=1? Also, could we see what a version of this plot
    looks like that uses (GalColor - ClusterMeanColor) for the x axis?
    I'm wondering which version of the plot would be better for the proposal
    -- one version is closer to the data, and the other is perhaps easier to
    understand quickly.

    Thanks, --S

    Marc Postman wrote:

    > Saul et al.,
    >
    > Here is a plot that may demonstrate the point that early type galaxies
    > are strongly localized in the clusters for z > 1. This is a histogram
    > of spectroscopic redshifts for the clusters RXJ0910+54, RXJ1252-29,
    > and CL0848+44 (which are at z=1.10, 1.24, and 1.27, respectively). The
    > red histo is E+S0 galaxies and the blue histo is Sa or later. Relative
    > to the spikes seen in the field, the E+S0 overdensity in the cluster
    > is about a factor of 10 whereas the Sa+ overdensity is at best a
    > factor of 2. There may be some selection effects in the spectroscopic
    > selection to slightly favor early types, however. But these effects,
    > if corrected for, might only increase the Sa+ peak at dz=0 by about 20
    > - 30% (but would also probably increase the spikes in the field as
    > well so that the overall enhancement factor would probably still be
    > only about a factor of 2). The redshift range covered by this plot is
    > 0.9 < z < 1.47.
    >
    > Marc
    >
    >
    > -----------------------------------------------------------------
    > Marc Postman Email: postman@stsci.edu
    > STScI - CMO Phone: +1-410-338-4340
    > 3700 San Martin Drive Fax: +1-410-338-4424
    > Baltimore, MD 21218 U.S.A. http://www.stsci.edu/~postman



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