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  <h1 class="page-header">Data</h1>


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          <h3>
            Dark Energy Survey (Restricted data)
          </h3>

          <span class="text-success">Jul 14, 2014</span>

        <p>Introduction

We have used TPZ to produced photo-z PDFs and probabilistic star/galaxy classifications for all objects
on the DES SVA 1.0 gold catalog.

Data (You need DES credentials)

  SVA GOLD 1.0 TPZ PHOTO-Z and P(Z)
  SVA GOLD 1.0 TPZ S/G CLASS


If you have any questions about these data, please contact Robert
Brunner at: bigdog AT illinois.edu
</p>
        <a href="/data/2014/07/14/des.html">Read more...</a><br>
      
      
          <h3>
            SDSS DR7 Galaxy Correlation Function Data
          </h3>

          <span class="text-success">Dec 16, 2013</span>

        <p>Introduction We are publicly releasing both the angular correltaion function estimates (computed with the Landy &amp; Szalay estimor) and the associated covariance matrices for the SDSS DR7 galaxy sample first presented in Wang, Brunner, &amp; Dolence 2013. Data Angular Correlation Functions This first column of these files is the angle in degrees, the second column is the estimator, and the third column is the error of the estimator. Covariance Matrices: This first row and the...</p>
        <a href="/data/2013/12/16/tpacf.html">Read more...</a><br>
      
      
          <h3>
            SDSS DR7 Galaxy Angular Power Spectra
          </h3>

          <span class="text-success">Sep 6, 2013</span>

        <p>Introduction We are publically releasing the angular power spectra estimates and the corresponding Fisher matrices and Window functions first presented in Hayes, Brunner, &amp; Ross 2012. The naming of these files correspond to the samples they describe. The naming convention begins with the type of data. We provide the angular power spectrum and errors in the files prefixed with “C_”, the Fisher matrices in the files prefixed with “Fisher_”, and the window functions in the...</p>
        <a href="/data/2013/09/06/apsqe.html">Read more...</a><br>
      
      
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