<?xml version="1.0" encoding="UTF-8"?><rss version="2.0"
	xmlns:content="http://purl.org/rss/1.0/modules/content/"
	xmlns:dc="http://purl.org/dc/elements/1.1/"
	xmlns:atom="http://www.w3.org/2005/Atom"
	xmlns:sy="http://purl.org/rss/1.0/modules/syndication/"
		>
<channel>
	<title>Comments on: Rendering the Structure of the Universe in Your Spare Time</title>
	<atom:link href="http://blog.wolfram.com/2009/10/06/rendering-the-structure-of-the-universe-in-your-spare-time/feed/" rel="self" type="application/rss+xml" />
	<link>http://blog.wolfram.com/2009/10/06/rendering-the-structure-of-the-universe-in-your-spare-time/</link>
	<description>News, views, &#38; ideas from the front lines at Wolfram Research</description>
	<lastBuildDate>Thu, 09 Feb 2012 20:04:10 -0600</lastBuildDate>
	<generator>http://wordpress.org/?v=2.8.4</generator>
	<sy:updatePeriod>hourly</sy:updatePeriod>
	<sy:updateFrequency>1</sy:updateFrequency>
		<item>
		<title>By: Jeff Bryant</title>
		<link>http://blog.wolfram.com/2009/10/06/rendering-the-structure-of-the-universe-in-your-spare-time/comment-page-1/#comment-5235</link>
		<dc:creator>Jeff Bryant</dc:creator>
		<pubDate>Mon, 18 Apr 2011 16:01:05 +0000</pubDate>
		<guid isPermaLink="false">http://blog.internal.wolfram.com/?p=1971#comment-5235</guid>
		<description>Its been quite a while and I&#039;m not usually a database guy. I didn&#039;t make the database calls from Mathematica since their website didn&#039;t make it obvious how to do that, but I was able to get the data using the following SQL commands:

SELECT
         sp.bestObjID as oid,
         sp.z as z,
         sp.specClass as specClass,
         sp.ra as ra,
         sp.dec as dec,
         sp.mag_0 as mag_g,
         sp.mag_1 as mag_r,
         sp.mag_2 as mag_i,
         gal.expMag_r as emag_r,
         gal.expAB_r as AB,
         gal.expPhi_r as phi,
         gal.expRad_r as rad_r,
         gal.expRad_i as rad_i,
         gal.petroR90_r / gal.petroR50_r as conc90_50
 FROM SpecObj as sp,
      Galaxy as gal
 WHERE sp.bestObjID = gal.objID
   and sp.z = 16000

The last line needs to be tweaked to get a specific batch. Their site times out if the batch is too large. I downloaded each batch to a CSV file and then imported them. Each row had the form:

{&quot;oid&quot;, &quot;z&quot;, &quot;specClass&quot;, &quot;ra&quot;, &quot;dec&quot;, &quot;mag_g&quot;, &quot;mag_r&quot;, &quot;mag_i&quot;, &quot;emag_r&quot;, &quot;AB&quot;, &quot;phi&quot;, &quot;rad_r&quot;, &quot;rad_i&quot;, &quot;conc90_50&quot;}

To transform this data into something ready to be plotted in 3D, I used:

proj = reduceddata /. {z_, ra_, 
    dec_} :&gt; {z Cos[ra Degree] Sin[dec Degree + Pi/2], 
    z Sin[ra Degree] Sin[dec Degree + Pi/2], z Cos[dec Degree + Pi/2]}

DIstance was not computed. Only redshift is plotted directly.</description>
		<content:encoded><![CDATA[<p>Its been quite a while and I&#8217;m not usually a database guy. I didn&#8217;t make the database calls from Mathematica since their website didn&#8217;t make it obvious how to do that, but I was able to get the data using the following SQL commands:</p>
<p>SELECT<br />
         sp.bestObjID as oid,<br />
         sp.z as z,<br />
         sp.specClass as specClass,<br />
         sp.ra as ra,<br />
         sp.dec as dec,<br />
         sp.mag_0 as mag_g,<br />
         sp.mag_1 as mag_r,<br />
         sp.mag_2 as mag_i,<br />
         gal.expMag_r as emag_r,<br />
         gal.expAB_r as AB,<br />
         gal.expPhi_r as phi,<br />
         gal.expRad_r as rad_r,<br />
         gal.expRad_i as rad_i,<br />
         gal.petroR90_r / gal.petroR50_r as conc90_50<br />
 FROM SpecObj as sp,<br />
      Galaxy as gal<br />
 WHERE sp.bestObjID = gal.objID<br />
   and sp.z = 16000</p>
<p>The last line needs to be tweaked to get a specific batch. Their site times out if the batch is too large. I downloaded each batch to a CSV file and then imported them. Each row had the form:</p>
<p>{&#8221;oid&#8221;, &#8220;z&#8221;, &#8220;specClass&#8221;, &#8220;ra&#8221;, &#8220;dec&#8221;, &#8220;mag_g&#8221;, &#8220;mag_r&#8221;, &#8220;mag_i&#8221;, &#8220;emag_r&#8221;, &#8220;AB&#8221;, &#8220;phi&#8221;, &#8220;rad_r&#8221;, &#8220;rad_i&#8221;, &#8220;conc90_50&#8243;}</p>
<p>To transform this data into something ready to be plotted in 3D, I used:</p>
<p>proj = reduceddata /. {z_, ra_,<br />
    dec_} :&gt; {z Cos[ra Degree] Sin[dec Degree + Pi/2],<br />
    z Sin[ra Degree] Sin[dec Degree + Pi/2], z Cos[dec Degree + Pi/2]}</p>
<p>DIstance was not computed. Only redshift is plotted directly.</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Mark</title>
		<link>http://blog.wolfram.com/2009/10/06/rendering-the-structure-of-the-universe-in-your-spare-time/comment-page-1/#comment-5229</link>
		<dc:creator>Mark</dc:creator>
		<pubDate>Sun, 17 Apr 2011 22:36:04 +0000</pubDate>
		<guid isPermaLink="false">http://blog.internal.wolfram.com/?p=1971#comment-5229</guid>
		<description>great stuff, but trying to replicate all I got was a sphrical distribution of the points with a bright line in the middle. Could you please post the SQL code you used to obtain the data and also what distance scale did you use and how you converted from z to distance, here is what I used in the SQL:
select ra,dec,z
from specObj WHERE
z BETWEEN 0.001 AND 0.5

Thanks.</description>
		<content:encoded><![CDATA[<p>great stuff, but trying to replicate all I got was a sphrical distribution of the points with a bright line in the middle. Could you please post the SQL code you used to obtain the data and also what distance scale did you use and how you converted from z to distance, here is what I used in the SQL:<br />
select ra,dec,z<br />
from specObj WHERE<br />
z BETWEEN 0.001 AND 0.5</p>
<p>Thanks.</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Christian   louboutin online</title>
		<link>http://blog.wolfram.com/2009/10/06/rendering-the-structure-of-the-universe-in-your-spare-time/comment-page-1/#comment-1522</link>
		<dc:creator>Christian   louboutin online</dc:creator>
		<pubDate>Tue, 16 Mar 2010 03:18:36 +0000</pubDate>
		<guid isPermaLink="false">http://blog.internal.wolfram.com/?p=1971#comment-1522</guid>
		<description>It&#039;s so lucky for me to find your blog! So shocking and great! Just one suggestion: It will be better and easier to follow if your blog can offer rrs subscription service.</description>
		<content:encoded><![CDATA[<p>It&#8217;s so lucky for me to find your blog! So shocking and great! Just one suggestion: It will be better and easier to follow if your blog can offer rrs subscription service.</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: jason</title>
		<link>http://blog.wolfram.com/2009/10/06/rendering-the-structure-of-the-universe-in-your-spare-time/comment-page-1/#comment-1199</link>
		<dc:creator>jason</dc:creator>
		<pubDate>Wed, 07 Oct 2009 06:32:32 +0000</pubDate>
		<guid isPermaLink="false">http://blog.internal.wolfram.com/?p=1971#comment-1199</guid>
		<description>this is amazing!  thank you!</description>
		<content:encoded><![CDATA[<p>this is amazing!  thank you!</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Paul Eipper</title>
		<link>http://blog.wolfram.com/2009/10/06/rendering-the-structure-of-the-universe-in-your-spare-time/comment-page-1/#comment-1198</link>
		<dc:creator>Paul Eipper</dc:creator>
		<pubDate>Wed, 07 Oct 2009 04:36:19 +0000</pubDate>
		<guid isPermaLink="false">http://blog.internal.wolfram.com/?p=1971#comment-1198</guid>
		<description>Really cool. The Mathematica code really is short too, impressive.

I think I&#039;ve seen this rendered somewhere else too, oh yeah, the Millenium Simulation: http://www.mpa-garching.mpg.de/galform/millennium/

Awesome stuff</description>
		<content:encoded><![CDATA[<p>Really cool. The Mathematica code really is short too, impressive.</p>
<p>I think I&#8217;ve seen this rendered somewhere else too, oh yeah, the Millenium Simulation: <a href="http://www.mpa-garching.mpg.de/galform/millennium/" rel="nofollow">http://www.mpa-garching.mpg.de/galform/millennium/</a></p>
<p>Awesome stuff</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: David</title>
		<link>http://blog.wolfram.com/2009/10/06/rendering-the-structure-of-the-universe-in-your-spare-time/comment-page-1/#comment-1197</link>
		<dc:creator>David</dc:creator>
		<pubDate>Wed, 07 Oct 2009 02:53:56 +0000</pubDate>
		<guid isPermaLink="false">http://blog.internal.wolfram.com/?p=1971#comment-1197</guid>
		<description>Good post, but it could have been much better.  What were the MMA commands used to query the SDSS databases?  What processing was required for the data?  Did you try other view points?  

Answers to all these might have made a much much better post.</description>
		<content:encoded><![CDATA[<p>Good post, but it could have been much better.  What were the MMA commands used to query the SDSS databases?  What processing was required for the data?  Did you try other view points?  </p>
<p>Answers to all these might have made a much much better post.</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Shears</title>
		<link>http://blog.wolfram.com/2009/10/06/rendering-the-structure-of-the-universe-in-your-spare-time/comment-page-1/#comment-1195</link>
		<dc:creator>Shears</dc:creator>
		<pubDate>Tue, 06 Oct 2009 19:51:11 +0000</pubDate>
		<guid isPermaLink="false">http://blog.internal.wolfram.com/?p=1971#comment-1195</guid>
		<description>Unfortunately youtube seems to have some problems because i can&#039;t load the video. From your description it seems a very interesting animation.</description>
		<content:encoded><![CDATA[<p>Unfortunately youtube seems to have some problems because i can&#8217;t load the video. From your description it seems a very interesting animation.</p>
]]></content:encoded>
	</item>
</channel>
</rss>

