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	<title>Moog (code) - Revision history</title>
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	<updated>2026-05-14T04:15:00Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
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		<id>http://debianws.lexgopc.com/wiki143/index.php?title=Moog_(code)&amp;diff=3084664&amp;oldid=prev</id>
		<title>imported&gt;Crouch, Swale: Disambiguating links to Austin (link changed to Austin, Texas) using DisamAssist.</title>
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		<updated>2023-12-21T18:34:36Z</updated>

		<summary type="html">&lt;p&gt;Disambiguating links to &lt;a href=&quot;/wiki143/index.php?title=Austin&quot; title=&quot;Austin&quot;&gt;Austin&lt;/a&gt; (link changed to &lt;a href=&quot;/wiki143/index.php?title=Austin,_Texas&quot; title=&quot;Austin, Texas&quot;&gt;Austin, Texas&lt;/a&gt;) using &lt;a href=&quot;/wiki143/index.php?title=User:Qwertyytrewqqwerty/DisamAssist&amp;amp;action=edit&amp;amp;redlink=1&quot; class=&quot;new&quot; title=&quot;User:Qwertyytrewqqwerty/DisamAssist (page does not exist)&quot;&gt;DisamAssist&lt;/a&gt;.&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;&amp;#039;&amp;#039;&amp;#039;MOOG&amp;#039;&amp;#039;&amp;#039; is an astronomical [[software]] package. It is an example of [[Fortran]] code that performs a variety of [[spectral line]] analysis and [[spectrum synthesis]] tasks under the assumption of [[Thermodynamic equilibrium#Local thermodynamic equilibrium|local thermodynamic equilibrium]].  Moog uses a [[model photosphere]] together with a list of [[Atomic electron transition|atomic]] or [[Molecular electronic transition|molecular]] transitions to generate an emergent [[spectrum]] by solving the [[Radiative transfer#The equation of radiative transfer|equation of radiative transfer]].&lt;br /&gt;
&lt;br /&gt;
The typical use of MOOG is to assist in the determination of the [[Metallicity|chemical composition]] of a [[star]], e.g. Sneden (1973).&amp;lt;ref&amp;gt;{{citation |first = Christopher |last = Sneden |title = The nitrogen abundance of the very metal-poor star [[HD 122563]] |bibcode = 1973ApJ...184..839S |journal = Astrophysical Journal  |volume = 184 |date = 1973 |pages = 839–849 |doi = 10.1086/152374}}&amp;lt;/ref&amp;gt; This paper contains also the description of the first version of the code and has been cited about 240 times as of 2008-04-24 by publications in international journals studying the abundances of chemical elements in stars.&lt;br /&gt;
&lt;br /&gt;
The software package has been developed and is maintained by Christopher Sneden, [[University of Texas]] at [[Austin, Texas|Austin]]. The current supported version of the code was released in August 2010 and is described in the MOOG User&amp;#039;s Guide (see references below).  Moog is written in [[Fortran#FORTRAN 77|FORTRAN 77]].&lt;br /&gt;
&lt;br /&gt;
==Coding==&lt;br /&gt;
The coding is in various subroutines that are called from a few driver routines; these routines are written in standard FORTRAN. The standard MOOG version has been developed on unix, linux and macintosh computers.&lt;br /&gt;
&lt;br /&gt;
==References==&lt;br /&gt;
{{reflist}}&lt;br /&gt;
&lt;br /&gt;
== Further reading ==&lt;br /&gt;
*{{citation |first = Christopher |last = Sneden |title = The nitrogen abundance of the very metal-poor star HD 122563 |bibcode = 1973ApJ...184..839S |journal = Astrophysical Journal  |volume = 184 |date = 1973 |pages = 839–849 |doi = 10.1086/152374}}&lt;br /&gt;
*{{citation |title = MOOG User&amp;#039;s Guide |url = http://verdi.as.utexas.edu/codes/WRITEMOOG.ps |format = Postscript |url-status = dead |archiveurl = https://web.archive.org/web/20061230163208/http://verdi.as.utexas.edu/codes/WRITEMOOG.ps |archivedate = 2006-12-30 }}&lt;br /&gt;
&lt;br /&gt;
==External links==&lt;br /&gt;
*[http://www.as.utexas.edu/~chris/moog.html MOOG homepage] maintained by developer Chris Sneden&lt;br /&gt;
&lt;br /&gt;
[[Category:Astronomy software]]&lt;br /&gt;
[[Category:Fortran software]]&lt;/div&gt;</summary>
		<author><name>imported&gt;Crouch, Swale</name></author>
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