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	<title>Comments on: Spectral line analysis tools</title>
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	<link>http://www.astrobetter.com/spectral-line-analysis-tools/</link>
	<description>Tips and Tricks for Professional Astronomers</description>
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		<title>By: George Jacoby</title>
		<link>http://www.astrobetter.com/spectral-line-analysis-tools/comment-page-1/#comment-1598</link>
		<dc:creator>George Jacoby</dc:creator>
		<pubDate>Wed, 27 Jan 2010 13:40:32 +0000</pubDate>
		<guid isPermaLink="false">http://www.astrobetter.com/?p=933#comment-1598</guid>
		<description>Okay, I&#039;ll admit to being the original author of SPLOT and most of the ONEDSPEC package in IRAF. I find it both thrilling and shocking that most people (including myself) use these tools &quot;as is&quot; 25 years after I wrote them. (Note that Frank Valdes has provided many improvements and additions over the years.) My intent here is to encourage users to send suggestions to IRAF support at NOAO. Many improvements can be made relatively quickly and easily (e.g., a true database output from SPLOT). Although the resources at NOAO for IRAF are currently very limited, once improvements are made, the entire community benefits.</description>
		<content:encoded><![CDATA[<p>Okay, I&#8217;ll admit to being the original author of SPLOT and most of the ONEDSPEC package in IRAF. I find it both thrilling and shocking that most people (including myself) use these tools &#8220;as is&#8221; 25 years after I wrote them. (Note that Frank Valdes has provided many improvements and additions over the years.) My intent here is to encourage users to send suggestions to IRAF support at NOAO. Many improvements can be made relatively quickly and easily (e.g., a true database output from SPLOT). Although the resources at NOAO for IRAF are currently very limited, once improvements are made, the entire community benefits.</p>
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		<title>By: Pierre</title>
		<link>http://www.astrobetter.com/spectral-line-analysis-tools/comment-page-1/#comment-997</link>
		<dc:creator>Pierre</dc:creator>
		<pubDate>Mon, 21 Dec 2009 11:09:03 +0000</pubDate>
		<guid isPermaLink="false">http://www.astrobetter.com/?p=933#comment-997</guid>
		<description>Hi all,
in the same line of work as Gandalf, there is STECKMAP, which I wrote during my PhD and I am still using and upgrading, along with a number of believers. You can check it out here:
http://astro.u-strasbg.fr/~ocvirk/
drop me a line if youre interested, Ill keep you up to date with the latest developments.</description>
		<content:encoded><![CDATA[<p>Hi all,<br />
in the same line of work as Gandalf, there is STECKMAP, which I wrote during my PhD and I am still using and upgrading, along with a number of believers. You can check it out here:<br />
<a href="http://astro.u-strasbg.fr/~ocvirk/" rel="nofollow">http://astro.u-strasbg.fr/~ocvirk/</a><br />
drop me a line if youre interested, Ill keep you up to date with the latest developments.</p>
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		<title>By: Anca Constantin</title>
		<link>http://www.astrobetter.com/spectral-line-analysis-tools/comment-page-1/#comment-945</link>
		<dc:creator>Anca Constantin</dc:creator>
		<pubDate>Thu, 17 Dec 2009 16:00:02 +0000</pubDate>
		<guid isPermaLink="false">http://www.astrobetter.com/?p=933#comment-945</guid>
		<description>I didn&#039;t see here any mention of G. Kriss&#039; SPECFIT, IRAF again [included in the stsdas group, under contrib.spfitpkg package], but it&#039;s been pretty good to me.   And, definitely much more versatile than SPLOT.  The help file was sufficient for me when I first tried it, and a brief description can be found in the 1994,  PASP  Conf.  Series, Vol.  61,  p.  437.</description>
		<content:encoded><![CDATA[<p>I didn&#8217;t see here any mention of G. Kriss&#8217; SPECFIT, IRAF again [included in the stsdas group, under contrib.spfitpkg package], but it&#8217;s been pretty good to me.   And, definitely much more versatile than SPLOT.  The help file was sufficient for me when I first tried it, and a brief description can be found in the 1994,  PASP  Conf.  Series, Vol.  61,  p.  437.</p>
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		<title>By: Tim van K.</title>
		<link>http://www.astrobetter.com/spectral-line-analysis-tools/comment-page-1/#comment-925</link>
		<dc:creator>Tim van K.</dc:creator>
		<pubDate>Wed, 16 Dec 2009 08:48:01 +0000</pubDate>
		<guid isPermaLink="false">http://www.astrobetter.com/?p=933#comment-925</guid>
		<description>I would go for CLASS. It is a bit of a steeper learning curve, but Class 90 can do a lot of fitting and a lot of moments easily. I have been using it in the submm for years now, even converting starlink produced spectra to class. One big advantage of class that i found cumbersome in IDL routine is its ability to easily do spectral line maps with variable fits of different baseline orders.</description>
		<content:encoded><![CDATA[<p>I would go for CLASS. It is a bit of a steeper learning curve, but Class 90 can do a lot of fitting and a lot of moments easily. I have been using it in the submm for years now, even converting starlink produced spectra to class. One big advantage of class that i found cumbersome in IDL routine is its ability to easily do spectral line maps with variable fits of different baseline orders.</p>
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		<title>By: Fred Walter</title>
		<link>http://www.astrobetter.com/spectral-line-analysis-tools/comment-page-1/#comment-916</link>
		<dc:creator>Fred Walter</dc:creator>
		<pubDate>Wed, 16 Dec 2009 01:04:26 +0000</pubDate>
		<guid isPermaLink="false">http://www.astrobetter.com/?p=933#comment-916</guid>
		<description>ICUR, an IDL-based interactive spectroscopic package I started writing nearly 30 years ago, still works (though parts of it need to be updated).

See &lt;a href=&quot;http://www.astro.sunysb.edu/fwalter/ICUR/icur.html&quot; rel=&quot;nofollow&quot;&gt;the ICUR download page&lt;/a&gt;. Documentation is in &lt;a href=&quot;http://www.astro.sunysb.edu/fwalter/ICUR/icur.pdf&quot; rel=&quot;nofollow&quot;&gt;this pdf file&lt;/a&gt;.</description>
		<content:encoded><![CDATA[<p>ICUR, an IDL-based interactive spectroscopic package I started writing nearly 30 years ago, still works (though parts of it need to be updated).</p>
<p>See <a href="http://www.astro.sunysb.edu/fwalter/ICUR/icur.html" rel="nofollow">the ICUR download page</a>. Documentation is in <a href="http://www.astro.sunysb.edu/fwalter/ICUR/icur.pdf" rel="nofollow">this pdf file</a>.</p>
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		<title>By: Tolga Guver</title>
		<link>http://www.astrobetter.com/spectral-line-analysis-tools/comment-page-1/#comment-896</link>
		<dc:creator>Tolga Guver</dc:creator>
		<pubDate>Mon, 14 Dec 2009 22:24:32 +0000</pubDate>
		<guid isPermaLink="false">http://www.astrobetter.com/?p=933#comment-896</guid>
		<description>You can try SHERPA (from : http://cxc.harvard.edu/sherpa3.4/) it is an older version and basically written to analyze Chandra X-ray spectroscopic data. But it also accepts ASCII files, so you can fit any sort of data (optionally with errorbars) with a broad selection of features and models (Gaussian, Lorentz, etc. together with all other typical X-ray spectral and general mathematical models, and finally if you need your own models). It also supports all sorts of chi2 minimization techniques, confidence contour plots etc. The newer version of the software also supports Python and S-lang you you can easily write complicated scripts as well, but the older one is much easier to use, for interactive analysis.</description>
		<content:encoded><![CDATA[<p>You can try SHERPA (from : <a href="http://cxc.harvard.edu/sherpa3.4/)" rel="nofollow">http://cxc.harvard.edu/sherpa3.4/)</a> it is an older version and basically written to analyze Chandra X-ray spectroscopic data. But it also accepts ASCII files, so you can fit any sort of data (optionally with errorbars) with a broad selection of features and models (Gaussian, Lorentz, etc. together with all other typical X-ray spectral and general mathematical models, and finally if you need your own models). It also supports all sorts of chi2 minimization techniques, confidence contour plots etc. The newer version of the software also supports Python and S-lang you you can easily write complicated scripts as well, but the older one is much easier to use, for interactive analysis.</p>
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		<title>By: Eric Bubar</title>
		<link>http://www.astrobetter.com/spectral-line-analysis-tools/comment-page-1/#comment-886</link>
		<dc:creator>Eric Bubar</dc:creator>
		<pubDate>Sun, 13 Dec 2009 17:47:06 +0000</pubDate>
		<guid isPermaLink="false">http://www.astrobetter.com/?p=933#comment-886</guid>
		<description>I like to use SPECTRE from Chris Sneden.  It requires Supermongo to work, but its excellent for getting out equivalent widths interactively.  For automated extraction of equivalent widths, I&#039;ve tried to bend DAOSPEC from Peter Stetson to my will, but haven&#039;t gotten it working to my satisfaction yet.  Those would be my two choices.</description>
		<content:encoded><![CDATA[<p>I like to use SPECTRE from Chris Sneden.  It requires Supermongo to work, but its excellent for getting out equivalent widths interactively.  For automated extraction of equivalent widths, I&#8217;ve tried to bend DAOSPEC from Peter Stetson to my will, but haven&#8217;t gotten it working to my satisfaction yet.  Those would be my two choices.</p>
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		<title>By: Vinay Kashyap</title>
		<link>http://www.astrobetter.com/spectral-line-analysis-tools/comment-page-1/#comment-855</link>
		<dc:creator>Vinay Kashyap</dc:creator>
		<pubDate>Fri, 11 Dec 2009 22:47:49 +0000</pubDate>
		<guid isPermaLink="false">http://www.astrobetter.com/?p=933#comment-855</guid>
		<description>See also PINTofALE, at http://hea-www.harvard.edu/PINTofALE/

Designed for analysis of high-resolution EUV/X-ray stellar gratings spectra.  There is a gui line-fitting program called fitlines() that&#039;s pretty flexible and robust, if I may say so myself.</description>
		<content:encoded><![CDATA[<p>See also PINTofALE, at <a href="http://hea-www.harvard.edu/PINTofALE/" rel="nofollow">http://hea-www.harvard.edu/PINTofALE/</a></p>
<p>Designed for analysis of high-resolution EUV/X-ray stellar gratings spectra.  There is a gui line-fitting program called fitlines() that&#8217;s pretty flexible and robust, if I may say so myself.</p>
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		<title>By: Randall Smith</title>
		<link>http://www.astrobetter.com/spectral-line-analysis-tools/comment-page-1/#comment-854</link>
		<dc:creator>Randall Smith</dc:creator>
		<pubDate>Fri, 11 Dec 2009 22:20:22 +0000</pubDate>
		<guid isPermaLink="false">http://www.astrobetter.com/?p=933#comment-854</guid>
		<description>You could take a look at &lt;a href=&quot;http://heasarc.nasa.gov/docs/software/profit/&quot; rel=&quot;nofollow&quot;&gt;Profit&lt;/a&gt;

It was an attempt to develop a spectral line fitting program with the same ease-of-use of saoimage/ds9.  I won&#039;t say we succeeded (I think we set a high bar trying to be as good as ds9), and unfortunately development has stalled as both developers moved on, but it is still usable.

--Randall</description>
		<content:encoded><![CDATA[<p>You could take a look at <a href="http://heasarc.nasa.gov/docs/software/profit/" rel="nofollow">Profit</a></p>
<p>It was an attempt to develop a spectral line fitting program with the same ease-of-use of saoimage/ds9.  I won&#8217;t say we succeeded (I think we set a high bar trying to be as good as ds9), and unfortunately development has stalled as both developers moved on, but it is still usable.</p>
<p>&#8211;Randall</p>
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		<title>By: Gene Avrett</title>
		<link>http://www.astrobetter.com/spectral-line-analysis-tools/comment-page-1/#comment-851</link>
		<dc:creator>Gene Avrett</dc:creator>
		<pubDate>Fri, 11 Dec 2009 20:51:49 +0000</pubDate>
		<guid isPermaLink="false">http://www.astrobetter.com/?p=933#comment-851</guid>
		<description>See my website for some lecture notes on the atmospheric modeling aspect of spectral line analysis, as well as a description of the Pandora computer program I use to calculate a spectrum from given atmospheric parameters.</description>
		<content:encoded><![CDATA[<p>See my website for some lecture notes on the atmospheric modeling aspect of spectral line analysis, as well as a description of the Pandora computer program I use to calculate a spectrum from given atmospheric parameters.</p>
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