<?xml version="1.0" encoding="UTF-8"?>
 <rdf:RDF xmlns="http://purl.org/rss/1.0/" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:content="http://purl.org/rss/1.0/modules/content/" xmlns:taxo="http://purl.org/rss/1.0/modules/taxonomy/" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:cc="http://web.resource.org/cc/" xmlns:syn="http://purl.org/rss/1.0/modules/syndication/" xmlns:admin="http://webns.net/mvcb/">
  <channel rdf:about="http://pinboard.in">
    <title>Pinboard (Knusper2000)</title>
    <link>https://pinboard.in/u:Knusper2000/public/</link>
    <description>recent bookmarks from Knusper2000</description>
    <items>
      <rdf:Seq>	<rdf:li rdf:resource="https://github.com/ChrisBeaumont/mpl-modest-image"/>
	<rdf:li rdf:resource="http://nickcharlton.net/posts/drawing-animating-shapes-matplotlib.html"/>
	<rdf:li rdf:resource="http://www.walkingrandomly.com/?p=4731"/>
	<rdf:li rdf:resource="http://www.gnuplotting.org/"/>
	<rdf:li rdf:resource="http://stackoverflow.com/questions/2578752/how-can-i-plot-nan-values-as-a-special-color-with-imshow-in-matplotlib"/>
	<rdf:li rdf:resource="https://github.com/phn/lineid_plot"/>
	<rdf:li rdf:resource="http://packages.python.org/lineid_plot/"/>
	<rdf:li rdf:resource="http://www.astropython.org/resource/2011/10/lineid_plot"/>
	<rdf:li rdf:resource="http://star.physics.yale.edu/~ullrich/xyscanDistributionPage/"/>
	<rdf:li rdf:resource="http://aplpy.github.com/"/>
	<rdf:li rdf:resource="http://tobias.diekershoff.homeunix.net/?e=100"/>
	<rdf:li rdf:resource="http://home.gna.org/veusz/"/>
	<rdf:li rdf:resource="http://www.astro.princeton.edu/~rhl/sm/"/>
	<rdf:li rdf:resource="http://aplpy.sourceforge.net/"/>
	<rdf:li rdf:resource="http://www.stecf.org/conferences/adass/adassVII/warrensmithr.html"/>
      </rdf:Seq>
    </items>
  </channel><item rdf:about="https://github.com/ChrisBeaumont/mpl-modest-image">
    <title>ChrisBeaumont/mpl-modest-image</title>
    <dc:date>2015-02-20T21:22:40+00:00</dc:date>
    <link>https://github.com/ChrisBeaumont/mpl-modest-image</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[Friendlier matplotlib interaction with large images

ModestImage extends the matplotlib AxesImage class, and avoids unnecessary calculation and memory when rendering large images (where most image pixels aren't visible on the screen). It has the following benefits over AxesImage:

    Draw time is (roughly) independent of image size
    Large numpy.memmap arrays can be visualized, without making an in-memory copy of the entire array. This enables visualization of images too large to fit in memory.]]></description>
<dc:subject>work python plotting astronomy</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:ff1c2affb680/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:python"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:plotting"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:astronomy"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://nickcharlton.net/posts/drawing-animating-shapes-matplotlib.html">
    <title>Drawing and Animating Shapes with Matplotlib — nickcharlton.net</title>
    <dc:date>2013-06-01T00:53:18+00:00</dc:date>
    <link>http://nickcharlton.net/posts/drawing-animating-shapes-matplotlib.html</link>
    <dc:creator>Knusper2000</dc:creator><dc:subject>python plotting blog</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:06f4d31ea88a/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:python"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:plotting"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:blog"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://www.walkingrandomly.com/?p=4731">
    <title>Walking Randomly » xkcd style graphs in various languages</title>
    <dc:date>2012-12-29T20:39:27+00:00</dc:date>
    <link>http://www.walkingrandomly.com/?p=4731</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[xkcd style graphs in various languages

In a recent Mathematica StackExchange question, someone asked how such graphs could be automatically produced in Mathematica and code was quickly whipped up by the community.  Since then, various individuals and communities have developed code to do the same thing in a range of languages.  Here’s the list of examples I’ve found so far...]]></description>
<dc:subject>comic python mathematica latex plotting matlab</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:592e242de810/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:comic"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:python"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:mathematica"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:latex"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:plotting"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:matlab"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://www.gnuplotting.org/">
    <title>Gnuplotting · Create scientific plots using Gnuplot</title>
    <dc:date>2012-02-21T10:45:59+00:00</dc:date>
    <link>http://www.gnuplotting.org/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[On these sites there exist already introductions to Gnuplot, but I want to do it in a slightly different way that concentrates on the way I’m using Gnuplot.
And this way means, that I will present no introduction to the interactive Gnuplot prompt, but will start directly with writing some text files. These files can then be executed by Gnuplot.]]></description>
<dc:subject>blog plotting visualization work</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:77ac43b8d335/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:blog"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:plotting"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:visualization"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://stackoverflow.com/questions/2578752/how-can-i-plot-nan-values-as-a-special-color-with-imshow-in-matplotlib">
    <title>python - How can I plot NaN values as a special color with imshow in matplotlib? - Stack Overflow</title>
    <dc:date>2012-02-17T11:48:39+00:00</dc:date>
    <link>http://stackoverflow.com/questions/2578752/how-can-i-plot-nan-values-as-a-special-color-with-imshow-in-matplotlib</link>
    <dc:creator>Knusper2000</dc:creator><dc:subject>python plotting work tricks tips</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:edf151d7f231/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:python"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:plotting"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:tricks"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:tips"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="https://github.com/phn/lineid_plot">
    <title>phn/lineid_plot - GitHub</title>
    <dc:date>2011-10-22T17:10:27+00:00</dc:date>
    <link>https://github.com/phn/lineid_plot</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[Manually labeling features in a crowed plot can be very time consuming. Functions in this module can be used to automatically place labels without the labels overlapping each other. This is useful, for example, in creating plots of spectrum with lines identified with labels.
]]></description>
<dc:subject>work astronomy software plotting</dc:subject>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:8c792b8ea0f1/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:astronomy"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:software"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:plotting"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://packages.python.org/lineid_plot/">
    <title>Line identification plots with automatic label layout — Line Identification Plots v0.1 documentation</title>
    <dc:date>2011-10-22T17:10:26+00:00</dc:date>
    <link>http://packages.python.org/lineid_plot/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[Line Identification Plots v0.1 documentation
Line identification plots with automatic label layout
]]></description>
<dc:subject>python plotting work matplotlib astronomy</dc:subject>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:72f3d774b569/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:python"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:plotting"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:matplotlib"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:astronomy"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://www.astropython.org/resource/2011/10/lineid_plot">
    <title>lineid_plot @ Astropython</title>
    <dc:date>2011-10-22T17:08:11+00:00</dc:date>
    <link>http://www.astropython.org/resource/2011/10/lineid_plot</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[This module has functions for automatically placing labels in a plot in such a way that the labels do not overlap with each other. This is very useful, for example, in creating plots that have labels identifying features in a spectrum.
]]></description>
<dc:subject>python plotting work</dc:subject>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:d8255ac7bcc4/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:python"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:plotting"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://star.physics.yale.edu/~ullrich/xyscanDistributionPage/">
    <title>xyscan Distribution Page</title>
    <dc:date>2011-06-11T14:03:13+00:00</dc:date>
    <link>http://star.physics.yale.edu/~ullrich/xyscanDistributionPage/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[xyscan is a tool for scientist in the need to extract data points, i.e. numeric values, from a plot. It allows to scan the plots and extract data points including the size of the error bars (both in x and y). It can handle plots with linear and logarithmic scales. In fact xyscan can be used for extracting numeric values from any kind of 2D technical drawings.
]]></description>
<dc:subject>graphics graph linux tools science work physics plotting software opensource</dc:subject>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:581e114dc98e/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:graphics"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:graph"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:linux"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:tools"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:science"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:physics"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:plotting"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:software"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:opensource"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://aplpy.github.com/">
    <title>APLpy Home Page</title>
    <dc:date>2011-03-07T17:05:42+00:00</dc:date>
    <link>http://aplpy.github.com/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[APLpy (the Astronomical Plotting Library in Python) is a Python module aimed at producing publication-quality plots of astronomical imaging data in FITS format. The module uses Matplotlib, a powerful and interactive plotting package. It is capable of creating output files in several graphical formats, including EPS, PDF, PS, PNG, and SVG.
]]></description>
<dc:subject>graphics plotting python astronomy work astrophysics</dc:subject>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:8586bc24716d/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:graphics"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:plotting"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:python"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:astronomy"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:astrophysics"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://tobias.diekershoff.homeunix.net/?e=100">
    <title>Lessons Learned - 2: Histograms - Anything or more and less</title>
    <dc:date>2010-11-26T19:28:17+00:00</dc:date>
    <link>http://tobias.diekershoff.homeunix.net/?e=100</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[After I’ve covered basic plotting using matplotlib in this part I’ll show you two ways to display histograms of some data.
]]></description>
<dc:subject>plotting python work histograms data visualization programming opensource</dc:subject>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:bebf0281cdb0/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:plotting"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:python"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:histograms"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:data"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:visualization"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:programming"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:opensource"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://home.gna.org/veusz/">
    <title>Veusz</title>
    <dc:date>2009-10-03T13:41:34+00:00</dc:date>
    <link>http://home.gna.org/veusz/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[Veusz is a scientific plotting and graphing package written in Python. It uses PyQt (Wiki) and Numpy. Veusz is designed to produce publication-ready Postscript/PDF output. Veusz runs under Unix/Linux, Windows and Mac OS X.
]]></description>
<dc:subject>linux opensource science software visualization plotting plot python gui</dc:subject>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:ac556e540ca1/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:linux"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:opensource"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:science"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:software"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:visualization"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:plotting"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:plot"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:python"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:gui"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://www.astro.princeton.edu/~rhl/sm/">
    <title>Supermongo</title>
    <dc:date>2009-09-13T11:48:28+00:00</dc:date>
    <link>http://www.astro.princeton.edu/~rhl/sm/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[SM is a plotting programme written by Robert Lupton (]]></description>
<dc:subject>linux science software astronomy tools mathematics work graphics astro plotting</dc:subject>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:bd558c810e29/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:linux"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:science"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:software"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:astronomy"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:tools"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:mathematics"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:graphics"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:astro"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:plotting"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://aplpy.sourceforge.net/">
    <title>APLpy Home Page</title>
    <dc:date>2009-07-27T21:57:16+00:00</dc:date>
    <link>http://aplpy.sourceforge.net/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[APLpy (the Astronomical Plotting Library in Python) is a Python module aimed at producing publication-quality plots of astronomical imaging data in FITS format. The module uses Matplotlib, a powerful and interactive plotting package. It is capable of creating output files in several graphical formats, including EPS, PDF, PS, PNG, and SVG.
]]></description>
<dc:subject>science software astronomy free work python astro library plotting</dc:subject>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:2dae45c1a520/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:science"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:software"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:astronomy"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:free"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:python"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:astro"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:library"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:plotting"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://www.stecf.org/conferences/adass/adassVII/warrensmithr.html">
    <title>World Coordinate Systems as Objects</title>
    <dc:date>2009-06-19T15:40:52+00:00</dc:date>
    <link>http://www.stecf.org/conferences/adass/adassVII/warrensmithr.html</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[We describe a new library (AST) which provides a flexible high-level programming interface for handling world coordinate systems in astronomy and for producing graphical output. It includes, but is not limited to, a wide range of celestial coordinate systems and supports the Digitised Sky Survey plate solutions and the draft FITS WCS proposals amongst other possibilities. AST is portable and environment independent.
]]></description>
<dc:subject>astronomy plot plotting science work physics</dc:subject>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:5eb14a42b850/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:astronomy"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:plot"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:plotting"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:science"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:physics"/>
</rdf:Bag></taxo:topics>
</item>
</rdf:RDF>