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    <dc:creator>Knusper2000</dc:creator><description><![CDATA[The astrodendro package provides an easy way to compute dendrograms of observed or simulated Astronomical data in Python.]]></description>
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<dc:source>https://pinboard.in/</dc:source>
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<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:work"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:astronomy"/>
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<item rdf:about="http://www.unwise.me/">
    <title>unWISE: unblurred coadds from WISE</title>
    <dc:date>2014-11-20T12:58:06+00:00</dc:date>
    <link>http://www.unwise.me/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[unWISE: unofficial, unblurred coadds of the WISE imaging]]></description>
<dc:subject>work astronomy</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:e534a632300a/</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:Bag></taxo:topics>
</item>
<item rdf:about="http://people.math.sfu.ca/~cbm/aands/">
    <title>Abramowitz and Stegun: Handbook of Mathematical Functions</title>
    <dc:date>2014-11-17T18:45:09+00:00</dc:date>
    <link>http://people.math.sfu.ca/~cbm/aands/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[An electronic copy of the tenth printing of this famous reference.]]></description>
<dc:subject>book math reference work pdf</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:2a5bc04fb995/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:book"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:math"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:reference"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:pdf"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://colormap.org/">
    <title>Custom colormaps for Matlab and Matplotlib - Colormap.org</title>
    <dc:date>2014-10-31T12:03:42+00:00</dc:date>
    <link>http://colormap.org/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[Create a custom colormap by dragging points on the RGB intensity curves.]]></description>
<dc:subject>matplotlib python work color</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:09e06127524e/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:matplotlib"/>
	<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:color"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://docs.python-guide.org/en/latest/">
    <title>The Hitchhiker’s Guide to Python! — The Hitchhiker's Guide to Python</title>
    <dc:date>2014-10-15T18:38:22+00:00</dc:date>
    <link>http://docs.python-guide.org/en/latest/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[This opinionated guide exists to provide both novice and expert Python developers a best-practice handbook to the installation, configuration, and usage of Python on a daily basis. ]]></description>
<dc:subject>development programming python work</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:36fcc73d2b25/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:development"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:programming"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:python"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="https://github.com/troydm/dotfiles/blob/master/.mc/skins/zenburn.ini">
    <title>dotfiles/zenburn.ini at master · troydm/dotfiles · GitHub</title>
    <dc:date>2014-09-03T10:46:57+00:00</dc:date>
    <link>https://github.com/troydm/dotfiles/blob/master/.mc/skins/zenburn.ini</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[# This is a Zenburn 256 colors MidnightCommander color scheme
# based on the Xoria256 color scheme
]]></description>
<dc:subject>zenburn color work</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:af8c9bff5832/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:zenburn"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:color"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://www.springer.com/mathematics/book/978-0-387-94746-4">
    <title>Handbook of Mathematics and Computational Science</title>
    <dc:date>2014-08-01T16:01:34+00:00</dc:date>
    <link>http://www.springer.com/mathematics/book/978-0-387-94746-4</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[A reference handbook for modern mathematics. The Handbook of Mathematical Formulas is filled with formulas, equations, tables, and explanations. This fully up to date handbook contains new and expanded chapters on Graphs and Algebras, Probability Theory and Mathematical Statistics, Fuzzy Logic, Neural Networks, and the use of computers. It will be the standard reference tool of mathematicians for years to come.]]></description>
<dc:subject>book mathematics work wantlist</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:9a65e7e4a6d9/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:book"/>
	<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:wantlist"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://cars.uchicago.edu/software/python/mpfit.html">
    <title>Python: module mpfit</title>
    <dc:date>2014-07-10T14:32:36+00:00</dc:date>
    <link>http://cars.uchicago.edu/software/python/mpfit.html</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[Perform Levenberg-Marquardt least-squares minimization, based on MINPACK-1.
 
                                   AUTHORS
  The original version of this software, called LMFIT, was written in FORTRAN
  as part of the MINPACK-1 package by XXX.
 
  Craig Markwardt converted the FORTRAN code to IDL.  The information for the
  IDL version is:
     Craig B. Markwardt, NASA/GSFC Code 662, Greenbelt, MD 20770
     craigm@lheamail.gsfc.nasa.gov
     UPDATED VERSIONs can be found on my WEB PAGE: 
        http://cow.physics.wisc.edu/~craigm/idl/idl.html
 
  Mark Rivers created this Python version from Craig's IDL version.
    Mark Rivers, University of Chicago
    Building 434A, Argonne National Laboratory
    9700 South Cass Avenue, Argonne, IL 60439
    rivers@cars.uchicago.edu
    Updated versions can be found at http://cars.uchicago.edu/software]]></description>
<dc:subject>python work code</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:94d2665a9b21/</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:work"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:code"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://ulisse.pd.astro.it/Astro/ADPS/">
    <title>ADPS: the Asiago Database on Photometric Systems</title>
    <dc:date>2014-03-27T15:23:51+00:00</dc:date>
    <link>http://ulisse.pd.astro.it/Astro/ADPS/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[ the Asiago Database on Photometric Systems ]]></description>
<dc:subject>work astronomy</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:85f2b7f7b968/</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:Bag></taxo:topics>
</item>
<item rdf:about="https://zenodo.org/">
    <title>ZENODO</title>
    <dc:date>2014-03-24T18:38:52+00:00</dc:date>
    <link>https://zenodo.org/</link>
    <dc:creator>Knusper2000</dc:creator><dc:subject>data research work</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:c52f65e5e267/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:data"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:research"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="https://www.eso.org/sci/software/eclipse/qfits/index.html">
    <title>ESO - Eclipse</title>
    <dc:date>2014-03-06T20:05:12+00:00</dc:date>
    <link>https://www.eso.org/sci/software/eclipse/qfits/index.html</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[qfits is a stand-alone C library offering easy access to FITS files. ]]></description>
<dc:subject>work fits</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:29a3c0661a46/</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:fits"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://press.princeton.edu/titles/10159.html">
    <title>Ivezic, Z., Connolly, A.J., VanderPlas, J.T., Gray, A.: Statistics, Data Mining, and Machine Learning in Astronomy: A Practical Python Guide for the Analysis of Survey Data. (eBook and Cloth)</title>
    <dc:date>2014-02-06T10:46:43+00:00</dc:date>
    <link>http://press.princeton.edu/titles/10159.html</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[ 

As telescopes, detectors, and computers grow ever more powerful, the volume of data at the disposal of astronomers and astrophysicists will enter the petabyte domain, providing accurate measurements for billions of celestial objects. This book provides a comprehensive and accessible introduction to the cutting-edge statistical methods needed to efficiently analyze complex data sets from astronomical surveys such as the Panoramic Survey Telescope and Rapid Response System, the Dark Energy Survey, and the upcoming Large Synoptic Survey Telescope. It serves as a practical handbook for graduate students and advanced undergraduates in physics and astronomy, and as an indispensable reference for researchers.

Statistics, Data Mining, and Machine Learning in Astronomy presents a wealth of practical analysis problems, evaluates techniques for solving them, and explains how to use various approaches for different types and sizes of data sets. For all applications described in the book, Python code and example data sets are provided. The supporting data sets have been carefully selected from contemporary astronomical surveys (for example, the Sloan Digital Sky Survey) and are easy to download and use. The accompanying Python code is publicly available, well documented, and follows uniform coding standards. Together, the data sets and code enable readers to reproduce all the figures and examples, evaluate the methods, and adapt them to their own fields of interest.]]></description>
<dc:subject>work astronomy python statistics book</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:c01aa9184ba7/</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:python"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:statistics"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:book"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://zenodo.org/">
    <title>ZENODO</title>
    <dc:date>2014-01-28T15:30:22+00:00</dc:date>
    <link>http://zenodo.org/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[Research. Shared. — all research outputs from across all fields of science are welcome!
Citeable. Discoverable. — uploads gets a Digital Object Identifier (DOI) to make them easily and uniquely citeable.
Community Collections — accept or reject uploads to your own community collections (e.g workshops, EU projects or your complete own digital repository).
Funding — integrated in reporting lines for research funded by the European Commission via OpenAIRE.
Flexible licensing — because not everything is under Creative Commons.
Safe — your research output is stored safely for the future in same cloud infrastructure as research data from CERN's Large Hadron Collider.
DropBox integration — upload files straight from your DropBox.]]></description>
<dc:subject>data opendata repository science work</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:a42c5ed3c393/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:data"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:opendata"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:repository"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:science"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://thedata.org/">
    <title>The Dataverse Network</title>
    <dc:date>2014-01-28T15:24:48+00:00</dc:date>
    <link>http://thedata.org/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[A repository for research data that takes care of
long term preservation and good archival practices, while researchers can share, keep control of and get recognition for their data.]]></description>
<dc:subject>data opensource repository research work</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:7f1446cc76fe/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:data"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:opensource"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:repository"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:research"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://aladin.u-strasbg.fr/">
    <title>Aladin Sky Atlas</title>
    <dc:date>2014-01-21T12:15:25+00:00</dc:date>
    <link>http://aladin.u-strasbg.fr/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[Aladin is an interactive software sky atlas allowing the user to visualize digitized astronomical images, superimpose entries from astronomical catalogues or databases, ]]></description>
<dc:subject>astronomy work software</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:3ea0d02f80e9/</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:work"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:software"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://archive.stsci.edu/prepds/xdf/">
    <title>XDF Data Release</title>
    <dc:date>2013-11-05T16:44:33+00:00</dc:date>
    <link>http://archive.stsci.edu/prepds/xdf/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[This summary describes the Hubble eXtreme Deep Field (XDF) project data release. The XDF includes all optical and infrared data taken by Hubble covering the original Hubble Ultra-Deep Field (HUDF) program, with just a few exceptions. Small amounts of data taken with unusual or rarely used filters and spectroscopic data are not included. The XDF also includes images which only partially cover the HUDF, as shown in the figure below. The weight maps are appropriately adjusted for the partial coverage.]]></description>
<dc:subject>work astronomy hubble data</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:42aec160c636/</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:hubble"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:data"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://iopscience.iop.org/0067-0049/209/1/6/">
    <title>The HST eXtreme Deep Field (XDF): Combining All ACS and WFC3/IR Data on the HUDF Region into the Deepest Field Ever - Abstract - The Astrophysical Journal Supplement Series - IOPscience</title>
    <dc:date>2013-11-05T16:42:50+00:00</dc:date>
    <link>http://iopscience.iop.org/0067-0049/209/1/6/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[The eXtreme Deep Field (XDF) combines data from 10 years of observations with the Hubble Space Telescope Advanced Camera for Surveys (ACS) and the Wide-Field Camera 3 Infra-Red (WFC3/IR) into the deepest image of the sky ever in the optical/near-IR. Since the initial observations of the Hubble Ultra-Deep Field (HUDF) in 2003, numerous surveys and programs, including supernovae follow-up, HUDF09, CANDELS, and HUDF12, have contributed additional imaging data across this region. However, these images have never been combined and made available as one complete ultra-deep image dataset. We combine them now with the XDF program. Our new and improved processing techniques provide higher quality reductions of the total dataset. All WFC3/IR and optical ACS data sets have been fully combined and accurately matched, resulting in the deepest imaging ever taken at these wavelengths, ranging from 29.1 to 30.3 AB mag (5σ in a 0.''35 diameter aperture) in 9 filters. The combined image therefore reaches to 31.2 AB mag 5σ (32.9 at 1σ) for a flat f ν source. The gains in the optical for the four filters done in the original ACS HUDF correspond to a typical improvement of 0.15 mag, with gains of 0.25 mag in the deepest areas. Such gains are equivalent to adding ~130 to ~240 orbits of ACS data to the HUDF. Improved processing alone results in a typical gain of ~0.1 mag. Our 5σ (optical+near-IR) SExtractor catalogs reveal about 14,140 sources in the full field and about 7121 galaxies in the deepest part of the XDF.]]></description>
<dc:subject>hubble work astronomy journal article</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:50d9f3e81cf7/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:hubble"/>
	<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:journal"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:article"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://www3.cadc-ccda.hia-iha.nrc-cnrc.gc.ca/en/meetings/">
    <title>International Astronomy Meetings - Canadian Astronomy Data Centre</title>
    <dc:date>2013-10-29T14:11:38+00:00</dc:date>
    <link>http://www3.cadc-ccda.hia-iha.nrc-cnrc.gc.ca/en/meetings/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[This list of astronomy meetings was originally compiled by Liz Bryson, the now retired librarian of the Canada-France-Hawaii Telescope Corporation, from 1996 to 2011. The list is currently archived and maintained by the Canadian Astronomy Data Centre (CADC) of NRC Herzberg. Use the Search menu to view meetings by month or year or by keyword. Included with each entry of the Meetings List are links to the meeting web page, contact e-mail addresses, and abstracts provided by NASA's Astrophysics Data System (ADS) if, and when they are available.]]></description>
<dc:subject>astronomy conference work calendar</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:dd5a9223bff9/</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:conference"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:calendar"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://www.astro.utoronto.ca/~patton/astro/mags.html">
    <title>Astronomical Magnitude Systems</title>
    <dc:date>2013-10-23T16:09:02+00:00</dc:date>
    <link>http://www.astro.utoronto.ca/~patton/astro/mags.html</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[Definitions of astronomical magnitude systems:
Conversion from AB magnitudes to Johnson magnitudes
Photon Flux
Filter Transformations
Night Sky Brightnesses]]></description>
<dc:subject>astronomy work</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:5a587ef5d507/</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:work"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://cars9.uchicago.edu/software/python/lmfit/">
    <title>Non-Linear Least-Square Minimization for Python — Least-Squares Minimization with Constraints for Python</title>
    <dc:date>2013-09-02T09:23:39+00:00</dc:date>
    <link>http://cars9.uchicago.edu/software/python/lmfit/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[The lmfit Python package provides a simple, flexible interface to non-linear optimization or curve fitting problems. The package extends the optimization capabilities of scipy.optimize by replacing floating pointing values for the variables to be optimized with Parameter objects. These Parameters can be fixed or varied, have upper and/or lower bounds placed on its value, or written as an algebraic expression of other Parameters.]]></description>
<dc:subject>python work</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:4cff43643e06/</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:work"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://archive.eso.org/asm/ambient-server">
    <title>ESO Ambient Conditions Database</title>
    <dc:date>2013-07-04T18:19:13+00:00</dc:date>
    <link>http://archive.eso.org/asm/ambient-server</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[ESO Observatories
Ambient Conditions Database]]></description>
<dc:subject>work astronomy</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:a847912cccbf/</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:Bag></taxo:topics>
</item>
<item rdf:about="http://iopscience.iop.org/0004-637X/772/1/3">
    <title>The Angular Distribution of Lyα Resonant Photons Emerging from an Optically Thick Medium - Abstract - The Astrophysical Journal - IOPscience</title>
    <dc:date>2013-06-28T16:31:16+00:00</dc:date>
    <link>http://iopscience.iop.org/0004-637X/772/1/3</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[We investigate the angular distribution of Lyα photons scattering or emerging from an optically thick medium. Since the evolution of specific intensity I in frequency space and angular space are coupled with each other, we first develop the WENO numerical solver to find the time-dependent solutions of the integro-differential equation of I in frequency and angular space simultaneously. We first show that the solutions with the Eddington approximation, which assume that I is linearly dependent on the angular variable μ, yield similar frequency profiles of the photon flux as those without the Eddington approximation. However, the solutions of the μ distribution evolution are significantly different from those given by the Eddington approximation. First, the angular distribution of I is found to be substantially dependent on the frequency of the photons. For photons with the resonant frequency ν0, I contains only a linear term of μ. For photons with frequencies at the double peaks of the flux, the μ-distribution is highly anisotropic; most photons are emitted radially forward. Moreover, either at ν0 or at the double peaks, the μ distributions actually are independent of the initial μ distribution of photons of the source. This is because the photons with frequencies either at ν0 or the double peaks undergo the process of forgetting their initial conditions due to resonant scattering. We also show that the optically thick medium is a collimator of photons at the double peaks. Photons from the double peaks form a forward beam with a very small opening angle.]]></description>
<dc:subject>paper work math astronomy physics</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:fb98bddbe1a3/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:paper"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:math"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:astronomy"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:physics"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://www.nature.com/nature/journal/v487/n7407/full/nature11256.html">
    <title>High velocity dispersion in a rare grand-design spiral galaxy at redshift z = 2.18 : Nature : Nature Publishing Group</title>
    <dc:date>2013-06-25T22:39:49+00:00</dc:date>
    <link>http://www.nature.com/nature/journal/v487/n7407/full/nature11256.html</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[So-called grand-design spiral galaxies feature prominent and well-defined spiral arms, rather than the arguably less striking multi-arm flocculent spiral structure. Grand-design spiral galaxies are relatively common in the local Universe, but uncommon at redshifts of z > 2, prompting suggestions that conditions in the early Universe favoured the formation of less well-defined clumpy galaxies. But this paper reports observations of a distant grand design spiral galaxy Q2343-BX442 at z = 2.18 that show that the disk is dynamically hot — a condition that was thought to favour clumpy structures. The data indicate that the galaxy is a thick disk undergoing a minor merger with another system, and it may be this merger that is driving the formation of short-lived spiral structure.]]></description>
<dc:subject>work astronomy paper</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:8416e117d46f/</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:paper"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://bpython-interpreter.org/">
    <title>bpython interpreter</title>
    <dc:date>2013-05-21T19:15:17+00:00</dc:date>
    <link>http://bpython-interpreter.org/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[bpython is a fancy interface to the Python interpreter]]></description>
<dc:subject>programming python shell tools work</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:287684934613/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:programming"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:python"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:shell"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:tools"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://www.sussex.ac.uk/Users/sw376/XDF/">
    <title>XDF Multi-wavelength</title>
    <dc:date>2013-05-20T16:20:18+00:00</dc:date>
    <link>http://www.sussex.ac.uk/Users/sw376/XDF/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[The Hubble eXtreme Deep Field (XDF) is a project to combine all available Hubble Space Telescope imaging of the Hubble Ultra Deep Field (HUDF). Observations of the XDF field come from 19 different programmes though with the majority coming from 3 programmes: HUDF, HUDF09, HUDF12. The original HUDF. With the installation of Wide Field Camera 3 (WFC3) in 2009 the HUDF09 programme obtained deep near-IR observations of a portion of the HUDF. This was further augmented by the HUDF12 programme.]]></description>
<dc:subject>science work web web2.0 hubble astronomy</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:c0485390a54f/</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:work"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:web"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:web2.0"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:hubble"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:astronomy"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://tkf.github.io/emacs-jedi/">
    <title>Jedi.el - Python auto-completion for Emacs — Emacs Jedi 0.1.2alpha2 documentation</title>
    <dc:date>2013-04-27T10:25:15+00:00</dc:date>
    <link>http://tkf.github.io/emacs-jedi/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[Jedi.el is a Python auto-completion package for Emacs. It aims at helping your Python coding in a non-destructive way. It also helps you to find information about Python objects, such as docstring, function arguments and code location.]]></description>
<dc:subject>python emacs work programming productivity</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:060d70ecc323/</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:emacs"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:programming"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:productivity"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://www.aanda.org/index.php?option=com_article&amp;access=standard&amp;Itemid=129&amp;url=/articles/aa/abs/2010/15/aa15236-10/aa15236-10.html">
    <title>Predicted UV properties of very metal-poor starburst galaxies | A&amp;A</title>
    <dc:date>2013-04-09T18:31:38+00:00</dc:date>
    <link>http://www.aanda.org/index.php?option=com_article&amp;access=standard&amp;Itemid=129&amp;url=/articles/aa/abs/2010/15/aa15236-10/aa15236-10.html</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[Aims. We study the expected properties of starburst galaxies in order to provide the point of reference for interpretation of high-z galaxy surveys and of very metal-poor galaxies. We concentrate mainly on the UV characteristics such as the ionizing spectra, the UV continuum, the Lyα and He ii λ1640 line and two-photon continuum emission.

Methods. We use evolutionary synthesis models covering metallicities from Pop III to solar and a wide range of IMFs. We also combine the synthetic SEDs with the CLOUDY photoionization code for more accurate predictions of nebular emission, and to study possible departures from case B assumed in the synthesis models.

Results. The ionizing fluxes, UV continuum properties, and predicted Lyα and He ii λ1640 line strengths are presented for synthesis models covering a wider range of parameter space than our earlier calculations. Strong departures from case B predictions are obtained for Lyα and 2γ continuum at low metallicities. At low nebular densities both are shown to be enhanced proportionally to the mean energy carried by the Lyman continuum photons emitted by the ionizing source. Larger Lyα equivalent widths are therefore predicted at low metallicity. The He ii λ1640 line can be weaker than case B predicts (in terms of flux as well as the equivalent width) due to its ionization parameter dependence and to the enhanced underlying 2γ continuum.

Conclusions. Our results have implications for the interpretation of star-forming metal-poor and/or high redshift galaxies, for galaxies among the Lyα emitters (LAE) and Lyman Break galaxy (LBG) populations, and for searches of Population III stars in the distant Universe.]]></description>
<dc:subject>work paper reading data simulation</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:ce3a875c0326/</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:paper"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:reading"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:data"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:simulation"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://jakevdp.github.io/blog/2013/03/23/matplotlib-and-the-future-of-visualization-in-python/">
    <title>Matplotlib and the Future of Visualization in Python - Pythonic Perambulations</title>
    <dc:date>2013-04-08T17:43:34+00:00</dc:date>
    <link>http://jakevdp.github.io/blog/2013/03/23/matplotlib-and-the-future-of-visualization-in-python/</link>
    <dc:creator>Knusper2000</dc:creator><dc:subject>python matplotlib history work visualization</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:b5293d454302/</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:matplotlib"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:history"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:visualization"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://dan.iel.fm/">
    <title>Dan Foreman-Mackey</title>
    <dc:date>2013-04-04T16:48:17+00:00</dc:date>
    <link>http://dan.iel.fm/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[I'm a graduate student at NYU working on next generation astronomical data analysis under the supervision of David W. Hogg. When I'm not writing code, I'm probably climbing rocks somewhere. Take a look at my C.V. or scroll down to read about some of the projects that I'm working on.
]]></description>
<dc:subject>work astronomy code python</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:b056a2d05c28/</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:code"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:python"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://aer.aas.org/">
    <title>Astronomy Education Review</title>
    <dc:date>2013-04-02T14:17:42+00:00</dc:date>
    <link>http://aer.aas.org/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[Astronomy Education Review (AER) is a web-based journal for everyone who works in astronomy and space science education. Published by the American Astronomical Society, the journal welcomes research papers, short articles on innovative work, and comparative reviews of resources related to education and outreach. All papers and articles are refereed.]]></description>
<dc:subject>work science education astronomy</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:ce01793f7fed/</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:science"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:education"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:astronomy"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://arxiv.org/abs/1303.5961">
    <title>[1303.5961] Paper-and-pencil cosmological calculator</title>
    <dc:date>2013-03-28T12:43:03+00:00</dc:date>
    <link>http://arxiv.org/abs/1303.5961</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[The paper-and-pencil calculator is a cosmological nomogram which allows to find relations between redshift, distance, age of the Universe, physical and angular sizes, luminosity and apparent magnitude for the standard cosmological model with parameters from the Planck mission. ]]></description>
<dc:subject>astronomy work teaching cosmology science paper arxiv</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:17f41db12f0f/</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:work"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:teaching"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:cosmology"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:science"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:paper"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:arxiv"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="https://en.wikipedia.org/wiki/Sparse_matrix#CITEREFStoerBulirsch2002">
    <title>Sparse matrix - Wikipedia, the free encyclopedia</title>
    <dc:date>2013-03-27T11:35:17+00:00</dc:date>
    <link>https://en.wikipedia.org/wiki/Sparse_matrix#CITEREFStoerBulirsch2002</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[In the subfield of numerical analysis, a sparse matrix is a matrix populated primarily with zeros (Stoer & Bulirsch 2002, p. 619) as elements of the table. By contrast, if a larger number of elements differ from zero, then it is common to refer to the matrix as a dense matrix. The fraction of zero elements (non-zero elements) in a matrix is called the sparsity (density).]]></description>
<dc:subject>work mathematics science</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:1fac4a900751/</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:mathematics"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:science"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://docs.scipy.org/doc/scipy/reference/generated/scipy.spatial.KDTree.html">
    <title>scipy.spatial.KDTree — SciPy v0.11 Reference Guide (DRAFT)</title>
    <dc:date>2013-03-27T10:35:19+00:00</dc:date>
    <link>http://docs.scipy.org/doc/scipy/reference/generated/scipy.spatial.KDTree.html</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[This class provides an index into a set of k-dimensional points which can be used to rapidly look up the nearest neighbors of any point.]]></description>
<dc:subject>scipy work</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:cd778c85dca9/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:scipy"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://svnbook.red-bean.com/index.en.html">
    <title>Version Control with Subversion</title>
    <dc:date>2013-03-25T11:06:10+00:00</dc:date>
    <link>http://svnbook.red-bean.com/index.en.html</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[This is the home of Version Control with Subversion, a free book about the ubiquitous Apache™ Subversion® version control system and written by some of the developers of Subversion itself.]]></description>
<dc:subject>book svn work free ebook</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:4df7038f466d/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:book"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:svn"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:free"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:ebook"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://arxiv.org/abs/1201.2434">
    <title>[1201.2434] Observational Probes of Cosmic Acceleration</title>
    <dc:date>2013-03-20T10:57:40+00:00</dc:date>
    <link>http://arxiv.org/abs/1201.2434</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[The accelerating expansion of the universe is the most surprising cosmological discovery in many decades, implying that the universe is dominated by some form of "dark energy" with exotic physical properties, or that Einstein's theory of gravity breaks down on cosmological scales. The profound implications of cosmic acceleration have inspired ambitious experimental efforts to measure the history of expansion and growth of structure with percent-level precision or higher. We review in detail the four most well established methods for making such measurements: Type Ia supernovae, baryon acoustic oscillations (BAO), weak gravitational lensing, and galaxy clusters. We pay particular attention to the systematic uncertainties in these techniques and to strategies for controlling them at the level needed to exploit "Stage IV" dark energy facilities such as BigBOSS, LSST, Euclid, and WFIRST. We briefly review a number of other approaches including redshift-space distortions, the Alcock-Paczynski test, and direct measurements of H_0. We present extensive forecasts for constraints on the dark energy equation of state and parameterized deviations from GR, achievable with Stage III and Stage IV experimental programs that incorporate supernovae, BAO, weak lensing, and CMB data. We also show the level of precision required for other methods to provide constraints competitive with those of these fiducial programs. We emphasize the value of a balanced program that employs several of the most powerful methods in combination, both to cross-check systematic uncertainties and to take advantage of complementary information. Surveys to probe cosmic acceleration produce data sets with broad applications, and they continue the longstanding astronomical tradition of mapping the universe in ever greater detail over ever larger scales. ]]></description>
<dc:subject>science reference review work</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:debdb4a4b22c/</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:reference"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:review"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://www.subversion-server.com/">
    <title>Subversion-Hosting :: Made in Germany.</title>
    <dc:date>2013-03-08T18:51:20+00:00</dc:date>
    <link>http://www.subversion-server.com/</link>
    <dc:creator>Knusper2000</dc:creator><dc:subject>work subversion web service hosting</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:4142cba4e308/</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:subversion"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:web"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:service"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:hosting"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://www.springer.com/astronomy/book/978-1-4614-3766-6">
    <title>Astrophysics of the Interstellar Medium</title>
    <dc:date>2013-03-01T11:55:40+00:00</dc:date>
    <link>http://www.springer.com/astronomy/book/978-1-4614-3766-6</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[    Although this book presents comprehensive material on the interstellar medium, it has a simpler presentation and is intended specifically for astrophysics students
    Simple numerical estimates are given throughout the book, making it an ideal undergraduate textbook
    Offers more than just basic knowledge of the structure and evolution of galaxies

The space between the stars includes a large variety of objects, where physical processes occur that are fundamental for the structure and evolution of galaxies. This book gives the reader some basic knowledge of these processes and at the same time, presents estimates of the main quantities relevant to the study of the interstellar medium. The book could be used as an introductory course on the interstellar medium  by science students or by readers interested in astrophysics with an adequate physics and mathematics background.]]></description>
<dc:subject>book astronomy work</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:fbaacab71ca7/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:book"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:astronomy"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="https://github.com/gabrielelanaro/emacs-for-python#readme">
    <title>gabrielelanaro/emacs-for-python · GitHub</title>
    <dc:date>2013-02-22T19:51:36+00:00</dc:date>
    <link>https://github.com/gabrielelanaro/emacs-for-python#readme</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[I’m collecting and customizing the perfect environment for python developement, using the most beautiful emacs customization to obtain a really modern and exciting (yet stable) way to edit text files.]]></description>
<dc:subject>python emacs work</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:6db96bdd9c9a/</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:emacs"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://www.mpa-garching.mpg.de/halo2013/index.php">
    <title>The Physical Link between Galaxies and their Halos, An International Conference, Garching bei München, Germany, 25-29 June 2013</title>
    <dc:date>2013-02-18T13:15:22+00:00</dc:date>
    <link>http://www.mpa-garching.mpg.de/halo2013/index.php</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[Galaxies are surrounded by extended halos of stars, gas and dark matter. The stars appear to be debris from accreted dwarfs. The gas flows both in and out, forming hydrostatic atmospheres in massive systems. The dark matter dominates the overall mass budget, providing the gravitational context for the growth and evolution of the central galaxy. Recent observations have shed light on all these components: resolved star studies and low surface brightness photometry on the stellar halo; UV absorption, X-ray emission, and stacked 21cm and SZ measurements on circumgalactic gas; and galaxy-galaxy lensing and dynamical studies based on a variety of tracers on dark matter halos. In our current paradigm for structure formation, the three kinds of halos interact strongly and play an important role in shaping the galaxies we see. This conference aims to bring together observers and theorists in the broad range of areas providing insight into the physical mechanisms governing these galaxy-halo connections. ]]></description>
<dc:subject>conference astronomy work</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:c312023d1823/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:conference"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:astronomy"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://www.astropy.org/">
    <title>Astropy</title>
    <dc:date>2013-02-13T16:55:49+00:00</dc:date>
    <link>http://www.astropy.org/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[
The Astropy project is a common effort to develop a single core package for Astronomy that brings together almost 100 developers from around the world.]]></description>
<dc:subject>astronomy programming python work</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:1ddcdce23589/</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:programming"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:python"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://blockdiag.com/en/">
    <title>blockdiag - simple diagram images generator — blockdiag 1.0 documentation</title>
    <dc:date>2013-02-07T19:44:13+00:00</dc:date>
    <link>http://blockdiag.com/en/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[blockdiag and its family generate diagram images from simply text file]]></description>
<dc:subject>graphics python software work</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:947b4e20e5df/</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:python"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:software"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://www.secnetix.de/olli/Python/lambda_functions.hawk">
    <title>Python: Lambda Functions</title>
    <dc:date>2013-02-06T16:32:17+00:00</dc:date>
    <link>http://www.secnetix.de/olli/Python/lambda_functions.hawk</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[ Python supports the creation of anonymous functions (i.e. functions that are not bound to a name) at runtime, using a construct called "lambda". This is not exactly the same as lambda in functional programming languages, but it is a very powerful concept that's well integrated into Python and is often used in conjunction with typical functional concepts like filter(), map() and reduce(). ]]></description>
<dc:subject>python work programming</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:bd67392035a4/</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:work"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:programming"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://kmike.ru/python-data-structures/">
    <title>Fast Non-Standard Data Structures for Python</title>
    <dc:date>2013-01-29T16:07:44+00:00</dc:date>
    <link>http://kmike.ru/python-data-structures/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[Python provides great built-in types like dict, list, tuple and set; there are also array, collections, heapq modules in the standard library; this article is an overview of external lesser known packages with fast C/C++ based data structures usable from Python.]]></description>
<dc:subject>data python work programming</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:70eac32bce8f/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:data"/>
	<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:programming"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://astronomy.swin.edu.au/s2plot/index.php?title=S2PLOT">
    <title>S2PLOT - S2PLOT</title>
    <dc:date>2013-01-28T09:56:38+00:00</dc:date>
    <link>http://astronomy.swin.edu.au/s2plot/index.php?title=S2PLOT</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[S2PLOT is an advanced three-dimensional plotting library with support for standard and enhanced display devices. The S2PLOT library was written in C and can be used with C, C++ and FORTRAN programs on GNU/Linux and Apple/OSX. The S2PLOT architecture supports dynamic geometry and can be used to plot both static and time-evolving data sets. S2PLOT is based on the OpenGL graphics library.

]]></description>
<dc:subject>science work 3d astronomy visualization</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:2eb2111b7d5e/</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:work"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:3d"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:astronomy"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:visualization"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://www.physics.ox.ac.uk/users/msshin/science/code/index.html">
    <title>SDSS tools and other codes developed by Min-Su Shin</title>
    <dc:date>2012-12-30T22:45:45+00:00</dc:date>
    <link>http://www.physics.ox.ac.uk/users/msshin/science/code/index.html</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[I've developed several scripts and codes for my research. Some of them might be useful to other people. Feel free to use and modify the following codes. However, please let me know it. (E-mail address : Min-Su.Shin @ astro.ox.ac.uk)]]></description>
<dc:subject>work astronomy software code script scripting science</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:cd1236353479/</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:code"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:script"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:scripting"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:science"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://www.geological-supplies.com/scripts/?page=scripts">
    <title>Scripts for researchers - GeoLogic – Buy Geological Hammers and Supplies</title>
    <dc:date>2012-11-26T21:00:53+00:00</dc:date>
    <link>http://www.geological-supplies.com/scripts/?page=scripts</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[Scripts for researchers

Research can be tedious; we have written a variety of scripts to make finding and reading journal articles easier.]]></description>
<dc:subject>greasemonkey science script work browser help tools</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:25ca6efe4435/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:greasemonkey"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:science"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:script"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:browser"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:help"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:tools"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://www.mpe.mpg.de/~forster/SINS/sins_nmfs.html">
    <title>The SINS Survey</title>
    <dc:date>2012-11-21T09:41:43+00:00</dc:date>
    <link>http://www.mpe.mpg.de/~forster/SINS/sins_nmfs.html</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[SINS, the Spectroscopic Imaging survey in the Near-infrared with SINFONI, is a large and coherent program to investigate in detail the dynamics and physical properties of representative samples of distant luminous galaxy populations. This on-going survey is providing new insights into the assembly and the evolution of young galaxies present in the Universe just a few billion years after the Big Bang. SINS takes advantage of the unique opportunities afforded by SINFONI at ESO's Very Large Telescope, a near-infrared integral field spectrometer combined with an adaptive optics system that delivers sharp images simultaneously with high resolution spectral information. ]]></description>
<dc:subject>work astronomy survey</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:bc55e50fda0d/</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:survey"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://arxiv.org/abs/1211.3663v1">
    <title>[1211.3663v1] CLASH: Three Strongly Lensed Images of a Candidate z ~ 11 Galaxy</title>
    <dc:date>2012-11-17T22:11:54+00:00</dc:date>
    <link>http://arxiv.org/abs/1211.3663v1</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[We present a candidate for the most distant galaxy known to date with a photometric redshift z = 10.7 +0.6 / -0.4 (95% confidence limits; with z < 9.5 galaxies of known types ruled out at 7.2-sigma). This J-dropout Lyman Break Galaxy, named MACS0647-JD, was discovered as part of the Cluster Lensing and Supernova survey with Hubble (CLASH). We observe three magnified images of this galaxy due to strong gravitational lensing by the galaxy cluster MACSJ0647.7+7015 at z = 0.591. The images are magnified by factors of ~8, 7, and 2, with the brighter two observed at ~26th magnitude AB (~0.15 uJy) in the WFC3/IR F160W filter (~1.4 - 1.7 um) where they are detected at >~ 12-sigma. All three images are also confidently detected at >~ 6-sigma in F140W (~1.2 - 1.6 um), dropping out of detection from 15 lower wavelength HST filters (~0.2 - 1.4 um), and lacking bright detections in Spitzer/IRAC 3.6um and 4.5um imaging (~3.2 - 5.0 um). We rule out a broad range of possible lower redshift interlopers, including some previously published as high redshift candidates. Our high redshift conclusion is more conservative than if we had neglected a Bayesian photometric redshift prior. Given CLASH observations of 17 high mass clusters to date, our discoveries of MACS0647-JD at z ~ 10.8 and MACS1149-JD1 at z ~ 9.6 are consistent with a lensed luminosity function extrapolated from lower redshifts. This would suggest that low luminosity galaxies could have reionized the universe. However given the significant uncertainties based on only two galaxies, we cannot yet rule out the sharp drop off in number counts at z >~ 10 suggested by field searches. ]]></description>
<dc:subject>arxiv work reading</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:f951edee7d1c/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:arxiv"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:reading"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://jsky.sourceforge.net/">
    <title>JSky</title>
    <dc:date>2012-11-16T18:24:28+00:00</dc:date>
    <link>http://jsky.sourceforge.net/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[JSky - Java Components for Astronomy

The aim of the JSky project is to build a collection of reusable Java components for use in astronomy. The project originally grew out of the development of the Skycat application at ESO and a first draft of the design ideas were presented at the ADASS'99 conference. JSky was originally developed at ESO and then later as part of the Gemini Observing Tool , which astronomers use to plan their observations at the Gemini Telescope. ]]></description>
<dc:subject>work astronomy software</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:97c246135c7f/</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:Bag></taxo:topics>
</item>
<item rdf:about="http://www.pa.uky.edu/~peter/atomic/index.html">
    <title>Atomic Line List v2.04</title>
    <dc:date>2012-11-15T20:45:42+00:00</dc:date>
    <link>http://www.pa.uky.edu/~peter/atomic/index.html</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[This is a compilation of approximately 923,000 allowed, intercombination and forbidden atomic transitions with wavelengths in the range from 0.5 Å to 1000 µm. It's primary intention is to allow the identification of observed atomic absorption or emission features. The wavelengths in this list are all calculated from the difference between the energy of the upper and lower level of the transition. No attempt has been made to include observed wavelengths. Most of the atomic energy level data have been taken from the Atomic Spectra Database provided by the National Institute of Standards and Technology (NIST). ]]></description>
<dc:subject>work astronomy</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:4bf0a10b94a5/</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:Bag></taxo:topics>
</item>
<item rdf:about="http://fuse.pha.jhu.edu/support/tools/vlsr.html">
    <title>Ed Murphy's VLSR Calculator Version 1.0</title>
    <dc:date>2012-11-13T09:06:12+00:00</dc:date>
    <link>http://fuse.pha.jhu.edu/support/tools/vlsr.html</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[This routine will calculate the radial velocity of the observer with respect to a given RA and DEC on the date of observation for a number of popular standards of rest.]]></description>
<dc:subject>astronomy work calculator</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:ac20ef32ca38/</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:work"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:calculator"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://prezi.com/">
    <title>Prezi - Ideas matter.</title>
    <dc:date>2012-11-12T09:48:07+00:00</dc:date>
    <link>http://prezi.com/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[Prezi is a communication tool that helps you organize, present, and share your ideas.]]></description>
<dc:subject>presentation presentations tools visualization work</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:2e38979089be/</dc:identifier>
<taxo:topics><rdf:Bag>	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:presentation"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:presentations"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:tools"/>
	<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://xdvi.sourceforge.net/">
    <title>Xdvik Homepage</title>
    <dc:date>2012-10-31T18:39:00+00:00</dc:date>
    <link>http://xdvi.sourceforge.net/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[Xdvik is a program for displaying DVI files (generated e.g. by Troff or TeX) on the X window system. It is based on the regular (non-k) xdvi of the same version number. ]]></description>
<dc:subject>linux software work opensource</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:e541dfb0dba3/</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:software"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:work"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:opensource"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://roban.github.com/CosmoloPy/">
    <title>CosmoloPy: a cosmology package for Python.</title>
    <dc:date>2012-10-08T16:30:29+00:00</dc:date>
    <link>http://roban.github.com/CosmoloPy/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[ a cosmology package for Python. ]]></description>
<dc:subject>work astronomy python cosmology programming code</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:5069157bb86c/</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:python"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:cosmology"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:programming"/>
	<rdf:li rdf:resource="https://pinboard.in/u:Knusper2000/t:code"/>
</rdf:Bag></taxo:topics>
</item>
<item rdf:about="http://irlab.astro.ucla.edu/mosfire/">
    <title>MOSFIRE Home Page</title>
    <dc:date>2012-10-02T15:29:53+00:00</dc:date>
    <link>http://irlab.astro.ucla.edu/mosfire/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[The leaders of the MOSFIRE team are Prof. Ian McLean (UCLA) and Prof. Charles Steidel (Caltech), with other leading roles in instrumentation, optics and astronomical software being played by Keith Matthews (Caltech), Prof. Harland Epps (UCSC), and Prof. James Larkin (UCLA) respectively. The project is managed by Sean Adkins for the W.M. Keck Observatory. ]]></description>
<dc:subject>astronomy instrument work</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:d352fcc7cfd6/</dc:identifier>
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<item rdf:about="http://casa.nrao.edu/">
    <title>CASA</title>
    <dc:date>2012-09-30T16:51:29+00:00</dc:date>
    <link>http://casa.nrao.edu/</link>
    <dc:creator>Knusper2000</dc:creator><description><![CDATA[CASA, the Common Astronomy Software Applications package, is being developed with the primary goal of supporting the data post-processing needs of the next generation of radio astronomical telescopes such as ALMA and EVLA. The package can process both interferometric and single dish data, and is developed by an international consortium of scientists based at the National Radio Astronomical Observatory (NRAO), the European Southern Observatory (ESO), the National Astronomical Observatory of Japan (NAOJ), the CSIRO Australia Telescope National Facility (CSIRO/ATNF), and the Netherlands Institute for Radio Astronomy (ASTRON) under the guidance of NRAO. ]]></description>
<dc:subject>astronomy python software 3d work</dc:subject>
<dc:source>https://pinboard.in/</dc:source>
<dc:identifier>https://pinboard.in/u:Knusper2000/b:5903b04b1d1d/</dc:identifier>
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