@INPROCEEDINGS{2016IAUS..319...17G,
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  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}


@ARTICLE{2016A&ARv..24...10T,
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@ARTICLE{2016ASSL..418..317B,
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@ARTICLE{2006ApJ...645.1092Q,
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@ARTICLE{2016AN....337..410T,
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@ARTICLE{2017arXiv170306889H,
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@ARTICLE{2006ApJS..163....1H,
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@conference{springelfeedback,
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}



@unpublished{koristafeedback,
  title        = {Quasars and the Birth \& Evolution of Galaxies},
  year         = 2016,
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}


@book{maoz2007astrophysics,
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@ARTICLE{2017ApJ...837..149G,
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@ARTICLE{2010A&A...523A..32K,
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@ARTICLE{2006astro.ph..8019L,
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 @misc{ wiki:MILLENRUN,
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 @misc{ wiki:AGN,
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 @misc{ wiki:LCDM,
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@ARTICLE{2005Natur.435..629S,
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@ARTICLE{2005MNRAS.361..776S,
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@ARTICLE{2005ApJ...620L..79S,
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@ARTICLE{2006MNRAS.366..397S,
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@Article{C3CS60279F,
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year  ="2014",
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issue  ="7",
pages  ="2098-2111",
publisher  ="The Royal Society of Chemistry",
doi  ="10.1039/C3CS60279F",
url  ="http://dx.doi.org/10.1039/C3CS60279F",
abstract  ="Currently{,} organic crystal structure prediction (CSP) methods are based on searching for the most thermodynamically stable crystal structure{,} making various approximations in evaluating the crystal energy. The most stable (global minimum) structure provides a prediction of an experimental crystal structure. However{,} depending on the specific molecule{,} there may be other structures which are very close in energy. In this case{,} the other structures on the crystal energy landscape may be polymorphs{,} components of static or dynamic disorder in observed structures{,} or there may be no route to nucleating and growing these structures. A major reason for performing CSP studies is as a complement to solid form screening to see which alternative packings to the known polymorphs are thermodynamically feasible."}

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@ONLINE{empyrean,
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@techreport{advlabxrd,
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@misc{Xraybinary,
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@article{doi:10.1111/j.1365-2966.2005.08886.x,
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@book{Feldman1986,
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@book{Ziegler_1975, place={United States}, title={New uses of ion accelerators}, abstractNote={A review is given of new uses of ion accelerators and includes discussion of sample preparation, ion beam and energy selection, detector methods, and data collection and analysis. Topics include: (1) ion-excited x-ray analysis of environmental samples; (2) material analysis by nuclear backscattering; (3) material analysis by means of nuclear reactions; (4) lattice location of impurities in metals and semiconductors; (5) ion implantation in metals; (6) ion implantation in superconductors; (7) ion-induced x-rays from gas collisions; and (8) ion-induced x-rays in solids. A separate abstract was prepared for each chapter for ERDA Energy Research Abstracts (ERA). (PMA)}, publisher={Plenum Press,New York}, author={Ziegler, J.F.}, year={1975}, month={Jan}}


@book{tesmer1995handbook,
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@techreport{ADVLABACCEL,
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@book{Carroll&Ostlie,
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@book{Chuetal,
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@ONLINE{codatarecommended,
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@INPROCEEDINGS{2001sac..conf....3P,
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@INPROCEEDINGS{2016ASSL..439..249B,
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    pages = {249},
      doi = {10.1007/978-3-319-39739-9_13},
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  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@MISC{ngc5548photo,
  author       = {Davide de Martin}, 
  title        = {Supermassive black hole at the heart of NGC 5548},
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  note         = {CC BY}
}




@ARTICLE{2016ApJ...821...56F,
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