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}

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@TECHREPORT{bradley2006,
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@ARTICLE{bradley_et_al2008,
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}

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@ARTICLE{deoliveira2008,
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}

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}

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}

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}

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}

@ARTICLE{lewis_challinor_2007,
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}

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 keywords = {cosmology: observations, dark ages, reionization, first stars,
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}


@ARTICLE{greenhill_bernardi2012,
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  journal = {ArXiv e-prints},
archivePrefix = "arXiv",
   eprint = {1201.1700},
 primaryClass = "astro-ph.CO",
 keywords = {Astrophysics - Cosmology and Extragalactic Astrophysics,
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     year = 2012,
    month = jan,
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@ARTICLE{burns_et_al2012,
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    {Loeb}, A. and {Pritchard}, J.},
    title = "{Probing the first stars and black holes in the early Universe with
the Dark Ages Radio Explorer (DARE)}",
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archivePrefix = "arXiv",
   eprint = {1106.5194},
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     year = 2012,
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   volume = 49,
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      doi = {10.1016/j.asr.2011.10.014},
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@ARTICLE{liu_et_al2009,
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 primaryClass = "astro-ph.CO",
 keywords = {methods: data analysis , techniques: interferometric , early
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}

@ARTICLE{pober_et_al2014,
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J.~E. and 
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    {DeBoer}, D.~R. and {Hewitt}, J.~N. and {Jacobs}, D.~C. and 
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    {Tegmark}, M. and {Werthimer}, D.~J.},
    title = "{What Next-generation 21 cm Power Spectrum Measurements can Teach
us About the Epoch of Reionization}",
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archivePrefix = "arXiv",
   eprint = {1310.7031},
 keywords = {dark ages, reionization, first stars, techniques: interferometric
},
     year = 2014,
    month = feb,
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}

@ARTICLE{george_et_al2014,
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    {Zahn}, O.},
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     year = 2014,
    month = aug,
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}


@ARTICLE{schenker_et_al2013,
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    title = "{The UV Luminosity Function of Star-forming Galaxies via Dropout
Selection at Redshifts z \~{} 7 and 8 from the 2012 Ultra Deep Field Campaign}",
  journal = {\apj},
archivePrefix = "arXiv",
   eprint = {1212.4819},
 primaryClass = "astro-ph.CO",
 keywords = {dark ages, reionization, first stars, galaxies: evolution,
galaxies: formation},
     year = 2013,
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}

@article{treu_et_al2013,
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    {Stiavelli}, M.},
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  journal = {\apjl},
archivePrefix = "arXiv",
   eprint = {1308.5985},
 primaryClass = "astro-ph.CO",
 keywords = {galaxies: evolution, galaxies: high-redshift },
     year = 2013,
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      doi = {10.1088/2041-8205/775/1/L29},
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}

@ARTICLE{faisst_et_al2014,
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     year = 2014,
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}

@ARTICLE{bolton_et_al2011,
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= 7.085 quasar ULAS J1120+0641?}",
  journal = {\mnras},
archivePrefix = "arXiv",
   eprint = {1106.6089},
 primaryClass = "astro-ph.CO",
 keywords = {dark ages, reionization, first stars, intergalactic medium,
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     year = 2011,
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      doi = {10.1111/j.1745-3933.2011.01100.x},
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@article{clark_et_al2013,
author = {Clark, M.A. and Plante, PC La and Greenhill, L.J.}, 
title = {Accelerating radio astronomy cross-correlation with graphics processing
units},
volume = {27}, 
number = {2}, 
pages = {178-192}, 
year = {2013}, 
doi = {10.1177/1094342012444794}, 
abstract ={We present a highly parallel implementation of the cross-correlation
of time-series data using graphics processing units (GPUs), which is scalable to
hundreds of independent inputs and suitable for the processing of signals from
‘large-
                  
               ’ arrays of many radio antennas. The computational part of the
algorithm, the X-engine, is implemented efficiently on NVIDIA’s Fermi
architecture, sustaining up to 79% of the peak single-precision floating-point
throughput. We compare performance obtained for hardware- and software-managed
caches, observing significantly better performance for the latter. The high
performance reported involves use of a multi-level data tiling strategy in
memory and use of a pipelined algorithm with simultaneous computation and
transfer of data from host to device memory. The speed of code development,
flexibility, and low cost of the GPU implementations compared with
application-specific integrated circuit (ASIC) and field programmable gate array
(FPGA) implementations have the potential to greatly shorten the cycle of
correlator development and deployment, for cases where some power-consumption
penalty can be tolerated.}, 
URL = {http://hpc.sagepub.com/content/27/2/178.abstract}, 
eprint = {http://hpc.sagepub.com/content/27/2/178.full.pdf+html}, 
journal = {International Journal of High Performance Computing Applications} 
}

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    {Williams}, A. and {Williams}, C.~L.},
    title = "{WSCLEAN: an implementation of a fast, generic wide-field imager for radio astronomy}",
  journal = {\mnras},
archivePrefix = "arXiv",
   eprint = {1407.1943},
 primaryClass = "astro-ph.IM",
 keywords = {instrumentation: interferometers, methods: observational, techniques: interferometric, radio continuum: general},
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      doi = {10.1093/mnras/stu1368},
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}

@ARTICLE{presley_et_al2015,
   author = {{Presley}, M. and {Liu}, A. and {Parsons}, A.},
    title = "{Measuring the Cosmological 21 cm Monopole with an Interferometer}",
  journal = {ArXiv e-prints},
archivePrefix = "arXiv",
   eprint = {1501.01633}, keywords = {Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Instrumen
tation and Methods for Astrophysics},
     year = 2015,
    month = jan,
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}


@ARTICLE{jacobs_et_al2014,
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    {Carilli}, C.~L. and {DeBoer}, D.~R. and {Dexter}, M.~R. and 
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    {Manley}, J.~R. and {Moore}, D.~F. and {Stefan}, I.~I. and {Walbrugh}, W.~P.
    },
    title = "{Multi-redshift limits on the 21cm power spectrum from PAPER}",
  journal = {ArXiv e-prints},
archivePrefix = "arXiv",
   eprint = {1408.3389},
 keywords = {Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics},
     year = 2014,
    month = aug,
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@ARTICLE{harker_et_al2009,
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  journal = {\mnras},
archivePrefix = "arXiv",
   eprint = {0903.2760},
 primaryClass = "astro-ph.CO",
 keywords = {methods: statistical , cosmology: theory , diffuse radiation , radio lines: general},
     year = 2009,
    month = aug,
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      doi = {10.1111/j.1365-2966.2009.15081.x},
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