deletions | additions       diff --git a/bibliography/biblio.bib b/bibliography/biblio.bib  index 4749b6a..8d1a053 100644  --- a/bibliography/biblio.bib  +++ b/bibliography/biblio.bib 
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BibTeX export options can be customized via Options -> BibTeX in Mendeley Desktop  @online{h5py, @misc{JonesOliphantPeterson2001,  annote = {http://www.scipy.org/},  author = {{Andrew Collette}}, {Jones, Eric and Oliphant, Travis and Peterson, Pearu},  keywords = {scientific{\_}computing},  title = {{HDF5 {{SciPy: Open source scientific tools  for Python}}, url = {http://www.h5py.org},  year = {2008} {http://www.scipy.org}  }  @article{Oesch2010b,  abstract = {We present a first morphological study of z {\~{}} 7-8 Lyman break galaxies (LBGs) from Oesch et al. and Bouwens et al. detected in ultra-deep near-infrared imaging of the Hubble Ultra-Deep Field (HUDF) by the HUDF09 program. With an average intrinsic size of 0.7 ± 0.3 kpc, these galaxies are found to be extremely compact, having an average observed surface brightness of $\mu$ J {\#}{\#}IMG{\#}{\#} [http://ej.iop.org/icons/Entities/sime.gif] {\{}sime{\}} 26 mag arcsec –2 , and only two out of the full sample of 16 z {\~{}} 7 galaxies show extended features with resolved double cores. By comparison to lower redshift LBGs, it is found that only little size evolution takes place from z {\~{}} 7 to z {\~{}} 6, while galaxies between z {\~{}} 4-5 show more extended wings in their apparent profiles. The average size scales as (1 + z ) – m with m = 1.12 ± 0.17 for galaxies with luminosities in the range (0.3-1) L * z =3 and with m = 1.32 ± 0.52 for (0.12-0.3) L * z =3 , consistent with galaxies having constant comoving sizes. The peak of the size distribution changes only slowly from z {\~{}} 7 to z {\~{}} 4. However, a tail of larger galaxies ( {\#}{\#}IMG{\#}{\#} [http://ej.iop.org/icons/Entities/gsim.gif] {\{}gsim{\}} 1.2 kpc) is gradually built up toward later cosmic times, possibly via hierarchical build-up or via enhanced accretion of cold gas. Additionally, the average star formation surface density of LBGs with luminosities (0.3-1) L * z =3 is nearly constant at $\Sigma$ SFR = 1.9 M {\#}{\#}IMG{\#}{\#} [http://ej.iop.org/icons/Entities/sun.gif] {\{}sun{\}} yr –1 kpc –2 over the entire redshift range z {\~{}} 4-7 suggesting similar star formation efficiencies at these early epochs. The above evolutionary trends seem to hold out to z {\~{}} 8 though the sample is still small and possibly incomplete.}, 
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title = {{Hierarchical data format version 5}},  url = {http://www.hdfgroup.org/HDF5}  }  @online{h5py,  author = {Collette, Andrew},  title = {{HDF5 for Python}},  url = {http://www.h5py.org},  year = {2008}  }