Dan Gifford edited bibliography/biblio.bib  about 10 years ago

Commit id: 8d63287921c8579c518531fb5f149f000df0ba28

deletions | additions      

       

@ARTICLE{Gifford13a,   author = {Gifford, D. and Miller, C. and Kern, N.},   title = {{A Systematic Analysis of Caustic Methods for Galaxy Cluster Masses}},   journal = {\apj},   archiveprefix = {arXiv},   eprint = {1307.0017},   primaryclass = {astro-ph.CO},   keywords = {galaxies: clusters: general galaxies: halos},   year = {2013},   month = {aug},   volume = {773},   eid = {116},   pages = {116},   doi = {10.1088/0004-637X/773/2/116},   adsurl = {http://adsabs.harvard.edu/abs/2013ApJ...773..116G},   adsnote = {Provided by the SAO/NASA Astrophysics Data System},   }       @article{Evrard09,   title = {{Virial Scaling of Massive Dark Matter Halos: Why Clusters Prefer a High Normalization Cosmology}},   volume = {672},   url = {http://dx.doi.org/10.1086/521616},   doi = {10.1086/521616},   number = {1},   journal = {The Astrophysical Journal},   publisher = {IOP Publishing},   author = {Evrard, A. E. and Bialek, J. and Busha, M. and White, M. and Habib, S. and Heitmann, K. and Warren, M. and Rasia, E. and Tormen, G. and Moscardini, L. and et al.},   year = {2008},   month = {Jan},   pages = {122-137},   }     @ARTICLE{Evrard08,  author = {{Evrard}, A.~E. and {Bialek}, J. and {Busha}, M. and {White}, M. and   {Habib}, S. and {Heitmann}, K. and {Warren}, M. and {Rasia}, E. and  

adsnote = {Provided by the SAO/NASA Astrophysics Data System}  }  @ARTICLE{Gifford13a,   author = {{Gifford}, D. and {Miller}, C. and {Kern}, N.},   title = "{A Systematic Analysis of Caustic Methods for Galaxy Cluster Masses}",   journal = {\apj},   archivePrefix = "arXiv",   eprint = {1307.0017},   primaryClass = "astro-ph.CO",   keywords = {galaxies: clusters: general, galaxies: halos },   year = 2013,   month = aug,   volume = 773,   eid = {116},   pages = {116},   doi = {10.1088/0004-637X/773/2/116},   adsurl = {http://adsabs.harvard.edu/abs/2013ApJ...773..116G},   adsnote = {Provided by the SAO/NASA Astrophysics Data System}   }