tokens: We thank Chris Pritchet and Dennis Zaritsky for help carrying out the MENeaCS spectroscopic survey, Patrick Kelly for making his python SLR code publicly available, and Radek Wojtak for suggesting an assessment of orientation bias. C.S., H.H., and M.V. acknowledge support from the European Research Council under FP7 grant number 279396. H.H., M.C. and R.F.J.vdB. acknowledge support from the Netherlands Organisation for Scientific Research grant number 639.042.814. Based on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/IRFU, at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institut National des Science de l’Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii. Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the U.S. Department of Energy Office of Science. The SDSS-III web site is http:// [0]www. [0]sdss3. [0]org/. This research has made use of the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. This publication makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation. This research has made use of NASA’s Astrophysics Data System Bibliographic Services. This work has made use of the python packages scipy (http:// [0]www. [0]scipy. [0]org) and matplotlib (http:// [0]matplotlib. [0]org; Hunter 2007 ) and of IPython ( Pérez Granger 2007 ).
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