tokens: We thank all the python , numpy and scipy communities for the high-quality free software they made available. MS thanks Philipp Edelmann for all the technical support during the developing of this work. EEOI acknowledges financial support from Brazilian agencies FAPESP (2011/09525-3) and CAPES (9229-13-2). Supported by German DFG Cluster of Excellence ‘Origin and Structure of the Universe’ and the DFG Transregio Project 33 ‘Dark Universe’. We thank Dan Birchall for observing assistance, the technical and scientific staffs of the Palomar Observatory, the High Performance Wireless Radio Network (HPWREN) and the University of Hawaii 2.2-m telescope. We recognize the significant cultural role of Mauna Kea within the indigenous Hawaiian community, and we appreciate the opportunity to conduct observations from this revered site. This work was supported by the Director, Office of Science, Office of High Energy Physics, of the US Department of Energy under Contract No. DE-AC02-05CH11231; by a grant from the Gordon Betty Moore Foundation; in France by support from CNRS/IN2P3, CNRS/INSU, PNCG and the Lyon Institute of Origins under grant ANR-10-LABX-66; and in Germany by the DFG through TRR33 ‘The Dark Universe’. Some results were obtained using resources and support from the National Energy Research Scientific Computing Center, supported by the Director, Office of Science, Office of Advanced Scientific Computing Research, of the US Department of Energy under Contract No. DE-AC02-05CH11231. HPWREN is funded by National Science Foundation Grant Number ANI-0087344, and the University of California, San Diego. This work was written using the collaborative ShareLaTeX platform.
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