Gerard Auger

TL;DR: The eLISA mission as discussed by the authors is the first mission to study the entire universe with gravitational waves, and it will offer a wide view of a dynamic cosmos using gravitational waves as new and unique messengers to unveil The Gravitational Universe.

TL;DR: Yield ratios for light particles and fragments with atomic number Z < or = 5 obey the exponential law of isotopic scaling, and deduced scaling parameters decrease strongly with increasing centrality to values smaller than 50% of those obtained for the peripheral event groups.

TL;DR: In this paper, a correlation technique for the relative velocity between light charged particles (LCP) and fragments was used to extract the multiplicities and average kinetic energy of secondary evaporated LCP.

TL;DR: Many user-defined parameters allow the code to study different configurations of LISA thus helping to finalize the definition of the detector, and another important use of LISACode is in generating time-series for data analysis developments.

TL;DR: The Mock LISA data challenges as discussed by the authors have been released in rounds of increasing complexity and realism: here we present the results of Challenge 2, issued in Jan 2007, which successfully demonstrated the recovery of signals from nonspinning supermassive-black-hole binaries with optimal SNRs between ~10 and 2000, from ~20 000 overlapping galactic white-dwarf binaries (among a realistically distributed population of 26 million), and from the extreme-mass-ratio inspirals of compact objects into central galactic black holes.