Spinning test-body orbiting around Schwarzschild black hole: circular dynamics and gravitational-wave fluxes

We release gravitational wave fluxes at null-infinity from a spinning test-body in circular equatorial orbits around a Schwarzschild black hole. Four different prescriptions are used for the dynamics:  the Mathisson-Papapetrou formalism under the Tulczyjew (TUL) spin-supplementary-condition (SSC), the Pirani (PIR) SSC and the Ohashi-Kyrian-Semerak (OKS) SSC, and the spinning particle limit of the effective-one-body Hamiltonian (HAM) of [Phys.~Rev.~D.90,~044018(2014)]. For more details see xxxx .

The multipolar fluxes are given for l=2,3 m=1,2,3 at the Boyer-Lindquist radii

  r =  4 5 6 7 8 10 12 15 20 30   ,

in cases they were not computed the data contains a "42". Note that the fluxes in these data files are assumed to contain both the +m and -m contributions, since they are identical for equatorial orbits and aligned spins. 
Additionally, the data files contain the key numbers describing the circular dynamics (see paper).

Units c=G=1.