作者: J. Aird , A. L. Coil , A. Georgakakis
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摘要: We provide measurements of the probability distribution function specific black hole accretion rates within a sample galaxies given stellar mass and redshift, \(p(\log \lambda_{sBHAR} | M_*,z)\). Measurements are provided for all galaxies, star-forming quiescent galaxies. We also provide estimates AGN duty cycle, \(f(\lambda_{sBHAR} >0.01)\) i.e. fraction with an above limit in accretion rate, based on functions. Full details provided Aird et al. (2017b, MNRAS, press, arXiv:1705.01132); please cite this publication if you use these measurements.