Observation and model parameters for cycles #1 (2002–2003, left) and #2 (2004–2005, right). From top to bottom: X-ray flux and power-law fraction in the 3 − 200 keV range, power-law index, 9 GHz radio flux, transition radius r_J, and inner accretion rate ṁ_in (at ISCO). For the first 4 panels, i.e., the constraints, black squares are observations. Each figure uses the same color-code: green upper- (lower-) triangles for the rising (decaying) hard, blue circles for hard-intermediate, yellow crosses for soft-intermediate, and red crosses for soft-states. Additionally, in the state-associated colors we draw the 5% and 10% confidence intervals (i.e., 5% and 10% bigger ζ_X + R, see Paper IV). Double arrows are drawn when radio emission was also observed but has been interpreted as radio flares or interactions with the interstellar medium (Corbel et al., in prep.).