Jc. Lee et al., AN RXTE OBSERVATION OF MCG-6-30-15 - CONSTRAINTS ON THE IRON ABUNDANCE AND REFLECTIVE FRACTION RELATIONSHIP, Nuclear physics. B, Proceedings supplement, 69(1-3), 1999, pp. 486-489
We report on a 50 ks observation of the bright Seyfert 1 galaxy MCG-6-
30-15 with the Rossi X-ray Timing Explorer. The data clearly show the
broad fluorescent iron line (equivalent width similar to 242 eV for th
e scenario in which the primary X-ray source is above the accretion di
sk subtending an angle of 2 pi sr), and the Compton reflection continu
um at higher energies. Upper limit constraints on the abundance versus
reflective fraction relationship can already be placed at the 68 per
cent confidence level.