American Astronomical Society, Astrophysical Journal, 1(653), p. 152-158, 2006
DOI: 10.1086/508533
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We present new observations leading to an improved black hole mass estimate for the Seyfert 1 galaxy NGC 4593 as part of a reverberation-mapping campaign conducted at the MDM Observatory. Cross-correlation analysis of the H_beta emission-line light curve with the optical continuum light curve reveals an emission-line time delay of 3.73 (+-0.75) days. By combining this time delay with the H_beta line width, we derive a central black hole mass of M_BH = 9.8(+-2.1)x10^6 M_sun, an improvement in precision of a factor of several over past results. ; Comment: 22 pages, 3 tables, 5 figures, accepted for publication in ApJ