Erratum: “Multiwavelength Monitoring of the Dwarf Seyfert 1 Galaxy NGC 4395. I. A Reverberation‐based Measurement of the Black Hole Mass” (ApJ, 632, 799 [2005])

Abstract

A reverberation-mapping program on NGC 4395, the least luminous known Seyfert 1 galaxy, undertaken with the Space Telescope Imaging Spectrograph on the Hubble Space Telescope yields a measurement of the mass of the central black hole M BH ¼ (3:6 AE 1:1) ; 10 5 M. The observations consist of two visits of five orbits each, in 2004 April and July. During each of these visits, the UV continuum varied by at least 10% (rms), and only C iv k1549 showed corresponding variations large enough to reliably determine the emission-line lag, which was measured to be of order 1 hr for both visits. The size of the C iv-emitting region is about a factor of 3 smaller than expected if the slope of the broad-line region radius-luminosity relationship is identical to that for the H emission line. NGC 4395 is under-luminous even for its small black hole mass; the Eddington ratio of $1:2 ; 10 À3 is lower than that of any other active galactic nucleus for which a black hole mass measurement has been made by emission-line reverberation.