Emission-Line and Continuum Reverberation Mapping of the NLS1 Galaxy WPVS 48
arXiv:2511.09153 · doi:10.1051/0004-6361/202554969
Abstract
WPVS 48 is a nearby narrow-line Seyfert 1 galaxy without previous analysis of the broad-line region (BLR) by means of optical spectroscopic reverberation mapping. By studying the continuum and emission line variability of WPVS 48, we aim to infer the BLR size as well as the mass of the central supermassive black hole (SMBH). We analyse data from a dedicated optical spectroscopic reverberation mapping campaign of WPVS 48 taken with the 10 m Southern African Large Telescope (SALT) at 24 epochs over a period of 7 months between December 2013 and June 2014. WPVS 48 shows variability throughout the campaign. We find a stratified BLR, where the variability amplitude of the integrated emission lines decreases with distance to the ionizing continuum source. Specifically, the variable emission of H, H, H, He I originates at distances of , , and light-days, respectively, to the optical continuum at 5100 A. The He II lag is days. Based on the high S/N spectra, we identify variable emission of N III and C IV in the line complex with He II . We derive interband continuum delays increasing with wavelength up to days. These delays are consistent with an additional diffuse continuum originating at the same distance as the variable Balmer emission. We derive a central black hole mass of based on the integrated line-widths and distances of the BLR and discuss corrections for the inclination angle. This gives an Eddington ratio without correction for inclination.
arXiv comment22 pages, 17 figures
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