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Photometric reverberation mapping of Markarian 279

By using standard broad-band VRI photometry we were able to discriminate the variations of the broad hydrogen alpha line from the continuum variations for the active galaxy Mkn 279. Cross-correlating both light curves enabled us to determine the time lag of the broad line variations behind the continuum and thus to determine the BLR size (about 8 light days). Our preliminary results are rather consistent with the spectroscopic reverberation mapping results (about 12/17 days). This study is a part of an ambitious program to perform photometric reverberation mapping and determine BLR sizes (respectively - the central black hole masses) for more that 100 nearby AGN.

preprint2014arXivOpen access
R. BachevA. StrigachevE. SemkovS. BoevaS. PenevaS. IbryamovK. StoyanovB. SpassovS. TsvetkovaB. MihovG. LatevD. Dimitrov
astro-ph.COastro-ph.GA
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Open access12 authors2 topics
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R. BachevA. StrigachevE. SemkovS. BoevaS. PenevaS. IbryamovK. StoyanovB. SpassovS. TsvetkovaB. MihovG. LatevD. Dimitrov

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