Abstract / Description of output
Photometric and spectroscopic monitoring of 50 blue, nuclear
"transients" in PanSTARRS-1 has revealed different types of extremely
variable AGN. The majority show a gradual brightening by ~2 mag from the
SDSS observation a decade ago and may represent a new class of AGN
microlensed by foreground galaxies. Spectra from the William Herschel
Telescope identify these as z~1 AGN with atypical spectroscopic
properties. We present an analysis of their photometric and
spectroscopic variability in an effort to constrain the detailed
structure of the source AGN.
Original language | English |
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Publication status | Published - 1 Jan 2015 |