  We present ~800 days of photometric monitoring of Boyajian's Star (KIC
8462852) from the All-Sky Automated Survey for Supernovae (ASAS-SN) and ~4000
days of monitoring from the All Sky Automated Survey (ASAS). We show that from
2015 to the present the brightness of Boyajian's Star has steadily decreased at
a rate of 6.3 +/- 1.4 mmag yr^-1, such that the star is now 1.5% fainter than
it was in February 2015. Moreover, the longer time baseline afforded by ASAS
suggests that Boyajian's Star has also undergone two brightening episodes in
the past 11 years, rather than only exhibiting a monotonic decline. We analyze
a sample of ~1000 comparison stars of similar brightness located in the same
ASAS-SN field and demonstrate that the recent fading is significant at >99.4%
confidence. The 2015-2017 dimming rate is consistent with that measured with
Kepler data for the time period from 2009 to 2013. This long-term variability
is difficult to explain with any of the physical models for the star's behavior
proposed to date.
