Probing the time variability of five Fe low broad absorption line
  quasars
  We study the time variability of five Fe Low ionization Broad Absorption Line
(FeLoBAL) QSOs using repeated spectroscopic observations with the 2m telescope
at IUCAA Girawali observatory (IGO) spanning an interval of upto 10 years. We
report a dramatic variation in Al III and Fe III fine-structure lines in the
spectra of SDSS J221511.93-004549.9 (z_em ~ 1.478). However, there is no such
strong variability shown by the C IV absorption. This source is known to be
unusual with (i) the continuum emission dominated by Fe emission lines, (ii) Fe
III absorption being stronger than Fe II and (iii) the apparent ratio of Fe III
UV 48 to Fe III UV 34 absorption suggesting an inverted population ratio. This
is the first reported detection of time variability in the Fe III
fine-structure lines in QSO spectra. There is a strong reduction in the
absorption strength of these lines between year 2000 and 2008. Using the
template fitting techniques, we show that the apparent inversion of strength of
UV lines could be related to the complex spectral energy distribution of this
QSO. The observed variability can be related to change in the ionization state
of the gas or due to transverse motion of this absorbing gas. The shortest
variability timescale of Al III line gives a lower limit on the electron
density of the absorbing gas as n_e >= 1.1 x 10^4 cm^-3. The remaining 4
FeLoBALs do not show any changes beyond the measurement uncertainties either in
optical depth or in the velocity structure. We present the long-term
photometric light curve for all of our sources. Among them only SDSS
J221511.93-004549.9 shows significant (>= 0.2 mag) variability.
