The clustering of galaxies in the SDSS-III Baryon Oscillation
  Spectroscopic Survey: BAO measurement from the LOS-dependent power spectrum
  of DR12 BOSS galaxies
  [abridged] We present an anisotropic analysis of the baryonic acoustic
oscillation (BAO) scale in the twelfth and final data release of the Baryonic
Oscillation Spectroscopic Survey (BOSS). We independently analyse the LOWZ and
CMASS galaxy samples: the LOWZ sample contains contains 361 762 galaxies with
an effective redshift of $z_{\rm LOWZ}=0.32$; the CMASS sample consists of 777
202 galaxies with an effective redshift of $z_{\rm CMASS}=0.57$. We extract the
BAO peak position from the monopole power spectrum moment, $\alpha_0$, and from
the $\mu^2$ moment, $\alpha_2$, where $\mu$ is the cosine of the angle to the
line-of-sight. The $\mu^2$-moment provides equivalent information to that
available in the quadrupole but is simpler to analyse. After applying a
reconstruction algorithm to reduce the BAO suppression by bulk motions, we
measure the BAO peak position in the monopole and $\mu^2$-moment, which are
related to radial and angular shifts in scale. We report $H(z_{\rm
LOWZ})r_s(z_d)=(11.60\pm0.60)\cdot10^3 {\rm km}s^{-1}$ and $D_A(z_{\rm
LOWZ})/r_s(z_d)=6.66\pm0.16$ with a cross-correlation coefficient of
$r_{HD_A}=0.41$, for the LOWZ sample; and $H(z_{\rm
CMASS})r_s(z_d)=(14.56\pm0.37)\cdot10^3 {\rm km}s^{-1}$ and $D_A(z_{\rm
CMASS})/r_s(z_d)=9.42\pm0.13$ with a cross-correlation coefficient of
$r_{HD_A}=0.47$, for the CMASS sample. We combine these results with the
measurements of the BAO peak position in the monopole and quadrupole
correlation function of the same dataset \citep[][companion
paper]{Cuestaetal2015} and report the consensus values: $H(z_{\rm
LOWZ})r_s(z_d)=(11.63\pm0.69)\cdot10^3 {\rm km}s^{-1}$ and $D_A(z_{\rm
LOWZ})/r_s(z_d)=6.67\pm0.15$ with $r_{HD_A}=0.35$ for the LOWZ sample;
$H(z_{\rm CMASS})r_s(z_d)=(14.67\pm0.42)\cdot10^3 {\rm km}s^{-1}$ and
$D_A(z_{\rm CMASS})/r_s(z_d)=9.47\pm0.12$ with $r_{HD_A}=0.52$ for the CMASS
sample.
