@Article{NovaesBernFerrWuen:2014:SePrNo,
author = "Novaes, Camila Paiva and Bernu{\'{\i}}, Armando and Ferreira,
Ivan Soares and Wuensche, Carlos Alexandre",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and
{Observat{\'o}rio Nacional} and {Universidade de
Bras{\'{\i}}lia} and {Instituto Nacional de Pesquisas Espaciais
(INPE)}",
title = "Searching for primordial non-Gaussianity in Planck CMB maps using
a combined estimator",
journal = "Journal of Cosmology and Astroparticle Physics",
year = "2014",
volume = "2014",
number = "1",
pages = "18",
keywords = "primordial non-Gaussianity, Planck CMB maps, cosmic microwave
background radiation.",
abstract = "he extensive search for deviations from Gaussianity in cosmic
microwave background radiation (CMB) data is very important due to
the information about the very early moments of the universe
encoded there. Recent analyses from Planck CMB data do not exclude
the presence of non-Gaussianity of small amplitude, although they
are consistent with the Gaussian hypothesis. The use of different
techniques is essential to provide information about types and
amplitudes of non-Gaussianities in the CMB data. In particular, we
find interesting to construct an estimator based upon the
combination of two powerful statistical tools that appears to be
sensitive enough to detect tiny deviations from Gaussianity in CMB
maps. This estimator combines the Minkowski functionals with a
Neural Network, maximizing a tool widely used to study
non-Gaussian signals with a reinforcement of another tool designed
to identify patterns in a data set. We test our estimator by
analyzing simulated CMB maps contaminated with different amounts
of local primordial non-Gaussianity quantified by the
dimensionless parameter f NL. We apply it to these sets of CMB
maps and find < 98% of chance of positive detection, even for
small intensity local non-Gaussianity like f NL = 38±18, the
current limit from Planck data for large angular scales.
Additionally, we test the suitability to distinguish between
primary and secondary non-Gaussianities: first we train the Neural
Network with two sets, one of nearly Gaussian CMB maps (|f NL| 10)
but contaminated with realistic inhomogeneous Planck noise (i.e.,
secondary non-Gaussianity) and the other of non-Gaussian CMB maps,
that is, maps endowed with weak primordial non-Gaussianity (28 f
NL 48); after that we test an ensemble composed of CMB maps either
with one of these non-Gaussian contaminations, and find out that
our method successfully classifies < 95% of the tested maps as
being CMB maps containing primordial or secondary non-Gaussianity.
Furthermore, we analyze the foreground-cleaned Planck maps
obtaining constraints for non-Gaussianity at large-angles that are
in good agreement with recent constraints. Finally, we also test
the robustness of our estimator including cut-sky masks and
realistic noise maps measured by Planck, obtaining successful
results as well.",
doi = "10.1088/1475-7516/2014/01/018",
url = "http://dx.doi.org/10.1088/1475-7516/2014/01/018",
issn = "1475-7516",
label = "self-archiving-INPE-MCTI-GOV-BR",
language = "en",
targetfile = "MF+NN_jcap.pdf",
urlaccessdate = "27 abr. 2024"
}