128 research outputs found
Review of Person Re-identification Techniques
Person re-identification across different surveillance cameras with disjoint
fields of view has become one of the most interesting and challenging subjects
in the area of intelligent video surveillance. Although several methods have
been developed and proposed, certain limitations and unresolved issues remain.
In all of the existing re-identification approaches, feature vectors are
extracted from segmented still images or video frames. Different similarity or
dissimilarity measures have been applied to these vectors. Some methods have
used simple constant metrics, whereas others have utilised models to obtain
optimised metrics. Some have created models based on local colour or texture
information, and others have built models based on the gait of people. In
general, the main objective of all these approaches is to achieve a
higher-accuracy rate and lowercomputational costs. This study summarises
several developments in recent literature and discusses the various available
methods used in person re-identification. Specifically, their advantages and
disadvantages are mentioned and compared.Comment: Published 201
Adubos verdes e seus efeitos no rendimento da cana-de-açĂșcar em sistema de plantio direto.
O objetivo deste trabalho foi avaliar adubos verdes e seus efeitos no rendimento da cana-de-açĂșcar em sistema de plantio direto (SPD). O trabalho foi realizado em Campos dos Goytacazes (RJ), no perĂodo de dezembro de 2003 a julho de 2005. O delineamento experimental foi em blocos casualizados, com quatro repetiçÔes. Os tratamentos foram: feijĂŁo-de-porco (Canavalia ensiformis), mucuna-preta(Mucuna aterrimum), crotalĂĄria (CrotalĂĄria juncea) em plantio direto e vegetação espontĂąnea em preparo convencional (testemunha). Com crotalĂĄria aos 35 dias apĂłs emergĂȘncia (DAE) houve maior taxa de cobertura do solo â 87% â e, aos 92 DAE produziu 17.852 kg ha-1 de matĂ©ria seca, respectivamente, 41%, 78% e 407% superior ao feijĂŁo-de-porco, mucuna e vegetação espontĂąnea, alĂ©m de superĂĄ-las em acĂșmulos de K, Mg, S, Zn e Fe. O feijĂŁo-de-porco e a mucuna proporcionaram o maior teor de N na parte aĂ©rea. Com feijĂŁo-de-porco, os teores de P e Ca foram maiores que a crotalĂĄria e a mucuna. Com vegetação espontĂąnea, o maior teor de K foi na parte aĂ©rea. As leguminosas acumularam maiores quantidades de N e Cu do que a vegetação espontĂąnea. A crotalĂĄria e o feijĂŁo-de-porco acumularam 66% a mais de P na parte ĂĄrea que a mucuna. O SPD utilizando a adubação verde contribuiu significativamente para a maior produtividade de cana-de-açĂșcar, 135.863 kg ha-1, sendo 37% superior ao PC com a vegetação espontĂąnea
Update on the correlation of the highest energy cosmic rays with nearby extragalactic matter
Data collected by the Pierre Auger Observatory through 31 August 2007 showed
evidence for anisotropy in the arrival directions of cosmic rays above the
Greisen-Zatsepin-Kuz'min energy threshold, \nobreak{eV}. The
anisotropy was measured by the fraction of arrival directions that are less
than from the position of an active galactic nucleus within 75 Mpc
(using the V\'eron-Cetty and V\'eron catalog). An updated
measurement of this fraction is reported here using the arrival directions of
cosmic rays recorded above the same energy threshold through 31 December 2009.
The number of arrival directions has increased from 27 to 69, allowing a more
precise measurement. The correlating fraction is , compared
with expected for isotropic cosmic rays. This is down from the early
estimate of . The enlarged set of arrival directions is
examined also in relation to other populations of nearby extragalactic objects:
galaxies in the 2 Microns All Sky Survey and active galactic nuclei detected in
hard X-rays by the Swift Burst Alert Telescope. A celestial region around the
position of the radiogalaxy Cen A has the largest excess of arrival directions
relative to isotropic expectations. The 2-point autocorrelation function is
shown for the enlarged set of arrival directions and compared to the isotropic
expectation.Comment: Accepted for publication in Astroparticle Physics on 31 August 201
Atmospheric effects on extensive air showers observed with the Surface Detector of the Pierre Auger Observatory
Atmospheric parameters, such as pressure (P), temperature (T) and density,
affect the development of extensive air showers initiated by energetic cosmic
rays. We have studied the impact of atmospheric variations on extensive air
showers by means of the surface detector of the Pierre Auger Observatory. The
rate of events shows a ~10% seasonal modulation and ~2% diurnal one. We find
that the observed behaviour is explained by a model including the effects
associated with the variations of pressure and density. The former affects the
longitudinal development of air showers while the latter influences the Moliere
radius and hence the lateral distribution of the shower particles. The model is
validated with full simulations of extensive air showers using atmospheric
profiles measured at the site of the Pierre Auger Observatory.Comment: 24 pages, 9 figures, accepted for publication in Astroparticle
Physic
Search for First Harmonic Modulation in the Right Ascension Distribution of Cosmic Rays Detected at the Pierre Auger Observatory
We present the results of searches for dipolar-type anisotropies in different
energy ranges above eV with the surface detector array of
the Pierre Auger Observatory, reporting on both the phase and the amplitude
measurements of the first harmonic modulation in the right-ascension
distribution. Upper limits on the amplitudes are obtained, which provide the
most stringent bounds at present, being below 2% at 99% for EeV
energies. We also compare our results to those of previous experiments as well
as with some theoretical expectations.Comment: 28 pages, 11 figure
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