67,846 research outputs found
DeepVoting: A Robust and Explainable Deep Network for Semantic Part Detection under Partial Occlusion
In this paper, we study the task of detecting semantic parts of an object,
e.g., a wheel of a car, under partial occlusion. We propose that all models
should be trained without seeing occlusions while being able to transfer the
learned knowledge to deal with occlusions. This setting alleviates the
difficulty in collecting an exponentially large dataset to cover occlusion
patterns and is more essential. In this scenario, the proposal-based deep
networks, like RCNN-series, often produce unsatisfactory results, because both
the proposal extraction and classification stages may be confused by the
irrelevant occluders. To address this, [25] proposed a voting mechanism that
combines multiple local visual cues to detect semantic parts. The semantic
parts can still be detected even though some visual cues are missing due to
occlusions. However, this method is manually-designed, thus is hard to be
optimized in an end-to-end manner.
In this paper, we present DeepVoting, which incorporates the robustness shown
by [25] into a deep network, so that the whole pipeline can be jointly
optimized. Specifically, it adds two layers after the intermediate features of
a deep network, e.g., the pool-4 layer of VGGNet. The first layer extracts the
evidence of local visual cues, and the second layer performs a voting mechanism
by utilizing the spatial relationship between visual cues and semantic parts.
We also propose an improved version DeepVoting+ by learning visual cues from
context outside objects. In experiments, DeepVoting achieves significantly
better performance than several baseline methods, including Faster-RCNN, for
semantic part detection under occlusion. In addition, DeepVoting enjoys
explainability as the detection results can be diagnosed via looking up the
voting cues
The molecular spiral arms of NGC 6946
From CO-12(J=1 to 0) observations at 45 seconds resolution Tacconi and Young (1989) have found evidence for enhancements in both the CO emissivity and the massive star formation efficiency (MSFE) on optical spiral arms of the bright spiral galaxy NGC 6946. In the optically luminous and well-defined spiral arm in the NE quadrant, there are enhancements in both the H2 surface density and MSFE relative to the interarm regions. In contrast, a poorly defined arm in the SW shows no arm-interarm contrast in the MSFE. To further investigate the molecular gas content of these two spiral arms, researchers have made CO-12 J=2 to 1 and 3 to 2 observations with the James Clerk Maxwell Telescope. In the J=2 to 1 line, they made observations of the NE and SW spiral arm and interarm regions in 4 x 9 10 seconds spaced grids (36 points per grid). Because of decreased sensitivity in the J=3 to 2 line, they were limited to mapping the two arm regions in 2 x 3 10 seconds spaced grids (6 points per grid). The centers of each of the grids lie 2.4 minutes to the NE and 2.3 minutes to the SW of the nucleus of NGC 6946. With the CO J=2 to 1 data researchers are able to fully resolve the two observed spiral arms in NGC 6946. In both cases the CO emission is largely confined to the optical spiral arm regions with the peak observed T asterisk sub A being up to 4 times higher on the spiral arms than in the interarm regions. Researchers are currently estimating massive star formation efficiencies on and off the spiral arms through direct comparison of the CO maps with an H alpha image. They are also comparing the CO J=2 to 1 data with an HI map made at similar resolution. Thus, they will be able to determine structure in all components of the IS on scales of less than 20 inches
Dynamic microscopic structures and dielectric response in the cubic-to-tetragonal phase transition for BaTiO3 studied by first-principles molecular dynamics simulation
The dynamic structures of the cubic and tetragonal phase in BaTiO3 and its
dielectric response above the cubic-to-tetragonal phase transition temperature
(Tp) are studied by first-principles molecular dynamics (MD) simulation. It's
shown that the phase transition is due to the condensation of one of the
transverse correlations. Calculation of the phonon properties for both the
cubic and tetragonal phase shows a saturation of the soft mode frequency near
60 cm-1 near Tp and advocates its order-disorder nature. Our first-principles
calculation leads directly to a two modes feature of the dielectric function
above Tp [Phys. Rev. B 28, 6097 (1983)], which well explains the long time
controversies between experiments and theories
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