Efficient Depth Map Upsampling Method Using Standard Deviation

2015 ◽  
pp. 33-40
Author(s):  
Su-Min Hong ◽  
Yo-Sung Ho
Keyword(s):  
Standard Deviation ◽  
Depth Map ◽  
Depth Map Upsampling

A High Quality Depth Map Upsampling Method Robust to Misalignment of Depth and Color Boundaries

2013 ◽  
Vol 75 (1) ◽  
pp. 23-37 ◽  
Author(s):  
Jaekwang Kim ◽  
Jaeho Lee ◽  
Seung-Ryong Han ◽  
Dowan Kim ◽  
Jongsul Min ◽  
...  
Keyword(s):  
Depth Map ◽  
High Quality ◽  
Depth Map Upsampling

Objective Evaluation of Image Decomposition Algorithms for Depth Map Upsampling

2019 ◽  
Vol 14 (6) ◽  
pp. 2619-2624 ◽  
Author(s):  
Chanho Jung ◽  
Seungkwon Shin ◽  
Jiwon Lee ◽  
Wonjun Kim
Keyword(s):  
Depth Map ◽  
Image Decomposition ◽  
Objective Evaluation ◽  
Decomposition Algorithms ◽  
Depth Map Upsampling

Depth map upsampling using compressive sensing based model

2015 ◽  
Vol 154 ◽  
pp. 325-336 ◽  
Author(s):  
Longquan Dai ◽  
Haoxing Wang ◽  
Xiaopeng Zhang
Keyword(s):  
Compressive Sensing ◽  
Depth Map ◽  
Depth Map Upsampling

Challenges in searching for hydrocarbons in CRISM-IR data

2020 ◽  
Author(s):  
Paola Manzari ◽  
Cosimo Marzo ◽  
Eleonora Ammannito
Keyword(s):  
Standard Deviation ◽  
Spatial Resolution ◽  
Methane Concentration ◽  
High Spatial Resolution ◽  
Depth Map ◽  
Mars Atmosphere ◽  
High Concentrations ◽  
Band Depth

<p>After having observed  some absorptions around 3.3 μm band in some CRISM spectra, we begun a study in the range between 3.2 and 3.4 μm to exploit the high spatial resolution of CRISM spectrometer (~18 m/pixel) to look for methane or other C-H absorptions on Mars surface. Concerning methane, we were searching for high concentrations, comparable to the “methane spikes” concentrations detected by Curiosity on Mars surface and the methane plumes detected in Mars atmosphere from ground telescopes. The search for absorptions around 3.3 μm was carried out fitting the spectra of selected CRISM datasets with the MGM function in the 3.2-3.4 μm range.  From the MGM fit we obtained a map of the absorption depths. By this depth map, aside rare, suspected, absorptions, a spectral artifact was highlighted.  Therefore, we chose to consider spectra with absorptions around 3.3 μm not clearly related to known and unknown artifacts, and band depth values greater than 4*standard deviation of the depth map. We used the Planetary Spectrum Generator tool to find the relation between the absorption depths at 3.3 μm and methane concentration. We finally discuss the rare interesting spectra both as potentially true absorptions and as a still unknown artifact.</p>

Joint-adaptive bilateral depth map upsampling

2014 ◽  
Vol 29 (4) ◽  
pp. 506-513 ◽  
Author(s):  
Joohyeok Kim ◽  
Gwanggil Jeon ◽  
Jechang Jeong
Keyword(s):  
Depth Map ◽  
Depth Map Upsampling

Precise depth map upsampling and enhancement based on edge‐preserving fusion filters

2018 ◽  
Vol 12 (5) ◽  
pp. 651-658
Author(s):  
Ting‐An Chang ◽  
Jar‐Ferr Yang
Keyword(s):  
Depth Map ◽  
Edge Preserving ◽  
Depth Map Upsampling

Depth map upsampling using depth local features

2014 ◽  
Vol 50 (3) ◽  
pp. 170-171 ◽  
Author(s):  
Y.S. Kang ◽  
S.B. Lee ◽  
Y.S. Ho
Keyword(s):  
Depth Map ◽  
Local Features ◽  
Depth Map Upsampling

scholarly journals Integrated cosparse analysis model with explicit edge inconsistency measurement for guided depth map upsampling

2018 ◽  
Vol 27 (04) ◽  
pp. 1
Author(s):  
Yifan Zuo ◽  
Qiang Wu ◽  
Ping An ◽  
Xiwu Shang
Keyword(s):  
Depth Map ◽  
Analysis Model ◽  
Depth Map Upsampling
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