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71 results for “opacity”

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zenodo32/100

Experimental data for paper "strategFTO: Untimed control for timed opacity"

<p>This data set contains all experimental data for paper &quot;strategFTO: Untimed control for timed opacity&quot;.</p>

opencc-by-4.0Oct 2022View details →
zenodo32/100

Data for paper "Parametric Timed Model Checking for Guaranteeing Timed Opacity"

<p>Our zip contains all necessary scripts, models, binaries and instructions to reproduce the experiments of our paper<br> <em>Parametric Timed Model Checking for Guaranteeing Timed Opacity</em> published in the proceedings of ATVA 2019.</p> <p>It allows interested readers to reproduce exactly the content of <strong>Table 1</strong> and <strong>Table 2</strong> of our paper.<br> In addition, all result files are generated, containing the synthesized constraints, and the execution times of IMITATOR.</p>

opencc-by-4.0Jun 2019View details →
zenodo32/100

Supplementary tables for "Inconsistencies and opacity in retraction notices: Snapshot using 50 cases from Elsevier journals"

Open the record for dataset details and reuse information.

opencc-by-4.0Sep 2024View details →
zenodo32/100

Face detection dataset perturbed using Gimp's foggify filterwith turbulence=4.0 and opacity 100.

<p>This dataset is a perturbed version of the dataset&nbsp;https://zenodo.org/record/3879989#.Y-HBCXbMI2w</p> <p>Please refer to&nbsp;https://zenodo.org/record/3879989#.Y-HBCXbMI2w&nbsp; for eye coordinates and depth maps.&nbsp;</p>

opencc-by-4.0Feb 2023View details →
ClinicalTrials.gov32/100

Comparison Between Wedge Resection and Segmentectomy for Ground Glass Opacity- Dominant Stage IA NSCLC

ClinicalTrials.gov study NCT02718365. IPD Sharing: NO. Countries: 1. Publications: 5.

closedIPD-NOFeb 2026View details →
ClinicalTrials.gov32/100

A Clinical Study to Evaluate the KeraKlear Keratoprosthesis in Patients With Corneal Opacity

ClinicalTrials.gov study NCT03126903. IPD Sharing: NO. Countries: 1. Publications: 1.

closedIPD-NOFeb 2026View details →
ClinicalTrials.gov32/100

Occupational Cataracts and Lens Opacities in Interventional Cardiology : the O'CLOC Study

ClinicalTrials.gov study NCT01061463. IPD Sharing: Not stated. Countries: 1. Publications: 1.

restrictedIPD-UNDECIDEDFeb 2026View details →
ClinicalTrials.gov32/100

Wedge Resection for Ground-glass Opacity-featured Lung Cancer (ECTOP-1020)

ClinicalTrials.gov study NCT06102161. IPD Sharing: NO. Countries: 1. Publications: 1.

closedIPD-NOFeb 2026View details →
ClinicalTrials.gov32/100

Effectiveness of Infiltration With Resin in Treatment of MIH Incisors in Children Showing Opacities

ClinicalTrials.gov study NCT05597956. IPD Sharing: NO. Countries: 1. Publications: 1.

closedIPD-NOFeb 2026View details →
ClinicalTrials.gov32/100

The Effect of Ranibizumab on Eye Lens Opacity in Cases With Age-Related Macular Degeneration

ClinicalTrials.gov study NCT01330797. IPD Sharing: Not stated. Countries: 1. Publications: 5.

restrictedIPD-UNDECIDEDFeb 2026View details →
ClinicalTrials.gov32/100

Lipiodol Localization for Ground-glass-opacity Minimal Surgery

ClinicalTrials.gov study NCT02180568. IPD Sharing: Not stated. Countries: 1. Publications: 1.

restrictedIPD-UNDECIDEDFeb 2026View details →
ClinicalTrials.gov32/100

Phototherapeutic Keratectomy (PTK) With Mitomycin in Adenoviral Opacities

ClinicalTrials.gov study NCT00492245. IPD Sharing: Not stated. Countries: 1. Publications: 4.

restrictedIPD-UNDECIDEDFeb 2026View details →
ClinicalTrials.gov32/100

Ultrahigh-frequency Ultrasonography (UHFUS) in Detection of Small Pulmonary Ground Glass Opacity (GGO)

ClinicalTrials.gov study NCT05994898. IPD Sharing: YES. Countries: 1. Publications: 9.

controlledIPD-YESFeb 2026View details →
ClinicalTrials.gov32/100

Systematic Sampling of Lymph Nodes vs. Lymphadenectomy According to Intraoperative Frozen Pathology for Pulmonary Invasive Adenocarcinoma With Ground-glass Opacity

ClinicalTrials.gov study NCT03322826. IPD Sharing: NO. Countries: 1. Publications: 2.

closedIPD-NOFeb 2026View details →
zenodo28/100

Geometry and Opacity Data for Fractal Aggregates

<p>In a previous version of this archive, geometry data and tables of opacity calculations were given that could be used to calculate the radiative pressure and absorption on fractal dust grains under Asymptotic Giant Branch (AGB) conditions (with a peak stellar wavelength of ~ 1 micron) for aggregates containing up to 256 primary particles. &nbsp;Because the focus of that work was on radiative pressure from a stellar spectrum peaking at approximately 1 micron, these data only covered the wavelength range from 0.3 to 30 microns. &nbsp;In this updated archive the wavelength range of the data has been expanded to allow calculation of the emission of the grains at longer wavelengths. &nbsp;Data are calculated for three common dust materials: &nbsp;forsterite, (Mg2SiO4), olivine, (Mg_(2x)Fe_(2(1-x))SiO4) with x=0.5, and 'astronomical silicate' (B.T. Draine and H.M. Lee, Optical Properties of Interstellar Graphite and Silicate Grains, Astrophysical Journal, 1984). &nbsp;In this updated version the range of aggregate sizes (number of primary particles in the aggregate) of some of these materials has also been increased from a maximum of 256 to 1024 constituent particles.<br>&nbsp;<br>Example fractal aggregates were generated using the Diffusion Limited Aggregation (DLA) code as described in Wozniak M., Onofri F.R.A., Barbosa S., Yon J., Mroczka J., Comparison of methods to derive morphological parameters of multi-fractal samples of particle aggregates from TEM images, Journal of Aerosol Science 47: 12&ndash;26 (2012) and Onofri F.R.A., M. Wozniak, S. Barbosa, On the Optical Characterization of Nanoparticle and their Aggregates in Plasma Systems, Contributions to Plasma Physics 51(2-3):228-236 (2011). &nbsp;Aggregates were generated with a constant prefactor, kf=1.3, and two fractal dimensions (Df), representing open, porous (Df=1.8) aggregates and more compact (Df=2.8) aggregates.<br>&nbsp;<br>The geometry files were produced with the DLA software. &nbsp;An example run using this software is shown for aggregates with 256 primary particles and a fractal dimension of 2.8 in the file 'dla_example.png'<br>&nbsp;<br>For the fractal dimension=1.8 data, the number of primary particles in the aggregate, N, was increased up to 1024 from the previous maximum of 256 for all three dust materials investigated. &nbsp;In addition, the data for MgFeSiO4 with a fractal dimension of 2.8 was increased from 256 to 1024. &nbsp;As in the previous archive, 12 instances of each aggregate size were generated with primary particles having a radius of 0.5. &nbsp;These geometry data are given in:<br>aggregates_kf1.3_df1.8.zip &nbsp;--&gt; &nbsp;Geometry for a prefactor of 1.3 and fractal dimension 1.8<br>aggregates_kf1.3_df2.8.zip &nbsp;--&gt; &nbsp;Geometry for a prefactor of 1.3 and fractal dimension 2.8<br>&nbsp;<br>An example file name for an aggregate is 'N_00000032_Agg_00000008.dat' &nbsp;where the first number is the number of primary particles in the aggregate (N=32) and the second number is the instance number (e.g. 8 of 12).&nbsp; The radius of each primary particle in an aggregate is 0.5.&nbsp; The geometry files have 4 columns:&nbsp; the x, y and z coordinates of each primary particle followed by the primary particle radius.&nbsp; In each zip file there is also a pdf document that describes the geometry data and shows an image of each geometry file.</p> <p>&nbsp;<br>These geometry data were then used to calculate the opacity of the aggregates using the Multiple Sphere T-Matrix code (MSTM v 3.0) developed by Daniel Mackowski (D.W. Mackowski, M.I. Mishchenko, &nbsp;A multiple sphere T-matrix Fortran code for use on parallel computer clusters, Journal of Quantitative Spectroscopy and Radiative Transfer, Volume 112, Issue 13, 2011). &nbsp;Data were generated using the first 10 instances of each aggregate size, and the geometry data were appropriately scaled to calculate the opacity data for primary particle radii ranging from &nbsp;0.001 - 1.0 microns.&nbsp; As noted earlier, an earlier version of this archive was focused on radiative pressure on these aggregates and only covered the spectrum of a typical AGB star (0.3 to 30 microns wavelength).&nbsp; In this updated version this wavelength range has been increased to the longer wavelength limits of the optical data.&nbsp; By default, MSTM calculations are made along the z-axis of the geometry data. &nbsp;Additional calculations were made along the x and y axes for each aggregate. &nbsp; Therefore the final data set is the average of 30 values (10 instances each in the x,y,z directions).<br>&nbsp;<br>The opacity data files are given in:</p> <p>astronomical_silicate_df1.8.zip --&gt; astronomical silicate aggregates with fractal dimension 1.8<br>astronomical_silicate_df2.8.zip --&gt; astronomical silicate aggregates with fractal dimension 2.8<br>forsterite_df1.8.zip --&gt; forsterite aggregates with fractal dimension 1.8<br>forsterite_df2.8.zip --&gt; forsterite aggregates with fractal dimension 2.8<br>olivine_df1.8.zip --&gt; olivine aggregates with fractal dimension 1.8<br>olivine_df2.8.zip --&gt; olivine aggregates with fractal dimension 2.8</p> <p>In the previous version of this archive, only the table files with the averages of the 10 instances were provided. &nbsp;In this updated version each of the individual opacity files used to create these tables is now also provided. &nbsp;These opacity files are numbered similar to the geometry files. &nbsp;For example, the opacity calculations for N=32, instance=5, angle=3 is given by&nbsp;<br>'opacity_results_N000032_I05_A03_file.dat.' &nbsp;Each file begins with a short header describing the data. &nbsp;For example, the astronomical silicate header for this N=32, instance=5, angle=3 file is:</p> <p>#############################################################################################<br># Number of primary particles in aggregate: &nbsp; &nbsp; &nbsp; &nbsp;32&nbsp;<br># Geometry Instance Number: &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;5&nbsp;<br># Geometry File Name: &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;N_00000032_Agg_00000005.dat&nbsp;<br># Rotation Angles: &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;90.000 &nbsp; &nbsp;90.000 &nbsp; &nbsp; 0.000&nbsp;<br># Number of radius values: &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;30&nbsp;<br># Minimum and maximum radius values in microns: &nbsp; &nbsp; &nbsp; &nbsp;1.00000e-003 &nbsp;1.00000e+000&nbsp;<br># Number of wavelength values: &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;92&nbsp;<br># Minimum and maximum wavelength values in microns: &nbsp; &nbsp;3.00000e-001 &nbsp;1.00000e+004&nbsp;<br>#############################################################################################</p> <p>Afterwards the columns list the line number, the primary particle radius (microns), the wavelength (microns), the extinction efficiency factor, the absorption efficiency factor, the scattering absorption efficiency factor, &nbsp;the asymmetry factor and the radiation pressure efficiency factor. &nbsp;These efficiency factors are based on the effective radius of the aggregate described later in this document.</p> <p>Within each of these zipped folders is a file that contains the averages of these individual opacity files. &nbsp;For example 'astronomical_silicate_df1.8.dat' is the averaged data for the astronomical silicate aggregates with a fractal dimension 1.8. &nbsp;As in the previous archive, the first lines of these table files are a header starting with the '#' character describing the table and the source of the optical data used.<br>&nbsp;<br>After the header, the first line of data in the table has the following nine values giving the range for the data table and number of samples in N, (aggregate size), primary particle radius (microns) and wavelength (microns). &nbsp;These are:<br>&nbsp; Minimum aggregate size<br>&nbsp; Maximum aggregate size<br>&nbsp; Number of Aggregate samples<br>&nbsp; Primary Particle Minimum Radius (microns)<br>&nbsp; Primary Particle Maximum Radius (microns)<br>&nbsp; Number of Primary Particle radii samples<br>&nbsp; Wavelength minimum (microns)<br>&nbsp; Wavelength maximum (microns)<br>&nbsp; Number of Wavelength samples&nbsp;<br>&nbsp;<br>Subsequent lines contain 13 columns. &nbsp;These columns give the efficiency factors and asymmetry factor for aggregates. &nbsp;These efficiency factors are based on the effective radius of the aggregate given by:<br>&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;a_eff = a_primary*N^(1/3)<br>where a_primary is the primary particle radius and N is the number of primary particles in the aggregate.<br>&nbsp;<br>For example, the absorption opacity of an aggregate would then be = pi*a_eff^2 * Q_abs.<br>The values in each column are:<br>&nbsp; Column 1: &nbsp; Primary particle radius in microns<br>&nbsp; Column 2: &nbsp; Wavelength in microns<br>&nbsp; Column 3: &nbsp; Number of primary particles in aggregate<br>&nbsp; Column 4: &nbsp; Mean Q_ext, mean extinction efficiency factor<br>&nbsp; Column 5: &nbsp; Standard Deviation of Mean Q_ext&nbsp;<br>&nbsp; Column 6: &nbsp; Mean Q_abs, mean absorption efficiency factor<br>&nbsp; Column 7: &nbsp; Standard Deviation of Mean Q_abs<br>&nbsp; Column 8: &nbsp; Mean Q_sca, mean scattering efficiency factor<br>&nbsp; Column 9: &nbsp; Standard Deviation of mean Q_sca<br>&nbsp; Column 10: &nbsp;Mean g_cos, mean asymmetry factor<br>&nbsp; Column 11: &nbsp;Standard Deviation of mean asymmetry factor<br>&nbsp; Column 12: &nbsp;Mean Q_pr, mean radiation pressure efficiency factor<br>&nbsp; Column 13: &nbsp;Standard Deviation of mean&nbsp;</p>

opencc-by-4.0Sep 2024View details →
geo24/100

Asparagine alleviates naphthalene-induced lens opacity in SRA cells

GEO Series GSE290337. Homo sapiens. 12 samples. Type: Expression profiling by high throughput sequencing.

openGEO-OpenApr 2025View details →
geo24/100

The activity and safety of sintilimab on high-risk ground glass opacity lesions in multiple primary lung cancer patients

GEO Series GSE260770. Homo sapiens. 50 samples. Type: Expression profiling by high throughput sequencing.

openGEO-OpenMay 2024View details →
geo24/100

Single-cell RNA sequencing unravel distinct tumor microenvironment of different components of lung adenocarcinoma featured as mixed ground glass opacity

GEO Series GSE203360. Homo sapiens. 6 samples. Type: Expression profiling by high throughput sequencing.

openGEO-OpenMay 2022View details →
geo24/100

Copy Number of an Integron-Encoded Antibiotic Resistance Locus Regulates a Virulence and Opacity Switch in Acinetobacter baumannii AB5075

GEO Series GSE156206. Acinetobacter baumannii. 6 samples. Type: Expression profiling by high throughput sequencing.

openGEO-OpenAug 2020View details →
ClinicalTrials.gov24/100

A Randomized Study of Intraocular Caliper-assisted Capsulotomy for Age-related Cataract Patients With Corneal Limbus Opacity

ClinicalTrials.gov study NCT04977102. IPD Sharing: Not stated. Countries: 1. Publications: 0.

restrictedIPD-UNDECIDEDFeb 2026View details →

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