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671 results for “Window”
Correlated k coefficients for H2-He atmospheres; 180 spectral windows and 1460 pressure-temperature points
<p>There are 108 correlated k-coefficients datasets, using the naming convention sonora_2020_fehxxxx_co_yyy.data.196.tar.gz (78 models) or sonora_2020_fehxxxx_co_yyy_noTiOVO.data.196.tar.gz (78 models), where xxxx is the metallicity in 10x dex relative to solar, and yyy is the 100x C/O ratio relative to solar, as a multiplication factor. For example a metallicity of +000 and a C/O ratio of 100 indicates solar abundances, feh+070 should be read as a metallicity of +0.7 dex, feh-100 as -1.0 dex, co_025 should be read as 0.25x C/O relative to solar, and co_200 as 2x C/O relative to solar. We use the Lodders et al. 2010 value for the solar C/O=0.458. The files with “noTiOVO” in the filename contain the correlated k-coefficients calculated without the opacity of TiO and VO. The rest of the molecular abundances and opacities are the same as the equilibrium chemistry values in the regular files. These files are useful for calculating models without any TiO- and VO-induced temperature inversion in the atmosphere.</p> <p>The correlated-k coefficients are calculated using pre-mixed opacities, with abundances given by equilibrium chemistry for each metallicity-C/O combination, as described in Marley et al. 2021. There are 13 Fe/H values: 0.0, 0.3, 0.5, 0.7, 1.0, 1.3, 1.5, 1.7, 2.0, -0.3, -0.5, -0.7, and -1.0; and 6 C/O values: 0.25, 0.5, 1.0, 1.5, 2.0 and 2.5. The k-coefficients are calculated for a grid of 1460 pressure-temperature points, from10^−6 to 3000 bar and from 75 to 4000 K, listed in the file 1460_layer_list, and can be read in using the IDL script read_k_coefficients.pro. The spectral windows are listed in the file 180_windows.txt (intervals defined as starting at lambda1 and ending at lambda2). NB Please note that for metallicities between 1.3 and 2.0 the value of <em>max_windows</em> has changed from 200 to 1000.</p> <p>The opacity sources included in the calculations are: C2H2, C2H4, C2H6, CH4, CO, CO2, CrH, Fe, FeH, H2, H3+, H2O, H2S, HCN, LiCl, LiF, LiH, MgH, N2, NH3, OCS, PH3, SiO, TiO, and VO, in addition to alkali metals (Li, Na, K, Rb, Cs). The corresponding high resolution opacities for these atoms and molecules can be found in the Zenodo repository 10.5281/zenodo.6600976. The references for the line lists used in these opacity calculations are listed in the file Opacity_references_2021.pdf. Please include these references, as well as the reference to this Zenodo repository when publishing your paper.</p> <p>Each dataset contains the following files:</p> <p>ascii_data: the correlated k coefficients file in ascii format. This can be read by the included IDL code.</p> <p>binary_data: the correlated k coefficients file in binary format</p> <p>full_abunds: the relative abundances for all the species from the chemistry files, on the 1460-point pressure-temperature grid</p> <p>sum_in_atoms: relative abundances for the alkali metals</p> <p>sum_in_layer: relative abundances for all molecules included in the correlated k-coefficients calculations</p> <p><em>Resources supporting this work were provided by the NASA High-End Computing (HEC) Program through the NASA Advanced Supercomputing (NAS) Division at Ames Research Center.</em></p>
Correlated k coefficients for H2-He atmospheres; 11 spectral windows and 1460 pressure-temperature points
<p>There are 108 correlated k-coefficients datasets, using the naming convention sonora_2020_fehxxxx_co_yyy.data.196.tar.gz (78 models) or sonora_2020_fehxxxx_co_yyy_noTiOVO.data.196.tar.gz (78 models), where xxxx is the metallicity in 10x dex relative to solar, and yyy is the 100x C/O ratio relative to solar, as a multiplication factor. For example a metallicity of +000 and a C/O ratio of 100 indicates solar abundances, feh+070 should be read as a metallicity of +0.7 dex, feh-100 as -1.0 dex, co_025 should be read as 0.25x C/O relative to solar, and co_200 as 2x C/O relative to solar. We use the Lodders et al. 2010 value for the solar C/O=0.458. The files with “noTiOVO” in the filename contain the correlated k-coefficients calculated without the opacity of TiO and VO. The rest of the molecular abundances and opacities are the same as the equilibrium chemistry values in the regular files. These files are useful for calculating models without any TiO- and VO-induced temperature inversion in the atmosphere.</p> <p>The correlated-k coefficients are calculated using pre-mixed opacities, with abundances given by equilibrium chemistry for each metallicity-C/O combination, as described in Marley et al. 2021. There are 13 Fe/H values: 0.0, 0.3, 0.5, 0.7, 1.0, 1.3, 1.5, 1.7, 2.0, -0.3, -0.5, -0.7, and -1.0; and 6 C/O values: 0.25, 0.5, 1.0, 1.5, 2.0 and 2.5. The k-coefficients are calculated for a grid of 1460 pressure-temperature points, from10^−6 to 3000 bar and from 75 to 4000 K, listed in the file 1460_layer_list, and can be read in using the IDL script read_k_coefficients.pro. The spectral windows are listed in the file 11_windows.txt (intervals defined as starting at lambda1 and ending at lambda2). NB Please note that for metallicities between 1.3 and 2.0 the value of <em>max_windows</em> has changed from 200 to 1000.</p> <p>The opacity sources included in the calculations are: C2H2, C2H4, C2H6, CH4, CO, CO2, CrH, Fe, FeH, H2, H3+, H2O, H2S, HCN, LiCl, LiF, LiH, MgH, N2, NH3, OCS, PH3, SiO, TiO, and VO, in addition to alkali metals (Li, Na, K, Rb, Cs). The corresponding high resolution opacities for these atoms and molecules can be found in the Zenodo repository 10.5281/zenodo.6600976. The references for the line lists used in these opacity calculations are listed in the file Opacity_references_2021.pdf. Please include these references, as well as the reference to this Zenodo repository when publishing your paper.</p> <p>Each dataset contains the following files:</p> <p>ascii_data: the correlated k coefficients file in ascii format. This can be read by the included IDL code.</p> <p>binary_data: the correlated k coefficients file in binary format</p> <p>full_abunds: the relative abundances for all the species from the chemistry files, on the 1460-point pressure-temperature grid</p> <p>sum_in_atoms: relative abundances for the alkali metals</p> <p>sum_in_layer: relative abundances for all molecules included in the correlated k-coefficients calculations</p> <p><em>Resources supporting this work were provided by the NASA High-End Computing (HEC) Program through the NASA Advanced Supercomputing (NAS) Division at Ames Research Center.</em></p>
Correlated k coefficients for H2-He atmospheres; 30 spectral windows and 1460 pressure-temperature points
<p>There are 108 correlated k-coefficients datasets, using the naming convention sonora_2020_fehxxxx_co_yyy.data.196.tar.gz (78 models) or sonora_2020_fehxxxx_co_yyy_noTiOVO.data.196.tar.gz (78 models), where xxxx is the metallicity in 10x dex relative to solar, and yyy is the 100x C/O ratio relative to solar, as a multiplication factor. For example a metallicity of +000 and a C/O ratio of 100 indicates solar abundances, feh+070 should be read as a metallicity of +0.7 dex, feh-100 as -1.0 dex, co_025 should be read as 0.25x C/O relative to solar, and co_200 as 2x C/O relative to solar. We use the Lodders et al. 2010 value for the solar C/O=0.458. The files with “noTiOVO” in the filename contain the correlated k-coefficients calculated without the opacity of TiO and VO. The rest of the molecular abundances and opacities are the same as the equilibrium chemistry values in the regular files. These files are useful for calculating models without any TiO- and VO-induced temperature inversion in the atmosphere.</p> <p>The correlated-k coefficients are calculated using pre-mixed opacities, with abundances given by equilibrium chemistry for each metallicity-C/O combination, as described in Marley et al. 2021. There are 13 Fe/H values: 0.0, 0.3, 0.5, 0.7, 1.0, 1.3, 1.5, 1.7, 2.0, -0.3, -0.5, -0.7, and -1.0; and 6 C/O values: 0.25, 0.5, 1.0, 1.5, 2.0 and 2.5. The k-coefficients are calculated for a grid of 1460 pressure-temperature points, from10^−6 to 3000 bar and from 75 to 4000 K, listed in the file 1460_layer_list, and can be read in using the IDL script read_k_coefficients.pro. The spectral windows are listed in the file 30_windows.txt (intervals defined as starting at lambda1 and ending at lambda2). NB Please note that for metallicities between 1.3 and 2.0 the value of <em>max_windows</em> has changed from 200 to 1000.</p> <p>The opacity sources included in the calculations are: C2H2, C2H4, C2H6, CH4, CO, CO2, CrH, Fe, FeH, H2, H3+, H2O, H2S, HCN, LiCl, LiF, LiH, MgH, N2, NH3, OCS, PH3, SiO, TiO, and VO, in addition to alkali metals (Li, Na, K, Rb, Cs). The corresponding high resolution opacities for these atoms and molecules can be found in the Zenodo repository 10.5281/zenodo.6600976. The references for the line lists used in these opacity calculations are listed in the file Opacity_references_2021.pdf. Please include these references, as well as the reference to this Zenodo repository when publishing your paper.</p> <p>Each dataset contains the following files:</p> <p>ascii_data: the correlated k coefficients file in ascii format. This can be read by the included IDL code.</p> <p>binary_data: the correlated k coefficients file in binary format</p> <p>full_abunds: the relative abundances for all the species from the chemistry files, on the 1460-point pressure-temperature grid</p> <p>sum_in_atoms: relative abundances for the alkali metals</p> <p>sum_in_layer: relative abundances for all molecules included in the correlated k-coefficients calculations</p> <p><em>Resources supporting this work were provided by the NASA High-End Computing (HEC) Program through the NASA Advanced Supercomputing (NAS) Division at Ames Research Center.</em></p>
Symplectic lattice gauge theories on Grid: approaching the conformal window---data release
<p>This is the data release relative to the paper "Symplectic lattice gauge theories on Grid: approaching the conformal window" (arXiv:2306.11649).</p> <p>It contains pre-analysed data that can be plotted, and raw data that can be analysed and plotted through the analysis code in doi:10.5281/zenodo.8136514.</p>
Dataset for: Windows of opportunity for predicting seasonal climate extremes: Pakistan floods of 2022
<p>Data required to regenerate any of the figures in Nature Communications paper "Windows of opportunity for predicting seasonal climate extremes: Pakistan floods of 2022"</p>
Church window
I made this church window with photobashing technique, i hope you like it :) Source: Objaverse 1.0 / Sketchfab
Rose Window - Valencia Cathedral, Spain
Rose Window Valencia Cathedral, Spain Gothic style (14th century) The rose window illuminates one of the transepts of the church and still keeps remains of the old stained glass. It was called "the salomo" because of its elaborate structure and for holding the "Star of King David". Thus, Jesus was acclaimed as the Messiah and "David's Son", born in the "Mystic rose" Mary. We know nothing about the master builder of this entrance, former door of the mosque, since the artists worked only for God's glory. In 1354, it was completely finished, a fact that is derived from the coat of arms adorning the entrance (13th and 14th century) Source: Objaverse 1.0 / Sketchfab
Merlin- Window-17
Merlin or Doughiske Castle has a series of exquisitely decorated medieval windows. The carvings depict foliage and knotwork, with one windows showing a figure hanging from a round arched window. This has been identified as Ireland's smallest Sheela-na-Gig. The carvings largely function as decoration and may have been designed by the masons who carved them with little input from the castle owner. They may form a protective function on the building Source: Objaverse 1.0 / Sketchfab
WPMP window type 4
Realized within the project of the sourced-based reconstruction of the New Synagogue in Wroclaw/Breslau (Poland). Link to the 3D model documentation: http://www.vfu-oppler.hs-mainz.de/en/wisski/navigate/607/view. Supported by »The German Federal Government Commissioner for Culture and the Media « (02/2018-11/2019) and »The Foundation for Polish-German Cooperation« (05/2018). Magnified by https://architekturinstitut.hs-mainz.de/. Published under CC-BY-NC-SA 4.0. Source: Objaverse 1.0 / Sketchfab
Clonenagh - Window
A window fragment with was found beside the cross-slabs at Clonenagh.  Source: Objaverse 1.0 / Sketchfab
Carrick-on- Suir - Window Ormond
Window from Ormond Castle - This project is funded through the Irish Walled Towns Network programme in conjunction with Tipperary County Council' Source: Objaverse 1.0 / Sketchfab
Merlin- Window-9
Merlin or Doughiske Castle has a series of exquisitely decorated medieval windows. The carvings depict foliage and knotwork, with one windows showing a figure hanging from a round arched window. This has been identified as Ireland's smallest Sheela-na-Gig. The carvings largely function as decoration and may have been designed by the masons who carved them with little input from the castle owner. They may form a protective function on the building Source: Objaverse 1.0 / Sketchfab
Gothic Window in Brick Wall (1) Chrismas Gift
Gotické okno sakristie Sv. Ducha v Hradci Králové mapa: https://mapy.cz/s/nosesohusa Source: Objaverse 1.0 / Sketchfab
Loughrea - Window Decoration
This carving is located above a late medeival window on St. Marys Abbey in Loughread. The windows is the exterior wall on what would have been the closter side of the abbey. The carving shows a male figure holding a smaller figure in his arms. Both appear to have crowns, althouhg the large figure could show a headdress. The smaller figure appears to be christ. Source: Objaverse 1.0 / Sketchfab
NPAP window type 2
Realized within the project of the sourced-based reconstruction of the New Synagogue in Wroclaw/Breslau (Poland). Link to the 3D model documentation: http://www.vfu-oppler.hs-mainz.de/en/wisski/navigate/5061/view. Supported by »The German Federal Government Commissioner for Culture and the Media « (02/2018-11/2019) and »The Foundation for Polish-German Cooperation« (05/2018). Magnified by https://architekturinstitut.hs-mainz.de/. Published under CC-BY-NC-SA 4.0. Source: Objaverse 1.0 / Sketchfab
Ballynaclogh Church Window (TN027-003002-)
15th /16th century single-light ogee-headed unglazed limestone window with sunken spandrels and hood-moulding above located in southern wall of the nave of the medieval nave and chancel parish church ruins at Ballynaclogh, Co. Tipperary also known as Weyperous, in the diocese of Killaloe, Barony of Ormond Upper. The church which was entered through a chamfered pointed limestone doorway stands in the eastern quadrant of a rectangular-shaped graveyard (TN027-003006-), immediately southeast of a 19th century Protestant church built in 1802 with a gift of £500 from the Board of First Fruits. For more information on the church ruins, visit: https://maps.archaeology.ie/HistoricEnvironment/?SMRS=TN027-003002- Source: Objaverse 1.0 / Sketchfab
Azure Window - 3D scan before the collapse, 2016
The Azure Window was a limestone natural arch in Gozo, Malta. It collapsed on March 8th, 2017, during a strong storm.  This model was made from 102 still frames from [this video](https://www.youtube.com/watch?v=Rv_rLS_4bkc) by [The Maltese Drone](https://www.youtube.com/channel/UCDE3rpUz6ij-vanNW02by5g) About the Azure Window: https://en.wikipedia.org/wiki/Azure_Window Source: Objaverse 1.0 / Sketchfab
Rose Window of San Sabino Bari Cathedral, Italy
It was 3d designed with Tinkercad codeblocks and 3d printed, by the students of 3rd Junior High School of Kifissia, Athens, Greece. Bari Cathedral, or Cathedral of Saint Sabinus, is the cathedral of Bari, in Apulia, southern Italy. The cathedral is the seat of the Archbishop of Bari-Bitonto, as it was previously of the archbishops, earlier bishops, of Bari. It is dedicated to Saint Sabinus, a bishop of Canosa. The present building was constructed between the late 12th and late 13th centuries, mostly in the last thirty years of the 12th century, and was built on the site of the ruins of the Imperial Byzantine cathedral destroyed in 1156 by William I of Sicily known as the Wicked. Stylistically, this is an important example of Apulian Romanesque. The simple façade has three portals of the 11th century below a rose window, over which is a lintel carved with monsters and fantastic beasts. https://en.wikipedia.org/wiki/Bari_Cathedral Source: Objaverse 1.0 / Sketchfab
Top of Door and windows
Photo realistic Top of Door and windows. 100K triangles Reality Capture. Higher reslolution textures could be possible along with higher density triangle mesh. Some errors are present. If needed for large project, I can complete data capture, for a fee :-) Source: Objaverse 1.0 / Sketchfab
Window Study of Nivolumab With or Without Ipilimumab in Squamous Cell Carcinoma of the Oral Cavity
ClinicalTrials.gov study NCT02919683. IPD Sharing: NO. Countries: 1. Publications: 2.
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DANDI Archive for NWB datasets
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International Brain Laboratory public data
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OpenNeuro
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