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125 results for “Plato”
Figure 17 from: Prete PH, Cizauskas I, Brescovit AD (2018) Three new species of the spider genus Plato and the new genus Cuacuba from caves of the states of Pará and Minas Gerais, Brazil (Araneae, Theridiosomatidae). ZooKeys 753: 107-162. https://doi.org/10.3897/zookeys.753.20805
Figure 17 Distribution maps of Cuacuba mariana sp. n. (circle) and C. morrodopilar sp. n. (star) in state of Minas Gerais, Brazil.
Figure 1 from: Prete PH, Cizauskas I, Brescovit AD (2018) Three new species of the spider genus Plato and the new genus Cuacuba from caves of the states of Pará and Minas Gerais, Brazil (Araneae, Theridiosomatidae). ZooKeys 753: 107-162. https://doi.org/10.3897/zookeys.753.20805
Figure 1 Plato ferriferus sp. n. A male, dorsal view B female, dorsal view C male palp, ventral view D male palp, ventral view (SEM) E–F male palp, ventral view, expanded and with conductor removed G embolus, illustration. Abbreviations: C conductor; CY cymbium; E embolus; EA mesal embolic apophysis; MA median apophysis; O embolic opening; ST subtegulum; T tegulum. Scale bars: A 1.1; B 1; C–F 0.3; G 0.15 mm.
PLATO-ESR3-01-official-documents
<table> <tbody> <tr> <td> <p><strong>The politicisation and depoliticisation of EU policies such as state aid are key to the legitimation and contestation of the EU. However, the existing literature tends to focus on analysing these processes either in terms of politicisation or depoliticisation, but rarely both simultaneously. Rather, this thesis conceptualises politicisation and depoliticisation as embodying a fluid-like state within Multilevel Governance (MLG) structures, such as the EU, where agents play a key role. The thesis first explores 266 state aid cases labelled “Unlawful with Recovery of Aid” (UWRA) to identify which were appealed, and to gauge the degree of news coverage that each case gained. From the analysis of the 266 cases, the dissertation selects the cases of Apple in Ireland and Ilva in Italy for sustained and detailed analysis. It explores how actors have sought to politicise and depoliticise these state aid cases in the national news media. A claims-making analysis is performed to understand how actors attempt to legitimise or delegitimise their own actions or the actions of the other actors involved (the Commission, Apple, Ilva and the Irish and Italian governments). To perform the analysis, a set of 100 newspapers were gathered from the Factiva database, including two leading quality newspapers (centre-left and centre-right) from Ireland (<em>the Irish Times</em> and <em>the</em> <em>Irish Independent</em>) and Italy (<em>Il Sole 24 Ore</em> and <em>La Repubblica</em>). The results show that a key moment in the trajectory of both the politicisation and depoliticisation of a state aid case is the act of appealing by the member state. More specifically, in the Apple case, TINA (There Is No Alternative) was used as a strategy to discursively depoliticise the action of appealing which, interestingly contributed to the overall politicisation of the state aid case. In contrast, other depoliticising strategies (“appeasing” claims) which intended to calm past tensions between the Italian government and the Commission were used successfully. In terms of politicisation, the Apple case showed an “international conflict trajectory” (Irish government versus the Commission) while the Ilva case raised concerns about the Italian government and the management of the corporation. Overall, this dissertation advances understandings of the differentiated patterns of politicisation and depoliticisation by illustrating that the Apple case followed the “politics against policy” route while this was avoided in the Ilva state aid case.</strong></p> </td> </tr> </tbody> </table> <div> </div>
Plato 1024. Cerro de los Vientos
Plato cocción reductora realizado en un torno lento de la necrópolis del Cerro de los Vientos (Baeza, Jaén, España). Tiene un diámetro de 18 cm y no presenta ningún tipo de decoración. Forma parte de los materiales documentados en la estructura 28, que pudo haber tenido una función ritual de comensalidad asociada al ámbito funerario. En su interior se identificaron indicadores químicos de cera de abeja, lo que podría relacionarlo con el consumo de miel o hidromiel. Cronología: VIII-VII a.C. Modelo realizado por "esTRESd" Source: Objaverse 1.0 / Sketchfab
CE 1421 - PLATO
N° de Registro Nacional: 0000303424 DATOS DE IDENTIFICACIÓN BIEN CULTURAL: Plato MATERIAL: Cerámica CULTURA / ESTILO: Inca CRONOLOGIA: Horizonte Tardío (1,476 d.c. - 1,532 d.c.) Source: Objaverse 1.0 / Sketchfab
Fragmento de plato decorado con asa
Fragmento de plato decorado con asa procedente de el Yacimiento Arqueológico de El Tejar (Santa Brígida - GRAN CANARIA). Source: Objaverse 1.0 / Sketchfab
Platos gemelos de estilo Inca
Material: Cerámica Cultura/Estilo: Inca Datación: Horizonte Tardío (1,476 d.c. - 1,532 d.c.) Técnicas: Modelado, pintura positiva Source: Objaverse 1.0 / Sketchfab
Galactic Component Classification For the all-sky PLATO Input Catalog
<div> <h1>PLATO Targets Classification</h1> <p>This repository contains the full list of PLATO targets, classified into their Galactic Component membership. The basis for the catalogue is the all-sky PLATO input catalog (asPIC) by Montalto2021, crossmatched with Gaia DR3.</p> <h2>Files</h2> <p>There are four files included in this repository:</p> <ol> <li> <p><strong>targets_classified</strong>:</p> <ul> <li>Description: The entire sample, classified into thin disk, thick disk candidate, thick disk, halo candidate, and halo.</li> <li>Note : Classification is only performed if relative uncertainties no greater than 20% in the following columns: "ra", "dec", "pmra", "pmdec", "parallax", and "radial_velocity". For targets where this requirement is not fulfilled, the related columns are filled with NaN.</li> <li>Format: 2,675,538 rows, 61 columns</li> </ul> </li> <li> <p><strong>LOPS2</strong>:</p> <ul> <li>Description: A subselection of targets_classified in the LOPS2 field.</li> <li>Galactic Coordinates: l=255.9375°, b=-24.62432°</li> <li>Additional Column: "n_cameras" specifying the number of PLATO cameras that will observe the target.</li> <li>Format: 169,438 rows, 62 columns</li> </ul> </li> <li> <p><strong>LOPN1</strong>:</p> <ul> <li>Description: A subselection of targets_classified in the LOPN1 field.</li> <li>Galactic Coordinates: l=81.56250°, b=24.62432°</li> <li>Format: 173,735 rows, 62 columns</li> </ul> </li> <li> <p><strong>special_target_list</strong>:</p> <ul> <li>Description: A selection of 47 targets, kinematically classified as halo stars, within the high-SNR P1 PLATO sample.</li> <li>Additional Column: "n_cameras" specifying the number of PLATO cameras that will observe the target, and "Field" specifying if target belongs to LOPS2 or LOPN1 field</li> <li>Format: 47 rows, 63 columns</li> </ul> </li> </ol> <h2>Classification Criteria</h2> <p>We classify only those stars into Galactic components that have relatively certain kinematic parameters. Specifically, we require no more than 20% relative uncertainty in the following columns: "ra", "dec", "pmra", "pmdec", "parallax", "radial_velocity". This results in 2,283,538 out of the total 2,675,539 stars having a component classification.</p> <h2>Analysis Conditions</h2> <p>For the analysis in our paper, we applied the following additional conditions:</p> <ul> <li>Population.notnull()</li> <li>Stellar type = FGK</li> <li>Radius > 0</li> <li>Mass > 0</li> <li>Teff > 0</li> <li>Logg.notnull()</li> <li>[Fe/H].notnull()</li> </ul> <p>Applying these conditions results in 1,830,288 entries remaining.</p> <h2>Columns</h2> <p>The columns in the dataset are as follows:</p> <table> <tbody> <tr> <th>Column Name</th> <th>Description</th> </tr> </tbody> <tbody> <tr> <td>gaiaID_DR2</td> <td>Gaia DR2 ID (from asPIC catalog, Montalto2021)</td> </tr> <tr> <td>gaiaID_DR3</td> <td>Gaia DR3 ID (matched to DR2 catalog, based on angular distance)</td> </tr> <tr> <td>parallax</td> <td>Parallax of target (mas), from Gaia DR3</td> </tr> <tr> <td>e_parallax</td> <td>Error on parallax</td> </tr> <tr> <td>ra</td> <td>Right Ascension (deg) from Gaia DR3</td> </tr> <tr> <td>e_ra</td> <td>Error on Right Ascension</td> </tr> <tr> <td>dec</td> <td>Declination (deg) from Gaia DR3</td> </tr> <tr> <td>e_dec</td> <td>Error on declination</td> </tr> <tr> <td>pmra</td> <td>Proper motion in right ascension direction (mas/yr), from Gaia DR3</td> </tr> <tr> <td>e_pmra</td> <td>Error on proper motion in right ascension direction</td> </tr> <tr> <td>pmdec</td> <td>Proper motion in declination direction (mas/yr), from Gaia DR3</td> </tr> <tr> <td>e_pmdec</td> <td>Error on proper motion in declination direction</td> </tr> <tr> <td>radial_velocity</td> <td>Radial velocity (km/s), from Gaia DR3</td> </tr> <tr> <td>e_radial_velocity</td> <td>Radial velocity error</td> </tr> <tr> <td>[alpha/Fe]</td> <td>Alpha elemental abundance from Gaia RV spectra, alphafe_gspspec in Gaia DR3</td> </tr> <tr> <td>e_[alpha/Fe]_lower</td> <td>Lower error on alpha element abundance</td> </tr> <tr> <td>e_[alpha/Fe]_upper</td> <td>Upper error on alpha element abundance</td> </tr> <tr> <td>[Fe/H]</td> <td>Metallicity estimate, either from RVS spectra (mh_gsspec in Gaia DR3, with first 13 quality flags equal to 0, Recio-Blanco2023) or XGBOOST (Andrae2023)</td> </tr> <tr> <td>[Fe/H]_source</td> <td>Source of the metallicity estimate</td> </tr> <tr> <td>e_[Fe/H]_lower</td> <td>Lower error on the metallicity estimate (NaN in case of Andrae2023)</td> </tr> <tr> <td>e_[Fe/H]_upper</td> <td>Upper error on the metallicity estimate (NaN in case of Andrae2023)</td> </tr> <tr> <td>logg</td> <td>log g estimate, either from RVS spectra (logg_gsspec in Gaia DR3, with first 13 quality flags equal to 0, Recio-Blanco2023) or XGBOOST (Andrae2023)</td> </tr> <tr> <td>logg_source</td> <td>Source of the log g estimate</td> </tr> <tr> <td>e_logg_lower</td> <td>Lower error on the log g estimate (NaN in case of Andrae2023)</td> </tr> <tr> <td>e_logg_upper</td> <td>Upper error on the log g estimate (NaN in case of Andrae2023)</td> </tr> <tr> <td>[Fe/H]_apogee</td> <td>Metallicity estimate from APOGEE-DR17</td> </tr> <tr> <td>e_[Fe/H]_apogee</td> <td>Error on APOGEE metallicity estimate</td> </tr> <tr> <td>[alpha/M]_apogee</td> <td>Alpha abundance estimate from APOGEE-DR17</td> </tr> <tr> <td>e_[alpha/M]_apogee</td> <td>Error on APOGEE alpha estimate</td> </tr> <tr> <td>logg_apogee</td> <td>log g estimate from APOGEE-DR17</td> </tr> <tr> <td>e_logg_apogee</td> <td>Error on APOGEE log g estimate</td> </tr> <tr> <td>[Fe/H]_galah</td> <td>Metallicity estimate from GALAH DR3</td> </tr> <tr> <td>e_[Fe/H]_galah</td> <td>Error on GALAH metallicity</td> </tr> <tr> <td>[alpha/Fe]_galah</td> <td>Alpha abundance estimate from GALAH DR3</td> </tr> <tr> <td>e_[alpha/Fe]_galah</td> <td>Error on GALAH alpha abundance</td> </tr> <tr> <td>logg_galah</td> <td>log g estimate from GALAH DR3</td> </tr> <tr> <td>e_logg_galah</td> <td>Error on GALAH log g</td> </tr> <tr> <td>GLON</td> <td>Galactic longitude (deg)</td> </tr> <tr> <td>GLAT</td> <td>Galactic latitude (deg)</td> </tr> <tr> <td>U</td> <td>Heliocentric velocity in the direction of the Galactic center (km/s), calculated from ra, dec, parallax, pmra, pmdec, radial_velocity using galpy, only available if Population could be determined (see Classification Criteria)</td> </tr> <tr> <td>V</td> <td>Heliocentric velocity in the direction of the Galactic rotation (km/s), calculated from ra, dec, parallax, pmra, pmdec, radial_velocity using galpy, only available if Population could be determined (see Classification Criteria)</td> </tr> <tr> <td>W</td> <td>Heliocentric velocity in the direction of the North Galactic Pole (km/s), calculated from ra, dec, parallax, pmra, pmdec, radial_velocity using galpy, only available if Population could be determined (see Classification Criteria)</td> </tr> <tr> <td>UW</td> <td>Total non-circular velocity UW = sqrt(U^2 + W^2) (km/s), only available if Population could be determined (see Classification Criteria)</td> </tr> <tr> <td>R</td> <td>Distance from the Galactic center in the Galactic plane (kpc), only available if Population could be determined (see Classification Criteria)</td> </tr> <tr> <td>Z</td> <td>Distance from the Galactic plane (kpc), only available if Population could be determined (see Classification Criteria)</td> </tr> <tr> <td>gaiaV</td> <td>V-band magnitude (from asPIC catalog, Montalto2021)</td> </tr> <tr> <td>e_gaiaV</td> <td>Error on V-band magnitude</td> </tr> <tr> <td>Gmag</td> <td>Gaia G magnitude (from asPIC catalog, Montalto2021)</td> </tr> <tr> <td>e_Gmag</td> <td>Error on G magnitude</td> </tr> <tr> <td>Radius</td> <td>Radius of star (solar radii) (from asPIC catalog, Montalto2021)</td> </tr> <tr> <td>e_Radius</td> <td>Error on radius</td> </tr> <tr> <td>Mass</td> <td>Mass of star (solar masses) (from asPIC catalog, Montalto2021)</td> </tr> <tr> <td>e_Mass</td> <td>Error on mass</td> </tr> <tr> <td>Teff</td> <td>Effective temperature of star (K) (from asPIC catalog, Montalto2021)</td> </tr> <tr> <td>e_Teff</td> <td>Error on effective temperature</td> </tr> <tr> <td>Stellar Type</td> <td>Classification into M or FGK type, based on asPIC catalog (Montalto2021)</td> </tr> <tr> <td>u1</td> <td>The first quadratic limb-darkening parameter, based on grid by Morello2022</td> </tr> <tr> <td>u2</td> <td>The second quadratic limb-darkening parameter, based on grid by Morello2022</td> </tr> <tr> <td>TD/D</td> <td>Probability ratio thick disk/thin disk (see Section 2.2. in our paper), only available if Population could be determined (see Classification Criteria)</td> </tr> <tr> <td>TD/H</td> <td>Probability ratio thick disk/halo (see Section 2.2 in our paper), only available if Population could be determined (see Classification Criteria)</td> </tr> <tr> <td>Population</td> <td>Galactic component classification (Thin Disk, Thick Disk, Halo, Thick Disk Candidate, Halo Candidate), see paper for definitions, only available if Population could be determined (see Classification Criteria)</td> </tr> <tr> <td>n_cameras</td> <td>Number of PLATO cameras observing the target (Additional Column for LOPS2, LOPN1, and Special Target List)</td> </tr> <tr> <td>field</td> <td>Flag for LOPS2 or LOPN1 fields (Additional Column for Special Target List)</td> </tr> </tbody> </table> </div>
Plato estilo Chincha
Material: Cerámica Cultura/Estilo: Ica Datación: Intermedio Tardío (1,000 d.c. - 1,476 d.c.) Técnicas: Modelado Source: Objaverse 1.0 / Sketchfab
Plato de cerámica estilo Killke
N° de Registro Nacional: 0000297549 DATOS DE IDENTIFICACIÓN BIEN CULTURAL: Plato MATERIAL: Cerámica CULTURA / ESTILO: Killke CRONOLOGIA: Intermedio Tardío (1,000 d.c. - 1476 d.c.) Source: Objaverse 1.0 / Sketchfab
Plato mapuche de madera
Plato de madera, con asas. Mapuche. Loncoche, Región de la Araucanía, Chile. Source: Objaverse 1.0 / Sketchfab
Plato - Fajalauza-HD (54)
Plato (GR.CRSD.05.1006.31) producido en los talleres de Fajalauza (Granada, España). Ha sido modelado a torno y cocido en una atmósfera oxidante. Tiene una forma abierta, parte de un labio redondeado y borde exvasado con el cuerpo de perfil troncocónico abierto y base plana rehundida. Presenta una decoración interna y central de manganeso con un motivo floral y una cenefa de cadenas en el borde. * Cronología: Siglos XVII-XVIII. * Depósito: Dpto. de Historia Medieval y CCTTHH de la Universidad de Granada. * Yacimiento: Cuarto Real de Santo Domingo, Granada, excavaciones arqeuológicas del año 2005. [FAJALAUZA-Hd](https://acortar.link/bNsUsm) Colaboran: [PRINMA](http://blogs.ugr.es/prinma/), [UGR](http://www.ugr.es), [Fundación Fajalauza](https://acortar.link/shJ8ps) , [Museo Arqueológico y Etnológico de Granada](https://acortar.link/DF0cOC), [Patronato de la Alhambra y Generalife](https://acortar.link/FcstHW) Fotografías y modelo: [Francisco Lara Piñera](https://acortar.link/Bam3Op) Source: Objaverse 1.0 / Sketchfab
Plato - Fajalauza-HD (30)
Plato (DJ365-64) producido en los talleres de Fajalauza (Granada, España). Ha sido modelado a torno y cocido en una atmósfera oxidante. Tiene una forma abierta, parte de un labio redondeado y borde exvasado, que continúa en un cuerpo con perfil troncocónico abierto y base plana rehundida. Está decorado con una rama terminada en capullo con formas geométricas en el borde. * Cronología: 1511-1549. * Depósito: Museo Arqueológico y Etnológico de Granada. * Yacimiento: Excavación del Hospital Real, 1990. [FAJALAUZA-Hd](https://acortar.link/bNsUsm) Colaboran: [PRINMA](http://blogs.ugr.es/prinma/), [UGR](http://www.ugr.es), [Fundación Fajalauza](https://acortar.link/shJ8ps) , [Museo Arqueológico y Etnológico de Granada](https://acortar.link/DF0cOC), [Patronato de la Alhambra y Generalife](https://acortar.link/FcstHW) Fotografías y modelo: [Francisco Lara Piñera](https://acortar.link/Bam3Op) Source: Objaverse 1.0 / Sketchfab
Plato - Fajalauza-HD (4)
Plato (GR.CRSD.05.1373) producido en los talleres de Fajalauza (Granada, España). Ha sido modelado a torno y cocido en una atmósfera oxidante. Tiene una forma abierta, parte de un labio redondeado y borde exvasado con cuerpo de perfil troncocónico abierto y base plana rehundida. Presenta una decoración interna y central en azul con un motivo floral y una cenefa de cadenas en el borde. * Cronología: Siglos XVII-XVIII. * Depósito: Dpto. de Historia Medieval y CCTTHH de la Universidad de Granada. * Yacimiento: Cuarto Real de Santo Domingo, Granada, excavaciones arqeuológicas del año 2005. [FAJALAUZA-Hd](https://acortar.link/bNsUsm) Colaboran: [PRINMA](http://blogs.ugr.es/prinma/), [UGR](http://www.ugr.es), [Fundación Fajalauza](https://acortar.link/shJ8ps) , [Museo Arqueológico y Etnológico de Granada](https://acortar.link/DF0cOC), [Patronato de la Alhambra y Generalife](https://acortar.link/FcstHW) Fotografías y modelo: [Francisco Lara Piñera](https://acortar.link/Bam3Op) Source: Objaverse 1.0 / Sketchfab
CE 0180 - PLATO
N° de Registro Nacional: 0000303486 DATOS DE IDENTIFICACIÓN BIEN CULTURAL: Plato MATERIAL: Cerámica CULTURA / ESTILO: Inca CRONOLOGIA: Horizonte Tardío (1,476 d.c. - 1,532 d.c.) Source: Objaverse 1.0 / Sketchfab
PLATO - Medication Adherence in Transplant Recipients
ClinicalTrials.gov study NCT04078750. IPD Sharing: NO. Countries: 1. Publications: 0.
Plato Cajamarca
Source: Objaverse 1.0 / Sketchfab
Plato Cajamarca - Intermedio Temprano
Source: Objaverse 1.0 / Sketchfab
CE 1251 - PLATO
N° de Registro Nacional: 0000297542 DATOS DE IDENTIFICACION BIEN CULTURAL: Plato MATERIAL: Cerámica CULTURA / ESTILO: Inca CRONOLOGIA: Horizonte Tardío (1,476 d.c. – 1,532 d.c.) Source: Objaverse 1.0 / Sketchfab
CE 3334 - PLATO
N° de Registro Nacional: 0000297141 DATOS DE IDENTIFICACION BIEN CULTURAL: Plato MATERIAL: Cerámica CULTURA / ESTILO: Inca CRONOLOGIA: Horizonte Tardío (1,476 d.c. – 1,532 d.c.) Source: Objaverse 1.0 / Sketchfab
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