cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
A profile of the socialist movement in the western half of the Habsburg Monarchy in the second half of the nineteenth century
Creators: name: Black, John William
Publisher: name: University of British Columbia
Year: 2010

description: The purpose of this thesis is to examine several important aspects of social democracy in the Cisleithanian half of the Habsburg Monarchy in the years between 1867 and 1901. By exploring the environment in which the socialist movement developed, the socialist ideology, the development of the party and its organization, and the socialist leadership, it presents a profile of the Cisleithanian socialist movement. In spite of the fact that the socialist movement in Cisleithania was one of the largest in Europe by 1901, historians have tended to ignore both its development and its peculiarities. The Cisleithanian socialist movement, and particularly its German-speaking component, has been seen as merely a junior partner of the Reich-German socialist movement. To a certain extent this was true, for Cisleithanian socialists did import their ideology and their original conceptions of party and trade union organization from Germany. Yet the models imported from Germany all had to be adapted to the multi-national character of the socialist movement in Cisleithania. Marxism was adopted, but Cisleithanian socialists were forced to take a position on the complex nationality question in Cisleithania, a question for which there was no acceptable Marxist "answer." The German idea of a centralized party organization was also taken over, but it had to be abandoned in face of demands for autonomy on the part of Czech socialists. An entirely new and unique form of party organization was evolved. In the trade union movement, the concept of centralism was also adopted, and once more proved unsuitable in a multinational environment, in spite of convincing arguments in its favour. In these respects, and others, Cisleithanian socialists made an important contribution to the development of the European socialist movement, a contribution which deserves more attention from historians than it has received. The major problem the Cisleithanian social movement faced was the nationality question. The multi-national nature of the state and the socialist movement, in a context in which nationalist feeling was very strong, helped to determine both the development and the fate of the socialist movement of all nationalities in the western half of the Monarchy. In fact, the nationality conflict which developed in the Cisleithanian socialist movement mirrored the conflict in Cisleithania as a whole. Indeed, the contradiction between the theory of socialist internationalism and the practical reality of nationalism in the working class was apparent in the Cisleithanian socialist movement long before the outbreak of the First World War made it clear to non-socialists and socialists alike. In this sense, the study of the Cisleithanian socialist movement is also a study in nationalism.
K2: A new method for the detection of galaxy clusters based on CFHTLS multicolor images
Creators: name: Thanjavur, Karun
name: Willis, Jon
name: Crampton, David
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We have developed a new method, K2, optimized for the detection of galaxy clusters in multicolor images. Based on the Red Sequence approach, K2 detects clusters using simultaneous enhancements in both colors and position. The detection significance is robustly determined through extensive Monte-Carlo simulations and through comparison with available cluster catalogs based on two different optical methods, and also on X-ray data. K2 also provides quantitative estimates of the candidate clusters' richness and photometric redshifts. Initially K2 was applied to 161 sq deg of two color gri images of the CFHTLS-Wide data. Our simulations show that the false detection rate, at our selected threshold, is only ~1%, and that the cluster catalogs are ~80% complete up to a redshift of 0.6 for Fornax-like and richer clusters and to z ~0.3 for poorer clusters. Based on Terapix T05 release gri photometric catalogs, 35 clusters/sq deg are detected, with 1-2 Fornax-like or richer clusters every two square degrees. Catalogs containing data for 6144 galaxy clusters have been prepared, of which 239 are rich clusters. These clusters, especially the latter, are being searched for gravitational lenses -- one of our chief motivations for cluster detection in CFHTLS. The K2 method can be easily extended to use additional color information and thus improve overall cluster detection to higher redshifts. The complete set of K2 cluster catalogs, along with the supplementary catalogs for the member galaxies, are available on request from the authors.
description: Accepted in ApJ. 25 pages, including 10 figures. Latex with emulateapj v03/07/07
Population ageing, longevity and migration: an overlapping
generations approach
Creators: name: Melindi Ghidi, Paolo <1979>
Publisher: name: Alma Mater Studiorum - Università di Bologna
Year: 2008
Subjects: SECS-P/01 Economia politica

description: The silent demographic revolution characterizing the main industrialized countries is an
unavoidable factor which has major economic, social, cultural and psychological implications. This
thesis studies the main consequences of population ageing and the connections with the
phenomenon of migration, The theoretical analysis is developed using Overlapping Generations
Models (OLG). The thesis is divided in the following four chapters: 1) “A Model for Determining
Consumption and Social Assistance Demand in Uncertainty Conditions”, focuses on the relation
between demographic impact and social insurance and proposes the institution of a non selfsufficiency
fund for the elderly. 2) "Population Ageing, Longevity and Health", analyzes the effects
of health investment on intertemporal individual behaviour and capital accumulation. 3)
"Population Ageing and the Nursing Flow", studies the consequences of migration in the nursing
sector. 4) "Quality of Multiculturalism and Minorities' Assimilation", focuses on the problem of
assimilation and integration of minorities.
Tracking The Post-BBN Evolution Of Deuterium
Creators: name: Steigman, Gary
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The primordial abundance of deuterium produced during Big Bang Nucleosynthesis (BBN) depends sensitively on the universal ratio of baryons to photons, an important cosmological parameter probed independently by the Cosmic Microwave Background (CMB) radiation. Observations of deuterium in high-redshift, low-metallicity QSO Absorption Line Systems (QSOALS) provide a key baryometer, determining the baryon abundance at the time of BBN to a precision of 5%. Alternatively, if the CMB-determined baryon to photon ratio is used in the BBN calculation of the primordial abundances, the BBN-predicted deuterium abundance may be compared with the primordial value inferred from the QSOALS, testing the standard cosmological model. In the post-BBN universe, as gas is cycled through stars, deuterium is only destroyed so that its abundance measured anytime, anywhere in the Universe, bounds the primordial abundance from below. Constraints on models of post-BBN Galactic chemical evolution follow from a comparison of the relic deuterium abundance with the FUSE-inferred deuterium abundances in the chemically enriched, stellar processed material of the local ISM.
description: 8 pages, 5 figures, to appear in the Proceedings of the Future Directions in Ultraviolet Spectroscopy Conference
Structures of Local Galaxies Compared to High Redshift Star-forming Galaxies
Creators: name: Petty, Sara M.
name: de Mello, Duilia F.
name: Gallagher, John S.
name: Gardner, Jonathan P.
name: Lotz, Jennifer M.
name: Mountain, C. Matt
name: Smith, Linda J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The rest-frame far-ultraviolet (FUV) morphologies of 8 nearby interacting and starburst galaxies (Arp 269, M 82, Mrk 8, NGC 520, NGC 1068, NGC 3079, NGC 3310, NGC 7673) are compared with 54 galaxies at z ~ 1.5 and 46 galaxies at z ~ 4 observed in the GOODS-ACS field. The nearby sample is artificially redshifted to z ~ 1.5 and 4. We compare the simulated galaxy morphologies to real z ~ 1.5 and 4 UV-bright galaxy morphologies. We calculate the Gini coefficient (G), the second-order moment of the brightest 20% of the galaxy's flux (M_20), and the Sersic index (n). We explore the use of nonparametric methods with 2D profile fitting and find the combination of M_20 with n an efficient method to classify galaxies as having merger, exponential disk, or bulge-like morphologies. When classified according to G and M_20, 20/30% of real/simulated galaxies at z ~ 1.5 and 37/12% at z ~ 4 have bulge-like morphologies. The rest have merger-like or intermediate distributions. Alternatively, when classified according to the Sersic index, 70% of the z ~ 1.5 and z ~ 4 real galaxies are exponential disks or bulge-like with n > 0.8, and ~30% of the real galaxies are classified as mergers. The artificially redshifted galaxies have n values with ~35% bulge or exponential at z ~ 1.5 and 4. Therefore, ~20-30% of Lyman-break galaxies (LBGs) have structures similar to local starburst mergers, and may be driven by similar processes. We assume merger-like or clumpy star-forming galaxies in the GOODS field have morphological structure with values n < 0.8 and M_20 > -1.7. We conclude that Mrk 8, NGC 3079, and NGC 7673 have structures similar to those of merger-like and clumpy star-forming galaxies observed at z ~ 1.5 and 4.
description: Accepted by The Astronomical Journal May 2009. Changes include an added explanation of methods in Section 3
CNO enrichment by rotating AGB stars in globular clusters
Creators: name: Decressin, T.
name: Charbonnel, C.
name: Siess, L.
name: Palacios, A.
name: Meynet, G.
name: Georgy, C.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: AGB stars have long been held responsible for the important star-to-star variations in light elements observed in Galactic globular clusters. We analyse the main impacts of a first generation of rotating intermediate-mass stars on the chemical properties of second-generation globular cluster stars. The rotating models were computed without magnetic fields and without the effects of internal gravity waves. They account for the transports by meridional currents and turbulence. We computed the evolution of both standard and rotating stellar models with initial masses between 2.5 and 8 Msun within the metallicity range covered by Galactic globular clusters. During central He-burning, rotational mixing transports fresh CO-rich material from the core towards the hydrogen-burning shell, leading to the production of primary 14N. In stars more massive than M > 4 Msun, the convective envelope reaches this reservoir during the second dredge-up episode, resulting in a large increase in the total C+N+O content at the stellar surface and in the stellar wind. The corresponding pollution depends on the initial metallicity. At low- and intermediate-metallicity, it is at odds with the constancy of C+N+O observed among globular cluster low-mass stars. With the given input physics, our models suggest that massive rotating AGB stars have not shaped the abundance patterns observed in low- and intermediate-metallicity globular clusters. Our non-rotating models, on the other hands, do not predict surface C+N+O enhancements, hence are in a better position as sources of the chemical anomalies in globular clusters showing the constancy of the C+N+O. However at the moment, there is no reason to think that intermediate mass stars were not rotating.
description: Accepted in Astronomy and Astrophysics, 7 pages, 3 figures
Additional file 1 of Integrating metabolomic data with machine learning approach for discovery of Q-markers from Jinqi Jiangtang preparation against type 2 diabetes
Creators: name: Yang, Lele
name: Xue, Yan
name: Wei, Jinchao
name: Dai, Qi
name: Li, Peng
Publisher: name: figshare
Year: 2021
Subjects: subject: Artificial Intelligence and Image Processing
subject: FOS: Computer and information sciences

description: Additional file 1. Additional tables and figures.
Lingue meno diffuse e corpora: studio empirico sulla terminologia amministrativa ladina
Creators: name: Ties, Isabella <1977>
Publisher: name: Alma Mater Studiorum - Università di Bologna
Year: 2008
Subjects: L-LIN/14 Lingua e traduzione - Lingua tedesca

description: This study aims to the elaboration of juridical and administrative terminology in
Ladin language, actually on the Ladin idiom spoken in Val Badia. The necessity of this
study is strictly connected to the fact that in South Tyrol the Ladin language is not just
safeguarded, but the editing of administrative and normative text is guaranteed by law.
This means that there is a need for a unique terminology in order to support translators
and editors of specialised texts.
The starting point of this study are, on one side the need of a unique terminology,
and on the other side the translation work done till now from the employees of the
public administration in Ladin language. In order to document their efforts a corpus
made up of digitalized administrative and normative documents was build.
The first two chapters focuses on the state of the art of projects on terminology and
corpus linguistics for lesser used languages. The information were collected thanks to
the help of institutes, universities and researchers dealing with lesser used languages.
The third chapter focuses on the development of administrative language in Ladin
language and the fourth chapter focuses on the creation of the trilingual Italian –
German – Ladin corpus made up of administrative and normative documents.
The last chapter deals with the methodologies applied in order to elaborate the
terminology entries in Ladin language though the use of the trilingual corpus. Starting
from the terminology entry all steps are described, from term extraction, to the
extraction of equivalents, contexts and definitions and of course also of the elaboration
of translation proposals for not found equivalences. Finally the problems referring to the
elaboration of terminology in Ladin language are illustrated.
Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Sky Maps, Systematic Errors, and Basic Results
Creators: name: Jarosik, N.
name: Bennett, C. L.
name: Dunkley, J.
name: Gold, B.
name: Greason, M. R.
name: Halpern, M.
name: Hill, R. S.
name: Hinshaw, G.
name: Kogut, A.
name: Komatsu, E.
name: Larson, D.
name: Limon, M.
name: Meyer, S. S.
name: Nolta, M. R.
name: Odegard, N.
name: Page, L.
name: Smith, K. M.
name: Spergel, D. N.
name: Tucker, G. S.
name: Weiland, J. L.
name: Wollack, E.
name: Wright, E. L.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: (Abridged) New full sky temperature and polarization maps based on seven years of data from WMAP are presented. The new results are consistent with previous results, but have improved due to reduced noise from the additional integration time, improved knowledge of the instrument performance, and improved data analysis procedures. The improvements are described in detail. The seven year data set is well fit by a minimal six-parameter flat Lambda-CDM model. The parameters for this model, using the WMAP data in conjunction with baryon acoustic oscillation data from the Sloan Digital Sky Survey and priors on H_0 from Hubble Space Telescope observations, are: Omega_bh^2 = 0.02260 +-0.00053, Omega_ch^2 = 0.1123 +-0.0035, Omega_Lambda = 0.728 +0.015 -0.016, n_s = 0.963 +-0.012, tau = 0.087 +-0.014 and sigma_8 = 0.809 +-0.024 (68 % CL uncertainties). The temperature power spectrum signal-to-noise ratio per multipole is greater that unity for multipoles < 919, allowing a robust measurement of the third acoustic peak. This measurement results in improved constraints on the matter density, Omega_mh^2 = 0.1334 +0.0056 -0.0055, and the epoch of matter- radiation equality, z_eq = 3196 +134 -133, using WMAP data alone. The new WMAP data, when combined with smaller angular scale microwave background anisotropy data, results in a 3 sigma detection of the abundance of primordial Helium, Y_He = 0.326 +-0.075.The power-law index of the primordial power spectrum is now determined to be n_s = 0.963 +-0.012, excluding the Harrison-Zel'dovich-Peebles spectrum by >3 sigma. These new WMAP measurements provide important tests of Big Bang cosmology.
description: 42 pages, 9 figures, Submitted to Astrophysical Journal Supplement Series
Dark humour as a culture specific phenomenon: a study in screen translation
Creators: name: Bucaria, Chiara <1978>
Publisher: name: Alma Mater Studiorum - Università di Bologna
Year: 2008
Subjects: L-LIN/12 Lingua e traduzione - Lingua inglese

description: The present study aims at analyzing how dark humour as a cinematic genre travels
cross-culturally through a specific mode of audiovisual translation, i.e. dubbing.
In particular, it takes into consideration the processes involved in dubbing humour
from English into Italian as observed in the English- and Italian-language versions
of ten British and American dark comedies from the 1940s to the 2000s. In an
attempt to identify some of the main mechanisms of the dark humour genre, the
humorous content of the films was analyzed in terms of the elements on which
specific scenes are based, mainly the non-verbal and verbal components. In the
cases in which verbal elements were involved, i.e. the examples of verbally
expressed humour, the analysis was concerned with whether they were adapted
into Italian and to what effect.
Quantification of the different kinds of dark humour revealed that in the
sample of dark comedies verbal dark humour had a higher frequency (85.3%) than
non-verbal dark humour (14.7%), which partially disconfirmed the first part of the
research hypothesis. However, the significance of contextual elements in the
conveying of dark humour, both in the form of Nsp VEH (54.31%) and V-V
(V+VE) (21.68%), provided support for the hypothesis that, even when expressed
verbally, dark humour is more closely linked to context-based rather than purely
linguistic humour (4.9%).
The second part of the analysis was concerned with an investigation of the
strategies adopted for the translation of verbal dark humour elements from the SL
(English) into the TL (Italian) through the filter of dubbing. Four translational
strategies were identified as far as the rendering of verbal dark humour is
concerned: i) complete omission; ii) weakening; iii) close rendering; and iv)
increased effect. Complete omission was found to be the most common among
these strategies, with 80.9% of dark humour examples being transposed in a way
that kept the ST’s function substantially intact. Weakening of darkly humorous
lines was applied in 12% of cases, whereas increased effect accounted for 4.6%
and complete omission for 2.5%. The fact that for most examples of Nsp VEH
(84.9%) and V-AC (V+VE) (91.4%) a close rendering effect was observed and
that 12 out of 21 examples of V-AC (PL) (a combined 57%) were either omitted
or weakened seemed to confirm, on the one hand, the complexity of the
translation process required by cases of V-AC (PL) and V-AC (CS). On the other
hand, as suggested in the second part of the research hypothesis, the data might be
interpreted as indicating that lesser effort on the translator/adaptor’s part is
involved in the adaptation of V-AC (Nsp VEH) and V-V (V+VE). The issue of
the possible censorial intervention undergone by examples of verbal dark humour
in the sample still remains unclear.
Radio and $γ$-ray activity in the jet of the blazar S5 0716$+$714
Creators: name: Kim, Dae-Won
name: Kravchenko, Evgeniya V.
name: Kutkin, Alexander M.
name: Böttcher, Markus
name: Gómez, José L.
name: Gurwell, Mark
name: Jorstad, Svetlana G.
name: Lähteenmäki, Anne
name: Marscher, Alan P.
name: Ramakrishnan, Venkatessh
name: Tornikoski, Merja
name: Trippe, Sascha
name: Weaver, Zachary
name: Williamson, Karen E.
Publisher: name: arXiv
Year: 2021
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We explore the connection between the $γ$-ray and radio emission in the jet of the blazar 0716$+$714 by using 15, 37, and 230 GHz radio and 0.1$-$200 GeV $γ$-ray light curves spanning 10.5 years (2008$-$2019). We find significant positive and negative correlations between radio and $γ$-ray fluxes in different time ranges. The time delays between radio and $γ$-ray emission suggest that the observed $γ$-ray flares originated from multiple regions upstream of the radio core, within a few parsecs from the central engine. Using time-resolved 43 GHz VLBA maps we identified 14 jet components moving downstream along the jet. Their apparent speeds range from 6 to 26 $c$, showing notable variations in their position angles upstream the stationary component ($\sim$0.53 mas from the core). The brightness temperature declines as function of distance from the core according to a power-law which becomes shallower at the location of the stationary component. We also find that the periods at which significant correlations between radio and $γ$-ray emission occur overlap with the times when the jet was oriented to the north. Our results indicate that the passage of a propagating disturbance (or shock) through the radio core and the orientation of the jet might be responsible for the observed correlation between the radio and $γ$-ray variability. We present a scenario that connects the positive correlation and the unusual anti-correlation by combining the production of a flare and a dip at $γ$-rays by a strong moving shock at different distances from the jet apex.
description: 26 pages, 13 figures, 5 tables, Accepted for publication in ApJ
ASSEMBLY X86 – AN INTRODUCTION
Creators: name: Brandl, Edenilson
Publisher: name: Zenodo
Year: 2023
Subjects: x86 assembly
data transfer
control flow
syntax conventions
addressing modes
stack manipulation
system calls
interrupts
subroutine
CALL instruction

description: This article provides a comprehensive exploration of key concepts in x86 assembly language programming. Covering fundamental topics such as data transfer instructions, control flow mechanisms, syntax conventions, addressing modes, stack manipulation, and system calls, the article aims to equip readers with a solid understanding of low-level development in the x86 architecture. Through clear explanations, code snippets, and practical examples, both novice and experienced developers can gain insights into the intricacies of assembly programming, enabling them to write efficient and maintainable code.
Deliverable D3.9 Final report on the integration of services into EOSC
Creators: name: Röblitz, Thomas
name: Hansson, Emma-Lisa
name: Livenson, Ilja
Publisher: name: Zenodo
Year: 2022
Subjects: EOSC-Nordic
Final report

description: More than three years ago, work package 3 (WP3) in EOSC-Nordic started with the hypothesis that the European Open Science Cloud (EOSC) will be - at least initially - built from existing services offered by various stakeholders (called service providers in this document): universities, research organisations, national e-infrastructure providers, regional and pan-European organisations. Key questions we wanted to answer during the project were: ● How can we support the service providers to offer their services also through EOSC?
 ● Are the existing services mature enough to be accepted into the EOSC service catalog?
 ● How can we help the service providers to improve the maturity of their services?
 ● What needs to be done to foster interoperability of these services? In the document, we first provide some context about what EOSC is and what it aims to achieve, how the whole EOSC-Nordic project was structured and what aims of EOSC were addressed by work package 3. We then describe the approach taken in work package 3 of EOSC-Nordic and provide an overview of the work done in work package 3. We briefly present work package 5 (titled "Open research data & services") of EOSC-Nordic and discuss their key findings - how they are supported by EOSC goals and what solutions work package 3 provides for their requirements. In the section "Service Provider Interviews," we report on interviews with service providers we conducted at the end of the project. We conclude the report with key recommendations for future work.
title: Unkomplizierte Harnwegsinfektion. Brennen beim Wasserlassen, häufiger Harndrang – was tun bei Blasenentzündung?
Creators: name: Ärztliches Zentrum Für Qualität In Der Medizin (ÄZQ)
Publisher: name: Bundesärztekammer (BÄK); Kassenärztliche Bundesvereinigung (KBV); Ärztliches Zentrum für Qualität in der Medizin (ÄZQ)
Year: 2018
Subjects: subject: 610 Medical sciences; Medicine

description: Kurzinformation für Patienten
ניסויית-הרשמה מראש
Creators: name: מולאי נגה
name: Biran, Hilla
name: Brikman, Yael
Publisher: name: Open Science Framework
Year: 2023
Subjects: subject: Psychology
subject: FOS: Psychology
subject: Social and Behavioral Sciences

description: .זוהי הרשמה מראש למחקר שלנו על השפעת עצמאות כלכלית ויציבות כלכלית על סיפוק מעבודה, במסגרת קורס פסיכולוגיה ניסויית
Amaioua glomerulata Delprete & C. Persson, comb. nov.
Creators: name: Delprete, Piero G.
name: Persson, Claes
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Gentianales
Rubiaceae
Amaioua
Amaioua glomerulata

description: Amaioua glomerulata (Lam. ex Poir.) Delprete & C.Persson, comb. nov. (Fig. 2) Mussaenda glomerulata Lam.ex Poir., Encyclopédie méthodique, Botanique 4: 393 (1797). — Rondeletia glomerulata (Lam. ex Poir.) Spreng., Systema Vegetabilium 1: 707 (1824). — Type: French Guiana, s.d. [1781-1785], L.C. Richard s.n. (lecto-, P-Lam [P00308470!], here designated). Amaioua corymbosa Kunth in Humb. & Bonpl., Nova Genera et Species Plantarum 3: 419 (1820). — Type: Venezuela, Cumanacoa, Humboldt & Bonpland s.n. (holo-, P-Bonpl.!). Amaioua fagifolia Desf., Mémoires du Muséum national d’Histoire naturelle (Paris) 6: 14 (1820). — Type:French Guiana,s.d., J.Martin s.n. (syn-,P[2 specimens], P-Juss.!). SPECIMENS EXAMINED. — Mexico. Chiapas, Mun. Las Margaritas, W side of Laguna Miramar, E side of San Quintín, 350 m, 11.II.1973, fr., Breedlove 33144 (NY). Belize. Cayo, near Augustine, 450 m, 26.VIII.1980, fem. fl., Whiteford 2222 (BM). Nicaragua. Comarca de El Cabo Río Leicus, 28 km SW of Waspan, 66 m, 25.VIII.1965, fem. fl., Molina R. 15200 (NY). Guatemala. Izabal, Sto. Tomás de Castilla, c. 30 km SW of town, Sinai, 15°39’N, 88°35’W, 15.III.1988, fr., Marshall et al. 396 (NY). Panama. Panama, Las Perlas, San José Island, 19.VII.1967, male fl., Stimson 5328 (NY). Guyana. Kanuku Mts, Rupunini R., Crabwood Cr., 29.VI.1995, fr., Jansen-Jacobs et al. 4278 (CAY, GB, NY). — Rupununi Distr., Kuyuwini Landing,Kuyuwini R., 10.X.1992, imm. fr., Jansen-Jacobs et al.2832 (CAY, L, NY). Suriname. Distr. Suriname, Zanderij Savanne, Hekking 901 (L). — Mapane Creek, area near camp 8, Schulz 7548 (L, NY). French Guiana. Sinnamary, Brigandin, 26.III.1993, imm. fr., Puig 12055 (CAY). — Basse crique Courouaïe (affluent du Bas Approuague), à 5 km en amont des Deux Fourches, 15.I.1970, imm. fr., Oldeman B-2766 (CAY). DISTRIBUTION AND ECOLOGY Distributed from Mexico and Cuba to Colombia, Venezuela, the Guianas, and Brazil. It is found in low scrub forest, seasonally deciduous forest, or savanna forest on white sand, lateritic clay soil, brown sand on rocky substrate, sometimes along creeks on alluvial soils, from sea level to 800 m altitude.
description: Published as part of Delprete, Piero G. & Persson, Claes, 2012, Octavia sessiliflora DC. and Mussaenda glomerulata Lam. ex Poir., two obscure taxa from French Guiana synonymous with members of the Alibertia group (Rubiaceae, Gardenieae), pp. 353-363 in Adansonia (3) (3) 34 (2) on page 356, DOI: 10.5252/a2012n2a9, http://zenodo.org/record/5205961
A SURE Approach for Digital Signal/Image Deconvolution Problems
Creators: name: Pesquet, Jean-Christophe
name: Benazza-Benyahia, Amel
name: Chaux, Caroline
Publisher: name: arXiv
Year: 2008
Subjects: subject: Methodology (stat.ME)
subject: Statistics Theory (math.ST)
subject: FOS: Computer and information sciences
subject: FOS: Mathematics

description: In this paper, we are interested in the classical problem of restoring data degraded by a convolution and the addition of a white Gaussian noise. The originality of the proposed approach is two-fold. Firstly, we formulate the restoration problem as a nonlinear estimation problem leading to the minimization of a criterion derived from Stein's unbiased quadratic risk estimate. Secondly, the deconvolution procedure is performed using any analysis and synthesis frames that can be overcomplete or not. New theoretical results concerning the calculation of the variance of the Stein's risk estimate are also provided in this work. Simulations carried out on natural images show the good performance of our method w.r.t. conventional wavelet-based restoration methods.
The moderating effect of temperament in mindfulness-based interventions on children’s cognitive skills and mental health
Creators: name: Boglarka Vekety
name: Koncz, Adam
name: Aniko Lilla Patanyi
name: Reka Kassai
name: Takacs, Zsofia K.
Publisher: name: Open Science Framework
Year: 2023
Subjects: subject: Psychology
subject: FOS: Psychology
subject: Social and Behavioral Sciences
subject: School Psychology
subject: Child Psychology
subject: mindfulness
subject: SDQ
subject: individual differences
subject: temperament
subject: executive functions
subject: cortisol

description: We are utilizing data from four previous, small-scale pilot RCTs of various mindfulness-based programs for children. All of these studies assessed executive function skills and two of the studies applied baseline cortisol assessment as well. Additionally, these studies applied a measure of children’s temperament (emotionality, activity, shyness, and sociability) and behavior problems (based on parents’ reports) at baseline. These will be tested as potential moderators of intervention efficacy. At the end we use a meta analytic analysis on the four small-scale pilot RCTs.
REQUIREMENTS FOR SPEECH DEVELOPMENT OF PRESCHOOL CHILDREN
Creators: name: Tolipova. O.I.  teacher at Kokan State Pedagogical Institute,  candidate of pedagogical sciences.
Publisher: name: Zenodo
Year: 2023

description: The article describes the formation of two interrelated areas of speech education in preschool age: teaching the native language (phonetics, vocabulary, grammar) and linguistic cognitive activity and methods of communication.

Key words: Preschool age, environment, game, education, language, speech, development, personality, activity.
Small Angular Scale Measurements of the CMB Temperature Power Spectrum from QUaD
Creators: name: QUaD Collaboration
name: Friedman, R. B.
name: Ade, P.
name: Bock, J.
name: Bowden, M.
name: Brown, M. L.
name: Cahill, G.
name: Castro, P. G.
name: Church, S.
name: Culverhouse, T.
name: Ganga, K.
name: Gear, W. K.
name: Gupta, S.
name: Hinderks, J.
name: Kovac, J.
name: Lange, A. E.
name: Leitch, E.
name: Melhuish, S. J.
name: Memari, Y.
name: Murphy, J. A.
name: Orlando, A.
name: Sullivan, C. O'
name: Piccirillo, L.
name: Pryke, C.
name: Rajguru, N.
name: Rusholme, B.
name: Schwarz, R.
name: Taylor, A. N.
name: Thompson, K. L.
name: Turner, A. H.
name: Wu, E. Y. S.
name: Zemcov, M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present measurements of the cosmic microwave background (CMB) radiation temperature anisotropy in the multipole range 2000
description: 5 pages, 5 figures, updated beam model, full data release available online (see text), accepted to ApJL
Cuscuton and low energy limit of Horava-Lifshitz gravity
Creators: name: Afshordi, Niayesh
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: A proposal for a power-counting renormalizable theory of quantum gravity at a Lifshitz point was recently put forth by Horava (arXiv:0901.3775), and has been since dubbed as Horava-Lifshitz gravity. The theory explicitly breaks Lorentz invariance, which introduces an apparent extra scalar degree of freedom. In this note, we show that the low energy limit of (non-projectible) Horava-Lifshitz gravity is uniquely given by the quadratic cuscuton model: a covariant scalar field theory with an infinite speed of sound and a quadratic potential, which is minimally coupled to Einstein gravity. This implies that the extra scalar is non-dynamical to all orders in perturbation theory. Using current cosmological constraints on the quadratic cuscuton model, we can constrain the low energy Lorentz breaking parameter of Horava-Lifshitz theory (which leads to a running of Planck mass on the Hubble scale) to |lambda-1| < 0.014 (at 95% confidence level). We also point out that, with reasonable boundary conditions, the spatial hypersurfaces in this theory are constant mean curvature (CMC) or uniform expansion surfaces at low energies, and introduce geometrical symmetries that can protect the non-dynamical nature of these theories from quantum corrections. We also notice that the theory with lambda < 1 might suffer from a non-perturbative UV instability.
description: 5 pages, 1 figure, added references, submitted to PRD
Cluster properties and particle production in Poincaré invariant quantum mechanics
Creators: name: Polyzou, W. N.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Mathematical Physics (math-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: I outline the construction of exactly Poincaré invariant quantum models that satisfy cluster separability but do not conserve particle number.
description: 9 Pages, contribution to 19^th International IUPAP Conference on Few-Body Problems in Physics
About the strength of correlation effects in the electronic structure of iron
Creators: name: Sanchez-Barriga, J.
name: Fink, J.
name: Boni, V.
name: Di Marco, I.
name: Braun, J.
name: Minar, J.
name: Varykhalov, A.
name: Rader, O.
name: Bellini, V.
name: Manghi, F.
name: Ebert, H.
name: Katsnelson, M. I.
name: Lichtenstein, A. I.
name: Eriksson, O.
name: Eberhardt, W.
name: Duerr, H. A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Other Condensed Matter (cond-mat.other)
subject: FOS: Physical sciences

description: The strength of electronic correlation effects in the spin-dependent electronic structure of ferromagnetic bcc Fe(110) has been investigated by means of spin and angle-resolved photoemission spectroscopy. The experimental results are compared to theoretical calculations within the three-body scattering approximation and within the dynamical mean-field theory, together with one-step model calculations of the photoemission process. This comparison indicates that the present state of the art many-body calculations, although improving the description of correlation effects in Fe, give too small mass renormalizations and scattering rates thus demanding more refined many-body theories including non-local fluctuations.
description: 4 pages, 4 figures
Child-oral health literacy of primary health care professionals in Australia: A scoping review protocol
Creators: name: Andrew, Lesley
Publisher: name: Open Science Framework
Year: 2023
Subjects: subject: Medicine and Health Sciences
subject: Social and Behavioral Sciences
subject: Education

description: Early childhood cavities (ECCs) are a major cause of hospital admissions and chronic disease for Australian children. ECCs cause pain, feeding and speech problems for the child, and financial and emotional distress for the family. ECC prevalence can be reduced by improving primary caregiver child-oral health literacy. Primary health care professionals play a key role in enhancing this literacy. The measurement of primary health care professionals’ child-oral health literacy levels is warranted to ascertain requirements for further education. This measurement requires the selection of an instrument appropriate to the target context and population and to child oral health.
Analysis of variance, coefficient of determination and $F$-test for local polynomial regression
Creators: name: Huang, Li-Shan
name: Chen, Jianwei
Publisher: name: arXiv
Year: 2008
Subjects: subject: Statistics Theory (math.ST)
subject: FOS: Mathematics
subject: 62G08 (Primary) 62J10 (Secondary)

description: This paper provides ANOVA inference for nonparametric local polynomial regression (LPR) in analogy with ANOVA tools for the classical linear regression model. A surprisingly simple and exact local ANOVA decomposition is established, and a local R-squared quantity is defined to measure the proportion of local variation explained by fitting LPR. A global ANOVA decomposition is obtained by integrating local counterparts, and a global R-squared and a symmetric projection matrix are defined. We show that the proposed projection matrix is asymptotically idempotent and asymptotically orthogonal to its complement, naturally leading to an $F$-test for testing for no effect. A by-product result is that the asymptotic bias of the ``projected'' response based on local linear regression is of quartic order of the bandwidth. Numerical results illustrate the behaviors of the proposed R-squared and $F$-test. The ANOVA methodology is also extended to varying coefficient models.
description: Published in at http://dx.doi.org/10.1214/07-AOS531 the Annals of Statistics (http://www.imstat.org/aos/) by the Institute of Mathematical Statistics (http://www.imstat.org)
Clinical spectrum of Type 2 Familial Partial Lipodystrophy
Creators: name: Cobelo-Gómez, Silvia
name: Prado-Moraña, Teresa
name: Díaz-López, Everardo Josué
name: Castro, Ana I.
name: Araujo-Vilar, David
name: Sánchez-Iglesias, Sofía
name: Antía Fernández-Pombo
Publisher: name: Open Science Framework
Year: 2023
Subjects: subject: Medicine and Health Sciences
subject: Medical Specialties
subject: Endocrinology, Diabetes, and Metabolism
subject: Laminopathies
subject: LMNA
subject: Lipodystrophy
subject: Dyslipidemia
subject: Diabetes
subject: Insulin resistance
subject: Adipose tissue

description: Hypothesis To explore the published data regarding the clinical characterisation of type 2 Familial Partial Lipodystrophy. Design Plan Study type A systematic review of published studies. Blinding No blinding is involved in this study. Is there any additional blinding in this study? None Study design To show the current knowledge about the clinical characteristics, organ abnormalities and associated comorbidities of FPLD2, a systematic review based on the Preferred Reporting Items for Systematic Reviews and Meta-Analyses (PRISMA) protocol was conducted. For this purpose, a search on PubMed was performed using the terms “Dunnigan” OR “familial partial lipodystrophy” OR “FPLD”. The database was searched up to December 2022, without a time limitation and without language restrictions. To identify additional studies and expand our search, the references of the retrieved articles were also screened. A total of 788 articles were identified through this database search. Studies that report clinical and/or biochemical data on patients with FPLD2 were eligible for inclusion in the current review. The main exclusion criteria were a) articles not fulfilling the topic of interest of this review; b) review articles, meta-analyses, individual case reports, editorials or comments; and c) studies not conducted on humans. Two authors independently reviewed the abstracts of the retrieved articles, applying the previously-mentioned inclusion and exclusion criteria and, subsequently reviewed the full text of the studies to determine their final inclusion. 2.3. Identification and inclusion of studies From the 788 articles initially found, 454 were excluded taking into account that they did not fulfil the topic of interest of this review, two were excluded because they were published errata and 66 were excluded because they were focused on other FPLD subtypes or laminopathies other than Dunnigan disease. During the screening and eligibility processes, 79 review articles or meta-analyses, 71 individual case reports, eight letters to the editor and one comment were also excluded. In addition, a total of 6 studies were finally included after the screening of the references of the initial pool of retrieved articles. Thus, finally, 113 articles were included in the current review.
Diverging UV and Halpha fluxes of star forming galaxies predicted by the IGIMF theory
Creators: name: Pflamm-Altenburg, J.
name: Weidner, C.
name: Kroupa, P.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Although the stellar initial mass function (IMF) has only been directly determined in star clusters it has been manifoldly applied on galaxy-wide scales. But taking the clustered nature of star formation into account the galaxy-wide IMF is constructed by adding all IMFs of all young star clusters leading to an integrated galactic initial mass function (IGIMF). The IGIMF is top-light compared to the canonical IMF in star clusters and steepens with decreasing total star formation rate (SFR). This discrepancy is marginal for large disk galaxies but becomes significant for SMC-type galaxies and less massive ones. We here construct IGIMF-based relations between the total FUV and NUV luminosities of galaxies and the underlying SFR. We make the prediction that the Halpha luminosity of star forming dwarf galaxies decreases faster with decreasing SFR than the UV luminosity. This turn-down of the Halpha-UV flux ratio should be evident below total SFRs of 10^-2 M_sun/yr.
description: accepted by MNRAS
Labour Market Discrimination in the Gig Economy: A Field Experiment in Australia
Creators: name: Von Hippel, Bill
name: Albrecht, Sabina
name: Smerdon, David
name: Pearson, Sam
Publisher: name: Open Science Framework
Year: 2023
Subjects: subject: Psychology
subject: FOS: Psychology
subject: Economics
subject: Social and Behavioral Sciences

description: There is a long history in psychology and economics of measuring employment discrimination by sending people of different ethnicity, religion, etc., to apply for jobs with identical CVs. The researchers then see who gets a call-back on their application to assess whether some groups are the target of discrimination. With the advent of the modern ‘gig economy’, we now have the opportunity to see whether discrimination also runs the other way, and whether people would be less likely to work for someone of a different ethnic group, religion, etc. This project involves designing, running, and analysing a large online field experiment to investigate labour market discrimination in the ‘gig economy’. Students will post job advertisements on an online task-outsourcing platform. By manipulating the user profile and the job advertisement, we will examine discrimination by gig-economy employees across two dimensions: sexual orientation and gender. Additionally, the type of job will be varied by the degree of interpersonal contact of the work (e.g., whether or not the task can be performed remotely vs. in the home). Students will also have the opportunity to feed into the design of the experiment. The goal of the study is to assess whether people discriminate against potential employers as a function of their gender and sexual orientation, and whether they do so in their willingness to work for them and/or potentially charging them more. Additionally, and importantly, we will also be able to assess whether such discrimination differs as a function of whether the job requires personal contact.
Access Delay Constrained Activity Detection in Massive Random Access
Creators: name: Robin, Jyotish
name: Erkip, Elza
Publisher: name: arXiv
Year: 2021
Subjects: subject: Signal Processing (eess.SP)
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: In 5G and future generation wireless systems, massive IoT networks with bursty traffic are expected to co-exist with cellular systems to serve several latency-critical applications. Thus, it is important for the access points to identify the active devices promptly with minimal resource consumption to enable massive machine-type communication without disrupting the conventional traffic. In this paper, a frequency-multiplexed strategy based on group testing is proposed for activity detection which can take into account the constraints on network latency while minimizing the overall resource utilization. The core idea is that during each time-slot of active device discovery, multiple subcarriers in frequency domain can be used to launch group tests in parallel to reduce delay. Our proposed scheme is functional in the asymptotic and non-asymptotic regime of the total number of devices $(n)$ and the number of concurrently active devices $(k)$. We prove that, asymptotically, when the number of available time-slots scale as $Ω\big(\log (\frac{n}{k})\big)$, the frequency-multiplexed group testing strategy requires $O\big(k\log (\frac{n}{k})\big)$ time-frequency resources which is order-optimal and results in an $O(k)$ reduction in the number of time-slots with respect to the optimal strategy of fully-adaptive generalized binary splitting. Furthermore, we establish that the frequency-multiplexed GT strategy shows significant tolerance to estimation errors in $k$. Comparison with 3GPP standardized random access protocol for NB-IoT indicates the superiority of our proposed strategy in terms of access delay and overall resource utilization.
description: 5 pages, 4 figures
title: Mesotelioma Pleural Maligno: Características radiológicas, diagnóstico diferencial y estadificación radiológica.
Creators: name: Lorenzo Górriz, Antonio
Publisher: name: Sociedad Española de Radiología Médica
Year: 2014
Subjects: subject: Staging
subject: Oncology
subject: Thorax
subject: Lung
subject: Conventional radiography
subject: CT

description: Objetivo docente
Revisión del tema
Conclusiones
Bibliografía
description: Objetivo docente:
Analizar las características radiológicas y semiológicas típicas del Mesotelioma Pleural Maligno (MPM) así como las de otras entidades que pueden mimetizar esta entidad,
y repasar la estadificación radiológica de la...
Matter in Loop Quantum Gravity without time gauge: a non-minimally coupled scalar field
Creators: name: Cianfrani, F.
name: Montani, G.
Publisher: name: arXiv
Year: 2009
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We analyze the phase space of gravity non-minimally coupled to a scalar field in a generic local Lorentz frame. We reduce the set of constraints to a first-class one by fixing a specific hypersurfaces in the phase space. The main issue of our analysis is to extend the features of the vacuum case to the presence of scalar matter by recovering the emergence of an SU(2) gauge structure and the non-dynamical role of boost variables. Within this scheme, the super-momentum and the super-Hamiltonian are those ones associated with a scalar field minimally coupled to the metric in the Einstein frame. Hence, the kinematical Hilbert space is defined as in canonical Loop Quantum Gravity with a scalar field, but the differences in the area spectrum are outlined to be the same as in the time-gauge approach.
description: 6 pages