cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Pyrochlore-group minerals from the Loe-Shilman Carbonatite Complex, NW Pakistan: implications for evolution of carbonatite system
Creators: name: Khan, Asad
name: Faisal, Shah
name: Ullah, Zaheen
name: Ali, Liaqat
name: Ghaffari, Abuzar
name: Nawab, Javed
name: Rashid, Mehboob Ur
Publisher: name: Periodico di Mineralogia
Year: 2021

description: This study reports new occurrence of niobium mineralization from the Loe-Shilman carbonatite complex, NW Pakistan. The complex is predominantly comprised of calcite carbonatite, intruded by dolomite carbonatite, and minor late-stage carbonatite veins, intruding the earlier two varieties. Pyrochlore group minerals, which are the major Nb phases in the carbonatites and overlying supergene laterite, manifest numerous textural and compositional discrepancies. Pyrochlores observed in calcite and dolomite carbonatites of the complex are typified by oscillatory zoning, and are compositionally Ca-Na-pyrochlore, and therefore, illustrating crystallization under primary magmatic conditions. However, relatively Ta poor (2.42-5.11 wt%) and Nb rich (60.04-62.14 wt%) pyrochlores preserved in dolomite carbonatite are reflecting a more evolved nature of the dolomite carbonatite compared to Ta rich (6.89-10.11 wt%) pyrochlore of the calcite carbonatite. In addition, pyrochlores of the late-stage carbonatite veins record patchy zonation and are characterized by A-site vacancies, likely due to leaching of Na and Ca, and enrichment of Ba-REE-Sr during hydrothermal alteration by a relatively low pH, Na and/or Si poor fluids. Similarly, intensively patchy zoned, porous and Fe3+ bearing A-site deficient bariopyrochlore in supergene laterite are produced by complete leaching of Ca and Na from A-site, and by partial replacement of strongly-bounded Nb at B-site by Fe3+ during supergene conditions.
description: Periodico di Mineralogia, Vol. 90 No. 2 (2021): In progress
The environmental factors affecting the archaeological buildings in Egypt, "II Deterioration by severe human activities"
Creators: name: El-Gohary, Mohamed A.
name: Abdel Moneim, Ahmed A.
Publisher: name: Periodico di Mineralogia
Year: 2021

description: This paper is the second in a series that addresses the environmental factors affecting the archaeological buildings in Egypt. It presents the results of scientific studies and examinations carried out on one of the most severe deterioration factors affecting the monumental buildings in a crowded and populated environment (Esna Temple). This temple was built during the reign of Ptolemy V (205-180 BC) to memorialize the god Khnum “the holy local god” using Nubian sandstone. In order to understand the effects of a populated environment on this material, samples of sandstone from the temple were examined using some analytical techniques, i.e., XRF, XRD, AAS, PL, and SEM. The results revealed that the temple’s constituents include quartz as an essential component of sandstone, whereas the resulting weathering products are halite, anhydrite, niter, sylvite, and kaolinite. They resulted from numerous deterioration factors and relevant mechanisms because of human activities, including aggressive effects of ground and domestic wastewater, as well as deliberate and undeliberate damage. Moreover, vandalism, theft, looting, improper conservation, and other extrinsic and intrinsic factors, especially the alternative cycles between drying and wetting play a role in deterioration.
description: Periodico di Mineralogia, Vol. 90 No. 2 (2021): In progress
Measurability of Wilson loop operators
Creators: name: Beckman, David
name: Gottesman, Daniel
name: Kitaev, Alexei
name: Preskill, John
Publisher: name: arXiv
Year: 2001
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Lattice (hep-lat)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We show that the nondemolition measurement of a spacelike Wilson loop operator W(C) is impossible in a relativistic non-Abelian gauge theory. In particular, if two spacelike-separated magnetic flux tubes both link with the loop C, then a nondemolition measurement of W(C) would cause electric charge to be transferred from one flux tube to the other, a violation of relativistic causality. A destructive measurement of W(C) is possible in a non-Abelian gauge theory with suitable matter content. In an Abelian gauge theory, many cooperating parties distributed along the loop C can perform a nondemolition measurement of the Wilson loop operator if they are equipped with a shared entangled ancilla that has been prepared in advance. We also note that Abelian electric charge (but not non-Abelian charge) can be transported superluminally, without any accompanying transmission of information.
description: 17 pages, 7 figures, REVTeX
Jejunalsonden bei Kindern und Jugendlichen
Creators: name: Broekaert, Ilse
name: Bildheim, Victor
name: Brunert, Annette
name: Hauer, Almuthe
name: Schwarz, Christine
name: Schmidt-Choudhury, Anjona
Publisher: name: Universität Ulm
Year: 2020
Subjects: subject: Ernährung
subject: Ernährungssonde
subject: Gastroösophagealer Reflux
subject: Handlungsempfehlung
subject: Multidisziplinäres Team
subject: Clinical guide
subject: Feeding tube
subject: Gastroesophageal reflux
subject: Multidisciplinary team
subject: Nutrition
subject: DDC 610 / Medicine & health

description: Zusammenfassung Die Ernährung über eine jejunale Sonde wird immer häufiger bei jenen Kindern notwendig, deren kalorischer Bedarf durch gastrale Ernährung nicht ausreichend gedeckt werden kann. Ursächlich hierfür können die Intoleranz gastral zugeführter Nahrung oder eine ausgeprägte gastroösophageale Refluxkrankheit (GÖRK) sein. Da nach Anlage der Jejunalsonde häufig regelmäßige Sondenwechsel notwendig werden, ist eine jejunale Sonde oft nur eine vorübergehende Lösung bis zur perkutanen Anlage eines Jejunostomas (mit oder ohne Antirefluxoperation) oder als Alternative vor einer etwaigen Antirefluxoperation. Bevor eine jejunale Sonde gelegt wird, sollte eine Nahrungsintoleranz aufgrund anatomischer oder nicht gastrointestinal bedingter Probleme ausgeschlossen werden. Die Versorgung eines Kindes, bei dem die Anlage einer jejunalen Sonde geplant ist, sollte durch ein multidisziplinäres Team, bestehend aus u. a. einem Kindergastroenterologen/einer Kindergastroenterologin, einer Ernährungsfachkraft, einem Psychologen/einer Psychologin und einem Logopäden/einer Logopädin, erfolgen. Das multidisziplinäre Team sollte bereits vor Indikationsstellung die Nahrung anpassen, das Kind logopädisch evaluiert haben und die Familie psychologisch und medizinisch mitbetreuen. Eine adäquate Planung, welche auch ethische Aspekte beinhaltet, garantiert, dass sowohl der Patient/die Patientin, die Eltern und Betreuungspersonen wie auch das behandelnde Team ein klares Verständnis der Indikation und Gründe für die Anlage einer jejunalen Sonde haben. Dabei sollten auch die Fortsetzung einer möglichen oralen Ernährung und eine Sondenentwöhnung diskutiert werden. Diese Übersicht beinhaltet Handlungsempfehlungen zur Indikationsstellung für den Einsatz jejunaler Sonden, gepaart mit praktischen Überlegungen, welche die Verwendung und die Sicherheit der jejunalen Sondenernährung im Kindes- und Jugendalter optimieren sollen. /
Desarrollo y situación actual de la agricultura ecológica: elementos de análisis para entender el caso español
Creators: name: MIELGO, ANTONIO M. ALONSO
name: MIELGO, ANTONIO M. ALONSO
Publisher: name: Unknown
Year: 2001
Subjects: subject: Community/Rural/Urban Development
subject: Crop Production/Industries
subject: Farm Management
subject: International Relations/Trade
subject: Agricultura ecológica
subject: medidas agroambientales
subject: desarrollo rural
subject: desarrollo sostenible
subject: Organic farming
subject: agri-environmental measures
subject: rural development
subject: sustainable development

description: La agricultura ecológica es practicada actualmente en la mayoría de los países del mundo, constituyendo una alternativa a la agricultura convencional. El desarrollo de este sector en los países de la UE, donde se concentran más de 3,6 millones de hectáreas en alrededor de 130.000 explotaciones en la actualidad, ha sido notable. El principal objetivo de este artículo es determinar los factores que influyen en el desarrollo de la agricultura ecológica. El apoyo normativo y económico ha sido un factor importante en muchos países de la UE. Este soporte ha sido bajo en España, siendo el mercado de exportación el principal motor del desarrollo de la agricultura ecológica. Sin embasrgo, este mercado es actualmente inestable, debido a que varios países, que apoyan a su sector ecológico, compiten ventajosamente con la producción ecológica española en los principales mercados del centro y norte de Europa. Por ello, se hace necesario el establecimiento de planes integrales de apoyo en España a este sector, que se ha convertido en los últimos años en una de las principales actividades impulsoras del desarrollo rural sostenible, Organic farming are practised nowadays in the most of the countries in the world, constituting an alternative to the conventional farming. The development of this sector in the EU countries, where more than 3,6 million hectares are concentrated actually in around 130.000 farms, has been notorious. The main objective of this article is to determine the factors which have influence on the organic farming development. Normative and economical institutional support has been a very important factor in many EU countries. This support has been low in Spain, being the export market the main historical driving force of the organic farming development. However, the export market is not actually very stable, because there are several countries, which give institutional support to the organic sector, competing with Spain in the main markets of central and northern European countries. By this, it’s necessary to established integral planes in Spain to promote this sector, which have converted in the last years in one of the main driving force of sustainable rural development.
On choosing and bounding probability metrics
Creators: name: Gibbs, Alison L.
name: Su, Francis Edward
Publisher: name: arXiv
Year: 2002
Subjects: subject: Probability (math.PR)
subject: FOS: Mathematics
subject: 60B10

description: When studying convergence of measures, an important issue is the choice of probability metric. In this review, we provide a summary and some new results concerning bounds among ten important probability metrics/distances that are used by statisticians and probabilists. We focus on these metrics because they are either well-known, commonly used, or admit practical bounding techniques. We summarize these relationships in a handy reference diagram, and also give examples to show how rates of convergence can depend on the metric chosen.
description: To appear, International Statistical Review. Related work at http://www.math.hmc.edu/~su/papers.html
Echo Tomography of Black Hole Accretion Flows
Creators: name: Horne, Keith
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We discuss technologies for micro-arcsec echo mapping of black hole accretion flows in Active Galactic Nuclei (AGN). Echo mapping employs time delays, Doppler shifts, and photoionisation physics to map the geometry, kinematics, and physical conditions in the reprocessing region close to a compact time-variable source of ionizing radiation. Time delay maps are derived from detailed analysis of variations in lightcurves at different wavelengths. Echo mapping is a maturing technology at a stage of development similar to that of radio interferometry just before the VLA. The first important results are in, confirming the basic assumptions of the method, measuring the sizes of AGN emission line regions, delivering dozens of black hole masses, and showing the promise of the technique. Resolution limits with existing AGN monitoring datasets are typically ~5-10 light days. This should improve down to 1-2 light days in the next-generation echo mapping experiments, using facilities like Kronos and Robonet that are designed for and dedicated to sustained spectroscopic monitoring. A light day is 0.4 micro-arcsec at redshift 0.1, thus echo mapping probes regions 10^3 times smaller than VLBI, and 10^5 times smaller than HST.
description: To appear in: Astronomical Telescopes and Instrumentation, Future EUV, UV, and Visible Space Astrophysics Missions and Instrumentation, 22-28 Aug 2002, Waikoloa, HI, SPIE Proc 4856
Relations between phenomenological and physical parameters in the hot coronae of AGNs computed with the MoCA code
Creators: name: Middei, R.
name: Bianchi, S.
name: Marinucci, A.
name: Matt, G.
name: Petrucci, P. -O.
name: Tamborra, F.
name: Tortosa, A.
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The primary X-ray emission in active galactic nuclei (AGNs) is widely believed to be due to Comptonisation of the thermal radiation from the accretion disc in a corona of hot electrons. The resulting spectra can, in first approximation, be modelled with a cut-off power law, the photon index and the high-energy roll-over encoding information on the physical properties of the X-ray-emitting region. The photon index and the high-energy curvature of AGNs ($Γ$, E$_c$) have been largely studied since the launch of X-ray satellites operating above 10 keV. However, high-precision measurements of these two observables have only been obtained in recent years thanks to the unprecedented sensitivity of NuSTAR up to 79 keV. We aim at deriving relations between phenomenological parameters ($Γ$ and E$_c$) and the intrinsic properties of the X-ray-emitting region (the hot corona), namely the optical depth and temperature. We use MoCA (Monte Carlo code for Comptonisation in Astrophysics) to produce synthetic spectra for the case of an AGN with M$_{BH}$=1.5$\times$10$^8$ M$_{sun}$ and accretion rate of 10% and then compared them with the widely used power-law model with an exponential high-energy cutoff. We provide phenomenological relations relating $Γ$ and E$_c$ with the opacity and temperature of the coronal electrons for the case of spherical and slab-like coronae. These relations give origin to a well defined parameter space which fully contains the observed values. Exploiting the increasing number of high-energy cut-offs quoted in the literature, we report on the comparison of physical quantities obtained using MoCA with those estimated using commonly adopted spectral Comptonisation models. Finally, we discuss the negligible impact of different black hole masses and accretion rates on the inferred relations.
description: Accepted for publication in A&A, 10 pages, 9 figures
Additional file 1 of External application of liver compresses to reduce fatigue in patients with metastatic cancer undergoing radiation therapy, a randomized clinical trial
Creators: name: Pirus Ghadjar
name: Stritter, Wiebke
name: Von Mackensen, Irina
name: Mehrhof, Felix
name: Foucré, Clara
name: Ehrhardt, Vincent H.
name: Beck, Marcus
name: Pimrapat Gebert
name: Kalinauskaite, Goda
name: Luchte, Jacqueline S.
name: Stromberger, Carmen
name: Budach, Volker
name: Eggert, Angelika
name: Seifert, Georg
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Physiology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Cancer

description: Additional file 1. Figure 4: Line plot showing mean changes from baseline (t0) at one week (t1) and at end of treatment (t2) for all MFI-20 subscales after adjustments for different baseline values.
Effect of Binary Basicity (CaO/SiO2) on Selective Reduction of Lateritic Nickel Ore
Creators: name: Nurjaman, Fajar
name: Saekhan, Khulud
name: Bahfie, Fathan
name: Astuti, Widi
name: Suharno, Bambang
Publisher: name: Periodico di Mineralogia
Year: 2021

description: Selective reduction methods are being developed to process lateritic nickel ore to produce nickel with high content with low temperature or energy consumption. This research was carried out to study the effect of binary basicity (CaO/SiO2) in the lateritic nickel ore's selective reduction process. The lateritic nickel ore with 1.38% Ni and 38.2% Fe content was used in this study. The reduction was conducted at 1150°C for 60 minutes in a muffle furnace with 10 wt.% additives of sodium sulfate, bituminous coal as reductant, and calcium oxide addition to modify its binary basicity. The results showed that the nickel grades generates from the 0,1 basicity due to the breakage of magnesium, iron, and nickel silicate into metallic iron and nickel. However, the next increase of basicities decreased the nickel grade due to the formation of a high melting point compound. lateritic nickel ore, selective reduction, binary basicity, reductant, additive.
description: Periodico di Mineralogia, Vol. 90 No. 2 (2021): In progress
Calamine of the Bergamasque Alps as a possible source of zinc for Roman brass: Theoretical considerations and preliminary results
Creators: name: Merkel, Stephen William
Publisher: name: Periodico di Mineralogia
Year: 2021

description: The origins of brass are obscure and begin long before the Romans, however, it was the Romans who brought this gold-coloured alloy of copper and zinc from obscurity and placed it at the forefront of monetary policy and military power. Under the Romans, brass was produced on a scale never seen before, but until now there is little clarity on where brass was made and where they obtained zinc ore. Studies in the past focused on potential sources in Germany, but the lack of investigation on Italian sources represents a significant research gap. The major zinc source in Northern Italy (Gorno Pb-Zn district) could be the source mentioned by Pliny the Elder and may have played a major role in the Roman brass industry. Recent surveys around the area of Dossena, in the Gorno Pb-Zn district, have brought to light substantial traces of pre-modern calamine mining of unknown age. This study presents results from the mineralogical and geochemical characterisation of calamine ore from the Dossena area. A theoretical discussion on the sourcing of Roman brass through chemical and lead isotope analysis is provided along with a case study comparing analyses of brass with zinc ore sources. While the currently available lead isotope dataset on brass alloys is not ideal for exploring this issue, the lead isotope analyses confirm that the calamine from Dossena could have been used by the Romans for brass making and suggestions for future research are provided.
description: Periodico di Mineralogia, Vol. 90 No. 2 (2021): In progress
Dynamics of the Batch Minority Game with Inhomogeneous Decision Noise
Creators: name: Coolen, A. C. C.
name: Heimel, J. A. F.
name: Sherrington, D.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Trading and Market Microstructure (q-fin.TR)
subject: FOS: Physical sciences
subject: FOS: Economics and business

description: We study the dynamics of a version of the batch minority game, with random external information and with different types of inhomogeneous decision noise (additive and multiplicative), using generating functional techniques à la De Dominicis. The control parameters in this model are the ratio $α=p/N$ of the number $p$ of possible values for the external information over the number $N$ of trading agents, and the statistical properties of the agents' decision noise parameters. The presence of decision noise is found to have the general effect of damping macroscopic oscillations, which explains why in certain parameter regions it can effectively reduce the market volatility, as observed in earlier studies. In the limit $N\to\infty$ we (i) solve the first few time steps of the dynamics (for any $α$), (ii) calculate the location $α_c$ of the phase transition (signaling the onset of anomalous response), and (iii) solve the statics for $α>α_c$. We find that $α_c$ is not sensitive to additive decision noise, but we arrive at non-trivial phase diagrams in the case of multiplicative noise. Our theoretical results find excellent confirmation in numerical simulations.
description: 14 pages LaTeX, 8 postscript figures, in PRE style (minor textual changes in revision)
Reply to Deevsalar and Shinjo (2020) comments on "Petrogenesis of gabbroic rocks from the Malayer plutonic complex, Sanandaj-Sirjan zone, west Iran)" (Esna-Ashari and Tiepolo, PERIODICO di MINERALOGIA (89) 91-104, 2020)
Creators: name: Esna-Ashari, Amir
Publisher: name: Periodico di Mineralogia
Year: 2021

description: No abstract
description: Periodico di Mineralogia, Vol. 90 No. 2 (2021): In progress
Additional file 1 of A cohort study of membranous nephropathy, primary or secondary
Creators: name: Arghiani, Maryam
name: Boshra Hasan Zamani
name: Nazemian, Fatemeh
name: Samadi, Sara
name: Malihe Saber Afsharian
name: Habibzadeh, Mahmoud
name: Saeid Eslami
name: Sabbagh, Mahin Ghorban
Publisher: name: figshare
Year: 2021
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Marine Biology
subject: Cancer
subject: 60506 Virology

description: Additional file 1: Table S1. Data from 24-hour urine protein and serum creatinine showed no significant difference between primary and secondary MN.
El comportamiento del consumidor y la demanda de aceites vegetales en España: oliva virgen versus oliva/girasol
Creators: name: ROSA, MANUEL PARRAS
name: ROSA, MANUEL PARRAS
Publisher: name: Unknown
Year: 2001
Subjects: subject: Consumer/Household Economics
subject: Crop Production/Industries
subject: Institutional and Behavioral Economics
subject: Aceites de oliva
subject: aceite de oliva virgen
subject: comportamiento del consumidor
subject: demanda
subject: olive oils
subject: virgin olive oil
subject: consumer behavior
subject: demand

description: En este trabajo nos proponemos evaluar las posibilidades de incremento de la demanda de aceite de oliva virgen en el mercado español. Para ello, analizamos tanto la situación y evolución de la demanda de este producto en el marco del conjunto de los aceites vegetales comestibles como el comportamiento de compra de los consumidores españoles. Los datos en los que nos apoyamos para conseguir el primero de los objetivos proceden de estimaciones propias, obtenidas mediante un modelo a partir de estadísticas oficiales, considerando las grandes diferencias en los datos que las mismas ofrecen. Respecto del comportamiento del consumidor, la información procede de una investigación propia. Los análisis efectuados apuntan a que es factible incrementar el consumo de aceite de oliva virgen en el mercado español, para lo que es preciso implantar estrategias de diferenciación y posicionamiento, destinadas a segmentos de mercado específicos que localizamos en este trabajo, In this paper we aim to evaluate the possibilities of increasing virgin olive oil demand in the Spanish market. To that end, we analyze both the situation and evolution of the demand of this product in the framework of the edible vegetable oils group, and the buying behavior of Spanish consumers. The data on which we base to achieve the former goal come from our own estimates, obtained witf a model established from official statistics, considering the large differences in the data that they offer. As for the consumer behavior, the information comes from our own research. The carried out analysis point out that it is feasible to increase virgin olive oil consumption in the Spanish market, which requires the introduction of differentiation and positioning strategies, intended for specific market segments which we locate in this paper.
ALMA observations of fragmentation, sub-structure, and protostars in high-mass starless clump candidates
Creators: name: Svoboda, Brian E.
name: Shirley, Yancy L.
name: Traficante, Alessio
name: Battersby, Cara
name: Fuller, Gary A.
name: Zhang, Qizhou
name: Beuther, Henrik
name: Peretto, Nicolas
name: Brogan, Crystal
name: Hunter, Todd
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: (Abridged) The initial physical conditions of high-mass stars and protoclusters remain poorly characterized. To this end we present the first targeted ALMA 1.3mm continuum and spectral line survey towards high-mass starless clump candidates, selecting a sample of 12 of the most massive candidates ($400-4000\, M_\odot$) within 5 kpc. The joint 12+7m array maps have a high spatial resolution of $\sim 3000\, \mathrm{au}$ ($\sim 0.8^{\prime\prime}$) and have point source mass-completeness down to $\sim 0.3\, M_\odot$ at $6σ$ (or $1σ$ column density sensitivity of $1.1\times10^{22}\, \mathrm{cm^{-2}}$). We discover previously undetected signposts of low-luminosity star formation from CO (2-1) and SiO (5-4) bipolar outflows and other signatures towards 11 out of 12 clumps, showing that current MIR/FIR Galactic Plane surveys are incomplete to low- and intermediate-mass protostars ($\lesssim 50\, L_\odot$). We compare a subset of the observed cores with a suite of radiative transfer models of starless cores. We find a high-mass starless core candidate with a model-derived mass consistent with $29^{52}_{15}\, M_\odot$ when integrated over size scales of $2\times10^4\, \mathrm{au}$. Unresolved cores are poorly fit by starless core models, supporting the interpretation that they are protostellar even without detection of outflows. Substantial fragmentation is observed towards 10 out of 12 clumps. We extract sources from the maps using a dendrogram to study the characteristic fragmentation length scale. Nearest neighbor separations when corrected for projection are consistent with being equal to the clump average thermal Jeans length. Our findings support a hierarchical fragmentation process, where the highest density regions are not strongly supported against thermal gravitational fragmentation by turbulence or magnetic fields.
description: 32 pages, 17 figures, and 6 tables. Accepted for publication in ApJ (August 26, 2019)
MOESM2 of Expanding CAR T cells in human platelet lysate renders T cells with in vivo longevity
Creators: name: Chavez, Alejandro Torres
name: McKenna, Mary
name: Canestrari, Emanuele
name: Dann, Christina
name: Ramos, Carlos
name: Premal Lulla
name: Leen, Ann
name: Vera, Juan
name: Watanabe, Norihiro
Publisher: name: figshare
Year: 2019
Subjects: subject: Biophysics
subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Molecular Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Hematology
subject: Computational Biology

description: Additional file 2: Figure S1. Characteristics of CAR T cells maintained in different sera, Figure S2. Effect of lower dose of serum supplement on P28z T cell expansion and phenotype, Figure S3. CD107a expression in T cell subsets, Figure S4. Tumor status at the time of euthanasia, Figure S5. In vivo performance of CCR7KO P28z T cell expanded in HPL, Figure S6. In vivo performance of 1928z T cell expanded in different sera, Figure S7. Effect of TGFÎ²1 on T cell phenotype and in vitro / in vivo T cell function.
Análisis temporal de las ventas y estimación del valor residual de tractores en España
Creators: name: Martin, Pedro Arias
name: Martin, Pedro Arias
Publisher: name: Unknown
Year: 2001
Subjects: subject: Institutional and Behavioral Economics
subject: International Relations/Trade
subject: Research Methods/ Statistical Methods
subject: Serie temporal
subject: análisis de regresión
subject: maquinaria agrícola
subject: Time series
subject: regression analysis
subject: agricultural machinery

description: Los objetivos de este trabajo se han centrado en analizar el modelo de demanda de tractores en España, a través del número de inscripciones y estudiar su valor residual y depreciación en función de la antigüedad, del precio de venta de tractores de segunda mano y del nivel de potencia. Para ello, se realiza un análisis univariante de la serie temporal de inscripciones mensuales por medio de los modelos ARIMA y a través de los modelos de regresión se aborda el modelo de comportamiento del valor residual.......In this work two objectives are considered, to analyze the behaviour tractors´market throught the estimation model that the inscriptions follow in Spain and to study the remaining value and the depreciation with market’s price, age and level of power. Throught models ARIMA is studied the time serie of inscriptions and with regression models its remaining value.
Additional file 1 of Profiling SARS-CoV-2 mutation fingerprints that range from the viral pangenome to individual infection quasispecies
Creators: name: Lau, Billy T.
name: Pavlichin, Dmitri
name: Hooker, Anna C.
name: Almeda, Alison
name: Giwon Shin
name: Jiamin Chen
name: Sahoo, Malaya K.
name: Huang, Chun Hong
name: Pinsky, Benjamin A.
name: Lee, Ho Joon
name: Ji, Hanlee P.
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1:. Figure S1. Metadata k-mer indexing for mutations. Table S1. Genome assemblies included pangenome k-mer study. Table S2. K-mer filter criteria for primer design and selection. Table S3. Accession numbers of genomes included in in silico cross-reactivity analyses. Table S4. Multiplexed PCR primers used for amplicon generation and subsequent Illumina sequencing. Table S5. Concentrations of serially diluted contrived SARS-CoV-2 samples used for analytical sensitivity and specificity testing. Table S6. Strain-specific relative fractions of admixed SARS-CoV-2 contrived samples used for validaton of k-mer based analysis. Table S7. Strain-specific mutations detected from admixed SARS-CoV-2 contrived samples. Table S8. Cycle threshold (CT) values of externally tested clinical SARS-CoV-2 samples used for sequencing. Table S9. Expected translational changes from nonsynonymous mutations in orf7a and orf8 from clinical samples.
MOESM3 of Primary healthcare and school health service utilisation by adolescents and young adults in KwaZulu-Natal, South Africa
Creators: name: Doyle, Aoife
name: Lerato Mchunu
name: Koole, Olivier
name: Sandile Mthembu
name: Siphephelo Dlamini
name: Nothando Ngwenya
name: Ferguson, Jane
name: Seeley, Janet
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Additional file 3: Table S3. Number of records reviewed in the registers according to school. Information on the conditions identified among those screened/vaccinated were also recorded: oral health [14], minor ailments [10], intestinal worms [9], eye health [6], suspected TB [3], underweight [3], overweight [1], hearing [1], and psychosocial support [1]. A total of 36 (20.8%) of learners on the school health register were referred to other services: social worker [2], cardiac problems [3], trauma/injuries [1], urinary problems [3], dental carries [5], poor eyesight [5], clinic check-up [8], and to higher level (no reason given) [9].
Micro-Raman spectroscopy of selected Mo minerals from Su Seinargiu (Sardinia, Italy)
Creators: name: Mauro, Daniela
name: Biagioni, Cristian
name: Orlandi, Paolo
Publisher: name: Periodico di Mineralogia
Year: 2021

description: Raman spectra of selected molybdenum minerals, represented both by bismuth-molybdenum oxides (sardignaite, gelosaite, and mambertiite) and by molybdates [tancaite-(Ce), ichnusaite, nuragheite, and suseinargiuite] from the Su Seinargiu Mo-Bi prospect (Sardinia, Italy) are reported. Raman spectra were collected using samples previously characterized through X-ray diffraction and electron-microprobe analyses. Bismuth-molybdenum oxides are mainly characterized by bands in the range between 300 and 1000 cm-1, related to stretching modes of Mo–O and to Bi–O bonds. Broad bands related to O–H stretching modes were observed in the range between 3000 and 4000 cm-1. Raman spectra of molybdates are characterized by the four fundamental modes of MoO4 groups occurring between 250 and 1000 cm-1. Additionally, bending and stretching bands related to O–H bonds were observed. Micro-Raman spectroscopy may usually be an efficient tool for the discrimination of these rare phases, with some exceptions discussed in the text.
description: Periodico di Mineralogia, Vol. 90 No. 2 (2021): In progress
Geometrical Origin of Fermion Families in SU(2)xU(1) Gauge Theory
Creators: name: Guendelman, E. I.
name: Kaganovich, A. B.
Publisher: name: arXiv
Year: 2001
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Astrophysics (astro-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: A spontaneously broken SU(2)xU(1) gauge theory with just one "primordial" generation of fermions is formulated in the context of generally covariant theory which contains two measures of integration in the action: the standard \sqrt{-g}d^{4}x and a new Φd^{4}x, where Φis a density built out of degrees of freedom independent of the metric. Such type of models are known to produce a satisfactory answer to the cosmological constant problem. Global scale invariance is implemented. After SSB of scale invariance and gauge symmetry it is found that with the conditions appropriate to laboratory particle physics experiments, to each primordial fermion field corresponds three physical fermionic states. Two of them correspond to particles with constant masses and they are identified with the first two generations of the electro-weak theory. The third fermionic states at the classical level get non-polynomial interactions which indicate the existence of fermionic condensate and fermionic mass generation.
description: LATEX, 8 pages; misprint corrected
MOESM1 of Longitudinal immune characterization of syngeneic tumor models to enable model selection for immune oncology drug discovery
Creators: name: Taylor, Molly
name: Hughes, Adina
name: Walton, Josephine
name: Coenen-Stass, Anna
name: Lukasz Magiera
name: Mooney, Lorraine
name: Bell, Sigourney
name: Staniszewska, Anna
name: Sandin, Linda
name: Barry, Simon
name: Watkins, Amanda
name: Carnevalli, Larissa
name: Hardaker, Elizabeth
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Evolutionary Biology
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Cancer
subject: Computational Biology

description: Additional file 1: Table S1. Antibody panels.
Environmental Dependence of Type Ia Supernova Luminosities from the YONSEI Supernova Catalog
Creators: name: Kim, Young-Lo
name: Kang, Yijung
name: Lee, Young-Wook
Publisher: name: arXiv
Year: 2019
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: There is growing evidence for the dependence of Type Ia supernova (SN Ia) luminosities on their environments. While the impact of this trend on estimating cosmological parameters is widely acknowledged, the origin of this correlation is still under debate. In order to explore this problem, we first construct the YONSEI (YOnsei Nearby Supernova Evolution Investigation) SN catalog. The catalog consists of 1231 spectroscopically confirmed SNe Ia over a wide redshift range (0.01 < z < 1.37) from various SN surveys and includes the light-curve fit data from two independent light-curve fitters of SALT2 and MLCS2k2. For a sample of 674 host galaxies, we use the stellar mass and the star formation rate data in Kim et al. (2018). We find that SNe Ia in low-mass and star-forming host galaxies are $0.062\pm0.009$ mag and $0.057\pm0.010$ mag fainter than those in high-mass and passive hosts, after light-curve corrections with SALT2 and MLCS2k2, respectively. When only local environments of SNe Ia (e.g., locally star-forming and locally passive) are considered, this luminosity difference increases to $0.081\pm0.018$ mag for SALT2 and $0.072\pm0.018$ mag for MLCS2k2. Considering the significant difference in the mean stellar population age between the two environments, this result suggests that the origin of environmental dependence is most likely the luminosity evolution of SNe Ia with redshift.
description: 25 pages, 27 figures,and 10 tables. Accepted for publication in JKAS (Journal of the Korean Astronomical Society)
Hidden long range order in Heisenberg Kagome antiferromagnets
Creators: name: Syromyatnikov, A. V.
name: Maleyev, S. V.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We give a physical picture of the low-energy sector of the spin 1/2 Heisenberg Kagome antiferromagnet (KAF). It is shown that Kagome lattice can be presented as a set of stars which are arranged in a triangular lattice and contain 12 spins. Each of these stars has two degenerate singlet ground states which can be considered in terms of pseudospin. As a result of interaction between stars we get Hamiltonian of the Ising ferromagnet in magnetic field. So in contrast to the common view there is a long range order in KAF consisting of definite singlet states of the stars.
description: 4 pages, 3 figures, submitted to Physical Review Letters
Nota preliminar sobre los cambios estacionales de la producción y la riqueza de composición de la leche de vaca en España
Creators: name: ORDÓÑEZ, VICTORIANO CALCEDO
name: ORDÓÑEZ, VICTORIANO CALCEDO
Publisher: name: Unknown
Year: 2001
Subjects: subject: International Relations/Trade
subject: Livestock Production/Industries
subject: Estacionalidad de la producción lechera
subject: riqueza de la leche
subject: Seasonal changes in milk production
subject: milk composition

description: Tomando como base las cantidades de leche entregadas por mes a la industria transformadora entre 1996 y 2000, se observa la semejanza de las cifras porcentuales españolas con las de los EE.MM. de la UE (Alemania, Francia, Reino Unido, y Dinamarca) tomados para contraste. Cualquiera de los años puede servir provisionalmente para fundamentar una distribución porcentual del parámetro de cantidad considerado. No puede decirse lo mismo respecto al promedio mensual de la riqueza de composición (grasa y proteína), pues la divergencia con los porcentajes de los dos parámetros químicos de la leche en los referidos EE.MM. es notoria, de modo que la calidad media de composición de la leche española es netamente inferior. Parece recomendable complementar los datos nacionales relativos a los parámetros examinados con los de las CC.AA. más caracterizadas por su producción de leche.......On the basis of milk quantity delivered per month to dairy industry from 1996 to 2000 it can be observed the similarity between the Spanish percentage figures and those of Germany, France, United Kingdom and Denmark. Any of those years can be provisionally used to establish a percentage distribution of the milk quantity. Not the same can be said about the monthly average composition (butterfat and protein content) of milk. The divergence with the percentage of the two chemical parameters in those countries is well known, so the composition average of Spanish milk is clearly inferior. It seems recommendable to complement national data with those ones of the most characterised for its milk production Autonomous Regions.
Additional file 11 of Fe-doped chrysotile nanotubes containing siRNAs to silence SPAG5 to treat bladder cancer
Creators: name: Liu, Jianye
name: Zhang, Yi
name: Zeng, Hongliang
name: Wang, Long
name: Zhang, Qun
name: Wu, Pei
name: Liu, Xiaoming
name: Xie, Hongyi
name: Xiang, Wei
name: Liu, Biao
name: Liu, Jiahao
name: Liu, Xuewen
name: Xie, Jianfei
name: Tang, Jin
name: Long, Zhi
name: He, Leye
name: Xiao, Mengqing
name: Xiang, Liang
name: Cao, Ke
Publisher: name: figshare
Year: 2021
Subjects: subject: Biophysics
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Pharmacology
subject: Environmental Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Cancer

description: Additional file 11: Figure S11. After FeSiNTs-mediated SPAG5 knockdown in T24 cells, FACS was used to analyze the cell cycle. **P < 0.01.
Investigation of recently discovered common green opals from Anosy (Madagascar)
Creators: name: Caucia, Franca
name: Marinoni, Luigi
name: Gilio, Mattia
name: Dal Corso, Eleonora
Publisher: name: Periodico di Mineralogia
Year: 2021

description: The physical, chemical and gemological properties of recently discovered common green opals from Anosy (South-Eastern Madagascar) have been investigated using different analytical methods such as standard optical and gemological analyzes, X-ray powder diffraction (XRPD), Scanning Electron Microscopy (SEM), Micro-Raman Spectroscopy and Laser Ablation Microprobe (LA-ICP-MS). Anosy opals have a yellowish green color with a light yellowish rim, translucent / opaque diaphaneity with greasy luster, red oxide spots and are inert to long and short wavelength UV radiation (366–254 nm). The values for refractive index and specific gravity range between 1.435–1.460 and 2.03-2.07, respectively. According to XRPD and Raman analyses, the opals are CT type with tridymite more abundant than cristobalite and also contain clay minerals (saponite). Iron and, subordinately, V and Cu appear the main chromophores that determine the green-yellowish color, while Ni and Cr are very subordinate. Other detected trace elements are Mg, Al, Ca, K, and Na. The high contents of Ba are noteworthy since this element is rarely reported in opals worldwide. SEM observations show three types of structures already observed in the CT opals: homogeneous and very fine microspheres, lepispheric cauliflower structures and globular aggregates of different sizes formed by laminae.
description: Periodico di Mineralogia, Vol. 90 No. 2 (2021): In progress
About the connection between the $C_{\ell}$ power spectrum of the Cosmic Microwave Background and the $Γ_{m}$ Fourier spectrum of rings on the sky
Creators: name: Ansari, R.
name: Bargot, S.
name: Bourrachot, A.
name: Couchot, F.
name: Haïssinski, J.
name: Henrot-Versillé, S.
name: Meur, G. Le
name: Perdereau, O.
name: Piat, M.
name: Plaszczynski, S.
name: Touze, F.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In this article we present and study a scaling law of the $mΓ_m$ CMB Fourier spectrum on rings which allows us (i) to combine spectra corresponding to different colatitude angles (e.g. several detectors at the focal plane of a telescope), and (ii) to recover the $C_l$ power spectrum once the $Γ_m$ coefficients have been measured. This recovery is performed numerically below the 1% level for colatitudes $Θ> 80^\circ$ degrees. In addition, taking advantage of the smoothness of the $C_l$ and of the $Γ_m$, we provide analytical expressions which allow to recover one of the spectrum at the 1% level, the other one being known.
description: 8 pages, 8 figures
Dust production in the debris disk around HR 4796 A
Creators: name: Olofsson, J.
name: Milli, J.
name: Thébault, P.
name: Kral, Q.
name: Ménard, F.
name: Janson, M.
name: Augereau, J. -C.
name: Bayo, A.
name: Beamín, J. C.
name: Henning, Th.
name: Iglesias, D.
name: Kennedy, G. M.
name: Montesinos, M.
name: Pawellek, N.
name: Schreiber, M. R.
name: Zamora, C.
name: Carbillet, M.
name: Feautrier, P.
name: Fusco, T.
name: Madec, F.
name: Rabou, P.
name: Sevin, A.
name: Szulágyi, J.
name: Zurlo, A.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Debris disks are the natural by-products of the planet formation process. Scattered or polarized light observations are mostly sensitive to small dust grains that are released from the grinding down of bigger planetesimals. High angular resolution observations at optical wavelengths can provide key constraints on the radial and azimuthal distribution of the small dust grains. These constraints can help us better understand where most of the dust grains are released upon collisions. We present SPHERE/ZIMPOL observations of the debris disk around HR 4796 A, and model the radial profiles along several azimuthal angles of the disk with a code that accounts for the effect of stellar radiation pressure. This enables us to derive an appropriate description for the radial and azimuthal distribution of the small dust grains. Even though we only model the radial profiles along (or close to) the semi-major axis of the disk, our best-fit model is not only in good agreement with our observations but also with previously published datasets (from near-IR to sub-mm wavelengths). We find that the reference radius is located at $76.4\pm0.4$ au, and the disk has an eccentricity of $0.076_{-0.010}^{+0.016}$, with the pericenter located on the front side of the disk (north of the star). We find that small dust grains must be preferentially released near the pericenter to explain the observed brightness asymmetry. Even though parent bodies spend more time near the apocenter, the brightness asymmetry implies that collisions happen more frequently near the pericenter of the disk. Our model can successfully reproduce the shape of the outer edge of the disk, without having to invoke an outer planet shepherding the debris disk. With a simple treatment of the effect of the radiation pressure, we conclude that the parent planetesimals are located in a narrow ring of about $3.6$ au in width.
description: 14 pages, 10 figures, accepted by A&A