cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Revised Radii of Kepler Stars and Planets Using Gaia Data Release 2
Creators: name: Berger, Travis A.
name: Huber, Daniel
name: Gaidos, Eric
name: van Saders, Jennifer L.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: One bottleneck for the exploitation of data from the $Kepler$ mission for stellar astrophysics and exoplanet research has been the lack of precise radii and evolutionary states for most of the observed stars. We report revised radii of 177,911 $Kepler$ stars derived by combining parallaxes from $Gaia$ Data Release 2 with the DR25 $Kepler$ Stellar Properties Catalog. The median radius precision is $\approx$ 8%, a typical improvement by a factor of 4-5 over previous estimates for typical $Kepler$ stars. We find that $\approx$ 67% ($\approx$ 120,000) of all $Kepler$ targets are main-sequence stars, $\approx$ 21% ($\approx$ 37,000) are subgiants, and $\approx$ 12% ($\approx$ 21,000) are red giants, demonstrating that subgiant contamination is less severe than some previous estimates and that Kepler targets are mostly main-sequence stars. Using the revised stellar radii, we recalculate the radii for 2123 confirmed and 1922 candidate exoplanets. We confirm the presence of a gap in the radius distribution of small, close-in planets, but find that the gap is mostly limited to incident fluxes $>$ 200$F_\oplus$ and its location may be at a slightly larger radius (closer to $\approx$ 2$R_\oplus$) when compared to previous results. Further, we find several confirmed exoplanets occupying a previously-described "hot super-Earth desert" at high irradiance, show the relation between gas-giant planet radius and incident flux, and establish a bona-fide sample of eight confirmed planets and 30 planet candidates with $R_{\mathrm{p}}$ $
description: 17 pages, 10 figures, 2 tables. Accepted for publication in ApJ. Electronic versions of Tables 1 & 2 are available as ancillary files (sidebar on the right). For a brief video explaining this paper, see https://youtu.be/RmzkKjtaVf4
Die „Plünderungen“ in Oberungarn im Herbst 1918 – bolschewistische Anarchie oder nationale Revolution?
Creators: name: Szabó, Miloslav
Publisher: name: Zeitschrift für Ostmitteleuropa-Forschung
Year: 2024

description: .
description: Zeitschrift für Ostmitteleuropa-Forschung, Bd. 73 Nr. 1 (2024)
Felis leo Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Carnivora
Felidae
Felis
Felis leo

description: Felis leo [spec. nov.]
F. cauda elongata, corpore helvulo.
Felis cauda elongata floccosa, thorace jubato. Syst. nat. 6. p. 4. n. 1.
Leo. Gesn. quadr. 572. Aldr. dig. 2. Jonst. quadr. 72. Dodart. act. 1. t. 1. & 7. t. 7. Raj. quadr. 162.
Habitat in Africa.
Color luteo-rufus. Fons quadrata. Cor maximum. Maris Thorax hirsutus Caudaque floccosa.
Segnis, esuriens praedatur de Equis et majoribus quadrupedibus, nec nisi famelicus homine; fugatur accensa flamma; canibus coercetur. Retro mingit & coit? Rugitus horrrendus a tracheae annulis integris imbricatis.
Anatome. E. N. C. d. 1. a 2. obs. 6. Barth. act. 1671. n. 17.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 41, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
HST Star Counts at High Galactic Latitudes
Creators: name: Santiago, Basilio X.
name: Gilmore, Gerard
name: Elson, Rebecca A. W.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We use star counts from 13 deep HST fields imaged with the {\it Wide Field Camera - 2} in order to constrain the amount of dark matter in the Galaxy that can be in the form of low-mass main sequence stars or white-dwarfs. Based on the number of red stars found in our fields, we exclude the possibility that more than 25\% of the massive dark halo is made up of M dwarfs or subdwarfs; fairly massive ($M \sim 0.2 M_\odot$) and yet extremely faint ($M_I$ \gtsima $14.5$) stellar candidates would have to be invoked in order to make the observed number of stars compatible with that predicted by a stellar dark halo. White dwarfs must also be intrinsically very faint ($M_I$ \gtsima $14$) in order to be consistent with the observed number of faint stars in the HST fields. We also rule out an increasing or flat stellar luminosity function beyond $M_V \sim 13$. The inferred slope of the disk luminosity function is intermediary between local, volume-limited surveys and ground-based photometric ones. Finally, the magnitude counts are well fitted by existing models for the structure of the Galaxy, with only small changes in the fiducial values of the model parameters. The colour distribution, however, is not well reproduced by the models. It is unclear at present if this reflects inadequacies of the available models or uncertainties in the colour-magnitude diagrams for low metallicity stars and in the photometric calibration.
description: 18 pages plus 6 figures
Canis vulpes Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Carnivora
Canidae
Canis
Canis vulpes

description: Canis vulpes [spec. nov.]
C. cauda recta: apice albo. Syst. nat. 5.
Vulpes. Gesn. quadr. 966. Aldr. dig. 195. Jonst. quadr. 82. Raj. quadr. 177.
Habitat in Europa, Asia, Africa, antra fodiens.
Corpus flavo rufescens. Aures recti. Maxillae albae. Pedes antice nigrescentes.
Degit in antris, quae fodit animal astutissimum; saevit in Agnos, Anseres, Gallinas, Aviculas, non Accipitres foetidioresque; colligit stercora animalium. Fragrat ambrosiaco odore supra basin caudae.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 40, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Mechanism of C/EBP Alpha and C/EBP Beta in pathogenesis of hepatocellular carcinoma
Creators: name: Zhao, Xiaoyang
Publisher: name: Imperial College London
Year: 2017

description: Hepatocellular carcinoma (HCC) is generally accompanied by high morbidity and mortality as well as a low cure rate. Decades of investigations have provided insight into the molecular pathogenesis of HCC, where the majority of studies have been focused on transcription factors and their influence in aberrant cell growth. C/EBP Alpha is a member of the large CCAAT/enhancer-binding protein (C/EBP) family of bZIP transcription factors. C/EBP Alpha is a liver enriched transcription factor that regulates the expression of genes involved in hepatic glycogen synthesis, lipid homeostasis, and gluconeogenesis, as well as negatively modulating hepatocyte proliferation. It has previously been proved that enhancing C/EBP Alpha expression by short-activating RNAs (saRNA) can decrease tumour burden and improve liver function in cirrhotic rats with spontaneous HCC. New evidence is now emerging that C/EBP Alpha and C/EBP Beta may play a crucial role in regulating cell proliferation and hepatocyte function. Much is to be learnt about these transcription factors and their role as a potential tool for liver regeneration. The aim of this project is to further elucidate the mechanism of C/EBP Alpha and C/EBP Beta in the pathogenesis of hepatocellular carcinoma and investigate the molecular mechanistic character of saRNA induced RNA activation (RNAa). By doing so, we aim to understand how this protein encoded by an intronless gene can homodimerise and heterodimerise at the promoters and enhancers of a wide range of genes to regulate and maintain normal hepatocyte function. We found that C/EBP Alpha activation promotes anti-proliferative effect in differentiated HCC, and the addition of siRNA to another C/EBP family member-C/EBP Beta converts undifferentiated cell line into sensitive as it abrogates the dominant oncogenic effect of 30kDa isform of C/EBP Beta. Functional synergy of C/EBP Alpha and C/EBP Beta promotes anti-proliferative effect in both differentiated and undifferentiated HCC. For the mechanism of saRNA induced RNA activation, we confirmed that saRNA induced RNA activation works via interacting with hnRNPA2/B1 and DDXn in differentiated HCC by investigating the direct binding partners within saRNA protein complex which are involved in saRNA function. On this basis, we may reconstruct the journey of converting undifferentiated HCC to a more sensitive phenotype by upregulating the expression of these functional saRNA binding partners.
Canis familiaris subsp. extrarius Linnaeus, 1758, subspec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Carnivora
Canidae
Canis
Canis familiaris
Canis familiaris subsp. extrarius

description: Canis familiaris subsp. extrarius [subspec. nov.]
auriculis longis lanatis pendulis. Aldr. digit. 561.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 39, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Are Galaxies Optically Thin to Their Own Lyman Continuum Radiation? I. M33
Creators: name: Patel, K.
name: Wilson, C. D.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Halpha and UBV photometry of the inner kpc of M33 are used to study the distribution of OB stars and HII regions in the galaxy and to determine whether individual regions of the galaxy are in a state of ionization balance. Based on the surface brightness of the Halpha emission, we identify three distinct ionized gas environments (bright, halo and field). We find that 50% of the OB stars are located in the field, so that 1/2 of the lifetime of OB stars must be spent outside recognizable HII regions. If OB stars escape from bright HII regions by destroying their parent molecular clouds, this result would imply that molecular cloud lifetimes after forming OB stars could be as low as 5e6 yrs or 1/2 the typical lifetime of OB stars. Halpha fluxes predicted from ionization models reveal that none of the regions are in ionization balance: predicted fluxes are a factor of 3-7 greater than observed. The heaviest loss of ionizing photons appears to be taking place in the field. Our results suggest that star formation rates obtained from Halpha luminosities must underestimate the true star formation rate in these regions of M33.
description: Replaced version should now compile with standard aastex style files. 23 pages, aastex preprint format. Accepted in ApJ. Hardcopies of figures available on request to wilson@physics.mcmaster.ca
Canis aureus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Carnivora
Canidae
Canis
Canis aureus

description: Canis aureus [spec. nov.]
C. Lupus aureus dictus. �.
Lupus aureus. Kaempf. amoen. 413. t. 407. f. 3. Raj. quadr. 174.
Vulpes indiae orientalis. Valent. mus. 452. t. 452.
Adill. Bell. itin. 160.
Habitat in oriente.
Nitide flavus, catervatim incedit, furto deditus; uno clamante clamant remoti alii, ambulante sono nocturno; ululatus execrabilis, quasi ejulatus latratu interceptus. Descriptio vera animalis etiamnum deficit.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on pages 40-41, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Core-collapse supernovae in the hall of mirrors. A three-dimensional code-comparison project
Creators: name: Cabezón, Rubén M.
name: Pan, Kuo-Chuan
name: Liebendörfer, Matthias
name: Kuroda, Takami
name: Ebinger, Kevin
name: Heinimann, Oliver
name: Thielemann, Friedrich-Karl
name: Perego, Albino
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Modeling core-collapse supernovae (CCSNe) with neutrino transport in three dimensions (3D) requires tremendous computing resources and some level of approximation. We present a first comparison study of CCSNe in 3D with different physics approximations and hydrodynamics codes. We aim to assess the impact of the hydrodynamics code, approximations for the neutrino and gravity treatments, and rotation on the simulation of CCSNe in 3D. We use four different hydrodynamics codes in this work (ELEPHANT, FLASH, fGR1, and SPHYNX) in combination with two different neutrino treatments, the isotropic diffusion source approximation (IDSA) and two-moment M1, and three different gravity treatments: Newtonian, 1D General Relativity (GR) correction, and full GR). Additional parameters discussed in this study are the inclusion of neutrino-electron scattering via a parametrized deleptonization (PD) and the influence of rotation. The four codes compared in this work include Eulerian and fully Lagrangian (smoothed particle hydrodynamics) codes for the first time. They show agreement in the overall evolution of the collapse phase and early post-bounce within the range of 10% (20% in some cases). The comparison of the different neutrino treatments highlights the need to further investigate the antineutrino luminosities in IDSA, which tend to be relatively high. We also demonstrate the requirement for a more detailed heavy-lepton neutrino leakage. When comparing with a full GR code, including an M1 transport method, we confirm the influence of neutrino-electron scattering during the collapse phase, which is adequately captured by the PD scheme. Also, the effective GR potential reproduces the overall dynamic evolution correctly in all Newtonian codes. Additionally, we verify that rotation aids the shock expansion and estimate the overall angular momentum losses for each code in rotating scenarios.
description: 20 pages, 11 figures, 4 Tables. Published in A&A
Vom „erfolgreichen Durchdringen des nationalen Gedankens“ und dem „Sieg der demokratischen Grundsätze“. Deutungsmuster von Nation und Demokratie in Oberschlesien, dem Teschener Schlesien und der Orava (1918/19)
Creators: name: Ramisch-Paul, Sebastian
name: Wehowski, Matthäus
Publisher: name: Zeitschrift für Ostmitteleuropa-Forschung
Year: 2024

description: .
description: Zeitschrift für Ostmitteleuropa-Forschung, Bd. 73 Nr. 1 (2024)
Felis Linnaeus, 1758, gen. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Carnivora
Felidae
Felis

description: Felis [gen. nov.]
Dentes Primores aequales.
Molares terni.
Lingua retrorsum aculeata.
Ungues retractiles.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 41, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Wilsons Moment? Wilsons Deutungen von Demokratie und Nation, ihre nationalen Rezeptionen und die Bedeutung für die Grenzkonflikte in Oberschlesien, dem Teschener Schlesien und der Orava
Creators: name: Kailitz, Steffen
Publisher: name: Zeitschrift für Ostmitteleuropa-Forschung
Year: 2024

description: .
description: Zeitschrift für Ostmitteleuropa-Forschung, Bd. 73 Nr. 1 (2024)
Tank design modifications for the improved performance of froth flotation equipment
Creators: name: Morrison, Angus James
Publisher: name: Imperial College London
Year: 2017

description: Froth flotation is a physico-chemical technique used to separate the constituents of a mixed mineral slurry by their relative surface hydrophobicity. In order to do so economically, it is necessary to treat large volumes of material in ever-larger and more efficient tanks. The efficiency and efficacy of such tanks can be enhanced through mechanical modifications designed to improve froth handling, increase the likelihood of bubble-particle interactions in the pulp, and increase the residence time of suspended solids in the tank. However, design modifications suggested by computational modelling or bench-scale experiments often do not realise performance improvements at pilot and plant-scale because of imperfect scale-up from bench-scale, and differences in the type and intensity of the sub-processes affecting performance at different scales. The first outcome of this thesis is an intermediate, laboratory-scale froth flotation circuit that more closely resembles continuously-operated pilot-scale equipment, but which is better instrumented and controlled. This work describes not only the laboratory-scale system, but also detailed regression models of its behaviour and performance based on extensive monitoring and instrumentation. The resultant performance models provide a baseline against which to test design modifications, and the resultant behaviour models inform the design of such modifications. The second outcome of this thesis, a performance-enhancing design modification, was prompted by the discovery that minimising the variability of the pulp-froth interface leads to an increase in both indicative grade and recovery. The resultant tank modification was a horizontal mesh inserted into the pulp below the pulp-froth interface, designed to isolate it from the turbulent region around the impeller. The mesh pore size and thickness, and the position at which it was installed in the tank, were taken as design variables to be optimised by the genetic algorithm method. The result is a grade-recovery curve corresponding to an optimal mesh pore size of 123.4 +/- 3.1 mm. From this curve it was found that increasing the mesh thickness from 33 mm to 47 mm yields a maximum improvement in the recovery of 18.9% without compromising the grade, and increasing the depth of the mesh from 200 mm to 250 mm below the pulp-froth interface yields a maximum improvement in the grade of 3.2% without compromising the recovery. This grade-recovery curve, and the insights gained during the process of design and refinement, provides the rationale for a proposed program of mesh tests at pilot-scale.
Are Galaxies Optically Thin to Their Own Lyman Continuum Radiation? II. NGC 6822
Creators: name: Patel, K.
name: Wilson, C. D.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Halpha and UBV photometry of NGC 6822 are used to study the distribution of OB stars and HII regions in the galaxy and to determine whether individual regions of the galaxy are in a state of ionization balance. Four distinct components of the Halpha emission (bright, halo, diffuse and field) differentiated by their surface brightnesses are identified. We find that approximately 1/2 of all OB stars in NGC 6822 are located in the field while only 1/4 are found in the combined bright and halo regions, suggesting that OB stars spend roughly 3/4 of their lifetimes outside ``classical'' H II regions. Comparing the observed Halpha emission with that predicted from stellar ionizing flux models, we find that although the bright, halo and diffuse regions are probably in ionization balance, the field region is producing at least 6 times as much ionizing flux as is observed. The ionization balance results in NGC 6822 suggest that star formation rates obtained from Halpha luminosities must underestimate the true star formation rate in this galaxy by about 50%. Comparing our results for NGC 6822 with previous results for the spiral galaxy M33, we find that the inner kiloparsec of M33 is in a more serious state of ionization imbalance, perhaps due to its higher surface density of blue stars.
description: Replaced version should now compile with standard aastex style files. 28 pages, aastex preprint format. Accepted in ApJ. Hardcopies of figures available on request to wilson@physics.mcmaster.ca
Planning your rehabilitation
Creators: name: Kerr, Claire
Publisher: name: Murdoch Childrens Research Institute
Year: 2018
Subjects: Health Sciences

description: This booklet answers some of the questions children and their families may have about rehabilitation after an orthopaedic operation. Other children with cerebral palsy who had lower limb orthopaedic surgery and their families told us what was important for them. We have used that information to help write this booklet.
Felis tigris Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Carnivora
Felidae
Felis
Felis tigris

description: Felis tigris [spec. nov.]
F. cauda elongata, corpore maculis omnibus virgatis. Syst. nat. 4. n. 2.
Tigris. Gesn. quadr. 936. Aldr. dig. 101. Jonst. quadr. 84. Bont. jav. 52. t. 53. Raj. quadr. 165.
Habitat in Asia.
Magnitudo Leonis. Maculae virgatae, transversae. Pulcherrimum animal tremendae velocitatis, homini pessimus, desolat indos; Mas occidit proprios filios.
Anatome. E. N. C. d. 1. a. 2. obs. 7. & a 9. obs. 194.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 41, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Zeiten der Unsicherheiten. Demokratisierung und Nationalisierung in Ostmitteleuropa auf regionaler und lokaler Ebene (1918–1923)
Creators: name: Kailitz, Steffen
name: Buchen, Tim
name: Ramisch-Paul, Sebastian
Publisher: name: Zeitschrift für Ostmitteleuropa-Forschung
Year: 2024

description: .
description: Zeitschrift für Ostmitteleuropa-Forschung, Bd. 73 Nr. 1 (2024)
A translational genomics approach to dissect mechanisms of heart failure and recovery
Creators: name: Pesce, Francesco
Publisher: name: Imperial College London
Year: 2015

description: Dilated cardiomyopathy (DCM) is a progressive disease of heart muscle leading to end-stage heart failure (HF). In this study I used a novel RNA-Sequencing (RNA-Seq) dataset derived from left ventricle (LV) of a large cohort (n = 126) of patients with this condition. Different bioinformatics approaches were applied to combine data from cases, controls, in vivo and cell-based experimental models of fibrosis, as well as genetic data, in order to investigate pathways underlying end-stage HF in DCM, the potential for recovery and mechanisms resulting from Titin (TTN) truncating mutations in these patients. Multiple and functionally heterogeneous gene co-expression networks (n = 48) were identified in DCM, of which 26 were disease specific. Further prioritization of the networks focused on fibrosis as key process occurring in the LV of these patients. Finally, a Systems Genetics framework was implemented and identified the gene WW Domain Containing E3 Ubiquitin Protein Ligase 2 (WWP2) as a genetic regulator of a disease specific fibrosis-related network. In a second phase, I investigated the differences in the expression profile of DCM patients who received a left ventricular assist device (LVAD) (n = 61) compared to those who underwent elective heart transplant (n = 58). The results showed in the first group a prominence of mechanisms driven by cytokines and the role of a specific pattern of coordinated genes related to contractile function. Analysis of a subset of LVAD implanted patients who subsequently recovered function was limited by sample size. Likewise, testing whether truncating mutations in TTN, the single most common genetic cause of DCM, perturb downstream pathways lacked power. Based on comprehensive and unbiased analyses centered on RNA-Seq, these findings are unique in defining the transcriptional landscape of LV in end-stage HF due to DCM. In particular, Systems Genetics proved to be a useful translational framework having pointed towards WWP2 as novel candidate target gene for fibrosis in these patients.
Felis pardus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Carnivora
Felidae
Felis
Felis pardus

description: Felis pardus [spec. nov.]
F. cauda elongata, corpore maculis superioribus orbiculatis; inferioribus virgatis. Syst nat. 4. n. 3.
Panthera, Pardalis, Pardus, Leopardus. Gesn. quadr. 824.
F{?X}el{?X} genus sobrium, seandit facile arbores, noctu potissimum speculatur.
Pardus mas, Panthera femina. Alp. aegypt. 237. t. 15. f. 2.
Pardalis. Raj. quadr. 166.
Tigris mexicana. Hern. mex. 498. t. 498.
Pinum Dasypus. Nieremb. nat. 153. t. 153.
Habitat in Indiis.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on pages 41-42, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Magnetic Field Effects on the Structure and Evolution of Overdense Radiatively Cooling Jets
Creators: name: Cerqueira, Adriano H.
name: Pino, Elisabete M. de Gouveia Dal
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate the effect of magnetic fields on the propagation dynamics and morphology of overdense, radiatively cooling, supermagnetosonic jets, with the help of fully three-dimensional SPMHD simulations. Evaluated for a set of parameters which are mainly suitable for protostellar jets (with density ratios between the jet and the ambient medium 3-10, and ambient Mach number ~ 24), these simulations are also compared with baseline non-magnetic and adiabatic calculations. We find that, after amplification by compression and re-orientation in nonparallel shocks at the working surface, the magnetic field that is carried backward with the shocked gas into the cocoon improves the jet collimation relative to the purely hydrodynamic (HD) systems. Low-amplitude, approximately equally spaced internal shocks (which are absent in the HD systems) are produced by MHD K-H reflection pinch modes. The longitudinal field geometry also excites non-axisymmetric helical modes which cause some beam wiggling. The strength and amount of these modes are, however, reduced (by ~ twice) in the presence of radiative cooling relative to the adiabatic cases. Besides, a large density ratio between the jet and the ambient medium also reduces, in general, the number of the internal shocks. As a consequence, the weakness of the induced internal shocks makes it doubtful that the magnetic pinches could produce by themselves the bright knots observed in the overdense, radiatively cooling protostellar jets.
description: To appear in ApJ; 36 pages + 16 (gif) figures. PostScript files of figures are available at http://www.iagusp.usp.br/preprints/preprint.html
Single-crystal growth of iron-based superconductor La$_{0.34}$Na$_{0.66}$Fe$_2$As$_2$
Creators: name: Gu, Yanhong
name: Wang, Jia-Ou
name: Ma, Xiaoyan
name: Luo, Huiqian
name: Shi, Youguo
name: Li, Shiliang
Publisher: name: arXiv
Year: 2018
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We report single-crystal growth of La$_{0.34}$Na$_{0.66}$Fe$_2$As$_2$ iron-based superconductor with the size of several millimeters. The samples were accidentally obtained in trying to grow LaFeAsO$_{1-y}$F$_y$ ( $y \geq$ 0.8 ) single crystals with NaAs and NaF flux. The sample shows both antiferromagnetic and structural transitions at 106 K. The superconducting transition temperature is about 27 K with the superconducting anisotropy of about 1.9. These values and the temperature dependence of the Hall coefficient suggest that La$_{0.34}$Na$_{0.66}$Fe$_2$As$_2$ belongs to hole-doped "122" families of iron pnictides with the doping level slightly lower than optimal doping. Compared with previous reports on the polycrystalline samples, our results suggest that either $T_c$ of the this system can be further increased, or the superconducting dome may not be well formed in this system. In either case, the La$_{0.5-x}$Na$_{0.5+x}$Fe$_2$As$_2$ system provides a new platform to study the antiferromagnetic and superconducting properties of iron-based superconductors.
description: 11 pages, 5 figures
Felis catus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Carnivora
Felidae
Felis
Felis catus

description: Felis catus [spec. nov.]
F. cauda elongata, corpore fasciis nigricantibus; dorsalibus longitudinalibus tribus; lateralibus spiralibus.
Felis cauda elongata, auribus aequalibus. Faun. suec. 3. Syst. nat. 4. n. 6.
Felis vulgo Catus. Gesn. quadr. 98. Aldr. quadr. 565. Raj. quadr. 98.
Felis. Aldr. dig. 564. Jonst. quadr. 180. t. 72..
Habitat in Europae australis sylvis.
Moribus congenerum, tranquilla, ore molat, caudam erigit; excitata agilissima, scandit, irata fremit odore ambrosiaco, Murum Leo, in praedam intenta caudam movet, oculi noctu lucent, inhiando praedam haurit, clamando rixandoque misere amat. Pupilla interdin perpendiculari oblonga, noctu tereti ampliata; unguibus complicatis incedit, parce bibit, urina corrosiva, stercus sepelit, carnes edit vegetabiliaque respuit, os instante tempestate manu lavat, dorsum in tenebris electrisat; in altum acta decidit in pedes. Pulices non habet. Delectatur Maro, Nepeta, Valeriana.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 42, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
title:  Le Startup cooperative: l’esperienza Coopstartup
Creators: name: Moreschi  , Barbara
Publisher: name: RomaTrE-Press
Year: 2020

description: Il capitolo descrive l’alternativa cooperativa alle startup mainstream, le startup cooperative. Per farlo, si fa riferimento all’esperienza italiana di Coopstartup, con un’appendice sulle 44 startup cooperative nate dal programma. Il capitolo serve da transizione tra i capitoli teorici e le esperienze pratiche, sottolineando l’importanza di queste nuove esperienze cooperative. Le startup cooperative si inseriscono perfettamente nel quadro dell’intergenerazionalità, della gestione condivisa del bene comune e, in particolare, ribadiscono come l’impresa cooperativa sappia adattarsi ai bisogni della società, dando un’alternativa più inclusiva ai giovani che vogliono fare impresa.
description: Cooperative bene comune
Viverra Linnaeus, 1758, gen. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Carnivora
Viverridae
Viverra

description: Viverra [gen. nov.]
Dentes Primores VI: intermediis brevioribus.
Molares plures quam tres.
Lingua retrorsum aculeata.
Ungues exserti.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 43, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
3-D SPH Simulations of Radiatively Cooling Magnetized Jets
Creators: name: Pino, Elisabete M. de Gouveia Dal
name: Cerqueira, Adriano H.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In this work, we sumarize the results of three-dimensional smooth particle magnetohydrodynamic numerical simulations of supermagnetosonic, radiatively cooling jets.
description: 2 pages; To appear in the proceedings of the 1998 Numerical Astrophysics Conferences, Tokyo (Japan) 09-13 March 1998
Felis onca subsp. pardalis Linnaeus, 1758, subspec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Carnivora
Felidae
Felis
Felis onca
Felis onca subsp. pardalis

description: Felis onca subsp. pardalis [subspec. nov.]
F. cauda elongata, corpore maculis superioribus virgatis; inferioribus orbiculatis. Syst. nat. 4. n. 4.
Cato-Pardus mexicanus. Hern. mex. 512. t. 512.
Catus Pardus s. Catus americanorum. Raj. quadr. 169.
Habitat in America.
Magnitudo Melis supra fuscus, subtus albicans; Lineae punctaque nigra per totum corpus longitudinaliter sparsa, sed pedes & abdomen tantum punctis; Latera lineis latioribus albis & fuscis pinguntur. Aures breves, margine bisidae absque penicillis. Pedes 5-4. Cauda verticillato-variegata proportione Cati. Mystaces 4 ordinum: in singulo ordine setae 3. s. 5, albae basi nigrae, longitudine capitis.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 42, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Quantum Control with Measurements and Quantum Zeno Dynamics
Creators: name: Sørensen, Jens Jakob
name: Dalgaard, Mogens
name: Kiilerich, Alexander Holm
name: Mølmer, Klaus
name: Sherson, Jacob
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We introduce an efficient iterative method to prepare a target state in Hilbert spaces with high dimensionality using a combination of unitary evolution, measurements, and quantum Zeno dynamics. The latter confines the evolution within Zeno subspaces of decreasing size. This gives an exponential speed up relative to the case of states evolving in the full Hilbert space between projective measurements. We demonstrate our approach on the control problem of rapidly transferring a superfluid into the Mott insulator in the Bose-Hubbard model. We discuss the general applicability of the method by preparing arbitrary superpositions with random Hamiltonians.
The Dynamic Formation of Prominence Condensations
Creators: name: Antiochos, Spiro K.
name: MacNeice, Peter J.
name: Spicer, Daniel S.
name: James
name: Klimchuk, A.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present simulations of a model for the formation of a prominence condensation in a coronal loop. The key idea behind the model is that the spatial localization of loop heating near the chromosphere leads to a catastrophic cooling in the corona (Antiochos & Klimchuk 1991). Using a new adaptive grid code, we simulate the complete growth of a condensation, and find that after approx. 5,000 s it reaches a quasi-steady state. We show that the size and the growth time of the condensation are in good agreement with data, and discuss the implications of the model for coronal heating and SOHO/TRACE observations.
description: Astrophysical Journal latex file, 20 pages, 7 b-w figures (gif files)
Cesarean section diverticulum area predicting the intraoperative hemorrhage at suction curettage for cesarean scar pregnancy after focused ultrasound ablation surgery
Creators: name: Huang, Jun-rong
name: Sun, Li-ya
name: Tang, Ying
name: Wen, Ming-bo
name: Yang, Ming-tao
name: Xu, Fan
name: Shi, Qiuling
name: Hu, Hui-quan
Publisher: name: Taylor & Francis
Year: 2025
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Physiology
subject: Pharmacology
subject: Biotechnology
subject: Ecology
subject: Biological Sciences not elsewhere classified
subject: Marine Biology
subject: Science Policy
subject: Infectious Diseases
subject: FOS: Health sciences

description: To investigate the significance of the cesarean section diverticulum (CSD) area for predicting the intraoperative massive hemorrhage during suction curettage for cesarean scar pregnancy (CSP) after focused ultrasound ablation surgery (FUAS). Data from 90 patients undergoing suction curettage after FUAS were collected. According to their intraoperative bleeding volume, patients were categorized into three groups: Group 1 (n = 71, <200 mL), Group 2 (n = 9, 200–300 mL) and Group 3 (n = 10, ≥300 mL). Multiple liner regression analysis was performed to identify the influencing factors for CSD area and intraoperative blood loss. The ROC curve was plotted to identify the optimal cutoff values. The median CSD area size in Group 3 (336.8 mm2) was significantly greater than in Groups 1 (128.6 mm2) and 2 (121.6 mm2) (p < .05). Using multiple linear regression analysis, CSD area was associated with intraoperative blood loss (p < .05). The optimal cutoff CSD areas for predicting intraoperative massive hemorrhage volumes ≥ 200 mL and ≥ 300 mL were 202.05 mm2 and 241.90 mm2, respectively. The mean gestational sac diameter and preoperative symptoms (+) were positively related to CSD area, while residual myometrial thickness was negatively correlated with the CSD area. CSD area showed the greatest relationship to sonication time (rs = 0.42), treatment time (rs = 0.316) and total energy used for ablation (rs = 0.415). The preoperative CSD area could predict intraoperative massive hemorrhage during suction curettage after FUAS, which might inform therapy strategies for CSP patients.
Additional file 4: of β-blockers and risk of all-cause mortality in patients with chronic heart failure and atrial fibrillation—a meta-analysis
Creators: name: Xu, Tianyu
name: Huang, Yuli
name: Zhou, Haobin
name: Bai, Yujia
name: Huang, Xingfu
name: Hu, Yunzhao
name: Xu, Dingli
name: Zhang, Yuhui
name: Zhang, Jian
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Molecular Biology
subject: Pharmacology
subject: Sociology
subject: FOS: Sociology
subject: Developmental Biology
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences

description: Funnel plot of the comparison of β-blockers treatment versus no β-blockers treatment in patients with chronic heart failure and atrial fibrillation, outcomes: all-cause mortality. BBs: β-blockers; CI: confidence intervals; SE: standard error. (PDF 30 kb)
Scintillation and Ionization Ratio of Liquid Argon for Electronic and Nuclear Recoils at Drift-Fields up to 3 kV/cm
Creators: name: Washimi, T.
name: Kimura, M.
name: Tanaka, M.
name: Yorita, K.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: A two-phase argon detector has high discrimination power between electron recoil and nuclear recoil events based on the pulse shape discrimination and the ionization/scintillation ratio (S2/S1). This character is very suitable for the dark matter search to establish the low background experiment. However, the basic properties of S2/S1 of argon are not well known, as compared with xenon. We report the evaluation of S2/S1 properties with a two-phase detector at drift-fields of 0.2-3.0 kV/cm. Finally, the discrimination power against electron recoil background of S2/S1 is discussed.
The Age of the Universe
Creators: name: Chaboyer, Brian
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A minimum age of the universe can be estimated directly by determining the age of the oldest objects in the our Galaxy. These objects are the metal-poor stars in the halo of the Milky Way. Recent work on nucleochronology finds that the oldest stars are 15.2+/-3.7 Gyr old. White dwarf cooling curves have found a minimum age for the oldest stars of 8 Gyr. Currently, the best estimate for the age of the oldest stars is based upon the absolute magnitude of the main sequence turn-off in globular clusters. The oldest globular clusters are 11.5+/-1.3 Gyr old, implying a minimum age of the universe of t_universe > 9.5 Gyr (95% confidence level).
description: invited review to appear in Physics Reports
Coordination in a supply chain with two manufacturers, two substitute products, and one retailer
Creators: name: Thorstenson, Anders
name: Ramani, Vinay
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Sociology
subject: FOS: Sociology
subject: Plant Biology
subject: FOS: Biological sciences
subject: Computational Biology

description: This paper analyses a model of coordination in a supply chain consisting of two manufacturers, two products, and a single retailer under full information. Market demand for each of the manufacturer's products allows for both price and cross-price elasticities. We consider a Stackelberg game between the retailer and the two manufacturers and solve for the subgame perfect equilibrium wholesale price chosen by each of the manufacturers, the retail price charged by the retailer for each of two products, as well as the equilibrium demands for the two products. Unlike a classical dyadic supply chain, we show that only under certain allocations of the total profit between the manufacturers and the retailer is it the case that the vertically integrated chain is the preferred supply chain structure, even though it provides the highest total profit. An important result is that vertical integration is less advantageous when products are closer substitutes. We also show that a revenue sharing contract can coordinate this chain, but only when the manufacturers set their wholesale prices below their marginal costs of production. Finally, we show that the retailer can choose to integrate partially with one manufacturer to achieve a Pareto improving profit outcome.
Evidence for Color Dichotomy in the Primordial Neptunian Trojan Population
Creators: name: Lin, Hsing Wen
name: Gerdes, David W.
name: Hamilton, Stephanie J.
name: Adams, Fred C.
name: Bernstein, Gary M.
name: Sako, Masao
name: Bernadinelli, Pedro
name: Tucker, Douglas
name: Allam, Sahar
name: Becker, Juliette C.
name: Khain, Tali
name: Markwardt, Larissa
name: Franson, Kyle
name: Abbott, T. M. C.
name: Annis, J.
name: Avila, S.
name: Brooks, D.
name: Rosell, A. Carnero
name: Kind, M. Carrasco
name: Cunha, C. E.
name: D'Andrea, C. B.
name: da Costa, L. N.
name: De Vicente, J.
name: Doel, P.
name: Eifler, T. F.
name: Flaugher, B.
name: Garcia-Bellido, J.
name: Hollowood, D. L.
name: Honscheid, Klaus
name: James, D. J.
name: Kuehn, K.
name: Kuropatkin, N.
name: Maia, M. A. G.
name: Marshall, J. L.
name: Miquel, R.
name: Plazas, A. A.
name: Romer, A. K.
name: Sanchez, E.
name: Scarpine, V.
name: Sevilla-Noarbe, I.
name: Smith, M.
name: Smith, R. C.
name: Soares-Santos, M.
name: Sobreira, F.
name: Suchyta, E.
name: Tarle, G.
name: Walker, A. R.
name: Wester, W.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: In the current model of early Solar System evolution, the stable members of the Jovian and Neptunian Trojan populations were captured into resonance from the leftover reservoir of planetesimals during the outward migration of the giant planets. As a result, both Jovian and Neptunian Trojans share a common origin with the primordial disk population, whose other surviving members constitute today's trans-Neptunian object (TNO) populations. The cold classical TNOs are ultra-red, while the dynamically excited "hot" population of TNOs contains a mixture of ultra-red and blue objects. In contrast, Jovian and Neptunian Trojans are observed to be blue. While the absence of ultra-red Jovian Trojans can be readily explained by the sublimation of volatile material from their surfaces due to the high flux of solar radiation at 5AU, the lack of ultra-red Neptunian Trojans presents both a puzzle and a challenge to formation models. In this work we report the discovery by the Dark Energy Survey (DES) of two new dynamically stable L4 Neptunian Trojans,2013 VX30 and 2014 UU240, both with inclinations i >30 degrees, making them the highest-inclination known stable Neptunian Trojans. We have measured the colors of these and three other dynamically stable Neptunian Trojans previously observed by DES, and find that 2013 VX30 is ultra-red, the first such Neptunian Trojan in its class. As such, 2013 VX30 may be a "missing link" between the Trojan and TNO populations. Using a simulation of the DES TNO detection efficiency, we find that there are 162 +/- 73 Trojans with Hr < 10 at the L4 Lagrange point of Neptune. Moreover, the blue-to-red Neptunian Trojan population ratio should be higher than 17:1. Based on this result, we discuss the possible origin of the ultra-red Neptunian Trojan population and its implications for the formation history of Neptunian Trojans.
Additional file 7: of Î˛-blockers and risk of all-cause mortality in patients with chronic heart failure and atrial fibrillationâ a meta-analysis
Creators: name: Xu, Tianyu
name: Huang, Yuli
name: Zhou, Haobin
name: Bai, Yujia
name: Huang, Xingfu
name: Hu, Yunzhao
name: Xu, Dingli
name: Zhang, Yuhui
name: Zhang, Jian
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Molecular Biology
subject: Sociology
subject: FOS: Sociology
subject: Mathematical Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer

description: Risk of bias graph. (PDF 238 kb)
Variational study of U(1) and SU(2) lattice gauge theories with Gaussian states in 1+1 dimensions
Creators: name: Sala, P.
name: Shi, T.
name: Kühn, S.
name: Bañuls, M. C.
name: Demler, E.
name: Cirac, J. I.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We introduce a method to investigate the static and dynamic properties of both Abelian and non-Abelian lattice gauge models in 1+1 dimensions. Specifically, we identify a set of transformations that disentangle different degrees of freedom, and apply a simple Gaussian variational ansatz to the resulting Hamiltonian. To demonstrate the suitability of the method, we analyze both static and dynamic aspects of string breaking for the U(1) and SU(2) gauge models. We benchmark our results against tensor network simulations and observe excellent agreement, although the number of variational parameters in the Gaussian ansatz is much smaller.
description: 19 pages, 6 figures. Added references and corrected typos