cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Spontaneous decay of a soft optical phonon in the relaxor ferroelectric PbMg$_{1/3}$Nb$_{2/3}$O$_{3}$
Creators: name: Stock, C.
name: Gehring, P. M.
name: Ewings, R. A.
name: Xu, G.
name: Li, J.
name: Viehland, D.
name: Luo, H.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We report the spontaneous decay of a soft, optical phonon in a solid. Using neutron spectroscopy, we find that specific phonon lifetimes in the relaxor PbMg$_{1/3}$Nb$_{2/3}$O$_{3}$ are anomalously short within well-defined ranges of energy and momentum. This behavior is independent of ferroelectric order and occurs when the optical phonon with a specific energy and momentum can kinematically decay into two acoustic phonons with lower phase velocity. We interpret the well-known relaxor "waterfall" effect as a form of quasiparticle decay analogous to that previously reported in quantum spin liquids and quantum fluids.
description: (5 pages, 5 figures, to be published in Phys. Rev. Materials)
On Hyperfine Splittings of Strange Baryons in the Skyrme Model
Creators: name: Westerberg, Karl M.
name: Klebanov, Igor R.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We calculate the complete order $1/N$ corrections to baryon masses in the rigid rotator approach to the 3-flavor Skyrme model.
description: 14 pages, PUPT-1476
Additional file 1: of European Core Health Indicators - status and perspectives
Creators: name: Fehr, Angela
name: Tijhuis, Mariken
name: Hense, Sabrina
name: Urbanski, Dominika
name: Achterberg, Peter
name: Ziese, Thomas
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Biotechnology
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer
subject: Hematology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Table S1. Proportion of countries with available / unavailable / missing data in the preferred international data source (implementation section/n = 67). Table S2. Proportion of countries with available / unavailable / missing data in the preferred international data source (work-in-progress section/n = 5). (DOCX 21 kb)
Additional file 2: of Modeling of the GC content of the substituted bases in bacterial core genomes
Creators: name: Bohlin, Jon
name: Eldholm, Vegard
name: Brynildsrud, Ola
name: Petterson, John
name: Alfsnes, Kristian
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Space Science
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Evolutionary Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology

description: A detailed explanation of how sbGC and cgGC were derived in pdf-format. (PDF 190Â kb)
Possible Young Stellar Objects without Detectable CO Emission
Creators: name: Iwata, Ikuru
name: Okumura, Shin-ichiro
name: Saito, Mamoru
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We found that at least 18 Young Stellar Object candidates invisible at optical and near-infrared wavelengths, as well as ^12CO emission. They are IRAS point sources with FIR colors similar to those of usual YSOs, and the infrared spectral indices between 2.2 um and 25 um correspond to those of class I YSOs. These peculiar far-infrared objects are highly concentrated around the galactic plane and the distances are estimated to be around 1 kpc. Although their distribution is away from molecular clouds, some of them seem to be associated with large dark clouds or weak radio sources.
description: 10 pages with 4 figures, LaTeX, accepted for publication in PASJ. Images(fig2) are included in source file as JPEG files. PDF files are avilable at ftp.kusastro.kyoto-u.ac.jp/pub/iwata/preprint/
title: ADCO, Cartulaire de Cîteaux pour les possessions de Tontenant (c. 1504), Cart. 184 (11 H 987), 105 folios, f. 0167
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2015
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP

description: Cartulaire de Cîteaux pour les possessions de Tontenant (c. 1504), Archives départementales de la Côte-d'Or, Cart. 184 (11 H 987), 105 folios, f. 0167, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les possessions de Tontenant (c. 1504), Archives départementales de la Côte-d'Or, Cart. 184 (11 H 987), 105 folios, f. 0167, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
Inflammation–coagulation response and thrombotic effects induced by silica nanoparticles in zebrafish embryos
Creators: name: Duan, Junchao
name: Liang, Shuang
name: Yu, Yang
name: Li, Yang
name: Wang, Lijing
name: Wu, Zehao
name: Chen, Yueyue
name: Miller, Mark R.
name: Sun, Zhiwei
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Physiology
subject: Pharmacology
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Hematology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology

description: Nowadays, nanotechnology environmental health and safety (nanoEHS) is gaining attention. We previously found that silica nanoparticles (SiNPs) could induce vascular endothelial damage. However, the subsequent toxicologic response to SiNPs-induced endothelial damage was still largely unknown. In this study, we explored the inflammation–coagulation response and thrombotic effects of SiNPs in endothelial cells and zebrafish embryos. For in vitro study, swollen mitochondria and autophagosome were observed in ultrastructural analysis. The cytoskeleton organization was disrupted by SiNPs in vascular endothelial cells. The release of proinflammatory and procoagulant cytokines including IL-6, IL-8, MCP-1, PECAM-1, TF and vWF, were markedly elevated in a dose-dependent manner. For in vivo study, based on the NOAEL for dosimetry selection, and using two transgenic zebrafish, Tg(mpo:GFP) and Tg(fli-1:EGFP), SiNPs-induced neutrophil-mediated inflammation and impaired vascular endothelial cells. With the dosage higher than NOAEL, SiNPs significantly decreased blood flow and velocity, exhibiting a blood hypercoagulable state in zebrafish embryos. The thrombotic effect was assessed by o-dianisidine staining, showed that an increasing of erythrocyte aggregation occurred in SiNPs-treated zebrafish. Microarray analysis was used to screen the possible genes for inflammation–coagulation response to SiNPs in zebrafish, and the JAK1/TF signaling pathway was further verified by qRT-PCR and Western blot assays. For in-deepth study, il6st was knocked down with specific morpholinos. The whole-mount in situ hybridization and qRT-PCR analysis showed that the expression jak1 and f3b were attenuated in il6st knockdown groups. In summary, our data demonstrated that SiNPs could induce inflammation–coagulation response and thrombotic effects via JAK1/TF signaling pathway.
Microgreens – An Epitome of Nutritional Excellence
Creators: name: Dr. M. Dhivya1 and Dr. J. Kabariel2
Publisher: name: The Science world a Monthly e magazine
Year: 2024

description: Microgreens refer to the tiny and tender seedlings of various vegetables and herbs. These delicate greens are carefully harvested once their cotyledons, or seed leaves, have fully expanded and their first set of true leaves begin to emerge or partially expand. The size of microgreens typically ranges from 1 to 3 inches (2.5−7.6 cm) in height, which generally occurs around 7 to 14 days after the seeds have germinated. The timing of this growth can vary depending on the specific crop, variety, and environmental conditions.
Does oral contraceptives pretreatment affect the pregnancy outcome in polycystic ovary syndrome women undergoing ART with GnRH agonist protocol?
Creators: name: Xu, Zhihui
name: Meng, Lvhe
name: Pan, Chengshuang
name: Chen, Xia
name: Huang, Xuefeng
name: Yang, Haiyan
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Medicine
subject: Cell Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Mathematical Sciences not elsewhere classified
subject: Developmental Biology
subject: Science Policy

description: This study aims to investigate whether oral contraceptive pills (OCP) pretreatment impairs pregnancy outcomes in polycystic ovary syndrome (PCOS) women undergoing GnRH agonist protocol. A total of 1025 couples underwent their first cycle of in vitro fertilization. Patients were divided into GnRH agonist protocol group (LP group) and OCP dual suppression GnRH agonist protocol group (OC-LP group). Logistic regressions were performed to estimate the risk factors affecting live birth following fresh embryo transfer between groups. Frozen–thawed embryos from the first oocyte retrieval cycle were replaced into uterus for women did not get live birth. Cumulative live birth rates between groups were compared by Kaplan–Meier survival analysis. Serum luteinizing hormone level, endometrial thickness, and live birth rate were significantly reduced in the OC-LP group in fresh cycle. Thinner endometrium, higher progesterone, and poorer embryo quality were independent risk factors for failure in getting live birth following fresh embryo transfer. However, cumulative live birth rate, medium embryo transfer attempts required to achieve live birth were comparable between groups. OCP pretreatment in GnRH agonist protocol does not seem to impair the pregnancy outcome when calculated by cumulative live birth rate in PCOS women.
Fragmentation contribution to quarkonium production in hadron collision
Creators: name: Roy, D. P.
name: Sridhar, K.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We compute the contributions due to gluon and heavy-quark fragmentation to quarkonium production at large transverse momentum in $\bar p p$ and $p p$ collisions. For inclusive $J/ψ$ production, there is a large contribution from the $g \rightarrow χ_c$ fragmentation. At large $p_T$, this is comparable to the conventional charmonium model prediction via gluon fusion at the ISR and dominates over the latter at the Tevatron energy. This may help to explain, at least partly, the large $J/ψ$ production cross-section recently observed by the CDF experiment. However, the fragmentation contribution to $ψ^{\prime}$ production is not large enough to explain the corresponding CDF data. We also present the results for $Υ$ production at ISR and Tevatron energies.
description: 9 pages + 4 figures (available upon request), Latex File, CERN-TH.7329/94, TIFR/TH/94-21
Sertularia volubilis Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Cnidaria
Hydrozoa
Leptothecata
Sertulariidae
Sertularia
Sertularia volubilis

description: Sertularia volubilis [spec. nov.]
S. denticulis secundis acutis, calycibus campanulatis dentatis, pedunculis longissimis contortis.
Ellis corall. 24. n. 21. t. 14. f. A. Corallina minima scandens, vesiculas campaniformes in summo caule lineari contorto gerens.
Habitat in Oceano.
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 811, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Recent progress in adsorptive removal of per- and poly-fluoroalkyl substances (PFAS) from water/wastewater
Creators: name: Vu, Chi Thanh
name: Wu, Tingting
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Space Science
subject: Biotechnology
subject: Environmental Sciences not elsewhere classified
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Inorganic Chemistry
subject: FOS: Chemical sciences

description: Due to chemical and physiological inertness and wide usage in nearly every aspect of our daily life, per- and poly-fluoroalkyl substances (PFAS) are now ubiquitous in the environment, including drinking water sources. As most biological and chemical destruction methods have so far shown limited efficiencies, adsorption, a simple and cost-effective treatment, is widely adopted for the removal of PFAS from water/wastewater. This paper aims to review the recent progress in PFAS adsorption using various adsorbents. The performance of different types of adsorbents, including the traditional carbonaceous materials and resins as well as the newly-synthesized minerals, biomaterials, and polymers, in PFAS removal was summarized. Furthermore, the adsorption characteristics and mechanisms were critically reviewed. Real-life adsorption applications (large-scale setups, adsorption-involved treatment trains and point-of-use/point-of-entry systems) were also examined. Learned lessons, current challenges and recommendations on future research were provided regarding results of tests in real environmental matrices, pilot and/or field scale studies of promising newly-developed adsorbents, and the improvement of the removal of alternative PFAS (mostly short-chained ones).
Atomistic Studies and Machine Learning-Based Optimization of an Electrohydrodynamic Nano-Printing System
Creators: name: Singh, Sachin Kumar
Publisher: name: University of Illinois Chicago
Year: 2025

description: Electrohydrodynamic (EHD) nanoprinting is an emerging nanofabrication technology with applications in metamaterials patterning, quantum dot LED display devices, transparent electronics, and more. During EHD nanoprinting, fluid in the form of droplets or jets with sizes in tens of nanometers are ejected from a patterning nozzle under the influence of an electric field and patterned into features over a substrate, making the method particularly suitable for high-resolution nanopatterning. To design better nanofabrication systems with improved resolution, ejection stability, and patterning speed, it is important to understand the ejection mechanism of fluids from a nanoscale nozzle under the action of electric fields. To date, most modeling studies have utilized continuum approaches and have investigated the ejection of microscale droplets/jets from macroscopic nozzles with sizes ranging from hundreds of microns to millimeter ranges. However, when the size of nozzles approaches the nanoscale regime (below 100 nm), modeling fluid flows with continuum models becomes challenging as thermal fluctuations play a major role in the breakup of jets/droplets in the nanoscale regime, and the continuum model may not predict proper breakup of the jet into droplets. To model electric field actuated deformation of fluids from nanoscale nozzles, modeling techniques are required that can incorporate thermal fluctuation of constituent fluid particles, simulate slip flow at wall boundaries, and explicitly model charge dynamics. Many-body Dissipative Particle Dynamics (MDPD) is one particle-based technique that can explicitly model charge dynamics, incorporate thermal fluctuations of particles, and accurately model slip flows at walls in a nanoscale regime. Here, we present an MDPD model for studying the electric field deformation of fluids at the nanoscale regime and examine the ejection of fluids from nanoscale nozzles for printing applications. The MDPD model is later utilized within an active learning genetic algorithm framework to optimize the design and operation of an electrohydrodynamic nanoprinting system. The modeling/optimization tools presented here will enable a better understanding of the electrohydrodynamic nanoprinting process and advance the development of prototypes for nanoprinting applications.
Uncertainty Principles Associated with the Offset Linear Canonical Transform
Creators: name: Huo, Haiye
name: Sun, Wenchang
name: Xiao, Li
Publisher: name: arXiv
Year: 2018
Subjects: subject: Signal Processing (eess.SP)
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: As a time-shifted and frequency-modulated version of the linear canonical transform (LCT), the offset linear canonical transform (OLCT) provides a more general framework of most existing linear integral transforms in signal processing and optics. To study simultaneous localization of a signal and its OLCT, the classical Heisenberg's uncertainty principle has been recently generalized for the OLCT. In this paper, we complement it by presenting another two uncertainty principles, i.e., Donoho-Stark's uncertainty principle and Amrein-Berthier-Benedicks's uncertainty principle, for the OLCT. Moreover, we generalize the short-time LCT to the short-time OLCT. We likewise present Lieb's uncertainty principle for the short-time OLCT and give a lower bound for its essential support.
description: 13 pages
Bidding Machine: Learning to Bid for Directly Optimizing Profits in Display Advertising
Creators: name: Ren, Kan
name: Zhang, Weinan
name: Chang, Ke
name: Rong, Yifei
name: Yu, Yong
name: Wang, Jun
Publisher: name: arXiv
Year: 2018
Subjects: subject: Computer Science and Game Theory (cs.GT)
subject: Computers and Society (cs.CY)
subject: Information Retrieval (cs.IR)
subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: Real-time bidding (RTB) based display advertising has become one of the key technological advances in computational advertising. RTB enables advertisers to buy individual ad impressions via an auction in real-time and facilitates the evaluation and the bidding of individual impressions across multiple advertisers. In RTB, the advertisers face three main challenges when optimizing their bidding strategies, namely (i) estimating the utility (e.g., conversions, clicks) of the ad impression, (ii) forecasting the market value (thus the cost) of the given ad impression, and (iii) deciding the optimal bid for the given auction based on the first two. Previous solutions assume the first two are solved before addressing the bid optimization problem. However, these challenges are strongly correlated and dealing with any individual problem independently may not be globally optimal. In this paper, we propose Bidding Machine, a comprehensive learning to bid framework, which consists of three optimizers dealing with each challenge above, and as a whole, jointly optimizes these three parts. We show that such a joint optimization would largely increase the campaign effectiveness and the profit. From the learning perspective, we show that the bidding machine can be updated smoothly with both offline periodical batch or online sequential training schemes. Our extensive offline empirical study and online A/B testing verify the high effectiveness of the proposed bidding machine.
description: 18 pages, 10 figures, Final version published in IEEE Transactions on Knowledge and Data Engineering (TKDE), URL: http://ieeexplore.ieee.org/document/8115218/
Spectral variation in the X-ray pulsar GX 1+4 during a low-flux episode
Creators: name: Galloway, D. K.
name: Giles, A. B.
name: Greenhill, J. G.
name: Storey, M. C.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The X-ray pulsar GX 1+4 was observed with the RXTE satellite for a total of 51ks between 1996 July 19 - 21. During this period the flux decreased smoothly from an initial mean level of ~ 6 X 10^36 erg/s to a minimum of ~ 4 X 10^35 erg/s (2-60 keV, assuming a source distance of 10 kpc) before partially recovering towards the initial level at the end of the observation. BATSE pulse timing measurements indicate that a torque reversal took place approximately 10 d after this observation. Both the mean pulse profile and the photon spectrum varied significantly. The observed variation in the source may provide important clues as to the mechanism of torque reversals. The single best-fitting spectral model was based on a component originating from thermal photons with kT ~ 1 keV Comptonised by a plasma of temperature kT \~ 7 keV. Both the flux modulation with phase during the brightest interval and the evolution of the mean spectra over the course of the observation are consistent with variations in this model component; with, in addition, a doubling of the column density nH contributing to the mean spectral change. A strong flare of duration 50 s was observed during the interval of minimum flux, with the peak flux ~ 20 times the mean level. Although beaming effects are likely to mask the true variation in Mdot thought to give rise to the flare, the timing of a modest increase in flux prior to the flare is consistent with dual episodes of accretion resulting from successive orbits of a locally dense patch of matter in the accretion disc.
description: 8 pages, 3 figures, submitted to MNRAS
Additional file 1: of Modeling of the GC content of the substituted bases in bacterial core genomes
Creators: name: Bohlin, Jon
name: Eldholm, Vegard
name: Brynildsrud, Ola
name: Petterson, John
name: Alfsnes, Kristian
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics

description: A detailed mathematical derivation of the sbGC model gcMOD in pdf-format. (PDF 458Â kb)
High-velocity clouds as dark matter in the Local Group
Creators: name: Lopez-Corredoira, M.
name: Beckman, J. E.
name: Casuso, E.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The High-Velocity Clouds (HVCs) observed in the Galactic neighbourhood, have been proposed to be remnants of the formation of the galaxies in the Local Group, having distances, and thus masses, predominantly of dark matter, considerably larger than hitherto hypothesized. This hypothesis is plausibly supported by observational evidence that their kinematical centre is the Local Group barycentre. Evolutionary models to account for the evolution of the light elements in the Galaxy demand infall of metal poor gas to the plane, which could well be supplied by these HVCs. Modelling the time dependence of this infall, taking into account that an accreting galaxy shows an increasing cross-section to the infalling clouds, and produces increasing mean infall velocities, we deduce that the HVCs must currently represent at least around one half of the total mass of the Local Group, given that the accretion rate, as inferred from chemical evolution, has not decreased significantly during the disc lifetime. This fraction is consistent with dynamical estimates of the relative masses of the Local Group as a whole and its constituent galaxies. The HVCs may thus form a significant constituent of baryonic, and of non-baryonic, dark matter.
description: 5 pages; accepted in A&A
A HARDCORE model for constraining an exoplanet's core size
Creators: name: Suissa, Gabrielle
name: Chen, Jingjing
name: Kipping, David
Publisher: name: arXiv
Year: 2018
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The interior structure of an exoplanet is hidden from direct view yet likely plays a crucial role in influencing the habitability of the Earth analogues. Inferences of the interior structure are impeded by a fundamental degeneracy that exists between any model comprising more than two layers and observations constraining just two bulk parameters: mass and radius. In this work, we show that although the inverse problem is indeed degenerate, there exists two boundary conditions that enables one to infer the minimum and maximum core radius fraction, CRFmin and CRFmax. These hold true even for planets with light volatile envelopes, but require the planet to be fully differentiated and that layers denser than iron are forbidden. With both bounds in hand, a marginal CRF can also be inferred by sampling in-between. After validating on the Earth, we apply our method to Kepler-36b and measure CRFmin = (0.50 +/- 0.07), CRFmax = (0.78 +/- 0.02), and CRFmarg = (0.64 +/- 0.11), broadly consistent with the Earth's true CRF value of 0.55. We apply our method to a suite of hypothetical measurements of synthetic planets to serve as a sensitivity analysis. We find that CRFmin and CRFmax have recovered uncertainties proportional to the relative error on the planetary density, but CRFmarg saturates to between 0.03 and 0.16 once delta rho/rho drops below 1-2 per cent. This implies that mass and radius alone cannot provide any better constraints on internal composition once bulk density constraints hit around a per cent, providing a clear target for observers.
description: fixed some typos
Detection and Photometry of Hot Horizontal Branch Stars in the Core of M32
Creators: name: Brown, Thomas M.
name: Bowers, Charles W.
name: Kimble, Randy A.
name: Sweigart, Allen V.
name: Ferguson, Henry C.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the deepest near-UV image of M32 to date, which for the first time resolves hot HB stars in an elliptical galaxy. Given the near-solar metallicity of M32, much larger than that of globular clusters, the existence of an extended HB is a striking example of the 2nd parameter effect, and, most importantly, provides direct evidence that hot HB stars and their progeny are the major contributors to the UV upturn phenomenon observed in ellipticals. Our image, obtained with STIS, detects ~8000 stars in a 25"x25" field, centered 7.7" from the galaxy nucleus. These stars span a range of 21-28 mag in the STMAG system, and in the deepest parts of the image, our catalog is reasonably complete (25%) to a magnitude of 27. The hot HB spans a range of 25-27 mag at effective temperatures hotter than 8500 K. We interpret this near-UV luminosity function with an extensive set of HB and post-HB evolutionary tracks. Although the UV-to-optical flux ratio in M32 is weak enough to be explained solely by the presence of post-AGB stars, our image conclusively demonstrates that it arises from a small fraction (~5%) of the population passing through the hot HB phase. The majority of the population presumably evolves through the red HB and subsequent post-AGB phases; however, we see far fewer UV-bright stars than expected from the lifetimes of canonical hydrogen-burning low-mass post-AGB tracks. There are several possible explanations: (1) the transition from AGB to Teff > 60000K could be much more rapid than previously thought; (2) the vast majority of the post-AGB stars could be evolving along helium-burning tracks; (3) the post-AGB stars could be surrounded by circumstellar dust during the transition from the AGB to Teff > 60000K.
description: 15 pages, Latex. 7 figures. Color plate (JPEG & PS) available at http://omri.pha.jhu.edu/~tbrown/m32nuv . Uses corrected version of emulateapj.sty and apjfonts.sty (included). Accepted for publication in ApJ
Sertularia cuscuta Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Cnidaria
Hydrozoa
Leptothecata
Sertulariidae
Sertularia
Sertularia cuscuta

description: Sertularia cuscuta [spec. nov.]
S. denticulis obsoletis, calycibus ovatis axillaribus, ramis oppositis simplicibus.
Ellis corall. 28. n. 26. t. 14. f. C. Corallina cuscutae forma minima ramosa repens, ramulis oppositis, vesiculis minutissimis ovatis confertis geniculis ramorum insidentibus.
Habitat in Oceano.
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 812, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Neutron-rich rare isotope production with stable and radioactive beams in the mass range A=40-60 at beam energy around 15 MeV/nucleon
Creators: name: Papageorgiou, A.
name: Souliotis, G. A.
name: Tshoo, K.
name: Jeong, S. C.
name: Kang, B. H.
name: Kwon, Y. K.
name: Veselsky, M.
name: Yennello, S. J.
name: Bonasera, A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: We studied the production of neutron-rich nuclides in multinucleon transfer collisions of stable and radioactive beams in the mass range A=40-60. We first presented our experimental cross section data of projectile fragments from the reaction of 40Ar(15 MeV/nucleon) with 64Ni, 58Ni and 27Al. We then compared them with calculations based on either the deep-inelastic transfer (DIT) model or the constrained molecular dynamics (CoMD) model, followed by the statistical multifragmentation model (SMM). An overall good agreement of the calculations with the experimental data is obtained. We continued with calculations of the reaction of 40Ar (15 MeV/nucleon) with 238U target and then with reactions of 48Ca (15 MeV/nucleon) with 64Ni and 238U targets. In these reactions, neutron-rich rare isotopes with large cross sections are produced. These nuclides, in turn, can be assumed to form radioactive beams and interact with a subsequent target (preferably 238U), leading to the production of extremely neutron-rich and even new isotopes (e.g. 60Ca) in this mass range. We conclude that multinucleon transfer reactions with stable or radioactive beams at the energy of around 15 MeV/nucleon offer an effective route to access extremely neutron-rich rare isotopes for nuclear structure or reaction studies.
description: 28 pages, 11 figures
$b \rightarrow sγ$ Decay in Supergravity Grand Unification and Dark Matter
Creators: name: Nath, Pran
name: Arnowitt, R.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: An analysis of the $b \rightarrow sγ$ is given in supergravity grand unification using the framework of the radiative breaking of the electro-weak symmetry under three separate sets of constraints:1) neutralino relic density does not overclose the universe,2)p-stability constraint, and 3) the combined constraints of p-stability and COBE data .For case 1 it is found that the CLEO II data on the branching ratio already imposes very strong further constraints on dark matter analyses. For case2 the branching ratio is found to lie in the range (1.5-6.3)x$10^{-4}$ and thus the data does not at present significantly limit the analyses with p-stability constraint. It is shown that improvements by a factor of 3 in the $p \rightarrow\barνK^{+}$ lifetime will reduce SUSY effects to less than O(30$\%$) of the Standard Model value.For case3,the branching ratio lies in the interval (3.1-5.3)x$10^{-4}$, and the SUSY effects lie within (-10$\%$,+50$\%$) of the SM value. Thus as experimental bounds on $B(b \rightarrow sγ)$ improve, one would need in cases 2 and 3 the next-to-leading order QCD corrections to disentangle SUSY effects.
description: 10 pages LaTeX+ 2 Figs ( hard copies available on request) CERN-TH.7214/94,NUB-TH.3093/94,CTP-TAMU-32/94
Quasi-Separatrix Layers: Refined Theory and its Application to Solar Flares
Creators: name: Titov, V. S.
name: Demoulin, P.
name: Hornig, G.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Although the analysis of observational data indicates that quasi-separatrix layers (QSLs) have to play an important role in magnetic configurations of solar flares, the corresponding theory is only at an initial stage so far. In particular, there is still a need in a proper definition of QSL. This problem is analyzed here on the basis of geometrical properties of the mapping produced by the field lines which connect photospheric areas of positive and negative magnetic polarities of active regions. In general, one can find on the photosphere a unique pair of locally perpendicular line elements at one footpoint of a given field line, so that this pair is mapped into a similar pair of elements at the other footpoint. Along the directions of these elements the field line mapping only stretches and compresses the corresponding displacements of the neighboring field-line footpoints. This fact enables us to get a remarkably clear and concise definition of QSL as a volume filled by coronal field lines for which the ratio of the corresponding stretching and compressing coefficients is anomalously large. The new definition is also compared with the ones previously introduced by other authors. The theory is applied to flare events of the so-called sigmoid-type, using an analytical model of a twisted force-free configuration. It is shown that such a configuration may contain a QSL even if genuine separatrix surfaces are absent. Identifying QSLs is an essential prerequisite for understanding the mechanism of magnetic energy release in this type of flares. It is also demonstrated that the magnetic field under study has a Hamiltonian structure, which makes it possible to reveal a geometrical reason for the appearance of QSL in this case.
description: 8 pages, 4 figures, 9-th European Meeting on Solar Physics "Magnetic fields and solar processes", Firenze, Italy, September 12-18, 1999
Topologically nontrivial black holes in Lovelock-Born-Infeld gravity
Creators: name: Farhangkhah, N.
Publisher: name: arXiv
Year: 2018
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences
subject: 83D05

description: We present the black hole solutions possessing horizon with nonconstant-curvature and additional scalar restrictions on the base manifold in Lovelock gravity coupled to Born-Infeld (BI) nonlinear electrodynamics. The asymptotic and near origin behavior of the metric is presented and we analyze different behaviors of the singularity. We find that, in contrast to the case of the black hole solutions of BI-Lovelock gravity with constant curvature horizon and Maxwell-Lovelock gravity with nonconstant horizon which has only timelike singularities, spacelike, and timelike singularities may exist for BI-Lovelock black holes with nonconstant curvature horizon. By calculating the thermodynamic quantities, we study the effects of nonlinear electrodynamics via the Born-Infeld action. Stability analysis shows that black holes with positive sectional curvature, k, possess an intermediate unstable phase and large and small black holes are stable. We see that while Ricci flat Lovelock-Born-Infeld black holes having exotic horizons are stable in the presence of Maxwell field or either Born Infeld field with large born Infeld parameter beta, unstable phase appears for smaller values of beta, and therefore nonlinearity brings in the instability.
description: 15 pages, 5 figures, accepted version by Phys. Rev. D
Metasurface Optics for Full-color Computational Imaging
Creators: name: Colburn, Shane
name: Zhan, Alan
name: Majumdar, Arka
Publisher: name: arXiv
Year: 2018
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: Conventional imaging systems comprise large and expensive optical components which successively mitigate aberrations. Metasurface optics offers a route to miniaturize imaging systems by replacing bulky components with flat and compact implementations. The diffractive nature of these devices, however, induces severe chromatic aberrations and current multi-wavelength and narrowband achromatic metasurfaces cannot support full visible spectum imaging (400-700 nm). We combine principles of both computational imaging and metasurface optics to build a system with a single metalens of NA ~ 0.45 which generates in-focus images under white light illumination. Our metalens exhibits a spectrally invariant point spread function which enables computational reconstruction of captured images with a single digital filter. This work connects computational imaging and metasurface optics and demonstrates the capabilities of combining these disciplines by simultaneously reducing aberrations and downsizing imaging systems with simpler optics.
Safety and pharmacokinetics of a biosimilar of denosumab (KN012): Phase 1 and bioequivalence study in healthy Chinese subjects
Creators: name: Zhang, Hong
name: Li, Cuiyun
name: Liu, Jingrui
name: Wu, Min
name: Li, Xiaojiao
name: Zhu, Xiaoxue
name: Li, Qianqian
name: Wang, Boguang
name: Mao, Yanhong
name: Ding, Yanhua
name: Jin, Qinglong
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Neuroscience
subject: Pharmacology
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Mental Health

description: KN012 is a proposed biosimilar candidate for the reference drug denosumab, with the brand name Prolia®. This study explored the tolerance, variability, and pharmacokinetics (PK) of denosumab and its biosimilar in healthy Chinese subjects. A randomized, double-blind, parallel, two-arm study was performed to analyze the bioequivalence of denosumab biosimilar (60 mg) compared with denosumab. The PK properties of denosumab biosimilar were similar to those of denosumab. When denosumab biosimilar was compared to denosumab, the geometric mean ratios (GMRs) of Cmax, AUC0-t, and AUC0-∞ were 98.74%, 102.54%, and 102.18%, respectively, and the 90% confidence interval was observed to be within 80–125%. The inter-subject variability ranged from 31.4% to 34.6%. Five subjects in the denosumab biosimilar group and one subject in the denosumab group were positive for anti-drug antibodies (ADAs) and negative for neutralizing antibodies (NAbs). Adverse reactions were observed in 100% (52 subjects) and 94.0% (47 subjects) of the subjects in the denosumab biosimilar and denosumab groups, respectively. Reductions in the blood calcium and phosphate levels were the most common adverse reactions. The PK characteristics were comparable for the denosumab biosimilar and denosumab groups. Their safety profiles were also similar. : The trial is registered at the Chinese Clinical Trial website (http://www.chinadrugtrials.org.cn/index.html #CTR20181231).
Additional file 1: of MuscleJ: a high-content analysis method to study skeletal muscle with a new Fiji tool
Creators: name: Mayeuf-Louchart, Alicia
name: Hardy, David
name: Thorel, Quentin
name: Roux, Pascal
name: Gueniot, Lorna
name: Briand, David
name: Mazeraud, Aurélien
name: Bouglé, Adrien
name: Shorte, Spencer
name: Staels, Bart
name: Chrétien, Fabrice
name: Duez, Hélène
name: Danckaert, Anne
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Molecular Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology

description: Supplementary tables, figures and tutorial. (PDF 2355 kb)
title: ADCO, Premier cartulaire de Saint-Étienne de Dijon (XIIe siècle), Cart. 21 (G 125), 71 folios, f. 00141
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2015
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire

description: Premier cartulaire de Saint-Étienne de Dijon (XIIe siècle), Archives départementales de la Côte-d'Or, Cart. 21 (G 125), 71 folios, f. 00141, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Premier cartulaire de Saint-Étienne de Dijon (XIIe siècle), Archives départementales de la Côte-d'Or, Cart. 21 (G 125), 71 folios, f. 00141, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
Implications for Supersymmetric Dark Matter Detection from Radiative $b$ Decays
Creators: name: Borzumati, Francesca M.
name: Drees, Manuel
name: Nojiri, Mihoko M.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We point out that combinations of parameters that predict large counting rates in experiments searching for supersymmetric dark matter often tend to predict a very large branching ratio for the inclusive decay \bsg. The recent measurement of this branching ratio, therefore, indicates that searches for supersymmetric dark matter might be even more difficult than previously anticipated.
description: 12 pp + 5 uuencoded PS figures. The new upper and lower bounds on the $\br(\bsg)$ coming from the recent measurement by the CLEO Collaboration are implemented: the results are qualitatively unchanged.
Pauli energy spectrum for twist-deformed space-time
Creators: name: Daszkiewicz, Marcin
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In this article, we define the Pauli Hamiltonian function for twist-deformed N-enlarged Newton-Hooke space-time provided in article [12]. Further, we derive its energy spectrum, i.e., we find the corresponding eigenvalues as well as the proper eigenfunctions.
description: 8 pages, Latex source, no figures
MobiDataLab D2.9 Use Cases Definition V1
Creators: name: LAUER, Johannes
name: VAN DE HOEF, Sebastian
name: CHEVALLIER, Thierry
name: DE RYCK, Didier
name: RENSO, Chiara
Publisher: name: Zenodo
Year: 2021
Subjects: emission reporting
journey plannners
MaaS
ETA
optimisation of transport flow
Open Street Map
Geodata
OSM
QGIS

description: The deliverable 2.6 is a report providing an overview on the version 1 of the use cases. The listeduse cases are a representation of the project stakeholder capabilities. Therefore, they mainly focuson established tools and existing datasets. The use cases version 1 will be used to seed the livinglabs as well as for getting into data and standards discussions.Given the heterogeneity of data, tools and interfaces, as well as potential use cases and users, thisfirst set of use cases only claims a subset of potential use cases that will be possible within thecontext of MobiDataLab.
СИНДРОМ ДАУНА - СРАВНИТЕЛЬНАЯ ХАРАКТЕРИСТИКА АНТРОПОМЕТРИЧЕСКИХ ПОКАЗАТЕЛЕЙ У ДЕТЕЙ В ПОДРОСТКОВОМ ВОЗРАСТЕ
Creators: name: Очилова, Дилором
Publisher: name: Zenodo
Year: 2024

description: Данная статья посвящена сравнительному описанию антропометрических показателей у детей с синдромом Дауна в подростковом возрасте. В отделениях Репродуктивного центра Бухарской области, охраны здоровья матери и ребенка и наследственных заболеваний представлена степень встречаемости синдрома Дауна у имеющихся детей в подростковом возрасте, а также специфическая клиника синдрома Дауна и современные методы исследования.
Spectroscopic Study of the Vela-Shrapnel
Creators: name: Tsunemi, H.
name: Miyata, E.
name: Aschenbach, B.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Several shrapnels have been detected in the vicinity of Vela SNR by the ROSAT all-sky survey. We present here the spectral properties of shrapnel `A' observed with the ASCA satellite. A prominent Si-K emission line with relatively weak emission lines from other elements have been detected, revealing that the relative abundance of Si is a few ten-times higher than those of other elements. Combining with the ROSAT PSPC results, we obtained the electron temperature, $kT_{\rm e}$, to be $0.33 \pm 0.01$ keV. The total mass of shrapnel `A' is estimated to be $\sim 0.01 M_\odot$. If it is an ejecta of a supernova explosion, the interstellar matter (ISM) would be swept up in the leading edge while the ejecta material would be peeled off in the trailing edge, which should be confirmed by future observations.
description: 19pages, 5 figures, 1 table; Accepted for Publications of the Astronomical Society of Japan
title: ADCO, Cartulaire de Cîteaux pour le prieuré de Gilly : rachat de la rente due à Saint-Germain-des-Prés (c. 1501), Cart. 194 (11 H 636), 64 folios, f. 0073
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2015
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire

description: Cartulaire de Cîteaux pour le prieuré de Gilly : rachat de la rente due à Saint-Germain-des-Prés (c. 1501), Archives départementales de la Côte-d'Or, Cart. 194 (11 H 636), 64 folios, f. 0073, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour le prieuré de Gilly : rachat de la rente due à Saint-Germain-des-Prés (c. 1501), Archives départementales de la Côte-d'Or, Cart. 194 (11 H 636), 64 folios, f. 0073, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261