cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Planetary population synthesis
Creators: name: Mordasini, Christoph
Publisher: name: arXiv
Year: 2018
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: In stellar astrophysics, the technique of population synthesis has been successfully used for several decades. For planets, it is in contrast still a young method which only became important in recent years because of the rapid increase of the number of known extrasolar planets, and the associated growth of statistical observational constraints. With planetary population synthesis, the theory of planet formation and evolution can be put to the test against these constraints. In this review of planetary population synthesis, we first briefly list key observational constraints. Then, the work flow in the method and its two main components are presented, namely global end-to-end models that predict planetary system properties directly from protoplanetary disk properties and probability distributions for these initial conditions. An overview of various population synthesis models in the literature is given. The sub-models for the physical processes considered in global models are described: the evolution of the protoplanetary disk, the planets' accretion of solids and gas, orbital migration, and N-body interactions among concurrently growing protoplanets. Next, typical population synthesis results are illustrated in the form of new syntheses obtained with the latest generation of the Bern model. Planetary formation tracks, the distribution of planets in the mass-distance and radius-distance plane, the planetary mass function, and the distributions of planetary radii, semimajor axes, and luminosities are shown, linked to underlying physical processes, and compared with their observational counterparts. We finish by highlighting the most important predictions made by population synthesis models and discuss the lessons learned from these predictions - both those later observationally confirmed and those rejected.
description: 47 pages, 12 figures. Invited review accepted for publication in the 'Handbook of Exoplanets', planet formation section, section editor: Ralph Pudritz, Springer reference works, Juan Antonio Belmonte and Hans Deeg, Eds
Additional file 13 of Metabolic stimulation-elicited transcriptional responses and biosynthesis of acylated triterpenoids precursors in the medicinal plant Helicteres angustifolia
Creators: name: Huang, Yuying
name: An, Wenli
name: Yang, Zerui
name: Xie, Chunzhu
name: Liu, Shanshan
name: Zhan, Ting
name: Pan, Huaigeng
name: Zheng, Xiasheng
Publisher: name: figshare
Year: 2022
Subjects: subject: Biochemistry
subject: Pharmacology
subject: Environmental Sciences not elsewhere classified
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer

description: Additional file 13: Table S2. Primers for amplification of ten putative genes.
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IV, Cart. 188 (11 H 73), f. 0154v
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/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IV, Archives départementales de la Côte-d'Or, Cart. 188 (11 H 73), f. 0154v, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IV, Archives départementales de la Côte-d'Or, Cart. 188 (11 H 73), f. 0154v, 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
Ichneumon culpatorius Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eulophidae
Ichneumon
Ichneumon culpatorius

description: Ichneumon culpatorius [spec. nov.]
I. scutello flavicante, thorace maculato, abdominis segmento secundo tertioque ferrugineis, reliquis nigris.
Habitat in Europa.
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 561, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Losses in plasmonics: from mitigating energy dissipation to embracing loss-enabled functionalities
Creators: name: Boriskina, Svetlana V.
name: Cooper, Thomas Alan
name: Zeng, Lingping
name: Ni, George
name: Tong, Jonathan K.
name: Tsurimaki, Yoichiro
name: Huang, Yi
name: Meroueh, Laureen
name: Mahan, Gerald
name: Chen, Gang
Publisher: name: arXiv
Year: 2018
Subjects: subject: Optics (physics.optics)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: Applied Physics (physics.app-ph)
subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: Unlike conventional optics, plasmonics enables unrivalled concentration of optical energy well beyond the diffraction limit of light. However, a significant part of this energy is dissipated as heat. Plasmonic losses present a major hurdle in the development of plasmonic devices and circuits that can compete with other mature technologies. Until recently, they have largely kept the use of plasmonics to a few niche areas where loss is not a key factor, such as surface enhanced Raman scattering and biochemical sensing. Here, we discuss the origin of plasmonic losses and various approaches to either minimize or mitigate them based on understanding of fundamental processes underlying surface plasmon modes excitation and decay. Along with the ongoing effort to find and synthesize better plasmonic materials, optical designs that modify the optical powerflow through plasmonic nanostructures can help in reducing both radiative damping and dissipative losses of surface plasmons. Another strategy relies on the development of hybrid photonic-plasmonic devices by coupling plasmonic nanostructures to resonant optical elements. Hybrid integration not only helps to reduce dissipative losses and radiative damping of surface plasmons, but also makes possible passive radiative cooling of nano-devices. Finally, we review emerging applications of thermoplasmonics that leverage Ohmic losses to achieve new enhanced functionalities. The most successful commercialized example of a loss-enabled novel application of plasmonics is heat-assisted magnetic recording. Other promising technological directions include thermal emission manipulation, cancer therapy, nanofabrication, nano-manipulation, plasmon-enabled material spectroscopy and thermo-catalysis, and solar water treatment.
description: 43 pages, 18 figures
A comment on 'Testing Goodwin: growth cycles in ten OECD countries'
Creators: name: Grasselli, Matheus R.
name: Maheshwari, Aditya
Publisher: name: arXiv
Year: 2018
Subjects: subject: Econometrics (econ.EM)
subject: General Economics (econ.GN)
subject: FOS: Economics and business

description: We revisit the results of Harvie (2000) and show how correcting for a reporting mistake in some of the estimated parameter values leads to significantly different conclusions, including realistic parameter values for the Philips curve and estimated equilibrium employment rates exhibiting on average one tenth of the relative error of those obtained in Harvie (2000).
description: 8 pages, Cambridge Journal of Economics 2017
Ichneumon volutatorius Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eulophidae
Ichneumon
Ichneumon volutatorius

description: Ichneumon volutatorius [spec. nov.]
I. scutello flavicante, thorace variegato, abdominis segmentis omnibus dorso flavis.
Habitat in Europa.
Pedes rufi.
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 562, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
The Pan-STARRS1 Proper-motion Survey for Young Brown Dwarfs in Nearby Star-forming Regions. I. Taurus Discoveries and a Reddening-free Classification Method for Ultracool Dwarfs
Creators: name: Zhang, Zhoujian
name: Liu, Michael C.
name: Best, William M. J.
name: Magnier, Eugene A.
name: Aller, Kimberly M.
name: Chambers, K. C.
name: Draper, P. W.
name: Flewelling, H.
name: Hodapp, K. W.
name: Kaiser, N.
name: Kudritzki, R. -P.
name: Metcalfe, N.
name: Wainscoat, R. J.
name: Waters, C.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We are conducting a proper-motion survey for young brown dwarfs in the Taurus-Auriga molecular cloud based on the Pan-STARRS1 3$π$ Survey. Our search uses multi-band photometry and astrometry to select candidates, and is wider (370 deg$^{2}$) and deeper (down to $\approx$3 M$_{\rm Jup}$) than previous searches. We present here our search methods and spectroscopic follow-up of our high-priority candidates. Since extinction complicates spectral classification, we have developed a new approach using low-resolution ($R \approx 100$) near-infrared spectra to quantify reddening-free spectral types, extinctions, and gravity classifications for mid-M to late-L ultracool dwarfs ($\approx 100-3$ M$_{\rm Jup}$ in Taurus). We have discovered 25 low-gravity (VL-G) and the first 11 intermediate-gravity (INT-G) substellar (M6-L1) members of Taurus, constituting the largest single increase of Taurus brown dwarfs to date. We have also discovered 1 new Pleiades member and 13 new members of the Perseus OB2 association, including a candidate very wide separation (58 kAU) binary. We homogeneously reclassify the spectral types and extinctions of all previously known Taurus brown dwarfs. Altogether our discoveries have thus far increased the substellar census in Taurus by $\approx 40\%$ and added three more L-type members ($\approx 5-10$ M$_{\rm Jup}$). Most notably, our discoveries reveal an older ($>$10 Myr) low-mass population in Taurus, in accord with recent studies of the higher-mass stellar members. The mass function appears to differ between the younger and older Taurus populations, possibly due to incompleteness of the older stellar members or different star formation processes.
description: ApJ, in press. 95 pages, 40 figures, 14 tables. Machine-readable tables are available. For a brief video explaining about this paper, see https://youtu.be/yMd1OknJj7w
Ab initio Pseudopotential Plane-wave Calculations of the Electronic Structure of YBa_2Cu_3O_7
Creators: name: Kim, Hanchul
name: Ihm, Jisoon
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We present an ab initio pseudopotential local density functional calculation for stoichiometric high-Tc cuprate YBa_2Cu_3O_7 using the plane-wave basis set. We have overcome well-known difficulties in applying pseudopotential methods to first-row elements, transition metals, and rare-earth materials by carefully generating norm-conserving pseudopotentials with excellent transferability and employing an extremely efficient iterative diagonalization scheme optimized for our purpose. The self-consistent band structures, the total and site-projected densities of states, the partial charges and their symmetry-decompositions, and some characteristic charge densities near E_f are presented. We compare our results with various existing (F)LAPW and (F)LMTO calculations and establish that the ab initio pseudopotential method is competitive with other methods in studying the electronic structure of such complicated materials as high-Tc cuprates. [8 postscript files in uuencoded compressed form]
description: 14 pages, RevTeX v3.0, 8 figures (appended in postscript file), SNUTP 94-89
Pyrenacantha acuminata Engl.
Creators: name: Rio, Cédric Del
name: Stull, Gregory W.
name: Franceschi, Dario De
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Icacinales
Icacinaceae
Pyrenacantha
Pyrenacantha acuminata

description: Pyrenacantha acuminata Engl.
Fig. 23.10–23.18
Material examined
Specimen used for endocarp and fruit description
CENTRAL AFRICAN REPUBLIC • Boukoko; 18 Apr. 1951; R.P. Tisserant 2085; P [MNHN-P-P04495460].
Other material
CAMEROON • 1968; R. Letouzey 9166; P [MNHN-P-P04495454].
COUNTRY UNKNOWN • s. loc.; 18 May 1900; s. col. 1863; P [MNHN-P-P04495455].
Description
FRUIT. Elliptical, acuminate and accrescent at the apex. Epicarp puberulent, with yellow simple hairs with granular ornamentation, ridged when dry, revealing the underlying endocarp ridges. Mesocarp 192–612 µm thick when dry. Calyx persistent. Length 12–17 mm, width 8–12 mm, thickness 4–8 mm.
ENDOCARP. Brown, elliptical in lateral view, lenticular in transverse section, length ca 11 mm, width ca 8.4 mm, thickness ca 5.5 mm. Keel surrounding the endocarp in the plane of symmetry. Apex slightly asymmetrical and acute in lateral view; base rounded, symmetrical. Outer surface of the endocarp pitted and ridged. Pits circular and thin, ca 0.2–0.3 mm in diameter, randomly arranged with 8–11 pits longitudinally and 8–9 pits transversally (ca 93–106 pits per face). Pits associated with spiny tubercles protruding into the locule; tubercles ca 983–1718 µm in length and 352–456 µm in diameter at the base, with 17–18 cells spanning the width. Tubercle cells sclerotic, digitate and elongate. Ridges rounded and thin, more or less diffuse, faintly apparent, with a prominent median ridge running longitudinally from the base up to the apex. Endocarp wall 243–302 µm thick (excluding pits). Endocarp wall (excluding pits) with three cell layers: outermost layer composed of 1–2 rows of isodiametric to periclinally oriented cells, cells 11.8–20.1 µm in width, middle layer with 9–11 rows of periclinally oriented cells, cells 7.0– 35.6 µm in width; innermost layer with one row of periclinally oriented cells, cells 9.16–17.0 µm in width, lining the locule surface with inflated to papillate cells. Locule not lacunate.
description: Published as part of Rio, Cédric Del, Stull, Gregory W. & Franceschi, Dario De, 2020, Survey of the fruits and endocarps of Icacinaceae (Lamiids, Icacinales), pp. 1-130 in European Journal of Taxonomy 645 on page 71, DOI: 10.5852/ejt.2020.645, http://zenodo.org/record/3829651
Anomalous Spectral Characteristics of Ultrathin sub-nm Colloidal CdSe Nanoplatelets
Creators: name: Bose, Sumanta
name: Delikanli, Savas
name: Yeltik, Aydan
name: Sharma, Manoj
name: Erdem, Onur
name: Dang, Cuong
name: Fan, Weijun
name: Zhang, Dao Hua
name: Demir, Hilmi Volkan
Publisher: name: arXiv
Year: 2018
Subjects: subject: Applied Physics (physics.app-ph)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We demonstrate high quantum yield broad photoluminescence emission of ultrathin sub-nanometer CdSe nanoplatelets (two-monolayer). They also exhibit polarization-characterized lateral size dependent anomalous heavy hole and light/split-off hole absorption intensities.
description: Published in Conference on Lasers and Electro-Optics (CLEO): Science and Innovations 2017, San Jose, CA, USA, 14-19 May 2017 (2 pages, 3 figures)
SUT ACHITUVCHI BAKTERIYALARNING ANTIOKSIDANT FAOLLIGI
Creators: name: Abdulaxadova, G.Sh
Publisher: name: Zenodo
Year: 2024

description: Yuqori antioksidant faollikka ega bo'lgan probiotik sut achituvchi bakteriyalar  mezbon organizmni pathogen mikroorganizmlarning toksik ta'siridan himoya qila oladi va  kandidoz, yurak-qon tomir, yallig'lanish, onkologik kasalliklarning oldini olishga hissa qo'shadi. Tajribalarimiz davomida Pediococcus acidilactici 1G, Pediococcus acidilactici 2G, Lactiplantibacillus plantarum 3G, Levilactobacillus brevis 4G, Levilactobacillus brevis 6G, Lactobacillus fermentum LF1, Pediococcus acidilactici P1 shtammlarini antioksidantlik faolligi aniqlandi.
Ichneumon luctatorius Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eulophidae
Ichneumon
Ichneumon luctatorius

description: Ichneumon luctatorius [spec. nov.]
I. scutello flavicante, thorace maculato, abdominis segmento secundo tertioque luteis.
Habitat in Europa.
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 562, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Observation of contemporaneous optical radiation from a gamma-ray burst
Creators: name: Akerlof, C.
name: Balsano, R.
name: Barthelmy, S.
name: Bloch, J.
name: Butterworth, P.
name: Casperson, D.
name: Cline, T.
name: Fletcher, S.
name: Frontera, F.
name: Gisler, G.
name: Heise, J.
name: Hills, J.
name: Kehoe, R.
name: Lee, B.
name: Marshall, S.
name: McKay, T.
name: Miller, R.
name: Piro, L.
name: Priedhorsky, W.
name: Szymanski, J.
name: Wren, J.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The origin of gamma-ray bursts (GRBs) has been enigmatic since their discovery. The situation improved dramatically in 1997, when the rapid availability of precise coordinates for the bursts allowed the detection of faint optical and radio afterglows - optical spectra thus obtained have demonstrated conclusively that the bursts occur at cosmological distances. But, despite efforts by several groups, optical detection has not hitherto been achieved during the brief duration of a burst. Here we report the detection of bright optical emission from GRB990123 while the burst was still in progress. Our observations begin 22 seconds after the onset of the burst and show an increase in brightness by a factor of 14 during the first 25 seconds; the brightness then declines by a factor of 100, at which point (700 seconds after the burst onset) it falls below our detection threshold. The redshift of this burst, approximately 1.6, implies a peak optical luminosity of 5 times 10^{49} erg per second. Optical emission from gamma-ray bursts has been generally thought to take place at the shock fronts generated by interaction of the primary energy source with the surrounding medium, where the gamma-rays might also be produced. The lack of a significant change in the gamma-ray light curve when the optical emission develops suggests that the gamma-rays are not produced at the shock front, but closer to the site of the original explosion.
description: 10 pages, 2 figures. Accepted for publication in Nature. For additional information see http://www.umich.edu/~rotse/
NICMOS Observations of Luminous and Ultraluminous Infrared Galaxies
Creators: name: Evans, A. S.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: HST NICMOS observations of a sample of 24 luminous (LIGs: L_(IR) [8-1000 microns] = 10^(11.0-11.99) L_sun) and ultraluminous (ULIGs: L_(IR) > 10^(12.0) L_sun) infrared galaxies are presented. The observations provide, for the first time, high resolution HST imaging of the imbedded 1.1 - 2.2 micron nuclear regions of these mergers. All but one of the ULIGs are observed to have at least one compact (50-200 pc) nucleus, and more than half contain what appear to be blue star clusters. The warm infrared galaxies (i.e., the transition sources) are observed to have bright nuclei which account for most of the light of the galaxy. This, combined with the tendency for the light of ULIGs to become more centrally concentrated as a function of increasing wavelength, implies that most of their energy is generated within a region 50-200 pc across.
description: LaTex, 6 pages with 1 postscript and 1 jpg figure, and 1 postscript table, To appear in the proc. of the Ringberg workshop on "Ultraluminous Galaxies: Monsters or Babies" (Ringberg castle, Sept. 1998), Ap&SS, in press
Additional file 1: of Descriptive epidemiology and outcomes of bone sarcomas in adolescent and young adult patients in Japan
Creators: name: Fukushima, Takashi
name: Ogura, Koichi
name: Akiyama, Toru
name: Takeshita, Katsushi
name: Kawai, Akira
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer

description: Tumor size by age and sarcoma type. (DOCX 23 kb)
Pyrenacantha ambrensis Labat, El-Achkar & R. Rabev.
Creators: name: Rio, Cédric Del
name: Stull, Gregory W.
name: Franceschi, Dario De
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Icacinales
Icacinaceae
Pyrenacantha
Pyrenacantha ambrensis

description: Pyrenacantha ambrensis Labat, El-Achkar & R.Rabev.
Fig. 23.19–23.27
Material examined
Specimen used for endocarp and fruit description
MADAGASCAR • 1993; O. Andrianantoanina & A. Solotiana 62; P [MNHN-P-P00440603].
Description
FRUIT. Elliptical to globose, accrescent at the apex, brown-orange when mature. Epicarp puberulent with yellow small ovoid hairs with an acuminate apex and simple hairs with granular ornamentation, shriveled when dry. Mesocarp 480–500 µm thick when dry. Calyx persistent, separated from the fruit by an extended gynophore. Length 25–30 mm, width 19–22 mm, thickness 15.0– 16.6 mm.
ENDOCARP. Brown, elliptical to globose in lateral view, globose in transverse section, length ca 22.5 mm, width ca 17 mm, thickness ca 15 mm. Trace of keel present in the upper part. Apex with acute protuberance, asymmetrical in lateral view; base rounded, symmetrical. Outer surface of the endocarp pitted. Pits circular, occasionally elongated longitudinally, 0.4–1.4 mm in length, randomly arranged with 11–12 pits longitudinally and 12–15 pits transversally (ca 145–150 pits per face). Pits associated with spiny tubercles protruding into the locule; tubercles ca 3–4 mm in length and 647–931 µm in diameter at the base, faintly capitate at the apex, with 26–27 cells in width. Tubercle cells sclerotic, digitate and elongate. Endocarp wall 569–601 µm thick (excluding pits). Endocarp wall (excluding pits) with three cell layers: outermost layer with 8–14 rows of anticlinally oriented cells, cells 17.8–50.5 µm in length, followed by a layer with 3–9 rows of periclinally oriented cells, cells 17.7–23.7 µm in width; innermost layer with one row of periclinally oriented cells, cells 0.5–1.4 µm in width, lining the locule surface with regularly spaced and sessile rounded papillae; papillae 7.6–13.1 µm (av. 10.6 µm) in diameter, with ca 1000 papillae per 0.25 mm 2. Locule surface not lacunate.
Remarks
The innermost row of periclinally oriented cells, which have a small width, could be collapsed due to a dryness inside the locule.
description: Published as part of Rio, Cédric Del, Stull, Gregory W. & Franceschi, Dario De, 2020, Survey of the fruits and endocarps of Icacinaceae (Lamiids, Icacinales), pp. 1-130 in European Journal of Taxonomy 645 on pages 71-72, DOI: 10.5852/ejt.2020.645, http://zenodo.org/record/3829651
Additional file 1 of Sexually transmitted infections in the non-European Union and European Economic Area of the World Health Organization European Region 2021–2023
Creators: name: Otani, Machiko
name: Rowley, Jane
name: Grankov, Viatcheslav
name: Kuchukhidze, Giorgi
name: Bivol, Stela
Publisher: name: figshare
Year: 2025
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Supplementary Material 1.
Fractonic line excitations : an inroad from 3d elasticity theory
Creators: name: Pai, Shriya
name: Pretko, Michael
Publisher: name: arXiv
Year: 2018
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We demonstrate the existence of a fundamentally new type of excitation, fractonic lines, which are line-like excitations with the restricted mobility properties of fractons. These excitations, described using an amalgamation of higher-form gauge theories with symmetric tensor gauge theories, see direct physical realization as the topological lattice defects of ordinary three-dimensional quantum crystals. Starting with the more familiar elasticity theory, we show how it maps onto a rank-4 tensor gauge theory, with phonons corresponding to gapless gauge modes and disclination defects corresponding to line-like charges. We derive flux conservation laws which lock these line-like excitations in place, analogous to the higher moment charge conservation laws of fracton theories. This way of encoding mobility restrictions of lattice defects could shed light on melting transitions in three dimensions. This new type of extended object may also be a useful tool in the search for improved quantum error-correcting codes in three dimensions.
Thermally Activated Deviations from Quantum Hall Plateaus
Creators: name: Fogler, M. M.
name: Shklovskii, B. I.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: The Hall conductivity $σ_{\rm xy}$ of a two-dimensional electron system is quantized in units of $e^2/h$ when the Fermi level is located in the mobility gap between two Landau levels. We consider the deviation of $σ_{\rm xy}$ from a quantized value caused by the thermal activation of electrons to the extended states for the case of a long range random potential. This deviation is of the form $σ_{\rm xy}^*\exp(-Δ/T)$. The prefactor $σ_{\rm xy}^*$ is equal to $e^2/h$ at temperatures above a characteristic temperature $T_2$. With the temperature decreasing below $T_2$, $σ_{\rm xy}^*$ decays according to a power law: $σ_{\rm xy}^* = \frac{e^2}{h}(T/T_2)^γ$. Similar results are valid for a fractional Hall plateau near filling factor $p/q$ if $e$ is replaced by the fractional charge $e/q$.
description: 4 pages in PostScript (figures included)
Coefficient of Thermal Expansion Balancing for Field Assisted Bonding of Silicon to Glass
Creators: name: Sinev, Leonid S.
name: Ryabov, Vladimir T.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Applied Physics (physics.app-ph)
subject: FOS: Physical sciences

description: Stresses caused by thermal expansion coefficients mismatch of anodically bonded glass and silicon samples are studied. An analytical model to determine graphically the optimum bonding temperature is presented. It is essentially a model for thin-film stress but uses integration of the linear coefficient of thermal expansion difference between the bonding temperature and the working temperature. Recommendations for choosing the bonding temperature of silicon to two brands of glass (Corning 7740 and LK5) are made. Keywords: anodic bonding, field assisted bonding, thermal expansion, stress.
description: Accepted manuscript. 6 pages, 4 figures (with subfigures), written in russian language
Additional file 1 of History of anemia and long-term mortality due to infection: a cohort study with 12 years follow-up in South Korea
Creators: name: Oh, Tak Kyu
name: Song, Kyung-Ho
name: Song, In-Ae
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: Science Policy

description: Additional file 1.
Ichneumon saturatorius Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eulophidae
Ichneumon
Ichneumon saturatorius

description: Ichneumon saturatorius [spec. nov.]
I. scutello flavicante, thorace maculato, abdominis nigri segmento ultimo albido.
De Geer. ins. 1. t. 23. f. 16.
Habitat in Europa.
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 561, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Additional file 2 of History of anemia and long-term mortality due to infection: a cohort study with 12 years follow-up in South Korea
Creators: name: Oh, Tak Kyu
name: Song, Kyung-Ho
name: Song, In-Ae
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: Science Policy

description: Additional file 2.
Massive Accretion Disks
Creators: name: Scoville, N. Z.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Recent high resolution near infrared (HST-NICMOS) and mm-interferometric imaging have revealed dense gas and dust accretion disks in nearby ultra-luminous galactic nuclei. In the best studied ultraluminous IR galaxy, Arp 220, the 2 micron imaging shows dust disks in both of the merging galactic nuclei and mm-CO line imaging indicates molecular gas masses approx. 10^9 M_sun for each disk. The two gas disks in Arp 220 are counterrotating and their dynamical masses are approx. 2x10^9 M_sun, that is, only slightly larger than the gas masses. These disks have radii approx 100 pc and thickness 10-50 pc. The high brightness temperatures of the CO lines indicate that the gas in the disks has area filling factors of approx. 25-50% and mean densities of >~ 10^4 cm^(-3). Within these nuclear disks, the rate of massive star formation is undoubtedly prodigious and, given the high viscosity of the gas, there will also be high radial accretion rates, perhaps >~ 10 M_sun/yr. If this inflow persists to very small radii, it is enough to feed even the highest luminosity AGNs.
description: LaTex, 6 pages with 1 postscript and 1 jpg figure, and 1 postscript table, To appear in the proc. of the Ringberg workshop on "Ultraluminous Galaxies: Monsters or Babies" (Ringberg castle, Sept. 1998), Ap&SS, in press
The impact of feedback and the hot halo on the rates of gas accretion onto galaxies
Creators: name: Correa, Camila A.
name: Schaye, Joop
name: van de Voort, Freeke
name: Duffy, Alan R.
name: Wyithe, J. Stuart B.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We investigate the physics that drives the gas accretion rates onto galaxies at the centers of dark matter haloes using the EAGLE suite of hydrodynamical cosmological simulations. We find that at redshifts $z{\le}2$ the accretion rate onto the galaxy increases with halo mass in the halo mass range $10^{10}-10^{11.7}M_{\odot}$, flattens between the halo masses $10^{11.7}-10^{12.7}M_{\odot}$, and increases again for higher-mass haloes. However, the galaxy gas accretion does not flatten at intermediate halo masses when AGN feedback is switched off. To better understand these trends, we develop a physically motivated semi-analytic model of galaxy gas accretion. We show that the flattening is produced by the rate of gas cooling from the hot halo. The ratio of the cooling radius and the virial radius does not decrease continuously with increasing halo mass as generally thought. While it decreases up to ${\sim}10^{13}M_{\odot}$ haloes, it increases for higher halo masses, causing an upturn in the galaxy gas accretion rate. This may indicate that in high-mass haloes AGN feedback is not sufficiently efficient. When there is no AGN feedback, the density of the hot halo is higher, the ratio of the cooling and virial radii does not decrease as much and the cooling rate is higher. Changes in the efficiency of stellar feedback can also increase or decrease the accretion rates onto galaxies. The trends can plausibly be explained by the re-accretion of gas ejected by progenitor galaxies and by the suppression of black hole growth, and hence AGN feedback, by stellar feedback.
description: 17 pages, 9 figures. Accepted for publication in MNRAS. Comments welcome
MPEC 2025-H18 : 2024 TN1
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2025
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
Exact solution of a one-dimensional fermion model with interchain tunneling
Creators: name: Bariev, R. Z.
name: Klümper, A.
name: Schadschneider, A.
name: Zittartz, J.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: A fermion model consisting of two chains with interchain tunneling is formulated and solved exactly by the Bethe ansatz method. The interchain tunneling leads to Cooper pair like bound states and a threshold energy is required to overcome the binding energy. The correlation functions manifest superconducting properties.
description: 10 pages, 4 Postscript figures appended as uuencoded compressed tar-file to appear in PRB Rapid Communications, preprint Cologne-94-4743
Pyrenacantha capitata H. Perrier 1944
Creators: name: Rio, Cédric Del
name: Stull, Gregory W.
name: Franceschi, Dario De
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Icacinales
Icacinaceae
Pyrenacantha
Pyrenacantha capitata

description: Pyrenacantha capitata H.Perrier
Fig. 24.18–24.26
Material examined
Specimen used for endocarp and fruit description
MADAGASCAR • 2002; F. Ratovoson et al. 678; P [MNHN-P-P00440639].
Other material
MADAGASCAR • 2005; T. Andriamihajarivo et al. 638; P [MNHN-P-P06807829].
Description
FRUIT. Elliptical, slightly accrescent at the apex. Epicarp pilose with yellow long and thin hairs, shriveled when dry. Mesocarp 360–400 µm thick when dry. Calyx persistent. Length 17–21 mm, width 8–12 mm, thickness 4–6 mm.
ENDOCARP. Cream, elliptical in lateral view, lenticular in transverse section, length ca 17.1 mm, width ca 10.4 mm, thickness ca 4.5 mm. Trace of keel present in the upper part. Apex with acute protuberance but flattened laterally, asymmetrical in lateral view; base rounded, symmetrical. Outer surface of the endocarp pitted and ridged with only 1–2 longitudinal ridges present in the flattened apical part. Pits circular, occasionally elongate, 0.2–0.6 mm in diameter, more or less randomly arranged with 10–13 pits longitudinally and 8–10 pits transversally (ca 107–114 pits per face). Pits associated with spiny tubercles protruding into the locule; tubercles ca 1500 µm in length and 420–620 µm in diameter at the base, with 20–23 cells in width. Tubercle cells sclerotic, digitate and elongate. Endocarp wall 246–289 µm thick (excluding pits). Endocarp wall (excluding pits), with three cell layers: outermost layer with 4–7 rows of anticlinally oriented to isodiametric cells, cells 15.4–28.9 µm in length, followed by a layer with 9–12 rows of periclinally oriented cells, cells 10.0– 11.2 µm in width; innermost layer with one row of periclinally oriented cells, cells 5.0– 9.9 µm in width, lining the locule surface with more or less flattened cells. Locule surface not lacunate.
description: Published as part of Rio, Cédric Del, Stull, Gregory W. & Franceschi, Dario De, 2020, Survey of the fruits and endocarps of Icacinaceae (Lamiids, Icacinales), pp. 1-130 in European Journal of Taxonomy 645 on page 76, DOI: 10.5852/ejt.2020.645, http://zenodo.org/record/3829651
Laboratory Photoionization Fronts in Nitrogen Gas: A Numerical Feasibility and Parameter Study
Creators: name: Gray, William J
name: Keiter, P. A.
name: Lefevre, H.
name: Patterson, C. R.
name: Davis, J. S.
name: van Der Holst, B.
name: Powell, K. G.
name: Drake, R. P.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Photoionization fronts play a dominant role in many astrophysical situations, but remain difficult to achieve in a laboratory experiment. We present the results from a computational parameter study evaluating the feasibility of the photoionization experiment presented in the design paper by Drake, R. P., Hazak, G., Keiter, P. A., Davis, J. S., Patterson, C. R., Frank, A., Blackman, E. G., & Busquet, M. 2016, ApJ, 833, 249 in which a photoionization front is generated in a nitrogen medium . The nitrogen gas density and the Planckian radiation temperature of the x-ray source define each simulation. Simulations modeled experiments in which the x-ray flux is generated by a laser-heated gold foil, suitable for experiments using many kJ of laser energy, and experiments in which the flux is generated by a "z-pinch" device, which implodes a cylindrical shell of conducting wires. The models are run using CRASH, our block-adaptive-mesh code for multi-material radiation hydrodynamics. The radiative transfer model uses multi-group, flux-limited diffusion with thirty radiation groups. In addition, electron heat conduction is modeled using a single-group, flux-limited diffusion. In the theory, a photoionization front can exist only when the ratios of the electron recombination rate to the photoionization rate and the electron impact ionization rate to the recombination rate lie in certain ranges. These ratios are computed for several ionization states of nitrogen. Photoionization fronts are found to exist for laser driven models with moderate nitrogen densities ($\sim$10$^{21}$ cm$^{-3}$) and radiation temperatures above 90 eV. For "z-pinch" driven models, lower nitrogen densities are preferred ($
description: 22 pages, 14 figures, comments welcome
title: ADCO, Cartulaire de Cîteaux pour les domaines de Saint-Jean de Losne et Losne (XVIIIe siècle), Cart. 198-01 (11 H 1055), 185 folios, f. 0113
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/2019
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: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Cartulaire de Cîteaux pour les domaines de Saint-Jean de Losne et Losne (XVIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 198-01 (11 H 1055), 185 folios, f. 0113, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les domaines de Saint-Jean de Losne et Losne (XVIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 198-01 (11 H 1055), 185 folios, f. 0113, 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
Values of H_0 from Models of the Gravitational Lens 0957+561
Creators: name: Bernstein, Gary
name: Fischer, Philippe
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The lensed double QSO 0957+561 has a well-measured time delay and hence is useful for a global determination of H0. Uncertainty in the mass distribution of the lens is the largest source of uncertainty in the derived H0. We investigate the range of \hn produced by a set of lens models intended to mimic the full range of astrophysically plausible mass distributions, using as constraints the numerous multiply-imaged sources which have been detected. We obtain the first adequate fit to all the observations, but only if we include effects from the galaxy cluster beyond a constant local magnification and shear. Both the lens galaxy and the surrounding cluster must depart from circular symmetry as well. Lens models which are consistent with observations to 95% CL indicate H0=104^{+31}_{-23}(1-\kthirty) km/s/Mpc. Previous weak lensing measurements constrain the mean mass density within 30" of G1 to be kthirty=0.26+/-0.16 (95% CL), implying H0=77^{+29}_{-24}km/s/Mpc (95% CL). The best-fitting models span the range 65--80 km/s/Mpc. Further observations will shrink the confidence interval for both the mass model and \kthirty. The range of H0 allowed by the full gamut of our lens models is substantially larger than that implied by limiting consideration to simple power law density profiles. We therefore caution against use of simple isothermal or power-law mass models in the derivation of H0 from other time-delay systems. High-S/N imaging of multiple or extended lensed features will greatly reduce the H0 uncertainties when fitting complex models to time-delay lenses.
description: AASTEX, 48 pages 4 figures, 2 tables. Also available at: http://www.astro.lsa.umich.edu:80/users/philf/www/papers/list.html
Phase Separation of Crystal Surfaces: A Lattice Gas Approach
Creators: name: Shore, Joel D.
name: Bukman, Dirk Jan
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We consider both equilibrium and kinetic aspects of the phase separation (``thermal faceting") of thermodynamically unstable crystal surfaces into a hill--valley structure. The model we study is an Ising lattice gas for a simple cubic crystal with nearest--neighbor attractive interactions and weak next--nearest--neighbor repulsive interactions. It is likely applicable to alkali halides with the sodium chloride structure. Emphasis is placed on the fact that the equilibrium crystal shape can be interpreted as a phase diagram and that the details of its structure tell us into which surface orientations an unstable surface will decompose. We find that, depending on the temperature and growth conditions, a number of interesting behaviors are expected. For a crystal in equilibrium with its vapor, these include a low temperature regime with logarithmically--slow separation into three symmetrically--equivalent facets, and a higher temperature regime where separation proceeds as a power law in time into an entire one--parameter family of surface orientations. For a crystal slightly out of equilibrium with its vapor (slow crystal growth or etching), power--law growth should be the rule at late enough times. However, in the low temperature regime, the rate of separation rapidly decreases as the chemical potential difference between crystal and vapor phases goes to zero.
description: 16 pages (RevTex 3.0); 12 postscript figures available on request (shore@physics.mcgill.ca). Submitted to Physical Review E. SFU-JDSDJB-94-02
The Impact of Star Formation and Active Nuclei on the Interstellar Medium in Ultraluminous Infrared Galaxies
Creators: name: Maloney, Philip R.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The energy input into the interstellar medium in Ultraluminous Infrared Galaxies (ULIRGs) is enormous, regardless of the nature of the power source. I discuss some of the major consequences for the structure and energetics of the ISM in these galaxies. Observationally, the column densities in the nuclear regions of ULIRGs are known to be very high, which makes distinguishing starbursts from AGN quite difficult. The level of energy and momentum injection means that the pressure in the ISM must be extremely high, at least 3-4 orders of magnitude larger than in the local ISM or typical giant molecular clouds. It also means that the luminosity of GMCs in ULIRGs must be very high, as they must radiate many times their binding energy over their lifetimes. I briefly review the influence which X-ray irradiation can have on the ISM in AGN-powered ULIRGs. Finally, I show that the presence of PAH features in ULIRGs does not imply that they must be starburst-dominated, since at the column densities and pressures typical of the ISM in ULIRGs PAHs can survive even at tens of parsec distances from the AGN.
description: Invited review talk at the Ringberg Conference on Ultraluminous Galaxies; 23 pages, 5 figures; proceedings to appear in Astrophysics and Space Science (ed. D. Lutz and L. Tacconi)