cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Look for the Perfect Cell Therapy_TERMIS2018.pdf
Creators: name: O.A. Krasilnikova
name: I.D. Klabukov
name: M.V. Balyasin
name: A.V. Lyundup
Publisher: name: figshare
Year: 2018
Subjects: subject: Pathology
subject: Physiology
subject: FOS: Biological sciences

description: Background: Diabetic foot ulcer (DFU) is one of common and serious diabetes mellitus complications that affects approximately 6% of patients with diabetes1. Besides causing pain and amputation, DFU also imposes substantial economic burden on the healthcare system. Various clinical trials and meta-analysis confirmed that cell-based therapy is capable of enhancing current DFU treatment 2,3. Our objective was to perform systematic review of the research examining the effectiveness of various stem cells (SCs) types administered by different ways in order to improve DFU healing. Methods: In total, we identified 458 relevant publications in PubMed and 438 were excluded after review of content for not meeting the inclusion criteria. Efficiency of different types of stem cells were compared according to the re-epithelialization rate calculation. Results: Overall, our findings indicate that BM-MSCs can be considered as the most effective stem cell type for the treatment of DFU (p<0,05) in comparison with BM-MNCs, adipose tissue-derived stem cells (ADSCs), and peripheral blood CD34+ cells. However, BM-MSCs differ in their efficiency. Topical way of stem cells administration significantly increases the effectiveness of stem cell therapy in humans (p<0,05). No significant data about allogeneic stem cells effectiveness in comparison with autologous was actually presented in articles. Cell dosage and concentration per wound area require additional data. Conclusion: We consider that differences in BM-MSCs efficiency might be result of unequal quality of cell culture processing and isolating in different trials. In our opinion, further clinical trials are essentially required in order to discover huge potential of stem cell-based therapies and to learn more about therapeutic properties of autologous and allogeneic stem cells.
Measurement of the Bs Meson Lifetime
Creators: name: The CDF Collaboration
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The lifetime of the $B_s$ meson is measured using the semileptonic decay $B_s \to D_s^- \ell^+ νX$. The data sample consists of 19.3 pb$^{-1}$ of $p \bar{p}$ collisions at $\sqrt{s} = 1.8$ TeV collected by the CDF detector at the Fermilab Tevatron collider during 1992-1993. There are $76 \pm 8$ $\ell^{+} D_s^{-}$ signal events where the $D_s$ is identified via the decay $D_s^{-} \to ϕπ^{-}$,~$ϕ\to K^+ K^-$. Using these events, the $B_s$ meson lifetime is determined to be $τ_{s} = 1.42^{+ 0.27}_{- 0.23} {\rm (stat)} \pm 0.11 {\rm (syst)}$ ps. A measurement of the $B_s$ lifetime in a low statistics sample of exclusive $B_s \to J/ψϕ$ decays is also presented in this paper.
description: 18 pages, 3 figures (2 .ps 1 .eps)
Oniscus asilus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Isopoda
Oniscidae
Oniscus
Oniscus asilus

description: Oniscus asilus [spec. nov.]
O. abdomine foliis duobus obtecto, cauda semiovali. Mus. Ad. Fr. 1. p. 88.
Bell. aquat. 443. Asilus s. oestrum.
Rond. pisc. 576. Pediculus marinus.
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 636, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
The Bulge-Disk Orthogonal Decoupling in Galaxies: NGC 4698
Creators: name: Bertola, F.
name: Corsini, E. M.
name: Beltran, J. C. Vega
name: Pizzella, A.
name: Sarzi, M.
name: Cappellari, M.
name: Funes, J. G.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The R-band isophotal map of the Sa galaxy NGC 4698 shows that the inner region of the bulge structure is elongated perpendicularly to the major axis of the disk, this is also true for the outer parts of the bulge if a parametric photometric decomposition is adopted. At the same time the stellar component is characterized by an inner velocity gradient and a central zero-velocity plateau along the minor and major axis of the disk respectively. This remarkable geometric and kinematic decoupling suggests that a second event occurred in the formation history of this galaxy.
description: 12 pages, LaTex, with 4 PostScript figures. Accepted for publication in The Astrophysical Journal Letters
Fractal Modeling and Fractal Dimension Description of Urban Morphology
Creators: name: Chen, Yanguang
Publisher: name: arXiv
Year: 2018
Subjects: subject: Physics and Society (physics.soc-ph)
subject: FOS: Physical sciences

description: The conventional mathematical methods are based on characteristic length, while urban form has no characteristic length in many aspects. Urban area is a measure of scale dependence, which indicates the scale-free distribution of urban patterns. Thus, the urban description based on characteristic lengths should be replaced by urban characterization based on scaling. Fractal geometry is one powerful tool for scaling analysis of cities. Fractal parameters can be defined by entropy and correlation functions. However, how to understand city fractals is still a pending question. By means of logic deduction and ideas from fractal theory, this paper is devoted to discussing fractals and fractal dimensions of urban landscape. The main points of this work are as follows. First, urban form can be treated as pre-fractals rather than real fractals, and fractal properties of cities are only valid within certain scaling ranges. Second, the topological dimension of city fractals based on urban area is 0, thus the minimum fractal dimension value of fractal cities is equal to or greater than 0. Third, fractal dimension of urban form is used to substitute urban area, and it is better to define city fractals in a 2-dimensional embedding space, thus the maximum fractal dimension value of urban form is 2. A conclusion can be reached that urban form can be explored as fractals within certain ranges of scales and fractal geometry can be applied to the spatial analysis of the scale-free aspects of urban morphology.
description: 33 pages, 3 figures, 10 tables
Additional file 5 of The lungs were on fire: a pilot study of 18F-FDG PET/CT in idiopathic-inflammatory-myopathy-related interstitial lung disease
Creators: name: Liang, Junyu
name: Cao, Heng
name: Liu, Yinuo
name: Ye, Bingjue
name: Sun, Yiduo
name: Ke, Yini
name: He, Ye
name: Xu, Bei
name: Lin, Jin
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Molecular Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy
subject: Plant Biology
subject: FOS: Biological sciences

description: Additional file 5. Correlation of bilateral lung SUVmean, infection, MYOACT score and time gap after RS onset
L Dwarfs and the Substellar Mass Function
Creators: name: Reid, I. N.
name: Kirkpatrick, J. D.
name: Liebert, J.
name: Burrows, A.
name: Gizis, J. E.
name: Burgasser, A.
name: Dahn, C. C.
name: Monet, D.
name: Cutri, R.
name: Beichman, C. A.
name: Skrutskie, M.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Analysis of initial observations from near-infrared sky surveys has shown that the resulting photometric catalogues, combined with far-red optical data, provide an extremely effective method of finding isolated, very low-temperature objects in the general field. Follow-up observations have already identified more than 25 sources with temperatures cooler than the latest M dwarfs. A comparison with detailed model predictions (Burrows & Sharp) indicates that these L dwarfs have effective temperatures between ~2000\pm100 K and 1500\pm100 K, while the available trigonometric parallax data place their luminosities at between 10^{-3.5} and 10^{-4.3} L_solar. Those properties, together with the detection of lithium in one-third of the objects, are consistent with the majority having substellar masses. The mass function cannot be derived directly, since only near-infrared photometry and spectral types are available for most sources, but we can incorporate VLM/brown dwarf models in simulations of the Solar Neighbourhood population and constrain Psi(M) by comparing the predicted L-dwarf surface densities and temperature distributions against observations from the DENIS and 2MASS surveys. The data, although sparse, can be represented by a power-law mass function, Psi(M) ~ M^{-alpha}, with 1 < alpha < 2. Current results favour a value nearer the lower limit. If alpha = 1.3, then the local space density of 0.075 > M/M_solar > 0.01 brown dwarfs is 0.10 systems pc^{-3}. In that case brown dwarfs are twice as common as main-sequence stars, but contribute no more than ~15% of the total mass of the disk.
description: To appear in Astrophysical Journal (20 August 1999). 44 Pages. For related preprints, see http://www.ipac.caltech.edu/2mass/overview/ldwarfs.html
Exclusive Radiative B-Decays in the Light-Cone QCD Sum Rule Approach
Creators: name: Ali, A.
name: Braun, V. M.
name: Simma, H.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We carry out a detailed study of exclusive radiative rare $B$-decays in the framework of the QCD sum rules on the light cone, which combines the traditional QCD sum rule technique with the description of final state vector mesons in terms of the light-cone wave functions of increasing twist. The decays considered are: $B_{u,d} \to K^* +γ, B_{u,d}\to ρ+γ, B_d\to ω+γ$ and the corresponding decays of the $B_s$ mesons, $B_s\to ϕ+γ$ and $B_s\to K^*+γ$. Based on our estimate of the transition form factor $F_1^{B \to K^*\pg}(0) =0.32\pm0.05$, we find for the branching ratio $BR(B \to K^* + γ) = (4.8\pm 1.5)\times 10^{-5}$, which is in agreement with the observed value measured by the CLEO collaboration. We present detailed estimates for the ratios of the radiative decay form factors, which are then used to predict the rates for the exclusive radiative B-decays listed above. This in principle allows the extraction of the CKM matrix element $|V_{td}|$ from the penguin-dominated CKM-suppressed radiative decays when they are measured. We give a detailed discussion of the dependence of the form factors on the $b$-quark mass and on the momentum transfer, as well as their interrelation with the CKM-suppressed semileptonic decay form factors in $B\to ρ+\ell+ν$, which we also calculate in our approach.
description: 32 pages, 10 uuencoded figures, LaTeX, preprint CERN-TH 7118/93
Additional file 1 of The progression rate of spinocerebellar ataxia type 3 varies with disease stage
Creators: name: Peng, Linliu
name: Peng, Yun
name: Chen, Zhao
name: Wang, Chunrong
name: Long, Zhe
name: Peng, Huirong
name: Shi, Yuting
name: Shen, Lu
name: Xia, Kun
name: Leotti, Vanessa B.
name: Jardim, Laura Bannach
name: Tang, Beisha
name: Qiu, Rong
name: Jiang, Hong
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Cancer

description: Additional file 1. Parameter estimates, fit statistics of fitted models with sex or RAO as a fixed effect.
Cosmological Constraints on the Host Halos of GRBs
Creators: name: Xu, Wen
name: Fang, Li-Zhi
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The recently observed bright optical transients(OT) of high redshift GRBs indicate that they are in a violent dynamical state. We think it is reasonable to assume that the GRBs form in the environment of gravitationally collapsed halos of the cosmic matter field, and we investigate the basic parameters of the halos which are favored to host GRBs. If the harboring coefficient $f$ of GRBs per halo is weakly dependent on the mass of the halo, the redshift data of GRB OTs can yield significant constraints on the massive halos hosting GRBs. We show that, in the framework of popular cold dark matter (CDM) models, the GRB-favored environments are newly collapsed halos (i.e. their ages less than about $2 \times 10^9$ yr) with masses around $10^9$ $h^{-1}$ M$_{\odot}$. In this scenario, low redshift GRBs, if they exist, could not have the same cosmic origin as the high redshift ones. To fit with the observed rate of GRBs, we conclude that each GRB halo can host probably no more than one GRB event on average. This result implies that GRBs may be related to the merging of the halos.
description: AAS Latex file, 9 pages+ 3 figures, accepted for publication in ApJL
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome V, Cart. 189 (11 H 74), 316 folios, f. 0072v
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: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
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 V, Archives départementales de la Côte-d'Or, Cart. 189 (11 H 74), 316 folios, f. 0072v, 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 V, Archives départementales de la Côte-d'Or, Cart. 189 (11 H 74), 316 folios, f. 0072v, 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
The Nonperturbative Wave Functions, Transverse Momentum Distribution and QCD Vacuum Structure
Creators: name: Zhitnitsky, A.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: It is shown that there is one-to-one correspondence between two, apparently different problems: \\ 1. The determination of the meanvalues of transverse moments $\la \vec{k}_{\perp}^{2n} \ra $ for the nonperturbative pion wave function $ψ(\k, x)$ and \\ 2. The evaluation of the mixed vacuum condensates $ \la \bar{q}G_{μν}^n q\ra $. eneral properties of the theory. We define and model $ψ(\k, x)$, satisfying all these constraints.
description: 14pages, Cut down to meet Phys. Lett. space requirement and some additional references included
Detection of the Supercycle in V4140 Sagittarii: First Eclipsing ER Ursae Majoris-like Object
Creators: name: Kato, Taichi
name: Hambsch, Franz-Josef
name: Cook, Lewis M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We observed the deeply eclipsing SU UMa-type dwarf nova V4140 Sgr and established the very short supercycle of 69.7(3) d. There were several short outbursts between superoutbursts. These values, together with the short orbital period (0.06143 d), were similar to, but not as extreme as, those of ER UMa-type dwarf novae. The object is thus the first, long sought, eclipsing ER UMa-like object. This ER UMa-like nature can naturally explain the high (apparent) quiescent viscosity and unusual temperature profile in quiescence, which were claimed observational features against the thermal-tidal instability model. The apparently unusual outburst behavior can be reasonably explained by a combination of this ER UMa-like nature and the high orbital inclination and there is no need for introducing mass transfer bursts from its donor star.
description: 5 pages, 1 figure, accepted for publication in PASJ
Oniscus oestrum Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Isopoda
Oniscidae
Oniscus
Oniscus oestrum

description: Oniscus oestrum [spec. nov.]
O. abdomine foliis sex obtecto, cauda retusa. Mus. Reg. 89.
Marcgr. bras. 155. f. 3, 4. Animalculum crustaceum.
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 636, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Electric field correlation measurements on the electromagnetic vacuum state
Creators: name: Benea-Chelmus, Ileana-Cristina
name: Settembrini, Francesca Fabiana
name: Scalari, Giacomo
name: Faist, Jérôme
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Quantum mechanics ascribes to the ground state of the electromagnetic radiation zero-point electric field fluctuations that permeate empty space at all frequencies. No energy can be extracted from the ground state of a system and, therefore, these fluctuations cannot be measured directly with an intensity detector. The experimental proof of their existence came thus from more indirect evidence, such as the Lamb shift, the Casimir force between close conductors or spontaneous emission. A direct method to determine the spectral characteristics of vacuum field fluctuations has been missing so far. In this work, we perform a direct measurement of the field correlation on these fluctuations in the terahertz frequency range using electro-optic detection in a non-linear crystal placed in a cryogenic environment. We investigate their temporal and spatial coherence, which, at zero time delay and spatial distance, has a peak value of $6.2\cdot 10^{-2}~V^2/m^2$, corresponding to a fluctuating vacuum field of 0.25 V/m. With this measurement, we determine the spectral composition of the ground state of electromagnetic radiation which lies within the bandwidth of electro-optic detection.
Additional file 1 of The lungs were on fire: a pilot study of 18F-FDG PET/CT in idiopathic-inflammatory-myopathy-related interstitial lung disease
Creators: name: Liang, Junyu
name: Cao, Heng
name: Liu, Yinuo
name: Ye, Bingjue
name: Sun, Yiduo
name: Ke, Yini
name: He, Ye
name: Xu, Bei
name: Lin, Jin
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Molecular Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy
subject: Plant Biology
subject: FOS: Biological sciences

description: Additional file 1. Enrollment and groupings of IIM-ILD patients
title: ADCO, Cartulaire de Cîteaux pour les possessions de Chaugey et Maison-Dieu (Fin XVe siècle), Cart. 181 (11 H 754), 165 folios, f. 0228
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/2017
name: Petot, Frédéric
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 Chaugey et Maison-Dieu (Fin XVe siècle), Archives départementales de la Côte-d'Or, Cart. 181 (11 H 754), 165 folios, f. 0228, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les possessions de Chaugey et Maison-Dieu (Fin XVe siècle), Archives départementales de la Côte-d'Or, Cart. 181 (11 H 754), 165 folios, f. 0228, 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
X-Ray/Gamma-Ray Observations of the PSR B1259-63/SS 2883 system near Apastron
Creators: name: Hirayama, M.
name: Cominsky, L. R.
name: Kaspi, V. M.
name: Nagase, F.
name: Tavani, M.
name: Kawai, N.
name: Grove, J. E.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the results from X-ray and hard X-ray observations of the PSR B1259-63/SS 2883 system with the ASCA and CGRO satellites, performed between 1995 February and 1996 January when the pulsar was near apastron. The system was clearly detected in each of the two ASCA observations with luminosity in the 1-10 keV band of Lx = (9 +- 3) x10^32 (d/2 kpc)^2 erg/s, while CGRO/OSSE did not detect significant hard X-rays from the system. X-ray spectra obtained with ASCA are well-fit by a single power-law spectrum with a photon index of 1.6 +- 0.3. No pulsations were detected in either the ASCA or the OSSE data. We combine all existing X-ray and hard X-ray observations and present the orbital modulation in the luminosity and photon index for the entire orbit. The results are in agreement with predictions based on a synchrotron emission model from relativistic particles in a shocked pulsar wind interacting with the gaseous outflow from the Be star.
description: 14 pages, 4 figures, accepted for publicatoin in ApJ
pbarp partial wave analysis and NbarN potentials
Creators: name: de Swart, J. J.
name: Rijken, Th. A.
name: Timmermans, R.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Invited talk given at the NAN '93 Conference in Moscow, Russia, sept 1993. A review is given of the different ways to describe pbarp scattering. Next the Nijmegen partial wave analyses of the pbarp data as well as the corresponding Nijmegen NbarN database are discussed. These partial wave analyses are finally used as a tool to construct a better NbarN potential model and also to clarify questions raised in the literature.
description: 20 pages latex and 4 fig in ps, Nijmegen report THEF-NYM-94.01
Mid-infrared imaging of the young binary star Hen 3-600: Evidence for a dust disk around the primary
Creators: name: Jayawardhana, Ray
name: Hartmann, Lee
name: Fazio, Giovanni
name: Fisher, R. Scott
name: Telesco, Charles M.
name: Pina, Robert K.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present high-resolution mid-infrared observations of the nearby late-type young binary system Hen 3-600. The binary, at a distance of $\sim$ 50 pc, could be a member of the TW Hydrae Association, the nearest known group of young stars, with an age of a few million years. Our images make it possible for the first time to determine which star in the pair, separated by 1.4'', harbors the mid-infrared excess detected by IRAS. In the near-infrared, where the radiation is primarily photospheric, Hen 3-600A (M3) and Hen 3-600B (M3.5) have a flux ratio of 1.6. At 4.8$μ$m, 10.8$μ$m, and 18.2$μ$m, the primary becomes increasingly dominant over the secondary, suggesting that most of the circumstellar dust in the system resides around Hen 3-600A. Comparison of the spectral energy distribution (SED) of Hen 3-600A to the median SED of classical T Tauri stars suggests that its disk may be truncated by the secondary and provides tentative evidence for a central disk hole. The distribution of dust in the Hen 3-600 system may provide important clues to the formation and evolution of protoplanetary disks in close binaries.
description: 9 pages, 2 PostScript figures, accepted for publication in The Astrophysical Journal Letters
Roman Catholic Diocese of Varaždin (Dioecesis Varasdinum)
Creators: name: Župan, Robert
name: Frangeš, Stanislav
name: Jagetić, Jurica
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: The paper describes the research and creation of the map of the Diocese of Varaždin. After many changes in the Diocese over the years, this map has finally been completed and published for the first time. The process of the map making is described. Furthermore, it points at the problems related to some specific contents of the map and provides solutions to those problems, specifically, the divergence of the borders gathered from different sources. This extensive project resulted in the creation of a map in A2 paper format on a 1:225,000 scale. The GIS and the data collected about the specific map content were both the starting point and the source of data for the visualization of the map of the Diocese of Varaždin. This is important because there are none that precede it. Such a thematic map would therefore mark an advance in the field and be appropriate.
Oniscus psora Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Isopoda
Oniscidae
Oniscus
Oniscus psora

description: Oniscus psora [spec. nov.]
O. abdomine subtus nudo, cauda semiovali acuta.
Habitat in mari Norvegico. D. C. Solander.
Magnitudo praecedentium. Thorax segmentis 7 aequalibus. Cauda segmentis quinque angustioribus, praeter ultimum quod semiovale sed acutum. Antennae 1/4 totius longitudinis. Pedes XIV, quorum 6 primi antrorsum versi digito incurvo & affixi corpori articulo arcuato. Abdomen nudum. Cauda obtecta foliolis angustis non evidentibus.
Ovarium externe contra scabiem Specificum Norvegis. Solander.
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 636, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Infrared Candidates for the Intense Galactic X-ray Source GX 17+2
Creators: name: Deutsch, Eric W.
name: Margon, Bruce
name: Anderson, Scott F.
name: Wachter, Stefanie
name: Goss, W. M.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present new astrometric solutions and infrared Hubble Space Telescope observations of GX 17+2 (X1813-140), one of the brightest X-ray sources on the celestial sphere. Despite 30 years of intensive study, and the existence of a strong radio counterpart with a sub-arcsecond position, the object remains optically unidentified. The observed X-ray characteristics strongly suggest that it is a so-called "Z-source," the rare but important category that includes Sco X-1 and Cyg X-2. Use of the USNO-A2.0 catalog enables us to measure the position of optical and infrared objects near the radio source to sub-arcsecond precision within the International Celestial Reference Frame, for direct comparison with the radio position, which we also recompute using modern calibrators. With high confidence we eliminate the V~17.5 star NP Ser, often listed as the probable optical counterpart of the X-ray source, as a candidate. Our HST NICMOS observations show two faint objects within our 0.5" radius 90% confidence error circle. Even the brighter of the two, Star A, is far fainter than expected (H~19.8), given multiple estimates of the extinction in this field and our previous understanding of Z sources, but it becomes the best candidate for the counterpart of GX 17+2. The probability of a chance coincidence of an unrelated faint object on the radio position is high. However, if the true counterpart is not Star A, it is fainter still, and our conclusion that the optical counterpart is surprisingly underluminous is but strengthened.
description: 15 pages including 3 figures and 3 tables. Accepted for publication in The Astrophysical Journal
LensKit for Python: Next-Generation Software for Recommender System Experiments
Creators: name: Ekstrand, Michael D.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Information Retrieval (cs.IR)
subject: Artificial Intelligence (cs.AI)
subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences
subject: H.3.3

description: LensKit is an open-source toolkit for building, researching, and learning about recommender systems. First released in 2010 as a Java framework, it has supported diverse published research, small-scale production deployments, and education in both MOOC and traditional classroom settings. In this paper, I present the next generation of the LensKit project, re-envisioning the original tool's objectives as flexible Python package for supporting recommender systems research and development. LensKit for Python (LKPY) enables researchers and students to build robust, flexible, and reproducible experiments that make use of the large and growing PyData and Scientific Python ecosystem, including scikit-learn, TensorFlow, and PyTorch. To that end, it provides classical collaborative filtering implementations, recommender system evaluation metrics, data preparation routines, and tools for efficiently batch running recommendation algorithms, all usable in any combination with each other or with other Python software. This paper describes the design goals, use cases, and capabilities of LKPY, contextualized in a reflection on the successes and failures of the original LensKit for Java software.
description: 8 pages; accepted for publication in CIKM 2020
Synchronicity and pure bending of piezoelectric bimorphs: a new approach to kinetic energy harvesting
Creators: name: Pozzi, Michele
Publisher: name: arXiv
Year: 2018
Subjects: subject: Applied Physics (physics.app-ph)
subject: Signal Processing (eess.SP)
subject: FOS: Physical sciences
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: Kinetic energy harvesting with piezoelectric bimorphs has attracted considerable research interest in recent years. Many works have been dedicated to the modelling and optimisation of the cantilevered geometry to increase power density, bandwidth, etc. The increased efficiency coming from the use of trapezoidal beams has been recognised, but little has been done to produce the same uniform strain within the most commonly available rectangular beams. This work proposes a new approach via a smart compliant structure which permits to deform a set of bimorphs in pure bending. Furthermore, since the deflections are synchronous, the power signals produced are in phase and power conditioning is simplified and made more efficient. The kinematic requirements for uniform strain are discussed, the novel structure is proposed and modelled with finite elements, a prototype is presented and characterised to support the modelling. The proposed structure induces almost perfectly uniform strain in the piezoelectric beams for all useful rotation angles, demonstrating that, compared to a traditional cantilever, twice as many charges can be produced when the same maximum strain is applied to the material. Synchronicity is also experimentally verified for the prototype, as power signals resulting from impact excitation are observed to be in phase. The principle of synchronous pure bending via helper structures can be applied in general to increase the performance of piezoelectric energy harvesters.
description: 17 pages, 9 figures, 2 tables, 27 references, 1.5 MByte
Neural Network Operations and Susuki-Trotter evolution of Neural Network States
Creators: name: Freitas, Nahuel
name: Morigi, Giovanna
name: Dunjko, Vedran
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: It was recently proposed to leverage the representational power of artificial neural networks, in particular Restricted Boltzmann Machines, in order to model complex quantum states of many-body systems [Science, 355(6325), 2017]. States represented in this way, called Neural Network States (NNSs), were shown to display interesting properties like the ability to efficiently capture long-range quantum correlations. However, identifying an optimal neural network representation of a given state might be challenging, and so far this problem has been addressed with stochastic optimization techniques. In this work we explore a different direction. We study how the action of elementary quantum operations modifies NNSs. We parametrize a family of many body quantum operations that can be directly applied to states represented by Unrestricted Boltzmann Machines, by just adding hidden nodes and updating the network parameters. We show that this parametrization contains a set of universal quantum gates, from which it follows that the state prepared by any quantum circuit can be expressed as a Neural Network State with a number of hidden nodes that grows linearly with the number of elementary operations in the circuit. This is a powerful representation theorem (which was recently obtained with different methods) but that is not directly useful, since there is no general and efficient way to extract information from this unrestricted description of quantum states. To circumvent this problem, we propose a step-wise procedure based on the projection of Unrestricted quantum states to Restricted quantum states. In turn, two approximate methods to perform this projection are discussed. In this way, we show that it is in principle possible to approximately optimize or evolve Neural Network States without relying on stochastic methods such as Variational Monte Carlo, which are computationally expensive.
Equivalence between the Arquès-Walsh sequence formula and the number of connected Feynman diagrams for every perturbation order in the fermionic many-body problem
Creators: name: Castro, Erick
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mathematical Physics (math-ph)
subject: Quantum Gases (cond-mat.quant-gas)
subject: FOS: Physical sciences

description: From the perturbative expansion of the exact Green function, an exact counting formula is derived to determine the number of different types of connected Feynman diagrams. This formula coincides with the Arquès-Walsh sequence formula in the rooted map theory, supporting the topological connection between Feynman diagrams and rooted maps. A classificatory summing-terms approach is used, in connection to discrete mathematical theory.
Saint-Pétersbourg, Институ́т ру́сской литерату́ры (Institut de littérature russe), Собрание Смирнова, n° 6, fol. 239v-256r, transcription normalisée (Gregorius Digital R9-1)
Creators: name: Nivière, Antoine
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2025

description: Ce document PDF est une transcription normalisée du manuscrit Saint-Pétersbourg, Институ́т ру́сской литерату́ры (Institut de littérature russe), Собрание Смирнова, n° 6, fol. 239v-256r, contient le récit du Bon Pécheur et est édité dans le cadre du projet Gregorius Digital sous le sigle R9-1 (dir. Peter Andersen – ARCHE UMR 3400 – Université de Strasbourg)
Relativistic Quark Model Based Description of Low Energy NN Scattering
Creators: name: Antalik, R.
name: Lyubovitskij, V. E.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: A description of the NN scattering is constructed starting from the $π, η, η'$ pseudoscalar-, the $ρ, ϕ, ω$ vector-, and the $\varepsilon(600), a_0, f_0(1400)$ scalar - meson-nucleon coupling constants, which we obtain within a relativistic quark model. Working within the Blankenbecler-Sugar-Logunov-Tavkhelidze quasipotential dynamics we thus describe the NN phase shifts in a relativistically invariant way. In this procedure we use the phenomenological form factor cutoff masses and the effective $\varepsilon$ and $ω$ meson-nucleon coupling constants, only. The comparison of our NN phase shifts to the both empirical data and the Bonn OBEP fit shows good agreement -- the ratio of the $χ^2$ for the present results to the $χ^2$ for Bonn OBEP description is 1.2.
description: 20 LaTeX pages, 2 postscript figures are available on request. Preprint IPSAS-RA-9401
Изучение влияния ацетата свинца на процессы перекисного окисления липидов у животных с экспериментальными опухолями / О. Ю. Баленков, М. С. Гильдиева, А. А. Абдувалиев и др. // Петровские чтения: Тезисы 10-й конференции по фундаментальной онкологии. — Санкт-Петербург, 2014. — С. 10.
Creators: name: Balenkov, Oleg
Publisher: name: figshare
Year: 2021

description: Lead acetate creates pronounced multidirectional changes in the processes of lipid peroxidation (LPO) and antioxidant defense (AOD) systems in animals with experimental tumors.

Ацетат свинца оказывает выраженные разнонаправленные изменения в процессах систем перекисного окисления липидов (ПОЛ) и антиоксидантной защиты (АОЗ) у животных с экспериментальными опухолями.
Miospores from the Brigantian stratotype section at Janny Wood, Cumbria
Creators: name: McLean, Duncan
name: Owens, Bernard
name: Bodman, David J.
name: McLean, Finlay D.
Publisher: name: Geological Society of London
Year: 2018
Subjects: subject: Geology
subject: FOS: Earth and related environmental sciences

description: A full biostratigraphical range chart
Baryonic and Gluonic Correlators in Hot QCD
Creators: name: Hansson, T. H.
name: Sporre, M.
name: Zahed, I.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We extend our earlier work on static color singlet correlators in high T QCD (DeTar correlators) to baryonic and gluonic sources, and estimate the corresponding screening masses using the dimensionally reduced theory. We discuss spin and polarization dependence of meson and baryon masses in the $T \rightarrow \infty$ limit, and possible nonperturbative effects at non-asymptotic temperatures.
description: 20 pages, USITP-94-1 (SUNY-NTG-93-12)
One loop calculations on the Wess-Zumino-Witten anomalous functional at finite temperature
Creators: name: Alvarez-Estrada, R. F.
name: Dobado, A.
name: Nicola, A. Gomez
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We analyze the finite temperature (T) extension of the Wess-Zumino- Witten functional, discussed in a previous work, to one loop in chiral perturbation theory. As a phenomenological application, we calculate finite temperature corrections to the amplitude of the $π^0$ decay into two photons. This calculation is performed in three limits : i)$T/M_π<<1$, ii)the chiral limit at finite T and iii)$T/M_π>>1$ ($M_π$ being the pion mass). The $T$-corrections tend to vanish in the chiral limit, where only the kaon contribution remains (although it is exponentially suppressed).
description: Latex, 13 pages and 3 figures avalaible upon request
Tensor network representations from the geometry of entangled states
Creators: name: Christandl, Matthias
name: Lucia, Angelo
name: Vrana, Péter
name: Werner, Albert H.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: Tensor network states provide successful descriptions of strongly correlated quantum systems with applications ranging from condensed matter physics to cosmology. Any family of tensor network states possesses an underlying entanglement structure given by a graph of maximally entangled states along the edges that identify the indices of the tensors to be contracted. Recently, more general tensor networks have been considered, where the maximally entangled states on edges are replaced by multipartite entangled states on plaquettes. Both the structure of the underlying graph and the dimensionality of the entangled states influence the computational cost of contracting these networks. Using the geometrical properties of entangled states, we provide a method to construct tensor network representations with smaller effective bond dimension. We illustrate our method with the resonating valence bond state on the kagome lattice.
description: 35 pages, 9 figures
Hadron Radiation in Leptonic $Z$ Decays
Creators: name: Hoang, A. H.
name: Jeżabek, M.
name: Kühn, J. H.
name: Teubner, T.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The rate for the final state radiation of hadrons in leptonic $Z$ decays is evaluated, using as input experimental data for $σ(e^+e^-\to hadrons)$ in the low energy region. Configurations with a lepton pair of large and a hadronic state of low invariant mass are dominant. A relative rate $Γ_{l\bar l had}/Γ_{l\bar l}=6.3\times 10^{-4}$ is calculated. This result is about twice the prediction based on a parton model calculation with a quark mass of $300$ MeV. The rate for secondary production of heavy quarks is calculated in the same formalism.
description: 7 pages, LaTex (uses epsf.sty, 2 figures appended as uuencoded eps files). Errors of some numerical values corrected. Conclusions are not affected by these modifications
An Application of Kerr Blackhole Fly-Wheel Model to Statistical Properties of QSOs/AGNs
Creators: name: Nitta, Shin-ya
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The aim of this work is to demonstrate the properties of the magnetospheric model around Kerr blackholes (BHs), so-called the fly-wheel (rotation driven) model. The fly-wheel engine of the BH-accretion disk system is applied to the statistics of QSOs/AGNs. In the model, the central BH is assumed to be formed at $z \sim 10^2$ and obtains nearly maximum but finite rotation energy ($\sim$ extreme Kerr BH) at the formation stage. The inherently obtained rotation energy of the Kerr BH is released through an magnetohydrodynamic process. This model naturally leads finite lifetime of AGN activity. Nitta et al. (1991) clarified individual evolution of Kerr BH fly-wheel engine which is parametrized by BH mass, initial Kerr parameter, magnetic field near the horizon and a dimension-less small parameter. We impose a statistical model for the initial mass function (IMF) of ensemble of BHs by the Press-Schechter formalism. By the help of additional assumptions, we can discuss the evolution of the luminosity function and the spatial number density of QSOs/AGNs.
description: 12 pages, 7 figures Fig.7 has been replaced
Supplementary document for All-pass phase shifting enabled by symmetric topological unidirectional guided resonances - 5852324.pdf
Creators: name: zhang, zixuan
name: Wang, Feifan
name: Wang, Haoran
name: Hu, Yuefeng
name: Yin, Xuefan
name: Hu, Weiwei
name: Peng, Chao
Publisher: name: Optica Publishing Group
Year: 2022
Subjects: Uncategorized

description: supplement information
On the temperature dependence of correlation functions in the space like direction in hot QCD
Creators: name: Koch, Volker
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We study the temperature dependence of quark antiquark correlations in the space like direction. In particular, we predict the temperature dependence of space like Bethe-Salpeter amplitudes using recent Lattice gauge data for the space like string potential. We also investigate the effect of the space like string potential on the screening mass and discuss possible corrections which may arise when working with point sources.
description: 15 pages 8 figures (not included, will be sent on request), (SUNY-NTG-94-3)
Quark-Induced Correlations between Instantons Drive the Chiral Phase Transition
Creators: name: Ilgenfritz, E. -M.
name: Shuryak, E. V.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: A simple model for the instanton ensemble at finite temperature T is proposed, including ``random" and strongly correlated ``molecular" component. T-dependence of fermionic zero modes naturally leads to chiral symmetry restoration, without instanton suppression. Moreover, at $T=(1-2) T_c$ the non-perturbative effects due to ``molecules" are so strong, that they even dominate the global thermodynamics. % two figures are enclosed as .ps files
Local Flexibility for Open Partial Differential Relations
Creators: name: Baer, Christian
name: Hanke, Bernhard
Publisher: name: arXiv
Year: 2018
Subjects: subject: Differential Geometry (math.DG)
subject: FOS: Mathematics
subject: Primary: 53C23, 58A20, Secondary: 53C20, 53C42, 53C50, 58A10

description: We show that local deformations, near closed subsets, of solutions to open partial differential relations can be extended to global deformations, provided all but the highest derivatives stay constant along the subset. The applicability of this general result is illustrated by a number of examples, dealing with convex embeddings of hypersurfaces, differential forms, and lapse functions in Lorentzian geometry. The main application is a general approximation result by sections which have very restrictive local properties an open dense subsets. This shows, for instance, that given any $K \in \mathbb{R}$ every manifold of dimension at least two carries a complete $C^{1,1}$-metric which, on a dense open subset, is smooth with constant sectional curvature $K$. Of course this is impossible for $C^2$-metrics in general.
description: Appendix on Gauss-Bonnet for metrics of low regularity added. Some further minor changes. To appear in Comm. Pure Appl. Math