cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Building Aspiration in the Creative and Performing Arts
Creators: name: English, Helen
name: McKinnon, Jocelyn
name: Lawry, Miranda
name: Grushka, Kathryn
Publisher: name: figshare
Year: 2018
Subjects: subject: 130103 Higher Education
subject: FOS: Educational sciences

description: This project focused on developing skills in creative thinking, project design and realisation in the areas of music, visual arts and/or performance among low socioeconomic status high school students. Addressing the relatively low enrolments into Creative and Performing Arts (CAPA) degrees from this cohort, a series of workshops in the creative arts-technology nexus were conducted for Years 8 and 9 students from seven high schools.
Highlights: Optical/NIR Spectroscopy of Ultraluminous Infrared Galaxies
Creators: name: Veilleux, S.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: This paper reviews the results from recent optical and near-infrared spectroscopic studies of ultraluminous infrared galaxies.
description: 6 pages, 2 embedded figures, Review Talk presented at the September 1998 Ringberg Meeting "Ultraluminous Galaxies: Monsters or Babies?"
Is there a Floquet Lindbladian?
Creators: name: Schnell, Alexander
name: Eckardt, André
name: Denisov, Sergey
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Quantum Gases (cond-mat.quant-gas)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: The stroboscopic evolution of a time-periodically driven isolated quantum system can always be described by an effective time-independent Hamiltonian. Whether this concept can be generalized to open Floquet systems, described by a Markovian master equation with time-periodic Lindbladian generator, remains an open question. By using a two level system as a model, we explicitly show the existence of two well-defined parameter regions. In one region the stroboscopic evolution can be described by a Markovian master equation with a time-independent Floquet Lindbladian. In the other it cannot; but here the one-cycle evolution operator can be reproduced with an effective non-Markovian master equation that is homogeneous but non-local in time. Interestingly, we find that the boundary between the phases depends on when the evolution is stroboscopically monitored. This reveals the non-trivial role played by the micromotion in the dynamics of open Floquet systems.
Difference Image Analysis of Galactic Microlensing I. Data Analysis
Creators: name: Alcock, C.
name: Allsman, R. A.
name: Alves, D.
name: Axelrod, T. S.
name: Becker, A. C.
name: Bennett, D. P.
name: Cook, K. H.
name: Drake, A. J.
name: Freeman, K. C.
name: Griest, K.
name: Lehner, M. J.
name: Marshall, S. L.
name: Minniti, D.
name: Peterson, B. A.
name: Pratt, M. R.
name: Quinn, P. J.
name: Stubbs, C. W.
name: Sutherland, W.
name: Tomaney, A.
name: Vandedei, T.
name: Welch, D. L.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: This is a preliminary report on the application of Difference Image Analysis (DIA) to galactic bulge images. The aim of this analysis is to increase the sensitivity to the detection of gravitational microlensing. We discuss how the DIA technique simplifies the process of discovering microlensing events by detecting only objects which have variable flux. We illustrate how the DIA technique is not limited to detection of so called ``pixel lensing'' events, but can also be used to improve photometry for classical microlensing events by removing the effects of blending. We will present a method whereby DIA can be used to reveal the true unblended colours, positions and light curves of microlensing events. We discuss the need for a technique to obtain the accurate microlensing time scales from blended sources, and present a possible solution to this problem using the existing HST colour magnitude diagrams of the galactic bulge and LMC. The use of such a solution with both classical and pixel microlensing searches is discussed. We show that one of the major causes of systematic noise in DIA is differential refraction. A technique for removing this systematic by effectively registering images to a common airmass is presented. Improvements to commonly used image differencing techniques are discussed.
description: 18 pages, 8 figures, uses AAS LaTEX 4.0, To appear in Astrophysical Journal
Hemerobius phalaenoides Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Neuroptera
Chrysopidae
Hemerobius
Hemerobius phalaenoides

description: Hemerobius phalaenoides [spec. nov.]
H. testaceus, alis basi mucronatis; margine dorsali postice excisis.
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 550, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
title: "Catino ovale in granito", ambito romano, inv. CCIV (ITA/EN)
title: Scheda catalogo digitale Borghese
titleType: AlternativeTitle
Creators: name: Felici, Sonja
name: Galleria Borghese
Publisher: name: Galleria Borghese
Year: 2024

description: Pubblicazione delle schede delle opere conservate nel museo ed estratte dal catalogo digitale di Galleria Borghese, nelle due versioni esistenti online, in italiano e inglese.

Collegamento al catalogo digitale:

ITA: https://www.collezionegalleriaborghese.it/

EN: https://www.collezionegalleriaborghese.it/en
Phryganea flava Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Trichoptera
Phryganeidae
Phryganea
Phryganea flava

description: Phryganea flava [spec. nov.]
P. alis flavo-reticulatis, antennis longitudine abdominis.
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 549, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
The kinematics and the origin of ionized gas in NGC 4036
Creators: name: Cinzano, P.
name: Rix, H. -W.
name: Sarzi, M.
name: Corsini, E. M.
name: Zeilinger, W. W.
name: Bertola, F.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the kinematics and photometry of the stars and of the ionized gas near the centre of the S0 galaxy NGC4036. Dynamical models based on the Jeans Equation have been constructed from the stellar data to determine the gravitational potential in which the ionized gas is expected to orbit. Inside 10'', the observed gas rotation curve falls well short of the predicted circular velocity. Over a comparable radial region the observed gas velocity dispersion is far higher than the one expected from thermal motions or small scale turbulence, corroborating that the gas cannot be following the streamlines of nearly closed orbits. We explore several avenues to understand the dynamical state of the gas: (1) We treat the gas as a collisionless ensemble of cloudlets and apply the Jeans Equation to it; this modeling shows that inside 4'' the gas velocity dispersion is just high enough to explain quantitatively the absence of rotation. (2) Alternatively, we explore whether the gas may arise from the `just shed' mass-loss envelopes of the bulge stars, in which case their kinematics should simply mimic that of the stars. he latter approach matches the data better than (1), but still fails to explain the low velocity dispersion and slow rotation velocity of the gas for 5''
description: 17 pages, 17 figures. Accepted for publication in MNRAS
Phryganea fusca Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Trichoptera
Phryganeidae
Phryganea
Phryganea fusca

description: Phryganea fusca [spec. nov.]
P. fusca immaculata. Fn. svec. 749.
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 549, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Additional file 4 of Trajectories of persisting Covid- 19 symptoms up to 24 months after acute infection: findings from the Predi-Covid cohort study
Creators: name: Fischer, Aurélie
name: Zhang, Lu
name: Elbéji, Abir
name: Wilmes, Paul
name: Snoeck, Chantal J.
name: Larché, Jérôme
name: Oustric, Pauline
name: Ollert, Markus
name: Fagherazzi, Guy
Publisher: name: figshare
Year: 2025
Subjects: subject: Medicine
subject: Neuroscience
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Science Policy
subject: Mental Health
subject: Computational Biology

description: Additional file 4: Supplementary Fig. 1: Complete case analysis: total symptom score evolution in T1 and T2 from baseline up to 24 months afterfor 84 participants who completed the 4 timepoints
Marangoni stress induced by rotation frustration in a liquid foam
Creators: name: Antoine, Bérut
name: Isabelle, Cantat
Publisher: name: arXiv
Year: 2018
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: The role of surface tension gradients in the apparent viscosity of liquid foams remains largely unexplained. In this article, we develop a toy-model based on a periodic array of 2D hexagonal bubbles, each bubble being separated from its neighbors by a liquid film of uniform thickness. The two interfaces of this thin liquid film are allowed to slide relatively to each other, thus shearing the liquid phase in between. We solve the dynamics under external shear of this minimal system and we show that the continuity of the surface tension around the whole bubble is the relevant condition to determine the bubble rotation rate and the energy dissipation. This result is expected to be robust in more complex situations and illustrates that thin film dynamics should be solve at the scale of the whole bubble interface when interface rheology matters.
description: 9 pages, 11 figures
A Search for Very Low-mass Stars and Brown Dwarfs in the Young sigma Orionis Cluster
Creators: name: Bejar, V. J. S.
name: Osorio, M. R. Zapatero
name: Rebolo, R.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a CCD-based photometric survey covering 870 sq. arcmin in a young stellar cluster around the young multiple star sigma Orionis. Our survey limiting R, I, and Z magnitudes are 23.2, 21.8, and 21.0, respectively. From our colour-magnitude diagrams, we have selected 49 faint objects, which smoothly extrapolate the photometric sequence defined by more massive known members. Adopting the currently accepted age interval of 2-10 Myr for the Orion 1b association and considering recent evolutionary models, our objects may span a mass range from 0.1 down to 0.02 Msun, well within the substellar regime. Follow-up low-resolution optical spectroscopy (635-920 nm) for eight of our candidates (I=16-19.5) shows that they have spectral types M6-M8.5 which are consistent with the expectations for true members. Compared with their Pleiades counterparts of similar types, Halpha emission is generally stronger, while NaI and KI absorption lines appear weaker, as expected for lower surface gravities and younger ages. Additionally, TiO bands and in particular VO bands appear clearly enhanced in our candidate with the latest spectral type, SOri 45 (M8.5, I=19.5), compared to objects of similar types in older clusters and the field. We have estimated the mass of this candidate at only 0.020-0.040 Msun, hence it is one of the least massive brown dwarfs yet discovered. We also discuss in this paper the potential role of deuterium as a tracer of both substellar nature and age in very young clusters.
description: Accepted for publication in ApJ Main Journal. 32 pages of text and tables + 9 pages of figures. Figures 3a and 3b (gif format) provided separately
Hemerobius Linnaeus, 1758, gen. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Neuroptera
Chrysopidae
Hemerobius

description: Hemerobius [gen. nov.]
Os dentibus duobus.
Alae deflexae, nec plicatae.
Antennae thorace convexo longiores.
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 549, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Mappia Jacq.
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
Mappia

description: Genus Mappia Jacq.
Figs 17.10–17.26, 18.1–18.8
Description
FRUIT. Elliptical to globose, laterally compressed, red when mature. Epicarp glabrous.
ENDOCARP. Cream, elliptical to globose in lateral view, lenticular in transverse section. Keel surrounding the endocarp in the plane of symmetry. Apex asymmetrical in lateral view; base symmetrical. Outer surface of the endocarp rugose, almost smooth. Vasculature of the endocarp generally resting between rugosities. Endocarp primary vascular bundle outside the endocarp wall. Endocarp wall with two layers, including layer with rows of periclinally oriented cells and another with rows of anticlinally oriented cells. Locule surface smooth, sometimes slightly lacunate.
Key to the genus Mappia
1. Endocarp surface quite smooth ......................................................................................................... 2
– Endocarp surface rugose with channels and mounds ...................................... M. multiflora Lundell
2. Endocarp elliptical, without clear ridges .............................................................. M. racemosa Jacq.
– Endocarp globose, short ridge at the apex .......................................................... M. longipes Lundell
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 50, DOI: 10.5852/ejt.2020.645, http://zenodo.org/record/3829651
Additional file 1 of Identifying potential regulators of JAGGED1 expression in portal mesenchymal cells
Creators: name: Nishino, Teppei
name: Yoshihara, Masaharu
name: Nakayama, Takahiro
name: Tsuchiya, Takaho
name: Tahara, Saeko
name: Ozaki, Haruka
name: Takahashi, Satoru
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1. This table shows all the transcription factors listed in DoRothEA that have an association with JAGGED1 as their target gene. SNAI2 (SLUG), SOX2, and SOX13 had DoRothEA levels of A, B, and C, respectively. The other 32 transcription factors had DoRothEA levels of D. The line number indicates the corresponding positions in DoRothEA.
Solution of the two-impurity Kondo model: critical point, Fermi-liquid phase, and crossover
Creators: name: Gan, Junwu
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: An asymptotically exact solution is presented for the two-impurity Kondo model for a finite region of the parameter space surrounding the critical point. This region is located in the most interesting intermediate regime where RKKY interaction is comparable to the Kondo temperature. After several exact simplifications involving reduction to one dimension and abelian bosonization, the critical point is explicitly identified, making clear its physical origin. By using controlled low energy projection, an effective Hamiltonian is mapped out for the finite region in the phase diagram around the critical point. The completeness of the effective Hamiltonian is rigorously proved from general symmetry considerations. The effective Hamiltonian is solved exactly not only at the critical point but also for the surrounding Fermi-liquid phase. Analytic crossover functions from the critical to Fermi-liquid behavior are derived for the specific heat and staggered susceptibility. It is shown that applying a uniform magnetic field has negligible effect on the critical behavior.
Bite Size Maths: Building Mathematics Capability of Low SES Students in Regional/Remote Australia
Creators: name: Woolcott, Geoff
name: Mason, Rain
name: Markopoulos, Christos
name: Boyd, William
name: Ouhao Chen
name: Seton, Carolyn
name: Lake, Warren
name: Whannell, Robert
name: Foster, Allen
name: Galligan, Linda
name: Marshman, Margaret
name: Schmalz, Jelena
name: Sultanova, Nargiz
Publisher: name: figshare
Year: 2018
Subjects: subject: 130103 Higher Education
subject: FOS: Educational sciences

description: This project built on the mathematics capability of low socioeconomic status students in regional and remote universities by improving access to mathematics resources based on students’ own rates and levels of learning. The project delivered a set of interactive modules as an online learning system to be used singly or together in a MOOC. Further innovations and improvements included enabling point-of-contact feedback.
Temporal and Spectral Correlations of Cyg X-1
Creators: name: Li, T. P.
name: Feng, Y. X.
name: Chen, L.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Temporal and spectral properties of X-ray rapid variability of Cyg X-1 are studied by an approach of correlation analysis in the time domain on different time scales. The correlation coefficients between the total intensity in 2-60 keV and the hardness ratio of 13-60 keV to 2-6 keV band on the time scale of about 1 ms are always negative in all states. For soft states, the correlation coefficients are positive on all the time scales from about 0.01 s to 100 s, which is significantly different with that for transition and low states. Temporal structures in high energy band are narrower than that in low energy band in quite a few cases. The delay of high energy photons relative to low energy ones in the X-ray variations has also been revealed by the correlation analysis. The implication of observed temporal and spectral characteristics to the production region and mechanism of Cyg X-1 X-ray variations is discussed.
description: 17 pages, 6 figures included, to appear in ApJ
Experimentally well-constrained masses of $^{27}$P and $^{27}$S: Implications for studies of explosive binary systems
Creators: name: Sun, L. J.
name: Xu, X. X.
name: Hou, S. Q.
name: Lin, C. J.
name: José, J.
name: Lee, J.
name: He, J. J.
name: Li, Z. H.
name: Wang, J. S.
name: Yuan, C. X.
name: Herwig, F.
name: Keegans, J.
name: Budner, T.
name: Wang, D. X.
name: Wu, H. Y.
name: Liang, P. F.
name: Yang, Y. Y.
name: Lam, Y. H.
name: Ma, P.
name: Duan, F. F.
name: Gao, Z. H.
name: Hu, Q.
name: Bai, Z.
name: Ma, J. B.
name: Wang, J. G.
name: Zhong, F. P.
name: Wu, C. G.
name: Luo, D. W.
name: Jiang, Y.
name: Liu, Y.
name: Hou, D. S.
name: Li, R.
name: Ma, N. R.
name: Ma, W. H.
name: Shi, G. Z.
name: Yu, G. M.
name: Patel, D.
name: Jin, S. Y.
name: Wang, Y. F.
name: Yu, Y. C.
name: Zhou, Q. W.
name: Wang, P.
name: Hu, L. Y.
name: Wang, X.
name: Zang, H. L.
name: Li, P. J.
name: Zhao, Q. Q.
name: Yang, L.
name: Wen, P. W.
name: Yang, F.
name: Jia, H. M.
name: Zhang, G. L.
name: Pan, M.
name: Wang, X. Y.
name: Sun, H. H.
name: Hu, Z. G.
name: Chen, R. F.
name: Liu, M. L.
name: Yang, W. Q.
name: Zhao, Y. M.
name: Zhang, H. Q.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: The mass of $^{27}$P was predicted to impact the X-ray burst (XRB) model predictions of burst light curves and the composition of the burst ashes. To address the uncertainties and inconsistencies in the reported $^{27}$P masses in literature, a wealth of information has been extracted from the $β$-decay spectroscopy of the drip-line nucleus $^{27}$S. We determine the most precise mass excess of $^{27}$P to date to be $-659(9)$~keV, which is 63~keV (2.3$σ$) higher than the AME2016 recommended value of $-722(26)$~keV. The experimentally unknown mass excess of $^{27}$S was estimated to be 17030(400)~keV in AME2016, and we constrain this mass to be 17678(77)~keV based on the measured $β$-delayed two-proton energy. In the temperature region of $(0.06-0.3)$~GK, the $^{26}$Si$(p,γ)^{27}$P reaction rate determined in this work is significantly lower than the rate recommended in the reaction rate libraries, up to two orders of magnitude around 0.1~GK. The impact of these newly determined masses and well-constrained rate on the modeling of the explosive astrophysical scenarios has been explored by hydrodynamic nova and post-processing XRB models. No substantial change was found in the nova contribution to the synthesis of galactic $^{26}$Al or in the XRB energy generation rate, but we found that the calculated abundances of $^{26}$Al and $^{26}$Si at the last stage of XRB are increased by a factor of 2.4. We also conclude that $^{27}$S is not a significant waiting point in the rapid proton capture process.
Hemerobius formicaleo Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Neuroptera
Chrysopidae
Hemerobius
Hemerobius formicaleo

description: Hemerobius formicaleo [spec. nov.]
H. hirtus, alis nebulosis: vasis pilosis, antennis clavatis.
Fn. svec. 733. It. oel. 149, 206. Hemerobius formicaleo.
Reaum. ins 4. t. 14. f. 18, 19. & t. 11. f. 8. & 6. t. 32, 33, 34.
Roes. ins. 3. p. 101. t. 17, 18, 19, 20.
Vallisn. oper. 1. p. 77. t. 2.
Habitat in Europae arena, retrogradus in fovea excavata fornicis instar, Formicis imprimis victitans.
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 550, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
A cascading nonlinear magneto-optical effect in topological insulators
Creators: name: Mondal, Richarj
name: Saito, Yuta
name: Aihara, Yuki
name: Fons, Paul
name: Kolobov, Alexander V.
name: Tominaga, Junji
name: Murakami, Shuichi
name: Hase, Muneaki
Publisher: name: arXiv
Year: 2018
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Topological insulators (TIs) are characterized by possessing metallic (gapless) surface states and a finite band-gap state in the bulk. As the thickness of a TI layer decreases down to a few nanometer, hybridization between the top and bottom surfaces takes place due to quantum tunneling, consequently at a critical thickness a crossover from a 3D-TI to a 2D insulator occurs. Although such a crossover is generally accessible by scanning tunneling microscopy, or by angle-resolved photoemission spectroscopy, such measurements require clean surfaces. Here, we demonstrate that a cascading nonlinear magneto-optical effect induced via strong spin-orbit coupling can examine such crossovers. The helicity dependence of the time-resolved Kerr rotation exhibits a robust change in periodicity at a critical thickness, from which it is possible to predict the formation of a Dirac cone in a film several quintuple layers thick. This method enables prediction of a Dirac cone using a fundamental nonlinear optical effect that can be applied to a wide range of TIs and related 2D materials.
description: 7 pages, 6 figures
Chiral and Spin Order in the 2D \pm J Xy Spin Glass : Domain Wall Scaling Analysis
Creators: name: Ney-Nifle, M.
name: Hilhorst, H. J.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: This is an analytic study of the two-dimensional XY spin glass with $\pm J$ disorder. The Hamiltonian has a continuous spin symmetry and a discrete chiral symmetry, and therefore possesses, potentially, two different order parameters and correlation lengths. The cost of breaking the symmetries is probed by comparing the ground state energy under periodic (P) boundary conditions with the one under antiperiodic (AP) and under reflecting (R) boundary conditions. Two energy differences (``domain wall energies'') appear, $ΔE^{AP}$ and $ΔE^R$, whose scaling behavior with system size is nontrivially related to the correlation length exponents. For a specific distribution of the $\pm J$ disorder we show that the chiral and spin correlation lengths diverge with the same exponent as $T\downarrow 0$. The common exponent has a common cause, viz. the low reversal energy of domains of chiral variables. For general disorder we give a heuristic argumentation in terms of droplet excitations that leads to spin ordering on a longer, or equal, scale than chiral ordering. These results are in contrast with interpretations of Monte Carlo simulations.
description: 18 pages in revtex, LPTHE Orsay 94/23
Hemerobius testaceus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Neuroptera
Chrysopidae
Hemerobius
Hemerobius testaceus

description: Hemerobius testaceus [spec. nov.]
H. fusco-testaceus, alis nigris corpore triplo longioribus.
Habitat in America. Rolander.
Corpus totum obscure testaceum. Caput atrum, glaberrimum. Antennae testaceae ex globis pilosis, vix thorace longiores. Abdomen brevissimum. Alae planae incumbentes una supra alteram.
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 550, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Mappia longipes Lundell 1942
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
Mappia
Mappia longipes

description: Mappia longipes Lundell
Fig. 17.10–17.18
Material examined
Specimen used for endocarp and fruit description
MEXICO • 1982; M. Guillermo Ibarra 72; U [U.1343380].
Description
FRUIT. Globose, symmetrical at the apex. Epicarp smooth or slightly rugose when dry, revealing the endocarp faint rugosities. Mesocarp ca 350 µm thick when dry. Calyx persistent. Length 18.8 mm, width 14.7 mm, thickness 10.4 mm.
ENDOCARP. Globose in lateral view, length ca 15.8 mm, width ca 13.6 mm, thickness ca 10.2 mm. Keel surrounding the endocarp in the plane of symmetry, with a central channel. Base with a small rounded protuberance at the point of the base. Outer surface of the endocarp smooth with sparse rugosities randomly distributed, and short ridge beginning the apex and running transversally and subapically over 0.5 mm at the most. Vasculature of the endocarp free. Endocarp wall 714–809 µm thick. Endocarp wall with two cell layers: outermost layer with ca 17 rows of anticlinally oriented cells, cells 21.7–32.8 µm in length; innermost layer with 14 rows of periclinally oriented cells, cells 16.9–26.7 µm in width. Inner endocarp surface smooth, 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 51, DOI: 10.5852/ejt.2020.645, http://zenodo.org/record/3829651
Additional file 1 of Anticancer activity of Elsholtzia winitiana var. dongvanensis Phuong on gastric cancer cells: phytochemical profiling, cell proliferation inhibition, senescence induction, and cell cycle arrest
Creators: name: Hoang, Van Hung
name: Le, Thi Thanh Huong
name: Nguyen, Phu Hung
name: Nguyen, Duy Hung
name: Luc, Quang Tan
name: Nguyen, Thi Kieu Oanh
name: Do, Khac Hung
Publisher: name: figshare
Year: 2025
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Molecular Biology
subject: Pharmacology
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Virology

description: Additional file 1.
Systematic investigation of methods for multiple freeform optimization in multi-lens imaging systems
Creators: name: Liu, Chang
name: Gross, Herbert
Publisher: name: arXiv
Year: 2018
Subjects: subject: Applied Physics (physics.app-ph)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: With the development in freeform technology, it has now become more and more feasible to use freeform surfaces in real system designs. While the freeform surfaces helping optical designers achieve more and more challenging system features, the methods for multiple freeform implementations are still underdeveloped. We therefore investigate strategies to use freeform surfaces properly in imaging optical systems with one Scheimpflug system and one lithographic system. Based on the studies of the influences of the freeform normalization radius, freeform order and system eccentricity, the methods of determining the optimal location for implementing one freeform surface are discussed. Different optimization strategies to optimize two freeform surfaces are discussed to compare their resulting influences on the system performance. On top of that, ways to implement more than one freeform surface in the optical system is also investigated. In the end, a workflow is presented as guidance for implementing multiple freeform surfaces with respect to system aberration constitutions.
Difference Image Analysis of Galactic Microlensing II. Microlensing Events
Creators: name: Alcock, C.
name: Allsman, R. A.
name: Alves, D.
name: Axelrod, T. S.
name: Becker, A. C.
name: Bennett, D. P.
name: Cook, K. H.
name: Drake, A. J.
name: Freeman, K. C.
name: Griest, K.
name: Lehner, M. J.
name: Marshall, S. L.
name: Minniti, D.
name: Peterson, B. A.
name: Pratt, M. R.
name: Quinn, P. J.
name: Stubbs, C. W.
name: Sutherland, W.
name: Tomaney, A.
name: Vandedei, T.
name: Welch, D. L.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The MACHO collaboration has been carrying out Difference Image Analysis (DIA) since 1996 with the aim of increasing the sensitivity to the detection of gravitational microlensing. This is a preliminary report on the application of DIA to galactic bulge images in one field. We show how the DIA technique significantly increases the number of detected lensing events, by removing the positional dependence of traditional photometry schemes and lowering the microlensing event detection threshold. This technique, unlike PSF photometry, gives the unblended colours and positions of the microlensing source stars. We present a set of criteria for selecting microlensing events from objects discovered with this technique. The 16 pixel and classical microlensing events discovered with the DIA technique are presented.
description: 13 pages, 6 figures, uses AAS LaTEX 4.0, To appear in ApJS
Planar Cooperative Extremum Seeking with Guaranteed Convergence Using A Three-Robot Formation
Creators: name: Skobeleva, Anna
name: Fidan, Baris
name: Ugrinovskii, V.
name: Petersen, Ian R.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Systems and Control (eess.SY)
subject: Robotics (cs.RO)
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: FOS: Computer and information sciences

description: In this paper, a combined formation acquisition and cooperative extremum seeking control scheme is proposed for a team of three robots moving on a plane. The extremum seeking task is to find the maximizer of an unknown two-dimensional function on the plane. The function represents the signal strength field due to a source located at maximizer, and is assumed to be locally concave around maximizer and monotonically decreasing in distance to the source location. Taylor expansions of the field function at the location of a particular lead robot and the maximizer are used together with a gradient estimator based on signal strength measurements of the robots to design and analyze the proposed control scheme. The proposed scheme is proven to exponentially and simultaneously (i) acquire the specified geometric formation and (ii) drive the lead robot to a specified neighborhood disk around maximizer, whose radius depends on the specified desired formation size as well as the norm bounds of the Hessian of the field function. The performance of the proposed control scheme is evaluated using a set of simulation experiments.
description: Presented at the 2018 IEEE Conference on Decision and Control (CDC), Miami Beach, FL, USA
Code to identify enclaves and exclaves based on point set topology
Creators: name: Xiaonan Wang
name: Tomko, Martin
name: Winter, Stephan
Publisher: name: Zenodo
Year: 2021

description: calculating4_4matrix_v03.html is a file which includes the relate16im() function to produce a string of 16-Intersection Matrix. possible matrix of enclaves_v1.html is a file which employs conditions of intersection for enclaves to get 74 possible spatial configurations of enclaves. validating_polygon_v3.html is a file which visualize and validate 74 possible geometric interpretations of enclaves.
Nested Quantum Annealing Correction at Finite Temperature: $p$-spin models
Creators: name: Matsuura, Shunji
name: Nishimori, Hidetoshi
name: Vinci, Walter
name: Lidar, Daniel A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: Quantum annealing in a real device is necessarily susceptible to errors due to diabatic transitions and thermal noise. Nested quantum annealing correction is a method to suppress errors by using an all-to-all penalty coupling among a set of physical qubits representing a logical qubit. We show analytically that nested quantum annealing correction can suppress errors effectively in ferromagnetic and antiferromagnetic Ising models with infinite-range interactions. Our analysis reveals that the nesting structure can significantly weaken or even remove first-order phase transitions, in which the energy gap closes exponentially. The nesting structure also suppresses thermal fluctuations by reducing the effective temperature.
description: 28 pages
Automated Netlist Generation for 3D Electrothermal and Electromagnetic Field Problems
Creators: name: Casper, Thorben
name: Duque, David
name: Schöps, Sebastian
name: De Gersem, Herbert
Publisher: name: arXiv
Year: 2018
Subjects: subject: Computational Engineering, Finance, and Science (cs.CE)
subject: FOS: Computer and information sciences
subject: I.6.3; J.2
subject: 35Q61, 35Q79, 65Z05, 78A25, 78M12, 94C99, 80A20, 80M25

description: We present a method for the automatic generation of netlists describing general three-dimensional electrothermal and electromagnetic field problems. Using a pair of structured orthogonal grids as spatial discretisation, a one-to-one correspondence between grid objects and circuit elements is obtained by employing the finite integration technique. The resulting circuit can then be solved with any standard available circuit simulator, alleviating the need for the implementation of a custom time integrator. Additionally, the approach straightforwardly allows for field-circuit coupling simulations by appropriately stamping the circuit description of lumped devices. As the computational domain in wave propagation problems must be finite, stamps representing absorbing boundary conditions are developed as well. Representative numerical examples are used to validate the approach. The results obtained by circuit simulation on the generated netlists are compared with appropriate reference solutions.
description: This is a pre-print of an article published in the Journal of Computational Electronics. The final authenticated version is available online at: https://dx.doi.org/10.1007/s10825-019-01368-6. All numerical results can be reproduced by the Matlab code openly available at https://github.com/tc88/ANTHEM
Hemerobius marginalis Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Neuroptera
Chrysopidae
Hemerobius
Hemerobius marginalis

description: Hemerobius marginalis [spec. nov.]
H. flavus, alis hyalinis margine fuscis corpore triplo longioribus.
Habitat in America. Rolander.
Similis priori, excepto colore & Antennis paulo longioribus.
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 550, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Studying the inertias of LCM matrices and revisiting the Bourque-Ligh conjecture
Creators: name: Mattila, Mika
name: Haukkanen, Pentti
name: Mäntysalo, Jori
Publisher: name: arXiv
Year: 2018
Subjects: subject: Number Theory (math.NT)
subject: Combinatorics (math.CO)
subject: FOS: Mathematics

description: Let $S=\{x_1,x_2,\ldots,x_n\}$ be a finite set of distinct positive integers. Throughout this article we assume that the set $S$ is GCD closed. The LCM matrix $[S]$ of the set $S$ is defined to be the $n\times n$ matrix with $\mathrm{lcm}(x_i,x_j)$ as its $ij$ element. The famous Bourque-Ligh conjecture used to state that the LCM matrix of a GCD closed set $S$ is always invertible, but currently it is a well-known fact that any nontrivial LCM matrix is indefinite and under the right circumstances it can be even singular (even if the set $S$ is assumed to be GCD closed). However, not much more is known about the inertia of LCM matrices in general. The ultimate goal of this article is to improve this situation. Assuming that $S$ is a meet closed set we define an entirely new lattice-theoretic concept by saying that an element $x_i\in S$ generates a double-chain set in $S$ if the set $\mathrm{meetcl}(C_S(x_i))\setminus C_S(x_i)$ can be expressed as a union of two disjoint chains (here the set $C_S(x_i)$ consists of all the elements of the set $S$ that are covered by $x_i$ and $\mathrm{meetcl}(C_S(x_i))$ is the smallest meet closed subset of $S$ that contains the set $C_S(x_i)$). We then proceed by studying the values of the Möbius function on sets in which every element generates a double-chain set and use the properties of the Möbius function to explain why the Bourque-Ligh conjecture holds in so many cases and fails in certain very specific instances. After that we turn our attention to the inertia and see that in some cases it is possible to determine the inertia of an LCM matrix simply by looking at the lattice-theoretic structure of $(S,|)$ alone. Finally, we are going to show how to construct LCM matrices in which the majority of the eigenvalues is either negative or positive.
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VIII, Cart. 192 (11 H 77), 295 folios, f. 0033v
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/2012
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 général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VIII, Archives départementales de la Côte-d'Or, Cart. 192 (11 H 77), 295 folios, f. 0033v, 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 VIII, Archives départementales de la Côte-d'Or, Cart. 192 (11 H 77), 295 folios, f. 0033v, 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 differential magnification of high-redshift ultraluminous infrared galaxies
Creators: name: Blain, Andrew W.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: This proceeding discusses the potential modifications to the mid-infrared spectral energy distribution (SED) of a high-redshift dusty AGN that is graviationally lensed by a foreground galaxy. The mid-infrared colour of a lensed galaxy would typically be bluer than that of the same galaxy in the absence of magnification. This effect would make it more difficult to interpret the very small sample of high-redshift dusty AGN for which broad-band SEDs are known in terms of the viewing angle of an obscuring dust torus, as all are known to be lensed by galaxies.
description: 6 pages, 1 two-panel figure. To appear in proceedings of Ringberg ULIRG meeting, edited by D. Lutz and L. Tacconi. In press at Astrophysics and Space Science. Differential magnification: Ringberg proceeding. See also astro-ph/9812415
Hemerobius formicalynx Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Neuroptera
Chrysopidae
Hemerobius
Hemerobius formicalynx

description: Hemerobius formicalynx [spec. nov.]
H. alis hyalinis immaculatis, antennis clavatis.
Roes. ins. 3. t. 21. f. 2.
Habitat in Africa.
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 550, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Physical performance of the students of music schools compared with reference values
Creators: name: Apanowicz, Mateusz
Publisher: name: figshare
Year: 2018
Subjects: subject: 110317 Physiotherapy
subject: FOS: Clinical medicine

description: Apanowicz Mateusz. Physical performance of the students of music schools compared with reference values. Journal of Education, Health and Sport. 2018;8(9):308-326. eISNN 2391-8306. DOI http://dx.doi.org/10.6084/m9.figshare.6983936 http://ojs.ukw.edu.pl/index.php/johs/article/view/5840

 The journal has had 7 points in Ministry of Science and Higher Education parametric evaluation. Part b item 1223 (26/01/2017). 1223 Journal of Education, Health and Sport eissn 2391-8306 7
 © The Authors 2018; This article is published with open access at Licensee Open Journal Systems of Kazimierz Wielki University in Bydgoszcz, Poland Open Access. This article is distributed under the terms of the Creative Commons Attribution Noncommercial License which permits any noncommercial use, distribution, and reproduction in any medium, provided the original author (s) and source are credited. This is an open access article licensed under the terms of the Creative Commons Attribution Non commercial license Share alike. (http://creativecommons.org/licenses/by-nc-sa/4.0/) which permits unrestricted, non commercial use, distribution and reproduction in any medium, provided the work is properly cited.
 The authors declare that there is no conflict of interests regarding the publication of this paper.
 Received: 01.08.2018. Revised: 17.08.2018. Accepted: 20.08.2018.

 Physical performance of the students of music schools compared with reference values
 Mateusz Apanowicz
 FizjoMedica, Poniatowskiego 1/4, 86-300 Grudziądz

 Key words: physical performance, reference values, Eurofit test battery

 Abstract Introduction. Physical activity is the first method of treatment which prevents a great number of diseases. Material and methods. 393 students from randomly selected music schools in Poland and Germany were qualified for the study. The level of physical fitness was assessed by means of the Eurofit test in each of the schools. The obtained test results were confronted with reference levels. Conclusions 1. The level of the skills specific for musicians was significantly higher as compared with reference values. 2. The level of physical performance among musicians significantly differed from reference values.
Hearing the sirens of the early Universe: Primordial Black Holes and Gravitational Waves
Creators: name: Kavanagh, Bradley J
Publisher: name: Zenodo
Year: 2019
Subjects: Dark Matter
Primordial Black Holes
Gravitational Waves
New Physics

description: Since the first detections of gravitational waves (GW) from merging binary black holes (BH), there has been a renewed interest in the possibility that at least some of these BHs could be primordial in origin. I will briefly discuss motivations for such primordial black holes (PBHs), formed from the collapse of large over-densities in the early Universe. I will then examine the on-going debate over whether LIGO and Virgo have indeed detected merging PBHs, and what we might learn if they did. Of course, the power of GWs in probing PBHs extends far beyond these 'direct' detections. I will also discuss more indirect probes, such as the stochastic GW background which may be produced along with PBH formation. The observation of GWs has thus opened up a new way to detect and study PBHs and to learn about the physics of the early Universe from which they formed.
description: Overview talk at GW4FP 2019. Some associated code at https://github.com/bradkav/PBHbounds