cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
A pulsational distance to Omega Centauri based on Near-Infrared Period-Luminosity relations of RR Lyrae stars
Creators: name: Del Principe, M.
name: Piersimoni, A. M.
name: Storm, J.
name: Caputo, F.
name: Bono, G.
name: Stetson, P. B.
name: Castellani, M.
name: Buonanno, R.
name: Calamida, A.
name: Corsi, C. E.
name: Dall'Ora, M.
name: Ferraro, I.
name: Freyhammer, L. M.
name: Iannicola, G.
name: Monelli, M.
name: Nonino, M.
name: Pulone, L.
name: Ripepi, V.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present new Near-Infrared (J,K) magnitudes for 114 RR Lyrae stars in the globular cluster Omega Cen (NGC 5139) which we combine with data from the literature to construct a sample of 180 RR Lyrae stars with J and K mean magnitudes on a common photometric system. This is presently the largest such sample in any stellar system. We also present updated predictions for J,K-band Period-Luminosity relations for both fundamental and first-overtone RR Lyrae stars, based on synthetic horizontal branch models with metal abundance ranging from Z=0.0001 to Z=0.004. By adopting for the Omega Cen variables with measured metal abundances an alpha-element enhancement of a factor of 3 (about 0.5 dex) with respect to iron we find a true distance modulus of 13.70 (with a random error of 0.06 and a systematic error of 0.06), corresponding to a distance d=5.5 Kpc (with both random and systematic errors equal to 0.03 Kpc). Our estimate is in excellent agreement with the distance inferred for the eclipsing binary OGLEGC-17, but differ significantly from the recent distance estimates based on cluster dynamics and on high amplitude Delta Scuti stars.
description: 24 pages, 7 figures, accepted for publication on The Astrophysical Journal
Inelastic Black Hole Production and Large Extra Dimensions
Creators: name: Anchordoqui, Luis A.
name: Feng, Jonathan L.
name: Goldberg, Haim
name: Shapere, Alfred D.
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Astrophysics (astro-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Experiment (hep-ex)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Black hole production in elementary particle collisions is among the most promising probes of large extra spacetime dimensions. Studies of black holes at particle colliders have assumed that all of the incoming energy is captured in the resulting black hole. We incorporate the inelasticity inherent in such processes and determine the prospects for discovering black holes in colliders and cosmic ray experiments, employing a dynamical model of Hawking evolution. At the Large Hadron Collider, inelasticity reduces rates by factors of 10^3 to 10^6 in the accessible parameter space, moderating, but not eliminating, hopes for black hole discovery. At the Pierre Auger Observatory, rates are suppressed by a factor of 10. We evaluate the impact of cosmic ray observations on collider prospects.
description: References added
Linum perenne Linnaeus 1753
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Malpighiales
Linaceae
Linum
Linum perenne

description: Linum perenne Linnaeus, Species Plantarum 1: 277. 1753.
"Habitat in Sibiria et Cantabrigiae." RCN: 2205.
 Lectotype (Ockenden in Watsonia 8: 209. 1971): Herb. Linn. No. 396.8 (LINN).
 Current name: Linum perenne L. (Linaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part L), pp. 610-650 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 634, DOI: 10.5281/zenodo.291971
Paratopula
Creators: name: Luo, Ying Y.
name: Benoit Guénard
Publisher: name: Zenodo
Year: 2016
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Paratopula

description: Synoptic species list of global Paratopula species Paratopula andamensis Forel, 1903 (Andaman Is.) – known from male only Paratopula ankistra Bolton, 1988 (Brunei) Paratopula catocha Bolton, 1988 (Sulawesi) Paratopula ceylonica Emery, 1901 (Bangladesh, India, Myanmar, Pakistan, Sri Lanka, Taiwan) Paratopula demeta Bolton, 1988 (Indonesia, E. Malaysia) Paratopula longispina Stitz, 1938 (E. Malaysia) – known from female only Paratopula macta Bolton, 1988 Malaysia, Philippines, Thailand) (Brunei, Paratopula oculata Smith, 1857 (Borneo, W. Malaysia, Singapore) – known from male and female only Paratopula sumatrensis Forel 1913 (Philippines, Sumatra) - known from female only Paratopula intermedia 1998 (India) Sheela & Narendran, Paratopula zhengi Xu & Xu, 2011 (Xizang, China) Paratopula bauhinia sp. nov. (Hong Kong) Updated key to global Paratopula species
description: Published as part of Ying Y. Luo & Benoit Guénard, 2016, Descriptions of a new species and the gyne in the rarely collected arboreal genera Paratopula and Rotastruma (Hymenopytera: Formicidae) from Hong Kong, with a discussion on their ecology, pp. 1-16 in Asian Myrmecology 8 on pages 8-10, DOI: 10.20362/am.008016, http://zenodo.org/record/270012
description: {"references": ["Bolton B., 1988. A review of Paratopula Wheeler, a forgotten genus of Myrmicine ants (Hym., Formicidae). Entomologist's Monthly Magazine, 125 - 143.", "Emery, C., 1901. Ameisen gesammelt in Ceylon con Dr. W. Horn, 1899, Dt. Ent. Z., 113 - 122.", "Xu Z. H., & Xu G. L., 2011. A new species of the genus Paratopula Wheeler (Hymenoptera, Formicidae). Acta Zootaxonomica, 36 (3): 595 - 597."]}
Additional file 3 of Physicians’ knowledge on specific rare diseases and its associated factors: a national cross-sectional study from China
Creators: name: Zhang, Huanyu
name: Xiao, Ying
name: Zhao, Xinyue
name: Tian, Zhuang
name: Zhang, Shu-yang
name: Dong, Dong
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Science Policy
subject: Mental Health

description: Additional file 3. Frequencies of physicians in different specialties based on 34 rare diseases of concern.
Three-dimensional antipodal and norm-equilateral sets
Creators: name: Schuermann, Achill
name: Swanepoel, Konrad
Publisher: name: arXiv
Year: 2005
Subjects: subject: Metric Geometry (math.MG)
subject: Differential Geometry (math.DG)
subject: FOS: Mathematics
subject: 52A21 (Primary) 49Q15 (Secondary)

description: We characterize the three-dimensional spaces admitting at least six or at least seven equidistant points. In particular, we show the existence of $C^\infty$ norms on $\R^3$ admitting six equidistant points, which refutes a conjecture of Lawlor and Morgan (1994, Pacific J. Math \textbf{166}, 55--83), and gives the existence of energy-minimizing cones with six regions for certain uniformly convex norms on $\R^3$. On the other hand, no differentiable norm on $\R^3$ admits seven equidistant points. A crucial ingredient in the proof is a classification of all three-dimensional antipodal sets. We also apply the results to the touching numbers of several three-dimensional convex bodies.
description: 20 pages, 15 figures
Sensitivity of an underwater Cerenkov km3 telescope to TeV neutrinos from Galactic Microquasars
Creators: name: Distefano, C.
name: Collaboration, the NEMO
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In this paper are presented the results of Monte Carlo simulations on the capability of the proposed NEMO-km$^3$ telescope to detect TeV muon neutrinos from Galactic microquasars. For each known microquasar we compute the number of detectable events, together with the atmospheric neutrino and muon background events. We also discuss the detector sensitivity to neutrino fluxes expected from known microquasars, optimizing the event selection also to reject the background; the number of events surviving the event selection are given. The best candidates are the steady microquasars SS433 and GX339-4 for which we estimate a sensitivity of about $5\cdot10^{-11}$ erg/cm$^2$ s; the predicted fluxes are expected to be well above this sensitivity. For bursting microquasars the most interesting candidates are Cygnus X-3, GRO J1655-40 and XTE J1118+480: their analyses are more complicated because of the stochastic nature of the bursts.
description: 20 pages, 3 figures, accepted by Astroparticle Physics
Statistical Physics of Design
Creators: name: Klishin, Andrei A.
name: Shields, Colin P. F.
name: Singer, David J.
name: van Anders, Greg
Publisher: name: arXiv
Year: 2017
Subjects: subject: Physics and Society (physics.soc-ph)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: A key challenge in complex design problems that permeate science and engineering is the need to balance design objectives for specific design elements or subsystems with global system objectives. Global objectives give rise to competing design pressures, whose effects can be difficult to trace in subsystem design. Here, using examples from arrangement problems, we show that the systems-level application of statistical physics principles, which we term "systems physics", provides a detailed characterization of subsystem design in terms of the concepts of stress and strain from materials physics. We analyze instances of routing problems in naval architectures, and show that systems physics provides a direct means of classifying architecture types, and quantifying trade-offs between subsystem- and overall performance. Our approach generalizes straightforwardly to design problems in a wide range of other disciplines that require concrete understanding of how the pressure to meet overall design objectives drives the outcomes for component subsystems.
description: 9 RevTeX pages, 7 figures
Orientation of deoxyhemoglobin at high magnetic fields: structural insights from RDCs in solution.
Creators: name: Sarata C. Sahu
name: Simplaceanu, Virgil
name: Qingguo  Gong
name: Ho, Nancy T.
name: Glushka, John G.
name: Prestegard, James H.
name: Ho, Chien
Publisher: name: Carnegie Mellon University
Year: 2006
Subjects: subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: Human normal adult hemoglobin (Hb A) is a tetrameric protein molecule of ~64 kDa consisting of two identical -chains and two identical -chains of 141 and 146 amino acid residues each and four bound heme moieties. In the oxygen-free form of Hb A, also known as deoxyhemoglobin A (deoxy-Hb A), the hemes are paramagnetic with S = 2. We have measured the one-bond spin-spin couplings (1JNH + 1DNH) on (15N,2H)-labeled deoxy-Hb A in solution as a function of magnetic field strengths from 11.7 to 21.1 T and found that these couplings are linearly proportional to the square of the magnetic field. This field dependence provides an opportunity to extract the residual dipolar couplings (RDCs, 1DNH) and, thus, to compare predictions about the solution structure of deoxy-Hb A to crystal structures for this molecule. Such comparison is essential for our understanding of the structure, dynamics, and function of this allosteric protein under conditions close to the physiological state. This report illustrates the usefulness of using the magnetic-field dependent RDCs to determine the solution structure of a large paramagnetic protein. This method is especially valuable for those proteins whose structures must be determined in an oxygen-free environment.
Organelle tethering by a homotypic PDZ interaction underlies formation of the Golgi membrane network.
Creators: name: Debrup  Sengupta
name: Truschel, Steven T.
name: Bachert, Collin
name: Linstedt, Adam
Publisher: name: Carnegie Mellon University
Year: 2009
Subjects: subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: Formation of the ribbon-like membrane network of the Golgi apparatus depends on GM130 and GRASP65, but the mechanism is unknown. We developed an in vivo organelle tethering assaying in which GRASP65 was targeted to the mitochondrial outer membrane either directly or via binding to GM130. Mitochondria bearing GRASP65 became tethered to one another, and this depended on a GRASP65 PDZ domain that was also required for GRASP65 self-interaction. Point mutation within the predicted binding groove of the GRASP65 PDZ domain blocked both tethering and, in a gene replacement assay, Golgi ribbon formation. Tethering also required proximate membrane anchoring of the PDZ domain, suggesting a mechanism that orientates the PDZ binding groove to favor interactions in trans. Thus, a homotypic PDZ interaction mediates organelle tethering in living cells.
The political factor influencing youth unemployment in Mogadishu Somalia.
Creators: name: Najma, Isse Mohamud
Publisher: name: Zenodo
Year: 2025
Subjects: The political
factor
influencing
youth
unemployment
in Mogadishu Somalia.

description: Abstract

This study critically examines the political factors influencing youth unemployment in Mogadishu, Somalia. The main objective of the study is to critically assess To find out the current situation of youth unemployment Mogadishu, Somalia, the key question that the study seeks to answer is the factors influencing youth unemployment in Mogadishu. This study which aimed to find out the politics contributed to youth unemploymentin Mogadishu a conducted quantitative approach with used in this research to get as much information as possible and to avoid judgments. This study also methodology utilized questioner, to collect data for the questionnaire.

It also identified government organs and individuals who have been involved either directly or indirectly in dealing with the political factors influencing youth unemployment in Mogadishu. Inanition to that this study the role of youth unemployment, the current situation of youth unemployment politics contributed to youth unemployment in Mogadishu, and the strategies to reduce youth unemployment, the research found out that the political factors influencing youth unemployment in Mogadishu, Somalia The study recommends the federalgovernment of Somali should create job opportunities in the market for the youth.
O PAPEL DA ESPIRITUALIDADE NA ADAPTAÇÃO AO LUTO
Creators: name: COSTA, Luís Henrique da Silva
name: DA SILVA, Vânia de Cassia Souza
name: ROCHA, Ágatha Fialho
Publisher: name: Zenodo
Year: 2024
Subjects: Espiritualidade
Luto
Apoio Espiritual
Calma.

description: O luto é uma experiência complexa que envolve não apenas aspectos emocionais e psicológicos, mas também espirituais e religiosos para muitas pessoas. A espiritualidade e a religiosidade desempenham papéis significativos na forma como as pessoas lidam com a perda, buscando significado, consolo e esperança em suas crenças e práticas espirituais
Linum quadrifolium Linnaeus 1753
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Malpighiales
Linaceae
Linum
Linum quadrifolium

description: Linum quadrifolium Linnaeus, Species Plantarum 1: 281. 1753.
"Habitat in Aethiopia." RCN: 2224.
 Lectotype (Rogers in Nordic J. Bot. 1:718. 1981): Herb. Linn. No. 396.39 (LINN).
 Current name: Linum quadrifolium L. (Linaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part L), pp. 610-650 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 635, DOI: 10.5281/zenodo.291971
Pion Form Factor Phase, PIon Pion Elasticity and New Electron-Positron Data
Creators: name: Eidelman, S.
name: Lukaszuk, L.
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: New precise data on the low energy electron-positron annihilation into hadrons from Novosibirsk are used to obtain bounds on the elasticity parameter and the difference between the phase of the pion form factor and that of pion pion scattering
description: 9 pages, 4 figures, submitted to Physics Letters B
O'Brien et al., 2021. Modelling aural language skills and reading ability: Preregistered study of bilingual children in Singapore
Creators: name: SH Annabel Chen, PhD
name: Ke, Han
name: O'Brien, Beth Ann
name: Lim, Nicole Cybil
name: Styles, Suzy J
Publisher: name: OSF
Year: 2023
Subjects: Bilingualism
Code mixing
Language Acquisition
Language Development
Language Planning
Language skills
Multilingualism
Singapore
Translanguaging

description: Conference paper presented at SRCD April 7-9 2021 Virtual Biennial Meeting
Optimal time scale for spike-time reliability: theory, simulations, and experiments.
Creators: name: Galán, Roberto F.
name: G Bard  Ermentrout
name: Urban, Nathan
Publisher: name: Carnegie Mellon University
Year: 2008
Subjects: subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: Use of spike timing to encode information requires that neurons respond with high temporal precision and with high reliability. Fast fluctuating stimuli are known to result in highly reproducible spike times across trials, whereas constant stimuli result in variable spike times. Here, we first studied mathematically how spike-time reliability depends on the rapidness of aperiodic stimuli. Then, we tested our theoretical predictions in computer simulations of neuron models (Hodgkin-Huxley and modified quadratic integrate-and-fire), as well as in patch-clamp experiments with real neurons (mitral cells in the olfactory bulb and pyramidal cells in the neocortex). As predicted by our theory, we found that for firing frequencies in the beta/gamma range, spike-time reliability is maximal when the time scale of the input fluctuations (autocorrelation time) is in the range of a few milliseconds (2-5 ms), coinciding with the time scale of fast synapses, and decreases substantially for faster and slower inputs. Finally, we comment how these findings relate to mechanisms causing neuronal synchronization.
title: Mémoires pour servir à l'histoire ecclésiastique des six premiers siècles- justifiés par les citations des auteurs originaux. Avec une chronologie où l'on fait un abrégé de l'histoire ecclésiastique et profane ; et des notes pour éclaircir les difficultés des faits et de la chronologie.
Creators: name: :Unkn
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2022

description: created: 1693-1712
Design and Evaluation of Vision-based Head and Face Tracking Interfaces for Assistive Input
Creators: name: Morikawa, Chamin
name: Lyons, Michael J.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Human-Computer Interaction (cs.HC)
subject: FOS: Computer and information sciences
subject: H.1.2

description: Interaction methods based on computer-vision hold the potential to become the next powerful technology to support breakthroughs in the field of human-computer interaction. Non-invasive vision-based techniques permit unconventional interaction methods to be considered, including use of movements of the face and head for intentional gestural control of computer systems. Facial gesture interfaces open new possibilities for assistive input technologies. This chapter gives an overview of research aimed at developing vision-based head and face-tracking interfaces. This work has important implications for future assistive input devices. To illustrate this concretely we describe work from our own research in which we developed two vision-based facial feature tracking algorithms for human computer interaction and assistive input. Evaluation forms a critical component of this research and we provide examples of new quantitative evaluation tasks as well as the use of model real-world applications for the qualitative evaluation of new interaction styles.
description: Current manuscript is not satisfactory with all authors
Singularity points for first passage percolation
Creators: name: Yukich, J. E.
name: Zhang, Yu
Publisher: name: arXiv
Year: 2005
Subjects: subject: Probability (math.PR)
subject: FOS: Mathematics
subject: 60K35 (Primary)

description: Let $0
description: Published at http://dx.doi.org/10.1214/009117905000000819 in the Annals of Probability (http://www.imstat.org/aop/) by the Institute of Mathematical Statistics (http://www.imstat.org)
Towards formalization of the soliton counting technique for the Khovanov-Rozansky invariants in the deformed $\mathcal{R}$-matrix approach
Creators: name: Anokhina, A.
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We consider recently developed Cohomological Field Theory soliton counting diagram technique for Khovanov and Khovanov-Rozansky invariants [1,2]. Although the expectation to obtain a new way for computing the invariants has not yet come true, we demonstrate that soliton counting technique can be totally formalized at an intermediate stage, at least in particular cases. We present the corresponding algorithm, based on the approach involving deformed $\mathcal{R}$-matrix and minimal positive division, developed previously in [3]. We start from a detailed review of the minimal positive division approach, comparing it with other methods, including the rigorous mathematical treatment [4]. Pieces of data obtained within our approach are presented in the Appendices.
description: 38 pp.+ 12 pp. of Appendices, contains many tables and figures
Optimal haplotype block-free selection of tagging SNPs for genome-wide association studies.
Creators: name: Halldórsson, Bjarni V.
name: Bafna, Vineet
name: Lippert, Ross
name: Schwartz, Russell
name: Vega, Francisco M De La
name: Clark, Andrew G.
name: Istrail, Sorin
Publisher: name: Carnegie Mellon University
Year: 2004
Subjects: subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: It is widely hoped that the study of sequence variation in the human genome will provide a means of elucidating the genetic component of complex diseases and variable drug responses. A major stumbling block to the successful design and execution of genome-wide disease association studies using single-nucleotide polymorphisms (SNPs) and linkage disequilibrium is the enormous number of SNPs in the human genome. This results in unacceptably high costs for exhaustive genotyping and presents a challenging problem of statistical inference. Here, we present a new method for optimally selecting minimum informative subsets of SNPs, also known as "tagging" SNPs, that is efficient for genome-wide selection. We contrast this method to published methods including haplotype block tagging, that is, grouping SNPs into segments of low haplotype diversity and typing a subset of the SNPs that can discriminate all common haplotypes within the blocks. Because our method does not rely on a predefined haplotype block structure and makes use of the weaker correlations that occur across neighboring blocks, it can be effectively applied across chromosomal regions with both high and low local linkage disequilibrium. We show that the number of tagging SNPs selected is substantially smaller than previously reported using block-based approaches and that selecting tagging SNPs optimally can result in a two- to threefold savings over selecting random SNPs.
Mass Evaporation Rate of Globular Clusters in a Strong Tidal Field
Creators: name: Madrid, Juan P.
name: Leigh, Nathan W. C.
name: Hurley, Jarrod R.
name: Giersz, Mirek
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The mass evaporation rate of globular clusters evolving in a strong Galactic tidal field is derived through the analysis of large, multi-mass $N$-body simulations. For comparison, we also study the same evaporation rates using MOCCA Monte Carlo models for globular cluster evolution. Our results show that the mass evaporation rate is a dynamical value; that is, far from a constant single number found in earlier analytical work and commonly used in the literature. Moreover, the evaporation rate derived with these simulations is higher than values previously published. These models also show that the value of the mass evaporation rate depends on the strength of the tidal field. We give an analytical estimate of the mass evaporation rate as a function of time and galactocentric distance xi(R_{GC},t). Upon extrapolating this formula to smaller R_{GC} values, our results provide tentative evidence for a very high xi value at small R_{GC}. Our results suggest that the corresponding mass loss in the inner Galactic potential could be high and it should be accounted for when star clusters pass within it. This has direct relevance to nuclear cluster formation/growth via the infall of globular clusters through dynamical friction. As an illustrative example, we estimate how the evaporation rate increases for a ~10^5 solar masses globular cluster that decays through dynamical friction into the galactic centre. We discuss the findings of this work in relation to the formation of nuclear star clusters by inspiraling globular clusters.
description: MNRAS in press
Survival of a brown dwarf after engulfment by a red giant star
Creators: name: Maxted, P. F. L.
name: Napiwotzki, R.
name: Dobbie, P. D.
name: Burleigh, M. R.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: (Summary of paper) High resolution optical spectroscopy of the white dwarf WD0137-349 reveals a weak Halpha line in emission, due to a low mass companion in a close orbit. Using this emission feature, and the narrow NLTE core of the white dwarf's Halpha absorption line, we measure the orbital period at 116 minutes, the separation at 0.65Rsun, and the mass ratio m2/m1 = K1/K2 = 0.134+/-0.006. From the mass of the white dwarf (0.39+/-0.035Msun) we derive a mass for the companion of 0.053+/-0.006Msun. This is well below the limit of about 0.075Msun commonly used to distinguish stars from brown dwarfs. The observed infrared flux distribution of WD0137-349 is also consistent with a model of an old brown dwarf spectral type mid T or slightly earlier. The system is detached, and the brown dwarf must have survived a previous phase of common envelope evolution, providing a key observational test for models of this interaction.
description: To appear in Nature on August 3 2006. 13 Pages, 2 figures, 2 tables
Radiola linoides Roth 1789
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Malpighiales
Linaceae
Radiola
Radiola linoides

description: Linum radiola Linnaeus, Species Plantarum 1: 281. 1753.
"Habitat in Europae sabulo inundato." RCN: 2223.
 Lectotype (Jonsell & Jarvis in Nordic J. Bot. 22: 79. 2002): Herb. Clifford: 114, Linum 6 (BM-000558461).
 Current name: Radiola linoides Roth (Linaceae).
 Note: Smith (in Hubbard & Milne-Redhead, Fl. Trop. E. Africa, Linaceae: 11. 1966) wrongly indicated 396.38 (LINN) as a syntype but as this statement implies no intention to indicate a single nomenclatural type (unlike the use of holotype, lectotype or neotype), this is not regarded as a correctable error.
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part L), pp. 610-650 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 635, DOI: 10.5281/zenodo.291971
Searching For Dark Matter with Neutrino Telescopes
Creators: name: Hooper, Dan
name: Silk, Joseph
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: One of the most interesting mysteries of astrophysics is the puzzle of dark matter. Although numerous techniques have been explored and developed to detect this elusive substance, its nature remains unknown. One such method uses large high-energy neutrino telescopes to look for the annihilation products of dark matter annihilations. In this summary article, we briefly review this technique. We describe the calculations used to find the rate of capture of WIMPs in the Sun or Earth and the spectrum of neutrinos produced in the resulting dark matter annihilations. We will discuss these calculations within the context of supersymmetry and models with universal extra dimensions, the lightest supersymmetric particle and lightest Kaluza-Klein particle providing the WIMP candidate in these cases, respectively. We will also discuss the status of some of the experiments relevant to these searches: AMANDA, IceCube and ANTARES.
description: For "Focus on Neutrino Physics" issue of New Journal of Physics
Pulsar Braking Indices, Glitches and Energy Dissipation In Neutron Stars
Creators: name: Alpar, M. A.
name: Baykal, A.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Almost all pulsars with anomalous positive $\ddot Ω$ measurements (corresponding to anomalous braking indices in the range 5$$ 10$^{-7}$) as well as post glitch or interglitch $\ddot Ω$ measurements obey the scaling between $\ddot Ω$ and glitch parameters originally noted in the Vela pulsar. Negative second derivative values can be understood in terms of glitches that were missed or remained unresolved. We discuss the glitch rates and a priori probabilities of positive and negative braking indices according to the model developed for the Vela pulsar. This behavior supports the universal occurrence of a nonlinear dynamical coupling between the neutron star crust and an interior superfluid component. The implied lower limit to dynamical energy dissipation in a neutron star with spindown rate $\dot Ω$ is $\dot E_{diss}> 1.7 \times 10 ^{-6} \dot E_{rot}$. Thermal luminosities and surface temperatures due to dynamical energy dissipation are estimated for old neutron stars which are spinning down as rotating magnetic dipoles beyond the pulsar death line.
description: Accepted for publication in MNRAS
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VIII, Cart. 192 (11 H 77), 295 folios, f. 0202r
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: 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 VIII, Archives départementales de la Côte-d'Or, Cart. 192 (11 H 77), 295 folios, f. 0202r, 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. 0202r, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
Linum strictum Linnaeus 1753
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Malpighiales
Linaceae
Linum
Linum strictum

description: Linum strictum Linnaeus, Species Plantarum 1: 279. 1753.
"Habitat in Monspelii, Hispaniae, Siciliae squalidis." RCN: 2216.
 Lectotype (Hajra in Jain & al. in Fasc. Fl. India 13: 8. 1983): Löfling 246a , Herb. Linn. No. 396.29 (LINN).
 Current name: Linum strictum L. (Linaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part L), pp. 610-650 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 635, DOI: 10.5281/zenodo.291971
An optical search for Low Surface Brightness Galaxies in the Arecibo HI Strip Survey
Creators: name: Trachternach, Clemens
name: Bomans, Dominik J.
name: Haberzettl, Lutz
name: Dettmar, Ralf-Juergen
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In order to estimate the contribution of low surface brightness (LSB) galaxies to the local (z<0.1) galaxy number density, we performed an optical search for LSB candidates in a 15.5 deg^2 part of the region covered by the 65 deg^2 blind Arecibo HI Strip Survey (AHISS). Object detection and galaxy profile fitting were done with analytical algorithms. The detection efficiency and the selection effects were evaluated using large samples of artificial galaxies. Our final catalogue is diameter-limited and contains 306 galaxies with diameters >18" at the limiting surface brightness of mu_{B,lim}=25.2+-0.31 mag/arcsec^2. Of these 306 galaxies, 148 were not catalogued previously. Our results indicate that low surface brightness galaxies contribute at least to 30 % to the local galaxy number density. Without additional distance information, choosing the limiting diameter and the surface brightness at which the diameter is measured is crucial. Depending on these choices, diameter-limited optical catalogues are either biased against LSB galaxies, or contaminated with cosmologically dimmed high surface brightness galaxies, which affects the implied surface brightness distribution. The comparison to the AHISS showed that although optical surveys detect more galaxies per deg^2 than HI surveys, their drawback is the need for spectroscopic follow up observations to derive distances. Blind HI surveys have no diameter limits, but tend to miss gas-poor galaxies and all galaxies which lie outside their redshift limits. HI and optical surveys thus provide complementary information and sample different parts of the LSB galaxy population.
description: 9 pages, 4 tables, 6 figures, accepted by A&A
Electromagnetic form factor of the pion in the space- and time-like regions within the front-form dynamics
Creators: name: de Melo, J. P. B. C.
name: Frederico, T.
name: Pace, E.
name: Salme`, G.
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The pion electromagnetic form factor is calculated in the space- and time-like regions from -10 $(GeV/c)^2$ up to 10 $(GeV/c)^2$, within a front-form model. The dressed photon vertex where a photon decays in a quark-antiquark pair is depicted generalizing the vector meson dominance ansatz, by means of the vector meson vertex functions. An important feature of our model is the description of the on-mass-shell vertex functions in the valence sector, for the pion and the vector mesons, through the front-form wave functions obtained within a realistic quark model. The theoretical results show an excellent agreement with the data in the space-like region, while in the time-like region the description is quite encouraging.
description: 9 pages + 4 figures. To appear in Phys. Lett. B
The Infrared Emission from the Narrow Line Region
Creators: name: Groves, Brent
name: Dopita, Michael
name: Sutherland, Ralph
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present models for the mid- and far- infrared emission from the Narrow Line Region (NLR) of Active Galactic Nuclei (AGN). Using the MAPPINGS III code we explore the effect of typical NLR parameters on the spectral characteristics of the IR emission. These include useful IR emission line ratio diagnostic diagrams for the determination of these parameters, as well as Star formation--AGN mixing diagnostics. We also examine emission line to continuum correlations which would assist in separating the IR emission arising from the NLR from that coming from the inner torus. We find for AGN like NGC 1068 and NGC 4151 that the NLR only contributes ~10% to the total IRAS 25 mum flux, and that other components such as a dusty torus are necessary to explain the total AGN IR emission.
description: 15 pages, 12 figures, accepted for publication in A&A. Paper with full resolution figures available at http://www.mpa-garching.mpg.de/~brent/publications/bgrovesnlrIRpaper.pdf
Growing Surface Tension of Amorphous-Amorphous Interfaces on Approaching the Colloidal Glass Transition
Creators: name: Ganapathi, Divya
name: Nagamanasa, Hima K
name: Sood, A. K.
name: Ganapathy, Rajesh
Publisher: name: arXiv
Year: 2017
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: There is mounting evidence indicating that relaxation dynamics in liquids approaching their glass transition not only becomes increasingly cooperative (1,2) but the relaxing regions also become more compact in shape(3-7). While the surface tension of the interface separating neighboring relaxing regions is thought to play a crucial role in deciding both their size and morphology(8-10), owing to the amorphous nature of these regions, even identifying these interfaces has not been possible in bulk liquids. Here, by devising a scheme to identify self-induced disorder sites in bulk colloidal liquids, we directly quantified the dynamics of interfaces delineating regions of high and low configurational overlap. This procedure also helped unveil a non-monotonicity in dynamical correlations that has never been observed in bulk supercooled liquids. Using the capillary fluctuation method (11,12), we measured the surface tension of amorphous-amorphous interfaces with supercooling and find that it increases rapidly across the mode-coupling area fraction. Remarkably, a similar growth in the surface tension is also seen in the presence of a pinned amorphous wall. Our observations help prune theories of glass formation and opens up new research avenues aimed at tuning the properties of amorphous-amorphous interfaces, and hence the glass itself, in a manner analogous to grain boundary engineering in polycrystals (13).
Ongoing in vivo experience triggers synaptic metaplasticity in the neocortex.
Creators: name: Clem, Roger L.
name: Celikel, Tansu
name: Barth, Alison L.
Publisher: name: Carnegie Mellon University
Year: 2008
Subjects: subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: In vivo experience can occlude subsequent induction of long-term potentiation and enhance long-term depression of synaptic responses. Although a reduced capacity for synaptic strengthening may function to prevent excessive excitation, such an effect paradoxically implies that continued experience or training should not improve and may even degrade neural representations. In mice, we examined the effect of ongoing whisker stimulation on synaptic strengthening at layer 4-2/3 synapses in the barrel cortex. Although N-methyl-d-aspartate receptors were required to initiate strengthening, they subsequently suppressed further potentiation at these synapses in vitro and in vivo. Despite this transition, synaptic strengthening continued with additional sensory activity but instead required the activation of metabotropic glutamate receptors, suggesting a mechanism by which continued experience can result in increasing synaptic strength over time.
Linum tenuifolium subsp. suffruticosum Linnaeus 1753
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Malpighiales
Linaceae
Linum
Linum tenuifolium
Linum tenuifolium l. subsp. suffruticosum (l.) litard.

description: Linum suffruticosum Linnaeus, Species Plantarum 1: 279. 1753.
"Habitat in Regno Valentino." RCN: 2217.
 Neotype (Nicholls in Bot.J. Linn. Soc. 91: 486. 1986): Herb. Tournefort No. 3089 (P).
 Current name: Linum tenuifolium L. subsp. suffruticosum (L.) Litard. (Linaceae).
 Note: Although the Tournefort collection was not studied by Linnaeus, and cannot be the holotype as suggested by Nicholls, the absence of any original material for the name means that this collection can be treated as a neotype (under Art. 9.8).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part L), pp. 610-650 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 635, DOI: 10.5281/zenodo.291971
title: 02_0398
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
Particle Accelerator in Pulsar Magnetospheres: Super Goldreich-Julian Current with Ion Emission from the Neutron Star Surface
Creators: name: Hirotani, Kouichi
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate the self-consistent electrodynamic structure of a particle accelerator in the Crab pulsar magnetosphere on the two-dimensional poloidal plane, solving the Poisson equation for the electrostatic potential together with the Boltzmann equations for electrons, positrons and gamma-rays. If the trans-field thickness of the gap is thin, the created current density becomes sub-Goldreich-Julian, giving the traditional outer-gap solution but with negligible gamma-ray luminosity. As the thickness increases, the created current increases to become super-Goldreich-Julian, giving a new gap solution with substantially screened acceleration electric field in the inner part. In this case, the gap extends towards the neutron star with a small-amplitude positive acceleration field, extracting ions from the stellar surface as a space-charge-limited flow. The acceleration field is highly unscreened in the outer magnetosphere, resulting in a gamma-ray spectral shape which is consistent with the observations.
description: 36 pages, 14 figures, accepted to Astroph. J
Separation of noncommutative differential calculus on quantum Minkowski space
Creators: name: Bachmaier, Fabian
name: Blohmann, Christian
Publisher: name: arXiv
Year: 2005
Subjects: subject: Quantum Algebra (math.QA)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 81R60; 17B37; 46L87

description: Noncommutative differential calculus on quantum Minkowski space is not separated with respect to the standard generators, in the sense that partial derivatives of functions of a single generator can depend on all other generators. It is shown that this problem can be overcome by a separation of variables. We study the action of the universal L-matrix, appearing in the coproduct of partial derivatives, on generators. Powers of he resulting quantum Minkowski algebra valued matrices are calculated. This leads to a nonlinear coordinate transformation which essentially separates the calculus. A compact formula for general derivatives is obtained in form of a chain rule with partial Jackson derivatives. It is applied to the massive quantum Klein-Gordon equation by reducing it to an ordinary q-difference equation. The rest state solution can be expressed in terms of a product of q-exponential functions in the separated variables.
description: 33 pages
Linum tenuifolium Linnaeus 1753
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Malpighiales
Linaceae
Linum
Linum tenuifolium

description: Linum tenuifolium Linnaeus, Species Plantarum 1: 278. 1753.
"Habitat in Galliae, Helvetiae aridis herbosis." RCN: 2209.
 Lectotype (Nicholls in Bot. J. Linn. Soc. 91: 480. 1986 [1985]): Herb. Linn. No. 396.12 (LINN).
 Current name: Linum tenuifolium L. (Linaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part L), pp. 610-650 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 635, DOI: 10.5281/zenodo.291971