cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Magnetic order and energy-scale hierarchy in artificial spin ice
Creators: name: Stopfel, Henry
name: Östman, Erik
name: Chioar, Ioan-Augustin
name: Arnalds, Unnar B.
name: Greving, David
name: Hase, Thomas P. A.
name: Stein, Aaron
name: Hjörvarsson, Björgvin
name: Kapaklis, Vassilios
Publisher: name: arXiv
Year: 2017
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: In order to explain and predict the properties of many physical systems, it is essential to understand the interplay of different energy-scales. Here we present investigations of the magnetic order in thermalised artificial spin ice structures, with different activation energies of the interacting Ising-like elements. We image the thermally equilibrated magnetic states of the nano-structures using synchrotron-based magnetic microscopy. By comparing results obtained from structures with one or two different activation energies, we demonstrate a clear impact on the resulting magnetic order. The differences are obtained by the analysis of the magnetic spin structure factors, in which the role of the activation energies is manifested by distinct short-range order. This demonstrates that artificial spin systems can serve as model systems, allowing the definition of energy-scales by geometrical design and providing the backdrop for understanding their interplay.
description: 8 pages, 5 figures (+ supplementary 6 pages, 4 figures)
Sprawozdanie z I Kongresu Teologii Praktycznej pt. „Polska krajem misyjnym?”, Warszawa, 19–21 września 2016
Creators: name: Giemza, Ks. Bogdan
Publisher: name: Wrocławski Przegląd Teologiczny
Year: 2019

description: Wrocławski Przegląd Teologiczny, Tom 24 Nr 2 (2016)
Cosmology from Planck
Creators: name: Balbi, Amedeo
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: I briefly review some of the main scientific outputs expected from the upcoming Planck mission. Planck will map the CMB sky with 5' resolution and $μ$K sensitivity, with minimal foreground contribution and superb control on systematics. It will collect the entire information enclosed in the temperature primary anisotropy signal and will also get a good measurement of the polarized component of the CMB. This will have profound implications on our knowledge of the physics of the early universe and on the determination of cosmological parameters.
description: Proceedings of the Francesco Melchiorri Memorial Conference (Rome, Italy, April 12-14 2006). To appear in New Astron. Rev
Franz Posset, Johann Reuchlin (1455–1522). A Theological Biography, Arbeiten zur Kirchengeschichte 129, Berlin–Boston: De Gruyter, 2015, XXVI, ss. 917
Creators: name: Pietkiewicz, Ks. Rajmund
Publisher: name: Wrocławski Przegląd Teologiczny
Year: 2019

description: Wrocławski Przegląd Teologiczny, Tom 24 Nr 2 (2016)
Sgt. John Burns's Last Letter
Creators: name: Project Team, Their Finest Hour
Publisher: name: University of Oxford
Year: 2024
Subjects: classificationCode: 430304
subject: British history
classificationCode: 430308
subject: European history (excl. British, classical Greek and Roman)
classificationCode: 430316
subject: International history

description: This record contains the transcript of the last letter sent from Sgt. John Burns to his brother Michael Burns.
Tlaxcala: ¿Un distrito Industrial?
Creators: name: Ortega, Rocío Rosales
Publisher: name: figshare
Year: 2018
Subjects: subject: 160810 Urban Sociology and Community Studies
subject: FOS: Sociology

description: En este artículo se revisan las principales características del distrito industrial y se cuestiona la existencia de un modelo estático y único, ante la diversidad de realidades socioterritoriales. Con base en antecedentes históricos y las características más recientes de la organización territorial de Tlaxcala se analizan las posibilidades de conformación de un distrito industrial textil mexicano. El trabajo se apoya principalmente en la realización de encuestas y entrevistas a empresarios de la entidad.

This article examines the main characteristics of the industrial district. It also questions the existence of a unique and static model with regard to the diversity of socio-territorial realities. Based on the historical background and on the most recent characteristics of industrial organization in Tlaxcala, the possibilities of structuring an industrial district of Mexican textiles are analyzed. This work is mainly founded on polls and interviews carried out to local enterpreneurs
Prompt J/psi plus photon associated electroproduction at DESY HERA
Creators: name: Kniehl, Bernd A.
name: Palisoc, Caesar P.
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We study the production of a prompt J/psi meson in association with a prompt photon in ep deep-inelastic scattering within the factorisation formalism of non-relativistic quantum chromodynamics (NRQCD) and demonstrate that this process provides a clean probe of the colour-octet mechanism at DESY HERA. Our analysis is based on an updated set of non-perturbative NRQCD matrix elements obtained through a joint fit to data on charmonium inclusive hadroproduction from runs I and II at the Fermilab Tevatron.
description: 11 pages, 1 figure, to appear in Eur. Phys. J. C
Spartina cynosuroides Roth 1806
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Poaceae
Spartina
Spartina cynosuroides

description: Dactylis cynosuroides Linnaeus, Species Plantarum 1: 71. 1753.
"Habitat in Virginia, Canada, Lusitania." RCN: 600.
 Lectotype (Hitchcock in Contr. U. S. Natl. Herb. 12: 121. 1908): Clayton 577, Herb. Linn. No. 90.1 (LINN; iso- BM, US).
 Current name:  Spartina cynosuroides  (L.) Roth (Poaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part D), pp. 474-489 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 474, DOI: 10.5281/zenodo.291971
Thomas William Willmott
Creators: name: Project Team, Their Finest Hour
Publisher: name: University of Oxford
Year: 2024
Subjects: classificationCode: 430304
subject: British history
classificationCode: 430308
subject: European history (excl. British, classical Greek and Roman)
classificationCode: 430316
subject: International history

description: The record contains photographs and documents relating to the wartime experiences of Thomas William Willmott.
Quantum Fluctuations from Thermal Fluctuations in Jacobson Formalism
Creators: name: Faizal, Mir
name: Ashour, Amani
name: Alcheikh, Mohammad
name: Asfar, Lina Al
name: Alsaleh, Salwa
name: Mahroussah, Ahmed
Publisher: name: arXiv
Year: 2017
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In the Jacobson formalism general relativity is obtained from thermodynamics. This is done by using the Bekenstein-Hawking entropy-area relation. However, as a black holes will gets smaller, its temperature will increase. This will cause the thermal fluctuations to also increase, and these will in turn correct the Bekenstein-Hawking entropy-area relation. Furthermore, with the reduction in the size of the black hole, quantum effects will also start to dominate. Just as the general relativity can be obtained from thermodynamics in the Jacobson formalism, we propose that the quantum fluctuations to the geometry can be obtained from thermal fluctuations.
description: 9 pages, 3 figues. Publsihed in EPJC, author's affiliation corrected
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome III, Cart. 187 (11 H 72), f. 0042r
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
name: Petot, Frédéric
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: cartulaire
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome III, Archives départementales de la Côte-d'Or, Cart. 187 (11 H 72), f. 0042r, 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 III, Archives départementales de la Côte-d'Or, Cart. 187 (11 H 72), f. 0042r, 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
Additional file 1: of Application of intraoperative lung-protective ventilation varies in accordance with the knowledge of anaesthesiologists: a single-Centre questionnaire study and a retrospective observational study
Creators: name: Kim, Seung
name: Sungwon Na
name: Lee, Woo
name: Hyunwoo Choi
name: Jeongmin Kim
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Questionnaire for the setting up of intraoperative respiratory parameters. (DOCX 12 kb)
Dactylis glomerata subsp. glomerata 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
Liliopsida
Poales
Poaceae
Dactylis
Dactylis glomerata
Dactylis glomerata l. subsp. glomerata

description: Dactylis glomerata Linnaeus, Species Plantarum 1: 71. 1753.
"Habitat in Europae cultis ruderatis." RCN: 601.
 Lectotype (Clayton in Milne-Redhead & Polhill, Fl. Trop. E. Africa, Gramineae 1: 43. 1970): Herb. Linn. No. 90.3 (LINN).
 Generitype of Dactylis Linnaeus (vide Hitchcock, Prop. Brit. Bot.: 120. 1929).
 Current name:  Dactylis glomerata  L. subsp.  glomerata  (Poaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part D), pp. 474-489 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 474, DOI: 10.5281/zenodo.291971
XALQ OG'ZAKI IJODI VOSITASIDA BO'LAJAK BOSHLANG'ICH SINF O'QITUVCHILARINI O'QUVCHILARNING O'QISH SAVODXONLIGINI RIVОJLАNTIRISHNING METОDIK JIHАTLАRI
Creators: name: Oxunova, N.M.
Publisher: name: Zenodo
Year: 2025

description: Ushbu maqolada xalq og‘zaki ijodi namunalari milliy madaniyatning o‘ziga xos qirralarini, urf-odat va qadriyatlarini o‘zida saqlab kelishi hamda belgilangan asarlarning badiiy va axloqiy ma’nosi o‘quvchilarda milliy iftixor, ma’naviy ong va axloqiy tarbiyani mustahkamlashi haqida so’z yuritiladi.
On Universality of Classical Probability with Contextually Labeled Random Variables
Creators: name: Dzhafarov, Ehtibar N.
name: Kon, Maria
Publisher: name: arXiv
Year: 2017
Subjects: subject: Probability (math.PR)
subject: Quantum Physics (quant-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 81P13, 81Q99, 60A99

description: One can often encounter claims that classical (Kolmogorovian) probability theory cannot handle, or even is contradicted by, certain empirical findings or substantive theories. This note joins several previous attempts to explain that these claims are unjustified, illustrating this on the issues of (non)existence of joint distributions, probabilities of ordered events, and additivity of probabilities. The specific focus of this note is on showing that the mistakes underlying these claims can be precluded by labeling all random variables involved contextually. Moreover, contextual labeling also enables a valuable additional way of analyzing probabilistic aspects of empirical situations: determining whether the random variables involved form a contextual system, in the sense generalized from quantum mechanics. Thus, to the extent the Wang-Busemeyer QQ equality for the question order effect holds, the system describing them is noncontextual. The double-slit experiment and its behavioral analogues also turn out to form a noncontextual system, having the same probabilistic format (cyclic system of rank 4) as the one describing spins of two entangled electrons.
description: 10 pp. Version 3 is a minor revision
The quadruple-lined, doubly-eclipsing system V482 Persei
Creators: name: Torres, Guillermo
name: Lacy, Claud H. Sandberg
name: Fekel, Francis C.
name: Wolf, Marek
name: Muterspaugh, Matthew W.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We report spectroscopic and differential photometric observations of the A-type system V482 Per that reveal it to be a rare hierarchical quadruple system containing two eclipsing binaries. One has the previously known orbital period of 2.4 days and a circular orbit, and the other a period of 6 days, a slightly eccentric orbit (e = 0.11), and shallow eclipses only 2.3% deep. The two binaries revolve around their common center of mass in a highly elongated orbit (e = 0.85) with a period of 16.67 yr. Radial velocities are measured for all components from our quadruple-lined spectra, and are combined with the light curves and with measurements of times of minimum light for the 2.4 day binary to solve for the elements of the inner and outer orbits simultaneously. The line-of-sight inclination angles of the three orbits are similar, suggesting they may be close to coplanar. The available observations appear to indicate that the 6 day binary experiences significant retrograde apsidal motion in the amount of about 60 degrees per century. We derive absolute masses for the four stars good to better than 1.5%, along with radii with formal errors of 1.1% and 3.5% for the 2.4 day binary and about 9% for the 6 day binary. A comparison of these and other physical properties with current stellar evolution models gives excellent agreement for a metallicity of [Fe/H] = -0.15 and an age of 360 Myr.
description: 15 pages in emulateapj format, including figures and tables. Accepted for publication in The Astrophysical Journal
Aeluropus lagopoides Thwaites
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Poaceae
Aeluropus
Aeluropus lagopoides

description: Dactylis lagopoides Linnaeus, Systema Naturae, ed. 12, 2: 95; Mantissa Plantarum: 33. 1767.
"Habitat in India. Burmannus." RCN: 603.
 Lectotype (Renvoize in Cafferty & al. in Taxon 49: 250. 2000): J. Burman s.n., Herb. Linn. No. 90.5 (LINN), see p. 196.
 Current name:  Aeluropus lagopoides  (L.) Trin. ex Thwaites (Poaceae).
 Note: Bor (in Rechinger, Fl. Iranica 70: 419. 1970) indicated a Burman specimen at L as type, but no relevant material has been traced there. Meikle (Fl. Cyprus 2: 1846. 1985) and Sherif & Siddiqi (in Jafri & El-Gadi, Fl. Libya 145: 233. 1988) indicated material at LINN as type, but as they did not distinguish between three possible sheets at LINN, which are not part of a single gathering (Art. 9.15), no effective choice of type was made.
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part D), pp. 474-489 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 474, DOI: 10.5281/zenodo.291971
Sprawozdanie z Konferencji Międzynarodowej „Stones, Tablets and Scrolls. Four Periods of the Formation of the Bible Pontificio Istituto Biblico”, Rzym, 11–13 maja 2017 r.
Creators: name: Rambiert-Kwaśniewska, Anna
Publisher: name: Wrocławski Przegląd Teologiczny
Year: 2019

description: Wrocławski Przegląd Teologiczny, Tom 25 Nr 1 (2017)
The Tale of Father and Son Lost to War
Creators: name: Project Team, Their Finest Hour
Publisher: name: University of Oxford
Year: 2024
Subjects: classificationCode: 430304
subject: British history
classificationCode: 430308
subject: European history (excl. British, classical Greek and Roman)
classificationCode: 430316
subject: International history

description: My grandfather, Thomas, was a Royal Marine who died on his 40th birthday in 1914, leaving behind a widow and four sons. One of those sons, my uncle Jim, died at El Alamein, leaving a widow and two young children. His mother (my grandmother) was already dying and was not informed of the news. A wife and mother so affected by war!
North-South Asymmetry of Solar Activity during Cycle 23
Creators: name: Joshi, Bhuwan
name: Pant, P.
name: Manoharan, P. K.
name: Pandey, Kavita
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In this paper, we have made a statistical analysis of solar H$α$ flares that occurred during the period 1996 to 2005 to investigate their spatial distribution with respect to northern and southern hemispheres of the Sun. The analysis includes a total of 21608 single events. The study shows a significant N$-$S asymmetry which is persistent with the evolution of the solar cycle. The flare activity favors the northern hemisphere in general during the rising and maximum phase of the solar cycle (i.e., in 1997, 1999, and 2000), while the declining phase (i.e., from 2001 to 2005) shows a southern dominance. Further, the monthly N$-$S asymmetry index for flares, sunspot numbers and sunspot areas suggests similar variations for these phenomena with the progress of solar cycle. We also find that in terms of asymmetric behavior of solar flares, cycle 23 seems to act quite differently from cycle 22 but comparably to cycle 21.
description: Published in "Physics of Chromospheric Plasmas", ASP Conference Series, 368, 539 (2007)
An Alternative Explanation of the Varying Boron to Carbon in Galactic Cosmic rays
Creators: name: Eichler, David
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: It is suggested that the decline with energy of the boron to carbon abundance ratio in Galactic cosmic rays is due, in part, to a correlation between the maximum energy attainable by shock acceleration in a given region of the Galactic disk and the grammage traversed before escape. In this case the energy dependence of the escape rate from the Galaxy may be less than previously thought and the spectrum of antiprotons becomes easier to understand.
description: published in the Astrophysical Journal
Harnessing optical micro-combs for microwave photonics
Creators: name: Wu, Jiayang
name: Xu, Xingyuan
name: Nguyen, Thach G.
name: Chu, Sai T.
name: Little, Brent E.
name: Morandotti, Roberto
name: Mitchell, Arnan
name: Moss, David J.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: In the past decade, optical frequency combs generated by high-Q micro-resonators, or micro-combs, which feature compact device footprints, high energy efficiency, and high-repetition-rates in broad optical bandwidths, have led to a revolution in a wide range of fields including metrology, mode-locked lasers, telecommunications, RF photonics, spectroscopy, sensing, and quantum optics. Among these, an application that has attracted great interest is the use of micro-combs for RF photonics, where they offer enhanced functionalities as well as reduced size and power consumption over other approaches. This article reviews the recent advances in this emerging field. We provide an overview of the main achievements that have been obtained to date, and highlight the strong potential of micro-combs for RF photonics applications. We also discuss some of the open challenges and limitations that need to be met for practical applications.
description: 32 Pages, 13 Figures, 172 References
Dais cotinifolia Linnaeus 1762
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
Malvales
Thymelaeaceae
Dais
Dais cotinifolia

description: Dais cotinifolia Linnaeus, Species Plantarum, ed. 2, 1: 556. 1762.
"Habitat ad Cap. b. spei." RCN: 3066.
 Lectotype (Peterson in Polhill, Fl. Trop. E. Africa, Thymelaeaceae: 16. 1978): Herb. Linn. No. 554.1 (LINN).
 Generitype of Dais Linnaeus.
 Current name:  Dais cotinifolia  L. (Thymelaeaceae).
 Note: Fuchs in Acta Bot. Neerl. 11: 74. 1962) argued that as Linnaeus’ description came from David van Royen, an illustration of the plant from Leiden, published later by Meerburg, should be the holotype. This could have been an effective neotypification (Art. 9.8) but for the existence of original material (Herb. Linn. 554.1, LINN), subsequently designated as type by Peterson.
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part D), pp. 474-489 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 474, DOI: 10.5281/zenodo.291971
Additional file 1: of Social value of a nutritional counselling and support program for breastfeeding in urban poor settings, Nairobi
Creators: name: Goudet, Sophie
name: Griffiths, Paula
name: Wainaina, Caroline
name: Macharia, Teresia
name: Wekesah, Frederick
name: Wanjohi, Milka
name: Muriuki, Peter
name: Kimani-Murage, Elizabeth
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Cancer
subject: 60506 Virology
subject: FOS: Biological sciences
subject: Computational Biology

description: Table S1.Steps in the proposed Baby Friendly Community Initiative (BFCI) program in Kenya, Step Description, Table S2. Content of counselling messages, Table S4.List of stakeholders, Table S5. Assumptions for base case scenario variables. (DOCX 18Â kb)
Lepton Number Violation: Seesaw Models and Their Collider Tests
Creators: name: Cai, Yi
name: Han, Tao
name: Li, Tong
name: Ruiz, Richard
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The Majorana nature of neutrinos is strongly motivated from the theoretical and phenomenological point of view. A plethora of neutrino mass models, known collectively as Seesaw models, exist that could generate both a viable neutrino mass spectrum and mixing pattern. They can also lead to rich, new phenomenology, including lepton number non-conservation as well as new particles, that may be observable at collider experiments. It is therefore vital to search for such new phenomena and the mass scale associated with neutrino mass generation at high energy colliders. In this review, we consider a number of representative Seesaw scenarios as phenomenological benchmarks, including the characteristic Type I, II, and III Seesaw mechanisms, their extensions and hybridizations, as well as radiative constructions. We present new and updated predictions for analyses featuring lepton number violation and expected coverage in the theory parameter space at current and future colliders. We emphasize new production and decay channels, their phenomenological relevance and treatment across different facilities in $e^+e^-$, $e^-p$ and $pp$ collisions, as well as the available Monte Carlo tools available for studying Seesaw partners in collider environments.
description: 92 pages, 43 figures. Invited Article for the 'Frontiers in Physics' Research Topic 'The Physics Associated with Neutrino Masses'
Phaleria octandra Baill.
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
Malvales
Thymelaeaceae
Phaleria
Phaleria octandra

description: Dais octandra Linnaeus, Systema Naturae, ed. 12, 2: 297; Mantissa Plantarum: 69. 1767.
"Habitat in India." RCN: 3067.
 Lectotype (Ding Hou in van Steenis, Fl. Malesiana, ser. I, 6: 18. 1960): Herb. Linn. No. 554.2 (LINN).
 Current name:  Phaleria octandra  (L.) Baill. (Thymelaeaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part D), pp. 474-489 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 474, DOI: 10.5281/zenodo.291971
$η^{(\prime)}$ productions in semileptonic B decays
Creators: name: Chen, Chuan-Hung
name: Geng, Chao-Qiang
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: Inspired by the new measurements on $B^{-}\to η^{(\prime)}\ell \barν_{\ell}$ from the BaBar Collaboration, we examine the constraint on the flavor-singlet mechanism, proposed to understand the large branching ratios for $B\to η^{\prime} K$ decays. Based on the mechanism, we study the decays of $\bar B_{d,s}\to η^{(\prime)} \ell^{+} \ell^{-}$ and find that they are sensitive to the flavor-singlet effects. In particular, we show that the decay branching ratios of $\bar B_{d,s}\to η^{\prime} \ell^{+} \ell^{-}$ can be as large as $O(10^{-8})$ and $O(10^{-6})$, respectively.
description: 10 pages, 2 figures, final version to appear in Phys. Lett. B
Additional file 1: of Implementation of clinical practice guidelines on lifestyle interventions in Swedish primary healthcare – a two-year follow up
Creators: name: Kardakis, Therese
name: Jerdén, Lars
name: Nyström, Monica
name: Weinehall, Lars
name: Johansson, Helene
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 60506 Virology

description: Questionnaire. (DOCX 19 kb)
Manchester's Best Kept WW2 Secret, Perhaps?
Creators: name: Project Team, Their Finest Hour
Publisher: name: University of Oxford
Year: 2024
Subjects: classificationCode: 430304
subject: British history
classificationCode: 430308
subject: European history (excl. British, classical Greek and Roman)
classificationCode: 430316
subject: International history

description: I am the owner of the Greater Manchester Blitz Victims website www.greatermanchesterblitzvictims.co.uk and I stumbled across 12 deaths whose cause of death had been lost in the midst of time and, of course, the efficiency of the war-time censor. The full story is attached in a local history document that I wrote in 2020.
Dalechampia scandens 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
Euphorbiaceae
Dalechampia
Dalechampia scandens

description: Dalechampia scandens Linnaeus, Species Plantarum 2: 1054. 1753.
"Habitat in America meridionali." RCN: 7261.
 Lectotype (Howard, Fl. Lesser Antilles 5: 42. 1989): [icon] "Lupulus folio trifido, fructu tricocco et hispido" in Plumier, Descr. Pl. Amér.: 87, t. 101. 1693.
 Generitype of Dalechampia Linnaeus.
 Current name:  Dalechampia scandens  L. (Euphorbiaceae).
 Note: Radcliffe-Smith (in Polhill, Fl. Trop. E. Africa, Euphorbiaceae: 287 (1987) wrongly indicated 1138.3 (LINN), a sheet annotated only by Linnaeus filius and not original material for the name, as holotype. Armbruster (in Syst. Bot. 13: 310. 1988) stated the type "is presumably in Hortus Cliffortianus Herb. (BM)", but no specimen is preserved there.
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part D), pp. 474-489 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 474, DOI: 10.5281/zenodo.291971
Relativistic shock breakout from a stellar wind
Creators: name: Granot, Alon
name: Nakar, Ehud
name: Levinson, Amir
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We construct an analytic model for the breakout of a relativistic radiation mediated shock from a stellar wind, and exploit it to calculate the observational diagnostics of the breakout signal. The model accounts for photon escape through the finite optical depth wind, and treats the fraction of downstream photons escaping to infinity as an adiabatic parameter that evolves in a quasi-steady manner. It is shown that the shock is mediated by radiation even when a large fraction of the downstream photons escape, owing to self-generation and adjustment of opacity through accelerated pair creation. Relativistic breakout occurs at radii at which the total optical depth of the wind ahead of the shock is $\sim (m_e/m_p)Γ_{sh}$, provided that the local shock Lorentz factor $Γ_{sh}$ exceeds unity at this location. Otherwise the breakout occurs in the Newtonian regime. A relativistic breakout is expected in a highly energetic spherical explosion ($10^{52}-10^{53}$ erg) of a Wolf-Rayet star, or in cases where a smaller amount of energy ($\sim 10^{51}$ erg) is deposited by a jet in the outer layers of the star. The properties of the emission observed in such explosions during the relativistic breakout are derived. We find that for typical parameters about $10^{48}$ ergs are radiated in the form of MeV gamma-rays over a duration that can range from a fraction of a second to an hour. Such a signal may be detectable out to 10-100 Mpc by current gamma-ray satellites.
A note on Sen’s representation of the Gini coefficient: Revision and repercussions
Creators: name: Stark, Oded
Publisher: name: Unknown
Year: 2024
Subjects: subject: International Development
subject: Sen’s definition of the Gini coefficient of income inequality
subject: Aggregate income-related depression of a population
subject: A “well-behaved” Gini coefficient

description: Sen (1973 and 1997) presents the Gini coefficient of income inequality in a population as follows. “In any pair-wise comparison the man with the lower income can be thought to be suffering from some depression on finding his income to be lower. Let this depression be proportional to the difference in income. The sum total of all such depressions in all possible pair-wise comparisons takes us to the Gini coefficient.” (This citation is from Sen 1973, p. 8.) Sen’s verbal account is accompanied by a formula (Sen 1997, p. 31, eq. 2.8.1), which is replicated in the text of this note as equation (1). The formula yields a coefficient bounded from above by a number smaller than 1. This creates a difficulty, because the “mission” of a measure of inequality defined on the unit interval is to accord 0 to perfect equality (maximal equality) and 1 to perfect inequality (maximal inequality). In this note we show that when the Gini coefficient is elicited from a neat measure of the aggregate income-related depression of the population that consists of the people who experience income-related depression, then the obtained Gini coefficient is “well behaved” in the sense that it is bounded from above by 1. We conjecture a reason for a drawback of Sen’s definition, and we present repercussions of the usage of the “well-behaved” Gini coefficient.
Reverberation Mapping of High-Luminosity Quasars: First Results
Creators: name: Kaspi, Shai
name: Brandt, W. N.
name: Maoz, Dan
name: Netzer, Hagai
name: Schneider, Donald P.
name: Shemmer, Ohad
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Reverberation mapping of nearby active galactic nuclei has led to estimates of broad-line-region (BLR) sizes and central-object masses for some 37 objects to date. However, successful reverberation mapping has yet to be performed for quasars of either high luminosity (above L_opt~10^{46} erg/s) or high redshift (z>0.3). Over the past six years, we have carried out, at the Hobby-Eberly Telescope, rest-frame-ultraviolet spectrophotometric monitoring of a sample of six quasars at redshifts z=2.2--3.2, with luminosities of L_opt~10^{46.4}--10^{47.6} erg/s, an order of magnitude greater than those of previously mapped quasars. The six quasars, together with an additional five having similar redshift and luminosity properties, were monitored photometrically at the Wise Observatory during the past decade. All 11 quasars monitored show significant continuum variations of order 10%--70%. This is about a factor of two smaller variability than for lower luminosity quasars monitored over the same rest-frame period. In the six objects which have been spectrophotometrically monitored, significant variability is detected in the CIV1550 broad emission line. In several cases the variations track the continuum variations in the same quasar, with amplitudes comparable to, or even greater than, those of the corresponding continua. In contrast, no significant Lyαvariability is detected in any of the four objects in which it was observed. Thus, UV lines may have different variability trends in high-luminosity and low-luminosity AGNs. For one quasar, S5~0836+71 at z=2.172, we measure a tentative delay of 595 days between CIV and UV-continuum variations, corresponding to a rest-frame delay of 188 days and a central black-hole mass of 2.6\times10^9 M_\odot.
description: 11 pages, 6 figures, emulateapj, accepted for publication in The Astrophysical Journal
Long-term photometric study of a faint W UMa binary in the direction of M31
Creators: name: Joshi, Yogesh C.
name: Jagirdar, Rukmini
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We carry out a re-analysis of the photometric data in Cousin RI bands which was taken under the Nainital Microlensing Survey during 1998 to 2002 with the aim to detect gravitational microlensing events in the direction of M31. Here, we do photometric analysis of a faint W UMa binary CSS_J004259.3+410629 identified in the target field. The orbital period of this star is found to be 0.266402+/-0.000018 day. The photometric mass ratio, q, is found to be 0.28+/-0.01. The photometric light curves are investigated using the Wilson-Devinney code and absolute parameters are determined using empirical relations which provide masses and radii of the binary as M1 = 1.19+/-0.09 Msun, M2 = 0.33+/-0.02 Msun and R1 = 1.02+/-0.04 Rsun, R2 = 0.58+/-0.08 Rsun based on the Rc band data. Almost similar values are found by analysing Ic band data. From the photometric light curve examination, the star is understood to be a low mass-ratio over-contact binary of A-subtype with a high fill-out factor of about 47%. The binary system is found to be located approximately at a distance of 2.64+/-0.03 kpc having a separation of 2.01+/-0.05 Rsun between the two components.
description: 14 pages, 8 figures, 4 tables, accepted for publication in Research in Astronomy and Astrophysics
The Angular Diameter of $λ$ Boötis}
Creators: name: Ciardi, David R.
name: van Belle, Gerard T.
name: Boden, Andrew F.
name: Brummelaar, T. ten
name: McAlister, H. A.
name: Bagnuolo,, W. G.
name: Goldfinger, P. J.
name: Sturmann, J.
name: Sturmann, L.
name: Turner, N.
name: Berger, D. H.
name: Thompson, R. R.
name: Ridgway, S. T.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Using the CHARA Array and the Palomar Testbed Interferometer, the chemically peculiar star $λ$ Boötis has been spatially resolved. We have measured the limb darkened angular diameter to be $θ_{LD} = 0.533\pm0.029$ mas, corresponding to a linear radius of $R_{\star} = 1.70 \pm 0.10 R_\odot$. The measured angular diameter yields an effective temperature for $λ$ Boo of $T_{eff} = 8887 \pm 242$ K. Based upon literature surface gravity estimates spanning $\log{(g)} = 4.0-4.2$ $[\rm{cm s}^{-\rm{2}}]$, we have derived a stellar mass range of $M_{\star} = 1.1 - 1.7$ $M_\odot$. For a given surface gravity, the linear radius uncertainty contributes approximately $σ(M_\star) = 0.1-0.2 M_\odot$ to the total mass uncertainty. The uncertainty in the mass (i.e., the range of derived masses) is primarily a result of the uncertainty in the surface gravity. The upper bound of our derived mass range ($\log(g)=4.2, M_\star = 1.7\pm0.2 M_\odot$) is consistent with 100-300 MYr solar-metallicity evolutionary models. The mid-range of our derived masses ($\log(g)=4.1, M_\star = 1.3\pm0.2 M_\odot$) is consistent with 2-3 GYr metal-poor evolutionary models. A more definitive surface gravity determination is required to determine a more precise mass for $λ$ Boo.
description: Accepted for publication in The Astrophysical Journal
A repetition code of 15 qubits
Creators: name: Wootton, James R.
name: Loss, Daniel
Publisher: name: arXiv
Year: 2017
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The repetition code is an important primitive for the techniques of quantum error correction. Here we implement repetition codes of at most $15$ qubits on the $16$ qubit \emph{ibmqx3} device. Each experiment is run for a single round of syndrome measurements, achieved using the standard quantum technique of using ancilla qubits and controlled operations. The size of the final syndrome is small enough to allow for lookup table decoding using experimentally obtained data. The results show strong evidence that the logical error rate decays exponentially with code distance, as is expected and required for the development of fault-tolerant quantum computers. The results also give insight into the nature of noise in the device.
description: 7 pages
Magnetic Stability Analysis for Abelian and Non-Abelian Superconductors
Creators: name: He, Lianyi
name: Jin, Meng
name: Zhuang, Pengfei
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We investigate the origin of Abelian and non-Abelian type magnetic instabilities induced by Fermi surface mismatch between the two pairing fermions in a non-relativistic model. The Abelian type instability occurs only in gapless state and the Meissner mass squared becomes divergent at the gapless-gapped transition point, while the non-Abelian type instability happens in both gapless and gapped states and the divergence vanishes. The non-Abelian type instability can be cured in strong coupling region.
description: 7 pages, 2 figures, more references added, accepted for publication in PRD
Dalibarda repens 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
Rosales
Rosaceae
Dalibarda
Dalibarda repens

description: Dalibarda repens Linnaeus, Species Plantarum 1: 491. 1753.
"Habitat in Canada. Kalm." RCN: 3768.
 Replaced synonym of: Rubus dalibarda L. (1762), nom. illeg.
 Lectotype (Reveal in Jarvis & al, Regnum Veg. 127: 41. 1993): Kalm, Herb. Linn. No. 653.24 (LINN).
 Generitype of Dalibarda Linnaeus.
 Current name:  Dalibarda repens  L. (Rosaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part D), pp. 474-489 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 474, DOI: 10.5281/zenodo.291971
Illuminating the Hidden Sector of String Theory by Shining Light through a Magnetic Field
Creators: name: Abel, Steven A.
name: Jaeckel, Joerg
name: Khoze, Valentin V.
name: Ringwald, Andreas
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Many models of physics beyond the Standard Model predict minicharged particles to which current and near future low-energy experiments are highly sensitive. Such minicharges arise generically from kinetic-mixing in theories containing at least two U(1) gauge factors. Here, we point out that the required multiple U(1) factors, the size of kinetic-mixing, and suitable matter representations to allow for a detection in the near future occur naturally in the context of string theory embeddings of the Standard Model. A detection of minicharged particles in a low energy experiment would likely be a signal of an underlying string theory and may provide a means of testing it.
description: 6 pages, 4 figures; v2 contains an extended discussion of some technical issues and an update on the experimental situation
Additional file 9: of Unexpected conservation of the RNA splicing apparatus in the highly streamlined genome of Galdieria sulphuraria
Creators: name: Qiu, Huan
name: Rossoni, Alessandro W.
name: Weber, Andreas
name: Yoon, Hwan
name: Debashish Bhattacharya
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology

description: Table S5. The intron statistics in red algal and Viridiplantae genomes. (PDF 71Â kb)
Multi-wavelength Study of Young Massive Star Clusters in the Interacting Galaxy ARP 24
Creators: name: Cao, Chen
name: Wu, Hong
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We made a multi-wavelength study of young massive star clusters (YSCs) in the interacting galaxy ARP 24, using the optical and ultraviolet images from Hubble Space Telescope (HST), Sloan Digital Sky Survey, and Galaxy Evolution Explorer; the mid-infrared images from Spitzer Space Telescope; and the narrow-band Ha image and optical spectra from the NAOC 2.16m telescope. Based on the HST images, we found that the brightest infrared knot in ARP 24 is associated with a complex of five young massive star clusters, within a region of ~ 0.95" radius (127pc) in size. The ages and masses of the star clusters in this complex and other regions were estimated using HST broadband photometries and the Starburst99 synthesis models. The star clusters in this complex are very young (within ages of ~ 3-5 Myr) and massive (masses of ~ 10^5 Msun). The ionization parameter and metallicity of the complex were estimated using the emission line ratios, and the star formation rates were calculated using monochromatic 24um, FUV, and Ha line luminosities. We speculate that ARP 24 may formed by a retrograde fly-by encounter indicated by its one-armed appearance and fan-like structure, and the formation of the YSCs in this galaxy is triggered by the interaction. The clusters in the YSC complex may formed in a single giant molecular cloud simultaneously. From the ultraviolet to mid-infrared spectral energy distributions, we found that the region of the YSC complex is relatively bluer in optical and has higher 24um dust emission relative to the starlight and 8um emission. This warm infrared color may due to strong UV radiation field or other mechanisms (e.g., shocks) within this region which may destroy the Polycyclic Aromatic Hydrocarbons and enhance the small grain emission at 24um.
description: 33 pages, 9 figures, accepted for publication in AJ
Daphne alpina 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
Malvales
Thymelaeaceae
Daphne
Daphne alpina

description: Daphne alpina Linnaeus, Species Plantarum 1: 356. 1753.
"Habitat in Alpibus Helvetiae, Genevae, Italiae." RCN: 2822.
 Lectotype (Urbani in Taxon 40: 494. 1991): [icon] "Chamelaea Alpina incana" in Plantin, Pl. Stirp. Icon.: 370. 1581.
 Current name:  Daphne alpina  L. (Thymelaeaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part D), pp. 474-489 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 474, DOI: 10.5281/zenodo.291971
On the theory of magnetar QPOs
Creators: name: Levin, Yuri
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We consider torsional oscillations of magnetars. This problem features rich dynamics due to the strong interaction between the normal modes of a magnetar's crust and a continuum of Magneto-Hydro-Dynamic (MHD) modes in its fluid core. We study the dynamics using a simple model of a magnetar possessing a uniform magnetic field and a thin spherical crust. Firstly, we show that global torsional modes only exist when one introduces unphysically large dissipative terms into the equations of motion; thus global modes are not helpful for understanding the magnetar Quasi-Periodic Oscillations (QPOs). Secondly, we solve the initial-value problem by simulating the sudden release of an initially strained crust and monitoring the subsequent crustal motion. We find that the crustal torsional modes quickly exchange their energy with the MHD continuum in the core, and decay by several orders of magnitude over the course of about 10 oscillation periods. After the initial rapid decay, the crustal motion is stabilized and several time-varying QPOs are observed. The dynamical spectrum of the simulated crustal motion is in qualitative agreement with that of the x-ray light-curve in the tail of a giant magnetar flare. The asymptotic frequencies of some of the QPOs are associated with the special spectral points--the turning points or edges--of the MHD continuum, and are not related to those of the crust. The observed steady low-frequency QPO at 18 Hz is almost certainly associated with the lowest frequency of the MHD continuum, or its first overtone. We also find that drifting QPOs get amplified when they come near the frequencies of the crustal modes. This explains why some of the observed QPOs have frequencies close to the expected crustal frequencies, and why these QPOs are highly variable with time.
description: 10 pages, submitted to MNRAS
Additional file 8: of Unexpected conservation of the RNA splicing apparatus in the highly streamlined genome of Galdieria sulphuraria
Creators: name: Qiu, Huan
name: Rossoni, Alessandro W.
name: Weber, Andreas
name: Yoon, Hwan
name: Debashish Bhattacharya
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology

description: Figure S3. Sequence conservation in Galdieria sulphuraria genes. (PDF 181Â kb)