cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: Re:Collections - Collection Motivations and Methodologies as Imagery, Metaphor and Process in Contemporary Art
Creators: name: Berry, Jessica
Publisher: name: Griffith University
Year: 2006
Subjects: subject: Collection art
subject: ethnographic art
subject: museum interventions
subject: museum fictions
subject: artist museums
subject: collection motivations
subject: contemporary art

description: By the 1990's many modes of artwork incorporated the constructs of the museum. Art forms including, 'ethnographic art', 'museum interventions', 'museum fictions' and 'artist museums' were considered to be located in similar realms to each other. These investigations into this emerging 'genre' of collection-art have primarily focussed upon the critique of the public museum and its grand-narratives. This thesis will attempt to recognise that the critique of institutional hierarchical systems is now considered integral to much collection art and extends this enquiry to incorporate private collections which examine the narratives of everyday existence. This paper adopts an interdisciplinary approach to material culture and art criticism in examining everyday objects within contemporary collection-art. In this context, this paper argues that: the investigation of collection motivations (fetish, souvenir and system) as metaphor, process and imagery in conjunction with the mimicking of museology methodologies (classification, order and display) is an effective model for interpreting everyday objects within contemporary collection-art. In formulating this argument, this paper examines the ways in which artists emulate museology methodologies in order to convey cultural significance for everyday objects. This is explored in conjunction with the employment of collection motivations by artists as a device to understand elements of human/object relations. In doing so, it contemplates the convergence between the practices of museums and collection-artists. These issues are explored through the visual and analytic investigations of key artist case studies including: Damien Hirst, Sylvie Fleury, Mike Kelley, Christian Boltanski, On Kawara, Luke Roberts, Jason Rhoades, Karsten Bott and Elizabeth Gower. In doing so, this paper argues that the everyday objects of collection-art can represent a broad range of socio/cultural concerns, so delineating a closer relationship between collection-art and material culture.
title: Offence Specialization and Versatility in Men Convicted of Sexual Offences and Referred for Civil Commitment
Creators: name: Harris, Danielle Arlanda
Publisher: name: Griffith University
Year: 2008
Subjects: subject: sexual offences
subject: offence specialization
subject: offence specialisation
subject: persistent offenders
subject: offence versatility
subject: criminal history
subject: criminal histories
subject: criminal offenders
subject: criminal offences
subject: criminal psychology
subject: criminal rehabilitation

description: It has long been recognized that, while many offenders have only a limited or occasional involvement in crime, a small group of persistent offenders is responsible for a disproportionately large volume of crime. The question of whether persistent offenders repeatedly engage in a particular type of crime (offence specialization) or commit a diverse range of offences (offence versatility) has in turn generated considerable research attention. Persistent offenders have generally been found to be versatile in their criminal activity, although offence specialization has also been observed to varying degrees for certain offence types. Persistence and offence specialization are implied in much of the existing theoretical and empirical literature on sexual offending, but researchers have only recently begun to systematically test these assumptions. The present thesis presents three empirical studies that together aim to contribute to emerging knowledge concerning offence specialization and versatility among sexual offenders. All three studies are based on a sample of 566 sexual offenders who were referred to the Massachusetts Treatment Center for Sexually Dangerous Persons (MTC) in Bridgewater, Massachusetts between 1959 and 1984. Approximately half (n = 315) (the ‘observed’ group) were assessed as not sexually dangerous, and released either into the community or back into prison to serve the remainder of their sentence. The remainder (n = 251) (the ‘committed’ group) were adjudged to be sexually dangerous, civilly committed, and eventually released. Criminal histories, MTC assessment data, and post-release recidivism data were obtained...
Additional file 1 of Alkaline post-incubation improves the saccharification of poplar after hydrogen peroxide–acetic acid pretreatment
Creators: name: Wen, Peiyao
name: Zhang, Ying
name: Zhu, Junjun
name: Xu, Yong
name: Zhang, Junhua
Publisher: name: figshare
Year: 2021
Subjects: subject: Biochemistry
subject: Space Science
subject: Physical Sciences not elsewhere classified
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Neuroscience
subject: Physiology
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: Astronomical and Space Sciences not elsewhere classified
subject: Plant Biology
subject: Cardiology

description: Additional file 1: Fig. S1 Relationship between lignin contents and the monosaccharide yields of HPAA- and HPAA–SH-pretreated poplar. Fig. S2 Relationship between acetyl contents and the monosaccharide yields of HPAA- and HPAA–SH-pretreated poplar.
Where is the Inner Edge of an Accretion Disk Around a Black Hole?
Creators: name: Krolik, Julian H.
name: Hawley, John F.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: What is meant by the "inner edge" of an accretion disk around a black hole depends on the property that defines the edge. We discuss four such definitions using data from recent high-resolution numerical simulations. These are: the "turbulence edge", where flux-freezing becomes more important than turbulence in determining the magnetic field structure; the "stress edge", where plunging matter loses dynamical contact with the outer accretion flow; the "reflection edge", the smallest radius capable of producing significant X-ray reflection features; and the "radiation edge", the innermost place from which significant luminosity emerges. All these edges are dependent on the accretion rate and are non-axisymmetric and time-variable. Although all are generally located in the vicinity of the marginally stable orbit, significant displacements can occur, and data interpretations placing the disk edge precisely at this point can be misleading. If observations are to be used successfully as diagnostics of accretion in strong gravity, the models used to interpret them must take careful account of these distinctions.
description: accepted by Ap.J., 26 pp
Editorial: Higher Education and Democracy: a work in progress…
Creators: name: Kamarianos, Ioannis
name: Katsills, Michael
name: Zorbas, Vasilis
Publisher: name: Academia
Year: 2017
Subjects: Higher Education, Democracy, Citizenship

description: Presentation of the specific Issue.
description: Academia, No 9 (2017): Higher Education, Citizenship and Democracy: a work in progress
Reversible thermal diode and energy harvester with a superconducting quantum interference single-electron transistor
Creators: name: Goury, Donald
name: Sánchez, Rafael
Publisher: name: arXiv
Year: 2019
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: The density of states of proximitized normal nanowires interrupting superconducting rings can be tuned by the magnetic flux piercing the loop. Using these as the contacts of a single-electron transistor allows to control the energetic mirror asymmetry of the conductor, this way introducing rectification properties. In particular, we show that the system works as a diode that rectifies both charge and heat currents and whose polarity can be reversed by the magnetic field and a gate voltage. We emphasize the role of dissipation at the island. The coupling to substrate phonons enhances the effect and furthermore introduces a channel for phase tunable conversion of heat exchanged with the environment into electrical current.
description: 5 pages, 4 figures. Accepted version
L'enseignement supérieur brésilien: Repères historiques, statistiques et politiques
Creators: name: Charlot, Bernard
name: Anahí Da Silva, Veleida
Publisher: name: Academia
Year: 2017
Subjects: Higher education in Brazil; Universities; Policies of democratization

description: Cet article présente les repères historiques, statistiques et politiques permettant de connaître et comprendre l'enseignement supérieur brésilien. Les universités brésiliennes sont apparues tardivement et aujourd'hui encore l'enseignement supérieur brésilien est constitué principalement par une multitude d'établissements privés, souvent de petite taille. Les gouvernements de gauche (2003-2016) ont développé et démocratisé l'enseignement supérieur, par la création d'universités publiques fédérales, l'implantation de quotas sociaux et raciaux etc., mais aussi par l'aide à l'accès d'étudiants dans des établissements privés This article presents the historical, statistical and political benchmarks that make it possible to know about and understand Brazilian higher education. Brazilian universities have recently made their appearance, but even today Brazilian higher education still consists mainly of a multitude of private institutions, often small in size. Left wing governments (2003-2016) have developed and democratized higher education through the creation of federal public universities, the establishment of social and racial quotas, etc., as well as by helping students to gain access to private higher education institutions.
description: Academia, No 10 (2017): Brazilian Higher Education
HP Lyr - possibly the hottest RV Tau type object
Creators: name: Graczyk, Dariusz
name: Mikolajewski, Maciej
name: Leedjarv, Laurits
name: Frackowiak, Sylwia M.
name: Osiwala, Jedrzej P.
name: Puss, Alar
name: Tomov, Toma
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report Johnson's UBVRI photometric and optical spectroscopic observations of a long period variable HP Lyr which up to now has been considered an eclipsing binary with a period of 140 days. The spectral type changes continually from A2-3 at maxima to A7-F2 at minima. We propose that the brightness changes are caused by the pulsation of the star with two periods: P1=69.35, and P2=2xP1=138.7 days. These periods decreased by more than 1% between 1960 and 1980. The spectral luminosity class determination gives an A type supergiant Iab. HP Lyr is also the optical counterpart of the infrared source IRAS 19199+3950. Relatively high galactic latitude (b=+11.7 degr) and high radial velocity (-113 km/s) indicate that HP Lyr is an evolved, most likely post-AGB star. All presented features argue that this star is an RV Tau type object.
description: 13 pages, 10 figures
Tetrapogon cenchriformis Clayton, Kew Bull.
Creators: name: Prunera-Olivé, Joan
name: Vorontsova, Maria S.
name: Williams, Emma V.
name: Mollel, Neduvoto P.
name: Hemp, Andreas
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Poaceae
Tetrapogon
Tetrapogon cenchriformis

description: Tetrapogon cenchriformis (A.Rich.) Clayton, Kew Bull. 16: 250 (1962).
 Distribution: Cape Verde to Arabian Pen. and Tanzania
 Specimens: MOSHI Holili, Hemp, A. 1845 (NHT, UBT); Kilima Kifaru Peak, Greenway, P.J. 9533 (K); Kisangiro, Peterson, P. 24192 (K); Kiuo Hill, Hemp, A. 1733 (NHT, UBT); Lake Chala, Hemp, A. 1836 (B, C, NHT, UBT).
description: Published as part of Prunera-Olivé, Joan, Vorontsova, Maria S., Williams, Emma V., Mollel, Neduvoto P. & Hemp, Andreas, 2021, Checklist of Kilimanjaro grasses shows that both plot and herbarium methods are necessary to record diversity, pp. 201-244 in Phytotaxa 501 (2) on page 242, DOI: 10.11646/phytotaxa.501.2.1, http://zenodo.org/record/5424816
A proposed theoretical basis for a MOND cosmology: I. The inertial frame
Creators: name: Roscoe, D F
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: This first of two papers is a speculation on the nature of Mach's Principle, derived from the formulation of two questions: (A) Can a globally inertial space and time be associated with a non-trivial global matter distribution? (B) If so, what are the general properties of such a global distribution? The answers are yes subject to the condition that mass is distributed fractally with D=2. Such a prediction is supported, for example, in Joyce, Montuori, Labini astro-ph/9901290. The second paper then shows how gravitational phenomena arise as consequences of perturbations of this equilibrium D=2 distribution, and applies this theory to spiral galaxy dynamics. Specifically, the second paper derives a gravitational model for an idealized spiral, defined to have perfect cylindrical symmetry. One of the main results of this analysis is that, *in the disc*, V_rot = A/R^alpha where (A, alpha) are constants which vary between spirals. See astro-ph/0107305, which concludes that a power-law model is powerfully confirmed for ORCs as a statistical generality over large samples, and astro-ph/0107300 for new phenomonology discovered via this analysis. Thus, unlike MOND, we have only been concerned with model predictions made for idealized matter distributions, and tested over very large numbers of ORCs. But, like those of MOND, the predictions are very powerfully supported on the data. For this reason, we hypothesize that perspectives of MOND are buried within our own formalism. This remains a topic for future work.
description: 30 pages, no figures. Appears in GRG (below) under different title: "Clocks and rods - or something more fundamental"
Tuponia (Tuponia) ayasensis Wagner 1963
Creators: name: Linnavuori, Rauno E.
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Miridae
Tuponia
Tuponia ayasensis

description: Tuponia (Tuponia) ayasensis Wagner, 1963
 Material examined. GILAN: Lowshan, 9 specimens, 8.vii.1996. ZANJAN: Abbar, 2 specimens, 12-14.v.2001; Mamalan, 5 specimens, 12-14.v.2001.
 Comments. On Tamarix. Syrio-Anatolian.
description: Published as part of Linnavuori, Rauno E., 2007, Studies on the Miridae (Heteroptera) of Gilan and the adjacent provinces in northern Iran. II. List of species, pp. 17-56 in Acta Entomologica Musei Nationalis Pragae 47 on page 54, DOI: 10.5281/zenodo.5328235
XMM-Newton Reflection Grating Spectrometer Observations of Discrete Soft-X-ray Emission Features from NGC 1068
Creators: name: Kinkhabwala, A.
name: Sako, M.
name: Behar, E.
name: Kahn, S. M.
name: Paerels, F.
name: Brinkman, A. C.
name: Kaastra, J. S.
name: Gu, M. F.
name: Liedahl, D. A.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the first high-resolution, soft-X-ray spectrum of the prototypical Seyfert 2 galaxy, NGC 1068. This spectrum was obtained with the XMM-Newton Reflection Grating Spectrometer. Emission lines from H-like and He-like low-Z ions (from C to Si) and Fe-L-shell ions dominate the spectrum. Strong, narrow radiative recombination continua (RRC) for several ions are also present, implying that most of the observed soft-X-ray emission arises in low-temperature (few eV) plasma. This plasma is photoionized by the inferred nuclear continuum (obscured along our line of sight), as in the unified model of active galactic nuclei (AGN). We find excess emission (compared with pure recombination) in all resonance lines (np to 1s) up to the photoelectric edge, demonstrating the importance of photoexcitation as well. We introduce a simple model of a cone of plasma irradiated by the nuclear continuum; the line emission we observe along our line of sight perpendicular to the cone is produced through recombination/radiative cascade following photoionization and radiative decay following photoexcitation. A remarkably good fit is obtained to the H-like/He-like ionic line series, with inferred radial ionic column densities consistent with recent observations of warm absorbers in Seyfert 1 galaxies. Previous Chandra imaging revealed a large (extending out to 500 pc) ionization cone containing most of the X-ray flux, implying that the warm absorber in NGC 1068 is a large-scale outflow. To explain the ionic column densities, a broad, flat distribution in the logarithm of the ionization parameter ($ξ=L_X/n_e r^2$) is necessary, spanning $\logξ=0$--3. This suggests either radially-stratified ionization zones or the existence of a broad density distribution (spanning a few orders of magnitude) at each radius.
description: 23 pages, 16 figures, ApJ (accepted). XSPEC local model "photo" is available at http://xmm.astro.columbia.edu/research.html
Supplementary document for Vector light field display based on an intertwined flat lens with large depth of focus - 5658255.pdf
Creators: name: Zhou, Fengbin
name: Zhou, Feng
name: Chen, Yang
name: Hua, Jianyu
name: Qiao, Wen
name: Chen, Linsen
Publisher: name: Optica Publishing Group
Year: 2022
Subjects: Optical Technology

description: the supplement of data and measurement method
Capital concentration and financialization in Brazilian private higher education
Creators: name: De Carvalho, Cristina Helena Almeida
Publisher: name: Academia
Year: 2017
Subjects: Private Higher Education; Capital Concentration; Financialization; Brazil

description: The main objective of this paper is to facilitate an understanding of the recent phenomenon of the growth of for-profit higher education institutions in Brazil, whose trajectory has been the adoption of various market strategies aimed at financialization and market concentration. The movement of capital concentration can be observed through the number of mergers and acquisitions in the educational sector. Brazil is now credited with the largest higher education company in the world due to a merger between Kroton and Anhanguera groups. Together they have had more than 1 million students. It holds 16.5% of the market share. The financialization in Brazilian private higher education can be observed in two different movements: the acquisitions carried out by private equity funds and the opening of capital of educational companies (IPOs) on the Brazilian stock exchange, which has been taking place since 2007. The mechanisms of raising funds through the capital market allow the time-intensive capitalization of resources to subsidize the acquisitions and mergers, aiming at large-scale growth. There are more than 2,000 educational institutions, although, the four largest groups account for 34% of enrollments and 25% of net revenue. In conclusion, the process of financialization has fueled the concentration of capital in Brazilian private higher education. L'objectif principal de cet article est de comprendre le phénomène récent de la croissance des établissements d'enseignement supérieur à but lucratif au Brésil, dont la trajectoire a été l'adoption de diverses stratégies de marché en matière de financiarisation et de concentration du marché. Le mouvement de concentration du capital peut être observé par le nombre de fusions et acquisitions dans le secteur de l'éducation. Le Brésil est désormais crédité de la plus grande société d'enseignement supérieur du monde en raison d'une fusion entre les groupes Kroton et Anhanguera. De nos jours, ensemble, ils ont plus de 1 million d'étudiants. Ils détiennent 16,5% de la part de marché. La financiarisation de l'enseignement supérieur privé brésilien peut être observée dans deux mouvements différents: les acquisitions effectuées par les fonds de capital-investissement et l'ouverture du capital des sociétés d'éducation à la bourse brésilienne depuis 2007. Les mécanismes de collecte de fonds à travers le marché des capitaux permettent une capitalisation de ressources à forte intensité pour subventionner les acquisitions et les fusions, visant une croissance à grande échelle. Il existe plus de 2.000 établissements d'enseignement, mais les quatre plus grands groupes représentent 34% des effectifs et 25% des revenus nets. En conclusion, le processus de financiarisation a alimenté la concentration du capital dans l'enseignement supérieur privé brésilien.
description: Academia, No 10 (2017): Brazilian Higher Education
Additional file 9 of Comparative proteomic and transcriptomic analyses provide new insight into the formation of seed size in castor bean
Creators: name: Yu, Anmin
name: Li, Fei
name: Liu, Aizhong
Publisher: name: figshare
Year: 2020
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology

description: Additional file 9: Figure S4. Cis-element analysis of promoter sequences of genes in hormone signal transduction pathways.
Tetrapogon roxburghiana P. M. Peterson
Creators: name: Prunera-Olivé, Joan
name: Vorontsova, Maria S.
name: Williams, Emma V.
name: Mollel, Neduvoto P.
name: Hemp, Andreas
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Poaceae
Tetrapogon
Tetrapogon roxburghiana

description: Tetrapogon roxburghiana (Schult.) P.M.Peterson, Taxon 64: 460 (2015).
 Distribution: Eritrea to S. Africa, Madagascar, SW. Arabian Pen., S. India, Myanmar
 Specimens: MOSHI Arusha Chini, Haarer, A.E. 1088 (K); Karanga River, Haarer, A.E. 1217 (K); Lake Chala, Geilinger, W. 4764 (K); Lake Chala, Hemp, A. 658 (B, NHT, UBT); Lake Chala, Hemp, A. 658_neu (B, UBT); Lume River, Greenway, P.J. 8583 (K); Moshi, Hitchcock, A.S. 24562 (K).
description: Published as part of Prunera-Olivé, Joan, Vorontsova, Maria S., Williams, Emma V., Mollel, Neduvoto P. & Hemp, Andreas, 2021, Checklist of Kilimanjaro grasses shows that both plot and herbarium methods are necessary to record diversity, pp. 201-244 in Phytotaxa 501 (2) on page 242, DOI: 10.11646/phytotaxa.501.2.1, http://zenodo.org/record/5424816
Additional file 6: of C3aR signaling and gliosis in response to neurodevelopmental damage in the cerebellum
Creators: name: Young, Kevin
name: Keqin Yan
name: Picketts, David
Publisher: name: figshare
Year: 2019
Subjects: subject: Cell Biology
subject: Molecular Biology
subject: Neuroscience
subject: Physiology
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Cancer

description: Bergmann glia and Purkinje cell disorganization in different lobes of the P10 Smarca5; C3aR dKO and control cerebellum. The higher magnification images are from reconstructed optical sections. Scale bar = 100 Îźm in lower magnification image; 50 Îźm in higher magnification image. (DOCX 122 kb)
Universities, inequalities and public policy: A brief discussion of affirmative action in higher education in Brazil
Creators: name: Neves, Paulo S. C.
Publisher: name: Academia
Year: 2017
Subjects: Affirmative Action; University; Education inequalities; Racism

description: In this article, affirmative actions for Afro-Brazilians and poor people in Brazilian public universities will be analyzed. Introduced in the early 2000s, these measures provoked intense public debate in the country, calling into question not only the viability of their application in a country with such a high level of miscegenation as Brazil, but also their effects on the quality of Brazilian universities. Our starting point is that these policies should not be considered only educational policies, since they are also ways to symbolically reframe the place of some social groups (poor people and black people) in the national imaginary. With this objective, we propose to understand the transformations in university education over the last two decades (an increase in the number of students, social and ethnic-racial diversification of the student population etc.) as evidence of changes not only in universities but also in Brazilian society as a whole. Dans cet article, nous analysons les mesures de discriminations positives mises en place dans les universités publiques brésiliennes au bénéfice des populations noires et des pauvres. Introduites au début des années 2000, ces mesures ont provoqué un grand débat public qui remettait en cause non seulement la faisabilité de leur application dans un pays métissé comme le Brésil comme aussi leurs effets sur la qualité des universités brésiliennes. Notre point de départ est que ces politiques ne doivent pas être considérées uniquement comme des politiques éducationnelles, car elles sont également des moyens symboliques qui redimensionnent la place de certains groupes sociaux (pauvres, noirs) dans l'imaginaire national. De ce fait, nous proposons de comprendre les changements qui se produisent dans l'enseignement supérieur au cours des deux dernières décennies (augmentation du nombre d'étudiants, la diversité sociale et ethnique de la population étudiante, etc.) comme preuve des changements non seulement dans les universités, mais aussi dans l'ensemble de la société brésilienne
description: Academia, No 10 (2017): Brazilian Higher Education
Spatially Resolved Millimeter Interferometry of SMMJ02399-0136: a Very Massive Galaxy at z=2.8
Creators: name: Genzel, Reinhard
name: Baker, Andrew J.
name: Tacconi, Linda J.
name: Lutz, Dieter
name: Cox, Pierre
name: Guilloteau, Stephane
name: Omont, Alain
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report high-resolution millimeter mapping with the IRAM Plateau de Bure interferometer of rest-frame 335 micron continuum and CO(3-2) line emission from the z=2.8 submillimeter galaxy SMMJ02399-0136. The continuum emission comes from a ~3" diameter structure whose elongation is approximately east-west and whose centroid is coincident within the astrometric errors with the brightest X-ray and rest-UV peak (L1). The line data show that this structure is most likely a rapidly rotating disk. Its rotation velocity of >420 km/s implies a total dynamical mass of >3x10^11 solar masses within an intrinsic radius of 8 kpc, most of which is plausibly in the form of stars and gas. SMMJ02399-0136 is thus a very massive system, whose formation at z~3 is not easy to understand in current CDM hierarchical merger cosmogonies.
description: 19 pages, 6 figures (5 PS + 1 GIF), accepted by ApJ; added color versions of Figures 1, 5, & 6
Tuponia (Chlorotuponia) prasina
Creators: name: Linnavuori, Rauno E.
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Miridae
Tuponia
Tuponia prasina

description: Tuponia (Chlorotuponia) prasina (Fieber, 1864)
 Material examined. Numerous specimens: GILAN: Dasht-e-Veel, 8.-9.x.2000; Ganjeh, 14.v.-13.vi.1995; Lowshan, 7.ix.2000, 18.-20.viii.2002; Parudbar, 29.-30.vii.2003; Rasht, iv.-vi.1995; Tutkabon – Rudbar, 6.-8.vi.2002, 25.- 26.vi.2004. ARDABIL: near Firuzabad, 28.vii.2004; Khalkhal – Kivi, 4.viii.1996, 9.-11.viii.1998, 6.vii.2002. ZANJAN: Gilankesh 15 km NW of Gilvan, 26.-27.vi.2004; Mamalan, 4.-6.vi.2002. TEHRAN: Gachsar, 15.vii.2002; Karadj, 12.-14.vii.2002. GOLESTAN: Inche Borun, Alagol, 4.-5.vii.2004.
 Comments. On Tamarix and Myricaria. Pontomediterranean, extending to Middle Asia.
description: Published as part of Linnavuori, Rauno E., 2007, Studies on the Miridae (Heteroptera) of Gilan and the adjacent provinces in northern Iran. II. List of species, pp. 17-56 in Acta Entomologica Musei Nationalis Pragae 47 on page 54, DOI: 10.5281/zenodo.5328235
Additional file 5: of Bibliometric analysis of cardiometabolic disorders studies involving NO2, PM2.5 and noise exposure
Creators: name: Yu-Kai Huang
name: Hanneke, Rosie
name: Jones, Rachael
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Cell Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Table S2. Difference in index keywords between cardiometabolic referencesÂ involving noise exposure with H-designs and NH-designs. (PDF 86 kb)
Scaling relations of supersonic turbulence in star-forming molecular clouds
Creators: name: Boldyrev, Stanislav
name: Nordlund, Aake
name: Padoan, Paolo
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: Chaotic Dynamics (nlin.CD)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: We present a direct numerical and analytical study of driven supersonic MHD turbulence that is believed to govern the dynamics of star-forming molecular clouds. We describe statistical properties of the turbulence by measuring the velocity difference structure functions up to the fifth order. In particular, the velocity power spectrum in the inertial range is found to be close to E(k) \~ k^{-1.74}, and the velocity difference scales as ~ L^{0.42}. The results agree well with the Kolmogorov--Burgers analytical model suggested for supersonic turbulence in [astro-ph/0108300]. We then generalize the model to more realistic, fractal structure of molecular clouds, and show that depending on the fractal dimension of a given molecular cloud, the theoretical value for the velocity spectrum spans the interval [-1.74 ... -1.89], while the corresponding window for the velocity difference scaling exponent is [0.42 ... 0.78].
description: 17 pages, 6 figures included
Topology analysis for anomalous Hall effect in the non-collinear antiferromagnetic states of Mn$_3\mathit{A}$N ($A$ = Ni, Cu, Zn, Ga, Ge, Pd, In, Sn, Ir, Pt)
Creators: name: Huyen, Vu Thi Ngoc
name: Suzuki, Michi-To
name: Yamauchi, Kunihiko
name: Oguchi, Tamio
Publisher: name: arXiv
Year: 2019
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We investigate topological features of electronic structures which produce large anomalous Hall effect in the non-collinear antiferromagnetic metallic states of anti-perovskite manganese nitrides by first-principles calculations. We first predict the stable magnetic structures of these compounds to be non-collinear antiferromagnetic structures characterized by either $T_{1g}$ or $T_{2g}$ irreducible representation by evaluating the total energy for all of the magnetic structures classified according to the symmetry and multipole moments. The topology analysis is next performed for the Wannier tight-binding models obtained from the first-principles band structures. Our results reveal the small Berry curvature induced through the coupling between occupied and unoccupied states with the spin-orbit coupling, which is widely spread around the Fermi surface in the Brillouin zone, dominantly contributes after the $k$-space integration to the anomalous Hall conductivity, while the local divergent Berry curvature around Weyl points has a rather small contribution to the anomalous Hall conductivity.
description: accepted for publication in Physical Review B
Plagiognathus (Plagiognathus) chrysanthemi
Creators: name: Linnavuori, Rauno E.
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Miridae
Plagiognathus
Plagiognathus chrysanthemi

description: Plagiognathus (Plagiognathus) chrysanthemi (Wolff, 1864)
 Material examined. ARDABIL: 25 km E of Kivi, 1 specimen, 7.-9.vii.2002.
 Comments. In a meadow in hills. Found on Chrysanthemum, Achillea, Trifolium, Verbascum, etc. Holopalaearctic.
description: Published as part of Linnavuori, Rauno E., 2007, Studies on the Miridae (Heteroptera) of Gilan and the adjacent provinces in northern Iran. II. List of species, pp. 17-56 in Acta Entomologica Musei Nationalis Pragae 47 on page 50, DOI: 10.5281/zenodo.5328235
Des universités plus hétérogènes. Recherches sur le rapport au savoir des étudiants brésiliens
Creators: name: Charlot, Bernard
name: Dias Neves, Eloiza
name: Anahí Da Silva, Veleida
Publisher: name: Academia
Year: 2017
Subjects: Relationship to knowledge; University; Brazil; Students from working-class families

description: Whenever a new type of student arrives at university, he must face new difficulties. The Brazilian university has not yet been touched by a large wave of democratization, but it is already more heterogeneous than in the past. This article examines the relationship of Brazilian students to knowledge and the university and the atypical stories of young people from the working class who have successfully passed the entrance examination in a federal university. It is based on field research conducted in various parts of Brazil during the last ten years. The Brazilian students say that in the course of their lives, they have achieved, above all, relational, emotional, ethical and personal learning. Even at university, new ways of seeing the world and oneself are as important as cognitive learning. The stories of students from working-class families confirm that their relationships to knowledge are built into a broader network of relationships to the world, to others and to oneself - between pride in their success, nostalgia for their previous relationship with the community, and protection against the feeling of having betrayed their origins. Chaque fois qu'un nouveau type d'étudiant arrive à l'université, celle-ci doit affronter de nouvelles difficultés. L'université brésilienne n'a pas encore été atteinte par une grande vague de démocratisation, mais elle est déjà plus hétérogène qu'autrefois. Parmi toutes les questions que cette évolution pose à la recherche, le présent article s'intéresse au rapport d'étudiants brésiliens au savoir et à l'université et aux histoires atypiques de jeunes de milieux populaires qui ont réussi le concours d'entrée dans une université fédérale. Il s'appuie sur des recherches de terrain conduites en divers endroits du Brésil durant ces dernières dix années. Les étudiants brésiliens disent avoir appris dans leur vie, avant tout, des apprentissages relationnels, affectifs, éthiques et liés à leur développement personnel. Même à l'université, les nouvelles façons de voir le monde et de s'y voir sont pour eux aussi importantes que les apprentissages cognitifs. Les récits des étudiants issus de familles populaires confirment que leurs rapports au savoir se construisent dans un réseau plus ample de rapports au monde, aux autres et à soi-même – entre fierté de la réussite, nostalgie de la relation antérieure avec la communauté et protection contre le sentiment d'avoir trahi.
description: Academia, No 10 (2017): Brazilian Higher Education
Recent Progress in CdTe and CdZnTe Detectors
Creators: name: Takahashi, Tadayui
name: Watanabe, Shin
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Cadmium telluride (CdTe) and cadmium zinc telluride (CdZnTe) have been regarded as promising semiconductor materials for hard X-ray and Gamma-ray detection. The high atomic number of the materials (Z_{Cd} =48, Z_{Te} =52) gives a high quantum efficiency in comparison with Si. The large band-gap energy (Eg ~ 1.5 eV) allows us to operate the detector at room temperature. However, a considerable amount of charge loss in these detectors produces a reduced energy resolution. This problem arises due to the low mobility and short lifetime of holes. Recently, significant improvements have been achieved to improve the spectral properties based on the advances in the production of crystals and in the design of electrodes. In this overview talk, we summarize (1) advantages and disadvantages of CdTe and CdZnTe semiconductor detectors and (2) technique for improving energy resolution and photopeak efficiencies. Applications of these imaging detectors in future hard X-ray and Gamma-ray astronomy missions are briefly discussed.
description: 9 pages, 15 figures, Based on the invited overview talk at 2000 IEEE Nuclear Science Symposium (Lyon, France). will appear in IEEE NS
A generating integral for the matrix elements of the Coulomb Green's function with the Coulomb wave functions
Creators: name: Dzikowski, K.
name: Skoromnik, O. D.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Quantum Physics (quant-ph)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: We analytically evaluate the generating integral $K_{nl}(β,β') = \int_{0}^{\infty}\int_{0}^{\infty} e^{-βr - β' r'}G_{nl} r^{q} r'^{q'} dr dr'$ and integral moments $J_{nl}(β, r) = \int_{0}^{\infty} dr' G_{nl}(r,r') r'^{q} e^{-βr'}$ for the reduced Coulomb Green's function $G_{nl}(r,r')$ for all values of the parameters $q$ and $q'$, when the integrals are convergent. These results can be used in second-order perturbation theory to analytically obtain the complete energy spectra and local physical characteristics such as electronic densities of multi-electron atoms or ions.
description: 23 pages
title: Improving Diversification in Local Search for Propositional Satisfiability
Creators: name: Duong, Thach-Thao Nguyen
Publisher: name: Griffith University
Year: 2014
Subjects: subject: Propositional Satisfiability (SAT)
subject: Artificial Intelligence (AI)
subject: Constraint Programming (CP)
subject: Complex constrained problems
subject: Conjunctive Normal Form (CNF)

description: In recent years, the Propositional Satisfiability (SAT) has become standard for encoding real world complex constrained problems. SAT has significant impacts on various research fields in Artificial Intelligence (AI) and Constraint Programming (CP). SAT algorithms have also been successfully used in solving many practical and industrial applications that include electronic design automation, default reasoning, diagnosis, planning, scheduling, image interpretation, circuit design, and hardware and software verification. The most common representation of a SAT formula is the Conjunctive Normal Form (CNF). A CNF formula is a conjunction of clauses where each clause is a disjunction of Boolean literals. A SAT formula is satisfiable if there is a truth assignment for each variable such that all clauses in the formula are satisfied. Solving a SAT problem is to determine a truth assignment that satisfies a CNF formula. SAT is the first problem proved to be NP-complete [20]. There are many algorithmic methodologies to solve SAT. The most obvious one is systematic search; however another popular and successful approach is stochastic local search (SLS). Systematic search is usually referred to as complete search or backtrack-style search. In contrast, SLS is a method to explore the search space by randomisation and perturbation operations. Although SLS is an incomplete search method, it is able to find the solutions effectively by using limited time and resources. Moreover, some SLS solvers can solve hard SAT problems in a few minutes while these problems could be beyond the capacity of systematic search solvers.
Extremely metal-poor galaxies with HST/COS: laboratories for models of low-metallicity massive stars and high-redshift galaxies
Creators: name: Senchyna, Peter
name: Stark, Daniel P.
name: Chevallard, Jacopo
name: Charlot, Stéphane
name: Jones, Tucker
name: García, Alba Vidal
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Ultraviolet (UV) observations of local star-forming galaxies have begun to establish an empirical baseline for interpreting the rest-UV spectra of reionization-era galaxies. However, existing high-ionization emission line measurements at $z>6$ ($\mathrm{W_{C IV, 0}} \gtrsim 20$ Å) are uniformly stronger than observed locally ($\mathrm{W_{C IV, 0}} \lesssim 2$ Å), likely due to the relatively high metallicities ($Z/Z_\odot > 0.1$) typically probed by UV surveys of nearby galaxies. We present new HST/COS spectra of six nearby ($z<0.01$) extremely metal-poor galaxies (XMPs, $Z/Z_\odot \lesssim 0.1$) targeted to address this limitation and provide constraints on the highly-uncertain ionizing spectra powered by low-metallicity massive stars. Our data reveal a range of spectral features, including one of the most prominent nebular C IV doublets yet observed in local star-forming systems and strong He II emission. Using all published UV observations of local XMPs to-date, we find that nebular C IV emission is ubiquitous in very high specific star formation rate systems at low metallicity, but still find equivalent widths smaller than those measured in individual lensed systems at $z>6$. Our moderate-resolution HST/COS data allow us to conduct an analysis of the stellar winds in a local nebular C IV emitter, which suggests that some of the tension with $z>6$ data may be due to existing local samples not yet probing sufficiently high $\mathrm{α/Fe}$ abundance ratios. Our results indicate that C IV emission can play a crucial role in the JWST and ELT era by acting as an accessible signpost of very low metallicity ($Z/Z_\odot < 0.1$) massive stars in assembling reionization-era systems.
description: 17 pages, 9 figures, published in MNRAS
Mass-to-light ratios from the fundamental plane of spiral galaxy disks
Creators: name: Graham, Alister W.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The best-fitting 2-dimensional plane within the 3-dimensional space of spiral galaxy disk observables (rotational velocity v_{rot}, central disk surface brightness μ_0 = -2.5log I_0, and disk scale-length h) has been constructed. Applying a three-dimensional bisector method of regression analysis to a sample of ~100 spiral galaxy disks that span more than four mag arcsec^{-2} in central disk surface brightness yields v_{rot} ~ I_0^{0.50+/-0.05}h^{0.77+/-0.07} (B-band) and v_{rot} ~ I_0^{0.43+/-0.04}h^{0.69+/-0.07} (R-band). Contrary to popular belief, these results suggest that in the B-band, the dynamical mass-to- light ratio (within 4 disk scale-lengths) is largely independent of surface brightness, varying as I_0^{0.00+/-0.10}h^{0.54+/-0.14}. Consistent results were obtained when the expanse of the analysis was truncated by excluding the low surface brightness galaxies. Previous claims that M/L_B varies with I_0^{-1/2} are shown to be misleading and/or due to galaxy selection effects. Not all low-surface-brightness disk galaxies are dark matter dominated. The situation is however different in the near-infrared where L_{K'} \~ v^4 and M/L_{K'} is shown to vary as I_0^{-1/2}. Theoretical studies of spiral galaxy disks should not assume a constant M/L ratio within any given passband. The B-band dynamical mass-to-light ratio (within 4 disk scale-lengths) has no obvious correlation with (B-R) disk colour, while in the K'-band it varies as -1.25+/-0.28(B-R). Combining the present observational data with recent galaxy model predictions implies that the logarithm of the stellar-to-dynamical mass ratio is not a constant value, but increases as disks become redder, varying as 1 .70+/-0.28(B-R).
description: Accepted by MNRAS Jan 23. 16 pages (including figures and tables)
Superconducting nanowires as high-rate photon detectors in strong magnetic fields
Creators: name: Polakovic, T.
name: Armstrong, W. R.
name: Yefremenko, V.
name: Pearson, J. E.
name: Hafidi, K.
name: Karapetrov, G.
name: Meziani, Z. -E.
name: Novosad, V.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Superconductivity (cond-mat.supr-con)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: Superconducting nanowire single photon detectors are capable of single-photon detection across a large spectral range, with near unity detection efficiency, picosecond timing jitter, and sub-10 $μ$m position resolution at rates as high as 10$^{9}$ counts/s. In an effort to bring this technology into nuclear physics experiments, we fabricate Niobium Nitride nanowire detectors using ion beam assisted sputtering and test their performance in strong magnetic fields. We demonstrate that these devices are capable of detection of 400 nm wavelength photons with saturated internal quantum efficiency at temperatures of 3 K and in magnetic fields potentially up to 5 T at high rates and with nearly zero dark counts.
How Neutral is the Intergalactic Medium at z ~ 6?
Creators: name: Lidz, Adam
name: Hui, Lam
name: Zaldarriaga, Matias
name: Scoccimarro, Roman
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Recent observations of high redshift quasar spectra reveal long gaps with little flux. A small or no detectable flux does not by itself imply the intergalactic medium (IGM) is neutral. Inferring the average neutral fraction from the observed absorption requires assumptions about clustering of the IGM, which the gravitational instability model supplies. Our most stringent constraint on the neutral fraction at z ~ 6 is derived from the mean Lyman-beta transmission measured from the z=6.28 SDSS quasar of Becker et al. -- the neutral hydrogen fraction at mean density has to be larger than 4.7 times 10^{-4}. This is substantially higher than the neutral fraction of ~ 3-5 times 10^{-5} at z = 4.5 - 5.7, suggesting that dramatic changes take place around or just before z ~ 6, even though current constraints are still consistent with a fairly ionized IGM at z ~ 6. An interesting alternative method to constrain the neutral fraction is to consider the probability of having many consecutive pixels with little flux, which is small unless the neutral fraction is high. This constraint is slightly weaker than the one obtained from the mean transmission. We show that while the derived neutral fraction at a given redshift is sensitive to the power spectrum normalization, the size of the jump around z ~ 6 is not. We caution that systematic uncertainties include spatial fluctuations in the ionizing background, and the continuum placement. Tests are proposed. In particular, the sightline to sightline dispersion in mean transmission might provide a useful diagnostic. We express the dispersion in terms of the transmission power spectrum, and develop a method to calculate the dispersion for spectra that are longer than the typical simulation box.
description: 20 pages, 5 figures; ApJ accepted version; constraints revised due to a revised power spectrum normalization in fiducial model
Superintegrable systems from block separation of variables and unified derivation of their quadratic algebras
Creators: name: Chen, Zhe
name: Marquette, Ian
name: Zhang, Yao-Zhong
Publisher: name: arXiv
Year: 2019
Subjects: subject: Mathematical Physics (math-ph)
subject: Exactly Solvable and Integrable Systems (nlin.SI)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We present a new method for constructing $D$-dimensional minimally superintegrable systems based on block coordinate separation of variables. We give two new families of superintegrable systems with $N$ ($N\leq D$) singular terms of the partitioned coordinates and involving arbitrary functions. These Hamiltonians generalize the singular oscillator and Kepler systems. We derive their exact energy spectra via separation of variables. We also obtain the quadratic algebras satisfied by the integrals of motion of these models. We show how the quadratic symmetry algebras can be constructed by novel application of the gauge transformations from those of the non-partitioned cases. We demonstrate that these quadratic algebraic structures display an universal nature to the extent that their forms are independent of the functions in the singular potentials.
description: 13 pages, no figure; Version to appear in Annals of Physics