cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Delinking rhetorics of neoliberalism: An analysis of South American leftist presidents’ speeches
Creators: name: Angel, Adriana
name: López-Londoño, Luis Miguel
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Biotechnology
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 110309 Infectious Diseases

description: We analyze the so-called Socialism of the twenty-first century in which nine South American governments turned to the left over the last 15 years. This South American socialist turn is seen as a delinking from the logics of dependency and pure neoliberalism. To explore the rhetorics that underlie this delinking process, we conducted both a macroanalysis and an intradiscursive rhetorical analysis of the inauguration and most significant speeches of all of the leftist South American presidents elected after 1999. We claim that a common critique of neoliberalism underlies the South American presidents’ speeches, which manifests through specific rhetorics concerning participatory democracy, social inclusion, and environmental protection. When they became transnational, these delinking rhetorics crafted a decolonial critique that calls for more indigenous models of development.
Transfer-matrix scaling from disorder-averaged correlation lengths for diluted Ising systems
Creators: name: de Queiroz, S. L. A.
name: Stinchcombe, R. B.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: A transfer matrix scaling technique is developed for randomly diluted systems, and applied to the site-diluted Ising model on a square lattice in two dimensions. For each allowed disorder configuration between two adjacent columns, the contribution of the respective transfer matrix to the decay of correlations is considered only as far as the ratio of its two largest eigenvalues, allowing an economical calculation of a configuration-averaged correlation length. Standard phenomenological-renormalisation procedures are then used to analyse aspects of the phase boundary which are difficult to assess accurately by alternative methods. For magnetic site concentration $p$ close to $p_c$, the extent of exponential behaviour of the $T_c \times p$ curve is clearly seen for over two decades of variation of $p - p_c$. Close to the pure-system limit, the exactly-known reduced slope is reproduced to a very good approximation, though with non-monotonic convergence. The averaged correlation lengths are inserted into the exponent-amplitude relationship predicted by conformal invariance to hold at criticality. The resulting exponent $η$ remains near the pure value (1/4) for all intermediate concentrations until it crosses over to the percolation value at the threshold.
description: RevTeX 3, 11 pages +5 figures, uuencoded, to appear in Phys. Rev. B (1994), PUC/RJ preprint
The z=1.6748 C I Absorber Toward PKS 1756+237
Creators: name: Roth, K. C.
name: Bauer, J. M.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the detection of the 1560 A and 1657 A ground-state C I absorption features in the z(abs)=1.6748 system toward the QSO PKS 1756+237. We find no associated C I* lines with a resulting 3-sigma excitation temperature upper-limit of T(ex) <= 8.54 (+0.65,-0.56) K, which is consistent with the predicted CMBR temperature of T(CMBR)=7.291 K. Because the redshifted CMBR populates the J=1 level and leaves little room for additional local excitation through either collisions or UV pumping, our data place 2-3 times more stringent limits on particle densities and UV fields than existing Copernicus observations of similar column density sightlines in the Milky Way. We also detect several Ni II lines and the weak Fe II 1611 A line. From the Ni/Fe column density ratio we find evidence for dust at a dust-to-metals ratio similar to that seen toward warm Galactic disk clouds. Based on these findings and supported by our Ly-alpha spectrum we propose to reclassify this system as a damped Ly-alpha absorber.
description: 12 pages, 3 figures, to appear in Ap. J. Letters. For further information and associated images see http://www.ifa.hawaii.edu/~kroth/PKS1756.html
title: The influence of staff communication style on service user response: an exploratory study
Creators: name: Andrews, Sarah
Publisher: name: University of Glasgow
Year: 2008
Subjects: subject: Clinical psychology, communication, medical personnel, children, parents.

description: Background: Communication interventions for children with intellectual disabilities are increasingly being conducted using parent-focussed approaches. However, the effectiveness of such interventions in altering the communication style of parents remains somewhat unclear. This review aimed to investigate training based on the Interactive Model for mothers of children with intellectual disabilities. In addition, the effect of such training on the children's communicative and cognitive development was also considered. Method: Six databases were searched identifying a total of 32 articles. Twenty four studies were excluded, leaving a total of 8 studies for inclusion in the present review. All studies were screened using a structured rating scale. Results: Parent-focussed training was found to be generally delivered via three methods; group sessions, individual sessions, or a mixture of both. Whilst overall outcomes for the effect on mothers' interaction style were largely positive, several methodological issues were highlighted that may result in these findings being interpreted with caution. In addition, the gains made by children with intellectual disabilities were found to be more variable. Conclusions: Whilst initial results appear encouraging, there is a lack of well conducted studies in this area, with consistent methodological weaknesses identified. Moreover, future research must consider the individual characteristics of the parent and child, as well as the wider communication environment.
Glassy Solutions of the Kardar-Pasrisi-Zhang Equation
Creators: name: Moore, M. A.
name: Doherty, T. Blum J. P.
name: Marsili, M.
name: Bouchaud, J-P.
name: Claudin, P.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: It is shown that the mode-coupling equations for the strong-coupling limit of the KPZ equation have a solution for d>4 such that the dynamic exponent z is 2 (with possible logarithmic corrections) and that there is a delta function term in the height correlation function = (A/k^{d+4-z}) δ(w/k^z) where the amplitude A vanishes as d -> 4. The delta function term implies that some features of the growing surface h(x,t) will persist to all times, as in a glassy state.
description: 11 pages, Revtex, 1 figure available upon request (same as figure 1 in ref [10]) Important corrections have been made which yield a much simpler picture of what is happening. We still find "glassy" solutions for d>4 where z is 2 (with possible logarithmic corrections). However, we now find no glassy solutions below d=4. A (linear) stability analysis (for d>4) has been included. Also one Author has been added
NPA_ref3716
Creators: name: Santen, Jeffrey A Van
Publisher: name: Zenodo
Year: 2019

description: Citation for NP Atlas reference previously without DOI Citation:  Sun, Yi; Tian, Li; Huang, Yong-Fu; Sha, Yi; Pei, Yue-Hu A new cyclotetrapeptide from marine fungus Trichoderma reesei Die Pharmazie, 2006, 61(9), 809-810 PubMed ID: 17020165 Publisher Access: https://www.ingentaconnect.com/content/govi/pharmaz/2006/00000061/00000009/art00020
Phalaena colonella Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Noctuidae
Phalaena
Phalaena colonella

description: Phalaena colonella [spec. nov.]
P. Tinea alis oblongis cinereis: punctis duobus atris ante strigam curvam serratam obsoletam.
Fn. svec. 912.
Habitat in Europa.
Palpi duo, prominentes, distantes, ut in antecedenti.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 534, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Simulation of Coupling Strength of Capacitively Coupled Singlet-Triplet Qubits
Creators: name: Buterakos, Donovan
name: Throckmorton, Robert E.
name: Sarma, S. Das
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We consider a system of two purely capacitively-coupled singlet-triplet qubits, and numerically simulate the energy structure of four electrons in two double quantum dots with a large potential barrier between them. We calculate the interqubit coupling strength using an extended Hund-Mulliken approach which includes excited orbitals in addition to the lowest energy orbital for each quantum dot. We show the coupling strength as a function of the qubit separation, as well as plotting it against the detunings of the two double quantum dots, and show that the general qualitative features of our results can be captured by a potential-independent toy model of the system.
description: 9 pages, 6 figures
A formation timescale of the Galactic halo from Mg isotopes in dwarf stars
Creators: name: Carlos, Marilia
name: Karakas, Amanda I.
name: Cohen, Judith G.
name: Kobayashi, Chiaki
name: Melendez, Jorge
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We determine magnesium isotopic abundances of metal poor dwarf stars from the galactic halo, to shed light on the onset of asymptotic giant branch (AGB) star nucleossynthesis in the galactic halo and constrain the timescale of its formation. We observed a sample of eight new halo K dwarfs in a metallicity range of -1.9 < [Fe/H] < -0.9 and 4200 < $T_{eff}$(K) < 4950, using the HIRES spectrograph at the Keck Observatory (R~10^5 and 200 < S/N < 300). We obtain magnesium isotopic abundances by spectral synthesis on three MgH features and compare our results with galactic chemical evolution models. With the current sample, we almost double the number of metal poor stars with Mg isotopes determined from the literature. The new data allow us to determine the metallicity when the $^{26}$Mg abundances start to became important, $[Fe/H] \sim -1.4 \pm 0.1$. The data with $[Fe/H] > -1.4$ are somewhat higher (1-3 $σ$) than previous chemical evolution model predictions, indicating perhaps higher yields of the neutron-rich isotopes. Our results using only AGB star enrichment suggest a timescale for formation for the galactic halo of about 0.3 Gyr, but considering also supernova enrichment, the upper limit for the timescale formation is about 1.5 Gyr.
description: 8 pages, 5 figures. Accepted for publication on ApJ
title: ADCO, Sixième cartulaire de Saint-Étienne de Dijon (1662), Cart. 30 (G 133), 441 folios, f. 511
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: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire

description: Sixième cartulaire de Saint-Étienne de Dijon (1662), Archives départementales de la Côte-d'Or, Cart. 30 (G 133), 441 folios, f. 511, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Sixième cartulaire de Saint-Étienne de Dijon (1662), Archives départementales de la Côte-d'Or, Cart. 30 (G 133), 441 folios, f. 511, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
title: Attention bias for positively and negatively valenced sleep-related pictorial stimuli in psychophysiological insomnia, delayed sleep phase syndrome and normal sleep: an investigation using the dot-probe paradigm
Creators: name: Murie, Alison
Publisher: name: University of Glasgow
Year: 2008
Subjects: subject: Clinical psychology, sleep, sleep disorders, insomnia.

description: The efficacy of Cognitive-behavioural Therapy (CBT) for insomnia is well-established within the extant literature, where the impact of treatment upon sleep parameters, such as sleep onset latency and sleep efficiency, is generally the primary outcome measure. Several models now highlight the role of dysfunctional beliefs and attitudes about sleep in the development and maintenance of insomnia, and there is evidence to suggest that sleep-related cognitions are themselves amenable to change in response to treatment. A systematic review was conducted on 14 studies (n = 1339) published between 2000 and 2007 inclusively, the aim of which was to investigate the impact of CBT on dysfunctional beliefs and attitudes about sleep in insomnia; the association between treatment-induced cognitive change and improvements on sleep parameters was also examined. Thirteen of the studies report significant change in dysfunctional sleep-related beliefs in response to CBT, as indicated by reduced scores on the Dysfunctional Beliefs and Attitudes about Sleep Scale (DBAS). Three of the studies analysed the association between cognitive change and improvements in sleep; although positive correlations were observed, the level of association was generally modest. Overall, the findings suggest that CBT is effective in reducing dysfunctional sleep-related cognitions, and that reductions in such cognitions are associated with improvements on both subjective and objective measures of sleep. Furthermore, these improvements are maintained at follow-up assessment. However, a number of important methodological caveats to the evidence base presented herein must be considered when forming conclusions regarding the impact of CBT upon dysfunctional sleep-related cognitions in insomnia, and their association with improvements on an individual's overall sleep condition. KEYWORDS: sleep, insomnia, beliefs, attitudes, CBT.
Sub-Clustering Among Local Group Galaxies
Creators: name: Bergh, Sidney van den
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A new compilation of data on Local Group members shows that low-luminosity early-type galaxies are, at the 99% confidence level, more strongly concentrated in the M 31, and Galactic sub-clumps, than are dwarf irregular galaxies. It is not yet clear if star formation continued longer in dSph galaxies that are located far from M 31 and the Galaxy, than it did in those that are not associated with the Andromeda and Milky Way sub-clumps of the Local Group. Key words: galaxies: clustering - galaxies: Local Group
description: To be published in the May 1999 issue of the Astronomical Journal
Phalaena pusiella Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Noctuidae
Phalaena
Phalaena pusiella

description: Phalaena pusiella [spec. nov.]
P. Tinea alis superioribus albis: punctis lineaque communi longitudinali dentata atra; inferioribus nigris.
Habitat in Germania. P. Forssk�l.
Statura P. T. Evonymellae. Alae fuscae: sed superiores supra niveae, fascia longitudinali atra obtuse dentata, praeter puncta varia.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 534, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
El cuarto Sector en Colombia
Creators: name: Sánchez-Álvarez, César
name: Gutierrez-Torres, Diana Carolina
name: IE Center For The Governance Of Change
name: Secretaría General Iberoamericana
Publisher: name: Zenodo
Year: 2019
Subjects: Fourth Sector
Economy
Finance
Social aspects
Environmental aspects
Latinamerica
Colombia

description: En las próximas líneas de este apartado se presentan las características del ecosistema colombiano. Se pone el foco de atención en los aspectos macroeconómicos, la evolución histórica y las políticas públicas de promoción de la economía solidaria, el emprendimiento social y empresas que aplican prácticas de responsabilidad social en Colombia. Para iniciar la contextualización del ecosistema colombiano, los siguientes párrafos de este apartado introducen una breve revisión de bibliografía, con el propósito de contextualiza al lector sobre los enfoques de trabajo que se han dado en Colombia sobre el fenómeno del Cuarto Sector.
The Near-Infrared Tip of the Red Giant Branch. II. An Absolute Calibration in the Large Magellanic Cloud
Creators: name: Hoyt, Taylor J.
name: Freedman, Wendy L.
name: Madore, Barry F.
name: Seibert, Mark
name: Beaton, Rachael L.
name: Hatt, Dylan
name: Jang, In Sung
name: Lee, Myung Gyoon
name: Monson, Andrew J.
name: Rich, Jeffrey A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present a new empirical \(JHK\) absolute calibration of the tip of the red giant branch (TRGB) in the Large Magellanic Cloud (LMC). We use published data from the extensive \emph{Near-Infrared Synoptic Survey} containing 3.5 million stars, of which 65,000 are red giants that fall within one magnitude of the TRGB. Adopting the TRGB slopes from a companion study of the isolated dwarf galaxy IC\,1613 as well as an LMC distance modulus of \(μ_0 = \)~18.49~mag from (geometric) detached eclipsing binaries, we derive absolute \(JHK\) zero-points for the near-infrared TRGB. For comparison with measurements in the bar alone, we apply the calibrated \(JHK\) TRGB to a 500 deg\textsuperscript{2} area of the 2MASS survey. The TRGB reveals the 3-dimensional structure of the LMC with a tilt in the direction perpendicular to the major axis of the bar, in agreement with previous studies.
description: 14 pages, 8 figures, Accepted to ApJ
Antiferromagnetic and van Hove Scenarios for the Cuprates: Taking the Best of Both Worlds
Creators: name: Dagotto, Elbio
name: Nazarenko, Alexander
name: Moreo, Adriana
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: A theory for the high temperature superconductors is proposed. Holes are spin-1/2, charge e, quasiparticles strongly dressed by spin fluctuations. Based on their dispersion, it is claimed that the experimentally observed van Hove singularities of the cuprates are likely originated by antiferromagnetic (AF) correlations. From the two carriers problem in the 2D t-J model, an effective Hamiltonian for holes is defined with %no free parameters. This effective model has superconductivity in the ${\rm d_{x^2-y^2}}$ channel, a critical temperature ${\rm T_c \sim 100K}$ at the optimal hole density, ${\rm x=0.15}$, and a quasiparticle lifetime linearly dependent with energy. Other experimental results are also $quantitatively$ reproduced by the theory.
description: 12 pages, 4 figures (on request), RevTeX (version 3.0), preprint NHMFL
Theoretical design of azaacene-based non-fullerene electron transport material used in inverted perovskite solar cells
Creators: name: Keke Wen
name: Pan, Xiao
name: Songyan Feng
name: Wenpeng Wu
name: Xugeng Guo
name: Jinglai Zhang
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Biochemistry
subject: Genetics
subject: FOS: Biological sciences
subject: Physiology
subject: Pharmacology
subject: Biotechnology
subject: Evolutionary Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Cancer

description: Inverted perovskite solar cells (PSCs) have attracted much attention due to their low-temperature and solution-based process. Electron transport layers are important components in inverted PSCs. Non-fullerene n-type organic small molecules seem to be more attractive as electron transport layers, because their structures are easy to be synthesised and modified. In this paper, density functional theory and semi-classical Marcus electron transfer theory were used to explore the electron transport properties in three azaacene derivatives, including one experimentally reported molecule, 1,4,9,16-tetrakis((triisopropylsilyl)ethynyl)quinoxalino[2‴,3‴:4″,5″]cyclopenta[1″,2″,3″:5′,6′]acenaphtho[1′,2′:5,6]pyrazino[2,3-b]phenazine (1), and two theoretically designed molecules (2 and 3). Compound 2 is formed by substituting i-Pr groups in compound 1 with H atoms, which is designed to evaluate the effect of i-Pr groups on the electron transport properties. Compound 3 is designed by adding one more benzopyrazine group to the conjugation structure of compound 1. It shows that i-Pr group can increase HOMO and LUMO energy levels and improve solubility in organic solvent and hydrophobicity. Enlarging conjugation can not only decrease LUMO energy level and electron reorganisation energy, but also can increase solubility and electron mobility. So our designed compound 3 is expected to be a potential electron transport material in inverted PSCs.
Phalaena bella Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Noctuidae
Phalaena
Phalaena bella

description: Phalaena bella [spec. nov.]
P. Tinea alis flavis: superioribus fasciis sex punctorum nigrorum.
Catesb. car. 2. p. 96. t. 96.
Habitat in America septentxionali.
Alae fasciis ex punctis nigris in totidem series transversas digestis.
Variat punctis alarum superiorum simplicissimis & ocellatis.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 534, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
MOESM4 of Benchmarking transposable element annotation methods for creation of a streamlined, comprehensive pipeline
Creators: name: Ou, Shujun
name: Su, Weija
name: Liao, Yi
name: Chougule, Kapeel
name: Agda, Jireh
name: Hellinga, Adam
name: Lugo, Carlos
name: Elliott, Tyler
name: Ware, Doreen
name: Peterson, Thomas
name: Jiang, Ning
name: Hirsch, Candice
name: Hufford, Matthew
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Developmental Biology
subject: Inorganic Chemistry
subject: FOS: Chemical sciences

description: Additional file 4. Review history.
Phalaena pulchella Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Noctuidae
Phalaena
Phalaena pulchella

description: Phalaena pulchella [spec. nov.]
P. Tinea alis albis: superioribus nigro sanguineoque punctatis; inferioribus apice nigris.
Pet. gaz. t. 3. f. 3.
Habitat in Europa australi; in Mauritania. Brander.
Similis Tineae Evonymellae sed duplo major, pulcherrima. Alae superiores Punctis rubris & nigris sparsis mixtis; margo superiorum posticus nigro punctatus.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 534, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
New limits on $Ω_Λ$ and $Ω_M$ from old galaxies at high redshift
Creators: name: Alcaniz, J. S.
name: Lima, J. A. S.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The ages of two old galaxies (53W091, 53W069) at high redshifts are used to constrain the value of the cosmological constant in a flat universe ($Λ$CDM) and the density parameter $Ω_M$ in Friedmann-Robertson-Walker (FRW) models with no $Λ$-term. In the case of $Λ$CDM models, the quoted galaxies yield two lower limits for the vacuum energy density parameter, $Ω_Λ\geq 0.42$ and $Ω_Λ\geq 0.5$, respectively. Although compatible with the limits from statistics of gravitational lensing (SGL) and cosmic microwave background (CMB), these lower bounds are more stringent than the ones recently determined using SNe Ia as standard candles. For matter dominated universes ($Ω_Λ=0$), the existence of these galaxies imply that the universe is open with the matter density parameter constrained by $Ω_M \leq 0.45$ and $Ω_M \leq 0.37$, respectively. In particular, these results disagree completely with the analysis of field galaxies which gives a lower limit $Ω_M \geq 0.40$.
description: submitted to Astrophysical Journal Letters, 16 ApJ preprint pages including 4 figures
Twin-Boundary Pinning of Superconducting Vortex Arrays
Creators: name: Marchetti, M. C.
name: Vinokur, V. M.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We discuss the low-temperature dynamics of magnetic flux lines in high-temperature superconductors in the presence of a family of parallel twin planes that contain the $c$ axis. A current applied along the twin planes drives flux motion in the direction transverse to the planes and acts like an electric field applied to {\it one-dimensional} carriers in disordered semiconductors. As in flux arrays with columnar pins, there is a regime where the dynamics is dominated by superkink excitations that correspond to Mott variable range hopping (VRH) of carriers. In one dimension, however, rare events, such as large regions void of twin planes, can impede VRH and dominate transport in samples that are sufficiently long in the direction of flux motion. In short samples rare regions can be responsible for mesoscospic effects. The phase boundaries separating various transport regimes are discussed. The effect of tilting the applied field out of the twin planes is also considered. In this case the resistivity from flux motion is found to depend strongly on the tilt angle.
description: 30pages, 1 table and 7 figures (figures available - send requests to cris@npac.syr.edu)
The Near-Infrared Tip of the Red Giant Branch. I. A Calibration in the Isolated Dwarf Galaxy IC 1613
Creators: name: Madore, Barry F.
name: Freedman, Wendy L.
name: Hatt, Dylan
name: Hoyt, Taylor J.
name: Monson, Andrew J.
name: Beaton, Rachael L.
name: Rich, Jeffrey A.
name: Jang, In Sung
name: Lee, Myung Gyoon
name: Scowcroft, Victoria
name: Seibert, Mark
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Based on observations from the \emph{FourStar} near-infrared camera on the 6.5m Baade-Magellan telescope at Las Campanas, Chile, we present calibrations of the $JHK$ luminosities of stars defining the tip of the red giant branch (TRGB) in the halo of the Local Group dwarf galaxy IC 1613. We employ metallicity-independent (rectified) T-band magnitudes---constructed using $J,H$ and $K$-band magnitudes and both $(J-H)~ \& ~(J-K)$ colors in order to flatten the upward-sloping red giant branch tips as otherwise seen in their apparent color-magnitude diagrams. We describe and quantify the advantages of working at these particular near-infrared wavelengths, which are applicable to both \emph{HST} and \emph{JWST}. We also note that these same wavelengths can be accessed from the ground for an eventual tie-in to \emph{Gaia} for absolute astrometry and parallaxes to calibrate the intrinsic luminosity of the TRGB. Adopting the color terms derived from the IC 1613 data, as well as the zero-points from a companion study of the Large Magellanic Cloud whose distance is anchored to the geometric distances of detached eclipsing binaries, we find a true distance modulus of 24.32 $\pm$ 0.02~ (statistical) $\pm$ 0.06~mag (systematic) for IC 1613, which compares favorably with the recently published multi-wavelength, multi-method consensus modulus of 24.30 $\pm$ 0.05~mag by Hatt et al. (2017).
description: 20 pages, 13 figures, Accepted to ApJ
title: Биосферосовместимые технологии в строительстве, архитектуре и градостроительстве: расчет уровня реализации функций города
title: Учебное пособие
titleType: Subtitle
Creators: name: Скобелева Е.А.
name:  Черняева И.В.
Publisher: name: Вузовское образование
Year: 2020

description: Учебное пособие предназначено для решения практических задач в области обеспечения экологической безопасности городской среды. В нем рассматриваются подходы и методики расчета уровня реализации функций биосферосовместимого поселения для удовлетворения рациональных потребностей человека. Подготовлено в соответствии с Федеральным государственным образовательным стандартом высшего образования. Предназначено для студентов, обучающихся по направлениям подготовки 07.03.01 «Архитектура», 07.03.04 «Градостроительство», 08.03.01 «Строительство» и может быть полезно при выполнении практических занятий по дисциплинам «Биосферосовместимые технологии в строительстве, архитектуре и градостроительстве», «Современные принципы формирования экологической среды городских поселений», «Основы проектирования экологически безопасной среды», «Экология городской среды» и «Основы урбоэкологии».
A Model for the Density Distribution of Virialized CDM Halos
Creators: name: Kull, A.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: An analytic collapse model for the formation and density distribution of virialized cold dark matter halos is proposed. Hierarchical structure formation is taken into account explicitly. Monte Carlo methods are used to generate samples of mass histories of virialized halos. The mean density distribution found from the collapse model is in good agreement with numerical results in the mass range from $10^{11}M_\odot$ to $10^{15}M_\odot$ and in the radial range form $0.05 r_{200}$ to $r_{200}$.
description: 8 pages, 3 figures. Accepted for publication in ApJ Letters
Novel Magnetic Properties of Carbon Nanotubes
Creators: name: Lu, Jian Ping
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: An external magnetic field is found to have strong effects on the electronic structure of carbon nanotubes. A field-induced metal-insulator transition is predicted for all pure nanotubes. In a weak field, nanotubes exhibit both large diamagnetic and paramagnetic responses which depend on the field direction, the position of the Fermi energy, the helicity, and the size of the nanotube. Universal scalings are found for the susceptibility as functions of the Fermi energy, the temperature, and the size of nanotubes. These results are in agreement with experiments.
description: 14 pages, Revtex, UNC-CH-94
Coperfectly Hopfian Groups and Shape Fibrator's Properties
Creators: name: Vasilevska, Violeta
Publisher: name: arXiv
Year: 2018
Subjects: subject: Geometric Topology (math.GT)
subject: FOS: Mathematics
subject: Primary 57N15, 57M07, Secondary 57N25, 54B15

description: This paper provides further investigation of the concept of shape m$_{\rm simpl}$-fibrators (previously introduced by the author). The main results identify shape m$_{\rm simpl}$-fibrators among direct products of Hopfian manifolds. First it is established that every closed orientable manifold homotopically determined by $π_1$ with coperfectly Hopfian group (a new class of Hopfian groups that are introduced here) is a shape m$_{\rm simpl}$o-fibrator if it is a codimension-2 fibrator (Theorem 5.4). The main result (Theorem 6.2) states that the direct product of two closed orientable manifolds (of different dimension) homotopically determined by $π_1$ and with coperfectly Hopfian fundamental groups (one normally incommensurable with the other one) is a shape m$_{\rm simpl}$o-fibrator, if it is a Hopfian manifold and a codimension-2 fibrator.
description: 16 pages
EUV images of the Clusters of Galaxies A2199 and A1795: clear evidence for a separate and luminous emission component
Creators: name: Lieu, Richard
name: Bonamente, Massimiliano
name: Mittaz, Jonathan P. D.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Since all of the five clusters of galaxies observed by the Extreme Ultraviolet Explorer deep survey telescope are found to possess a diffuse EUV emitting component which is unrelated to the virial gas at X-ray temperatures, the question concerning the nature of this new component has been a subject of controversy. Here we present results of an EUV and soft X-ray spatial analysis of the rich clusters Abell 2199 and 1795. The EUV emission does not resemble the X-ray morphology of clusters: at the cluster core the EUV contours are organized, but at larger radii they are anisotropic, and therefore need not have originated from a hydrostatically stable medium. The ratio of EUV to soft X-ray intensity rises with respect to cluster radius, to reach values ~10 times higher than that expected from the virial gas. The strong EUV excess which exists in the absence of soft X-ray excess poses formidable problems to the non-thermal (inverse-Compton) scenario, but may readily be explained as due to emission lines present only in the EUV range. In particular, warm gas produced by shock heating could account for such lines without proliferation of bolometric luminosities and mass budgets.
description: 13 pages, 7 figures (4 in color), minor typos corrected; ApJL accepted
Carnet nº 6, commencé à Irkoutsk (p. 7)
Creators: name: Péraire, Lucien
name: CNRS
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2023

description: created: 12-1-1930
Enhanced Electron Pairing in a Lattice of Berry Phase Molecules
Creators: name: Manini, N.
name: Tosatti, E.
name: Doniach, S.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We show that electron hopping in a lattice of molecules possessing a Berry phase naturally leads to pairing. Our building block is a simple molecular site model inspired by C$_{60}$, but realized in closer similarity with Na$_3$. In the resulting model electron hopping must be accompanied by orbital operators, whose function is to switch on and off the Berry phase as the electron number changes. The effective hamiltonians (electron-rotor and electron-pseudospin) obtained in this way are then shown to exhibit a strong pairing phenomenon, by means of 1D linear chain case studies. This emerges naturally from numerical studies of small $N$-site rings, as well as from a BCS-like mean-field theory formulation. The pairing may be explained as resulting from the exchange of singlet pairs of orbital excitations, and is intimately connected with the extra degeneracy implied by the Berry phase when the electron number is odd. The relevance of this model to fullerides, to other molecular superconductors, as well as to present and future experiments, is discussed.
description: 30 pages, RevTex
On the Spatial Distribution of Stellar Populations in the Large Magellanic Cloud
Creators: name: Harris, Jason
name: Zaritsky, Dennis
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We measure the angular correlation function of stars in a region of the Large Magellanic Cloud (LMC) that spans 2 degrees by 1.5 degrees. We find that the correlation functions of stellar populations are represented well by exponential functions of the angular separation for separations between 2 and 40 arcmin (corresponding to ~ 30 pc and 550 pc for an LMC distance of 50 kpc). The inner boundary is set by the presence of distinct, highly correlated structures, which are the more familiar stellar clusters, and the outer boundary is set by the observed region's size and the presence of two principal centers of star formation within the region. We also find that the normalization and scale length of the correlation function changes systematically with the mean age of the stellar population. The existence of positive correlation at large separations (~300 pc), even in the youngest population, argues for large-scale hierarchical structure in current star formation. The evolution of the angular correlation toward lower normalizations and longer scale lengths with stellar age argues for the dispersion of stars with time. We show that a simple, stochastic, self-propagating star formation model is qualitatively consistent with this behavior of the correlation function.
description: 30 pages, 13 Figures. Scheduled for publication in AJ in June 1999
Kinetic Roughening in Growth Models with Diffusion in Higher Dimensions
Creators: name: Šmilauer, P.
name: Kotrla, M.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We present results of numerical simulations of kinetic roughening for a growth model with surface diffusion (the Wolf-Villain model) in 3+1 and 4+1~dimensions using lattices of a linear size up to $L=64$ in 3+1~D and $L=32$ in 4+1~D. The effective exponents calculated both from the surface width and from the height--height correlation function are much larger than those expected based on results in lower dimensions, due to a growth instability which leads to the evolution of large mounded structures on the surface. An increase of the range for incorporation of a freshly deposited particle leads to a decrease of the roughness but does not suppress the instability.
description: 8 pages, LaTeX 2.09, IC-DDV-93-004
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IV, Cart. 188 (11 H 73), f. 0155r
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IV, Archives départementales de la Côte-d'Or, Cart. 188 (11 H 73), f. 0155r, 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 IV, Archives départementales de la Côte-d'Or, Cart. 188 (11 H 73), f. 0155r, 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
title: Polarization observables in strangeness photoproduction with CLAS at Jefferson Lab
Creators: name: Paterson, Craig Alexander
Publisher: name: University of Glasgow
Year: 2008
Subjects: subject: High energy physics, nuclear physics and radiation, photons, polarized beams.

description: This work presents measurements of several polarization observables for the reactions gammap → K+Lambda0 and gammap → K+ Sigma0. The data were collected in the summer of 2005 at the Thomas Jefferson National Accelerator Facility, using a linearly polarized photon beam in the energy range 1.66 GeV < √s < 2.24 GeV. In addition to measuring the photon asymmetry, target asymmetry and hyperon recoil polarization, first ever measurements are made for the double polarization observables O[x] and O[z]. The measurements of the photon and target asymmetries vastly increase the precision of the current world dataset, as well as extending the angular coverage.
A New Evolutionary Path to Type Ia Supernovae: Helium-Rich Super-Soft X-Ray Source Channel
Creators: name: Hachisu, Izumi
name: Kato, Mariko
name: Nomoto, Ken'ichi
name: Umeda, Hideyuku
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have found a new evolutionary path to Type Ia supernovae (SNe Ia) which has been overlooked in previous work. In this scenario, a carbon-oxygen white dwarf (C+O WD) is originated, not from an asymptotic giant branch star with a C+O core, but from a red-giant star with a helium core of $\sim 0.8-2.0 M_\odot$. The helium star, which is formed after the first common envelope evolution, evolves to form a C+O WD of $\sim 0.8-1.1 M_\odot$ with transferring a part of the helium envelope onto the secondary main-sequence star. This new evolutionary path, together with the optically thick wind from mass-accreting white dwarf, provides a much wider channel to SNe Ia than previous scenarios. A part of the progenitor systems are identified as the luminous supersoft X-ray sources or the recurrent novae like U Sco, which are characterized by the accretion of helium-rich matter. The white dwarf accretes hydrogen-rich, helium-enhanced matter from a lobe-filling, slightly evolved companion at a critical rate and blows excess matter in the wind. The white dwarf grows in mass to the Chandrasekhar mass limit and explodes as an SN Ia. A theoretical estimate indicates that this channel contributes a considerable part of the inferred rate of SNe Ia in our Galaxy, i.e., the rate is about ten times larger than the previous theoretical estimates for white dwarfs with slightly evolved companions.
description: 19 pages including 12 figures, to be published in ApJ, 519, No.1
Self-Organized Criticality in Non-conserved Systems
Creators: name: Middleton, A. Alan
name: Tang, Chao
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: The origin of self-organized criticality in a model without conservation law (Olami, Feder, and Christensen, Phys. Rev. Lett. {\bf 68}, 1244 (1992)) is studied. The homogeneous system with periodic boundary condition is found to be periodic and neutrally stable. A change to open boundaries results in the invasion of the interior by a ``self-organized'' region. The mechanism for the self-organization is closely related to the synchronization or phase-locking of the individual elements with each other. A simplified model of marginal oscillator locking on a directed lattice is used to explain many of the features in the non-conserved model: in particular, the dependence of the avalanche-distribution exponent on the conservation parameter $α$ is examined.
description: 11 pages, 4 separate figures, REVTEX
Phalaena evonymella Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Noctuidae
Phalaena
Phalaena evonymella

description: Phalaena evonymella [spec. nov.]
P. Tinea alis superioribus albis: punctis 50 nigris; inferioribus fuscis.
Habitat in Evonymo! Pado, Sorbo & c.
Larvae vivunt in societate sub tentoriis.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on pages 534-535, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
A Wide Symbiotic Channel to Type Ia Supernovae
Creators: name: Hachisu, Izumi
name: Kato, Mariko
name: Nomoto, Ken'ichi
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: As a promising channel to Type Ia supernovae (SNe Ia), we have proposed a symbiotic binary system consisting of a white dwarf (WD) and a low mass red-giant (RG), where strong winds from the accreting WD play a key role to increase the WD mass to the Chandrasekhar mass limit. Here we propose two new evolutionary processes which make the symbiotic channel to SNe Ia much wider. (1) We first show that the WD + RG close binary can form from a wide binary even with such a large initial separation as $a_i \lesssim 40000 R_\odot$. Such a binary consists of an AGB star and a low mass main-sequence (MS) star, where the AGB star is undergoing superwind before becoming a WD. If the superwind at the end of AGB evolution is as fast as or slower than the orbital velocity, the wind outflowing from the system takes away the orbital angular momentum effectively. As a result the wide binary shrinks greatly to become a close binary. Therefore, the WD + RG binary can form from much wider binaries than our earlier estimate. (2) When the RG fills its inner critical Roche lobe, the WD undergoes rapid mass accretion and blows a strong optically thick wind. Our earlier analysis has shown that the mass transfer is stabilized by this wind only when the mass ratio of RG/WD is smaller than 1.15. Our new finding is that the WD wind can strip mass from the RG envelope, which could be efficient enough to stabilize the mass transfer even if the RG/WD mass ratio exceeds 1.15. With the above two new effects (1) and (2), the symbiotic channel can account for the inferred rate of SNe Ia in our Galaxy.
description: 29 pages including 14 firgures, to be published in ApJ, 521, No.2
Kybernetische Modellierung der 5D-Strukturprojektion
Creators: name: Klemm, Sebastian
Publisher: name: Zenodo
Year: 2025

description: Diese wissenschaftliche Facharbeit formuliert ein erkenntnistheoretisches und kybernetisches Modell der fünften Dimension als strukturgebendes Informationsfeld.

"Das Tor Gottes ist kein Ort. It's Britney, b***h."- Kronos; Sanduhr & Sense
NPA_ref3778
Creators: name: Santen, Jeffrey A Van
Publisher: name: Zenodo
Year: 2019

description: Citation for NP Atlas reference previously without DOI Citation:  Suzuki, S; Nakamura, G; Okuma, K; Tomiyama, Y Celluloid, a new antibiotic Journal of Antibiotics, 1958, 11(3), 81-83 PubMed ID: 13563326 Publisher Access: NONE
NPA_ref3830
Creators: name: Santen, Jeffrey A Van
Publisher: name: Zenodo
Year: 2019

description: Citation for NP Atlas reference previously without DOI Citation:  COHEN, R Four new fungicides for Coccidioides immitis: 1. Sodium caprylate. 2. Ethyl vanillate 3. Fradicin. 4. Thiolutin Archives of Pediatrics, 1951, 68(6), 259-264 PubMed ID: 14847786 Publisher Access: NONE