cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Towards an MDD Based Framework for Self Adaptive IoT Applications Development
Creators: name: Abuseta, Yousef
Publisher: name: arXiv
Year: 2018
Subjects: subject: Software Engineering (cs.SE)
subject: FOS: Computer and information sciences

description: As technology and communication advances, more devices (and things) are able to connect to the Internet and talk to each other to achieve a common goal which results in the emergence of the Internet of Things (IoT) era. It is believed that IoT will bring up a limitless number of applications and business opportunities that will affect almost every aspect of our life. Research has already been conducted to investigate the challenges that obstruct the realization of IoT along with the promising solutions that pave the way for the acceptance and enabling of IoT. Among the research areas that is of a great importance to making IoT paradigm possible is the presence of a unified programming framework that masks the heterogeneity of the involved devices of the IoT platform. Such a framework guides system developers throughout the IoT application development process. In this paper, we investigate the IoT concept and its high level architecture in general and focus more on the application development aspect. We believe that IoT applications are highly dynamic in nature and thus need to be engineered with the self adaptive and autonomic concepts in mind. Therefore, our proposed IoT software development lifecycle was based on the IBM architecture blueprint for autonomic systems. To cater for the runtime dynamic and heterogeneity aspects of IoT applications, we adopt the MDD paradigm for our proposed development framework. We highlight the core requirements of a resilient development framework that accommodates the necessary concepts and processes for a successful IoT application.
description: 11 pages. arXiv admin note: text overlap with arXiv:1508.01330
An alternative model for the electroweak symmetry breaking sector and its signature in future e-gamma colliders
Creators: name: Rosenfeld, Rogerio
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We perform a preliminary study of the deviations from the Standard Model prediction for the cross section for the process $e γ\rightarrow ν_e W γ$. We work in the context of a higgsless chiral lagrangian model that includes an extra vector resonance $V$ and an anomalous $γW V$ coupling. We find that this cross section can provide interesting constraints on the free parameters of the model once it is measured in future $e γ$ colliders.
description: LaTex , 14 pages, 5 figures not included but available as postscript files upon request, NUB-3086/94-Th
Depth dependant element analysis of PbMg$_{1/3}$Nb$_{2/3}$O$_{3}$ using muonic X-rays
Creators: name: Brown, K. L.
name: Stockdale, C. P. J.
name: Luo, H.
name: Zhao, X.
name: Li, J. -F.
name: Viehland, D.
name: Xu, G.
name: Gehring, P. M.
name: Ishida, K.
name: Hillier, A. D.
name: Stock, C.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The relaxor PbMg$_{1/3}$Nb$_{2/3}$O$_{3}$ (PMN) has received attention due to its potential applications as a piezoelectric when doped with PbTiO$_{3}$ (PT). Previous results have found that there are two phases existing in the system, one linked to the near-surface regions of the sample, the other in the bulk. However, the exact origin of these two phases is unclear. In this paper, depth dependant analysis results from negative muon implantation experiments are presented. It is shown that the Pb content is constant throughout all depths probed in the sample, but the Mg and Nb content changes in the near-surface region below 100$μ$m. At a implantation depth of 60$μ$m, it is found that there is a 25% increase in Mg content, with a simultaneous 5% decrease in Nb content in order to maintain charge neutrality. These results show that the previously observed skin effects in PMN are due to a change in concentration and unit cell.
description: 5 pages, 3 figures, to be published in Journal of Physics: Condensed Matter
Short Note on Space Wind Powered by Disorder: Dark Energy
Creators: name: Kavak, Mesut
Publisher: name: figshare
Year: 2018
Subjects: General Relativity
Quantum Mechanics
Special Relativity
Entropy

description: After midnight just before sleeping, I noticed in my bed, that free space itself can cause a parachute effect on the moving bodies especially the bodies move in low gravitational fields like in Pioneer Anomaly. Because of this reason, while speed of a satellite is decreasing, speed of another one which spins around the world on different axis can increase; a satellite wandering in interstellar medium can speed up as also it can slow down; low frequency light and high frequency light behavior differently; galaxies have lower mass can spin faster since mutual gravitation is not only option. These are only a few examples.
title: ADCO, Troisième cartulaire de Saint-Étienne de Dijon (XVIe), Cart. 23 (G 127), 310 folios, f. 00042
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/2011
name: Petot, Frédéric
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: Troisième cartulaire de Saint-Étienne de Dijon (XVIe), Archives départementales de la Côte-d'Or, Cart. 23 (G 127), 310 folios, f. 00042, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Troisième cartulaire de Saint-Étienne de Dijon (XVIe), Archives départementales de la Côte-d'Or, Cart. 23 (G 127), 310 folios, f. 00042, 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: Рациональное и мифическое в сознании: от анализа к синтезу
Creators: name: Ставицкий, А.
Publisher: name: Новгородский государственный университет имени Ярослава Мудрого (НовГУ)
Year: 2021

description: Статья рассматривает и раскрывает проблемы взаимодействия и соотношения рационального и мифического в сознании в свете новейших когнитивных исследований, включая изучение нейропсихологами дефолт-системы. В статье показано, что, несмотря на большую разницу, рациональное и мифическое мышление работают по принципу взаимной дополнительности, помогая человеку решать те
задачи, которые силами одного рационального мышления недостижимы.
Link cobordism and the intersection of slice discs
Creators: name: Ogasa, Eiji
Publisher: name: arXiv
Year: 2018
Subjects: subject: Geometric Topology (math.GT)
subject: FOS: Mathematics

description: It is well-known that all 2-knots are slice. Are all 2-links slice? This is an outstanding open question. In this paper we prove the following: For any 2-component 2-link (J,K)in the 4-sphere which bounds the 5-ball B^5, there is an embedded disc 2-disc D^2_J (respectively, D^2_K) in B^5 with the following properties: J (respectively K) bounds D^2_J (respectively, D^2_K). D^2_J and D^2_K intersect transversely. the intersection of D^2_J and D^2_K in D^2_J (respectively, D^2_K) is a trivial 1-knot.
description: 7 pages
MA'LUMOTLAR BAZASIDA FUNKSIONAL DASTURLASH VA UNING AMALIY MASALALARINI HAL QILISH
Creators: name: Shogʻdarova, Sakinabonu
name: Tojimahmudov, Farhodjon
name: Rajabov, Jahongir
Publisher: name: Zenodo
Year: 2024

description: Dasturlash sohasidagi rivojlanishlar bilan birga, funksional dasturlash paradigramasi ham yuqori darajada o’zgarish yaratilgan. Funksional dasturlash , amaliy masalalarini halqilishga oid yangi usullar va qulayliklar taqdim etadi. Ushbu maqola funksional dasturlashning maqsadi, undagi amaliy masalalarni hal qilishning asosiy qadamlari va dasturchilar uchun foydali bo’lgan mulohazalar olg’a surilgan.
Electronic and optical properties of La-doped Sr$_3$Ir$_2$O$_7$ epitaxial thin-films
Creators: name: Souri, M.
name: Terzic, J.
name: Johnson, J. M.
name: Connell, J. G.
name: Gruenewald, J. H.
name: Thompson, J.
name: Brill, J. W.
name: Hwang, J.
name: Cao, G.
name: Seo, A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Materials Science (cond-mat.mtrl-sci)
subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We have investigated structural, transport, and optical properties of tensile strained (Sr$_{1-x}$La$_x$)$_3$Ir$_2$O$_7$ (x = 0, 0.025, 0.05) epitaxial thin-films. While High-T$_c$ superconductivity is predicted theoretically in the system, we have observed that all of the samples remain insulating with finite optical gap energies and Mott variable-range hopping characteristics in transport. Cross-sectional scanning transmission electron microscopy indicates that structural defects such as stacking faults appear in this system. The insulating behavior of the La-doped Sr$_3$Ir$_2$O$_7$ thin-films is presumably due to disorder-induced localization and ineffective electron-doping of La, which brings to light the intriguing difference between epitaxial thin films and bulk single crystals of the iridates.
description: 4 figures
title: Цифровое бегство или бегство от цифровизации?
Creators: name: Труфанова, Елена
Publisher: name: Новгородский государственный университет имени Ярослава Мудрого (НовГУ)
Year: 2021

description: В статье представлен анализ трансформаций социальной роли цифровых коммуникаций в контексте их связи с феноменом эскапизма. Эскапизм при этом понимается не как исключительно негативное психическое явление, а как неотъемлемая потребность человека в поиске новизны. Показано, что взаимодействие с виртуальным пространством Интернета долгое время рассматривалось как причина
эскапизма, поскольку Интернет обеспечивал возможность психологического «бегства» в вымышленный мир, возможность анонимности, ухода от ответственности, конструирования альтернативных идентичностей.
Pair Creation by Very High Energy Photons in Gamma-Ray Bursts: A Unified Picture for Various Energetics of GRBs
Creators: name: Totani, Tomonori
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The extreme energetics of the gamma-ray burst (GRB) 990123 has revealed that some of GRBs emit quite a large amount of energy, and total energy release from GRBs seems to change from burst to burst by a factor of 10^{2-3} as E_{gamma, iso} \sim 10^{52-55} erg, where E_{gamma, iso} is the observed GRB energy when radiation is isotropic. If all GRBs are triggered by similar events, such a wide dispersion in energy release seems odd. Here we propose a unified picture for these various energetics of GRBs, in which all GRB events release roughly the same amount of energy of E_{iso} \sim 10^{55-56} erg as relativistic motion, with the baryon load problem almost resolved. A mild dispersion in the initial Lorentz factor (Γ) results in difference of E_{gamma, iso} up to a factor of m_p/m_e \sim 10^3. Protons work as ``a hidden energy reservoir'' of the total GRB energy, and E_{gamma, iso} depends on the energy transfer efficiency from protons into electrons (or positrons) in the internal shock. We show that this transfer occurs via e^{+-} pair-creation by very high energy photons of proton-synchrotron radiation, and this efficiency depends quite sensitively on Γ. We also show that, in spite of the wide dispersion in E_{gamma, iso}, this model predicts roughly a constant photon energy range of the e^{+-} pair-synchrotron at \sim MeV, which is well consistent with GRB observations. The optical flash of GRB 990123 can be explained by the internal shock origin in our model. The apparent no-correlation between E_{gamma, iso} and observed afterglow luminosity is consistent with the expectation of our scenario.
description: 6 pages, no figure. Accepted by MNRAS, pink pages
Search for Anomalous Couplings at $eγ$ Colliders
Creators: name: Cheung, K.
name: Dawson, S.
name: Han, T.
name: Valencia, G.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We consider the possibility of observing deviations from the Standard Model gauge-boson self-couplings at future $eγ$ colliders. We concentrate on the process $e^-γ\rightarrow νW^- Z$, which is particularly sensitive to the parity violating coupling $g_5^Z$ at high energies. We find that a 2~TeV $e^+ e^-$ collider operating in the $e^- γ$ mode could reach a sensitivity of order $5\times 10^{-3}$ to $g_5^Z$.
description: 16 pg in LATEX format, UCD-94-6, NUHEP-TH-94-2. Figures included as uuencoded file
Internal Kinematics of the Andromeda II Dwarf Spheroidal Galaxy
Creators: name: Cote, Patrick
name: Mateo, Mario
name: Olszewski, Edward
name: Cook, Kem
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The High Resolution Echelle Spectrometer on the Keck I telescope has been used to measure nine radial velocities having a median precision of 2 km/s for seven red giants belonging to the isolated dwarf spheroidal galaxy Andromeda II. We find a weighted mean radial velocity of -188+/-3 km/s and a central velocity dispersion of 9.3+/-2.7 km/s. There may be evidence for a radial velocity gradient across the face of the galaxy, although the significance of this result is low due to the small number of stars having measured velocities. Our best estimate for the global mass-to-light ratio of And II is M/L_V = 20.9^{+13.9}_{-10.1} in solar units. This value is similar to those of several Galactic dwarf spheroidal galaxies and is consistent with the presence of a massive dark halo in Andromeda II.
description: 9 pages, 3 postscript figures. Accepted for publication in the Astrophysical Journal
Gravitational uncertainties from dimension-six operators on supersymmetric GUT predictions
Creators: name: Datta, Alakabha
name: Pakvasa, Sandip
name: Sarkar, Utpal
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We consider the gravity induced dimension six terms in addition to the dimension five terms in the SUSY GUT Lagrangian and find that the prediction for $α_s$ may be washed out completely in supersymmetric grand unified theories unless the triplet higgs mass is smaller than $ 7\times 10^{16} $ GeV.
description: 7 pages,latex.Title of original version changed,text added and a figure has been added.Figure is available on request.To appear as a brief Report in Phys.Rev.D
Acquisition and analysis of adaptive optics imaging polarimetry data
Creators: name: Ageorges, N.
name: Walsh, J. R.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The process of data taking, reduction and calibration of near-infrared imaging polarimetry data taken with the ESO Adaptive Optics System ADONIS is described. The ADONIS polarimetric facility is provided by a rotating wire grid polarizer. Images were taken at increments of 22.5 degrees of polarizer rotation from 0 to 180 degrees, over-sampling the polarization curve but allowing the effects of photometric variations to be assessed. Several strategies to remove the detector signature are described. The instrumental polarization was determined, by observations of stars of negligible polarization, to be 1.7% at J, H and K bands. The lack of availability of unpolarized standard stars in the IR, in particular which are not too bright as to saturate current IR detectors, is highlighted. The process of making polarization maps is described. Experiments at restoring polarimetry data, in order to reach diffraction limited polarization, are outlined, with particular reference to data on the Homunculus reflection nebula around Eta Carinae.
description: 20 pages, A&A LaTeX2e, 11 figures. To appear in Astronomy & Astrophysics, Supplement Series
Hyperbits: the information quasiparticles
Creators: name: Pawlowski, M.
name: Winter, A.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Information theory has its particles, bits and qubits, just as physics has electrons and photons. However, in physics we have a special category of objects with no clear counterparts in information theory: quasiparticles. They are introduced to simplify complex emergent phenomena making otherwise very difficult calculations possible and providing additional insight into the inner workings of the system. We show that we can adopt a similar approach in information theory. We introduce the hyperbits, the first information quasiparticles which we prove to be a resource equivalent to entanglement and classical communication, and give examples how they can be used to simplify calculations and get more insight into communication protocols.
description: Published version
Galactic winds and circulation of the ISM in dwarf galaxies
Creators: name: D'Ercole, A.
name: Brighenti, F.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We study, through 2D hydrodynamical simulations, the feedback of a starburst on the ISM of typical gas rich dwarf galaxies. The main goal is to address the circulation of the ISM and metals following the starburst. We assume a single-phase rotating ISM in equilibrium in the galactic potential generated by a stellar disk and a spherical dark halo. The starburst is assumed to occur in a small volume in the center of the galaxy, and it generates a mechanical power of 3.8e39 erg/s or 3.8e40 erg/s for 30 Myr. We found, consistently with previous investigations, that the galactic wind is not very effective in removing the ISM. The metal rich stellar ejecta, instead, may be efficiently expelled from the galaxy and dispersed in the intergalactic medium. Moreover, we found that the central region of the galaxy is always replenished with cold and dense gas after a few 100 Myr from the starbust, achieving the requisite for a new star formation event in 0.5-1 Gyr. The hydrodynamical evolution of galactic winds is thus consistent with the episodic star formation regime suggested by many chemical evolution studies. We also discuss the X-ray emission of these galaxies and find that the observable (emission averaged) abundance of the hot gas underestimates the real one if thermal conduction is effective. This could explain the very low hot gas metallicities estimated in starburst galaxies.
description: 15 pages, 10 figures, accepted for publication in MNRAS
KVN observations suggest multiple $γ$-ray emission regions in 3C 84
Creators: name: Hodgson, Jeffrey A.
name: Rani, Bindu
name: Lee, Sang-Sung
name: Algaba, Juan Carlos
name: Kino, Motoki
name: Trippe, Sascha
name: Park, Jong-Ho
name: Zhao, Guang-Yao
name: Byun, Do-Young
name: Kang, Sincheol
name: Kim, Jae-Young
name: Kim, Jeong-Sook
name: Kim, Soon-Wook
name: Miyazaki, Atsushi
name: Wajima, Kiyoaki
name: Oh, Junghwan
name: Kim, Dae-won
name: Gurwell, Mark
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: 3C 84 (NGC 1275) is a well-studied mis-aligned Active Galactic Nucleus (AGN), which has been active in Gamma rays since at least 2008. We have monitored the source at four wavelengths (14 mm, 7 mm, 3 mm and 2 mm) using the Korean VLBI network (KVN) since 2013 as part of the interferometric monitoring of $γ$-ray bright AGN (iMOGABA) program. 3C 84 exhibits bright radio emission both near the central supermassive black hole (SMBH) feature known as C1 and from a moving feature located to the south known as C3. Other facilities have also detected these short-term variations above a slowly rising trend at shorter wavelengths, such as in Gamma ray and 1 mm total intensity light-curves. We find that the variations in the $γ$ rays and 1 mm total intensity light-curves are correlated, with the $γ$ rays leading and lagging the radio emission. Analysis of the 2 mm KVN data shows that both the Gamma rays and 1 mm total intensity short-term variations are better correlated with the SMBH region than C3, likely placing the short-term variations in C1. We interpret the emission as being due to the random alignment of spatially separated emission regions. We place the slowly rising trend in C3, consistent with previous results. Additionally, we report that since mid-2015, a large mm-wave radio flare has been occurring in C3, with a large Gamma ray flare coincident with the onset of this flare at all radio wavelengths.
description: 12 pages, 12 figures, accepted to MNRAS
Angular Distributions in the Drell-Yan Process: A Closer Look at Higher Twist Effects
Creators: name: Brandenburg, A.
name: Brodsky, S. J.
name: Khoze, V. V.
name: Müller, D.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We calculate the angular distribution of the lepton produced in the Drell-Yan reaction taking into account pion bound state effects. We work in the kinematic region where one of the pion constituents goes far off-shell, which allows us to treat the bound state problem perturbatively. We show that the angular distribution is very sensitive to the shape of the pion distribution amplitude. The model we discuss fits the data if we choose a two-humped pion distribution amplitude suggested by QCD sum rules.
description: Plain Tex, 9 pages, 3 appended figures, SLAC-PUB-6464-revised
Light propagation in 2PN approximation in the field of one moving monopole: I. Initial value problem
Creators: name: Zschocke, Sven
Publisher: name: arXiv
Year: 2018
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: In this investigation the light propagation in the gravitational field of one arbitrarily moving body with monopole structure is considered in the second post-Newtonian approximation. It is found that the light trajectory depends on the acceleration of the body. Some of these acceleration terms are important in order to get well-defined logarithmic functions with dimensionless arguments, while all the other acceleration terms are negligible on the pico-second level of accuracy in time-delay measurements. The expressions of the observables total light deflection and time delay are determined.
description: 53 pages, 1 figure
Synergies between Different Types of Agricultural Technologies in the Kenyan Small Farm Sector
Creators: name: Wainaina, Priscilla
name: Songporne Tongruksawattana
name: Matin Qaim
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Ecology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy
subject: Plant Biology

description: Sustainable intensification of agriculture will have to build on various innovations, but synergies between different types of technologies are not yet sufficiently understood. We use representative data from small farms in Kenya and propensity score matching to compare effects of input-intensive technologies and natural resource management practices on household income. When adopted in combination, positive income effects tend to be larger than when individual technologies are adopted alone. The largest gains occur when improved seeds are adopted together with organic manure and zero tillage. These results point at important synergies between plant breeding technologies and natural resource management practices.
Alexandrium gaarderae Nguyen-Ngoc et Larsen
Creators: name: Hernández-Becerril, David U.
name: Pichardo-Velarde, Jorge G.
name: Alonso-Rodríguez, Rosalba
name: Maciel-Baltazar, Ebodio
name: Morquecho, Lourdes
name: Esqueda-Lara, Karina
name: Barón-Campis, Sofía A.
name: Quiroz-González, Nataly
Publisher: name: Zenodo
Year: 2023
Subjects: Biodiversity
Taxonomy
Chromista
Myzozoa
Dinophyceae
Gonyaulacales
Ostreopsidaceae
Alexandrium
Alexandrium gaarderae

description: 3.1.2 Alexandrium gaarderae Nguyen-Ngoc et Larsen (Figures 9–11)
References: Nguyen and Larsen 2004, 90, pl. 6, figs 1–8; Menezes et al. 2018, 4.
 Synonyms = Goniodoma concavum Gaarder, Gonyaulax concava (Gaarder) Balech, Alexandrium concavum (Gaarder) Balech.
Reference: Balech 1995, 60, pl. XVII, figs 24–29.
A very characteristic species with solitary and large cells, pentagonal in shape (Figure 9). Epitheca irregularly conical with somewhat sinuous margins, hypotheca more rounded, flattened at the posterior margin, wide and excavated cingulum, and wide and deep sulcus (Figures 9 and 10). Apical pore (Po) large and conspicuous (Figure 11).
Measurements: 58–68 μm L, 48–55 μm W (Table 1).
Toxicity: this species is not considered to be toxic (Long et al. 2021).
Distribution: in the Gulf of Tehuantepec.
description: Published as part of Hernández-Becerril, David U., Pichardo-Velarde, Jorge G., Alonso-Rodríguez, Rosalba, Maciel-Baltazar, Ebodio, Morquecho, Lourdes, Esqueda-Lara, Karina, Barón-Campis, Sofía A. & Quiroz-González, Nataly, 2023, Diversity and distribution of species of the planktonic dinoflagellate genus Alexandrium (Dinophyta) from the tropical and subtropical Mexican Pacific Ocean, pp. 539-557 in Botanica Marina (Warsaw, Poland) (Warsaw, Poland) 66 (6) on page 542, DOI: 10.1515/bot-2023-0037, http://zenodo.org/record/11000291
MOESM1 of A resonance Rayleigh scattering sensor for sensitive differentiation of telomere DNA length and monitoring special motifs (G-quadruplex and i-motif) based on the Ag nanoclusters and NAND logic gate responding to chemical input signals
Creators: name: Wang, Shuai
name: Qu, Fei
name: Han, Wenli
name: You, Jinmao
Publisher: name: figshare
Year: 2018
Subjects: Biophysics
Biochemistry
Space Science
Medicine
Molecular Biology
Information Systems not elsewhere classified
Cancer
Virology

description: Additional file 1: Figure S1. UV-vis absorption and fluorescence spectra of PEI-Ag NCs. Figure S2. TEM images of PEI-Ag-NCs. Figure S3. RRS spectra of PEI-Ag NCs/telomere DNA (C-rich strands, Ael 10, 22, 40 and 64) system. Figure S4. Influence of PEI-Ag NCs concentration on the detection of telomere DNA. Figure S5. Influence of pH values on the detection of Tel 22 and Tel 64. Figure S6. Influence of reaction temperature on the detection of Tel 22 and Tel 64. Figure S7. Influence of reaction time on the detection of Tel 22 and Tel 64. Figure S8. RRS signals of free G-rich strands with different concentrations. Figure S9. RRS spectra of PEI-Ag NCs upon addition of different concentrations of C-rich strands and the corresponding linear ranges. Figure S10. RRS signals of free C-rich strands with different concentrations. Figure S11. Comparison of RRS spectra of PEI-Ag NCs/Tel 64 and PEI/Tel 64. Figure S12. RRS signals of free DNA (PSM.2 and HIV) with different concentrations. Figure S13. RRS spectra of PEI-Ag NCs upon addition of different concentrations of DNA (PSM.2 and HIV) and the corresponding linear ranges. Figure S14. Comparison of RRS signals of different PEI-Ag NCs/DNA system (Tel 10, PSM.2, Tel 22, HIV, Tel 40 and Tel 64). Figure S15. Comparison of RRS spectra of PEI-Ag NCs, motifs and PEI-Ag NCs/motif system. Figure S16. CD spectra of G-rich strands and C-rich strands in the presence or absence of K+ or H+. Figure S17. RRS spectra of PEI-Ag NCs, DNA and PEI-Ag NCs/DNA system. Figure S18. The RRS signals of DNA in absence and presence of PEI-Ag NCs. Table S1. Oligonucleotides used in this work. Table S2. Reproducibility of RRS method. Table S3. Linear ranges and correlation coefficients of the calibration graphs, and the detection limits for telomere DNA.
Linking Risk Aversion, Time Preference and Fertiliser Use in Burkina Faso
Creators: name: Cotty, Tristan Le
name: D’Hôtel, Elodie Maître
name: Soubeyran, Raphael
name: Subervie, Julie
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Biotechnology
subject: Ecology
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Cancer
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: Plant Biology

description: This paper investigates whether Burkinabe maize farmers’ fertiliser-use decisions are correlated with their risk and time preferences. We conducted a survey and a series of hypothetical experiments on a sample of 1500 farmers. We find that more patient farmers do use more fertiliser, but it is only because they plant more maize (a fertiliser-intensive crop) rather than because they use more fertiliser per hectare of maize planted. Conversely, we find no statistically significant link between risk aversion and fertiliser use. We use a simple two-period model, which suggests that risk aversion may indeed have an ambiguous effect on fertiliser use.
CHIMERA: a wide-field, multi-color, high-speed photometer at the prime focus of the Hale telescope
Creators: name: Harding, Leon K.
name: Hallinan, Gregg
name: Milburn, Jennifer
name: Gardner, Paul
name: Konidaris, Nick
name: Singh, Navtej
name: Shao, Michael
name: Sandhu, Jagmit
name: Kyne, Gillian
name: Schlichting, Hilke E.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: The Caltech HIgh-speed Multi-color camERA (CHIMERA) is a new instrument that has been developed for use at the prime focus of the Hale 200-inch telescope. Simultaneous optical imaging in two bands is enabled by a dichroic beam splitter centered at 567 nm, with Sloan u' and g' bands available on the blue arm and Sloan r', i' and z_s' bands available on the red arm. Additional narrow-band filters will also become available as required. An Electron Multiplying CCD (EMCCD) detector is employed for both optical channels, each capable of simultaneously delivering sub-electron effective read noise under multiplication gain and frame rates of up to 26 fps full frame (several 1000 fps windowed), over a fully corrected 5 x 5 arcmin field of view. CHIMERA was primarily developed to enable the characterization of the size distribution of sub-km Kuiper Belt Objects via stellar occultation, a science case that motivates the frame-rate, the simultaneous multi-color imaging and the wide field of view of the instrument. In addition, it also has unique capability in the detection of faint near-Earth asteroids and will be used for the monitoring of short duration transient and periodic sources, particularly those discovered by the intermediate Palomar Transient Factory (iPTF), and the upcoming Zwicky Transient Facility (ZTF).
description: Accepted to Mon. Not. R. Astron. Soc. (MNRAS), 15 pages, 9 figures, 3 tables
MCP detector development for UV space missions
Creators: name: Conti, Lauro
name: Barnstedt, Jürgen
name: Hanke, Lars
name: Kalkuhl, Christoph
name: Kappelmann, Norbert
name: Rauch, Thomas
name: Stelzer, Beate
name: Werner, Klaus
name: Elsener, Hans-Rudolf
name: Schaadt, Daniel M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: We are developing imaging and photon counting UV-MCP detectors, which are sensitive in the wavelength range from far ultraviolet to near ultraviolet. A good quantum efficiency, solar blindness and high spatial resolution is the aim of our development. The sealed detector has a Cs-activated photoactive layer of GaN (or similarly advanced photocathode), which is operated in semitransparent mode on (001)-MgF 2 . The detector comprises a stack of two long-life MCPs and a coplanar cross strip anode with advanced readout electronics. The main challenge is the flawless growth of the GaN photocathode layer as well as the requirements for the sealing of the detector, to prevent a degradation of the photocathode. We present here the detector concept and the experimental setup, examine in detail the status in the production and describe the current status of the readout electronics development.
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome I, Cart. 185 (11 H 70), f. 0027r
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 I, Archives départementales de la Côte-d'Or, Cart. 185 (11 H 70), f. 0027r, 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 I, Archives départementales de la Côte-d'Or, Cart. 185 (11 H 70), f. 0027r, 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
Graph Theoretic Investigations on Inefficiencies in Network Models
Creators: name: Cenciarelli, Pietro
name: Gorla, Daniele
name: Salvo, Ivano
Publisher: name: arXiv
Year: 2016
Subjects: subject: Discrete Mathematics (cs.DM)
subject: FOS: Computer and information sciences

description: We consider network models where information items flow %are sent from a source to a sink node. We start with a model where routing is constrained by energy available on nodes in finite supply (like in Smartdust) and efficiency is related to energy consumption. We characterize graph topologies ensuring that every saturating flow under every energy-to-node assignment is maximum and provide a polynomial-time algorithm for checking this property. We then consider the standard flow networks with capacity on edges, where again efficiency is related to maximality of saturating flows, and a traffic model for selfish routing, where efficiency is related to latency at a Wardrop equilibrium. Finally, we show that all these forms of inefficiency yield different classes of graphs (apart from the acyclic case, where the last two forms generate the same class). Interestingly, in all cases inefficient graphs can be made efficient by removing edges; this resembles a well-known phenomenon, called Braess's paradox.
The Lithium Depletion Boundary and the Age of the Young Open Cluster IC~2391
Creators: name: Navascues, D. Barrado y
name: Stauffer, J. R.
name: Patten, B. M.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have obtained new photometry and intermediate resolution ($Δλ= 2.7$ Å ) spectra of 19 of these objects (14.9 $\le$ $I_c$ $\le$ 17.5) in order to confirm cluster membership. We identify 15 of our targets as likely cluster members based on their $VRI$ photometry, spectral types, radial velocity, and H$α$ emission strengths. Higher S/N spectra were obtained for 8 of these probable cluster members in order to measure the strength of the lithium 6708 Å doublet and thus obtain an estimate of the cluster's age. One of these 8 stars has a definite lithium detection and two other (fainter) stars have possible lithium detections. A color-magnitude diagram for our program objects shows that the lithium depletion boundary in IC~2391 is at $I_c$=16.2. Using recent theoretical model predictions, we derive an age for IC~2391 of 53$\pm$5 Myr. While this is considerably older than the age most commonly attributed for this cluster ($\sim$35 Myr) this result for IC~2391 is comparable those recently derived for the Pleiades and Alpha Persei clusters and can be explained by new models for high mass stars that incorporate a modest amount of convective core overshooting.
description: ApJ Letters, acccepted
A Polynomial-time Algorithm for Detecting the Possibility of Braess Paradox in Directed Graphs
Creators: name: Cenciarelli, Pietro
name: Gorla, Daniele
name: Salvo, Ivano
Publisher: name: arXiv
Year: 2016
Subjects: subject: Data Structures and Algorithms (cs.DS)
subject: FOS: Computer and information sciences

description: A directed multigraph is said vulnerable if it can generate Braess paradox in Traffic Networks. In this paper, we give a graph-theoretic characterisation of vulnerable directed multigraphs; analogous results appeared in the literature only for undirected multigraphs and for a specific family of directed multigraphs. The proof of our characterisation also provides an algorithm that checks if a multigraph is vulnerable in O(|V| |E|^2); this is the first polynomial time algorithm that checks vulnerability for general directed multigraphs. The resulting algorithm also contributes to another well known problem, i.e. the directed subgraph homeomorphism problem without node mapping, by providing another pattern graph for which a polynomial time algorithm exists.
description: arXiv admin note: text overlap with arXiv:1603.01983
LHC Detection of Neutral MSSM Higgs Bosons via $gg\rta b\anti b \h\rta b\anti b b\anti b$
Creators: name: Dai, J.
name: Gunion, J. F.
name: Vega, R.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We demonstrate that simultaneous detection of two of the neutral Higgs bosons of the Minimal Supersymmetric Model will be possible at the LHC in the $b\anti b b\anti b$ final state, provided $\tanb$ is large and $b$-tagging can be performed with good efficiency and purity. This mode enhances the already established guarantee that there is no region of supersymmetric parameter space for which {\it none} of the Higgs bosons of the model can be seen at the LHC.
description: 10 pages; requires phyzzx.tex and tables.tex; revised to use top quark mass of 175 GeV and to include additional comments on detection of small signal/background Higgs bumps; full postscript file including embedded figures available via anonymous ftp at ucdhep.ucdavis.edu as [anonymous.gunion]bbbb_susy_revised.ps, preprint UCD-94-7
Mendeley Manual for Librarians
Creators: name: Aribowo, Eric Kunto
Publisher: name: figshare
Year: 2018
Subjects: subject: 160511 Research, Science and Technology Policy
subject: FOS: Political science
subject: 10206 Operations Research
subject: FOS: Mathematics

description: This manual was written to be used by Librarians, Academic Liaisons and others enrolled in the Mendeley Certification Program for Librarians. New users of Mendeley may consult this document throughout the certification program as required.
Note: Investigation of a Marx generator imitating a Tesla transformer
Creators: name: McGuyer, B. H.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: Applied Physics (physics.app-ph)
subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: A compact Marx generator was built to mimic a spark-gap Tesla transformer. The generator produced radio-frequency pulses of up to $\pm$200 kV and $\pm$15 A with a frequency between 110 to 280 kHz at a repetition rate of 120 Hz. The generator tolerated larger circuit-parameter perturbations than is expected for conventional Tesla transformers. Possible applications include research on the control and laser guiding of spark discharges.
description: 9 pages, 11 figures, includes supplementary material (but not supplementary video)
Direct Photoproduction of Jets in the KT Factorisation Prescription
Creators: name: Forshaw, J. R
name: Roberts, R. G.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study the cross section for dijet production via direct photons, as seen at the HERA collider. Rather than assuming the standard factorisation formula for the cross section (where the incoming partons are assumed to be on-shell), we use the $k_T$-factorisation formula. This formalism ought to be more appropriate for jet production in regions where the cross section is sensitive to the small-$x$ parton distribution functions. We study the rapidity distribution and the azimuthal angular distribution of the jets and compare with the traditional approach. Our calculations reveal a breakdown of the traditional approach as one moves into the regime of small $x$.
description: 8 pages report no. RAL-94-028
Theoretical investigation of N (2D) + HOX (Cl, Br) reaction
Creators: name: Jagannath Pal
name: Subramanian, Ranga
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Biophysics
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Inorganic Chemistry

description: The doublet potential-energy surface for the reaction, N (2D) + HOX (X = Cl, Br) has been studied employing both second-order Møller-Plesset and density-functional theory. The energies of the involved species have been refined using the complete basis set and coupled-cluster singles and double (triples) methods. Angular momentum-resolved (i.e. J-resolved) microcanonical variational transition state theory rate constant calculations are carried out to gain insight into the dynamics of this reaction. The minimum energy path of the title reaction occurs predominantly via the insertion-dissociation mechanism. The energetically most favourable product channels lead to the formation of HNO + X and NO + HX. The results indicate that the reaction shows positive temperature dependence in the temperature range of 200–500 K.
X-ray observations of low-power radio galaxies from the B2 catalogue
Creators: name: Canosa, C. M.
name: Worrall, D. M.
name: Hardcastle, M. J.
name: Birkinshaw, M.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present an analysis of X-ray data, taken with ROSAT, for a well defined sample of low-power radio galaxies from the Bologna B2 catalogue. Where possible, the HRI has been used in order to take advantage of the higher spatial resolution provided by this instrument. A variety of models are fitted to radial profiles in order to separate the resolved and unresolved X-ray emission from the galaxies. We demonstrate a strong, approximately linear, correlation between the luminosities of the unresolved X-ray components and the 5-GHz luminosities of the radio cores in this sample. This suggests a physical relationship between the soft X-ray emission of radio galaxies and the jet-generated radio core emission. We infer a nuclear jet-related origin for at least some of the X-ray emission.
description: To appear in MNRAS. 13 pages, 3 figures
What We Learn from Quantitative Ultraviolet Spectroscopy of Naked White D warfs in Cataclysmic Variables
Creators: name: Long, Knox S.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Using the Hopkins Ultraviolet Telescope and Hubble Space Telescope, observers have now obtained UV spectra with sufficient signal to noise and resolution to allow quantitative spectroscopic analyses of the WDs in several DNe. In the ``cleanest'' DNe, such as U Gem, the observations are allowing the basic physical parameters of the WD -- temperature, radius, gravity, rotation rate, and surface abundances -- to be established. A second component also exists in these systems, which may either be the disk or may be related to the WD itself. Here I summarize the current state of the observations and our understanding of the data, highlighting some of the uncertainties in the analyses as well the prospects for fundamentally advancing our understanding of DNe and WDs with future observations.
description: 6 pages, 8 figures, to be published in the proc. for Cataclysmic Variables: A 60th Birthday Symposium in Honour of Brian Warner
Evolution of defect signatures at ferroelectric domain walls in Mg-doped LiNbO3
Creators: name: Nataf, Guillaume F.
name: Guennou, Mael
name: Haußmann, Alexander
name: Barrett, Nick
name: Kreisel, Jens
Publisher: name: arXiv
Year: 2018
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The domain structure of uniaxial ferroelectric lithium niobate single crystals is investigated using Raman spectroscopy mapping. The influence of doping with magnesium and poling at room temperature is studied by analysing frequency shifts at domain walls and their variations with dopant concentration and annealing conditions. It is shown that defects are stabilized at domain walls and that changes in the defect structures with Mg concentration can be probed by the shift of Raman modes. We show that the signatures of polar defects in the bulk and at the domain walls differ.
description: 10 pages, 3 figures
Gravitino Production in the Inflationary Universe and the Effects on Big-Bang Nucleosynthesis
Creators: name: Kawasaki, M.
name: Moroi, T.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Gravitino production and decay in the inflationary universe are reexamined. Assuming that the gravitino mainly decays into a photon and a photino, we calculate the upperbound on the reheating temperature. Compared to previous works, we have essentially improved the following two points: (i) the helicity $\pm\frac{3}{2}$ gravitino production cross sections are calculated by using the full relevant terms in the supergravity lagrangian, and (ii) the high energy photon spectrum is obtained by solving the Boltzmann equations numerically. Photo-dissociation of the light elements (D, T, $^3$He, $^4$He) leads to the most stringent upperbound on the reheating temperature, which is given by ($10^{6}$--$10^{9}$)GeV for the gravitino mass 100GeV--1TeV. On the other hand, requiring that the present mass density of photino should be smaller than the critical density, we find that the reheating temperature have to be smaller than ($10^{11}$--$10^{12}$)GeV for the photino mass (10--100)GeV, irrespectively of the gravitino mass. The effect of other decay channels is also considered.