cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Integral-field near-infrared spectroscopy of two blue dwarf galaxies: NGC 5253 and He 2-10
Creators: name: Cresci, Giovanni
name: Vanzi, Leonardo
name: Sauvage, Marc
name: Santangelo, Gina
name: van der Werf, Paul
Publisher: name: arXiv
Year: 2010
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present integral field spectroscopy in the near infrared (NIR) of He 2-10 and NGC 5253, two well known nearby dwarf irregular galaxies showing high star-formation rates. Our data provide an unprecedented detailed view of the interstellar medium and star formation in these galaxies, allowing us to obtain spatially resolved information from the NIR emission and absorption line tracers. We study the spatial distribution and kinematics of different components of the interstellar medium (ISM) mostly through the Bracket series lines, the molecular hydrogen spectrum, [FeII] emission, and CO absorptions. Although the ISM is mostly photo-excited, as derived by the [FeII]/Bry and H2 line ratios, some regions corresponding to non-thermal radio sources show a [FeII]/Bry excess due to a significant contribution of SN driven shocks. In He 2-10 we find that the molecular gas clouds, as traced by CO(2-1) and H2 infrared line, show consistent morphologies and velocities when studied with the two different tracers. Moreover, there is a clear association with the youngest super star clusters as traced by the ionized gas. In the same galaxy we observe a cavity depleted of gas, which is surrounded by some of the most active regions of star formation, that we interpret as a signature of feedback-induced star formation from older episodes of star formation. Finally, we measured high turbulence in the ISM of both galaxies, sigma~30-80 km/s, driven by the high star-formation activity.
description: 12 pages, 10 figures, accepted for publication in A&A
Additional file 5 of Screening for the prevention and early detection of cervical cancer: protocol for systematic reviews to inform Canadian recommendations
Creators: name: Gates, Allison
name: Pillay, Jennifer
name: Reynolds, Donna
name: Stirling, Rob
name: Traversy, Gregory
name: Korownyk, Christina
name: Moore, Ainsley
name: Thériault, Guylène
name: Thombs, Brett D.
name: Little, Julian
name: Popadiuk, Catherine
name: Niekerk, Dirk Van
name: Keto-Lambert, Diana
name: Vandermeer, Ben
name: Hartling, Lisa
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Cancer
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 5. Search Strategies for Key Questions 1, 2 and 4.
Responsibility Modeling for the Sociotechnical Risk Analysis of Coalitions of Systems
Creators: name: Greenwood, David
name: Sommerville, Ian
Publisher: name: arXiv
Year: 2011
Subjects: subject: Software Engineering (cs.SE)
subject: FOS: Computer and information sciences

description: Society is challenging systems engineers by demanding ever more complex and integrated systems. With the rise of cloud computing and systems-of-systems (including cyber-physical systems) we are entering an era where mission critical services and applications will be dependent upon 'coalitions-of-systems'. Coalitions-of-systems (CoS) are a class of system similar to systems-of-systems but they differ in that they interact to further overlapping self-interests rather than an overarching mission. Assessing the sociotechnical risks associated with CoS is an open research question of societal importance as existing risk analysis techniques typically focus on the technical aspects of systems and ignore risks associated with coalition partners reneging on responsibilities or leaving the coalition. We demonstrate that a responsibility modeling based risk analysis approach enables the identification of sociotechnical risks associated with CoS. The approach identifies hazards and associated risks that may arise when relying upon a coalition of human/organizational/technical agents to provision a service or application. Through a case study of a proposed cloud IT infrastructure migration we show how the technique identifies vulnerabilities that may arise because of human, organizational or technical agents failing to discharge responsibilities.
description: Submitted for consideration for the IEEE SMC2011 conference
The SIMO Pre-Log Can Be Larger Than the SISO Pre-Log
Creators: name: Morgenshtern, Veniamin I.
name: Durisi, Giuseppe
name: Bölcskei, Helmut
Publisher: name: arXiv
Year: 2010
Subjects: subject: Information Theory (cs.IT)
subject: FOS: Computer and information sciences

description: We establish a lower bound on the noncoherent capacity pre-log of a temporally correlated Rayleigh block-fading single-input multiple-output (SIMO) channel. Surprisingly, when the covariance matrix of the channel satisfies a certain technical condition related to the cardinality of its smallest set of linearly dependent rows, this lower bound reveals that the capacity pre-log in the SIMO case is larger than that in the single-input single-output (SISO) case.
Additional file 12 of Polycomb group genes are required for neuronal pruning in Drosophila
Creators: name: Bu, Shufeng
name: Lau, Samuel Song Yuan
name: Yong, Wei Lin
name: Zhang, Heng
name: Thiagarajan, Sasinthiran
name: Bashirullah, Arash
name: Yu, Fengwei
Publisher: name: figshare
Year: 2023
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 12: A list of fly strains used in all the figures.
On integer partitions and the Wilcoxon rank-sum statistic
Creators: name: Sills, Andrew V.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Statistics Theory (math.ST)
subject: Number Theory (math.NT)
subject: FOS: Mathematics

description: In the literature, derivations of exact null distributions of rank-sum statistics is often avoided in cases where one or more ties exist in the data. By deriving the null distribution in the no-ties case with the aid of classical $q$-series results of Euler and Rothe, we demonstrate how a natural generalization of the method may be employed to derive exact null distributions even when one or more ties are present in the data. It is suggested that this method could be implemented in a computer algebra system, or even a more primitive computer language, so that the normal approximation need not be employed in the case of small sample sizes, when it is less likely to be very accurate. Several algorithms for determining exact distributions of the rank-sum statistic (possibly with ties) have been given in the literature (see Streitberg and Röhmel (1986) and Marx et al. (2016)), but none seem as simple as the procedure discussed here which amounts to multiplying out a certain polynomial, extracting coefficients, and finally dividing by a binomal coefficient.
description: 14 pages
Sonnenfleckenzeichnung Nr. 185.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 01.08.2019, 09:45, erstellt von Andrea Manna
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 2019

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Additional file 2 of Screening for the prevention and early detection of cervical cancer: protocol for systematic reviews to inform Canadian recommendations
Creators: name: Gates, Allison
name: Pillay, Jennifer
name: Reynolds, Donna
name: Stirling, Rob
name: Traversy, Gregory
name: Korownyk, Christina
name: Moore, Ainsley
name: Thériault, Guylène
name: Thombs, Brett D.
name: Little, Julian
name: Popadiuk, Catherine
name: Niekerk, Dirk Van
name: Keto-Lambert, Diana
name: Vandermeer, Ben
name: Hartling, Lisa
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Cancer
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 2. Outcome Definitions and Baseline Risks.
title: ÐÐ¾Ð»Ð¸ÑÐ¸ÐºÐ¾ - Ð¿ÑÐ°Ð²Ð¾Ð²ÑÐµ Ð¿Ð¾ÑÐ»ÐµÐ´ÑÑÐ²Ð¸Ñ ÑÐ°ÑÐ¿ÑÐ¾ÑÑÑÐ°Ð½ÐµÐ½Ð¸Ñ ÑÐºÑÑÑÐµÐ¼Ð¸Ð·Ð¼Ð° Ð² ÐºÐ¸Ð±ÐµÑÐ¿ÑÐ¾ÑÑÑÐ°Ð½ÑÑÐ²Ðµ
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
title: Political - legal consequences of the spread of extremism in cyberspace
Creators: name: ÐÐ°ÑÐ¿Ð¾Ð²Ð°, ÐÐ¾Ð»Ð¸Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2019
Subjects: ÑÐºÑÑÑÐµÐ¼Ð¸Ð·Ð¼
ÐºÐ¸Ð±ÐµÑÐ¿ÑÐ¾ÑÑÑÐ°Ð½ÑÑÐ²Ð¾
ÐºÐ¸Ð±ÐµÑÑÐºÑÑÑÐµÐ¼Ð¸Ð·Ð¼
ÑÐµÑÑÐ¾ÑÐ¸Ð·Ð¼
Ð²Ð¸ÑÑÑÐ°Ð»ÑÐ½Ð°Ñ ÑÐµÐ°Ð»ÑÐ½Ð¾ÑÑÑ
ÑÐ°ÑÐ¿ÑÐ¾ÑÑÑÐ°Ð½ÐµÐ½Ð¸Ðµ ÑÐºÑÑÑÐµÐ¼Ð¸Ð·Ð¼Ð°
extremism
cyberspace
extremism in cyberspace
terrorism
virtual reality
extremism distribution

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÐºÐ¾-Ð¿ÑÐ°Ð²Ð¾Ð²ÑÐµ Ð¾ÑÐ½Ð¾Ð²Ñ ÑÐºÑÑÑÐµÐ¼Ð¸Ð·Ð¼Ð°, ÑÐ°ÑÐ¿ÑÐ¾ÑÑÑÐ°Ð½ÑÐµÐ¼Ð¾Ð³Ð¾ Ð² ÐºÐ¸Ð±ÐµÑÐ¿ÑÐ¾ÑÑÑÐ°Ð½ÑÑÐ²Ðµ Ð¸ ÑÐ²Ð»ÑÑÑÐµÐ³Ð¾ÑÑ ÑÐ³ÑÐ¾Ð·Ð¾Ð¹ Ð´Ð»Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð»Ð¸ÑÐ½Ð¾ÑÑÐ¸, Ð¾Ð±ÑÐµÑÑÐ²Ð° Ð¸ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²Ð°, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ñ Ð¿ÑÐ¾ÑÐ¸Ð²Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ ÑÐºÑÑÑÐµÐ¼Ð¸Ð·Ð¼Ñ Ð² Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð±ÑÐ»Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ Ð¿Ð¾Ð½ÑÑÐ¸Ðµ Ð¸ ÑÑÑÐ½Ð¾ÑÑÑ ÑÐºÑÑÑÐµÐ¼Ð¸Ð·Ð¼Ð°, Ð¿Ð¾ÑÐ»ÐµÐ´ÑÑÐ²Ð¸Ñ ÑÐ°ÑÐ¿ÑÐ¾ÑÑÑÐ°Ð½ÐµÐ½Ð¸Ñ ÑÐºÑÑÑÐµÐ¼Ð¸Ð·Ð¼Ð°. ÐÐ·Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð·Ð°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÑÑÐ²Ð° Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸, ÑÐµÐ³ÑÐ»Ð¸ÑÑÑÑÐµÐ³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¾ â Ð¿ÑÐ°Ð²Ð¾Ð²ÑÐµ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ Ð¸ Ð¿Ð¾ÑÐ»ÐµÐ´ÑÑÐ²Ð¸Ñ ÑÐ°ÑÐ¿ÑÐ¾ÑÑÑÐ°Ð½ÐµÐ½Ð¸Ñ ÑÐºÑÑÑÐµÐ¼Ð¸Ð·Ð¼Ð° Ð¸ ÑÐµÑÑÐ¾ÑÐ¸Ð·Ð¼Ð° Ð² ÐºÐ¸Ð±ÐµÑÐ¿ÑÐ¾ÑÑÑÐ°Ð½ÑÑÐ²Ðµ.
description: This graduation thesis work examines the theoretical and legal bases of extremism, which extends in a cyberspace and is threat for the personality, society, the state and also ways of counteraction to extremism in Russian Federation. This work investigates the concept and essence of extremism, consequences of extremism distribution and suggestions for improvement of the legislation of Russian Federation, which regulates in the sphere of distribution of extremism in cyberspace.
X-ray bursts from the Terzan 5 transient IGR J17480-2446: nuclear rather than gravitational
Creators: name: Chakraborty, Manoneeta
name: Bhattacharyya, Sudip
Publisher: name: arXiv
Year: 2011
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Nuclear Experiment (nucl-ex)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The 2010 outburst of the transient neutron star low-mass X-ray binary IGR J17480-2446 has exhibited a series of unique X-ray bursts, as well as millihertz (mHz) quasi-periodic oscillations (QPOs) related to these bursts. It has been recently proposed that these are type-II bursts, powered by the gravitational energy. This implies that the current nuclear-burning based model of mHz QPOs is not correct, and this timing feature cannot be used as a tool to measure the neutron star parameters. We report the analysis of the Rossi X-ray Timing Explorer data of IGR J17480-2446 to show that the burst properties of this source are quite different from the properties of the type-II bursts observed from the rapid burster and GRO J1744-28. For example, the inferred ratio (~ 50-90) of the non-burst fluence to burst fluence is consistent with the thermonuclear origin of IGR J17480-2446 bursts, and is significantly different from this ratio (< 4) for type-II bursts. Our results suggest that the bursts and the mHz QPOs from IGR J17480-2446 are powered by the nuclear energy.
description: six pages, 1 table, 2 figures, accepted for publication in ApJ Letters
title: ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ ÑÐ»Ð°Ð±ÑÑ ÑÐ²ÑÐ·ÐµÐ¹ Ð² ÑÐ»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼Ð°Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð¼ ÑÐ¸Ð½Ð³ÑÐ»ÑÑÐ½Ð¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð°
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
title: Determination of weak links in electric power systems by the method of singular analysis
Creators: name: ÐÐ°ÑÐ²Ð¸ÐµÐ½ÐºÐ¾, ÐÐ»ÑÐ³Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2019
Subjects: Ð­Ð»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ
ÑÐ¸Ð½Ð³ÑÐ»ÑÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð·
Ð¼Ð°ÑÑÐ¸ÑÐ° Ð¯ÐºÐ¾Ð±Ð¸
Ð¼Ð°ÑÑÐ¸ÑÐ° ÑÐ·Ð»Ð¾Ð²ÑÑ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸Ð¼Ð¾ÑÑÐµÐ¹
Ð¼ÐµÑÐ¾Ð´ ÑÑÐ¸Ð»ÐµÐ½Ð¸Ñ ÑÐµÑÐ¸

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÐµÐ¼Ñ ÑÐ½ÐµÑÐ³Ð¾ÑÐ¸ÑÑÐµÐ¼Ñ ÐÐ°Ð»Ð¸Ð½Ð¸Ð½Ð³ÑÐ°Ð´ÑÐºÐ¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð½Ð° ÑÐ°Ð²Ð½Ð¾Ð¿ÑÐ¾ÑÐ½Ð¾ÑÑÑ ÑÐµÑÐ¸ Ð¿ÑÑÐµÐ¼ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð½Ð°Ð¸Ð¼ÐµÐ½ÑÑÐµÐ³Ð¾ ÑÐ¸Ð½Ð³ÑÐ»ÑÑÐ½Ð¾Ð³Ð¾ Ð·Ð½Ð°ÑÐµÐ½Ð¸Ñ Ð¼Ð°ÑÑÐ¸ÑÑ Ð¯ÐºÐ¾Ð±Ð¸. ÐÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð´Ñ Ð¿Ð¾ ÑÐ½Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð²Ð¾ÑÐ¿ÑÐ¸Ð¸Ð¼ÑÐ¸Ð²Ð¾ÑÑÐ¸ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¸ ÑÐµÐ°ÐºÑÐ¸Ð¸ Ð¾ÑÐ´ÐµÐ»ÑÐ½ÑÑ ÐµÐµ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² Ð½Ð° Ð²Ð½ÐµÑÐ½Ð¸Ðµ Ð²Ð¾Ð·Ð¼ÑÑÐµÐ½Ð¸Ñ. ÐÐ½Ð°Ð»Ð¸Ð· Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸Ð»ÑÑ Ð½Ð° Ð±Ð°Ð·Ðµ ÐÐ MATLAB. Ð¢Ð°ÐºÐ¶Ðµ Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ Ð¿Ð¾Ð¸ÑÐº ÑÐµÐ½ÑÐ¾ÑÐ½ÑÑ Ð¿Ð¾ ÑÐ¾ÐºÑ Ð²ÐµÑÐ²ÐµÐ¹ ÑÐµÑÐµÐ· ÑÑÐ²ÑÑÐ²Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÑÐ·Ð»Ð¾Ð² Ð¿Ð¾ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð½ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ ÑÑÐ²ÑÑÐ²Ð¸ÑÐµÐ»ÑÐ½ÑÐµ Ðº Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸ÑÐ¼ Ð½Ð°Ð³ÑÑÐ·Ð¾Ðº ÑÐ»ÐµÐ¼ÐµÐ½ÑÑ ÑÑÐµÐ¼Ñ ÑÐ½ÐµÑÐ³Ð¾ÑÐ¸ÑÑÐµÐ¼Ñ ÐÐ°Ð»Ð¸Ð½Ð¸Ð½Ð³ÑÐ°Ð´ÑÐºÐ¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸. ÐÑÐµ ÑÐ°ÑÑÐµÑÑ Ð¿Ð¾Ð´ÑÐ²ÐµÑÐ¶Ð´ÐµÐ½Ñ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½Ð¾ Ð² ÐÐ RastrWIN.
description: This paper presents an analysis of the power system circuits of the Kaliningrad region based on the equal strength of the network based on the analysis of the minimal singular value of the Jacobi matrix. The methods for reducing the sensitivity of the system and the reaction of its individual elements to the external disturbances are proposed. The analysis was based on the MATLAB PC. It also searches for current-sensing branches through the voltage sensitivity of the nodes. Based on the conducted research, the load-sensitive elements of the power grid circuit of the Kaliningrad region were determined. All calculations are confirmed experimentally in the RastrWIN PC.
Sonnenfleckenzeichnung Nr. 181.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 27.07.2019, 08:45, erstellt von Marco Cagnotti
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 2019

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 2.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
title: Ð§Ð¸ÑÐ»ÐµÐ½Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð´Ð²ÑÐ³Ð¾ÑÐ±Ð¾Ð³Ð¾ ÑÐ¿Ð»Ð¾ÑÐ½ÐµÐ½Ð¸Ñ Ð´Ð»Ñ Ð¿Ð¾Ð´Ð²Ð¾Ð´Ð½Ð¾Ð³Ð¾ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð½ÐµÑÑÐµÐ´Ð¾Ð±ÑÑÐ¸
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
title: Numerical analysis of a double-humped seal for subsea oil production equipment
Creators: name: ÐÐ»ÐºÐ¸Ð½, ÐÐ»ÐµÐºÑÐµÐ¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2022
Subjects: ÐÐ¾Ð½ÐµÑÐ½ÑÑ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² Ð¼ÐµÑÐ¾Ð´
Ð§Ð¸ÑÐ»ÐµÐ½Ð½ÑÐµ Ð¼ÐµÑÐ¾Ð´Ñ
ÐÐµÑÑÐµÐ´Ð¾Ð±ÑÑÐ°
ÑÐµÐ·Ð¸Ð½Ð¾Ð²Ð¾Ðµ ÑÐ¿Ð»Ð¾ÑÐ½ÐµÐ½Ð¸Ðµ
Ð½ÐµÑÑÑÐ½Ð¾Ðµ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ
Ð½ÐµÐ»Ð¸Ð½ÐµÐ¹Ð½Ð°Ñ ÑÐµÐ¾ÑÐ¸Ñ ÑÐ¿ÑÑÐ³Ð¾ÑÑÐ¸
rubber seal
oil equipment
nonlinear elasticity theory

description: ÐÐ·ÑÑÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð´Ñ ÑÐ°ÑÑÐµÑÐ¾Ð² Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹ ÑÐµÐ·Ð¸Ð½Ð¾Ð²ÑÑ ÑÐ¿Ð»Ð¾ÑÐ½ÐµÐ½Ð¸Ð¹ Ð´Ð»Ñ Ð¿Ð¾Ð´Ð²Ð¾Ð´Ð½Ð¾Ð³Ð¾ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð½ÐµÑÑÐµÐ´Ð¾Ð±ÑÑÐ¸. Ð¥Ð°ÑÐ°ÐºÑÐµÑ ÑÐ°Ð±Ð¾ÑÑ â ÑÐ°ÑÑÐµÑ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÑ Ð¼ÐµÑÐ¾Ð´ ÐºÐ¾Ð½ÐµÑÐ½ÑÑ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² Ð² ÑÐ¾Ð²Ð¾ÐºÑÐ¿Ð½Ð¾ÑÑÐ¸ Ñ ÑÐ¾ÑÐ¼ÑÐ»Ð°Ð¼Ð¸ Ð½ÐµÐ»Ð¸Ð½ÐµÐ¹Ð½Ð¾Ð¹ ÑÐµÐ¾ÑÐ¸Ð¸ ÑÐ¿ÑÑÐ³Ð¾ÑÑÐ¸.Â Ð Ð¿ÐµÑÐ²Ð¾Ð¹Â Ð³Ð»Ð°Ð²ÐµÂ Ð¸Ð·Ð»Ð°Ð³Ð°ÑÑÑÑÂ Ð¸Ð·Ð²ÐµÑÑÐ½ÑÐµÂ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸ÐµÂ Ð¾ÑÐ½Ð¾Ð²Ñ, Ð¾Ð±ÑÐ¸Ðµ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸ ÑÐµÐ·Ð¸Ð½, ÑÐ°ÐºÐ¶Ðµ Ð²Ð¾ Ð²ÑÐ¾ÑÐ¾Ð¹ Ð³Ð»Ð°Ð²Ðµ Ð´Ð°Ð½Ñ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¸ ÑÐ¾ÑÐ¼ÑÐ»Ñ Ð´Ð»Ñ Ð³Ð¸Ð¿ÐµÑÑÐ¿ÑÑÐ³Ð¸Ñ ÑÐµÐ», ÑÐ¾ÑÐ¼ÑÐ»Ñ Ð´Ð»Ñ ÑÐ°ÑÑÐµÑÐ° Ð¿Ð¾ ÐºÑÐ¸ÑÐµÑÐ¸Ñ Ð¿ÑÐ¾ÑÐ½Ð¾ÑÑÐ¸. Ð ÑÑÐµÑÑÐµÐ¹ Ð³Ð»Ð°Ð²Ðµ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ ÑÐ°ÑÑÐµÑÐ¾Ð² ÑÑÐµÐ´ÑÑÐ²Ð°Ð¼Ð¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ ABAQUS, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ ÑÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿Ð¾ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÐ¼ Ð´Ð°Ð½Ð½ÑÐ¼.
description: The methods of calculations and research of rubber seals for underwater oil production equipment are studied. The nature of the work is the calculation of stress using the finite element method in conjunction with the formulas of nonlinear elasticity theory.Â The first chapter presents the known theoretical foundations and general characteristics of rubbers; the second chapter gives information and formulas for hyperelastic bodies and formulas for calculating the strength criterion. The third chapter presents the results of calculations by means of ABAQUS software and a comparative analysis of the data obtained.
ModZoo: A Large-Scale Study of Modded Android Apps and Their Markets.
Creators: name: Saavedra, Luis Adan
name: Dutta, Hridoy S
name: Beresford, Alastair R
name: Hutchings, Alice
Publisher: name: IEEE
Year: 2024

description: We present the results of the first large-scale study into Android markets that offer modified or modded apps: apps whose features and functionality have been altered by a third-party. We analyse over 146k (thousand) apps obtained from 13 of the most popular modded app markets. Around 90% of them are altered in some way when compared to the official counterparts on Google Play. Modifications include games cheats, such as infinite coins or lives; mainstream apps with premium features provided for free; and apps with modified advertising identifiers or excluded ads. We find the original app developers lose significant potential revenue due to: the provision of paid for apps for free (around 5% of the apps across all markets); the free availability of premium features that require payment in the official app; and modified advertising identifiers. While some modded apps have all trackers and ads removed (3%), in general, the installation of these apps is significantly more risky for the user than the official version: modded apps are ten times more likely to be marked as malicious and often request additional permissions.
MuSR method and tomographic probability representation of spin states
Creators: name: Belousov, Yu. M.
name: Filippov, S. N.
name: Gorelkin, V. N.
name: Man'ko, V. I.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Quantum Physics (quant-ph)
subject: Materials Science (cond-mat.mtrl-sci)
subject: Other Condensed Matter (cond-mat.other)
subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: Muon spin rotation/relaxation/resonance (MuSR) technique for studying matter structures is considered by means of a recently introduced probability representation of quantum spin states. A relation between experimental MuSR histograms and muon spin tomograms is established. Time evolution of muonium, anomalous muonium, and a muonium-like system is studied in the tomographic representation. Entanglement phenomenon of a bipartite muon-electron system is investigated via tomographic analogues of Bell number and positive partial transpose (PPT) criterion. Reconstruction of the muon-electron spin state as well as the total spin tomography of composed system is discussed.
description: 20 pages, 4 figures, LaTeX, submitted to Journal of Russian Laser Research
title: ÐÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¿ÑÐ¸Ð¾Ð±ÑÐºÐ¾Ð³Ð¾ Ð¼ÐµÑÑÐ¾ÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ñ Ð´Ð»Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¿Ð¾Ð´Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ñ Ð¿Ð»Ð°ÑÑÐ¾Ð²Ð¾Ð³Ð¾ Ð´Ð°Ð²Ð»ÐµÐ½Ð¸Ñ
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ° Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ 01.04.03 - ÐÐµÑ Ð°Ð½Ð¸ÐºÐ° Ð¸ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ; 01.04.03_04 - ÐÐ°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð² Ð½ÐµÑÑÐµÐ³Ð°Ð·Ð¾Ð´Ð¾Ð±ÑÑÐ¸
titleType: Subtitle
Creators: name: ÐÐ¾Ð³Ð²Ð¸Ð½ÑÐº, ÐÑÑÐµÐ½Ð¸Ð¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2019
Subjects: ÐÐµÑÑÑÐ½ÑÐµ Ð¸ Ð³Ð°Ð·Ð¾Ð²ÑÐµ Ð¼ÐµÑÑÐ¾ÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ñ Ð Ð¾ÑÑÐ¸Ð¸
ÐÐ°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð¥Ð°Ð½ÑÑ-ÐÐ°Ð½ÑÐ¸Ð¹ÑÐº, Ð³Ð¾ÑÐ¾Ð´
Ð³Ð¸Ð´ÑÐ¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
ÑÐ¸ÑÑÐµÐ¼Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸
Ð¼ÐµÐ¶ÑÐºÐ²Ð°Ð¶Ð¸Ð½Ð½Ð¾Ðµ ÑÐ°ÑÑÑÐ¾ÑÐ½Ð¸Ðµ
ÑÐµÐ³Ð¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐ¹ ÑÑÑÐµÑÑ
ÑÑÐµÑÐ¸Ð½Ð° Ð°Ð²ÑÐ¾Ð³ÑÐ¿
Ð½Ð°Ð³Ð½ÐµÑÐ°ÑÐµÐ»ÑÐ½Ð°Ñ ÑÐºÐ²Ð°Ð¶Ð¸Ð½Ð°

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð¾Ð´Ð½Ð¾ÑÐ¾Ð´Ð½Ð°Ñ ÑÐ¿ÑÐ¾ÑÐµÐ½Ð½Ð°Ñ Ð¸ ÑÐµÐ°Ð»ÑÐ½Ð°Ñ Ð³ÐµÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ°Ñ 3D Ð³Ð¸Ð´ÑÐ¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸, Ð¿Ð¾Ð»Ð½Ð¾ÑÑÑÑ Ð¾Ð¿Ð¸ÑÑÐ²Ð°ÑÑÐ¸Ðµ Ð¿ÑÐ¾ÑÐµÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð½Ð¾Ð²Ð¾Ð³Ð¾ ÑÑÐ°ÑÑÐºÐ° ÐÑÐ¸Ð¾Ð±ÑÐºÐ¾Ð³Ð¾ Ð½ÐµÑÑÑÐ½Ð¾Ð³Ð¾ Ð¼ÐµÑÑÐ¾ÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ñ.
ÐÐ¾Ð´ÑÐ²ÐµÑÐ¶Ð´ÐµÐ½Ð° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ Ð·Ð°Ð²Ð¾Ð´Ð½ÐµÐ½Ð¸Ñ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð½Ð°Ð³Ð½ÐµÑÐ°ÑÐµÐ»ÑÐ½ÑÑ ÑÐºÐ²Ð°Ð¶Ð¸Ð½ Ð² Ð½Ð¸Ð·ÐºÐ¾Ð¿ÑÐ¾Ð½Ð¸ÑÐ°ÐµÐ¼ÑÑ ÐºÐ¾Ð»Ð»ÐµÐºÑÐ¾ÑÐ°Ñ. ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¾ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð¾Ðµ Ð²ÑÐµÐ¼Ñ Ð¿ÐµÑÐµÐ²Ð¾Ð´Ð° Ð´Ð¾Ð±ÑÐ²Ð°ÑÑÐ¸Ñ ÑÐºÐ²Ð°Ð¶Ð¸Ð½ Ð² Ð½Ð°Ð³Ð½ÐµÑÐ°Ð½Ð¸Ðµ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ Ð¼ÐµÐ¶ÑÐºÐ²Ð°Ð¶Ð¸Ð½Ð½Ð¾Ð³Ð¾ ÑÐ°ÑÑÑÐ¾ÑÐ½Ð¸Ñ Ð¸ ÑÐ°ÑÐ¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ cÐºÐ²Ð°Ð¶Ð¸Ð½ Ð½Ð° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸.
description: This thesis presents homogeneous simplified and real geological 3D hydrodynamic models that fully describe the process of developing a new section of the Priobskoye oil field. The effectiveness of the use of the waterflood system using injection wells in low-permeable reservoirs is confirmed. The optimal time for producing wells transfer to injection has been determined. The influence of the interwell distance and location on the development efficiency is investigated.
On the Vanishing of the CP Asymmetry in Leptogenesis due to Form Dominance
Creators: name: Choubey, Sandhya
name: King, S. F.
name: Mitra, Manimala
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We emphasize that the vanishing of the CP asymmetry in leptogenesis, previously observed for models with tri-bimaximal mixing and family symmetry, may be traced to a property of the type I see-saw mechanism satisfied by such models known as Form Dominance, corresponding to the case of a diagonal Casas-Ibarra R-matrix. Form Dominance leads to vanishing flavour-dependent CP asymmetries irrespective of whether one has tri-bimaximal mixing or a family symmetry. Successful leptogenesis requires violation of Form Dominance, but not necessarily violation of tri bimaximal mixing. This may be achieved in models where the family symmetry responsible for tri-bimaximal mixing is implemented indirectly and a strong neutrino mass hierarchy is present with the Form Dominance broken only softly by the right-handed neutrino responsible for the lightest neutrino mass, as in constrained sequential dominance.
description: 19 pages
Sonnenfleckenzeichnung Nr. 220.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 10.09.2019, 07:15, erstellt von Marco Cagnotti
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 2019

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Additional file 1 of Efficacy and safety of Cook staged Extubation Set in patients with difficult airway: a systematic review and meta-analysis
Creators: name: Lu, Cheng
name: Li, Jian
name: Zhao, Shibing
name: Zhang, Yajun
Publisher: name: figshare
Year: 2023
Subjects: Space Science
Medicine
Biological Sciences not elsewhere classified
Science Policy

description: Supplementary Material 1
Heating up the Baryonic Branch with U-duality: a unified picture of conifold black holes
Creators: name: Caceres, Elena
name: Nunez, Carlos
name: Zayas, Leopoldo A. Pando
Publisher: name: arXiv
Year: 2011
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study different aspects of a U-duality recently presented by Maldacena and Martelli and apply it to non-extremal backgrounds. In particular, starting from new non-extremal wrapped D5 branes we generate new non-extremal generalizations of the Baryonic Branch of the Klebanov-Strassler solution. We also elaborate on different conceptual aspects of these U-dualities, like its action on (extremal and non-extremal) Dp branes, dual models for Yang-Mills-like theories, generic asymptotics and decoupling limit of the generated solutions.
description: 20 pages plus various appendices. Ten figures. Version to appear in JHEP
Benessere socio-emotivo e rapporti con gli adulti a scuola
Creators: name: Pedrozzi, Sara
Publisher: name: Scuola Universitaria della Svizzera Italiana (SUPSI)
Year: 2013

description: Il presente lavoro di diploma ha l’obiettivo di indagare il benessere socio-emotivo dei preadolescenti del primo biennio delle scuole medie ticinesi e in particolare si prefigge di sondare quali rapporti sussistono tra la percezione che gli allievi hanno del supporto e del sostegno fornito dai docenti della loro scuola e le competenze socio-emotive che posseggono. I dati sono stati raccolti attraverso la somministrazione di un questionario tradotto e leggermente adattato alla realtà locale dal suo precursore canadese MDI. Ai fini delle analisi, gli items delle domande relative al rapporto con gli adulti a scuola sono state suddivise a seconda della presenza, della quantità e della qualità delle interazioni tra docente e allievo. I risultati emersi hanno permesso di confermare l’esistenza di un legame tra il benessere socio-emotivo e i rapporti con gli adulti a scuola, allineandosi con studi precedenti. In particolare, la ricerca ha dimostrato come la presenza e la numerosità di adulti di riferimento a scuola siano positivamente correlate allo sviluppo del preadolescente. Inoltre è emerso che il benessere degli allievi viene influenzato dalla qualità del rapporto con gli adulti presenti a scuola. I dati raccolti possono essere di interesse per interrogarsi sulla centralità della relazione docente-allievo, nell’ottica di migliorare il rapporto con gli allievi ma anche di promuovere progetti più ampi, come dei percorsi di alfabetizzazione emotiva. Relatori: Luciana Castelli, Alberto Crescentini, Luca Sciaroni. Materia: scienze dell'educazione
Sonnenfleckenzeichnung Nr. 237.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 28.09.2019, 08:30, erstellt von Sergio Cortesi
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 2019

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Valutazione sommativa in matematica: relazione tra quinta elementare e prima media
Creators: name: Torroni, Mattia
Publisher: name: Scuola Universitaria della Svizzera Italiana (SUPSI)
Year: 2011

description: Con questa ricerca di tipo esplicativo si è voluto verificare se nella scuola obbligatoria ticinese vi sia coerenza e continuità per quel che concerne la valutazione sommativa di matematica in vista anche della scadenza per l’introduzione del Concordato HarmoS. A tal proposito sono state raccolte le note di matematica di quinta elementare e prima media di 333 allievi provenienti da due sedi di scuola media. I dati raccolti sono poi stati analizzati con metodi statistici anche in base alle sedi frequentate e ai docenti avuti per ricercare eventuali relazioni. I risultati della ricerca hanno messo in evidenza come in generale con il passaggio alla scuola media mediamente il 60% degli allievi riscontra una diminuzione della nota di matematica conseguita in quinta elementare. Il restante 40% invece la riconferma o addirittura l’aumenta. Le analisi particolareggiate hanno permesso di rilevare che questa tendenza sostanzialmente non è significativamente influenzata dalle sedi frequentate o dai docenti avuti. Questa ricerca ha permesso pertanto di rilevare come la valutazione sommativa tra i due ordini non sia completamente discorde. Il fatto però che siano maggioritari gli allievi con una diminuzione lascia intendere che alcuni correttivi potrebbero essere attuati al fine di invertire tale tendenza. Relatore: Gianfranco Arrigo, Materia: matematica
Sonnenfleckenzeichnung Nr. 284.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 23.12.2019, 08:45, erstellt von Marco Cagnotti
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 2019

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 1.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Additional file 1 of MiR-942-5p targeting the IFI27 gene regulates HCT-8 cell apoptosis via a TRAIL-dependent pathway during the early phase of Cryptosporidium parvum infection
Creators: name: Xie, Fujie
name: Zhang, Yajun
name: Li, Juanfeng
name: Sun, Lulu
name: Zhang, Longxian
name: Qi, Meng
name: Zhang, Sumei
name: Jian, Fuchun
name: Li, Xiaoying
name: Li, Junqiang
name: Ning, Changsheng
name: Wang, Rongjun
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine

description: Additional file 1: Table S1. Primers used in RT-qPCR and sequences used for construct generating. Table S2. RNA oligonucleotides for miRNA and siRNA.
Evidence for core-hole-mediated inelastic x-ray scattering from metallic Fe$_{1.087}$Te
Creators: name: Hancock, J. N.
name: Viennois, R.
name: van der Marel, D.
name: Rønnow, H. M.
name: Guarise, M.
name: Lin, P. -H.
name: Grioni, M.
name: Sala, M. Moretti
name: Ghiringhelli, G.
name: Strocov, V. N.
name: Schlappa, J.
name: Schmitt, T.
Publisher: name: arXiv
Year: 2010
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 present a detailed analysis of resonant inelastic scattering (RIXS) from Fe$_{1.087}$Te with unprecedented energy resolution. In contrast to the sharp peaks typically seen in insulating systems at the transition metal $L_3$ edge, we observe spectra which show different characteristic features. For low energy transfer, we experimentally observe theoretically predicted many-body effects of resonant Raman scattering from a non-interacting gas of fermions. Furthermore, we find that limitations to this many-body electron-only theory are realized at high Raman shift, where an exponential lineshape reveals an energy scale not present in these considerations. This regime, identified as emission, requires considerations of lattice degrees of freedom to understand the lineshape. We argue that both observations are intrinsic general features of many-body physics of metals.
description: 4 pages, 4 figures
Additional file 6 of Screening for the prevention and early detection of cervical cancer: protocol for systematic reviews to inform Canadian recommendations
Creators: name: Gates, Allison
name: Pillay, Jennifer
name: Reynolds, Donna
name: Stirling, Rob
name: Traversy, Gregory
name: Korownyk, Christina
name: Moore, Ainsley
name: Thériault, Guylène
name: Thombs, Brett D.
name: Little, Julian
name: Popadiuk, Catherine
name: Niekerk, Dirk Van
name: Keto-Lambert, Diana
name: Vandermeer, Ben
name: Hartling, Lisa
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Cancer
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 6. Data Extraction Items for Each Key Question.
Sonnenfleckenzeichnung Nr. 250.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 12.10.2019, 07:15, erstellt von Marco Cagnotti
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 2019

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 4.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Sonnenfleckenzeichnung Nr. 143.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 17.06.2019, 07:15, erstellt von Marco Cagnotti
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 2019

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
title: How Social Enterprises Contribute to Alternative Food Systems
Creators: name: Costantini,, Anastasia
name: Pastorelli,, Gianluca
name: Sebillo,, Alessia
Publisher: name: CIRIEC
Year: 2019
Subjects: subject: Social Economy
subject: Social Enterprise
subject: Sustainable Food
subject: Social Innovation
subject: Sustainable Development
subject: Resilience
subject: Food Sovereignty
subject: Rural development

description: CIRIEC Working Papers, 2019/14
title: At-Sea Hake Observer Program 2025 Sampling Manual
Creators: name: Tuttle, Vanessa
name: Donovan, Cassandra
name: Memoly, Jeannine
Publisher: name: NOAA National Marine Fisheries Service Northwest Fisheries Science Center
publisherIdentifier: https://ror.org/05r7z1k40
publisherIdentifierScheme: ROR
Year: 2025

description: Information collected through the observer program is used to: (1) monitor catch and bycatch; (2) understand the population status and trends of fish stocks and protected species, as well as the interactions between them; (3) determine the quantity and distribution of net benefits derived from living marine resources; (4) predict the biological, ecological, and economic impacts of existing management actions and proposed management options; and (5) ensure that the observer programs can safely and efficiently collect the information required for the previous four uses.
Applications of Bayesian model averaging to the curvature and size of the Universe
Creators: name: Vardanyan, M.
name: Trotta, R.
name: Silk, J.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Bayesian model averaging is a procedure to obtain parameter constraints that account for the uncertainty about the correct cosmological model. We use recent cosmological observations and Bayesian model averaging to derive tight limits on the curvature parameter, as well as robust lower bounds on the curvature radius of the Universe and its minimum size, while allowing for the possibility of an evolving dark energy component. Because flat models are favoured by Bayesian model selection, we find that model-averaged constraints on the curvature and size of the Universe can be considerably stronger than non model-averaged ones. For the most conservative prior choice (based on inflationary considerations), our procedure improves on non model-averaged constraints on the curvature by a factor of ~ 2. The curvature scale of the Universe is conservatively constrained to be R_c > 42 Gpc (99%), corresponding to a lower limit to the number of Hubble spheres in the Universe N_U > 251 (99%).
description: Fixed typos, added ref, added non model-averaged constraints for comparison. Matches version accepted by MNRAS Lett
Sonnenfleckenzeichnung Nr. 255.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 23.10.2019, 08:00, erstellt von Marco Cagnotti
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 2019

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Giant Nonlocality near the Dirac Point in Graphene
Creators: name: Abanin, D. A.
name: Morozov, S. V.
name: Ponomarenko, L. A.
name: Gorbachev, R. V.
name: Mayorov, A. S.
name: Katsnelson, M. I.
name: Watanabe, K.
name: Taniguchi, T.
name: Novoselov, K. S.
name: Levitov, L. S.
name: Geim, A. K.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Transport measurements have been a powerful tool for uncovering new electronic phenomena in graphene. We report nonlocal measurements performed in the Hall bar geometry with voltage probes far away from the classical path of charge flow. We observe a large nonlocal response near the Dirac point in fields as low as 0.1T, which persists up to room temperature. The nonlocality is consistent with the long-range flavor currents induced by lifting of spin/valley degeneracy. The effect is expected to contribute strongly to all magnetotransport phenomena near the neutrality point.
Sonnenfleckenzeichnung Nr. 101.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 27.04.2019, 06:45, erstellt von Marco Cagnotti
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 2019

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
New light on the Gaia DR2 parallax zero-point: influence of the asteroseismic approach, in and beyond the Kepler field
Creators: name: Khan, Saniya
name: Miglio, Andrea
name: Mosser, Benoît
name: Arenou, Frédéric
name: Belkacem, Kévin
name: Brown, Anthony G. A.
name: Katz, David
name: Casagrande, Luca
name: Chaplin, William J.
name: Davies, Guy R.
name: Rendle, Ben M.
name: Rodrigues, Thaíse S.
name: Bossini, Diego
name: Cantat-Gaudin, Tristan
name: Elsworth, Yvonne P.
name: Girardi, Leo
name: North, Thomas S. H.
name: Vallenari, Antonella
Publisher: name: Zenodo
Year: 2019
Subjects: asteroseismology
astrometry
parallaxes
stars: low-mass

description: The importance of studying the Gaia DR2 parallax zero-point by external means was underlined by Lindegren et al. (2018), and initiated by several works making use of Cepheids, eclipsing binaries, and asteroseismology. Despite a very efficient elimination of basic-angle variations, a small fluctuation remains and shows up as a small offset in the Gaia DR2 parallaxes.

By combining astrometric, asteroseismic, spectroscopic, and photometric constraints, we undertake a new analysis of the Gaia parallax offset for nearly 3000 red-giant branch (RGB) and 2200 red clump (RC) stars observed by Kepler, as well as about 500 and 700 red giants (both RGB and RC) selected by the K2 Galactic Archaeology Program in campaigns 3 and 6. Engaging into a thorough comparison of the astrometric and asteroseismic parallaxes, we are able to highlight the influence of the asteroseismic method, and measure parallax offsets in the Kepler field that are compatible with independent estimates from literature and open clusters.

Moreover, adding the K2 fields to our investigation allows us to retrieve a clear illustration of the positional dependence of the zero-point, in general agreement with the information provided by quasars.

Lastly, we initiate a two-step methodology to make progress in the simultaneous calibration of the asteroseismic scaling relations and of the Gaia DR2 parallax offset, which will greatly benefit from the gain in precision with the third Data Release of Gaia.
CP-violating MSSM Higgs at Tevatron and LHC
Creators: name: Das, Siba Prasad
name: Drees, Manuel
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We analyze the prospect for observing the intermediate neutral Higgs boson ($h_2$) in its decay to two lighter Higgs bosons ($h_1$) at the presently operating hadron colliders in the framework of the CP violating MSSM using the PYTHIA event generator. We consider the lepton+ 4-jets+ $\met$ channel from associate $W h_2$ production, with $W h_2 \ra W h_1 h_1 \ra \ell ν_\ell b \bar b b\bar b$. We require two or three tagged $b$-jets. We explicitly consider all relevant Standard Model backgrounds, treating $c$-jets separately from light flavor and gluon jets and allowing for mistagging. We find that it is very hard to observe this signature at the Tevatron, even with 20 fb$^{-1}$ of data, in the LEP--allowed region of parameter space due to the small signal efficiency. At the LHC, a priori huge SM backgrounds can be suppressed by applying judiciously chosen kinematical selections. After all cuts, we are left with a signal cross section of around 0.5 fb, and a signal to background ratio between 1.2 and 2.9. According to our analysis this Higgs signal should be viable at the LHC in the vicinity of present LEP exclusion once 20 to 50 fb$^{-1}$ of data have been accumulated at $\sqrt{s}=14$ TeV.
description: 6 pages, 2 figures, talk presented at PASCOS 2010(Valencia) and SUSY 10(Bonn)