cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
How are new citation-based journal indicators adding to the bibliometric toolbox?
Creators: name: Leydesdorff, Loet
Publisher: name: arXiv
Year: 2009
Subjects: subject: Physics and Society (physics.soc-ph)
subject: Digital Libraries (cs.DL)
subject: Data Analysis, Statistics and Probability (physics.data-an)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: The launching of Scopus and Google Scholar, and methodological developments in Social Network Analysis have made many more indicators for evaluating journals available than the traditional Impact Factor, Cited Half-life, and Immediacy Index of the ISI. In this study, these new indicators are compared with one another and with the older ones. Do the various indicators measure new dimensions of the citation networks, or are they highly correlated among them? Are they robust and relatively stable over time? Two main dimensions are distinguished -- size and impact -- which together shape influence. The H-index combines the two dimensions and can also be considered as an indicator of reach (like Indegree). PageRank is mainly an indicator of size, but has important interactions with centrality measures. The Scimago Journal Ranking (SJR) indicator provides an alternative to the Journal Impact Factor, but the computation is less easy.
Appendix B. Baseline characteristics for 64 men treated with rectal cancer included in time-to-recurrence analysis.docx
Creators: name: Tapper, John
name: Arver, Stefan
name: Holm, Torbjörn
name: Bottai, Matteo
name: Machado, Mikael
name: Jasuja, Ravi
name: Martling, Anna
name: Buchli, Christian
Publisher: name: figshare
Year: 2021
Subjects: Medicine

description: Baseline characteristics for 64 men treated for rectal cancer included in time-to-recurrence analysis.
Translating Charlottes. Clare Boylan’s “The Secret Diary of Mrs Rochester”: Between Red Rooms and Yellow Wallpapers
Creators: name: Tallone, Giovanna
Publisher: name: Biblioteca di Studi di Filologia Moderna: Series, Journals and Workshop
Year: 2013

description: In her short story “The Secret Diary of Mrs Rochester”, Clare Boylan playfully uses a variation of the postmodern trend of “writing back” Victorian classics to create a sequel of Charlotte Brontë’s Jane Eyre (1847). Shedding light on Jane’s married life, Boylan makes a parody of Brontë’s language and narrative conventions making Jane an eccentric. In particular, the presence of closed spaces in the story replicates the claustrophobia of the red room in Jane Eyre, and from this point of view Boylan’s story bears parallelisms with Charlotte Perkins Gilman’s short story “The Yellow Wallpaper” (1892). Intertextuality and metanarrative perspectives of both stories draw attention to the textual space of the story and the elusive text that is being written/read. The “secret diary” assumed in the title is not the text that appears on the page. In both stories the protagonist and first-person narrator is engaged in writing an elusive text while confined in a secluded space.
description: Studi irlandesi. A Journal of Irish Studies, No 3 (2013)
Theory of fractional vortex escape in a 0-kappa long Josephson junction
Creators: name: Vogel, K.
name: Kato, T.
name: Schleich, W. P.
name: Koelle, D.
name: Kleiner, R.
name: Goldobin, E.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We consider a fractional Josephson vortex in an infinitely long 0-kappa Josephson junction. A uniform bias current applied to the junction exerts a Lorentz force acting on a vortex. When the bias current becomes equal to the critical (or depinning) current, the Lorentz force tears away an integer fluxon and the junction switches to the resistive state. In the presence of thermal and quantum fluctuations this escape process takes place with finite probability already at subcritical values of the bias current. We analyze the escape of a fractional vortex by mapping the Josephson phase dynamics to the dynamics of a single particle in a metastable potential and derive the effective parameters of this potential. This allows us to predict the behavior of the escape rate as a function of the topological charge of the vortex.
A cosmological independent calibration of the Ep,i-Eiso correlation for Gamma Ray Bursts
Creators: name: Capozziello, Salvatore
name: Izzo, Luca
Publisher: name: arXiv
Year: 2010
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The relation connecting the emitted isotropic energy and the rest-frame peak energy of the \nuFνspectra of Gamma-Ray Bursts (the Amati relation), strictly depends on the cosmological model, so we need a method to obtain an independent calibration of it. Using the Union Supernovae Ia catalog, we obtain a cosmographic luminosity distance in the y-redshift and demonstrate that this parametrization approximates very well the fiducial standard comsomlogical model \LambdaCDM. Furthermore, by this cosmographic luminosity distance dl, it is possible to achieve the Amati relation independent on the cosmological model. The cosmographic Amati relation that we obtain agrees, in the errors, with other cosmological-independent calibrations proposed in the literature. This could be considered a good indication in view to obtain standard candles by Gamma-Ray Bursts Key words. Gamma rays : bursts - Cosmology
description: 6 pages, 3 figures
title: ÐÐ¾Ð²ÑÑÐµÐ½Ð¸Ðµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð·Ð°ÐºÑÐ¿Ð¾Ðº Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸ÑÑ Ð½ÐµÑÑÐµÐ³Ð°Ð·Ð¾Ð²Ð¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ°
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: Ð¢Ð¾Ð¿Ð¾ÑÐ¾Ð², 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: 2017
Subjects: ÐÐµÑÑÑÐ½Ð°Ñ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾ÑÑÑ
ÐÐ°Ð·Ð¾Ð²Ð°Ñ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾ÑÑÑ
Ð·Ð°ÐºÑÐ¿Ð¾ÑÐ½Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ðµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸
ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¸Ðµ Ð·Ð°ÐºÑÐ¿ÐºÐ¸

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ Ð·Ð°ÐºÑÐ¿Ð¾ÑÐ½Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð½ÐµÑÑÐµÐ³Ð°Ð·Ð¾Ð²ÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¹. Ð¦ÐµÐ»ÑÑ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸ ÑÐ²Ð»ÑÐµÑÑÑ Ð°Ð½Ð°Ð»Ð¸Ð· Ð·Ð°ÐºÑÐ¿Ð¾ÑÐ½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð½ÐµÑÑÐµÐ³Ð°Ð·Ð¾Ð²Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¾Ð¹ Ð¡Ð»ÑÐ¶Ð±Ñ ÐÐÐ Â«ÐÐ°Ð·Ð¿ÑÐ¾Ð¼Ð½ÐµÑÑÑ-Ð¡Ð½Ð°Ð±Ð¶ÐµÐ½Ð¸ÐµÂ» Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÑÐµÐ¹ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐ¸ÑÑÐµÐ¼Ñ Ð·Ð°ÐºÑÐ¿Ð¾Ðº ÑÑÐ»ÑÐ³. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð·Ð°ÐºÑÐ¿Ð¾ÑÐ½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¾Ð¹ Ð¡Ð»ÑÐ¶Ð±Ñ ÐÐÐ Â«ÐÐ°Ð·Ð¿ÑÐ¾Ð¼Ð½ÐµÑÑÑ-Ð¡Ð½Ð°Ð±Ð¶ÐµÐ½Ð¸ÐµÂ» Ð±ÑÐ»Ð¸ Ð²ÑÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸, Ð±ÑÐ»Ð¸ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð»ÑÑÑÐ¸Ðµ Ð¼Ð¸ÑÐ¾Ð²ÑÐµ Ð¿ÑÐ°ÐºÑÐ¸ÐºÐ¸ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð·Ð°ÐºÑÐ¿Ð¾Ðº, Ð½Ð° Ð¸Ñ Ð¾ÑÐ½Ð¾Ð²Ðµ Ð²ÑÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¼ÐµÑÐ¾Ð´Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð·Ð°ÐºÑÐ¿Ð¾Ðº. ÐÑÐ»Ð¾ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ ÑÐµÑÐ½Ð¸ÐºÐ¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð¸ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ¾Ð² Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð·Ð°ÐºÑÐ¿Ð¾Ðº. ÐÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð° Ðº Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ð° ÐºÐ»ÑÑÐµÐ²ÑÑ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ Ð´Ð»Ñ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð² ÐÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÑÑ Ð¡Ð»ÑÐ¶Ð±Ñ ÐÐÐ Â«ÐÐ°Ð·Ð¿ÑÐ¾Ð¼Ð½ÐµÑÑÑ-Ð¡Ð½Ð°Ð±Ð¶ÐµÐ½Ð¸ÐµÂ».
Additional file 1 of Incidence and cost of haemolytic uraemic syndrome in urban China: a national population-based analysis
Creators: name: Feng, Jingnan
name: Xu, Ke
name: Shi, Xinmiao
name: Xu, Lu
name: Liu, Lili
name: Wang, Fang
name: Zhong, Xuhui
name: Liu, Guozhen
name: Wang, Jinxi
name: Gao, Pei
name: Ding, Jie
name: Wang, Shengfeng
name: Zhan, Siyan
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Biotechnology
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Science Policy

description: Additional file 1: Supplementary table 1. Sixteen provinces in China were included in this research.  Supplementary table 2. Basic characteristics of the populations in 16 provinces in China in 2016.
Elizabeth Vesey and the Art of Educating Oneself, Between London and Lucan
Creators: name: Stefanelli, Maria Anita
Publisher: name: Biblioteca di Studi di Filologia Moderna: Series, Journals and Workshop
Year: 2013

description: A 1926 publication describes the Library of Mrs. Elizabeth Vesey (1715- 1791), a Bluestocking and the wife, by second marriage, of Agmondisham Vesey, a member of the Irish Parliament. The essay examines the books that refer to the cultural background and critical abilities of an Irish literary lady who transmitted but a small record of her literary competence to posterity. The excursus points to her historical, philosophical, and theological formation as the daughter of the Bishop of Ossory, besides her acquaintance with foreign literatures (most prominently the Italian one) and her ideological involvement with the question of the American colonies that she only briefly hints at in a letter to her friend Mrs. Montague in order not to trespass the borders of the public sphere. Vesey’s portrait would be mostly imperfect if this collection was ignored.
description: Studi irlandesi. A Journal of Irish Studies, No 3 (2013)
title: ÐÐ°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð° "ÐÐ±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð² Ð¶Ð¸Ð·Ð½ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ¸ÐºÐ»Ð° Ð¸Ð·Ð´ÐµÐ»Ð¸Ñ"
title: Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ðº Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ (Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸)
titleType: Subtitle
Creators: name: ÐÐ¸ÐºÐ¸ÑÐ¾ÑÐ¾Ð², ÐÐ°Ð»ÐµÑÐ¸Ð¹
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2016
Subjects: 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

description: ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ, ÑÐ°ÑÐºÑÑÐ²Ð°ÑÑÐ¸Ðµ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ðµ, Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÑ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¸ Ð¾ÑÐ¾ÑÐ¼Ð»ÐµÐ½Ð¸Ñ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ (Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸) ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ²Ð¾Ð¹ Ð¾ÑÐ½Ð¾Ð²Ð½Ð¾Ð¹ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ðµ Â«ÐÐ±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð² Ð¶Ð¸Ð·Ð½ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ¸ÐºÐ»Ð° Ð¸Ð·Ð´ÐµÐ»Ð¸ÑÂ» Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² 15.04.05 Â«ÐÐ¾Ð½ÑÑÑÑÐºÑÐ¾ÑÑÐºÐ¾-ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÑ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Â». ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¿Ð¾ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐµÑÐµÐ²Ð¾Ð³Ð¾ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð²ÑÐ·Ð¾Ð², ÑÑÐºÐ¾Ð²Ð¾Ð´ÑÑÐ²Ð° ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼Ð¸, Ð¿Ð¾ÑÑÐ´ÐºÑ Ð·Ð°ÑÐ¸ÑÑ Ð¸ ÑÑÐ°Ð½ÐµÐ½Ð¸Ñ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¸Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¹. ÐÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ñ Ð´Ð»Ñ Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»ÐµÐ¹, Ð¾ÑÑÑÐµÑÑÐ²Ð»ÑÑÑÐ¸Ñ ÑÑÐºÐ¾Ð²Ð¾Ð´ÑÑÐ²Ð¾ Ð²ÑÐ¿ÑÑÐºÐ½ÑÐ¼Ð¸ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐ¼Ð¸ ÑÐ°Ð±Ð¾ÑÐ°Ð¼Ð¸ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² 15.04.05 Â«ÐÐ¾Ð½ÑÑÑÑÐºÑÐ¾ÑÑÐºÐ¾- ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÑ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Â», Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², Ð¿Ð¾Ð´Ð³Ð¾ÑÐ°Ð²Ð»Ð¸Ð²Ð°ÑÑÐ¸Ñ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¸Ðµ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð´Ð»Ñ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÐºÐ¾Ð², Ð¾ÑÐ³Ð°Ð½Ð¸Ð·ÑÑÑÐ¸Ñ Ð¸ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ð¸ÑÑÑÑÐ¸Ñ Ð¿ÑÐ¾ÑÐµÑÑ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð².
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ Ð¡Ð¾Ð²ÐµÑÐ° Ð¿Ð¾ Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð£ÑÐµÐ½Ð¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ° ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾.
Design of a Bilateral Microstrip MIMO Antenna in S-Band for Satellite Communication
Creators: name: M. Annapoorna
name: Dr. I. Kalphana
Publisher: name: Institute for Interdisciplinary and Venture Publication
Year: 2025
Subjects: Fixed Satellite Service
Direct Broadcast Satellites
Direct-To-Home Television
Global Navigation Satellite Systems
Multiple-Input Multiple-Output
Axial Ratio
High-Frequency Structure Simulator
Voltage Standing Wave Ratio
Mobile Satellite Service

description: This project centers on the design and development of a bilateral microstrip MIMO antenna for S-band satellite communication, especially for mobile satellite services for high-speed communication, Earth observation data transmission, IoT networks in remote areas, military communication, and telemedicine. The microstrip MIMO antenna is designed with dimensions of 55.9 mm × 71.7 mm, operating at 2.8 GHz on low-cost FR-4 substrate with a thickness of 1.6mm is selected for its cost-effectiveness and availability. High Frequency Structural Simulator (HFSS) is used to design and simulate the antenna. Through simulation-based optimization, parameters like return loss, VSWR, radiation pattern, directivity, H-plane co-cross polarization, E-plane co-cross polarization, and gain are thoroughly analyzed to meet stringent requirements for satellite communication at 2.8 GHz.
A Zero-Gravity Instrument to Study Low Velocity Collisions of Fragile Particles at Low Temperatures
Creators: name: Salter, D. M.
name: Heißelmann, D.
name: Chaparro, G.
name: van der Wolk, G.
name: Reißaus, P.
name: Borst, A. G.
name: Dawson, R. W.
name: de Kuyper, E.
name: Drinkwater, G.
name: Gebauer, K.
name: Hutcheon, M.
name: Linnartz, H.
name: Molster, F. J.
name: Stoll, B.
name: van der Tuijn, P. C.
name: Fraser, H. J.
name: Blum, J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: We discuss the design, operation, and performance of a vacuum setup constructed for use in zero (or reduced) gravity conditions to initiate collisions of fragile millimeter-sized particles at low velocity and temperature. Such particles are typically found in many astronomical settings and in regions of planet formation. The instrument has participated in four parabolic flight campaigns to date, operating for a total of 2.4 hours in reduced gravity conditions and successfully recording over 300 separate collisions of loosely packed dust aggregates and ice samples. The imparted particle velocities achieved range from 0.03-0.28 m s^-1 and a high-speed, high-resolution camera captures the events at 107 frames per second from two viewing angles separated by either 48.8 or 60.0 degrees. The particles can be stored inside the experiment vacuum chamber at temperatures of 80-300 K for several uninterrupted hours using a built-in thermal accumulation system. The copper structure allows cooling down to cryogenic temperatures before commencement of the experiments. Throughout the parabolic flight campaigns, add-ons and modifications have been made, illustrating the instrument flexibility in the study of small particle collisions.
description: D. M. Salter, D. Hei{\ss}elmann, G. Chaparro, G. van der Wolk, P. Rei{\ss}aus, A. G. Borst, R. W. Dawson, E. de Kuyper, G. Drinkwater, K. Gebauer, M. Hutcheon, H. Linnartz, F. J. Molster, B. Stoll, P. C. van der Tuijn, H. J. Fraser, and J. Blum
title: Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿Ð¾ ÑÑÐ°Ð½ÑÑÐ·ÑÐºÐ¾Ð¼Ñ ÑÐ·ÑÐºÑ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð²âÐ»Ð¸Ð½Ð³Ð²Ð¸ÑÑÐ¾Ð² Ð·Ð°Ð¾ÑÐ½Ð¾Ð³Ð¾ Ð¾ÑÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÐÐ¨ÐÐÐÐ¸ÐÐ ÐÐ Ð¡ÐÐ±ÐÐ£ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Creators: name: ÐÐºÑÐ¿Ð¾Ð²Ð°, ÐÐ¸ÐºÑÐ¾ÑÐ¸Ñ
name: Ð¡Ð¿Ð¸ÑÐ¸Ð´Ð¾Ð½Ð¾Ð²Ð°, ÐÐ°ÑÐ°Ð»ÑÑ
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: ÑÑÐ°Ð½ÑÑÐ·ÑÐºÐ¸Ð¹ ÑÐ·ÑÐº
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: ÐÐ°Ð½Ð½Ð¾Ðµ ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð²-Ð»Ð¸Ð½Ð³Ð²Ð¸ÑÑÐ¾Ð² Ð·Ð°Ð¾ÑÐ½Ð¾Ð³Ð¾ Ð¾ÑÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÐÐ¨ÐÐÐÐ¸ÐÐ ÐÐ Ð¡ÐÐ±ÐÐ£ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾, Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ð¹ ÑÑÐ°Ð½ÑÑÐ·ÑÐºÐ¸Ð¹ ÑÐ·ÑÐº ÐºÐ°Ðº Ð²ÑÐ¾ÑÐ¾Ð¹ Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½ÑÐ¹. Ð¦ÐµÐ»Ñ - Ð² Ð¾ÑÐµÐ½Ñ Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð½ÑÑ Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ ÑÑÐ»Ð¾Ð²Ð¸ÑÑ Ð½Ðµ ÑÐ¾Ð»ÑÐºÐ¾ Ð´Ð°ÑÑ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¾ Ð±Ð°Ð·Ð¾Ð²ÑÑ Ð³ÑÐ°Ð¼Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÑÑÑÐºÑÑÑÐ°Ñ Ð¸ Ð¿ÑÐµÐ´Ð¾ÑÑÐ°Ð²Ð¸ÑÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÑ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ Ð¿ÐµÑÐ²Ð¾Ð³Ð¾ Ð¾Ð¿ÑÑÐ° Ð¿ÐµÑÐµÐ²Ð¾Ð´Ð°, Ð½Ð¾ Ð¸ ÑÐ¿Ð¾ÑÐ¾Ð±ÑÑÐ²Ð¾Ð²Ð°ÑÑ Ð¸Ð½Ð¸ÑÐ¸Ð°ÑÐ¸Ð¸ Ð´Ð¸Ð°Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÐµÑÐ¸ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¿ÐµÑÐ²Ð¸ÑÐ½ÑÑ Ð½Ð°Ð²ÑÐºÐ¾Ð² Ð°ÑÐ´Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð¾Ð²Ð¾Ð³Ð¾ Ð´Ð»Ñ Ð½Ð¸Ñ Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½Ð¾Ð³Ð¾ ÑÐ·ÑÐºÐ°, Ð° ÑÐ°Ð¼Ð¾Ðµ Ð³Ð»Ð°Ð²Ð½Ð¾Ðµ â Ð¼Ð¾ÑÐ¸Ð²Ð¸ÑÐ¾Ð²Ð°ÑÑ ÑÑÑÐ´ÐµÐ½ÑÐ° Ð½Ð° Ð´Ð°Ð»ÑÐ½ÐµÐ¹ÑÑÑ ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½ÑÑ ÑÐ°Ð±Ð¾ÑÑ, Ð·Ð°ÑÐ¾Ð´Ð¸ÑÑ Ð¸ Ð²Ð·ÑÐ°ÑÑÐ¸ÑÑ Ð¸Ð½ÑÐµÑÐµÑ Ð¸ Ð¶ÐµÐ»Ð°Ð½Ð¸Ðµ Ð´Ð¾ÑÑÐ¸Ð³Ð½ÑÑÑ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ¾Ð²Ð½Ñ ÐµÐ³Ð¾ Ð²Ð»Ð°Ð´ÐµÐ½Ð¸Ñ. Ð Ð´Ð°Ð½Ð½Ð¾Ð¼ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð¾ÑÐ½Ð¾Ð²Ð½Ð¾Ðµ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ ÑÐ´ÐµÐ»ÑÐµÑÑÑ Ð³ÑÐ°Ð¼Ð¼Ð°ÑÐ¸ÐºÐµ. Ð¢Ð°ÐºÐ¸Ðµ Ð²Ð¸Ð´Ñ ÑÐµÑÐµÐ²Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸, ÐºÐ°Ðº Ð°ÑÐ´Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ, Ð³Ð¾Ð²Ð¾ÑÐµÐ½Ð¸Ðµ, ÑÑÐµÐ½Ð¸Ðµ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´ÑÐµÑÑÑ Ð´Ð¾Ð±Ð°Ð²Ð»ÑÑÑ Ðº Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð³ÑÐ°Ð¼Ð¼Ð°ÑÐ¸ÐºÐ¸ Ð½Ð° ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð¸Ðµ Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»Ñ Ð² Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÐ¸ Ð¾Ñ Ð¸ÑÑÐ¾Ð´Ð½ÑÑ Ð´Ð°Ð½Ð½ÑÑ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÐºÐ°Ð¶Ð´Ð¾Ð¹ Ð½Ð¾Ð²Ð¾Ð¹ Ð³ÑÑÐ¿Ð¿Ñ. ÐÐµÐ»Ð°ÑÑ ÑÑÐ¾ Ð»ÑÑÑÐµ Ð² ÐºÐ°ÑÐµÑÑÐ²Ðµ Ð¸Ð»Ð»ÑÑÑÑÐ°ÑÐ¸Ð¸ Ðº Ð¸Ð·ÑÑÐµÐ½Ð½Ð¾Ð¼Ñ Ð³ÑÐ°Ð¼Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð¼Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ Ñ ÑÐµÐ»ÑÑ Ð½Ð°Ð¸Ð»ÑÑÑÐµÐ³Ð¾ ÐµÐ³Ð¾ Ð·Ð°ÐºÑÐµÐ¿Ð»ÐµÐ½Ð¸Ñ Ð¸ Ñ ÑÐµÐ»ÑÑ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ Ð½Ð°Ð²ÑÐºÐ° Ð¿ÐµÑÐµÐ²Ð¾Ð´Ð°.
Against the Oedipal Politics of Formation in Edna O’Brien’s A Pagan Place: “Women do not Count, Neither Shall they be Counted”
Creators: name: Mansouri, Shahriyar
Publisher: name: Biblioteca di Studi di Filologia Moderna: Series, Journals and Workshop
Year: 2013

description: Edna O’Brien’s A Pagan Place is one of her lesser-known novels, which discusses decades of women’s sexual oppression and anomalous formations; it is a sexually conscious narrative of an Irish formation which enjoyed the socio-cultural and intellectual liberties of the “sexy sixties”, and critiqued the Oedipal Irish society of the 1930s and 1940s. Obsessed with physical and spiritual decency, the masculinized Society formed “moral codes” that by definition exiled the Irish woman to social and political marginalia. Socio-politically conscious narratives such as O’Brien’s A Pagan Place, however, functioned as not just social critiques, drawing on a culture of post-revolution stasis and neoconservative identity politics but also as vehicles for enabling a generation of oppressed women to voice their concerns and struggles with their feminine formation in a dominantly masculinized Society. By drawing on a Deleuzian definition of Oedipal Society, this study explores boundaries, limitations and alternatives of feminine formation in Ireland in the 1930s and 1940s.
description: Studi irlandesi. A Journal of Irish Studies, No 3 (2013)
Computational Imaging and Artificial Intelligence: The Next Revolution of Mobile Vision
Creators: name: Suo, Jinli
name: Zhang, Weihang
name: Gong, Jin
name: Yuan, Xin
name: Brady, David J.
name: Dai, Qionghai
Publisher: name: arXiv
Year: 2021
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Artificial Intelligence (cs.AI)
subject: Image and Video Processing (eess.IV)
subject: FOS: Computer and information sciences
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: Signal capture stands in the forefront to perceive and understand the environment and thus imaging plays the pivotal role in mobile vision. Recent explosive progresses in Artificial Intelligence (AI) have shown great potential to develop advanced mobile platforms with new imaging devices. Traditional imaging systems based on the "capturing images first and processing afterwards" mechanism cannot meet this unprecedented demand. Differently, Computational Imaging (CI) systems are designed to capture high-dimensional data in an encoded manner to provide more information for mobile vision systems.Thanks to AI, CI can now be used in real systems by integrating deep learning algorithms into the mobile vision platform to achieve the closed loop of intelligent acquisition, processing and decision making, thus leading to the next revolution of mobile vision.Starting from the history of mobile vision using digital cameras, this work first introduces the advances of CI in diverse applications and then conducts a comprehensive review of current research topics combining CI and AI. Motivated by the fact that most existing studies only loosely connect CI and AI (usually using AI to improve the performance of CI and only limited works have deeply connected them), in this work, we propose a framework to deeply integrate CI and AI by using the example of self-driving vehicles with high-speed communication, edge computing and traffic planning. Finally, we outlook the future of CI plus AI by investigating new materials, brain science and new computing techniques to shed light on new directions of mobile vision systems.
Compensation of Field-Induced Frequency Shifts in Ramsey Spectroscopy of Optical Clock Transitions
Creators: name: Taichenachev, A. V.
name: Yudin, V. I.
name: Oates, C. W.
name: Barber, Z. W.
name: Lemke, N. D.
name: Ludlow, A. D.
name: Sterr, U.
name: Lisdat, Ch.
name: Riehle, F.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Optics (physics.optics)
subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: We have extended Ramsey spectroscopy by stepping the probe frequency during the two Ramsey excitation pulses to compensate frequency shifts induced by the excitation itself. This makes precision Ramsey spectroscopy applicable even for transitions that have Stark and Zeeman shifts comparable to the spectroscopic resolution. The method enables a new way to evaluate and compensate key frequency shifts, which benefits in particular, optical clocks based on magnetic field-induced, spectroscopy, two-photon transitions, or heavily forbidden transitions.
description: 5 pages, 3 figures
First evidence for spectral state transitions in the ESO243-49 hyper luminous X-ray source HLX-1
Creators: name: Godet, O.
name: Barret, D.
name: Webb, N. A.
name: Farrell, S. A.
name: Gehrels, N.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The brightest Ultra-Luminous X-ray source (ULX), ESO 243-49 HLX-1, with a 0.2 - 10 keV X-ray luminosity of up to 10^42 erg s^-1, provides the strongest evidence to date for the existence of intermediate mass black holes. Although small scale X-ray spectral variability has already been demonstrated, we have initiated a monitoring campaign with the X-ray Telescope onboard the Swift satellite to search for luminosity-related spectral changes and to compare its behavior with the better studied stellar mass black holes. In this paper, we report a drop in the XRT count rate by a factor of ~8 which occurred simultaneously with a hardening of the X-ray spectrum. A second observation found that the source had re-brightened by a factor of ~21 which occurred simultaneously with a softening of the X-ray spectrum. This may be the first evidence for a transition between the low/hard and high/soft states.
description: Accepted by ApJ Letter, 2 figures
title: ÐÑÐ¸Ñ Ð¾Ð»Ð¾Ð³Ð¾âÐ¿ÐµÐ´Ð°Ð³Ð¾Ð³Ð¸ÑÐµÑÐºÐ°Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ° Ð¼Ð¾Ð»Ð¾Ð´ÑÑ ÑÐ¿Ð¾ÑÑÑÐ¼ÐµÐ½Ð¾Ð²âÐ¸Ð½Ð²Ð°Ð»Ð¸Ð´Ð¾Ð² Ðº Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¼Ñ ÑÐ°Ð¼Ð¾Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ
title: Psychological and pedagogical preparation of young athletes with disabilities for professional selfâdetermination
Creators: name: ÐÑÐµÑÐ¾Ð², ÐÐ½Ð´ÑÐµÐ¹
name: ÐÐ¾ÑÐ¾Ð±ÑÑÐ², Ð¡ÐµÑÐ³ÐµÐ¹
name: "Ð¡Ð¿Ð¾ÑÑ, ÑÐµÐ»Ð¾Ð²ÐµÐº, Ð·Ð´Ð¾ÑÐ¾Ð²ÑÐµ", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¹ Ð½Ð°ÑÑÐ½ÑÐ¹ ÐºÐ¾Ð½Ð³ÑÐµÑÑ
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2023
Subjects: ÑÐ¿Ð¾ÑÑÑÐ¼ÐµÐ½ÑâÐ¸Ð½Ð²Ð°Ð»Ð¸Ð´Ñ
Ð¿Ð°ÑÐ°Ð»Ð¸Ð¼Ð¿Ð¸Ð¹ÑÐºÐ¸Ð¹ ÑÐ¿Ð¾ÑÑ
Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð°Ñ Ð¾ÑÐ¸ÐµÐ½ÑÐ°ÑÐ¸Ñ
disabled athletes
Paralympic sports
professional orientation

description: Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐ°Ð¼Ð¾Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÑÐ¿Ð¾ÑÑÑÐ¼ÐµÐ½Ð¾Ð²âÐ¸Ð½Ð²Ð°Ð»Ð¸Ð´Ð¾Ð² Ð¿Ð¾ÑÐ»Ðµ Ð¾ÐºÐ¾Ð½ÑÐ°Ð½Ð¸Ñ Ð¿ÐµÑÐ¸Ð¾Ð´Ð° Ð²ÑÑÑÑÐ¿Ð»ÐµÐ½Ð¸Ð¹. ÐÐ½Ð°Ð»Ð¸Ð·Ð¸ÑÑÑÑÑÑ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¿ÑÐ¾ÑÐ¾ÑÐ¸ÐµÐ½ÑÐ°ÑÐ¸Ð¸ Ð¼Ð¾Ð»Ð¾Ð´ÑÑ Ð¸Ð½Ð²Ð°Ð»Ð¸Ð´Ð¾Ð² Ð¸ Ð¸Ñ ÑÑÑÐ´Ð¾ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð°, ÑÐ¿ÐµÑÐ¸ÑÐ¸ÐºÐ° ÑÐ°ÐºÐ¸Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼ Ð² ÑÐ¿Ð¾ÑÑÐµ, Ð¼Ð¾ÑÐ¸Ð²Ð°ÑÐ¸Ñ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¹ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð°Ð´Ð°Ð¿ÑÐ¸Ð²Ð½Ð¾Ð¹ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð¹ ÐºÑÐ»ÑÑÑÑÑ. ÐÑÐ¸Ð²Ð¾Ð´ÑÑÑÑ Ð¿ÑÐ¸Ð¼ÐµÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ¾Ðº Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¹ Ð¾ÑÐ¸ÐµÐ½ÑÐ°ÑÐ¸Ð¸ ÑÐ¿Ð¾ÑÑÑÐ¼ÐµÐ½Ð¾Ð²âÐ¸Ð½Ð²Ð°Ð»Ð¸Ð´Ð¾Ð², Ð½Ð°Ð¼ÐµÑÐ°ÑÑÑÑ Ð¿ÑÑÐ¸ Ð¸Ñ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ.
description: The problems of professional selfâdetermination of disabled athletes after the end of the performance period are considered. The problems of career guidance of young disabled people and their employment are analyzed. The article considers the specifics of the problems of building a sports career for disabled people, and the motivation of education in the field of adaptive physical culture. Examples of developments in the field of professional orientation of disabled athletes are discussed. The directions of development improvement are considered.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÐºÐ°Ð´ÑÐ¾Ð²Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸ Ð¸ Ð¸Ñ Ð¾ÑÐµÐ½ÐºÐ° (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÐÐÐ Â«ÐÐ¦ Â«ÐÑÐµÐ½Ð¸ÐµÂ»)
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
Creators: name: ÐÐµÑÐµÑÐºÐ¾Ð²Ð°, ÐÐ°ÑÐ¸Ñ
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: 2018
Subjects: ÐºÐ°Ð´ÑÐ¾Ð²Ð°Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ°
ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼
Ð¾ÑÑÐ°Ð»ÑÐ¼Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÑÐ»ÑÐ³Ð¸
Ð¿ÐµÑÑÐ¾Ð½Ð°Ð» Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ

description: Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÐºÐ°Ð´ÑÐ¾Ð²Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸ Ð¸ Ð¸Ñ Ð¾ÑÐµÐ½ÐºÐ° Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÐÐÐ Â«ÐÐ¦ Â«ÐÑÐµÐ½Ð¸ÐµÂ». Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð´Ð²Ð° Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸ ÐºÐ°Ð´ÑÐ¾Ð²: Ð½Ð°Ð¹Ð¼ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¼ÐµÐ½ÐµÐ´Ð¶ÐµÑÐ° Ð¿Ð¾ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ñ; Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ðµ Ð¾Ð±ÑÑÐµÐ½Ð¸Ðµ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÐºÐ¾Ð².
The Multiplication Formulas of Weighted Quantum Cluster Functions
Creators: name: Chen, Zhimin
name: Xiao, Jie
name: Xu, Fan
Publisher: name: arXiv
Year: 2021
Subjects: subject: Quantum Algebra (math.QA)
subject: Representation Theory (math.RT)
subject: FOS: Mathematics

description: By applying the property of Ext-symmetry and the affine space structure of certain fibers, we introduce the notion of weighted quantum cluster functions and prove their multiplication formulas associated to abelian categories with Ext-symmetry and 2-Calabi-Yau triangulated categories with cluster-tilting objects.
A multi-wavelength survey of AGN in the XMM-LSS field: I. Quasar selection via the KX technique
Creators: name: Nakos, Th.
name: Willis, J. P.
name: Andreon, S.
name: Surdej, J.
name: Riaud, P.
name: Hatziminaoglou, E.
name: Garcet, O.
name: Alloin, D.
name: Baes, M.
name: Galaz, G.
name: Pierre, M.
name: Quintana, H.
name: Page, M. J.
name: Tedds, J. A.
name: Ceballos, M. T.
name: Corral, A.
name: Ebrero, J.
name: Krumpe, M.
name: Mateos, S.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: AIMS: We present a sample of candidate quasars selected using the KX-technique. The data cover 0.68 deg^2 of the X-ray Multi-Mirror (XMM) Large-Scale Structure (LSS) survey area where overlapping multi-wavelength imaging data permits an investigation of the physical nature of selected sources. METHODS: The KX method identifies quasars on the basis of their optical (R and z') to near-infrared (Ks) photometry and point-like morphology. We combine these data with optical (u*,g'r',i',z') and mid-infrared (3.6-24 micron) wavebands to reconstruct the spectral energy distributions (SEDs) of candidate quasars. RESULTS: Of 93 sources selected as candidate quasars by the KX method, 25 are classified as quasars by the subsequent SED analysis. Spectroscopic observations are available for 12/25 of these sources and confirm the quasar hypothesis in each case. Even more, 90% of the SED-classified quasars show X-ray emission, a property not shared by any of the false candidates in the KX-selected sample. Applying a photometric redshift analysis to the sources without spectroscopy indicates that the 25 sources classified as quasars occupy the interval 0.7 < z < 2.5. The remaining 68/93 sources are classified as stars and unresolved galaxies.
description: 13 pages, 9 figures, A&A 494, p. 579-589. Replaced with published version. Fig. 9 in first astro-ph submission has been updated
Entrepreneurship Education-Educating for Life-LongSustainable and Functional Skills-19-Nov-201912-06-051.pdf
Creators: name: Aglazor, Genevieve
Publisher: name: figshare
Year: 2022
Subjects: Education

description: The centrality of education to training and development of human resources in any society is indisputable. However, the type and content of education could be debatable. In the context of human resources, the focus is a broad knowledge base; unique skills, capacities, and global oriented which when effectively harnessed can transform people, communities, businesses, consequently nations. Entrepreneurship education has the potential to reduce national poverty levels by sustaining individuals and families as well as fostering national development. This paper’s content is geared towards educating for life-long sustainable and functional entrepreneurship skills. It is believed that with appropriate entrepreneurship education, Nigeria has the potential to join other developing nations in the global economic drive.
Constraining exotic compact stars composed of bosonic and fermionic dark matter with gravitational wave events
Creators: name: Wystub, Stephan
name: Dengler, Yannick
name: Christian, Jan-Erik
name: Schaffner-Bielich, Jürgen
Publisher: name: arXiv
Year: 2021
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We investigate neutron star-black hole (NS-BH) merger candidates as a test for compact exotic objects. Using the events GW190814, GW200105 and GW200115 measured by the LIGO-Virgo collabration, which represent a broad profile of the masses in the NS mass spectrum, we demonstrate the constraining power for the parameter spaces of compact stars consisting of dark matter for future measurements. We consider three possible cases of dark matter stars: self-interacting, purely bosonic or fermionic dark matter stars, stars consisting of a mixture of interacting bosonic and fermionic matter, as well as the limiting case of selfbound stars. We find that the scale of those hypothetical objects are dominated by the one of the strong interaction. The presence of fermionic dark matter requires a dark matter particle of the GeV mass scale, while the bosonic dark matter particle mass can be arbitrarily large or small. In the limiting case of a selfbound linear equation of state, we find that the vacuum energy of those configurations has to be similar to the one of QCD.
description: 6 pages, 4 figures, 3 tables. In accordance with the CRC-TR 211 Data Management Policy, the research data for section 1 and 4 of this study are available as ancilliary files, while the research data of section 3 is made available under http://cloud.itp.uni-frankfurt.de/s/QYARcPkmqKW5ain
title: ÐÑÐ¸Ð½ÑÐ¸Ð¿Ñ Ð¼Ð¸ÐºÑÐ¾ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ¸. Ð§. 1
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: Ð¡ÐµÐ¹ÑÑÐ½, Ð ÑÐ±ÐµÐ½
Publisher: name: [ÐÐÐ¢Ð£]
Year: 1991
Subjects: ÐÐ¸ÐºÑÐ¾ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ°

description: Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ ÑÐ·Ð»Ð¾Ð²ÑÐµ Ð¸Ð´ÐµÐ¸, Ð»ÐµÐ¶Ð°ÑÐ¸Ðµ Ð² Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ð¸Ñ Ð¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¼Ð¸ÐºÑÐ¾ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ¸, Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÑÑÑÑÑ ÑÐ²Ð»ÐµÐ½Ð¸Ñ, ÑÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð¶Ð´Ð°ÑÑÐ¸Ðµ ÐµÐµ Ð¿ÑÐ¾Ð³ÑÐµÑÑ ; Ð·Ð°ÐºÐ»Ð°Ð´ÑÐ²Ð°ÐµÑÑÑ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ°Ñ Ð±Ð°Ð·Ð° Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ Ð²Ð°Ð¶Ð½ÑÑ ÑÑÑÐµÐºÑÐ¾Ð² Ð¼Ð¸ÐºÑÐ¾ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ¸ Ð¸ Ð»ÐµÐ¶Ð°ÑÐµÐ³Ð¾ Ð² ÐµÐµ Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¸Ð½ÑÐµÐ³ÑÐ°Ð»ÑÐ½Ð¾-Ð³ÑÑÐ¿Ð¿Ð¾Ð²Ð¾Ð³Ð¾ Ð¼ÐµÑÐ¾Ð´Ð° Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð° - ÑÐ°ÐºÐ¸Ñ, ÐºÐ°Ðº Ð¸Ð½ÑÐµÐ³ÑÐ°Ð»ÑÐ½Ð°Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ, Ð½Ð°Ð´ÐµÐ¶Ð½Ð¾ÑÑÑ, Ð¼Ð¸Ð½Ð¸Ð°ÑÑÑÐ¸Ð·Ð°ÑÐ¸Ñ, Ð² Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÐ¸ Ð¾Ñ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ Ð¸Ð½ÑÐµÐ³ÑÐ°Ð»ÑÐ½Ð¾Ð¹ ÑÑÐµÐ¼Ñ Ð¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ°, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¸Ñ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ Ð½Ð° Ð¼Ð¸ÐºÑÐ¾ÑÑÐµÐ¼Ð¾- Ð¸ ÑÐ¸ÑÑÐµÐ¼Ð¾ÑÐµÑÐ½Ð¸ÐºÑ. ÐÐ½Ð°Ð»Ð¸Ð·Ð¸ÑÑÐµÑÑÑ Ð²ÑÑÐ¾Ð´ Ð¼Ð¸ÐºÑÐ¾ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÑ ÑÑÑÑÐºÑÑÑ Ð¸ Ð¿Ð¾Ð´ÑÐ¾Ð´Ñ Ðº Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ Ð¸Ð½ÑÐµÐ³ÑÐ°Ð»ÑÐ½ÑÑ ÑÑÐµÐ¼. ÐÑÐ¸Ð³Ð¸Ð½Ð°Ð»ÑÐ½ÑÐµ Ð²ÑÐ²Ð¾Ð´Ñ Ð¸ Ð¾Ð±Ð¾Ð±ÑÐµÐ½Ð¸Ñ, Ð°Ð½Ð°Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ¾ÑÐ¼ÑÐ»Ñ, Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÐµ Ð² ÑÐ°Ð±Ð¾ÑÐµ, Ð¿ÑÐ¾Ð²ÐµÑÐµÐ½Ñ Ð² Ð¿ÑÐ¾ÑÐµÑÑÐµ Ð½Ð°ÑÑÐ½ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ¾Ðº Ð½Ð° Ð¾Ð´Ð½Ð¾Ð¼ Ð¸Ð· Ð½Ð°ÑÑÐ½Ð¾-Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½ÑÑ Ð¾Ð±ÑÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ð¹. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐ°ÐµÑÑÑ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÐ°Ð´Ð¸Ð¾ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¸Ñ,ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹ Ð¸ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¿Ð¾Ð»ÐµÐ·Ð½Ð¾ ÑÐ¸ÑÐ¾ÐºÐ¾Ð¼Ñ ÐºÑÑÐ³Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð², ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÑ Ñ ÑÐ°ÑÑÐµÑÐ¾Ð¼ Ð¸ ÐºÐ¾Ð½ÑÑÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð¸Ð½ÑÐµÐ³ÑÐ°Ð»ÑÐ½ÑÑ ÑÑÐµÐ¼ Ð¸ ÑÐ°Ð´Ð¸Ð¾ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð¾Ð¹ Ð°Ð¿Ð¿Ð°ÑÐ°ÑÑÑÑ Ñ Ð¸Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼.
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ð¹ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° ÐÐµÐ½Ð¸Ð½Ð³ÑÐ°Ð´ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
title: ÐÑÑ Ð³Ð°Ð»ÑÐµÑÑÐºÐ¸Ð¹ ÑÑÐµÑ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÑÑÑÐ¾ÑÐºÐ¸Ð½Ð°, ÐÑÐ±Ð¾Ð²Ñ
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2010
Subjects: Ð±ÑÑ Ð³Ð°Ð»ÑÐµÑÑÐºÐ¸Ð¹ ÑÑÐµÑ
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ñ ÑÐµÐ´ÐµÑÐ°Ð»ÑÐ½Ð¾Ð¹ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ Ð¡Ð 04 Â«ÐÑÑÐ³Ð°Ð»ÑÐµÑÑÐºÐ¸Ð¹ ÑÑÐµÑÂ» Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ° Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ 080500.62 Â«ÐÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÂ» Ð¸ 0880100.62 Â«Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ°Â». Ð¡Ð¾Ð´ÐµÑÐ¶Ð¸Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð¾ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐ¼ ÑÐµÐ¼Ð°Ð¼ Ð¸Ð·ÑÑÐ°ÐµÐ¼Ð¾Ð¹ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ. ÐÐ°Ð½Ð½ÑÐ¹ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð» Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ñ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ Ð¾Ð²Ð»Ð°Ð´ÐµÑÑ Ð¼ÐµÑÐ¾Ð´Ð¾Ð»Ð¾Ð³Ð¸ÐµÐ¹ Ð±ÑÑÐ³Ð°Ð»ÑÐµÑÑÐºÐ¾Ð³Ð¾ Ð¾ÑÑÐ°Ð¶ÐµÐ½Ð¸Ñ ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸, Ð¿ÑÐ¸Ð¾Ð±ÑÐµÑÑÐ¸ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð½Ð°Ð²ÑÐºÐ¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¸Ðº ÑÑÐµÑÐ° Ð°ÐºÑÐ¸Ð²Ð¾Ð² Ð¸ Ð¿Ð°ÑÑÐ¸Ð²Ð¾Ð² Ð² Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÐÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð¹ Ð²ÑÑÑÐµÐ¹ ÑÐºÐ¾Ð»Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ, Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ñ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ Â«ÐÑÑÐ³Ð°Ð»ÑÐµÑÑÐºÐ¸Ð¹ ÑÑÐµÑÂ», Ð° ÑÐ°ÐºÐ¶Ðµ Ð´Ð»Ñ ÑÐ»ÑÑÐ°ÑÐµÐ»ÐµÐ¹ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð²ÑÑÑÐµÐ³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ.
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
Automated Damage Inspection of Power Transmission Towers from UAV Images
Creators: name: Barreiro, Aleixo Cambeiro
name: Seibold, Clemens
name: Hilsmann, Anna
name: Eisert, Peter
Publisher: name: arXiv
Year: 2021
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: Infrastructure inspection is a very costly task, requiring technicians to access remote or hard-to-reach places. This is the case for power transmission towers, which are sparsely located and require trained workers to climb them to search for damages. Recently, the use of drones or helicopters for remote recording is increasing in the industry, sparing the technicians this perilous task. This, however, leaves the problem of analyzing big amounts of images, which has great potential for automation. This is a challenging task for several reasons. First, the lack of freely available training data and the difficulty to collect it complicate this problem. Additionally, the boundaries of what constitutes a damage are fuzzy, introducing a degree of subjectivity in the labelling of the data. The unbalanced class distribution in the images also plays a role in increasing the difficulty of the task. This paper tackles the problem of structural damage detection in transmission towers, addressing these issues. Our main contributions are the development of a system for damage detection on remotely acquired drone images, applying techniques to overcome the issue of data scarcity and ambiguity, as well as the evaluation of the viability of such an approach to solve this particular problem.
description: 8 pages, 10 figures, accepted for VISAPP 2022
Neural Weight Step Video Compression
Creators: name: Czerkawski, Mikolaj
name: Cardona, Javier
name: Atkinson, Robert
name: Michie, Craig
name: Andonovic, Ivan
name: Clemente, Carmine
name: Tachtatzis, Christos
Publisher: name: arXiv
Year: 2021
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Graphics (cs.GR)
subject: FOS: Computer and information sciences

description: A variety of compression methods based on encoding images as weights of a neural network have been recently proposed. Yet, the potential of similar approaches for video compression remains unexplored. In this work, we suggest a set of experiments for testing the feasibility of compressing video using two architectural paradigms, coordinate-based MLP (CbMLP) and convolutional network. Furthermore, we propose a novel technique of neural weight stepping, where subsequent frames of a video are encoded as low-entropy parameter updates. To assess the feasibility of the considered approaches, we will test the video compression performance on several high-resolution video datasets and compare against existing conventional and neural compression techniques.
description: Accepted to the pre-registration workshop at NeurIPS 2021
Non connective K-theory via universal invariants
Creators: name: Cisinski, Denis-Charles
name: Tabuada, Goncalo
Publisher: name: arXiv
Year: 2009
Subjects: subject: K-Theory and Homology (math.KT)
subject: Category Theory (math.CT)
subject: FOS: Mathematics

description: In this article, we further the study of higher K-theory of dg categories via universal invariants, initiated by the second named author. Our main result is the co-representability of non-connective K-theory by the base ring in the universal localizing motivator. As an application, we obtain for free higher Chern characters, resp. higher trace maps, e.g. from non-connective K-theory to cyclic homology, resp. to topological Hochschild homology.
description: This is a slight revision in the exposition of the paper previously entitled "Negative K-theory via universal invariants"; hopefully for the best
Cosmic Cartography of the Large-Scale Structure with Sloan Digital Sky Survey Data Release 6
Creators: name: Kitaura, Francisco S.
name: Jasche, Jens
name: Li, Cheng
name: Ensslin, Torsten A.
name: Metcalf, R. Benton
name: Wandelt, Benjamin D.
name: Lemson, Gerard
name: White, Simon D. M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present the largest Wiener reconstruction of the cosmic density field made to date. The reconstruction is based on the Sloan Digital Sky Survey data release 6 covering the northern Galactic cap. We use a novel supersampling algorithm to suppress aliasing effects and a Krylov-space inversion method to enable high performance with high resolution. These techniques are implemented in the ARGO computer code. We reconstruct the field over a 500 Mpc cube with Mpc grid-resolution while accounting both for the angular and radial selection functions of the SDSS, and the shot noise giving an effective resolution of the order of ~10 Mpc. In addition, we correct for the redshift distortions in the linear and nonlinear regimes in an approximate way. We show that the commonly used method of inverse weighting the galaxies by the corresponding selection function heads to excess noise in regions where the density of the observed galaxies is small. It is more accurate and conservative to adopt a Bayesian framework in which we model the galaxy selection/detection process to be Poisson-binomial. This results in heavier smoothing in regions of reduced sampling density. Our results show a complex cosmic web structure with huge void regions indicating that the recovered matter distribution is highly non-Gaussian. Filamentary structures are clearly visible on scales up to ~20 Mpc. We also calculate the statistical distribution of density after smoothing the reconstruction with Gaussian kernels of different radii r_S and find good agreement with a log-normal distribution for ~10 Mpc < r_S < ~30 Mpc.
description: 24 pages, 12 figures, 2 tables
Discrete-modulation continuous-variable quantum key distribution with high key rate
Creators: name: Wang, Pu
name: Liu, Jianqiang
name: Lu, Zhenguo
name: Wang, Xuyang
name: Li, Yongmin
Publisher: name: arXiv
Year: 2021
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Discrete-modulation continuous-variable quantum key distribution has the potential for large-scale deployment in the secure quantum communication networks due to low implementation complexity and compatibility with the current telecom systems. The security proof for four coherent states phase-shift keying (4-PSK) protocol has recently been established by applying numerical methods. However, the achievable key rate is relatively low compared with the optimal Gaussian modulation scheme. To enhance the key rate of discrete-modulation protocol, we first show that 8-PSK increases the key rate by about 60\% in comparison to 4-PSK, whereas the key rate has no significant improvement from 8-PSK to 12-PSK. We then expand the 12-PSK to two-ring constellation structure with four states in the inner ring and eight states in the outer ring, which significantly improves the key rate to be 2.4 times of that of 4-PSK. The key rate of the two-ring constellation structure can reach 70\% of the key rate achieved by Gaussian modulation in long distance transmissions, making this protocol an attractive alternative for high-rate and low-cost application in secure quantum communication networks.
description: Welcome comments
Mechanisms for Relaxin’s Modulation of MMPs and Matrix Loss in Fibrocartilages
Creators: name: Kapila, Sunil
name: Park, Young
name: Ahmad, Nisar
name: Hosomichi, Jun
name: Hayami, Takayuki
name: Tacon, Claire
Publisher: name: Italian Journal of Anatomy and Embryology
Year: 2014

description: Italian Journal of Anatomy and Embryology, Vol 118, No 1 (Supplement) 2013
Bona-fide, strong-variable galactic Luminous Blue Variable stars are fast rotators: detection of a high rotational velocity in HR Carinae
Creators: name: Groh, Jose H.
name: Damineli, Augusto
name: Hillier, D. John
name: Barba, Rodolfo
name: Fernandez-Lajus, Eduardo
name: Gamen, Roberto C.
name: Moises, Alessandro
name: Solivella, Gladys
name: Teodoro, Mairan
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We report optical observations of the Luminous Blue Variable (LBV) HR Carinae which show that the star has reached a visual minimum phase in 2009. More importantly, we detected absorptions due to Si IV 4088-4116 Angstroms. To match their observed line profiles from 2009 May, a high rotational velocity of vrot=150 +- 20 km/s is needed (assuming an inclination angle of 30 degrees), implying that HR Car rotates at ~0.88 +- 0.2 of its critical velocity for break-up (vcrit). Our results suggest that fast rotation is typical in all strong-variable, bona-fide galactic LBVs, which present S Dor-type variability. Strong-variable LBVs are located in a well-defined region of the HR diagram during visual minimum (the "LBV minimum instability strip"). We suggest this region corresponds to where vcrit is reached. To the left of this strip, a forbidden zone with vrot/vcrit>1 is present, explaining why no LBVs are detected in this zone. Since dormant/ex LBVs like P Cygni and HD 168625 have low vrot, we propose that LBVs can be separated in two groups: fast-rotating, strong-variable stars showing S-Dor cycles (such as AG Car and HR Car) and slow-rotating stars with much less variability (such as P Cygni and HD 168625). We speculate that SN progenitors which had S-Dor cycles before exploding (such as in SN 2001ig, SN 2003bg, and SN 2005gj) could have been fast rotators. We suggest that the potential difficulty of fast-rotating Galactic LBVs to lose angular momentum is an additional evidence that such stars could explode during the LBV phase.
description: 6 pages, 4 figures, accepted for publication in ApJ Letters ; uses emulateapj.cls