cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Una torre esagonale nel cielo di Saturno
Creators: Maura Sandri
Publisher: name: Media Inaf
Year: 2018

Un nuovo studio ha individuato quelli che sembrerebbero essere i primi scorci di un vortice al polo nord di Saturno che si è formato nella parte alta dell'atmosfera, mentre nell'emisfero settentrionale si stava avvicinando l'estate. Questo caldo vortice si trova a centinaia di chilometri al di sopra delle nuvole, in uno strato di atmosfera conosciuto come stratosfera e sembra molto simile al famoso esagono sottostante, come se in realtà fosse un’unica struttura che si sviluppa in altezza.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¸ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð° ÑÐ¸Ð½ÑÐµÐ·Ð° ÑÐ¸ÑÑÐµÐ¼ Ð¿ÐµÑÐµÑ Ð¾Ð´Ð¾Ð² Ð´Ð»Ñ GR(1)âÑÐ¾ÑÐ¼ÑÐ» Ð¿ÑÐ¸ Ð¿Ð¾Ð¼Ð¾ÑÐ¸ BDD
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
Creators: name: ÐÑÑÐ¸Ð¿Ð¾Ð², Ð¢Ð¸Ð¼Ð¾Ñ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: 2018
Subjects: ÐÐ»Ð³Ð¾ÑÐ¸ÑÐ¼Ñ
ÐÐ¾Ð½ÑÑÐ¾Ð»Ð»ÐµÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½ÑÐµ
ÐÐ²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ
ÑÐµÐ°Ð³Ð¸ÑÑÑÑÐ¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ
ÑÐ¸Ð¼Ð²Ð¾Ð»ÑÐ½ÑÐµ Ð²ÑÑÐ¸ÑÐ»ÐµÐ½Ð¸Ñ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ Ð·Ð°Ð´Ð°ÑÐ° ÑÐ¸Ð½ÑÐµÐ·Ð° ÐºÐ¾Ð½ÑÑÐ¾Ð»Ð»ÐµÑÐ° Ð´Ð»Ñ
ÑÐµÐ°Ð³Ð¸ÑÑÑÑÐµÐ¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¿Ð¾ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸ÑÐ¼, Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÐ¼ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ
Ð¿Ð¾Ð´ÐºÐ»Ð°ÑÑÐ° LTL-ÑÐ¾ÑÐ¼ÑÐ» - GR(1)-ÑÐ¾ÑÐ¼ÑÐ». Ð¡Ð¸Ð½ÑÐµÐ· Ð¾ÑÐ½Ð¾Ð²ÑÐ²Ð°ÐµÑÑÑ Ð½Ð° ÑÐ¸Ð¼Ð²Ð¾Ð»ÑÐ½Ð¾Ð¼ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ðµ, Ð¾Ð¿Ð¸ÑÐ°Ð½Ð½Ð¾Ð¼ Ð² ÑÐ°Ð±Ð¾ÑÐµ. Ð¡Ð¸Ð¼Ð²Ð¾Ð»ÑÐ½Ð°Ñ Ð·Ð°Ð¿Ð¸ÑÑ ÑÑÐ°Ð½Ð¸ÑÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾ Ð² Ð²Ð¸Ð´Ðµ BDD.
ÐÑÐ¸ Ð·Ð°Ð´Ð°Ð½Ð½ÑÑ Ð¿Ð¾Ð²ÐµÐ´ÐµÐ½Ð¸ÑÑ ÑÑÐµÐ´Ñ Ð¸ ÑÐµÐ°Ð³Ð¸ÑÑÑÑÐµÐ¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¸ Ð²ÑÐ¸Ð³ÑÑÑÐ½Ð¾Ð¼ ÑÑÐ»Ð¾Ð²Ð¸Ð¸, Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð½Ð¾Ð¼ Ð² Ð²Ð¸Ð´Ðµ GR(1)-ÑÐ¾ÑÐ¼ÑÐ», Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÑÑ Ð²ÑÑÐ¸ÑÐ»ÐµÐ½Ð¸Ðµ Ð²ÑÐ¸Ð³ÑÑÑÐ½Ð¾Ð³Ð¾ ÑÐµÐ³Ð¸Ð¾Ð½Ð° Ð¸ ÑÐ¸Ð½ÑÐµÐ· ÑÐ¾Ð²Ð¼ÐµÑÑÐ½Ð¾Ð³Ð¾ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ð»ÐµÑÐ°, ÑÐ´Ð¾Ð²Ð»ÐµÑÐ²Ð¾ÑÑÑÑÐµÐ³Ð¾ Ð·Ð°Ð´Ð°Ð½Ð½ÑÐ¼ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸ÑÐ¼.
ÐÐ»Ñ ÑÐ¼ÐµÐ½ÑÑÐµÐ½Ð¸Ñ ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²Ð° ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ð¹ ÑÐ¸Ð½ÑÐµÐ·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ð»ÐµÑÐ° Ðº Ð¼Ð¾Ð´ÐµÐ»Ð¸ ÐµÐ³Ð¾ Ð¿Ð¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¿ÑÐ¸Ð¼ÐµÐ½ÑÐµÑÑÑ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼ Ð¼Ð¸Ð½Ð¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸. ÐÐ¾ÑÐ»Ðµ ÑÑÐ¾Ð¹ Ð¼Ð¸Ð½Ð¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ ÑÑÐ°Ð½ÑÐ»Ð¸ÑÑÐµÑÑÑ Ð² ÑÐ¾ÑÐ¼Ð°Ñ DOT Ð´Ð»Ñ ÐµÑ Ð¿Ð¾ÑÐ»ÐµÐ´ÑÑÑÐµÐ¹ Ð²Ð¸Ð·ÑÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸.
Discovery of photospheric CaX emission lines in the far-UV spectrum of the hottest known white dwarf (KPD0005+5106)
Creators: name: Werner, K.
name: Rauch, T.
name: Kruk, J. W.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: For the first time, we have identified photospheric emission lines in the far-UV spectrum of a white dwarf. They were discovered in the Far Ultraviolet Spectroscopic Explorer spectrum of the hot (Teff~200,000 K) DO white dwarf KPD0005+5106 and they stem from extremely highly ionized calcium (CaX 1137, 1159 Ang). Their photospheric origin is confirmed by non-LTE line-formation calculations. This is the highest ionisation stage of any element ever observed in a stellar photosphere. Calcium has never been detected before in any hot white dwarf or central star of planetary nebula. The calcium abundance determination for KPD0005+5106 (1-10 times solar) is difficult, because the line strengths are rather sensitive to current uncertainties in the knowledge of effective temperature and surface gravity. We discuss the possibility that the calcium abundance is much lower than expected from diffusion/levitation equilibrium theory. The same emission lines are exhibited by the [WCE]-type central star NGC2371. Another CaX line pair (1461, 1504 Ang) is probably present in a Hubble Space Telescope spectrum of the PG1159-type central star NGC246.
description: Accepted for publication in A&A Letters
Associated production of charged Higgs and top at LHC: the role of the complete electroweak supersymmetric contribution
Creators: name: Beccaria, M.
name: Macorini, G.
name: Panizzi, L.
name: Renard, F. M.
name: Verzegnassi, C.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The process of charged Higgs production in association with a top quark at the LHC has been calculated at the complete NLO electroweak level both in a Two Higgs Doublets Model and in the Minimal Supersymmetric Standard Model, assuming a mSUGRA breaking scheme. We have numerically explored the size of the one-loop corrections in two typical supersymmetric scenarios, with particular attention to the tan beta dependence, and we have found that they remain perturbatively small but possibly sizable, reaching a 20% limit for extreme values of tan beta, when the complete set of Feynman diagrams is taken into account.
description: 22 pages, 5 figures, reference added
Impact of Employment Concentration in High-tech Industries on Income Inequality
Creators: name: Lei, Feihong
Publisher: name: University of Chicago
Year: 2023
Subjects: subject: income inequality
subject: employment concentration
subject: high-tech industry

description: In this study, we investigated the relationship between income inequality and high-tech employment in developed and developing nations using time-series and cross-sectional data from various sources. Our empirical analysis revealed a negative relationship between high-tech employment share and income inequality, with varying impacts across manufacturing and non-manufacturing sectors. Additionally, utilizing a hierarchical clustering algorithm, we categorized sample countries into two groups based on five parameters representing different levels of economic development. Our empirical findings reveal that the impact of high-tech industry concentration on income inequality is not significant in emerging economies. However, in advanced economies, the observed pattern remains consistent with that found in the overall sample.
Supernove, lo shock è nascosto sotto al velo
Creators: Francesca Aloisio
Publisher: name: Media Inaf
Year: 2018

Uno studio firmato, tra gli altri, anche da Filomena Bufano dell’Inaf di Catania dimostra come lo ‘shock breakout’ – quel breve lampo di luce che ci si aspettava di osservare quando esplode una supergigante rossa – sia in realtà un fenomeno raro in natura. La ragione va ricercata nella densità del materiale circumstellare, molto maggiore di quanto i modelli prevedessero
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ° Ð´Ð»Ñ ÑÐ»ÑÐ¶Ð±Ñ Ð³Ð»Ð°Ð²Ð½Ð¾Ð³Ð¾ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð° Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð¾ÑÐµÐ½Ð¾Ðº
title: Development of the information complex for the department of the main technologist with using of information assessments
Creators: name: Ð¡ÑÐ´Ð°ÐºÐ¾Ð²Ð°, ÐÐ¸Ð´Ð¸Ñ
name: ÐÐ¸ÑÐµÐ½ÐºÐ¾Ð²Ð°, ÐÐºÑÐ°Ð½Ð°
name: Ð§ÐµÑÐ½ÐµÐ½ÑÐºÐ°Ñ , ÐÑÐ´Ð¼Ð¸Ð»Ð°
name: "Ð¡Ð¸ÑÑÐµÐ¼Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð² Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¸", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð°Ñ Ð½Ð°ÑÑÐ½Ð°Ñ Ð¸ ÑÑÐµÐ±Ð½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (24; 2020; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2020
Subjects: ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ

description: Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ Ð·Ð°Ð´Ð°ÑÐ° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ°
Ð´Ð»Ñ Ð¡Ð»ÑÐ¶Ð±Ñ Ð³Ð»Ð°Ð²Ð½Ð¾Ð³Ð¾ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. ÐÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÑÑ Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð·Ð°Ð´Ð°ÑÐ¸ ÑÐ²Ð»ÑÐµÑÑÑ
Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÑ Ð¾ÑÐµÐ½ÐºÐ¸ Ð²ÐµÑÐ¾ÑÑÐ½Ð¾ÑÑÐ¸ Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ñ ÑÐµÐ»Ð¸ ÑÑÑÐµÑÑÐ²ÑÑÑÐµÐ³Ð¾ Ð¸ Ð¿ÑÐµÐ´Ð»Ð°Ð³Ð°ÐµÐ¼Ð¾Ð³Ð¾ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ¾Ð². Ð¦ÐµÐ»ÑÑ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ°, ÑÐ´Ð¾Ð²Ð»ÐµÑÐ²Ð¾ÑÑÑÑÐµÐ³Ð¾ ÑÐµÐ»ÑÐ¼ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÐºÐ¾Ð² Ñ ÑÑÐµÑÐ¾Ð¼ Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð¸Ð¹, Ð½Ð°ÐºÐ»Ð°Ð´ÑÐ²Ð°ÐµÐ¼ÑÑ Ð½Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÑ. Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ ÑÐ¾ÑÑÐ°Ð² Ð½Ð¾Ð²Ð¾Ð¹
Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð´Ð»Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° ÐµÐµ Ð¾ÑÐµÐ½ÐºÐ°.
description: The problem of the development of the Information complex for the department of the Main technologist of the enterprise is considered. A peculiarity of the
problem formulation is the necessity for estimation of the probability of achieving the goal
by existing and proposed information systems. The purpose of the work is to develop an
Information complex that meets the goals of employees, taking into account the restrictions
imposed on the development. As a result, the structure of the new information system of the
enterprise is presented and its assessment is carried out.
Fountain Codes Based Distributed Storage Algorithms for Large-scale Wireless Sensor Networks
Creators: name: Aly, Salah A.
name: Kong, Zhenning
name: Soljanin, Emina
Publisher: name: arXiv
Year: 2009
Subjects: subject: Information Theory (cs.IT)
subject: Data Structures and Algorithms (cs.DS)
subject: Networking and Internet Architecture (cs.NI)
subject: FOS: Computer and information sciences

description: We consider large-scale sensor networks with n nodes, out of which k are in possession, (e.g., have sensed or collected in some other way) k information packets. In the scenarios in which network nodes are vulnerable because of, for example, limited energy or a hostile environment, it is desirable to disseminate the acquired information throughout the network so that each of the n nodes stores one (possibly coded) packet and the original k source packets can be recovered later in a computationally simple way from any (1 + ε)k nodes for some small ε> 0. We developed two distributed algorithms for solving this problem based on simple random walks and Fountain codes. Unlike all previously developed schemes, our solution is truly distributed, that is, nodes do not know n, k or connectivity in the network, except in their own neighborhoods, and they do not maintain any routing tables. In the first algorithm, all the sensors have the knowledge of n and k. In the second algorithm, each sensor estimates these parameters through the random walk dissemination. We present analysis of the communication/transmission and encoding/decoding complexity of these two algorithms, and provide extensive simulation results as well
description: A method to estimate the total number of nodes in a graph is presented in this 12 pages
Additional file 2 of Men’s sheds as community-based health promotion for men aged 50 plus: protocol for a mixed-methods systematic review
Creators: name: Albrecht, Birte Marie
name: Foettinger, Linda
name: Bammann, Karin
Publisher: name: figshare
Year: 2021
Subjects: subject: Space Science
subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Science Policy

description: Additional file 2: Piloted search strategy
Iau, nel 2024 per la prima volta in Africa
Creators: Sara Venturi
Publisher: name: Media Inaf
Year: 2018

L’International Astronomical Union (Iau) ha annunciato che la 32esima Assemblea generale, nel 2024, sarà ospitata – per la prima volta dal 1919, anno di fondazione dell’Unione – nel continente africano, in Sud Africa. Con un commento di Pierguido Sarti, addetto scientifico all’ambasciata italiana a Pretoria
title: Ð¢ÑÐ°Ð½ÑÐ³ÑÐ°Ð½Ð¸ÑÐ½Ð¾Ðµ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÑÐµÑÑÐ²Ð¾ Ð² ÑÑÐµÑÐµ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ð¹ Ð¼ÐµÐ¶Ð´Ñ Ð¿ÑÐ¾Ð²Ð¸Ð½ÑÐ¸ÐµÐ¹ Ð¥ÑÐ¹Ð»ÑÐ½ÑÐ·ÑÐ½ Ð¸ ÐÐ¼ÑÑÑÐºÐ¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑ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¤Ð¸Ð»Ð°ÑÐ¾Ð², ÐÐ°Ð½Ð¸Ð¸Ð»
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: 2016
Subjects: ÐÐ¼ÑÑÑÐºÐ°Ñ Ð¾Ð±Ð»Ð°ÑÑÑ (ÐÐ°Ð»ÑÐ½Ð¸Ð¹ ÐÐ¾ÑÑÐ¾Ðº Ð Ð¾ÑÑÐ¸Ð¸)
ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¾-ÐºÐ¸ÑÐ°Ð¹ÑÐºÐ¾Ðµ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÑÐµÑÑÐ²Ð¾
Ð²Ð½ÐµÑÐ½ÑÑ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ñ
Russian-Chinese cooperation
foreign trade

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð±ÑÐ» ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½ Ð¸ÑÑÐ¾ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÑÑ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÑÐ°Ð½ÑÐ³ÑÐ°Ð½Ð¸ÑÐ½Ð¾Ð³Ð¾ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÑÐµÑÑÐ²Ð° ÑÐµÐ³Ð¸Ð¾Ð½Ð¾Ð², ÐºÐ°Ðº ÑÐ°ÑÑÐ¸ Ð¸ÑÑÐ¾ÑÐ¸Ð¸ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ð¹ Ð Ð¾ÑÑÐ¸Ð¸ Ð¸ ÐÐ¸ÑÐ°Ñ, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿ÑÐ°Ð²Ð¾Ð²ÑÑ Ð¾ÑÐ½Ð¾Ð² Ð¿ÑÐ¸Ð³ÑÐ°Ð½Ð¸ÑÐ½Ð¾Ð³Ð¾ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÑÐµÑÑÐ²Ð°, Ð¾Ð±Ð¾Ð·Ð½Ð°ÑÐµÐ½Ñ Ð¼ÐµÑÑÐ¾ Ð¸ ÑÐ¾Ð»Ñ Ð¿ÑÐ¸Ð³ÑÐ°Ð½Ð¸ÑÐ½Ð¾Ð³Ð¾ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÑÐµÑÑÐ²Ð° Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ Ð¼Ð¸ÑÐ¾Ð²Ð¾Ð¹ ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸, Ð´Ð°Ð½Ð° Ð¿Ð¾Ð´ÑÐ¾Ð±Ð½Ð°Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ ÐÐ¼ÑÑÑÐºÐ¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð¸ Ð¿ÑÐ¾Ð²Ð¸Ð½ÑÐ¸Ð¸ Ð¥ÑÐ¹Ð»ÑÐ½ÑÐ·ÑÐ½, Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ðµ Ð¿ÑÐ¸Ð³ÑÐ°Ð½Ð¸ÑÐ½Ð¾Ð³Ð¾ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÑÐµÑÑÐ²Ð° Ð¼ÐµÐ¶Ð´Ñ ÐÐ¼ÑÑÑÐºÐ¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÑÑ Ð¸ Ð¿ÑÐ¾Ð²Ð¸Ð½ÑÐ¸ÐµÐ¹ Ð¥ÑÐ¹Ð»ÑÐ½ÑÐ·ÑÐ½, Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ ÑÐ¾ÑÐ³Ð¾Ð²Ð¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¸Ð³ÑÐ°Ð½Ð¸ÑÐ½Ð¾Ð³Ð¾ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÑÐµÑÑÐ²Ð° Ð¼ÐµÐ¶Ð´Ñ ÑÐºÐ°Ð·Ð°Ð½Ð½ÑÐ¼Ð¸ ÑÐµÐ³Ð¸Ð¾Ð½Ð°Ð¼Ð¸ Ð¸ Ð½Ð°Ð¼ÐµÑÐµÐ½Ñ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ñ ÐµÐ³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ.
description: In this work was reviewed a historical path of development transboundary cooperation of regions, as part of the history of relations between Russia and China, analyzed the legal basis of cross-border cooperation, were designated place and role of cross-border cooperation in the system of world economic activity, was given a detailed description of the current state of the Amur Region and Heilongjiang Province and identified the main problems of trade and economic cross-border cooperation between these regions.
Mantova, c’è la scienza al Festivaletteratura
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2018

All’interno del programma della manifestazione che apre i battenti domani, mercoledì 5 settembre, ci sarà uno spazio quotidiano dedicato alla scienza: “Scienceground”. Uno spazio con una formula molto innovativa. Ne parliamo con Matteo Polettini, consulente scientifico del festival
Analytic continuation of the critical line: suggestions for QCD
Creators: name: Cea, Paolo
name: Cosmai, Leonardo
name: D'Elia, Massimo
name: Manneschi, Chiara
name: Papa, Alessandro
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We perform a numerical study of the systematic effects involved in the determination of the critical line at real baryonic chemical potential by analytic continuation from results obtained at imaginary chemical potentials. We present results obtained in theories free of the sign problem, such as two-color QCD with finite baryonic density and three-color QCD with finite isospin chemical potential, and comment on general features which could be relevant also to the continuation of the critical line in real QCD at finite baryonic density.
description: 12 pages, 13 figures, 7 tables (revised version accepted by Phys. Rev. D80, 034501(2009))
The disintegration of neon by fast neutrons
Creators: name: Monier, Louis Ferdinand
Publisher: name: University of British Columbia
Year: 2011

description: A study has been made of the fast neutron induced reactions in natural neon gas. The neon was contained in a cylindrical geometry fast gridded ionization chamber, and the irradiating monokinetic neutrons were obtained by bombarding thin heavy ice targets with monokinetic deuterons accelerated by the U.B.C. Van de Graaff accelerator. Pulse height analysis, after amplification of the pulses, gave the energy distribution of the induced reactions, the primary reaction proceeding being Ne²⁰(n,∝)O¹⁷, with two alpha groups resulting from transitions to both the ground and first excited state of the O¹⁷ nucleus. The excitation function showed the existence of resonances in the Ne²¹ compound nucleus at the following energies, in Mev 10.04, 10.20, 10.32, 10.46, 10.63, 10.90, 11.06, 11.33, 11.44, 11.63, 11.76, 11.88, 11.96, 12.05 and 12.24. The total (n,∝) cross section varies from 90 mb to 500 mb in this energy range.
Tributo al Padre dell’astrofisica
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2018

C’è chi pensa che dovrebbe essere ricordato tra i fondatori dell’astronomia moderna, assieme a Galileo e Newton, eppure il nome di Padre Angelo Secchi non è fra i più conosciuti nella scienza.  A 200 anni dalla nascita diverse iniziative gli rendono omaggio, tra cui una conferenza internazionale, un video-racconto, una mostra virtuale, mentre uno spettacolo teatrale in allestimento metterà in risalto gli aspetti “rivoluzionari” di questa figura
title: Ð Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð¾ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ Â«Ð¢ÑÑÑÐ¾ÑÑÐºÐ¾Ðµ ÑÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð¶Ð´ÐµÐ½Ð¸Ðµ Ð¿Ð¾ Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½Ð¾Ð¼Ñ ÑÐ·ÑÐºÑÂ» Ð² ÐÐ½ÑÑÐ¸ÑÑÑÐµ Ð´Ð¸ÑÑÐ°Ð½ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ
title: On the issue of the implementation of the educational program âTutor support in a foreign languageâ at the Institute of Distance Learning
Creators: name: Ð¢Ð°ÑÐ°ÑÐ¾Ð²Ð°, Ð.
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2022
Subjects: ÑÑÑÑÐ¾Ñ
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Ð¾Ð¿ÑÐ¾Ñ
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Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ðµ
tutor
linguistic research
survey
competencies
professional activity
interaction

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÑÐ°ÑÑÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½ÑÐµ Ð¿ÑÑÐ¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¸Ð½ÑÑÐ¸ÑÑÑÐ° ÑÑÑÑÐ¾ÑÑÑÐ²Ð° Ð² Ð Ð¾ÑÑÐ¸Ð¸, Ð²Ð½Ðµ Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÐ¸ Ð¾Ñ ÑÐ¾Ð³Ð¾, Ð² ÐºÐ°ÐºÐ¾Ð¹ Ð¸ÑÑÐ¾Ð´Ð½Ð¾Ð¹ ÑÐ¾ÑÐºÐµ Ð¾Ð½ Ð½Ð°ÑÐ¾Ð´Ð¸ÑÑÑ. ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð°Ð½Ð°Ð»Ð¸Ð·Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ Â«Ð¢ÑÑÑÐ¾ÑÑÐºÐ¾Ðµ ÑÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð¶Ð´ÐµÐ½Ð¸Ðµ Ð¿Ð¾ Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½Ð¾Ð¼Ñ ÑÐ·ÑÐºÑÂ» Ð² ÐÐ½ÑÑÐ¸ÑÑÑÐµ Ð´Ð¸ÑÑÐ°Ð½ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ. ÐÐ»Ñ ÑÑÐ¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÑÑÑÑÑ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¸ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸, Ð¿ÑÐ¸Ð²Ð¾Ð´ÑÑÑÑ Ð´Ð°Ð½Ð½ÑÐµ Ð¿Ð¾ Ð¾Ð¿ÑÐ¾ÑÑ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð². ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð° Ð¿Ð¾Ð¿ÑÑÐºÐ° ÑÐ¾Ð·Ð´Ð°ÑÑ ÑÐµÐ¿ÑÐµÐ·ÐµÐ½ÑÐ°ÑÐ¸Ð²Ð½ÑÑ Ð¼Ð¾Ð´ÐµÐ»Ð¸ ÑÑÑÑÐ¾ÑÐ°, ÐºÐ¾ÑÐ¾ÑÐ°Ñ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð° ÐºÐ°Ðº Ð´Ð»Ñ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð½Ð¾Ð²ÑÑ Ð¿Ð»Ð°Ð½Ð¾Ð² ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÐºÐ¾Ð¼Ð¿ÐµÑÐµÐ½ÑÐ¸Ð¹ ÑÑÑÑÐ¾ÑÐ°, ÑÐ°Ðº Ð¸ Ð´Ð»Ñ Ð°Ð´Ð°Ð¿ÑÐ°ÑÐ¸Ð¸ ÑÐ¶Ðµ ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ñ.
description: This article presents possible ways to develop the institute of tutoring in Russia, regardless of what starting point it is located at. This work is devoted to the analysis of the implementation of the educational program âTutor support in a foreign languageâ at the Institute of Distance Learning. To do this, various sources of information are analyzed, data on the survey of students are provided.
On the isolated dwarf galaxies: from cuspy to flat dark matter density profiles and metallicity gradients
Creators: name: Pasetto, S.
name: Grebel, E. K.
name: Berczik, P.
name: Spurzem, R.
name: Dehnen, W.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The chemodynamical evolution of spherical multi-component self-gravitating models for isolated dwarf galaxies is studied. We compare their evolution with and without feedback effects from star formation processes. We find that initially cuspy dark matter profiles flatten with time as a result of star formation, without any special tuning conditions. Thus the seemingly flattened profiles found in many dwarfs do not contradict the cuspy profiles predicted by cosmological models. We also calculate the chemical evolution of stars and gas, to permit comparisons with observational data.
description: Accepted the 28/01/10
Additional file 1 of Comparison of clinical manifestation of dengue fever in Bangladesh: an observation over a decade
Creators: name: Hasan, Mohammad Jahid
name: Tabassum, Tamanna
name: Sharif, Mohiuddin
name: Khan, Md. Abdullah Saeed
name: Bipasha, Akhi Roy
name: Basher, Ariful
name: Islam, Mohammad Rafiqul
name: Amin, Mohammad Robed
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Neuroscience
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Cancer
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 1: Figure 1. Searching details of the study underwent in DMCH and reporting dengue outbreak in Bangladesh. Figure 2. Flow chart of patient selection. Table 1. STROBE Statement—Checklist of items that should be included in reports of cross-sectional studies. Table 2. Study characteristics that not included for comparison. Table 3. Clinical characteristics of confirmed and probable dengue cases* (n = 747). Table 4. Laboratory findings of the confirmed and probable dengue cases of the study.
Legge di Hubble, è ora di cambiarle nome
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2018

Approvata a Vienna la settimana scorsa, in chiusura dell’Assemblea generale dell’Unione astronomica internazionale, una risoluzione per rinominare la legge sull’espansione dell’universo “Hubble-Lemaître law”. Massimo Della Valle (Inaf): «Mi pare doveroso»
MPEC 2025-C124 : DAILY ORBIT UPDATE (2025 February 8)
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2025
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
Comment on "Superfluid turbulence from quantum Kelvin wave to classical Kolmogorov cascade". [arXiv:0905.0159v1]
Creators: name: Krstulovic, Giorgio
name: Brachet, Marc
Publisher: name: arXiv
Year: 2009
Subjects: subject: Chaotic Dynamics (nlin.CD)
subject: FOS: Physical sciences

description: In this comment we point out that the high wavenumber $k^{-3}$ power-law observed by the PRL, [v. 103, 084501 (2009) by J. Yepez, G. Vahala, L.Vahala and M. Soe, arXiv:0905.0159] is an artifact stemming from the definition of the kinetic energy spectra and is thus not directly related to a Kelvin wave cascade. We also clarify a confusion about the wavenumber intervals on which Kolmogorov and Kelvin wave cascades are expected to take place.
description: submitted to PRL
title: ÐÑÐ¼ÑÐµÑÑÐ»Ð¸Ð½Ð³
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ¾Ð»Ð¸ÑÐ¾Ð², ÐÐ½Ð´ÑÐµÐ¹
name: Ð¡ÐµÐ½Ñ, Ð¡ÐµÑÐ³ÐµÐ¹
name: Ð¡ÑÑÐµÐ½ÐºÐ¾, ÐÐ°Ð»ÐµÑÐ¸Ð¹
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2022
Subjects: ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ°Ñ ÐºÑÐ»ÑÑÑÑÐ° Ð¸ ÑÐ¿Ð¾ÑÑ
Ð°ÑÐ¼ÑÐµÑÑÐ»Ð¸Ð½Ð³
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: Ð ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐ½ÑÑ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð², Ð° ÑÐ°ÐºÐ¶Ðµ Ð¾ÑÐµÑÐµÑÑÐ²ÐµÐ½Ð½ÑÑ Ð¸ Ð·Ð°ÑÑÐ±ÐµÐ¶Ð½ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð¿Ð¾Ð´Ð¾Ð±ÑÐ°Ð½Ñ Ð¸ Ð¾Ð±Ð¾Ð±ÑÐµÐ½Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ, ÑÐ°ÑÐºÑÑÐ²Ð°ÑÑÐ¸Ðµ ÐºÐ»ÑÑÐµÐ²ÑÐµ Ð°ÑÐ¿ÐµÐºÑÑ Ð°ÑÐ¼ÑÐµÑÑÐ»Ð¸Ð½Ð³Ð° ÐºÐ°Ðº Ð²Ð¸Ð´Ð° ÑÐ¿Ð¾ÑÑÐ° Ð½Ð° ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¼ ÑÑÐ°Ð¿Ðµ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ. ÐÐ·Ð»Ð¾Ð¶ÐµÐ½Ñ ÑÐµÑÐ½Ð¸ÐºÐ° Ð¸ ÑÐ°ÐºÑÐ¸ÐºÐ° Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð±Ð¾ÑÑÐ±Ñ Ð² Ð°ÑÐ¼ÑÐµÑÑÐ»Ð¸Ð½Ð³Ðµ, Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ Ð¸ ÑÑÐµÐ½Ð¸ÑÐ¾Ð²ÐºÐ¸, Ð´Ð°Ð½Ñ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸, Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÐµ Ð² Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ð¸ ÑÑÐµÐ±Ð½Ð¾-ÑÑÐµÐ½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ°, ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð¸ÑÑÐ¾ÑÐ¸Ð¸ Ð¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð·Ð°Ð½ÑÑÐ¸Ð¹ Ð°ÑÐ¼ÑÐµÑÑÐ»Ð¸Ð½Ð³Ð¾Ð¼, Ð²Ð¾Ð¿ÑÐ¾ÑÑ ÑÐµÑÐ¼Ð¸Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸, ÑÐ¸ÑÑÐµÐ¼Ð° Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð·Ð°Ð½ÑÑÐ¸Ð¹ Ð°ÑÐ¼ÑÐµÑÑÐ»Ð¸Ð½Ð³Ð¾Ð¼, ÑÐ°ÑÐºÑÑÐ²Ð°ÑÑÑÑ Ð¿ÑÐ°Ð²Ð¸Ð»Ð° ÑÐ¾ÑÐµÐ²Ð½Ð¾Ð²Ð°Ð½Ð¸Ð¹, Ð½Ð¾ÑÐ¼Ñ Ð¸ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ñ Ðº Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½ÑÑ ÑÐ°Ð·ÑÑÐ´Ð¾Ð² Ð¸ Ð·Ð²Ð°Ð½Ð¸Ð¹, ÑÑÐ´ÐµÐ¹ÑÐºÐ¸Ñ ÐºÐ°ÑÐµÐ³Ð¾ÑÐ¸Ð¹ Ð¿Ð¾ Ð²Ð¸Ð´Ñ ÑÐ¿Ð¾ÑÑÐ° Â«Ð°ÑÐ¼ÑÐµÑÑÐ»Ð¸Ð½Ð³Â». ÐÐ²ÑÐ¾ÑÐ°Ð¼Ð¸ ÑÑÐµÐ±Ð½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ ÑÐ²Ð»ÑÑÑÑÑ: Ð¿ÑÐµÐ·Ð¸Ð´ÐµÐ½Ñ ÑÐµÐ³Ð¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¾ÑÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÐÐ±ÑÐµÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸ Ð°ÑÐ¼ÑÐµÑÑÐ»Ð¸Ð½Ð³Ð° Ð Ð¾ÑÑÐ¸Ð¸ â Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸ Ð°ÑÐ¼ÑÐµÑÑÐ»Ð¸Ð½Ð³Ð° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ð° Ð. Ð. ÐÐ¾Ð»Ð¸ÑÐ¾Ð², Ð·Ð°ÑÐ»ÑÐ¶ÐµÐ½Ð½ÑÐ¹ ÑÑÐµÐ½ÐµÑ Ð Ð¾ÑÑÐ¸Ð¸ Ð¿Ð¾ Ð°ÑÐ¼ÑÐµÑÑÐ»Ð¸Ð½Ð³Ñ Ð¡. Ð. Ð¡ÐµÐ½Ñ, Ð´Ð¸ÑÐµÐºÑÐ¾Ñ ÐÐ½ÑÑÐ¸ÑÑÑÐ° ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð¹ ÐºÑÐ»ÑÑÑÑÑ ÑÐ¿Ð¾ÑÑÐ° Ð¸ ÑÑÑÐ¸Ð·Ð¼Ð° 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, Ð´Ð¾ÐºÑÐ¾Ñ Ð¿ÐµÐ´Ð°Ð³Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð½Ð°ÑÐº, Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ñ Ð. Ð. Ð¡ÑÑÐµÐ½ÐºÐ¾. ÐÑÐ¾Ð¼Ðµ ÑÐ¾Ð³Ð¾, Ð² Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¼Ð½Ð¾Ð³Ð¾Ð»ÐµÑÐ½ÐµÐ³Ð¾ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¾Ð¿ÑÑÐ° Ð±Ð¾Ð»ÑÑÐ¾Ð¹ Ð³ÑÑÐ¿Ð¿Ñ ÑÑÐµÐ½ÐµÑÐ¾Ð² Ð² Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐµ ÑÐ¿Ð¾ÑÑÑÐ¼ÐµÐ½Ð¾Ð². Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÐµÐ½ÐµÑÐ¾Ð², Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»ÐµÐ¹ (ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð²) ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð²Ð¾ÑÐ¿Ð¸ÑÐ°Ð½Ð¸Ñ, Ð¾Ð½Ð¾ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¾ ÑÐ¿Ð¾ÑÑÑÐ¼ÐµÐ½Ð°Ð¼Ð¸ (Ð½Ð¾Ð²Ð¸ÑÐºÐ°Ð¼Ð¸, Ð»ÑÐ±Ð¸ÑÐµÐ»ÑÐ¼Ð¸) Ð´Ð»Ñ ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½ÑÑ Ð·Ð°Ð½ÑÑÐ¸Ð¹.
Entropy entrainment and dissipation in superfluid Helium
Creators: name: Andersson, N.
name: Comer, G. L.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Other Condensed Matter (cond-mat.other)
subject: FOS: Physical sciences

description: Building on a general variational framework for multi-fluid dynamics, we discuss finite temperature effects in superfluids. The main aim is to provide insight into the modelling of more complex finite temperature superfluid systems, like the mixed neutron superfluid/proton superconductor that is expected in the outer core of a neutron star. Our final results can also (to a certain extent) be used to describe colour-flavour locked quark superconductors that may be present at the extreme densities in the deep neutron star core. As a demonstration of the validity of the model, which is based on treating the excitations in the system as a massless ``entropy'' fluid, we show that it is formally equivalent to the traditional two-fluid approach for superfluid Helium. In particular, we highlight the fact that the entropy entrainment encodes the ``normal fluid density'' of the traditional approach. We also show how the superfluid constraint of irrotationality reduces the number of dissipation coefficients in the system. This analysis provides insight into the more general problem when vortices are present in the superfluid, and we discuss how the so-called mutual friction force can be accounted for in our framework. The end product is a hydrodynamic formalism for finite temperature effects in a single superfluid condensate. This framework can readily be extended to more complex situations.
description: revised version, clarifies points regarding entrainment in different contexts
The spherical collapse model and cluster formation beyond the $Λ$ cosmology: Indications for a clustered dark energy?
Creators: name: Basilakos, S.
name: Sanchez, J. C. Bueno
name: Perivolaropoulos, Leandros
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We generalize the small scale dynamics of the universe by taking into account models with an equation of state which evolves with time, and provide a complete formulation of the cluster virialization attempting to address the nonlinear regime of structure formation. In the context of the current dark energy models, we find that galaxy clusters appear to form at z\sim 1-2, in agreement with previous studies. Also, we investigate thoroughly the evolution of spherical matter perturbations, as the latter decouple from the background expansion and start to ``turn around'' and finally collapse. Within this framework, we find that the concentration parameter depends on the choice of the considered dark energy (homogeneous or clustered). In particular, if the distribution of the dark energy is clustered then we produce more concentrated structures with respect to the homogeneous dark energy. Finally, comparing the predicted concentration parameter with the observed concentration parameter, measured for four massive galaxy clusters, we find that the scenario which contains a pure homogeneous dark energy is unable to reproduce the data. The situation becomes somewhat better in the case of an inhomogeneous (clustered) dark energy.
description: 12 pages, 4 figures. Accepted in Phys. Rev. D (to appear)
Additional file 1 of DNA methylation of the KLK8 gene in depression symptomatology
Creators: name: Starnawska, Anna
name: Bukowski, Lina
name: Chernomorchenko, Ana
name: Elfving, Betina
name: Müller, Heidi Kaastrup
name: van den Oord, Edwin
name: Aberg, Karolina
name: Guintivano, Jerry
name: Grove, Jakob
name: Mors, Ole
name: Børglum, Anders D.
name: Nielsen, Anders L.
name: Qvist, Per
name: Staunstrup, Nicklas Heine
Publisher: name: figshare
Year: 2021
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Neuroscience
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: Hematology

description: Additional file 1: Figure S1. Overview of pyrosequencing primer design to quantify KLK8 DNAm levels at CpG1 and CpG2.
Con gli antineutrini nel cuore delle supernove
Creators: Matteo Boni
Publisher: name: Media Inaf
Year: 2018

Uno studio pubblicato su Physical Review Letters propone un nuovo metodo per studiare i processi che avvengono in una esplosione di supernova. Utilizzando le meteoriti. L’idea è di cercare al loro interno isotopi di elementi radioattivi la cui produzione sia associata a una particolare particella: l’antineutrino elettronico
Classical density-functional theory of inhomogeneous water including explicit molecular structure and nonlinear dielectric response
Creators: name: Lischner, Johannes
name: Arias, T. A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We present an accurate free-energy functional for liquid water written in terms of a set of effective potential fields in which fictitious noninteracting water molecules move. The functional contains an \emph{exact} expression of the entropy of noninteracting molecules and thus provides an ideal starting point for the inclusion of complex inter-molecular interactions which depend on the \emph{orientation} of the interacting molecules. We show how an excess free-energy functional can be constructed to reproduce the following properties of water: the dielectric response; the experimental site-site correlation functions; the surface tension; the bulk modulus of the liquid and the variation of this modulus with pressure; the density of the liquid and the vapor phase; and liquid-vapor coexistence. As a demonstration, we present results for the application of this theory to the behavior of liquid water in a parallel plate capacitor. In particular, we make predictions for the dielectric response of water in the nonlinear regime, finding excellent agreement with known data.
description: 10 pages, 6 figures
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¸ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ðµ ÑÐ°Ð¹ÑÐ° Ð´Ð»Ñ ÑÐ¾ÑÐ¾ÑÑÑÐ´Ð¸Ð¸ "Ð¦Ð¸ÐºÐ»Ð¾ÑÐ°Ð¼Ð°"
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ½Ð¾Ð³Ð¾Ð»ÐµÑ, ÐÐ¼Ð¸ÑÑÐ¸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: 2016
Subjects: Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ðµ ÑÐ°Ð¹ÑÐ°
Ð¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÐµÐ»ÑÑÐºÐ¸Ð¹ Ð¸Ð½ÑÐµÑÑÐµÐ¹Ñ
ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐµ ÑÐ°Ð¹Ð»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 Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ° ÑÐ²Ð»ÑÐµÑÑÑ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÐ¸ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð²ÐµÐ±-ÑÐ°Ð¹ÑÐ° Ð´Ð»Ñ ÑÐ¾ÑÐ¾ÑÑÑÐ´Ð¸Ð¸ Ñ ÑÐµÐ»ÑÑ ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¸Ð±ÑÐ»Ð¸. ÐÐ»Ñ Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ñ ÑÐµÐ»Ð¸ Ð±ÑÐ» Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¾Ð±ÑÐµÐºÑÐ° Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¸ Ð¿ÑÑÐ¸ Ð¸Ñ ÑÐµÑÐµÐ½Ð¸Ñ. ÐÑÐ¾Ð¼Ðµ ÑÐ¾Ð³Ð¾, Ð±ÑÐ»Ð¸ Ð²ÑÑÐ²Ð»ÐµÐ½Ñ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ñ Ðº ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»Ñ Ð¸ Ð¸Ð½ÑÐµÑÑÐµÐ¹ÑÑ Ð²ÐµÐ±-ÑÐ°Ð¹ÑÐ° ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ Ð¸ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½ Ð²ÑÐ±Ð¾Ñ ÑÐ¸Ð¿Ð° ÑÐ°Ð¹ÑÐ°, ÐºÐ¾ÑÐ¾ÑÐ¾Ð¹ Ð±ÑÐ´ÐµÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½ Ð´Ð»Ñ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ ÑÐ°Ð¹ÑÐ°. Ð¢Ð°ÐºÐ¶Ðµ Ð±ÑÐ»Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ Ð¸ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÑ Ð¾ÑÐµÐ½ÐºÐ¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð²ÐµÐ±-ÑÐ°Ð¹ÑÐ¾Ð². ÐÑÐµÐ´Ð¿Ð¾Ð»Ð°Ð³Ð°ÐµÐ¼ÑÐµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¾Ñ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð²ÐµÐ±-ÑÐ°Ð¹ÑÐ° Ð¿ÑÐµÐ´Ð¿Ð¾Ð»Ð°Ð³Ð°ÑÑ: ÑÐ¾ÑÑ Ð¼ÐµÑÑÑÐ½Ð¾Ð³Ð¾ ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²Ð° Ð·Ð°ÐºÐ°Ð·Ð¾Ð² Ð°ÑÐµÐ½Ð´Ñ ÑÐ¾ÑÐ¾ÑÑÑÐ´Ð¸Ð¸ Ð¸ Ð¾Ð±ÑÐµÐ¹ Ð²ÑÑÑÑÐºÐ¸, Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ðµ ÑÑÐµÐ¿ÐµÐ½Ð¸ ÑÐ·Ð½Ð°Ð²Ð°ÐµÐ¼Ð¾ÑÑÐ¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð½Ð° ÑÑÐ½ÐºÐµ, ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ðµ Ð¿Ð¾Ð»Ð¾Ð¶Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¸Ð¼Ð¸Ð´Ð¶Ð°.
Production of a highly-ionized gas by an electromagnetically-driven shock wave
Creators: name: Cormack, George Douglas
Publisher: name: University of British Columbia
Year: 2011

description: A study has been made of the properties of an electromagnetically generated shock wave travelling through both argon and helium. An initial capacitive energy of 450 joules has been rapidly discharged into the gas and has resulted in shock wave velocities of up to five centimeters per microsecond. The high velocities obtained can be attributed to careful design of the main discharge circuit. Preliminary results of measurements of the properties of the shock wave are given. Of primary interest has been the results of measurements of the properties of the plasma associated with the shock wave. A magnetic field deflection method has been developed for the measurement of the electrical conductivity of this plasma.
The crossover from single file to Fickian diffusion
Creators: name: Sané, J.
name: Padding, J. T.
name: Louis, A. A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: The crossover from single-file diffusion, where the mean-square displacement scales as ~t^(1/2), to normal Fickian diffusion, where ~t$, is studied as a function of channel width for colloidal particles. By comparing Brownian dynamics to a hybrid molecular dynamics and mesoscopic simulation technique, we can study the effect of hydrodynamic interactions on the single file mobility and on the crossover to Fickian diffusion for wider channel widths. For disc-like particles with a steep interparticle repulsion, the single file mobilities for different particle densities are well described by the exactly solvable hard-rod model. This holds both for simulations that include hydrodynamics, as well as for those that don't. When the single file constraint is lifted, then for particles of diameter σand pipe of width $L$ such that (L- 2 σ)/σ= δ_c << 1 the particles can be described as hopping past one-another in an average time t_{hop}. For shorter times t << t_{hop} the particles still exhibit sub-diffusive behaviour, but at longer times t > t_{hop}, normal Fickian diffusion sets in with an effective diffusion constant D_{hop} ~ t_{hop}^(1/2). For the Brownian particles, t_{hop} ~ 1/δ_c^(2) when δ<< 1, but when hydrodynamic interactions are included, we find a stronger dependence than δ_c^{-2}. We attribute this difference to short-range lubrication forces that make it more difficult for particles to hop past each other in very narrow channels.
Additional file 2 of DNA methylation of the KLK8 gene in depression symptomatology
Creators: name: Starnawska, Anna
name: Bukowski, Lina
name: Chernomorchenko, Ana
name: Elfving, Betina
name: Müller, Heidi Kaastrup
name: van den Oord, Edwin
name: Aberg, Karolina
name: Guintivano, Jerry
name: Grove, Jakob
name: Mors, Ole
name: Børglum, Anders D.
name: Nielsen, Anders L.
name: Qvist, Per
name: Staunstrup, Nicklas Heine
Publisher: name: figshare
Year: 2021
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Neuroscience
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: Hematology

description: Additional file 2: Supplementary Table 1. Conditions for PCR amplification of KLK8 promoter region containing CpG1 and CpG2 for pyrosequencing analysis. Supplementary Table 2. Overview of sex and age distribution of PRISME individuals after quality control filtering for each tested CpG site. Supplementary Table 3. Power calculations for PRISME, NESDA, GSMS, BioMom, and BrainMDD cohorts to replicate the association between KLK8 DNAm levels and depression-related phenotypes.
title: Ð¤Ð¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿Ð»Ð°ÑÑ Ð·Ð° Ð¿Ð¾Ð´ÐºÐ»ÑÑÐµÐ½Ð¸Ðµ Ðº ÑÐ¸ÑÑÐµÐ¼Ð°Ð¼ ÑÐµÐ¿Ð»Ð¾ÑÐ½Ð°Ð±Ð¶ÐµÐ½Ð¸Ñ Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ð°
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Ñ, Ð¡ÐµÑÐ³ÐµÐ¹
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: Ð¿Ð¾Ð´ÐºÐ»ÑÑÐµÐ½Ð¸Ðµ Ðº ÑÐ¸ÑÑÐµÐ¼Ðµ ÑÐµÐ¿Ð»Ð¾ÑÐ½Ð°Ð±Ð¶ÐµÐ½Ð¸Ñ
Ð·Ð°ÑÐ²Ð¸ÑÐµÐ»Ñ
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ÑÐ°ÑÑÐµÑ Ð¿Ð»Ð°ÑÑ

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Photochemistry of the PAH pyrene in water ice: the case for ion-mediated solid-state astrochemistry
Creators: name: Bouwman, J.
name: Cuppen, H. M.
name: Bakker, A.
name: Allamandola, L. J.
name: Linnartz, H.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: Context. Icy dust grains play an important role in the formation of complex inter- and circumstellar molecules. Observational studies show that polycyclic aromatic hydrocarbons (PAHs) are abundantly present in the ISM in the gas phase. It is likely that these non-volatile species freeze out onto dust grains as well and participate in the astrochemical solid-state network, but experimental PAH ice studies are largely lacking. Methods. Near UV/VIS spectroscopy is used to track the in situ VUV driven photochemistry of pyrene containing ices at temperatures ranging from 10 to 125 K. Results. The main photoproducts of VUV photolyzed pyrene ices are spectroscopically identified and their band positions are listed for two host ices, \water and CO. Pyrene ionisation is found to be most efficient in \water ices at low temperatures. The reaction products, triplet pyrene and the 1-hydro-1-pyrenyl radical are most efficiently formed in higher temperature water ices and in low temperature CO ice. Formation routes and band strength information of the identified species are discussed. Additionally, the oscillator strengths of Py, Py^+ and PyH are derived and a quantitative kinetic analysis is performed by fitting a chemical reaction network to the experimental data. Conclusions. Pyrene is efficiently ionised in water ice at temperatures below 50 K. Hydrogenation reactions dominate the chemistry in low temperature CO ice with trace amounts of water. The results are put in an astrophysical context by determining the importance of PAH ionisation in a molecular cloud. The photoprocessing of a sample PAH in ice described in this manuscript indicates that PAH photoprocessing in the solid state should also be taken into account in astrochemical models.
description: 11 pages, 8 figures, accepted for publication in A&A
title: ÐÐ¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð¾Ðµ Ð¿ÑÐ°Ð²Ð¾Ð²Ð¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ Ð²ÑÑÑÐµÐ³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð² Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸. Ð¢. 2
Creators: name: ÐÐ¾ÑÐ¾Ð²ÐºÐ¾Ð², ÐÐ»ÐµÐºÑÐµÐ¹
name: Ð Ð¾Ð¼Ð°Ð½Ð¾Ð², ÐÐ°Ð²ÐµÐ»
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: 2016
Subjects: Ð²ÑÑÑÐµÐµ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ðµ
Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½ÑÐµ Ð°ÐºÑÑ

description: Ð ÐºÐ½Ð¸Ð³Ðµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½ÑÐµ Ð¿ÑÐ°Ð²Ð¾Ð²ÑÐµ Ð°ÐºÑÑ, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½ÑÐµ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð¸ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Ð¤ÐµÐ´ÐµÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð·Ð°ÐºÐ¾Ð½Ð° Ð¾Ñ 29 Ð´ÐµÐºÐ°Ð±ÑÑ 2012 Ð³. â 273-Ð¤Ð Â«ÐÐ± Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð² Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸Â». Ð ÑÐ¾Ð¼Ðµ 1 ÑÐ¾Ð´ÐµÑÐ¶Ð°ÑÑÑ ÑÐµÐ´ÐµÑÐ°Ð»ÑÐ½ÑÐµ Ð·Ð°ÐºÐ¾Ð½Ñ Ð¸ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½ÑÐµ Ð¿ÑÐ°Ð²Ð¾Ð²ÑÐµ Ð°ÐºÑÑ ÐÑÐ°Ð²Ð¸ÑÐµÐ»ÑÑÑÐ²Ð° Ð Ð¾ÑÑÐ¸Ð¸. Ð ÑÐ¾Ð¼Ðµ 2 ÑÐ°Ð·Ð¼ÐµÑÐµÐ½Ñ Ð¿ÑÐ¸ÐºÐ°Ð·Ñ ÐÐ¸Ð½Ð¾Ð±ÑÐ½Ð°ÑÐºÐ¸ Ð Ð¾ÑÑÐ¸Ð¸. Ð ÑÐ¾Ð¼Ðµ 3 ÑÐ°Ð·Ð¼ÐµÑÐµÐ½Ñ Ð¿Ð¸ÑÑÐ¼Ð° ÐÐ¸Ð½Ð¾Ð±ÑÐ½Ð°ÑÐºÐ¸ Ð Ð¾ÑÑÐ¸Ð¸, ÑÑÐ¾ÑÐ½ÑÑÑÐ¸Ðµ Ð¾ÑÐ´ÐµÐ»ÑÐ½ÑÐµ Ð°ÑÐ¿ÐµÐºÑÑ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐµÐ´ÐµÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð·Ð°ÐºÐ¾Ð½Ð°.
Alla ricerca della galassia di Barnard
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2018

La galassia di Barnard è uno degli oggetti celesti che caratterizzano il cielo di questo mese. I consigli per individuarla, insieme a quelli per osservare le costellazioni, i pianeti e i principali fenomeni astronomici visibili a settembre
Additional file 3 of DNA methylation of the KLK8 gene in depression symptomatology
Creators: name: Starnawska, Anna
name: Bukowski, Lina
name: Chernomorchenko, Ana
name: Elfving, Betina
name: Müller, Heidi Kaastrup
name: van den Oord, Edwin
name: Aberg, Karolina
name: Guintivano, Jerry
name: Grove, Jakob
name: Mors, Ole
name: Børglum, Anders D.
name: Nielsen, Anders L.
name: Qvist, Per
name: Staunstrup, Nicklas Heine
Publisher: name: figshare
Year: 2021
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Neuroscience
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: Hematology

description: Additional file 3: Figure S2. Overview of pyrosequencing primer location, genomic context of analyzed sites CpG1 and CpG2 from KLK8 promoter region, and regulatory elements (CpG island and H3K27A mark).
Recent algorithm and machine developments for lattice QCD
Creators: name: Ishikawa, Ken-Ichi
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: I review recent machine trends and algorithmic developments for dynamical lattice QCD simulations with the HMC algorithm for Wilson-type fermions. The topics include the trend toward multi-core processors and general purpose GPU (GPGPU) computing, and improvements on the quark determinant preconditioning, molecular dynamics integrator, and quark solvers. I also discuss the prospect on the use of these techniques on the forthcoming petaflops machines.
description: 21 pages, 2 figures; talk presented at Lattice 2008, XXVI International Symposium on Lattice Field Theory, July 14-19, 2008, Williamsburg, Virginia, USA
title: ÐÐ½Ð°Ð»Ð¸Ð· Ð¸ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¾Ð¿Ð»Ð°ÑÑ ÑÑÑÐ´Ð° Ð¸ Ð¼Ð¾ÑÐ¸Ð²Ð°ÑÐ¸Ð¸ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¼ÐµÐ»ÑÑÐ½ÐµÐ½ÐºÐ¾, Ð¢Ð°ÑÑÑ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: 2017
Subjects: ÑÐ¸ÑÑÐµÐ¼Ñ Ð¾Ð¿Ð»Ð°ÑÑ ÑÑÑÐ´Ð°
Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ
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description: Ð Ð¿ÑÐ¾ÑÐµÑÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸Ð»Ð¸ÑÑ: Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð°ÐºÑÐ¸Ð¾Ð½ÐµÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐµÑÑÐ²Ð°; Ð°Ð½Ð°Ð»Ð¸Ð· Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¾Ð¿Ð»Ð°ÑÑ ÑÑÑÐ´Ð° Ð¸ Ð¼Ð¾ÑÐ¸Ð²Ð°ÑÐ¸Ð¸ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð² ÐÐ Â«ÐÐ¾Ð´Ð½ÑÐ¹ ÐºÐ¾Ð½ÑÐ¸Ð½ÐµÐ½ÑÂ»; Ð°Ð½Ð°Ð»Ð¸Ð· Ð²Ð»Ð¸ÑÐ½Ð¸Ñ ÑÐ°ÐºÑÐ¾ÑÐ¾Ð² Ð½Ð° ÑÑÐ¾Ð²ÐµÐ½Ñ, Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÑ Ð¾Ð¿Ð»Ð°ÑÑ ÑÑÑÐ´Ð° Ð¸ ÑÑÑÑÐºÑÑÑÑ Ð·Ð°ÑÐ°Ð±Ð¾ÑÐ½Ð¾Ð¹ Ð¿Ð»Ð°ÑÑ. Ð ÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð¼ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼ Ð¾Ð¿Ð»Ð°ÑÑ ÑÑÑÐ´Ð° Ð¸ Ð¼Ð¾ÑÐ¸Ð²Ð°ÑÐ¸Ð¸ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð² ÐÐ Â«ÐÐ¾Ð´Ð½ÑÐ¹ ÐºÐ¾Ð½ÑÐ¸Ð½ÐµÐ½ÑÂ». ÐÐ½Ð°ÑÐ¸Ð¼Ð¾ÑÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð·Ð°ÐºÐ»ÑÑÐ°ÐµÑÑÑ Ð² ÑÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð¿ÑÐ¸Ð¼ÐµÐ½ÑÐµÐ¼Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¾Ð¿Ð»Ð°ÑÑ ÑÑÑÐ´Ð° Ð¸ Ð¼Ð¾ÑÐ¸Ð²Ð°ÑÐ¸Ð¸ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð°, ÑÑÐ¾ Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ñ Ð¾Ð±ÐµÑÐ¿ÐµÑÐ¸ÑÑ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð¸ ÑÐ»ÑÑÑÐµÐ½Ð¸Ðµ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÑ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸.