cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The case for Zero Trust Digital Forensics
Creators: name: Neale, Christoper
name: Kennedy, Ian
name: Price, Blain
name: Nuseibeh, Bashar
Publisher: name: arXiv
Year: 2022
Subjects: subject: Computers and Society (cs.CY)
subject: FOS: Computer and information sciences

description: It is imperative for all stakeholders that digital forensics investigations produce reliable results to ensure the field delivers a positive contribution to the pursuit of justice across the globe. Some aspects of these investigations are inevitably contingent on trust, however this is not always explicitly considered or critically evaluated. Erroneously treating features of the investigation as trusted can be enormously damaging to the overall reliability of an investigations findings as well as the confidence that external stakeholders can have in it. As an example, digital crime scenes can be manipulated by tampering with the digital artefacts left on devices, yet recent studies have shown that efforts to detect occurrences of this are rare and argue that this leaves digital forensics investigations vulnerable to accusations of inaccuracy. In this paper a new approach to digital forensics is considered based on the concept of Zero Trust, an increasingly popular design in network security. Zero Trust describes the practitioner mindset and principles upon which the reliance on trust in network components is eliminated in favour of dynamic verification of network interactions. An initial definition of Zero Trust Digital Forensics will be proposed and then a specific example considered showing how this strategy can be applied to digital forensic investigations to mitigate against the specific risk of evidence tampering. A definition of Zero Trust Digital Forensics is proposed, specifically that it is a strategy adopted by investigators whereby each aspect of an investigation is assumed to be unreliable until verified. A new principle will be introduced, namely the multifaceted verification of digital artefacts that can be used by practitioners who wish to adopt a Zero Trust Digital Forensics strategy during their investigations...
title: Ð¤ÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð°Ñ ÑÑÐ¸Ð»Ð¸ÑÑÐ¸ÐºÐ° ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÑÑÑÐºÐ¾Ð³Ð¾ ÑÐ·ÑÐºÐ°
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ¾Ð½Ð¾ÑÐ¾Ð½Ð¾Ðº, Ð.
name: ÐÑÑÐ½Ð´ÑÑÐµÐ²Ð°, ÐÐ½Ð½Ð°
name: Ð¡ÑÑÑÐ¸ÑÐ¸Ð½Ð°, ÐÑÐ´Ð¼Ð¸Ð»Ð°
name: Ð¥Ð¾ÑÐ»Ð¾Ð², ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
name: Ð¨ÑÑÐºÐ°ÑÑÑÐ¾Ð²Ð°, ÐÐ°Ð»Ð¸Ð½Ð°
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2009
Subjects: ÑÑÑÑÐºÐ¸Ð¹ ÑÐ·ÑÐº
ÑÑÐ¸Ð»Ð¸ÑÑÐ¸ÐºÐ°
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð°Ð´ÑÐµÑÐ¾Ð²Ð°Ð½Ð¾ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ Ð³ÑÐ¼Ð°Ð½Ð¸ÑÐ°ÑÐ½ÑÑ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ¾Ð², Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ð¼ ÐºÑÑÑ Â«Ð¤ÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð°Ñ ÑÑÐ¸Ð»Ð¸ÑÑÐ¸ÐºÐ° ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÑÑÑÐºÐ¾Ð³Ð¾ ÑÐ·ÑÐºÐ°Â». Ð Ð½ÐµÐ¼ ÑÐ¾Ð´ÐµÑÐ¶Ð°ÑÑÑ ÐºÑÐ°ÑÐºÐ¸Ðµ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ Ð¿Ð¾ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÑÐ¸Ð»Ð¸ÑÑÐ¸ÐºÐµ. Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð½Ð°ÑÑÐ½ÑÐ¹, Ð¾ÑÐ¸ÑÐ¸Ð°Ð»ÑÐ½Ð¾-Ð´ÐµÐ»Ð¾Ð²Ð¾Ð¹, Ð¿ÑÐ±Ð»Ð¸ÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ð¹, ÑÐ°Ð·Ð³Ð¾Ð²Ð¾ÑÐ½ÑÐ¹ ÑÑÐ¸Ð»Ð¸ ÑÐµÑÐ¸. ÐÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ°ÑÑÑ Ð²ÐºÐ»ÑÑÐ°ÐµÑ Ð±Ð¾Ð»ÑÑÐ¾Ðµ ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²Ð¾ ÑÐ¿ÑÐ°Ð¶Ð½ÐµÐ½Ð¸Ð¹, Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÑ Ð½Ð° Ð²ÑÑÐ°Ð±Ð¾ÑÐºÑ ÑÐ¼ÐµÐ½Ð¸Ð¹ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÑÑ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð²Ð½ÑÐµ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÑÐ¸Ð»ÐµÐ¹, Ð¸Ñ Ð´Ð¾Ð¼Ð¸Ð½Ð°Ð½ÑÐ½ÑÐµ Ð¿ÑÐ¸Ð·Ð½Ð°ÐºÐ¸. ÐÐ°Ð´Ð°Ð½Ð¸Ñ, ÑÐ°Ð±Ð»Ð¸ÑÑ Ð¸ ÑÑÐµÐ¼Ñ Ð¿Ð¾Ð¼Ð¾Ð³Ð°ÑÑ ÑÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°ÑÑ Ð½Ð°Ð²ÑÐºÐ¸ ÑÐ·Ð½Ð°Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÐºÑÑÐ¾Ð² Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ¸Ð»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°.
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÐ½ÐºÐ° Ð¾ÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ¸Ñ ÑÑÐ»ÑÐ³ Ð´Ð»Ñ Ð¡ÐÐ± ÐÐÐ£Ð Â«ÐÐ¾ÑÐ¾Ð´ÑÐºÐ°Ñ ÐÐ¾ÐºÑÐ¾Ð²ÑÐºÐ°Ñ Ð±Ð¾Ð»ÑÐ½Ð¸ÑÐ°Â»
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ³Ð¾ÑÐ¾Ð²Ð°, ÐÐºÐ°ÑÐµÑÐ¸Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ
Ð¾Ð¿ÑÐ¾Ñ
Ð°Ð½Ð°Ð»Ð¸Ð· ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾Ð²
ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ
marketing research
survey
competitor analysis
economic efficiency

description: Ð Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð±ÑÐ» Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÑÐ½Ð¸ÐºÐ¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ Ð¸ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¡ÐÐ± ÐÐÐ£Ð Â«ÐÐ¾ÑÐ¾Ð´ÑÐºÐ°Ñ ÐÐ¾ÐºÑÐ¾Ð²ÑÐºÐ°Ñ Ð±Ð¾Ð»ÑÐ½Ð¸ÑÐ°Â». ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð¾Ð¿ÑÐ¾Ñ ÑÐµÑÐ¿Ð¾Ð½Ð´ÐµÐ½ÑÐ¾Ð² Ñ ÑÐµÐ»ÑÑ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ ÑÐ¿ÑÐ¾ÑÐ° Ð½Ð° Ð¿Ð»Ð°ÑÐ½ÑÐµ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ¸Ðµ ÑÑÐ»ÑÐ³Ð¸. ÐÑÑÐ²Ð»ÐµÐ½Ñ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÑ Ð±Ð¾Ð»ÑÐ½Ð¸ÑÑ, Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÐ½ Ð½Ð° ÑÑÐ´ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ¸Ñ ÑÑÐ»ÑÐ³.
description: The bachelor thesis discusses made analysis of technical - economic index and marketing activity of SPb GBIH "Gorodskaya Pokrovskaya Hospital". In order to study the demand for paid services the questionnaire was done. Main rivals of hospital were revealed, and analysis of prices for some services was made.
Additional file 1 of A brazilian nationwide multicenter study on deficiency of deaminase-2 (DADA2)
Creators: name: Melo, Adriana
name: de Carvalho, Luciana Martins
name: Ferriani, Virginia Paes Leme
name: Cavalcanti, André
name: Appenzeller, Simone
name: Oliveira, Valéria Rossato
name: Neto, Herberto Chong
name: Rosário, Nelson Augusto
name: de Oliveira Poswar, Fabiano
name: Guimaraes, Matheus Xavier
name: Kokron, Cristina Maria
name: Maia, Rayana Elias
name: Silva, Guilherme Diogo
name: Keller, Gabriel
name: Ferreira, Mauricio Domingues
name: Vasconcelos, Dewton Moraes
name: Toledo-Barros, Myrthes Anna Maragna
name: Barros, Samar Freschi
name: Neto, Nilton Salles Rosa
name: Krieger, Marta Helena
name: Kalil, Jorge
name: Mendonça, Leonardo Oliveira
Publisher: name: figshare
Year: 2023
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Supplementary Material 1
Fragmentation of a viscoelastic food by human mastication
Creators: name: Kobayashi, Naoki
name: Kohyama, Kaoru
name: Shiozawa, Kouichi
Publisher: name: arXiv
Year: 2010
Subjects: subject: Data Analysis, Statistics and Probability (physics.data-an)
subject: Soft Condensed Matter (cond-mat.soft)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Pattern Formation and Solitons (nlin.PS)
subject: Biological Physics (physics.bio-ph)
subject: FOS: Physical sciences

description: Fragment-size distributions have been studied experimentally in masticated viscoelastic food (fish sausage).The mastication experiment in seven subjects was examined. We classified the obtained results into two groups, namely, a single lognormal distribution group and a lognormal distribution with exponential tail group. The facts suggest that the individual variability might affect the fragmentation pattern when the food sample has a much more complicated physical property. In particular, the latter result (lognormal distribution with exponential tail) indicates that the fragmentation pattern by human mastication for fish sausage is different from the fragmentation pattern for raw carrot shown in our previous study. The excellent data fitting by the lognormal distribution with exponential tail implies that the fragmentation process has a size-segregation-structure between large and small parts.In order to explain this structure, we propose a mastication model for fish sausage based on stochastic processes.
description: JPSJ3, 4 pages, 8 figures, minor corrections made for publication in J. Phys. Soc. Jpn
title: Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð¼Ð°Ð»Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÑÑÐµÑÑ ÑÑÐ»ÑÐ³ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ ÑÐµÐ¼Ð¾Ð½ÑÑ Ð±ÑÑÐ¾Ð²Ð¾Ð¹ ÑÐµÑ Ð½Ð¸ÐºÐ¸)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð®ÑÑÐµÐ½ÐºÐ¾, ÐÐ»ÑÐ³Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ
Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ°
ÑÑÐµÑÐ° ÑÑÐ»ÑÐ³
ÐºÑÐ¸ÑÐµÑÐ¸Ð¸ Ð¾ÑÐµÐ½ÐºÐ¸
ÑÐ¿ÐµÑÐ¸ÑÐ¸ÐºÐ° ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ
Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ½ÑÑ Ð¿Ð¾Ð·Ð¸ÑÐ¸Ð¹
Ð°Ð½Ð°Ð»Ð¸Ð· Ð±ÐµÐ·ÑÐ±ÑÑÐ¾ÑÐ½Ð¾ÑÑÐ¸
ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ°
ÑÐ¸ÑÐºÐ¸

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð° Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ñ, ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÑÑÐµÑÑ ÑÑÐ»ÑÐ³. ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ñ ÑÐ°ÑÑÐµÑÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ ÑÐµÐ¼Ð¾Ð½ÑÑ Ð±ÑÑÐ¾Ð²Ð¾Ð¹ ÑÐµÑÐ½Ð¸ÐºÐ¸ ÐÐÐ Â«Ð ÑÐ½Ð¾Â». Ð Ð°ÑÑÐ¸ÑÐ°Ð½ ÑÑÐ¾Ðº Ð¿ÑÐ¾ÐµÐºÑÐ°. ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð° Ð¸ Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¸ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð° ÑÐ¾ÑÐºÐ° Ð±ÐµÐ·ÑÐ±ÑÑÐ¾ÑÐ½Ð¾ÑÑÐ¸. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ° Ð¸ Ð¾ÑÐµÐ½ÐºÐ° ÑÐ¸ÑÐºÐ¾Ð². Ð¡Ð´ÐµÐ»Ð°Ð½ Ð²ÑÐ²Ð¾Ð´ Ð¸ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¾Ð± ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¼ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð¿ÑÐ¾ÐµÐºÑÐ° Ð¸ ÑÐ½Ð¸Ð¶ÐµÐ½Ð¸Ñ ÑÐ¸ÑÐºÐ¾Ð² Ð¿Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð² ÑÐµÐ»Ð¾Ð¼.
Il rapporto 3 a 2 fa il buco nero intermedio
Creators: Francesco Rea
Publisher: name: Media Inaf
Year: 2015

Esiste una via di mezzo tra i buchi neri di poche masse solari e i supermassicci delle dimensioni di milioni di miliardi di masse solari già conosciuti dagli astronomi? I ricercatori pensano di si, ma con qualche dubbio che illustrammo qualche anno fa su Media INAF (Il buco nero medio non esiste?). Esistono una mezza dozzina di possibili candidati, ma non si è ancora certi. Un team di astronomi della Università del Maryland e del Goddard Institute della NASA pensa di aver trovato un nuovo candidato ad esser classificato come buco nero intermedio, grande circa 5000 masse solari
Water relations in the Douglas-fir region on Vancouver Island
Creators: name: McMinn, Robert Gordon
Publisher: name: University of British Columbia
Year: 2012

description: In an evaluation of the role of water relations in forest distribution and growth in the Douglas-fir region on Vancouver Island, a section of the Nanaimo River Valley, lying from five to twelve miles inland from the east coast, was chosen as a suitable study area to exemplify conditions in the central mountains and on the eastern side of southern Vancouver Island. The study was conducted in mature stands typical of the principal forest associations found within the range of climates, topographies and soils represented in this area. The vegetation and soils of twenty-four, quarter-acre plots were analysed in order to characterize stands and relate such characteristics to the influence of water relations. The soil moisture regimes and microclimates of each plot were defined by measuring soil moisture levels, precipitation beneath the tree canopy, evaporation rates and soil and air temperatures. Variation in soil moisture contents was followed over a thirty-month period from July, 1951 to November, 1953, and precipitation and maximum/minimum temperatures at various open stations were measured at monthly intervals from June, 1951 until December, 1956 in order to delineate climatic variations within the study area. It was concluded that variation in soil moisture regimes was a most significant factor in the differentiation of sites. In moist, relatively nutritive soils Pseudotsuga menziesii so completely dominated Tsuga heterophylla that the latter species was restricted to the secondary canopy and formed only a small proportion of stand volume. In strongly leached soils, the growth of Pseudotsuga and Tsuga was impaired, so that trees of both species were smaller than in more nutritive soils. Where strongly leached soils were moist throughout the growing season, Tsuga could compete with Pseudotsuga on nearly equal terms and both species reached the upper tree canopy. In droughty, leached soils the growth of Tsuga was more impaired than the growth of Pseudotsuga. and Tsuga formed small to negligible proportions of stand volume. Thuja plicata appeared in the upper tree canopy only on moist to very wet, relatively nutritive sites. The dominant influence in the geographical location of the Douglas-fir region on Vancouver Island appears to be its rainshadow climate. Within this region of low summer rainfall Pseudotsuga can dominate other species on nearly all sites. In wetter climates, outside pronounced rainshadow areas, stands dominated by Pseudotsuga are evidently confined to moist, relatively nutritive sites. Within the different climatic areas encountered, topographic position and concomitant climatic and edaphic influences would seem largely responsible for site differentiation. Such site differentiation followed a definite catenary sequence, which regulated the sequence of forest associations on hillsides. Differences in local topography, aspect, parent material, soil texture and soil depth, however, may cause variation from the typical arrangements.
title: ÐÐ·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ðµ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¸ ÑÑÐ¸Ð´Ð¸ÑÐµÑÐºÐ¸Ñ Ð½Ð¾ÑÐ¼ Ð² Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¼ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²Ðµ
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ»Ð°Ð´ÐºÐ¾Ð², ÐÐ½ÑÐ¾Ð½
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»Ð¸ÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ¸ÑÑÐµÐ¼Ð°
Ð¿Ð¾Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð½Ð¾ÑÐ¼Ñ
ÑÑÐ¸Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ Ð½Ð¾ÑÐ¼Ñ
Ð²Ð½ÑÑÑÐµÐ½Ð½ÑÑ Ð¿ÑÐ¸ÑÐ¾Ð´Ð° Ð¿Ð¾Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð½Ð¾ÑÐ¼
Ñ Ð°ÑÐ°ÐºÑÐµÑ Ð¸ ÑÐ¿ÐµÑÐ¸ÑÐ¸ÐºÐ° ÑÑÐ¸Ð´Ð¸ÑÐµÑÐºÐ¸Ñ Ð½Ð¾ÑÐ¼

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ðµ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¸ ÑÑÐ¸Ð´Ð¸ÑÐµÑÐºÐ¸Ñ Ð½Ð¾ÑÐ¼ Ð² ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¼ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²Ðµ. Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¸ ÑÑÐ¸Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ Ð½Ð¾ÑÐ¼Ñ, Ð¸Ñ Ð²Ð·Ð°Ð¸Ð¼Ð½Ð¾Ðµ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð½Ð° ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²Ð°. ÐÑÐ¾Ð²Ð¾Ð´Ð¸ÑÑÑ Ð°Ð½Ð°Ð»Ð¸Ð· Ð·Ð°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÑÑÐ²Ð°, ÑÐ²ÑÐ·Ð°Ð½Ð½Ð¾Ð³Ð¾ Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ð¼Ð¸ Ð¸ ÑÑÐ¸Ð´Ð¸ÑÐµÑÐºÐ¸Ð¼Ð¸ Ð½Ð¾ÑÐ¼Ð°Ð¼Ð¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¸ÑÑÐ»ÐµÐ´ÑÑÑÑÑ Ð¼Ð½ÐµÐ½Ð¸Ñ ÑÑÐµÐ½ÑÑ Ð¸ ÑÐµÐ¾ÑÐµÑÐ¸ÐºÐ¾Ð².
Quella rara fusione di buchi neri
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2015

Le coppie di buchi neri supermassicci all’interno delle galassie di grande massa sembrano essere più rare di quanto si pensasse fino ad ora. Uno studio condotto analizzando 100 galassie nelle onde radio ha svelato un tasso di fusioni pari a un quinto delle stime precedenti
The Complete Initial Mass Function Down to the Sub-Solar Regime in the Large Magellanic Cloud with Hubble Space Telescope ACS Observations
Creators: name: Da Rio, Nicola
name: Gouliermis, Dimitrios
name: Henning, Thomas
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: In this photometric study of the stellar association LH 95 in the Large Magellanic Cloud (LMC) we focus on the pre-main Sequence (PMS) population in order to construct, for the first time, the sub-solar initial mass function (IMF) in the LMC. We use the deepest photometry ever performed in the LMC with the Advanced Camera for Surveys (ACS) on-board the Hubble Space Telescope(HST). We carry out a Monte Carlo technique to subtract the contribution of the general field of LMC and we isolate the central region in the observed area of the association. We study the mass function of its field-subtracted population. For this purpose, we introduce a new set of evolutionary models, derived from the calculations on the evolution of PMS stars by Siess et al. We use these models with our observations of LH 95 to derive the IMF of the system, which is reliably constructed down to 0.43 M_sun, the lowest mass ever observed within reasonable completeness in the Magellanic Clouds. Consequently, its construction offers an outstanding improvement in our understanding of the low-mass star formation in the LMC. The system IMF of LH 95 shows a definite change in its slope at 1 M_sun, where it becomes more shallow. In general, the shape of this IMF agrees very well with the average Galactic IMF, down to the sub-solar regime. As far as the slope of this system IMF is concerned, it is found to be somewhat more shallow than the corresponding classical Galactic IMF in the sub-solar regime, probably due to unresolved binarity, while for stars with M>1M_sun it becomes slightly steeper. We do not find significant differences in the shape of the overall IMF of LH 95 from that of each of the three individual sub-clusters, suggesting that the IMF of LH 95 is not subject to local variability.
description: 19 pages, 13 figures. Accepted for publication to ApJ
title: Life cycle management of it products based on agile methodologies
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
title: ÐÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ Ð³Ð¸Ð±ÐºÐ¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð² ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¸ Ð¶Ð¸Ð·Ð½ÐµÐ½Ð½ÑÐ¼ ÑÐ¸ÐºÐ»Ð¾Ð¼ ÐÐ¢-Ð¿ÑÐ¾Ð´ÑÐºÑÐ¾Ð²
Creators: name: Abdelwahab, Mahmoud
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Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸
Ð³Ð¸Ð±ÐºÐ¾Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾Ð´ÑÐºÑÐ°Ð¼Ð¸
Ð¶Ð¸Ð·Ð½ÐµÐ½Ð½ÑÐ¹ ÑÐ¸ÐºÐ» Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ
Ð¿Ð¾ÑÑÐµÐ±Ð½Ð¾ÑÑÐ¸ ÐºÐ»Ð¸ÐµÐ½ÑÐ¾Ð²
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description: The target of this study is to find out the main role of software product managers and how they are leading and managing their software products in an easy way that can be understudied for nontechnical people.The Thesis is divided into five chapters. The first chapter is introduction and contain the research questions, however the second, third and fourth are focusing on the importance of managing products, client needs and product planning, While the last chapter is considered an sum up for what i have noticed personally during a real experience in company based in St. Petersburg and how the product management process looks like inside out.
description: Ð¦ÐµÐ»ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐµÐ¹ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸ÐµÐ¼ Ð¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸ÐµÐ¼ ÐÐ¢-Ð¿ÑÐ¾Ð´ÑÐºÑÐ°Ð¼Ð¸ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¼ÐµÑÐ¾Ð´Ð¾Ð»Ð¾Ð³Ð¸Ð¸ agile. ÐÐ¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ ÑÐ¾ÑÑÐ¾Ð¸Ñ Ð¸Ð· Ð¿ÑÑÐ¸ Ð³Ð»Ð°Ð². ÐÐµÑÐ²Ð°Ñ Ð³Ð»Ð°Ð²Ð° Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÑÐµÑ ÑÐ¾Ð±Ð¾Ð¹ Ð²Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ, Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð°ÐºÑÑÐ°Ð»ÑÐ½Ð¾ÑÑÐ¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð¿Ð¾ÑÑÐ°Ð½Ð¾Ð²ÐºÑ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ. ÐÑÐ¾ÑÐ°Ñ, ÑÑÐµÑÑÑ Ð¸ ÑÐµÑÐ²ÐµÑÑÐ°Ñ Ð³Ð»Ð°Ð²Ñ ÑÐ¾ÐºÑÑÐ¸ÑÑÑÑÑÑ Ð½Ð° Ð²Ð°Ð¶Ð½Ð¾ÑÑÐ¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÐÐ¢-Ð¿ÑÐ¾Ð´ÑÐºÑÐ°Ð¼Ð¸, Ð¿Ð¾ÑÑÐµÐ±Ð½Ð¾ÑÑÑÑ ÐºÐ»Ð¸ÐµÐ½ÑÐ¾Ð² Ð¸ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ ÐÐ¢-Ð¿ÑÐ¾Ð´ÑÐºÑÐ°. ÐÐ¾ÑÐ»ÐµÐ´Ð½ÑÑ Ð³Ð»Ð°Ð²Ð° - ÑÑÐ¾ Ð¿Ð¾Ð´Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð¸ÑÐ¾Ð³Ð¾Ð² ÑÐ¾Ð³Ð¾, ÑÑÐ¾ Ð°Ð²ÑÐ¾ÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð±ÑÐ»Ð¾ Ð²ÑÑÐ²Ð»ÐµÐ½Ð¾ Ð²Ð¾ Ð²ÑÐµÐ¼Ñ ÑÐ°Ð±Ð¾ÑÑ Ð² ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸, Ð½Ð°ÑÐ¾Ð´ÑÑÐµÐ¹ÑÑ Ð² Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ðµ, Ð¸ ÐºÐ°Ðº Ð¿ÑÐ¾ÑÐµÑÑ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¾Ð¼ Ð²ÑÐ³Ð»ÑÐ´Ð¸Ñ Ð¸Ð·Ð½ÑÑÑÐ¸.
Eucys 2015: la sfida dei giovani scienziati
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2015

Il concorso per la seconda volta si è svolto a Milano, dopo l'edizione del 1997. Tanti i progetti in lizza e a giudicarli anche una nostra astronoma dell'INAF-Osservatorio Astronomico di Padova, Lina Tomasella, che ha presieduto la giuria
Is the United States losing ground in science? A global perspective on the world science system
Creators: name: Leydesdorff, Loet
name: Wagner, Caroline
Publisher: name: arXiv
Year: 2009
Subjects: subject: Physics and Society (physics.soc-ph)
subject: FOS: Physical sciences

description: Based on the Science Citation IndexExpanded webversion, the USA is still by far the strongest nation in terms of scientific performance. Its relative decline in percentage share of publications is largely due to the emergence of China and other Asian nations. In 2006, China has become the second largest nation in terms of the number of publications within this database. In terms of citations, the competitive advantage of the American domestic market is diminished, while the European Union EU is profiting more from the enlargement of the database over time than the US. However, the USA is still outperforming all other countries in terms of highly cited papers and citationpublication ratios, and it is more successful than the EU in coordinating its research efforts in strategic priority areas like nanotechnology. In this field, the Peoples Republic of China PRC has become second largest nation in both numbers of papers published and citations behind the USA.
Water in Comets 71P/Clark and C/2004 B1 (LINEAR) with Spitzer
Creators: name: Bockelee-Morvan, Dominique
name: Woodward, Charles E.
name: Kelley, Michael S.
name: Wooden, Diane H.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We present 5.5 to 7.6 micron spectra of comets 71P/Clark (2006 May 27.56 UT, r_h = 1.57 AU pre-perihelion) and C/2004 B1 (LINEAR) (2005 October 15.22 UT, r_h = 2.21 AU pre-perihelion and 2006 May 16.22 UT, r_h = 2.06 AU post-perihelion) obtained with the Spitzer Space Telescope. The nu_2 vibrational band of water is detected with a signal-to-noise ratio of 11 to 50. Fitting the spectra using a fluorescence model of water emission yields a water rotational temperature of < 18 K for 71P/Clark and approximately less than or equivalent to 14 +/- 2 K (pre-perihelion) and 23 +/- 4 K (post-perihelion) for C/2004 B1 (LINEAR). The water ortho-to-para ratio in C/2004 B1 (LINEAR) is measured to be 2.31 +/- 0.18, which corresponds to a spin temperature of 26^{+3}_{-2} K. Water production rates are derived. The agreement between the water model and the measurements is good, as previously found for Spitzer spectra of C/2003 K4 (LINEAR). The Spitzer spectra of these three comets do not show any evidence for emission from PAHs and carbonate minerals, in contrast to results reported for comets 9P/Tempel~1 and C/1995 O1 (Hale-Bopp).
description: 16 pages, 1 table, 7 figures, ApJ accepted 2009
title: ÐÐ»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ ÐºÑÑÐ³Ð¾Ð²Ð¾Ð³Ð¾ Ð¾Ð±Ð·Ð¾ÑÐ° Ð´Ð»Ñ Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½ÑÑ ÑÐ¾Ð±Ð¾ÑÐ¾ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ¸Ñ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ¾Ð²
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Ð°ÑÐ»Ð°ÑÐ¸Ð½, ÐÐ¸ÐºÑÐ¾Ñ
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±Ð¾ÑÐ¾ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ
Ð Ð°ÑÐ¿Ð¾Ð·Ð½Ð°Ð²Ð°Ð½Ð¸Ðµ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²
ÐÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¼Ð°ÑÐ¸Ð½Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐµ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»ÑÐ½ÑÐµ
ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ðµ Ð·ÑÐµÐ½Ð¸Ðµ
Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½ÑÐµ ÑÐ¾Ð±Ð¾ÑÑ

description: ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð¾ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ðµ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ðµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ Ð°Ð´ÐµÐºÐ²Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð²Ð¾ÑÐ¿ÑÐ¸ÑÑÐ¸Ñ Ð¾Ð¿ÐµÑÐ°ÑÐ¾ÑÐ¾Ð¼ ÑÑÐµÐ´Ñ, Ð¾ÐºÑÑÐ¶Ð°ÑÑÐµÐ¹ Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐ¾Ð±Ð¾ÑÐ°. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð¾Ð±Ð·Ð¾Ñ ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼ ÐºÑÑÐ³Ð¾Ð²Ð¾Ð³Ð¾ Ð¾Ð±Ð¾ÑÐ°. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð¼Ð°ÐºÐµÑ ÑÐ¸ÑÑÐµÐ¼Ñ ÐºÑÑÐ³Ð¾Ð²Ð¾Ð³Ð¾ Ð¾Ð±Ð·Ð¾ÑÐ°. ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð°ÑÑÐ¸ÑÐµÐºÑÑÑÑ Ð¸ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ. Ð ÐµÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ð¾ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ Ð´Ð»Ñ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ Ð¿Ð°Ð½Ð¾ÑÐ°Ð¼Ñ ÐºÑÑÐ³Ð¾Ð²Ð¾Ð³Ð¾ Ð¾Ð±Ð·Ð¾ÑÐ°, Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð²Ð¸Ð´Ð° ÑÐ²ÐµÑÑÑ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð¿Ð°Ð½Ð¾ÑÐ°Ð¼Ñ ÐºÑÑÐ³Ð¾Ð²Ð¾Ð³Ð¾ Ð¾Ð±Ð·Ð¾ÑÐ° Ð¸ Ð¼Ð°ÑÑÐ¸Ñ Ð³Ð¾Ð¼Ð¾Ð³ÑÐ°ÑÐ¸Ð¸. Ð ÐµÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ð¾ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ Ð´Ð»Ñ Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ ÑÐ°ÐºÑÑÑÐ° Ð½Ð°Ð±Ð»ÑÐ´ÐµÐ½Ð¸Ñ ÑÑÐµÐ½Ñ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð¸Ð³ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð´Ð²Ð¸Ð¶ÐºÐ° Unity. ÐÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ñ Ð¼ÐµÑÐ¾Ð´Ñ Ð´Ð¾Ð¿Ð¾Ð»Ð½ÐµÐ½Ð½Ð¾Ð¹ ÑÐµÐ°Ð»ÑÐ½Ð¾ÑÑÐ¸ Ð´Ð»Ñ ÑÐ¾Ð²Ð¼ÐµÑÐµÐ½Ð¸Ñ Ð²Ð¸ÑÑÑÐ°Ð»ÑÐ½Ð¾Ð¹ Ð¼Ð¾Ð´ÐµÐ»Ð¸ ÑÐ¾Ð±Ð¾ÑÐ° Ñ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÐ¼Ð¸ Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸ÑÐ¼Ð¸.
Thermodynamics of Black Holes in Horava-Lifshitz Gravity
Creators: name: Cai, Rong-Gen
name: Cao, Li-Ming
name: Ohta, Nobuyoshi
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: By using the canonical Hamiltonian method, we obtain the mass and entropy of the black holes with general dynamical coupling constant $λ$ in Hoř ava-Lifshitz Gravity. Regardless of whether the horizon is sphere, plane or hyperboloid, we find these black holes are thermodynamically stable in some parameter space and unstable phase also exists in other parameter space. The relation between the entropy and horizon area of the black holes has an additional coefficient depending on the coupling constant $λ$, compared to the $λ=1$ case. For $λ=1$, the well-known coefficient of one quarter is recovered in the infrared region.
description: Latex, 13 pages, 3 figures, v2: two references added,v3: discussion and references added, accepted by Phys.Lett.B
Additional file 2 of Building an inpatient addiction medicine consult service in Sudbury, Canada: preliminary data and lessons learned in the era of COVID-19
Creators: name: Leary, Tara
name: Aubin, Natalie
name: Marsh, David C.
name: Roach, Michael
name: Nikodem, Paola
name: Caswell, Joseph M.
name: Irwin, Bridget
name: Pillsworth, Emma
name: Mclelland, Maureen
name: Long, Brad
name: Bhagavatula, Sastry
name: Eibl, Joseph K
name: Morin, Kristen A.
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Supplementary Material 2
Resolution Trees with Lemmas: Resolution Refinements that Characterize DLL Algorithms with Clause Learning
Creators: name: Buss, Samuel R.
name: Hoffmann, Jan
name: Johannsen, Jan
Publisher: name: arXiv
Year: 2008
Subjects: subject: Logic in Computer Science (cs.LO)
subject: Computational Complexity (cs.CC)
subject: FOS: Computer and information sciences
subject: F.2.2; I.2.8

description: Resolution refinements called w-resolution trees with lemmas (WRTL) and with input lemmas (WRTI) are introduced. Dag-like resolution is equivalent to both WRTL and WRTI when there is no regularity condition. For regular proofs, an exponential separation between regular dag-like resolution and both regular WRTL and regular WRTI is given. It is proved that DLL proof search algorithms that use clause learning based on unit propagation can be polynomially simulated by regular WRTI. More generally, non-greedy DLL algorithms with learning by unit propagation are equivalent to regular WRTI. A general form of clause learning, called DLL-Learn, is defined that is equivalent to regular WRTL. A variable extension method is used to give simulations of resolution by regular WRTI, using a simplified form of proof trace extensions. DLL-Learn and non-greedy DLL algorithms with learning by unit propagation can use variable extensions to simulate general resolution without doing restarts. Finally, an exponential lower bound for WRTL where the lemmas are restricted to short clauses is shown.
title: ÐÐ»Ð³Ð¾ÑÐ¸ÑÐ¼ Ð¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð°Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð¼ÐµÑÐ¾Ð´Ð° ÑÐµÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÑ Ð¸ Ð¿Ð»Ð¾ÑÐ½Ð¾ÑÑÐ¸ Ð¿Ð»Ð°Ð·Ð¼Ñ Ð¿Ð¾ Ñ Ð¾ÑÐ´Ð¾Ð²ÑÐ¼ Ð¸Ð·Ð¼ÐµÑÐµÐ½Ð¸ÑÐ¼ Ð½Ð° ÑÐ¾ÐºÐ°Ð¼Ð°Ðº Â«ÐÐ»Ð¾Ð±ÑÑ-ÐÂ» Ð² ÑÐºÐ²Ð°ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð¹ Ð¿Ð»Ð¾ÑÐºÐ¾ÑÑÐ¸ Ñ ÑÑÐµÑÐ¾Ð¼ ÐºÐ¾Ð½ÐµÑÐ½Ð¾ÑÑÐ¸ ÐºÐ¾Ð½ÑÑÐ°
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¤ÐµÐ¾ÑÐ¸Ð»Ð°ÐºÑÐ¾Ð², ÐÐ¸ÑÐ°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: 2018
Subjects: ÑÐ¾ÐºÐ°Ð¼Ð°Ðº
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Ð¸Ð½ÑÐµÑÐ²Ð°Ð»ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð·
Ð´Ð¾Ð¿ÑÑÐºÐ¾Ð²Ð¾Ðµ Ð¼Ð½Ð¾Ð¶ÐµÑÑÐ²Ð¾ ÑÐµÑÐµÐ½Ð¸Ð¹
Ð¾Ð±ÑÐµÐ´Ð¸Ð½ÐµÐ½Ð½Ð¾Ðµ Ð¼Ð½Ð¾Ð¶ÐµÑÑÐ²Ð¾ ÑÐµÑÐµÐ½Ð¸Ð¹

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ ÑÐºÐ²Ð°ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ðµ ÑÐµÑÐµÐ½Ð¸Ðµ ÑÐ¾ÐºÐ°Ð¼Ð°ÐºÐ° Â«ÐÐ»Ð¾Ð±ÑÑ-ÐÂ», Ð² ÐºÐ¾ÑÐ¾ÑÐ¾Ð¹ Ð¸Ð·ÑÑÐ°ÑÑÑÑ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° Ð¿Ð»Ð°Ð·Ð¼Ñ. ÐÑÐ½Ð¾Ð²Ð½Ð°Ñ Ð¸Ð´ÐµÑ ÑÐ¾ÑÑÐ¾Ð¸Ñ Ð² Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ð¸ ÐºÐ¾Ð½ÑÑÐ¾Ð² Ð½Ð°Ð±Ð»ÑÐ´ÐµÐ½Ð¸Ð¹, Ð¿ÐµÑÐµÑÐµÐºÐ°ÑÑÐ¸Ñ ÑÐ°ÑÑÐµÑÐ½ÑÐµ Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐ¸ Ð¿Ð»Ð°Ð·Ð¼Ñ Ð² ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐµ. ÐÐ¾ Ð´Ð°Ð½Ð½ÑÐ¼ Ð³ÐµÐ¾Ð¼ÐµÑÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð²ÑÑÐ¸ÑÐ»ÐµÐ½Ð¸Ð¹ ÑÑÑÐ¾Ð¸ÑÑÑ Ð¸Ð½ÑÐµÑÐ²Ð°Ð»ÑÐ½Ð¾ Ð·Ð°Ð´Ð°Ð½Ð½Ð°Ñ Ð¼Ð°ÑÑÐ¸ÑÐ° Ð¸ ÑÐµÑÐ°ÐµÑÑÑ Ð¾Ð±ÑÐ°ÑÐ½Ð°Ñ Ð·Ð°Ð´Ð°ÑÐ° ÑÐµÐ½ÑÐ³ÐµÐ½Ð¾Ð²ÑÐºÐ¾Ð¹ ÑÐ¼Ð¸ÑÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ¾Ð¼Ð¾Ð³ÑÐ°ÑÐ¸Ð¸ Ð¿Ð»Ð°Ð·Ð¼Ñ. ÐÐ°Ð»ÐµÐµ Ð¿ÑÐ¸Ð¼ÐµÐ½ÑÐµÑÑÑ Ð¸Ð½ÑÐµÑÐ²Ð°Ð»ÑÐ½Ð°Ñ ÑÐµÐ³ÑÐ»ÑÑÐ¸Ð·Ð°ÑÐ¸Ñ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÐ°ÑÐ¿Ð¾Ð·Ð½Ð°ÑÑÐµÐ³Ð¾ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»Ð°. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¾Ð¿ÑÐ¸Ð¼ÑÐ¼Ð° ÑÑÑÐ¾Ð¸ÑÑÑ Ð¼Ð¾Ð´ÐµÐ»Ñ ÑÐ¼Ð¸ÑÑÐ¸Ð¸ Ð¿Ð»Ð°Ð·Ð¼Ñ.
Compactness of Cold Gas in High-Redshift Galaxies
Creators: name: Obreschkow, Danail
name: Rawlings, Steve
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Galaxies in the early Universe were more compact and contained more molecular gas than today. In this paper, we revisit the relation between these empirical findings, and we quantitatively predict the cosmic evolution of the surface densities of atomic (HI) and molecular (H2) hydrogen in regular galaxies. Our method uses a pressure-based model for the H2/HI-ratio of the Interstellar Medium, applied to ~3*10^7 virtual galaxies in the Millennium Simulation. We predict that, on average, the HI-surface density of these galaxies saturates at Sigma_HI<10 Msun/pc^2 at all redshifts (z), while H2-surface densities evolve dramatically as Sigma_H2(1+z)^2.4. This scaling is dominated by a (1+z)^2 surface brightness scaling originating from the (1+z)^-1 size scaling of galaxies at high z. Current measurements of Sigma_H2 at high z, derived from CO-observations, tend to have even higher values, which can be quantitatively explained by a selection bias towards merging systems. However, despite the consistency between our high-z predictions and the sparse empirical data, we emphasize that the empirical data potentially suffer from serious selection biases and that the semi-analytic models remain in many regards uncertain. As a case study, we investigate the cosmic evolution of simulated galaxies, which resemble the Milky Way at z=0. We explicitly predict their HI- and H2-distribution at z=1.5, corresponding to the CO-detected galaxy BzK-21000, and at z=3, corresponding to the primary science goal of the Atacama Large Millimeter/submillimeter Array (ALMA).
description: 5 pages, 3 figures, 2 tables
Additional file 1 of Does adjuvant hepatic artery infusion chemotherapy improve patient outcomes for hepatocellular carcinoma following liver resection? A meta-analysis
Creators: name: Hu, Lingbo
name: Zheng, Yu
name: Lin, Jiangyin
name: Shi, Xingpeng
name: Wang, Aidong
Publisher: name: figshare
Year: 2023
Subjects: subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Cancer

description: Additional file 1: Supplementary materials 1. Search strategy. Supplementary materials 2. The differences of included studies between our and previous studies. Supplementary materials 3. Risk assessment of RCTs. Supplementary materials 4. Plot of publication bias. Supplementary materials 5. Plot of sensitivity analysis. Supplementary materials 6. Plot of OS and DFS after omitting some studies. Supplementary materials 7. GRADE analysis of OS and DFS in the HAIC group.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ ÑÐ°ÑÑÐµÑÐ° Ð¿Ð¾ÑÐµÑÑ Ð² Ð¼Ð¾ÑÐ½ÑÑ ÑÐ¾ÑÐ¾Ð¸Ð´Ð°Ð»ÑÐ½ÑÑ ÑÑÐ°Ð½ÑÑÐ¾ÑÐ¼Ð°ÑÐ¾ÑÐ°Ñ , Ð²Ñ Ð¾Ð´ÑÑÐ¸Ñ Ð² ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÑ Ð´Ð»Ñ ÐºÐ¾Ð½ÑÐ°ÐºÑÐ½Ð¾Ð¹ ÑÐ²Ð°ÑÐºÐ¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ°Ð»ÑÐ½ÑÑ Ð³Ð°Ð·Ð¾Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¾Ð²
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: Ð ÐµÐ·Ð¸Ð½ÐºÐ¸Ð½, ÐÐ½ÑÐ¾Ð½
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: Ð­Ð»ÐµÐºÑÑÐ¾ÑÐ²Ð°ÑÐºÐ° ÐºÐ¾Ð½ÑÐ°ÐºÑÐ½Ð°Ñ ÑÑÑÐºÐ¾Ð²Ð°Ñ
Ð¢ÑÐ°Ð½ÑÑÐ¾ÑÐ¼Ð°ÑÐ¾ÑÑ ÑÐ¾ÑÐ¾Ð¸Ð´Ð°Ð»ÑÐ½ÑÐµ

description: Ð Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸ Ð¾Ð¿Ð¸ÑÐ°Ð½Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÐºÐ¾Ð½ÑÐ°ÐºÑÐ½Ð¾Ð¹ ÑÑÑÐºÐ¾Ð²Ð¾Ð¹ ÑÐ²Ð°ÑÐºÐ¸ Ð¾Ð¿Ð»Ð°Ð²Ð»ÐµÐ½Ð¸ÐµÐ¼, Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿ ÑÐ°Ð±Ð¾ÑÑ ÑÐ¾ÑÐ¾Ð¸Ð´Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°Ð½ÑÑÐ¾ÑÐ¼Ð°ÑÐ¾ÑÐ°, ÑÐµÐ»Ð¸, Ð·Ð°Ð´Ð°ÑÐ¸ ÑÐ°ÑÑÐµÑÐ° Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð², ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ñ, Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð´Ð»Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼ ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¸Ðº ÑÐ°ÑÑÐµÑÐ°. ÐÐ° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐ¡Ð¡-04 Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½ ÑÐ°ÑÑÐµÑ Ð¿Ð¾ÑÐµÑÑ ÑÑÐ°Ð½ÑÑÐ¾ÑÐ¼Ð°ÑÐ¾ÑÐ°, ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÑÐ°Ð¿Ñ ÑÐ°ÑÑÐµÑÐ° ÑÐ»ÐµÐºÑÑÐ¾Ð¼Ð°Ð³Ð½Ð¸ÑÐ½ÑÑ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² Ð² Ð½ÑÐ¼ Ð¿ÑÐ¸ Ð¿Ð¾Ð¼Ð¾ÑÐ¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½ÑÑ Ð¿Ð°ÐºÐµÑÐ¾Ð² ELCUT Ð¸ COMSOL, Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð´Ð°Ð½Ð½ÑÑ ÑÐ°ÑÑÑÑÐ¾Ð² Ð¿ÑÐ¾Ð´ÐµÐ¼Ð¾Ð½ÑÑÑÐ¸ÑÐ¾Ð²Ð°Ð½ ÐºÐ¾ÑÑÑÐ¸ÑÐ¸ÐµÐ½Ñ Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐ½Ð¾Ð³Ð¾ ÑÑÑÐµÐºÑÐ°, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐµÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½ ÑÐ°ÑÑÐµÑ 3D-Ð¼Ð¾Ð´ÐµÐ»Ð¸ ÑÐ¸Ð½ Ð² Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð¼ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ð¸ COMSOL.
The X-ray View of Abell 3120
Creators: name: Henriksen, Mark
name: Finoguenov, Alexis
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Identification of Abell 3120 as a galaxy cluster has recently been questioned with alternative suggestions including: a fossil remnant of a group merger, non-thermal emission from a radio galaxy, and projected emission from of a filamentary string of galaxies. We report on our analysis of the Chandra observation and evaluate these hypotheses based on our results. Abell 3120 shows X-ray emission extending 158 kpc, well beyond the central galaxy. The spatial distribution of X-rays in the core more closely follows the radio emission showing a jet-like structure extending to the north that is misaligned with the stellar light distribution of the central galaxy. At larger radii the X-ray emission is aligned with the SE-NW running axis of the galaxy distribution in the cluster core. Modeling the X-ray spectrum excludes purely non-thermal emission. The emission weighted temperature is 1.93 - 2.19 keV and the 0.3 - 10 keV luminosity is 1.23$\times10^{43}$ ergs s$^{-1}$. Abell 3120 appears to be a poor cluster with Virgo and MKW 4 as peers. The best fitting model consists of a thermal component and a second component that may be either thermal or non-thermal, with luminosity 25% of the total X-ray luminosity. While, a more detailed spatial-spectral search failed to detect a central AGN, there is some evidence for an extended hard X-ray component. Cooler gas, 1.28 - 1.80 was detected in the central 20 kpc. The second thermal component marginally requires a higher redshift, >0.12, which may be due to a second cluster in the rich surrounding environment consisting of nearly a thousand catalogued galaxies.
description: 15 pages, 8 figures
La nuova era della Cina in SKA
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2015

Il governo cinese ha di recente firmato una lettera d'intenti con la SKA Organisation affermando ufficialmente di voler iniziare le negoziazioni con le altre nazioni. La Cina si unisce a un gruppo ristretto di 6 nazioni (Australia, Italia, Olanda, Nuova Zelanda, Sudafrica e Regno Unito) che si occupano della trasformazione di SKA in un’organizzazione intergovernativa (IGO)
title: Ð Ð°Ð·Ð²Ð¸ÑÐ¸Ðµ ÐºÑÐµÐ°ÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¿Ð¾ÑÑÐµÐ´ÑÑÐ²Ð¾Ð¼ Ð½Ð°Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ ÐºÐ¾Ð¼Ð¸ÐºÑÐ¾Ð² Ð½Ð° ÑÑÐ¾ÐºÐ°Ñ Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð³Ð¾ ÑÐ·ÑÐºÐ°
title: Developing creativity through writing comics at the lessons of english
Creators: name: ÐÐ°ÑÐºÐ°ÐºÐ¾Ð²Ð°, ÐÐ°ÑÐ¸Ñ
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2022
Subjects: Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¸Ð¹ ÑÐ·ÑÐº

description: Ð Ð¿ÑÐ¾ÑÐµÑÑÐµ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð²Ð½Ð¾Ð¹ ÐºÐ¾Ð¼Ð¿ÐµÑÐµÐ½ÑÐ¸Ð¸ Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»Ñ Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½Ð¾Ð³Ð¾ ÑÐ·ÑÐºÐ° Ð²ÑÐ±Ð¸ÑÐ°ÐµÑ ÑÐ°Ð·Ð½ÑÐµ Ð¼ÐµÑÐ¾Ð´Ñ, ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸, Ð¿ÑÐ¸ÐµÐ¼Ñ Ð¸ ÑÑÐµÐ´ÑÑÐ²Ð° Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ. ÐÐµÑÐ¾Ð´ ÐºÑÐµÐ°ÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð¿Ð¸ÑÑÐ¼Ð° ÑÐ²Ð»ÑÐµÑÑÑ Ð¾Ð´Ð½Ð¸Ð¼ Ð¸Ð· Ð°ÐºÑÐ¸Ð²Ð½ÑÑ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ, ÐºÐ¾ÑÐ¾ÑÑÐ¹ Ð²ÑÐ·ÑÐ²Ð°ÐµÑ Ð¸Ð½ÑÐµÑÐµÑ Ñ Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ ÑÑÐ°ÑÑÐ¸Ñ ÐºÐ»Ð°ÑÑÐ¾Ð² Ð¸ Ð½Ð°ÑÐ¾Ð´Ð¸Ñ ÑÐ¼Ð¾ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐ¹ Ð¾ÑÐºÐ»Ð¸Ðº. ÐÐ¾Ð´ ÐºÑÐµÐ°ÑÐ¸Ð²Ð½Ð¾Ð¹ Ð¿Ð¸ÑÑÐ¼ÐµÐ½Ð½Ð¾Ð¹ ÑÐµÑÑÑ Ð¿Ð¾Ð½Ð¸Ð¼Ð°ÐµÑÑÑ Ð¿Ð¸ÑÑÐ¼ÐµÐ½Ð½Ð°Ñ ÑÐµÑÑ, Ð² ÐºÐ¾ÑÐ¾ÑÐ¾Ð¹ Ð¿ÑÐ¾ÑÐ²Ð»ÑÑÑÑÑ Ð½ÐµÑÑÐ°Ð½Ð´Ð°ÑÑÐ½ÑÐµ Ð·Ð°Ð´Ð°ÑÐ¸, ÑÐ¾Ð¾ÑÐ½ÐµÑÐµÐ½Ð½ÑÐµ Ñ ÑÐµÑÐµÐ½Ð¸ÐµÐ¼ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð²Ð½Ð¾Ð¹ Ð·Ð°Ð´Ð°ÑÐ¸, Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÐ°Ð½ÑÐ°Ð·Ð¸Ð¸, Ð²Ð¾Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ñ, Ð»Ð¸ÑÐ½Ð¾Ð³Ð¾ Ð¾Ð¿ÑÑÐ°, Ð° ÑÐ°ÐºÐ¶Ðµ Ð°ÑÑÐ¾ÑÐ¸Ð°ÑÐ¸Ð¸ Ð¿Ð¾ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐµÐ¼Ðµ.
title: Immutable Log Storage as a Service
Creators: name: Pourmajidi, William
name: Zhang, Lei
name: Steinbacher, John
name: Erwin, Tony
name: Miranskyy, Andriy
Publisher: name: IEEE
Year: 2019
Subjects: subject: Blockchain, Hierarchical Ledger, bitcoin, privacy, log systems, Cloud log systems Log tampering, Log storage, Ethereum

description:  2019 IEEE/ACM 41st International Conference on Software Engineering: Companion Proceedings (ICSE-Companion)
description: Logs contain critical information about the quality of the rendered services on the Cloud and can be used as digital evidence. Hence, we argue that the critical nature of logs calls for immutability and verification mechanism without a presence of a single trusted party. In this paper, we propose a blockchain-based log system, called Logchain, which can be integrated with existing private and public blockchains. To validate the mechanism, we create Logchain as a Service (LCaaS) by integrating it with Ethereum public blockchain network. We show that the solution is scalable (being able to process 100 log files per second) and fast (being able to "seal" a log file in 23 seconds, on average).
title: ÐÐ½Ð°Ð»Ð¸Ð· ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÑÑÐºÐ¿ÑÐ¾Ð¼Ð³Ð°Ð·Â»)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÑÐ³Ð°Ð»Ð¸ÐµÐ², ÐÐ¼Ð¸ÑÑÐ°Ð½
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°Ð½Ð°Ð»Ð¸Ð· ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð°Ñ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÑ
Ð»Ð¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÑ
Ð¿Ð»Ð°ÑÐµÐ¶ÐµÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÑ
Ð´ÐµÐ»Ð¾Ð²Ð°Ñ Ð°ÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð° Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÑÑÑÐ°ÑÐµÐ³Ð¸Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. ÐÐ°Ð½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ.
Astronomy Fellowships in Italy 2
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2015

Riparte il programma AstroFIt, la ricetta dell’INAF per portare in Italia i migliori ricercatori. Il primo bando del programma AstroFIt2, Astronomy Fellowships in Italy, finanzia nove progetti di ricerca, ciascuno della durata di trentasei mesi
Additional file 3 of Building an inpatient addiction medicine consult service in Sudbury, Canada: preliminary data and lessons learned in the era of COVID-19
Creators: name: Leary, Tara
name: Aubin, Natalie
name: Marsh, David C.
name: Roach, Michael
name: Nikodem, Paola
name: Caswell, Joseph M.
name: Irwin, Bridget
name: Pillsworth, Emma
name: Mclelland, Maureen
name: Long, Brad
name: Bhagavatula, Sastry
name: Eibl, Joseph K
name: Morin, Kristen A.
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Supplementary Material 3
Tuning electronic properties of corrugated graphene: confinement, curvature and band gap opening
Creators: name: Atanasov, Victor
name: Saxena, Avadh
Publisher: name: arXiv
Year: 2010
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: It is shown that for monolayer graphene electrons are confined on a perfect two dimensional surface. The implications for the electronic properties of corrugated graphene are discussed in view of a derivation of the constrained relativistic dynamics for the massless carriers in two dimensions. Surface curvature is related to a series of phenomena with practical applications such as curvature induced p-n junctions, band gap opening and decoherence. We also establish a bending free energy by treating graphene as a soft electronic membrane.
description: 8 pages, 5 figures
Quanti eventi per la Notte dei ricercatori!
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2015

Vi proponiamo un aggiornamento sulle iniziative organizzate dall'INAF per questa settimana e soprattutto per venerdì 25 settembre, tra seminari scientifici, mostre, documentari, laboratori e visite guidate nei Centri di Ricerca. In particolare gli eventi di Roma, Cagliari e Palermo
Lampi radio per mappare l’universo
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2015

Sfruttare gli elusivi lampi radio veloci (FRB) per ricavare la distanza e la distribuzione delle galassie distanti nell'universo. Questa l'idea proposta da due ricercatori della University of British Columbia in Canada. Il commento di Andrea Possenti (INAF)
The redshift and afterglow of the extremely energetic gamma-ray burst GRB 080916C
Creators: name: Greiner, J.
name: Clemens, C.
name: Kruehler, T.
name: Kienlin, A. v.
name: Rau, A.
name: Sari, R.
name: Fox, D. B.
name: Kawai, N.
name: Afonso, P.
name: Ajello, M.
name: Berger, E.
name: Cenko, S. B.
name: Cucchiara, A.
name: Filgas, R.
name: Klose, S.
name: Yoldas, A. Kuepue
name: Lichti, G. G.
name: Loew, S.
name: McBreen, S.
name: Nagayama, T.
name: Rossi, A.
name: Sato, S.
name: Szokoly, G.
name: Yoldas, A.
name: Zhang, X. -L.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The detection of GeV photons from gamma-ray bursts (GRBs) has important consequences for the interpretation and modelling of these most-energetic cosmological explosions. The full exploitation of the high-energy measurements relies, however, on the accurate knowledge of the distance to the events. Here we report on the discovery of the afterglow and subsequent redshift determination of GRB 080916C, the first GRB detected by the Fermi Gamma-Ray Space Telescope with high significance detection of photons at >0.1 GeV. Observations were done with 7-channel imager GROND at the 2.2m MPI/ESO telescope, the SIRIUS instrument at the Nagoya-SAAO 1.4m telescope in South Africa, and the GMOS instrument at Gemini-S. The afterglow photometric redshift of z=4.35+-0.15, based on simultaneous 7-filter observations with the Gamma-Ray Optical and Near-infrared Detector (GROND), places GRB 080916C among the top 5% most distant GRBs, and makes it the most energetic GRB known to date. The detection of GeV photons from such a distant event is rather surprising. The observed gamma-ray variability in the prompt emission together with the redshift suggests a lower limit for the Lorentz factor of the ultra-relativistic ejecta of Gamma > 1090. This value rivals any previous measurements of Gamma in GRBs and strengthens the extreme nature of GRB 080916C.
description: 6 pages, 5 figures; subm. to A&A
Al via il progetto DESI
Creators: Corrado Ruscica
Publisher: name: Media Inaf
Year: 2015

Lo strumento DESI, destinato al telescopio di 4m Mayall situato al Kitt Peak National Observatory, produrrà una nuova mappa 3D del cielo che permetterà di approfondire il ruolo che ha l'energia oscura per l'espansione cosmica. Il Dipartimento dell'Energia USA ha dato il via libera al progetto, autorizzandone le finalità scientifiche, la programmazione e i relativi fondi
title: Ð¡Ð¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð±ÑÑ Ð³Ð°Ð»ÑÐµÑÑÐºÐ¾Ð³Ð¾ Ð¸ Ð½Ð°Ð»Ð¾Ð³Ð¾Ð²Ð¾Ð³Ð¾ ÑÑÐµÑÐ° Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð² (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ "Ð'ÐÐÐ")
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¨Ð¸ÑÐ¼Ð°ÑÐµÐ²Ð°, ÐÐ°Ð»ÐµÑ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: 2016
Subjects: Ð±ÑÑ Ð³Ð°Ð»ÑÐµÑÑÐºÐ¸Ð¹ ÑÑÐµÑ
Ð½Ð°Ð»Ð¾Ð³Ð¾Ð²ÑÐ¹ ÑÑÐµÑ
ÑÑÐµÑÐ½Ð°Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ°
Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ¾Ð¾Ð±Ð¾ÑÐ¾Ñ
accounting
fiscal accounting
accounting policy
flow of documents

description: Ð Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÐ¿Ð¾ÑÐ¾Ð± ÑÑÐµÑÐ° ÑÐ°Ð·Ð½Ð¸ÑÑ Ð¼ÐµÐ¶Ð´Ñ Ð±ÑÑÐ³Ð°Ð»ÑÐµÑÑÐºÐ¸Ð¼ Ð¸ Ð½Ð°Ð»Ð¾Ð³Ð¾Ð²ÑÐ¼ ÑÑÐµÑÐ¾Ð¼ Ð¿Ð¾ ÑÐ¿Ð¸ÑÐ°Ð½Ð¸Ñ ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÐ¸ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð², ÑÐ¿Ð¾ÑÐ¾Ð± Ð²ÐµÐ´ÐµÐ½Ð¸Ñ ÑÑÐµÑÐ° Ð¿Ð¾ÑÑÑÐ¿Ð»ÐµÐ½Ð¸Ñ, Ð²ÑÐ´Ð°ÑÐ¸ Ð¸ ÑÐ¿Ð¸ÑÐ°Ð½Ð¸Ñ ÑÐ¿ÐµÑÐ¾Ð´ÐµÐ¶Ð´Ñ Ð² ÐÐÐ "Ð'ÐÐÐ", ÑÑÐµÑÐ½Ð°Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ° Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ¾Ð¾Ð±Ð¾ÑÐ¾ÑÐ° Ð¸ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð¿ÑÐµÐ´Ð»Ð°Ð³Ð°ÐµÐ¼Ð¾Ð³Ð¾ ÑÑÐµÑÐ° Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾-Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½ÑÑ Ð·Ð°Ð¿Ð°ÑÐ¾Ð².
description: In the bachelor work is developed a method of accounting the differences between the accounting and tax accounting disposal of the cost of materials, the method of accounting proceeds, issue and disposal of workwear "O'KEY" LTD, the accounting policy of document circulation and economic substantiation of application of the proposed accounting of material-industrial inventories.