cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: A case study of the contributions of public health nurses to infant mental health promotion in Newfoundland and Labrador
Creators: name: Norton, Emily Catherine
Publisher: name: Memorial University of Newfoundland
Year: 2021

description: Promoting infant mental health or supporting the baby’s healthy social and emotional development during the first year of life is critical for a child’s healthy development and future mental health well-being. This knowledge has been slow to be integrated into the education of public health nurses, who provide key maternal-child services in Newfoundland and Labrador. This single instrumental case study explored public health nurses’ education about infant mental health (IMH), and their work experiences in dealing with young families, in order to identify ways to better promote infant mental health. Data collected through key document review and semi-structured interviews with key informants and public health nurses indicate that public health nurses provide numerous maternal-child services. However, they have many other roles that limit their time and ability to promote maternal-infant mental health, as mothers and babies wellbeing are very much interconnected. Most nurses stated feeling under-prepared to effectively promote maternal-infant mental health when they first started in public health and reported having varying levels of education in this field. Furthermore, they declared mostly relying on experiential knowledge to supplement their education. Time, resource, and geographical barriers may impede nurses’ access to education about infant mental health and its promotion. Effectively educating public health nurses about infant mental health promotion and addressing institutional barriers such as time, supportive infrastructure, and expanding scope of practice will aid in promoting lifelong mental wellness for these populations.
title: ÐÐµÑÑÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ðµ ÑÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð¶Ð´ÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ ÑÐ°ÑÑ Ð¾Ð´Ð¾Ð¼ÐµÑÐ¾Ð² ÑÐµÐ¿Ð»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¸Ð¼Ð¾Ð², Ð¢Ð¸Ð¼Ñ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: 2017
Subjects: Ð¡ÑÐµÑÑÐ¸ÐºÐ¸
Ð Ð°ÑÑ Ð¾Ð´Ð¾Ð¼ÐµÑÑ ÑÐµÐ¿Ð»Ð¾Ð²ÑÐµ
ÑÐµÐ¿Ð»Ð¾ÑÑÐµÑÑÐ¸ÐºÐ¸
ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²Ð¾ Ð¿Ð¾ÑÑÐµÐ±Ð»ÐµÐ½Ð½Ð¾Ð¹ ÑÐµÐ¿Ð»Ð¾ÑÑ
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ÐÐÐ¡Ð¢ Ð ÐÐ 1434

description: ÐÐ°ÑÑÐ¾ÑÑÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ Ð¼ÐµÑÑÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð¸Ð·Ð¼ÐµÑÐµÐ½Ð¸Ð¹ ÑÐµÐ¿Ð»Ð°, Ð¿Ð¾ÑÑÐµÐ±Ð»ÑÐµÐ¼Ð¾Ð³Ð¾ Ð½Ð° Ð¾Ð±Ð¾Ð³ÑÐµÐ² Ð¶Ð¸Ð»ÑÑ Ð´Ð¾Ð¼Ð¾Ð². Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ ÐºÑÐ¸ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð¾Ð±Ð·Ð¾Ñ Ð´ÐµÐ¹ÑÑÐ²ÑÑÑÐµÐ¹ Ð¼ÐµÑÑÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð¾Ð¹ Ð±Ð°Ð·Ñ. ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¾ ÑÐ¸ÑÐ»ÐµÐ½Ð½Ð¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¾ÑÐµÑÑÐ° ÑÑÐ°Ð½ÑÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾Ð³ÑÐµÑÐ½Ð¾ÑÑÐµÐ¹ Ð¿ÐµÑÐ²Ð¸ÑÐ½ÑÑ Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÐµÐ¹ ÑÐµÐ¿Ð»Ð¾ÑÑÐµÑÑÐ¸ÐºÐ° Ð² Ð¿Ð¾Ð³ÑÐµÑÐ½Ð¾ÑÑÑ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ° ÐºÐ¾ÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¸Ð·Ð¼ÐµÑÐµÐ½Ð¸Ñ ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²Ð° Ð¿Ð¾ÑÑÐµÐ±Ð»ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐµÐ¿Ð»Ð°. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½ Ð¸Ñ Ð°Ð½Ð°Ð»Ð¸Ð·. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð°Ñ Ð±Ð¸Ð±Ð»Ð¸Ð¾ÑÐµÐºÐ° Ð´Ð»Ñ ÑÐµÐ¿Ð»Ð¾Ð²ÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»Ñ, Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑÑÐ°Ñ Ð¾ÑÑÑÐµÑÑÐ²Ð»ÑÑÑ ÑÐ°ÑÑÐµÑ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð¸Ð·Ð¼ÐµÑÐµÐ½Ð¸Ñ ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²Ð° Ð¸Ð·ÑÐ°ÑÑÐ¾Ð´Ð¾Ð²Ð°Ð½Ð½Ð¾Ð¹ ÑÐµÐ¿Ð»Ð¾ÑÑ Ð¾Ð´Ð½Ð¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾ Ñ ÑÐ°ÑÑÐµÑÐ¾Ð¼ Ð¸Ñ Ð¼ÐµÑÑÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸Ðº.
Zero-point Divacancy Concentration in the Shadow Wave-Function Model for Solid 4He
Creators: name: Pessoa, R.
name: de Koning, M.
name: Vitiello, S. A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Other Condensed Matter (cond-mat.other)
subject: FOS: Physical sciences

description: We address the issue of interaction between zero-point vacancies in solid 4He as described within the shadow wave-function model. Applying the reversible-work method and taking into account finite-size effects, we obtain a zero-point monovacancy concentration of (2.03 +- 0.02) 10^{-3}, which is slightly higher than the result due to Reatto et al. for the same model. Utilizing the same methodology, we then consider the divacancy, taking into account both the in-plane as well as out-of-plane configurations with respect to the basal plane. We find no significant anisotropy between both conformation. Furthermore, although there is a small binding tendency, the expected divacancy concentration is only ~4-5 times larger than the value expected in the absence of any clustering propensity, 2.5 10^{-5}. This result suggests that, within the employed model description, no vacancy aggregation leading to phase separation is to be expected in the ground state.
description: 10 pages, 1 figure
Superconductivity with the enhanced upper critical field in the Pt-Doping CuRh2Se4 spinel
Creators: name: He, Yiyi
name: You, Yi-Xin
name: Zeng, Lingyong
name: Guo, Shu
name: Zhou, Huawei
name: Li, Kuan
name: Huang, Yanhao
name: Yu, Peifeng
name: Zhang, Chao
name: Cao, Chao
name: Luo, Huixia
Publisher: name: arXiv
Year: 2022
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We report the effect of Pt doping on the superconductivity in CuRh2Se4 spinel using a combined experimental and theoretical study. Our XRD results reveal that the Cu(Rh1-xPtx)2Se4 crystallizes in the structure with a space group of Fd3-m (No. 227), and the lattice parameter a increases with Pt doping. The resistivity and magnetic susceptibility measurement results verify that the superconducting transition temperature (Tc) forms a dome-like shape with a maximum value of 3.84 K at x = 0.06. It is also observed that the Pt-doping slightly reduces the lower critical magnetic field from 220 Oe in CuRh2Se4 to 168 Oe in Cu(Rh0.94Pt0.06)2Se4, while it significantly enhances the upper critical magnetic field, reaching the maximum of 4.93 T in the Cu(Rh0.94Pt0.06)2Se4 sample. The heat capacity result indicates that the sample Cu(Rh0.91Pt0.09)2Se4 is a bulk superconductor. First-principles calculations suggest that the Pt-doping leads to a red-shift of a density of state peak near the Fermi level, consistent with the dome-like Tc observed experimentally.
description: 33 pages, 7 figures, 2 tables; The manuscript with the same title will be published by PRB, 2022
Trauma Informed Policing: A Scoping Review Protocol
Creators: name: Guala, Tahnee
Publisher: name: OSF Registries
Year: 2023
Subjects: subject: Social and Behavioral Sciences
subject: Psychology
subject: FOS: Psychology
subject: criminology
subject: policing
subject: psychology
subject: trauma informed care

description: The scoping review aims to review the current literature on trauma informed policing to identify pathways for future research.
title: ÐÐ¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² Ð±ÐµÑÐ¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð±ÑÑÐ¾Ð½Ð°Ð±Ð¸Ð²Ð½ÑÑ ÑÐ²Ð°Ð¹ Ð² Ð·Ð¸Ð¼Ð½Ð¸Ð¹ Ð¿ÐµÑÐ¸Ð¾Ð´ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð°
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐ²Ð°Ð½Ð¾Ð², 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: 2016
Subjects: ÐÐµÑÐ¾Ð½
Ð¡ÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð¾
Ð¡Ð²Ð°Ð¸ Ð½Ð°Ð±Ð¸Ð²Ð½ÑÐµ
Ð·Ð¸Ð¼Ð½ÐµÐµ Ð±ÐµÑÐ¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð¿ÑÐ¾Ð³ÑÐµÐ² Ð±ÐµÑÐ¾Ð½Ð°
ÐºÑÐ¸ÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¿ÑÐ¾ÑÐ½Ð¾ÑÑÑ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÐ° Ð¾ Ð·Ð¸Ð¼Ð½ÐµÐ¼ Ð±ÐµÑÐ¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ Ð±ÑÑÐ¾Ð½Ð°Ð±Ð¸Ð²Ð½ÑÑ ÑÐ²Ð°Ð¹ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ°, Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð½Ð°Ñ Ð½Ð° Ð¼ÐµÑÐ¾Ð´Ðµ ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ð³Ð¾ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ, Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑÑÐ°Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°ÑÑ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÑ Ð±ÐµÑÐ¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¸ Ð¾ÑÑÐ¸ÑÐ°ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÐµ. ÐÑÐµÐ´Ð»Ð°Ð³Ð°ÐµÐ¼ÑÐ¹ ÑÐ°ÑÑÐµÑÐ½ÑÐ¹ Ð¼ÐµÑÐ¾Ð´, Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð½ÑÐ¹ Ð½Ð° ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ð¼ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÐµÑ Ð¾Ð±ÐµÑÐ¿ÐµÑÐ¸ÑÑ ÑÑÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ ÑÐ½ÐµÑÐ³Ð¾ÑÐ±ÐµÑÐµÐ¶ÐµÐ½Ð¸Ðµ Ð·Ð° ÑÑÐµÑ Ð¿Ð¾Ð»ÐµÐ·Ð½Ð¾Ð³Ð¾ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÐ¿Ð»Ð¾Ð²Ð¾Ð¹ Ð¸Ð½ÐµÑÑÐ¸Ð¸ Ð±ÐµÑÐ¾Ð½Ð° Ð¿ÑÐ¸ ÑÐµÐ³ÑÐ»Ð¸ÑÑÐµÐ¼ÑÑ ÑÐµÐ¶Ð¸Ð¼Ð°Ñ ÐµÐ³Ð¾ ÑÐµÐ¿Ð»Ð¾Ð²Ð¾Ð¹ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸, Ð¾Ð±ÐµÑÐ¿ÐµÑÐ¸ÑÑ Ð³Ð°ÑÐ°Ð½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ðµ Ð¾ÑÑÑÑÑÑÐ²Ð¸Ðµ Ð´ÐµÑÑÑÑÐºÑÐ¸Ð²Ð½ÑÑ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð² Ð² Ð¾Ð³Ð¾Ð»Ð¾Ð²ÐºÐµ Ð±ÑÑÐ¾Ð½Ð°Ð±Ð¸Ð²Ð½ÑÑ ÑÐ²Ð°Ð¹, ÑÑÐ¸ÑÑÐ²Ð°ÐµÑ ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÐ½Ð¾Ðµ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ðµ Ð±ÐµÑÐ¾Ð½Ð½Ð¾Ð¹ ÑÐ¼ÐµÑÐ¸ Ð¸ Ð¿ÑÐ¾Ð¼ÐµÑÐ·ÑÐµÐ³Ð¾ Ð³ÑÑÐ½ÑÐ° Ð¿ÑÐ¸ Ð·Ð¸Ð¼Ð½ÐµÐ¼ Ð±ÐµÑÐ¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ Ð±ÑÑÐ¾Ð½Ð°Ð±Ð¸Ð²Ð½ÑÑ ÑÐ²Ð°Ð¹, Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÐµÑ Ð¾Ð±ÐµÑÐ¿ÐµÑÐ¸ÑÑ ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½ÑÐ¹ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ ÑÐ°Ð±Ð¾Ñ Ð·Ð¸Ð¼Ð½ÐµÐ³Ð¾ Ð±ÐµÑÐ¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð±ÑÑÐ¾Ð½Ð°Ð±Ð¸Ð²Ð½ÑÑ ÑÐ²Ð°Ð¹ Ð½Ð° ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð¿Ð»Ð¾ÑÐ°Ð´ÐºÐµ, Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÐµÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð¾Ð²Ð°ÑÑ ÑÐ°Ð±Ð¾ÑÑ Ð½Ð° ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð¿Ð»Ð¾ÑÐ°Ð´ÐºÐµ Ñ ÑÑÐµÑÐ¾Ð¼ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸Ð¸ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾-ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐµÑÑÑÑÐ¾Ð². ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð´Ð°Ð½Ð½ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ°Ñ ÐºÐ°ÑÑÐ°.
The updated spectral catalogue of INTEGRAL Gamma-Ray Bursts
Creators: name: Vianello, G.
name: Götz, D.
name: Mereghetti, S.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a catalogue with the properties of all the bursts detected and localized by the IBIS instrument onboard the INTEGRAL satellite from November 2002 to September 2008. The sample is composed of 56 bursts, corresponding to a rate of ~ 0.8 GRB per month. Thanks to the performances of the INTEGRAL Burst Alert System, 50% of the IBIS GRBs have detected afterglows, while 5% have redshift measurements. A spectral analysis of the 43 bursts in the INTEGRAL public archive has been carried out using the most recent software and calibration, deriving an updated, homogeneous and accurate catalogue with the spectral features of the sample. When possible also a time-resolved spectral analysis has been carried out. The GRBs in the sample have 20-200 keV fluences in the range 5 x 1E-8 --2.5 x 1E-4 erg cm-2, and peak fluxes in the range 0.11 - 56 ph cm-2 s-1. While most of the spectra are well fitted by a power law with photon index ~ 1.6, we found that 9 bursts are better described by a cut-off power law, resulting in Ep values in the range 35--190 keV. Altough these results are comparable with those obtained with BAT onboard Swift, there is a marginal evidence that ISGRI detects dimmer bursts than Swift/BAT. Using the revised spectral parameters and an updated sky exposure map that takes into account also the effects of the GRB trigger efficiency, we strengthen the evidence for a spatial correlation with the super galactic plane of the faint bursts with long spectral lag (Foley et al.,2008).
description: Corrected some typos, added some references; Accepted by Astronomy & Astrophysics, in press
title: Ð¡Ð¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ðµ Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ðµ: Ð½Ð°ÑÐºÐ° Ð¸ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ðµ 2021 (MMESE-2021)
title: Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ 10-Ð¹ ÐÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð¹ Ð½Ð°ÑÑÐ½Ð¾Ð¹ Ð¾Ð½Ð»Ð°Ð¹Ð½-ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ð¸, 24 Ð¸ÑÐ½Ñ 2021 Ð³Ð¾Ð´Ð°
titleType: Subtitle
title: Modern mechanical engineering: science and education 2021 (MMESE-2021)
Creators: name: "Ð¡Ð¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ðµ Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ðµ: Ð½Ð°ÑÐºÐ° Ð¸ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ðµ 2021 (MMESE-2021)", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð°Ñ Ð½Ð°ÑÑÐ½Ð°Ñ Ð¾Ð½Ð»Ð°Ð¹Ð½-ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (10; 2021; 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: 2021
Subjects: ÐÐ°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ðµ
Ð½Ð°ÑÐºÐ°
Ð²ÑÑÑÐµÐµ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ðµ

description: Ð ÑÐ±Ð¾ÑÐ½Ð¸ÐºÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ, Ð¾ÑÑÐ°Ð¶Ð°ÑÑÐ¸Ðµ Ð¾Ð¿ÑÑ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ Ð²ÑÐ·Ð¾Ð² Ð² Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐµ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð², ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð² Ð¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐ¸Ð»Ñ. ÐÑÐ¾Ð±Ð¾Ðµ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ ÑÐ´ÐµÐ»ÐµÐ½Ð¾ Ð¾ÑÑÐ°Ð¶ÐµÐ½Ð¸Ñ Ð² ÑÑÐµÐ±Ð½ÑÑ Ð¿Ð»Ð°Ð½Ð°Ñ Ð¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð°Ñ ÑÑÐµÐ±Ð½ÑÑ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ð¹, Ð¿ÑÐµÐ´ÑÑÐ²Ð»ÑÐµÐ¼ÑÑ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐ¼ Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸ÐµÐ¼ Ðº ÑÑÐ¾Ð²Ð½Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð²ÑÐ¿ÑÑÐºÐ½Ð¸ÐºÐ¾Ð² Ð²ÑÐ·Ð¾Ð². ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐ°ÐºÐ¶Ðµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð½Ð°ÑÑÐ½Ð¾-Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÑÐºÐ¸Ñ ÑÐ°Ð±Ð¾Ñ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ. Ð¡Ð±Ð¾ÑÐ½Ð¸Ðº Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½ Ð´Ð»Ñ Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»ÐµÐ¹ Ð²ÑÐ·Ð¾Ð², Ð·Ð°Ð½Ð¸Ð¼Ð°ÑÑÐ¸ÑÑÑ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¾Ð¹ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð², ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð² Ð¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐ¸Ð»Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ¾Ð² Ð¸ Ð½Ð°ÑÑÐ½ÑÑ ÑÐ°Ð±Ð¾ÑÐ½Ð¸ÐºÐ¾Ð², ÑÐ°Ð±Ð¾ÑÐ°ÑÑÐ¸Ñ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ.
When finite-size corrections vanish: The S=1/2 XXZ model and the Razumov-Stroganov state
Creators: name: Banchi, Leonardo
name: Colomo, Filippo
name: Verrucchi, Paola
Publisher: name: arXiv
Year: 2009
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We study the one-dimensional $S=1/2$ XXZ model on a finite lattice at zero temperature, varying the exchange anisotropy $Δ$ and the number of sites $N$ of the lattice. Special emphasis is given to the model with $Δ=1/2$ and $N$ odd, whose ground state, the so-called Razumov-Stroganov state, has a peculiar structure and no finite-size corrections to the energy per site. We find that such model corresponds to a special point on the $Δ$-axis which separates the region where adding spin-pairs increases the energy per site from that where the longer the chain the lower the energy. Entanglement properties do not hold surprises for $Δ=1/2$ and $N$ odd. Finite-size corrections to the energy per site non trivially vanish also in the ferromagnetic $Δ\to -1^+$ isotropic limit, which is consequently addressed; in this case, peculiar features of some entanglement properties, due to the finite length of the chain and related with the change in the symmetry of the Hamiltonian, are evidenced and discussed. In both the above models the absence of finite-size corrections to the energy per site is related to a peculiar structure of the ground state, which has permitted us to provide new exact analytic expressions for some correlation functions.
description: 10 pages, 5 figures
title: Ð¡Ð¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÐºÐ°Ð´ÑÐ¾Ð²Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«Ð¢ÑÐµÑÐ¸Ð¹ Ð¿Ð°ÑÐºÂ»
title: Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¡Ð¸Ð·Ð¾Ð², ÐÐµÐ½Ð¸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: ÐºÐ°Ð´ÑÐ¾Ð²Ð°Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ°
ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½ÑÐµÑÐºÐ°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
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ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾ÑÐµÑÐ¸
personnel policy
management activity
organization
economic losses

description: ÐÐ°Ð´ÑÐ¾Ð²Ð°Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ° ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ¾ÑÑÐ°Ð²Ð½Ð¾Ð¹ ÑÐ°ÑÑÑÑ Ð²ÑÐµÐ¹ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½ÑÐµÑÐºÐ¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¸ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸. ÐÐ´Ð½Ð°ÐºÐ¾ Ð½ÐµÐ²ÐµÑÐ½Ð¾Ðµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ðµ ÐºÐ°Ð´ÑÐ¾Ð²Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸ Ð¿ÑÐ¸Ð²Ð¾Ð´Ð¸Ñ Ðº Ð±Ð¾Ð»ÑÑÐ¸Ð¼ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¼ Ð¿Ð¾ÑÐµÑÑÐ¼. ÐÐ¾ ÑÑÐ¾Ð¹ Ð¿ÑÐ¸ÑÐ¸Ð½Ðµ Ð² ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÐºÐ°Ð´ÑÐ¾Ð²Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸ Ð½Ð° ÐºÐ¾Ð½ÐºÑÐµÑÐ½Ð¾Ð¼ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸, Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð¾ÑÐ¸Ð±ÐºÐ¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸, Ð° ÑÐ°ÐºÐ¶Ðµ ÐµÑ ÑÐ»Ð°Ð±ÑÐµ Ð¼ÐµÑÑÐ°. ÐÑÐ¾Ð³Ð¾Ð¼ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÐºÐ°Ð´ÑÐ¾Ð²Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸.
description: Personnel policy is one part of a production policy of the organization. In addition, it is an important part of the overall management of the organization. That is why incorrect use of the personnel policy can lead to huge economic losses. For this reason, in this paper we analyzed the human resources policy on a particular company, the use of policy errors have been identified, as well as its weaknesses. The result of the writing of this paper is to make recommendations on improving human resources policy.
title: Ð Ð¾Ð»Ñ ÑÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¸Ð´ÐµÐ½ÑÐ¸ÑÐ½Ð¾ÑÑÐ¸ Ð² ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ ÑÐµÐ¿Ð°ÑÐ°ÑÐ¸ÑÑÑÐºÐ¸Ñ Ð½Ð°ÑÑÑÐ¾ÐµÐ½Ð¸Ð¹ Ð² ÐÑÐ¿Ð°Ð½Ð¸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Ð»Ð¸Ð½Ð¾Ð²Ð°, 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: 2018
Subjects: ÐÑÐ¿Ð°Ð½Ð¸Ñ
ÑÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐµÐ¿Ð°ÑÐ°ÑÐ¸Ð·Ð¼
ÑÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÐºÐ¾Ð½ÑÐ»Ð¸ÐºÑ
Ð±Ð°ÑÐºÐ¸

description: ÐÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð°Ð½Ð°Ð»Ð¸Ð·Ñ Ð²Ð·Ð°Ð¸Ð¼Ð¾ÑÐ²ÑÐ·Ð¸, ÑÑÑÐµÑÑÐ²ÑÑÑÐµÐ¹ Ð¼ÐµÐ¶Ð´Ñ Ð±Ð°ÑÐºÐ¾Ð¹ Ð¸ ÐºÐ°ÑÐ°Ð»Ð¾Ð½ÑÐºÐ¾Ð¹ ÑÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¸Ð´ÐµÐ½ÑÐ¸ÑÐ½Ð¾ÑÑÑÑ Ð¸ ÑÐµÐ¿Ð°ÑÐ°ÑÐ¸ÑÑÑÐºÐ¸Ð¼Ð¸ Ð½Ð°ÑÑÑÐ¾ÐµÐ½Ð¸ÑÐ¼Ð¸ Ð² Ð´Ð°Ð½Ð½ÑÑ ÑÐµÐ³Ð¸Ð¾Ð½Ð°Ñ. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½ ÑÑÐ½Ð¾ÐºÑÐ»ÑÑÑÑÐ½ÑÐ¹ Ð°ÑÐ¿ÐµÐºÑ Ð±Ð°ÑÐºÑÐºÐ¾Ð¹ Ð¸ ÐºÐ°ÑÐ°Ð»Ð¾Ð½ÑÐºÐ¾Ð¹ Ð¸Ð´ÐµÐ½ÑÐ¸ÑÐ½Ð¾ÑÑÐµÐ¹, Ð¸ÑÑÐ¾ÑÐ¸Ñ, ÑÐ¿ÐµÑÐ¸ÑÐ¸ÐºÐ° ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÑÐ°Ð¿Ð° ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐµÐ¿Ð°ÑÐ°ÑÐ¸Ð·Ð¼Ð°.
Gamma ray lines: what will they tell us about SUSY?
Creators: name: Yaguna, Carlos E.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Neutralino dark matter can be indirectly detected by observing the gamma ray lines from the annihilation processes XX-->gg and XX-->gZ. In this paper we study the implications that the observation of these two lines could have for the determination of the supersymmetric parameter space. Within the minimal supergravity framework, we find that, independently of the dark matter distribution in the Galaxy, such observations by themselves would allow to differentiate between the coannihilation region, the funnel region, and the focus point region. As a result, several restrictions on the msugra parameters can be derived. Within a more general MSSM scenario, we show that the observation of gamma-ray lines might be used to discriminate between a bino-, a wino-, and a higgsino-like neutralino, with important consequences for cosmology and for models of supersymmetry breaking. The detection of the gamma ray lines, therefore, will not only provide an unmistakable signature of dark matter, it will also open a new road toward the determination of supersymmetric parameters.
description: 19 pages, 10 figures
Thermal Infrared MMTAO Observations of the HR 8799 Planetary System
Creators: name: Hinz, Philip M.
name: Rodigas, Timothy J.
name: Kenworthy, Matthew A.
name: Sivanandam, Suresh
name: Heinze, Aren N.
name: Mamajek, Eric E.
name: Meyer, Michael R.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We present direct imaging observations at wavelengths of 3.3, 3.8 (L',band), and 4.8 (M band) microns, for the planetary system surrounding HR 8799. All three planets are detected at L'. The c and d component are detected at 3.3 microns, and upper limits are derived from the M band observations. These observations provide useful constraints on warm giant planet atmospheres. We discuss the current age constraints on the HR 8799 system, and show that several potential co-eval objects can be excluded from being co-moving with the star. Comparison of the photometry is made to models for giant planet atmospheres. Models which include non-equilibrium chemistry provide a reasonable match to the colors of c and d. From the observed colors in the thermal infrared we estimate T_eff < 960 K for b, and T_eff=1300 and 1170 K for c and d, respectively. This provides an independent check on the effective temperatures and thus masses of the objects from the Marois 2008 results.
description: 16 pages, 6 figures, accepted to ApJ
title: ÐÐ²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð² ÑÐ·ÑÐºÐ¾Ð·Ð½Ð°Ð½Ð¸Ðµ
title: ÑÑÐµÐ±Ð½Ð¸Ðº Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÐ¸Ð»Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹ Ð²ÑÑÑÐ¸Ñ ÑÑÐµÐ±Ð½ÑÑ Ð·Ð°Ð²ÐµÐ´ÐµÐ½Ð¸Ð¹
titleType: Subtitle
Creators: name: ÐÐ°ÑÐ»Ð¾Ð², Ð®ÑÐ¸Ð¹
Publisher: name: ÐÑÑÑÐ°Ñ ÑÐºÐ¾Ð»Ð°
Year: 1987
Subjects: ÑÐ·ÑÐºÐ¾Ð·Ð½Ð°Ð½Ð¸Ðµ
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: Ð ÑÑÐµÐ±Ð½Ð¸ÐºÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¿ÑÐµ ÑÐ°Ð·Ð´ÐµÐ»Ñ ÐºÑÑÑÐ° Â«ÐÐ²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð² ÑÐ·ÑÐºÐ¾Ð·Ð½Ð°Ð½Ð¸ÐµÂ». Ð¢ÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ ÑÐ°Ð·ÑÑÑÐ½ÑÑÑÑÑ Ð½Ð° ÐºÐ¾Ð½ÐºÑÐµÑÐ½Ð¾Ð¼ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ðµ ÑÐ»Ð°Ð²ÑÐ½ÑÐºÐ¸Ñ,
Ð³ÐµÑÐ¼Ð°Ð½ÑÐºÐ¸Ñ, ÑÐ¾Ð¼Ð°Ð½ÑÐºÐ¸Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð»Ð°ÑÐ¸Ð½ÑÐºÐ¾Ð³Ð¾ Ð¸ Ð½ÐµÐºÐ¾ÑÐ¾ÑÑÑ Ð´ÑÑÐ³Ð¸Ñ ÑÐ·ÑÐºÐ¾Ð². ÐÐ¾ 2-Ð¼ Ð¸Ð·Ð´Ð°Ð½Ð¸Ð¸ (1-Ðµ - Ð² 1975 Ð³.) Ð´Ð¾Ð±Ð°Ð²Ð»ÐµÐ½Ñ ÑÐ°Ð·Ð´ÐµÐ»Ñ Ð¾ Ð³ÐµÐ½ÐµÐ°Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ ÑÐ·ÑÐºÐ¾Ð², Ð¾ Ð¿ÑÐ¾Ð¸ÑÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ð¸ ÑÐ·ÑÐºÐ°, Ð¾ÑÐ´ÐµÐ»ÑÐ½ÑÐµ ÑÐ°Ð·Ð´ÐµÐ»Ñ ÑÐ°ÑÑÐ¸ÑÐµÐ½Ñ Ð¸ Ð¿ÐµÑÐµÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ. Ð
ÐºÐ½Ð¸Ð³Ðµ Ð´Ð°Ð½ Ð¿ÑÐµÐ´Ð¼ÐµÑÐ½ÑÐ¹ ÑÐºÐ°Ð·Ð°ÑÐµÐ»Ñ.
title:  Never too late to communicate. Constructive and critical input from national private law judges before and after preliminary ruling procedures
Creators: name: Sieburgh  ,  Carla
Publisher: name: Roma TrE-Press
Year: 2021

description: Il contributo prende in considerazione il caso Abercrombie & Fitch c. Bordonaro quale esempio di ‘cattiva’ comunicazione tra la CGUE e i giudici nazionali. Qui la CGUE non si è limitata a fornire un rimedio, ma si è ritenuta in grado di esprimere una valutazione sul sistema giuridico nazionale e ha preso una decisione di enorme impatto. A causa della limitata comprensione del quadro fattuale nazionale, la sentenza della CGUE è poco convincente. In casi come questo i giudici nazionali non devono considerare chiuso il caso, ma prendere la sentenza della CGUE come nuovo punto di partenza: possono per esempio, rivolgersi alla propria corte costituzionale o rivolgersi nuovamente alla CG per ragioni differenti da quelle invocate nel primo rinvio, in modo che la comunicazione continui, giacché non è mai troppo tardi per comunicare.
description: National Judges and the Case Law of the Court of Justice of the European Union
title: Ð ÑÐ°ÑÐ¿ÑÐ¾ÑÑÑÐ°Ð½ÐµÐ½Ð¸Ð¸ Ð½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»Ð¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð½Ð°ÑÑÑÐ¾ÐµÐ½Ð¸Ð¹ Ð² Ð¤Ð¸Ð½Ð»ÑÐ½Ð´Ð¸Ð¸ Ð½Ð° ÑÐ¾Ð½Ðµ Ð¿ÑÐ¸ÑÐ¾ÐºÐ° Ð±ÐµÐ¶ÐµÐ½ÑÐµÐ²
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐ¾ÑÐ´ÐµÐµÐ²Ð°, ÐÐ½Ð½Ð°
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: Ð½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»Ð¸Ð·Ð¼
Ð¸Ð¼Ð¼Ð¸Ð³ÑÐ°ÑÐ¸Ñ
Ð¼Ð¸Ð³ÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ ÐºÑÐ¸Ð·Ð¸Ñ
Ð¤Ð¸Ð½Ð»ÑÐ½Ð´Ð¸Ñ
Ð±ÐµÐ¶ÐµÐ½ÑÑ

description: ÐÐ°Ð½Ð½Ð°Ñ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð°Ð½Ð°Ð»Ð¸Ð·Ñ ÑÐ°ÐºÑÐ¾ÑÐ¾Ð², Ð¿Ð¾Ð²Ð»Ð¸ÑÐ²ÑÐ¸Ñ Ð½Ð° Ð²Ð¾Ð·Ð½Ð¸ÐºÐ½Ð¾Ð²ÐµÐ½Ð¸Ðµ Ð¸ ÑÐ°ÑÐ¿ÑÐ¾ÑÑÑÐ°Ð½ÐµÐ½Ð¸Ðµ Ð½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»Ð¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð½Ð°ÑÑÑÐ¾ÐµÐ½Ð¸Ð¹ Ð² Ð¤Ð¸Ð½Ð»ÑÐ½Ð´Ð¸Ð¸, Ð²ÑÐ·Ð²Ð°Ð½Ð½ÑÑ Ð¿ÑÐ¸ÑÐ¾ÐºÐ¾Ð¼ Ð±ÐµÐ¶ÐµÐ½ÑÐµÐ² Ð¸Ð· ÑÑÑÐ°Ð½ ÐÑÑÐ¸ÐºÐ¸ Ð¸ ÐÐ»Ð¸Ð¶Ð½ÐµÐ³Ð¾ ÐÐ¾ÑÑÐ¾ÐºÐ°. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° Ð¸ÑÑÐ¾ÑÐ¸Ñ Ð¼Ð¸Ð³ÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ ÐºÑÐ¸Ð·Ð¸ÑÐ°, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ° ÑÑÑÐ°Ð½ ÐÐ°Ð¿Ð°Ð´Ð°, Ð¿Ð¾Ð²Ð»Ð¸ÑÐ²ÑÐ°Ñ Ð½Ð° ÐµÐ³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð¸ÑÑÐ¾ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð°ÑÐ¿ÐµÐºÑ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»Ð¸Ð·Ð¼Ð° Ð² Ð¤Ð¸Ð½Ð»ÑÐ½Ð´Ð¸Ð¸ Ð¸ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð° Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»Ð¸ÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¿Ð°ÑÑÐ¸Ð¸ Ð¤Ð¸Ð½Ð»ÑÐ½Ð´Ð¸Ð¸ Â«ÐÑÑÐ¸Ð½Ð½ÑÐµ ÑÐ¸Ð½Ð½ÑÂ».
Orbital-Free Density Functional Theory: Linear Scaling Methods for Kinetic Potentials, and Applications to Solid Al and S
Creators: name: Chai, Jeng-Da
name: Ligneres, Vincent L.
name: Ho, Gregory
name: Carter, Emily A.
name: Weeks, John D.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Other Condensed Matter (cond-mat.other)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: In orbital-free density functional theory the kinetic potential (KP), the functional derivative of the kinetic energy density functional, appears in the Euler equation for the electron density and may be more amenable to simple approximations. We study properties of two solid-state systems, Al and Si, using two nonlocal KPs that gave good results for atoms. Very accurate results are found for Al, but results for Si are much less satisfactory, illustrating the general need for a better treatment of extended covalent systems. A different integration pathway in the KP formalism may prove useful in attacking this fundamental problem.
description: Submitted to Chemical Physics Letters
title: Ð¤Ð¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ°ÑÐ¸Ñ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾Ð³Ð¾ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¸Ð½ÑÐµÐ³ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÑ ÑÑÑÑÐºÑÑÑ Ñ Ð¿ÑÐ¸Ð²Ð»ÐµÑÐµÐ½Ð¸ÐµÐ¼ Ð²Ð½ÐµÑÐ½ÐµÐ³Ð¾ ÑÐ¸Ð½Ð°Ð½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ
title: Ð¼Ð¾Ð½Ð¾Ð³ÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: Ð¡Ð¾ÐºÐ¾Ð»Ð¸ÑÑÐ½Ð°, ÐÐ°ÑÐ°Ð»ÑÑ
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2023
Subjects: ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ°
ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ
Ð²Ð½ÐµÑÐ½ÐµÐµ ÑÐ¸Ð½Ð°Ð½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð¸Ð½ÑÐµÐ³ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÐµ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÐµ ÑÑÑÑÐºÑÑÑÑ

description: Ð Ð¼Ð¾Ð½Ð¾Ð³ÑÐ°ÑÐ¸Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð°ÑÐ¿ÐµÐºÑÑ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ°ÑÐ¸Ñ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾Ð³Ð¾ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¸Ð½ÑÐµÐ³ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÑ ÑÑÑÑÐºÑÑÑ Ñ Ð¿ÑÐ¸Ð²Ð»ÐµÑÐµÐ½Ð¸ÐµÐ¼ Ð²Ð½ÐµÑÐ½ÐµÐ³Ð¾ ÑÐ¸Ð½Ð°Ð½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ñ ÑÑÐµÑÐ¾Ð¼ Ð½ÐµÐ¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð²Ð½ÐµÑÐ½ÐµÐ¹ ÑÑÐµÐ´Ñ. ÐÑÐ¸Ð¼ÐµÐ½Ð¸ÑÐµÐ»ÑÐ½Ð¾ Ðº Ð¸ÑÑÐ»ÐµÐ´ÑÐµÐ¼ÑÐ¼ Ð²Ð¸Ð´Ð°Ð¼ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð±Ð¸Ð·Ð½ÐµÑ-ÐµÐ´Ð¸Ð½Ð¸Ñ Ð¸Ð½ÑÐµÐ³ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ ÑÑÑÑÐºÑÑÑ Ð² ÐºÐ°ÑÐµÑÑÐ²Ðµ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ°ÑÐ¸Ñ Ð²ÑÑÑÑÐ¿Ð°ÐµÑ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ Ð¼Ð¾Ð´ÐµÐ»ÐµÐ¹ Ð¿Ð¾ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ Ð±Ð¸Ð·Ð½ÐµÑ-ÐµÐ´Ð¸Ð½Ð¸Ñ Ð¸Ð½ÑÐµÐ³ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ ÑÑÑÑÐºÑÑÑ, Ð¾ÑÑÑÐµÑÑÐ²Ð»ÑÐµÐ¼ÑÑ ÐºÐ°Ðº Ð·Ð° ÑÑÐµÑ ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½ÑÑ ÑÑÐµÐ´ÑÑÐ², ÑÐ°Ðº Ð¸ ÐºÑÐµÐ´Ð¸ÑÐ°. Ð ÐºÐ°ÑÐµÑÑÐ²Ðµ ÑÐµÐ»ÐµÐ²Ð¾Ð¹ ÑÑÐ½ÐºÑÐ¸Ð¸ Ð²ÑÑÑÑÐ¿Ð°ÐµÑ Ð¼Ð°ÐºÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿Ð¾Ð»ÑÑÐ°ÐµÐ¼Ð¾Ð¹ Ð¿ÑÐ¸Ð±ÑÐ»Ð¸, ÑÑÐ¾ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÐµÑ Ð¿Ð¾Ð²ÑÑÐ¸ÑÑ ÑÑÐ¾Ð²ÐµÐ½Ñ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾Ð³Ð¾ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð±Ð¸Ð·Ð½ÐµÑ-ÐµÐ´Ð¸Ð½Ð¸Ñ. Ð¡Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¾ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½ÑÑ Ð±Ð°Ð½ÐºÐ¾Ð²ÑÐºÐ¸Ñ ÑÑÐ°Ð²Ð¾Ðº Ð¸ Ð·Ð½Ð°ÑÐµÐ½Ð¸Ð¹ Ð¿ÑÐµÐ´Ð¾ÑÑÐ°Ð²Ð»ÑÐµÐ¼Ð¾Ð³Ð¾ ÐºÑÐµÐ´Ð¸ÑÐ°. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð°Ð¿ÑÐ¾Ð±Ð°ÑÐ¸Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ° Ð¼Ð¾Ð´ÐµÐ»ÐµÐ¹. ÐÐ¾Ð½Ð¾Ð³ÑÐ°ÑÐ¸Ñ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð° Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ¾Ð², Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»ÐµÐ¹ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹ Ð²ÑÐ·Ð¾Ð², ÑÑÐºÐ¾Ð²Ð¾Ð´ÑÑÐ¸Ñ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÐºÐ¾Ð² Ð¸Ð½ÑÐµÐ³ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÑ ÑÑÑÑÐºÑÑÑ, ÑÐ¸ÑÐ¾ÐºÐ¾Ð³Ð¾ ÐºÑÑÐ³Ð° ÑÐ¸ÑÐ°ÑÐµÐ»ÐµÐ¹, Ð¸Ð½ÑÐµÑÐµÑÑÑÑÐ¸ÑÑÑ Ð²Ð¾Ð¿ÑÐ¾ÑÐ°Ð¼Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²ÑÐ¼ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¼ ÑÐ°Ð·Ð²Ð¸ÑÐ¸ÐµÐ¼ Ð¸Ð½ÑÐµÐ³ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÑ ÑÑÑÑÐºÑÑÑ Ð¸ Ð±Ð¸Ð·Ð½ÐµÑ-ÐµÐ´Ð¸Ð½Ð¸Ñ Ñ Ð¿ÑÐ¸Ð²Ð»ÐµÑÐµÐ½Ð¸ÐµÐ¼ Ð²Ð½ÐµÑÐ½Ð¸Ñ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð² ÑÐ¸Ð½Ð°Ð½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ.
Comparison of long jump GRFs and “flex over shape” curves of able-bodied and paralympic amputee athletes
Creators: name: Breban, Samira Giuliana
name: Toniutto, Anna
name: Di Marco, Roberto
name: Cutti, Andrea Giovanni
name: Migliore, Gian Luca
name: Petrone, Nicola
Publisher: name: Loughborough University
Year: 2024

description: Engineering of Sport 15 - Proceedings from the 15th International Conference on the Engineering of Sport (ISEA 2024)
Running-specific prostheses (RSPs) have enabled people with lower limb amputations to substantially increase their performance in sports competitions. Long jumping is one of the disciplines in which prostheses are enabling athletes to compete at the highest level, achieving performance comparable to that of able-bodied athletes. The aim of the current work is to analyze long jumping biomechanics of two able bodied athletes and of an elite Paralympic transtibial athlete, focusing on Ground Reaction Forces (GRFs) and Roll Over Shape (ROS). Data collected will be used by orthopedic technicians to optimize the RPS setup, by trainers to improve athletes performance and by engineers for in-vitro RSP correct mechanical characterization.
Resolving the hot dust around HD69830 and eta Corvi with MIDI and VISIR
Creators: name: Smith, R.
name: Wyatt, M. C.
name: Haniff, C. A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Most of the known debris discs exhibit cool dust in regions analogous to the Edgeworth-Kuiper Belt. However, a rare subset show hot excess from within a few AU, which is often inferred to be transient. We examine 2 such sources to place limits on their location to help distinguish between different interpretations for their origin. We use MIDI on the VLTI to observe the debris discs around eta Corvi and HD69830 using baseline lengths from 44-130m. New VISIR observations of HD69830 at 18.7um are also presented. These observations are compared with disc models to place limits on disc size. The visibility functions measured with MIDI for both sources show significant variation with wavelength across 8-13um in a manner consistent with the disc flux being well resolved, notably with a dip at 10-11.5um due to the silicate emission feature. The average ratio of visibilities measured between 10-11.5um and 8-9um is 0.934+/-0.015 for HD69830 and 0.880+/-0.013 for eta Corvi over the 4 baselines for each source, a departure of 4 and 9sigma from that expected if the discs were unresolved. HD69830 is unresolved by VISIR at 18.7um. The combined limits from MIDI and 8m imaging constrain the warm dust to lie within 0.05-2.4AU for HD69830 and 0.16-2.98AU for eta Corvi. These results represent the first resolution in the mid-IR of dust around main sequence stars. The constraints placed on the location of the dust are consistent with radii predicted by SED modelling. Tentative evidence for a common position angle for the dust at 1.7AU with that at 150AU around eta Corvi, which might be expected if the hot dust is fed from the outer disc, demonstrates the potential of this technique for constraining the origin of the dust and more generally for the study of dust in the terrestrial regions of main sequence stars.
description: Accepted for publication in Astronomy and Astrophysics
title: Information resource utilisation: accessibility based on concerns
Creators: name: Rolfe, Richard
Publisher: name: University of Kent
Year: 2023

description: The utilisation of the information resource is a key requirement of an effective information system within the organisation. With computing technology generating increasingly complex applications but with an increasing spread of computing contactability through the organisation, an inherent conflict is presented which can only worsen as hypermedia and multimedia applications are brought to the organisation. This work identified user participation as the key ingredient in improving information resource utilisation. A two pronged approach was taken: initially a field based investigation of the utilisation of a complex information system within a large organisation and secondly the development of a user interface environment to tackle the issues raised. The fieldwork provided evidence to suggest the level of accessibility to Health Service information left wide scope for development. Several variables were identified as having a key relationship with information resource utilisation. Of these complexity predominated, both in terms of the database structures in the application and the functionality provided through the interface itself. The prototype focused on this complexity issue directly, providing a user driven interpretative environment in which both user and organisation based information can be combined to form a dynamic, user based semantic model. Such a graphical representation evolves in paralell with user requirements, enabling the user to manipulate his/her own view of the application for the expression of database queries. The basis for this interpretation is the generalised conceptual model which is captured from the data modeller during the initial application data modelling process. This view forms the basis for user accessibility, acting as an initial interpretation which the user tailors towards a personal interpretation using 'concerns'. The provision of such an environment promotes user accessibility and hence utilisation, being personalised by the individual to the task at hand.
title: ÐÐµÐºÑÐ¾ÑÑ Ð¸ ÑÐµÐ½Ð·Ð¾ÑÑ Ð²ÑÐ¾ÑÐ¾Ð³Ð¾ ÑÐ°Ð½Ð³Ð° Ð² ÑÑÐµÑ Ð¼ÐµÑÐ½Ð¾Ð¼ Ð¿ÑÐ¾ÑÑÑÐ°Ð½ÑÑÐ²Ðµ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ¸Ð»Ð¸Ð½, ÐÐ°Ð²ÐµÐ»
Publisher: name: [Ð¡ÐÐ±ÐÐ¢Ð£]
Year: 1992
Subjects: Ð¢ÐµÐ½Ð·Ð¾ÑÐ½Ð¾Ðµ Ð¸ÑÑÐ¸ÑÐ»ÐµÐ½Ð¸Ðµ
ÐÐµÐºÑÐ¾ÑÐ½Ð¾Ðµ Ð¸ÑÑÐ¸ÑÐ»ÐµÐ½Ð¸Ðµ

description: Ð¡Ð¾Ð´ÐµÑÐ¶Ð°ÑÑÑ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÐµ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¾ Ð²ÐµÐºÑÐ¾ÑÐ°Ñ Ð¸ ÑÐµÐ½Ð·Ð¾ÑÐ°Ñ Ð²ÑÐ¾ÑÐ¾Ð³Ð¾ ÑÐ°Ð½Ð³Ð° Ð² ÑÑÐµÑÐ¼ÐµÑÐ½Ð¾Ð¼ Ð¿ÑÐ¾ÑÑÑÐ°Ð½ÑÑÐ²Ðµ. ÐÐµÑÑÐ°Ð½Ð´Ð°ÑÑÐ½Ð¾ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½ ÑÐ¿Ð¾ÑÐ¾Ð± Ð²Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð»ÑÑÐ½ÑÑ Ð¸ Ð°ÐºÑÐ¸Ð°Ð»ÑÐ½ÑÑ Ð²ÐµÐºÑÐ¾ÑÐ¾Ð²; ÑÐ¿ÑÐ¾ÑÐµÐ½Ð¾ Ð´Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÑÑÑÐ²Ð¾ ÑÐµÐ¾ÑÐµÐ¼Ñ Ð­Ð¹Ð»ÐµÑÐ° Ð¾ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¸ ÑÐµÐ½Ð·Ð¾ÑÐ° Ð¿Ð¾Ð²Ð¾ÑÐ¾ÑÐ°, Ð¿ÑÐ¸ÑÐµÐ¼ ÑÐµÐ¾ÑÐµÐ¼Ð° Ð¾ ÑÐ¿ÐµÐºÑÑÐ°Ð»ÑÐ½Ð¾Ð¼ ÑÐ°Ð·Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¸ Ð½ÐµÑÐ¸Ð¼Ð¼ÐµÑÑÐ¸ÑÐ½Ð¾Ð³Ð¾ ÑÐµÐ½Ð·Ð¾ÑÐ° Ð½Ðµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÑÑÑ Ð²ÑÐ²ÐµÐ´ÐµÐ½Ð¾ Ð¿ÑÐ°Ð²Ð¸Ð»Ð¾ ÐºÐ²Ð°Ð·Ð¸Ð¿ÐµÑÐµÑÑÐ°Ð½Ð¾Ð²Ð¾ÑÐ½Ð¾ÑÑÐ¸ Ð¿Ð¾Ð²Ð¾ÑÐ¾ÑÐ¾Ð², Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑÑÐµÐµ Ð´Ð°ÑÑ Ð½Ð¾Ð²ÑÑ ÑÑÐ°ÐºÑÐ¾Ð²ÐºÑ ÑÐ³Ð»Ð°Ð¼ Ð­Ð¹Ð»ÐµÑÐ° Ð¸ ÑÐ°ÑÑÐ¸ÑÐ¸ÑÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐ¸ Ð¸Ñ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² 1 Ð¸ 2 ÐºÑÑÑÐ¾Ð² Ð²ÑÐµÑ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ¾Ð² Ð¿ÑÐ¸ Ð¸Ð·ÑÑÐµÐ½Ð¸Ð¸ ÐºÑÑÑÐ¾Ð² ÑÐ¸Ð·Ð¸ÐºÐ¸, Ð¼ÐµÑÐ°Ð½Ð¸ÐºÐ¸, ÑÐ¾Ð¿ÑÐ¾ÑÐ¸Ð²Ð»ÐµÐ½Ð¸Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð², ÑÐµÐ¾ÑÐ¸Ð¸ Ð¼Ð°ÑÐ¸Ð½ Ð¸ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð¾Ð² Ð¸ Ñ. Ð¿.
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 ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
Anomalous Flux in the Cosmic Optical Background Detected With New Horizons Observations
Creators: name: Lauer, Tod R.
name: Postman, Marc
name: Spencer, John R.
name: Weaver, Harold A.
name: Stern, S. Alan
name: Gladstone, G. Randall
name: Binzel, Richard P.
name: Britt, Daniel T.
name: Buie, Marc W.
name: Buratti, Bonnie J.
name: Cheng, Andrew F.
name: Grundy, W. M.
name: Horányi, Mihaly
name: Kavelaars, J. J.
name: Linscott, Ivan R.
name: Lisse, Carey M.
name: McKinnon, William B.
name: McNutt, Ralph L.
name: Moore, Jeffrey M.
name: Núñez, Jorge I.
name: Olkin, Catherine B.
name: Parker, Joel W.
name: Porter, Simon B.
name: Reuter, Dennis C.
name: Robbins, Stuart J.
name: Schenk, Paul M.
name: Showalter, Mark R.
name: Singer, Kelsi N.
name: Verbiscer, Anne. J.
name: Young, Leslie A.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We used New Horizons LORRI images to measure the optical-band ($0.4\lesssimλ\lesssim0.9{\rmμm}$) sky brightness within a high galactic-latitude field selected to have reduced diffuse scattered light from the Milky Way galaxy (DGL), as inferred from the IRIS all-sky $100~μ$m map. We also selected the field to significantly reduce the scattered light from bright stars (SSL) outside the LORRI field. Suppression of DGL and SSL reduced the large uncertainties in the background flux levels present in our earlier New Horizons COB results. The raw total sky level, measured when New Horizons was 51.3 AU from the Sun, is $24.22\pm0.80{\rm ~nW ~m^{-2} ~sr^{-1}}.$ Isolating the COB contribution to the raw total required subtracting scattered light from bright stars and galaxies, faint stars below the photometric detection-limit within the field, and the hydrogen plus ionized-helium two-photon continua. This yielded a highly significant detection of the COB at ${\rm 16.37\pm 1.47 ~nW ~m^{-2} ~sr^{-1}}$ at the LORRI pivot wavelength of 0.608 $μ$m. This result is in strong tension with the hypothesis that the COB only comprises the integrated light of external galaxies (IGL) presently known from deep HST counts. Subtraction of the estimated IGL flux from the total COB level leaves a flux component of unknown origin at ${\rm 8.06\pm1.92 ~nW ~m^{-2} ~sr^{-1}}.$ Its amplitude is equal to the IGL.
description: Accepted for publication in the Astrophysical Journal Letters
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸, Ð¿Ð¾ÑÑÑÐ¿Ð°ÑÑÐµÐ¹ Ð¾Ñ Ð´ÐµÐºÐ°Ð¼ÐµÑÑÐ¾Ð²ÑÑ ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾-ÑÐ°Ð·Ð½ÐµÑÐµÐ½Ð½ÑÑ ÑÐ°Ð´Ð¸Ð¾ÑÐµÐ½ÑÑ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ÑÑÐ¾Ð², ÐÐ°Ð»ÐµÑ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: 2017
Subjects: ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ñ
Ð Ð°Ð´Ð¸Ð¾ÑÐµÐ½ÑÑÑ
Ð Ð°Ð´Ð¸Ð¾Ð²Ð¾Ð»Ð½Ñ Ð´ÐµÐºÐ°Ð¼ÐµÑÑÐ¾Ð²ÑÐµ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ Ð¼ÐµÑÐ¾Ð´ Ð´Ð¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸ Ð¾Ñ Ð¿Ð¾Ð´Ð²Ð¸Ð¶Ð½ÑÑ Ð³Ð»Ð¾Ð±Ð°Ð»ÑÐ½Ð¾ ÑÐ´Ð°Ð»ÐµÐ½Ð½ÑÑ Ð¾Ð±ÑÐµÐºÑÐ¾Ð² Ð¿ÑÐ¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ²ÑÐ·Ð¸ Ð² Ð´ÐµÐºÐ°Ð¼ÐµÑÑÐ¾Ð²Ð¾Ð¼ Ð´Ð¸Ð°Ð¿Ð°Ð·Ð¾Ð½Ðµ Ð´Ð»Ð¸Ð½ Ð²Ð¾Ð»Ð½ Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½Ð¾Ð³Ð¾ ÑÐ¾Ð´Ð° Ð¿Ð¾Ð¼ÐµÑ. ÐÐ»Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð·Ð°Ð´Ð°Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ Ð¿Ð¾Ð¼ÐµÑÐ¾ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ Ð² ÑÐºÐ°Ð·Ð°Ð½Ð½ÑÑ ÑÑÐ»Ð¾Ð²Ð¸ÑÑ ÑÐ¸ÑÐ¾ÐºÐ¾Ðµ ÑÐ°ÑÐ¿ÑÐ¾ÑÑÑÐ°Ð½ÐµÐ½Ð¸Ðµ Ð¿Ð¾Ð»ÑÑÐ¸Ð»Ð¸ Ð¼ÐµÑÐ¾Ð´Ñ ÑÐ°Ð·Ð½ÐµÑÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¸ÐµÐ¼Ð°, Ð¾Ð´Ð½Ð°ÐºÐ¾ Ð² ÑÑÐ´Ðµ ÑÐ»ÑÑÐ°ÐµÐ² Ð´Ð°Ð½Ð½ÑÐµ Ð¼ÐµÑÐ¾Ð´Ñ Ð½Ðµ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑÑ Ð¾Ð±ÐµÑÐ¿ÐµÑÐ¸ÑÑ Ð·Ð°Ð´Ð°Ð½Ð½Ð¾Ðµ ÐºÐ°ÑÐµÑÑÐ²Ð¾ ÑÐ²ÑÐ·Ð¸. Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ ÑÐ¾ÑÑÐ¾Ð¸Ñ Ð² Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð¸ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¼ÐµÑÐ¾Ð´Ð° ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾-ÑÐ°Ð·Ð½ÐµÑÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¸ÐµÐ¼Ð° Ð¸ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸, Ð¿Ð¾ÑÑÑÐ¿Ð°ÑÑÐµÐ¹ Ð¾Ñ ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾-ÑÐ´Ð°Ð»ÐµÐ½Ð½ÑÑ ÑÐ°Ð´Ð¸Ð¾ÑÐµÐ½ÑÑÐ°Ñ. Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÐµ Ð´Ð»Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ°Ð´Ð¸Ð¾ÑÐ²ÑÐ·Ð¸ Ð² Ð´ÐµÐºÐ°Ð¼ÐµÑÑÐ¾Ð²Ð¾Ð¼ Ð´Ð¸Ð°Ð¿Ð°Ð·Ð¾Ð½Ðµ Ð²Ð¾Ð»Ð½. ÐÐ°Ð´Ð°Ð½Ð¸Ðµ Ð½Ð° Ð²ÑÐ¿ÑÑÐºÐ½ÑÑ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ°Ð±Ð¾ÑÑ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¾ Ð² Ð¿Ð¾Ð»Ð½Ð¾Ð¼ Ð¾Ð±ÑÐµÐ¼Ðµ.
Formation of a narrow baryon resonance with positive strangeness in K^+ collisions with Xe nuclei
Creators: name: Barmin, V. V.
name: Asratyan, A. E.
name: Borisov, V. S.
name: Curceanu, C.
name: Davidenko, G. V.
name: Dolgolenko, A. G.
name: Guaraldo, C.
name: Kubantsev, M. A.
name: Larin, I. F.
name: Matveev, V. A.
name: Shebanov, V. A.
name: Shishov, N. N.
name: Sokolov, L. I.
name: Tumanov, G. K.
name: Verebryusov, V. S.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The data on the charge-exchange reaction K^+Xe --> K^0 p Xe, obtained with the bubble chamber DIANA, are reanalyzed using increased statistics and updated selections. Our previous evidence for formation of a narrow pK^0 resonance with mass near 1538 MeV is confirmed and reinforced. The statistical significance of the signal reaches some 8σ(6σ) when estimated as S/\sqrt{B} (S/\sqrt{B+S}). The mass and intrinsic width of the Θ^+ baryon are measured as m = (1538+-2) MeV and Γ= (0.39+-0.10) MeV.
description: 13 pages, 9 figures
title: ÐÐ½Ð°Ð»Ð¸Ð· ÑÑÑÐ°Ð½Ð¾Ð²Ð¸Ð²ÑÐ¸Ñ ÑÑ Ð¸ Ð¿ÐµÑÐµÑ Ð¾Ð´Ð½ÑÑ ÑÐµÐ¶Ð¸Ð¼Ð¾Ð² Ð² ÑÐ»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ðµ 750/330 ÐºÐ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÑÑÐ¾Ð², ÐÐ»ÐµÐºÑÐµÐ¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÑÐ¸ÑÑÐµÐ¼Ð° ÑÐ»ÐµÐºÑÑÐ¾ÑÐ½Ð°Ð±Ð¶ÐµÐ½Ð¸Ñ
Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ°Ñ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÑ
ÑÐµÐ¶Ð¸Ð¼ Ð¼Ð¸Ð½Ð¸Ð¼Ð°Ð»ÑÐ½ÑÑ Ð½Ð°Ð³ÑÑÐ·Ð¾Ðº
ÑÑÑÐ°Ð½Ð¾Ð²Ð¸Ð²ÑÐ¸Ð¹ÑÑ ÑÐµÐ¶Ð¸Ð¼
ÑÐµÐ¶Ð¸Ð¼ Ð¼Ð°ÐºÑÐ¸Ð¼Ð°Ð»ÑÐ½ÑÑ Ð½Ð°Ð³ÑÑÐ·Ð¾Ðº
Ð½ÐµÑÐ¸Ð¼Ð¼ÐµÑÑÐ¸ÑÐ½Ð¾Ðµ ÐºÐ¾ÑÐ¾ÑÐºÐ¾Ðµ Ð·Ð°Ð¼ÑÐºÐ°Ð½Ð¸Ðµ

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¸Ð·ÑÑÐµÐ½Ð° ÑÐ¸ÑÑÐµÐ¼Ð° ÑÐ»ÐµÐºÑÑÐ¾ÑÐ½Ð°Ð±Ð¶ÐµÐ½Ð¸Ñ 750/330 ÐºÐ. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ Ð²ÑÐ±Ð¾Ñ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² ÑÐ»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ: ÑÑÐ°Ð½ÑÑÐ¾ÑÐ¼Ð°ÑÐ¾ÑÐ¾Ð² Ð¸ ÑÐµÑÐµÐ½Ð¸Ð¹ ÐÐ­Ð. Ð¡Ð´ÐµÐ»Ð°Ð½Ñ ÑÐ°ÑÑÐµÑÑ ÑÑÑÐ°Ð½Ð¾Ð²Ð¸Ð²ÑÐµÐ³Ð¾ÑÑ ÑÐµÐ¶Ð¸Ð¼Ð° ÑÐ°Ð±Ð¾ÑÑ âÐ²ÑÑÑÐ½ÑÑâ Ð¸ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ RastrWIN, Ð° ÑÐ°Ðº Ð¶Ðµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐµÐ¶Ð¸Ð¼Ñ Ð¼Ð°ÐºÑÐ¸Ð¼Ð°Ð»ÑÐ½ÑÑ Ð¸ Ð¼Ð¸Ð½Ð¸Ð¼Ð°Ð»ÑÐ½ÑÑ Ð½Ð°Ð³ÑÑÐ·Ð¾Ðº. ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ ÑÐ¾ÐºÐ¸ Ð¸ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ Ð¿ÑÐ¸ Ð´Ð²ÑÑÑÐ°Ð·Ð½Ð¾Ð¼ ÐºÐ¾ÑÐ¾ÑÐºÐ¾Ð¼ Ð·Ð°Ð¼ÑÐºÐ°Ð½Ð¸Ð¸ Ð² ÑÐ·Ð»Ðµ Ð¿ÐµÑÐµÑÐµÑÐµÐ½Ð¸Ñ Ð»Ð¸Ð½Ð¸Ð¹ Ð¾ÑÑÐ¾Ð´ÑÑÐ¸Ñ Ð¾Ñ Ð´Ð²ÑÑ Ð³ÐµÐ½ÐµÑÐ°ÑÐ¾ÑÐ¾Ð² Ð¸ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ñ Ð²ÐµÐºÑÐ¾ÑÐ½ÑÐµ Ð´Ð¸Ð°Ð³ÑÐ°Ð¼Ð¼Ñ. Ð Ð·Ð°ÐºÐ»ÑÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐ°ÑÑÐ¸ ÑÐ°Ð±Ð¾ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð° Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ°Ñ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÑ ÑÐ¸ÑÑÐµÐ¼Ñ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Dymola.
title:  Some Practical Consequences Of The Achmea Judgment For Intra Eu Investment Arbitration
Creators: name: Hartkamp ,  Arthur
Publisher: name: Roma TrE-Press
Year: 2021

description: Nella sentenza Achmea, la Corte di giustizia dell’Unione europea ha stabilito che i Trattati di Investimento Bilaterali (TBI) stipulati tra Stati membri dell’Unione europea sono incompatibili con il Trattato sul funzionamento dell’Unione europea. La sentenza non dovrebbe influire sulla validità degli atti procedurali anteriori alla data della sentenza e le corti nazionali dovrebbero astenersi dal negare l’esecutività dei lodi arbitrali per contrasto con l’ordine pubblico. Il contributo, quindi, analizza se e in quale misura la sentenza avrà un impatto con riferimento (i) alle procedure arbitrali basate sui vari trattati sugli investimenti che non siano trattati bilaterali intra-UE, e (II) sulle procedure arbitrali in materia di investimenti basate su accordi diversi da trattati sugli investimenti.
description: National Judges and the Case Law of the Court of Justice of the European Union
The first gigayear of bulge star formation in Virgo ellipticals: constraints from their globular cluster systems
Creators: name: Spitler, Lee R.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Data products from the Advanced Camera for Surveys Virgo Cluster Survey are used to understand the bulge star formation history in early-type galaxies at redshifts z > 2. A new technique is developed whereby observed high-redshift age-metallicity relationships are utilized to constrain the typical formation epochs of metal-rich or "bulge" globular clusters. This analysis supports a model where massive Virgo galaxies underwent an extremely intense mode of bulge globular cluster formation at z ~ 3.5 that was followed by an era of significant bulge growth and little globular cluster production. Intermediate-mass galaxies showed a less-intense period of globular cluster formation at z ~ 2.5 that was synchronized with the bulk of bulge star growth. The transition between the massive and intermediate-mass galaxy star formation modes occurs at a galaxy stellar mass of M_stellar ~ 3 x 10^10 M_sun, the mass where many other galaxy properties are observed to change. Dwarf early-type galaxies in Virgo may have experienced no significant period of bulge globular cluster formation, thus the intense star bursts associated with globular cluster formation may be difficult to directly observe at redshifts z < 4. Though the above conclusions are preliminary because they are based upon uncertain relationships between age and metallicity, the technique employed will yield more stringent constraints as high-redshift galaxy observations and theoretical models improve.
description: Accepted by MNRAS. 9 pages text. 6 figures.
Increasing access to evidence synthesis methods through tool development and capacity-building
Creators: name: Grames, Eliza
name: Young, Sarah
Publisher: name: Zenodo
Year: 2022
Subjects: ESMARConf2022
evidence synthesis
meta-analysis
RStats

description: Building methods and tools is only a first step toward facilitating and supporting evidence synthesis -- improving access for end users is a critical next step in making these methods and tools usable, sustainable and effective. This presentation will discuss how access to the R package litsearchr, used for information retrieval in evidence synthesis, was improved through two approaches: training and curriculum development and the development of a graphical user interface. We'll reflect on considerations for developers and end users in the building and maintenance of open source tools for access and accessibility.