cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ÐÐ¾Ð²ÑÑÐµÐ½Ð¸Ðµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð² Ð¿ÑÑÐµÐ¼ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð¸Ð½ÑÐµÑÐ½ÐµÑ-ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¹
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐ¾Ð»ÑÐºÐ¾Ð²Ð°, ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ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: 2017
Subjects: ÐÐ½ÑÐµÑÐ½ÐµÑ
ÐÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ·ÑÐºÐ¸
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description: ÐÐ°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð¸Ð½ÑÐµÑÐ½ÐµÑ-ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð´Ð»Ñ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ð¸ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð² Ñ ÑÐµÐ»ÑÑ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸. Ð ÐºÐ°ÑÐµÑÑÐ²Ðµ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð² Ð²ÑÐ±ÑÐ°Ð½Ñ Ð¿ÑÐ¾ÑÐµÑÑÑ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¸ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð·Ð°ÑÐ²Ð¾Ðº Ð½Ð° ÑÐµÑÑÐ¾ÑÐ°Ð½Ð½Ð¾Ðµ Ð¾Ð±ÑÐ»ÑÐ¶Ð¸Ð²Ð°Ð½Ð¸Ðµ ÑÑÐ°ÑÑÐ½Ð¸ÐºÐ¾Ð² Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð¹ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ð¸. Ð¡Ð¾Ð·Ð´Ð°Ð½Ð¾ Ð¼Ð½Ð¾Ð³Ð¾Ð¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÐµÐ»ÑÑÐºÐ¾Ðµ Ð¸Ð½ÑÐµÑÐ½ÐµÑ-Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð½Ð°ÑÑÐ½ÑÑ ÑÑÐ°ÑÐµÐ¹ Ðº Ð¿ÑÐ±Ð»Ð¸ÐºÐ°ÑÐ¸Ð¸, Ð´Ð»Ñ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ ÐºÐ¾ÑÐ¾ÑÐ¾Ð³Ð¾ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°ÑÑ Ð¸Ð½ÑÑÑÑÐºÑÐ¸Ñ Ð´Ð»Ñ ÑÐµÐ³Ð¸ÑÑÑÐ°ÑÐ¸Ð¸ Ð¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÐµÐ»ÐµÐ¹ Ð½Ð° Ð´Ð²ÑÑ ÑÐ·ÑÐºÐ°Ñ, ÑÑÑÑÐºÐ¾Ð¼ Ð¸ Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð¼, Ð¸ ÑÐ°Ð¹Ð»Ñ Ð¿Ð¾Ð¼Ð¾ÑÐ¸ Ð´Ð»Ñ ÑÐ°Ð±Ð¾ÑÑ Ð² Ð»Ð¸ÑÐ½ÑÑ ÐºÐ°Ð±Ð¸Ð½ÐµÑÐ°Ñ Ð·Ð°ÑÐµÐ³Ð¸ÑÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÐµÐ»ÐµÐ¹ Ð² ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ð¸ Ñ Ð·Ð°ÑÐ²Ð»ÐµÐ½Ð½ÑÐ¼Ð¸ ÑÑÐ°ÑÑÑÐ°Ð¼Ð¸. ÐÐ»Ñ ÑÐ°Ð·Ð¼ÐµÑÐµÐ½Ð¸Ñ ÑÐ¾Ð·Ð´Ð°Ð½Ð½ÑÑ Ð¸Ð½ÑÑÑÑÐºÑÐ¸Ð¹ Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ Ð½Ð°Ð¿Ð¸ÑÐ°ÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½ÑÐµ ÐºÐ¾Ð´Ñ. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¾Ð¿Ð¸ÑÐ°Ð½Ñ Ð¿ÑÐ¾ÑÐµÑÑÑ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð½Ð°ÑÑÐ½ÑÑ ÑÑÐ°ÑÐµÐ¹ Ðº Ð¿ÑÐ±Ð»Ð¸ÐºÐ°ÑÐ¸Ð¸, Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¾, ÐºÐ°ÐºÐ¸Ð¼ Ð¾Ð±ÑÐ°Ð·Ð¾Ð¼ Ð¾ÑÑÑÐµÑÑÐ²Ð»ÐµÐ½Ð¾ ÑÐµÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¸ ÐµÐµ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ðµ. ÐÐ»Ñ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð·Ð°ÑÐ²Ð¾Ðº Ð½Ð° ÑÐµÑÑÐ¾ÑÐ°Ð½Ð½Ð¾Ðµ Ð¾Ð±ÑÐ»ÑÐ¶Ð¸Ð²Ð°Ð½Ð¸Ðµ ÑÐ¾Ð·Ð´Ð°Ð½Ð¾ Ð¼Ð½Ð¾Ð³Ð¾Ð¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÐµÐ»ÑÑÐºÐ¾Ðµ Ð¸Ð½ÑÐµÑÐ½ÐµÑ-Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ ÑÐµÐ³Ð¸ÑÑÑÐ°ÑÐ¸Ð¸ ÑÑÐ°ÑÑÐ½Ð¸ÐºÐ¾Ð² Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ Ð¸ Ð¾ÑÐ¾ÑÐ¼Ð»ÐµÐ½Ð¸Ñ Ð·Ð°ÐºÐ°Ð·Ð¾Ð² Ð½Ð° ÐºÐ°Ð¶Ð´ÑÐ¹ Ð´ÐµÐ½Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ð¸. Ð ÑÐ¾Ð´Ðµ ÑÐ°Ð±Ð¾ÑÑ ÑÐ°ÑÑÐ¼Ð°ÑÑÐµÐ½Ð° ÑÐ¸ÑÑÐµÐ¼Ð° ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Joomla 3, Ð¸Ð·ÑÑÐµÐ½Ñ ÑÐ·ÑÐºÐ¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ HTML, PHP, CSS Ð¸ Ð±Ð°Ð·Ð° Ð´Ð°Ð½Ð½ÑÑ MySQL. Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ð¾ ÑÐµÑÐ½Ð¸ÐºÐ¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¾ÐµÐºÑÐ°.
The ROB-MEN Shiny app to evaluate risk of bias due to missing evidence in network meta-analysis
Creators: name: Chiocchia, Virginia
Publisher: name: Zenodo
Year: 2022
Subjects: ESMARConf2022
evidence synthesis
meta-analysis
RStats

description: We recently proposed a framework to evaluate the impact of reporting bias on the meta-analysis of a network of interventions, which we called ROB-MEN (Risk Of Bias due to Missing Evidence in Network meta-analysis). In this presentation we will show the ROB-MEN Shiny app which we developed to facilitate this risk of bias evaluation process. ROB-MEN first evaluates the risk of bias due to missing evidence for each pairwise comparison separately. This step considers possible bias due to the presence of studies with unavailable results and the potential for unpublished studies. The second step combines the overall judgements about the risk of bias in pairwise comparisons with the percentage contribution of direct comparisons on the network meta-analysis (NMA) estimates, the likelihood of small-study effects, and any bias from unobserved comparisons. Then, a level of “low risk”, “some concerns” or “high risk” of bias due to missing evidence is assigned to each estimate. The ROB-MEN Shiny app runs the required analysis, semi-automates some of the steps and built-in algorithm to assign the overall risk of bias level for the NMA estimates and produces the tool’s output tables. We will present how the ROB-MEN app works using an illustrative example from a published NMA. ROB-MEN is the first tool for assessing the risk of bias due to missing evidence in NMA and is also incorporated in the reporting bias domain of the CINeMA software for evaluating the confidence in the NMA results.
The Phase Diagram for Wess-Zumino Models
Creators: name: Synatschke, Franziska
name: Gies, Holger
name: Wipf, Andreas
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Dynamical supersymmetry breaking is an important issue for applications of supersymmetry in particle physics. The functional renormalization group equations allow for a nonperturbative approach that leaves supersymmetry intact. Therefore they offer a promising tool to investigate dynamical supersymmetry breaking. Here we will employ this method to derive the phase diagram and a surprisingly rich RG fixed-point structure with corresponding critical exponents for the $\mathcal N=1$ Wess-Zumino model in two dimensions.
description: 4 pages, 4 figures, talk given at SUSY09, Boston, MA, 5-10 June 2009, to appear in the proceedings
A pseudo adrenal lesion: Gastric diverticulum on CT and MR imaging
Creators: name: Kantarci, Mecit
Publisher: name: EURORAD
Year: 2014
Subjects: subject: Abdomen
subject: CT
subject: MR
subject: Contrast agent-intravenous
subject: Education
subject: Pathology

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: female, 47 years
description: Clinical History: A 47-year-old female patient had a palpitation symptoms for two weeks. She underwent to our department for investigation of hypertension. Final Diagnosis: Gastric diverticulum
Integrated River Management Models: Implications for Collaborative Governance and Management of the Angat River Basin, Philippines
Creators: name: Fresco, Theresa
Publisher: name: The University of British Columbia
Year: 2016

description: As the main municipal water source for Metro Manila’s 12 million residents, supplier of irrigation water to 26,791 hectares of farmland in Pampanga and Bulacan provinces, flood control for downstream municipalities and provider of 10% of the nation’s hydroelectricity, the Angat River Basin is of prime socioeconomic importance to Luzon, the central island and economic centre of the Philippines. According to the National Irrigation Administration (NIA), the Manila Waterworks and Sewerage Board (MWSS) and the National Power Corporation (NPC), future water requirements for domestic, commercial and industrial purposes on Luzon Island show remarkable increases. In addition to the challenges of climate change, longer droughts and intense weather events, the already stressed Angat River is projected to face increased water demand due to rural to urban migration into Metro Manila, projected doubling of population in Bulacan Province in the next decade, increased industrialization and increased demand for hydroelectricity. Given the complexity, breadth of competing uses and interrelated nature of natural systems such as river basins, collaborative governance has been an effective strategy to grapple with the challenges of fragmented and siloed agencies dealing with water management. In order to provide insight on a potential response to these challenges of governance in the Angat River system, this study seeks to explore existing, international case studies of collaborative governance models, their implications and potential recommendations for Angat’s management.
title: ÐÐ½Ð°Ð»Ð¸Ð· ÐºÐ»ÐµÑÐ¾ÑÐ½ÑÑ ÑÑÑÑÐºÑÑÑ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ ÑÐ¸ÑÑÐµÐ¼ ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ð³Ð¾ Ð·ÑÐµÐ½Ð¸Ñ
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°ÑÐºÐ¾Ð², ÐÐ½Ð´ÑÐµÐ¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸
ÐÐ·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ñ
ÐÐ»ÐµÑÐºÐ° (Ð±Ð¸Ð¾Ð».)
ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ðµ Ð·ÑÐµÐ½Ð¸Ðµ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐ¸ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ð¹ ÐºÐ»ÐµÑÐ¾ÑÐ½ÑÑ ÑÑÑÑÐºÑÑÑ. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½ Ð¾Ð±Ð·Ð¾Ñ ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð°Ð½Ð°Ð»Ð¸Ð·Ð¾Ð² Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ð¹. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð²ÑÐ´Ð²Ð¸Ð³Ð°ÐµÐ¼ÑÑ Ðº ÑÐ°Ð·ÑÐ°Ð±Ð°ÑÑÐ²Ð°ÐµÐ¼Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ðµ. Ð ÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð¼ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ð° Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ð¹ ÐºÐ»ÐµÑÐ¾ÑÐ½ÑÑ ÑÑÑÑÐºÑÑÑ.
Vetting Asteroseismic $Δν$ Measurements using Neural Networks
Creators: name: Reyes, Claudia
name: Stello, Dennis
name: Hon, Marc
name: Zinn, Joel C.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Precise asteroseismic parameters allow one to quickly estimate radius and mass distributions for large samples of stars. A number of automated methods are available to calculate the frequency of maximum acoustic power ($ν_{\mathrm{max}}$) and the frequency separation between overtone modes ($Δν$) from the power spectra of red giants. However, filtering through the results requires either manual vetting, elaborate averaging across multiple methods, or sharp cuts in certain parameters to ensure robust samples of stars free of outliers. Given the importance of ensemble studies for Galactic archaeology and the surge in data availability, faster methods for obtaining reliable asteroseismic parameters are desirable. We present a neural network classifier that vets $Δν$ by combining multiple features from the visual $Δν$ vetting process. Our classifier is able to analyse large numbers of stars determining whether their measured $Δν$ are reliable thus delivering clean samples of oscillating stars with minimal effort. Our classifier is independent of the method used to obtain $ν_{\mathrm{max}}$ and $Δν$, and therefore can be applied as a final step to any such method. Tests of our classifier's performance on manually vetted $Δν$ measurements reach an accuracy of 95%. We apply the method to giants observed by K2 Galactic Archaeology Program and find that our results retain stars with astrophysical oscillation parameters consistent with the parameter distributions already defined by well-characterised Kepler red giants.
description: Accepted for publication in Monthly Notices of the Royal Astronomical Society Main Journal
title: ÐÐ½ÐµÑÐ½ÐµÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÐÐ¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ½Ð¸ÑÐ°ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¢Ð°Ð´Ð¶Ð¸ÐºÑÐºÐ¾Ð¹ Ð°Ð»ÑÐ¼Ð¸Ð½Ð¸ÐµÐ²Ð¾Ð¹ ÐºÐ¾Ð¼Ð¿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°ÑÑÐ»Ð¾Ð², ÐÐ¾Ð±ÑÑ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð²Ð½ÐµÑÐ½ÐµÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
ÑÐºÑÐ¿Ð¾ÑÑ Ð°Ð»ÑÐ¼Ð¸Ð½Ð¸Ñ
ÐÐ£Ð Ð¢ÐÐÐÐ
Ð¿ÑÐ¸Ð±ÑÐ»Ñ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐ£Ð Ð¢ÐÐÐÐ
Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð°Ð½Ð°Ð»Ð¸Ð· Ð²Ð½ÐµÑÐ½ÐµÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐÐ£Ð Ð¢ÐÐÐÐ, Ð´Ð»Ñ Ð¿ÑÐ¾Ð³Ð½Ð¾Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð²Ð½ÐµÑÐ½ÐµÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸.
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title: ÐÐ½Ð°Ð»Ð¸Ð· Ð¸ Ð¿ÑÐ¾Ð³Ð½Ð¾Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¾Ð±ÑÐµÐ¼Ð° Ð¾Ð±Ð¾ÑÐ¾ÑÐ° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°Ð·Ð°ÑÐ¾Ð², ÐÐ½Ð´Ñ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Ð¾Ð²Ð°ÑÐ¾Ð¾Ð±Ð¾ÑÐ¾Ñ
ÑÐ¾Ð·Ð½Ð¸ÑÐ½Ð¾Ðµ ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ðµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ðµ
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description: ÐÐ°Ð½Ð° Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° ÐÐÐ Â«Ð¢ÐµÐ¼Ð¿Â», Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½ SWOT- Ð¸ PEST-Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ°ÐºÑÐ¾ÑÐ¾Ð² Ð²Ð½ÐµÑÐ½ÐµÐ¹ ÑÑÐµÐ´Ñ, Ð¾ÐºÐ°Ð·ÑÐ²Ð°ÑÑÐ¸Ñ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð½Ð° ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½ÑÑ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÑÐ¾Ð·Ð½Ð¸ÑÐ½Ð¾Ð³Ð¾ ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¾Ð·Ð½Ð¸ÑÐ½Ð¾Ð³Ð¾ ÑÐ¾Ð²Ð°ÑÐ¾Ð¾Ð±Ð¾ÑÐ¾ÑÐ° ÐÐÐ Â«Ð¢ÐµÐ¼Ð¿Â» Ð¿Ð¾ Ð¾Ð±ÑÐµÐ¼Ñ Ð¸ ÑÑÑÑÐºÑÑÑÐµ Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ñ Ð¾Ð±ÑÐµÐ¼Ð° Ð¾Ð±Ð¾ÑÐ¾ÑÐ° Ð¸ÑÑÐ»ÐµÐ´ÑÐµÐ¼Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð½Ð° Ð¿Ð»Ð°Ð½Ð¸ÑÑÐµÐ¼ÑÐ¹ 2017 Ð³Ð¾Ð´.
SuperWASP observations of long timescale photometric variations in cataclysmic variables
Creators: name: Thomas, N. L.
name: Norton, A. J.
name: Pollacco, D.
name: West, R. G.
name: Wheatley, P. J.
name: Enoch, B.
name: Clarkson, W. I.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We investigated whether the predictions and results of Stanishev et al (2002) concerning a possible relationship between eclipse depths in PX And and its retrograde disc precession phase, could be confirmed in long term observations made by SuperWASP. In addition, two further CVs (DQ Her and V795 Her) in the same SuperWASP data set were investigated to see whether evidence of superhump periods and disc precession periods were present and what other, if any, long term periods could be detected. The results of our period and eclipse analysis on PX And confirm that the negative superhump period is 0.1417 \pm 0.0001d. We find no evidence of positive superhumps in our data suggesting that PX And may have been in a low state during our observations. We improve on existing estimates of the disc precession period and find it to be 4.43 \pm 0.05d. Our results confirm the predictions of Stanishev et al (2002). We find that DQ Her does not appear to show a similar variation for we find no evidence of negative superhumps or of a retrograde disc precession. We also find no evidence of positive superhumps or of a prograde disc precession and we attribute the lack of positive superhumps in DQ Her to be due to the high mass ratio of this CV. We do however find evidence for a modulation of the eclipse depth over a period of 100 days which may be linked with solar-type magnetic cycles which give rise to long term photometric variations. The periodogram analysis for V795 Her detected the likely positive superhump period 0.1165d, however, neither the 0.10826d orbital period or the prograde 1.53d disc precession period were seen. Here though we have found a variation in the periodogram power function at the positive superhump period, over a period of at least 120 days.
description: 13 figures
"Doing Meta-Analysis with R": Motivation, Concept and Features of an Open-Source Guide for Beginners
Creators: name: Harrer, Mathias
Publisher: name: Zenodo
Year: 2022
Subjects: ESMARConf2022
evidence synthesis
meta-analysis
RStats

description: Meta-analytic methods have become an indispensable tool in many research disciplines. Worldwide, students and applied researchers acquire meta-analytic skills to address scientific questions pertinent to their field. Along with its extensions, R now arguably provides the most comprehensive, state-of-the-art toolkit for conducting meta-analyses. For novices, however, this wealth of R-based tools is often difficult to navigate and translate into practice, which may limit the uptake of available infrastructure. The “Doing Meta-Analysis with R” guide is one example of a project aiming to facilitate access to the R meta-analysis universe. It is primarily geared towards individuals without prior knowledge of R, meta-analysis, or both. We present the motivation, teaching concept, and core features of the guide. A brief overview of the technical implementation as an online, open-source resource based on {bookdown}, {shiny} and GitHub is also provided. Lastly, we discuss potential limitations of our approach, point to other user-friendly tools for new meta-analysts, and share general ideas to make the R meta-analysis infrastructure more accessible for everyone.
Baryon Resonance Analysis from SAID
Creators: name: Arndt, R. A.
name: Briscoe, W. J.
name: Paris, M. W.
name: Strakovsky, I. I.
name: Workman, R. L.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Nuclear Theory (nucl-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Experiment (hep-ex)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: We discuss the analysis of data from piN elastic scattering and single pion photo- and electroproduction. The main focus is a study of low-lying non-strange baryon resonances. Here we concentrate on some difficulties associated with resonance identification, in particular the Roper and higher P11 states.
description: 4 pages, 6 figures; Nstar2009 Conf Proceedings; small revision
title: ÐÐ¾Ð²ÑÑÐµÐ½Ð¸Ðµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐ¸ÑÐº-Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÐ° Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑ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»Ð¾ÑÐµÐ½ÐºÐ¾Ð²Ð°, ÐÐ°Ð»ÐµÐ½Ñ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: 2017
Subjects: ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ
Ð¿Ð¾Ð·Ð¸ÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð¼Ð°ÑÑÐ¸ÑÐ° ÑÐ¸ÑÐºÐ¾Ð²

description: Ð¦ÐµÐ»ÑÑ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¸ÑÐº Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÐ° Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸. ÐÐ»Ñ Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ñ ÑÐµÐ»Ð¸ Ð±ÑÐ»Ð° Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð° ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ ÑÐ¸ÑÐºÐ¾Ð², Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ Ð¸ Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð´Ñ Ð¾ÑÐµÐ½ÐºÐ¸ Ð¸ ÑÐ¿Ð¾ÑÐ¾Ð±Ñ Ð¼Ð¸Ð½Ð¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ¸ÑÐºÐ¾Ð² Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸, Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÑÐ°Ð¿Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ¸ÑÐºÐ°Ð¼Ð¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð° Ð¸Ð´ÐµÐ½ÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ Ð²Ð»Ð¸ÑÑÐµÐ»ÑÐ½ÑÑ ÑÐ¸ÑÐºÐ¾Ð² Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸, Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÑÐµÑÐ±Ð° ÐºÐ¾Ð½ÐºÑÐµÑÐ½Ð¾Ð³Ð¾ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¸ÑÐºÐ° Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸, Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð´Ñ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¸ÑÐº Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÐ° Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸, Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÐµÐµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¼Ð°ÑÑÐ¸ÑÑ ÑÐ¸ÑÐºÐ¾Ð². ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¸ Ð¾ÑÐµÐ½ÐºÐ¸ ÑÐ¸ÑÐºÐ¾Ð² Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð±ÑÐ» ÑÐ´ÐµÐ»Ð°Ð½ Ð²ÑÐ²Ð¾Ð´ Ð¾ Ð·Ð½Ð°ÑÐ¸Ð¼Ð¾ÑÑÐ¸ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ¸ÑÐºÐ°Ð¼Ð¸ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸, Ð¾ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÐ¸ Ð¸Ñ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ, Ð¾ Ð·Ð½Ð°ÑÐ¸Ð¼Ð¾ÑÑÐ¸ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð° Ð¼Ð°ÑÑÐ¸ÑÑ ÑÐ¸ÑÐºÐ¾Ð² Ð´Ð»Ñ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐ¸ÑÑÐµÐ¼ ÑÐ¸ÑÐº Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÐ°.
title: ÐÑÐ¸Ð½Ñ ÑÐ¾Ð½Ð½ÑÐ¹ ÑÐ°ÑÑÐ¾ÑÐ½Ð¾-ÑÐ¿ÑÐ°Ð²Ð»ÑÐµÐ¼ÑÐ¹ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ Ð´Ð»Ñ Ð¿ÑÐ¸Ð²Ð¾Ð´Ð° ÑÑÐ³Ð¾Ð²Ð¾Ð¹ Ð»ÐµÐ±ÐµÐ´ÐºÐ¸ Ð¿ÑÑÐµÑÐºÐ»Ð°Ð´Ð¾ÑÐ½Ð¾Ð³Ð¾ ÐºÑÐ°Ð½Ð°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÑÐ·ÐµÐ²Ð°, 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Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¼Ð°ÑÐ¸Ð½Ñ
Ð°ÑÐ¸Ð½Ñ ÑÐ¾Ð½Ð½ÑÐ¹ ÑÑÐ³Ð¾Ð²ÑÐ¹ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ
ÑÐ°ÑÑÐ¾ÑÐ½Ð¾-ÑÐµÐ³ÑÐ»Ð¸ÑÑÐµÐ¼ÑÐ¹ ÑÐ»ÐµÐºÑÑÐ¾Ð¿ÑÐ¸Ð²Ð¾Ð´
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description: Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½ Ð¸ ÑÐ¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½ Ð°ÑÐ¸Ð½ÑÑÐ¾Ð½Ð½ÑÐ¹ ÑÐ»ÐµÐºÑÑÐ¾Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ Ñ ÐºÐ¾ÑÐ¾ÑÐºÐ¾Ð·Ð°Ð¼ÐºÐ½ÑÑÑÐ¼ ÑÐ¾ÑÐ¾ÑÐ¾Ð¼ Ð´Ð»Ñ Ð¿ÑÐ¸Ð²Ð¾Ð´Ð° ÐºÑÐ°Ð½Ð¾Ð²Ð¾Ð¹ Ð»ÐµÐ±ÑÐ´ÐºÐ¸, Ð¼Ð¾ÑÐ½Ð¾ÑÑÑÑ 30 ÐºÐÑ, ÑÑÐµÐ¿ÐµÐ½ÑÑ Ð·Ð°ÑÐ¸ÑÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¾Ñ Ð²Ð½ÐµÑÐ½Ð¸Ñ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ð¹ IP 44, ÑÐ¿Ð¾ÑÐ¾Ð±Ð¾Ð¼ Ð¼Ð¾Ð½ÑÐ°Ð¶Ð° IM 1001 Ð¸ ÑÐ¿Ð¾ÑÐ¾Ð±Ð¾Ð¼ Ð¾ÑÐ»Ð°Ð¶Ð´ÐµÐ½Ð¸Ñ IC01 Ñ Ð²ÐµÐ½ÑÐ¸Ð»ÑÑÐ¾ÑÐ¾Ð¼. Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐ°Ð·Ð¼ÐµÑÑ Ð°ÑÐ¸Ð½ÑÑÐ¾Ð½Ð½Ð¾Ð³Ð¾ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ (Ð²ÑÑÐ¾ÑÐ° Ð¾ÑÐ¸ Ð²ÑÐ°ÑÐµÐ½Ð¸Ñ, Ð²Ð½ÑÑÑÐµÐ½Ð½Ð¸Ð¹ Ð´Ð¸Ð°Ð¼ÐµÑÑ ÑÑÐ°ÑÐ¾ÑÐ°, Ð¿Ð¾Ð»ÑÑÐ½Ð¾Ðµ Ð´ÐµÐ»ÐµÐ½Ð¸Ðµ, ÑÐ°Ð·Ð¼ÐµÑÑ Ð·ÑÐ±ÑÐ¾Ð²Ð¾Ð¹ Ð·Ð¾Ð½Ñ Ð¸ Ð²Ð¾Ð·Ð´ÑÑÐ½Ð¾Ð³Ð¾ Ð·Ð°Ð·Ð¾ÑÐ°), ÑÐ»ÐµÐºÑÑÐ¾Ð¼Ð°Ð³Ð½Ð¸ÑÐ½ÑÐµ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÑ (Ð»Ð¸Ð½ÐµÐ¹Ð½Ð°Ñ ÑÐ¾ÐºÐ¾Ð²Ð°Ñ Ð½Ð°Ð³ÑÑÐ·ÐºÐ°, Ð¿Ð»Ð¾ÑÐ½Ð¾ÑÑÑ ÑÐ¾ÐºÐ°). ÐÑÐ» Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ ÑÐ°ÑÑÐµÑ Ð¼Ð°Ð³Ð½Ð¸ÑÐ½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ, Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ Ð¸ Ð´Ð¾Ð±Ð°Ð²Ð¾ÑÐ½ÑÑ Ð¿Ð¾ÑÐµÑÑ. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ ÑÑÐ¸Ñ Ð´Ð°Ð½Ð½ÑÑ Ð±ÑÐ»Ð¸ ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½Ñ ÑÐ°Ð±Ð¾ÑÐ¸Ðµ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÐµÐ¿Ð»Ð¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ. ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð° ÑÐ°Ð±Ð¾ÑÐ° Ð°ÑÐ¸Ð½ÑÑÐ¾Ð½Ð½Ð¾Ð³Ð¾ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ Ð¿ÑÐ¸ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÑÐ°ÑÑÐ¾ÑÐ°Ñ.
The $E_{p}$ Evolutionary Slope within the Decay Phase of "FRED" Gamma-ray Burst Pulses
Creators: name: Peng, Z. Y.
name: Ma, L.
name: Zhao, X. H.
name: Yin, Y.
name: Fang, L. M.
name: Bao, Y. Y.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Employing two samples containing of 56 and 59 well-separated FRED (fast rise and exponential decay) gamma-ray burst (GRB) pulses whose spectra are fitted by the Band spectrum and Compton model, respectively, we have investigated the evolutionary slope of $E_{p}$ (where $E_{p}$ is the peak energy in the $νFν$ spectrum) with time during the pulse decay phase. The bursts in the samples were observed by the Burst and Transient Source Experiment (BATSE) on the Compton Gamma-Ray Observatory. We first test the $E_{p}$ evolutionary slope during the pulse decay phase predicted by Lu et al. (2007) based on the model of highly symmetric expanding fireballs in which the curvature effect of the expanding fireball surface is the key factor concerned. It is found that the evolutionary slopes are normally distributed for both samples and concentrated around the values of 0.73 and 0.76 for Band and Compton model, respectively, which is in good agreement with the theoretical expectation of Lu et al. (2007). However, the inconsistence with their results is that the intrinsic spectra of most of bursts may bear the Comptonized or thermal synchrotron spectrum, rather than the Band spectrum. The relationships between the evolutionary slope and the spectral parameters are also checked. We show the slope is correlated with $E_{p}$ of time-integrated spectra as well as the photon flux but anticorrelated with the lower energy index $α$. In addition, a correlation between the slope and the intrinsic $E_{p}$ derived by using the pseudo-redshift is also identified. The mechanisms of these correlations are unclear currently and the theoretical interpretations are required.
description: 25 pages, 9 figures, accepted for publication in The Astrophysical Journal
title: ÐÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾-Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ ÑÐµÑ Ð° Ð¿Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ñ Ð¿Ð¾Ð»ÑÑÐ°Ð±ÑÐ¸ÐºÐ°ÑÐ¾Ð² Ð¸Ð· Ð¾Ð²Ð¾ÑÐµÐ¹ Ð¼Ð¾ÑÐ½Ð¾ÑÑÑÑ 4,5 ÑÐ¾Ð½Ð½Ñ Ð² ÑÑÑÐºÐ¸ Ð´Ð»Ñ ÑÐ½Ð°Ð±Ð¶ÐµÐ½Ð¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ Ð¸ ÑÐ¾Ð·Ð½Ð¸ÑÑ Ð³. Ð¢Ð¸Ñ Ð²Ð¸Ð½
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ²Ð°Ð½Ð¾Ð²Ð°, Ð£Ð»ÑÑÐ½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÐ¹ ÑÐµÑ
Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð¾ Ð¿Ð¾Ð»ÑÑÐ°Ð±ÑÐ¸ÐºÐ°ÑÐ¾Ð²
Ð¾Ð²Ð¾ÑÐ¸
ÑÐ½Ð°Ð±Ð¶ÐµÐ½Ð¸Ðµ
Ð°ÑÑÐ¾ÑÑÐ¸Ð¼ÐµÐ½Ñ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸

description: ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¾ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ, Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ°ÑÑÐµÑÑ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð° Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÑÑÑÐºÑÑÑÐ° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÑÐµÐ¼Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, ÐµÐ³Ð¾ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½Ð¾Ðµ ÑÐµÑÐµÐ½Ð¸Ðµ Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸.
Using the bayesmeta R package for Bayesian random-effects meta-regression
Creators: name: Röver, Christian
Publisher: name: Zenodo
Year: 2022
Subjects: ESMARConf2022
evidence synthesis
meta-analysis
RStats

description: The bayesmeta R package facilitates Bayesian meta-analysis within the simple normal-normal hierarchical model (NNHM). Using the same numerical approach, we extended the bayesmeta package to include several covariables instead of only a single "overall mean" parameter. We demonstrate the use of the package for several meta-regression applications, including modifications of regressor matrix and prior settings to implement model variations. Possible applications include consideration of continuous covariables, comparison of study subgroups, and network-meta-analysis.
Brief report on `Radiative $ϕ$ decays with derivative interactions'
Creators: name: Giacosa, Francesco
name: Pagliara, Giuseppe
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study the line shapes of radiative $ϕ$-decays with a direct coupling of the $ϕ$ meson to the $f_{0}(980)$ and $a_{0}(980)$ scalar mesons. The latter couple via derivative interactions to $π_0 π_0$ and $π_0 η$, respectively. Although the kaon-loop mechanism is usually regarded as the dominant mechanism in radiative $ϕ$ decays, here we test a different possibility: we set the kaon-loop to zero and we fit the theoretical curves to the data by retaining only the direct coupling. Remarkably, satisfactory fits can be achieved, mainly due to the effects of derivative interactions of scalar with pseudoscalar mesons.
description: Based on a presentation held at Confinement8, Quark Confinement and the Hadron Spectrum, Mainz (Germany), 1-6 September 2008. To appear in Proceedings of Science
Design Scheme for Mach-Zehnder Interferometric CWDM Wavelength Splitters/Combiners
Creators: name: Cherchi, Matteo
Publisher: name: arXiv
Year: 2009
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We propose an analytical approach to design flattened wavelength splitters with cascaded Mach-Zehnder interferometers when wavelength dependence of the directional couplers cannot be neglected. We start from a geometrical representation of the action of a doubly point symmetrical filter, assuming no wavelength dependence of the couplers. Next we derive the analytical formulas behind its working principle and we extend them to the wavelength dependent case. We also show how the geometrical representation allows to broaden the class of working structures.
title: ÐÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½ÑÐ¹ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐµÑÐ¸ÑÐ°Ð¹Ð»Ð¾, ÐÐ³Ð¾ÑÑ
Publisher: name: Ð¢Ð­Ð
Year: 2012
Subjects: ÐÑÐ¸Ð½ÑÑÐ¸Ðµ ÑÐµÑÐµÐ½Ð¸Ð¹
Ð°Ð½Ð°Ð»Ð¸Ð· Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ
ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð·
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¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¾ Ð² ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ð¸ Ñ ÑÐ°Ð±Ð¾ÑÐµÐ¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¾Ð¹ ÐºÑÑÑÐ° Â«ÐÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½ÑÐ¹ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸Â». ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´ÑÐµÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÑ Ð¿ÑÐ¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ð¸ Ð»ÐµÐºÑÐ¸Ð¹ Ð¸ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð·Ð°Ð½ÑÑÐ¸Ð¹, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐ¸ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐµ Ðº ÑÐµÐºÑÑÐµÐ¼Ñ Ð¸ Ð¿ÑÐ¾Ð¼ÐµÐ¶ÑÑÐ¾ÑÐ½Ð¾Ð¼Ñ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ Ð·Ð½Ð°Ð½Ð¸Ð¹ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð².
Smoothness of Hill's potential and lengths of spectral gaps
Creators: name: Mikhailets, Vladimir
name: Molyboga, Volodymyr
Publisher: name: arXiv
Year: 2010
Subjects: subject: Spectral Theory (math.SP)
subject: FOS: Mathematics
subject: 34L40 (Primary), 47A10 (Secondary), 47A75

description: Let ${γ_q(n)}_{n \in \mathbb{N}}$ be the lengths of spectral gaps in a continuous spectrum of the Hill-Schrödinger operators S(q)u=-u''+q(x)u,\quad x\in \mathbb{R}, with 1-periodic real-valued potentials $q \in L^{2}(\mathbb{T})$. Let weight function $ω:\;[1,\infty)\to (0,\infty)$. We prove that under the condition \exists s\in [0,\infty):\quad k^{s}\llω(k)\ll k^{s+1},\; k\in \mathbb{N}, the map $γ:\, q \mapsto \{γ_{q}(n)}_{n \in \mathbb{N}}$ satisfies the equalities: \verb"i")\quad γ(H^ω) = h_{+}^ω, \verb"ii")\quad γ^{-1}(h_{+}^ω) = H^ω, where the real function space H^ω & ={f=\sum_{k\in \mathbb{Z}}\hat{f}\,(k)e^{i k2πx}\in L^{2}(\mathbb{T})| \sum_{k\in \mathbb{N}} ω^{2}(k)|\hat{f}(k)|^{2}1,c>1:\qquad c^{-1}\leq \frac{ω(λt)}{ω(t)}\leq c\quad\forall t\geq 1,\;λ\in [1,a] then the function class $H^ω$ is a real Hörmander space $H_{2}^ω(\mathbb{T},\mathbb{R})$ with the weight $ω(\sqrt{1+ξ^{2}})$.
description: 8 pages
Screening promising CsV3Sb5-like kagome materials from systematic first-principles evaluation
Creators: name: Jiang, Yutao
name: Yu, Ze
name: Wang, Yuxin
name: Lu, Tenglong
name: Meng, Sheng
name: Jiang, Kun
name: Liu, Miao
Publisher: name: arXiv
Year: 2022
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences

description: CsV3Sb5 kagome lattice holds the promise for manifesting electron correlation, topology and superconducting. However, by far only three CsV3Sb5-like kagome materials have been experimentally spotted. In this work, we enlarge this family of materials to 1386 compounds via element species substitution, and the further screening process suggests that 28 promising candidates have superior thermodynamic stability, hence they are highly likely to be synthesized. Moreover, these compounds possess several identical electronic structures, and can be categorized into five non-magnetic and three magnetic groups accordingly. It is our hope that this work can greatly expand the viable phase space of the CsV3Sb5-like materials for investigating or tuning the novel quantum phenomena in kagome lattice.
MCDHF calculations of the electric dipole moment of radium induced by the nuclear Schiff moment
Creators: name: Bieron, Jacek
name: Gaigalas, Gediminas
name: Gaidamauskas, Erikas
name: Fritzsche, Stephan
name: Indelicato, Paul
name: Jönsson, Per
Publisher: name: arXiv
Year: 2009
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: The multiconfiguration Dirac-Hartree-Fock theory (MCDHF) has been employed to calculate the electric dipole moment of the 7s6d 3D2 state of radium induced by the nuclear Schiff moment. The results are dominated by valence and core-valence electron correlation effects. We show that the correlation effects can be evaluated in a converged series of multiconfiguration expansions.
title: Ð Ð°ÑÑÐµÑ Ð¿ÑÐ¸Ñ Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÑÐµÐ½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½Ð¾Ð³Ð¾ Ð·Ð°Ð½ÑÑÐ¸Ñ Ð² Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐµ ÑÐµÑ ÑÐ¾Ð²Ð°Ð»ÑÑÐ¸ÐºÐ¾Ð²
title: Calculation of the mental tension of a training lesson in the preparation of fenters
Creators: name: Ð ÑÐ¶ÐºÐ¾Ð²Ð°, Ð.
name: "Ð¡Ð¿Ð¾ÑÑ, ÑÐµÐ»Ð¾Ð²ÐµÐº, Ð·Ð´Ð¾ÑÐ¾Ð²ÑÐµ", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¹ Ð½Ð°ÑÑÐ½ÑÐ¹ ÐºÐ¾Ð½Ð³ÑÐµÑÑ
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2021
Subjects: ÑÑÐµÐ½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½Ð¾Ðµ Ð·Ð°Ð½ÑÑÐ¸Ðµ
Ð²Ð¸Ð´Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ Ð½Ð°Ð³ÑÑÐ·ÐºÐ¸
Ð¿ÑÐ¸Ñ Ð¸ÑÐµÑÐºÐ°Ñ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð½Ð¾ÑÑÑ
ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÐµ ÑÐµÑ ÑÐ¾Ð²Ð°Ð»ÑÑÐ¸ÐºÐ¸

description: Ð ÑÑÐ°ÑÑÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ ÑÐ¿Ð¾ÑÐ¾Ð± ÑÐ°ÑÑÐµÑÐ° Ð¿ÑÐ¸ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÑÐµÐ½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½ÑÑ Ð·Ð°Ð½ÑÑÐ¸Ð¹, Ñ ÑÑÐµÑÐ¾Ð¼ Ð¸Ñ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ñ Ð¸ Ð²ÑÐµÐ¼ÐµÐ½Ð¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð·Ð°Ð´Ð°Ð½Ð¸Ð¹. ÐÐ½ÐµÐ´ÑÐµÐ½Ð¸Ðµ Ð² ÑÑÐµÐ½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½ÑÐ¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð° ÑÐ°ÑÑÐµÑÐ° ÑÑÐµÐ¿ÐµÐ½Ð¸ Ð¿ÑÐ¸ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð½Ð° ÑÐµÑÑÐ¾Ð²Ð°Ð»ÑÑÐ¸ÐºÐ¾Ð² Ð²Ð¸Ð´Ð¾Ð² ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ Ð½Ð°Ð³ÑÑÐ·ÐºÐ¸ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÐµÑ Ð´Ð¾Ð±Ð¸ÑÑÑÑ ÑÐ°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÑÑÐµÐ½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½ÑÑ Ð·Ð°Ð½ÑÑÐ¸Ð¹, ÑÐ°Ð·Ð»Ð¸ÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð²ÐµÐ»Ð¸ÑÐ¸Ð½Ðµ Ð¸ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð½Ð°Ð³ÑÑÐ·ÐºÐ¸, ÑÑÐ¾, Ð±ÐµÐ·ÑÑÐ»Ð¾Ð²Ð½Ð¾, ÑÐ¿Ð¾ÑÐ¾Ð±ÑÑÐ²ÑÐµÑ ÑÑÐ¿ÐµÑÐ½Ð¾Ð¼Ñ Ð²ÑÑÑÑÐ¿Ð»ÐµÐ½Ð¸Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ ÑÐµÑÑÐ¾Ð²Ð°Ð»ÑÑÐ¸ÐºÐ¾Ð² Ð½Ð° ÑÐ¾ÑÐµÐ²Ð½Ð¾Ð²Ð°Ð½Ð¸ÑÑ.
description: The article presents a method for calculating the mental tension of training sessions, taking into account their content and the time of performing specialized tasks. The introduction into the training process of the mechanism for calculating the degree
of mental impact of types of specialized load on fencers allows to achieve a rational distribution of training sessions that differ in size and direction of the load, which undoubtedly contributes to the successful performance of qualified fencers at competitions.
Phakellia robusta Bowerbank 1866
Creators: name: Pereira, Raquel
name: Larsson, Mats
name: Cárdenas, Paco
name: Thollesson, Mikael
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Animalia
Porifera
Demospongiae
Bubarida
Bubaridae
Phakellia
Phakellia robusta

description: Phakellia robusta Bowerbank, 1866
Phakellia robusta Bowerbank 1866: 120–122.
Phakellia robusta – Fristedt 1885: 45 (key), 46–47. – Alander 1942: 70 (key), 71 (description).
Material examined (3 specimens)
SWEDEN • 1 spec.; Kosterhavet; 58.8833° N, 11.0833° E; 1 Nov. 2002; Fredrik Pleijel leg. [TML-02]; dredge; P009-021111-1; voucher: GNM Porifera 1094 • 1 spec.; 58.9537° N, 11.0189° E; 24 Aug. 2007; Artprojektets Skagerrak-inventering leg. [SK94]; dredge; P009-111010-1; voucher: GNM Porifera 706 • 1 spec.; 58.459° N, 10.548° E; 296–250 m depth; 12 Oct. 2012; leg. [PM14-556]; dredge; P009- 130125-1; voucher: GNM Porifera 1095.
Description
The specimens have a thinly lamellated morphology. The colour is yellow when preserved in ethanol and unknown live. Furthermore, the specimens were covered in sediment, most likely due to collection method. The consistency is stiff.
Skeleton
The skeleton is composed of: curved styles measuring 1925–580 ×23–30 µm (N=2) straight oxeas and strongyles 460–630 ×20–30 µm (N= 4), and flexuous/“vermiformˮ oxeas 975–1250× 28–38 µm (N=4).
description: Published as part of Pereira, Raquel, Larsson, Mats, Cárdenas, Paco & Thollesson, Mikael, 2025, Swedish marine demosponge fauna (Porifera: Demospongiae) sampled 80 years after Jägerskiöld's inventory, pp. 1-64 in European Journal of Taxonomy 983 on pages 28-29, DOI: 10.5852/ejt.2025.983.2835, http://zenodo.org/record/15168665
Reentrant phenomenon in the exactly solvable mixed spin-1/2 and spin-1 Ising-Heisenberg model on diamond-like decorated planar lattices
Creators: name: Canova, Lucia
name: Strecka, Jozef
Publisher: name: arXiv
Year: 2009
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: Ground-state and finite-temperature behaviour of the mixed spin-1/2 and spin-1 Ising-Heisenberg model on decorated planar lattices consisting of inter-connected diamonds is investigated by means of the generalised decoration-iteration mapping transformation. The obtained exact results clearly point out that this model has a rather complex ground state composed of two unusual quantum phases, which is valid regardless of the lattice topology as well as the spatial dimensionality of the investigated system. It is shown that the diamond-like decorated planar lattices with a sufficiently high coordination number may exhibit a striking critical behaviour including reentrant phase transitions with two or three consecutive critical points.
description: 11 pages, 7 figures, submitted to Physica Status Solidi B
title: Supercomputer simulation of the fire detection system on the ship-museum Aurora
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
title: Ð¡ÑÐ¿ÐµÑÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¾Ð±Ð½Ð°ÑÑÐ¶ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð¶Ð°ÑÐ° Ð½Ð° ÐºÐ¾ÑÐ°Ð±Ð»Ðµ-Ð¼ÑÐ·ÐµÐµ ÐÐ²ÑÐ¾ÑÐ°
Creators: name: ÐÑÑ Ð°Ð¼Ð¼Ð°Ð´ ÐÐ°ÑÐ¼Ð°Ð½ Ð¨Ð°Ñ 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: 2017
Subjects: ÐÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
ÐÐ¾Ð¶Ð°ÑÑ
ÐÐ¾Ð¶Ð°ÑÐ½Ð°Ñ ÑÐ¸Ð³Ð½Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ

description: Fire dynamics can provide valuable information to a fire officer or a firefighter to understand how a fire will grow and spread within a structure and how best to control that growth. Researchers have generated experimental results and computer models to explain how fire dynamics taken at the most basic level, the fire triangle, applies to the fire ground. The purpose of this research is to demonstrate the impact that changes in the two level placement of fire sensors in a room of Aurora have had on the fire detection and how the standard deviation and rate of change of generated data of sensors' influence to initiate emergency response. These changes have transformed the typical fire behavior instructed to the fire service for many years. In addition, protective apparatus of firefighter has also changed over the decades. All these reasons lead to an evaluation that fire-fighting strategies may need to progress to keep a balance with the emerging circumstances on the fire ground.
description: Ð¦ÐµÐ»Ñ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ - Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÑ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸Ð¹ Ð² ÑÑÐ¾Ð²Ð½Ðµ ÑÐ°Ð·Ð¼ÐµÑÐµÐ½Ð¸Ñ Ð¿Ð¾Ð¶Ð°ÑÐ½ÑÑ Ð´Ð°ÑÑÐ¸ÐºÐ¾Ð² Ð² Ð½Ð¾Ð¼ÐµÑÐµ Ð³Ð¾ÑÑÐ¸Ð½Ð¸ÑÑ ÐÐ²ÑÐ¾ÑÐ° Ð½Ð° Ð¾Ð±Ð½Ð°ÑÑÐ¶ÐµÐ½Ð¸Ðµ Ð¿Ð¾Ð¶Ð°ÑÐ° Ð¸ ÐºÐ°Ðº ÑÑÐ°Ð½Ð´Ð°ÑÑÐ½Ð¾Ðµ Ð¾ÑÐºÐ»Ð¾Ð½ÐµÐ½Ð¸Ðµ Ð¸ ÑÐºÐ¾ÑÐ¾ÑÑÑ Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð´Ð°Ð½Ð½ÑÑ, Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÑ Ð¾Ñ Ð´Ð°ÑÑÐ¸ÐºÐ¾Ð² Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð´Ð»Ñ Ð¸Ð½Ð¸ÑÐ¸Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐºÑÑÑÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐµÐ°Ð³Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ. Ð­ÑÐ¸ Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ ÑÑÐ°Ð½ÑÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð»Ð¸ Ð¿ÑÐ¸Ð²ÑÑÐ½ÑÐµ Ð¿Ð¾Ð¶Ð°ÑÐ½Ð¾Ð¹ Ð¿Ð¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¿Ð¾ÑÑÑÐ¸Ð» Ð¿ÑÐ¾ÑÐ¸Ð²Ð¾Ð¿Ð¾Ð¶Ð°ÑÐ½Ð¾Ð¹ ÑÐ»ÑÐ¶Ð±Ñ Ð² ÑÐµÑÐµÐ½Ð¸Ðµ Ð¼Ð½Ð¾Ð³Ð¸Ñ Ð»ÐµÑ. ÐÑÐ¾Ð¼Ðµ ÑÐ¾Ð³Ð¾, Ð·Ð°ÑÐ¸ÑÐ½ÑÐ¹ Ð°Ð¿Ð¿Ð°ÑÐ°Ñ Ð¿Ð¾Ð¶Ð°ÑÐ½ÑÐ¹ Ð¸Ð·Ð¼ÐµÐ½Ð¸Ð»ÑÑ Ð·Ð° Ð¿Ð¾ÑÐ»ÐµÐ´Ð½Ð¸Ðµ Ð´ÐµÑÑÑÐ¸Ð»ÐµÑÐ¸Ñ. ÐÑÐµ ÑÑÐ¸ Ð¿ÑÐ¸ÑÐ¸Ð½Ñ Ð¿ÑÐ¸Ð²Ð¾Ð´ÑÑ Ðº Ð¾ÑÐµÐ½ÐºÐµ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¹ Ð¿Ð¾Ð¶Ð°ÑÐ¾ÑÑÑÐµÐ½Ð¸Ñ Ð¼Ð¾Ð¶ÐµÑ Ð¿Ð¾ÑÑÐµÐ±Ð¾Ð²Ð°ÑÑÑÑ Ð¿ÑÐ¾Ð³ÑÐµÑÑÐ°, ÑÑÐ¾Ð±Ñ ÑÐ¾ÑÑÐ°Ð½Ð¸ÑÑ ÑÐ°Ð²Ð½Ð¾Ð²ÐµÑÐ¸Ðµ Ð¿ÑÐ¸ Ð²Ð¾Ð·Ð½Ð¸ÐºÑÐ¸Ñ Ð¾Ð±ÑÑÐ¾ÑÑÐµÐ»ÑÑÑÐ²Ð°Ñ, Ð½Ð° Ð¾Ð³Ð¾Ð½Ñ Ð·ÐµÐ¼Ð»ÐµÐ¹.
Morphology of Peripheral Blood Cells from Various Species of Turkish Herpetofauna
Creators: name: ARIKAN, Hüseyin
name: CICEK, Kerim
Publisher: name: Acta Herpetologica
Year: 2011

description: In this study, measurements of morphological and size parameters of peripheral blood cells (erythrocyte, leucocyte, thrombocyte) on blood smear preparation devices stained with Wright’s stain were given for 87 species from Turkish herpetofauna (19 amphibian species including 7 urodeles and 12 anurans as well as 68 reptile species including 4 turtles, 30 lizards and 34 snakes).  It was determined that erythrocyte and nucleus sizes showed great variations among the species of herpetofauna and even among the preparations of the same species; the largest blood cells (erythrocyte, leucocyte, thrombocyte) were found in urodeles; aquatic and semiaquatic species had larger erythrocytes than terrestrials, and the largest erythrocytes were in turtles among the reptile species examined. Lymphocytes were determined as the predominant cells among the blood leucocytes in blood smears of all the examined species.
description: Acta Herpetologica, Vol 5, No 2 (2010)
Could Park and Ride Become Bike and Ride? Assessing the Potential for Bike Cages at Metro Vancouver's Park and Ride Lots
Creators: name: Rolfe, Debra
Publisher: name: The University of British Columbia
Year: 2016

description: This study provides a multi-faceted approach to prioritizing which of TransLink’s park-and-ride lots would be the best locations for secure bike cages. Ultimately, it argues that increasing evidence finds that cycling facilities are both the result and the motivation for increased cycling levels. Further, compared to other forms of transportation infrastructure, bike parking is relatively low cost and low risk. These factors support the need for TransLink to expand its bike parking options at its park-and-ride lots, and installing bike cages at selected lots is a strong start.
Monte Carlo Simulations of Globular Cluster Evolution. V. Binary Stellar Evolution
Creators: name: Chatterjee, Sourav
name: Fregeau, John M.
name: Umbreit, Stefan
name: Rasio, Frederic A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We study the dynamical evolution of globular clusters containing primordial binaries, including full single and binary stellar evolution using our Monte Carlo cluster evolution code updated with an adaptation of the single and binary stellar evolution codes SSE/BSE from Hurley et. al (2000, 2002). We describe the modifications we have made to the code. We present several test calculations and comparisons with existing studies to illustrate the validity of the code. We show that our code finds very good agreement with direct N-body simulations including primordial binaries and stellar evolution. We find significant differences in the evolution of the global properties of the simulated clusters using stellar evolution compared to simulations without any stellar evolution. In particular, we find that the mass loss from stellar evolution acts as a significant energy production channel simply by reducing the total gravitational binding energy and can significantly prolong the initial core contraction phase before reaching the binary-burning quasi steady state of the cluster evolution as noticed in Paper IV. We simulate a large grid of clusters varying the initial cluster mass, binary fraction, and concentration and compare properties of the simulated clusters with those of the observed Galactic globular clusters (GGCs). We find that our simulated cluster properties agree well with the observed GGC properties. We explore in some detail qualitatively different clusters in different phases of their evolution, and construct synthetic Hertzprung-Russell diagrams for these clusters.
description: 46 preprint pages, 18 figures, 3 tables, submitted to ApJ
A multiwavelength-motivated X-ray model for the Circinus Galaxy
Creators: name: Andonie, Carolina
name: Ricci, Claudio
name: Paltani, Stéphane
name: Arévalo, Patricia
name: Treister, Ezequiel
name: Bauer, Franz
name: Stalevski, Marko
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Reprocessed X-ray emission in Active Galactic Nuclei (AGN) can provide fundamental information about the circumnuclear environments of supermassive black holes. Recent mid-infrared studies have shown evidence of an extended dusty structure perpendicular to the torus plane. In this work, we build a self-consistent X-ray model for the Circinus Galaxy including the different physical components observed at different wavelengths and needed to reproduce both the morphological and spectral properties of this object in the mid-infrared. The model consists of four components: the accretion disk, the broad line region (BLR), a flared disk in the equatorial plane and a hollow cone in the polar direction. Our final model reproduces well the 3--70 keV Chandra and NuSTAR spectra of Circinus, including the complex Fe K$α$ zone and the spectral curvature, although several additional Gaussian lines, associated to either ionized iron or to broadened Fe K$α$/K$β$ lines, are needed. We find that the flared disk is Compton thick ($ N_{\rm H,d}= \rm 1.01^{+0.03}_{-0.24}\times 10^{25}\: cm^{-2}$) and geometrically thick ($CF=0.55^{+0.01}_{-0.05}$), and that the hollow cone has a Compton-thin column density ($ N_{\rm H,c}= \rm 2.18^{+0.47}_{-0.43}\times 10^{23}\: cm^{-2}$), which is consistent with the values inferred by mid-infrared studies. Including also the BLR, the effective line of sight column density is $ N_{\rm H}= \rm 1.47^{+0.03}_{-0.24}\times 10^{25}\: cm^{-2}$. This approach to X-ray modelling, i.e. including all the different reprocessing structures, will be very important to fully exploit data from future X-ray missions.
description: Accepted for publication in MNRAS. 15 pages, 10 figures, 8 tables