cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ÐÐ¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾-Ð¿ÑÐ°Ð²Ð¾Ð²Ð¾Ðµ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð°Ð³ÑÐ¾Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ²ÑÐ°Ð¼ÐºÐ¾Ð² , Ð®ÑÐ¸Ð¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð°Ð³ÑÐ¾Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÐ¹ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ
Ð°Ð³ÑÐ¾Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
Ð°Ð³ÑÐ°ÑÐ½ÑÐµ Ð¿ÑÐ°Ð²Ð¾Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾-Ð¿ÑÐ°Ð²Ð¾Ð²Ð¾Ðµ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð°Ð³ÑÐ¾Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸. Ð Ð¸Ð¼ÐµÐ½Ð½Ð¾, ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ Ð¿Ð¾Ð½ÑÑÐ¸Ðµ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð°Ð³ÑÐ¾Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸, Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸ÑÑÑ Ð¸ÑÑÐ¾ÑÐ¸ÐºÐ¾-Ð¿ÑÐ°Ð²Ð¾Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð·Ð°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÑÑÐ²Ð° Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð°Ð³ÑÐ¾Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸, Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸ÑÑÑ ÑÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½Ð¾-Ð¿ÑÐ°Ð²Ð¾Ð²Ð¾Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð·Ð°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÑÑÐ²Ð° Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð°Ð³ÑÐ¾Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð² Ð·Ð°ÑÑÐ±ÐµÐ¶Ð½ÑÑ ÑÑÑÐ°Ð½Ð°Ñ, Ð´Ð°ÐµÑÑÑ Ð¿Ð¾Ð½ÑÑÐ¸Ðµ Ð°Ð³ÑÐ°ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ°Ð²Ð° ÐºÐ°Ðº Ð¾ÑÑÐ°ÑÐ»Ð¸ Ð¿ÑÐ°Ð²Ð° Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÐµÑÑÑ Ð¼ÐµÑÑÐ¾ Ð°Ð³Ð°ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ°Ð²Ð° Ð² ÑÑÑÑÐºÑÑÑÐµ Ð¿ÑÐ°Ð²Ð° Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸, Ð¸Ð·ÑÑÐ°ÑÑÑÑ Ð°Ð³ÑÐ°ÑÐ½ÑÐµ Ð¿ÑÐ°Ð²Ð¾Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ Ð² Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸. Ð ÑÐ°ÐºÐ¶Ðµ, Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸ÑÑÑ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿ÑÐ°Ð²Ð¾Ð½Ð°ÑÑÑÐµÐ½Ð¸Ð¹ Ð¸ ÑÑÐ´ÐµÐ±Ð½Ð¾Ð¹ Ð¿ÑÐ°ÐºÑÐ¸ÐºÐ¸ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð°Ð³ÑÐ¾Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸.
Tuning CLD Maps
Creators: name: Marazzato, Roberto
name: Sparavigna, Amelia Carolina
Publisher: name: arXiv
Year: 2010
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: The Coherence Length Diagram and the related maps have been shown to represent a useful tool for image analysis. Setting threshold parameters is one of the most important issues when dealing with such applications, as they affect both the computability, which is outlined by the support map, and the appearance of the coherence length diagram itself and of defect maps. A coupled optimization analysis, returning a range for the basic (saturation) threshold, and a histogram based method, yielding suitable values for a desired map appearance, are proposed for an effective control of the analysis process.
description: Keywords: coherence length, image analysis, 2D textures; texture functions; defect localisation; directional defect pattern; optimization; histogram
Automatic stabilization of finite-element simulations using neural networks and hierarchical matrices
Creators: name: Sluzalec, Tomasz
name: Dobija, Mateusz
name: Paszynska, Anna
name: Muga, Ignacio
name: Paszynski, Maciej
Publisher: name: arXiv
Year: 2022
Subjects: subject: Numerical Analysis (math.NA)
subject: Machine Learning (cs.LG)
subject: FOS: Mathematics
subject: FOS: Computer and information sciences
subject: G.1.8; I.6.1; I.1.2; G.4

description: Petrov-Galerkin formulations with optimal test functions allow for the stabilization of finite element simulations. In particular, given a discrete trial space, the optimal test space induces a numerical scheme delivering the best approximation in terms of a problem-dependent energy norm. This ideal approach has two shortcomings: first, we need to explicitly know the set of optimal test functions; and second, the optimal test functions may have large supports inducing expensive dense linear systems. Nevertheless, parametric families of PDEs are an example where it is worth investing some (offline) computational effort to obtain stabilized linear systems that can be solved efficiently, for a given set of parameters, in an online stage. Therefore, as a remedy for the first shortcoming, we explicitly compute (offline) a function mapping any PDE-parameter, to the matrix of coefficients of optimal test functions (in a basis expansion) associated with that PDE-parameter. Next, as a remedy for the second shortcoming, we use the low-rank approximation to hierarchically compress the (non-square) matrix of coefficients of optimal test functions. In order to accelerate this process, we train a neural network to learn a critical bottleneck of the compression algorithm (for a given set of PDE-parameters). When solving online the resulting (compressed) Petrov-Galerkin formulation, we employ a GMRES iterative solver with inexpensive matrix-vector multiplications thanks to the low-rank features of the compressed matrix. We perform experiments showing that the full online procedure as fast as the original (unstable) Galerkin approach. In other words, we get the stabilization with hierarchical matrices and neural networks practically for free. We illustrate our findings by means of 2D Eriksson-Johnson and Hemholtz model problems.
description: 28 pages, 16 figures, 4 tables, 6 algorithms
title: Ð¡Ð¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð° ÐºÐ¾Ð½Ð´Ð¸ÑÐµÑÑÐºÐ¸Ñ Ð¸Ð·Ð´ÐµÐ»Ð¸Ð¹ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð¿Ð»Ð¾Ð´Ð¾Ð²Ð¾Ð³Ð¾ ÑÑÑÑÑ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¸Ð»ÑÐ¼ÑÐ»Ð¸Ð½Ð°, Ð®Ð»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: 2017
Subjects: ÑÐ»Ð°Ð´ÐºÐ¸Ðµ Ð¶ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÐµ Ð±Ð»ÑÐ´Ð°
Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ
Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð°Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð°
Ð¿Ð»Ð¾Ð´Ð¾Ð²Ð¾Ðµ ÑÑÑÑÐµ

description: Ð£ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð° ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ ÑÐ»Ð°Ð´ÐºÐ¸Ñ Ð¶ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð±Ð»ÑÐ´, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾ Ð¾ÑÐ³Ð°Ð½Ð¾Ð»ÐµÐ¿ÑÐ¸ÑÐµÑÐºÐ¸Ð¼ Ð¸ ÑÐ¸Ð·Ð¸ÐºÐ¾-ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¼ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÑÐ¼ Ð´Ð°Ð½Ð½ÑÑ Ð¸Ð·Ð´ÐµÐ»Ð¸Ð¹, 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 ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ ÑÐ¾Ð»Ð¾Ð´Ð½Ð¾Ð³Ð¾ ÑÐµÑÐ°. 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ÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½Ð¾Ðµ ÑÐµÑÐµÐ½Ð¸Ðµ ÑÐ¾Ð»Ð¾Ð´Ð½Ð¾Ð³Ð¾ ÑÐµÑÐ°.
title: ÐÑÐµÐ½ÐºÐ° Ð¿Ð¾ÑÐ»ÐµÐ´ÑÑÐ²Ð¸Ð¹ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÑÐ½ÐºÐ° ÑÐ¾Ð·Ð½Ð¸ÑÐ½Ð¾Ð¹ Ð¸Ð½ÑÐµÑÐ½ÐµÑ-ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸ Ð² Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸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Ð¾Ð²Ð¸ÐºÐ¾Ð², ÐÐ°Ð½Ð¸Ð¸Ð»
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð¸Ð½ÑÐµÑÐ½ÐµÑ-ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ñ
Ð¸Ð½ÑÐµÑÐ½ÐµÑ-Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½
ÑÑÐ°Ð½Ð·Ð°ÐºÑÐ¸Ñ
ÑÐ°Ð¼Ð¾Ð¶ÐµÐ½Ð½Ð°Ñ Ð¿Ð¾ÑÐ»Ð¸Ð½Ð°

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÑÑÐ½Ð¾Ðº ÑÐ¾Ð·Ð½Ð¸ÑÐ½Ð¾Ð¹ Ð¸Ð½ÑÐµÑÐ½ÐµÑ-ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸ Ð² Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸.
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ÐÐ²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ ÑÐ±Ð°Ð»Ð°Ð½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð¸Ñ Ð¾ÐºÐ°Ð¶ÐµÑ ÑÑÐ¸Ð¼ÑÐ»Ð¸ÑÑÑÑÐ¸Ð¹ ÑÑÑÐµÐºÑ Ð½Ð° Ð»Ð¾ÐºÐ°Ð»ÑÐ½ÑÐ¹ ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¸Ð¹ ÑÑÐ½Ð¾Ðº Ð¸Ð½ÑÐµÑÐ½ÐµÑ-ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸ Ð¸ Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ñ Ð¿Ð¾Ð»ÑÑÐ¸ÑÑ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¿Ð¾ÑÑÑÐ¿Ð»ÐµÐ½Ð¸Ñ Ð² Ð±ÑÐ´Ð¶ÐµÑ Ð¾Ñ Ð·Ð°ÑÑÐ±ÐµÐ¶Ð½ÑÑ Ð¸Ð½ÑÐµÑÐ½ÐµÑ-Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð¾Ð².
title: Characterising the relationship between empathy and emotion regulation
Creators: name: Thompson, Nicholas
Publisher: name: University of Reading
Year: 2019

description: Empathy and emotion regulation are both processes that are vital for effective social functioning and emotional wellbeing. Broadly speaking, empathy refers to understanding and/or sharing another’s emotion, and emotion regulation refers to the processes by which one manages emotions. Despite increasing awareness that empathy and emotion regulation may be closely related, there has been little empirical study of this topic and the nature of the inter-relationships between their different component processes are not well characterised. This thesis addresses current gaps in the literature by utilising a range of approaches, including self-report, behavioural, eye-tracking, and psychophysiology measures, to examine the relationship between different trait and task measures of empathy and emotion regulation. It was predicted that the cognitive (i.e. understanding others’ emotions) and affective (i.e. sharing others’ emotions) dimensions of empathy would show different relationships with emotion regulation. Broadly speaking, it was expected that emotion regulation abilities would be positively associated with cognitive empathy but negatively associated with affective empathy. There was strong support for the hypothesis that empathy and emotion regulation are related. Furthermore, in most studies there was evidence to suggest that cognitive and affective empathy are related to emotion regulation abilities and behaviours in different ways. Divergent 3 relationships between trait and task metrics of cognitive and affective empathy were observed for various emotion regulation measures, including habitual strategy use, implicit emotion regulation ability, and reappraisal ability. While there was some support for the hypothesis that emotion regulation abilities are positively associated with cognitive empathy but negatively associated with affective empathy, conflicting findings were observed. This thesis makes a significant contribution to current knowledge and represents an important step towards elucidating the nature of the relationship between empathy and emotion regulation. The findings also highlight some important considerations regarding the relationship between different methods used to assess empathy and emotion regulation, and prompt actionable research questions to be addressed by future work.
Optimal stopping of a risk process when claims are covered immediately
Creators: name: Muciek, Bogdan K.
name: Szajowski, Krzysztof J.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Probability (math.PR)
subject: Optimization and Control (math.OC)
subject: FOS: Mathematics
subject: 60G40; 60K99; 90A46

description: The optimal stopping problem for the risk process with interests rates and when claims are covered immediately is considered. An insurance company receives premiums and pays out claims which have occured according to a renewal process and which have been recognized by them. The capital of the company is invested at interest rate $α\in\Re^{+}$, the size of claims increase at rate $β\in\Re^{+}$ according to inflation process. The immediate payment of claims decreases the company investment by rate $α_1$. The aim is to find the stopping time which maximizes the capital of the company. The improvement to the known models by taking into account different scheme of claims payment and the possibility of rejection of the request by the insurance company is made. It leads to essentially new risk process and the solution of optimal stopping problem is different.
description: 8 pages
title: Ð¡Ð²Ð°ÑÐºÐ° ÑÑÐµÐ½Ð¸ÐµÐ¼ Ñ Ð¿ÐµÑÐµÐ¼ÐµÑÐ¸Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÐ°Ð·Ð½Ð¾ÑÐ¾Ð´Ð½ÑÑ ÑÐ¿Ð»Ð°Ð²Ð¾Ð² Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Al Ð¸ Cu
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: Ð¢ÐµÑÐ»ÐµÐ²Ð°, 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: 2018
Subjects: Ð¼ÐµÐ´Ñ
Ð°Ð»ÑÐ¼Ð¸Ð½Ð¸Ð¹
ÑÐ°Ð·Ð½Ð¾ÑÐ¾Ð´Ð½Ð¾Ðµ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ðµ
Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ
ÑÐ²Ð°ÑÐºÐ° ÑÑÐµÐ½Ð¸ÐµÐ¼ Ñ Ð¿ÐµÑÐµÐ¼ÐµÑÐ¸Ð²Ð°Ð½Ð¸ÐµÐ¼

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ð° Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ñ Ð¾ ÑÐ°Ð·Ð½Ð¾ÑÐ¾Ð´Ð½ÑÑ Ð¼ÐµÐ´Ð½ÑÑ Ð¸ Ð°Ð»ÑÐ¼Ð¸Ð½Ð¸ÐµÐ²ÑÑ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð°Ñ, ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð½ÑÐ¼ Ð¼ÐµÑÐ¾Ð´Ð¾Ð¼ Ð¡Ð¢Ð. Ð¢Ð°ÐºÐ¶Ðµ Ð¾Ð±ÑÑÐ¶Ð´ÐµÐ½Ñ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÑ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð¡Ð¢Ð Ð¸ Ð¸Ñ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð½Ð° ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° ÑÐ°Ð·Ð½Ð¾ÑÐ¾Ð´Ð½Ð¾Ð³Ð¾ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ñ Cu-Al. ÐÑÐ¾Ð¼Ðµ ÑÐ¾Ð³Ð¾, Ð¾Ð¿Ð¸ÑÐ°Ð½Ñ ÑÑÑÑÐºÑÑÑÐ½ÑÐµ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÐ²Ð°ÑÐ½Ð¾Ð³Ð¾ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ñ.
Population of X-ray Sources in the Intermediate-Age Cluster NGC 3532: a Test Bed for Machine-Learning Classification
Creators: name: Chen, Steven
name: Kargaltsev, Oleg
name: Yang, Hui
name: Hare, Jeremy
name: Volkov, Igor
name: Rangelov, Blagoy
name: Tomsick, John
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Open clusters are thought to be the birth place of most stars in the Galaxy. Thus, they are excellent laboratories for investigating stellar evolution, and X-ray properties of various types of stars (including binary stars, evolved stars, and compact objects). In this work, we investigate the population of X-ray sources in the nearby 300-Myr-old open cluster NGC 3532 using Chandra X-ray Observatory and multi-wavelength data from several surveys. We apply a random-forest machine-learning pipeline (MUWCLASS) to classify all confidently detected X-ray sources (S/N$>5$) in the field of NGC 3532. We also perform a more detailed investigation of brighter sources, including their X-ray spectra and lightcurves. Most X-ray sources are confirmed as coronally-active low-mass stars, many of which are confidently identified by MUWCLASS. Several late B or early A-type \textbf{stars} are relatively bright in X-rays, most of which are likely binaries. We do not find any compact objects among X-ray sources reliably associated with NGC 3532, down to the limiting X-ray flux of $\sim 2\times10^{-15}$ erg s$^{-1}$ cm$^{-2}$, corresponding to $L_X\sim 6\times 10^{28}$ erg s$^{-1}$ at the cluster's distance. We also identify several Galactic sources beyond NGC 3532 that differ from typical coronally active stars, and were classified by MUWCLASS as potential compact objects. Detailed investigation reveals that these sources may indeed belong to rarer classes, and deserve follow up observations.
description: Accepted for publication in Astrophysical Journal, 41 pages, 23 figures
title: ÐÑÐ°Ð²Ð¾Ð²Ð¾Ðµ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ Ð¸ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð·Ð°ÑÐ¸ÑÑ Ð¿ÑÐ°Ð² Ð°ÐºÑÐ¸Ð¾Ð½ÐµÑÐ¾Ð² Ð² ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¼ Ð¼Ð¸ÑÐµ
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Ð¸ÑÐ¾Ð²Ð°, ÐÐ°Ñ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: Ð·Ð°ÑÐ¸ÑÐ° Ð¿ÑÐ°Ð² Ð°ÐºÑÐ¸Ð¾Ð½ÐµÑÐ¾Ð²
Ð¿ÑÐ°Ð²Ð¾Ð²ÑÐµ Ð·Ð°ÑÐ¸ÑÑ Ð¿ÑÐ°Ð² Ð°ÐºÑÐ¸Ð¾Ð½ÐµÑÐ¾Ð²
Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
ÑÑÑÐ´Ð¾Ð²ÑÐµ Ð¿ÑÐ°Ð²Ð¾Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ
ÑÐ¸Ð¿Ñ Ð¸ Ð²Ð¸Ð´Ñ Ð°ÐºÑÐ¸Ð¾Ð½ÐµÑÐ½ÑÑ Ð¾Ð±ÑÐµÑÑÐ²

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð¾ÑÐ½Ð¾Ð²Ñ Ð¿ÑÐ°Ð² Ð°ÐºÑÐ¸Ð¾Ð½ÐµÑÐ¾Ð², ÑÐ°Ð·Ð´ÐµÐ»ÐµÐ½Ð¸Ð¸ Ð° ÑÐ°ÐºÐ¶Ðµ Ð¸Ñ Ð·Ð°ÑÐ¸ÑÑ. Ð Ð¸Ð¼ÐµÐ½Ð½Ð¾, ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¸Ð´Ñ Ð¿ÑÐ°Ð²Ð¾Ð²ÑÑ Ð°ÐºÑÐ¾Ð² Ð·Ð°ÑÐ¸ÑÑ Ð¿ÑÐ°Ð² Ð°ÐºÑÐ¸Ð¾Ð½ÐµÑÐ¾Ð² Ð¸ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¸Ñ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ, Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸. ÐÐ·ÑÑÐµÐ½Ð¸Ðµ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐµÐ¹ Ð¸ ÑÐµÐ½Ð´ÐµÐ½ÑÐ¸Ð¹ Ð·Ð°ÑÐ¸ÑÑ Ð¿ÑÐ°Ð² Ð°ÐºÑÐ¸Ð¾Ð½ÐµÑÐ¾Ð².
The Formation of the Collisional Family around the Dwarf Planet Haumea
Creators: name: Leinhardt, Zoe M.
name: Marcus, Robert A.
name: Stewart, Sarah T.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Haumea, a rapidly rotating elongated dwarf planet (~ 1500 km in diameter), has two satellites and is associated with a "family" of several smaller Kuiper Belt objects (KBOs) in similar orbits. All members of the Haumea system share a water ice spectral feature that is distinct from all other KBOs. The relative velocities between the Haumea family members are too small to have formed by catastrophic disruption of a large precursor body, which is the process that formed families around much smaller asteroids in the Main Belt. Here we show that all of the unusual characteristics of the Haumea system are explained by a novel type of giant collision: a graze-and-merge impact between two comparably sized bodies. The grazing encounter imparted the high angular momentum that spun off fragments from the icy crust of the elongated merged body. The fragments became satellites and family members. Giant collision outcomes are extremely sensitive to the impact parameters. Compared to the Main Belt, the largest bodies in the Kuiper Belt are more massive and experience slower velocity collisions; hence, outcomes of giant collisions are dramatically different between the inner and outer solar system. The dwarf planets in the Kuiper Belt record an unexpectedly large number of giant collisions, requiring a special dynamical event at the end of solar system formation.
description: Accepted for publication in ApJ, 12 pages, 4 figures, 2 tables.
Additional file 7 of A robust immune-related gene pairs signature for predicting the overall survival of esophageal cancer
Creators: name: Zheng, Wei
name: Fang, Gaofeng
name: Huang, Qiao
name: Shi, Dan
name: Xie, Biao
Publisher: name: figshare
Year: 2023
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Cancer

description: Table S2. Model information about the IRGPI
title: ÐÐ½Ð°Ð»Ð¸Ð· Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐ¸ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ Ð½Ð°Ð´ÑÐ¶Ð½Ð¾ÑÑÐ¸ Ð³Ð¸Ð´ÑÐ°Ð²Ð»Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼
title: Analysis of the possibility of improving the reliability of hydraulic systems
Creators: name: ÐÐ°Ð¹Ð³Ð¾ÑÐ¾Ð´Ð¾Ð², Ð¡.
name: "ÐÐ¸Ð´ÑÐ°Ð²Ð»Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¼Ð°ÑÐ¸Ð½Ñ, Ð³Ð¸Ð´ÑÐ¾Ð¿ÑÐ¸Ð²Ð¾Ð´Ñ Ð¸ Ð³Ð¸Ð´ÑÐ¾Ð¿Ð½ÐµÐ²Ð¼Ð¾Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÐºÐ°. Ð¡Ð¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ðµ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ðµ Ð¸ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ", Ð²ÑÐµÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ°Ñ Ð½Ð°ÑÑÐ½Ð¾-ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (2022; 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: 2022
Subjects: ÐÐ¸Ð´ÑÐ°Ð²Ð»Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ
Ð³Ð¸Ð´ÑÐ¾Ð´Ð¸Ð¾Ð´
ÐºÐ¾Ð½ÑÑ
Ð´Ð¸Ð¾Ð´Ð½Ð¾ÑÑÑ
Ð´Ð°Ð²Ð»ÐµÐ½Ð¸Ðµ
ÑÐ°ÑÑ Ð¾Ð´
hydrodiode
cone
diode
pressure
flow rate

description: ÐÐ»Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ Ð½Ð°Ð´ÑÐ¶Ð½Ð¾ÑÑÐ¸ Ð³Ð¸Ð´ÑÐ¾- Ð¸ Ð¿Ð½ÐµÐ²Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼ Ð² Ð½Ð°ÑÑÐ¾ÑÑÐµÐµ Ð²ÑÐµÐ¼Ñ Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ Ð¸Ð½ÑÐµÑÐµÑÐ½ÑÐ¼Ð¸ Ð¸ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ð½ÑÐ¼Ð¸ ÑÐ²Ð»ÑÑÑÑÑ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ Ð³Ð¸Ð´ÑÐ°Ð²Ð»Ð¸ÑÐµÑÐºÐ¸Ñ Ð´Ð¸Ð¾Ð´Ð¾Ð². Ð Ð°Ð·Ð»Ð¸ÑÐ½ÑÐµ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð²Ð½ÑÐµ ÑÐµÑÐµÐ½Ð¸Ñ Ð³Ð¸Ð´ÑÐ¾Ð´Ð¸Ð¾Ð´Ð¾Ð² Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÑ Ð¸Ñ Ð½Ðµ ÑÐ¾Ð»ÑÐºÐ¾ Ð² ÐºÐ°ÑÐµÑÑÐ²Ðµ Ð¾Ð±ÑÐ°ÑÐ½Ð¾Ð³Ð¾ ÐºÐ»Ð°Ð¿Ð°Ð½Ð°, Ð½Ð¾ Ð¸ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»Ð¸ÑÐµÐ»Ñ.
description: To improve the reliability of hydro-pneumatic systems, currently the most interesting and promising are the use of hydraulic diodes. Various design solutions of hydrodiodes allow them to be used not only as a check valve, but also as a distributor.
title: Ð¡ÐµÑÐ²Ð¸Ñ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ Ð¼Ð°ÑÑÑÑÑÐ¾Ð² Ð²Ð½ÑÑÑÐ¸ Ð·Ð´Ð°Ð½Ð¸Ð¹
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾ÑÐ¸ÑÐ¾Ð², ÐÐ»Ð°Ð´Ð¸ÑÐ»Ð°Ð²
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·Ð°Ð´Ð°ÑÐ° ÐºÐ¾Ð¼Ð¼Ð¸Ð²Ð¾ÑÐ¶ÐµÑÐ°
Ð³ÐµÐ½ÐµÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼
Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼ Ð¿ÑÐ¸Ð¼Ð°-ÑÐ¹Ð»ÐµÑÐ°
Ð²ÐµÐ±-ÑÐµÑÐ²Ð¸Ñ
ÐºÑÐ¸ÑÐµÑÐ¸Ð¹ Ð¾ÑÑÐ°Ð½Ð¾Ð²Ð°

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ñ Ð´Ð»Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð·Ð°Ð´Ð°ÑÐ¸ ÐºÐ¾Ð¼Ð¼Ð¸Ð²Ð¾ÑÐ¶ÐµÑÐ°. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ ÑÑÐ¸Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð²ÑÐ±ÑÐ°Ð½ Ð³ÐµÐ½ÐµÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð¾ Ð²ÐµÐ±-Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ Ð¼Ð°ÑÑÑÑÑÐ¾Ð² Ð²Ð½ÑÑÑÐ¸ Ð·Ð´Ð°Ð½Ð¸Ð¹ Ð¿ÑÐ¸ Ð¿Ð¾Ð¼Ð¾ÑÐ¸ Ð³ÐµÐ½ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð°. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ñ ÑÐ°ÑÑÐµÑÑ Ð²ÑÐµÐ¼ÐµÐ½Ð¸ Ð¸ ÑÐ°ÑÑÑÐ¾ÑÐ½Ð¸Ñ Ð»ÑÑÑÐµÐ³Ð¾ Ð¸ ÑÑÐ´ÑÐµÐ³Ð¾ Ð¿ÑÑÐ¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð²ÑÐµÐ¼Ñ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ ÑÐ°Ð±Ð¾ÑÑ Ð³ÐµÐ½ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð°, Ð° Ð¸Ð¼ÐµÐ½Ð½Ð¾ Ð²ÑÐ²Ð¾Ð´ Ð²ÑÐµÑ Ð¿Ð¾ÐºÐ¾Ð»ÐµÐ½Ð¸Ð¹ Ð´Ð¾ Ð¾ÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð°, Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½ÑÐµ Ð¼Ð°ÑÑÑÑÑÑ Ð½Ð° Ð·Ð°Ð´Ð°Ð½Ð½Ð¾Ð¼ Ð¿Ð¾ÐºÐ¾Ð»ÐµÐ½Ð¸Ð¸, Ð²ÑÐ²Ð¾Ð´ Ð²ÑÐµÑ ÐºÐ°Ð½Ð´Ð¸Ð´Ð°ÑÐ¾Ð² Ð½Ð° ÑÐºÑÐµÑÐ¸Ð²Ð°Ð½Ð¸Ðµ Ð¸ Ð¾ÑÐ±Ð¾Ñ Ð»ÑÑÑÐ¸Ñ Ð´Ð²ÑÑ. Ð ÐµÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ð° Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÑ Ð·Ð°Ð³ÑÑÐ¶Ð°ÑÑ ÑÐ²Ð¾Ð¸ ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½ÑÐµ ÐºÐ°ÑÑÑ Ð² ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÑÐ¾ÑÐ¼Ð°ÑÐ°Ñ ÑÐ°ÑÑÑÐ¾Ð²Ð¾Ð¹ Ð¸ Ð²ÐµÐºÑÐ¾ÑÐ½Ð¾Ð¹ Ð³ÑÐ°ÑÐ¸ÐºÐ¸. Ð­ÑÐ¾ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÐµÑ ÑÑÑÐ¾Ð¸ÑÑ Ð¼Ð°ÑÑÑÑÑÑ Ð½Ðµ ÑÐ¾Ð»ÑÐºÐ¾ Ð´Ð»Ñ ÐºÐ°ÑÑ, ÐºÐ¾ÑÐ¾ÑÑÐµ ÐµÑÑÑ Ð² Ð½Ð°Ð»Ð¸ÑÐ¸Ð¸, Ð½Ð¾ Ð¸ Ð´Ð»Ñ ÑÐ²Ð¾Ð¸Ñ ÐºÐ°ÑÑ. ÐÐ»Ð°Ð²Ð½Ð¾Ðµ, ÑÑÐ¾Ð±Ñ Ð·Ð°Ð³ÑÑÐ¶ÐµÐ½Ð½ÑÐµ ÐºÐ°ÑÑÑ Ð±ÑÐ»Ð¸ Ð½Ð° ÑÐµÑÐ½Ð¾Ð¼ ÑÐ¾Ð½Ðµ, Ð¸Ð½Ð°ÑÐµ Ð²ÐµÐ»Ð¸ÐºÐ° Ð²ÐµÑÐ¾ÑÑÐ½Ð¾ÑÑÑ Ð¿Ð¾Ð»ÑÑÐ¸ÑÑ Ð½ÐµÐºÐ¾ÑÑÐµÐºÑÐ½ÑÐ¹ ÑÐµÐ·ÑÐ»ÑÑÐ°Ñ. Ð¢Ð°ÐºÐ¶Ðµ ÐµÑÑÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÑ Ð½Ð°Ð³Ð»ÑÐ´Ð½Ð¾ Ð¿Ð¾ÑÐ¼Ð¾ÑÑÐµÑÑ Ð¸ ÑÑÐ°Ð²Ð½Ð¸ÑÑ Ð»ÑÑÑÐ¸Ð¹ Ð¸ ÑÑÐ´ÑÐ¸Ð¹ Ð¼Ð°ÑÑÑÑÑ.
Pupil dilation during reward anticipation forecasts self-reported affect in the Monetary Incentive Delay (MID) task
Creators: name: Srirangarajan, Tara
name: Yan, Yan
Publisher: name: OSF Registries
Year: 2024
Subjects: subject: Cognitive Neuroscience
subject: Life Sciences
subject: Behavioral Economics
subject: Cognitive Psychology
subject: Economics
subject: Neuroscience and Neurobiology
subject: Cognition and Perception
subject: Social and Behavioral Sciences
subject: Psychology
subject: FOS: Psychology

description: In this study, participants completed an adapted version of the Monetary Incentive Delay (MID) task in a VR headset, reporting their affective state (valence and arousal) during the course of the task. The size and motion of the cue was manipulated. This per-registration is independent of the hypotheses about cue size and motion, and mainly focuses on the relation between pupil dilation and subjective affective state. Data has been collected but has not been processed.
title: Ð¢ÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð¸Ð·Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ Ð´ÐµÑÐ°Ð»Ð¸ Â«ÐÐ¾ÑÐ¾Ð±ÐºÐ°Â» Ñ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ°Ð¼Ð¸ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÐ¶ÑÑÐµÐ³Ð¾ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¡Ð°Ð»ÑÐ½Ð¸ÐºÐ¾Ð², 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: 2016
Subjects: ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ
ÑÐµÐ¶Ð¸Ð¼Ñ ÑÐµÐ·Ð°Ð½Ð¸Ñ
ÑÐ¸ÐºÐ»Ð¾Ð³ÑÐ°Ð¼Ð¼Ð°
Ð·Ð°Ð³ÑÑÐ·Ð¾ÑÐ½Ð¾Ðµ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾

description: Ð Ð¿ÐµÑÐ²Ð¾Ð¼ ÑÐ°Ð·Ð´ÐµÐ»Ðµ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ° Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐ½Ð¾ÑÑÐ¸ Ð¾Ð±ÑÐ°Ð±Ð°ÑÑÐ²Ð°ÐµÐ¼Ð¾Ð¹ Ð´ÐµÑÐ°Ð»Ð¸ âÐÐ¾ÑÐ¾Ð±ÐºÐ°â, Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð²ÑÐ±Ð¾ÑÐ° Ð·Ð°Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² ÐµÐµ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð¸Ð·Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ Ð´ÐµÑÐ°Ð»Ð¸, Ð²ÑÐ±Ð¾Ñ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð¾ÑÐ½Ð°ÑÑÐºÐ¸, ÑÐ°ÑÑÐµÑ ÑÐµÐ¶Ð¸Ð¼Ð¾Ð² ÑÐµÐ·Ð°Ð½Ð¸Ñ Ð¸ Ð½Ð¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¹. ÐÐ¾ Ð²ÑÐ¾ÑÐ¾Ð¼ ÑÐ°Ð·Ð´ÐµÐ»Ðµ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ° Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð¿Ð¾ÑÑÐ´Ð¾Ðº ÑÐ°ÑÑÐµÑÐ° ÑÐµÐ¶ÑÑÐ¸Ñ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ¾Ð² Ð´Ð»Ñ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð·Ð°Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð½Ð° Ð¾ÑÐ´ÐµÐ»ÑÐ½ÑÑ Ð¾Ð¿ÐµÑÐ°ÑÐ¸ÑÑ: ÑÐ°ÑÐ¾Ð½Ð½ÑÐ¹ Ð¿ÑÐ¸Ð·Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ ÑÐµÐ·ÐµÑ, ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ Ð¼ÐµÑÑÐ¸ÐºÐ¾Ð² Ð¸ ÑÐµÑÐ²ÑÑÐ½Ð°Ñ ÑÑÐµÐ·Ð° Ð´Ð»Ñ Ð½Ð°ÑÐµÐ·Ð°Ð½Ð¸Ñ ÑÐ¸Ð»Ð¸Ð½Ð´ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð·ÑÐ±ÑÐ°ÑÑÑ ÐºÐ¾Ð»ÐµÑ. Ð ÑÑÐµÑÑÐµÐ¼ ÑÐ°Ð·Ð´ÐµÐ»Ðµ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ° Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð° Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ñ Ð¾Ð´Ð½Ð¾Ð³Ð¾ Ð¿ÐµÑÐµÑÐ¾Ð´Ð° Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð·Ð°Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸. ÐÑÐ»Ð¸ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¸ Ð²ÑÐ±ÑÐ°Ð½Ñ Ð·Ð°Ð³ÑÑÐ·Ð¾ÑÐ½Ð¾Ðµ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾ Ð¸ Ð¾ÑÑÐµÐºÐ°ÑÐµÐ»Ñ. Ð¢Ð°ÐºÐ¶Ðµ Ð±ÑÐ» Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ ÑÐ°ÑÑÐµÑ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² Ð·Ð°Ð³ÑÑÐ·Ð¾ÑÐ½Ð¾Ð³Ð¾ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° Ð¸ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð° ÑÐ¸ÐºÐ»Ð¾Ð³ÑÐ°Ð¼Ð¼Ð° ÑÐ°Ð±Ð¾ÑÑ Ð·Ð°Ð³ÑÑÐ·Ð¾ÑÐ½Ð¾Ð³Ð¾ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° Ð¸ ÑÑÐ°Ð½ÐºÐ°.
Volterra-Prabhakar derivative of distributed order and some applications
Creators: name: Górska, K.
name: Pietrzak, T.
name: Sandev, T.
name: Tomovsky, {Ž}.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: The paper studies the exact solution of two kinds of generalized Fokker-Planck equations in which the integral kernels are given either by the distributed order function $k_{1}(t) = \int_{0}^{1} t^{-μ}/Γ(1- μ) dμ$ or the distributed order Prabhakar function $k_{2}(α, γ; λ; t) = \int_{0}^{1} e^{-γ}_{α, 1 - μ}(λ; t) dμ$, where the Prabhakar function is denoted as $e^{-γ}_{α, 1 - μ}(λ; t)$. Both of these integral kernels can be called the fading memory functions and are the Stieltjes functions. It is also shown that their Stieltjes character is enough to ensure the non-negativity of the mean square values and higher even moments. The odd moments vanish. Thus, the solution of generalized Fokker-Planck equations can be called the probability density functions. We introduce also the Volterra-Prabhakar function and its generalization which are involved in the definition of $k_{2}(α, γ; λ; t)$ and generated by it the probability density function $p_2(x, t)$.
Bridging Data Silos Using Big Data Integration
Creators: name: Patel, Jayeshkumar
Publisher: name: Zenodo
Year: 2025

description: With cloud computing, cheap storage and technology advancements, an enterprise uses multiple applications to operate business functions. Applications are not limited to just transactions, customer service, sales, finance but they also include security, application logs, marketing, engineering, operations, HR and many more. Each business vertical uses multiple applications which generate a huge amount of data. On top of that, social media, IoT sensors, SaaS solutions, and mobile applications record exponential growth in data volume. In almost all enterprises, data silos exist through these applications. These applications can produce structured, semi-structured, or unstructured data at different velocity and in different volume. Having all data sources integrated and generating timely insights helps in overall decision making. With recent development in Big Data Integration, data silos can be managed better and it can generate tremendous value for enterprises. Big data integration offers flexibility, speed and scalability for integrating large data sources. It also offers tools to generate analytical insights which can help stakeholders to make effective decisions. This paper presents the overview on data silos, challenges with data silos and how big data integration can help to stun them.
title: Ð¡ÑÐ¾Ð¸Ð¼Ð¾ÑÑÑ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð° Ð³Ð¸Ð´ÑÐ¾ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ð¹
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: Ð¢ÐµÐ»ÐµÑÐµÐ², ÐÐ¸ÐºÑÐ¾Ñ
name: ÐÐ¾ÑÐ¾Ð±ÑÐµÐ², ÐÐ¾ÑÐ¸Ñ
name: ÐÐµÐ»Ð¾Ð»Ð¸ÐºÐ¾Ð², ÐÐ¸ÑÐ°Ð»Ð¸Ð¹
name: ÐÑÑÐ°ÑÐ¾Ð²Ð°, ÐÑÐµÐ½Ð¸Ñ
Publisher: name: ÐÐÐ
Year: 1986
Subjects: ÐÐ¸Ð´ÑÐ¾ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ¾Ðµ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð¾

description: Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÐµÑ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹ Ð³Ð¸Ð´ÑÐ¾ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ°, Ð²ÑÐ¿Ð¾Ð»Ð½ÑÑÑÐ¸Ñ ÐºÑÑÑÐ¾Ð²ÑÐµ Ð¿ÑÐ¾ÐµÐºÑÑ Ð¸ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÑÑÐ¸Ðµ ÑÐ°Ð·Ð´ÐµÐ»Ñ Ð¿Ð¾ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐµ Ð³Ð¸Ð´ÑÐ¾ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð° Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½ÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ¾Ð², Ð° ÑÐ°ÐºÐ¶Ðµ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¾ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ°Ð¼Ð¸ Ð´Ð»Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð·Ð°Ð´Ð°Ñ ÑÐµÑÐ½Ð¸ÐºÐ¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð²ÑÐ±Ð¾ÑÐ° Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½ÑÑ Ð²Ð°ÑÐ¸Ð°Ð½ÑÐ¾Ð² ÑÐµÑÐµÐ½Ð¸Ñ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð²Ð½ÑÑ, ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð·Ð°Ð´Ð°Ñ. Ð ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð´Ð°Ð½Ñ Ð¾ÑÐ½Ð¾Ð²Ñ ÑÐµÐ½Ð¾Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð² ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ðµ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ°ÑÑÐµÑÐ¾Ð² ÑÐ¼ÐµÑÐ½Ð¾Ð¹ ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÐ¸ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð° ÑÑÐ°Ð´Ð¸ÑÐ¸Ð¾Ð½Ð½ÑÐ¼Ð¸ ÑÐ¿Ð¾ÑÐ¾Ð±Ð°Ð¼Ð¸ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð­ÐÐ.
Absolute frequency measurement of a Yb optical clock at the limit of the Cs fountain
Creators: name: Goti, Irene
name: Condio, Stefano
name: Clivati, Cecilia
name: Risaro, Matias
name: Gozzelino, Michele
name: Costanzo, Giovanni A.
name: Levi, Filippo
name: Calonico, Davide
name: Pizzocaro, Marco
Publisher: name: arXiv
Year: 2022
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: We present the new absolute frequency measurement of ytterbium (171Yb) obtained at INRiM with the optical lattice clock IT-Yb1 against the cryogenic caesium (133Cs) fountain IT-CsF2, evaluated through a measurement campaign that lasted 14 months. Measurements are performed by either using a hydrogen maser as a transfer oscillator or by synthesizing a low-noise microwave for Cs interrogation using an optical frequency comb. The frequency of the 171Yb unperturbed clock transition 1S0 - 3P0 results to be 518 295 836 590 863.44(14) Hz, with a total fractional uncertainty of 2.7e-16 that is limited by the uncertainty of IT-CsF2. Our measurement is in agreement with the Yb frequency recommended by the Consultative Committee for Time and Frequency (CCTF). This result confirms the reliability of Yb as a secondary representation of the second and is relevant to the process of redefining the second in the International System of Units (SI) on an optical transition
GJ 3236: a new bright, very low-mass eclipsing binary system discovered by the MEarth observatory
Creators: name: Irwin, Jonathan
name: Charbonneau, David
name: Berta, Zachory K.
name: Quinn, Samuel N.
name: Latham, David W.
name: Torres, Guillermo
name: Blake, Cullen H.
name: Burke, Christopher J.
name: Esquerdo, Gilbert A.
name: Furesz, Gabor
name: Mink, Douglas J.
name: Nutzman, Philip
name: Szentgyorgyi, Andrew H.
name: Calkins, Michael L.
name: Falco, Emilio E.
name: Bloom, Joshua S.
name: Starr, Dan L.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We report the detection of eclipses in GJ 3236, a bright (I = 11.6) very low mass binary system with an orbital period of 0.77 days. Analysis of light- and radial velocity curves of the system yielded component masses of 0.38 +/- 0.02 and 0.28 +/- 0.02 Msol. The central values for the stellar radii are larger than the theoretical models predict for these masses, in agreement with the results for existing eclipsing binaries, although the present 5% observational uncertainties limit the significance of the larger radii to approximately 1 sigma. Degeneracies in the light curve models resulting from the unknown configuration of surface spots on the components of GJ 3236 currently dominate the uncertainties in the radii, and could be reduced by obtaining precise, multi-band photometry covering the full orbital period. The system appears to be tidally synchronized and shows signs of high activity levels as expected for such a short orbital period, evidenced by strong Halpha emission lines in the spectra of both components. These observations probe an important region of mass-radius parameter space around the predicted transition to fully-convective stellar interiors, where there are a limited number of precise measurements available in the literature.
description: 14 pages, 5 figures, 10 tables, emulateapj format. Accepted for publication in ApJ
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ Ð²ÑÐ±Ð¾ÑÐ° Ð±Ð¸Ð·Ð½ÐµÑ-Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð´Ð»Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¼Ð°Ð»Ð¾Ð³Ð¾ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ)
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¸Ð¼Ð¾ÑÐµÐµÐ²Ð°, ÐÐºÐ°ÑÐµÑÐ¸Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð±Ð¸Ð·Ð½ÐµÑ-Ð¼Ð¾Ð´ÐµÐ»Ñ
ÑÑÑÐ°ÑÐµÐ³Ð¸Ñ
ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¸Ñ

description: ÐÐ½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¿ÑÐ¾Ð´ÑÐºÑÑ Ð±Ð¾Ð»ÑÑÐµ Ð½Ðµ ÑÐ²Ð»ÑÑÑÑÑ Ð³Ð°ÑÐ°Ð½ÑÐ¸ÐµÐ¹ ÑÑÐ¿ÐµÑÐ° Ð½Ð° ÑÑÐ½ÐºÐµ. ÐÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÐµÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ´ÐµÑÐ¶Ð°ÑÑÑÑ Ð½Ð° ÑÑÐ½ÐºÐµ Ð¸ Ð¾Ð´Ð½Ð¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾ ÑÐ²Ð»ÑÐµÑÑÑ ÑÑÐ¸Ð¼ÑÐ»Ð¾Ð¼ Ð´Ð»Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¾ÑÑÐ°ÑÐ»Ð¸ Ð² ÑÐµÐ»Ð¾Ð¼. Ð­ÑÑÐµÐºÑÐ¸Ð²Ð½Ð°Ñ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¼Ð¾Ð´ÐµÐ»Ñ - ÑÑÐ¾ Ð±Ð°Ð»Ð°Ð½Ñ ÑÐµÑÑÑÑÐ¾Ð², Ð¼Ð¾ÑÐ½Ð¾ÑÑÐµÐ¹ Ð¸ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐµÐ¸Ð¼ÑÑÐµÑÑÐ²Ð°.
title: On the treatment of correlated observation errors in data assimilation
Creators: name: Tabeart, Jemima M.
Publisher: name: University of Reading
Year: 2019

description: Data assimilation combines information from observations of a dynamical system with a previous forecast, with each term weighted by its respective uncertainty. An important recent area of research has been the introduction of correlated observation error covariance (OEC) matrices in numerical weather prediction systems. The benefits of correlated OEC matrices are multiple: they permit the use of high density observation networks, allow the capture of small scale processes and help make best use of available data. However, their use is often associated with convergence problems for iterative methods. In this thesis we study the theoretical impact of introducing correlated OEC matrices on the conditioning of variational data assimilation problems. We develop new bounds on the condition number of the Hessian for two data assimilation formulations and illustrate our findings with numerical examples in an idealised framework. The minimum eigenvalue of the OEC matrix is a key term for both problems, which motivates the use of reconditioning methods to reduce the condition number of correlation matrices. We develop theory for two reconditioning methods: ridge regression and the minimum eigenvalue method. We show for the first time that standard deviations are increased by both methods. Ridge regression reduces absolute correlations, whereas the minimum eigenvalue method makes smaller changes to correlations and variances. We then present the first in-depth study of the ridge regression method for an operational data assimilation system, using the Met Office 1D-Var system. Reconditioning improves convergence, but alters the quality control procedure, which is used to select appropriate observations for further assimilation. The results in this thesis provide guidance on how to include correlation information in general variational data assimilation problems while ensuring computational efficiency.
Inelastic Neutron Scattering in Weakly Coupled Triangular Spin Tubes CsCrF$_4$
Creators: name: Kikuchi, Hodaka
name: Asai, Shinichiro
name: Manaka, Hirotaka
name: Hagihala, Masato
name: Itoh, Shinichi
name: Masuda, Takatsugu
Publisher: name: arXiv
Year: 2022
Subjects: subject: Other Condensed Matter (cond-mat.other)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We performed inelastic neutron scattering (INS) experiments to measure spin dynamics on a polycrystalline sample of a spin tube candidate CsCrF$_{4}$. The compound exhibits a successive phase transition from a paramagnetic phase through an intermediate temperature (IT) phase of a 120$^{\circ}$ structure to a low temperature (LT) phase of another 120$^{\circ}$ structure. Elaborate comparison between observed and calculated neutron spectra in LT phase reveals that the spin Hamiltonian is identified as antiferromagnetic spin tubes including perturbative terms of intertube interaction, Dzyaloshinskii-Moriya interaction, and single ion anisotropy. A phase diagram for the ground state is classically calculated. A set of parameters in the spin Hamiltonian obtained from the INS spectra measured in LT phase is quite close to a boundary to the phase of the 120$^{\circ}$ structure of IT phase. The INS spectra measured in IT phase is, surprisingly, the same as those in LT phase in the level of powder averaged spectra, even though the magnetic structures in IT and LT phases are different. Identical dynamical structures compatible with two different static structures are observed. No difference in the observed spectra indicates no change of the spin Hamiltonian with the temperature, suggesting that the origin of the successive phase transition being order-by-disorder mechanism.
Nuclear Physics from QCD
Creators: name: van Kolck, U.
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Effective field theories provide a bridge between QCD and nuclear physics. I discuss light nuclei from this perspective, emphasizing the role of fine-tuning.
description: 10 pages, 5 figures; talk at Quark Confinement and the Hadron Spectrum, September 1-6 2008, Mainz, Germany
Additional file 6 of A robust immune-related gene pairs signature for predicting the overall survival of esophageal cancer
Creators: name: Zheng, Wei
name: Fang, Gaofeng
name: Huang, Qiao
name: Shi, Dan
name: Xie, Biao
Publisher: name: figshare
Year: 2023
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Cancer

description: Table S3. The significant biological processes enriched by genes consisted in the IRGPI.
title: ÐÑÐ¸Ð½ÑÑÐ¸Ðµ ÑÐµÑÐµÐ½Ð¸Ð¹ Ð² ÑÑÐµÐ·Ð²ÑÑÐ°Ð¹Ð½ÑÑ ÑÐ¸ÑÑÐ°ÑÐ¸ÑÑ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: Ð ÑÐ±Ð¸Ð½Ð¸Ð½Ð°, ÐÐ»ÐµÐ½Ð°
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¸Ð½ÑÑÐ¸Ðµ ÑÐµÑÐµÐ½Ð¸Ð¹
ÐÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÑ Ð¶Ð¸Ð·Ð½ÐµÐ´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÐµÐ»Ð¾Ð²ÐµÐºÐ°
ÑÑÐµÐ·Ð²ÑÑÐ°Ð¹Ð½ÑÐµ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¸
ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½ÑÐµÑÐºÐ¸Ðµ ÑÐµÑÐµÐ½Ð¸Ñ

description: Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ Â«ÐÑÐ¸Ð½ÑÑÐ¸Ðµ ÑÐµÑÐµÐ½Ð¸Ð¹ Ð² ÑÑÐµÐ·Ð²ÑÑÐ°Ð¹Ð½ÑÑ ÑÐ¸ÑÑÐ°ÑÐ¸ÑÑÂ» Ð¿Ð¾ÑÐ²ÑÑÐµÐ½ ÑÐµÐ¾ÑÐ¸Ð¸ Ð¸ Ð¿ÑÐ°ÐºÑÐ¸ÐºÐµ Ð¿ÑÐ¸Ð½ÑÑÐ¸Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½ÑÐµÑÐºÐ¸Ñ ÑÐµÑÐµÐ½Ð¸Ð¹, Ð² ÑÐ¾Ð¼ ÑÐ¸ÑÐ»Ðµ Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½ÑÑ ÑÑÐµÐ·Ð²ÑÑÐ°Ð¹Ð½ÑÑ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¹. Ð Ð½ÐµÐ¼ Ð¿Ð¾Ð´ÑÐ¾Ð±Ð½Ð¾ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÑÐ°Ð¿Ñ Ð¿ÑÐ¸Ð½ÑÑÐ¸Ñ Ð¸ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐµÑÐµÐ½Ð¸Ð¹. ÐÑÐ¾Ð±Ð¾Ðµ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ ÑÐ´ÐµÐ»ÐµÐ½Ð¾ Ð°Ð½Ð°Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ð¼ Ð¸ Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¸Ð¼ ÑÐ¿Ð¾ÑÐ¾Ð±Ð°Ð¼ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð¿ÑÐ¸ÑÐ¸Ð½ Ð²Ð¾Ð·Ð½Ð¸ÐºÐ½Ð¾Ð²ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼, Ð¼ÐµÑÐ¾Ð´Ð°Ð¼ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð²Ð°ÑÐ¸Ð°Ð½ÑÐ¾Ð² ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½ÑÐµÑÐºÐ¸Ñ ÑÐµÑÐµÐ½Ð¸Ð¹, ÑÐ¿Ð¾ÑÐ¾Ð±Ð°Ð¼ Ð¾ÑÐµÐ½ÐºÐ¸ Ð¸ Ð²ÑÐ±Ð¾ÑÑ ÑÐµÑÐµÐ½Ð¸Ð¹ Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½Ð¾ÑÑÐ¸, ÑÐ¸ÑÐºÐ° Ð¸ Ð½ÐµÐ¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½Ð¾ÑÑÐ¸. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÐºÐ¾Ð»Ð»ÐµÐ³Ð¸Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¸ Ð¿ÑÐ¸Ð½ÑÑÐ¸Ð¸ ÑÐµÑÐµÐ½Ð¸Ð¹. ÐÐ¿Ð¾ÑÐ½ÑÐ¹ ÐºÐ¾Ð½ÑÐ¿ÐµÐºÑ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½ Ð´Ð»Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð² ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð¿ÑÐ¾ÑÐµÑÑÐµ Ð´Ð»Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÑÑÐµÐ³Ð¾ ÑÑÐµÐ±Ð½Ð¾Ð³Ð¾ Ð·Ð°Ð²ÐµÐ´ÐµÐ½Ð¸Ñ, Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÐ¼ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Â«Ð¢ÐµÑÐ½Ð¾ÑÑÐµÑÐ½Ð°Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÑÂ» (20.03.01; 20.04.01; 20.06.01).
The generating of Fractal Images Using MathCAD Program
Creators: name: Stefan, Laura
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mathematical Software (cs.MS)
subject: FOS: Computer and information sciences

description: This paper presents the graphic representation in the z-plane of the first three iterations of the algorithm that generates the Sierpinski Gasket. It analyzes the influence of the f(z) map when we represent fractal images.
description: 10 pages, exposed on 2nd "European Conference on Computer Science and Applications" - XA2008, Timisoara, Romania
title: ÐÐ´Ð¾ÑÐ¾Ð²ÑÐµ - Ð¾ÑÐ½Ð¾Ð²Ð° ÑÐµÐ»Ð¾Ð²ÐµÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»Ð°: Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¸ Ð¿ÑÑÐ¸ Ð¸Ñ ÑÐµÑÐµÐ½Ð¸Ñ. Ð¢. 12, Ñ. 2
title: ÑÑÑÐ´Ñ XII ÐÑÐµÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð½Ð°ÑÑÐ½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ð¸ Ñ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¼ ÑÑÐ°ÑÑÐ¸ÐµÐ¼, 23-25 Ð½Ð¾ÑÐ±ÑÑ 2017 Ð³.
titleType: Subtitle
Creators: name: "ÐÐ´Ð¾ÑÐ¾Ð²ÑÐµ-Ð¾ÑÐ½Ð¾Ð²Ð° ÑÐµÐ»Ð¾Ð²ÐµÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»Ð°: Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¸ Ð¿ÑÑÐ¸ Ð¸Ñ  ÑÐµÑÐµÐ½Ð¸Ñ", Ð²ÑÐµÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ°Ñ Ð½Ð°ÑÑÐ½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ Ñ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¼ ÑÑÐ°ÑÑÐ¸ÐµÐ¼ (12; 2017; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
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·Ð´Ð¾ÑÐ¾Ð²ÑÐµ
Ð´ÐµÐ¼Ð¾Ð³ÑÐ°ÑÐ¸Ñ

description: Ð ÐºÐ½Ð¸Ð³Ðµ Ð¾Ð¿ÑÐ±Ð»Ð¸ÐºÐ¾Ð²Ð°Ð½Ñ ÑÐµÐ·Ð¸ÑÑ Ð´Ð¾ÐºÐ»Ð°Ð´Ð¾Ð² Ð¸ ÑÑÐ°ÑÑÐ¸, Ð¾ÑÑÐ°Ð¶Ð°ÑÑÐ¸Ðµ ÑÑÐ¾Ð²ÐµÐ½Ñ Ð¸ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÑ Ð·Ð°Ð±Ð¾Ð»ÐµÐ²Ð°ÐµÐ¼Ð¾ÑÑÐ¸ Ð¸ ÑÐ¼ÐµÑÑÐ½Ð¾ÑÑÐ¸ Ð¿Ð¾ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐ¼ Ð³ÑÑÐ¿Ð¿Ð°Ð¼ Ð·Ð°Ð±Ð¾Ð»ÐµÐ²Ð°Ð½Ð¸Ð¹ ÑÑÐµÐ´Ð¸ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð¸Ñ. ÐÑÐ¸Ð²Ð¾Ð´ÑÑÑÑ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¾ Ð´ÐµÐ¼Ð¾Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ°Ñ Ð² Ð½Ð°ÑÐµÐ¹ ÑÑÑÐ°Ð½Ðµ Ð¸ Ð·Ð° ÑÑÐ±ÐµÐ¶Ð¾Ð¼ Ñ ÑÑÐµÑÐ¾Ð¼ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ Ð¸ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð°ÑÐ¿ÐµÐºÑÐ¾Ð². ÐÐ¾Ð´Ð½Ð¸Ð¼Ð°ÑÑÑÑ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ ÑÐºÐ¾Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¸ Ð²ÑÑÑÐµÐ³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð¿ÑÐ¸ÑÐ¾Ð»Ð¾Ð³Ð¸Ð¸, Ð¿ÐµÐ´Ð°Ð³Ð¾Ð³Ð¸ÐºÐ¸, ÑÐ¾ÑÐ¸Ð¾Ð»Ð¾Ð³Ð¸Ð¸, ÑÐ¸Ð»Ð¾ÑÐ¾ÑÐ¸Ð¸ Ð¸ Ð¸ÑÑÐ¾ÑÐ¸Ð¸ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½Ñ Ð¸ Ð·Ð´ÑÐ°Ð²Ð¾Ð¾ÑÑÐ°Ð½ÐµÐ½Ð¸Ñ. ÐÑÐ²ÐµÑÐ°ÑÑÑÑ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð¿ÑÐ¾Ð´Ð¾Ð²Ð¾Ð»ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸. ÐÑÐµÐ´Ð»Ð°Ð³Ð°ÑÑÑÑ Ð¿ÑÑÐ¸ ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ Ð·Ð´Ð¾ÑÐ¾Ð²ÑÑ Ð½Ð°ÑÐ¾Ð´Ð° Ð² ÑÑÑÐ°Ð½Ðµ Ð¸ ÐµÐµ Ð¾ÑÐ´ÐµÐ»ÑÐ½ÑÑ ÑÐµÐ³Ð¸Ð¾Ð½Ð°Ñ, Ð³Ð¾ÑÐ¾Ð´Ð°Ñ Ð¸ ÑÑÑÐµÐ¶Ð´ÐµÐ½Ð¸ÑÑ.
Interpolation and Exponentially Suppressed Cosmological Constant in Non-Supersymmetric Heterotic Strings with General $\mathbb{Z}_{2}$ Twists
Creators: name: Koga, Yuichi
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study general non-supersymmetric heterotic string models, including so-called interpolating models, $d$-dimensionally compactified with the arbitrary number of freely acting $\mathbb{Z}_{2}$ twisted directions. Taking the limits of the compactified radii to zero and infinity (the endpoint limits), we show some examples of the various interpolation patterns in the $d=2$ (8-dimensional) case. In the region where supersymmetry is asymptotically restored, we derive the formula for the one-loop cosmological constant of $(10-d)$ dimensional non-supersymmetric heterotic string models with general $\mathbb{Z}_{2}$ twists, which does not depend on all the other endpoints and find out the points in the moduli space where the cosmological constant is exponentially suppressed. The moduli stability of the cosmological constant is also analyzed.
description: 39 pages, 4 figures; 2nd version, minor changes made and references added
The linear rms-flux relation in an Ultraluminous X-ray Source
Creators: name: Heil, L. M.
name: Vaughan, S.
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We report the first detection of a linear correlation between rms variability amplitude and flux in the Ultraluminous X-ray source NGC 5408 X-1. The rms-flux relation has previously been observed in several Galactic black hole X-ray binaries (BHBs), several Active Galactic Nuclei (AGN) and at least one neutron star X-ray binary. This result supports the hypothesis that a linear rms-flux relation is common to all luminous black hole accretion and perhaps even a fundamental property of accretion flows about compact objects. We also show for the first time the cross-spectral properties of the variability of this ULX, comparing variations below and above 1 keV. The coherence and time delays are poorly constrained but consistent with high coherence between the two bands, over most of the observable frequency range, and a significant time delay (with hard leading soft variations). The magnitude and frequency dependence of the lags are broadly consistent with those commonly observed in BHBs, but the direction of the lag is reversed. These results indicate that ULX variability studies, using long X-ray observations, hold great promise for constraining the processes driving ULXs behaviour, and the position of ULXs in the scheme of black hole accretion from BHBs to AGN.
description: 4 Pages, 3 figures, accepted for publication by MNRAS.