cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Supplement of Comparison of Different Diagnostic Criteria of 68Ga-Pentixafor PET-CT for the Classification of Primary Aldosteronism.docx
Creators: name: Zhang, Xiangshuang
name: Song, Ying
name: Jing, Ying
Publisher: name: figshare
Year: 2024
Subjects: classificationCode: 320208
subject: Endocrinology

description: Supplement of Comparison of Different Diagnostic Criteria of 68Ga-Pentixafor PET/CT for the Classification of Primary Aldosteronism
Consequences of planet formation on the stellar composition
Creators: name: Kunitomo, Masanobu
name: Guillot, Tristan
Publisher: name: Zenodo
Year: 2021

description: Circumstellar disks have an evolving composition due to planet formation processes such as grain growth, planetesimal formation, and disk winds. Therefore, the accretion of disk gas may alter the stellar composition. In order to determine the magnitude of this effect, a key ingredient is the stellar surface convective zone whose thickness determines the dilution of the “planet pollution” signature. Thus, first I will present the thermal evolution of young stellar objects. From stellar evolution calculations, we find that the evolution can deviate from the standard picture depending on accretion heat. Using up-to-date stellar evolution models, we estimate the compositional changes due to planet formation. In this poster, I will focus particularly on the Sun. The Sun has a refractory-poor surface composition compared to solar twins. We find that if the ice-to-rock ratio in the Solar-System planets is less than 0.4, then the anomaly can be originated from the accretion of predominantly volatile elements in the early Solar System due to planet formation. We also find that the signature of planet formation is imprinted in the central region. The central metallicity is enhanced by up to 5%, which is qualitatively in accordance with recent neutrino observations. Therefore, we conclude that accretion including planet formation processes is crucial for a realistic solar model.
description: {"references": ["Kunitomo & Guillot (2021), arXiv e-prints, arXiv:2109.06492", "Kunitomo et al. (2018), A&A, 618, A132", "Kunitomo et al. (2017), A&A, 599, A49"]}
Additional file 24 of Expanded catalogue of metagenome-assembled genomes reveals resistome characteristics and athletic performance-associated microbes in horse
Creators: name: Li, Cunyuan
name: Li, Xiaoyue
name: Guo, Rongjun
name: Ni, Wei
name: Liu, Kaiping
name: Liu, Zhuang
name: Dai, Jihong
name: Xu, Yueren
name: Abduriyim, Shamshidin
name: Wu, Zhuangyuan
name: Zeng, Yaqi
name: Lei, Bingbing
name: Zhang, Yunfeng
name: Wang, Yue
name: Zeng, Weibin
name: Zhang, Qiang
name: Chen, Chuangfu
name: Qiao, Jun
name: Liu, Chen
name: Hu, Shengwei
Publisher: name: figshare
Year: 2023
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics

description: Additional file 24: Figure S6. The racehorse gut is rich in microbes that can synthesize acetate and butyrate. The microbes enriched in racehorses contain a large number of enzymes that synthesize acetate and butyrate. At the bottom of the heatmap are the difference MAG ID, and the top are the taxonomic information of the MAG.
title: ÐÐ½Ð°Ð»Ð¸Ð· ÑÐµÐ¶Ð¸Ð¼Ð¾Ð² Ð² ÑÐ»Ð°Ð±ÑÑ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐµÑÑÑ Ñ Ð¼Ð¾ÑÐ½Ð¾Ð¹ Ð½ÐµÐ»Ð¸Ð½ÐµÐ¹Ð½Ð¾Ð¹ Ð½Ð°Ð³ÑÑÐ·ÐºÐ¾Ð¹
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐ²Ð°Ð½Ð¾Ð², ÐÐ¸ÑÐ°Ð¸Ð»
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐµÑÐ¸
ÐÐ¾Ð¼Ð¿ÐµÐ½ÑÐ°ÑÐ¾ÑÑ (ÑÐ»ÐµÐºÑÑ.)
Ð¡ÑÐ°Ð»ÐµÐ¿Ð»Ð°Ð²Ð¸Ð»ÑÐ½ÑÐµ Ð¿ÐµÑÐ¸ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ
ÐÐ°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð½ÐµÐ»Ð¸Ð½ÐµÐ¹Ð½ÑÐµ Ð½Ð°Ð³ÑÑÐ·ÐºÐ¸

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÐ¶Ð¸Ð¼Ð¾Ð² Ð² ÑÐ»Ð°Ð±ÑÑ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐµÑÑÑ Ñ Ð¼Ð¾ÑÐ½Ð¾Ð¹ Ð½ÐµÐ»Ð¸Ð½ÐµÐ¹Ð½Ð¾Ð¹ Ð½Ð°Ð³ÑÑÐ·ÐºÐ¾Ð¹ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐºÑÑÐ±Ð¸Ð½ÑÐºÐ¾Ð³Ð¾ Ð·Ð°Ð²Ð¾Ð´Ð° ÑÐµÑÑÐ¾ÑÐ¿Ð»Ð°Ð²Ð¾Ð². ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¿ÑÐ¸ÑÐ¸Ð½Ñ Ð²Ð¾Ð·Ð½Ð¸ÐºÐ½Ð¾Ð²ÐµÐ½Ð¸Ñ Ð°Ð²Ð°ÑÐ¸Ð¹Ð½ÑÑ Ð¾ÑÐºÐ»ÑÑÐµÐ½Ð¸Ð¹ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¼Ð¾Ð´ÐµÐ»Ñ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐµÑÐ¸ Ð² Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð¼ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐµ MatLab Simulik. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð¸ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð±ÐµÐ·Ð°Ð²Ð°ÑÐ¸Ð¹Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð° ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ Ð¾ÑÐµÐ½ÐºÐ° ÑÐµÐ»ÐµÑÐ¾Ð¾Ð±ÑÐ°Ð·Ð½Ð¾ÑÑÐ¸ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸ ÑÑÐ°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ¸ÑÐ¸ÑÑÐ¾ÑÐ½Ð¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿ÐµÐ½ÑÐ°ÑÐ¾ÑÐ° Ð½Ð° ÐÐºÑÑÐ±Ð¸Ð½ÑÐºÐ¾Ð¼ Ð·Ð°Ð²Ð¾Ð´Ðµ ÑÐµÑÑÐ¾ÑÐ¿Ð»Ð°Ð²Ð¾Ð² Ð·Ð° ÑÑÐµÑ ÑÐ½Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð¾ÑÐµÑÑ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ½ÐµÑÐ³Ð¸Ð¸. ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ ÑÑÐ»Ð¾Ð²Ð¸Ñ Ð´Ð»Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð¶Ð¸Ð·Ð½ÐµÐ´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¾Ð±ÑÐ»ÑÐ¶Ð¸Ð²Ð°ÑÑÐµÐ³Ð¾ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð¿ÑÐ¸ ÑÐ°Ð±Ð¾ÑÐµ Ñ ÑÐ»ÐµÐºÑÑÐ¾ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ°Ð¼Ð¸ Ð¿Ð¾ÑÑÐ¾ÑÐ½Ð½Ð¾Ð³Ð¾ Ð¸ Ð¿ÐµÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ¾ÐºÐ°.
Magnetic fileds of coalescing neutron stars and the luminosity function of short gamma-ray burst
Creators: name: Postnov, K. A.
name: Kuranov, A. G.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Coalescing neutron star binaries are believed to be the most reliable sources for ground-based detectors of gravitational waves and likely progenitors of short gamma-ray bursts. In the process of coalescence, magnetic fields of neutron stars can induce interesting observational manifestations and affect the form of gravitational wave signal. In this papaer we use the population synthesis method to model the expected distribution of neutron star magnetic fields during the coalescence under different assumptions on the initial parameters of neutron stars and their magnetic field evolution. We discuss possible elecotrmagnetic phenomena preceding the coalescence of magnetized neutron star binaries and the effect of magnetic field on the gravitational wave signal. We find that a log-normal (Gaussian in logarithms) distribution of the initial magnetic fields of neutron stars, which agrees with observed properties of radio pulsars, produces the distribution of the magnetic field energy during the coalescence that adequately describes the observed luminosity function of short gamma-ray bursts under different assumptions on the field evolution and initial parameters of neutron stars. This agreement lends further support to the model of coalescing neutron star binaries as progenitors of gamma-ray bursts.
description: v.2, LATEX, 25 pages, inc. 7 ps figures, Astron. Lett., in press. Typos corrected, reference added
title: Ð¡Ð¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ ÑÐ²Ð°ÑÐºÐ¸ ÑÑÑÐ± Ð¼Ð°Ð»Ð¾Ð³Ð¾ Ð´Ð¸Ð°Ð¼ÐµÑÑÐ°
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ¾ÑÐµÐµÐ², ÐÐ¼Ð¸ÑÑÐ¸Ð¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÐµÐ³ÑÐ»ÑÑÐ¾Ñ Ð´Ð°Ð²Ð»ÐµÐ½Ð¸Ñ
ÑÐ²Ð°ÑÐ¾ÑÐ½Ð°Ñ Ð¿ÑÐ¾Ð²Ð¾Ð»Ð¾ÐºÐ°
Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ²Ð°ÑÐºÐ°
ÑÐ²Ð°ÑÐ¾ÑÐ½ÑÐ¹ ÑÑÐµÐ½Ð´
ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ðµ ÐºÐ¾Ð»ÑÑÐ¾

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐ½Ð¾Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð½Ð° ÑÐµÐ¼Ñ ÑÐ²Ð°ÑÐºÐ¸ Ð°ÑÑÑÐµÐ½Ð¸ÑÐ½ÑÑ ÑÑÐ°Ð»ÐµÐ¹ Ð² Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ð¸. ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð¾ Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¸Ðµ ÑÐµÐ³ÑÐ»ÑÑÐ¾ÑÐ° Ð´Ð°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÑÑÐ±Ð¾Ð¿ÑÐ¾Ð²Ð¾Ð´Ð° Ð¸ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ Ð¸Ð·Ð´ÐµÐ»Ð¸Ñ. Ð¡ÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ñ ÑÐµÐ»Ñ Ð¸ Ð·Ð°Ð´Ð°ÑÐ¸, ÑÑÐµÐ±ÑÑÑÐ¸Ðµ ÑÐµÑÐµÐ½Ð¸Ñ Ð² ÑÐ°Ð±Ð¾ÑÐµ. ÐÑÐ±ÑÐ°Ð½Ñ ÑÐ¿Ð¾ÑÐ¾Ð±Ñ ÑÐ²Ð°ÑÐºÐ¸, Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ, Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ ÑÐ½Ð¸Ð¶ÐµÐ½Ð¸Ñ ÑÐ²Ð°ÑÐ¾ÑÐ½ÑÑ Ð´ÐµÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¹ Ð¸ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ð¹, ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ ÑÐ²Ð°ÑÐ½ÑÑ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ð¹, ÑÐ²Ð°ÑÐ¾ÑÐ½ÑÐµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð° Ð·Ð°Ð¼ÐµÐ½Ð° ÑÑÑÐ½Ð¾Ð¹ Ð´ÑÐ³Ð¾Ð²Ð¾Ð¹ ÑÐ²Ð°ÑÐºÐ¸ Ð½Ð° Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÑÑ ÑÐ²Ð°ÑÐºÑ Ð¿Ð¾Ð´ ÑÐ»ÑÑÐ¾Ð¼ ÐºÐ¾Ð»ÑÑÐµÐ²ÑÑ ÑÐ²Ð¾Ð² Ð´Ð¸ÑÐºÐ° ÑÐµÐ³ÑÐ»ÑÑÐ¾ÑÐ°. Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ñ ÑÐµÐ¶Ð¸Ð¼Ñ ÑÐ²Ð°ÑÐºÐ¸, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ ÑÐ±Ð¾ÑÐºÐ¸ Ð¸ ÑÐ²Ð°ÑÐºÐ¸ Ð¸Ð·Ð´ÐµÐ»Ð¸Ñ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½ÑÐµ Ð¿ÑÐ¸ÑÐ¿Ð¾ÑÐ¾Ð±Ð»ÐµÐ½Ð¸Ñ Ð´Ð»Ñ ÑÐ±Ð¾ÑÐºÐ¸ Ð¸ ÑÐ²Ð°ÑÐºÐ¸.
title: Ð¦Ð¸Ð»Ð¸Ð½Ð´Ñ ÑÑÐµÐ´Ð½ÐµÐ³Ð¾ Ð´Ð°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð°ÑÐ¾ÑÑÑÐ±Ð¸Ð½Ð½Ð¾Ð¹ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸ Ð-300-240-2
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÑÑÐ°ÑÐ¾Ð², ÐÐ¾Ð½ÑÑÐ°Ð½ÑÐ¸Ð½
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÐÐ°ÑÐ¾Ð²ÑÐµ ÑÑÑÐ±Ð¸Ð½Ñ
ÐÐ°ÑÐ¾ÑÑÑÐ±Ð¸Ð½Ð½ÑÐµ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸
ÑÐµÐ¿Ð»Ð¾Ð²ÑÐµ ÑÑ ÐµÐ¼Ñ
Ð³Ð°Ð·Ð¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ°ÑÑÐµÑ
Ð¿ÑÐ¾ÑÐ½Ð¾ÑÑÐ½Ð¾Ð¹ ÑÐ°ÑÑÐµÑ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ð° Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð¿Ð°ÑÐ¾ÑÑÑÐ±Ð¸Ð½Ð½Ð¾Ð¹ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐ¶Ðµ ÑÑÑÐµÑÑÐ²ÑÑÑÐµÐ³Ð¾ Ð¿ÑÐ¾ÑÐ¾ÑÐ¸Ð¿Ð° Ð-300-240-2 ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ ÐÐÐ. ÐÐ°Ð½Ð¾ Ð¾Ð±ÑÐµÐµ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸-Ð¿ÑÐ¾ÑÐ¾ÑÐ¸Ð¿Ð° Ð¸ Ð½ÐµÐºÐ¾ÑÐ¾ÑÑÐµ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð³Ð°Ð·Ð¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ°ÑÑÐµÑ ÑÐµÐ¿Ð»Ð¾Ð²Ð¾Ð¹ ÑÑÐµÐ¼Ñ Ð¸ Ð¿ÑÐ¾ÑÐ½Ð¾ÑÑÐ½Ð¾Ð¹ ÑÐ°ÑÑÐµÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ ÑÐ·Ð»Ð¾Ð² ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸. ÐÐ·ÑÑÐµÐ½Ð° ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÑÐ¸Ñ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð².
A route to quasi-perfect invisibility cylindrical cloaks without extreme values in the parameters
Creators: name: Xi, Sheng
name: Chen, Hongsheng
name: Zhang, Baile
name: Wu, Bae-Ian
name: Kong, Jin Au
Publisher: name: arXiv
Year: 2008
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: The method of coordinate transformation offers a way to realize perfect cloaks, but provides less ability to characterize the performance of a multilayered cloak in practice. Here, we propose an analytical model to predict the performance of a multilayered cylindrical cloak, based on which, the cloak in practice can be optimized to diminish the intrinsic scatterings caused by discretization and simplification. Extremely low scattering or "quasi-perfect invisibility" can be achieved with only a few layers of anisotropic metamaterials without following the transformation method. Meanwhile, the permittivity and permeability parameters of the layers are relatively small, which is a remarkable advantage of our approach.
description: 9 pages, 6 figures
Demographics of Exoplanets in Binaries (DEB). I. Architecture of S-Type Planetary Systems Revealed by the RV Sample
Creators: name: Su, Xiang-Ning
name: Xie, Ji-Wei
name: Zhou, Ji-Lin
name: Thebault, Philippe
Publisher: name: Zenodo
Year: 2021

description: Although the sample of exoplanets in binaries has been greatly expanded, the sample heterogeneity and observational bias are obstacles toward a clear figure of exoplanet demographics in the binary environment. To overcome the obstacles, we conduct a statistical study that focuses on S-type planetary systems detected by the Radial Velocity method. We try to account for observational biases by estimating, from available RV data, planet detection efficiencies for each individual system. Our main results are as follows: (1) Single (multiple) planetary systems are mostly found in close (wide) binaries with separation aB<(>)100-300 AU. (2) In binaries, single and multiple-planet systems are similar in 1-D distributions of mass and period as well as eccentricity (in contrast to the "eccentricity dichotomy" found in single-star systems) but different in the 2-D period-mass diagram. Specifically, there is a rectangular-shaped gap in the period-mass diagram of single-planet systems but not for multiples. This gap also depends on binary separation and is more prominent in close binaries. (3) There is a rising upper envelope in the period-mass diagram for planets in wide binaries as well as in single stars but not in close binaries. More specifically, there is a population of massive short period planets in close binaries but almost absent in wide binaries or single stars. We suggest that enhanced planetary migration, collision, and /or ejection in close binaries could be the potential underlying explanation for these three features.
Lyophilized fecal microbiota transplantation mitigates antibiotic-induced pathology and alters the intestinal epithelial barrier in Muc2-/- mice
Creators: name: Chan, Jocelyn Joy
Publisher: name: University of British Columbia
Year: 2024

description: Background: MUC2 is the primary mucin comprising the intestinal mucus layer that separates noxious luminal stimuli, such as bacteria, from the underlying intestinal epithelium. Muc2-deficient mice (Muc2⁻⧸⁻) display a severely compromised intestinal mucus barrier and develop spontaneous colitis as they age. Defects in the colonic mucus barrier are often observed in patients with ulcerative colitis (UC). Studies have explored whether fecal microbiota transplantation (FMT) is therapeutic in UC. While FMT is highly effective in treating recurrent C. difficile infections with cure rates over 90%, its efficacy in UC shows promising but more variable outcomes, with approximately 36% of patients achieving remission. Here, we utilized Muc2⁻⧸⁻ mice to model FMT for UC, testing its efficacy and exploring underlying mechanisms. Method: Prior to FMT, mice deficient in Muc2 (Muc2⁻⧸⁻) and heterozygous for Muc2 (Muc2⁺⧸⁻) were pretreated with an antifungal drug (amphotericin B) and given broad-spectrum antibiotics (vancomycin, ampicillin, neomycin, metronidazole) for a week in their drinking water. Following a 24-hour antibiotic washout period, lyophilized FMT from pooled C57BL/6 mice stool or a lyophilized sucrose control was administered ad libitum for three consecutive days. Mice were euthanized at several key timepoints to examine both acute and long-term effects: Day 3 of administering FMT, 2 weeks post-FMT, and 20 weeks post-FMT. Results: Without FMT, antibiotic-treated Muc2⁻⧸⁻ mice developed spontaneous colitis, experienced bacterial translocation, and required humane euthanasia at early timepoints. Lyophilized FMT engrafted in Muc2⁻⧸⁻ mice, restoring microbial diversity and enhancing intestinal barrier function. FMT reduced intestinal permeability, prevented bacterial penetration of colonic crypts, mitigated colitic pathology, and stimulated changes in the intestinal epithelium characterized by elevated transcription and production of trefoil factor 3 (TFF3) and mucins, including mucin 5AC (MUC5AC). Conclusion: FMT delayed the onset of spontaneous colitis in Muc2⁻⧸⁻ mice and increased their survival rates following antibiotic treatment. The protective effects were evident in terms of colonic pathology as early as the third day of treatment. FMT-treated Muc2⁻⧸⁻ mice exhibited improved mucosal epithelial integrity, characterized by reduced intestinal permeability and absence of bacterial translocation, and elevated gene expression of goblet cell-secreted factors such as TFF3, MUC3, and MUC5AC.
title: Ð¢ÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð° Ð¿ÐµÑÐ¾ÑÐ½Ð¾Ð³Ð¾ Ð¿ÐµÑÐµÐ½ÑÑ Ñ Ð´Ð¾Ð±Ð°Ð²Ð»ÐµÐ½Ð¸ÐµÐ¼ Ð»ÑÐ½ÑÐ½Ð¾Ð¹ Ð¼ÑÐºÐ¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°Ð½Ð¸Ð»ÑÑÑÐº, ÐÐ¸ÐºÐ¸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: ÐºÐ¾Ð½Ð´Ð¸ÑÐµÑÑÐºÐ¸Ðµ Ð¸Ð·Ð´ÐµÐ»Ð¸Ñ
Ð»ÑÐ½ÑÐ½Ð°Ñ Ð¼ÑÐºÐ°
Ð¿ÐµÑÐµÐ½ÑÐµ
ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÑ ÐµÐ¼Ñ

description: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° ÑÑÑÑÑ Ð´Ð»Ñ Ð¿ÑÐ¸Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÐ¾ÑÐ½Ð¾Ð³Ð¾ Ð¿ÐµÑÐµÐ½ÑÑ Ñ Ð´Ð¾Ð±Ð°Ð²ÐºÐ°Ð¼Ð¸ Ð»ÑÐ½ÑÐ½Ð¾Ð¹ Ð¼ÑÐºÐ¸, Ð¸Ð·ÑÑÐµÐ½Ð¾ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð»ÑÐ½ÑÐ½Ð¾Ð¹ Ð¼ÑÐºÐ¸ Ð½Ð° Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ Ð³Ð¾ÑÐ¾Ð²Ð¾Ð¹ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸, 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°ÑÑÑÐ¸ÑÐ°Ð½Ð¾ ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²Ð¾ ÑÐµÐ»Ð¾Ð²ÐµÐº, Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÑ Ð´Ð»Ñ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ ÑÐ°Ð±Ð¾ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾Ñ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Ð¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐµÑÐ°.
Search for a low-mass Higgs boson in Y(3S)-->gamma A^0, A^0-->tau^+tau^- at BABAR
Creators: name: The BABAR Collaboration
name: Aubert, B.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We search for a light Higgs boson, $A^0$, in the radiative decay $Υ(3S)\toγA^0$, $A^0\toτ^+τ^-$, $τ^+\to e^+ν_e \barν_τ$ or $τ^+\to μ^+ ν_μ \barν_τ$. The data sample contains 122 million $Υ(3S)$ events recorded with the \babar detector. We find no evidence for a narrow structure in the studied $τ^+τ^-$ invariant mass region of $4.03(1.5-16)\times 10^{-5}$ across the $m_{τ^+τ^-}$ range. We also set a 90% C.L. upper limit on the $τ^+τ^-$-decay of the $η_b$ at ${\mathcal{B}}(η_b\to τ^+τ^-)<8%$.
Supplement of Comparison of Different Diagnostic Criteria of 68Ga-Pentixafor PET:CT for the Classification of Primary Aldosteronism.docx
Creators: name: Zhang, Xiangshuang
name: Song, Ying
name: Jing, Ying
Publisher: name: figshare
Year: 2024
Subjects: classificationCode: 320208
subject: Endocrinology

description: Supplement of Comparison of Different Diagnostic Criteria of 68Ga-Pentixafor PET/CT for the Classification of Primary Aldosteronism
Additional file 1 of Exosome-based detection of EGFR T790M in plasma and pleural fluid of prospectively enrolled non-small cell lung cancer patients after first-line tyrosine kinase inhibitor therapy
Creators: name: Yoonjung Kim
name: Saeam Shin
name: Lee, Kyung-A
Publisher: name: figshare
Year: 2021
Subjects: subject: Biophysics
subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Hematology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: 60506 Virology

description: Additional file 1: Fig. S1. Nucleic acid yield plots from exoTNA and cfDNA; Fig. S2. Assessment of T790M mutant alleles according to different sources of tumor-derived nucleic acids (exosomes, cell pellet and supernatant) from the pleural fluid and extraction methods; Fig. S3. The distribution of isolated nucleic acids; Table S1. List of genes included in Oncomine Pan-Cancer Cell-Free Assay; Table S2. Clinical characteristics and plasma mutation test results from 54 patients; Table S3. Clinical characteristics and EGFR mutation results identified in the pleural fluid from 13 patients.
title: Ð¤Ð¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¾Ð½ÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð½Ð°Ð²ÑÐºÐ¾Ð² Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¿ÑÐ¸ÐµÐ¼Ð¾Ð² Ð²Ð¸Ð·ÑÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸
title: Phonetic skills formation through visualization techniques
Creators: name: ÐÐ°ÑÑÑÐ½ÐµÐ½ÐºÐ¾, ÐÐ¸Ð»Ð¸Ñ
name: ÐÐ¾Ð²Ð°Ð»ÑÐº, ÐÐ½Ð½Ð°
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2022
Subjects: Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½ÑÐµ ÑÐ·ÑÐºÐ¸
Ð¾Ð±ÑÑÐµÐ½Ð¸Ðµ
ÑÐ¾Ð½ÐµÑÐ¸ÐºÐ°

description: Ð¤Ð¾Ð½ÐµÑÐ¸ÑÐµÑÐºÐ¸Ð¹ ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½Ñ ÑÐ²Ð»ÑÐµÑÑÑ Ð¾Ð´Ð½Ð¸Ð¼ Ð¸Ð· Ð²Ð°Ð¶Ð½ÐµÐ¹ÑÐ¸Ñ ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÐ¾Ð² ÑÐ·ÑÐºÐ¾Ð²Ð¾Ð¹ ÐºÐ¾Ð¼Ð¿ÐµÑÐµÐ½ÑÐ¸Ð¸, Ð¿Ð¾ÑÐºÐ¾Ð»ÑÐºÑ Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½Ð¾Ð³Ð¾ ÑÐ·ÑÐºÐ°, ÐºÐ°Ðº Ð¿ÑÐ°Ð²Ð¸Ð»Ð¾, Ð½Ð°ÑÐ¸Ð½Ð°ÐµÑÑÑ Ð¸Ð¼ÐµÐ½Ð½Ð¾ Ñ ÑÐ¾Ð½ÐµÑÐ¸ÐºÐ¸.
ВЛИЯНИЕ СВОБОДНЫХ ЭКОНОМИЧЕСКИХ ЗОН НА РЕГИОНАЛЬНЫЙ ЭКОНОМИЧЕСКИЙ РОСТ: ПРИМЕР НАВОИЙСКОЙ СВОБОДНОЙ ИНДУСТРИАЛЬНО-ЭКОНОМИЧЕСКОЙ ЗОНЫ
Creators: name: Кулдошев, Хуршид
Publisher: name: Zenodo
Year: 2024

description: В статье рассматривается влияние свободных экономических зон (СЭЗ) на региональный экономический рост на примере Навоийской свободной индустриально-экономической зоны (СЭЗ). Анализируется роль СЭЗ в привлечении инвестиций, создании рабочих мест, развитии промышленного производства и улучшении инфраструктуры. Особое внимание уделено экономическим и социальным аспектам, связанным с деятельностью Навоийской СЭЗ.
Hemitrichia serpula Lister 1894
Creators: name: Kluša, Julita
Publisher: name: Zenodo
Year: 2023
Subjects: Biodiversity
Taxonomy
Protozoa
Mycetozoa
Myxomycetes
Trichiales
Trichiaceae
Hemitrichia
Hemitrichia serpula

description: Hemitrichia serpula (Scop.) Rostaf. ex Lister,
režģa gļotsēne
- leg. S.Ruskule, 1984, det. S.Ruskule, 1986; (NMKK), moderately common in suitable, humid habitats on decidous logs, overall distribution uneven.
description: Published as part of Kluša, Julita, 2023, Complete Checklist Of Myxomycetes In Latvia, pp. 127-151 in Acta Biologica Universitatis Daugavpiliensis 23 (2) on pages 127-151, DOI: 10.59893/abud.23(2).002, http://zenodo.org/record/12650118
title: ÐÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾-ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÐµÑÑÐ¾ÑÐ°Ð½Ð° ÑÐ¾ÑÐ»Ð°Ð½Ð´ÑÐºÐ¾Ð¹ ÐºÑÑ Ð½Ð¸ Ð½Ð° 60 Ð¼ÐµÑÑ Ð² Ð¦ÐµÐ½ÑÑÐ°Ð»ÑÐ½Ð¾Ð¼ ÑÐ°Ð¹Ð¾Ð½Ðµ Ð³. Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ð°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°ÐºÑÐ»Ð¸Ð½, 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: ÑÐ¾ÑÐ»Ð°Ð½Ð´ÑÐºÐ°Ñ ÐºÑÑ Ð½Ñ
Ð¼ÐµÐ½Ñ
ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ°ÑÑÐµÑÑ
ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»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 Â«ÐÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾-ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÐµÑÑÐ¾ÑÐ°Ð½Ð° ÑÐ¾ÑÐ»Ð°Ð½Ð´ÑÐºÐ¾Ð¹ ÐºÑÑÐ½Ð¸ Ð½Ð° 60 Ð¿Ð¾ÑÐ°Ð´Ð¾ÑÐ½ÑÑ Ð¼ÐµÑÑ, ÐºÐ¾ÑÐ¾ÑÑÐ¹ ÑÐ°ÑÐ¿Ð¾Ð»Ð¾Ð¶ÐµÐ½ Ð² Ð¦ÐµÐ½ÑÑÐ°Ð»ÑÐ½Ð¾Ð¼ ÑÐ°Ð¹Ð¾Ð½Ðµ Ð³Ð¾ÑÐ¾Ð´Ð° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Â», 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¸.
Centaurus A at Hard X-rays and Soft Gamma-rays
Creators: name: Steinle, H.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Centaurus A, at a distance of less than 4 Mpc, is the nearest radio-loud AGN. Its emission is detected from radio to very-high energy gamma-rays. Despite the fact that Cen A is one of the best studied extragalactic objects the origin of its hard X-ray and soft gamma-ray emission (100 keV < E < 50 MeV) is still uncertain. Observations with high spatial resolution in the adjacent soft X-ray and hard gamma-ray regimes suggest that several distinct components such as a Seyfert-like nucleus, relativistic jets, and even luminous X-ray binaries within Cen A may contribute to the total emission in the MeV regime that has been detected with low spatial resolution. As the Spectral Energy Distribution of Cen A has its second maximum around 1 MeV, this energy range plays an important role in modeling the emission of (this) AGN. As there will be no satellite mission in the near future that will cover this energies with higher spatial resolution and better sensitivity, an overview of all existing hard X-ray and soft gamma-ray measurements of Cen A is presented here defining the present knowledge on Centaurus A in the MeV energy range.
description: 8 pages, 5 figures, article for conference proceedings "The Many Faces of Centaurus A"; accepted for publication in PASA
title: Ð­Ð»ÐµÐºÑÑÐ¾Ð¿ÑÐ¸Ð²Ð¾Ð´ Ð¿ÐµÑÐµÐ¼ÐµÑÐµÐ½Ð¸Ñ Ð´ÐµÐºÐ¾Ñ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ÐµÑÐ¸Ðº, ÐÐ³Ð¾Ñ
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ÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¼Ð°ÑÐ¸Ð½Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐµ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»ÑÐ½ÑÐµ
Ð­Ð»ÐµÐºÑÑÐ¾Ð¿ÑÐ¸Ð²Ð¾Ð´Ñ
ÐÐ½ÑÐµÑÑÐµÐ¹ÑÑ
ÐÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»Ð¸ ÑÐ°ÑÑÐ¾ÑÑ
Ð°Ð¿Ð¿Ð»Ð¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¼Ð¾Ð´ÑÐ»Ð¸

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð¿ÑÐ¸Ð²Ð¾Ð´ Ð¸ ÑÐ¸ÑÑÐµÐ¼Ð° ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÐµÐ¼ÐµÑÐµÐ½Ð¸ÐµÐ¼ Ð´ÐµÐºÐ¾ÑÐ°ÑÐ¸Ð¸. ÐÑÐ±ÑÐ°Ð½ Ð¼Ð¾ÑÐ¾Ñ-ÑÐµÐ´ÑÐºÑÐ¾Ñ, ÑÐ¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ñ ÑÐ¸Ð»Ð¾Ð²Ð°Ñ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ°ÑÑÑ Ð¸ Ð°Ð¿Ð¿Ð°ÑÐ°ÑÐ½Ð¾-Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ð° ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ. ÐÐ¿Ð¸ÑÐ°Ð½ Ð²Ð²Ð¾Ð´ Ð² ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ñ Ð¸ Ð½Ð°ÑÑÑÐ¾Ð¹ÐºÐ° Ð¿ÑÐ¸Ð²Ð¾Ð´Ð° Ð¸ Ð°Ð¿Ð¿Ð»Ð¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¼Ð¾Ð´ÑÐ»Ñ Â«Ð¢Ð°Ð±Ð»Ð¸ÑÐ½Ð¾Ðµ Ð¿Ð¾Ð·Ð¸ÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿Ð¾ ÑÐ¸Ð½ÐµÂ». ÐÐ»Ñ ÑÐ´Ð¾Ð±Ð½Ð¾Ð³Ð¾ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÐµÐ»ÐµÐ¼ ÑÐ»ÐµÐºÑÑÐ¾Ð¿ÑÐ¸Ð²Ð¾Ð´Ð¾Ð¼ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð¸Ð½ÑÐµÑÑÐµÐ¹Ñ, ÑÐµÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ð½ÑÐ¹ Ð½Ð° Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¼ ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐµ.
A fall from grace? : examining retired ballet dancers' experiences with body image and embodiment across the life course
Creators: name: Thompson, Regan
Publisher: name: University of British Columbia
Year: 2024

description: According to master choreographer George Balanchine, the ‘ideal ballet body’ for women is to be tall and incredibly slender, with small breasts, small hips, long limbs, and a short torso (Langdon, 2012). Women ballet dancers often experience negative body image and embodiment due to these narrow ideals; yet, how ballet training influences dancers’ relationships to their bodies following ballet retirement remained unexplored. The purpose of this study was to examine i.) how women’s history with ballet training shaped and constrained their body image and embodiment over time and following retirement, and ii.) how women ballet retirees storied their long-term body image and embodied experiences both verbally and artistically. Adopting narrative constructionism (Smith & Sparkes, 2009), I conducted one life history interview and two body mapping sessions with five retired women ballet dancers (15 sessions). Through narrative thematic analysis (Riessman, 2008), I constructed stories for each participant and three overarching themes across these stories. The first theme, Act I, The Battle: Deeply Rooted Ballet Ideals and the Changing Body examined participants’ ongoing body dissatisfaction and negative embodiment due to the lasting internalization of ballet body ideals, particularly amidst navigating the aging process, as many participants redrew their body maps to appear thinner. The second theme, Act II, Waltz of the Snowflakes: Recognition of Positive Ballet Embodiment examined participants’ positive embodiment and body image in terms of aesthetics, functionality, and ballet values (artistically demonstrated by participants’ use of glitter and bright colours on certain areas of their body maps), yet these experiences remained contingent on traditional ballet body ideals. The third theme, Act III, Pas de Deux: Tensions of Traditional and 21st Century Ballet Pedagogy explored participants’ concurrent perpetuations and rejections of traditional ballet values in their teaching practices and views toward the (slowly) evolving ballet world. These findings illustrate how ballet training can impact women’s relationship with their bodies long after dance retirement, can inform future arts-based research in physical cultural and sport psychology studies, and denote the importance of centering pedagogical approaches that support dancers’ positive body image and embodiment both during and following retirement of ballet training in Canada.
Relativistic Brownian Motion
Creators: name: Dunkel, Jörn
name: Hänggi, Peter
Publisher: name: arXiv
Year: 2008
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Astrophysics (astro-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Stimulated by experimental progress in high energy physics and astrophysics, the unification of relativistic and stochastic concepts has re-attracted considerable interest during the past decade. Focusing on the framework of special relativity, we review, here, recent progress in the phenomenological description of relativistic diffusion processes. After a brief historical overview, we will summarize basic concepts from the Langevin theory of nonrelativistic Brownian motions and discuss relevant aspects of relativistic equilibrium thermostatistics. The introductory parts are followed by a detailed discussion of relativistic Langevin equations in phase space. We address the choice of time parameters, discretization rules, relativistic fluctuation-dissipation theorems, and Lorentz transformations of stochastic differential equations. The general theory is illustrated through analytical and numerical results for the diffusion of free relativistic Brownian particles. Subsequently, we discuss how Langevin-type equations can be obtained as approximations to microscopic models. The final part of the article is dedicated to relativistic diffusion processes in Minkowski spacetime. Due to the finiteness of velocities in relativity, nontrivial relativistic Markov processes in spacetime do not exist; i.e., relativistic generalizations of the nonrelativistic diffusion equation and its Gaussian solutions must necessarily be non-Markovian. We compare different proposals that were made in the literature and discuss their respective benefits and drawbacks. The review concludes with a summary of open questions, which may serve as a starting point for future investigations and extensions of the theory.
description: review article, 159 pages, references updated, misprints corrected, App. A.4. corrected
title: Ð¢ÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½Ð¾-Ð¿ÐµÑÐµÐ³ÑÑÐ·Ð¾ÑÐ½Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ð° Ð´Ð»Ñ Ð¾Ð±ÑÐ»ÑÐ¶Ð¸Ð²Ð°Ð½Ð¸Ñ ÑÐ°Ð¼Ð¾Ð»ÐµÑÐ¾Ð² Sukhoi Superjet 100
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ°
titleType: Subtitle
Creators: name: Ð¡ÑÑÐ¾Ð¹, ÐÐ²Ð°Ð½
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÐ°ÑÑÐµÑ Ð¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ
Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ð°
Ð¿Ð¾Ð³ÑÑÐ·ÐºÐ°/ÑÐ°Ð·Ð³ÑÑÐ·ÐºÐ° Ð±Ð°Ð³Ð°Ð¶Ð°
ÐºÐ¾Ð½ÑÐµÐ¹Ð½ÐµÑ
ÐºÐ¾Ð½Ð²ÐµÐ¹ÐµÑ
ÑÐµÐ»ÐµÐ¶ÐºÐ°
Sukhoi Superjet 100

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð° ÑÐ¸ÑÑÐµÐ¼Ð° Ð¿Ð¾Ð³ÑÑÐ·ÐºÐ¸ Ð±Ð°Ð³Ð°Ð¶Ð° Ð¿Ð°ÑÑÐ°Ð¶Ð¸ÑÐ¾Ð² Ð´Ð»Ñ ÑÐ°Ð¼Ð¾Ð»ÐµÑÐ° Sukhoi Superjet 100. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð¼Ð¾Ð´ÐµÐ»Ñ ÐºÐ¾Ð½ÑÐµÐ¹Ð½ÐµÑÐ°, ÑÐµÐ»ÐµÐ¶ÐºÐ¸ Ð´Ð»Ñ Ð¿ÐµÑÐµÐ¼ÐµÑÐµÐ½Ð¸Ñ ÐºÐ¾Ð½ÑÐµÐ¹Ð½ÐµÑÐ¾Ð² Ð¸ ÐºÐ¾Ð½Ð²ÐµÐ¹ÐµÑ. ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ñ Ð¿ÑÐ¾Ð²ÐµÑÐ¾ÑÐ½ÑÐµ ÑÐ°ÑÑÐµÑÑ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹ Ð² ÑÑÐµÐ´Ðµ NX Nastran. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÐºÐ°Ð¿Ð¸ÑÐ°Ð»Ð¾Ð²Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Ð² Ð¿ÑÐ¾ÐµÐºÑ. Ð ÐµÑÐµÐ½Ñ Ð²ÑÐµ Ð²Ð¾Ð¿ÑÐ¾ÑÑ, ÐºÐ°ÑÐ°ÑÑÐ¸ÐµÑÑ ÑÐµÑÐ½Ð¸ÐºÐ¸ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸, Ð¾ÑÑÐ°Ð½Ñ ÑÑÑÐ´Ð°.
Additional file 9 of An ensemble learning approach for modeling the systems biology of drug-induced injury
Creators: name: Aguirre-Plans, Joaquim
name: Piñero, Janet
name: Terezinha Souza
name: Callegaro, Giulia
name: Kunnen, Steven J.
name: Sanz, Ferran
name: Fernandez-Fuentes, Narcis
name: Furlong, Laura I.
name: Guney, Emre
name: Oliva, Baldo
Publisher: name: figshare
Year: 2021
Subjects: subject: Space Science
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Pharmacology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences

description: Additional file 9.
title: Ð­Ð»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐµ Ð¸ ÐºÐ²Ð°Ð½ÑÐ¾Ð²ÑÐµ Ð¿ÑÐ¸Ð±Ð¾ÑÑ Ð¡ÐÐ§
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ðº Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÐ¼ ÑÐ°Ð±Ð¾ÑÐ°Ð¼
titleType: Subtitle
Creators: name: ÐÐ¾ÑÐ½Ð¸Ð»Ð¾Ð², Ð¡ÐµÑÐ³ÐµÐ¹
Publisher: name: ÐÐÐ Ð¸Ð¼ÐµÐ½Ð¸ Ð. Ð. ÐÐ°Ð»Ð¸Ð½Ð¸Ð½Ð°
Year: 1977
Subjects: Ð¡Ð²ÐµÑÑ Ð²ÑÑÐ¾ÐºÐ¸Ðµ ÑÐ°ÑÑÐ¾ÑÑ

description: ÐÐ°Ð½Ð½Ð¾Ðµ ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ²Ð»ÑÐµÑÑÑ Ð¿ÑÐ¾Ð´Ð¾Ð»Ð¶ÐµÐ½Ð¸ÐµÐ¼ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ, Ð²ÑÐ¿ÑÑÐµÐ½Ð½Ð¾Ð³Ð¾ Ð² 1975 Ð³. Ð¦ÐµÐ»Ñ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ - ÑÐ¸ÑÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ð¾Ð² Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð¸ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸Ðº ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÑ Ð¿ÑÐ¸Ð±Ð¾ÑÐ¾Ð², Ñ ÐºÐ¾ÑÐ¾ÑÑÐ¼Ð¸ ÑÑÑÐ´ÐµÐ½ÑÑ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹ 0701 Ð¸ 0704 Ð·Ð½Ð°ÐºÐ¾Ð¼ÑÑÑÑ Ð² ÑÑÐµÐ±Ð½Ð¾Ð¹ Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ¸Ð¸ Ð¿Ð¾ ÐºÑÑÑÑ Â«Ð­Ð»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐµ Ð¸ ÐºÐ²Ð°Ð½ÑÐ¾Ð²ÑÐµ Ð¿ÑÐ¸Ð±Ð¾ÑÑ Ð¡ÐÐ§Â». Ð Ð°ÑÐ¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ Ð¸ ÑÐ°ÑÐ°ÐºÑÐµÑ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð° ÑÐ¾Ð³Ð»Ð°ÑÐ¾Ð²Ð°Ð½Ñ Ñ ÐºÑÑÑÐ¾Ð¼ Ð»ÐµÐºÑÐ¸Ð¹ Ð¸ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑÑ ÑÐ²ÐµÐ»Ð¸ÑÐ¸ÑÑ Ð¾Ð±ÑÐµÐ¼ ÑÐ°Ð·Ð´ÐµÐ»Ð¾Ð², Ð²ÑÐ´ÐµÐ»ÑÐµÐ¼ÑÑ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ Ð´Ð»Ñ ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ. Ð Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð¿Ð¾Ð¼ÐµÑÐµÐ½Ñ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÑ ÑÐ°Ð±Ð¾Ñ Ð¿Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð»Ð°Ð¼Ð¿Ñ Ð±ÐµÐ³ÑÑÐµÐ¹ Ð²Ð¾Ð»Ð½Ñ (Ð°Ð²ÑÐ¾Ñ - Ð´Ð¾Ñ., Ðº. Ñ. Ð½. ÐÑÐ»Ð°ÐºÐ¾Ð² Ð. Ð.), Ð»Ð°Ð¼Ð¿Ñ Ð¾Ð±ÑÐ°ÑÐ½Ð¾Ð¹ Ð²Ð¾Ð»Ð½Ñ (Ð°Ð²ÑÐ¾Ñ - Ð¿ÑÐ¾Ñ., Ð´. Ñ. Ð¸. ÐÐ¾ÑÐ½Ð¸Ð»Ð¾Ð² Ð¡. Ð.) Ð¸ Ð¼Ð½Ð¾Ð³Ð¾ÑÐµÐ·Ð¾Ð½Ð°ÑÐ¾ÑÐ½Ð¾Ð³Ð¾ Ð¼Ð°Ð³Ð½ÐµÑÑÐ¾Ð½Ð° (Ð°Ð²ÑÐ¾Ñ - Ð´Ð¾Ñ., Ðº. Ñ. Ð½. ÐÐ¾ÑÐ¾Ð»ÐµÐ² Ð®. Ð¡.).
Rank-Sparsity Incoherence for Matrix Decomposition
Creators: name: Chandrasekaran, Venkat
name: Sanghavi, Sujay
name: Parrilo, Pablo A.
name: Willsky, Alan S.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Optimization and Control (math.OC)
subject: Statistics Theory (math.ST)
subject: FOS: Mathematics

description: Suppose we are given a matrix that is formed by adding an unknown sparse matrix to an unknown low-rank matrix. Our goal is to decompose the given matrix into its sparse and low-rank components. Such a problem arises in a number of applications in model and system identification, and is NP-hard in general. In this paper we consider a convex optimization formulation to splitting the specified matrix into its components, by minimizing a linear combination of the $\ell_1$ norm and the nuclear norm of the components. We develop a notion of \emph{rank-sparsity incoherence}, expressed as an uncertainty principle between the sparsity pattern of a matrix and its row and column spaces, and use it to characterize both fundamental identifiability as well as (deterministic) sufficient conditions for exact recovery. Our analysis is geometric in nature, with the tangent spaces to the algebraic varieties of sparse and low-rank matrices playing a prominent role. When the sparse and low-rank matrices are drawn from certain natural random ensembles, we show that the sufficient conditions for exact recovery are satisfied with high probability. We conclude with simulation results on synthetic matrix decomposition problems.
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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£ÑÐºÐ¸Ð½, ÐÐ½Ð°ÑÐ¾Ð»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: 2018
Subjects: IT-ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸
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description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ð° ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ðµ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÑÐ°Ð»Ð°, Ñ ÑÑÐ½ÐºÑÐ¸ÐµÐ¹ Ð¾Ð¿Ð¾Ð²ÐµÑÐµÐ½Ð¸Ñ Ð¾Ð± Ð°Ð²Ð°ÑÐ¸ÑÑ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¾ÑÐºÑÑÑÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Apache, Java, Spring Ð¸ PostgreSQL. ÐÐ°Ð½Ñ Ð¾Ð±ÑÐ¸Ðµ Ð¿Ð¾Ð½ÑÑÐ¸Ñ Ð¸ ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ IT-ÑÐ¸ÑÑÐµÐ¼ ÑÐ°ÐºÐ¾Ð³Ð¾ ÐºÐ»Ð°ÑÑÐ°. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð°Ð½Ð°Ð»Ð¾Ð³Ð¸ÑÐ½ÑÑ ÑÐ¸ÑÑÐµÐ¼. ÐÐ·ÑÑÐµÐ½Ð° ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ ÑÐºÐ°Ð·Ð°Ð½Ð½Ð¾Ð³Ð¾ ÐºÐ»Ð°ÑÑÐ° Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÐºÐ¾Ð½ÐºÑÐµÑÐ½Ð°Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð°Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÑÐ°Ð»Ð°.
Multistability and localization in coupled nonlinear split-ring resonators
Creators: name: Lazarides, Nikos
name: Molina, Mario I.
name: Tsironis, George P.
name: Kivshar, Yuri S.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We study the dynamics of a pair of nonlinear split-ring resonators (a `metadimer') excited by an alternating magnetic field and coupled magnetically. Linear metadimers of this kind have been recently used as the elementary components for three-dimensional metamaterials or 'stereometamaterials' [N. Liu {\em et al}, Nature Photon. {\bf 3}, 157 (2009)]. We demonstrate that nonlinearity offers more possibilities with respect to real-time tunability and a multiplicity of states which can be reached by varying the external field. Moreover, we demonstrate almost total localization of the energy in one of the resonators in a broad range of parameters.
description: 3 pages, 5 figures
Aberrasine aberrans subsp. aberrans
Creators: name: Koshkin, Evgeny S.
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Erebidae
Aberrasine
Aberrasine aberrans
Aberrasine aberrans aberrans (butler, 1877)

description: Aberrasine aberrans aberrans (Butler, 1877)
(Figs 1E–H, 2B, C, 3B, C)
Miltochrista aberrans Butler, 1877: 397. Type locality: Japan: Yokohama.
Material. 1 ♂, Vietnam, Vinh Phuc Province, Tam Dao, 21°27’24” N, 105°38’23” E, 900 m, 4.IV.2024, leg. Evgeny S. Koshkin (EKC); 1 ♀, with the same data as for the male, but 2.IV.2024.
Remarks. This is the first record of this species for Vietnam and the Indochina peninsula. However, Aberrasine aberrans is widespread throughout East Asia, reaching as far south as Guangdong Province and the Guangxi Zhuang Autonomous Region (China), which border Vietnam.
Specimens from northern Vietnam have a well-defined, slightly curved dark medial line on the forewings (Figs 1E, F), as do many specimens from Southern and Eastern China (Fang 2000; Dubatolov et al. 2012b; Wu & Kishida 2020). In many specimens from the northern part of the species range this line is not pronounced, it is either absent or yellow (Figs 1G, H). The genitalia of male and female Aberrasine aberrans from Vietnam do not differ significantly from more northern specimens (Figs 2B, C, 3B, C).
Following is an updated list of valid taxa in the genus Aberrasine based on the works by Volynkin & Huang (2019), Volynkin (2020), and Singh et al. (2021), taking into account recently described taxa, and newly clarified data on species distributions.
description: Published as part of Koshkin, Evgeny S., 2025, New contribution to the knowledge of the genus Aberrasine Volynkin & Huang, 2019 (Lepidoptera, Erebidae, Arctiinae, Lithosiini) of Vietnam, with description of a new species, pp. 565-574 in Zootaxa 5604 (4) on pages 569-570, DOI: 10.11646/zootaxa.5604.4.8, http://zenodo.org/record/15214199
title: ÐÐ¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð±ÐµÑÐµÐ¶Ð»Ð¸Ð²Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°
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Ð²ÐµÐ·Ð´ÐºÐ¸Ð½Ð°, ÐÑÐµÐ½Ð¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÐ¸ÑÑÐµÐ¼Ð° Ð±ÐµÑÐµÐ¶Ð»Ð¸Ð²Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°
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Photoproduction of J/psi and of high mass e+e- in ultra-peripheral Au+Au collisions at sqrt(s_NN) = 200 GeV
Creators: name: PHENIX Collaboration
name: Afanasiev, A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: We present the first measurement of photoproduction of J/psi and of two-photon production of high-mass e+e- pairs in electromagnetic (or ultra-peripheral) nucleus-nucleus interactions, using Au+Au data at sqrt(s_NN) = 200 GeV. The events are tagged with forward neutrons emitted following Coulomb excitation of one or both Au^{star} nuclei. The event sample consists of 28 events with m_{e+e-} > 2 GeV/c^2 with zero like-sign background. The measured cross sections at midrapidity of dσ/ dy (J/psi + Xn, y=0) = 76 +/- 33 (stat) +/- 11 (syst) micro b and d^2σ/dm dy (e^+e^- + Xn, y=0) = 86 +/- 23 (stat) +/- 16 (syst) micro b/(GeV/c^2) for m_{e+e-} \in [2.0,2.8] GeV/c^2 are consistent with various theoretical predictions.
description: 345 authors from 52 institutions, 20 pages, 4 figures, 3 tables. Submitted to Physics Letters B. Plain text data tables for the points plotted in figures for this and previous PHENIX publications are (or will be) publicly available at http://www.phenix.bnl.gov/papers.html
title: Social media as a political instrument in Russia
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÑÐ¹ÑÐµÐ¼Ð±Ð¸Ð½Ð°, 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Ð½ÑÐµÑÐ½ÐµÑ
Ð¿Ð¾Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ°Ñ Ð½Ð°ÑÐºÐ°
ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð°Ñ Ð°ÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ

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Tests of Gravity from Imaging and Spectroscopic Surveys
Creators: name: Guzik, Jacek
name: Jain, Bhuvnesh
name: Takada, Masahiro
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Tests of gravity on large-scales in the universe can be made using both imaging and spectroscopic surveys. The former allow for measurements of weak lensing, galaxy clustering and cross-correlations such as the ISW effect. The latter probe galaxy dynamics through redshift space distortions. We use a set of basic observables, namely lensing power spectra, galaxy-lensing and galaxy-velocity cross-spectra in multiple redshift bins (including their covariances), to estimate the ability of upcoming surveys to test gravity theories. We use a two-parameter description of gravity that allows for the Poisson equation and the ratio of metric potentials to depart from general relativity. We find that the combination of imaging and spectroscopic observables is essential in making robust tests of gravity theories. The range of scales and redshifts best probed by upcoming surveys is discussed. We also compare our parametrization to others used in the literature, in particular the gamma parameter modification of the growth factor.
description: 18 pages, 10 figures, to be submitted