cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Searches for leptoquark production and compositeness at the Tevatron
Creators: name: Nunnemann, Thomas
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: Recent searches for leptoquark production and compositeness in p-anti-p collisions at sqrt{s}=1.96 TeV are presented using data samples with integrated luminosities up to 4 fb^{-1} recorded with the D0 and CDF detectors at the Tevatron collider.
description: Invited talk at European Physical Society Europhysics Conference on High Energy Physics, EPS-HEP 2009, Krakow, Poland
title: ÐÑÐ¾ÑÐµÑÑÐ¸Ð¸ Ð±ÑÐ´ÑÑÐµÐ³Ð¾ Ð¸ ÐºÐ¾Ð¼Ð¿ÐµÑÐµÐ½ÑÐ¸Ð¸ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð² Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÐºÐ°ÑÐµÑÑÐ²Ð¾Ð¼
Creators: name: ÐÐ¾Ð»Ð¶ÐµÐ½ÐºÐ¾Ð²Ð°, ÐÐ»ÐµÐºÑÐ°Ð½Ð´ÑÐ°
name: "Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÐºÐ°ÑÐµÑÑÐ²Ð¾Ð¼ Ð² Ð¸Ð½ÑÐµÑÐµÑÐ°Ñ  ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾Ð³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ", Ð¼ÐµÐ¶Ð²ÑÐ·Ð¾Ð²ÑÐºÐ°Ñ Ð½Ð°ÑÑÐ½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (2019; 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: 2019

description: Ð ÑÑÐ°ÑÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ ÐºÐ¾Ð¼Ð¿ÐµÑÐµÐ½ÑÐ¸Ð¸, Ð½Ð°Ð²ÑÐºÐ¸ Ð¸ ÑÐ¼ÐµÐ½Ð¸Ñ, ÐºÐ¾ÑÐ¾ÑÑÐ¼Ð¸ Ð´Ð¾Ð»Ð¶Ð½Ñ Ð²Ð»Ð°Ð´ÐµÑÑ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÑ, Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÐºÐ¾ÑÐ¾ÑÑÑ Ð½Ð°Ð¿ÑÑÐ¼ÑÑ ÑÐ²ÑÐ·Ð°Ð½Ð° Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÐµÐ¼ ÐºÐ°ÑÐµÑÑÐ²Ð¾Ð¼. Ð¢Ð°ÐºÐ¶Ðµ Ð¿ÑÐµÐ´Ð»Ð°Ð³Ð°ÑÑÑÑ Ðº Ð¾Ð±ÑÑÐ¶Ð´ÐµÐ½Ð¸Ñ Ð½Ð¾Ð²ÑÐµ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¸ â Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¸ Ð±ÑÐ´ÑÑÐµÐ³Ð¾, Ð¸Ñ Ð¼ÐµÑÑÐ¾ Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸. ÐÑÐ´ÑÑÐµÐµ Ð¼ÐµÑÑÐ¾ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð² Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÐºÐ°ÑÐµÑÑÐ²Ð¾Ð¼ Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÑÐµÑÑÑ Ð¿Ð¾Ð´ Ð¿ÑÐ¸Ð·Ð¼Ð¾Ð¹ Ð½Ð¾Ð²ÑÑ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¹, Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÐµÑÑÑ ÑÐ¾Ð»Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÐºÐ°ÑÐµÑÑÐ²Ð¾Ð¼ Ð½Ð° ÑÑÐ½ÐºÐµ ÑÑÑÐ´Ð°. Ð ÐºÐ°ÑÐµÑÑÐ²Ðµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð²Ð°ÐºÐ°Ð½ÑÐ¸Ð¹, ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÑ Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÐµÐ¼ ÐºÐ°ÑÐµÑÑÐ²Ð¾Ð¼ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð° ÑÐ²Ð¾Ð´Ð½Ð°Ñ ÑÐ°Ð±Ð»Ð¸ÑÐ°, Ð¾ÑÑÐ°Ð¶Ð°ÑÑÐ°Ñ ÐºÐ»ÑÑÐµÐ²ÑÐµ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð² Ð² Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸.
Additional file 1 of Does curve magnitude in adolescent idiopathic scoliosis (AIS) affect frequency and quality of sport participation? A feasibility study
Creators: name: Youssef, Michael
name: Soliman, John
name: Burrow, Sarah
name: Kishta, Waleed
name: Simunovic, Nicole
name: Duong, Andrew
name: Olufemi R. Ayeni
name: Peterson, Devin
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 1: Questionnaires (Appendix 1).
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)
Miltochrista aberrans Butler, 1877: 397 (Type locality: «Yokohama»).
Distribution: Far East of Russia (southern Amur Oblast’, Jewish Autonomous Oblast’, southern Khabarovsk Krai, Primorsky Krai and Kunashir Island), Korea, China (Heilongjiang, Jilin, Shaanxi, Henan, Jiangsu, Zhejiang, Jiangxi, Fujian, Hubei, Hunan, Sichuan, Guangdong and Hainan Provinces, Guangxi Zhuang Autonomous Region, Beijing), Northern Vietnam (present study), Japan (Hokkaido, Honshu, Shikoku, Kyushu, Yakushima Islands) (Fang 2000; Dubatolov et al. 2012a, 2012b; Kishida 2011; Wu & Kishida, 2020; Spitsyna & Spitsyn, 2023).
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 page 571, DOI: 10.11646/zootaxa.5604.4.8, http://zenodo.org/record/15214199
Measurement of the Slope Parameter $α$ for the $η\to 3π^0$ decay with the Crystal Ball detector at the Mainz Microtron (MAMI-C)
Creators: name: Prakhov, S.
name: Nefkens, B. M. K.
name: Aguar-Bartolome, P.
name: Akasoy, L. K.
name: Annand, J. R. M.
name: Arends, H. J.
name: Bantawa, K.
name: Beck, R.
name: Bekrenev, V.
name: Berghauser, H.
name: Boillat, B.
name: Braghieri, A.
name: Branford, D.
name: Briscoe, W. J.
name: Brudvik, J.
name: Cherepnya, S.
name: Codling, R. F. B.
name: Downie, E. J.
name: Drexler, P.
name: Fil'kov, L. V.
name: Glazier, D. I.
name: Gregor, R.
name: Heid, E.
name: Hornidge, D.
name: Jahn, O.
name: Jude, T. C.
name: Kashevarov, V. L.
name: Kellie, J. D.
name: Kondratiev, R.
name: Korolija, M.
name: Kotulla, M.
name: Koulbardis, A.
name: Krambrich, D.
name: Kruglov, S.
name: Krusche, B.
name: Lang, M.
name: Lisin, V.
name: Livingston, K.
name: MacGregor, I. J. D.
name: Maghrbi, Y.
name: Manley, D. M.
name: Martinez, M.
name: McGeorge, J. C.
name: McNicoll, E. F.
name: Mekterovic, D.
name: Metag, V.
name: Micanovic, S.
name: Nikolaev, A.
name: Novotny, R.
name: Ostrick, M.
name: Otte, P. B.
name: Pedroni, P.
name: Pheron, F.
name: Polonski, A.
name: Robinson, J.
name: Rosner, G.
name: Rost, M.
name: Rostomyan, T.
name: Schumann, S.
name: Sikora, M. H.
name: Sober, D. I.
name: Starostin, A.
name: Suarez, I. M.
name: Supek, I.
name: Tarbert, C. M.
name: Thiel, M.
name: Thomas, A.
name: Unverzagt, M.
name: Watts, D. P.
name: Zamboni, I.
name: Zehr, F.
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The dynamics of the $η\to 3π^0$ decay have been studied with the Crystal Ball multiphoton spectrometer and the TAPS calorimeter. Bremsstrahlung photons produced by the 1.5-GeV electron beam of the Mainz microtron MAMI-C and tagged by the Glasgow photon spectrometer were used for $η$-meson production. The analysis of $3 \times 10^6$ $γp \to ηp \to 3π^0 p \to 6γp$ events yields the value $α=-0.032\pm0.003$ for the $η\to 3π^0$ slope parameter, which agrees with the majority of recent experimental results and has the smallest uncertainty. The $π^0π^0$ invariant-mass spectrum was investigated for the occurrence of a cusplike structure in the vicinity of the $π^+π^-$ threshold. The observed effect is small and does not affect our measured value for the slope parameter.
title: ÐÑÐ³Ð¾Ð³Ð°ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ðµ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾ Ð°Ð²ÑÐ¾ÐºÐ¾Ð¼Ð¿ÑÐµÑÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ ÑÐ»ÐµÐ³Ð°Ð·Ð¾Ð²Ð¾Ð³Ð¾ Ð²ÑÐºÐ»ÑÑÐ°ÑÐµÐ»Ñ 110 ÐºÐ, 50 ÐºÐ
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Ð¾Ð²ÑÐºÐ¸Ð¹, Ð Ð¾Ð¼Ð°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ÑÐºÐ»ÑÑÐ°ÑÐµÐ»Ð¸ Ð²ÑÑÐ¾ÐºÐ¾Ð³Ð¾ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ
ÐÐ°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ

description: ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸Ð¼ÑÑ Ð² Ð½Ð°ÑÑÐ¾ÑÑÐµÐµ Ð²ÑÐµÐ¼Ñ ÑÐ»ÐµÐ³Ð°Ð·Ð¾Ð²ÑÑ Ð²ÑÐºÐ»ÑÑÐ°ÑÐµÐ»ÐµÐ¹ Ñ Ð°Ð²ÑÐ¾ÐºÐ¾Ð¼Ð¿ÑÐµÑÑÐ¸Ð¾Ð½Ð½ÑÐ¼ Ð´ÑÐ³Ð¾Ð³Ð°ÑÐ¸ÑÐµÐ»ÑÐ½ÑÐ¼ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾Ð¼. ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð¿ÑÐµÐ´ÑÑÐ²Ð»ÑÐµÐ¼ÑÐµ Ðº Ð²ÑÑÐ¾ÐºÐ¾Ð²Ð¾Ð»ÑÑÐ½ÑÐ¼ Ð²ÑÐºÐ»ÑÑÐ°ÑÐµÐ»ÑÐ¼ Ð¿ÑÐ¸ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ð¸ Ð²ÑÐºÐ»ÑÑÐ°ÑÐµÐ»Ñ Ñ ÑÐµÑÑÑ. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð¾ ÑÐ¸ÑÐ»ÐµÐ½Ð½Ð¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð², Ð¿ÑÐ¾ÑÐµÐºÐ°ÑÑÐ¸Ñ Ð² Ð°Ð²ÑÐ¾ÐºÐ¾Ð¼Ð¿ÑÐµÑÑÐ¸Ð¾Ð½Ð½Ð¾Ð¼ Ð´ÑÐ³Ð¾Ð³Ð°ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ð¼ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ðµ Ð¸ ÐµÐ³Ð¾ Ð¾ÑÐºÐ»ÑÑÐ°ÑÑÐµÐ¹ ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸.
An iterative approach for generating statistically realistic populations of households
Creators: name: Gargiulo, Floriana
name: Ternes, Sonia
name: Huet, Sylvie
name: Deffuant, Guillaume
Publisher: name: arXiv
Year: 2009
Subjects: subject: Multiagent Systems (cs.MA)
subject: Computers and Society (cs.CY)
subject: FOS: Computer and information sciences

description: Background: Many different simulation frameworks, in different topics, need to treat realistic datasets to initialize and calibrate the system. A precise reproduction of initial states is extremely important to obtain reliable forecast from the model. Methodology/Principal Findings: This paper proposes an algorithm to create an artificial population where individuals are described by their age, and are gathered in households respecting a variety of statistical constraints (distribution of household types, sizes, age of household head, difference of age between partners and among parents and children). Such a population is often the initial state of microsimulation or (agent) individual-based models. To get a realistic distribution of households is often very important, because this distribution has an impact on the demographic evolution. Usual techniques from microsimulation approach cross different sources of aggregated data for generating individuals. In our case the number of combinations of different households (types, sizes, age of participants) makes it computationally difficult to use directly such methods. Hence we developed a specific algorithm to make the problem more easily tractable. Conclusions/Significance: We generate the populations of two pilot municipalities in Auvergne region (France), to illustrate the approach. The generated populations show a good agreement with the available statistical datasets (not used for the generation) and are obtained in a reasonable computational time.
description: 16 oages, 11 figures
Luminosities of cool stars
Creators: name: Cifuentes, Carlos
name: Caballero, José Antonio
name: Cortés-Contreras, Miriam
name: Montes, David
name: CARMENES Consortium
Publisher: name: Zenodo
Year: 2021
Subjects: cool stars
fundamental parameters

description: Planetary sizes and bulk compositions rely fundamentally on the stellar masses and radii. For the vast majority of stars, these parameters cannot be directly measured and must be inferred from temperature and luminosity. Therefore, reliable stellar luminosities are essential for a proper characterisation of the planetary companions. Once the flux of a star in multiple passbands (from UV to mid-IR) is known, one can produce a low-resolution spectrum or spectral energy distribution (SED) and derive empirically the bolometric luminosity from it. We did this in Cifuentes et al. (2020) on almost 2500 cool stars. We determined the average values of very important astrophysical parameters, including colours, absolute magnitudes, luminosities, temperatures, masses and radii.
title: Ð¡ÑÑÐ°ÑÐµÐ³Ð¸Ñ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»Ñ Ð½Ð° ÑÐ¾Ð»Ð½ÐµÑÐ½ÑÑ Ð±Ð°ÑÐ°ÑÐµÑÑ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¯Ð³Ð°Ð½Ð¾Ð², ÐÐ»ÐµÐºÑÐµÐ¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð¾Ð±Ð·Ð¾Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»Ñ Ð½Ð° ÑÐ¾Ð»Ð½ÐµÑÐ½ÑÑ Ð±Ð°ÑÐ°ÑÐµÑÑ
Ð²Ð½ÐµÑÐ½Ð¸Ð¹ Ð²Ð¸Ð´ Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»Ñ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ ÑÐ¸Ð¿Ð°
ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»Ñ
Ð¼Ð¾Ð´ÐµÐ»Ñ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ ÑÐ½ÐµÑÐ³Ð¸Ð¸
Ð¼Ð¾Ð´ÐµÐ»Ñ ÑÐ°ÑÑ Ð¾Ð´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ½ÐµÑÐ³Ð¸Ð¸

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð¾Ð±Ð·Ð¾Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»Ñ Ð½Ð° ÑÐ¾Ð»Ð½ÐµÑÐ½ÑÑ Ð±Ð°ÑÐ°ÑÐµÑÑ. ÐÑÐ» ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½ Ð²Ð½ÐµÑÐ½Ð¸Ð¹ Ð²Ð¸Ð´ Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»Ñ Ð¸ ÐµÐ³Ð¾ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸. ÐÑÐ»Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¼Ð¾Ð´ÐµÐ»Ñ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»Ñ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ ÑÐ¸Ð¿Ð°, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ ÐºÑÐ¸ÑÐµÑÐ¸Ð¹ ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÐ¸. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿Ð°ÐºÐµÑÐ° Ð¿ÑÐ¸ÐºÐ»Ð°Ð´Ð½ÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼ Ð´Ð»Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð·Ð°Ð´Ð°Ñ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ñ Ð²ÑÑÐ¸ÑÐ»ÐµÐ½Ð¸Ð¹ Â«MATLABÂ». Ð¡ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð²ÑÐ±ÑÐ°Ð½Ð½Ð¾Ð³Ð¾ ÑÑÐµÐ´ÑÑÐ²Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð±ÑÐ»Ð° ÑÐ¾Ð·Ð´Ð°Ð½Ð° Ð¼Ð¾Ð´ÐµÐ»Ñ Ð´Ð»Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸. Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ»Ð¾ ÑÐ¾Ð·Ð´Ð°Ð½Ð¾ GUI Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ Ð´Ð»Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¼Ð¾Ð´ÐµÐ»ÑÑ Ð¿ÑÐ¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ Ð¸ Ð´Ð»Ñ Ð¼Ð¾Ð½Ð¸ÑÐ¾ÑÐ¸Ð½Ð³Ð° ÑÐ¶Ðµ Ð³Ð¾ÑÐ¾Ð²Ð¾Ð¹ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸.
Additional file 1 of A volunteer-supported walking programme to improve physical function in older people (the POWER Study): study protocol for a randomised controlled trial
Creators: name: Grede, Nina
name: Rieckert, Anja
name: Muth, Julia
name: Steinbuck, Joana
name: Weissbach, Sabine
name: Schneider, Annika
name: Weber-Schicker, Beate
name: Freiberger, Ellen
name: Jegan, Nikita
name: Donner-Banzhoff, Norbert
name: Sönnichsen, Andreas
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 1. TIDieR Checklist.
D2.1: Modelling Requirements for System's and Interface Specifications
Creators: name: VECTOR
name: KIT
name: UOP
name: QUB
Publisher: name: XANDAR consortium
Year: 2021

description: This deliverable describes the results of Task T2.1 Requirements for Models, Interfaces & Tools, which derives and specifies the requirements that are necessary to accurately model the non-functional constraints, the safety/security concepts and the system function, network, hardware, and software architecture.

Based on the results of Task T1.1 – Pilot Trials Specifications & Assessment Protocol, which targets analysis and specification of functional and non-functional requirements for the industrial validators, it, at first, introduces the XANDAR development process in Chapter 2. This process shows the general approach of XANDAR and defines the interaction of data, models, and tools. In Chapter 3, the document specifies the essential requirements to accurately model a system's architecture, constraints, and the interfaces to other tools. These requirements represent the result of the further chapters and, thus, the main contribution of the task.

Starting with Chapter 4, the status quo is described. This starts off with an introduction of existing modelling tools that are an essential part of the XANDAR process. Chapter 5 continues with a presentation of existing data models e.g., EAST-ADL, AMALTHEA, to highlight their possible usage to fulfil the previous modelling requirements. Finally, in Chapter 6, the data flow of the XANDAR process is described by presenting the existing interfaces of the aforementioned modelling tools.

With the description of the status quo and a list of requirements, which are directly derived from the work on the demonstrator, a clear view of the existing deficits and, consequently, of the next steps to achieve a X-by-Construction Design framework for Engineering Autonomous & Distributed Real-time Embedded Software Systems is given.
Lamproderma arcyrioides Rostaf.
Creators: name: Kluša, Julita
Publisher: name: Zenodo
Year: 2023
Subjects: Biodiversity
Taxonomy
Protozoa
Mycetozoa
Myxomycetes
Stemonitidales
Stemonitidaceae
Lamproderma
Lamproderma arcyrioides

description: ● Lamproderma arcyrioides (Sommerf.) Rostaf.,
tīklotā lampīte
- leg. M.ŠlapakovaPjankova, 27 Apr 2023, Ozolaine p., on a small deciduous branch in litter in old humid deciduous forest near melting snow, det. J. Kluša, 2023; (NMKK), one locality.
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
The Relation Between Compact, Quiescent High Redshift Galaxies and Massive Nearby Elliptical Galaxies: Evidence for Hierarchical, Inside-Out Growth
Creators: name: Bezanson, Rachel
name: van Dokkum, Pieter G.
name: Tal, Tomer
name: Marchesini, Danilo
name: Kriek, Mariska
name: Franx, Marijn
name: Coppi, Paolo
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Recent studies have shown that massive quiescent galaxies at high redshift are much more compact than present-day galaxies of the same mass. Here we compare the radial stellar density profiles and the number density of a sample of massive galaxies at z ~ 2.3 to nearby massive elliptical galaxies. We confirm that the average stellar densities of the z ~ 2.3 galaxies within the effective radius, rho(
description: 9 pages, 4 figures, accepted for publication in the Astrophysical Journal
title: ÐÑÐ°Ð²Ð¾Ð²ÑÐµ Ð¾ÑÐ½Ð¾Ð²Ñ Ð±ÑÐ´Ð¶ÐµÑÐ½Ð¾Ð³Ð¾ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ Ð² Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸ Ð¸ Ð² Ð¤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Ð¾ÑÐ¾ÑÐ¸Ð½, 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: Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ°Ñ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ñ
Ð±ÑÐ´Ð¶ÐµÑÐ½ÑÐ¹ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ
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description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼ Ð±ÑÐ´Ð¶ÐµÑÐ½Ð¾Ð³Ð¾ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ Ð¸ Ð¸Ñ Ð¿ÑÐ°Ð²Ð¾Ð²ÑÑ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð² Ð½Ð° ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸ ÑÐ°ÐºÐ¸Ñ ÑÑÑÐ°Ð½, ÐºÐ°Ðº Ð¤Ð Ð Ð¸ Ð Ð¤. Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° ÑÑÑÑÐºÑÑÑÐ° Ð±ÑÐ´Ð¶ÐµÑÐ½Ð¾Ð³Ð¾ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ ÐºÐ°Ðº Ð½Ð° ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸ Ð Ð¤, ÑÐ°Ðº Ð¸ Ð½Ð° ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸ Ð¤Ð Ð. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° Ð¸ÑÑÐ¾ÑÐ¸Ñ Ð²Ð¾Ð·Ð½Ð¸ÐºÐ½Ð¾Ð²ÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ Ð±ÑÐ´Ð¶ÐµÑÐ½Ð¾Ð³Ð¾ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ Ð½Ð° ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸ ÑÑÐ¸Ñ ÑÑÑÐ°Ð½, Ð¸ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ, Ñ ÐºÐ¾ÑÐ¾ÑÑÐ¼Ð¸ Ð¾Ð±Ðµ ÑÑÑÐ°Ð½Ñ ÑÑÐ¾Ð»ÐºÐ½ÑÐ»Ð¸ÑÑ. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð±ÑÐ»Ð¸ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¸ Ð±ÑÐ´Ð¶ÐµÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ°Ð²Ð°, Ð´ÐµÐ¹ÑÑÐ²ÑÑÑÐ¸Ðµ Ð½Ð° ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸ Ð¤Ð Ð Ð¸ Ð Ð¤.
Automatic unsupervised classification of all SDSS/DR7 galaxy spectra
Creators: name: Almeida, J. Sanchez
name: Aguerri, J. A. L.
name: Munoz-Tunon, C.
name: de Vicente, A.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Using the 'k-means' cluster analysis algorithm, we carry out an unsupervised classification of all galaxy spectra in the seventh and final Sloan Digital Sky Survey data release (SDSS/DR7). Except for the shift to restframe wavelengths, and the normalization to the g-band flux, no manipulation is applied to the original spectra. The algorithm guarantees that galaxies with similar spectra belong to the same class. We find that 99 % of the galaxies can be assigned to only 17 major classes, with 11 additional minor classes including the remaining 1%. The classification is not unique since many galaxies appear in between classes, however, our rendering of the algorithm overcomes this weakness with a tool to identify borderline galaxies. Each class is characterized by a template spectrum, which is the average of all the spectra of the galaxies in the class. These low noise template spectra vary smoothly and continuously along a sequence labeled from 0 to 27, from the reddest class to the bluest class. Our Automatic Spectroscopic K-means-based (ASK) classification separates galaxies in colors, with classes characteristic of the red sequence, the blue cloud, as well as the green valley. When red sequence galaxies and green valley galaxies present emission lines, they are characteristic of AGN activity. Blue galaxy classes have emission lines corresponding to star formation regions. We find the expected correlation between spectroscopic class and Hubble type, but this relationship exhibits a high intrinsic scatter. Several potential uses of the ASK classification are identified and sketched, including fast determination of physical properties by interpolation, classes as templates in redshift determinations, and target selection in follow-up works (we find classes of Seyfert galaxies, green valley galaxies, as well as a significant number of outliers). The ASK classification is publicly accessible through various websites.
description: Accepted for publication in ApJ. 15 figs. 20 pages. Free classification @ ftp://ask:galaxy@ftp.iac.es/
Additional file 1 of Integration of sperm ncRNA-directed DNA methylation and DNA methylation-directed histone retention in epigenetic transgenerational inheritance
Creators: name: Beck, Daniel
name: Millissia Ben Maamar
name: Skinner, Michael K.
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1: Figure S1. Vinclozolin lineage F3 generation conserved DMR in common with DHR and F1 generation ncRNA. Figure S2. DDT lineage F3 generation conserved DMR in common with DHR and F1 generation ncRNA. Table S1. Vinclozolin lineage F1 generation ncRNA & F1, F2 and F3 generation DMR overlap list. Table S2. DDT lineage F1 generation ncRNA & F1, F2 and F3 generation DMR overlap list. Table S3. F3 generation vinclozolin DMR & F3 generation DHR overlap list. Table S4. F3 generation DDT DMR & F3 generation DHR overlap list. Table S5. Vinclozolin lineage F1, F2, F3 generation DMR overlap list. Table S6. DDT lineage F1, F2, F3 generation DMR overlap list.
title: ÐÑÐ¾ÐµÐºÑ ÑÐµÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸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±ÑÑÑÑÐ¾Ð·Ð°Ð¼Ð¾ÑÐ¾Ð¶ÐµÐ½Ð½ÑÑ Ñ Ð»ÐµÐ±Ð¾Ð±ÑÐ»Ð¾ÑÐ½ÑÑ Ð¸Ð·Ð´ÐµÐ»Ð¸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Ð½, ÐÐ°Ð»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¸ÑÐµÐ²ÑÐµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
Ð±ÑÑÑÑÐ¾Ð·Ð°Ð¼Ð¾ÑÐ¾Ð¶ÐµÐ½Ð½ÑÐµ Ñ Ð»ÐµÐ±Ð¾Ð±ÑÐ»Ð¾ÑÐ½ÑÐµ Ð¿Ð¾Ð»ÑÑÐ°Ð±ÑÐ¸ÐºÐ°ÑÑ
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description: ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÐ½ÐºÐ° Ð±ÑÑÑÑÐ¾Ð·Ð°Ð¼Ð¾ÑÐ¾Ð¶ÐµÐ½Ð½ÑÑ ÑÐ»ÐµÐ±Ð¾Ð±ÑÐ»Ð¾ÑÐ½ÑÑ Ð¸Ð·Ð´ÐµÐ»Ð¸Ð¹ Ð² Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ðµ. ÐÐ·ÑÑÐµÐ½Ñ ÑÑÐ°Ð¿Ñ Ð¸ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ Ð²Ð¸Ð´Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð° Ð±ÑÑÑÑÐ¾Ð·Ð°Ð¼Ð¾ÑÐ¾Ð¶ÐµÐ½Ð½ÑÑ ÑÐ»ÐµÐ±Ð¾Ð±ÑÐ»Ð¾ÑÐ½ÑÑ Ð¸Ð·Ð´ÐµÐ»Ð¸Ð¹. ÐÐ¿Ð¸ÑÐ°Ð½Ñ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ñ Ðº Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ°. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð½Ð° Ð´ÐµÐ¹ÑÑÐ²ÑÑÑÐµÐ¼ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð¿ÑÐ¾ÐµÐºÑ ÑÐµÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ñ Ð±ÑÑÑÑÐ¾Ð·Ð°Ð¼Ð¾ÑÐ¾Ð¶ÐµÐ½Ð½ÑÑ ÑÐ»ÐµÐ±Ð¾Ð±ÑÐ»Ð¾ÑÐ½ÑÑ Ð¿Ð¾Ð»ÑÑÐ°Ð±ÑÐ¸ÐºÐ°ÑÐ¾Ð².
Electron transport through a quantum wire coupled with a mesoscopic ring
Creators: name: Maiti, Santanu K.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Electronic transport through a quantum wire sandwiched between two metallic electrodes and coupled to a quantum ring, threaded by a magnetic flux $ϕ$, is studied. An analytic approach for the electron transport through the bridge system is presented based on the tight-binding model. The transport properties are discussed in three aspects: (a) presence of an external magnetic filed, (b) strength of the wire to electrode coupling, and (c) presence of in-plane electric field.
description: 6 pages, 5 figures
title: Ð¢ÐµÑÐ¼Ð¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° ÑÐ¸Ð·Ð¸ÐºÐ¾-Ñ Ð¸Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼, Ð¸Ñ Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÑ Ð¾Ñ ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÑ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÑÑÐºÐ°ÑÐµÐ², ÐÐ¸ÐºÑÐ¾Ñ
name: Ð¤ÐµÐ´Ð¾ÑÐ¾Ð², ÐÑÑÐµÑÐ»Ð°Ð²
Publisher: name: ÐÐÐÐ°Ñ
Year: 1997
Subjects: Ð¤Ð¸Ð·Ð¸ÐºÐ¾-Ñ Ð¸Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ
Ð¢ÐµÑÐ¼Ð¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐ°

description: Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð¿ÑÐ¾ÑÐµÑÑÑ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð´Ð¸ÑÑÐ¾ÑÐ¸Ð°ÑÐ¸Ð¸ Ð´Ð²Ð¾Ð¹Ð½ÑÑ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ð¹ Ð¸Ð· Ð¸Ñ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² - Ð¾ÐºÑÐ¸Ð´Ð¾Ð², ÑÑÐ»ÑÑÐ¸Ð´Ð¾Ð², ÑÐ»Ð¾ÑÐ¸Ð´Ð¾Ð², ÐºÐ°ÑÐ±Ð¸Ð´Ð¾Ð², Ð° ÑÐ°ÐºÐ¶Ðµ Ð¾ÐºÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½Ð¾-Ð²Ð¾ÑÑÑÐ°Ð½Ð¾Ð²Ð¸ÑÐµÐ»ÑÐ½ÑÐµ ÑÐµÐ°ÐºÑÐ¸Ð¸ Ð² Ð¸Ð½ÑÐµÑÐ²Ð°Ð»Ðµ ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑ 298 ... 6000 Ñ ÑÑÑÑÐ¾Ð¼ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐµÐ¹ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ ÑÐ²Ð°ÑÐ¾ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°. Ð¡Ð¾Ð´ÐµÑÐ¶Ð¸Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð°Ð»Ð»Ð¾ÑÑÐ¾Ð¿Ð¸ÑÐµÑÐºÐ¸Ñ Ð¸ Ð¿Ð¾Ð»Ð¸Ð¼Ð¾ÑÑÐ½ÑÑ Ð¿ÑÐµÐ²ÑÐ°ÑÐµÐ½Ð¸Ð¹ Ð¼ÐµÑÐ°Ð»Ð»Ð¾Ð² Ð¸ ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ð¹, Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ ÑÐ²Ð¾Ð¹ÑÑÐ² ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð¸ÑÐµÑÐºÐ¸Ñ ÑÑÑÑÐºÑÑÑ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¾Ð±ÑÐ·Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÐµÑÐµÑÐ¾Ð´Ð° ÑÑÐ¸Ñ Ð²ÐµÑÐµÑÑÐ² Ð¸Ð· ÑÐ²ÑÑÐ´Ð¾Ð³Ð¾ ÑÐµÑÐµÐ· Ð¶Ð¸Ð´ÐºÐ¾Ðµ Ð² Ð³Ð°Ð·Ð¾Ð¾Ð±Ð¾Ð°Ð·Ð½Ð¾Ðµ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ðµ. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÑ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹ Ð²ÑÑÑÐ¸Ñ ÑÑÐµÐ±Ð½ÑÑ Ð·Ð°Ð²ÐµÐ´ÐµÐ½Ð¸Ð¹ Ð¿ÑÐ¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ð¸ Ð¸Ð½Ð´Ð¸Ð²Ð¸Ð´ÑÐ°Ð»ÑÐ½Ð¾Ð¹ Ð½Ð°ÑÑÐ½Ð¾-Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð¿Ð¾ ÐºÑÑÑÑ "Ð¤Ð¸Ð·Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð¼Ð¸Ñ. Ð¢ÐµÐ¾ÑÐ¸Ñ Ð¼ÐµÑÐ°Ð»Ð»ÑÑÐ³Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð²", Ð° ÑÐ°ÐºÐ¶Ðµ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¿Ð¾Ð»ÐµÐ·Ð½ÑÐ¼ Ð´Ð»Ñ Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»ÐµÐ¹, Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ¾Ð², Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ¾Ð².
Additional file 1 of IgM mesangial deposition as a risk factor for relapses of adult-onset minimal change disease
Creators: name: Yang, Cheng-Wen
name: Fan-Yu Chen
name: Fu-Pang Chang
name: Ho, Yang
name: Wu, Bo-Sheng
name: An-Hang Yang
name: Der-Cherng Tarng
name: Yang, Chih-Yu
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: Marine Biology
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: FOS: Biological sciences

description: Additional file 1: Supplementary Table 1. Dosage of immunosuppressive agents in adult-onset minimal change disease.
Fermion particle production in semi-classical Boltzmann-Vlasov transport theory
Creators: name: Dawson, John F.
name: Mihaila, B.
name: Cooper, F.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We present numerical solutions of the semi-classical Boltzmann-Vlasov equation for fermion particle-antiparticle production by strong electric fields in boost-invariant coordinates in (1+1) and (3+1) dimensional QED. We compare the Boltzmann-Vlasov results with those of recent quantum field theory calculations and find good agreement. We conclude that extending the Boltzmann-Vlasov approach to the case of QCD should allow us to do a thorough investigation of how back-reaction affects recent results on the dependence of the transverse momentum distribution of quarks and anti-quarks on a second Casimir invariant of color SU(3).
description: 8 figures
Perception of and Behavior Congruent With Gender Roles - URU-O | URU-P
Creators: name: LIRA Lab
Publisher: name: OSF
Year: 2019
Subjects: femininity
gender norms
gender roles
gender values
masculinity
perception of gender roles

description: Part of REPOPSI - Repository of Psychological Instruments in Serbian https://www.repopsi.f.bg.ac.rs/en/
Research-based theatre in counselling psychology : centering trans ways of knowing
Creators: name: Cook, Christina Olivia MacLeod
Publisher: name: University of British Columbia
Year: 2024

description: The research presented in this dissertation draws on research-based theatre (RbT) to create a playscript. The playscript explores two overarching narrative strands: (1) auto-narratives from Christina’s coming out as a nonbinary transgender woman while undertaking graduate studies in counselling psychology; (2) narratives from the author’s grandmother and mother’s experiences in doctoral programs in the 1940s and 1970s, respectively. Through the playscript, Christina considers the methodological possibilities that emerge when research-based theatre is applied within counselling psychology to explore auto-narratives of graduate school and transitioning. Furthermore, Christina examines the methodological options that arise from a trans-informed approach to RbT creation. A critical commentary and thematic analysis accompany the playscript, providing multiple entry points for knowledge translation.
title: ÐÐ¸Ð»Ð¾Ðµ Ð¼Ð½Ð¾Ð³Ð¾ÑÑÐ°Ð¶Ð½Ð¾Ðµ Ð·Ð´Ð°Ð½Ð¸Ðµ ÑÐ¾ Ð²ÑÑÑÐ¾ÐµÐ½Ð½Ð¾-Ð¿ÑÐ¸ÑÑÑÐ¾ÐµÐ½Ð½ÑÐ¼Ð¸ Ð¿Ð¾Ð¼ÐµÑÐµÐ½Ð¸ÑÐ¼Ð¸ Ð¸ Ð¿Ð¾Ð´Ð·ÐµÐ¼Ð½Ð¾Ð¹ Ð°Ð²ÑÐ¾ÑÑÐ¾ÑÐ½ÐºÐ¾Ð¹
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±Ð°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: ÑÐ¼Ð½ÑÐ¹ Ð´Ð¾Ð¼
Ð¶Ð¸Ð»Ð¾Ðµ Ð¼Ð½Ð¾Ð³Ð¾ÑÑÐ°Ð¶Ð½Ð¾Ðµ Ð·Ð´Ð°Ð½Ð¸Ðµ
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ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð²Ð½ÑÐµ ÑÐµÑÐµÐ½Ð¸Ñ

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Aberrasine aberrans subsp. okinawana
Creators: name: Koshkin, Evgeny S.
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Erebidae
Aberrasine
Aberrasine aberrans
Aberrasine aberrans okinawana (matsumura, 1930)

description: Aberrasine aberrans okinawana (Matsumura, 1930)
Miltochrista okinawana Matsumura, 1930: 39 (Type locality: « Okinawa »).
Distribution: Southern Japan (Okinawa, Amamioshima and Tokunoshima Islands) (Matsumura 1930; Kishida 2011).
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 page 571, DOI: 10.11646/zootaxa.5604.4.8, http://zenodo.org/record/15214199
title: ÐÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½Ð¾Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÐºÐ°ÑÐµÑÑÐ²Ð¾Ð¼. Ð§. 2
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÑÑÐ¾ÑÐºÐ¸Ð½Ð°, ÐÐ½Ð½Ð°
name: Ð¥Ð°ÑÐ»Ð°Ð¼Ð¾Ð², ÐÐ½Ð´ÑÐµÐ¹
name: Ð¡ÐµÐ¼ÐµÐ½Ð¾Ð²Ð°, Ð®Ð»Ð¸Ñ
Publisher: name: Ð¡ÐÐ±Ð¢Ð­Ð
Year: 2011
Subjects: ÐºÐ°ÑÐµÑÑÐ²Ð¾ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: Ð ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ ÑÐ¾Ð»Ñ ÑÐµÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ Ð¸ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ¸Ð·Ð°ÑÐ¸Ð¸ Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½Ð¾Ð³Ð¾ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÐºÐ°ÑÐµÑÑÐ²Ð¾Ð¼. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¸ÑÑÐ¾ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾Ð´ÑÐ¾Ð´Ð° Ð¿Ð¾ÐºÐ°Ð·ÑÐ²Ð°ÐµÑÑÑ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐ¹ ÑÑÐ¾Ð²ÐµÐ½Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÑ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ¾Ð². Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ Â«ÐÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½Ð¾Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÐºÐ°ÑÐµÑÑÐ²Ð¾Ð¼Â», Ð¾ÑÐ½Ð¾ÑÑÑÐµÐ¹ÑÑ Ðº Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ð°Ð¼ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐ¸ÐºÐ»Ð° (Ð²Ð°ÑÐ¸Ð°ÑÐ¸Ð²Ð½Ð°Ñ ÑÐ°ÑÑÑ), ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ ÑÑÐµÐ±Ð½Ð¾Ð¼Ñ Ð¿Ð»Ð°Ð½Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ 080200 Â«ÐÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÂ» Ð² ÑÐ°Ð¼ÐºÐ°Ñ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ Â«ÐÐ±ÑÐ¸Ð¹ Ð¸ ÑÑÑÐ°ÑÐµÐ³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½Ñ Ð² ÑÐ¾ÑÐ³Ð¾Ð²Ð»ÐµÂ». ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² (Ð¼Ð°Ð³Ð¸ÑÑÑÐ°Ð½ÑÐ¾Ð²), Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ðµ Â«ÐÐ±ÑÐ¸Ð¹ Ð¸ ÑÑÑÐ°ÑÐµÐ³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½Ñ Ð² ÑÐ¾ÑÐ³Ð¾Ð²Ð»ÐµÂ».
A Search for molecules in the atmosphere of HD 189733b
Creators: name: Barnes, J. R.
name: Barman, Travis S.
name: Jones, H. R. A.
name: Barber, R. J.
name: Hansen, Brad M. S.
name: Prato, L.
name: Rice, E. L.
name: Leigh, C. J.
name: Cameron, A. Collier
name: Pinfield, D. J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We use signal enhancement techniques and a matched filter analysis to search for the K band spectroscopic absorption signature of the close orbiting extrasolar giant planet, HD 189733b. With timeseries observations taken with NIRSPEC at the Keck II telescope, we investigate the relative abundances of H2O and carbon bearing molecules, which have now been identified in the dayside spectrum of HD 189733b. We detect a candidate planet signature with a low level of significance, close to the ~153 km/s velocity amplitude of HD 189733b. However, some systematic variations, mainly due to imperfect telluric line removal, remain in the residual spectral timeseries in which we search for the planetary signal. The robustness of our candidate signature is assessed, enabling us to conclude that it is not possible to confirm the presence of any planetary signal which appears at Fp/F* contrasts deeper than the 95.4 per cent confidence level. Our search does not enable us to detect the planet at a contrast ratio of Fp/F* = 1/1920 with 99.9 per cent confidence. We also investigate the effect of model uncertainties on our ability to reliably recover a planetary signal. The use of incorrect temperature, model opacity wavelengths and model temperature-pressure profiles have important consequences for the least squares deconvolution procedure that we use to boost the S/N ratio in our spectral timeseries observations. We find that mismatches between the empirical and model planetary spectrum may weaken the significance of a detection by ~30-60 per cent, thereby potentially impairing our ability to recover a planetary signal with high confidence.
description: 11 pages, 7 figures (MNRAS, accepted)
D3.1: Programming Model Specification
Creators: name: KIT
name: UOP
name: AVN
name: VECTOR
name: QUB
name: FENTISS
Publisher: name: XANDAR consortium
Year: 2021

description: This document describes the XANDAR programming model, which lays the foundation to enable both the simulation-based verification of functional requirements and the realization of non-functional requirements (such as safety and security) by pattern-based model and code transformations. Both aspects are subject to research in the further course of the XANDAR project.

Section 1 describes the XANDAR design methodology, which is the procedure for developing software for embedded systems according to the XANDAR approach. It is based on the XANDAR process as described in deliverable 2.1.

Section 2 describes central aspects of target platforms and runtime environments to which software applications are deployed during the system generation of the XANDAR process.

Finally, section 3 describes the programming model that the XANDAR toolchain user, i.e. the developer of the system under consideration, is expected to follow during the software component implementation step of the XANDAR process. This enables further processing of the implementations in the XANDAR toolchain, both for simulation and for deployment on the target platform.
1/N Expansion in Correlated Graphene
Creators: name: Kotov, Valeri N.
name: Uchoa, Bruno
name: Neto, A. H. Castro
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We examine the 1/N expansion, where N is the number of two-component Dirac fermions, for Coulomb interactions in graphene with a gap of magnitude $Δ= 2 m$. We find that for $Nα\gg1$, where $α$ is graphene's "fine structure constant", there is a crossover as a function of distance $r$ from the usual 3D Coulomb law, $V(r) \sim 1/r$, to a 2D Coulomb interaction, $V(r) \sim \ln(Nα/mr)$, for $m^{-1} \ll r \ll m^{-1} N α/6$. This effect reflects the weak "confinement" of the electric field in the graphene plane. The crossover also leads to unusual renormalization of the quasiparticle velocity and gap at low momenta. We also discuss the differences between the interaction potential in gapped graphene and usual QED for different coupling regimes.
description: 7 pages, 2 figures; expanded presentation, references added
Lamproderma columbinum Rostaf.
Creators: name: Kluša, Julita
Publisher: name: Zenodo
Year: 2023
Subjects: Biodiversity
Taxonomy
Protozoa
Mycetozoa
Myxomycetes
Stemonitidales
Stemonitidaceae
Lamproderma
Lamproderma columbinum

description: Lamproderma columbinum (Pers.) Rostaf.,
garkājas lampīte
- leg. G. Adamonytė, 2005, det. G. Adamonytė, 2006; (NMKK), moderately common.
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
On post-Newtonian orbits and the Galactic-center stars
Creators: name: Preto, Miguel
name: Saha, Prasenjit
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Stars near the Galactic center reach a few percent of light speed during pericenter passage, which makes post-Newtonian effects potentially detectable. We formulate the orbit equations in Hamiltonian form such that the $O(v^2/c^2)$ and $O(v^3/c^3)$ post-Newtonian effects of the Kerr metric appear as a simple generalization of the Kepler problem. A related perturbative Hamiltonian applies to photon paths. We then derive a symplectic integrator with adaptive time-steps, for fast and accurate numerical calculation of post-Newtonian effects. Using this integrator, we explore relativistic effects. Taking the star S2 as an example, we find that general relativity would contribute tenths of mas in astrometry and tens of $\rm km s^{-1}$ in kinematics. (For eventual comparison with observations, redshift and time-delay contributions from the gravitational field on light paths will need to be calculated, but we do attempt these in the present paper.) The contribution from stars, gas, and dark matter in the Galactic center region is still poorly constrained observationally, but current models suggest that the resulting Newtonian perturbation on the orbits could plausibly be of the same order as the relativistic effects for stars with semi-major axes $\gtrsim 0.01$ pc (or 250 mas). Nevertheless, the known and distinctive {\it time dependence} of the relativistic perturbations may make it possible to disentangle and extract both effects from observations.
description: 25 pages, 6 figures, accepted for publication in Astrophysical Journal. Section 3 (on symplectic integrators) rewritten with more details, new section 5 on comparison with other post-Newtonian formulations, new figure 6, corrected typos, added references
FRAMING THE MEANING ACROSS THE TITLES IN DIFFERENT MODES
Creators: name: Babayeva, Iroda
Publisher: name: Zenodo
Year: 2025

description: The title serves as a crucial cognitive and conceptual device in both fiction and newspaper texts, guiding readers' interpretations and framing their understanding. This article examines the dual role of titles as cognitive markers and conceptual frameworks that encapsulate the essence of the text they precede. The study analyzes the linguistic, cultural, and contextual factors that influence the construction and interpretation of titles, emphasizing their role in shaping reader engagement. Through a comparative approach, this paper identifies similarities and differences in title usage between the two genres, exploring their impact on readers' cognitive processes and interpretative strategies.
Additional file 1 of Serial whole-body cryotherapy in fibromyalgia is effective and alters cytokine profiles
Creators: name: Klemm, Philipp
name: Becker, Johanna
name: Aykara, Iris
name: Asendorf, Thomas
name: Dischereit, Gabriel
name: Neumann, Elena
name: Müller-Ladner, Ulf
name: Lange, Uwe
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: Science Policy
subject: Computational Biology

description: Additional file 1.
title: Ð¨ÐµÑÑÑÐ´ÐµÑÑÑ Ð»ÐµÑ Ð² ÑÑÑÐ¾Ñ
title: Ð²Ð¾ÑÐ¿Ð¾Ð¼Ð¸Ð½Ð°Ð½Ð¸Ñ Ð²ÑÐ¿ÑÑÐºÐ½Ð¸ÐºÐ¾Ð² ÑÐ¸Ð·Ð¸ÐºÐ¾-Ð¼ÐµÑ Ð°Ð½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ° ÐÐÐ 1955 Ð³Ð¾Ð´Ð°
titleType: Subtitle
Creators: name: Ð§ÐµÑÐ½Ð¾ÐºÐ¾Ð², Ð.
name: Ð¤ÐµÐ´Ð¾ÑÐ¾Ð²Ð¸Ñ, ÐÐ²Ð³ÐµÐ½Ð¸Ð¹
name: ÐÐ¸ÐºÐ¸ÑÐ¸Ð½, Ð.
name: Ð¢Ð¾Ð¿ÑÑÐ³Ð¸Ð½, ÐÐ³Ð¾ÑÑ
name: ÐÐ²Ð°Ð½Ð¾Ð²Ð°, Ð¢.
name: ÐÐ³Ð¾ÑÐ¾Ð², Ð.
name: ÐÐ¾ÑÐ¾Ð±ÑÐµÐ², Ð.
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2015
Subjects: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½ÑÐ¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ â Ð¤Ð¸Ð·Ð¸ÐºÐ¾-Ð¼ÐµÑ Ð°Ð½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ°ÐºÑÐ»ÑÑÐµÑ
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

description: Ð¡Ð±Ð¾ÑÐ½Ð¸Ðº Ð¿Ð¾ÑÐ²ÑÑÐµÐ½ 60-Ð»ÐµÑÐ¸Ñ ÑÐ¾ Ð²ÑÐµÐ¼ÐµÐ½Ð¸ Ð¾ÐºÐ¾Ð½ÑÐ°Ð½Ð¸Ñ ÐµÐ³Ð¾ ÑÐ¾ÑÑÐ°Ð²Ð¸ÑÐµÐ»ÑÐ¼Ð¸ ÑÐ¸Ð·Ð¸ÐºÐ¾-Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ° ÐÐÐ. Ð¡Ð¾Ð´ÐµÑÐ¶Ð¸Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ Ð±Ð¸Ð¾Ð³ÑÐ°ÑÐ¸Ð¹ Ð²ÑÐ¿ÑÑÐºÐ½Ð¸ÐºÐ¾Ð² 1955 Ð³Ð¾Ð´Ð°, Ð½Ð°ÑÑÐ½Ð°Ñ ÑÑÐ´ÑÐ±Ð° ÐºÐ¾ÑÐ¾ÑÑÑ Ð±ÑÐ»Ð° Ð½ÐµÑÐ°Ð·ÑÑÐ²Ð½Ð¾ ÑÐ²ÑÐ·Ð°Ð½Ð° Ñ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸ÐµÐ¼ ÑÐ°ÐºÐµÑÐ½Ð¾-ÑÐ´ÐµÑÐ½Ð¾Ð³Ð¾ ÑÐ¸ÑÐ° Ð½Ð°ÑÐµÐ¹ ÑÑÑÐ°Ð½Ñ. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½ Ð´Ð»Ñ Ð¸Ð½ÑÐµÑÐµÑÑÑÑÐ¸ÑÑÑ Ð¸ÑÑÐ¾ÑÐ¸ÐµÐ¹ Ð½Ð°ÑÐºÐ¸ Ð¸ Ð½Ð°ÑÑÐ½Ð¾Ð¹ Ð¼Ð¾Ð»Ð¾Ð´ÐµÐ¶Ð¸. ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð² Ð°Ð²ÑÐ¾ÑÑÐºÐ¾Ð¹ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¸.
Entanglement of two qubits in a relativistic orbit
Creators: name: Doukas, Jason
name: Carson, Benedict
Publisher: name: arXiv
Year: 2010
Subjects: subject: Quantum Physics (quant-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The creation and destruction of entanglement between a pair of interacting two-level detectors accelerating about diametrically opposite points of a circular path is investigated. It is found that any non-zero acceleration has the effect of suppressing the vacuum entanglement and enhancing the acceleration radiation thereby reducing the entangling capacity of the detectors. Given that for large accelerations the acceleration radiation is the dominant effect, we investigate the evolution of a two detector system initially prepared in a Bell state using a perturbative mater equation and treating the vacuum fluctuations as an unobserved environment. A general function for the concurrence is obtained for stationary and symmetric worldlines in flatspace. The entanglement sudden death time is computed.
description: v2: Some typo's fixed, figures compressed to smaller filesize and added some references.
Inner and outer edge states in graphene rings: A numerical investigation
Creators: name: Bahamon, D. A.
name: Pereira, A. L. C.
name: Schulz, P. A.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We numerically investigate quantum rings in graphene and find that their electronic properties may be strongly influenced by the geometry, the edge symmetries and the structure of the corners. Energy spectra are calculated for different geometries (triangular, hexagonal and rhombus-shaped graphene rings) and edge terminations (zigzag, armchair, as well as the disordered edge of a round geometry). The states localized at the inner edges of the graphene rings describe different evolution as a function of magnetic field when compared to those localized at the outer edges. We show that these different evolutions are the reason for the formation of sub-bands of edge states energy levels, separated by gaps (anticrossings). It is evident from mapping the charge densities that the anticrossings occur due to the coupling between inner and outer edge states.
description: 8 pages, 7 figures. Figures in low resolution due to size requirements - higher quality figures on request
Pulse Shaping, Localization and the Approximate Eigenstructure of LTV Channels
Creators: name: Jung, Peter
Publisher: name: arXiv
Year: 2009
Subjects: subject: Information Theory (cs.IT)
subject: FOS: Computer and information sciences

description: In this article we show the relation between the theory of pulse shaping for WSSUS channels and the notion of approximate eigenstructure for time-varying channels. We consider pulse shaping for a general signaling scheme, called Weyl-Heisenberg signaling, which includes OFDM with cyclic prefix and OFDM/OQAM. The pulse design problem in the view of optimal WSSUS--averaged SINR is an interplay between localization and "orthogonality". The localization problem itself can be expressed in terms of eigenvalues of localization operators and is intimately connected to the concept of approximate eigenstructure of LTV channel operators. In fact, on the L_2-level both are equivalent as we will show. The concept of "orthogonality" in turn can be related to notion of tight frames. The right balance between these two sides is still an open problem. However, several statements on achievable values of certain localization measures and fundamental limits on SINR can already be made as will be shown in the paper.
description: 6 pages, 2 figures, invited paper