cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: Ð¡Ð¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐµ ÐºÐ¾Ð½ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ ÑÐµÐ³Ð¸Ð¾Ð½Ð° ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸. Ð ÐµÐ»Ð¸Ð³Ð¸Ñ Ð¸ ÑÐµÑÐºÐ¾Ð²Ñ Ð² ÑÑÑÐ°Ð½Ð°Ñ Ð¡ÐµÐ²ÐµÑÐ½Ð¾Ð¹ ÐÐ²ÑÐ¾Ð¿Ñ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÑÑÐ°ÐµÐ², ÐÐ°Ð´Ð¸Ð¼
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2012
Subjects: ÑÐµÐ»Ð¸Ð³Ð¸Ñ
Ñ ÑÐ¸ÑÑÐ¸Ð°Ð½ÑÑÐ²Ð¾
ÑÐµÑÐºÐ¾Ð²Ñ
ÑÑÑÐ°Ð½Ñ Ð¡ÐµÐ²ÐµÑÐ½Ð¾Ð¹ ÐÐ²ÑÐ¾Ð¿Ñ
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ ÐºÐ¾Ð½ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð°Ñ Ð¸ÑÑÐ¾ÑÐ¸Ñ ÑÑÑÐ°Ð½ Ð¡ÐµÐ²ÐµÑÐ½Ð¾Ð¹ ÐÐ²ÑÐ¾Ð¿Ñ - ÐÐ°Ð½Ð¸Ð¸, Ð¨Ð²ÐµÑÐ¸Ð¸, Ð¤Ð¸Ð½Ð»ÑÐ½Ð´Ð¸Ð¸, ÐÐ¾ÑÐ²ÐµÐ³Ð¸Ð¸ Ð¸ ÐÑÐ»Ð°Ð½Ð´Ð¸Ð¸, Ð¸ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ðµ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ ÑÐµÐ»Ð¸Ð³Ð¸Ð¸ Ð¸ ÑÐµÑÐºÐ²Ð¸ Ð² ÑÑÐ¸Ñ ÑÑÑÐ°Ð½Ð°Ñ. ÐÑÐ½Ð¾Ð²Ð½Ð¾Ðµ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ ÑÐ´ÐµÐ»ÐµÐ½Ð¾ Ð¸ÑÑÐ¾ÑÐ¸Ð¸ Ð¸ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¼Ñ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ ÐµÐ²Ð°Ð½Ð³ÐµÐ»Ð¸ÑÐµÑÐºÐ¾-Ð»ÑÑÐµÑÐ°Ð½ÑÐºÐ¸Ñ ÑÐµÑÐºÐ²ÐµÐ¹, ÐºÐ¾ÑÐ¾ÑÑÐµ ÑÐ²Ð»ÑÑÑÑÑ Ð³Ð¾ÑÐ¿Ð¾Ð´ÑÑÐ²ÑÑÑÐ¸Ð¼Ð¸ Ð² Ð½Ð°Ð·Ð²Ð°Ð½Ð½Ð¾Ð¼ ÑÐµÐ³Ð¸Ð¾Ð½Ðµ. Ð¢Ð°ÐºÐ¶Ðµ Ð¸Ð¼ÐµÑÑÑÑ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¾ ÑÐ²Ð¾Ð±Ð¾Ð´Ð½ÑÑ ÑÐµÑÐºÐ²Ð°Ñ Ð¸ Ð¸Ð½Ð¾ÐºÐ¾Ð½ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÑ Ð¾Ð±ÑÐ¸Ð½Ð°Ñ, Ð´ÐµÐ¹ÑÑÐ²ÑÑÑÐ¸Ñ Ð² ÑÑÐ¸Ñ ÑÑÑÐ°Ð½Ð°Ñ. Ð¯Ð²Ð»ÑÐµÑÑÑ ÑÑÐµÐ±Ð½ÑÐ¼ Ð¿Ð¾ÑÐ¾Ð±Ð¸ÐµÐ¼ Ð¿Ð¾ ÐºÑÑÑÑ Â«Ð¡Ð¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð°Ñ ÐºÐ¾Ð½ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð°Ñ ÑÑÑÑÐºÑÑÑÐ° ÑÑÑÐ°Ð½ Ð¡ÐµÐ²ÐµÑÐ½Ð¾Ð¹ ÐÐ²ÑÐ¾Ð¿ÑÂ», Ð¸Ð·ÑÑÐ°ÐµÐ¼Ð¾Ð¼Ñ Ð½Ð° Ð¿ÐµÑÐ²Ð¾Ð¼ ÐºÑÑÑÐµ Ð¼Ð°Ð³Ð¸ÑÑÑÐ°ÑÑÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Â«Ð ÐµÐ³Ð¸Ð¾Ð½Ð¾Ð²ÐµÐ´ÐµÐ½Ð¸ÐµÂ» Ð¿ÑÐ¸ ÐºÐ°ÑÐµÐ´ÑÐµ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÑ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ð¹ ÐÐ½ÑÑÐ¸ÑÑÑÐ° Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÑ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½ÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼ Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
Growth index with the exact analytic solution of sub-horizon scale linear perturbation for dark energy models with constant equation of state
Creators: name: Lee, Seokcheon
name: Ng, Kin-Wang
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Three decades ago Heath found the integral form of the exact analytic growing mode solution of the linear density perturbation $δ$ on sub-horizon scales including the cosmological constant or the curvature term. Recently, we obtained the exact analytic form of this solution in our previous work \cite{SK}. Interestingly, we are able to extend this solution for general dark energy models with the constant equation of state $ω_{de}$ in a flat universe. This analytic solution provides the accurate and efficient tools for probing the properties of dark energy models such as the behavior of the growth factor and the growth index. We investigate the growth index and its parameter at any epoch with this exact solution for different dark energy models and find that the growth index is quite model dependent in the redshift space, $0.25 \leq z \leq 1.5$, so observations of the structure growth around this epoch would be very interesting. Also one may be able to rule out some dark energy models by using the analysis from this exact solution. Thus, the analytic solution for the growth factor provides the very useful tools for future observations to constrain the exact values of observational quantities at any epoch related to the growth factor in the dark energy models.
description: 8pages, 3figures, 1Table, minor revisions to match version accepted by PLB (add Fig1)
A inseguir le stelle sopra Ragusa
Creators: Giuseppe Fiasconaro
Publisher: name: Media Inaf
Year: 2020

Il lockdown di questi giorni ha fermato tutto e tutti. Quello che non ha fermato è il movimento apparente delle stelle nella volta celeste, dovuto alla rotazione della Terra attorno al proprio asse. Un movimento che l’astrofotografo ragusano Gianni Tumino ha immortalato dalla terrazza di casa in una foto che la Nasa ha scelto lo scorso 28 marzo come Apod, Astronomy Picture Of the Day. Lo abbiamo intervistato
Mimicking the cosmological constant for more than one observable with large scale inhomogeneities
Creators: name: Romano, Antonio Enea
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Assuming the definition of the inversion problem (IP) as the exact matching of the terms in the low redshift expansion of cosmological observables calculated for different cosmological models, we solve the IP for $D_L(z)$ and the redshift spherical shell mass density $mn(z)$ for a central observer in a LTB space without cosmological constant and a generic $ΛCDM $ model. We show that the solution of the IP is unique, corresponds to a matter density profile which is not smooth at the center and that the same conclusions can be reached expanding self-consistently to any order all the relevant quantities. On contrary to the case of a single observable inversion problem, it is impossible to solve the IP (LTB vs. $Λ$CDM) for both $mn(z)$ and $D_L(z)$ while setting one the two functions $k(r)$ or $t^b(r)$ to zero, even allowing not smooth matter profiles. Our conclusions are general, since they are exclusively based on comparing directly physical observables in redshift space, and don't depend on any special ansatz or restriction for the functions defining a LTB model.
description: 20 pages, accepted by Physical Review D (D15), references added, appendices removed, text revised and improved with additional explanation of the calculation mothod and results
Che tempo farà su Marte?
Creators: Rossella Spiga
Publisher: name: Media Inaf
Year: 2020

Un nuovo modello degli strati alti dell’atmosfera marziana permetterà di fare previsioni meteo del Pianeta rosso molto più accurate rispetto al passato, grazie all’analisi delle onde di gravità capaci di influenzare periodicamente la dinamica atmosferica. Ne parliamo con Gabriella Gilli dell’Instituto de Astrofísica e Ciências do Espaço portoghese, prima autrice dell’articolo appena uscito su Journal of Geophysical Research
title: ÐÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð´Ð»Ñ Ð¿ÐµÑÐµÐ´Ð°ÑÐ¸ Ð² ÑÐ»ÑÐ¶Ð±Ñ ÑÐºÑÐ¿Ð»ÑÐ°Ñ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° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾Ð²Ð¸ÐºÐ¾Ð², ÐÐ»ÐµÐºÑÐ°Ð½Ð´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°Ð·Ñ Ð´Ð°Ð½Ð½ÑÑ
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description: Ð¦ÐµÐ»ÑÑ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸ ÑÑÐ°Ð»Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ BIM-Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð´Ð»Ñ Ð¿ÐµÑÐµÐ´Ð°ÑÐ¸ Ð² ÑÐ»ÑÐ¶Ð±Ñ ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ð¸. ÐÐ»Ñ Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ñ ÑÑÐ¾Ð¹ ÑÐµÐ»Ð¸ Ð±ÑÐ» Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½ ÑÑÐ¾Ð²ÐµÐ½Ñ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ BIM Ð² Ð¼Ð¸ÑÐµ Ð¸ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½ Ð¾Ð¿ÑÑ Ð²ÐµÐ´ÑÑÐ¸Ñ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¹, Ð¿ÑÐ¸Ð¼ÐµÐ½ÑÑÑÐ¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð² ÑÐ²Ð¾ÐµÐ¹ ÑÐ°Ð±Ð¾ÑÐµ, ÑÑÐ¾ Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ð»Ð¾ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°ÑÑ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐµ BIM-Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð² ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ñ. ÐÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð²ÐºÐ»ÑÑÐ°ÐµÑ Ð² ÑÐµÐ±Ñ: Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼ Ð´Ð»Ñ Ð¾ÑÐ¸ÑÑÐºÐ¸ Ð¼Ð¾Ð´ÐµÐ»Ð¸, ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´ÑÐµÐ¼ÑÐµ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÑ, Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÐµ Ð½Ð° ÑÑÐ°Ð´Ð¸Ð¸ ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ð¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ñ, Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑÑÐ¸Ðµ Ð¿ÑÐ°Ð²Ð¸Ð»ÑÐ½Ð¾ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð¾Ð²Ð°ÑÑ Ð¿ÑÐ¾ÑÐµÑÑ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð² ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸ÑÑ, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð²Ð½ÐµÐ´ÑÑÑÑ Ð¸Ð»Ð¸ Ð½Ð°ÑÐ¸Ð½Ð°ÑÑ Ð²Ð½ÐµÐ´ÑÑÑÑ BIM.
Additional file 2 of Efficacy and safety of butylphthalide in secondary prevention of stroke: study protocol for a multicenter, real world trial based on Internet
Creators: name: Lv, Junchao
name: Zhao, Di
name: Zhao, Gang
name: Xie, Zhen
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Neuroscience
subject: Pharmacology
subject: Biotechnology
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 2: Appendix 2.The informed consent form.
Magnetic amplifiers
Creators: name: Tebby, John Charles
Publisher: name: University of British Columbia
Year: 2012

description: Direct current controlled transductors, now known as magnetic amplifiers, were used successfully by the Germans in the 1939-1945 war for the amplification and mixing of powers down to a microwatt. The desire to know more about their operations than has been given in various periodicals prompted this thesis. An explanation of magnetic amplifier action is given and the waveforms of flux and output current predicted. The behaviour of circuits containing a magnetic amplifier is then explained by the use of waveforms and a mathematical investigation is made. A use for a magnetic amplifier in an oscillator tank circuit is described. Graphs of the characteristics of the magnetic amplifier and photographs of the waveforms are shown and the observed waveforms compared with the predicted ones. A sensitivity test on three circuits containing a magnetic amplifier is described and results given showing that by placing a condenser across the supply windings increases the sensitivity considerably but decreases the power amplification. The proper way to secure a thorough understanding of the properties of the magnetic amplifier by the use of an oscilloscope is discussed and the thesis concludes by listing the advantages and disadvantages of a magnetic amplifier. The mathematical approach to the solution of the magnetic amplifier problem using Frolich's equation for the magnetization curve is given in a special appendix.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐºÐ¸Ð´Ð¾Ðº (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ âÐ¢ÐÐ ÐÐ Ð­Ð½ÐµÑÐ³Ð¾â)
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Ð¾Ð·Ð¾Ð², ÐÐ½Ð´ÑÐµÐ¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÑÐ¸Ð¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ±ÑÑÐ°
ÑÐºÐ¸Ð´ÐºÐ¸
ÑÐ¸ÑÑÐµÐ¼Ð° ÑÐºÐ¸Ð´Ð¾Ðº
ÑÐ±ÑÑ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐÐ âÐ¢ÐÐ ÐÐ Ð­Ð½ÐµÑÐ³Ð¾â.
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ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð±ÑÐ»Ð¸ Ð²ÑÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¾ÑÐºÐ»Ð¾Ð½ÐµÐ½Ð¸Ñ Ð¾Ñ Ð½Ð¾ÑÐ¼Ñ Ð² ÐÐÐ âÐ¢ÐÐ ÐÐ Ð­Ð½ÐµÑÐ³Ð¾â.
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Ð ÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð¼ÐµÑ Ð¿Ð¾ ÑÑÐ¸Ð¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ±ÑÑÐ° Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÑ Ðº Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÑ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ Ð¸ ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¸Ð±ÑÐ»Ð¸ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸.
MOESM6 of Identification of a small mutation panel of coding sequences to predict the efficacy of immunotherapy for lung adenocarcinoma
Creators: name: Li, Ying
name: Jiang, Wenbin
name: Li, Tianhao
name: Li, Mengyue
name: Li, Xin
name: Zhang, Zheyang
name: Zhang, Sainan
name: Liu, Yixin
name: Zhao, Wenyuan
name: Gu, Yunyan
name: Qi, Lishuang
name: Ao, Lu
name: Guo, Zheng
Publisher: name: figshare
Year: 2020
Subjects: subject: Biochemistry
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology

description: Additional file 6: Table S5. The functional pathways enriched with differently expressed genes.
Inference in particle tracking experiments by passing messages between images
Creators: name: Chertkov, M.
name: Kroc, L.
name: Krzakala, F.
name: Vergassola, M.
name: Zdeborová, L.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Data Analysis, Statistics and Probability (physics.data-an)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Chaotic Dynamics (nlin.CD)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: Methods to extract information from the tracking of mobile objects/particles have broad interest in biological and physical sciences. Techniques based on simple criteria of proximity in time-consecutive snapshots are useful to identify the trajectories of the particles. However, they become problematic as the motility and/or the density of the particles increases due to uncertainties on the trajectories that particles followed during the images' acquisition time. Here, we report an efficient method for learning parameters of the dynamics of the particles from their positions in time-consecutive images. Our algorithm belongs to the class of message-passing algorithms, known in computer science, information theory and statistical physics as Belief Propagation (BP). The algorithm is distributed, thus allowing parallel implementation suitable for computations on multiple machines without significant inter-machine overhead. We test our method on the model example of particle tracking in turbulent flows, which is particularly challenging due to the strong transport that those flows produce. Our numerical experiments show that the BP algorithm compares in quality with exact Markov Chain Monte-Carlo algorithms, yet BP is far superior in speed. We also suggest and analyze a random-distance model that provides theoretical justification for BP accuracy. Methods developed here systematically formulate the problem of particle tracking and provide fast and reliable tools for its extensive range of applications.
description: 18 pages, 9 figures
The effect of subfilter-scale physics on regularization models
Creators: name: Graham, Jonathan Pietarila
name: Holm, Darryl D.
name: Mininni, Pablo
name: Pouquet, Annick
Publisher: name: arXiv
Year: 2010
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: Chaotic Dynamics (nlin.CD)
subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: The subfilter-scale (SFS) physics of regularization models are investigated to understand the regularizations' performance as SFS models. The strong suppression of spectrally local SFS interactions and the conservation of small-scale circulation in the Lagrangian-averaged Navier-Stokes alpha-model (LANS-alpha) is found to lead to the formation of rigid bodies. These contaminate the superfilter-scale energy spectrum with a scaling that approaches k^1 as the SFS spectra is resolved. The Clark-alpha and Leray-alpha models, truncations of LANS-alpha, do not conserve small-scale circulation and do not develop rigid bodies. LANS-alpha, however, is closest to Navier-Stokes in intermittency properties. All three models are found to be stable at high Reynolds number. Differences between L^2 and H^1 norm models are clarified. For magnetohydrodynamics (MHD), the presence of the Lorentz force as a source (or sink) for circulation and as a facilitator of both spectrally nonlocal large to small scale interactions as well as local SFS interactions prevents the formation of rigid bodies in Lagrangian-averaged MHD (LAMHD-alpha). We find LAMHD-alpha performs well as a predictor of superfilter-scale energy spectra and of intermittent current sheets at high Reynolds numbers. We expect it may prove to be a generally applicable MHD-LES.
description: Proceedings of the Quality and Reliability of Large-Eddy Simulations II 2009 Workshop, Springer ERCOFTAC volume 16 (2011); submitted to Journal of Scientific Computing; 22 pages, 8 figures
title: Ð¡Ð¸Ð½ÑÐµÐ· ÐºÐ¾Ð¼Ð¿Ð¾Ð·Ð¸ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð¿Ð¾ÑÐ¾ÑÐºÐ¾Ð² ÑÐ¸ÑÑÐµÐ¼Ñ "AL-SiâNâ" Ð´Ð»Ñ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÑ Ð¿Ð¾ÐºÑÑÑÐ¸Ð¹ Ñ Ð²ÑÑÐ¾ÐºÐ¾Ð¹ ÑÐ²ÐµÑÐ´Ð¾ÑÑÑÑ Ð¸ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÑÐ¼Ð¸ Ð¸Ð·Ð½Ð¾ÑÐ¾ÑÑÐ¾Ð¹ÐºÐ¾ÑÑÐ¸
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¡Ð¾ÐºÐ¾Ð»Ð¾Ð²Ð°, ÐÐ°ÑÐ°Ð»ÑÑ
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Year: 2018
Subjects: ÐÐ¾Ð¼Ð¿Ð¾Ð·Ð¸ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ Ð¿Ð¾ÑÐ¾ÑÐºÐ¾Ð²ÑÐµ
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title: Ð ÐµÐ´Ð°ÐºÑÐ¾ÑÑ Ð°ÑÑ Ð¸ÑÐµÐºÑÑÑÐ½Ð¾Ð³Ð¾ ÑÑÐ¾Ð²Ð½Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ¼Ð¾ÑÐ¾Ð², ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
name: ÐÐµÑÑÐ¾Ð², ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
name: Ð¢ÑÑÐºÐµÐ²Ð¸Ñ, ÐÐ½ÑÐ¾Ð½
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Year: 2021
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

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title: ÐÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð·Ð°Ð½ÑÑÐ¸Ñ Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ Â«Ð¢ÐµÐ¾ÑÐ¸Ñ ÑÑÑÐ±Ð¾Ð¼Ð°ÑÐ¸Ð½Â»
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ°Ð¿ÑÐ¸Ð½, ÐÐ¸ÑÐ¸Ð»Ð»
name: ÐÐ½Ð´ÑÐµÐµÐ², 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: 2019
Subjects: Ð¢ÑÑÐ±Ð¾Ð¼Ð°ÑÐ¸Ð½Ñ

description: ÐÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð·Ð°Ð½ÑÑÐ¸Ñ Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ Â«Ð¢ÐµÐ¾ÑÐ¸Ñ ÑÑÑÐ±Ð¾Ð¼Ð°ÑÐ¸Ð½Â» Ð¿ÑÐµÑÐ»ÐµÐ´ÑÑÑ ÑÐµÐ»Ñ Ð·Ð°ÐºÑÐµÐ¿Ð¸ÑÑ Ð¸ ÐºÐ¾Ð½ÐºÑÐµÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°ÑÑ Ð·Ð½Ð°Ð½Ð¸Ñ, Ð¿ÑÐ¸Ð¾Ð±ÑÐµÑÐ°ÐµÐ¼ÑÐµ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼Ð¸ Ð¿ÑÐ¸ Ð¸Ð·ÑÑÐµÐ½Ð¸Ð¸ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÐºÑÑÑÐ°.
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title: ÐÐ½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ðµ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»Ð¸ÑÐµÐ»ÑÐ½Ð¾Ðµ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾ Ð´Ð»Ñ Ð´Ð¸Ð·ÐµÐ»Ñ-Ð³ÐµÐ½ÐµÑÐ°ÑÐ¾ÑÐ½ÑÑ Ð¸ Ð³Ð°Ð·Ð¾ÑÑÑÐ±Ð¸Ð½Ð½ÑÑ ÑÑÑÐ°Ð½Ð¾Ð²Ð¾Ðº
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¸ÑÐµÐ½ÐºÐ¾, ÐÐ¸ÐºÐ¾Ð»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¢ÐµÐ¿Ð»Ð¾ÑÐ»ÐµÐºÑÑÐ¾ÑÐµÐ½ÑÑÐ°Ð»Ð¸
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description: ÐÑÐ» Ð¿ÑÐ¾Ð²ÐµÐ´ÑÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ ÑÐ»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ¸ Ð¸ ÑÐµÐ¿Ð»Ð¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ¸ Ð Ð¾ÑÑÐ¸Ð¸, ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¸ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½ÑÐµ Ð¿ÑÑÐ¸ Ð¸Ñ ÑÐµÑÐµÐ½Ð¸Ñ. ÐÐ¾ÐºÐ°Ð·Ð°Ð½Ð° Ð²Ð¾Ð·ÑÐ°ÑÑÐ°ÑÑÐ°Ñ ÑÐ¾Ð»Ñ Ð¼Ð°Ð»Ð¾Ð¹ ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ¸. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° ÑÐ°Ð±Ð¾ÑÐ° Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð² ÑÐ½ÐµÑÐ³Ð¸Ð¸, Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð½ÑÑ Ð½Ð° Ð´Ð¸Ð·ÐµÐ»Ñ-Ð³ÐµÐ½ÐµÑÐ°ÑÐ¾ÑÐ½ÑÑ Ð¸ Ð³Ð°Ð·Ð¾ÑÑÑÐ±Ð¸Ð½Ð½ÑÑ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ°Ñ. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ð° Ð·Ð°ÑÐ¸ÑÑ ÑÑÐ°ÑÑÐºÐ° Ð»Ð¸Ð½Ð¸Ð¸ Ð¼ÐµÐ¶Ð´Ñ ÐºÐ¾Ð½ÑÐµÐ¹Ð½ÐµÑÐ½Ð¾Ð¹ ÑÑÐ°Ð½ÑÐ¸ÐµÐ¹ Ð¸ Ð Ð£ Ð¿Ð¾ÑÑÐµÐ±Ð¸ÑÐµÐ»Ñ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÑÐµÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ ÐºÐ¾ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð¸ Ð¿ÑÐµÐ´Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð¾ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ Ð¿Ð¾ ÐµÑ ÑÐµÑÐµÐ½Ð¸Ñ. Ð¢Ð°Ðº Ð¶Ðµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ñ ÑÐ°ÑÑÐµÑÑ Ð´Ð»Ñ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð Ð£ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ Ð´Ð»Ñ Ð¼Ð°Ð»Ð¾Ð¹ ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ¸ Ð¸ Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÑÐ½ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ ÐºÐ¾ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð² Ð¼Ð¸Ð½Ð¸-Ð¢Ð­Ð¦ Ñ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸ÐµÐ¼ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ ÑÐ¸Ð¿Ð° Ð Ð£.
Omaggio a Raffaello Sanzio, il principe delle arti
Creators: Frida Paolella e Roberto Della Ceca
Publisher: name: Media Inaf
Year: 2020

Lunedì prossimo, 6 aprile 2020, ricorre il cinquecentenario della morte di Raffaello Sanzio. Per l’occasione, Frida Paolella e Roberto Della Ceca ripercorrono la fortissima connessione tra arte e scienza – e in particolare l’astronomia – in alcuni capolavori del grande artista, al quale è stato dedicato anche un modulo della Stazione spaziale internazionale
Is Bax/Bcl-2 Ratio Considered as a Prognostic Marker with Age and Tumor Location in Colorectal Cancer?
Creators: name: Khodapasand, Ehsan
name: Jafarzadeh, Narges
name: Farrokhi, Farid
name: Kamalidehghan, Behnam
name: Houshmand, Massoud
Publisher: name: the Pasteur Institute of Iran
Year: 1996
Subjects: subject: Basic Sciences

description: Iranian Biomedical Journal (IBJ); ISSN 1028-852X
title: Le rôle des comptines dans l’identification et la discrimination des phonèmes au cycle 1
title: Le rôle des comptines dans l’identification et la discrimination des phonèmes au cycle 1
titleType: AlternativeTitle
Creators: name: Santoro, Simona
name: Petet, Camille
Publisher: name: Unknown
Year: 0

description: Notre objet de recherche porte sur le rôle des comptines dans le développement du langage chez l’enfant. Nous avons décidé de nous concentrer sur des phonèmes spécifiques présents dans la langue française. En raison de la crise sanitaire liée au Coronavirus que nous traversons actuellement, nous avons dû réduire le choix du nombre de phonèmes à travailler avec les élèves. Nous nous sommes donc concentrées essentiellement sur 3 phonèmes, pour nous adapter à l’enseignement à distance et à la disponibilité de chaque famille. Il nous importait aussi de rendre les exercices simples afin que l’élève soit le plus autonome possible fasse aux tâches proposées. L’objectif était que les parents n’interviennent pas dans les échanges afin que les réponses des élèves partent réellement d’eux et que nos données ne soient pas influencées. Lors de notre recherche, nous avons comparé trois groupes d’élèves travaillant les phonèmes avec diverses comptines créées par nos soins en utilisant des supports d’apprentissages différents. Le premier groupe a travaillé en chantant la comptine, tandis que le second groupe a travaillé le rythme de la comptine avec divers exercices corporels. Le troisième groupe, le « groupe contrôle », n’a quant à lui fait aucune activité musicale ou rythmique et a reçu une approche traditionnelle. Les résultats de ce groupe-là ont donc été témoins de ce type d’approche de l’enseignement de la langue française. En effet, afin de rendre compte de l’évolution des apprentissages de nos élèves, nous avons mis en place des tâches d’identification et de discrimination de phonèmes pour le « groupe chant », et pour le « groupe rythme ». Elle a joué le rôle d’évaluation afin de constater si les élèves ayant travaillé uniquement avec la partie rythmique avaient eu plus de facilité ou non à identifier et discriminer les phonèmes proposés.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»Ð° Ð´Ð¾Ñ Ð¾Ð´Ð½Ð¾Ð¹ Ð½ÐµÐ´Ð²Ð¸Ð¶Ð¸Ð¼Ð¾ÑÑÐ¸
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐ²Ð´Ð¾ÐºÐ¸Ð¼Ð¾Ð², 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: 2017
Subjects: Ð¾Ð±ÑÐµÐºÑÑ Ð½ÐµÐ´Ð²Ð¸Ð¶Ð¸Ð¼Ð¾ÑÑÐ¸
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description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ Ð½ÐµÐ´Ð²Ð¸Ð¶Ð¸Ð¼Ð°Ñ ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½Ð¾ÑÑÑ - ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ Ð·ÐµÐ¼ÐµÐ»ÑÐ½ÑÑ ÑÑÐ°ÑÑÐºÐ¾Ð² Ñ ÑÐ°ÑÐ¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÐ¼Ð¸ Ð½Ð° Ð½ÑÐ¼ ÑÐ»ÑÑÑÐµÐ½Ð¸ÑÐ¼Ð¸. ÐÑÐ½Ð¾Ð²Ð½Ð°Ñ ÑÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ Ð·Ð°ÐºÐ»ÑÑÐ°ÐµÑÑÑ Ð² ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ð¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¾Ð±ÑÐµÐºÑÐ° Ð½ÐµÐ´Ð²Ð¸Ð¶Ð¸Ð¼Ð¾ÑÑÐ¸ Ñ ÑÑÑÑÐ¾Ð¼ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ð¹. Ð ÐºÐ¾Ð½ÐµÑÐ½Ð¾Ð¼ Ð¸ÑÐ¾Ð³Ðµ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð° Ð´Ð¾Ð»Ð¶Ð½Ð° Ð¿Ð¾Ð²ÑÑÐ¸ÑÑ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð» Ð¸ ÑÑÐ½Ð¾ÑÐ½ÑÑ ÑÐµÐ½Ð½Ð¾ÑÑÑ Ð¾Ð±ÑÐµÐºÑÐ°. ÐÑÐ»Ð¾ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½Ð¾Ðµ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ Ð¸ÑÑÐ»ÐµÐ´ÑÐµÐ¼Ð¾Ð³Ð¾ Ð¾Ð±ÑÐµÐºÑÐ° Ð½ÐµÐ´Ð²Ð¸Ð¶Ð¸Ð¼Ð¾ÑÑÐ¸ Ñ Ð²ÑÑÐ²Ð»ÐµÐ½Ð¸ÐµÐ¼ ÐµÐ³Ð¾ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ Ð¿ÑÐµÐ¸Ð¼ÑÑÐµÑÑÐ². ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐµÐ½Ð´ÐµÐ½ÑÐ¸Ð¸ Ð½Ð° ÑÑÐ½ÐºÐµ Ð½ÐµÐ´Ð²Ð¸Ð¶Ð¸Ð¼Ð¾ÑÑÐ¸ Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ð°. ÐÐ½Ð°ÑÐ¸ÑÐµÐ»ÑÐ½Ð°Ñ ÑÐ°ÑÑÑ ÑÐ°Ð±Ð¾ÑÑ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð° Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½ÑÑ Ð¿ÑÐ¾ÑÐ°Ð±Ð¾ÑÐºÑ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ñ ÑÐµÐ»ÑÑ Ð²ÑÐ±Ð¾ÑÐ° Ð½Ð°Ð¸Ð»ÑÑÑÐµÐ³Ð¾ Ð¸ Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð²Ð°ÑÐ¸Ð°Ð½ÑÐ° Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¾Ð±ÑÐµÐºÑÐ°. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²ÑÐµ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð²Ð°ÑÐ¸Ð°Ð½ÑÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾Ð³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¸ÑÑÐ»ÐµÐ´ÑÐµÐ¼Ð¾Ð³Ð¾ Ð¾Ð±ÑÐµÐºÑÐ° Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸ÐµÐ¼ ÐµÐ³Ð¾ ÑÑÐ½Ð¾ÑÐ½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»Ð°. Ð£Ð´ÐµÐ»ÐµÐ½Ð¾ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ñ ÑÐ¸ÑÐºÐ¾Ð² Ð´Ð»Ñ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ Ð±Ð¾Ð»ÐµÐµ Ð´Ð¾ÑÑÐ¾Ð²ÐµÑÐ½Ð¾Ð³Ð¾ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ°. Ð Ð¿ÑÐ¾ÑÐµÑÑÐµ Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ñ ÑÐµÐ»Ð¸ ÑÐ°Ð±Ð¾ÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð»Ð¸ÑÑ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ (Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¸ ÑÐ¸Ð½ÑÐµÐ·, Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ) Ð¸ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ðµ (ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ðµ, Ð¸Ð·Ð¼ÐµÑÐµÐ½Ð¸Ðµ) Ð¼ÐµÑÐ¾Ð´Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ. Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ ÑÐ°Ð±Ð¾ÑÑ Ð½Ð°Ð¹Ð´ÐµÐ½ Ð½Ð¾Ð²ÑÐ¹ Ð¿Ð¾Ð´ÑÐ¾Ð´ Ðº ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¾ÐµÐºÑÐ° ÑÐµÐ´ÐµÐ²ÐµÐ»Ð¾Ð¿Ð¼ÐµÐ½ÑÐ°, ÐºÐ¾ÑÐ¾ÑÑÐ¹ Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ñ Ð´Ð¾ÑÑÐ¸ÑÑ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ¾Ð² Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð¶Ð¸Ð·Ð½ÐµÐ´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸.
Second-order Relativistic Hydrodynamic Equations for Viscous Systems; how does the dissipation affect the internal energy?
Creators: name: Tsumura, Kyosuke
name: Kunihiro, Teiji
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We derive the second-order dissipative relativistic hydrodynamic equations in a generic frame with a continuous parameter from the relativistic Boltzmann equation. We present explicitly the relaxation terms in the energy and particle frames. Our results show that the viscosities are frame-independent but the relaxation times are generically frame-dependent. We confirm that the dissipative part of the energy-momentum tensor in the particle frame satisfies $δT^μ_μ= 0$ obtained for the first-order equation before, in contrast to the Eckart choice $u_μδT^{μν} u_ν= 0$ adopted as a matching condition in the literature. We emphasize that the new constraint $δT^μ_μ= 0$ can be compatible with the phenomenological derivation of hydrodynamics based on the second law of thermodynamics.
description: 8 pages, 2 figures. The significance of clear definition of local rest frames for a viscous relativistic fluid is emphasized as an unsolved problem. The relaxation equations are corrected by adding the vorticity and acceleration terms, which were missed in the previous version.
Additional file 2 of Pharmacogenomic profiling reveals molecular features of chemotherapy resistance in IDH wild-type primary glioblastoma
Creators: name: Nam, Yoonhee
name: Koo, Harim
name: Yang, Yingxi
name: Shin, Sang
name: Zhu, Zhihan
name: Kim, Donggeon
name: Cho, Hee Jin
name: Mu, Quanhua
name: Choi, Seung Won
name: Sa, Jason K.
name: Seo, Yun Jee
name: Kim, Yejin
name: Lee, Kyoungmin
name: Oh, Jeong-Woo
name: Kwon, Yong-Jun
name: Park, Woong-Yang
name: Kong, Doo-Sik
name: Seol, Ho Jun
name: Lee, Jung-Il
name: Park, Chul-Kee
name: Lee, Hye Won
name: Yoon, Yeup
name: Wang, Jiguang
Publisher: name: figshare
Year: 2023
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 2: Fig. S1. Timeline of sample acquisition, sequencing, in vitro culture and TMZ screening. Fig. S2. Gaussian Mixture Model used to identify genes with the same expression profile between patient-derived cells (PDCs) and tumor tissues. Fig. S3. Principal Component Analysis and differentially expressed gene analysis on 34 tissue RNA-seq samples. Fig. S4. Association of MGMT promoter methylation status to survival and in vitro TMZ screening in the main cohort. Fig. S5. Copy number estimation by GliomaSCAN. Fig. S6. Copy number estimation by RNA-seq. Fig. S7. Machine learning model feature importance. Fig. S8. Correlations between GBM subtypes and TMZ response. Fig. S9. Comparison of survival prediction in TCGA cohort. Fig. S10. Genomic landscape of multi-sector samples. Fig. S11. TMZ-resistant marker expression and CNV comparison in patient M13 and M14. Fig. S12. Progression free survival difference in patients with multi-sector samples.
title: Analysis of Impact of Natural Supply on Smoke Exhaust in a Ship Cabin by Comparison of a Full-scale Experiment and Fire Simulations
Creators: name: Wang, W.
name: Peng, C.
name: Guo, Y.
name: Peng, H.
name: Zhu, D.
name: Lu, J.
name: International Seminar On Fire And Explosion Hazards (9; 2019; Saint Petersburg, Russia)
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: 2019

description: Ship cabin fire accidents, on the one hand, might badly affect the integrity of ships and the safety of
people, on the other hand, possibly result in the loss of safety-related equipment functions. Therefore, it is
sensible to evaluate fire risk in ship cabins. Based on full-scale experimental tests, fire simulations by
CFAST and FDS were conducted in this study to evaluate the effect of the size of the supply opening on
smoke exhausts, and the size was changed by adjusting the upper height of the supply opening in the fullscale
experimental tests and fire simulations. According to the experimental configurations, six groups of
tests in this study were conducted by changing the upper heights as 0.1, 0.3, 0.5, 0.7, 0.9, and 1.1 m, and
smoke layer temperatures, and smoke layer heights from experimental tests and fire simulations were
selected as several indicators for the evaluation. By comparing full-scale experimental tests with fire
simulations, it was shown that different sizes of natural supply vents have different effects on the
effectiveness of smoke exhausts. More specifically, having a supply opening, compared with no supply
opening, can effectively reduce smoke layer temperatures and increase smoke layer heights, which has
been proven by full-scale experimental tests and fire simulations in this study.
Additional file 2: of Deletion of high-molecular-weight glutenin subunits in wheat significantly reduced dough strength and bread-baking quality
Creators: name: Zhang, Yingjun
name: Hu, Mengyun
name: Liu, Qian
name: Sun, Lijing
name: Chen, Xiyong
name: Lv, Liangjie
name: Liu, Yuping
name: Jia, Xu
name: Li, Hui
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology

description: Table S2. The probe regions for different genes used for DNA methylation analysis. (DOCX 14 kb)
Following Gibbs States Adiabatically - The Energy Landscape of Mean Field Glassy Systems
Creators: name: Krzakala, Florent
name: Zdeborová, Lenka
Publisher: name: arXiv
Year: 2009
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We introduce a generalization of the cavity, or Bethe-Peierls, method that allows to follow Gibbs states when an external parameter, e.g. the temperature, is adiabatically changed. This allows to obtain new quantitative results on the static and dynamic behavior of mean field disordered systems such as models of glassy and amorphous materials or random constraint satisfaction problems. As a first application, we discuss the residual energy after a very slow annealing, the behavior of out-of-equilibrium states, and demonstrate the presence of temperature chaos in equilibrium. We also explore the energy landscape, and identify a new transition from an computationally easier canyons-dominated region to a harder valleys-dominated one.
description: 6 pages, 7 figures
title: Ð ÐµÐ·Ð¾Ð½Ð°Ð½ÑÐ½Ð¾Ðµ ÑÐ°ÑÑÐµÑÐ½Ð¸Ðµ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð° Ð½Ð° Ð¿Ð¾Ð·Ð¸ÑÑÐ¾Ð½Ðµ Ð² ÑÐ²ÐµÑÐ¾Ð²Ð¾Ð¼ Ð¿Ð¾Ð»Ðµ Ð´Ð»Ñ Ð°Ð½Ð½Ð¸Ð³Ð¸Ð»ÑÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð°Ð¼Ð¿Ð»Ð¸ÑÑÐ´Ñ
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Ð¾Ð±ÑÐ»ÐµÐ², 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°Ð¼Ð¿Ð»Ð¸ÑÑÐ´Ð° ÑÐ°ÑÑÐµÑÐ½Ð¸Ñ
Ð°Ð½Ð½Ð¸Ð³Ð¸Ð»ÑÑÐ¸Ð¾Ð½Ð½Ð°Ñ Ð°Ð¼Ð¿Ð»Ð¸ÑÑÐ´Ð°
Ð²Ð¸ÑÑÑÐ°Ð»ÑÐ½Ð°Ñ ÑÐ°ÑÑÐ¸ÑÐ°
Ð»Ð°Ð·ÐµÑÐ½Ð¾Ðµ Ð¿Ð¾Ð»Ðµ
Ð¿Ð¾Ð·Ð¸ÑÑÐ¾Ð½

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¾ÑÐµÑÑÐ° ÑÐµÐ·Ð¾Ð½Ð°Ð½ÑÐ½Ð¾Ð³Ð¾ Ð°Ð½Ð½Ð¸Ð³Ð¸Ð»ÑÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ ÑÐ°ÑÑÐµÑÐ½Ð¸Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð° Ð½Ð° Ð¿Ð¾Ð·Ð¸ÑÑÐ¾Ð½Ðµ Ð² Ð¿Ð¾Ð»Ðµ Ð¿Ð»Ð¾ÑÐºÐ¾Ð¹ Ð¼Ð¾Ð½Ð¾ÑÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ»ÐµÐºÑÑÐ¾Ð¼Ð°Ð³Ð½Ð¸ÑÐ½Ð¾Ð¹ Ð²Ð¾Ð»Ð½Ñ. ÐÐ¾Ð»ÑÑÐµÐ½Ð° Ð°Ð½Ð½Ð¸Ð³Ð¸Ð»ÑÑÐ¸Ð¾Ð½Ð½Ð°Ñ Ð°Ð¼Ð¿Ð»Ð¸ÑÑÐ´Ð° ÑÐ°ÑÑÐµÑÐ½Ð¸Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð° Ð½Ð° Ð¿Ð¾Ð·Ð¸ÑÑÐ¾Ð½Ðµ Ð² Ð¿Ð¾Ð»Ðµ Ð¿Ð»Ð¾ÑÐºÐ¾Ð¹ ÑÐ»ÐµÐºÑÑÐ¾Ð¼Ð°Ð³Ð½Ð¸ÑÐ½Ð¾Ð¹ Ð²Ð¾Ð»Ð½Ñ Ð´Ð»Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð»ÑÐ½ÑÑ Ð¸Ð½ÑÐµÐ½ÑÐ¸Ð²Ð½Ð¾ÑÑÐµÐ¹ Ð¸ Ð¿Ð¾Ð»ÑÑÐ¸Ð·Ð°ÑÐ¸Ð¹ Ð²Ð¾Ð»Ð½Ñ. ÐÐ·ÑÑÐµÐ½Ñ ÑÐµÐ·Ð¾Ð½Ð°Ð½ÑÐ½ÑÐµ ÑÑÐ»Ð¾Ð²Ð¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð´Ð»Ñ ÑÐ»Ð°Ð±Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ñ. ÐÐ¾ÐºÐ°Ð·Ð°Ð½Ð¾, ÑÑÐ¾ ÑÐµÐ·Ð¾Ð½Ð°Ð½Ñ Ð¸Ð¼ÐµÐµÑ Ð¼ÐµÑÑÐ¾ Ð² ÑÐ»ÑÑÐ°Ðµ ÑÐ»ÑÑÑÐ°ÑÐµÐ»ÑÑÐ¸Ð²Ð¸ÑÑÑÐºÐ¸Ñ ÑÐ½ÐµÑÐ³Ð¸Ð¹ ÑÐ°ÑÑÐ¸Ñ Ð¸ Ð¼Ð°Ð»Ð¾Ð³Ð¾ ÑÐ³Ð»Ð° Ð¼ÐµÐ¶Ð´Ñ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÐ¼Ð¸ Ð¸Ñ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ. ÐÐ¾Ð»ÑÑÐµÐ½Ð° ÑÐµÐ·Ð¾Ð½Ð°Ð½ÑÐ½Ð°Ñ Ð°Ð¼Ð¿Ð»Ð¸ÑÑÐ´Ð° Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð² ÑÐ»ÑÑÐ°Ðµ ÑÐ»Ð°Ð±Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ñ Ð¸ ÑÐ¸ÑÐºÑÐ»ÑÑÐ½Ð¾Ð¹ Ð¿Ð¾Ð»ÑÑÐ¸Ð·Ð°ÑÐ¸Ð¸ Ð²Ð¾Ð»Ð½Ñ.
Correlation function of quasars in real and redshift space from the Sloan Digital Sky Survey Data Release 7
Creators: name: Ivashchenko, G.
name: Zhdanov, V. I.
name: Tugay, A. V.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We analyze the quasar two-point correlation function (2pCF) within the redshift interval $0.810\,h^{-1}$ Mpc the parameter describing the large-scale infall to density inhomogeneities is $β=0.63\pm0.10$ with the linear bias $b=1.44\pm0.22$ that marginally (within 2$σ$) agrees with the linear theory of cosmological perturbations. We discuss possibilities to obtain a statistical estimate of the random component of quasars velocities (different from the large-scale infall). We note rather slight dependence of quasars velocity dispersion upon the 2pCF parameters in the region $r<2$ Mpc.
description: 15 pages, 17 figures, online published in MNRAS; final version to match the published version
Tng, un italiano da tre metri e mezzo sull’Isla Bonita
Creators: Valentina Guglielmo
Publisher: name: Media Inaf
Year: 2020

Il Telescopio nazionale Galileo dell’Inaf, con il suo specchio primario da 3.58 metri, è il più grande telescopio interamente italiano al mondo. Si trova sull’isola di La Palma, alle Canarie, e in questi giorni è chiuso per l’emergenza Covid-19. Ce ne parla Avet Harutyunyan, astronomo residente e responsabile scientifico di uno degli strumenti di punta del telescopio, lo spettrografo Giano-B
Additional file 3 of Pharmacogenomic profiling reveals molecular features of chemotherapy resistance in IDH wild-type primary glioblastoma
Creators: name: Nam, Yoonhee
name: Koo, Harim
name: Yang, Yingxi
name: Shin, Sang
name: Zhu, Zhihan
name: Kim, Donggeon
name: Cho, Hee Jin
name: Mu, Quanhua
name: Choi, Seung Won
name: Sa, Jason K.
name: Seo, Yun Jee
name: Kim, Yejin
name: Lee, Kyoungmin
name: Oh, Jeong-Woo
name: Kwon, Yong-Jun
name: Park, Woong-Yang
name: Kong, Doo-Sik
name: Seol, Ho Jun
name: Lee, Jung-Il
name: Park, Chul-Kee
name: Lee, Hye Won
name: Yoon, Yeup
name: Wang, Jiguang
Publisher: name: figshare
Year: 2023
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 3. Supplementary methods.
Event-chain Monte Carlo algorithms for hard-sphere systems
Creators: name: Bernard, Etienne P.
name: Krauth, Werner
name: Wilson, David B.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: In this paper we present the event-chain algorithms, which are fast Markov-chain Monte Carlo methods for hard spheres and related systems. In a single move of these rejection-free methods, an arbitrarily long chain of particles is displaced, and long-range coherent motion can be induced. Numerical simulations show that event-chain algorithms clearly outperform the conventional Metropolis method. Irreversible versions of the algorithms, which violate detailed balance, improve the speed of the method even further. We also compare our method with a recent implementations of the molecular-dynamics algorithm.
description: 5 pages, 6 figures
La ricerca per tutti, a portata di click
Creators: Ufficio stampa Inaf
Publisher: name: Media Inaf
Year: 2020

I migliori contributi del mondo della ricerca pubblica italiana da oggi online in un’unica piattaforma. Tra le tante proposte dell’Inaf già presenti nel portale web, vi sono quelle pensate per facilitare il compito degli insegnanti nelle classi, ma anche video rivolti direttamente agli studenti e mostre virtuali da visitare online per tutta la famiglia, magari con l’aiuto di un semplice visore per cellulari
Coronavirus, ripercussioni sulle missioni spaziali
Creators: Patrizia Caraveo
Publisher: name: Media Inaf
Year: 2020

In questo articolo, ripreso con il consenso dell’autrice dal sito Startup Italia, Patrizia Caraveo fa il punto sulle missioni spaziali – in corso o in procinto di partire – costrette a fare i conti con l’emergenza Covid-19
Raro buco nero di “taglia M” scovato da Hubble
Creators: Maura Sandri
Publisher: name: Media Inaf
Year: 2020

Il telescopio spaziale di Nasa ed Esa ha fornito la prova finora più convincente dell’esistenza dei buchi neri di massa intermedia. Hubble conferma, con le sue immagini ad alta risoluzione, che questo buco nero – di massa pari a 50mila volte la massa del Sole – osservato da Chandra e Xmm-Newton risiede all'interno di un denso ammasso stellare. Tutti i dettagli su ApJ Letters
Faccia a faccia con la galassia Ngc 3344
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2020

La splendida galassia a spirale Ngc 3344 è solo uno degli oggetti celesti che impreziosisce i cieli serali di aprile. Ma questo mese si preannuncia ricco di fenomeni astronomici davvero interessanti, nuvole permettendo. I nostri consigli per osservarli al meglio
Thermal nature of charmonium transverse momentum spectra from Au-Au collisions at the highest energies available at the BNL Relativistic Heavy Ion Collider (RHIC)
Creators: name: Akkelin, S. V.
name: Braun-Munzinger, P.
name: Sinyukov, Yu. M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: We analyze the transverse momentum distribution of $J/ψ$ mesons produced in Au + Au collisions at the top RHIC energy within a blast-wave model that accounts for a possible inhomogeneity of the charmonium distribution and/or flow fluctuations. The results imply that the transverse momentum spectra of$J/ψ$, $ϕ$ and $Ω$ hadrons measured at the RHIC can be described well if kinetic freeze-out takes place just after chemical freeze-out for these particles.
description: 17 pages, 5 figures, minor corrections, to appear in Phys. Rev. C
Cantieri lunari e pipì d’astronauta
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2020

Gli elementi presenti nell’urina umana potrebbero essere utilizzati come additivi in leganti cementizi alternativi. E la colonizzazione della Luna dipende dalla capacità di produrre materiali da costruzione in loco, con quel c’è. L’intervista a Luca Valentini dell’Università di Padova
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐ½Ð¸ÑÐ¸ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð¼Ð°ÑÑÐ¸Ð²Ð¾Ð² Ð´Ð°Ð½Ð½ÑÑ MES-ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿Ð°ÐºÐ¾Ð²Ð¾ÑÐ½Ð¾Ð¹ Ð»Ð¸Ð½Ð¸Ð¸ Ð² ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ð¸ ÑÐ¾ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ¾Ð¼ PackML
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ÑÐµÐ¼Ð¾Ð², 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: 2018
Subjects: ÐÐ¾Ð½ÑÑÐ¾Ð»Ð»ÐµÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½ÑÐµ
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Crea il tuo astro-documentario con Scratch
Creators: Maura Sandri
Publisher: name: Media Inaf
Year: 2020

L’Istituto nazionale di astrofisica da oggi propone una nuova attività dedicata ai bambini che li porterà a diventare piccoli divulgatori in giro per lo spazio, descrivendo le bellissime immagini del telescopio spaziale Spitzer scaricabili con la app gratuita Nasa Selfies e programmando il loro astro-documentario con Scratch. Tutti i dettagli sulla pagina di Inaf Oas Bologna