cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÑÐ²Ð¸ÑÐ° Ð´Ð»Ñ Ð¾ÑÐµÐ½ÐºÐ¸ ÑÐ´Ð¾Ð±Ð¾ÑÐ¸ÑÐ°ÐµÐ¼Ð¾ÑÑÐ¸ ÑÐµÐºÑÑÐ° Ñ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸ÐµÐ¼ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð¼Ð°ÑÐ¸Ð½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ
title: Development of a service for text readability assessment via machine learning technologies
Creators: name: ÐÐ¸ÐºÑÐ»Ð¸Ð½Ð°, ÐÐ»Ð¸Ð·Ð°Ð²ÐµÑÐ°
name: Ð§ÐµÑÐºÐ°Ñ, ÐÐ»Ð¸Ð½Ð°
name: ÐÐ¾Ð·Ð¸Ð½Ð°, ÐÐºÐ°ÑÐµÑÐ¸Ð½Ð°
name: ÐÐ¾Ð¹ÐºÐ¾, ÐÐ½Ð½Ð°
name: ÐÐ¼Ð¸ÑÑÐ¸ÐµÐ²Ð°, ÐÐ¸Ð´Ð¸Ñ
name: "Ð¡Ð¸ÑÑÐµÐ¼Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð² Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¸", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð°Ñ Ð½Ð°ÑÑÐ½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (26; 2022; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2023
Subjects: ÐÐ°ÑÐ¸Ð½Ð½Ð¾Ðµ Ð¾Ð±ÑÑÐµÐ½Ð¸Ðµ
ÐÐµÐ¹ÑÐ¾Ð½Ð½ÑÐµ ÑÐµÑÐ¸
ÑÐ´Ð¾Ð±Ð¾ÑÐ¸ÑÐ°ÐµÐ¼Ð¾ÑÑÑ
Ð³ÑÐ°Ð´Ð¸ÐµÐ½ÑÐ½ÑÐ¹ Ð±ÑÑÑÐ¸Ð½Ð³
readability
gradient boosting

description: Ð¦ÐµÐ»ÑÑ Ð½Ð°ÑÑÐ¾ÑÑÐµÐ³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ° ÑÑÐ°Ð»Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÑÐ²Ð¸ÑÐ° Ð´Ð»Ñ Ð¾ÑÐµÐ½ÐºÐ¸ ÑÐ´Ð¾Ð±Ð¾ÑÐ¸ÑÐ°ÐµÐ¼Ð¾ÑÑÐ¸ Ð¸ Ð²Ð¾ÑÐ¿ÑÐ¸Ð½Ð¸Ð¼Ð°ÐµÐ¼Ð¾ÑÑÐ¸ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð¾Ð³Ð¾ ÑÐµÐºÑÑÐ° ÐºÐ°Ðº ÑÐ¿Ð¾ÑÐ¾Ð± Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÐºÐ°ÑÐµÑÑÐ²Ð° Ð½Ð¾Ð²Ð¾ÑÑÐ½Ð¾Ð³Ð¾, Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¸ Ð½Ð°ÑÑÐ½Ð¾Ð³Ð¾ ÐºÐ¾Ð½ÑÐµÐ½ÑÐ° Ð²ÐµÐ±-ÑÐ°Ð¹ÑÐ° Ð²ÑÑÑÐµÐ³Ð¾ ÑÑÐµÐ±Ð½Ð¾Ð³Ð¾ Ð·Ð°Ð²ÐµÐ´ÐµÐ½Ð¸Ñ. Ð ÑÑÐ°ÑÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¿Ð¾Ð´ÑÐ¾Ð´Ñ Ðº Ð¾ÑÐµÐ½ÐºÐµ ÑÐ´Ð¾Ð±Ð¾ÑÐ¸ÑÐ°ÐµÐ¼Ð¾ÑÑÐ¸, ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½Ð¾ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ðµ ÐºÐ»Ð°ÑÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¼ÐµÑÑÐ¸Ðº Ð¾ÑÐµÐ½ÐºÐ¸ ÑÐ»Ð¾Ð¶Ð½Ð¾ÑÑÐ¸ ÑÐµÐºÑÑÐ° Ð¸ ÑÐºÑÐ¿ÐµÑÑÐ½ÑÑ Ð¾ÑÐµÐ½Ð¾Ðº, Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½ ÐºÐ¾Ð¼Ð±Ð¸Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÐ¹ Ð¿Ð¾Ð´ÑÐ¾Ð´ Ðº Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÑÑÐ¾Ð²Ð½Ñ ÑÐ´Ð¾Ð±Ð¾ÑÐ¸ÑÐ°ÐµÐ¼Ð¾ÑÑÐ¸ ÑÐµÐºÑÑÐ°. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼ Ð³ÑÐ°Ð´Ð¸ÐµÐ½ÑÐ½Ð¾Ð³Ð¾ Ð±ÑÑÑÐ¸Ð½Ð³Ð° XGBoost ÐºÐ°Ðº Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½Ñ Ð´Ð»Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð½ÐµÐ¹ÑÐ¾ÑÐµÑÐµÐ²Ð¾Ð³Ð¾ Ð¿Ð¾Ð´ÑÐ¾Ð´Ð° Ðº Ð¾ÑÐµÐ½ÐºÐµ ÑÐ´Ð¾Ð±Ð¾ÑÐ¸ÑÐ°ÐµÐ¼Ð¾ÑÑÐ¸. ÐÐ¿Ð¸ÑÐ°Ð½Ñ ÑÑÐ°Ð¿Ñ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð½ÐµÐ¹ÑÐ¾ÑÐµÑÐµÐ²Ð¾Ð¹ Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð¸ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÐµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ.
description: The purpose of this work is to develop a tool for assessing the readability and perceptibility of electronic texts as a way to improve the quality of news, educational, and scientific content of a higher educational institution's website. The article considers approaches to the assessment of readability, the correspondence of classical metrics for assessing the text complexity and expert assessments calculated, the combined approach to determining the level of text readability proposed. The gradient boosting algorithm XGBoost is described as a tool for implementing a neural network approach to the readability evaluation. The stages of a neural network model development and the results obtained are outlined.
title: Lehre:digital: Erwerb digitaler Lehrkompetenz im fächerübergreifenden Kontext Chemie, Biologie und Physik
Creators: name: Huwer, Johannes
name: Thyssen, Christoph
name: Vogelsang, Christoph
Publisher: name: Publikationsserver der Pädagogischen Hochschule Thurgau
Year: 2020

description: Digitale Innovationen und Kompetenzen in der Lehramtsausbildung, p. 353
How to Specify and How to Prove Correctness of Secure Routing Protocols for MANET
Creators: name: Papadimitratos, P.
name: Haas, Z. J.
name: Hubaux, J. -P.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cryptography and Security (cs.CR)
subject: Networking and Internet Architecture (cs.NI)
subject: FOS: Computer and information sciences

description: Secure routing protocols for mobile ad hoc networks have been developed recently, yet, it has been unclear what are the properties they achieve, as a formal analysis of these protocols is mostly lacking. In this paper, we are concerned with this problem, how to specify and how to prove the correctness of a secure routing protocol. We provide a definition of what a protocol is expected to achieve independently of its functionality, as well as communication and adversary models. This way, we enable formal reasoning on the correctness of secure routing protocols. We demonstrate this by analyzing two protocols from the literature.
Higher order corrections to beyond-all-order effects in a fifth order Korteweg-de Vries equation
Creators: name: Fodor, Gyula
name: Forgács, Péter
name: Mushtaq, Muneeb
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Pattern Formation and Solitons (nlin.PS)
subject: FOS: Physical sciences

description: A perturbative scheme is applied to calculate corrections to the leading, exponentially small (beyond-all-orders) amplitude of the ``trailing'' wave asymptotics of weakly localized solitons. The model considered is a Korteweg-de Vries equation modified by a fifth order derivative term, $ε^2\partial_x^5$ with $ε\ll1$ (fKdV). The leading order corrections to the tail amplitude are calculated up to ${\cal{O}}(ε^5)$. An arbitrary precision numerical code is implemented to solve the fKdV equation and to check the perturbative results. Excellent agreement is found between the numerical and analytical results. Our work also clarifies the origin of a long-standing disagreement between the ${\cal{O}}(ε^2)$ perturbative result of Grimshaw and Joshi [SIAM J. Appl. Math. 55, 124 (1995)] and the numerical results of Boyd [Comp. Phys. 9, 324 (1995)].
description: 37 pages, 5 figures, minor corrections, version to appear in Phys. Rev. D
title: ÐÐ¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐ¾ÑÐ¼Ñ Ð¾Ð³Ð¸Ð±Ð°ÑÑÐµÐ¹ Ð¤Ð-ÑÐ¸Ð³Ð½Ð°Ð»Ð¾Ð² Ð² Ð¼Ð½Ð¾Ð³Ð¾ÐºÐ°Ð½Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ðµ Ð¿ÐµÑÐµÐ´Ð°ÑÐ¸ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÑÐ½ ÐÐ°Ð¹Ñ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: 2016
Subjects: Ð Ð°Ð´Ð¸Ð¾ÑÐ¸Ð³Ð½Ð°Ð»Ñ
ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ñ
Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½ÑÐ¹ Ð¸Ð¼Ð¿ÑÐ»ÑÑ
ÑÐ°Ð·Ð½Ð¾Ñ Ð½ÐµÑÑÑÐ¸Ñ ÑÐ°ÑÑÐ¾Ñ
optimal pulse
the spacing of the carrier frequencies

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿Ð¾Ð»ÑÑÐµÐ½Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½ÑÐµ ÑÐ¾ÑÐ¼Ñ Ð¾Ð³Ð¸Ð±Ð°ÑÑÐµÐ¹ ÑÐ°Ð·Ð¾Ð¼Ð°Ð½Ð¸Ð¿ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ ÑÐ¸Ð³Ð½Ð°Ð»Ð¾Ð² Ñ Ð¿Ð¾Ð»Ð½ÑÐ¼ Ð¾ÑÐºÐ»Ð¸ÐºÐ¾Ð¼ Ð¿ÑÐ¸ Ð·Ð°Ð´Ð°Ð½Ð½Ð¾Ð¼ ÑÐ°Ð·Ð½Ð¾ÑÐµ Ð½ÐµÑÑÑÐ¸Ñ ÑÐ°ÑÑÐ¾Ñ ÑÐ¾ÑÐµÐ´Ð½Ð¸Ñ ÐºÐ°Ð½Ð°Ð»Ð¾Ð² Ð¿ÐµÑÐµÐ´Ð°ÑÐ¸ Ð¿ÑÐ¸ ÑÑÐ»Ð¾Ð²Ð¸Ð¸ Ð½Ð¾ÑÐ¼Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð±ÐµÐ»Ð¾Ð³Ð¾ ÑÑÐ¼Ð° Ð½Ð° Ð²ÑÐ¾Ð´Ðµ Ð¿ÑÐ¸ÐµÐ¼Ð½Ð¸ÐºÐ°. Ð Ð°Ð±Ð¾ÑÐ° ÑÐ¾ÑÑÐ¾Ð¸Ñ Ð¸Ð· Ð´Ð²ÑÑ ÑÐ°Ð·Ð´ÐµÐ»Ð¾Ð². Ð ÑÐ°Ð·Ð´ÐµÐ»Ðµ 1 Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸ÑÑÑ ÑÐ¸Ð½ÑÐµÐ· Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¸Ð¼Ð¿ÑÐ»ÑÑÐ°, Ð¾Ð±ÐµÑÐ¿ÐµÑÐ¸Ð²Ð°ÑÑÐ¸Ð¹ Ð¼Ð°ÐºÑÐ¸Ð¼Ð°Ð»ÑÐ½ÑÑ ÐºÐ¾Ð½ÑÐµÐ½ÑÑÐ°ÑÐ¸Ñ ÑÑÐµÐ´Ð½ÐµÐ¹ Ð¼Ð¾ÑÐ½Ð¾ÑÑÐ¸ ÑÐ¸Ð³Ð½Ð°Ð»Ð¾Ð² Ð² Ð·Ð°Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð¿Ð¾Ð»Ð¾ÑÐµ ÑÐ°ÑÑÐ¾Ñ. Ð ÑÐ°Ð·Ð´ÐµÐ»Ðµ 2 Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸ÑÑÑ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼ Ð¿ÑÐ¸ÐµÐ¼Ð° ÑÐ¸Ð³Ð½Ð°Ð»Ð¾Ð². ÐÑÐ±Ð¾Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ¼Ñ Ð¸Ð¼Ð¿ÑÐ»ÑÑÐ¾Ð².
description: In this paper we obtain the optimum shape of the envelope of phase-shift keyed signals with complete response at a given spacing of the carrier frequencies of adjacent channels of transmission under normal white noise at the receiver input. The work consists of two sections. In section 1 is synthesis of optimal pulse providing the maximum concentration of average power of signals in a given frequency band. In section 2 is the algorithm of reception signals. Selection of the optimal form of pulses.
Using the longitudinal space charge instability for generation of VUV and X-ray radiation
Creators: name: Schneidmiller, E. A.
name: Yurkov, M. V.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Accelerator Physics (physics.acc-ph)
subject: FOS: Physical sciences

description: Longitudinal space charge (LSC) driven microbunching instability in electron beam formation systems of X-ray FELs is a recently discovered effect hampering beam instrumentation and FEL operation. The instability was observed in different facilities in infrared and visible wavelength ranges. In this paper we propose to use such an instability for generation of VUV and X-ray radiation. A typical longitudinal space charge amplifier (LSCA) consists of few amplification cascades (drift space plus chicane) with a short undulator behind the last cascade. If the amplifier starts up from the shot noise, the amplified density modulation has a wide band, on the order of unity. The bandwidth of the radiation within the central cone is given by inverse number of undulator periods. A wavelength compression could be an attractive option for LSCA since the process is broadband, and a high compression stability is not required. LSCA can be used as a cheap addition to the existing or planned short-wavelength FELs. In particular, it can produce the second color for a pump-probe experiment. It is also possible to generate attosecond pulses in the VUV and X-ray regimes. Some user experiments can profit from a relatively large bandwidth of the radiation, and this is easy to obtain in LSCA scheme. Finally, since the amplification mechanism is broadband and robust, LSCA can be an interesting alternative to self-amplified spontaneous emission free electron laser (SASE FEL) in the case of using laser-plasma accelerators as drivers of light sources.
The Fast X-ray Transient XRT 210423 and its Host Galaxy
Creators: name: Eappachen, D.
name: Jonker, P. G.
name: Levan, A. J.
name: Quirola-Vasquez, J.
name: Torres, M. A. P.
name: Bauer, F. E.
name: Dhillon, V. S.
name: Marsh, T.
name: Littlefair, S. P.
name: Ravasio, M. E.
name: Fraser, M.
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Fast X-ray Transients (FXTs) are X-ray flares with a duration ranging from a few hundred seconds to a few hours. Possible origins include the tidal disruption of a white dwarf by an intermediate-mass black hole, a supernova shock breakout, and a binary neutron star merger. We present the X-ray light curve and spectrum, and deep optical imaging of the FXT XRT 210423, which has been suggested to be powered by a magnetar produced in a binary neutron star merger. Our Very Large Telescope and Gran Telescopio Canarias (GTC) observations began on May 6, 2021, thirteen days after the onset of the flare. No transient optical counterpart is found in the 1" (3$σ$) X-ray uncertainty region of the source to a depth $g_{s}$=27.0 AB mag. A candidate host lies within the 1" X-ray uncertainty region with a magnitude of 25.9 $\pm$ 0.1 in the GTC/HiPERCAM $g_s$-filter. Due to its faintness, it was not detected in other bands, precluding a photometric redshift determination. We detect two additional candidate host galaxies; one with $z_{\rm spec}=1.5082 \pm 0.0001$ and an offset of 4.2$\pm$1" (37$\pm$9 kpc) from the FXT and another one with $z_{\rm phot}=1.04^{+0.22}_{-0.14}$, at an offset of 3.6$\pm$1" (30$\pm$8 kpc). Based on the properties of all the prospective hosts we favour a binary neutron star merger, as previously suggested in the literature, as explanation for XRT 210423.
description: 14 pages, 6 figures. Accepted for publication in ApJ
title: ÐÐ°ÑÑÐ¸Ð¾ÑÐ¸Ð·Ð¼ Ð² ÐÑÐ¿Ð°Ð½Ð¸Ð¸. Ð­ÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½Ñ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°ÑÑÐ¾Ð²Ð°, Ð ÐµÐ½Ð°ÑÐ°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð¿Ð°ÑÑÐ¸Ð¾ÑÐ¸Ð·Ð¼
Ð½Ð°ÑÐ¸Ñ
ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ñ
Ð½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð°Ñ Ð¸Ð´ÐµÑ ÐÑÐ¿Ð°Ð½Ð¸Ð¸

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ðµ Ð¿Ð°ÑÑÐ¸Ð¾ÑÐ¸Ð·Ð¼Ð° Ð² ÐÑÐ¿Ð°Ð½Ð¸Ð¸. Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ: Ð²ÑÐµ ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ðµ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð¿Ð°ÑÑÐ¸Ð¾ÑÐ¸Ð·Ð¼Ð°, ÐµÐ³Ð¾ Ð²Ð¸Ð´Ñ Ð¸ ÑÐ¾ÑÐ¼Ñ, ÑÑÑÐ½Ð¾ÑÑÑ Ð¿Ð¾Ð½ÑÑÐ¸Ñ Â«ÑÐ¾Ð´Ð¸Ð½Ð°Â», ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ Ð¿Ð°ÑÑÐ¸Ð¾ÑÐ¸Ð·Ð¼Ð° Ð½Ð° ÑÐ¾Ð½Ðµ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ ÑÐ²Ð¾Ð»ÑÑÐ¸Ð¸, Ð·Ð°Ð´Ð°ÑÐ¸ Ð¸ Ð¼ÐµÑÐ¾Ð´Ñ Ð¿Ð°ÑÑÐ¸Ð¾ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð²Ð¾ÑÐ¿Ð¸ÑÐ°Ð½Ð¸Ñ, Ð¸Ð´ÐµÑ Ð¸ÑÐ¿Ð°Ð½ÑÐºÐ¾Ð¹ Ð½Ð°ÑÐ¸Ð¸ Ð¸ ÐµÐµ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ Ñ Ð²Ð¸Ð´Ð¾Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸ÐµÐ¼ Ð¸ÑÑÐ¾ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐµÐ°Ð»Ð¸Ð¹, ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° Ð¸ÑÐ¿Ð°Ð½ÑÐºÐ¾Ð³Ð¾ Ð½Ð°ÑÐ¾Ð´Ð° Ð¸ ÑÑÐµÑ Ð½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÑ Ð¼ÐµÐ½ÑÑÐ¸Ð½ÑÑÐ², ÑÐ¾ÑÑÐ°Ð²Ð»ÑÑÑÐ¸Ñ ÐÑÐ¿Ð°Ð½Ð¸Ñ Ð¸ ÐºÐ°Ðº ÑÑÑÐ°Ð½Ñ Ð¸ ÐºÐ°Ðº Ð½Ð°ÑÐ¸Ñ. ÐÑÐ¾Ð¼Ðµ ÑÐ¾Ð³Ð¾, Ð² ÑÐ°Ð±Ð¾ÑÐµ Ð±ÑÐ»Ð¸ Ð¸Ð·ÑÑÐµÐ½Ñ ÑÐ¾ÑÐ¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸Ð²ÑÐ¸ÐµÑÑ Ð² ÐÑÐ¿Ð°Ð½Ð¸Ð¸ Ð½Ð° ÑÐµÐ¼Ñ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð¸Ð´ÐµÐ½ÑÐ¸ÑÐ½Ð¾ÑÑÐ¸ Ð¸ÑÐ¿Ð°Ð½ÑÐºÐ¾Ð³Ð¾ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð¸Ñ ÑÐ¾ ÑÐ²Ð¾ÐµÐ¹ ÑÑÑÐ°Ð½Ð¾Ð¹ Ð¸Ð»Ð¸ Ñ Ð°Ð²ÑÐ¾Ð½Ð¾Ð¼Ð½ÑÐ¼ ÑÐ¾Ð¾Ð±ÑÐµÑÑÐ²Ð¾Ð¼, Ð½Ð° ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸ ÐºÐ¾ÑÐ¾ÑÐ¾Ð³Ð¾ Ð¾Ð½Ð¾ Ð¿ÑÐ¾Ð¶Ð¸Ð²Ð°ÐµÑ. Ð¢Ð°Ðº Ð¶Ðµ, Ð²Ð°Ð¶Ð½Ð¾Ð¹ ÑÐ¾ÑÑÐ°Ð²Ð»ÑÑÑÐµÐ¹ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð½Ð¾Ðµ Ð² ÐÑÐ¿Ð°Ð½Ð¸Ð¸, ÑÐ¾ÑÐ¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ, ÐºÐ¾ÑÐ¾ÑÐ¾Ðµ Ð·Ð°ÑÑÐ¾Ð½ÑÐ»Ð¾ Ð²Ð¾Ð¿ÑÐ¾ÑÑ, ÐºÐ°ÑÐ°ÑÑÐ¸ÐµÑÑ Ð¸Ð´ÐµÐ½ÑÐ¸ÑÐ½Ð¾ÑÑÐ¸, Ð³Ð¾ÑÐ¾Ð²Ð½Ð¾ÑÑÐ¸ Ð·Ð°ÑÐ¸ÑÐ°ÑÑ ÑÐ²Ð¾Ñ ÑÐ¾Ð´Ð¸Ð½Ñ, Ð´Ð¾Ð±ÑÐ¾Ð²Ð¾Ð»ÑÐ½Ð¾Ð¹ Ð°ÑÐ¼Ð¸Ð¸, Ð¶ÐµÐ»Ð°Ð½Ð¸Ñ Ð¿ÑÐ¾Ð´Ð¾Ð»Ð¶Ð°ÑÑ Ð¶Ð¸ÑÑ Ð² ÐÑÐ¿Ð°Ð½Ð¸Ð¸ Ð½ÐµÑÐ¼Ð¾ÑÑÑ Ð½Ð° ÐµÐµ ÑÑÑÐ´Ð½Ð¾ÑÑÐ¸ Ð¸ ÑÐ°Ð±Ð¾ÑÐ°ÑÑ Ð½Ð° Ð±Ð»Ð°Ð³Ð¾ ÑÑÑÐ°Ð½Ñ. Ð­ÑÐ¾ ÑÐ¾ÑÐ¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð±ÑÐ»Ð¾ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ Ð² ÑÐ°Ð¼ÐºÐ°Ñ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ, Ð° Ð°Ð½Ð°Ð»Ð¸Ð· ÐµÐ³Ð¾ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð½Ð°Ð³Ð»ÑÐ´Ð½Ð¾ Ð¿Ð¾ÐºÐ°Ð·Ð°Ð» Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ðµ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¹ ÐÑÐ¿Ð°Ð½Ð¸Ð¸ Ðº ÑÐµÐ¼Ðµ Ð¿Ð°ÑÑÐ¸Ð¾ÑÐ¸Ð·Ð¼Ð°.
Hitchin's Projectively Flat Connection, Toeplitz Operators and the Asymptotic Expansion of TQFT Curve Operators
Creators: name: Andersen, Jørgen Ellegaard
name: Gammelgaard, Niels Leth
Publisher: name: arXiv
Year: 2009
Subjects: subject: Differential Geometry (math.DG)
subject: Mathematical Physics (math-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences

description: In this paper, we will provide a review of the geometric construction, proposed by Witten, of the SU(n) quantum representations of the mapping class groups which are part of the Reshetikhin-Turaev TQFT for the quantum group U_q(sl(n, C)). In particular, we recall the differential geometric construction of Hitchin's projectively flat connection in the bundle over Teichmuller space obtained by push-forward of the determinant line bundle over the moduli space of rank n, fixed determinant, semi-stable bundles fibering over Teichmuller space. We recall the relation between the Hitchin connection and Toeplitz operators which was first used by the first named author to prove the asymptotic faithfulness of the SU(n) quantum representations of the mapping class groups. We further review the construction of the formal Hitchin connection, and we discuss its relation to the full asymptotic expansion of the curve operators of Topological Quantum Field Theory. We then go on to identifying the first terms in the formal parallel transport of the Hitchin connection explicitly. This allows us to identify the first terms in the resulting star product on functions on the moduli space. This is seen to agree with the first term in the star product on holonomy functions on these moduli spaces defined by Andersen, Mattes and Reshetikhin.
description: 24 pages
“Re-elect Regional Chief Puglaas/Jody Wilson-Raybould : Building on OUR Success" : Platform, Sept. 9, 2009, Rev. Oct. 30, 2012“
Creators: name: Wilson-Raybould, Jody, 1971-
Publisher: name: The University of British Columbia
Year: 2019

description: Official campaign, “Re-elect Regional Chief Puglaas/Jody Wilson-Raybould,” BCAFN, "Building on OUR Success" : Platform, Sept. 9, 2009, Rev. Oct. 30, 2012“
Proximal Exploration of Venus Volcanism with Teams of Autonomous Buoyancy-Controlled Balloons
Creators: name: Rossi, Federico
name: Saboia, Maira
name: Krishnamoorthy, Siddharth
name: Hook, Joshua Vander
Publisher: name: arXiv
Year: 2023
Subjects: subject: Robotics (cs.RO)
subject: Multiagent Systems (cs.MA)
subject: FOS: Computer and information sciences

description: Altitude-controlled balloons hold great promise for performing high-priority scientific investigations of Venus's atmosphere and geological phenomena, including tectonic and volcanic activity, as demonstrated by a number of recent Earth-based experiments. In this paper, we explore a concept of operations where multiple autonomous, altitude-controlled balloons monitor explosive volcanic activity on Venus through infrasound microbarometers, and autonomously navigate the uncertain wind field to perform follow-on observations of detected events of interest. We propose a novel autonomous guidance technique for altitude-controlled balloons in Venus's uncertain wind field, and show the approach can result in an increase of up to 63% in the number of close-up observations of volcanic events compared to passive drifters, and a 16% increase compared to ground-in-the-loop guidance. The results are robust to uncertainty in the wind field, and hold across large changes in the frequency of explosive volcanic events, sensitivity of the microbarometer detectors, and numbers of aerial platforms.
description: 44 pages, 19 figures. Accepted for publication by Acta Astronautica
title: Soil mites as forensic markers of decomposition of corpses and carcasses
Creators: name: Che Kamaruzaman, Naila Azma
Publisher: name: University of Reading
Year: 2019

description: The use of forensic entomology in providing reliable death-time estimates using knowledge of carrion insect species’ ecology and larval development has been used for many years. Aside from insects, mites (Acari) can act as reliable indicators of time of death. The use of forensic acarology is growing rapidly into a valuable additional input into forensic analysis. This field of forensic analysis has always been closely connected to forensic entomology. This study aimed to identify and qualitatively assess the mites of forensic importance within the outdoor environment. The outcomes from this study provide data that will enable a basic forensic acarology service to be provided in other research, as well as initiate further development of forensic acarology in crime scene investigations. The ubiquitous of mites in the soil beneath corpses adding valuable information on decomposition process and reconstruct the scene of death. Using the micro-habitat specific to mites, the abundance, species richness and composition of mite orders was examined and compared and the unique presence of certain mites would be uncovered. Two outdoor settings for forensic study were set up by using pigs as proxies for human cadavers: 1) seasonal study of temperate area with four different seasons in almost 2 years (November of 2013 – August 2015) 2) carcass position/condition over a year (Jun 2013 – September 2014). The majority of mites found were phoretic with the mesostigmatid families, Macrochelidae and Parasitidae the most abundant. There are few quantitative data available on the carcass colonisation patterns of insects and other arthropods; however these data are forensically valuable. There may be differences in the taxa collected during this successional study on pigs and those that occur on human bodies from different habitats. Therefore, mites collected from three crime cases were used to prove the reliable approaches in using pig carcasses to the real cases. The mites present on the corpses were compared with those collected from the pig carcasses and there was extremely close agreement between the mite presence from bodies and carcasses.
title: ÐÐ¸Ð·Ð½ÐµÑ-ÑÐµÐ½ÑÑ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÐ¸ÑÑÐµÐ¼Ñ ÐºÐ¾Ð½Ð´Ð¸ÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð²Ð¾Ð·Ð´ÑÑ Ð° Ñ ÑÐ¶ÐµÐºÑÐ¸Ð¾Ð½Ð½ÑÐ¼Ð¸ Ð´Ð¾Ð²Ð¾Ð´ÑÐ¸ÐºÐ°Ð¼Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¡Ð¸Ð½ÐµÐ½ÐºÐ¾, Ð¯ÑÐ¾Ñ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Ð¶ÐµÐºÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð´Ð¾Ð²Ð¾Ð´ÑÐ¸ÐºÐ¸
ÑÐ¸ÑÑÐµÐ¼Ð° ÐºÐ¾Ð½Ð´Ð¸ÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð²Ð¾Ð·Ð´ÑÑ Ð°
Ð¾Ð±ÑÐµÐ¼Ð½Ð¾-Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½ÑÐµ ÑÐµÑÐµÐ½Ð¸Ñ
ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð²Ð½ÑÐµ ÑÐµÑÐµÐ½Ð¸Ñ

description: ÐÐ°Ð½Ð½Ð°Ñ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÑÑ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ°ÑÐ¸Ñ Ð½Ð° Ð²Ð¾Ð·Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð±Ð¸Ð·Ð½ÐµÑ-ÑÐµÐ½ÑÑÐ° Ñ ÑÐµÑÑÐ¾ÑÐ°Ð½Ð¾Ð¼ Ð¸ Ð¿Ð¾Ð´Ð·ÐµÐ¼Ð½Ð¾Ð¹ Ð°Ð²ÑÐ¾ÑÑÐ¾ÑÐ½ÐºÐ¾Ð¹. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð½Ð°Ñ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ°ÑÐ¸Ñ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð° Ð² ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ð¸ Ñ ÐÐ¾ÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ð¸ÐµÐ¼ Ð¿ÑÐ°Ð²Ð¸ÑÐµÐ»ÑÑÑÐ²Ð° Ð Ð¤ Ð¾Ñ 16 ÑÐµÐ²ÑÐ°Ð»Ñ 2008 Ð³. â 87 Â«Ð ÑÐ¾ÑÑÐ°Ð²Ðµ ÑÐ°Ð·Ð´ÐµÐ»Ð¾Ð² Ð¿ÑÐ¾ÐµÐºÑÐ½Ð¾Ð¹ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ°ÑÐ¸Ð¸ Ð¸ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸ÑÑ Ðº Ð¸Ñ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸ÑÂ» Ð¸ Ð¸Ð½ÑÐ¼Ð¸ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½ÑÐ¼Ð¸ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ°Ð¼Ð¸, Ð´ÐµÐ¹ÑÑÐ²ÑÑÑÐ¸Ð¼Ð¸ Ð½Ð° ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸ Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸. Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ»Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¾Ð±ÑÐµÐ¼Ð½Ð¾-Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½ÑÐµ ÑÐµÑÐµÐ½Ð¸Ñ Ð·Ð´Ð°Ð½Ð¸Ñ; ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÑÑÐµÐ¼Ð° Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½Ð¾Ð¹ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð·ÐµÐ¼ÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°ÑÑÐºÐ°; Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ ÑÐ°ÑÑÐµÑÐ° Ð² ÐÐ Â«SCADÂ» Ð¿ÑÐ¸Ð½ÑÑÑ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð²Ð½ÑÐµ ÑÐµÑÐµÐ½Ð¸Ñ; ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÑÐ¸ÑÑÐµÐ¼Ð° Ð¾Ð±ÑÐµÐ¾Ð±Ð¼ÐµÐ½Ð½Ð¾Ð¹ Ð²ÐµÐ½ÑÐ¸Ð»ÑÑÐ¸Ð¸ Ð¸ ÐºÐ¾Ð½Ð´Ð¸ÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¾ÑÐ¸ÑÐ½ÑÑ Ð¿Ð¾Ð¼ÐµÑÐµÐ½Ð¸Ð¹ Ð±Ð¸Ð·Ð½ÐµÑ-ÑÐµÐ½ÑÑÐ°; ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½ Ð¿ÑÐ¾ÐµÐºÑ Ð¿Ð¾ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð°; Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½ÑÐµ ÑÐµÑÐµÐ½Ð¸Ñ Ð¿Ð¾ Ð¾ÑÑÐ°Ð½Ðµ Ð¾ÐºÑÑÐ¶Ð°ÑÑÐµÐ¹ ÑÑÐµÐ´Ñ, Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð¿Ð¾Ð¶Ð°ÑÐ½Ð¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð¸ Ð´Ð¾ÑÑÑÐ¿Ð° Ð¼Ð°Ð»Ð¾Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½ÑÑ Ð³ÑÑÐ¿Ð¿ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð¸Ñ; ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½ ÑÐ²Ð¾Ð´Ð½ÑÐ¹ ÑÐ¼ÐµÑÐ½ÑÐ¹ ÑÐ°ÑÑÐµÑ Ð½Ð° ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÑÐµÐ¼Ð¾Ð³Ð¾ Ð·Ð´Ð°Ð½Ð¸Ñ. Ð ÑÐ¾Ð´Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ ÐºÐ¾Ð½Ð´Ð¸ÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð²Ð¾Ð·Ð´ÑÑÐ° Ñ ÑÐ¶ÐµÐºÑÐ¸Ð¾Ð½Ð½ÑÐ¼Ð¸ Ð´Ð¾Ð²Ð¾Ð´ÑÐ¸ÐºÐ°Ð¼Ð¸, Ð¿ÑÐ¾ÑÐµÑÑ ÑÐ°Ð±Ð¾ÑÑ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¸ ÑÐ°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾ÑÑÑ ÐµÑ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ Ð¿Ð¾Ð´Ð±Ð¾Ñ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ.
A numerical investigation of the steady states of the spherically symmetric Einstein-Vlasov-Maxwell system
Creators: name: Andreasson, Hakan
name: Eklund, Mikael
name: Rein, Gerhard
Publisher: name: arXiv
Year: 2009
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We construct, by numerical means, static solutions of the spherically symmetric Einstein-Vlasov-Maxwell system and investigate various features of the solutions. This extends a previous investigation \cite{AR1} of the chargeless case. We study the possible shapes of the energy density profile as a function of the area radius when the electric charge of an individual particle is varied as a parameter. We find profiles which are multi-peaked, where the peaks are separated either by vacuum or a thin atmosphere, and we find that for a sufficiently large charge parameter there are no physically meaningful solutions. Furthermore, we investigate if the inequality \sqrt{M}\leq \frac{\sqrt{R}}{3}+\sqrt{\frac{R}{9}+\frac{Q^2}{3R}}, derived in \cite{An2}, is sharp within the class of solutions to the Einstein-Vlasov-Maxwell system. Here M is the ADM mass, Q the charge, and R the area radius of the boundary of the static object. We find two classes of solutions with this property, while there is only one in the chargeless case. In particular we find numerical evidence for the existence of arbitrarily thin shell solutions to the Einstein-Vlasov-Maxwell system. Finally, we consider one parameter families of steady states, and we find spirals in the mass-radius diagram for all examples of the microscopic equation of state which we consider.
description: 25 pages, 16 figures
An SMA Survey of Chemistry in Disks around Herbig AeBe Stars
Creators: name: Pegues, Jamila
name: Öberg, Karin I.
name: Qi, Chunhua
name: Andrews, Sean M.
name: Huang, Jane
name: Law, Charles J.
name: Gal, Romane Le
name: Matrà, Luca
name: Wilner, David J.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Protoplanetary disks around Herbig AeBe stars are exciting targets for studying the chemical environments where giant planets form. Save for a few disks, however, much of Herbig AeBe disk chemistry is an open frontier. We present a Submillimeter Array (SMA) $\sim$213-268 GHz pilot survey of mm continuum, CO isotopologues, and other small molecules in disks around five Herbig AeBe stars (HD 34282, HD 36112, HD 38120, HD 142666, and HD 144432). We detect or tentatively detect $^{12}$CO 2--1 and $^{13}$CO 2--1 from four disks; C$^{18}$O 2--1 and HCO$^+$ 3--2 from three disks; HCN 3--2, CS 5--4, and DCO$^+$ 3--2 from two disks; and C$_2$H 3--2 and DCN 3--2 from one disk each. H$_2$CO 3--2 is undetected at the sensitivity of our observations. The mm continuum images of HD 34282 suggest a faint, unresolved source $\sim$5\farcs0 away, which could arise from a distant orbital companion or an extended spiral arm. We fold our sample into a compilation of T Tauri and Herbig AeBe/F disks from the literature. Altogether, most line fluxes generally increase with mm continuum flux. Line flux ratios between CO 2--1 isotopologues are nearest to unity for the Herbig AeBe/F disks. This may indicate emitting layers with relatively similar, warmer temperatures and more abundant CO relative to disk dust mass. Lower HCO$^+$ 3--2 flux ratios may reflect less ionization in Herbig AeBe/F disks. Smaller detection rates and flux ratios for DCO$^+$ 3--2, DCN 3--2, and H$_2$CO 3--2 suggest smaller regimes of cold chemistry around the luminous Herbig AeBe/F stars.
description: 43 pages (23 pages in the main document, 20 pages in the appendix), 16 figures, 16 tables. Accepted in ApJ (February 2023)
title: ÐÐ¾ÑÑÑÐ¾ÐµÐ½Ð¸Ðµ Ð¸ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿Ð½ÐµÐ²Ð¼Ð¾ÑÐµÑÐ¸ ÐºÐ¾Ð¼Ð¿ÑÐµÑÑÐ¾ÑÐ½Ð¾Ð³Ð¾ ÑÐµÑ Ð° Ð½Ð° Ð¿ÑÐ¸ÑÐ¾Ð´Ð½Ð¾Ð¼ Ð³Ð°Ð·Ðµ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°Ð±ÐµÐ»Ð¸Ð½, ÐÐ°ÑÐº
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: ÐºÐ¾Ð¼Ð¿ÑÐµÑÑÐ¾ÑÐ½Ð°Ñ ÑÑÐ°Ð½ÑÐ¸Ñ (ÐÐ¡)
Ð¿Ð½ÐµÐ²Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐµÑÑ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¸ Ð½Ð°Ð¿Ð¸ÑÐ°Ð½Ð¸Ð¸ ÑÐ°Ð±Ð¾ÑÑ Ð¿Ð¾ÑÐ»ÑÐ¶Ð¸Ð»Ð° Ð¿Ð½ÐµÐ²Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐµÑÑ ÐºÐ¾Ð¼Ð¿ÑÐµÑÑÐ¾ÑÐ½Ð¾Ð³Ð¾ ÑÐµÑÐ°. Ð Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½ÑÑ ÑÐ°Ð±Ð¾ÑÑ Ð²ÑÐ¾Ð´Ð¸Ñ Ð²Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ, Ð¾Ð´Ð½Ð° Ð³Ð»Ð°Ð²Ð°, Ð²ÑÐ²Ð¾Ð´. ÐÐ¾ Ð²Ð²ÐµÐ´ÐµÐ½Ð¸Ð¸ Ð²Ð²Ð¾Ð´Ð¸ÑÑÑ Ð¿Ð¾Ð½ÑÑÐ¸Ðµ ÐºÐ¾Ð¼Ð¿ÑÐµÑÑÐ¾ÑÐ½Ð¾Ð¹ ÑÑÐ°Ð½ÑÐ¸Ð¸, ÐµÑ Ð³ÐµÐ¾Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ, Ð¾Ð±ÑÐ»ÑÐ¶Ð¸Ð²Ð°Ð½Ð¸Ðµ, Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ. Ð Ð³Ð»Ð°Ð²Ðµ ÑÐ°ÑÐºÑÑÐ²Ð°ÐµÑÑÑ Ð¿Ð¾Ð½ÑÑÐ¸Ðµ Ð¿Ð½ÐµÐ²Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐµÑÐ¸, Ð½Ð° ÐºÐ°ÐºÐ¸Ðµ ÑÐ¾ÑÑÐ°Ð²Ð»ÑÑÑÐ¸Ðµ Ð¾Ð½Ð° Ð´ÐµÐ»Ð¸ÑÑÑ, Ð¿ÑÐ¸Ð²Ð¾Ð´Ð¸ÑÑÑ ÑÐ°ÑÑÐµÑ ÐºÐ°Ð¶Ð´Ð¾Ð¹ ÑÐ¾ÑÑÐ°Ð²Ð»ÑÑÑÐµÐ¹ Ð¿Ð½ÐµÐ²Ð¼Ð¾ÑÐµÑÐ¸. Ð Ð²ÑÐ²Ð¾Ð´Ðµ Ð¿ÑÐ¸Ð²Ð¾Ð´Ð¸ÑÑÑ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸ Ð¾ÑÐµÐ½ÐºÐ° ÑÐ°ÑÑÐµÑÐ¾Ð², Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð¾ ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ ÑÐ°Ð±Ð¾ÑÑ ÐºÐ¾Ð¼Ð¿ÑÐµÑÑÐ¾ÑÐ½Ð¾Ð¹ ÑÑÐ°Ð½ÑÐ¸Ð¸ Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¸ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ¾ÑÐºÐ¸ Ð·ÑÐµÐ½Ð¸Ñ.
Globular cluster formation histories, masses and radii inferred from gravitational waves
Creators: name: Fishbach, Maya
name: Fragione, Giacomo
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Globular clusters (GCs) are found in all types of galaxies and harbor some of the most extreme stellar systems, including black holes that may dynamically assemble into merging binaries (BBHs). Uncertain GC properties, including when they formed, their initial masses and sizes, affect their production rate of BBH mergers. Using the gravitational-wave catalog GWTC-3, we measure that dynamically-assembled BBHs -- those that are consistent with isotropic spin directions -- make up ${61^{+29}_{-44}\%}$ of the total merger rate, with a local merger rate of ${10.9^{+16.8}_{-9.3}}$ Gpc$^{-3}$ yr$^{-1}$ rising to ${58.9^{+149.4}_{-46.0}}$ Gpc$^{-3}$ yr$^{-1}$ at $z = 1$. We assume this inferred rate describes the contribution from GCs and compare it against the Cluster Monte Carlo (CMC) simulation catalog to directly fit for the GC initial mass function, virial radius distribution, and formation history. We find that GC initial masses are consistent with a Schechter function with slope ${β_m = -1.9^{+0.8}_{-0.8}}$. Assuming a mass function slope of $β_m = -2$ and a mass range between $10^4$--$10^8\,M_\odot$, we infer a GC formation rate at $z = 2$ of ${5.0^{+9.4}_{-4.0}}$ Gpc$^{-3}$ yr$^{-1}$, or ${2.1^{+3.9}_{-1.7}}\times 10^6\,M_\odot$ Gpc$^{-3}$ yr$^{-1}$ in terms of mass density. We find that the GC formation rate probably rises more steeply than the global star formation rate between $z = 0$ and $z = 3$ ({82\%} credibility) and implies a local number density that is ${f_\mathrm{ev} = 22.6^{+29.9}_{-16.2}}$ times higher than the observed density of survived GCs. This is consistent with expectations for cluster evaporation, but may suggest that other environments contribute to the rate of BBH mergers with significantly tilted spins.
description: 7 pages + 5 pages Appendix, 9 figures. Updated to match version accepted by MNRAS
Robust Watermarking in Multiresolution Walsh-Hadamard Transform
Creators: name: Bhatnagar, Gaurav
name: Raman, Balasubramanian
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cryptography and Security (cs.CR)
subject: Information Theory (cs.IT)
subject: Multimedia (cs.MM)
subject: FOS: Computer and information sciences

description: In this paper, a newer version of Walsh-Hadamard Transform namely multiresolution Walsh-Hadamard Transform (MR-WHT) is proposed for images. Further, a robust watermarking scheme is proposed for copyright protection using MRWHT and singular value decomposition. The core idea of the proposed scheme is to decompose an image using MR-WHT and then middle singular values of high frequency sub-band at the coarsest and the finest level are modified with the singular values of the watermark. Finally, a reliable watermark extraction scheme is developed for the extraction of the watermark from the distorted image. The experimental results show better visual imperceptibility and resiliency of the proposed scheme against intentional or un-intentional variety of attacks.
description: 6 Pages, 16 Figure, 2 Tables
Dualisation of free fields
Creators: name: Abakumova, V. A.
name: Lyakhovich, S. L.
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We consider the general free field theory such that system of equations of motion includes a subsystem with a special property. If the subsystem is considered by itself, it would be a topological field theory having no local degrees of freedom. Various well-known field theories admit such a subsystem, including Einstein's gravity. As the subsystem is a topological theory, the general solution is a pure gauge, modulo global degrees of freedom. Gauge symmetry of the subsystem of linear theory can be explicitly found, providing the general solution to the subsystem. Substituting this solution into entire system, we arrive at an equivalent field theory where the role of the field variables is played by the gauge parameters of the topological subsystem. These fields can be viewed as the potentials for the original ones. A general procedure is proposed for constructing a "parent action" which includes the fields of both dual formulations. At the level of this action, one can switch between dual formulations by imposing appropriate gauge fixing conditions. This general dualisation procedure is exemplified by massless and massive spin two fields. For the massless case, the hook type tensor serves as a potential for the metric, while for the massive case it is the fourth rank tensor with window Young diagram.
description: 31 pages, minor corrections
The Stellar Mass - Black Hole Mass Relation at $z\sim2$ Down to $\mathcal{M}_\mathrm{BH}\sim10^7 M_\odot$ Determined by HETDEX
Creators: name: Zhang, Yechi
name: Ouchi, Masami
name: Gebhardt, Karl
name: Liu, Chenxu
name: Harikane, Yuichi
name: Cooper, Erin Mentuch
name: Davis, Dustin
name: Farrow, Daniel J.
name: Gawiser, Eric
name: Hill, Gary J.
name: Kollatschny, Wolfram
name: Ono, Yoshiaki
name: Schneider, Donald P.
name: Finkelstein, Steven L.
name: Gronwall, Caryl
name: Jogee, Shardha
name: Krumpe, Mirko
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We investigate the stellar mass - black hole mass ($\mathcal{M}_*-\mathcal{M}_\mathrm{BH}$) relation with type 1 AGN down to $\mathcal{M}_\mathrm{BH}=10^7 M_\odot$, corresponding to a $\simeq -21$ absolute magnitude in rest-frame ultraviolet (UV), at $z = 2-2.5$. Exploiting the deep and large-area spectroscopic survey of the Hobby-Eberly Telescope Dark Energy Experiment (HETDEX), we identify 66 type 1 AGN with $\mathcal{M}_\mathrm{BH}$ ranging from $10^7$ to $10^{10} M_\odot$ that are measured with single-epoch virial method using C{\sc iv} emission lines detected in the HETDEX spectra. $\mathcal{M}_*$ of the host galaxies are estimated from optical to near-infrared photometric data taken with Spitzer, WISE, and ground-based 4-8m class telescopes by CIGALE SED fitting. We further assess the validity of SED fitting in two cases by host-nuclear decomposition performed through surface brightness profile fitting on spatially-resolved host galaxies with JWST/NIRCam CEERS data. We obtain the $\mathcal{M}_*-\mathcal{M}_\mathrm{BH}$ relation covering the unexplored low-mass ranges of $\mathcal{M}_\mathrm{BH}~\sim~10^7-10^8~M_\odot$, and conduct forward modelling to fully account for the selection biases and observational uncertainties. The intrinsic $\mathcal{M}_*-\mathcal{M}_\mathrm{BH}$ relation at $z\sim 2$ has a moderate positive offset of $0.52\pm0.14$~dex from the local relation, suggestive of more efficient black hole growth at higher redshift even in the low-mass regime of $\mathcal{M}_\mathrm{BH}~\sim~10^7-10^8~M_\odot$. Our $\mathcal{M}_*-\mathcal{M}_\mathrm{BH}$ relation is inconsistent with the $\mathcal{M}_\mathrm{BH}$ suppression at the low-$\mathcal{M}_*$ regime predicted by recent hydrodynamic simulations at a $98\%$ confidence level, suggesting that feedback in the low-mass systems may be weaker than those produced in hydrodynamic simulations.
description: 16 pages, 8 figures, accepted for publication in ApJ
The Strategies To Develop An Interactive Learning Media Using UMU On Family Vocabulary Material
Creators: name: Gustin Hidayanti
name: Nurhidayati, Anita
Publisher: name: Zenodo
Year: 2021

description: Final exam Project by Gustin Hidayanti and Anita Nurhidayati from class A, TBI of State Islamic Institute Of Palangka Raya. This ppt discuss about the strategies to make an interactive learning using UMU flatform.
Contrôle de gestion et la bonne gouvernance dans les collectivités territoriales : Une revue de littérature
Creators: name: EL KEZAZY, Hamza
Publisher: name: Zenodo
Year: 2022

description: Cette étude explore l'impact de l'adoption d'outils de gestion du secteur privé sur la gouvernance des organisations publiques, en se concentrant sur les collectivités territoriales. En intégrant des concepts tels que le contrôle de gestion, le nouveau management public et la bonne gouvernance, l'objectif est de comprendre dans quelle mesure le contrôle de gestion territorial contribue à améliorer la gouvernance des collectivités territoriales.

S'inscrivant dans le domaine des Sciences de Gestion, l'étude met en lumière le concept de bonne gouvernance, promu par des initiatives internationales. L’article explore les évolutions en cours, interrogeant la persistance des spécificités des organisations publiques par rapport aux entreprises privées.
Study on the weak decay between two heavy baryons $ \mathcal{B}_i(\frac{1}{2}^+)\to \mathcal{B}_f(\frac{3}{2}^+)$ in the light-front quark model
Creators: name: Lu, Fang
name: Ke, Hong-Wei
name: Liu, Xiao-Hai
name: Shi, Yan-Liang
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: In this work, we study the weak decay between two heavy baryons $ \mathcal{B}_i(\frac{1}{2}^+)\to \mathcal{B}_f(\frac{3}{2}^+)$ in the light-front quark model where three-quark picture is employed for baryon. We derive general form of transition amplitude of $ \mathcal{B}_i(\frac{1}{2}^+)\to \mathcal{B}_f(\frac{3}{2}^+)$, and analyze two specific cases of transitions: the weak decays of single heavy baryon $Σ_{b} \to Σ_{c}^*$ and the decays of double-charmed baryon $Ξ_{cc}\to Σ_{c}^*(Ξ_{c}^*)$. We compute the hadronic form factors for the transitions and apply them to study the decay widths of the semi-leptonic $\mathcal B_i(\frac{1}{2}^+)\to\mathcal B_f(\frac{3}{2}^+) l\barν_l$ and non-leptonic $\mathcal B_i(\frac{1}{2}^+)\to\mathcal B_f(\frac{3}{2}^+)M$. Previously we studied the transition $Σ_{b} \to Σ_{c}^*$ with the quark-diquark picture of baryon in the light-front quark model. Here we revisit this transition with three-quark picture of baryon. At the quark level, the transition $Σ_{b} \to Σ_{c}^*$ is induced by the $b\rightarrow c$ transition.The subsystem of the two unchanged light quarks which possesses definite and same spin in initial and final state can be viewed as a spectator, so the spectator approximation can be applied directly. For the weak decay of doubly charmed baryon $Ξ_{cc}$, a $c$ quark decays to a light quark $q_1$, so both the initial state $cc$ and final state $q_1q_2$ ($q_1$ and the original $q_2$ in initial state may be the same flavor quarks) which possess definite spin are no longer spectators. A rearrangement of quarks for initial and final states is adopted to isolate the unchanged subsystem $cq_2$ which can be viewed as the spectator approximately. Future measurements on these channels will constrain the nonperturbative parameter in the wavefunctions and test the model predictions.
description: 20 pages, 6 figures and 10 tables
title: Exploration of prescribing patterns of benzodiazepine and non-benzodiazepine (Zdrugs) medications in the management of primary insomnia in adults in Saudi Arabia
Creators: name: Dobia, Ali Mohammed A.
Publisher: name: University of Reading
Year: 2019

description: Background: Despite the increasing use of benzodiazepines and Z-drugs for insomnia, there are no guidelines for their use nor data on prescribing patterns in the Kingdom of Saudi Arabia (KSA). Aim: To explore the prescribing practices for treating insomnia in the KSA and begin the development of national guidelines, taking into account patients’ perspectives. Method: A mixed methods design was used in four phases. First, a retrospective audit of patients prescribed benzodiazepines or Z-drugs for insomnia (April 2012–March 2017) in King Fahad Central Hospital, Jazan, KSA, based on two US guidelines, was performed. Descriptive statistics, using Stata, were used to report findings. Second, a qualitative study, using NVivo, of physicians’ knowledge, perceptions and attitudes regarding treating primary insomnia and using US guidelines was performed. Third, an e-Delphi technique was used for guideline development. Twenty-seven insomnia experts participated in developing the consensus (≥ 80% agreement) around future national guidelines. Fourth, a cross-sectional survey (unrestricted, self-selected online survey) was utilised to explore patients’ knowledge, experiences and perceptions about using hypnotics to manage primary insomnia in the KSA. The data were encoded and analysed using Stata. Results: Of the 504 records reviewed, 379 patients (75%) were prescribed benzodiazepines or Z-drugs; only 182 (48%) had documented diagnoses. Of the 307 patients (60%) diagnosed with insomnia, none received cognitive behavioural therapy for insomnia (CBT-I). No patients were reviewed by physicians for long-term use. No records met all criteria. Physicians’ perceptions and attitudes in KSA toward using US or other international guidelines were based on knowledge, resistance and the presence of barriers and facilitators. In the Delphi study, sixteen 4 statements achieved the consensus to be included in future KSA guidelines. The survey study revealed that patients have limited knowledge of insomnia and its treatment. Patients are often prescribed hypnotics for insomnia, do not receive CBT-I as first-line treatment, and are rarely involved in treatment decisions. Most patients are on long-term hypnotics use and are not reviewed regularly by their doctors or provided with a plan for discontinuation. There is considerable resistance among patients to using nonpharmacological treatment options for insomnia. Conclusion: The Ministry of Health should enhance public awareness of insomnia, provide training for physicians on prescribing hypnotics and CBT-I, improve hospital administration and encourage documentation. The produced consensus statements can be used, taking into consideration patients’ perspectives, in the development of national guidelines that will standardise the use of benzodiazepines and Z-drugs for the treatment of primary insomnia in adults in the KSA.
title: ÐÐ°Ð´ÑÐ¾Ð²Ð°Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ° Ð² Ð¾ÑÐ³Ð°Ð½Ð°Ñ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¸ Ð¼ÑÐ½Ð¸ÑÐ¸Ð¿Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÑÐ´ÑÐ¾Ð²Ð°, ÐÐ»ÐµÐ½Ð°
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2017
Subjects: ÐºÐ°Ð´ÑÐ¾Ð²Ð°Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ°
Ð¾ÑÐ³Ð°Ð½Ñ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ
Ð¾ÑÐ³Ð°Ð½Ñ Ð¼ÑÐ½Ð¸ÑÐ¸Ð¿Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

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title: Ð¢ÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ Ð¿Ð¾Ð»ÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¸ÐºÐ¾Ð²Ð¾Ð¹ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ¸
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ»ÑÐ¸Ð½, ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
Publisher: name: [ÐÐÐ]
Year: 1979
Subjects: ÐÐ¾Ð»ÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¸ÐºÐ¾Ð²ÑÐµ Ð¿ÑÐ¸Ð±Ð¾ÑÑ

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Recent Evidence for Convection in Sunspot Penumbrae
Creators: name: Scharmer, G. B.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Whereas penumbral models during the last 15 years have been successful in explaining Evershed flows and magnetic field inclination variations in terms of flux tubes, the lack of contact between these models and a convective process needed to explain the penumbral radiative heat flux has been disturbing. We report on recent observational and theoretical evidence that challenge flux tube interpretations and conclude that the origin of penumbral filamentary structure is overturning convection.
description: Accepted for publication in Space Science Reviews
Additional file 3 of Granulocyte-colony stimulating factor gene therapy as a novel therapeutics for stroke in a mouse model
Creators: name: Menzie-Suderam, Janet M.
name: Modi, Jigar
name: Xu, Hongyaun
name: Bent, Andrew
name: Trujillo, Paula
name: Medley, Kristen
name: Jimenez, Eugenia
name: Shen, Jessica
name: Marshall, Michael
name: Tao, Rui
name: Prentice, Howard
name: Wu, Jang-Yen
Publisher: name: figshare
Year: 2020
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Neuroscience
subject: Physiology
subject: Biological Sciences not elsewhere classified
subject: Science Policy
subject: Hematology

description: Additional file 3: Table S1. List of Antibodies used for Western Blotting