cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The survey of planetary nebulae in Andromeda (M31) VI. Kinematics of M31 inner-halo substructures and comparison with major-merger simulation predictions
Creators: name: Bhattacharya, Souradeep
name: Arnaboldi, Magda
name: Hammer, Francois
name: Yang, Yanbin
name: Gerhard, Ortwin
name: Caldwell, Nelson
name: Freeman, Kenneth C.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: M31 has experienced a recent tumultuous merger history as evidenced from the many substructures that are still present in its inner halo, particularly the G1-Clump, NE- and W- shelves, and the Giant Stream (GS). We present planetary nebulae (PNe) line-of-sight velocity (LOSV) measurements covering the entire spatial extent of these four substructures. We further use predictions for the satellite and host stellar particle phase space distributions for a major merger (mass ratio = 1:4) simulation to help interpret the data. The measured PN LOSVs for the two shelves and GS are consistent with those from red giant branch stars. Their projected radius vs. LOSV phase space, links the formation of these substructures in a single unique event, consistent with a major merger. We find the G1-clump to be dynamically cold compared to the M31 disc ($\rmσ_{LOS, PN}=27$ km s$^{-1}$), consistent with pre-merger disc material. Such a structure can not form in a minor merger (mass ratio $\sim$1:20), and is therefore a smoking gun for the recent major merger event in M31. The simulation also predicts the formation of a predominantly in-situ halo from splashed-out pre-merger disc material, in qualitative agreement with observations of a metal-rich inner halo in M31. Juxtaposed with previous results for its discs, we conclude that M31 has had a recent (2.5 - 4 Gyr ago) `wet' major merger with the satellite falling along the GS, heating the pre-merger disc to form the M31 thicker disc, rebuilding the M31 thin disc, and creating the aforementioned inner-halo substructures.
description: 14 pages, 10 figures, 3 tables, accepted for publication at MNRAS
Additional file 1 of Frailty and its combined effects with lifestyle factors on cognitive function: a cross-sectional study
Creators: name: Li, Fangqing
name: Yan, Yike
name: Zheng, Lei
name: Wang, Chenming
name: Guan, Xin
name: Hong, Shiru
name: Guo, Huan
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Neuroscience
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Mental Health

description: Additional file 1: Figure S1. Flow chart of the study. Table S1. Factors used for frailty index calculation. Figure S2. Stratified analysis for the association of frailty status with cognitive impairment.
Environment and self-regulation in galaxy formation
Creators: name: Thomas, Daniel
name: Maraston, Claudia
name: Schawinski, Kevin
name: Sarzi, Marc
name: Silk, Joseph
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The environment is known to affect the formation and evolution of galaxies considerably best visible through the well-known morphology-density relationship. In this paper we study the effect of environment on the evolution of early-type galaxies by analysing the stellar population properties of 3,360 galaxies morphologically selected by visual inspection from the SDSS in the redshift range 0.05
description: MNRAS, accepted. Galaxy catalogue online at http://www.icg.port.ac.uk/~thomasd
title: Ð¡Ð¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ "Ð¥Ð»ÐµÐ±Ð¾Ð¿ÑÐº")
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾ÑÑÑ, ÐÐ°ÑÐ°Ð»ÑÑ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÑÑÑÐ°ÑÐµÐ³Ð¸Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼
ÐºÐ°Ð´ÑÐ¾Ð²Ð°Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ°
ÑÐµÐºÑÑÐµÑÑÑ ÐºÐ°Ð´ÑÐ¾Ð²
Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð° Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¸ Ð¾ÑÐµÐ½ÐºÐ¸ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÑÐ»ÐµÐ±Ð¾Ð¿ÐµÐºÐ°ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÐÐÐ Â«Ð¥Ð»ÐµÐ±Ð¾Ð¿ÑÐºÂ». Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ñ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸, ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸Ð·ÑÑÑÐ¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼, Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð½ÐµÐ´Ð¾ÑÑÐ°ÑÐºÐ¸ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ Ð¸Ñ ÑÑÑÑÐ°Ð½ÐµÐ½Ð¸Ñ. ÐÐ°Ð½Ð¾ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹.
Bursts from Space: MeerKAT - The first citizen science project dedicated to commensal radio transients
Creators: name: Andersson, Alex
name: Lintott, Chris
name: Fender, Rob
name: Bright, Joe
name: Carotenuto, Francesco
name: Driessen, Laura
name: Espinasse, Mathilde
name: Gaseahalwe, Kelebogile
name: Heywood, Ian
name: van der Horst, Alexander J.
name: Motta, Sara
name: Rhodes, Lauren
name: Tremou, Evangelia
name: Williams, David R. A.
name: Woudt, Patrick
name: Zhang, Xian
name: Bloemen, Steven
name: Groot, Paul
name: Vreeswijk, Paul
name: Giarratana, Stefano
name: Saikia, Payaswini
name: Andersson, Jonas
name: Arroyo, Lizzeth Ruiz
name: Baert, Loïc
name: Baumann, Matthew
name: Domainko, Wilfried
name: Eschweiler, Thorsten
name: Forsythe, Tim
name: Gaudenzi, Sauro
name: Grenier, Rachel Ann
name: Iannone, Davide
name: Lahoz, Karla
name: Melville, Kyle J.
name: Nascimento, Marianne De Sousa
name: Navarro, Leticia
name: Parthasarathi, Sai
name: Piilonen
name: Rahman, Najma
name: Smith, Jeffrey
name: Stewart, B.
name: Temoke, Newton
name: Tworek, Chloe
name: Whittle, Isabelle
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: The newest generation of radio telescopes are able to survey large areas with high sensitivity and cadence, producing data volumes that require new methods to better understand the transient sky. Here we describe the results from the first citizen science project dedicated to commensal radio transients, using data from the MeerKAT telescope with weekly cadence. Bursts from Space: MeerKAT was launched late in 2021 and received ~89000 classifications from over 1000 volunteers in 3 months. Our volunteers discovered 142 new variable sources which, along with the known transients in our fields, allowed us to estimate that at least 2.1 per cent of radio sources are varying at 1.28 GHz at the sampled cadence and sensitivity, in line with previous work. We provide the full catalogue of these sources, the largest of candidate radio variables to date. Transient sources found with archival counterparts include a pulsar (B1845-01) and an OH maser star (OH 30.1-0.7), in addition to the recovery of known stellar flares and X-ray binary jets in our observations. Data from the MeerLICHT optical telescope, along with estimates of long time-scale variability induced by scintillation, imply that the majority of the new variables are active galactic nuclei. This tells us that citizen scientists can discover phenomena varying on time-scales from weeks to several years. The success both in terms of volunteer engagement and scientific merit warrants the continued development of the project, whilst we use the classifications from volunteers to develop machine learning techniques for finding transients.
description: Accepted to MNRAS, 14 pages + an appendix containing our main data table
Hexadecapole strength in the rare isotopes $^{74,76}$Kr
Creators: name: Spieker, M.
name: Agbemava, S. E.
name: Bazin, D.
name: Cottle, S. Biswas P. D.
name: Farris, P. J.
name: Gade, A.
name: Ginter, T.
name: Giraud, S.
name: Kemper, K. W.
name: Li, J.
name: Nazarewicz, W.
name: Noji, S.
name: Pereira, J.
name: Riley, L. A.
name: Smith, M.
name: Weisshaar, D.
name: Zegers, R. G. T.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: In the Ge-Sr mass region, isotopes with neutron number $N \leq 40$ are known to feature rapid shape changes with both nucleon number and angular momentum. To gain new insights into their structure, inelastic proton scattering experiments in inverse kinematics were performed on the rare isotopes $^{74,76}$Kr. This work focuses on observables related to the $J^π = 4^+_1$ states of the Kr isotopes and, in particular, on the hexadecapole degree of freedom. By performing coupled-channels calculations, hexadecapole deformation parameters $β_4$ were determined for the $J^π = 4^+_1$ states of $^{74,76}$Kr from inelastic proton scattering cross sections. Two possible coupled-channels solutions were found. A comparison to predictions from nuclear energy density functional theory, employing both non-relativistic and relativistic functionals, clearly favors the large, positive $β_4$ solutions. These $β_4$ values are unambiguously linked to the well deformed prolate configuration. Given the $β_2 - β_4$ trend, established in this work, it appears that $β_4$ values could provide a sensitive measure of the nuclear shell structure.
description: 7 pages, 4 figures, accepted for publication in Physics Letters B
title: ÐÐµÑÐ°ÑÐ¸ÑÐ½Ð¾Ðµ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ. Ð§. 4, Ð¢Ð¾Ð²Ð°ÑÑ, Ð¿ÐµÑÐµÐ¼ÐµÑÐµÐ½Ð¸Ðµ ÐºÐ¾ÑÐ¾ÑÑÑ ÑÐµÑÐµÐ· ÑÐ°Ð¼Ð¾Ð¶ÐµÐ½Ð½ÑÑ Ð³ÑÐ°Ð½Ð¸ÑÑ Ð¢Ð°Ð¼Ð¾Ð¶ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ¾ÑÐ·Ð° ÑÐµÐ³ÑÐ»Ð¸ÑÑÐµÑÑÑ Ð½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐ¼ Ð·Ð°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÑÑÐ²Ð¾Ð¼
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ°ÑÑÑÐºÐ¸Ð½, ÐÐ²Ð³ÐµÐ½Ð¸Ð¹
name: ÐÑÐ»ÐµÑÐ¾Ð², ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
name: ÐÐ°Ð¹ÑÑÑÐ´Ð¸Ð½Ð¾Ð², Ð.
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2012
Subjects: ÑÐ°Ð¼Ð¾Ð¶ÐµÐ½Ð½ÑÐµ Ð¿ÑÐ°Ð²Ð¸Ð»Ð°
ÑÐ°Ð¼Ð¾Ð¶ÐµÐ½Ð½ÑÐ¹ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ
Ð²Ð½ÐµÑÐ½ÑÑ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ñ
Ð²Ð½ÐµÑÐ½ÐµÑÐ¾ÑÐ³Ð¾Ð²ÑÐµ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¸
Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ðµ ÑÐ°Ð¼Ð¾Ð¶ÐµÐ½Ð½Ð¾Ðµ Ð¿ÑÐ°Ð²Ð¾
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Â«ÐÐµÑÐ°ÑÐ¸ÑÐ½Ð¾Ðµ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸ÐµÂ» ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Â«ÐÐ¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ Ð¸ Ð¼ÑÐ½Ð¸ÑÐ¸Ð¿Ð°Ð»ÑÐ½Ð¾Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÐµÂ» (Ð¿ÑÐ¾ÑÐ¸Ð»Ñ Â«ÐÐ¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐ°Ð¼Ð¾Ð¶ÐµÐ½Ð½ÑÐ¼Ð¸ Ð¿ÑÐ¾ÑÐµÑÑÐ°Ð¼Ð¸Â»). Ð ÑÐ°Ð·Ð´ÐµÐ»Ð°Ñ ÑÑÐµÐ±Ð½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð¼ÐµÑ Ð½ÐµÑÐ°ÑÐ¸ÑÐ½Ð¾Ð³Ð¾ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ, Ð·Ð°Ð¿ÑÐµÑÐ¾Ð² Ð¸ Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð¸Ð¹ Ð²Ð¾ Ð²Ð½ÐµÑÐ½ÐµÑÐ¾ÑÐ³Ð¾Ð²ÑÑ Ð¾Ð¿ÐµÑÐ°ÑÐ¸ÑÑ, Ð¿Ð¾ÑÑÐ´Ð¾Ðº Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ ÑÐ°Ð·ÑÐµÑÐ¸ÑÐµÐ»ÑÐ½ÑÑ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ¾Ð², Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÑ Ð´Ð»Ñ Ð¿Ð¾Ð¼ÐµÑÐµÐ½Ð¸Ñ ÑÐ¾Ð²Ð°ÑÐ¾Ð² Ð¿Ð¾Ð´ ÑÐ°Ð¼Ð¾Ð¶ÐµÐ½Ð½ÑÐµ Ð¿ÑÐ¾ÑÐµÐ´ÑÑÑ Ð¸ Ð¿Ð¾Ð´Ð¿Ð°Ð´Ð°ÑÑÐ¸Ñ Ð¿Ð¾Ð´ Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð¸Ñ, Ð¿Ð¾ÑÑÐ´Ð¾Ðº Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ ÑÐ°Ð¼Ð¾Ð¶ÐµÐ½Ð½ÑÑ Ð¾ÑÐ³Ð°Ð½Ð¾Ð² Ñ ÐºÐ¾Ð¼Ð¿ÐµÑÐµÐ½ÑÐ½ÑÐ¼Ð¸ Ð¾ÑÐ³Ð°Ð½Ð°Ð¼Ð¸ ÑÐµÐ´ÐµÑÐ°Ð»ÑÐ½Ð¾Ð¹ Ð¸ÑÐ¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð²Ð»Ð°ÑÑÐ¸ Ð¿ÑÐ¸ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ð¸ Ð·Ð°Ð¿ÑÐµÑÐ¾Ð² Ð¸ Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð¸Ð¹. ÐÐ¾Ð´Ð¾Ð±ÑÐ°Ð½Ð½ÑÐµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ Ð¿Ð¾Ð»ÑÑÐ¸ÑÑ Ð¿Ð¾Ð»Ð½Ð¾Ðµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¾ ÑÐ¸ÑÑÐµÐ¼Ðµ Ð·Ð°Ð¿ÑÐµÑÐ¾Ð² Ð¸ Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð¸Ð¹ Ð²Ð¾ Ð²Ð½ÐµÑÐ½ÐµÐ¹ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ðµ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¾Ð± Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÑÑ ÑÐ¾Ð²ÐµÑÑÐµÐ½Ð¸Ñ ÑÐ°Ð¼Ð¾Ð¶ÐµÐ½Ð½ÑÑ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¹ Ð² Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ð¸ ÑÐ¾Ð²Ð°ÑÐ¾Ð², Ð¿Ð¾Ð´Ð¿Ð°Ð´Ð°ÑÑÐ¸Ñ Ð¿Ð¾Ð´ Ð·Ð°Ð¿ÑÐµÑÑ Ð¸ Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð¸Ñ, Ð¿ÑÐ¸ Ð¸Ñ Ð¿ÐµÑÐµÐ¼ÐµÑÐµÐ½Ð¸Ð¸ ÑÐµÑÐµÐ· ÑÐ°Ð¼Ð¾Ð¶ÐµÐ½Ð½ÑÑ Ð³ÑÐ°Ð½Ð¸ÑÑ Ð¢Ð°Ð¼Ð¾Ð¶ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ¾ÑÐ·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°.
Kinematics of stellar substructures in the Small Magellanic Cloud
Creators: name: Youssoufi, Dalal El
name: Cioni, Maria-Rosa L.
name: Kacharov, Nikolay
name: Bell, Cameron P. M.
name: Matijević, Gal
name: Bekki, Kenji
name: de Grijs, Richard
name: Ivanov, Valentin D.
name: van Loon, Jacco Th.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a kinematic analysis of the Small Magellanic Cloud using 3700 spectra extracted from the European Southern Observatory archive. We used data from Gaia and near-infrared photometry to select stellar populations and discard Galactic foreground stars. The sample includes main-sequence, red giant branch and red clump stars, observed with the Fibre Large Array Multi Wavelength Spectrograph. The spectra have a resolving power lambda/Delta(lambda) from 6500 to 38000. We derive radial velocities by employing a full spectrum fitting method using a penalised pixel fitting routine. We obtain a mean radial velocity for the galaxy of 159+/-2 km/s, with a velocity dispersion of 33+/-2 km/s. Our velocities agree with literature estimates for similar (young or old) stellar populations. The radial velocity of stars in the Wing and bar-like structure differ as a consequence of the dynamical interaction with the Large Magellanic Cloud. The higher radial velocity of young main-sequence stars in the bar compared to that of supergiants can be attributed to star formation around 40 Myr ago from gas already influenced by tidal stripping. Similarly, young main-sequence stars in the northern part of the bar, resulting from a prominent episode 25 Myr ago, have a higher radial velocity than stars in the southern part. Radial velocity differences between the northern and southern bar over densities are also traced by giant stars. They are corroborated by studies of the cold gas and proper motion indicating stretching/tidal stripping of the galaxy.
description: 18 pages, 13 figures, accepted for publication in MNRAS
Additional file 6 of Increased expression of miR-194-5p through the circPVRL3/miR-194-5p/SOCS2 axis promotes proliferation and metastasis in pancreatic ductal adenocarcinoma by activating the PI3K/AKT signaling pathway
Creators: name: Chi, Bojing
name: Zheng, Yao
name: Xie, Fuming
name: Fu, Wen
name: Wang, Xianxing
name: Gu, Jianyou
name: Yang, Jiali
name: Yin, Jingyang
name: Cai, Lei
name: Tang, Peng
name: Li, Jianbo
name: Guo, Shixiang
name: Wang, Huaizhi
Publisher: name: figshare
Year: 2023
Subjects: subject: Biophysics
subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer

description: Additional file 6. Same as Figure S4. Uncropped original western blots.
Space Assets: International synergies for resilient communities and ecosystems
Creators: name: Mantas, V.
Publisher: name: Zenodo
Year: 2021

description: Presentation given at the 'Ciência 2019' conference, at the session promoted by UT Austin Portugal (Enhancing international collaboration in R&D to address major societal challenges – the UT Austin Portugal Program). The presentation summarizes the use of remote sensing tools to rack disturbances in forests. Results obtained in the monitoring of Pinewood Nematode during Project FOCUS are discussed.
Evidence of a lepto-hadronic two-zone emission in flare states
Creators: name: Aguilar-Ruiz, E.
name: Fraija, N.
name: ámez, A. Galván-G
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The BL Lac Markarian 501 exhibited two flaring activities in the very-high-energy (VHE) band in May 2009. The lack of correlation between X-rays and TeV gamma-rays without increasing in other bands suggested that more than one emission zone could be involved. Moreover, fast variability in the flaring state was observed, indicating that the emission zones responsible must have small sizes. We use a lepto-hadronic model with two-zone emission to explain the spectral energy distribution during quiescent and these flaring states. In the proposed scenario, the photopion processes explain the VHE flaring activities successfully, and variability constraints place the activity in a zone located near the jet's base or named inner blob, while synchrotron self-Compton emission describing the X-ray signature during that flaring state occurs in the zone situated far the central engine or named outer blob.
description: Accepted in The European Physical Journal C
Interacting galaxies in the IllustrisTNG simulations -- V: Comparing the influence of star-forming vs. passive companions
Creators: name: Brown, Westley
name: Patton, David R.
name: Ellison, Sara L.
name: Faria, Lawrence
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We study interacting galaxy pairs in the TNG100-1 and TNG300-1 cosmological simulations using previously generated closest companion samples. We study the specific star formation rates (sSFR) of massive ($10^{10} M_{\odot} < M_* < 10^{12} M_{\odot}$) galaxies at $z \leq 0.2$ as a function of separation from the closest companion galaxy. We split our sample based on whether the companion galaxy is star-forming or passive. We find that galaxies with close star-forming companions have sSFRs that are enhanced (on average) by a factor of $2.9 \pm 0.3$ in TNG100-1 and $2.27 \pm 0.06$ in TNG300-1 compared to controls, with enhancements present out to separations of $\sim 300$ kpc. Galaxies with passive companions in TNG300-1 exhibit mild sSFR suppression ($\sim12$ percent) at 100-300 kpc and small sSFR enhancements at separations below 50 kpc. sSFR suppression is strongest in pairs where the galaxy's stellar mass is more than 2 times that of its passive companion. By generating a stellar mass-matched ("twinned") sample in TNG300-1, we show that differences in sSFR trends between companion types are not a result of intrinsic stellar mass differences in star-forming vs. passive galaxies. We compare with an analogous sample of galaxy pairs from SDSS, finding consistent results between observations and simulations. Overall, we find that star-forming galaxies show enhanced sSFRs regardless of companion type, but that galaxies with close passive companions are more likely to be passive themselves.
description: 16 pages, 12 figures. Accepted for publication in MNRAS
A heat-wave of accretion energy traced by masers in the G358-MM1 high-mass protostar
Creators: name: Burns, R. A.
name: Sugiyama, K.
name: Hirota, T.
name: Kim, Kee-Tae
name: Sobolev, A. M.
name: Stecklum, B.
name: MacLeod, G. C.
name: Yonekura, Y.
name: Olech, M.
name: Orosz, G.
name: Ellingsen, S. P.
name: Hyland, L.
name: Garatti, A. Caratti o
name: Brogan, C.
name: Hunter, T. R.
name: Phillips, C.
name: Heever, S. P. van den
name: Eislöffel, J.
name: Linz, H.
name: Surcis, G.
name: Chibueze, J. O.
name: Baan, W.
name: Kramer, B.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: High-mass stars are thought to accumulate much of their mass via short, infrequent bursts of disk-aided accretion. Such accretion events are rare and difficult to observe directly but are known to drive enhanced maser emission. In this Letter we report high-resolution, multi-epoch methanol maser observations toward G358.93-0.03 which reveal an interesting phenomenon; the sub-luminal propagation of a thermal radiation "heat-wave" emanating from an accreting high-mass proto-star. The extreme transformation of the maser emission implies a sudden intensification of thermal infrared radiation from within the inner (40 mas, 270 au) region. Subsequently, methanol masers trace the radial passage of thermal radiation through the environment at $\geq$ 4-8\% the speed of light. Such a high translocation rate contrasts with the $\leq$ 10 km s$^{-1}$ physical gas motions of methanol masers typically observed using very long baseline interferometry (VLBI). The observed scenario can readily be attributed to an accretion event in the high-mass proto-star G358.93-0.03-MM1. While being the third case in its class, G358.93-0.03-MM1 exhibits unique attributes hinting at a possible `zoo' of accretion burst types. These results promote the advantages of maser observations in understanding high-mass star formation, both through single-dish maser monitoring campaigns and via their international cooperation as VLBI arrays.
description: Published in Nature Astronomy in 2020
Additional file 3 of Male and female mice display consistent lifelong ability to address potential life-threatening cues using different post-threat coping strategies
Creators: name: Liu, Xue
name: Feng, Xiaolong
name: Huang, Hongren
name: Huang, Kang
name: Xu, Yang
name: Ye, Shuwei
name: Tseng, Yu-Ting
name: Wei, Pengfei
name: Wang, Liping
name: Wang, Feng
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Neuroscience
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Ecology
subject: Mental Health

description: Additional file 3: Figure S2. There were no sex and estrus-phase differences in auditory-induced defensive behavior.
A Keplerian disk with a four-arm spiral birthing an episodically accreting high-mass protostar
Creators: name: Burns, R. A.
name: Uno, Y.
name: Sakai, N.
name: Blanchard, J.
name: Rosli, Z.
name: Orosz, G.
name: Yonekura, Y.
name: Tanabe, Y.
name: Sugiyama, K.
name: Hirota, T.
name: Kim, Kee-Tae
name: Aberfelds, A.
name: Volvach, A. E.
name: Bartkiewicz, A.
name: Garatti, A. Caratti o
name: Sobolev, A. M.
name: Stecklum, B.
name: Brogan, C.
name: Phillips, C.
name: Ladeyschikov, D. A.
name: Johnstone, D.
name: Surcis, G.
name: MacLeod, G. C.
name: Linz, H.
name: Chibueze, J. O.
name: Brand, J.
name: Eislöffel, J.
name: Hyland, L.
name: Uscanga, L.
name: Olech, M.
name: Durjasz, M.
name: Bayandina, O.
name: Breen, S.
name: Ellingsen, S. P.
name: Heever, S. P. van den
name: Hunter, T. R.
name: Chen, X.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: High-mass protostars (M$_{\star} >$ 8 M$_{\odot}$) are thought to gain the majority of their mass via short, intense bursts of growth. This episodic accretion is thought to be facilitated by gravitationally unstable and subsequently inhomogeneous accretion disks. Limitations of observational capabilities, paired with a lack of observed accretion burst events has withheld affirmative confirmation of the association between disk accretion, instability and the accretion burst phenomenon in high-mass protostars. Following its 2019 accretion burst, a heat-wave driven by a burst of radiation propagated outward from the high-mass protostar G358.93-0.03-MM1. Six VLBI (very long baseline interferometry) observations of the raditively pumped 6.7 GHz methanol maser were conducted during this period, tracing ever increasing disk radii as the heat-wave propagated outward. Concatenating the VLBI maps provided a sparsely sampled, milliarcsecond view of the spatio-kinematics of the accretion disk covering a physical range of $\sim$ 50 - 900 AU. We term this observational approach `heat-wave mapping'. We report the discovery of a Keplerian accretion disk with a spatially resolved four-arm spiral pattern around G358.93-0.03-MM1. This result positively implicates disk accretion and spiral arm instabilities into the episodic accretion high-mass star formation paradigm.
description: Published in Nature Astronomy in 2023
Anomalous Hall effect and magnetic structure of the topological semimetal (Mn$_{0.78}$Fe$_{0.22}$)$_{3}$Ge
Creators: name: Rai, Venus
name: Stunault, Anne
name: Schmidt, Wolfgang
name: Jana, Subhadip
name: Perßon, Jörg
name: Brückel, Thomas
name: Nandi, Shibabrata
Publisher: name: arXiv
Year: 2023
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Me$_{3+δ}$Ge, being a Weyl semimetal, shows a large anomalous Hall effect (AHE), which decreases slowly with an increase in $δ$ from 0.1 to 0.4. However, AHE in this compound remains significantly large in the whole range of $δ$ because of the robust nature of the topology of bands. To explore the possibility of tuning the anomalous transport effects in Weyl semimetals, we have studied the single-crystal hexagonal-(Mn$_{0.78}$Fe$_{0.22}$)$_3$Ge compound. Magnetization of this compound shows two magnetic transitions at 242 K ($T_{\text{N1}}$) and 120 K ($T_{\text{N2}}$). We observed that the AHE persists between $T_{\text{N2}}$ - $T_{\text{N1}}$ and vanishes below $T_{\text{N2}}$. Further, we performed single-crystal neutron diffraction experiments (using spherical neutron polarimetry and unpolarized neutron diffraction) to determine the magnetic structures of (Mn$_{0.78}$Fe$_{0.22}$)$_3$Ge at different temperatures. Our neutron diffraction results show that the sample possesses a collinear antiferromagnetic structure below $T_{\text{N2}}$. However, the magnetic structure of the sample remains noncollinear antiferromagnetic, the same as Mn$_3$Ge, between $T_{\text{N1}}$ to $T_{\text{N2}}$. The presence of AHE, and noncollinear magnetic structure in (Mn$_{0.78}$Fe$_{0.22}$)$_3$Ge, between $T_{\text{N1}}$ and $T_{\text{N2}}$, suggest the existence of Weyl points in this temperature regime. Below $T_{\text{N2}}$, AHE is absent, and the magnetic structure also changes to a collinear antiferromagnetic structure. These observations signify a strong link between the magnetic structure of the sample and AHE.
description: Accepted in Physical Review B
Invariant Representations in Deep Learning for Optoacoustic Imaging
Creators: name: Vera, Matias
name: Gonzalez, Martin G.
name: Vega, Leonardo Rey
Publisher: name: arXiv
Year: 2023
Subjects: subject: Image and Video Processing (eess.IV)
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: 68T07, 78A46

description: Image reconstruction in optoacoustic tomography (OAT) is a trending learning task highly dependent on measured physical magnitudes present at sensing time. The large number of different settings, and also the presence of uncertainties or partial knowledge of parameters, can lead to reconstructions algorithms that are specifically tailored and designed to a particular configuration which could not be the one that will be ultimately faced in a final practical situation. Being able to learn reconstruction algorithms that are robust to different environments (e.g. the different OAT image reconstruction settings) or invariant to such environments is highly valuable because it allows to focus on what truly matters for the application at hand and discard what are considered spurious features. In this work we explore the use of deep learning algorithms based on learning invariant and robust representations for the OAT inverse problem. In particular, we consider the application of the ANDMask scheme due to its easy adaptation to the OAT problem. Numerical experiments are conducted showing that, when out-of-distribution generalization (against variations in parameters such as the location of the sensors) is imposed, there is no degradation of the performance and, in some cases, it is even possible to achieve improvements with respect to standard deep learning approaches where invariance robustness is not explicitly considered.
description: paper accepted for publication in Review Scientific Instruments
Spontaneous magnetization of a vacuum in high temperature gluodynamics (two-loop approximation
Creators: name: Skalozub, V.
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In SU(N) gluodynamics, at high temperature the spontaneous magnetization, b(T) not equal to 0, of a vacuum happens in the approximation to the effective potential - the tree plus the one-loop, plus daisy diagrams, W(b)= b^2/2 g^2 + W^(1)(b) + W^(daisy)(b). At the same time, in two-loop approximation, W(A_0)= W^(1)(A_0) + W^(2)(A_0), other classical field - A_0 condensate directly related to the Polyakov loop - is also spontaneously generated. To investigate the creation of the condensates together, the two loop effective potential of both fields should be calculated. This program was realized recently for SU(2) in [1]. However, the generation of magnetic field in two-loop order was not studied in detail. In the present paper, we compute the value of chromomagnetic field b(T) for latter case. Then, considering the spectrum of color charged gluons at the background of both condensates, we conclude that the A_0 stabilizes the magnetized vacuum at high temperature. This is in agreement with the lattice simulations carried out already and clarifies the mechanism of the magnetic field stabilization. Key words: condetsation, high temperature, gluodynamics, A0 condensate, spontaneous magnetization, vacuum
description: arXiv admin note: text overlap with arXiv:2112.01043
Magnetic order and dynamics of the charge-ordered antiferromagnet La1.5Sr0.5CoO4
Creators: name: Helme, L. M.
name: Boothroyd, A. T.
name: Coldea, R.
name: Prabhakaran, D.
name: Frost, C. D.
name: Keen, D. A.
name: Regnault, L. P.
name: Freeman, P. G.
name: Enderle, M.
name: Kulda, J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We describe neutron scattering experiments performed to investigate the magnetic order and dynamics of half-doped La1.5Sr0.5CoO4. This layered perovskite exhibits a near-ideal checkerboard pattern of Co2+/Co3+ charge order at temperatures below ~ 800 K. Magnetic correlations are observed at temperatures below ~ 60 K but static magnetic order only becomes established at 31 K, a temperature at which a kink is observed in the susceptibility. On warming above 31 K we observed a change in the magnetic correlations which we attribute either to a spin canting or to a change in the proportion of inequivalent magnetic domains. The magnetic excitation spectrum is dominated by an intense band extending above a gap of approximately 3 meV up to a maximum energy of 16 meV. A weaker band exists in the energy range 20-30 meV. We show that the excitation spectrum is in excellent quantitative agreement with the predictions of a spin-wave theory generalized to include the full magnetic degrees of freedom of high-spin Co2+ ions in an axially distorted crystal field, coupled by Heisenberg exchange interactions. The magnetic order is found to be stabilized by dominant antiferromagnetic Co2+ -- Co2+ interactions acting in a straight line through Co3+. No evidence is found for magnetic scattering from the Co3+ ions, supporting the view that Co3+ is in the S = 0 state in this material.
description: 17 pages, 10 figures. Accepted for publication in Phys. Rev. B
Onthophagus mexicanus Bates 1887
Creators: name: Kohlmann, Bert
name: Solís, Ángel
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Scarabaeidae
Onthophagus
Onthophagus mexicanus

description: Onthophagus mexicanus species group.
The males of this group have a slightly emarginate clypeus (O. mexicanus), or a small clypeal projection (O. championi), or a distinct vertical clypeal horn protrusion present in O. guatemalensis and O. pseudoguatemalensis (Fig. 5.11); slender male protibiae (Figs. 1.26 –28); apical and internal male protibial margin acuminate (Figs. 1.26 –28); male protibial apex with some short setae (Figs. 1.26 –28); male pronotum with a plate-like projection, distally more-or-less distinctly emarginated at middle (Fig. 5.11).
Zunino & Halffter (1988) established this species group based on the Boucomont (1932) “7 e Groupe”. Zunino & Halffter (1997) later defined this group, giving a detailed morphological characterization. Interestingly and opposed to this study, they considered that contrary to groups such as O. clypeatus and O. landolti, this group had a robust internal homogeneity that did not allow for the separation of species groups. Bates (1887) described in the Biologia Centrali-Americana for the first time an O. mexicanus species group comprised of O. championi Bates, O. eulophus Bates, O. guatemalensis Bates, and O. mexicanus Bate s. Moctezuma & Halffter (2021) considered that the group included at least 18 species. We consider the existence of only four species in this group (Appendix 1). The present analysis proposes the idea that at least three new species groups previously considered to form part of the O. mexicanus species group exist within: O. eulophus, O. hecate, and O. velutinus (Figs. 1–2). The present barcode and gene tree analyses (Figs. 1–2, 8–9) suggest a very close relationship between the O. mexicanus and O. velutinus species groups with a bootstrap support of 93, while the O. hecate species group is distantly related. The O. mexicanus species group is distributed in the mountains from northwestern Mexico to Costa Rica.
description: Published as part of Kohlmann, Bert & Solís, Ángel, 2025, A review of the species groups of the Western Hemisphere Onthophagus Latreille (Coleoptera: Scarabaeidae: Scarabaeinae) using COI barcoding and gene trees, pp. 401-447 in Zootaxa 5604 (4) on pages 428-429, DOI: 10.11646/zootaxa.5604.4.1, http://zenodo.org/record/15213967
title: ÐÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼Ð¾Ð´ÑÐ»Ñ ÑÐµÑÐ²Ð¸ÑÐ° Ð¿Ð¾ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð³Ð¾ ÑÐ·ÑÐºÐ°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¦Ð²Ð¸ÑÐºÑÐ½, ÐÑÐµÐ½Ð¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð²ÐµÐ±-ÑÐµÑÐ²Ð¸Ñ
ÑÐ¸ÑÑÐµÐ¼Ð° Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ ÑÐ·ÑÐºÐ¾Ð²

description: Ð¢ÐµÐ¼Ð° Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð¾ÑÐ½Ð¾ÑÐ¸ÑÑÑ Ðº Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼. Ð Ð¿ÐµÑÐ²Ð¾Ð¹ ÑÐ°ÑÑÐ¸ ÑÐ°Ð±Ð¾ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ Ð¼ÐµÑÐ¾Ð´Ñ Ð¸ ÑÐ¿Ð¾ÑÐ¾Ð±Ñ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð³Ð¾ ÑÐ·ÑÐºÐ°, Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÑÑÐºÑÑÑÑ Ð¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐµÑÐ²Ð¸ÑÐ¾Ð² Ð² ÑÐµÑÐ¸ ÐÐ½ÑÐµÑÐ½ÐµÑ, Ð¿ÑÐµÐ´Ð¾ÑÑÐ°Ð²Ð»ÑÑÑÐ¸Ñ Ð´Ð¾ÑÑÑÐ¿ Ðº Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð°Ð¼ Ð¿Ð¾ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð³Ð¾ ÑÐ·ÑÐºÐ°. ÐÐ¾ Ð²ÑÐ¾ÑÐ¾Ð¹ ÑÐ°ÑÑÐ¸ ÑÐ°Ð±Ð¾ÑÑ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ð° Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ Ð¸ Ð²ÑÐ±Ð¾ÑÐ° Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ¾Ð² Ð´Ð»Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐµÑÐ²Ð¸ÑÐ¾Ð² Ð² ÑÐµÑÐ¸ ÐÐ½ÑÐµÑÐ½ÐµÑ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð¼Ð¾Ð´ÑÐ»Ñ ÑÐµÑÐ²Ð¸ÑÐ° Ð¿Ð¾ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð³Ð¾ ÑÐ·ÑÐºÐ° Ð² ÑÐµÑÐ¸ ÐÐ½ÑÐµÑÐ½ÐµÑ, Ð³Ð»Ð°Ð²Ð½Ð¾Ð¹ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÑÑ ÐºÐ¾ÑÐ¾ÑÐ¾Ð³Ð¾ ÑÐ²Ð»ÑÐµÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ðµ ÐºÐ¾ÑÐ¾ÑÐºÐ¸Ñ Ð²Ð¸Ð´ÐµÐ¾ÑÑÐ°Ð³Ð¼ÐµÐ½ÑÐ¾Ð² Ñ Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð¹ ÑÐµÑÑÑ Ð¸ Ð¸Ð½ÑÐµÑÐ°ÐºÑÐ¸Ð²Ð½ÑÐ¼Ð¸ ÑÑÐ±ÑÐ¸ÑÑÐ°Ð¼Ð¸.
title: Ð¤Ð¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Â«ÐÑÑÐºÐ¾Ðµ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ Ð¾ÑÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ ÑÐ¸Ð»Ð¸Ð°Ð»Ð° ÐÐÐ Â«ÐÐ Ð¡Ð ÐÐ¾Ð»Ð³Ð¸Â»-Â«ÐÑÐµÐ½Ð±ÑÑÐ³ÑÐ½ÐµÑ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Ð°ÑÑÐºÐ¸Ð½Ð°, Ð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°Ð½Ð°Ð»Ð¸Ð· ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
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Ð¿ÑÐ¸Ð±ÑÐ»Ñ
ÑÐµÐ½ÑÐ°Ð±ÐµÐ»ÑÐ½Ð¾ÑÑÑ
Ð»Ð¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÑ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ Â«ÐÑÑÐºÐ¾Ðµ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ Ð¾ÑÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ ÑÐ¸Ð»Ð¸Ð°Ð»Ð° ÐÐÐ Â«ÐÐ Ð¡Ð ÐÐ¾Ð»Ð³Ð¸Â»-ÐÑÐµÐ½Ð±ÑÑÐ³ÑÐ½ÐµÑÐ³Ð¾Â».
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title: Ð¤Ð¸Ð·Ð¸ÐºÐ° ÑÐ²ÐµÑÐ´Ð¾Ð³Ð¾ ÑÐµÐ»Ð°. ÐÐ¸ÑÑÐ°ÐºÑÐ¸Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¾Ð² Ð½Ð° ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ðµ Ñ Ð°ÐºÑÑÑÐ¸ÑÐµÑÐºÐ¸Ð¼Ð¸ ÐºÐ¾Ð»ÐµÐ±Ð°Ð½Ð¸ÑÐ¼Ð¸. Ð§. 2
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ¾Ð´ÑÐ²Ð¸ÑÐ¾Ð², ÐÐ»ÐµÐ³
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ Ð¡ÐÐ±ÐÐÐ£
Year: 2003
Subjects: Ð­Ð»ÐµÐºÑÑÐ¾Ð½Ñ

description: ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ Ð°Ð²ÑÐ¾ÑÑÐºÐ¾Ð¼Ñ ÐºÑÑÑÑ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ Â«Ð¤Ð¸Ð·Ð¸ÐºÐ° ÑÐ²ÐµÑÐ´Ð¾Ð³Ð¾ ÑÐµÐ»Ð°Â» Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ Ð¸ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ 553100 Â«Ð¢ÐµÑÐ½Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°Â». Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° ÐºÐ¸Ð½ÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ°Ñ Ð´Ð¸ÑÑÐ°ÐºÑÐ¸Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¾Ð² Ð² ÐºÐ¾Ð½ÑÐµÐ¿ÑÐ¸Ð¸ Ð¼ÑÐ³ÐºÐ¾Ð³Ð¾ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»Ð°, ÑÑÐ¸ÑÑÐ²Ð°ÑÑÐµÐ³Ð¾ Ð² Ð¿ÐµÑÐ²Ð¾Ð¼ Ð¿ÑÐ¸Ð±Ð»Ð¸Ð¶ÐµÐ½Ð¸Ð¸ Ð´ÐµÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½ÑÑ Ð¸Ð¾Ð½Ð½Ð¾Ð¹ Ð¸ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð¾Ð¹ Ð¿Ð»Ð¾ÑÐ½Ð¾ÑÑÐµÐ¹. Ð£ÑÐµÑ ÑÑÐ¸Ñ ÑÐ²Ð¾Ð¹ÑÑÐ² Ð¿ÑÐ¸Ð²Ð¾Ð´Ð¸Ñ Ðº Ð¿Ð¾ÑÐ²Ð»ÐµÐ½Ð¸Ñ ÑÑÐ´Ð° Ð½Ð¾Ð²ÑÑ ÑÑÑÐµÐºÑÐ¾Ð² Ð² ÑÐ°ÑÑÐµÑÐ½Ð¸Ð¸ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¾Ð², ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ Ð´Ð»Ñ Ð¼ÐµÑÐ°Ð»Ð»Ð¾Ð², Ð¿Ð¾Ð»ÑÑÐ½ÑÑ Ð¸ Ð½ÐµÐ¿Ð¾Ð»ÑÑÐ½ÑÑ Ð´Ð¸ÑÐ»ÐµÐºÑÑÐ¸ÐºÐ¾Ð² Ð¸ Ð¿Ð¾Ð»ÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¸ÐºÐ¾Ð². ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ¾Ð² Ð¸ ÑÐ¾Ð¸ÑÐºÐ°ÑÐµÐ»ÐµÐ¹, Ð¿ÑÐ¾Ð²Ð¾Ð´ÑÑÐ¸Ñ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½ÑÐµ Ð¸ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÑÐ¼ 01.04.02 Â«Ð¢ÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°Â», 01.04.04 Â«Ð¤Ð¸Ð·Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ°Â», 01.04.07 Â«Ð¤Ð¸Ð·Ð¸ÐºÐ° ÐºÐ¾Ð½Ð´ÐµÐ½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸ÑÂ».
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°.
title: ÐÐµÑÐ¾Ð´Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸. ÐÐ°Ð´Ð°ÑÐ¸ Ð²ÑÐ¿ÑÐºÐ»Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐµÑÑÑÐ¾Ð², ÐÐµÐ¾Ð½Ð¸Ð´
name: Ð¡ÐµÑÐµÐ³Ð¸Ð½, Ð.
name: Ð Ð¾Ð´Ð¸Ð¾Ð½Ð¾Ð²Ð°, Ð.
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2014
Subjects: ÐÑÐ¿ÑÐºÐ»Ð¾Ðµ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ

description: ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¼Ñ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¼Ñ ÑÑÐ°Ð½Ð´Ð°ÑÑÑ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ Â«ÐÐµÑÐ¾Ð´Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸Â» Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Â«ÐÑÐ¸ÐºÐ»Ð°Ð´Ð½Ð°Ñ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ° Ð¸ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸ÐºÐ°Â» Ð¸ Ð´ÑÑÐ³Ð¸Ñ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð². Ð ÐºÑÐ°ÑÐºÐ¾Ð¼ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¸ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ ÑÐµÐ¾ÑÐ¸Ñ Ð°ÑÑÐ¸Ð½Ð½ÑÑ Ð¼Ð½Ð¾Ð¶ÐµÑÑÐ², Ð¿Ð¾Ð»Ð¸ÑÐ´ÑÐ¾Ð², Ð²ÑÐ¿ÑÐºÐ»ÑÑ Ð¼Ð½Ð¾Ð¶ÐµÑÑÐ², ÑÐµÐ¾ÑÐ¸Ñ Ð¾ÑÐ´ÐµÐ»Ð¸Ð¼Ð¾ÑÑÐ¸ Ð²ÑÐ¿ÑÐºÐ»ÑÑ Ð¼Ð½Ð¾Ð¶ÐµÑÑÐ², Ð²ÑÐ¿ÑÐºÐ»ÑÐµ ÑÑÐ½ÐºÑÐ¸Ð¸. Ð¡ÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¸ Ð´Ð¾ÐºÐ°Ð·Ð°Ð½Ñ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÐµ Ð¸ Ð´Ð¾ÑÑÐ°ÑÐ¾ÑÐ½ÑÐµ ÑÑÐ»Ð¾Ð²Ð¸Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸ Ð´Ð»Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÑÐ¸Ð¿Ð¾Ð² Ð·Ð°Ð´Ð°Ñ Ð²ÑÐ¿ÑÐºÐ»Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÑÐ»ÐµÐ¼ÐµÐ½ÑÑ ÑÐµÐ¾ÑÐ¸Ð¸ Ð´Ð²Ð¾Ð¹ÑÑÐ²ÐµÐ½Ð½Ð¾ÑÑÐ¸. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð·Ð°Ð´Ð°ÑÐ¸ Ð»Ð¸Ð½ÐµÐ¹Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ ÑÐ¸Ð¼Ð¿Ð»ÐµÐºÑ-Ð¼ÐµÑÐ¾Ð´ Ð¸Ñ ÑÐµÑÐµÐ½Ð¸Ñ. ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¼Ð¸Ð½Ð¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÑÐ½ÐºÑÐ¸Ð¹. ÐÐ½Ð¾ ÑÐ°ÐºÐ¶Ðµ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¿Ð¾Ð»ÐµÐ·Ð½Ð¾ Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ°Ð¼ Ð¸ Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»ÑÐ¼ Ð²ÑÐ·Ð¾Ð². Ð­ÑÐ¾ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÑÐµÑ ÑÐ¾Ð±Ð¾Ð¹ Ð´Ð¾Ð¿Ð¾Ð»Ð½ÐµÐ½Ð½Ð¾Ðµ Ð¿ÐµÑÐµÐ¸Ð·Ð´Ð°Ð½Ð¸Ðµ ÑÑÐµÐ±Ð½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Â«ÐÐµÑÐ¾Ð´Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð·Ð°Ð´Ð°Ñ Ð²ÑÐ¿ÑÐºÐ»Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸ÑÂ» Ð.Ð. ÐÐµÑÑÑÐ¾Ð²Ð°, Ð.Ð. Ð¡ÐµÑÑÐ³Ð¸Ð½Ð°, Ð¸Ð·Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð² 1991 Ð³Ð¾Ð´Ñ Ð² ÐÐÐ¢Ð£. Ð Ð½Ð°ÑÑÐ¾ÑÑÐµÐµ Ð¸Ð·Ð´Ð°Ð½Ð¸Ðµ Ð²ÐºÐ»ÑÑÐµÐ½ ÑÑÐ´ Ð½Ð¾Ð²ÑÑ ÑÐ°Ð·Ð´ÐµÐ»Ð¾Ð², Ð´Ð¾Ð¿Ð¾Ð»Ð½ÐµÐ½Ñ ÑÐ°Ð·Ð´ÐµÐ»Ñ, Ð¸Ð¼ÐµÐ²ÑÐ¸ÐµÑÑ Ð² Ð¿ÑÐµÐ¶Ð½ÐµÐ¼, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ñ Ð´Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÑÑÑÐ²Ð° Ð½ÐµÐºÐ¾ÑÐ¾ÑÑÑ ÑÐµÐ¾ÑÐµÐ¼. Ð ÑÐ¿Ð¸ÑÐ¾Ðº Ð»Ð¸ÑÐµÑÐ°ÑÑÑÑ Ð²ÐºÐ»ÑÑÐµÐ½Ñ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐµ ÐºÐ½Ð¸Ð³Ð¸ Ð¿Ð¾ ÑÐµÐ¼Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ.
Original scans of illustrations in “Planning Toronto: the planners, the plans, their legacies, 1940-80”
Creators: name: White, Richard
Publisher: name: UBC Press
Year: 2016

description: Toronto is known for being a “city that works.” In this lavishly illustrated, meticulously researched book, Richard White analyzes the city’s planning and how it contributed to Toronto becoming a functional, world-class city. Focusing on the critical period from 1940 to 1980, he examines how planners sought to shape the city and the region amid a maelstrom of local and international obstacles and influences. Planning Toronto offers the first comprehensive explanation of how Toronto’s postwar plans – city, metropolitan, and regional – came to be, who devised them, and what impact they had. As this definitive history reveals, planning matters – though not always as expected.
Archaeological assessment reveals Earth’s early transformation through land use
Creators: name: Stephens, Lucas
name: Ellis, Erle
Publisher: name: Science
Year: 2019
Subjects: land use
Holocene
archaeology

description: Humans began to leave lasting impacts on Earth's surface starting 10,000 to 8000 years ago. Through a synthetic collaboration with archaeologists around the globe, Stephens et al. compiled a comprehensive picture of the trajectory of human land use worldwide during the Holocene (see the Perspective by Roberts). Hunter-gatherers, farmers, and pastoralists transformed the face of Earth earlier and to a greater extent than has been widely appreciated, a transformation that was essentially global by 3000 years before the present.
description: Environmentally transformative human use of land accelerated with the emergence of agriculture, but the extent, trajectory, and implications of these early changes are not well understood. An empirical global assessment of land use from 10,000 years before the present (yr B.P.) to 1850 CE reveals a planet largely transformed by hunter-gatherers, farmers, and pastoralists by 3000 years ago, considerably earlier than the dates in the land-use reconstructions commonly used by Earth scientists. Synthesis of knowledge contributed by more than 250 archaeologists highlighted gaps in archaeological expertise and data quality, which peaked for 2000 yr B.P. and in traditionally studied and wealthier regions. Archaeological reconstruction of global land-use history illuminates the deep roots of Earth’s transformation and challenges the emerging Anthropocene paradigm that large-scale anthropogenic global environmental change is mostly a recent phenomenon.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿Ð¾Ð´ÑÐ¸ÑÑÐµÐ¼Ñ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ñ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ°Ð¼Ð¸ Ð¾Ñ ÑÐ°Ð½Ð½Ð¾Ð¹ ÑÐ¸Ð³Ð½Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¿ÑÐ¾ÑÐ¾ÐºÐ¾Ð»Ð° ModBus
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°Ð»ÑÑÑÐ¾Ð²Ð°, ÐÐ¾Ð»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¸Ð³Ð½Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð¾Ñ ÑÐ°Ð½Ð½Ð°Ñ
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