cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: A Computational Study on the Effect of Horizontal Openings on Fire Dynamics within Informal Dwellings
Creators: name: Beshir, M.
name: Wang, Y.
name: Gibson, L.
name: Welch, S.
name: Rush, D.
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: Fires in informal settlements are a major risk facing big cities within the developing countries, not only
concerning life safety but also because they exert social and economic pressures on these communities.
One of the cities most affected by informal settlement fires is Cape Town, Western Cape, South Africa. A
research project, namely IRIS-Fire, was launched in order to develop a fundamental understanding of the
technical issues regarding fire spread within the informal settlements of the Western Cape. In early
investigations it was found that one of the main fire spread mechanisms between dwellings is external
flaming and the heat flux from the vertical openings of the burning dwelling to its surroundings. In this
paper a computational study is reported which seeks to quantify the effect of adding horizontal roof
openings to the design of these informal dwellings. The main parameters in the design of the
computational simulations were determined based on surveys done in the informal settlements in the
Western Cape. Twenty different cases were investigated using different assumed fuel loads as 270, 410,
550 and 690 MJ/m2 and horizontal opening sizes of 0.04, 0.16, 0.32 and 0.64 m2. It was found that:
adding horizontal openings with sizes larger than 0.16 m2 can significantly increase the time for the
dwelling to reach flashover, reduce the heat flux from external flaming to the surroundings, and reduce
the size of the external flame plume.
Si fa presto a dire equinozio
Creators: Francesca Aloisio
Publisher: name: Media Inaf
Year: 2014

Domani è l’equinozio d’autunno e ufficialmente terminerà l'estate e comincerà la stagione autunnale. Nell'immaginario collettivo il dì e la notte avranno la stessa durata, mentre in realtà la differenza c’è
Relating basic properties of bright early-type dwarf galaxies to their location in Abell 901/902
Creators: name: Barazza, F. D.
name: Wolf, C.
name: Gray, M. E.
name: Jogee, S.
name: Balogh, M.
name: McIntosh, D. H.
name: Bacon, D.
name: Barden, M.
name: Bell, E. F.
name: Boehm, A.
name: Caldwell, J. A. R.
name: Haeussler, B.
name: Heiderman, A.
name: Heymans, C.
name: van Kampen, K. Jahnke. E.
name: Lane, K.
name: Marinova, I.
name: Meisenheimer, K.
name: Peng, C. Y.
name: Sanchez, S. F.
name: Taylor, A.
name: Wisotzki, L.
name: Zheng, X.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present a study of the population of bright early-type dwarf galaxies in the multiple-cluster system Abell 901/902. We use data from the STAGES survey and COMBO-17 to investigate the relation between the color and structural properties of the dwarfs and their location in the cluster. The definition of the dwarf sample is based on the central surface brightness and includes galaxies in the luminosity range -16 >= M_B >~-19 mag. Using a fit to the color magnitude relation of the dwarfs, our sample is divided into a red and blue subsample. We find a color-density relation in the projected radial distribution of the dwarf sample: at the same luminosity dwarfs with redder colors are located closer to the cluster centers than their bluer counterparts. Furthermore, the redder dwarfs are on average more compact and rounder than the bluer dwarfs. These findings are consistent with theoretical expectations assuming that bright early-type dwarfs are the remnants of transformed late-type disk galaxies involving processes such as ram pressure stripping and galaxy harassment. This indicates that a considerable fraction of dwarf elliptical galaxies in clusters are the results of transformation processes related to interactions with their host cluster.
description: 12 pages, 8 figures, accepted for publication in A&A, typo corrected in abstract
NOEMA: l’esercito delle 12 antenne alpine
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2014

Inaugurata la nuova parabola da 15 metri che andrà a comporre la schiera da complessive 12 antenne del radiotelescopio millimetrico NOEMA, successore dell’attuale osservatorio sul Plateau de Bure sulle alpi francesi. Sarà il più potente nella sua banda di frequenza per l’emisfero settentrionale
title: Anaerobic biodegradation of perfluorooctane sulfonate (PFOS) and microbial community composition in soil amended with a dechlorinating culture and chlorinated solvents
Creators: name: Lorah, Michelle M.
name: He, Ke
name: Blaney, Lee
name: Akob, Denise M.
name: Harris, Cassandra
name: Tokranov, Andrea
name: Hopkins, Zachary
name: Shedd, Brian P.
Publisher: name: Elsevier
Year: 2024
Subjects: subject: Perfluorinated sulfonate
subject: Sulfate reducers
subject: PFAS contaminated soil
subject: Chlorinated volatile organic compounds
subject: Dehalogenating culture
subject: PFAS biodegradation

description: Perfluorooctane sulfonate (PFOS), one of the most frequently detected per- and polyfluoroalkyl substances (PFAS) occurring in soil, surface water, and groundwater near sites contaminated with aqueous film-forming foam (AFFF), has proven to be recalcitrant to many destructive remedies, including chemical oxidation. We investigated the potential to utilize microbially mediated reduction (bioreduction) to degrade PFOS and other PFAS through addition of a known dehalogenating culture, WBC-2, to soil obtained from an AFFF-contaminated site. A substantial decrease in total mass of PFOS (soil and water) was observed in microcosms amended with WBC-2 and chlorinated volatile organic compound (cVOC) co-contaminants — 46.4 ± 11.0 % removal of PFOS over the 45-day experiment. In contrast, perfluorooctanoate (PFOA) and 6:2 fluorotelomer sulfonate (6:2 FTS) concentrations did not decrease in the same microcosms. The low or non-detectable concentrations of potential metabolites in full PFAS analyses, including after application of the total oxidizable precursor assay, indicated that defluorination occurred to non-fluorinated compounds or ultrashort-chain PFAS. Nevertheless, additional research on the metabolites and degradation pathways is needed. Population abundances of known dehalorespirers did not change with PFOS removal during the experiment, making their association with PFOS removal unclear. An increased abundance of sulfate reducers in the genus Desulfosporosinus (Firmicutes) and Sulfurospirillum (Campilobacterota) was observed with PFOS removal, most likely linked to initiation of biodegradation by desulfonation. These results have important implications for development of in situ bioremediation methods for PFAS and advancing knowledge of natural attenuation processes.
Pisa: 100° congresso SIF
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2014

La Società Italiana di Fisica inaugura il centesimo congresso nazionale: a Pisa, ospite del dipartimento di fisica dell’Università, si ritrova la vasta comunità dei fisici italiani. È occasione per consegnare il premio all’outreach, da quest’anno dedicato a Romeo Bassoli. A riceverlo dalle mani del presidente SIF, Luisa Cifarelli, Marco Galliani di INAF
title: ÐÐ¸ÑÐµÐ¹Ð½ÑÐµ ÑÐ¿Ð»Ð°Ð²Ñ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐºÐ¸Ð¼Ð¾Ð²Ð°, ÐÐ»ÐµÐ½Ð°
name: Ð¢ÑÐµÐ½Ð¸Ð½Ð°, ÐÐ°ÑÐ¸Ð½Ð°
name: ÐÐ¼ÐµÐ»ÑÑÐ½Ð¾Ð², ÐÐ°Ð´Ð¸Ð¼
name: ÐÐ°ÑÑÑÐ½Ð¾Ð², ÐÐ¾Ð½ÑÑÐ°Ð½ÑÐ¸Ð½
name: ÐÑÐ»ÑÐµÐ²Ð°, Ð¢Ð°ÑÑÑÐ½Ð°
name: Ð¥Ð¾Ð¼ÐµÐ½ÐºÐ¾, ÐÐ°Ð´ÐµÐ¶Ð´Ð°
Publisher: name: ÐÐÐÐ°Ñ
Year: 2012
Subjects: Ð¡Ð¿Ð»Ð°Ð²Ñ

description: ÐÐ·Ð»Ð¾Ð¶ÐµÐ½Ñ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¾Ð± Ð¾ÑÐ½Ð¾Ð²Ð°Ñ ÑÐµÐ¾ÑÐ¸Ð¸ Ð»Ð¸ÑÐµÐ¹Ð½ÑÑ ÑÐ¿Ð»Ð°Ð²Ð¾Ð² Ð¸ Ð¿ÑÐ¾ÑÐµÑÑÐ°Ñ Ð¸Ñ ÑÐµÑÐ¼Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸, Ð¾Ð¿Ð¸ÑÐ°Ð½Ñ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¾ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð°Ñ Ð»Ð¸ÑÐµÐ¹Ð½ÑÑ ÑÐ¿Ð»Ð°Ð²Ð¾Ð², Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ°Ñ Ð¸Ñ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð¸ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ ÑÐ»ÑÐ¶ÐµÐ±Ð½ÑÑ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸Ðº ÑÐ¿Ð»Ð°Ð²Ð¾Ð² Ð² Ð¾ÑÐ»Ð¸Ð²ÐºÐ°Ñ. ÐÑÐ²ÐµÑÐµÐ½Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð»Ð¸ÑÐµÐ¹Ð½ÑÑ ÑÐ²Ð¾Ð¹ÑÑÐ² Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ ÑÐ°ÑÐ¿ÑÐ¾ÑÑÑÐ°Ð½ÐµÐ½Ð½ÑÑ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÑ ÑÐ¿Ð»Ð°Ð²Ð¾Ð², Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¾ Ð¼Ð°ÑÐºÐ°Ñ Ð»Ð¸ÑÐµÐ¹Ð½ÑÑ ÑÐ¿Ð»Ð°Ð²Ð¾Ð² Ð¸ Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸ âÐÐ°ÑÐ¸Ð½Ñ Ð¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð»Ð¸ÑÐµÐ¹Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°â, Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ñ ÐºÑÑÑ âÐÐ¸ÑÐµÐ¹Ð½ÑÐµ ÑÐ¿Ð»Ð°Ð²Ñ Ð¸ Ð¿Ð»Ð°Ð²ÐºÐ°â.
Color Magnitude Relation and Morphology of Low-Redshift ULIRGs in SDSS
Creators: name: Chen, Yuxi
name: Lowenthal, James D.
name: Yun, Min S.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present color-magnitude and morphological analysis of 54 low-redshift ULIRGs, a subset of the IRAS 1Jy sample (Kim & Sanders, 1998), in the SDSS. The ULIRGs are on average 1 magnitude brighter in M0.1r than the SDSS galaxies within the same redshift range. The majority of the ULIRGs (~87%) have the colors typical of the blue cloud, and only 4 sources (~7%) are located in the red sequence. While ULIRGs are popularly thought to be precursors to a QSO phase, we find few (~6%) in the "green valley" where the majority of the X-ray and IR selected AGNs are found, and none of which harbors an AGN. For the 14 previously spectroscopic identified AGNs (~28%), we perform PSF subtractions and find that on average the central point sources contribute less than one third to the total luminosity, and that their high optical luminosities and overall blue colors are apparently the result of star formation activity of the host galaxies. Visual inspection of the SDSS images reveals a wide range of disturbed morphologies. A detailed morphology analysis using Gini and M20 coefficients shows that slightly less than one half (~42% in g band) of the ULIRGs are located in the region where most local mergers are found. The heterogeneous distribution of ULIRGs in the G-M20 space is qualitatively consistent with the results found by numerical simulations of disk-disk mergers. Our study also shows that the measured morphological parameters are systematically affected by the SNR and thus the merging galaxies can appear at various regions in the G-M20 space. In general, our results reinforce the view that ULIRGs contain young stellar populations and are mergers in progress. Our study provides a uniform comparison sample for studying ULIRGs at higher redshifts such as Spitzer mid-IR selected ULIRGs at z=1~2 and submm galaxies.
description: 42 pages, 11 figures, ApJ accepted
In silico molecular docking study, synthesis and α-amylase inhibitory activity evaluation of phosphorylated derivatives of purine
Creators: name: Kumar, M. Pavan Phani
name: Anuradha, V.
name: Subramanyam, Ch.
name: Babu, V. V. Hari
Publisher: name: Taylor & Francis
Year: 2021
Subjects: subject: Biochemistry
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 60506 Virology

description: A series of phosphorylated derivatives of purine were synthesized in good yields (88–95%) by the reaction of 2‐chloro‐4‐{[(9H‐purin‐9‐yl)methoxy]methyl}‐1,3,2-λ5‐dioxaphospholan‐2‐one with various heterocyclic amines. In silico molecular docking study was performed for all the designed compounds to assess their potential ability to inhibit the pancreatic α-amylase enzyme. The compounds (6a–j) with good inhibition toward the target enzyme were prompted for the synthesis. Spectroscopic analyses of all the newly synthesized compounds were performed to confirm their structures. In vitro α-amylase inhibitory activity of the synthesized compounds was also carried out using acarbose as a standard drug. The compounds 2‐[(6‐chloro‐1,3‐benzothiazol‐2‐yl)amino]‐4‐{[(9H‐purin‐9‐yl)methoxy]methyl}‐1,3,2λ5‐dioxaphospholan‐2‐one (6j) (IC50, 94.3 ± 0.5 μg/mL) and 1‐methyl‐6‐[(2‐oxo‐4‐{[(9H‐purin‐9‐yl)methoxy]methyl}‐1,3,2λ5‐dioxaphospholan‐2‐yl)amino]‐1,2,3,4‐tetrahydropyrimidine‐2,4‐dione (6f) (IC50, 99.0 ± 0.4 μg/mL) reported the highest inhibition among the synthesized compounds. All the remaining compounds exhibited good to moderate inhibition with IC50 values in the range of 102.9 ± 0.6 to 233.5 ± 0.6 μg/mL when compared with the standard drug, acarbose (IC50, 50.47 ± 0.28 μg/mL).
Toxic leukoencephalopathy after heroin inhalation
Creators: name: Taberner Lopez, Ester
Publisher: name: EURORAD
Year: 2015
Subjects: subject: Neuroradiology brain
subject: CT
subject: MR
subject: MR-Diffusion/Perfusion
subject: Contrast agent-intravenous
subject: Diagnostic procedure
subject: Drugs / Reactions

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: male, 29 years
description: Clinical History: A 29-years-old man, with a history of drug and alcohol abuse, was admitted to the intensive care unit in coma.Schizophrenia was diagnosed three years before, but he voluntarily rejected treatment. Parents reveled suspicion of heroin inhalation... Final Diagnosis: Toxic leukoencephalopathy after heroin inhalation
Generalized scaling function from light-cone gauge AdS_5 x S^5 superstring
Creators: name: Giombi, S.
name: Ricci, R.
name: Roiban, R.
name: Tseytlin, A. A.
name: Vergu, C.
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We revisit the computation of the 2-loop correction to the energy of a folded spinning string in AdS_5 with an angular momentum J in S^5 in the scaling limit log S, J >>1 with J / log S fixed. This correction gives the third term in the strong-coupling expansion of the generalized scaling function. The computation, using the AdS light-cone gauge approach developed in our previous paper, is done by expanding the AdS_5 x S^5 superstring partition function near the generalized null cusp world surface associated to the spinning string solution. The result corrects and extends the previous conformal gauge result of arXiv:0712.2479 and is found to be in complete agreement with the corresponding terms in the generalized scaling function as obtained from the asymptotic Bethe ansatz in arXiv:0805.4615 (and also partially from the quantum O(6) model and the Bethe ansatz data in arXiv:0809.4952). This provides a highly nontrivial strong coupling comparison of the Bethe ansatz proposal with the quantum AdS_5 x S^5 superstring theory, which goes beyond the leading semiclassical term effectively controlled by the underlying algebraic curve. The 2-loop computation we perform involves all the structures in the AdS light-cone gauge superstring action of hep-th/0009171 and thus tests its ultraviolet finiteness and, through the agreement with the Bethe ansatz, its quantum integrability. We do most of the computations for a generalized spinning string solution or the corresponding null cusp surface that involves both the orbital momentum and the winding in a large circle of S^5.
description: 50 pages, latex
Status of CP Violation
Creators: name: Sinha, Nita
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The Standard Model parametrization of CP violation is described. Tests of this parametrization using the observed heavy flavour decays and implications for New physics are discussed.
description: 6 pages, 3 figures, presented at the 18th International Conference on Particles And Nuclei (PANIC08), 9-14 November 2008, Eilat, Israel
La Notte della Ricerca a Palermo e Teramo
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2014

La Notte dei Ricercatori è un'iniziativa promossa dalla Commissione Europea fin dal 2005 con l'obiettivo è di creare occasioni di incontro tra ricercatori e cittadini, per diffondere la cultura scientifica. Dopo Roma, perugia, Bologna e Padova oggi presentiamo le iniziative a Palermo e Teramo
title: Ð¤Ð¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐµÐºÐ»Ð°Ð¼Ð½Ð¾Ð¹ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ ÑÐ¸ÑÐ¼Ñ Ð½Ð° ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ½Ð¾Ð¼ ÑÑÐ½ÐºÐµ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ "ÐÑÐ¸Ð·")
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: Ð¡Ð°Ð´Ð¾Ð²ÑÐºÐ¸Ð¹, Ð Ð¾Ð¼Ð°Ð½
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÐºÐ»Ð°Ð¼Ð½Ð¾Ð¹ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸
ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ½ÑÐ¹ ÑÑÐ½Ð¾Ðº
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Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÐºÐ»Ð°Ð¼Ð½Ð¾Ð¹ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¸ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÐµÐºÐ»Ð°Ð¼Ð½Ð¾Ð¹ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸. ÐÐ°Ð½Ñ Ð¾Ð±ÑÐ¸Ðµ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÑÐµÑÐ¼Ð¸Ð½Ð¾Ð², ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÑ Ñ Ð¿Ð¾Ð½ÑÑÐ¸ÐµÐ¼ ÑÐµÐºÐ»Ð°Ð¼Ð½Ð¾Ð¹ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸, Ð¸Ð·ÑÑÐµÐ½Ð° ÐµÐµ ÑÐ¾Ð»Ñ Ð² Ð±Ð¸Ð·Ð½ÐµÑÐµ. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ñ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ ÑÐµÐºÐ»Ð°Ð¼Ð½Ð¾Ð¹ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÐµ ÑÑÐ»Ð¾Ð²Ð¸Ñ Ð´Ð»Ñ ÑÑÐ¿ÐµÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ¾Ðº.
Symmetry analysis of magneto-optical effects: The case of x-ray diffraction and x-ray absorption at the transition metal L23 edge
Creators: name: Haverkort, M. W.
name: Hollmann, N.
name: Krug, I. P.
name: Tanaka, A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: A general symmetry analysis of the optical conductivity or scattering tensor is used to rewrite the conductivity tensor as a sum of fundamental spectra multiplied by simple functions depending on the local magnetization direction. Using this formalism, we present several numerical examples at the transition metal L23 edge. From these numerical calculations we can conclude that large deviations from the magneto-optical effects in spherical symmetry are found. These findings are in particular important for resonant x-ray diffraction experiments where the polarization dependence and azimuthal dependence of the scattered Bragg intensity is used to determine the local ordered magnetization direction.
title: ÐÐ¾ÑÑÐ¾Ð·Ð¸Ñ ÑÐ²Ð°ÑÐ½ÑÑ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ð¹ Ð¸ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ°Ð¹ÑÐµÐ², ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2011
Subjects: Ð¡Ð²Ð°ÑÐ½ÑÐµ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ñ Ð¸ ÑÐ²Ñ

description: Ð¡Ð¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ñ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ "ÐÐ¾ÑÑÐ¾Ð·Ð¸Ñ ÑÐ²Ð°ÑÐ½ÑÑ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ð¹ Ð¸ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹" Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ° 150100 "ÐÐµÑÐ°Ð»Ð»ÑÑÐ³Ð¸Ñ", ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÑ 150107 "ÐÐµÑÐ°Ð»Ð»ÑÑÐ³Ð¸Ñ ÑÐ²Ð°ÑÐ¾ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°". Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¸Ð´Ñ ÐºÐ¾ÑÑÐ¾Ð·Ð¸Ð¸ Ð¸ ÐºÐ¾ÑÑÐ¾Ð·Ð¸Ð¾Ð½Ð½ÑÑ ÑÐ°Ð·ÑÑÑÐµÐ½Ð¸Ð¹ Ð¼ÐµÑÐ°Ð»Ð»Ð¾Ð², Ð¼ÐµÑÐ¾Ð´Ñ Ð·Ð°ÑÐ¸ÑÑ Ð¾Ñ ÐºÐ¾ÑÑÐ¾Ð·Ð¸Ð¸ Ð¸ Ð¼ÐµÑÐ¾Ð´Ñ ÐºÐ¾ÑÑÐ¾Ð·Ð¸Ð¾Ð½Ð½ÑÑ Ð¸ÑÐ¿ÑÑÐ°Ð½Ð¸Ð¹. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¾Ð± Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÑÑ ÐºÐ¾ÑÑÐ¾Ð·Ð¸Ð¸ ÑÐ²Ð°ÑÐ½ÑÑ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ð¹ Ð¸ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹ Ð¸ Ð¾ Ð¼ÐµÑÐ¾Ð´Ð°Ñ Ð·Ð°ÑÐ¸ÑÑ Ð¸Ñ Ð¾Ñ ÐºÐ¾ÑÑÐ¾Ð·Ð¸Ð¸. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¤Ð¢ÐÐ, ÑÐ»ÑÑÐ°ÑÐµÐ»ÐµÐ¹ ÐºÑÑÑÐ¾Ð² Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð² ÑÐ²Ð°ÑÐ¾ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð° Ð² Ð¡ÐÐ±ÐÐÐ£ Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ ÐÐ°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð°Ð³ÐµÐ½ÑÑÑÐ²Ð° ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ ÑÐ²Ð°ÑÐºÐ¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð´Ð»Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð² ÑÐ²Ð°ÑÐ¾ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð° Ð² ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ Ð¾ÑÑÐ°ÑÐ»ÑÑ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¸ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð°.
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°.
Era il Big Bang? Chiedi alla polvere
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2014

Pubblicati online i primi risultati del satellite ESA sull’emissione polarizzata della polvere a elevate latitudini galattiche. Risultati che pongono un pesante punto interrogativo sul segnale rilevato al Polo Sud da BICEP2, troppo contaminato per essere la firma inequivocabile delle onde gravitazionali primordiali
title: ÐÐ½Ð°Ð»Ð¸Ð· Ð¿Ð¾ÑÑÐµÐ±Ð¸ÑÐµÐ»ÑÑÐºÐ¸Ñ ÑÐ²Ð¾Ð¹ÑÑÐ² Ð¸ ÑÐºÑÐ¿ÐµÑÑÐ¸Ð·Ð° ÐºÐ°ÑÐµÑÑÐ²Ð° ÑÑÑÑÐ¶Ð½ÑÑ ÑÑÑÐ¾Ð²
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ¾ÑÑ, ÐÑ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: ÑÑÑÑÐ¶Ð½ÑÐµ ÑÑÑÑ
Ð°ÑÑÐ¾ÑÑÐ¸Ð¼ÐµÐ½Ñ ÑÑÑÑÐ¶Ð½ÑÑ ÑÑÑÐ¾Ð²
Ð¾ÑÐ³Ð°Ð½Ð¾Ð»ÐµÐ¿ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸
ÑÐ¸Ð·Ð¸ÐºÐ¾-Ñ Ð¸Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸
ÑÐºÑÐ¿ÐµÑÑÐ¸Ð·Ð° ÐºÐ°ÑÐµÑÑÐ²Ð°

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð» Ð¿Ð¾ ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¼Ñ ÑÐ¾ÑÑÐ°Ð²Ñ, ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¸ Ð°ÑÑÐ¾ÑÑÐ¸Ð¼ÐµÐ½ÑÑ ÑÑÑÑÐ¶Ð½ÑÑ ÑÑÑÐ¾Ð², ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð´ÐµÑÐµÐºÑÑ Ð¸ Ð¿Ð¾ÑÐ¾ÐºÐ¸ Ð¸Ñ, Ð²Ð¾Ð·Ð½Ð¸ÐºÐ°ÑÑÐ¸Ðµ Ð¿ÑÐ¸ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ðµ Ð¸ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÑÐ¸ Ð¸Ñ Ð¿ÑÐµÐ´Ð¾ÑÐ²ÑÐ°ÑÐµÐ½Ð¸Ñ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° ÑÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½Ð°Ñ ÑÐ¾Ð²Ð°ÑÐ¾Ð²ÐµÐ´Ð½Ð°Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° ÑÑÑÑÐ¶Ð½ÑÑ ÑÑÑÐ¾Ð² ÑÐ°Ð·Ð½ÑÑ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÐµÐ»ÐµÐ¹, ÑÐµÐ°Ð»Ð¸Ð·ÑÐµÐ¼ÑÐµ Ð² ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð¹ ÑÐµÑÐ¸ Ð³. Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ð°. ÐÑÐ»Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ³Ð°Ð½Ð¾Ð»ÐµÐ¿ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¸ ÑÐ¸Ð·Ð¸ÐºÐ¾-ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ ÑÑÑÐ¾Ð² ÑÐ¾Ð³Ð»Ð°ÑÐ½Ð¾ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½ÑÐ¼ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ°Ð¼. Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð±ÑÐ»Ð¾ ÑÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ð¾, ÑÑÐ¾ Ð½Ðµ Ð²ÑÐµ Ð¾Ð±ÑÐ°Ð·ÑÑ ÑÑÑÐ¾Ð² ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÑÑ ÑÑÐ°Ð½Ð´Ð°ÑÑÑ. Ð ÑÐ°Ð·Ð´ÐµÐ»Ðµ Ð¾ÑÐµÐ½ÐºÐ¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÑÑÑÐ¶Ð½ÑÑ ÑÑÑÐ¾Ð² Ð² ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð¼ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ Â«ÐÐµÐ½ÑÐ°Â» Ð±ÑÐ»Ð° ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° ÐµÐ³Ð¾ ÑÑÑÑÐºÑÑÑÐ°, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÑÐ¾Ð³Ð¾ Ð³Ð¸Ð¿ÐµÑÐ¼Ð°ÑÐºÐµÑÐ°. ÐÑÐ»Ð¾ ÑÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ð¾, ÑÑÐ¾ Ð² ÑÐµÐ»Ð¾Ð¼ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð°.
Sculpting an AGB Mass-Loss Envelope into a Bipolar Planetary Nebula: High-Velocity Outflows in V Hydrae
Creators: name: Sahai, Raghvendra
name: Sugerman, Ben E. K.
name: Hinkle, Kenneth
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We have carried out high-resolution spectroscopic observations of the carbon star V Hya, covering the 4.6 micron band of CO. These data, taken over 7 epochs, show that the circumstellar environment of V Hya consists of a complex high-velocity (HV) outflow containing at least six kinematic components with expansion velocities ranging between 70 and 120 km/s, together with a slow-moving normal outflow at about 10 km/s. Physical changes occur in the HV outflow regions on a time-scale as short as two days, limiting their extent to < ~ 10^{16} cm. The intrinsic line-width for each HV component is quite large (6-8 km/s) compared to the typical values (~1 km/s) appropriate for normal AGB circumstellar envelopes (CSEs), due to excess turbulence and/or large velocity gradients resulting from the energetic interaction of the HV outflow with the V Hya CSE. We have modelled the absorption features to set constraints on the temperature distribution in, and the mass ejection-rates for gas in the main HV components.
description: 33 pages, 6 figures
Maven nell’orbita di Marte
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2014

Dopo dieci mesi di viaggio la sonda della NASA Maven è giunta nel'orbita del pianeta rosso. La manovra si è conclusa nella notte tra domenica e lunedì in Italia. E' la prima sonda completamente dedicata allo studio dell'atmosfera di Marte
Modeling Gamma-Ray Burst X-Ray Flares within the Internal Shock Model
Creators: name: Maxham, Amanda
name: Zhang, Bing
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: X-ray afterglow light curves have been collected for over 400 Swift gamma-ray bursts with nearly half of them having X-ray flares superimposed on the regular afterglow decay. Evidence suggests that gamma-ray prompt emission and X-ray flares share a common origin and that at least some flares can only be explained by long-lasting central engine activity. We have developed a shell model code to address the question of how X-ray flares are produced within the framework of the internal shock model. The shell model creates randomized GRB explosions from a central engine with multiple shells and follows those shells as they collide, merge and spread, producing prompt emission and X-ray flares. We pay special attention to the time history of central engine activity, internal shocks, and observed flares, but do not calculate the shock dynamics and radiation processes in detail. Using the empirical E_p - E_iso (Amati) relation with an assumed Band function spectrum for each collision and an empirical flare temporal profile, we calculate the gamma-ray (Swift/BAT band) and X-ray (Swift/XRT band) lightcurves for arbitrary central engine activity and compare the model results with the observational data. We show that the observed X-ray flare phenomenology can be explained within the internal shock model. The number, width and occurring time of flares are then used to diagnose the central engine activity, putting constraints on the energy, ejection time, width and number of ejected shells. We find that the observed X-ray flare time history generally reflects the time history of the central engine, which reactivates multiple times after the prompt emission phase with progressively reduced energy...
description: 32 pages, 11 figures. ApJ, in press
Additional file 1 of circACTR2 attenuates gemcitabine chemoresiatance in pancreatic cancer through PTEN mediated PI3K/AKT signaling pathway
Creators: name: Xu, Chao
name: Ye, Qinwen
name: Ye, Chao
name: Liu, Shaojun
Publisher: name: figshare
Year: 2023
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Neuroscience
subject: Pharmacology
subject: Chemical Sciences not elsewhere classified
subject: Cancer
subject: Hematology

description: Supplementary Material 1: Table S1. List of primers used for qRT-PCR in this study
title: Ð¡ÐµÐºÑÐ¾ÑÐ½ÑÐ¹ Ð¼Ð½Ð¾Ð³Ð¾Ð¾Ð±Ð¾ÑÐ¾ÑÐ½ÑÐ¹ Ð²ÑÐµÐ¼ÑÐ¿ÑÐ¾Ð»ÐµÑÐ½ÑÐ¹ Ð¼Ð°ÑÑ-Ð°Ð½Ð°Ð»Ð¸Ð·Ð°ÑÐ¾Ñ Ñ ÑÐ¾ÐºÑÑÐ¸ÑÐ¾Ð²ÐºÐ¾Ð¹ Ð²ÑÐ¾ÑÐ¾Ð³Ð¾ Ð¿Ð¾ÑÑÐ´ÐºÐ° Ð²ÑÐµÐ¼ÐµÐ½Ð¸ Ð¿ÑÐ¾Ð»ÑÑÐ° Ð¿Ð¾ Ð¿ÑÐ¾ÑÑÑÐ°Ð½ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¼Ñ ÑÐ°Ð·Ð±ÑÐ¾ÑÑ Ð¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿Ð°ÐºÐµÑ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ÑÐ»ÑÐµÐ², Ð ÑÑÐ»Ð°Ð½
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÐÐ°ÑÑ-ÑÐ¿ÐµÐºÑÑÐ¾Ð¼ÐµÑÑÑ
ÐÐ¾Ð½Ñ
Ð¢ÑÐ°ÐµÐºÑÐ¾ÑÐ¸Ð¸
ÐÐ¸Ð½Ð·Ñ

description: Ð ÑÐ¾Ð´Ðµ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð±ÑÐ»Ð¸ Ð¿Ð¾Ð»ÑÑÐµÐ½Ñ Ð´Ð²Ð° ÑÐ¿Ð¸ÑÐ°Ð»ÑÐ½ÑÑ Ð²ÑÐµÐ¼ÑÐ¿ÑÐ¾Ð»ÐµÑÐ½ÑÑ Ð¼Ð°ÑÑ-Ð°Ð½Ð°Ð»Ð¸Ð·Ð°ÑÐ¾ÑÐ° (ÐÐÐÐ¡). ÐÐ±Ð° ÐÐÐÐ¡ Ð¾Ð±Ð»Ð°Ð´Ð°ÑÑ ÑÐ¾ÐºÑÑÐ¸ÑÐ¾Ð²ÐºÐ¾Ð¹ Ð²ÑÐµÐ¼ÐµÐ½Ð¸ Ð¿ÑÐ¾Ð»ÐµÑÐ° Ð¿Ð¾ Ð¿ÑÐ¾ÑÑÑÐ°Ð½ÑÑÐ²ÐµÐ½Ð½ÑÐ¼ ÑÐ°Ð·Ð±ÑÐ¾ÑÐ°Ð¼ Ð¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿Ð°ÐºÐµÑÐ° Ð²ÑÐ¾ÑÐ¾Ð³Ð¾ Ð¿Ð¾ÑÑÐ´ÐºÐ° Ð¸ ÑÐ¾ÐºÑÑÐ¸ÑÐ¾Ð²ÐºÐ¾Ð¹ Ð²ÑÐµÐ¼ÐµÐ½Ð¸ Ð¿ÑÐ¾Ð»ÐµÑÐ° Ð¿Ð¾ ÑÐ½ÐµÑÐ³Ð¸Ð¸ Ð¿ÐµÑÐ²Ð¾Ð³Ð¾ Ð¿Ð¾ÑÑÐ´ÐºÐ°. ÐÑÐ»Ð° Ð¿ÑÐ¾Ð´ÐµÐ¼Ð¾Ð½ÑÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð° Ð¸Ñ Ð²ÑÑÐ¾ÐºÐ°Ñ ÑÐ°Ð·ÑÐµÑÐ°ÑÑÐ°Ñ ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÑ Ð² ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ð¸ Ñ ÑÐµÑÐ¸Ð¹Ð½Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ¸Ð¼ÑÑ Spiral TOF, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°Ð½Ð¾ Ð²ÑÑÐ¾ÐºÐ¾Ðµ ÐºÐ°ÑÐµÑÑÐ²Ð¾ ÑÐ¾ÐºÑÑÐ¸ÑÐ¾Ð²ÐºÐ¸ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÑ Ð¿ÑÐ¸Ð±Ð¾ÑÐ¾Ð².
title: 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¸. Ð§. 3
title: ÑÐ±Ð¾ÑÐ½Ð¸Ðº Ð½Ð°ÑÑÐ½ÑÑ ÑÑÑÐ´Ð¾Ð² XXIV ÐÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð¹ Ð½Ð°ÑÑÐ½Ð¾Ð¹ Ð¸ ÑÑÐµÐ±Ð½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ð¸, 13â14 Ð¾ÐºÑÑÐ±ÑÑ 2020 Ð³Ð¾Ð´Ð°
titleType: Subtitle
Creators: 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Ð½Ð°Ñ Ð¸ ÑÑÐµÐ±Ð½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (24; 2020; 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: 2020
Subjects: Ð¡Ð¸ÑÑÐµÐ¼Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð·
ÐÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÐµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ

description: Ð ÑÐ±Ð¾ÑÐ½Ð¸Ðº Ð½Ð°ÑÑÐ½ÑÑ ÑÑÑÐ´Ð¾Ð² XXIV ÐÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð¹ Ð½Ð°ÑÑÐ½Ð¾Ð¹ Ð¸ ÑÑÐµÐ±Ð½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ð¸ Â«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¸Â», Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸Ð¼Ð¾Ð¹ Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¼ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¼ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ¾Ð¼ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²Ð¼ÐµÑÑÐ½Ð¾ Ñ Ð®Ð¶Ð½ÑÐ¼ ÑÐµÐ´ÐµÑÐ°Ð»ÑÐ½ÑÐ¼ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ¾Ð¼,
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Ð¦ÐµÐ½ÑÑÐ¾Ð¼ Ð¿Ð¾ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸ÐºÐ¸ ÐÐ½ÑÑÐ¸ÑÑÑÐ° Ð½Ð°ÑÑÐ½Ð¾Ð¹ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸ Ð¿Ð¾ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½ÑÐ¼ Ð½Ð°ÑÐºÐ°Ð¼ Ð ÐÐ, Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¼ Ð¸Ð½ÑÑÐ¸ÑÑÑÐ¾Ð¼
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ÑÐ»ÐµÐºÑÑÐ¾ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¼ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ¾Ð¼ Â«ÐÐ­Ð¢ÐÂ» Ð¸Ð¼. Ð. Ð. Ð£Ð»ÑÑÐ½Ð¾Ð²Ð°-ÐÐµÐ½Ð¸Ð½Ð°, Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¼ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½ÑÐ¼ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¼ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ¾Ð¼,
Ð²ÐºÐ»ÑÑÐµÐ½Ñ ÑÐ°Ð±Ð¾ÑÑ ÑÑÐµÐ½ÑÑ, Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ¾Ð² Ð¸ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², ÑÐ°Ð±Ð¾ÑÐ°ÑÑÐ¸Ñ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐµÐ¾ÑÐ¸Ð¸ ÑÐ¸ÑÑÐµÐ¼ Ð¸ ÑÐ¸ÑÑÐµÐ¼Ð½Ð¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð°, Ð¸Ð· ÑÑÐ´Ð° Ð³Ð¾ÑÐ¾Ð´Ð¾Ð² Ð Ð¾ÑÑÐ¸Ð¸, Ð£ÐºÑÐ°Ð¸Ð½Ñ,
ÐÐµÐ»Ð¸ÐºÐ¾Ð±ÑÐ¸ÑÐ°Ð½Ð¸Ð¸, ÐÐµÑÐ¼Ð°Ð½Ð¸Ð¸, Ð¡Ð¨Ð, Ð¤Ð¸Ð½Ð»ÑÐ½Ð´Ð¸Ð¸, Ð­ÑÑÐ¾Ð½Ð¸Ð¸, ÐÐ¾Ð½Ð³Ð¾.
Un Mimete sulla Stazione Spaziale
Creators: Patrizia Caraveo
Publisher: name: Media Inaf
Year: 2014

La Stazione Spaziale Internazionale si doterà di una stampante 3d. O meglio testerà il suo funzionamento, ancora piuttosto 'acerbo' per rappresentare un valido supporto nello spazio. Verificherà se la microgravità manderà in tilt i suoi, pur lenti, processi di stampa. ma è indubbio che rappresenta il futuro, un futuro immaginato da Primo Levi 50 anni fa: la sua stampante tridimensionale si chiamava 'Mimete'
Selective P-C bond cleavage of tertiary phosphine boranes by sodium
Creators: name: Zhang, Jian-Qiu
name: Ye, Jing-Jing
name: Han, Li-Biao
Publisher: name: Taylor & Francis
Year: 2021
Subjects: subject: Biophysics
subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biotechnology
subject: Evolutionary Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Developmental Biology
subject: Cancer
subject: Plant Biology

description: Herein reported is the facial modification of tertiary phosphine boranes R3PBH3 by selective cleaving the P-Ph bond by sodium in which the phosphide borohydride R2PNa(BH3) is quantitatively generated and could be easily quenched by electrophiles to furnish a series of new phosphine boranes in high yields.
Magnetic Doppler imaging of alpha^2 Canum Venaticorum in all four Stokes parameters. Unveiling the hidden complexity of stellar magnetic fields
Creators: name: Kochukhov, O.
name: Wade, G. A.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Strong organized magnetic fields have been studied in the upper main sequence chemically peculiar stars for more than half a century. However, only recently have observational methods and numerical techniques become sufficiently mature to allow us to record and interpret high-resolution four Stokes parameter spectra, leading to the first assumption-free magnetic field models of these stars. Here we present a detailed magnetic Doppler imaging analysis of the spectropolarimetric observations of the prototypical magnetic Ap star alpha^2 CVn. The surface abundance distributions of Fe and Cr and a full vector map of the stellar magnetic field are reconstructed in a self-consistent inversion using our state-of-the-art magnetic Doppler imaging code Invers10. We succeeded in reproducing most of the details of the available spectropolarimetric observations of alpha^2 CVn with a magnetic map which combines a global dipolar-like field topology with localized spots of higher field intensity. We demonstrate that these small-scale magnetic structures are inevitably required to fit the linear polarization spectra; however, their presence cannot be inferred from the Stokes I and V observations alone. Our magnetic Doppler imaging analysis of alpha^2 CVn and previous results for 53 Cam support the view that the upper main sequence stars can harbour fairly complex surface magnetic fields which resemble oblique dipoles only at the largest spatial scales. Spectra in all four Stokes parameters are absolutely essential to unveil and meaningfully characterize this field complexity in Ap stars. We therefore suggest that understanding magnetism of stars in other parts of the H-R diagram is similarly incomplete without investigation of their linear polarization spectra.
description: 16 pages, 12 figures; Accepted for publication by Astronomy & Astrophysics
A C14 tracer study of the Friedel-Crafts alkylation.
Creators: name: Forman, Allan Guy
Publisher: name: University of British Columbia
Year: 2012

description: Anisole was alkylated with 2-phenylethanol-1-C¹⁴ and 2-phenylethyl-1-C¹⁴ chloride respectively, using aluminum chloride as catalyst, to give p-methoxydibenzyl. Radioactivity assay of the p-methoxydibenzyl and of the anisic acid obtained by oxidative degradation with alkaline permanganate showed that a 50% rearrangement of C¹⁴ from the C-1 to C-2 positions occurred with both alkylating agents. The reaction may proceed by means of electrophilic attack of a free carbonium ion, or by a nucleophilic attack of anisole on a polarized complex between the alkylating agent and catalyst, if it may be assumed that the observed rearrangement has taken place during the formation of the polarized complex. The possibility exists that the rearrangement may arise from a process separate from the alkylatlon reaction itself.
Reaction between acid N'-(2-oxo-2-phenyl-ethyl)hydrazides, acetylenic esters and alkyl isocyanides in the presence of silica sulfuric acid: One-pot synthesis of highly functionalized 2,3-dihydro-1H-pyrazoles
Creators: name: Ardakani, Leili Shaker
name: Mosslemin, Mohammad H.
name: Hassanabadi, Alireza
name: Hashemian, Saeedeh
Publisher: name: Taylor & Francis
Year: 2021
Subjects: subject: Biochemistry
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Neuroscience
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 110309 Infectious Diseases
subject: 60506 Virology

description: The reactive intermediate produced in the reaction between alkyl isocyanides and dialkyl acetylenedicarboxylates was trapped by acid N'-(2-oxo-2-phenyl-ethyl)hydrazides in the presence of a catalytic amount of silica sulfuric acid (SiO2-OSO3H2) to yield highly functionalized 2,3-dihydro-1H-pyrazoles in good yields. The reaction is characterized by mild conditions and tolerance to various functional groups such as cyclohexyl, t-butyl isocyanides, and Dimethyl-, diethyl- and di-tert-butyl acetylenedicarboxylates.
title: Hand gesture recognition using sEMG with XGBoost, and averaging for augmentation
title: Ð Ð°ÑÐ¿Ð¾Ð·Ð½Ð°Ð²Ð°Ð½Ð¸Ðµ Ð¶ÐµÑÑÐ¾Ð² ÑÑÐº Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ sEMG Ñ XGBoost Ð¸ ÑÑÑÐµÐ´Ð½ÐµÐ½Ð¸Ðµ Ð´Ð»Ñ ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ñ
Creators: name: Potekhin, Vyacheslav
name: Assalama, Lara
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 Ð°ÑÐ¿Ð¾Ð·Ð½Ð°Ð²Ð°Ð½Ð¸Ðµ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²
augmentation
averaging
Myo armband
ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ðµ
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Ð¿Ð¾Ð²ÑÐ·ÐºÐ° Myo

description: In the recent years, XGBoost has proved to be a powerful, quick machinelearning algorithm, and many researcher used it to solve different types of machine learning problems. In this work, we invested it to recognize hand gesture using sEMG signals, we used with it averaging data samples as an augmentation method to overcome the lack of big dataset size, which sEMG datasets suffer from due to difficulties of gathering samples. The presented augmentation method proved to be faster than many other methods, moreover it with XGBoost gave state-of-the-art results on the used dataset.
description: Ð Ð¿Ð¾ÑÐ»ÐµÐ´Ð½Ð¸Ðµ Ð³Ð¾Ð´Ñ XGBoost Ð·Ð°ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð¾Ð²Ð°Ð» ÑÐµÐ±Ñ ÐºÐ°Ðº Ð¼Ð¾ÑÐ½ÑÐ¹ Ð¸ Ð±ÑÑÑÑÑÐ¹ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼ Ð¼Ð°ÑÐ¸Ð½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ, Ð¸ Ð¼Ð½Ð¾Ð³Ð¸Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»Ð¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð»Ð¸ ÐµÐ³Ð¾ Ð´Ð»Ñ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÑÐ¸Ð¿Ð¾Ð² Ð·Ð°Ð´Ð°Ñ Ð³Ð»ÑÐ±Ð¾ÐºÐ¾Ð³Ð¾ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ. Ð ÑÑÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¼Ñ
Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð»Ð¸ ÐµÐ³Ð¾ Ð´Ð»Ñ ÑÐ°ÑÐ¿Ð¾Ð·Ð½Ð°Ð²Ð°Ð½Ð¸Ñ Ð¶ÐµÑÑÐ¾Ð² ÑÑÐº Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÐ¸Ð³Ð½Ð°Ð»Ð¾Ð² sEMG, Ð¼Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð»Ð¸ Ñ Ð½Ð¸Ð¼ ÑÑÑÐµÐ´Ð½ÐµÐ½Ð¸Ðµ Ð²ÑÐ±Ð¾ÑÐ¾Ðº Ð´Ð°Ð½Ð½ÑÑ Ð² ÐºÐ°ÑÐµÑÑÐ²Ðµ Ð¼ÐµÑÐ¾Ð´Ð° ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ñ, ÑÑÐ¾Ð±Ñ Ð¿ÑÐµÐ¾Ð´Ð¾Ð»ÐµÑÑ Ð½ÐµÐ´Ð¾ÑÑÐ°ÑÐ¾Ðº Ð±Ð¾Ð»ÑÑÐ¾Ð³Ð¾ ÑÐ°Ð·Ð¼ÐµÑÐ° Ð½Ð°Ð±Ð¾ÑÐ° Ð´Ð°Ð½Ð½ÑÑ, Ð¾Ñ ÐºÐ¾ÑÐ¾ÑÐ¾Ð³Ð¾ ÑÑÑÐ°Ð´Ð°ÑÑ Ð½Ð°Ð±Ð¾ÑÑ Ð´Ð°Ð½Ð½ÑÑ sEMG Ð¸Ð·-Ð·Ð° ÑÑÑÐ´Ð½Ð¾ÑÑÐµÐ¹ ÑÐ±Ð¾ÑÐ° Ð²ÑÐ±Ð¾ÑÐ¾Ðº. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÐ¹ Ð¼ÐµÑÐ¾Ð´ ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ñ Ð¾ÐºÐ°Ð·Ð°Ð»ÑÑ Ð±ÑÑÑÑÐµÐµ Ð¼Ð½Ð¾Ð³Ð¸Ñ Ð´ÑÑÐ³Ð¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð², Ð±Ð¾Ð»ÐµÐµ ÑÐ¾Ð³Ð¾, Ð¾Ð½ Ñ XGBoost Ð´Ð°Ð» ÑÐ°Ð¼ÑÐµ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¿Ð¾ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÐ¼Ð¾Ð¼Ñ Ð½Ð°Ð±Ð¾ÑÑ Ð´Ð°Ð½Ð½ÑÑ.
Comment on "Rovibrational quantum interferometers and gravitational waves"
Creators: name: Khriplovich, I. B.
name: Lamoreaux, S. K.
name: Sushkov, A. O.
name: Sushkov, O. P.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: In a recent paper, Wicht, Lämmerzahl, Lorek, and Dittus [Phys. Rev. {\bf A 78}, 013610 (2008)] come to the conclusion that a molecular rotational-vibrational quantum interferometer may possess the sensitivity necessary to detect gravitational waves. We do not agree with their results and demonstrate here that the true sensitivity of such interferometer is many orders of magnitude worse than that claimed in the mentioned paper. In the present comment we estimate the expected energy shifts and derive equations of motion for a quantum symmetric top (diatomic molecule or deformed nucleus) in the field of gravitational wave, and then estimate the sensitivity of possible experiments.
description: extended version
Le corone di Miranda
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2014

In uno studio appena pubblicato dalla Società Americana di Geologia, si afferma che nonostante le sue dimensioni ridotte, la luna Miranda sembra sia stata oggetto di processi geologici di emersione che hanno portato alla formazione di almeno tre aree caratteristiche quanto uniche sulla superficie, regioni a forma poligonale chiamate corone
Misfits in Skyrme-Hartree-Fock
Creators: name: Erler, J.
name: Klüpfel, P.
name: Reinhard, P. -G.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We address very briefly five critical points in the context of the Skyrme-Hartree-Fock (SHF) scheme: 1) the impossibility to consider it as an interaction, 2) a possible inconsistency of correlation corrections as, e.g., the center-of-mass correction, 3) problems to describe the giant dipole resonance (GDR) simultaneously in light and heavy nuclei, 4) deficiencies in the extrapolation of binding energies to super-heavy elements (SHE), and 5) a yet inappropriate trend in fission life-times when going to the heaviest SHE. While the first two points have more a formal bias, the other three points have practical implications and wait for solution.
description: 9 pages, 4 figures
Prove di CTA sull’Etna
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2014

Mercoledì 24 settembre presso la stazione osservativa di Serra la Nave dell'INAF-Osservatorio Astrofisico di Catania, inaugurazione di SST, il prototipo dei telescopi di piccola taglia che comporrà parte della estesa rete di rivelatori del Cherenkov Telescope Array (CTA). Giovanni Pareschi (INAF): «siamo il primo gruppo che farà un test con un telescopio prototipale completo che rispetta perfettamente i requisiti imposti dal programma CTA»
title: ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð¿Ð¾ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¼Ñ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ñ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½ÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ¾Ð² ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸ ÑÐ²Ð°ÑÐ¾ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°
Creators: name: Ð¤Ð°ÐµÑÐ¼Ð°Ð½, ÐÑÐ¾Ð½
Publisher: name: [ÐÐÐ]
Year: 1956
Subjects: Ð¡Ð²Ð°ÑÐºÐ°

description: Ð ÐºÐ½Ð¸Ð³Ðµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð²Ð¾Ð¿ÑÐ¾ÑÑ, ÑÐ°Ð·ÑÐ°Ð±Ð°ÑÑÐ²Ð°ÐµÐ¼ÑÐµ Ð²Ð¾ Ð²Ð²ÐµÐ´ÐµÐ½Ð¸Ð¸ Ðº Ð¿ÑÐ¾ÐµÐºÑÑ, Ð² ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ñ Ð³Ð»Ð°Ð²Ð°Ñ Ð¸ Ð² ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð³Ð»Ð°Ð²Ðµ Ð¿ÑÐ¾ÐµÐºÑÐ°, Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° ÑÐ±Ð¾ÑÐ° Ð¸ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð², Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÑ Ð´Ð»Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¾ÐµÐºÑÐ°, Ð¸ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ñ Ð²ÑÐ±Ð¾ÑÐ° Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð²Ð°ÑÐ¸Ð°Ð½ÑÐ° ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ° ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ²Ð°ÑÐºÐ¸ Ð¼ÐµÑÐ°Ð»Ð»Ð¸ÑÐµÑÐºÐ¸Ñ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹ Ð¸ Ð¸Ð·Ð´ÐµÐ»Ð¸Ð¹. ÐÐ½Ð¸Ð³Ð° Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð° Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð²-Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð°Ð½ÑÐ¾Ð² ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ ÑÐ²Ð°ÑÐ¾ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°.
De l’infinito, universo e mondi
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2014

Il concetto di infinito, affrontato dalla scienza e dagli uomini che ne hanno preso parte: Trinh Xuan Thuan, astrofisico con la passione per la divulgazione, torna in libreria con un lavoro tanto ambizioso quanto affascinante che tiene insieme numeri, uomini e universi
Renormalized effective actions for the O(N) model at next-to-leading order of the 1/N expansion
Creators: name: Fejos, G.
name: Patkos, A.
name: Szep, Zs.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: A fully explicit renormalized quantum action functional is constructed for the O(N)-model in the auxiliary field formulation at next-to-leading order (NLO) of the 1/N expansion. Counterterms are consistently and explicitly derived for arbitrary constant vacuum expectation value of the scalar and auxiliary fields. The renormalized NLO pion propagator is exact at this order and satisfies Goldstone's theorem. Elimination of the auxiliary field sector at the level of the functional provides with order N^0 accuracy the renormalized effective action of the model in terms of the original variables. Alternative elimination of the pion and sigma propagators provides the renormalized NLO effective potential for the expectation values of the N-vector and of the auxiliary field with the same accuracy.
description: RevTeX4, 19 pages, 3 figures. Version published Phys. Rev. D
title: ÐÑÐ¸Ñ Ð¾Ð»Ð¾Ð³Ð¾-ÑÐ¸Ð·Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ ÑÐ¸Ð·ÐºÑÐ»ÑÑÑÑÐ½Ð¾-ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ¾ÑÐ¸ÑÐ¾Ð², ÐÐ»ÐµÐºÑÐµÐ¹
name: ÐÐ¾ÑÐºÐ¾Ð²Ð°, ÐÐ»ÐµÐ½Ð°
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2021
Subjects: ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ°Ñ ÐºÑÐ»ÑÑÑÑÐ° Ð¸ ÑÐ¿Ð¾ÑÑ
Ð¿ÑÐ¸Ñ Ð¾ÑÐ¸Ð·Ð¸Ð¾Ð»Ð¾Ð³Ð¸Ñ
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 Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¾ Ð² ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ð¸ Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¾Ð¹ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¹ Ð¿ÐµÑÐµÐ¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Â«Ð¢ÑÐµÐ½ÐµÑ. Ð¢ÐµÐ¾ÑÐ¸Ñ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° ÑÑÐµÐ½ÐµÑÑÐºÐ¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿Ð¾ Ð²Ð¸Ð´Ñ ÑÐ¿Ð¾ÑÑÐ°Â» Ð¸ Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð¾ Ð¿ÐµÐ´Ð°Ð³Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¼Ñ Ð¸ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½Ð¾Ð¼Ñ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¸ÑÐ¾ÑÐ¸Ð·Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð¾ÑÐ½Ð¾Ð² ÑÐ¸Ð·ÐºÑÐ»ÑÑÑÑÐ½Ð¾-ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸. Ð Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð¾Ð±Ð¾Ð±ÑÐµÐ½Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾-Ð°Ð½Ð°Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ, Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÐµ Ð½Ð° Ð½Ð°ÑÑÐ½Ð¾-ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ðµ ÑÐ°ÑÐºÑÑÑÐ¸Ðµ Ð¿ÑÐ¸ÑÐ¾ÑÐ¸Ð·Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð¾Ð² Ð¸ Ð·Ð°ÐºÐ¾Ð½Ð¾Ð¼ÐµÑÐ½Ð¾ÑÑÐµÐ¹ Ð¾Ð½ÑÐ¾Ð³ÐµÐ½ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐ¿Ð¾ÑÑÑÐ¼ÐµÐ½Ð¾Ð² Ð¼Ð»Ð°Ð´ÑÐµÐ³Ð¾ Ð¸ Ð¿Ð¾Ð´ÑÐ¾ÑÑÐºÐ¾Ð²Ð¾Ð³Ð¾ Ð²Ð¾Ð·ÑÐ°ÑÑÐ¾Ð². ÐÐ¿Ð¸ÑÑÐ²Ð°ÑÑÑÑ ÑÑÐ°Ð¿Ñ Ð¸ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ð¸Ñ Ð¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½Ð¾Ð¹ ÐºÐ°ÑÑÐµÑÑ, Ð¿ÑÐ¸ÑÐ¸Ð½Ñ ÐµÐµ Ð¿ÑÐµÐ¶Ð´ÐµÐ²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐµÑÑÐ²Ð°Ð½Ð¸Ñ. Ð Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð²Ð¾Ð·ÑÐ°ÑÑÐ½Ð¾Ð¹ Ð¿ÑÐ¸ÑÐ¾ÑÐ¸Ð·Ð¸Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¸ ÑÐ¼Ð¾ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÐµÐ³ÑÐ»ÑÑÐ¸Ð¸ Ð² ÑÐ¿Ð¾ÑÑÐµ, Ð¼ÐµÑÐ¾Ð´Ñ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ Ð¿ÑÐ¸ÑÐ¾ÑÐ¸Ð·Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¸ ÑÐ¼Ð¾ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ ÑÐ¿Ð¾ÑÑÑÐ¼ÐµÐ½Ð¾Ð². Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÐ»ÑÑÐ°ÑÐµÐ»ÐµÐ¹ Ð¦ÐµÐ½ÑÑÐ° Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ ÐÐ½ÑÑÐ¸ÑÑÑÐ° ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð¹ ÐºÑÐ»ÑÑÑÑÑ, ÑÐ¿Ð¾ÑÑÐ° Ð¸ ÑÑÑÐ¸Ð·Ð¼Ð° Ñ ÑÐµÐ»ÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð´Ð°Ð½Ð½ÑÑ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð² Ð´Ð»Ñ ÑÑÐµÐ±Ð½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¸ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð±ÑÐ´ÑÑÐ¸Ñ ÑÑÐµÐ½ÐµÑÐ¾Ð².
VenetoNight 2014 e dintorni
Creators: Caterina Boccato
Publisher: name: Media Inaf
Year: 2014

Anche quest'anno l'INAF di Padova partecipa all'evento di Venerdì 26 settembre, Notte Europea dei Ricercatori. Giochi, mostre, aperitivi scientifici e speedgeeking per tutti!  Cos'è lo speed-geeking?? Lo saprete solo venendo in Specola