cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Esopianeti, l’ultravioletto sfina
Creators: Mario Guarcello
Publisher: name: Media Inaf
Year: 2020

La distribuzione bimodale di raggi degli esopianeti è una conseguenza della perdita di atmosfera causata della radiazione ultravioletta emessa dalla stella centrale e incidente sui pianeti. Lo dimostra uno studio guidato da Darius Modirrousta-Galian dell’Inaf di Palermo, che prevede anche l’esistenza di un numero relativamente elevato di super-Terre
title: Ð¢ÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð¼ÐµÑ Ð°Ð½Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÑÐ°ÐºÐ°Ð½Ð°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¥Ð¼ÐµÐ»ÐµÐ², ÐÐ¸ÑÐ°Ð¸Ð»
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ
ÑÑÐ°ÐºÐ°Ð½
ÑÐ¾ÑÐµÐ½Ð¸Ðµ
ÑÐ²ÐµÑÐ»ÐµÐ½Ð¸Ðµ
ÑÑÐµÐ·Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ

description: ÐÑÐ¿ÑÑÐºÐ½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÑÐ°ÐºÐ°Ð½Ð°. ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐ½Ð¾ÑÑÐ¸ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ Ð´ÐµÑÐ°Ð»Ð¸, Ð²ÑÐ±ÑÐ°Ð½ Ð¼ÐµÑÐ¾Ð´ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ Ð¸ÑÑÐ¾Ð´Ð½Ð¾Ð¹ Ð·Ð°Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸, ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½ Ð¿ÑÐ¸Ð¿ÑÑÐº, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÑÐ°ÐºÐ°Ð½Ð°, ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½Ñ ÑÐµÐ¶Ð¸Ð¼Ñ ÑÐµÐ·Ð°Ð½Ð¸Ñ Ð¸ Ð½Ð¾ÑÐ¼Ñ Ð²ÑÐµÐ¼ÐµÐ½Ð¸ Ð½Ð° Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ðµ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¹ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ°. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð¾ ÑÑÐ°Ð½Ð¾ÑÐ½Ð¾Ðµ Ð¸ ÐºÐ¾Ð½ÑÑÐ¾Ð»ÑÐ½Ð¾-Ð¸Ð·Ð¼ÐµÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ðµ Ð¿ÑÐ¸ÑÐ¿Ð¾ÑÐ¾Ð±Ð»ÐµÐ½Ð¸Ñ.
Lampi gamma dal collasso di campi magnetici
Creators: Maura Sandri
Publisher: name: Media Inaf
Year: 2020

Un nuovo studio internazionale condotto dall’Università di Bath, che vede coinvolti tre ricercatori associati Inaf, sembra fare luce sul misterioso fenomeno dei lampi gamma. Un livello sorprendentemente basso di polarizzazione della radiazione indica che il campo magnetico della stella potrebbe essere collassato, rilasciando l'energia che ha alimentato la prodigiosa esplosione. Tutti i dettagli su ApJ
Inattesi canali magnetici in una remota galassia
Creators: Ufficio stampa Inaf
Publisher: name: Media Inaf
Year: 2020

Insolite strutture che emettono onde radio e un probabile collegamento dei campi magnetici tra i due lobi della remota radiogalassia Eso 137-006: sono questi i sorprendenti risultati dello studio condotto da un team internazionale di astronomi guidati da Mpati Ramatsoku, della Rhodes University e associata Inaf, e che vede coinvolti molti ricercatori dell'Istituto nazionale di astrofisica, pubblicato su Astronomy and Astrophysics
Double Neutral Higgs production in the Two-Higgs doublet model at the LHC
Creators: name: Arhrib, Abdesslam
name: Benbrik, Rachid
name: Chen, Chuan-Hung
name: Guedes, Renato
name: Santos, Rui
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In this work we study the production and decay of two CP-even Higgs bosons in the general CP-conserving two-Higgs doublet model at the LHC. We also study the limiting case of the decoupling scenario. For each Yukawa version of the model, we look for the region of the parameter space where a signal would be seen at the LHC. Taking into account theoretical and experimental constraints on the two Higgs doublet model parameters, we show that the cross section can be two orders of magnitude above the corresponding Standard Model cross section. We have also studied in detail the decay profile of the Higgs bosons and showed that interesting signatures may emerge for some particular values of the parameters. In some scenarios, specific triple Higgs could be measured.
description: 16 pages, 11 figures
MOESM2 of Comparisons of microbiological characteristics and antibiotic resistance of Klebsiella pneumoniae isolates from urban rodents, shrews, and healthy people
Creators: name: Zhong, Xue-shan
name: Li, Yong-zhi
name: Ge, Jing
name: Xiao, Gang
name: Mo, Yun
name: Wen, Yu-qi
name: Liu, Jing-ping
name: Xiong, Yi-quan
name: Qiu, Min
name: Huo, Shu-ting
name: Cheng, Ming-ji
name: Chen, Qing
Publisher: name: figshare
Year: 2020
Subjects: subject: Space Science
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Biotechnology
subject: Evolutionary Biology
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology

description: Additional file 2: Table S1. Primer sequences of specific gene and resistant genes for K. pneumoniae. Table S2. Primer sequences of K. pneumoniae for hypervirulent serotypes and virulent genes. Table S3. Primer sequences of seven housekeeping genes of K. peumoniae for multilocus sequence typing. Table S4. Carriage rates of KP isolates from urban rodents, house shrews, and healthy people. Table S5. Prevalence of multidrug resistance and ESBL-production among KP isolates from rodents, shrews, and healthy people (%). Table S6. Detection of hypervirulent KP isolates and virulent genes from rodents, shrews, and healthy people.
Con un poco di zolfo, la foschia va su
Creators: Laura Leonardi
Publisher: name: Media Inaf
Year: 2020

Lo zolfo è un ingrediente essenziale per la vita sulla Terra, dunque potrebbe essere anche un elemento utile alla ricerca di vita su altri pianeti. Uno studio pubblicato su Nature Astronomy illustra i risultati di simulazioni condotte in laboratorio per valutare l’impatto della presenza di zolfo in esoatmosfere ricche di anidride carbonica
Tutto su Atlas, la cometa che non vedremo mai
Creators: Giulia Iafrate e Conrad Boehm
Publisher: name: Media Inaf
Year: 2020

Si chiama C/2019 Y4 Atlas, avrebbe dovuto dar spettacolo nel mese di maggio, ma le ultime osservazioni mostrano che è in corso un processo di frammentazione del nucleo che potrebbe portarla alla distruzione. L’ha però immortalata per noi lo scorso 2 aprile Giulia Iafrate dell’Inaf di Trieste (autrice, insieme a Conrad Boehm, di questo articolo), producendo un timelapse che la mostra mentre solca il Sistema solare
Location of faults in power cables by fault-generated surges
Creators: name: Hudak, Nicholas Edward
Publisher: name: University of British Columbia
Year: 2012

description: The object of this research is to develop a satisfactory method for locating high-impedance faults in underground cables. Most methods of locating faults require that the fault-impedance be reduced to a low value before the measurement can be made. After a careful investigation of the available literature, it was decided that the most desirable method would be one utilizing the traveling-wave. Of the traveling-wave methods, the fault-generated surge method appeared to have the greatest possibilities; yet, according to the author's knowledge, this method has not been applied to power cables. In this method, the cable itself may be considered as the network that generates the required surges. The cable is initially charged to a voltage sufficiently high to establish an arc at the fault. The sudden collapse of the high voltage at the fault generates a surge which travels along the cable to the monitoring end, where it Initiates a timing device and is reflected back along the cable toward the fault. The arc which is still conducting reflects the surge back to the station. The time interval between the first and second arrival of the fault-surge at the station is recorded by the timing device and is proportional to the distance to the fault. In mathematically analyzing the surge phenomena in cables, the La Place operational method of analysis is used. The calculations for the transient produced by the discharge of a distortionless cable are worked out in full detail. The wave-form calculated is plotted and substantiated with experimental results. The transient produced is a rectangular wave that is exponentially attenuated and whose period is 4δ, where δ is the one-way transmission time of the cable in seconds. It is this wave-form generated by the cable itself that is used to locate the fault. Basically, the fault-locator developed consists of, a high-voltage low-current power pack, a triggering unit, a timing-pip generator, two uniform delay lines, and a double-beam oscilloscope. The block diagram of the fault-locator and the circuit diagrams of the triggering unit and timing-pip generator are given. The operation of the circuits and the procedure for measuring cable faults are fully explained. The fault-locator was tested on coaxial cable only, since no power cables were available. The results obtained were very satisfactory. The oscilloscope traces obtained were photographed and the experimental results discussed. It is concluded that the fault-locator can be used without modification for locating low and medium-impedance faults, as well as high-impedance faults in power cables. If the timing-pip interval is increased, the fault-locator can also be used for locating faults on overhead transmission lines.
Kernel Approximation on Manifolds I: Bounding the Lebesgue Constant
Creators: name: Hangelbroek, Thomas
name: Narcowich, Fran J.
name: Ward, Joe D.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Classical Analysis and ODEs (math.CA)
subject: Numerical Analysis (math.NA)
subject: FOS: Mathematics
subject: 41A05, 41A63, 46E22, 46E35

description: The purpose of this paper is to establish that for any compact, connected C^{\infty} Riemannian manifold there exists a robust family of kernels of increasing smoothness that are well suited for interpolation. They generate Lagrange functions that are uniformly bounded and decay away from their center at an exponential rate. An immediate corollary is that the corresponding Lebesgue constant will be uniformly bounded with a constant whose only dependence on the set of data sites is reflected in the mesh ratio, which measures the uniformity of the data. The analysis needed for these results was inspired by some fundamental work of Matveev where the Sobolev decay of Lagrange functions associated with certain kernels on Ω\subset R^d was obtained. With a bit more work, one establishes the following: Lebesgue constants associated with surface splines and Sobolev splines are uniformly bounded on R^d provided the data sites Ξare quasi-uniformly distributed. The non-Euclidean case is more involved as the geometry of the underlying surface comes into play. In addition to establishing bounded Lebesgue constants in this setting, a "zeros lemma" for compact Riemannian manifolds is established.
description: 33 pages, 2 figures, new title, accepted for publication in SIAM J. on Math. Anal
Svelato il mistero della calda atmosfera di Saturno
Creators: Maura Sandri
Publisher: name: Media Inaf
Year: 2020

Un nuovo studio pubblicato su Nature Astronomy presenta la mappatura della temperatura e della densità dell'atmosfera superiore di Saturno, effettuata grazie ai dati della sonda Cassini presi durante il Gran Finale, e rivela il probabile motivo per cui la parte superiore della sua atmosfera è così calda: le bellissime aurore visibili ai poli nord e sud del pianeta
MOESM4 of Impact of AKAP6 polymorphisms on Glioma susceptibility and prognosis
Creators: name: Zhang, Ming
name: Zhao, Yonglin
name: Zhao, Junjie
name: Huang, Tingqin
name: Wu, Yuan
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Cancer

description: Additional file 4: Table S1. The information and HWE about the candidate SNPs in AKAP6.
Holographic Renormalisation and the Electroweak Precision Parameters
Creators: name: Round, Mark
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study the effects of holographic renormalisation on an AdS/QCD inspired description of dynamical electroweak symmetry breaking. Our model is a 5D slice of AdS_5 geometry containing a bulk scalar and SU(2) times SU(2) gauge fields. The scalar field obtains a VEV which represents a condensate that triggers electroweak symmetry breaking. Fermion fields are constrained to live on the UV brane and do not propagate in the bulk. The two-point functions are holographically renormalised through the addition of boundary counterterms. Measurable quantities are then expressed in terms of well defined physical parameters, free from any spurious dependence on the UV cut-off. A complete study of the precision parameters is carried out and bounds on physical quantities derived. The large-N scaling of results is discussed.
A lattice in more than two Kac--Moody groups is arithmetic
Creators: name: Caprace, Pierre-Emmanuel
name: Monod, Nicolas
Publisher: name: arXiv
Year: 2008
Subjects: subject: Group Theory (math.GR)
subject: Metric Geometry (math.MG)
subject: FOS: Mathematics

description: Let $Γ$ be an irreducible lattice in a product of n infinite irreducible complete Kac-Moody groups of simply laced type over finite fields. We show that if n is at least 3, then each Kac-Moody groups is in fact a simple algebraic group over a local field and $Γ$ is an arithmetic lattice. This relies on the following alternative which is satisfied by any irreducible lattice provided n is at least 2: either $Γ$ is an S-arithmetic (hence linear) group, or it is not residually finite. In that case, it is even virtually simple when the ground field is large enough. More general CAT(0) groups are also considered throughout.
description: Subsection 2.B was modified and an example was added there
Goodbye, Lady Stardust
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2020

L’astrofisica angloamericana Margaret Burbidge è morta domenica scorsa all’età di 100 anni. Fondamentali i suoi studi sui processi di nucleosintesi, e in particolare un articolo del 1957 – divenuto poi celebre con l’acronimo “B2FH” – sulla sintesi degli elementi nelle stelle. Ne parliamo con Claudia Travaglio dell’Inaf di Torino
title: Generation of Pressure Pulse in Water by Pulse Magnetic Impact
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: Md. Jakaria Sarker
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¸ÑÐ½Ð¾Ðµ Ð¿Ð¾Ð»Ðµ
ÐÐ¸Ð´ÑÐ¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐ°
pulse magnetic field
pressure wave
hidrodynamics
Lorenz force
eddy current

description: Correct measurement of generating high pressure pulse in water using pulsemagnetic impact can be applied in medicine, technology, navigation etc. Circuitand magnet parameters depend on time scale, pressure intensity and specificrequirements to the pulse shape. Modern CAD systems using high performancecomputers can solve magnetic pulse impact problems with some simplifyingassumptions.
Quantum walks and elliptic integrals
Creators: name: Konno, Norio
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Physics (quant-ph)
subject: Mathematical Physics (math-ph)
subject: Probability (math.PR)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: Polya showed in his 1921 paper that the generating function of the return probability for a two-dimensional random walk can be written in terms of an elliptic integral. In this paper we present a similar expression for a one-dimensional quantum walk.
description: 8 pages, Journal-ref added
Spremuta di galassie con getto relativistico
Creators: Ufficio stampa Inaf
Publisher: name: Media Inaf
Year: 2020

Un team di ricercatori del Clemson University College of Science, in collaborazione con ricercatori di tutto il mondo, è riuscito per la prima volta in assoluto a immortalare un getto relativistico che emerge da due galassie in collisione. È la prima prova fotografica che la fusione tra galassie può produrre getti di particelle cariche che viaggiano a una velocità quasi pari a quella della luce. Allo studio, realizzato grazie alle osservazioni fatte con telescopi spaziali e da terra e pubblicato su The Astrophysical Journal, ha partecipato anche Stefano Marchesi, professore a Clemson e ricercatore Inaf
Bedelho Fanzine: Um projecto algarvio para a dinamização da Banda Desenhada portuguesa
Creators: name: Gil, Francisco Baptista
Publisher: name: Zenodo
Year: 1993
Subjects: Banda Desenhada
Algarve
Bedelho

description: Página de análise e divulgação de Banda Desenhada, publicada no Semanário Regional "Algarve Região".
title: ÐÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð¸ Ð¼Ð¾Ð´ÐµÐ»ÐµÐ¹ ÑÐ¸ÑÑÐµÐ¼Ð½Ð¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¿ÑÐ¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¸ Ð¿ÑÐ¾ÐµÐºÑÐ°Ð¼Ð¸
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ð¿Ð¾ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÐºÑÑÑÐ¾Ð²Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ
titleType: Subtitle
Creators: name: ÐÐ¾Ð»ÐºÐ¾Ð²Ð°, ÐÐ¸Ð¾Ð»ÐµÑÑÐ°
name: ÐÐµÐ½Ð¸ÑÐ¾Ð², ÐÐ½Ð°ÑÐ¾Ð»Ð¸Ð¹
name: Ð¨Ð¸ÑÐ¾ÐºÐ¾Ð²Ð°, Ð¡Ð²ÐµÑÐ»Ð°Ð½Ð°
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ Ð¡ÐÐ±ÐÐ¢Ð£
Year: 2002
Subjects: Ð¡Ð¸ÑÑÐµÐ¼Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð·
Ð­ÐºÑÐ¿ÐµÑÑÐ½ÑÐµ Ð¾ÑÐµÐ½ÐºÐ¸

description: Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÐºÐ°ÑÐµÐ´ÑÑ ÐºÐ°ÑÐµÐ´ÑÑ âÐ¡Ð¸ÑÑÐµÐ¼Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµâ Ð¤Ð°ÐºÑÐ»ÑÑÐµÑÐ° ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð¹ ÐºÐ¸Ð±ÐµÑÐ½ÐµÑÐ¸ÐºÐ¸, Ð²ÑÐ¿Ð¾Ð»Ð½ÑÑÑÐ¸Ñ ÐºÑÑÑÐ¾Ð²ÑÑ ÑÐ°Ð±Ð¾ÑÑ Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ "Ð¡Ð¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ ÑÐ¸ÑÑÐµÐ¼Ð½Ð¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð°, ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¸ Ð¿ÑÐ¸Ð½ÑÑÐ¸Ñ ÑÐµÑÐµÐ½Ð¸Ð¹". Ð Ð½ÐµÐ¼ ÑÐ¾Ð´ÐµÑÐ¶Ð°ÑÑÑ Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÐºÑÑÑÐ¾Ð²Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð¸ ÐºÑÐ°ÑÐºÐ°Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¾ÑÐ´ÐµÐ»ÑÐ½ÑÑ ÑÑÐ°Ð¿Ð¾Ð² ÑÐ°Ð·ÑÐ°Ð±Ð°ÑÑÐ²Ð°ÐµÐ¼Ð¾Ð¹ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾ÐµÐºÑÐ°Ð¼Ð¸ ÑÐ°Ð·Ð½Ð¾Ð³Ð¾ ÑÐ¾Ð´Ð°. ÐÑÐ¸Ð²Ð¾Ð´ÑÑÑÑ Ð¿ÑÐ¸Ð¼ÐµÑÑ Ð¼ÐµÑÐ¾Ð´Ð¸Ðº ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾ÐµÐºÑÐ°Ð¼Ð¸ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ
Ð¸Ð»Ð¸ ÑÐµÑÑÑÑÐºÑÑÑÐ¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ (Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸), Ð¿ÑÐ¾ÐµÐºÑÐ°Ð¼Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÐ»Ð¾Ð¶Ð½ÑÑ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ñ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ¾Ð², ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸ÐµÐ¼
Ð½Ð¾Ð²Ð¾Ð²Ð²ÐµÐ´ÐµÐ½Ð¸Ð¹ Ð² ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ ÑÑÐµÑÑ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ: Ð¾Ð±Ð½Ð¾Ð²Ð»ÐµÐ½Ð¸Ð¹ ÑÐµÑÐ½Ð¸ÐºÐ¸,ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸,ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ.
Ecco cosa c’è al cuore del quasar 3C 279
Creators: Ufficio stampa Inaf
Publisher: name: Media Inaf
Year: 2020

Gli scienziati della collaborazione Event Horizon Telescope hanno per la prima volta osservato il getto relativistico di un buco nero supermassiccio rivelandone i dettagli, i più nitidi di sempre, con una risoluzione più fine di un anno luce. Obiettivo di questo studio è il quasar 3C 279, il centro brillante una galassia distante così lontano dalla Terra che la sua luce ha impiegato più di 5 miliardi di anni per raggiungerci
Effects of cosmological parameters and star formation models on the cosmic star formation history in LambdaCDM cosmological simulations
Creators: name: Choi, Jun-Hwan
name: Nagamine, Kentaro
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We investigate the effects of the change of cosmological parameters and star formation (SF) models on the cosmic SF history using cosmological smoothed particle hydrodynamics (SPH) simulations based on the cold dark matter (CDM) model. We vary the cosmological parameters within 1-sigma error from the WMAP best-fit parameters, and find that such changes in cosmological parameters mostly affect the amplitude of the cosmic SF history. At high redshift (hereafter high-z), the star formation rate (SFR) is sensitive to the cosmological parameters that control the small-scale power of the primordial power spectrum, while the cosmic matter content becomes important at lower redshifts. We also test two new SF models: 1) the `Pressure' model based on the work by Schaye & Dalla Vecchia (2008), and 2) the `Blitz' model that takes the effect of molecular hydrogen formation into account, based on the work by Blitz & Rosolowsky (2006). Compared to the previous conventional SF model, the Pressure model reduces the SFR in low-density regions and shows better agreement with the observations of the Kennicutt-Schmidt law. This model also suppresses the early star formation and shifts the peak of the cosmic SF history toward lower redshift, more consistently with the recent observational estimates of cosmic SFR density. The simulations with the new SF model also predict lower global stellar mass densities at high-z, larger populations of low-mass galaxies and a higher gas fraction in high-z galaxies. Our results suggest that there is room left in the model uncertainties to reconcile the discrepancy that was found between the theory and observations of cosmic SF history and stellar mass density. Nevertheless, our simulations still predict higher stellar mass densities than most of the observational estimates.
description: 15 pages, 8 figures, and 2 tables accepted for publication in MNRAS
MOESM5 of Impact of AKAP6 polymorphisms on Glioma susceptibility and prognosis
Creators: name: Zhang, Ming
name: Zhao, Yonglin
name: Zhao, Junjie
name: Huang, Tingqin
name: Wu, Yuan
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Plant Biology

description: Additional file 5: Table S2. The impact of clinical factors on glioma patient OS and PFS.
title: ÐÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð±ÑÑ Ð³Ð°Ð»ÑÐµÑÑÐºÐ¾Ð³Ð¾ Ð¸ Ð½Ð°Ð»Ð¾Ð³Ð¾Ð²Ð¾Ð³Ð¾ ÑÑÐµÑÐ° Ð² Ð¾Ð±Ð¾ÑÐ¾Ð±Ð»ÐµÐ½Ð½ÑÑ Ð¿Ð¾Ð´ÑÐ°Ð·Ð´ÐµÐ»ÐµÐ½Ð¸ÑÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¹
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð§ÑÐ²Ð¸Ð»Ð¸Ð½Ð°, ÐÐ¸ÐºÑÐ¾ÑÐ¸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: Ð¾Ð±Ð¾ÑÐ¾Ð±Ð»ÐµÐ½Ð½Ð¾Ðµ Ð¿Ð¾Ð´ÑÐ°Ð·Ð´ÐµÐ»ÐµÐ½Ð¸Ðµ
ÑÐµÐ½ÑÑÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ð½ÑÐ¹ ÑÑÐµÑ
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description: Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ° ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð±ÑÑÐ³Ð°Ð»ÑÐµÑÑÐºÐ¾Ð³Ð¾ Ð¸ Ð½Ð°Ð»Ð¾Ð³Ð¾Ð²Ð¾Ð³Ð¾ ÑÑÐµÑÐ° Ð² Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸ÑÑ, Ð¸Ð¼ÐµÑÑÐ¸Ñ Ð¾Ð±Ð¾ÑÐ¾Ð±Ð»ÐµÐ½Ð½ÑÐµ Ð¿Ð¾Ð´ÑÐ°Ð·Ð´ÐµÐ»ÐµÐ½Ð¸Ñ. ÐÐ»Ñ Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ñ ÑÐµÐ»Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½ Ð¿ÑÐ¾ÑÐµÑÑ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð¾Ð±Ð¾ÑÐ¾Ð±Ð»ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð´ÑÐ°Ð·Ð´ÐµÐ»ÐµÐ½Ð¸Ñ. ÐÑÑÐ²Ð»ÐµÐ½Ñ Ð²Ð°ÑÐ¸Ð°Ð½ÑÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð±ÑÑÐ³Ð°Ð»ÑÐµÑÑÐºÐ¾Ð³Ð¾ Ð¸ Ð½Ð°Ð»Ð¾Ð³Ð¾Ð²Ð¾Ð³Ð¾ ÑÑÐµÑÐ° Ð² Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸ÑÑ, Ð¸Ð¼ÐµÑÑÐ¸Ñ Ð¾Ð±Ð¾ÑÐ¾Ð±Ð»ÐµÐ½Ð½ÑÐµ Ð¿Ð¾Ð´ÑÐ°Ð·Ð´ÐµÐ»ÐµÐ½Ð¸Ñ. ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¸ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ Ð¸Ñ ÑÐµÑÐµÐ½Ð¸Ñ, Ð° Ð¸Ð¼ÐµÐ½Ð½Ð¾, Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ¾Ð¾Ð±Ð¾ÑÐ¾ÑÐ°, Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÑÐ¾ÑÑÐ°Ð²Ð° Ð²Ð½ÑÑÑÐ¸ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½ÑÑ ÑÐ°ÑÑÐµÑÐ¾Ð², ÑÐ¿Ð¾ÑÐ¾Ð±Ð°Ð¼ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð½Ð°Ð»Ð¾Ð³Ð¾Ð² Ð¸ Ñ.Ð´.
Mid-infrared time-domain study of recent dust production events in the extreme debris disc of TYC 4209-1322-1
Creators: name: Moór, A.
name: Ábrahám, P.
name: Kóspál, Á.
name: Su, K. Y. L.
name: Rieke, G. H.
name: Cataldi, G.
name: Bódi, A.
name: Bognár, Zs.
name: Cseh, B.
name: Csörnyei, G.
name: Egei, N.
name: Farkas, A.
name: Hanyecz, O.
name: Ignácz, B.
name: Kalup, Cs.
name: Könyves-Tóth, R.
name: Kriskovics, L.
name: Mészáros, L.
name: Pál, A.
name: Ordasi, A.
name: Sárneczky, K.
name: Seli, B.
name: Sódor, Á.
name: Szakáts, R.
name: Vinkó, J.
name: Zsidi, G.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Extreme debris discs are characterized by unusually strong mid-infrared excess emission, which often proves to be variable. The warm dust in these discs is of transient nature and is likely related to a recent giant collision occurring close to the star in the terrestrial region. Here we present the results of a 877 days long, gap-free photometric monitoring performed by the Spitzer Space Telescope of the recently discovered extreme debris disc around TYC 4209-1322-1. By combining these observations with other time-domain optical and mid-infrared data, we explore the disc variability of the last four decades with particular emphasis on the last 12 yr. During the latter interval the disc showed substantial changes, the most significant was the brightening and subsequent fading between 2014 and 2018 as outlined in WISE data. The Spitzer light curves outline the fading phase and a subsequent new brightening of the disc after 2018, revealing an additional flux modulation with a period of ~39 days on top of the long-term trend. We found that all these variations can be interpreted as the outcome of a giant collision that happened at an orbital radius of ~0.3 au sometime in 2014. Our analysis implies that a collision on a similar scale could have taken place around 2010, too. The fact that the disc was already peculiarly dust rich 40 yr ago, as implied by IRAS data, suggests that these dust production events belong to a chain of large impacts triggered by an earlier even more catastrophic collision.
description: 18 pages, 12 figures, published in MNRAS
FALSAFAH PANCASILA SEBAGAI LANDASAN PENDIDIKAN DALAM LAYANAN BIMBINGAN DAN KONSELING DI INDONSESIA
Creators: name: hasrul, hasrul
name: Habsyi, Irsan
name: Makki, M. Ismail
Publisher: name: Zenodo
Year: 2023

description: This research aims to find a conceptual explanation regarding Pencasila as a philosophical system and as a basis for education in the implementation of guidance and counseling in Indonesia. The method used is library research which refers to four steps, namely; selecting concepts to be reviewed, reading and analyzing (synthesizing) literature, and writing articles. The results of the conceptual analysis of this study explain that the Pancasila philosophy is closely related to guidance and counseling, because it is by its main essence, namely always prioritizing the principles of comfort and prosperity in living together among fellow humans. Apart from that, Pancasila is also a foundation of education and a basic foundation and framework for guidance and counseling teachers/school counselors in implementing guidance and counseling services in Indonesia. Currently and in the future, guidance and counseling teachers/school counselors and other guidance and counseling practitioners can implement two major issues, namely religious counseling and multicultural counseling which are in line with the essence of the Pancasila philosophy in Indonesia.
description: Tujuan penelitian ini ialah untuk mengetahui penjelasan secara konseptual mengenai Pencasila sebagai suatu sistem falsafah dan menjadi landasan pendidikan dalam pelaksanaan bimbingan dan konseling (BK) di Indonesia. Metode yang digunakan ialah penelitian kepustakaan (library research) yang mengacu pada empat langkah, yaitu;  memilih konsep yang akan diulas, membaca, dan menganalisis (sintesa) literatur, dan menulis artikel. Hasil telaah konseptual dari studi ini menjelaskan bahwa falsafah Pancasila sangat memiliki kaitan erat dengan bimbingan dan konseling, karena sesuai dengan hakikat utamanya yaitu senantiasa mengutamakan pada asas kenyamanan dan kesejahteraan hidup bersama antar sesama manusia. Selain itu, Pancasila juga merupakan suatu landasan pendidikan dan sebagai dasar pijakan serta kerangka kerja bagi guru BK/konselor sekolah dalam melaksanakan layanan BK di Indonesia. Saat ini dan ke depan nanti, guru BK/konselor sekolah dan praksis BK lainnya dapat mengimplementasikan dua isu besar yaitu konseling religius dan konseling multikultural yang sejalan dengan hakikat falsafah Pancasila di Indonesia.
An electromagnetic transducer for the production of shock waves in air
Creators: name: Cowie, Eric Gordon
Publisher: name: University of British Columbia
Year: 2012

description: The recent development of gas turbines, high speed aircraft, and similar machines, has made the study of shock waves of practical importance. This report concerns an electromagnetic method of producing repeated shock waves in air. The most simple shock wave generator, from a mathematical viewpoint, consists of a piston which starts from rest and moves with constant velocity into a tube containing the air. An attempt has been made here to approximate such piston motion by means of the forces acting on a conductor placed in a pulsed magnetic field. Although no shook waves have been produced, an electrical circuit has been developed to provide current pulses of the high amplitude necessary for such a device. A prototype transducer also has been constructed and tested. The report is primarily a description of this circuit. Basically, the pulse generator consists of two ignitrons, the first of which is in series with the transducer field coil and a high current source. The second ignitron is connected in such a manner that, when it is fired, it causes the extinction of the first. In this way, current pulses are passed through the field coil.
Immigrated urn models - asymptotic properties and applications
Creators: name: Zhang, Li-Xin
name: Hu, Feifang
name: Cheung, Siu Hung
name: Chan, Wei Sum
Publisher: name: arXiv
Year: 2008
Subjects: subject: Statistics Theory (math.ST)
subject: Probability (math.PR)
subject: Methodology (stat.ME)
subject: FOS: Mathematics
subject: FOS: Computer and information sciences
subject: 60F15, 62L05

description: Urn models have been widely studied and applied in both scientific and social science disciplines. In clinical studies, the adoption of urn models in treatment allocation schemes has been proved to be beneficial to both researchers, by providing more efficient clinical trials, and patients, by increasing the likelihood of receiving the better treatment. In this paper, we propose a new and general class of immigrated urn (IMU) models that incorporates the immigration mechanism into the urn process. Theoretical properties are developed and the advantages of the IMU models are discussed. In general, the IMU models have smaller variabilities than the classical urn models, yielding more powerful statistical inferences in applications. Illustrative examples are presented to demonstrate the wide applicability of the IMU models. The proposed IMU framework, including many popular classical urn models, not only offers a unify perspective for us to comprehend the urn process, but also enables us to generate several novel urn models with desirable properties.
Oh oh, abbiamo rotto la cometa aliena
Creators: Albino Carbognani
Publisher: name: Media Inaf
Year: 2020

Recenti osservazioni della cometa interstellare 2I/Borisov compiute con il telescopio spaziale Hubble hanno messo in evidenza un fenomeno di frammentazione del nucleo, come accade di frequente anche per le comete appartenenti al Sistema solare. Il frammento, con dimensioni stimate dell'ordine di 100 metri, si è dissolto in pochi giorni nello spazio
Additional file 1 of Efficacy and safety of butylphthalide in secondary prevention of stroke: study protocol for a multicenter, real world trial based on Internet
Creators: name: Lv, Junchao
name: Zhao, Di
name: Zhao, Gang
name: Xie, Zhen
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Neuroscience
subject: Pharmacology
subject: Biotechnology
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1: Appendix 1. The list of recruitment hospitals.
A new form of Tsallis distribution based on the probabilistically independent postulate
Creators: name: Du, Jiulin
Publisher: name: arXiv
Year: 2009
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The current form of Tsallis distribution for a Hamiltonian system with an arbitrary potential is found to represent a simple isothermal situation. In this letter, the q-exponential of a sum can be applied as the product of the q-exponential based on the probabilistically independent postulate employed in nonextensive statistical mechanics. Under this framework, a new form of Tsallis distribution is suggested. It is shown that the new form of Tsallis distribution can supply the statistical description for the nonequilibrium dynamical property of the Hamiltonian system governed by an arbitrary potential, and it is found to be one potential statistical distribution for the dark matter.
description: 11 pages
Macchie in vista: il Sole esce dal suo lungo letargo
Creators: Redazione Ansa
Publisher: name: Media Inaf
Year: 2020

Un gruppo di macchie nell’emisfero settentrionale della nostra stella indica che la riorganizzazione del campo magnetico solare è in corso, spiega Mauro Messerotti (Inaf Trieste) all’Ansa. Ma prima che il nuovo ciclo abbia effettivamente inizio potrebbero passare ancora diversi mesi
Supersymmetries of the spin-1/2 particle in the field of magnetic vortex, and anyons
Creators: name: Correa, Francisco
name: Falomir, Horacio
name: Jakubsky, Vit
name: Plyushchay, Mikhail S.
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The quantum nonrelativistic spin-1/2 planar systems in the presence of a perpendicular magnetic field are known to possess the N=2 supersymmetry. We consider such a system in the field of a magnetic vortex, and find that there are just two self-adjoint extensions of the Hamiltonian that are compatible with the standard N=2 supersymmetry. We show that only in these two cases one of the subsystems coincides with the original spinless Aharonov-Bohm model and comes accompanied by the super-partner Hamiltonian which allows a singular behavior of the wave functions. We find a family of additional, nonlocal integrals of motion and treat them together with local supercharges in the unifying framework of the tri-supersymmetry. The inclusion of the dynamical conformal symmetries leads to an infinitely generated superalgebra, that contains several representations of the superconformal osp(2|2) symmetry. We present the application of the results in the framework of the two-body model of identical anyons. The nontrivial contact interaction and the emerging N=2 linear and nonlinear supersymmetries of the anyons are discussed.
description: 18 pages, 1 figure, published version
title: ÐÐ°Ð»Ð¾Ð³Ð¾Ð¾Ð±Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ Ð¼Ð°Ð»Ð¾Ð³Ð¾ Ð±Ð¸Ð·Ð½ÐµÑÐ° Ð² Ð Ð¾ÑÑÐ¸Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾ Ð¦Ð·ÑÐ½Ñ,
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: Ð¼Ð°Ð»ÑÐ¹ Ð±Ð¸Ð·Ð½ÐµÑ
Ð½Ð°Ð»Ð¾Ð³Ð¾Ð¾Ð±Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ Ð¼Ð°Ð»Ð¾Ð³Ð¾ Ð±Ð¸Ð·Ð½ÐµÑÐ°
ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð½Ð°Ð»Ð¾Ð³Ð¾Ð¾Ð±Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ

description: ÐÐ±ÑÐµÐºÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ - Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½ÑÐµ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ, Ð²Ð¾Ð·Ð½Ð¸ÐºÐ°ÑÑÐ¸Ðµ ÑÐ²ÑÐ·Ð¸ Ñ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÐµÐ¼ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð°Ð»Ð¾Ð³Ð¾Ð¾Ð±Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¼Ð°Ð»Ð¾Ð³Ð¾ Ð±Ð¸Ð·Ð½ÐµÑÐ° Ð² Ð Ð¾ÑÑÐ¸Ð¸. ÐÑÐµÐ´Ð¼ÐµÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ - Ð½Ð¾ÑÐ¼Ñ Ð¿ÑÐ°Ð²Ð°, ÑÐµÐ³ÑÐ»Ð¸ÑÑÑÑÐ¸Ðµ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð°Ð»Ð¾Ð³Ð¾Ð¾Ð±Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¼Ð°Ð»Ð¾Ð³Ð¾ Ð±Ð¸Ð·Ð½ÐµÑÐ° Ð² Ð Ð¾ÑÑÐ¸Ð¸. Ð¦ÐµÐ»Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ - Ð¿ÑÐ¾Ð²ÐµÑÑÐ¸ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð°Ð»Ð¾Ð³Ð¾Ð¾Ð±Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¼Ð°Ð»Ð¾Ð³Ð¾ Ð±Ð¸Ð·Ð½ÐµÑÐ° Ð² Ð Ð¾ÑÑÐ¸Ð¸.
Srt, in ascolto del cosmo dall’altopiano del sangue
Creators: Giuseppe Fiasconaro
Publisher: name: Media Inaf
Year: 2020

È gestito dall’Istituto nazionale di astrofisica. Si trova nel comune di San Basilio, a sud della Sardegna, ed è uno fra i telescopi per astronomia radio più performanti che esistano. È il Sardinia Radio Telescope, un colosso da 3000 tonnellate alto quanto un palazzo di circa venti piani. Il suo “amministratore di condominio” è Sergio Poppi, dell’Inaf di Cagliari. Lo abbiamo intervistato per conoscere lo stato di operatività in cui si trova il telescopio
Targeted profiling of human extrachromosomal DNA by CRISPR-CATCH.
Creators: name: Hung, King L
name: Luebeck, Jens
name: Dehkordi, Siavash R
name: Colón, Caterina I
name: Li, Rui
name: Wong, Ivy Tsz-Lo
name: Coruh, Ceyda
name: Dharanipragada, Prashanthi
name: Lomeli, Shirley H
name: Weiser, Natasha E
name: Moriceau, Gatien
name: Zhang, Xiao
name: Bailey, Chris
name: Houlahan, Kathleen E
name: Yang, Wenting
name: González, Rocío Chamorro
name: Swanton, Charles
name: Curtis, Christina
name: Jamal-Hanjani, Mariam
name: Henssen, Anton G
name: Law, Julie A
name: Greenleaf, William J
name: Lo, Roger S
name: Mischel, Paul S
name: Bafna, Vineet
name: Chang, Howard Y
Publisher: name: The Francis Crick Institute
Year: 2022
Subjects: classificationCode: Tumour Biology
subject: Tumour Biology
classificationCode: Signalling & Oncogenes
subject: Signalling & Oncogenes
classificationCode: Genetics & Genomics
subject: Genetics & Genomics
classificationCode: Genome Integrity & Repair
subject: Genome Integrity & Repair
classificationCode: Human Biology & Physiology
subject: Human Biology & Physiology
classificationCode: Chemical Biology & High Throughput
subject: Chemical Biology & High Throughput
classificationCode: Ecology,Evolution & Ethology
subject: Ecology,Evolution & Ethology
classificationCode: Computational & Systems Biology
subject: Computational & Systems Biology

description: Extrachromosomal DNA (ecDNA) is a common mode of oncogene amplification but is challenging to analyze. Here, we adapt CRISPR-CATCH, in vitro CRISPR-Cas9 treatment and pulsed field gel electrophoresis of agarose-entrapped genomic DNA, previously developed for bacterial chromosome segments, to isolate megabase-sized human ecDNAs. We demonstrate strong enrichment of ecDNA molecules containing EGFR, FGFR2 and MYC from human cancer cells and NRAS ecDNA from human metastatic melanoma with acquired therapeutic resistance. Targeted enrichment of ecDNA versus chromosomal DNA enabled phasing of genetic variants, identified the presence of an EGFRvIII mutation exclusively on ecDNAs and supported an excision model of ecDNA genesis in a glioblastoma model. CRISPR-CATCH followed by nanopore sequencing enabled single-molecule ecDNA methylation profiling and revealed hypomethylation of the EGFR promoter on ecDNAs. We distinguished heterogeneous ecDNA species within the same sample by size and sequence with base-pair resolution and discovered functionally specialized ecDNAs that amplify select enhancers or oncogene-coding sequences.
Adaptive Mesh Refinement for Characteristic Grids
Creators: name: Thornburg, Jonathan
Publisher: name: arXiv
Year: 2009
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences

description: I consider techniques for Berger-Oliger adaptive mesh refinement (AMR) when numerically solving partial differential equations with wave-like solutions, using characteristic (double-null) grids. Such AMR algorithms are naturally recursive, and the best-known past Berger-Oliger characteristic AMR algorithm, that of Pretorius & Lehner (J. Comp. Phys. 198 (2004), 10), recurses on individual "diamond" characteristic grid cells. This leads to the use of fine-grained memory management, with individual grid cells kept in 2-dimensional linked lists at each refinement level. This complicates the implementation and adds overhead in both space and time. Here I describe a Berger-Oliger characteristic AMR algorithm which instead recurses on null \emph{slices}. This algorithm is very similar to the usual Cauchy Berger-Oliger algorithm, and uses relatively coarse-grained memory management, allowing entire null slices to be stored in contiguous arrays in memory. The algorithm is very efficient in both space and time. I describe discretizations yielding both 2nd and 4th order global accuracy. My code implementing the algorithm described here is included in the electronic supplementary materials accompanying this paper, and is freely available to other researchers under the terms of the GNU general public license.
description: 37 pages, 15 figures (40 eps figure files, 8 of them color; all are viewable ok in black-and-white), 1 mpeg movie, uses Springer-Verlag svjour3 document class, includes C++ source code. Changes from v1: revised in response to referee comments: many references added, new figure added to better explain the algorithm, other small changes, C++ code updated to latest version
Due stelle di elio per Lisa
Creators: Maura Sandri
Publisher: name: Media Inaf
Year: 2020

Dal Center for Astrophysics di Harvard arriva la conferma della scoperta di un sistema binario formato da due nane bianche con nucleo di elio, caratterizzato da un periodo orbitale estremamente breve: 1201 secondi – il terzo sistema binario con il periodo più breve a oggi conosciuto.  Si stima che tale sistema potrà essere osservato da Lisa con un rapporto segnale-rumore pari a 40 in 4 anni di osservazioni. I risultati dello studio saranno pubblicati su ApJ
D2.4 Geographic data and services inventory
Creators: name: Efthimiou, George
name: Tsegas, George
name: Barmpas, Fotios
Publisher: name: Zenodo
Year: 2020

description: This document aims to record all the necessary and available data that are required for the realization of the current project. This is accomplished by creating a list that summarizes the information provided by all stakeholders, especially from open sources. It includes data that has already been gathered as well as data that is still pending.
title: L' acceptation des différences culturelles en musique
title: L' acceptation des différences culturelles en musique
titleType: AlternativeTitle
Creators: name: Warga, Estelle Amélia
name: Pham, Minh Tu An
Publisher: name: Unknown
Year: 0
Subjects: subject: enseignement
subject: musique
subject: interculturalité
subject: acceptations des différences
subject: mouvement
subject: écoute

description: Notre recherche porte sur le thème de la diversité culturelle. Plus précisément, nous nous intéressons à l’utilisation de musiques étrangères pour travailler l’acceptation des différences culturelles au cycle 1. À travers une méthode expérimentale qualitative et une étude de cas nous tentons de répondre à la question suivante : « Comment l’écoute de musiques étrangères lors de leçons de musique en classe de 3e HarmoS peut-elle favoriser l’acceptation des différences culturelles ? » Dans ce but, nous mettons en place une séquence de cinq séances dans deux classes de 3e HarmoS. Dans chaque séance, nous présentons une musique étrangère propice aux mouvements et choisie selon des critères d’authenticité. Nous observons sept élèves lors de moments d’écoute en position assise, puis en mouvements. Finalement, nous donnons aux élèves un espace de parole pour qu’ils expriment leurs ressentis. Après analyse des résultats, nous remarquons que les élèves peuvent avoir des réactions diverses face aux musiques étrangères et que l’acceptation des différences semble plus difficile pour certains. En outre, nous observons que le sentiment d’étrangeté exprimé par certains élèves en début de séquence s’est progressivement atténué au cours des séances, et que les élèves y ont manifesté un plaisir croissant à travers celle-ci. Notre séquence a également permis aux élèves de découvrir des musiques d’autres pays et de dépasser certains préjugés les concernant. Aussi, à travers les moments de verbalisation, les élèves ont pu prendre conscience de leurs perceptions, ainsi que travailler sur la communication non violente. Au moyen de ces différents éléments, nous répondons à notre question de recherche. Finalement, les observations faites lors de notre travail amènent des points de discussion qu’il serait intéressant d’approfondir. Elles concernent le mouvement et ses effets sur le plaisir et sur l’acceptation des différences culturelles, ainsi que sur l’agitation des élèves face aux musiques qu’ils ont écoutées.
Perseverance al pit stop
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2020

Cambio gomme per il rover Nasa: ultimi test agli “pneumatici” in vista del lancio. Progettate per percorrere una media di 200 metri al giorno, le ruote di Perseverance sono una versione evoluta di quelle in dotazione a Curiosity. Per ora l’agenda della missione non ha subito rallentamenti a causa della pandemia in corso
title: ÐÑÐºÑÐ¸ÐºÐ°: Ð¸ÑÑÐ¾ÑÐ¸Ñ Ð¸ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾ÑÑÑ
title: ÑÑÑÐ´Ñ ÐµÐ¶ÐµÐ³Ð¾Ð´Ð½Ð¾Ð¹ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð¹ Ð½Ð°ÑÑÐ½Ð¾Ð¹ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ð¸, Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³, 18-19 Ð°Ð¿ÑÐµÐ»Ñ 2019 Ð³Ð¾Ð´Ð°
titleType: Subtitle
Creators: name: "ÐÑÐºÑÐ¸ÐºÐ°: Ð¸ÑÑÐ¾ÑÐ¸Ñ Ð¸ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾ÑÑÑ", ÐµÐ¶ÐµÐ³Ð¾Ð´Ð½Ð°Ñ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð°Ñ Ð½Ð°ÑÑÐ½Ð°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (4; 2019; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2019
Subjects: Ð­ÐºÐ¾Ð»Ð¾Ð³Ð¸Ñ
ÐÐµÐ¾Ð³ÑÐ°ÑÐ¸Ñ
ÐÑÐºÑÐ¸ÐºÐ°
Ð³ÐµÐ¾Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ°
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description: Ð XXI Ð²ÐµÐºÐµ ÐÑÐºÑÐ¸ÑÐµÑÐºÐ¸Ð¹ ÑÐµÐ³Ð¸Ð¾Ð½ Ð¸Ð³ÑÐ°ÐµÑ Ð¸ÑÐºÐ»ÑÑÐ¸ÑÐµÐ»ÑÐ½ÑÑ ÑÐ¾Ð»Ñ Ð² Ð³ÐµÐ¾Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐµ.
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BepiColombo saluta la Terra
Creators: Ufficio stampa Inaf
Publisher: name: Media Inaf
Year: 2020

L'appuntamento con il nostro pianeta è previsto il 10 aprile. Per arrivare alla meta, la sonda effettuerà altri voli ravvicinati per sfruttare le spinte gravitazionali: due attorno a Venere e sei attorno a Mercurio