cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Le cicatrici di Marte
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2013

Un gigantesco canyon marziano, creato dall'attività del più grande vulcano del sistema solare, è il protagonista di un dettagliatissimo mosaico di immagini riprese dalla sonda Mars Express. La regione, chiamata Hebes Chasma, porta su di sé i segni delle fasi più violente della storia del pianeta rosso.
title: ÐÑÐµÐ½ÐºÐ° Ð²Ð»Ð¸ÑÐ½Ð¸Ñ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸ ÐºÐ¾Ð¼Ð¿Ð¾Ð·Ð¸ÑÐ½ÑÑ Ð¾Ð¿Ð¾Ñ Ð½Ð° ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾Ð»Ñ Ð²Ð´Ð¾Ð»Ñ Ð³Ð¸ÑÐ»ÑÐ½Ð´Ñ Ð¸Ð·Ð¾Ð»ÑÑÐ¾ÑÐ¾Ð²
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·Ð½ÐµÑÐ¾Ð², ÐÐ°Ð´Ð¸Ð¼
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Ð¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð»Ð¸Ð½Ð¸Ð¸ Ð¿ÐµÑÐµÐ´Ð°ÑÐ¸ Ð²Ð¾Ð·Ð´ÑÑÐ½ÑÐµ
ÐÐ¿Ð¾ÑÑ Ð´Ð»Ñ Ð»Ð¸Ð½Ð¸Ð¹ ÑÐ»ÐµÐºÑÑÐ¾Ð¿ÐµÑÐµÐ´Ð°ÑÐ¸
ÐÐ¾Ð¼Ð¿Ð¾Ð·Ð¸ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ Ð¿Ð¾Ð»Ð¸Ð¼ÐµÑÐ½ÑÐµ
Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ½ÐµÑÐ³Ð¸Ñ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð²Ð¾Ð¿ÑÐ¾ÑÑ, ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÐµ Ñ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¾Ð¹ ÐºÐ¾Ð¼Ð¿Ð¾Ð·Ð¸ÑÐ½ÑÑ Ð¾Ð¿Ð¾Ñ Ð»Ð¸Ð½Ð¸Ð¹ ÑÐ»ÐµÐºÑÑÐ¾Ð¿ÐµÑÐµÐ´Ð°ÑÐ¸. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° Ð²Ð»Ð¸ÑÐ½Ð¸Ñ ÐºÐ¾Ð¼Ð¿Ð¾Ð·Ð¸ÑÐ½ÑÑ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð² Ð½Ð° ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾Ð»Ñ Ð²Ð´Ð¾Ð»Ñ Ð³Ð¸ÑÐ»ÑÐ½Ð´Ñ. ÐÐ¾ÑÑÑÐ¾ÐµÐ½Ñ Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð² Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ðµ Ð´Ð»Ñ Ð¼ÑÐ»ÑÑÐ¸ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð½ÑÑ ÑÐ°ÑÑÐµÑÐ¾Ð² Ð¿Ð¾Ð»ÑÑÐµÐ½Ñ Ð²ÐµÐ»Ð¸ÑÐ¸Ð½Ñ ÐºÐ¾ÑÑÑÐ¸ÑÐ¸ÐµÐ½ÑÐ° Ð½ÐµÐ¾Ð´Ð½Ð¾ÑÐ¾Ð´Ð½Ð¾ÑÑÐ¸.
Qui una volta era tutto un pianeta
Creators: Nicola Nosengo
Publisher: name: Media Inaf
Year: 2013

Attorno alla nana bianca GD 61 si vedono i resti di almeno un pianeta roccioso e con abbondanti quantità di acqua. Doveva trattarsi di un sistema planetario molto simile al nostro e sulla carta in grado di ospitare la vita, prima che la sua stella morisse. E anche il nostro sistema prima o poi finirà così. Lo studio su Science
Digi-Religion and How To Capture It: KADOC-KU Leuven's Website Archiving Project
Creators: name: Messens, Fien
name: Weyns, Katrien
Publisher: name: Zenodo
Year: 2023
Subjects: web archiving
born-digital heritage collections

description: This abstract for a poster presentation discusses the importance of creating a space in archives to incorporate website archiving next to an already existing workflow for physical data. The focal point is placed on the ethical questions of web archiving, and the hurdles that pop up - all this in dialogue with the research potential and the needs of future users.
Una galassia delicata come un fiore
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2013

Si vede nella costellazione dell'Idra ed è un bellissimo esempio di galassia ellittica con una struttura sfocata all'esterno. La particolarità della galassia PGC 6240 sono i numerosi cluster che le orbitano attorno, alcuni più antichi e altri molto giovani. Sono il risultato di una collisione tra galassie nel passato.
Strings on Bubbling Geometries
Creators: name: Lin, Hai
name: Morisse, Alexander
name: Shock, Jonathan P.
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We study gauge theory operators which take the form of a product of a trace with a Schur polynomial, and their string theory duals. These states represent strings excited on bubbling AdS geometries which are dual to the Schur polynomials. These geometries generically take the form of multiple annuli in the phase space plane. We study the coherent state wavefunction of the lattice, which labels the trace part of the operator, for a general Young tableau and their dual description on the droplet plane with a general concentric ring pattern. In addition we identify a density matrix over the coherent states on all the geometries within a fixed constraint. This density matrix may be used to calculate the entropy of a given ensemble of operators. We finally recover the BMN string spectrum along the geodesic near any circle from the ansatz of the coherent state wavefunction.
description: 41 pages, 12 figures, published version in JHEP
Volontari della cultura scientifica
Creators: Laura Daricello
Publisher: name: Media Inaf
Year: 2013

Il Servizio Civile Nazionale è per i volontari una grande opportunità di crescita sul piano personale e relazionale e di avvicinamento al mondo del lavoro. Ne sono testimonianza le esperienze di Servizio Civile Nazionale al Museo della Specola, presso l’INAF – Osservatorio Astronomico di Palermo.
In bilico fra stelle e pianeti
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2013

Scoperti due corpi celesti ardui da catalogare: pianeti solitari giganti o nane brune di massa estremamente ridotta? Entrambi di formazione assai recente – 12 milioni di anni uno, appena 2 milioni l’altro – si trovano rispettivamente a 80 e 500 anni luce da noi. Gli studi in uscita su ApJ e A&A.
Cosmological Moduli Problem from Thermal Effects
Creators: name: Nakayama, Kazunori
name: Takahashi, Fuminobu
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We estimate the cosmological abundance of a modulus field that has dilatonic couplings to gauge fields, paying particular attention to thermal corrections on the modulus potential. We find that a certain amount of the modulus coherent oscillations is necessarily induced by a linear thermal effect. We argue that such an estimate provides the smallest possible modulus abundance for a given thermal history of the Universe. As an example we apply our results to a saxion, a bosonic supersymmetric partner of an axion, and derive a tight bound on the reheating temperature. We emphasize that the problem cannot be avoided by fine-tuning the initial deviation of the modulus field, since the minimal amount of the modulus is induced by the dynamics of the scalar potential.
description: 9 pages, 1 figure; to appear in PLB
Un pezzo di cometa sulla Terra
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2013

Un frammento di diamante ritrovato in Egitto, e chiamato Ipazia, è il primo resto di una cometa caduta sulla Terra mai ritrovato. E potrebbe anche aiutare i ricercatori a scoprire i segreti della formazione del nostro Sistema solare. Lo studio su Earth and Planetary Science Letters.
The Nuclear Outflows and Feedback in the Seyfert 2 Galaxy Markarian 573
Creators: name: Schlesinger, K.
name: Pogge, Richard W.
name: Martini, Paul
name: Shields, Joseph C.
name: Fields, Dale
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a study of outflow and feedback in the well-known Seyfert 2 galaxy Markarian 573 using high angular resolution long-slit spectrophotometry obtained with the Hubble Space Telescope Imaging Spectrograph (STIS). Through analysis of the kinematics and ionization state of a biconical outflow region emanating from the nucleus, we find that the outflow does not significantly accelerate the surrounding host-galaxy interstellar gas and is too weak to be a strong ionization mechanism in the extended emission regions. Instead, the excitation of the extended regions is consistent with photoionization by the active nucleus. From energetics arguments we show that the nuclear outflow is slow and heavy and has a mechanical luminosity that is only ~1% of the estimated bolometric luminosity of the system. The energy in the outflow is able to mildly shape the gas in the extended regions but appears to be insufficient to unbind it, or even to plausibly disrupt star formation. These results are at odds with the picture of strong AGN feedback that has been invoked to explain certain aspects of galaxy evolution.
description: 31 pages, 7 figures, 4 tables
A geometric theory of zero area singularities in general relativity
Creators: name: Bray, Hubert L.
name: Jauregui, Jeffrey L.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Differential Geometry (math.DG)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 53C20, 53C80, 83C99

description: The Schwarzschild spacetime metric of negative mass is well-known to contain a naked singularity. In a spacelike slice, this singularity of the metric is characterized by the property that nearby surfaces have arbitrarily small area. We develop a theory of such "zero area singularities" in Riemannian manifolds, generalizing far beyond the Schwarzschild case (for example, allowing the singularities to have nontrivial topology). We also define the mass of such singularities. The main result of this paper is a lower bound on the ADM mass of an asymptotically flat manifold of nonnegative scalar curvature in terms of the masses of its singularities, assuming a certain conjecture in conformal geometry. The proof relies on the Riemannian Penrose Inequality. Equality is attained in the inequality by the Schwarzschild metric of negative mass. An immediate corollary is a version of the Positive Mass Theorem that allows for certain types of incomplete metrics.
description: 36 pages, 9 figures
title: ÐÐ¾Ð´Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¸ÑÐ¼Ð° ÐÐµ-Ð°ÑÐ¸-Ð±Ð°ÑÐ°Ð¹ Ð² Ð´Ð·ÑÐ´Ð¾: Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð¸ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ
title: The modification of De-ashi-harai as a technical action in judo: models and the technology of learning
Creators: name: ÐÐ¸ÑÐ°Ð¹Ð»Ð¾Ð²Ð°, ÐÐ°ÑÑÑ
name: "Ð¡Ð¿Ð¾ÑÑ, ÑÐµÐ»Ð¾Ð²ÐµÐº, Ð·Ð´Ð¾ÑÐ¾Ð²ÑÐµ", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¹ Ð½Ð°ÑÑÐ½ÑÐ¹ ÐºÐ¾Ð½Ð³ÑÐµÑÑ
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2023
Subjects: ÐÐµ-Ð°ÑÐ¸-Ð±Ð°ÑÐ°Ð¹
Ð´Ð·ÑÐ´Ð¾
Ð¼ÐµÑÐ¾Ð´ Â«ÐºÑÐºÐ¾Ð»Â»
Ð¼Ð¾Ð´ÐµÐ»Ñ
Ð¼Ð¾Ð´Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ
ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ
De-ashi-harai
judo
the âmethod of dollsâ
model
modification
technology of learning

description: Ð ÑÑÐ°ÑÑÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ ÑÐ¸ÑÑÐµÐ¼Ð½Ð¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¼Ð¾Ð´Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¹ ÑÐ»Ð¾Ð¶Ð½Ð¾Ð³Ð¾ Ð² ÐºÐ¾Ð¾ÑÐ´Ð¸Ð½Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¼ Ð¸ ÑÐ¸Ð»Ð¾Ð²Ð¾Ð¼ Ð¸ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ð¸ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¸ÑÐ¼Ð° ÑÑÐµÐ½Ð¸ÑÐµÑÐºÐ¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÑÐµÐ¿ÐµÐ½Ð¸ 5 ÐÑ â ÐÐµ-Ð°ÑÐ¸-Ð±Ð°ÑÐ°Ð¹ â Ð² Ð´Ð·ÑÐ´Ð¾. ÐÑÐ¾Ð´ÐµÐ¼Ð¾Ð½ÑÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¼Ð¾Ð´ÐµÐ»Ð¸ ÐÐµ-Ð°ÑÐ¸-Ð±Ð°ÑÐ°Ð¹, Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑÑÐ¸Ðµ ÐµÐ³Ð¾ Ð¿ÑÐ¸Ð¼ÐµÐ½ÑÑÑ Ð´Ð»Ñ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð·Ð°Ð´Ð°Ñ Ð¿Ð¾ÐµÐ´Ð¸Ð½ÐºÐ¾Ð² Ð² Ð´Ð·ÑÐ´Ð¾ Ð¿ÑÐ¸ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ð¸ Ð¿ÑÐ¾ÑÐ¸Ð²Ð½Ð¸ÐºÐ° Ð² ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÑ. ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð° ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ ÐÐµ-Ð°ÑÐ¸-Ð±Ð°ÑÐ°Ð¹ Ð´Ð»Ñ Ð´Ð·ÑÐ´Ð¾Ð¸ÑÑÐ¾Ð², ÑÑÐµÐ½Ð¸ÑÑÑÑÐ¸ÑÑÑ Ð² ÑÐ¼ÐµÑÐ°Ð½Ð½ÑÑ Ð³ÑÑÐ¿Ð¿Ð°Ñ, Ñ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸ÐµÐ¼ Ð°Ð²ÑÐ¾ÑÑÐºÐ¾Ð³Ð¾ Ð¼ÐµÑÐ¾Ð´Ð° Â«ÐºÑÐºÐ¾Ð»Â».
description: The article presents the results of a system analysis in the field of De-ashi-haraiâs modifications. On one hand, De-ashiharai is difficult in terms of coordination and power performance, and, on the other hand, it is one of technical actions for attestation on 5 Kyu â qualificationâs degree of an apprentice. The models of De-ashi-harai are demonstrated, which allow using them to solve tactical tasks of wrestling in judo, when the opponent moves in different directions. The technology of De-ashi-haraiâs learning using the authorâs âmethod of dollsâ for judokas, which train in mixed groups, has been determined.
Fortuitous diagnosis of a cardiac interatrial mass in a patient presenting with Diffuse Large B-cell Lymphoma (DLBCL): MRI and 18F-FDG PET/CT findings.
Creators: name: MAYER, Julie
Publisher: name: EURORAD
Year: 2015
Subjects: subject: Cardiac
subject: Thorax
subject: MR
subject: PET-CT
subject: Diagnostic procedure
subject: Lymphoma

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: male, 55 years
description: Clinical History: A 55-year-old man was recently diagnosed with a DLBCL on pathological examination of a cervical lymph node surgical biopsy. The patient had no cardiac symptom and no ECG abnormality.  Baseline contrast-enhanced CT and 18F-FDG PET/CT demonstrated an inter-... Final Diagnosis: Cardiac involvement of a DLBCL revealed on initial 18F-FDG PET/CT.
La luna scomparsa di Nettuno
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2013

Solo il Voyager 2 le aveva dato una fugace occhiata nel suo passaggio attorno a Nettuno nel 1989. Ora Naiade, la luna più prossima al pianeta, è stata scovata in immagini d’archivio del telescopio spaziale Hubble, grazie a nuove tecniche che hanno anche permesso di osservare meglio i peculiari anelli.
title: ÐÐ¾Ð²ÑÑÐµÐ½Ð¸Ðµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐµÐ¿Ð»Ð¾Ð¿Ð¾ÑÑÐµÐ±Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÐ¸ ÑÐµÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ ÑÐµÐ¿Ð»Ð¾Ð²ÑÑ Ð²Ð²Ð¾Ð´Ð¾Ð² Ð¶Ð¸Ð»ÑÑ Ð¸ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½ÑÑ Ð·Ð´Ð°Ð½Ð¸Ð¹
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÑÑÑÐ»Ð»Ð¸Ð½Ð°, ÐÑ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: ÐÐ¾Ð·Ð¾Ð±Ð½Ð¾Ð²Ð»ÑÐµÐ¼ÑÐµ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¸ ÑÐ½ÐµÑÐ³Ð¸Ð¸
Ð­Ð½ÐµÑÐ³Ð¸Ñ
ÐÐ°ÑÐ¾ÑÑ ÑÐµÐ¿Ð»Ð¾Ð²ÑÐµ
Ð¢ÐµÐ¿Ð»Ð¾Ð²ÑÐµ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸
ÐÐ¾Ð´Ð¾ÑÐ½Ð°Ð±Ð¶ÐµÐ½Ð¸Ðµ Ð³Ð¾ÑÑÑÐµÐµ

description: Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° ÑÐ¸ÑÑÐµÐ¼Ð° Ð³Ð¾ÑÑÑÐµÐ³Ð¾ Ð²Ð¾Ð´Ð¾ÑÐ½Ð°Ð±Ð¶ÐµÐ½Ð¸Ñ (ÐÐÐ¡) Ñ ÑÐµÐ¿Ð»Ð¾Ð½Ð°ÑÐ¾ÑÐ½Ð¾Ð¹ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¾Ð¹ (Ð¢ÐÐ£) Ð² Ð¸Ð½Ð´Ð¸Ð²Ð¸Ð´ÑÐ°Ð»ÑÐ½Ð¾Ð¼ ÑÐµÐ¿Ð»Ð¾Ð²Ð¾Ð¼ Ð¿ÑÐ½ÐºÑÐµ (ÐÐ¢Ð) Ð°Ð´Ð¼Ð¸Ð½Ð¸ÑÑÑÐ°ÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð·Ð´Ð°Ð½Ð¸Ñ Ð² Ð³Ð¾ÑÐ¾Ð´Ðµ ÐÐ°ÑÑÑÐ½-ÐÐ°Ñ (ÐÐµÐ½ÐµÑÐºÐ¸Ð¹ Ð°Ð²ÑÐ¾Ð½Ð¾Ð¼Ð½ÑÐ¹ Ð¾ÐºÑÑÐ³). ÐÐ·ÑÑÐµÐ½Ñ Ð²Ð¾Ð·Ð¾Ð±Ð½Ð¾Ð²Ð»ÑÐµÐ¼ÑÐµ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¸ ÑÐ½ÐµÑÐ³Ð¸Ð¸ Ð¸ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½ Ð¸Ñ Ð¾Ð¿ÑÑ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð² ÑÐ¸ÑÑÐµÐ¼Ð°Ñ Ð¾ÑÐ¾Ð¿Ð»ÐµÐ½Ð¸Ñ, Ð³Ð¾ÑÑÑÐµÐ³Ð¾ Ð²Ð¾Ð´Ð¾ÑÐ½Ð°Ð±Ð¶ÐµÐ½Ð¸Ñ, Ð²ÐµÐ½ÑÐ¸Ð»ÑÑÐ¸Ð¸ Ð¸ ÐºÐ¾Ð½Ð´Ð¸ÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð²Ð¾Ð·Ð´ÑÑÐ°. ÐÐ¾ÑÑÑÐ¾ÐµÐ½Ð° ÑÐ°ÑÑÐµÑÐ½Ð°Ñ ÑÑÐµÐ¼Ð° ÐÐ¢Ð Ñ Ð¢ÐÐ£ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð²ÑÐ±ÑÐ°Ð½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐµÐºÑÐ° Ð´Ð»Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ. ÐÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð¼ Ð½Ð¸Ð·ÐºÐ¾Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÐµÐ¿Ð»Ð¾ÑÑ ÑÑÐ°Ð» ÑÐ´Ð°Ð»ÑÐµÐ¼ÑÐ¹ Ð²Ð¾Ð·Ð´ÑÑ Ð¸Ð· Ð¿Ð¾Ð¼ÐµÑÐµÐ½Ð¸Ð¹ Ð¸ Ð³ÑÑÐ½Ñ. ÐÑÐ±ÑÐ°Ð½ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½ÑÐ¹ ÑÐ¸Ð¿ ÑÐ°Ð±Ð¾ÑÐµÐ³Ð¾ Ð°Ð³ÐµÐ½ÑÐ°, Ð¸ÑÑÐ¾Ð´Ñ Ð¸Ð· ÑÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð´ÑÑÐ³Ð¸Ñ ÑÑÐµÐ¾Ð½Ð¾Ð² Ð²ÑÑÐ¾ÐºÐ¾Ð¹ ÐºÐ¾Ð½Ð´ÐµÐ½ÑÐ°ÑÐ¸Ð¸. ÐÑÐµÐ½ÐµÐ½Ð° ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¸ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð¢ÐÐ£ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐ°ÑÑÐµÑÐ° ÑÐµÐ¿Ð»Ð¾Ð²ÑÑ Ð½Ð°ÑÐ¾ÑÐ¾Ð² Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ ÐÐÐ¡.
AGN population in the deepest hard X-ray extragalactic survey
Creators: name: Paltani, S.
name: Courvoisier, T. J. -L.
name: Dwelly, T.
name: McHardy, I. M.
name: Walter, R.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the results of the analysis of the AGN population in the deepest extragalactic hard X-ray survey. The survey is based on INTEGRAL observation of the 3C 273/Coma cluster region, and covers 2500 deg2 with a 20-60 keV flux limit 1.5 times lower than other surveys at similar energies, resolving about 2.5% of the cosmic hard X-ray background. Using this survey, we can constrain in an unbiased way the distribution of hydrogen column absorption up to Nh=10^25 cm-2. We put an upper limit of 24% to the fraction of Compton-thick objects. Compared to models of the AGN population selected in the 2-10 keV band, the Log N-Log S diagram is generally in good agreement, but the Nh distribution is significantly different, with significantly less unabsorbed sources (Nh<10^22 cm-2) at a given flux limit compared to the models. We also study the local hard X-ray luminosity function (LF), which is compatible with what is found in other recent hard X-ray surveys. The extrapolation of the 2-10 keV LF is lower than the hard X-ray LF. The discrepancy is resolved if AGN spectra typically present reflection humps with reflection fraction R~1. Finally, we use the population properties of this survey to show that a future ultra-deep INTEGRAL extragalactic survey can result in a quite large AGN sample with enough objects at redshifts larger than z=0.05 so that we can detect evolution in the hard X-ray LF.
description: 12 pages, Proc. 7th INTEGRAL Workshop, Copenhagen, 8-11 September 2008
Some Devonian brachiopods reported from western Canada
Creators: name: Fortescue, John Adrian Claude
Publisher: name: University of British Columbia
Year: 2012

description: The aim of this study was to compile a list of descriptions of genera and species of brachiopod fossils which have been reported by various authors from the Devonian rocks of Canada, West of the 110th meridian. This thesis is divided into two parts. The first part is essentially bibliographical. The second part contains descriptions of genera and species of brachiopods. The bibliography in Part I contains forty references from which brachiopod faunal lists were compiled. Part I also contains an index map showing the geographical location of outcrop areas from which the fossils were collected, and a chart showing the stratigraphic range of brachiopod genera in a typical Devonian section of the Southern Rocky Mountains. In Part II, the brachiopod faunal lists have been arranged in a systematic manner. They are supplemented by detailed descriptions of fifty-one genera and ninety-eight species. The descriptions are prefaced by a short discussion of biological classification; a note on the modern concept of species; a glossary of brachiopod terminology, and a short list of important references on this group of fossils. All the descriptions are taken from the literature on the subject because none of the type material is presently at the University of British Columbia. The brachiopod descriptions are arranged by superfamilies. Conclusions are drawn regarding the scope and limitations of this study. Some suggestions are offered for the further study of this group of fossils.
title: Real Estate Markets and Lending : Does Local Growth Fuel Risk?
Creators: name: Zurek, Maximilian
Publisher: name: University of Bayreuth
Year: 2021
Subjects: subject: Lending risk
subject: Regional banks
subject: Collateral
subject: Real estate markets
subject: 330

description: Real estate price growth affects credit risk for several reasons: it provides input for economic forecasts as it’s closely tied to economic growth; when used as collateral by banks, rising real estate prices may decrease both expected and actual losses; and banks may become less risk averse in lending practices in the presence of rising property prices. Therefore, we analyze these effects on loan portfolios’ estimated and realized risks on a local level. Using data of 390 German savings banks, however, we find that real estate prices have little or no impact on savings banks’ credit portfolio risk or risk precautions.
Quando la costanza viene meno
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2013

Una delle caratteristiche finora attribuite all'emissione di raggi gamma di una stella di neutroni era la sua costanza. Ma uno studio pubblicato sulla rivista Astrophysical Journal Letters sembra mettere in forse il paradigma della stabilità delle pulsar nei raggi gamma.
Optimal-order bounds on the rate of convergence to normality in the multivariate delta method
Creators: name: Pinelis, Iosif
name: Molzon, Raymond
Publisher: name: arXiv
Year: 2009
Subjects: subject: Statistics Theory (math.ST)
subject: Probability (math.PR)
subject: Methodology (stat.ME)
subject: FOS: Mathematics
subject: FOS: Computer and information sciences
subject: 60F05, 60E15, 62F12 (Primary), 60E10, 62G10, 62G20, 62F03, 62F05 (Secondary)

description: Uniform and nonuniform Berry--Esseen (BE) bounds of optimal orders on the closeness to normality for general abstract nonlinear statistics are given, which are then used to obtain optimal bounds on the rate of convergence in the delta method for vector statistics. Specific applications to Pearson's, non-central Student's and Hotelling's statistics, sphericity test statistics, a regularized canonical correlation, and maximum likelihood estimators (MLEs) are given; all these uniform and nonuniform BE bounds appear to be the first known results of these kinds, except for uniform BE bounds for MLEs. When applied to the well-studied case of the central Student statistic, our general results compare well with known ones in that case, obtained previously by specialized methods. The proofs use a Stein-type method developed by Chen and Shao, a Cramér-type of tilt transform, exponential and Rosenthal-type inequalities for sums of random vectors established by Pinelis, Sakhanenko, and Utev, as well as a number of other, quite recent results motivated by this study. The method allows one to obtain bounds with explicit and rather moderate-size constants, at least as far as the uniform bounds are concerned. For instance, one has the uniform BE bound $3.61\mathbb{E}(Y_1^6+Z_1^6)\,(1+σ^{-3})/\sqrt n$ for the Pearson sample correlation coefficient based on independent identically distributed random pairs $(Y_1,Z_1),\dots,(Y_n,Z_n)$ with $\mathbb{E} Y_1=\mathbb{E} Z_1=\mathbb{E} Y_1Z_1=0$ and $\mathbb{E} Y_1^2=\mathbb{E} Z_1^2=1$, where $σ:=\sqrt{\mathbb{E} Y_1^2Z_1^2}$.
description: Version 5: Besides previously given applications to Pearson's, non-central Student's and Hotelling's statistics, added now are applications to sphericity test statistics, a regularized canonical correlation, and maximum likelihood estimators. The title and abstract have changed
IEA Wind TCP: Global Collaboration in Wind Energy Technology
Creators: name: Barth, Stephan
Publisher: name: Zenodo
Year: 2021
Subjects: wind
wind power
wind turbines
floating wind
offshore wind

description: This presentation was part of the EERA JP Wind & SETWind Annual Event 2021, in collaboration with ETIPWind (September 20 - 24, Amsterdam & online).
title: ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½ÑÑ Ð¿Ð¾Ð¼ÐµÑÐµÐ½Ð¸Ð¹ Ð´Ð»Ñ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¾ÐµÐºÑÐ½ÑÑ ÑÐµÑÐµÐ½Ð¸Ð¹
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Ð¾Ð³Ð´Ð°Ð½Ð¾Ð², Ð¨Ð°Ð¼Ð¸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: 2018
Subjects: Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ Ð¼Ð¾Ð´ÐµÐ»Ñ
Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ Ð¿Ð¾Ð¼ÐµÑÐµÐ½Ð¸Ðµ
Ð½Ð°Ð·ÐµÐ¼Ð½Ð¾Ðµ Ð»Ð°Ð·ÐµÑÐ½Ð¾Ðµ ÑÐºÐ°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð¾Ð±Ð»Ð°ÐºÐ¾ ÑÐ¾ÑÐµÐº
Ð°Ð½Ð°Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¼Ð¾Ð´ÐµÐ»Ñ
Ð½Ð°Ð³ÑÑÐ·ÐºÐ¸
Ð´ÐµÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¸Ð·ÑÑÐµÐ½Ð¾ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ñ Ð¾Ð±ÑÐµÐºÑÐ¾Ð². ÐÐ¿Ð¸ÑÐ°Ð½ Ð¿ÑÐ¾ÑÐµÑÑ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð¼ÐµÑÐµÐ½Ð¸Ñ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð½Ð°Ð·ÐµÐ¼Ð½Ð¾Ð³Ð¾ Ð»Ð°Ð·ÐµÑÐ½Ð¾Ð³Ð¾ ÑÐºÐ°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ ÑÐ°ÑÑÐµÑ Ð°Ð½Ð°Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð½ÐµÑÑÑÐ¸Ñ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹.
L'orchestra del Teatro alla Scala nella prima met� dell'800. Organizzazione, funzioni, gerarchie.
Creators: name: STEFANI, DAVIDE
Publisher: name: Universit� degli Studi di Milano
Year: 2015

description: Nel corso del XIX secolo l?orchestra di teatro si afferma come realt� stabile, sociale e finanziaria, un organismo cio� che si identifica sempre pi� con la citt� e con il teatro in cui opera, trasformandosi in una istituzione professionale, regolata da contratti e statuti. A Milano tutto questo si verifica in una fase storica delicata che vede in particolare tra il 1796 e il 1815 un mutamento di strutture amministrative, economiche e sociali senza precedenti. Sul piano culturale il teatro � il principale catalizzatore di attenzioni da parte delle autorit� governative che ? se inizialmente lo considerano un efficace veicolo di consenso e di diffusione di ideali, centro della vita culturale cittadina e luogo di aggregazione e di svago ? trasformer� la loro azione in un crescente impegno di moralizzazione e di controllo poliziesco su ogni singolo aspetto dell?organizzazione teatrale. Scopo di questa tesi � analizzare come le diverse vicende politiche che hanno attraversato la Milano di quegli anni abbiano influito sull?amministrazione e la gestione quotidiana del Teatro alla Scala, e in particolare della sua orchestra.
title: Ð¤Ð¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¾Ð·Ð´Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÐÐÐÐ ÐÐ Ð£Ð®Ð©ÐÐ¯ ÐÐÐÐÐÐÐÐ¯ Â«ÐÐÐ£Ð¥ÐÐÐÐ­ÐÐÐ ÐÐÂ»)
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·Ð³ÐµÐ¹Ð¼, ÐÑÐµÐ½Ð¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð±Ð°Ð½ÐºÑÐ¾ÑÑÑÐ²Ð¾
Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¾Ð·Ð´Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ
ÑÑÐ°Ð¿Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¾Ð·Ð´Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ
Ð¾ÑÐµÐ½ÐºÐ° Ð²ÐµÑÐ¾ÑÑÐ½Ð¾ÑÑÐ¸ Ð±Ð°Ð½ÐºÑÐ¾ÑÑÑÐ²Ð°

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ½ÐµÑÐ³Ð¾ÑÐ½Ð°Ð±Ð¶Ð°ÑÑÐ°Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ ÐÐÐ Â«ÐÐÐÂ». Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¾ÑÐµÐ½ÐºÐ° Ð²ÐµÑÐ¾ÑÑÐ½Ð¾ÑÑÐ¸ Ð±Ð°Ð½ÐºÑÐ¾ÑÑÑÐ²Ð° ÐÐÐ Â«ÐÐÐÂ» Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¾Ð·Ð´Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ.
ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÑÐ½ÐºÐ° ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ¸ Ð³.Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ð° Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ½ÑÐµ Ð¿ÑÐµÐ¸Ð¼ÑÑÐµÑÑÐ²Ð° ÐÐÐ Â«ÐÐÐÂ». Ð¡ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð¼Ð¾Ð´ÐµÐ»ÐµÐ¹ Ð­. ÐÐ»ÑÑÐ¼Ð°Ð½Ð° (Ð´Ð²ÑÑÑÐ°ÐºÑÐ¾ÑÐ½Ð°Ñ, Ð¿ÑÑÐ¸ÑÐ°ÐºÑÐ¾ÑÐ½Ð°Ñ), Ð£. ÐÐ¸Ð²ÐµÑÐ°, R-ÑÑÐµÑÐ°, ÑÐµÐ¹ÑÐ¸Ð½Ð³Ð¾Ð²Ð¾Ð¹ (Ð . Ð¡. Ð¡Ð°Ð¹ÑÑÐ»Ð¸Ð½Ð°, Ð. Ð.ÐÐ°Ð´ÑÐºÐ¾Ð²Ð°), Ð±Ð°Ð»Ð»ÑÐ½Ð¾Ð¹ (Ð. Ð. ÐÐ¾Ð½ÑÐ¾Ð²Ð¾Ð¹, Ð. Ð. ÐÐ¸ÐºÐ¸ÑÐ¾ÑÐ¾Ð²Ð¾Ð¹) Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° Ð´Ð¸Ð°Ð³Ð½Ð¾ÑÑÐ¸ÐºÐ° Ð²ÐµÑÐ¾ÑÑÐ½Ð¾ÑÑÐ¸ ÑÐ³ÑÐ¾Ð·Ñ Ð±Ð°Ð½ÐºÑÐ¾ÑÑÑÐ²Ð°, Ð² ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ ÐºÐ¾ÑÐ¾ÑÐ¾Ð¹ Ð±ÑÐ»Ð¸ Ð²ÑÑÐ²Ð»ÐµÐ½Ñ ÐºÐ»ÑÑÐµÐ²ÑÐµ Ð¿ÑÐ¸Ð·Ð½Ð°ÐºÐ¸ Ð½Ð°Ð»Ð¸ÑÐ¸Ñ ÐºÑÐ¸Ð·Ð¸ÑÐ½Ð¾Ð¹ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¸, Ð² ÐºÐ¾ÑÐ¾ÑÐ¾Ð¹ Ð½Ð°ÑÐ¾Ð´Ð¸ÑÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ðµ. ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¸ ÑÑÑÐ°ÑÐµÐ³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð·Ð°Ð´Ð°ÑÐ¸, ÑÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÑÐ°Ð¿Ñ, Ð²ÑÐ¾Ð´ÑÑÐ¸Ðµ Ð² Ð¿ÑÐ¾ÑÐµÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¾Ð·Ð´Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ. Ð ÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÑ Ð·Ð°Ð´Ð°Ñ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÑ Ðº ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ñ Ð´Ð¾Ð»Ð¸ ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÐºÐ°Ð¿Ð¸ÑÐ°Ð»Ð° Ð² Ð¾Ð±ÑÐµÐ¹ ÑÑÑÑÐºÑÑÑÐµ Ð±Ð°Ð»Ð°Ð½ÑÐ°, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ¾ÑÑÑ ÑÐ¸ÑÑÐ¾Ð¹ Ð¿ÑÐ¸Ð±ÑÐ»Ð¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ.
Getting into Shape: Efficient Cooling Scheme for Fermionic Atoms in Optical Lattices
Creators: name: Bernier, Jean-Sebastien
name: Kollath, Corinna
name: Georges, Antoine
name: De Leo, Lorenzo
name: Gerbier, Fabrice
name: Salomon, Christophe
name: Köhl, Michael
Publisher: name: arXiv
Year: 2009
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We propose an experimental procedure to cool fermionic atoms loaded into an optical lattice. The central idea is to spatially divide the system into entropy-rich and -poor regions by shaping the confining potential profile. Atoms in regions of high entropy per particle are subsequently isolated from the system. We discuss how to experimentally carry out this proposal, and perform a quantitative study of its efficiency. We find that the entropy per particle, $s$, can typically be reduced by a factor of 10 such that entropies lower than $s/k_B \sim 0.2$ can be reached. Cooling into highly sought-after quantum phases (such as an antiferromagnet) can thus be achieved. We show that this procedure is robust against variations of the experimental conditions.
description: 4+ pages, 3 figures, version published in PRA(R)
On the Viterbi process with continuous state space
Creators: name: Chigansky, Pavel
name: Ritov, Yaacov
Publisher: name: arXiv
Year: 2009
Subjects: subject: Statistics Theory (math.ST)
subject: Probability (math.PR)
subject: FOS: Mathematics

description: This paper deals with convergence of the maximum a posterior probability path estimator in hidden Markov models. We show that when the state space of the hidden process is continuous, the optimal path may stabilize in a way which is essentially different from the previously considered finite-state setting.
description: Published in at http://dx.doi.org/10.3150/10-BEJ294 the Bernoulli (http://isi.cbs.nl/bernoulli/) by the International Statistical Institute/Bernoulli Society (http://isi.cbs.nl/BS/bshome.htm)
Una caraffa stellare a 1200 anni luce
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2013

Situata nella costellazione australe della Carena, la nebulosa della caraffa Toby Jug è un esempio di una nebulosa a riflessione. È  illuminata dall'interno da una stella chiamata HD 65750, una stella gigante rossa che ha cinque volte la massa del Sole. Questa immagine è stata prodotta come parte del programma dell'ESO "Gemme Cosmiche".
title: ÐÐ¸Ð»Ð¾Ð¹ Ð´Ð¾Ð¼ Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¾Ð¹ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð²Ð¾Ð·Ð²ÐµÐ´ÐµÐ½Ð¸Ñ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹ ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ¸ÑÑÐµÐ¼Ð¾Ð¹ Ð·ÐµÐ»ÐµÐ½Ð¾Ð¹ ÐºÑÐ¾Ð²Ð»Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÑÑÐµÐ½ÐºÐ¾, ÐÐ»Ð°Ð²Ð´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: Ð¢ÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð²Ð¾Ð·Ð²ÐµÐ´ÐµÐ½Ð¸Ñ
Ð·ÐµÐ»ÐµÐ½Ð°Ñ ÐºÑÐ¾Ð²Ð»Ñ
ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ¸ÑÑÐµÐ¼Ð°Ñ Ð·ÐµÐ»ÐµÐ½Ð°Ñ ÐºÑÐ¾Ð²Ð»Ñ

description: Ð Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð±ÑÐ»Ð¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ Autodesk Revit 2016, Autodesk AutoCAD 2016, SCAD Office 21.1, Microsoft Office, A0. Ð ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ð¸ Ñ ÐÐ¾ÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ð¸ÐµÐ¼ ÐÑÐ°Ð²Ð¸ÑÐµÐ»ÑÑÑÐ²Ð° Ð Ð¤ Ð¾Ñ 16.02.2008 N 87 (ÑÐµÐ´. Ð¾Ñ 28.04.2017) "Ð ÑÐ¾ÑÑÐ°Ð²Ðµ ÑÐ°Ð·Ð´ÐµÐ»Ð¾Ð² Ð¿ÑÐ¾ÐµÐºÑÐ½Ð¾Ð¹ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ°ÑÐ¸Ð¸ Ð¸ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸ÑÑ Ðº Ð¸Ñ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ñ" Ð±ÑÐ»Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð²ÑÐµ Ð¿ÑÐµÐ´ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð½ÑÐµ Ð·Ð°Ð´Ð°Ð½Ð¸ÐµÐ¼ ÑÐ°Ð·Ð´ÐµÐ»Ñ. ÐÑÐ»Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð²Ð¾Ð·Ð²ÐµÐ´ÐµÐ½Ð¸Ñ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹ ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ¸ÑÑÐµÐ¼Ð¾Ð¹ Ð·ÐµÐ»ÐµÐ½Ð¾Ð¹ ÐºÑÐ¾Ð²Ð»Ð¸.
Government Control of Cotton Production in the United States, 1933- 1935: A Selected List of References
Creators: name: Day, Emily L.
name: Day, Emily L.
Publisher: name: Unknown
Year: 1936
Subjects: subject: Agricultural and Food Policy
subject: Crop Production/Industries
subject: Demand and Price Analysis
subject: International Relations/Trade
subject: Marketing
subject: FOS: Economics and business
subject: Production Economics

description: Excerpts from the Foreword: Plans for the control of cotton production, including the enactment and administration of Federal legislation, have been the subject of many publications in recent years. References for this bibliography were selected from the period 1933-1935. For reference to earlier publications the bibliography on "Agricultural Relief" (number 50 in this series) should be consulted. Some references to the effect of production-control legislation on the tenant farmer are included but a more comprehensive bibliography on this phase of the subject has recently appeared as Agricultural Economics Bibliography No. 59, Farm Tenancy in the United States, 1925-1935. The bibliography is arranged alphabetically by author or by title if there is no author. An index of authors and subjects is appended.
АРХИТЕКТУРА ОСОБОГО ТИПА
Creators: name: Алексей Щербинин
Publisher: name: Университетский город: архитектура смыслов
Year: 2021

description: Университетский город – словосочетание, до сих пор не имеющее официального узаконения. Этот пробел позволяет использовать данное понятие как для городов, где возникли первые в мире университеты, так и для муниципальных образований, где наличествует хоть какой-то университет.
STM imaging of a bound state along a step on the surface of the topological insulator Bi$_2$Te$_3$
Creators: name: Alpichshev, Zhanybek
name: Analytis, J. G.
name: Chu, J. -H.
name: Fisher, I. R.
name: Kapitulnik, A.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Detailed study of the LDOS associated with the surface-state-band near a step-edge of the strong topological-insulator Bi2Te3, reveal a one-dimensional bound state that runs parallel to the stepedge and is bound to it at some characteristic distance. This bound state is clearly observed in the bulk gap region, while it becomes entangled with the oscillations of the warped surface band at high energy, and with the valence band states near the Dirac point. Using the full effective Hamiltonian proposed by Zhang et al., we obtain a closed formula for this bound state that fits the data and provide further insight into the general topological properties of the electronic structure of the surface band near strong structural defects.
description: 5 pages, 4 figures
title: ÐÐ¾Ð²ÑÑÐµÐ½Ð¸Ðµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð½ÐµÑÑÐµÐ´Ð¾Ð±ÑÐ²Ð°ÑÑÐµÐ¹ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð·Ð° ÑÑÐµÑ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð² Ð´Ð¾Ð±ÑÑÐ¸ Ð½ÐµÑÑÐ¸
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: ÐÑ Ð§Ð¶Ð°Ð¾Ð´Ñ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¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¸
ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ
ÑÐµÑ Ð½Ð¸ÐºÐ¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸
ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ Ð¾ÑÐµÐ½ÐºÐ°

description: ÐÐ°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ Ð¿Ð¾ ÑÐµÐ¼Ðµ Â«ÐÐ¾Ð²ÑÑÐµÐ½Ð¸Ðµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Â«ÐÑÐºÐ¾Ð¹Ð»Â»Â», Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð° Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð´Ð°Ð½Ð½ÑÑ Ð¸ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð², Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÑ Ð²Ð¾ Ð²ÑÐµÐ¼Ñ Ð¿ÑÐ¾ÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð¸ Ð¿ÑÐµÐ´Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð¹ Ð¿ÑÐ°ÐºÑÐ¸Ðº.
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Attenzione, arriva Juno
Creators: Livia Giacomini
Publisher: name: Media Inaf
Year: 2013

Attorno alle 21 ora italiana di mercoledì la sonda destinata a Giove sorvola la Terra, arrivando ad appena 500 km di distanza. ASI e INAF invitano astrofili e appassionati a tentare di osservarla, riprenderla e inviare le proprie immagini, che saranno poi pubblicate anche dalla NASA.
Silvia e le sue lune
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2013

Un gruppo di ricerca del SETI Institute ha ottenuto nuove informazioni sull’asteroide 87 Silvia e le sue due lune, grazie anche all’aiuto di astrofili che hanno osservato la tripletta durante l’occultazione di una lontana stella.
A weak notion of strict pseudo-convexity. Applications and examples
Creators: name: Amar, Eric
Publisher: name: arXiv
Year: 2009
Subjects: subject: Complex Variables (math.CV)
subject: Functional Analysis (math.FA)
subject: FOS: Mathematics
subject: 32A35, 42B30

description: Let $Ω$ be a bounded ${\mathcal{C}}^{\infty}$-smoothly bounded domain in ${\mathbb{C}}^{n}.$ For such a domain we define a new notion between strict pseudo-convexity and pseudo-convexity: the size of the set $W$ of weakly pseudo-convex points on $\partial Ω$ is small with respect to Minkowski dimension: near each point in the boundary $\partial Ω,$ there is at least one complex tangent direction in which the slices of $W$ has a upper Minkowski dimension strictly smaller than $2.$ We propose to call this notion "strong pseudo-convexity"; this word is free since "strict pseudo-convexity" gets the precedence in the case where all the points in $\partial Ω$ are stricly pseudo-convex. For such domains we prove that if $S$ is a separated sequence of points contained in the support of a divisor in the Blaschke class, then a canonical measure associated to $S$ is bounded. If moreover the domain is $p$-regular, and the sequence $S$ is dual bounded in the Hardy space $H^{p}(Ω),$ then the previous measure is Carleson. As an application we prove a theorem on interpolating sequences in bounded convex domains of finte type in ${\mathbb{C}}^{n}.$ Examples of such pseudo-convex domains are finite type domains in ${\mathbb{C}}^{2},$ finite type convex domains in ${\mathbb{C}}^{n},$ finite type domains which have locally diagonalizable Levi form, domains with real analytic boundary and of course, stricly pseudo-convex domains in ${\mathbb{C}}^{n}.$ Domains like $|{z_{1}}| ^{2}+\exp \{1-|{z_{2}}| ^{-2}\}<1,$ which are not of finite type are nevertheless strongly pseudo-convex, in this sense.
description: This is completely rewritten and expanded thanks to incisive questions and a lot of deep suggestions done by the referee. This will appear in Annali della Scuola Normale Superiore di Pisa
L’atmosfera di Plutone è dura a morire
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2013

Un team di ricercatori ha esaminato i dati raccolti dal 1988 al 2003, effettuando dei calcoli precisi sulla pressione atmosferica. Quest'anno gli astronomi hanno mostrato che l'atmosfera è più spessa rispetto al passato e che quindi è difficile che scomparirà nei prossimi secoli. Nonostante la lontananza dal Sole i gas non ghiacciano quasi mai.
In due per un bosone
Creators: Nicola Nosengo
Publisher: name: Media Inaf
Year: 2013

Con un po' di suspence (più di un'ora di ritardo per l'annuncio), il Nobel per la fisica 2013 va a Peter Higgs e Francois Englert, per la teoria che portato alla scoperta della particella responsabile della massa. Nessun riconoscimento agli esperimenti, ma lo stesso grande soddisfazione tra i fisici italiani.
ДВА СЦЕНАРИЯ БУДУЩЕГО МОЛОДЕЖИ: КАК УНИВЕРСИТЕТ ФОРМИРУЕТ ПОЗИТИВНЫЕ ПЕРСПЕКТИВЫ
Creators: name: Галина Градосельская
Publisher: name: Университетский город: архитектура смыслов
Year: 2021

description: Сетевые процессы стали отражением объективных социальных установок, складывающихся на протяжении долгого периода. В то же время сетевые взаимодействия превратились в механизм, консолидирующий группы граждан по сходству социально-политических взглядов.
Li non-stoichiometry and crystal growth of untwinned 1D quantum spin system Lix Cu2 O2
Creators: name: Hsu, H. C.
name: Liu, H. L.
name: Chou, F. C.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Floating-zone growth of untwinned single crystal of Li_xCu_2O_2 with high Li content of x ~ 0.99 is reported. Li content of Li_xCu_2O_2 has been determined accurately through combined iodometric titration and thermogravimetric methods, which also ruled out the speculation of chemical disorder between Li and Cu ions. The morphology and physical properties of single crystals obtained from slowing-cooling (SL) and floating-zone (FZ) methods are compared. The floating-zone growth under Ar/O_2=7:1 gas mixture at 0.64 MPa produces large area of untwinned crystal with highest Li content, which has the lowest helimagnetic ordering temperature ~19K in the Li_xCu_2O_2 system.
description: 4 pages, 3 figures
Una bomba a grappolo nell’orbita marziana
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2013

Affrontare la minaccia d’un asteroide in rotta verso la Terra facendolo a pezzi è una strategia che presenta alcuni rischi. L’esito potrebbe essere quello osservabile nel punto L5 dell’orbita di Marte: cinque dei sei satelliti troiani (ovvero che condividono l'orbita del pianeta rosso) presenti sembrerebbero essere frutto d’una collisione.
On imprimitive rank 3 permutation groups
Creators: name: Devillers, Alice
name: Giudici, Michael
name: Li, Cai Heng
name: Pearce, Geoffrey
name: Praeger, Cheryl E.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Group Theory (math.GR)
subject: FOS: Mathematics
subject: 20B05

description: A classification is given of rank 3 group actions which are quasiprimitive but not primitive. There are two infinite families and a finite number of individual imprimitive examples. When combined with earlier work of Bannai, Kantor, Liebler, Liebeck and Saxl, this yields a classification of all quasiprimitive rank 3 permutation groups. Our classification is achieved by first classifying imprimitive almost simple permutation groups which induce a 2-transitive action on a block system and for which a block stabiliser acts 2-transitively on the block. We also determine those imprimitive rank 3 permutation groups $G$ such that the induced action on a block is almost simple and $G$ does not contain the full socle of the natural wreath product in which $G$ embeds.
description: updated after revisions
La strana risonanza di Mercurio
Creators: Nicola Nosengo
Publisher: name: Media Inaf
Year: 2013

Perché il rapporto tra periodo di rivoluzione e periodo di rotazione di Mercurio è di 3:2, così diverso da tutti gli altri osservati nel Sistema solare? Uno studio belga prova a spiegarlo, e dimostra che quel rapporto potrebbe saltare fuori anche in molti pianeti extrasolari.
La calda coperta di una baby stella
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2013

Le grandi dimensioni del nucleo caldo scoperto da ALMA dimostrano che una giovane stella nella costellazione dell'Aquila emette molta più energia rispetto a quelle studiate finora. Gli studiosi sperano di capire meglio il processo di formazione stellare grazie ai nuovi risultati. Lo studio pubblicato su Astrophysical Journal.
Measuring the Dark Force at the LHC
Creators: name: Bai, Yang
name: Han, Zhenyu
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: A long-range ``dark force'' has recently been proposed to mediate the dark matter (DM) annihilation. If DM particles are copiously produced at the Large Hadron Collider (LHC), the light dark force mediator will also be produced through radiation. We demonstrate how and how precise we can utilize this fact to measure the coupling constant of the dark force. The light mediator's mass is measured from the ``lepton jet'' it decays to. In addition, the mass of the DM particle is determined using the MT2 technique. Knowing these quantities is critical for calculating the DM relic density.
description: 4 pages, 4 figures; final version for PRL
ИСКУССТВО ФОРМИРОВАНИЯ СОЦИОКУЛЬТУРНОЙ ОБРАЗОВАТЕЛЬНОЙ СРЕДЫ
Creators: name: Дмитрий Смирнов
Publisher: name: Университетский город: архитектура смыслов
Year: 2021

description: Социальным институтам, к которым относится и высшая школа, необходимо приложить максимум усилий для создания социокультурной среды, способной вдохновлять, мотивировать человека, побуждать его к движению из мира обывательского прозябания в пространство творчества и активного досуга. Но социокультурная среда не появляется сама по себе, она кропотливо формируется конкретными людьми, профессионалами и учеными различных специальностей.
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ²Ð¾Ð¹ÑÑÐ² Ð¸Ð·Ð¾Ð»ÑÑÐ¸Ð¾Ð½Ð½ÑÑ Ð¶Ð¸Ð´ÐºÐ¾ÑÑÐµÐ¹ Ð¿Ð¾Ð´ Ð´ÐµÐ¹ÑÑÐ²Ð¸ÐµÐ¼ Ð¸ÑÐºÑÐ¾Ð²ÑÑ ÑÐ°Ð·ÑÑÐ´Ð¾Ð²
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ´ÐºÐ¾Ð², ÐÐ°ÐºÑÐ¸Ð¼
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: Ð¸Ð·Ð¾Ð»ÑÑÐ¸Ð¾Ð½Ð½Ð°Ñ Ð¶Ð¸Ð´ÐºÐ¾ÑÑÑ
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ÑÐ²ÐµÑÐ¾Ð¿ÑÐ¾Ð¿ÑÑÐºÐ°Ð½Ð¸Ðµ
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description: ÐÑÐ»Ð¸ Ð¸Ð·ÑÑÐµÐ½Ñ Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½ÑÐµ ÑÑÐ°ÑÑÐ¸ Ð¿Ð¾ ÑÑÐ°Ð½ÑÑÐ¾ÑÐ¼Ð°ÑÐ¾ÑÐ½Ð¾Ð¼Ñ Ð¼Ð°ÑÐ»Ñ, Ð¿Ð¾ Ð¿ÑÐ¾Ð±Ð¾Ñ Ð¶Ð¸Ð´ÐºÐ¸Ñ Ð´Ð¸ÑÐ»ÐµÐºÑÑÐ¸ÐºÐ¾Ð² Ð¸ Ð¸Ñ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÑ Ð² Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð¾ÑÑÐ°ÑÐ»Ð¸. ÐÐ·ÑÑÐµÐ½Ñ Ð¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ Ð´Ð°Ð½Ð½ÑÑ Ð¾Ð¿ÑÑÐ¾Ð² Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾Ð²ÐµÑÑÐ¸ ÑÑÐ¾Ð¶Ð¸Ðµ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÑ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ñ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÑ Ð¿Ð¾ ÑÐ¾ÑÑÐ°ÑÐ¸Ð²Ð°Ð½Ð¸Ñ Ð¼Ð°ÑÐ»Ð°, Ð¿ÑÑÐµÐ¼ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð½Ð° Ð½ÐµÐ³Ð¾ Ð¸ÑÐºÑÐ¾Ð²ÑÑ ÑÐ°Ð·ÑÑÐ´Ð¾Ð². ÐÐ»Ñ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¾Ð¿ÑÑÐ°, Ð±ÑÐ»Ð° ÑÐ»ÑÑÑÐµÐ½Ð° ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ°. Ð¡Ð½ÑÑÑ ÑÐ¿ÐµÐºÑÑÑ Ð¿ÑÐ¾Ð¿ÑÑÐºÐ°Ð½Ð¸Ñ, Ð¿ÑÐ¸ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÑÑÐ°Ð¿Ð°Ñ Ð¿ÑÐ¾Ð±Ð¾Ñ Ð¼Ð°ÑÐ»Ð°. ÐÐ°Ð½Ð½ÑÐµ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð² ÑÐ°Ð·Ð½ÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð°Ñ, ÑÐµÑÐµÐ· ÐºÐ¾ÑÐ¾ÑÑÐµ Ð±ÑÐ»Ð¸ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÐ¸. ÐÑÐ»Ð¸ ÑÐ½ÑÑÑ Ð·Ð½Ð°ÑÐµÐ½Ð¸Ñ ÑÐ¾Ð¿ÑÐ¾ÑÐ¸Ð²Ð»ÐµÐ½Ð¸Ñ, Ð¿ÑÐ¸ ÐºÐ°Ð¶Ð´Ð¾Ð¼ Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸Ð¸ ÑÑÐ°Ð½ÑÑÐ¾ÑÐ¼Ð°ÑÐ¾ÑÐ½Ð¾Ð³Ð¾ Ð¼Ð°ÑÐ»Ð° Ð¸ ÑÐ°Ðº Ð¶Ðµ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð° Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÑ ÐµÐ³Ð¾ Ð¾Ñ Ð²ÑÐµÐ¼ÐµÐ½Ð¸.