cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The XMM-Newton Serendipitous Survey. VI. The X-ray Luminosity Function
Creators: name: Ebrero, J.
name: Carrera, F. J.
name: Page, M. J.
name: Silverman, J. D.
name: Barcons, X.
name: Ceballos, M. T.
name: Corral, A.
name: Della Ceca, R.
name: Watson, M. G.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the X-ray luminosity function of AGN in three energy bands (Soft: 0.5-2 keV, Hard: 2-10 keV and Ultrahard: 4.5-7.5 keV). We have used the XMS survey along with other highly complete flux-limited deeper and shallower surveys for a total of 1009, 435 and 119 sources in the Soft, Hard and Ultrahard bands, respectively. We have modeled the intrinsic absorption of the Hard and Ultrahard sources (NH function) and computed the intrinsic X-ray luminosity function in all bands using a Maximum Likelihood fit technique to an analytical model. We find that the X-ray luminosity function (XLF) is best described by a Luminosity-Dependent Density Evolution (LDDE) model. Our results show a good overall agreement with previous results in the Hard band, although with slightly weaker evolution. Our model in the Soft band present slight discrepancies with other works in this band, the shape of our present day XLF being significantly flatter. We find faster evolution in the AGN detected in the Ultrahard band than those in the Hard band. The fraction of absorbed AGN in the Hard and Ultrahard bands is dependent on the X-ray luminosity. We find evidence of evolution of this fraction with redshift in the Hard band but not in the Ultrahard band, possibly due to the low statistics. Our best-fit XLF shows that the high-luminosity AGN are fully formed earlier than the less luminous AGN. The latter sources account for the vast majority of the accretion rate and mass density of the Universe, according to an anti-hierarchical black hole growth scenario.
description: 16 pages, 12 figures, accepted for publication in Astronomy and Astrophysics
title: ÐÐ¸Ð°Ð³Ð½Ð¾ÑÑÐ¸ÐºÐ° Ð±Ð°Ð½ÐºÑÐ¾ÑÑÑÐ²Ð° Ð¸ Ð¼ÐµÑ Ð°Ð½Ð¸Ð·Ð¼ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ ÑÑÐ°Ð±Ð¸Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¡Ð¼Ð¾ÑÑÐºÐ¾Ð²Ð°, Ð¢Ð°ÑÑÑÐ½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð´Ð¸Ð°Ð³Ð½Ð¾ÑÑÐ¸ÐºÐ° Ð±Ð°Ð½ÐºÑÐ¾ÑÑÑÐ²Ð°
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð°Ñ ÑÑÐ°Ð±Ð¸Ð»Ð¸Ð·Ð°ÑÐ¸Ñ
Ð±Ð°Ð½ÐºÑÐ¾ÑÑÑÐ²Ð¾
Ð»Ð¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐÐ Â«Ð­ÐºÑÐ¿Ð¾ÑÐ¾ÑÐµÑÑÂ». Ð¦ÐµÐ»Ñ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ - Ð¿ÑÐ¾Ð²ÐµÑÑÐ¸ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸ Ð¾ÑÐµÐ½ÐºÑ Ð²ÐµÑÐ¾ÑÑÐ½Ð¾ÑÑÐ¸ Ð±Ð°Ð½ÐºÑÐ¾ÑÑÑÐ²Ð° Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«Ð­ÐºÑÐ¿Ð¾ÑÐ¾ÑÐµÑÑÂ», Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ ÑÑÐ°Ð±Ð¸Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¸ Ð¾ÑÐµÐ½ÐºÐ¸ Ð²ÐµÑÐ¾ÑÑÐ½Ð¾ÑÑÐ¸ Ð±Ð°Ð½ÐºÑÐ¾ÑÑÑÐ²Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÐÐÐ Â«Ð­ÐºÑÐ¿Ð¾ÑÐ¾ÑÐµÑÑÂ» Ð±ÑÐ»Ð¾ Ð²ÑÑÐ²Ð»ÐµÐ½Ð¾, ÑÑÐ¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ðµ Ð¸Ð¼ÐµÐµÑ Ð½ÐµÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾Ðµ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ðµ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ.
Preheating the Universe from the Standard Model Higgs
Creators: name: Figueroa, Daniel G.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We discuss Preheating after an inflationary stage driven by the Standard Model (SM) Higgs field non-minimally coupled to gravity. We find that Preheating is driven by a complex process in which perturbative and non-perturbative effects occur simultaneously. The Higgs field, initially an oscillating coherent condensate, produces non-perturbatively W and Z gauge fields. These decay very rapidly into fermions, thus preventing gauge bosons to accumulate and, consequently, blocking the usual parametric resonance. The energy transferred into the fermionic species is, nevertheless, not enough to reheat the Universe, and resonant effects are eventually developed. Soon after resonance becomes effective, also backreaction from the gauge bosons into the Higgs condensate becomes relevant. We have determined the time evolution of the energy distribution among the remnant Higgs condensate and the non-thermal distribution of the SM fermions and gauge fields, until the moment in which backreaction becomes important. Beyond backreaction our approximations break down and numerical simulations and theoretical considerations beyond this work are required, in order to study the evolution of the system until thermalization.
description: 10 pages, 1 figure. Proceedings of the "Invisible Universe International Conference", Paris 2009
Surface Plasmon Polariton microscope with Parabolic Reflectors
Creators: name: Drezet, Aurelien
name: Koller, Daniel
name: Hohenau, Andreas
name: Leitner, Alfred
name: Aussenegg, Franz R.
name: Krenn, Joachim R.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We report the realization of a two--dimensional optical microscope for surface plasmons polaritons (SPPs) based on parabolic Bragg mirrors. These mirrors are built from lithographically fabricated gold nanostructures on gold thin films. We show by direct imaging by leakage radiation microscopy that the magnification power of the SPP microscope follows basic predictions of geometrical optics. Spatial resolution down to the value set by the diffraction limit is demonstrated.
description: Opt.Lett.32, 2414 (2007)
Buchi neri nella Via Lattea: se i “mostri” sono due
Creators: Rossella Spiga
Publisher: name: Media Inaf
Year: 2017

Un candidato buco nero di grandi dimensioni, circa 100mila masse solari, è stato individuato all'interno di una nube di gas a 200 anni luce dal centro della Via Lattea. La scoperta, ottenuta grazie al radiotelescopio giapponese di Nobeyama e ad Alma, è illustrata sull’ultimo numero di Nature Astronomy
Additional file 1 of The effect of ambient PM2.5 exposure on survival of lung cancer patients after lobectomy
Creators: name: Liu, Changpeng
name: Yang, Dongjian
name: Liu, Yuxi
name: Piao, Heng
name: Zhang, Tao
name: Li, Xi
name: Zhao, Erjiang
name: Zhang, Di
name: Zheng, Yan
name: Tang, Xiance
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Cell Biology
subject: Biotechnology
subject: Environmental Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1: Table S1. Distribution of air pollutant specific-monthly exposure after lung cancer surgery. Table S2. Distribution of air pollutant exposure after lung cancer surgery. Figure S1. Hazard ratios (HRs) of postoperative death among lung cancer patients in association with specific monthly exposure to PM2.5, after adjusting for air pollution before the operation. Model 1 was adjusted for age at operation, sex, occupation type, ethnicity, marital status, length of hospitalization, operation season, and PM2.5 exposure for 6 months before the operation. Model 2 was adjusted for age at operation, sex, occupation type, ethnicity, marital status, length of hospitalization, operation season, and O3 exposure for 6 months before the operation. Model 3 was adjusted for age at operation, sex, occupation type, ethnicity, marital status, length of hospitalization, operation season, O3 exposure for 6 months before the operation, and PM2.5 exposure for 6 months before the operation. Figure S2. Hazard ratios (HRs) of postoperative death among lung cancer patients in association with specific monthly exposure to PM2.5, after adjusting for chronic diseases. Model 1 was adjusted for age at operation, sex, occupation type, ethnicity, marital status, length of hospitalization, operation season, and cardiovascular disease. Model 2 was adjusted for age at operation, sex, occupation type, ethnicity, marital status, length of hospitalization, operation season, and hypertension. Model 3 was adjusted for age at operation, sex, occupation type, ethnicity, marital status, length of hospitalization, operation season, and diabetes. Figure S3. Hazard ratios (HRs) of postoperative death among lung cancer patients in association with specific monthly exposure to PM2.5, after adjusting for different age subgroups. Model 1 was adjusted for age at operation, sex, occupation type, ethnicity, marital status, and length of hospitalization. Model 2 was adjusted for the factors in Model 1 and operation season. Model 3 was adjusted for the factors in Model 2 and smoking and alcohol consumption. Age groups are <50, 50~59, 60~69, and ≥70.
title: Ð¡ÑÐ¸Ð¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ HR-Ð¼ÐµÐ½ÐµÐ´Ð¶ÐµÐ½ÑÐ°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾Ð²Ð°Ð»ÐµÐ²Ð°, ÐÐºÐ°ÑÐµÑÐ¸Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼
ÑÑÐ¸Ð¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð¾Ð¿Ð»Ð°ÑÐ° ÑÑÑÐ´Ð°
Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½Ñ
Ð²Ð¾Ð·Ð½Ð°Ð³ÑÐ°Ð¶Ð´ÐµÐ½Ð¸Ðµ
HR-management
encouraging
payment
management

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐµÐ¼Ð° Ð°ÐºÑÑÐ°Ð»ÑÐ½Ð°, ÑÐ°Ðº ÐºÐ°Ðº ÑÐ¾Ð»Ñ ÑÑÐ¸Ð¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð² ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¸ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼ Ð½ÐµÑÐºÐ»Ð¾Ð½Ð½Ð¾ ÑÐ°ÑÑÑÑ. ÐÐ±ÑÐµÐºÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ°Ð±Ð¾ÑÑ - ÐÐÐ Â«ÐÑÐ¸Ð·Ð¼Ð°Â», Ð¿ÑÐµÐ´Ð¼ÐµÑ - ÑÐ¸ÑÑÐµÐ¼Ð° ÑÑÐ¸Ð¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð½Ð° Ð´Ð°Ð½Ð½Ð¾Ð¼ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸. Ð¦ÐµÐ»ÑÑ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÑÐ¸Ð¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ ÐÐÐ Â«ÐÑÐ¸Ð·Ð¼Ð°Â». ÐÐ°Ð´Ð°ÑÐ¸ ÑÐ°Ð±Ð¾ÑÑ: Ð¸Ð·ÑÑÐ¸ÑÑ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð°ÑÐ¿ÐµÐºÑÑ ÑÑÐ¸Ð¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð°, Ð¸Ð·ÑÑÐ¸ÑÑ ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ðµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ðµ ÐÐÐ Â«ÐÑÐ¸Ð·Ð¼Ð°Â» Ð¸ ÐµÐ³Ð¾ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÑÐ¸Ð¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ, Ð²ÑÑÐ²Ð¸ÑÑ ÐµÑ Ð½ÐµÐ´Ð¾ÑÑÐ°ÑÐºÐ¸ Ð¸ ÑÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°ÑÑ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ.
description: This topic is relevant, since the incentive role is steadily growing in HR-management. The object of research work - Ltd. "Prisma", the subject matter - the incentive system of personnel at the enterprise. The aim is to stimulate the improvement of the personnel system in the enterprise of Ltd."Prisma". Work Tasks: to study the theoretical aspects of incentives for staff to explore trade company Ltd. "Prisma" and its incentive system to identify its shortcomings and to generate proposals for improvement of the system.
Nondegenerate parametric amplification in superlattice and the limits of strong and weak dissipation
Creators: name: Hyart, Timo
name: Alekseev, Kirill N.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We develop a semiclassical theory of the nondegenerate parametric amplification in a single miniband of superlattice. We present the formulas describing absorption and gain of signal and idler fields in superlattice and analyze the limiting cases of strong and weak dissipation. We show how the well-known Manley-Rowe relations arise in the tight-binding lattice in the weak dissipation limit. Our results can be applied to an amplification of THz signals in semiconductor superlattices and a control of nonlinear transport of cold atoms in optical lattices.
description: Submitted to Proceedings of 32nd International Workshop on Condensed Matter Theories (birth centenary of L D Landau), Loughborough, UK, 13-18 August 2008, International Journal of Modern Physics B, 11 pages
Fotoni Zelig: si trasformano in assioni
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2017

Riproducendo la complessità del cosmo grazie a inedite simulazioni, una ricerca publicata su Physical Review Letters evidenzia l’importanza di un possibile comportamento dei fotoni ad altissima energia. Nel loro viaggio attraverso i campi magnetici intergalattici si potrebbero trasformare in assioni, evitando così di essere assorbiti
title: Public Recreation in Logan, Utah, 1946: An Appraisal
Creators: name: Carroll, Beatrice J.
Publisher: name: Utah State University
Year: 1948

description: Modern writers see varied values in recreation. The necessity for recreation in a machine age has become widely recognized. Its many-sided contribution to good living is being clarified by a constangly increasing member of writers--sociologists, educators, physicians, philosophers, etc. It seams appropriate to this inquiry to consider what some of these writers say.
Using Underapproximations for Sparse Nonnegative Matrix Factorization
Creators: name: Gillis, Nicolas
name: Glineur, François
Publisher: name: arXiv
Year: 2009
Subjects: subject: Optimization and Control (math.OC)
subject: FOS: Mathematics

description: Nonnegative Matrix Factorization consists in (approximately) factorizing a nonnegative data matrix by the product of two low-rank nonnegative matrices. It has been successfully applied as a data analysis technique in numerous domains, e.g., text mining, image processing, microarray data analysis, collaborative filtering, etc. We introduce a novel approach to solve NMF problems, based on the use of an underapproximation technique, and show its effectiveness to obtain sparse solutions. This approach, based on Lagrangian relaxation, allows the resolution of NMF problems in a recursive fashion. We also prove that the underapproximation problem is NP-hard for any fixed factorization rank, using a reduction of the maximum edge biclique problem in bipartite graphs. We test two variants of our underapproximation approach on several standard image datasets and show that they provide sparse part-based representations with low reconstruction error. Our results are comparable and sometimes superior to those obtained by two standard Sparse Nonnegative Matrix Factorization techniques.
description: Version 2 removed the section about convex reformulations, which was not central to the development of our main results; added material to the introduction; added a review of previous related work (section 2.3); completely rewritten the last part (section 4) to provide extensive numerical results supporting our claims. Accepted in J. of Pattern Recognition
title: ÐÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð´Ð° ÐºÐ¾Ð½ÐµÑÐ½ÑÑ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² Ð¿ÑÐ¸ ÑÐ°ÑÑÑÑÐµ ÐºÑÐ¸ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ°ÑÑÐ¾Ñ Ð²ÑÐ°ÑÐµÐ½Ð¸Ñ Ð²Ð°Ð»Ð¾Ð¿ÑÐ¾Ð²Ð¾Ð´Ð° Ð³Ð¸Ð´ÑÐ¾Ð³ÐµÐ½ÐµÑÐ°ÑÐ¾ÑÐ¾Ð² Ð² ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ð¸ Ñ Ð°Ð½Ð°Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ð¼ Ð¼ÐµÑÐ¾Ð´Ð¾Ð¼ ÑÐ°ÑÑÑÑÐ°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¨ÐµÑÑÐ°ÐºÐ¾Ð², ÐÐ½ÑÐ¾Ð½
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: Ð³Ð¸Ð´ÑÐ¾Ð³ÐµÐ½ÐµÑÐ°ÑÐ¾Ñ
Ð²Ð°Ð»Ð¾Ð¿ÑÐ¾Ð²Ð¾Ð´
ÐºÑÐ¸ÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ°ÑÑÐ¾ÑÐ° Ð²ÑÐ°ÑÐµÐ½Ð¸Ñ
ÐºÐ¾Ð½ÐµÑÐ½Ð¾-ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð·
Ð°Ð½Ð°Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð¼ÐµÑÐ¾Ð´
Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÑÑÑÐ¸Ð¹ Ð¿Ð¾Ð´ÑÐ¸Ð¿Ð½Ð¸Ðº
ÑÑÑÐ±Ð¸Ð½Ð°

description: Ð¦ÐµÐ»Ñ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ - ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ ÑÐ°ÑÑÑÑÐ° ÐºÑÐ¸ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ°ÑÑÐ¾Ñ Ð²ÑÐ°ÑÐµÐ½Ð¸Ñ Ð²Ð°Ð»Ð¾Ð¿ÑÐ¾Ð²Ð¾Ð´Ð° Ð³Ð¸Ð´ÑÐ¾Ð³ÐµÐ½ÐµÑÐ°ÑÐ¾ÑÐ° Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð³Ð¸Ð´ÑÐ¾Ð³ÐµÐ½ÐµÑÐ°ÑÐ¾ÑÐ° ÐÐ­Ð¡ ÐÐ° ÐÐ¸Ð½Ð°. Ð Ð°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÐ°ÑÑÑÑÑ ÐºÑÐ¸ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ°ÑÑÐ¾Ñ Ð²ÑÐ°ÑÐµÐ½Ð¸Ñ Ð²Ð°Ð»Ð¾Ð¿ÑÐ¾Ð²Ð¾Ð´Ð° Ð³Ð¸Ð´ÑÐ¾Ð³ÐµÐ½ÐµÑÐ°ÑÐ¾ÑÐ° ÐÐ­Ð¡ ÐÐ° ÐÐ¸Ð½Ð° (Ð§Ð¸Ð»Ð¸) Ð´Ð»Ñ Ð´Ð²ÑÑ Ð²Ð¸Ð´Ð¾Ð² Ð¾Ð¿Ð¾Ñ (Ð¶ÑÑÑÐºÐ¸Ðµ Ð¸ Ð¿Ð¾Ð´Ð°ÑÐ»Ð¸Ð²ÑÐµ). Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½Ð°Ñ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ñ ÑÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°ÑÑ ÑÐ°ÑÑÑÑÑ ÐºÑÐ¸ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ°ÑÑÐ¾Ñ Ð²ÑÐ°ÑÐµÐ½Ð¸Ñ Ð´Ð»Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹ Ð²Ð°Ð»Ð¾Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¾Ð² Ð³Ð¸Ð´ÑÐ¾Ð³ÐµÐ½ÐµÑÐ°ÑÐ¾ÑÐ¾Ð², ÑÑÐ¾ ÑÐ²Ð»ÑÐµÑÑÑ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÐ¼ Ð²ÑÐ»ÐµÐ´ÑÑÐ²Ð¸Ðµ Ð¼Ð½Ð¾Ð³Ð¾Ð¾Ð±ÑÐ°Ð·Ð¸Ñ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹ ÑÑÐ¸Ñ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¼Ð°ÑÐ¸Ð½.
Fonte d’energia inattesa per le aurore di Giove
Creators: Francesca Aloisio
Publisher: name: Media Inaf
Year: 2017

Uno studio pubblicato su Nature spiega che le aurore su Giove si comportano in modo diverso rispetto a quelle terrestri. Nuove osservazioni, effettuate grazie allo spettrografo ultravioletto in dotazione alla sonda Juno della Nasa hanno dimostrato che - contrariamente a quello che ci si aspettava - i processi di formazione delle aurore gioviane più intense non sono assimilabili a quelli terrestri
A study of waves in the open ocean and of waves on shear currents
Creators: name: Drent, Jan
Publisher: name: University of British Columbia
Year: 2012

description: The dimensions and periods of waves on the oceans are still very imperfectly known, as can be seen from the divergent opinions expressed by the relatively few authorities who have occupied themselves with this problem. For many years I have endeavoured to observe waves at sea. The results of these observations are given in Part I, both in graphical and tabular form. The directly determined quantities were wave height and wave period, both being based on visual observation. A distinction was carefully made between waves under the direct influence of wind (called sea) and those that were only under the influence of gravity (called swell). In Part II the interaction between waves and currents is studied. The approximation is not carried further than to quantities K²a², where K is the wave number = L/2π and a is the surface amplitude = ½H = ½ wave height.
title: ÐÐ²Ð°Ð·Ð¸ÐºÐ¾Ð½Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾Ð»ÐµÐ²ÑÐµ ÑÑÑÑÐºÑÑÑÑ Ð´Ð»Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð¾-Ð¾Ð¿ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÑÐµÐ´
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Ð¼Ð°ÑÐ¾ÐºÐ¾Ð²Ð°, Ð¢Ð°ÑÑÑÐ½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð¡Ð¿ÐµÐºÑÑÐ¾Ð³ÑÐ°ÑÑ
Ð¤ÑÐ½ÐºÑÐ¸Ð¸ (Ð¼Ð°Ñ.) Ð­Ð¹Ð»ÐµÑÐ°
Ð¢ÑÐ°ÐµÐºÑÐ¾ÑÐ¸Ð¸
ÐÐ½Ð°Ð»Ð¸Ð·Ð°ÑÐ¾ÑÑ ÑÐ¿ÐµÐºÑÑÐ°
ÑÐ½ÐµÑÐ³Ð¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð°ÑÐ¾ÑÑ

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð±ÑÐ»Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ Ð¿Ð¾Ð»ÐµÐ²ÑÐµ ÑÑÑÑÐºÑÑÑÑ, Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»ÑÐ½ÑÐµ Ð¿Ð¾ÑÑÑÐµÑÑ ÐºÐ¾ÑÐ¾ÑÑÑ ÑÐ²Ð»ÑÑÑÑÑ Ð¾Ð´Ð½Ð¾ÑÐ¾Ð´Ð½ÑÐ¼Ð¸ Ð¿Ð¾ Ð­Ð¹Ð»ÐµÑÑ ÑÑÐ½ÐºÑÐ¸ÑÐ¼Ð¸ Ð½ÑÐ»ÐµÐ²Ð¾Ð¹ ÑÑÐµÐ¿ÐµÐ½Ð¸ ÐºÑÐ°ÑÐ½Ð¾ÑÑÐ¸. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ñ ÑÐ°ÑÑÐµÑÑ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð¾-Ð¾Ð¿ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ²Ð¾Ð¹ÑÑÐ² Ð´Ð²ÑÑ ÑÐ°Ð±Ð¾ÑÐ¸Ñ ÑÐµÐ¶Ð¸Ð¼Ð¾Ð² ÑÐ¿ÐµÐºÑÑÐ¾Ð³ÑÐ°ÑÐ°, Ð½Ð° Ð±Ð°Ð·Ðµ Ð¿Ð¾Ð»Ñ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ ÑÐ¸Ð¿Ð°. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð²ÑÐ¾Ð´Ð½ÑÑ Ð¸ Ð²ÑÑÐ¾Ð´Ð½ÑÑ Ð¾ÑÐ²ÐµÑÑÑÐ¸Ð¹.
Burniat surfaces II: secondary Burniat surfaces form three connected components of the moduli space
Creators: name: Bauer, Ingrid
name: Catanese, Fabrizio
Publisher: name: arXiv
Year: 2009
Subjects: subject: Algebraic Geometry (math.AG)
subject: FOS: Mathematics
subject: 14J29,14J25,14J10,14D22,14H30,32G05,32Q30

description: We prove in one go that each of the 4 families of Burniat surfaces with K^2 = 6,5,4, is a connected component of the moduli space of surfaces of general type. We prove also the rationality of each component. In the nodal case (one of the two families for K^2_S = 4) a very surprising and new phenomenon occurs. Both the moduli space for the minimal models and the Gieseker moduli space for canonical models are everywhere non reduced. But the nilpotence order is higher for the first.
description: 26 pages, 1 figure, article dedicated to David Mumford on the occasion of his 2^3 . 3^2-th birthday
title: Participation in Social Institutions by Relief Families in a Selected Rooming House Area in Salt Lake City July 1933 to July 1934
Creators: name: Eames, D. Ivo
Publisher: name: Utah State University
Year: 1943

description: A series of happenlngs in Salt Lake City during the early years of the reoent depression strongly Indlcate that certain relief clients were, at that time, more or leas chronic trouble makers. They frequently threatened and sometimes inflicted bodily harm on social case workers; they inflicted riots, held protest meetings and wrote protest letters to state and national officials. A check-up on the addresses of these clients showed that the majority lived in the same or near-by areas.
Tempesta solare, arrivo previsto per venerdì 8
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2017

Tre brillamenti in pochi giorni, tutti nella stessa regione attiva del Sole. Uno lunedì scorso e due ieri, l’ultimo dei quali d’intensità record: X9.3, il più violento dell’attuale ciclo solare. Ed è la bolla di plasma prodotta da quest’ultimo che potrebbe interferire, nelle prossime ore, con alcuni sistemi di comunicazione
Additional file 4 of Initial treatment approaches and healthcare utilization among veterans with low back pain: a propensity score analysis
Creators: name: Schmidt, Catherine
name: Borgia, Matthew
name: Zhang, Tingting
name: Gochyyev, Perman
name: Shireman, Theresa I.
name: Resnik, Linda
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Neuroscience
subject: Pharmacology
subject: Biotechnology
subject: Ecology
subject: Cancer
subject: Science Policy
subject: Mental Health

description: Supplementary Material 4
Commissioning of the CMS High Level Trigger
Creators: name: Agostino, Lorenzo
name: Bauer, Gerry
name: Beccati, Barbara
name: Behrens, Ulf
name: Berryhil, Jeffrey
name: Biery, Kurt
name: Bose, Tulika
name: Brett, Angela
name: Branson, James
name: Cano, Eric
name: Cheung, Harry
name: Ciganek, Marek
name: Cittolin, Sergio
name: Coarasa, Jose Antonio
name: Dahmes, Bryan
name: Deldicque, Christian
name: Dusinberre, Elizabeth
name: Erhan, Samim
name: Gigi, Dominique
name: Glege, Frank
name: Gomez-Reino, Robert
name: Gutleber, Johannes
name: Hatton, Derek
name: Laurens, Jean-Francois
name: Loizides, Constantin
name: Ma, Frank
name: Meijers, Frans
name: Meschi, Emilio
name: Meyer, Andreas
name: Mommsen, Remigius K.
name: Moser, Roland
name: O'Dell, Vivian
name: Oh, Alexander
name: Orsini, Luciano
name: Patras, Vaios
name: Paus, Christoph
name: Petrucci, Andrea
name: Pieri, Marco
name: Racz, Attila
name: Sakulin, Hannes
name: Sani, Matteo
name: Schieferdeckerd, Philipp
name: Schwick, Christoph
name: Margaleff, Josep Francesc Serrano
name: Shpakov, Dennis
name: Simon, Sean
name: Sumorok, Konstanty
name: Yoon, Andre Sungho
name: Wittich, Peter
name: Zanetti, Marco
Publisher: name: arXiv
Year: 2009
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: The CMS experiment will collect data from the proton-proton collisions delivered by the Large Hadron Collider (LHC) at a centre-of-mass energy up to 14 TeV. The CMS trigger system is designed to cope with unprecedented luminosities and LHC bunch-crossing rates up to 40 MHz. The unique CMS trigger architecture only employs two trigger levels. The Level-1 trigger is implemented using custom electronics, while the High Level Trigger (HLT) is based on software algorithms running on a large cluster of commercial processors, the Event Filter Farm. We present the major functionalities of the CMS High Level Trigger system as of the starting of LHC beams operations in September 2008. The validation of the HLT system in the online environment with Monte Carlo simulated data and its commissioning during cosmic rays data taking campaigns are discussed in detail. We conclude with the description of the HLT operations with the first circulating LHC beams before the incident occurred the 19th September 2008.
title: ÐÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐµÐ½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð¶Ð¸Ð»Ð¸ÑÐ½ÑÑ Ð¿ÑÐ¾ÐµÐºÑ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°Ð·Ð¾Ð²Ð°, ÐÐ½Ð½Ð°
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¸Ð»ÑÐµ Ð·Ð´Ð°Ð½Ð¸Ñ
ÑÐµÐ½Ð¾Ð²Ð°ÑÐ¸Ñ

description: Ð¡Ð±Ð°Ð»Ð°Ð½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ðµ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ Ð³Ð¾ÑÐ¾Ð´Ð° Ð½ÐµÑÐ¾Ð¼Ð½ÐµÐ½Ð½Ð¾ Ð²Ð·Ð°Ð¸Ð¼Ð¾ÑÐ²ÑÐ·Ð°Ð½Ð¾ Ñ ÑÐ»ÑÑÑÐµÐ½Ð¸ÐµÐ¼ ÑÑÐ»Ð¾Ð²Ð¸Ð¹ Ð¶Ð¸Ð·Ð½Ð¸ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð¸Ñ. ÐÐ½Ð¾ Ð¼Ð¾Ð¶ÐµÑ Ð´Ð¾ÑÑÐ¸Ð³Ð°ÑÑÑÑ ÑÐµÑÐµÐ·
Ð²Ð¾ÑÐ¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð¾ Ð¶Ð¸Ð»Ð¸ÑÐ½Ð¾Ð³Ð¾ ÑÐ¾Ð½Ð´Ð°, ÐºÐ¾ÑÐ¾ÑÐ¾Ðµ, Ð² ÑÐ²Ð¾Ñ Ð¾ÑÐµÑÐµÐ´Ñ Ð¾Ð±ÐµÑÐ¿ÐµÑÐ¸Ð²Ð°ÐµÑÑÑ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸ÐµÐ¹ Ð¸Ð½ÑÐµÐ½ÑÐ¸Ð²Ð½ÑÑ Ð¸ ÑÐºÑÑÐµÐ½ÑÐ¸Ð²Ð½ÑÑ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² ÑÐµÐ½Ð¾Ð²Ð°ÑÐ¸Ð¸.
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° Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¾ÑÑÑÐµÑÑÐ²Ð»ÐµÐ½Ð¸Ñ Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ. ÐÐ»Ñ Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð½Ð¾Ð¹ ÑÐµÐ»Ð¸ Ð±ÑÐ» Ð¾ÑÑÑÐµÑÑÐ²Ð»ÐµÐ½ ÑÐ°Ð·Ð±Ð¾Ñ Ð¿Ð¾Ð½ÑÑÐ¸Ñ Â«ÑÐµÐ½Ð¾Ð²Ð°ÑÐ¸ÑÂ», Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÑ Ñ Ð½Ð¸Ð¼ Ð¿Ð¾Ð½ÑÑÐ¸Ð¹. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð·Ð°ÑÑÐ±ÐµÐ¶Ð½Ð¾Ð³Ð¾ Ð¾Ð¿ÑÑÐ° Ð¾ÑÑÑÐµÑÑÐ²Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼ ÑÐµÐ½Ð¾Ð²Ð°ÑÐ¸Ð¸ Ð¶Ð¸Ð»ÑÑ Ð·Ð´Ð°Ð½Ð¸Ð¹. ÐÐ°Ð½Ð° Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð¾ÑÐµÐ½ÐºÐ¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼ ÑÐµÐ½Ð¾Ð²Ð°ÑÐ¸Ð¸ Ð¶Ð¸Ð»ÑÑ. Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½ ÐºÐ¾ÑÑÑÐ¸ÑÐ¸ÐµÐ½Ñ ÑÐµÐ½Ð¾Ð²Ð°ÑÐ¸Ð¸, Ð²Ð½ÑÑÑÐµÐ½Ð½ÑÑ Ð½Ð¾ÑÐ¼Ð° Ð´Ð¾ÑÐ¾Ð´Ð½Ð¾ÑÑÐ¸, ÑÐ¸ÑÑÐ°Ñ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð½Ð°Ñ ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÑ.
ÐÑÐ¾Ð³Ð¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÑÐ°Ð» ÑÐ°ÑÑÐµÑ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ° ÑÐµÐ½Ð¾Ð²Ð°ÑÐ¸Ð¸ Ð² ÐÐ¾ÑÐºÐ²Ðµ.
Visceral leishmaniasis causing life-threatening digestive bleeding
Creators: name: Tonolini, Massimo
Publisher: name: EURORAD
Year: 2015
Subjects: subject: Lung
subject: Small bowel
subject: Spleen
subject: CT
subject: Diagnostic procedure
subject: Haemorrhage
subject: Infection

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: male, 27 years
description: Clinical History: Young immigrant from Ukraine suffering from high fever since one year, attributed to systemic lupus erythematosus and unsuccessfully treated with steroids in his native country. Physically found febrile, debilitated with generalized wasting, multiple cuta... Final Diagnosis: Visceral leishmaniasis complicated by small bowel haemorrhage requiring transarterial embolisation
Primordial black hole formation in the radiative era: investigation of the critical nature of the collapse
Creators: name: Musco, Ilia
name: Miller, John C.
name: Polnarev, Alexander G.
Publisher: name: arXiv
Year: 2008
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Following on after two previous papers discussing the formation of primordial black holes in the early universe, we present here results from an in-depth investigation of the extent to which primordial black hole formation in the radiative era can be considered as an example of the critical collapse phenomenon. We focus on initial supra-horizon-scale perturbations of a type which could have come from inflation, with only a growing component and no decaying component. In order to study perturbations with amplitudes extremely close to the supposed critical limit, we have modified our previous computer code with the introduction of an adaptive mesh refinement scheme. This has allowed us to follow black hole formation from perturbations whose amplitudes are up to eight orders of magnitude closer to the threshold than we could do before. We find that scaling-law behaviour continues down to the smallest black hole masses that we are able to follow and we see no evidence of shock production such as has been reported in some previous studies and which led there to a breaking of the scaling-law behaviour at small black-hole masses. We attribute this difference to the different initial conditions used. In addition to the scaling law, we also present other features of the results which are characteristic of critical collapse in this context.
description: 21 pages, 7 figures, the present version is updated with some changes and two new appendix. Accepted for pubblication in Classical and Quantum Gravity
Soziale Medien als politischer Informationskanal
Creators: name: Praprotnik, Katrin
name: Perlot, Flooh
name: Ingruber, Daniela
name: Filzmaier, Peter
Publisher: name: Österreichische Zeitschrift für Politikwissenschaft
Year: 2019

description: Ein lebendiger politischer Diskurs ist ein wesentlicher Bestandteil einer funktionierenden Demokratie. Mit steigenden Nutzerzahlen der sozialen Medien besitzt auch die politische Diskussion, die über diese Plattformen geführt wird, eine zunehmende Bedeutung. Die vorliegende Studie untersucht deshalb die KonsumentInnen von politischer Information über soziale Netzwerke anhand des wenig untersuchten Fallbeispiels Österreich. Unsere Modelle basieren auf einer Sekundärdatenauswertung der Studie Digitalmonitor (N=1.200). Die Ergebnisse zeigen, dass die NutzerInnen von politischer Information über soziale Netzwerke unter anderem politisch stark interessiert, auf einer Links-Rechts-Skala eher extrem eingestellt sind und ein geringes Vertrauen in traditionelle Medien haben. Der neue Informationskanal sorgt nicht zwangsläufig für einen gleichberechtigteren Zugang zu Information. Für Menschen, die mit dem bisherigen Angebot nicht zufrieden waren, bietet er jedoch eine Alternative.
description: Österreichische Zeitschrift für Politikwissenschaft, Bd. 48 Nr. 1 (2019): Offenes Heft
Multiple aneurysms in Takayasu arteritis: An uncommon presentation
Creators: name: Jain, Neeraj
Publisher: name: EURORAD
Year: 2015
Subjects: subject: Arteries / Aorta
subject: CT-Angiography
subject: Contrast agent-intravenous
subject: Aneurysms

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: male, 40 years
description: Clinical History: A 20-year-old young male presented with 2-year history of recurrent chest and abdominal pain. On further enquiry he reported a past history of low-grade fever and malaise. Physical examination was unremarkable. On routine blood examination elevated erythr... Final Diagnosis: Takayasu arteritis
title: An Evaluation of the Practices and Functions of the Clerk of the Board of Education in the State of Utah
Creators: name: Andrew, Dean C.
Publisher: name: Utah State University
Year: 1947

description: Regardless of the size, the school district has some person who is responsible for keeping the clerical and financial records of the school district. This position is frequently designated as the office of the clerk of the board of education. When the efficient clerk assumes the clerical and financial duties of the school district the superintendent is relieved of endless details, which allows him greater opportunity to perform those functions for which he is qualified, thus a smoother and a more efficient school system is the result
title: ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð² ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÑ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸ÑÑ
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ÐµÐ´Ð¼Ð¸ÑÐºÐ°Ñ, ÐÐºÐ°ÑÐµÑÐ¸Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸
Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐµ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ
ÑÐ¸ÑÑÐ¾Ð²ÑÐµ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸
Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÑ

description: ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð² Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÑ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸ÑÑ Ð²ÐºÐ»ÑÑÐ°ÑÑ Ð² ÑÐµÐ±Ñ Ð¼Ð½Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ°Ð²Ð»ÑÑÑÐ¸Ñ Ð¿Ð¾Ð½ÑÑÐ¸Ð¹. Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð·Ð½Ð°Ð½Ð¸Ð¹ Ð¾Ð± Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÑÑ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÑ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ð¹, ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð¸ Ð¸Ñ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð²Ð»Ð¸ÑÐ½Ð¸Ð¸ Ð¿ÑÐ¾Ð¸ÑÑÐ¾Ð´Ð¸Ñ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¾Ð»Ð¸ ÐÐÐ¢ Ð² ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÑ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸ÑÑ, ÑÑÐ¾ ÑÐ²Ð»ÑÐµÑÑÑ Ð´Ð¾ÑÑÐ°ÑÐ¾ÑÐ½Ð¾ Ð°ÐºÑÑÐ°Ð»ÑÐ½ÑÐ¼ Ð²Ð¾Ð¿ÑÐ¾ÑÐ¾Ð¼, ÐºÐ¾ÑÐ¾ÑÑÐ¹ Ð½Ð¸ÐºÐ¾Ð³Ð´Ð° Ð½Ðµ ÑÑÐ¾Ð´Ð¸Ñ Ñ Ð¿Ð¾Ð²ÐµÑÑÐºÐ¸ Ð´Ð½Ñ.
Un asteroide a colazione: il parere dell’astrofisico
Creators: Fabio Gironi
Publisher: name: Media Inaf
Year: 2017

Dobbiamo stare attenti ai meteoriti quando facciamo merenda in giardino? Abbiamo raccolto il parere di un esperto, Giovanni Valsecchi dell'Inaf Iaps di Roma. Nota: nessun astrofisico è stato maltrattato durante la conduzione di questa intervista
title: A Study of Thirty-Six Organizations of Logan, Utah, in 1945-46 to Determine Their Fields of Activity and the Amount of Duplication and Coordination that Exists Among Them
Creators: name: Capener, Harold R.
Publisher: name: Utah State University
Year: 1946

description: The city of Logan, Utah, was first settled in 1859 and derives its name from an old Indian Chief named "Logan," who had befriended the early white settlers.
Scoperta una pulsar binaria da record
Creators: Ufficio stampa Inaf
Publisher: name: Media Inaf
Year: 2017

Un sistema binario con accelerazioni fino a 70 g, formato da una pulsar e una stella di neutroni in orbita stretta l’una attorno all’altra, è stato scoperto analizzando i dati raccolti dal radiotelescopio da 64 metri di Parkes, in Australia. Fra gli autori della scoperta, presentata oggi al simposio Iau di Jodrell Bank, anche Andrea Possenti e Marta Burgay dell’Inaf di Cagliari
title: Some Factors Related to Student Achievement of Entering Freshmen at the Utah State Agricultural College
Creators: name: Day, James Francis
Publisher: name: Utah State University
Year: 1939

description: The need for study in regard to factors related to student achievement and their possible application as guidance devices for entering freshmen in any college is very evident in our modern life. We have only to look at the increasing college enrollments and to the scarcity of positions for college graduates to realize this. In an effort to meet this need, educators should more and more base their practices on the findings of statistical and experimental studies.
Spitzer-IRS Study of the Antennae Galaxies NGC 4038/39
Creators: name: Brandl, B. R.
name: Snijders, L.
name: Brok, M. den
name: Whelan, D. G.
name: Groves, B.
name: van der Werf, P.
name: Charmandaris, V.
name: Smith, J. D.
name: Armus, L.
name: Kennicutt,, R. C.
name: Houck, J. R.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Using the Infrared Spectrograph on the Spitzer Space Telescope, we observed the Antennae galaxies obtaining spectral maps of the entire central region and high signal-to-noise 5-38 um spectra of the two galactic nuclei and six infrared-luminous regions. The total infrared luminosity of our six IR peaks plus the two nuclei is L_IR = 3.8x10^10 L_o, with their derived star formation rates ranging between 0.2 and 2 M_o/yr, with a total of 6.6 M_o/yr. The hardest and most luminous radiation originates from two compact clusters in the southern part of the overlap region, which also have the highest dust temperatures. PAH emission and other tracers of softer radiation are spatially extended throughout and beyond the overlap region, but regions with harder and intenser radiation field show a reduced PAH strength. The strong H_2 emission is rather confined around the nucleus of NGC 4039, where shocks appear to be the dominant excitation mechanism, and the southern part of the overlap region, where it traces the most recent starburst activity. The luminosity ratio between the warm molecular gas (traced by the H_2 lines) and the total far-IR emission is ~1.6x10^-4, similar to that found in many starburst and ULIRGs. The total mass of warm H_2 in the Antennae is 2.5x10^7 M_o, with a fraction of warm to total H_2 gas mass of about 0.35%. The average warm H_2 temperature is 302+/-26 K and appears anti-correlated with the radiation field hardness, possibly due to an evolution of the PDR morphology. The previously reported tight correlation between the H_2 and PAH emission was not found but higher total PAH emission to continuum ratios were found in PDRs with warmer gas.
description: 24 pages, 13 figures, accepted by ApJ, full resolution version at http://www.strw.leidenuniv.nl/~brandl/ngc4038_brandl.pdf
Ufo a Varsavia: intervista a Francesco Tombesi
Creators: Livia Giacomini
Publisher: name: Media Inaf
Year: 2017

Si inaugura oggi, mercoledì 6 settembre, nella capitale polacca un congresso internazionale dedicato alla spettroscopia X. Abbiamo intervistato uno dei relatori, Francesco Tombesi, ”cervello” rientrato da poco in Italia, all’Università di Roma “Tor Vergata”, dopo un lungo periodo alla Nasa
Nature Astronomy dedica un numero a Cassini
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2017

Per celebrare il Grand Finale della sonda Nasa, la rivista dedicata all’astronomia del gruppo Nature ha invitato 12 scienziati della missione e un editor a commentare altrettante immagini. Fra loro anche Gianrico Filacchione dell’Inaf Iaps di Roma, la cui scelta è caduta sulla celebre “ll giorno in cui la Terra sorrise”
Dal radio al gamma, la Crab senza più segreti
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2017

Un nuovo modello descrive il comportamento delle particelle ad alta energia emessedalle vestigia delle esplosioni di supernova e spiega le osservazioni astronomiche su un intervallo di energia sorprendentemente largo. Il modello suggerisce che gli scienziati ancora non comprendono i processi all’origine dei raggi cosmici
The radio-infrared correlation in galaxies
Creators: name: Tabatabaei, F. S.
name: Beck, R.
name: Berkhuijsen, E. M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The radio-infrared correlation was explained as a direct and linear relationship between star formation and IR emission. However, one fact making the IR-star formation linkage less obvious is that the IR emission consists of at least two emission components, cold dust and warm dust. The cold dust emission may not be directly linked to the young stellar population. Furthermore, understanding the origin of the radio-IR correlation requires to discriminate between the two main components of the radio continuum emission, free-free and synchrotron emission. Here, we present a multi-scale study of the correlation of IR with both the thermal and non-thermal (synchrotron) components of the radio continuum emission from the nearby galaxies M33 and M31.
description: To appear in Highlights of Astronomy, Volume 15, XXVIIth IAU General Assembly, August 2009
title: ÐÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿Ð°ÑÑÐ°Ð¶Ð¸ÑÑÐºÐ¾Ð³Ð¾ Ð»Ð¸ÑÑÐ°: Ð³ÑÑÐ·Ð¾Ð¿Ð¾Ð´ÑÐµÐ¼Ð½Ð¾ÑÑÑ 500 ÐºÐ³, ÑÑÐ°Ð¶Ð½Ð¾ÑÑÑ 14, ÑÐºÐ¾ÑÐ¾ÑÑÑ 1,1 Ð¼/Ñ
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ÑÐ·ÑÐ¼Ð¸Ð½, ÐÐ°ÑÐº
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð¿Ð°ÑÑÐ°Ð¶Ð¸ÑÑÐºÐ¸Ð¹ Ð»Ð¸ÑÑ
Ð¿Ð¾Ð»Ð½ÑÐ¹ ÑÑÐ³Ð¾Ð²ÑÐ¹ ÑÐ°ÑÑÐµÑ
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description: Ð Ð°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð°ÑÑÐ°Ð¶Ð¸ÑÑÐºÐ¾Ð³Ð¾ Ð»Ð¸ÑÑÐ°. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð±ÑÐ»Ð¸ ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½Ñ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼ Ð¿Ð¾Ð´ÑÐµÐ¼Ð°, Ð¼ÐµÑÐ°Ð»Ð»Ð¾ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ñ ÐºÐ°ÑÐºÐ°ÑÐ° ÐºÐ°Ð±Ð¸Ð½Ñ Ð¸ Ð¾ÑÐ½Ð¾Ð²Ð½Ð¾Ðµ Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð»Ð¸ÑÑÐ°.
title: Building efficiency rating approach with indoor environmental quality assessment and building energy usage from sustainability certification data
Creators: name: Fahrich, Raik
Publisher: name: Technische Universität Berlin
Year: 2025
Subjects: subject: 600 Technik, Medizin, angewandte Wissenschaften::620 Ingenieurwissenschaften::624 Ingenieurbau
subject: Indoor Environmental Quality (IEQ)
subject: Building performance
subject: Sustainability certification
subject: Thermal comfort
subject: Energy demand
subject: Subject study
subject: Innenraumluftqualität
subject: Gebäudeleistung
subject: Nachhaltigkeitszertifizierung
subject: Thermischer Komfort
subject: Energiebedarf
subject: Probandenstudie

description: Assessing a building’s energy efficiency is a major goal to avoid unnecessary and inef- ficient energy-consuming renovations. Currently, building energy efficiency is measured primarily by the energy demand of the building. However, higher energy efficiency of the building is not always in alignment with greater comfort of the occupant, which is the main benefit a building provides. In this study, indoor environmental quality (IEQ) ratings and building energy demand are considered together to evaluate building energy efficiency. It compares the IEQ comfort achieved to the energy demand of the building. An example IEQ-Index calculation based on certification data of two buildings assessed by a German building sustainability certification system is used. The data includes scoring of different IEQ categories and information on energy usage for the buildings. Additionally, a survey on IEQ factors was conducted among building users and the results were compared to those based on the certification assessment data. The IEQ rating of the building certification data based on building design and measurement data for the individual factors differed from the subject study results by up to 50%. The considered buildings overall performance ranged from 0.13 to 0.16 IEQ-Score per MJ/m2a for the certification data and survey results.
title: A Study of a Remedial Speech Program in Operation in Four Rural Schools in the State of Utah
Creators: name: Anderson, John O.
Publisher: name: Utah State University
Year: 1948

description: Recent speech surveys conducted in Box Elder County showed that approximately 17% of the elementary school children there had speech defects of such seriousness that they needed clinical attention. A remedial speech program was organized and remedial speech training given at four schools in Box Elder County. The purpose of this project was to study this remedial speech program, as it was in operation, in an effort to determine the feasibility and value of such a program.
Che curioso quel lampo così vicino
Creators: Patrizia Caraveo
Publisher: name: Media Inaf
Year: 2017

Il Vlt dell'Eso, Fermi, Hubble, Chandra... Se nell’arco di pochi giorni tanti super telescopi si voltano tutti dalla stessa parte – un’anonima galassia ellittica a 130 milioni di anni luce – è inevitabile chiedersi perché. Come ha fatto domenica Patrizia Caraveo, direttrice dell’Inaf Iasf di Milano, con quest’articolo pubblicato sul Sole24Ore, che vi riproponiamo con la sua autorizzazione
title: Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ°ÑÑÑ ÑÑÐ°Ð½ÑÐ¸Ð¹ Ð¸ Ð¿Ð¾Ð´ÑÑÐ°Ð½ÑÐ¸Ð¹
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ°ÑÐ¸Ð»ÑÐµÐ²Ð°, ÐÐ»ÑÐ³Ð°
name: ÐÐµÑÑÐ¾Ð²Ð°, Ð¡Ð²ÐµÑÐ»Ð°Ð½Ð°
name: Ð¨Ð°ÑÐ¾Ð²Ð°, ÐÐ°ÑÐ¸Ñ
name: ÐÐ¾Ð¿Ð¾Ð², ÐÐ°ÐºÑÐ¸Ð¼
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2019
Subjects: Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÑÐ°Ð½ÑÐ¸Ð¸
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