cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Origin of Large Dielectric Constant with Large Remnant Polarization and Evidence of Magnetoelectric Coupling in Multiferroic La modified BiFeO3-PbTiO3 Solid Solution
Creators: name: Singh, Anupinder
name: Chatterjee, Ratnamala
name: Mishra, S. K.
name: Krishna, P. S. R.
name: Chaplot, S. L.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The presence of superlattice reflections and detailed analyses of the powder neutron and x-ray diffraction data reveal that La rich (BF$_{0.50}$-LF$_{0.50}$)$_{0.50}$-(PT)$_{0.50}$ (BF-LF-PT) has ferroelectric rhombohedral crystal structure with space group \textit{$R3c$} at ambient conditions. The temperature dependence of lattice parameters, tilt angle, calculated polarization $(P_{s})$, volume, and integrated intensity of superlattice and magnetic reflections show an anomaly around 170 K. Impedance spectroscopy, dielectric and ac conductivity measurements were performed in temperature range $473K \leq T \leq 573K$ to probe the origin of large remnant polarization and frequency dependent broad transitions with large dielectric constant near $T_c^{FE}$. Results of impedance spectroscopy measurements clearly show contributions of both grain and grain boundaries throughout the frequency range ($10^{3}$ Hz$\leq f\leq 10^{7} $ Hz). It could be concluded that the grain boundaries are more resistive and capacitive as compared to the grains, resulting in inhomogeneities in the sample causing broad frequency dependent dielectric anomalies. Enhancement in dielectric constant and remnant polarization values are possibly due to space charge polarization caused by piling of charges at the interface of grains and grain boundaries. The imaginary parts of dielectric constant ($ε^{\prime\prime}$) Vs frequency data were fitted using Maxwell-Wagner model at $T_c^{FE}(\sim 523$K) and model fits very well with the data up to $10^{5}$ Hz. Magnetodielectric measurements prove that the sample starts exhibiting magnetoelectric coupling at $\sim 170$ K, which is also validated by neutron diffraction data.
description: 20 pages, 10 figures
Extraoccular Orbital metastases as only site of metastatic spread from breast cancer: Case report
Creators: name: Emad, Sally
Publisher: name: EURORAD
Year: 2015
Subjects: subject: Neuroradiology brain
subject: MR
subject: Defecography
subject: Diagnostic procedure
subject: Neoplasia

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: female, 42 years
description: Clinical History: A 42-year old woman,  presented with swelling, diplopia, and pain in her right eye. She had been diagnosed with left cancer breast  (invasive lobular carcinoma) 2 years ago. She had been treated with left mastectomy followed by postoperative external beam... Final Diagnosis: Orbital metastases from breast carcinoma
Una cometa, o forse due per NEOWISE
Creators: Giuseppina Pulcrano
Publisher: name: Media Inaf
Year: 2016

La missione NASA per la caccia agli asteroidi  ha intercettato due oggetti celesti in avvicinamento. Per uno non c'è ancora la certezza che si tratti di un asteroide, l’altro è invece una cometa a tutti gli effetti: sta viaggiando verso il Sole all'interno dell'orbita di Mercurio
Links between self-reported and caregiver-reported sensory questionnaires and alexithymia traits.
Creators: name: Manning, Catherine
name: Taylor, Katie
name: King, Jodie
Publisher: name: OSF Registries
Year: 2023
Subjects: subject: Social and Behavioral Sciences
subject: Psychology
subject: FOS: Psychology

description: This project aims to investigate whether alexithymia traits are related to a discrepancy between self- and caregiver-reported sensory questionnaires.
Additional file 3 of CDKN2AIP is critical for spermiogenesis and germ cell development
Creators: name: Cao, Yuming
name: Sun, Qi
name: Chen, Zhenlie
name: Lu, Jing
name: Geng, Ting
name: Ma, Ling
name: Zhang, Yuanzhen
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 3: Figure S3. Cdkn2aip-/- mice exhibit abnormal autosomal synapsis at meiosis prophase I. (A) Immunostaining of SYCP3(red) and HORMAD1(green) in Cdkn2aip +/+ and Cdkn2aip-/- pachytene spermatocytes, n=3 mice for each group Scale bars, 10μm. (B) Statistical results of (A). Data are presented as average percentage, n=3 mice for each group, and 50 spermatocyte were counted for each mouse. (C) Frozen section staining of γH2AX (green) and DIPA (blue) in testicular tissue from P56 Cdkn2aip +/+ and Cdkn2aip-/- mice. Scale bar, 50μm. (D) Statistical results of abnormal γH2AX signals/tubule. n=3 mice for each group, and 20 tubules were counted for each mouse. Data are presented as mean±SD, ***P<0.001 by two-tailed Student’s-test. (E) Immunostaining of 53BP1 (green) and SYCP3(red) and on chromosome spreads of spermatocytes from P35 Cdkn2aip +/+ and Cdkn2aip-/- mice testes, n=3 mice for each group. Scale bars, 10μm. (F) Statistical analysis of abnormal location percentage of 53BP1 in pachytene spermatocytes. Data are presented as average percentage, n=3 mice for each group, and 100 pachytene spermatocytes were counted for each mouse.
Rate description of Fokker-Planck processes with time-periodic parameters
Creators: name: Kim, Changho
name: Talkner, Peter
name: Lee, Eok Kyun
name: Hanggi, Peter
Publisher: name: arXiv
Year: 2009
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: The large time dynamics of a periodically driven Fokker-Planck process possessing several metastable states is investigated. At weak noise transitions between the metastable states are rare. Their dynamics then represent a discrete Markovian process characterized by time dependent rates. Apart from the occupation probabilities, so-called specific probability densities and localizing functions can be associated to each metastable state. Together, these three sets of functions uniquely characterize the large time dynamics of the conditional probability density of the original process. Exact equations of motion are formulated for these three sets of functions and strategies are discussed how to solve them. These methods are illustrated and their usefulness is demonstrated by means of the example of a bistable Brownian oscillator within a large range of driving frequencies from the slow semiadiabatic to the fast driving regime.
Le antiche terme di Marte
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2016

Tracce convincenti di una passata attività idrotermale nell'Auki crater su Marte sono state individuate da un team di scienziati guidati da Filippo Giacomo Carrozzo dell'INAF. Auki Crater si candida così come uno fra i più importanti siti di interesse astrobiologico presenti sul Pianeta rosso: lì potrebbero essersi verificate le condizioni favorevoli alla formazione e al proliferare della vita
Development of runner reservoir and its effect on optical properties of small high-precision plastic injection molded parts
Creators: name: Shotwell, Demitri
name: Lin, Mong-Tung
name: Liu, Jia-Hau
name: Turng, Lih-Sheng
Publisher: name: Taylor & Francis
Year: 2023
Subjects: subject: Biophysics
subject: Space Science
subject: Medicine
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Adding reservoirs as extensions to a multi-cavity runner-system to regulate cavity fill-rate within small, high-precision optical parts during filling and fill-to-pack switch-over (F/P) was studied with the aid of simulations. This work aimed for a constant melt-front velocity inside the cavities with varying geometries. Three methods of reservoir designs were considered: first, using engineering intuition, second and third, using mass balance and mass and momentum balance equations, respectively. Eight reservoirs were designed and compared to two no-reservoir cases. For each case, 27 runs covering three levels of fill-rate, F/P, and packing pressure were simulated, resulting in 270 simulation runs. The quality variables of flow and thermally induced retardation and the average and standard deviation of volumetric shrinkage were considered and for each parameter, the minimum, best cases, occurred with a reservoir case. Thus, this study offers a proof-of-concept design for using reservoirs to improve molding of small, high-precision optical parts.
title: Ð¡Ð¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐµÐ½Ð¾Ð²Ð¾Ð¹ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÐÐÐ Â«Ð¢Ð¾ÑÐ³Ð¾Ð²ÑÐ¹ Ð´Ð¾Ð¼ Â«ÐÐ³ÑÐ¾ÐÑÐ¾Ð¼Ð¡Ð½Ð°Ð±Â»
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°ÑÐ°Ñ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: 2017
Subjects: Ð¾Ð±ÑÐµÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð·Ð½Ð°ÑÐµÐ½Ð¸Ðµ ÑÐµÐ½
ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±ÑÐ»ÑÐ¶Ð¸Ð²Ð°Ð½Ð¸Ðµ
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐµ Ð¿Ð¾ÑÐ¾ÐºÐ¸
ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ ÑÐ¾Ð²Ð°ÑÐ½Ð¾Ð¹ Ð¼Ð°ÑÑÑ
Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾-ÑÐ±ÑÑÐ¾Ð²Ð°Ñ ÑÑÑÑÐºÑÑÑÐ°

description: ÐÐ±ÑÐµÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð·Ð½Ð°ÑÐµÐ½Ð¸Ðµ ÑÐµÐ½ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÐµÑÑÑ ÑÐµÐ¼, ÑÑÐ¾ Ð¾Ð½Ð¸ Ð¾ÐºÐ°Ð·ÑÐ²Ð°ÑÑ ÑÐµÑÐ°ÑÑÐµÐµ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ðµ Ð½Ð° ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°, Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ðµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»ÑÐ½ÑÑ Ð¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÑ Ð¿Ð¾ÑÐ¾ÐºÐ¾Ð², ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ ÑÐ¾Ð²Ð°ÑÐ½Ð¾Ð¹ Ð¼Ð°ÑÑÑ, ÑÑÐ¾Ð²ÐµÐ½Ñ Ð±Ð»Ð°Ð³Ð¾ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð¸Ñ. ÐÑÐ¾Ð¼Ðµ ÑÐ¾Ð³Ð¾, ÑÐµÑÐµÐ· ÑÐµÐ½Ñ ÑÐµÐ°Ð»Ð¸Ð·ÑÑÑÑÑ ÐºÐ¾Ð½ÐµÑÐ½ÑÐµ ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¸Ðµ ÑÐµÐ»Ð¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÐµÑÑÑ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ ÑÐ°Ð±Ð¾ÑÑ Ð²ÑÐµÑ Ð·Ð²ÐµÐ½ÑÐµÐ² ÐµÐ³Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾-ÑÐ±ÑÑÐ¾Ð²Ð¾Ð¹ ÑÑÑÑÐºÑÑÑÑ. Ð¦ÐµÐ½Ð° - Ð³Ð¸Ð±ÐºÐ¸Ð¹ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¸ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸. ÐÑÐ»Ð¸ Ð½Ð° ÑÐµÐ±ÐµÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÑ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ðµ Ð¼Ð¾Ð¶ÐµÑ Ð²Ð»Ð¸ÑÑÑ Ð»Ð¸ÑÑ Ð² Ð¾ÑÐµÐ½Ñ Ð½ÐµÐ±Ð¾Ð»ÑÑÐ¸Ñ Ð¿ÑÐµÐ´ÐµÐ»Ð°Ñ, Ð¿Ð¾ÑÐºÐ¾Ð»ÑÐºÑ ÐµÑ Ð³Ð¸Ð±ÐºÐ¾ÑÑÑ Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð°, ÐºÐ°Ðº Ð¿ÑÐ°Ð²Ð¸Ð»Ð¾, ÑÑÐ¾Ð²Ð½ÐµÐ¼ ÑÐµÐ½ Ð½Ð° ÑÑÑÑÐµ, Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ, Ð¿Ð¾Ð»ÑÑÐ°Ð±ÑÐ¸ÐºÐ°ÑÑ Ð¸ ÑÐ°Ð±Ð¾ÑÑÑ ÑÐ¸Ð»Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð²Ð½ÑÑÑÐµÐ½Ð½Ð¸Ð¼Ð¸ ÑÐµÐ·ÐµÑÐ²Ð°Ð¼Ð¸ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð° Ð¿Ð¾ ÑÐ½Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾ÐµÐ¼ÐºÐ¾ÑÑÐ¸ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸, ÑÐ¾ ÑÐµÐ½Ñ Ð½Ð° ÑÐ²Ð¾Ñ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ðµ Ð¼Ð¾Ð¶ÐµÑ ÑÑÑÐ°Ð½Ð°Ð²Ð»Ð¸Ð²Ð°ÑÑ Ð² Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸ Ð½ÐµÐ¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð½ÑÑ Ð¿ÑÐµÐ´ÐµÐ»Ð°Ñ.
Austinograea Hessler & Martin 1989
Creators: name: Guinot, Danièle
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Bythograeidae
Austinograea

description: Genus Austinograea Hessler & Martin, 1989
TYPE SPECIES. — Austinograea williamsi Hessler & Martin, 1989, by original designation and monotypy.
REMARKS
The genus Austinograea currently consists of four species in the western Pacific: 1) A. williamsi Hessler & Martin, 1989, which seems to be confined to the northwestern Pacific, in the Mariana Back-Arc Basin (just west of the Mariana Island Arc) and found in abundance in snail beds filling the vent openings of the Mariana Trough; 2) A. alayseae, originally collected from the Lau Back-Arc Basin, subsequently found distributed across hydrothermal vent areas in the Southwest Pacific Ocean, e.g. along the Eastern Lau Spreading Center and also reported from the North Fiji Basin, Tonga Arc and Manus Basin (see below); 3) A. hourdezi, a widespread species encountered in the southwestern Pacific from numerous vent fields of the Lau and North Fiji Back-Arc Basins, now identified in the Woodlark Basin (see still from the video 190527174907236_15_1080 of La Scala vent Site) (Fig. 8A) and which cohabits with A. alayseae at a number of sites (see below); and 4) and the rare and enigmatic A. jolliveti from the southwestern Pacific, collected so far only from one site in the Lau Basin (ABE Site) and one site in the North Fiji Basin (Mussel Valley Site). Another species, A. rodriguezensis Tsuchida & Hashimoto, 2002, is located well apart, in the western Indian Ocean. The new Austinograea found in the Woodlarlk and Manus Basins described here would be the sixth species of the genus.
description: Published as part of Guinot, Danièle, 2025, Austinograea chubacarc n. sp. from the Manus and Woodlark Basins (western Pacific), and new records of A. alayseae Guinot, 1990 and A. hourdezi Guinot & Segonzac, 2018 (Crustacea, Decapoda, Brachyura, Bythograeidae), pp. 167-184 in Zoosystema 47 (12) on page 171, DOI: 10.5252/zoosystema2025v47a12, http://zenodo.org/record/15229985
title: Ð¢ÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð°ÑÐ¿ÐµÐºÑÑ Ð¼Ð¾Ð½Ð¸ÑÐ¾ÑÐ¸Ð½Ð³Ð° ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð²
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐµÐ½Ð³ÐµÑÐ¾Ð²Ð°, ÐÐ°ÑÐ°Ð»ÑÑ
name: ÐÐ¸ÑÐºÑÐ½, ÐÐ»ÐµÐ³
name: ÐÑÐ´Ð°ÑÐ¾Ð²Ð°, ÐÑÐ´Ð¼Ð¸Ð»Ð°
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2018
Subjects: ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ°Ñ ÐºÑÐ»ÑÑÑÑÐ°
ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ðµ Ð²Ð¾ÑÐ¿Ð¸ÑÐ°Ð½Ð¸Ðµ
ÑÑÑÐ´ÐµÐ½ÑÑ

description: Ð¡Ð¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ðµ ÑÑÐµÐ±Ð½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸ÑÐ¼ ÑÐµÐ´ÐµÑÐ°Ð»ÑÐ½ÑÑ
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Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ Â«Ð¤Ð¸Ð·Ð¸ÑÐµÑÐºÐ°Ñ ÐºÑÐ»ÑÑÑÑÐ°Â»: ÑÐ°Ð¼Ð¾ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð²,
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ÐÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð» Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð¿Ð¾Ð¼Ð¾Ð¶ÐµÑ Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»ÑÐ¼ ÐºÐ°ÑÐµÐ´Ñ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð¹ ÐºÑÐ»ÑÑÑÑÑ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ Ð¿Ð¾Ð²ÐµÑÑÐ¸ Ð¼Ð¾Ð½Ð¸ÑÐ¾ÑÐ¸Ð½Ð³ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¸ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÑÑÐµÐ¹ ÑÐºÐ¾Ð»Ñ.
Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½Ð¾ Ð½Ð° ÑÐ¸ÑÐ¾ÐºÐ¸Ð¹ ÐºÑÑÐ³ ÑÐ¸ÑÐ°ÑÐµÐ»ÐµÐ¹ â Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»ÐµÐ¹ ÐºÐ°ÑÐµÐ´Ñ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð¹ ÐºÑÐ»ÑÑÑÑÑ Ð²ÑÑÑÐµÐ¹ ÑÐºÐ¾Ð»Ñ, ÑÑÐ¸ÑÐµÐ»ÐµÐ¹ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð¹ ÐºÑÐ»ÑÑÑÑÑ ÑÑÐµÐ´Ð½ÐµÐ¹ Ð¾Ð±ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐºÐ¾Ð»Ñ, ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð².
Additional file 3 of Cis-acting super-enhancer lncRNAs as biomarkers to early-stage breast cancer
Creators: name: Ropri, Ali S.
name: DeVaux, Rebecca S.
name: Eng, Jonah
name: Chittur, Sridar V.
name: Herschkowitz, Jason I.
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 3: Figure S3: Specificity of H3K27ac ChIP antibody. Fold enrichment of the H3K27ac antibody between control promoter region of Myt1 and enhancer region of MYC.
Investigating various possibilities to solve the Fermi-Hubbard model using the kinetic energy part for quantum annealing
Creators: name: Vyas, Kunal
name: Jin, Fengping
name: Michielsen, Kristel
Publisher: name: Forschungzentrum Jülich
Year: 2023

description: Nonequilibrium Physics – Current Trends and Future Perspectives, Bad Honnef, Germany, 28 Aug 2023 - 1 Sep 2023
description: Quantum annealing can help in finding the ground state of Hamiltonians describing many body systems. One such Hamiltonian is the Fermi-Hubbard Hamiltonian. We investigate the possibility of utilizing quantum phase estimation after the quantum annealing process carried out using the kinetic energy part of the Hubbard model as driving Hamiltonian for ground state calculations. We also try to exploit some symmetries in order to reduce size of the Hilbert space and study minimum gap for the same. We further outline our plan to study quantum annealing for a system described by the Hubbard Hamiltonian and coupled to a bath to investigate the effect of the environmental temperature and disorder on the ideal quantum annealing process for finding the ground state.
Extending the eigCG algorithm to non-symmetric linear systems with multiple right-hand sides
Creators: name: Abdel-Rehim, Abdou
name: Orginos, Kostas
name: Stathopoulos, Andreas
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: For Hermitian positive definite linear systems and eigenvalue problems, the eigCG algorithm is a memory efficient algorithm that solves the linear system and simultaneously computes some of its eigenvalues. The algorithm is based on the Conjugate-Gradient (CG) algorithm, however, it uses only a window of the vectors generated by the CG algorithm to compute approximate eigenvalues. The number and accuracy of the eigenvectors can be increased by solving more right-hand sides. For Hermitian systems with multiple right-hand sides, the computed eigenvectors can be used to speed up the solution of subsequent systems. The algorithm was tested on Lattice QCD problems by solving the normal equations and was shown to give large speed up factors and to remove the critical slowing down as we approach light quark masses. Here, an extension to the non-symmetric case based on the two-sided Lanczos algorithm is given. The new algorithm is tested on Lattice QCD problems and is shown to give promising results. We also study the removal of the critical slowing down and compare results with those of the eigCG algorithm. We also discuss the case when the system is gamma5-Hermitian.
description: 8 pages, 3 figures, presented at the XXVII International Symposium on Lattice Field Theory, July 26-31, 2009, Peking University, Beijing, China
Austinograea hourdezi Guinot & Segonzac 2018
Creators: name: Guinot, Danièle
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Bythograeidae
Austinograea
Austinograea hourdezi

description: Austinograea hourdezi Guinot & Segonzac, 2018
Austinograea hourdezi Guinot & Segonzac, 2018: 880, figs 3A; 4A-E; 5A-H; 6A-E; 7A-H. — Lee et al. 2019a: fig. 1B, D. — Chabert 2021: table 2.
MATERIAL EXAMINED. — 3 ♀ 28.0 × 44.1 mm, 28.6 × 44.6 mm, 25.0 × 38.6 mm; Lau Basin, Tow Cam; PL730 – Panier; 20°19.080’S, 176°8.264’W; 2710 m; 26.IV.2019; CHUBACARC 2019 cruise; Hourdez det. Austinograea; MNHN-IU-2024-6023.
REMARKS
The Tow Cam Site in the Lau Basin is the type locality of Austinograea hourdezi, a widespread species in the southwestern Pacific, found in numerous vent fields of the Lau and North Fiji Back-Arc Basins (Guinot & Segonzac 2018: 80).
In a still from the video 190527174907236_15_1080 https://video.ifremer.fr/index) of the La Scala vent Field, PL738 (Fig. 8A), A. hourdezi is easily recognised by the thick patch of setae on the inner surface of the chelipedal palm: its presence is confimed in the Woodlark Basin at the La Scala vent Field, where it coexists with A. chubacarc n. sp.
Chabert (2021: table 2), using a barcode approach with the cytochrome c oxidase subunit I (COI) gene, identified Austinograea aff. hourdezi in the Woodlark Basin, and A. hourdezi in the North Fiji. In addition, she identified A. aff. williamsi in the Manus and Lau Basins, but we cannot determine which species they correspond to. S. Hourdez plans to carry out the correspondence between these genetic results and the different bythograeid species, after the publication of this paper (pers. comm.).
We did not identify A. williamsi among the bythograeids collected during the CHUBACARC 2019 cruise, and so far the species appears to be endemic to the Mariana Trough, a back-arc basin in the northwest Pacific (Fig. 1) (Kojima & Watanabe 2015).
Lee et al. (2019a), who determined the COI sequence of Austinograea hourdezi from three hydrothermal vent regions in the North Fiji Basin, found that all were identical. Lee et al. (2019b: 10, tables 3, 4, S1 table) obtained sequences of two mitochondrial genes (COI and 16S rDNA) of the species.
description: Published as part of Guinot, Danièle, 2025, Austinograea chubacarc n. sp. from the Manus and Woodlark Basins (western Pacific), and new records of A. alayseae Guinot, 1990 and A. hourdezi Guinot & Segonzac, 2018 (Crustacea, Decapoda, Brachyura, Bythograeidae), pp. 167-184 in Zoosystema 47 (12) on page 179, DOI: 10.5252/zoosystema2025v47a12, http://zenodo.org/record/15229985
Cartoline dal pianeta Saturno
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2016

Nella foto vediamo la famosa tempesta esagonale che viene studiata dal 2009. L'esagono è completamente illuminato dalla luce del Sole. Il prossimo 15 settembre la missione si concluderà con uno spettacolare e definitivo tuffo della sonda nell'atmosfera del sesto pianeta
title: Ð¢ÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð¸Ð·Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ Ð´ÐµÑÐ°Ð»Ð¸ Â«ÐÑÑÐ»ÐºÐ°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ÐµÑÐ°ÑÐ¸Ð¼Ð¾Ð², Ð Ð¾Ð¼Ð°Ð½
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ
ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ
ÑÐ¸Ð¿ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°
ÑÐµÑÐ¾Ñ Ð¾Ð²Ð°ÑÐ¾ÑÑÑ Ð¿Ð¾Ð²ÐµÑÑ Ð½Ð¾ÑÑÐ¸

description: Ð¢ÐµÐ¼Ð° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ - Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¸Ð·Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ Ð²ÑÑÐ»ÐºÐ¸, Ð´Ð»Ñ ÐºÐ¾ÑÐ¾ÑÐ¾Ð¹ Ð±ÑÐ»Ð¸ ÑÐ¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ñ Ð·Ð°Ð³Ð¾ÑÐ¾Ð²ÐºÐ°, ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¸ Ð¸ Ð¿ÐµÑÐµÑÐ¾Ð´Ñ, Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ñ ÑÐµÐ¶Ð¸Ð¼Ñ ÑÐµÐ·Ð°Ð½Ð¸Ñ Ð¸ Ð¿Ð¾ÑÑÐ¸ÑÐ°Ð½Ñ Ð½Ð°Ð»Ð°Ð´Ð¾ÑÐ½ÑÐµ ÑÐ°Ð·Ð¼ÐµÑÑ.
A Study of the Accuracy of Mass-Radius Relationships for Silicate-Rich and Ice-Rich Planets up to 100 Earth Masses
Creators: name: Grasset, O.
name: Schneider, J.
name: Sotin, C.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: A mass-radius relationship is proposed for solid planets and solid cores ranging from 1 to 100 Earth-mass planets. It relies on the assumption that solid spheres are composed of iron and silicates, around which a variable amount of water is added. The M-R law has been set up assuming that the planetary composition is similar to the averaged composition for silicates and iron obtained from the major elements ratio of 94 stars hosting exoplanets. Except on Earth for which a tremendous amount of data is available, the composition of silicate mantles and metallic cores cannot be constrained. Similarly, thermal profiles are poorly known. In this work, the effect of compositional parameters and thermal profiles on radii estimates is quantified. It will be demonstrated that uncertainties related to composition and temperature are of second order compared to the effect of the water amount. The Super-Earths family includes four classes of planets: iron-rich, silicate-rich, water-rich, or with a thick atmosphere. For a given mass, the planetary radius increases significantly from the ironrich to the atmospheric-rich planet. Even if some overlaps are likely, M-R measurements could be accurate enough to ascertain the discovery of an earth-like planet .The present work describes how the amount of water can be assessed from M-R measurements. Such an estimate depends on several assumptions including i) the accuracy of the internal structure model and ii) the accuracy of mass and radius measurements. It is shown that if the mass and the radius are perfectly known, the standard deviation on the amount of water is about 4.5 %. This value increases rapidly with the radius uncertainty but does not strongly depend on the mass uncertainty.
description: In press in The Astrophysical Journal
De-Rotation of the Cosmic Microwave Background Polarization: Full-Sky Formalism
Creators: name: Gluscevic, Vera
name: Kamionkowski, Marc
name: Cooray, Asantha
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Mechanisms have been proposed that might rotate the linear polarization of the cosmic microwave background (CMB) as it propagates from the surface of last scatter. In the simplest scenario, the rotation will be uniform across the sky, but the rotation angle may also vary across the sky. We develop in detail the complete set of full-sky quadratic estimators for the rotation of the CMB polarization that can be constructed from the CMB temperature and polarization. We derive the variance with which these estimators can be measured and show that these variances reduce to the simpler flat-sky expressions in the appropriate limit. We evaluate the variances numerically. While the flat-sky formalism may be suitable if the rotation angle arises as a realization of a random field, the full-sky formalism will be required to search for rotations that vary slowly across the sky as well as for models in which the angular power spectrum for the rotation angle peaks at large angles.
description: 13 pages, 7 figures; minor changes, added references and Appendix D; accepted for publication in PRD
Nuova tecnica di analisi per l’antimateria
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2016

L’accuratezza dei dati raccolti dall’esperimento AMS, a bordo della Stazione Spaziale Internazionale, ha permesso di rivelare con precisione la quantità di antimateria presente nei raggi cosmici. Un team di ricercatori ha messo a punto una nuova tecnica di analisi, grazie alla quale è possibile sviluppare previsioni dettagliate per il fondo astrofisico di antiprotoni e positroni
Limits of the seismogenic zone in the epicentral region of the 26 December 2004 great Sumatra-Andaman earthquake: Results from seismic refraction and wide-angle reflection surveys and thermal modeling
Creators: name: Klingelhoefer, Frauke
name: Gutscher, Marc-André
name: Ladage, S.
name: Dessa, J. -X.
name: Graindorge, David
name: Franke, D.
name: André, C.
name: Permana, Haryadi
name: Yudistira, T.
name: Chauhan, Ajay
Publisher: name: arXiv
Year: 2010
Subjects: subject: Geophysics (physics.geo-ph)
subject: FOS: Physical sciences

description: The 26 December 2004 Sumatra earthquake (Mw = 9.1) initiated around 30 km depth and ruptured 1300 km of the Indo-Australian Sunda plate boundary. During the Sumatra OBS (ocean bottom seismometer) survey, a wide angle seismic profile was acquired across the epicentral region. A seismic velocity model was obtained from combined travel time tomography and forward modeling. Together with reflection seismic data from the SeaCause II cruise, the deep structure of the source region of the great earthquake is revealed. Four to five kilometers of sediments overlie the oceanic crust at the trench, and the subducting slab can be imaged down to a depth of 35 km. We find a crystalline backstop 120 km from the trench axis, below the fore arc basin. A high velocity zone at the lower landward limit of the raycovered domain, at 22 km depth, marks a shallow continental Moho, 170 km from the trench. The deep structure obtained from the seismic data was used to construct a thermal model of the fore arc in order to predict the limits of the seismogenic zone along the plate boundary fault. Assuming 100C-150C as its updip limit, the seismogenic zone is predicted to begin 530 km from the trench. The downdip limit of the 2004 rupture as inferred from aftershocks is within the 350C 450C temperature range, but this limit is 210-250 km from the trench axis and is much deeper than the fore arc Moho. The deeper part of the rupture occurred along the contact between the mantle wedge and the downgoing plate.
title: Ð¦Ð¸ÑÑÐ¾Ð²ÑÐµ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÐºÐ°Ð´ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐµÐ·ÐµÑÐ²Ð° Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð¹ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ IT-ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸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¤Ð¸Ð»Ð¸Ð¿Ð¿Ð¾Ð²Ð°, 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ÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¸ÑÑÐ¾Ð²ÑÐµ
ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸
Ð´Ð¸ÑÑÐ°Ð½ÑÐ¸Ð¾Ð½Ð½Ð¾Ðµ Ð¾Ð±ÑÑÐµÐ½Ð¸Ðµ
ÐºÐ°Ð´ÑÐ¾Ð²ÑÐ¹ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½Ñ
ÐºÐ°Ð´ÑÐ¾Ð²ÑÐ¹ ÑÐµÐ·ÐµÑÐ²
Ð°ÑÑÑÐ¾ÑÑÐ¸Ð½Ð³
Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¹ Ð±Ð¸Ð·Ð½ÐµÑ

description: ÐÐ±ÑÐµÐºÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ - Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð°Ñ IT-ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ñ Luxoft Holding, Inc. ÐÑÐµÐ´Ð¼ÐµÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ â ÐºÐ°Ð´ÑÐ¾Ð²Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Luxoft Holding, Inc. Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ â ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°ÑÑ ÑÐ¸ÑÑÐµÐ¼Ñ Ð´Ð¸ÑÑÐ°Ð½ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ Ð½Ð° Ð±Ð°Ð·Ðµ ÑÐ¸ÑÑÐ¾Ð²ÑÑ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ Ð²Ð¸Ð´Ð¾Ð² Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÑ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Luxoft Holding, Inc. ÐÑÑÐ²Ð»ÐµÐ½Ñ ÑÑÐµÐ½Ð´Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ IT-ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð² Ð¾ÑÑÐ°ÑÐ»ÑÑ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸. ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐµÑÑÑ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¼Ð¾Ð´ÐµÐ»Ð¸ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÐ¼Ð¾Ð¹ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸. ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½ ÐºÐ°Ð´ÑÐ¾Ð²ÑÐ¹ ÑÐ¾ÑÑÐ°Ð² Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ ÐºÐ°Ð´ÑÐ¾Ð²Ð°Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ° Ð² Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ð¸ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÐºÐ°Ð´ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐµÐ·ÐµÑÐ²Ð°. ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð° Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÑ Ð´Ð¸Ð´Ð¶Ð¸ÑÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÐºÐ¾Ð². ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐµ, Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ñ Ðº ÑÐ¸ÑÑÐµÐ¼Ðµ Ð´Ð¸ÑÑÐ°Ð½ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ Ð½Ð° Ð±Ð°Ð·Ðµ ÑÐ¸ÑÑÐ¾Ð²ÑÑ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹. ÐÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½ Ð¿ÑÐ¾ÐµÐºÑ Ð¿Ð¾ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ Ð² ÐºÐ°Ð´ÑÐ¾Ð²ÑÑ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸.
ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ° Ð¿Ð¾ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð´Ð¸ÑÑÐ°Ð½ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ Ð² ÑÑÐµÑ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÑÑÐµÐ½Ð°ÑÐ¸ÑÑ Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ ÑÑÐ½Ð¾ÑÐ½Ð¾Ð¹ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¸. Ð ÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÐ¾ÐµÐºÑÐ° Ð¿Ð¾ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ Ð´Ð¸ÑÑÐ°Ð½ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ Ð½Ð° Ð±Ð°Ð·Ðµ ÑÐ¸ÑÑÐ¾Ð²ÑÑ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÑ Ðº ÑÐ¾ÑÑÑ Ð¿ÑÐ¸Ð±ÑÐ»Ð¸ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Luxoft Holding, Inc.
Additional file 1: of Post-surgical outcomes of patients with chronic kidney disease and end stage renal disease undergoing radical prostatectomy: 10-year results from the US National Inpatient Sample
Creators: name: Ning, Chen
name: Hu, Xinyi
name: Liu, Fangming
name: Lin, Jun
name: Zhang, Jian
name: Wang, Zhipeng
name: Zhu, Yichen
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: Mathematical Sciences not elsewhere classified
subject: Marine Biology
subject: Computational Biology

description: Table S1. Multivariate models of clinical outcomes by extent of kidney disease, demographic characteristics, hospital characteristics, and comorbidities (DOCX 23 kb)
Period-Luminosity Relations Derived from the OGLE-III Fundamental Mode Cepheids
Creators: name: Ngeow, C.
name: Kanbur, S.
name: Neilson, H.
name: Nanthakumar, A.
name: Buonaccorsi, J.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In this Paper, we have derived Cepheid period-luminosity (P-L) relations for the Large Magellanic Cloud (LMC) fundamental mode Cepheids, based on the data released from OGLE-III. We have applied an extinction map to correct for the extinction of these Cepheids. In addition to the VIW band P-L relations, we also include JHK and four Spitzer IRAC band P-L relations, derived by matching the OGLE-III Cepheids to the 2MASS and SAGE datasets, respectively. We also test the non-linearity of the Cepheid P-L relations based on extinction-corrected data. Our results (again) show that the LMC P-L relations are non-linear in VIJH bands and linear in KW and the four IRAC bands, respectively.
description: 6 pages, 3 figures and 3 tables, ApJ accepted
Un megamaser per Hubble
Creators: Giuseppina Pulcrano
Publisher: name: Media Inaf
Year: 2016

Il telescopio spaziale di ESA e NASA immortala IRAS 16399-0937, una galassia al cui interno si trova una potentissima sorgente che emette fasci collimati di microonde anziché luce visibile, anche oltre 100 milioni di volte più intensi di quelli prodotti nella nostra galassia, la Via Lattea
A comparative study of iodine metabolism in juvenile Oncorhynchus
Creators: name: Eales, John Geoffrey
Publisher: name: University of British Columbia
Year: 2011

description: Comparative histological and radiochemical studies of iodine metabolism in juvenile Oncorhynchus revealed good agreement between thyroid epithelial height and ability to convert I¹³¹ into protein-bound I¹³¹(PBI¹³¹). The ratio of I¹³¹ to PBl¹³¹ in plasma samples (Conversion Ratio) was considered superior to other thyroid assays reviewed. Peaks in thyroid activity and loss of I¹³¹ from the body occurred in sockeye and coho at the time of downstream migration, but in chum and pink only when postmigrants were retained in fresh water. In coho and sockeye these changes were transitory, in chum irreversible and in pink prolonged. On the above basis, thyroxine was assigned no specific role but a theory of smolt evolution was proposed and related to a phylogeny within the genus Oncorhynchus.
Bagliori d’aurora nel buio del solstizio
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2016

L’aurora boreale del 22 dicembre 2016 vista dall’alto dallo strumento VIIRS di Suomi NPP, un satellite della Noaa statunitense in orbita polare a oltre 830 km di altitudine. Le luci diffuse sono le emissioni generate dall’impatto con l’alta atmosfera di particelle energetiche provenienti dal Sole
title: ÐÐ±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ð¸ ÑÐ¾Ð¿Ð»Ð¸Ð²Ð° Ð´Ð»Ñ Ð¼Ð½Ð¾Ð³Ð¾ÑÑÑÐ¿ÐµÐ½ÑÐ°ÑÑÑ Ð±Ð°Ð»Ð»Ð¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ°ÐºÐµÑ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÐ³Ð¾Ð½ÑÐºÐ¾Ð²Ð°, ÐÐ°ÑÐ°Ð»ÑÑ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: ÑÐ¾Ð¿Ð»Ð¸Ð²Ð¾
ÑÐ¸ÑÑÐµÐ¼Ñ Ð¿Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸
ÑÐ°ÐºÐµÑÐ°-Ð½Ð¾ÑÐ¸ÑÐµÐ»Ñ
fuel
security system
booster

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÑÑÑÑ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ñ Ð¸ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° Ð´Ð»Ñ ÑÑÐ°Ð½ÐµÐ½Ð¸Ñ Ð¸ Ð·Ð°Ð¿ÑÐ°Ð²ÐºÐ¸ ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÐ¾Ð² ÑÐ¾Ð¿Ð»Ð¸Ð²Ð°. Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ - Ð¸Ð·ÑÑÐ¸ÑÑ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¿Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ð¸ ÑÐ¾Ð¿Ð»Ð¸Ð²Ð°, ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ¸ÑÐ¾Ð²ÐºÐ¸, ÑÑÐ°Ð½ÐµÐ½Ð¸Ñ Ð¸ Ð·Ð°Ð¿ÑÐ°Ð²ÐºÐ¸ ÑÐ¾Ð¿Ð»Ð¸Ð²Ð°, Ð¿ÑÐ¾ÑÐµÑÑÑ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ ÑÐ¾Ð¿Ð»Ð¸Ð²Ð°, ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð°, Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÐ¼ÑÐµ Ð½Ð° ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÑÑÐ°Ð´Ð¸ÑÑ Ð¿ÑÐ¸ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐµ ÑÐ°ÐºÐµÑÐ° - Ð½Ð¾ÑÐ¸ÑÐµÐ»Ñ Ðº Ð¿ÑÑÐºÑ.
description: Object of research are constructions and technical devices for storage and refuel of components .The work purpose - to study systems on safety when using fuel, the technological features of transportation, storage and refuel of components, processes of preparation of fuel, devices used at various stages by preparation the rocket - the carrier to start-up.
Stop ai test del JWST
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2016

Il 3 dicembre scorso, durante una fase di test alla struttura di specchi e strumenti scientifici del James Webb Space Telescope, i tecnici della NASA hanno registrato segnali anomali, interrompendo le simulazioni. L’analisi dei dati raccolti mostra comunque che il telescopio gode di ottima salute
title: Standing Committee on the Law of Trademarks, Industrial Designs and Geographical Indications :
title: Report adopted by the Standing Committee.
titleType: Subtitle
Creators: name: (:Unas)
Publisher: name: Unknown
Year: 0

description: The Standing Committee on the Law of Trademarks, Industrial Designs and Geographical Indications (hereinafter referred to as “the Standing Committee” or “the SCT”) held its ninth session, in Geneva, from November 11 to 15, 2002.
title: ÐÑÐ¾ÐµÐºÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¿Ð¾Ð´Ð´ÐµÑÐ¶ÐºÐ¸ Ð¿ÑÐ¸Ð½ÑÑÐ¸Ñ ÑÐµÑÐµÐ½Ð¸Ð¹ Ð¿Ð¾ Ð»Ð¸ÐºÐ²Ð¸Ð´Ð°ÑÐ¸Ð¸ Ð°Ð²Ð°ÑÐ¸Ð¹ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ Ð¢Ð¾ÑÐ¶Ð¾ÐºÑÐºÐ¾Ðµ ÐÐÐ£ÐÐ ÐÐÐ Â«ÐÐ°Ð·Ð¿ÑÐ¾Ð¼ ÑÑÐ°Ð½ÑÐ³Ð°Ð· Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Â»
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÑÐ¶ÐºÐ¾Ð²Ð°, ÐÐ»ÐµÐ½Ð°
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: Ð³Ð°Ð·Ð¾Ð²Ð°Ñ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾ÑÑÑ
Ð¼Ð°Ð³Ð¸ÑÑÑÐ°Ð»ÑÐ½ÑÐµ Ð³Ð°Ð·Ð¾Ð¿ÑÐ¾Ð²Ð¾Ð´Ñ
Ð»Ð¸ÐºÐ²Ð¸Ð´Ð°ÑÐ¸Ñ Ð°Ð²Ð°ÑÐ¸Ð¹
Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ðµ ÑÐ½ÐµÑÐ³Ð¾ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸
ÑÐ¸ÑÑÐµÐ¼Ð° Ð¿Ð¾Ð´Ð´ÐµÑÐ¶ÐºÐ¸ Ð¿ÑÐ¸Ð½ÑÑÐ¸Ñ ÑÐµÑÐµÐ½Ð¸Ð¹
wonderware intouch
gas industry
accidents elimination
decision support system

description: Ð ÑÐ¾Ð´Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ»Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÐºÐ¾Ð½ÑÐµÐ¿ÑÐ¸Ñ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¿Ð¾ Ð¿Ð¾Ð´Ð´ÐµÑÐ¶ÐºÐµ Ð¿ÑÐ¸Ð½ÑÑÐ¸Ñ ÑÐµÑÐµÐ½Ð¸Ð¹ Ð¿Ð¾ Ð»Ð¸ÐºÐ²Ð¸Ð´Ð°ÑÐ¸Ð¸ Ð°Ð²Ð°ÑÐ¸Ð¹ Ð½Ð° Ð»Ð¸Ð½ÐµÐ¹Ð½Ð¾Ð¼ ÑÑÐ°ÑÑÐºÐµ Ð¼Ð°Ð³Ð¸ÑÑÑÐ°Ð»ÑÐ½ÑÑ Ð³Ð°Ð·Ð¾Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¾Ð². ÐÑÑÐ²Ð»ÐµÐ½Ð° Ð¾ÑÐ½Ð¾Ð²Ð½Ð°Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ð°, ÑÐ²ÑÐ·Ð°Ð½Ð½Ð°Ñ Ñ Ð½ÐµÑÑÑÐµÐºÑÐ¸Ð²Ð½ÑÐ¼ Ð¿ÑÐ¸Ð½ÑÑÐ¸ÐµÐ¼ ÑÐµÑÐµÐ½Ð¸Ð¹ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÑÑÑÑÐºÑÑÑÐ° ÑÐ¸ÑÑÐµÐ¼Ñ Ð¿Ð¾Ð´Ð´ÐµÑÐ¶ÐºÐ¸ Ð¿ÑÐ¸Ð½ÑÑÐ¸Ñ ÑÐµÑÐµÐ½Ð¸Ð¹ Ð¸ ÐµÐµ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐµ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸. ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½ Ð±ÑÐ´Ð¶ÐµÑ Ð¿ÑÐ¾ÐµÐºÑÐ°, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð¿Ð»Ð°Ð½-Ð³ÑÐ°ÑÐ¸Ðº ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¾ÐµÐºÑÐ° Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ Microsoft Project.
Ecco come dimagrisce l’Universo
Creators: Corrado Ruscica
Publisher: name: Media Inaf
Year: 2016

La percentuale di materia oscura potrebbe essere oggi inferiore del 5 percento rispetto a quella che era presente nell’universo primordiale. È quanto emerge da uno studio recente, pubblicato su Physical Review D, che tenta di spiegare la discrepanza di alcuni parametri cosmologici nell’ambito di un modello che si basa sull’ipotesi del decadimento della materia oscura
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÑÑÐºÑÑÑÑ Ð¸ ÑÐ²Ð¾Ð¹ÑÑÐ² Ð½Ð°Ð½Ð¾ÑÐ°ÑÑÐ¸Ñ ÑÐ¸Ð½ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð³Ð¸Ð´ÑÐ¾ÐºÑÐ¸Ð°Ð¿Ð°ÑÐ¸ÑÐ°
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÐ»Ð¸Ð½Ð¾Ð²Ð°, ÐÐ¾Ð»Ð¸Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð½Ð°Ð½Ð¾ÑÐ°ÑÑÐ¸ÑÑ Ð³Ð¸Ð´ÑÐ¾ÐºÑÐ¸Ð°Ð¿Ð°ÑÐ¸ÑÐ°
ÑÐ¸ÑÐ¾ÑÐ¾ÐºÑÐ¸ÑÐ½Ð¾ÑÑÑ
Ð¼ÐµÐ·ÐµÐ½Ñ Ð¸Ð¼Ð½ÑÐµ ÑÑÐ²Ð¾Ð»Ð¾Ð²ÑÐµ ÐºÐ»ÐµÑÐºÐ¸
Ñ Ð¸ÑÐ¾Ð·Ð°Ð½

description: Ð¢ÑÐµÑÐ¼ÐµÑÐ½ÑÐµ Ð¿Ð¾ÑÐ¸ÑÑÑÐµ ÐºÐ¾Ð¼Ð¿Ð¾Ð·Ð¸ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¼Ð°ÑÑÐ¸ÑÑ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐ¸ÑÐ¾Ð·Ð°Ð½Ð° Ð¸ Ð½Ð°Ð½Ð¾ÑÐ°ÑÑÐ¸Ñ Ð³Ð¸Ð´ÑÐ¾ÐºÑÐ¸Ð°Ð¿Ð°ÑÐ¸ÑÐ° Ð±ÑÐ»Ð¸ Ð¿Ð¾Ð»ÑÑÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð¼ Ð»Ð¸Ð¾ÑÐ¸Ð»ÑÐ½Ð¾Ð¹ ÑÑÑÐºÐ¸. Ð£ÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ð¾, ÑÑÐ¾ ÑÐ»ÑÑÑÐ°Ð·Ð²ÑÐºÐ¾Ð²Ð¾Ðµ Ð´Ð¸ÑÐ¿ÐµÑÐ³Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¿Ð¾ÑÐ¾Ð±ÑÑÐ²ÑÐµÑ ÑÐ°Ð²Ð½Ð¾Ð¼ÐµÑÐ½Ð¾Ð¼Ñ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð½Ð°Ð½Ð¾ÑÐ°ÑÑÐ¸Ñ Ð³Ð¸Ð´ÑÐ¾ÐºÑÐ¸Ð°Ð¿Ð°ÑÐ¸ÑÐ° Ð¿Ð¾ Ð²ÑÐµÐ¼Ñ Ð¾Ð±ÑÐµÐ¼Ñ ÐºÐ¾Ð¼Ð¿Ð¾Ð·Ð¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð°. Ð¡ Ð¿Ð¾Ð¼Ð¾ÑÑÑ ÐÐ¢Ð¢-ÑÐµÑÑÐ° Ð±ÑÐ»Ð¾ Ð¿Ð¾ÐºÐ°Ð·Ð°Ð½Ð¾, ÑÑÐ¾ Ð³Ð¸Ð´ÑÐ¾ÐºÑÐ¸Ð°Ð¿Ð°ÑÐ¸Ñ Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾Ð¸ÑÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ñ Ð¼ÐµÐ½ÐµÐµ ÑÐ¸ÑÐ¾ÑÐ¾ÐºÑÐ¸ÑÐµÐ½ Ð¿Ð¾ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ Ñ ÑÐ¸Ð½ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ð¼ Ð³Ð¸Ð´ÑÐ¾ÐºÑÐ¸Ð°Ð¿Ð°ÑÐ¸ÑÐ¾Ð¼, Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÐ¼ Ð¼ÐµÑÐ¾Ð´Ð¾Ð¼ Ð¾ÑÐ°Ð¶Ð´ÐµÐ½Ð¸Ñ. ÐÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ ÑÑÐ°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¼ÐµÑÐ¾Ð´Ð° ÐºÑÐ»ÑÑÐ¸Ð²Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¼ÐµÐ·ÐµÐ½ÑÐ¸Ð¼Ð½ÑÑ ÑÑÐ²Ð¾Ð»Ð¾Ð²ÑÑ ÐºÐ»ÐµÑÐ¾Ðº Ð¶Ð¸ÑÐ¾Ð²Ð¾Ð¹ ÑÐºÐ°Ð½Ð¸ ÐºÑÐ¾Ð»Ð¸ÐºÐ° Ð¿Ð¾ÐºÐ°Ð·Ð°Ð»Ð¾ Ð±Ð¾Ð»ÐµÐµ Ð²ÑÑÐ¾ÐºÑÑ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð½Ð° ÑÐ°Ð½Ð½Ð¸Ñ ÑÑÐ¾ÐºÐ°Ñ ÐºÑÐ»ÑÑÐ¸Ð²Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ Ñ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¼, ÐºÐ¾ÑÐ¾ÑÑÐ¹ ÑÐ¿Ð¾ÑÐ¾Ð±ÑÑÐ²ÑÐµÑ Ð²ÑÐ¼ÑÐ²Ð°Ð½Ð¸Ñ ÐºÐ»ÐµÑÐ¾Ðº Ð¸Ð· Ð¼Ð°ÑÑÐ¸Ñ. ÐÑÐ¸ Ð½Ð°Ð¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ð¸ Ð¿Ð¾ÑÐ¸ÑÑÑÑ Ð¼Ð°ÑÑÐ¸Ñ ÑÐ°ÑÑÐ¸ÑÐ°Ð¼Ð¸ Ð³Ð¸Ð´ÑÐ¾ÐºÑÐ¸Ð°Ð¿Ð°ÑÐ¸ÑÐ° Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ ÐºÐ»ÐµÑÐ¾ÑÐ½Ð¾Ð¹ Ð°ÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð½Ð° ÐºÐ¾ÑÐ¾ÑÐºÐ¸Ñ ÑÑÐ¾ÐºÐ°Ñ Ð¾ÑÐ¼ÐµÑÐµÐ½Ð¾ Ð½Ðµ Ð±ÑÐ»Ð¾, Ñ.Ðµ. Ð¼Ð°ÑÑÐ¸ÑÑ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐ¸ÑÐ¾Ð·Ð°Ð½Ð° Ð¸ Ð³Ð¸Ð´ÑÐ¾ÐºÑÐ¸Ð°Ð¿Ð°ÑÐ¸ÑÐ° Ð½Ðµ Ð¾ÐºÐ°Ð·ÑÐ²Ð°ÑÑ ÑÐ¸ÑÐ¾ÑÐ¾ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÑÑÐµÐºÑÐ° Ð½Ð° ÐºÐ»ÐµÑÐºÐ¸.
Additional file 1 of Low methodological quality of systematic reviews on acupuncture: a cross-sectional study
Creators: name: Ho, Leonard
name: Ke, Fiona Y. T.
name: Wong, Charlene H. L.
name: Wu, Irene X. Y.
name: Cheung, Andy K. L.
name: Mao, Chen
name: Chung, Vincent C. H.
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Cancer
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1: eTable 1. Syntaxes for literature search. eTable 2. 17-item bibliographical characteristics questionnaire. eTable 3. List of included systematic reviews. eTable 4. List of excluded systematic reviews with justifications.
Proxima Centauri e le sue sorelle
Creators: Giuseppina Pulcrano
Publisher: name: Media Inaf
Year: 2016

Determinata l’orbita della stella più vicina al Sole. Sono stati necessari cent’anni e uno strumento di grande precisione, lo spettrografo HARSP dell’ESO. Ma ora sappiamo che Proxima ha la stessa velocità radiale della coppia di stelle Alfa Centauri. E che tutt’e tre hanno la stessa età: circa 6 miliardi di anni
Addio Vera Rubin, signora della materia oscura
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2016

L'astronoma americana ha cambiato per sempre la nostra idea di universo introducendo una variabile ancora oggi misteriosa: quel 27 per cento di universo che non emette né calore né luce ma che ci permette di comprendere l’esistenza di numerosi fenomeni altrimenti inspiegabili
Troppo calda la zuppa per il nostro buco nero
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2016

La zuppa di plasma che gorgheggia attorno al buco nero supermassiccio al centro della Via Lattea è talmente calda e diluita da non corrispondere bene alle ricette fluidodinamiche, ben rodate su più classici dischi di accrescimento. Un gruppo del Princeton Plasma Physics Laboratory, utilizzando un approccio “cinetico”, ha sfornato un modello più aderente alle osservazioni
Determining Quasar Black Hole Mass Functions from their Broad Emission Lines: Application to the Bright Quasar Survey
Creators: name: Kelly, Brandon C.
name: Vestergaard, Marianne
name: Fan, Xiaohui
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We describe a Bayesian approach to estimating quasar black hole mass functions (BHMF) when using the broad emission lines to estimate black hole mass. We show how using the broad line mass estimates in combination with statistical techniques developed for luminosity function estimation leads to statistically biased results. We derive the likelihood function for the BHMF based on the broad line mass estimates, and derive the posterior distribution for the BHMF, given the observed data. We develop our statistical approach for a flexible model where the BHMF is modelled as a mixture of Gaussian functions. Statistical inference is performed using markov chain monte carlo (MCMC) methods. Our method has the advantage that it is able to constrain the BHMF even beyond the survey detection limits at the adopted confidence level, accounts for measurement errors and the intrinsic uncertainty in broad line mass estimates, and provides a natural way of estimating the probability distribution of any quantities derived from the BHMF. We conclude by using our method to estimate the local active BHMF using the z < 0.5 Bright Quasar Survey sources. At z = 0.2, the quasar BHMF falls off approximately as a power law with slope ~ 2 for M_{BH} > 10^8. Our analysis implies that z < 0.5 broad line quasars have a typical Eddington ratio of ~ 0.4 and a dispersion in Eddington ratio of < 0.5 dex (abridged).
description: 25 pages, 14 figures, emulate ApJ style, accepted by ApJ
La tavolozza di colori di NGC 4707
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2016

Osservabile in direzione della costellazione dei Cani da caccia, la galassia si trova a 22 milioni di anni luce da noi. Guardandola con il telescopio appare come una spruzzata di stelle blu su un cielo scuro che fa da tela
Capodanno tra le stelle a Saint-Barthélemy
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2016

Dal 26 dicembre al primo gennaio, all’Osservatorio astronomico della Regione autonoma Valle d’Aosta e al Planetario di Lignan, si svolgerà la quarta edizione dello stage internazionale di astronomia dell’ESO. Il campo ospiterà 56 studenti delle scuole secondarie, tra i 16 e i 18 anni, provenienti da tutto il mondo. Una delle borse di partecipazione è offerta dall’INAF