cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð²Ð°ÑÐ¸Ð°Ð½ÑÐ¾Ð² Ð°Ð¿Ð¿Ð°ÑÐ°ÑÐ½Ð¾Ð¹ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ð»ÐµÑÐ¾Ð² ÑÐµÑÐµÐ¹ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ°ÑÐ½ÑÑ Ð½ÐµÑÐµÑÐºÐ¸Ñ Ð²ÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÐµÐ¹ Ð½Ð° Ð±Ð°Ð·Ðµ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÑÐµÐ¼ÑÑ Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð¸Ð½ÑÐµÐ³ÑÐ°Ð»ÑÐ½ÑÑ ÑÑ ÐµÐ¼
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐµÑÐµÐ²ÐµÑÐ·ÐµÐ², ÐÐ»ÐµÐºÑÐ°Ð½Ð´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Ð¾Ð½ÑÑÐ¾Ð»Ð»ÐµÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½ÑÐµ
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description: Ð Ð°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ Ð°Ð¿Ð¿Ð°ÑÐ°ÑÐ½Ð¾Ð¹ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ð»ÐµÑÐ° ÑÐµÑÐ¸ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ°ÑÐ½ÑÑ Ð½ÐµÑÐµÑÐºÐ¸Ñ Ð²ÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÐµÐ¹, ÐºÐ¾ÑÐ¾ÑÑÐ¹ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¸Ð½ÑÐµÐ³ÑÐ¸ÑÐ¾Ð²Ð°Ð½ Ð² Ð¼Ð¸ÐºÑÐ¾ÐºÐ¾Ð½ÑÑÐ¾Ð»Ð»ÐµÑÐ½Ð¾Ðµ ÑÐ´ÑÐ¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐµÐ¼ÐµÐ¹ÑÑÐ²Ð°. Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ ÑÐµÑÐµÐ²Ð¾Ð¹ Ð¿Ð¾Ð´ÑÐ¾Ð´ Ðº Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð½ÐµÑÐµÑÐºÐ¾Ð¹ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸, Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑÑÐ¸Ð¹ ÑÐ°ÑÑÐ¸ÑÐ¸ÑÑ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐµ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐ¸ Ð½ÐµÑÐµÑÐºÐ¾Ð³Ð¾ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ð»ÐµÑÐ°. ÐÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ Ð°Ð²ÑÐ¾ÑÑÐºÐ¸Ñ ÑÐµÑÐµÐ½Ð¸Ð¹ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÐµÑ ÑÐ½Ð¸Ð·Ð¸ÑÑ ÑÑÑÐ´Ð¾ÐµÐ¼ÐºÐ¾ÑÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð¿Ð¾Ð²ÑÑÐ¸ÑÑ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð½ÐµÑÐµÑÐºÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð²ÑÑÑÐ°Ð¸Ð²Ð°ÐµÐ¼ÑÑ Ð¼Ð¸ÐºÑÐ¾ÐºÐ¾Ð½ÑÑÐ¾Ð»Ð»ÐµÑÐ½ÑÑ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¹.
Smooth kinematic and metallicity gradients reveal that the Milky Way's nuclear star cluster and disc might be part of the same structure
Creators: name: Nogueras-Lara, F.
name: Feldmeier-Krause, A.
name: Schödel, R.
name: Sormani, M. C.
name: de Lorenzo-Cáceres, A.
name: Mastrobuono-Battisti, A.
name: Schultheis, M.
name: Neumayer, N.
name: Rich, R. M.
name: Nieuwmunster, N.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The innermost regions of most galaxies are characterised by the presence of extremely dense nuclear star clusters. Nevertheless, these clusters are not the only stellar component present in galactic nuclei, where larger stellar structures known as nuclear stellar discs, have also been found. Understanding the relation between nuclear star clusters and nuclear stellar discs is challenging due to the large distance towards other galaxies which limits their analysis to integrated light. The Milky Way's centre, at only 8 kpc, hosts a nuclear star cluster and a nuclear stellar disc, constituting a unique template to understand their relation and formation scenario. We aim to study the kinematics and stellar metallicity of stars from the Milky Way's nuclear star cluster and disc to shed light on the relation between these two Galactic centre components. We used publicly available photometric, proper motions, and spectroscopic catalogues to analyse a region of $\sim2.8'\times4.9'$ centred on the Milky Way's nuclear star cluster. We built colour magnitude diagrams, and applied colour cuts to analyse the kinematic and metallicity distributions of Milky Way's nuclear star cluster and disc stars with different extinction along the line of sight. We detect kinematics and metallicity gradients for the analysed stars along the line of sight towards the Milky Way's nuclear star cluster, suggesting a smooth transition between the nuclear stellar disc and cluster. We also find a bi-modal metallicity distribution for all the analysed colour bins, which is compatible with previous work on the bulk population of the nuclear stellar disc and cluster. Our results suggest that these two Galactic centre components might be part of the same structure with the Milky Way's nuclear stellar disc being the grown edge of the nuclear star cluster.
description: Accepted for publication in A&A. 13 pages, 9 figures
On the uniqueness of the unitary representations of the non commutative Heisenberg-Weyl algebra
Creators: name: Gouba, Laure
name: Scholtz, Frederik G.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: In this paper we discuss the uniqueness of the unitary representations of the non commutative Heisenberg-Weyl algebra. We show that, apart from a critical line for the non commutative position and momentum parameters, the Stone-von Neumann theorem still holds, which implies uniqueness of the unitary representation of the Heisenberg-Weyl algebra.
description: 4 pages
title: ÐÑÑÐµÑÐ½Ð¾ÑÑÑ Ð¿Ð¾ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐ¼ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ°Ð¼ Ð¸ ÐµÐµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð´Ð»Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸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Ð¸ÑÐ°Ð¹Ð»Ð¾Ð²Ð°, ÐÐ°Ð»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: ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ
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description: Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¹ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÑÐµÑÐ½Ð¾Ð¹ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸ Ð¾ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÑ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ°Ñ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÐÐÐ Â«ÐÐ²Ð¸Ð½Ð°Â».
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ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÑ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð¸ ÑÐ¿ÐµÑÐ¸ÑÐ¸ÐºÐ¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, Ð±ÑÐ»Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð´Ð»Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÑ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð´Ð»Ñ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð² ÐÐÐ Â«ÐÐ²Ð¸Ð½Ð°Â».
Approach to Intel Concept
Creators: name: Victoria, Artur
Publisher: name: Zenodo
Year: 2020

description: The union of intelligence with the knowledge of our own capabilities, and those of our allies, provides the foundation for the planning and execution of operations. Intelligence today is not only about cataloguing the forces of an adversary and evaluating his capabilities. It also encompasses an understanding of the adversary's culture, motivation, perspective, and goals.
Recent results on nucleon resonance electrocouplings from the studies of $π^{+}π^{-}p$ electroproduction with the CLAS detector
Creators: name: Mokeev, V. I.
name: Burkert, V. D.
name: Fedotov, G. V.
name: Golovach, E. N.
name: Ishkhanov, B. S.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: Recent results on nucleon resonance studies in $π^{+}π^{-}p$ electro- production off protons with the CLAS detector are presented. The analysis of CLAS data allowed us to determine all essential contributing mechanisms, providing a credible separation between resonant and non-resonant parts of the cross sections in a wide kinematical area of invariant masses of the final hadronic system $1.3
description: 7 pages, 5 figures, NSTAR 2009 conference
Baryon Number Violating Rate as A Function of the Proton-Proton Collision Energy
Creators: name: Qiu, Yu-Cheng
name: Tye, S. -H. Henry
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The baryon-number violation (BV) happens in the standard electroweak model. According to the Bloch-wave picture, the BV event rate shall be significantly enhanced when the proton-proton collision center of mass (COM) energy goes beyond the sphaleron barrier height $E_{\rm sph}\simeq 9.0\,{\rm TeV}$. Here we compare the BV event rates at different COM energies, using the Bloch-wave band structure and the CT18 parton distribution function data, with the phase space suppression factor included. As an example, the BV cross section at 25 TeV is 4 orders of magnitude bigger than its cross section at 13 TeV. The probability of detection is further enhanced at higher energies since an event at higher energy will produce on average more same sign charged leptons.
description: 7 pages, 6 figures, and 4 tables. This is the same as the published version
The Islamic State and the crises of COVID 19
Creators: name: Victoria, Artur
Publisher: name: Zenodo
Year: 2020

description: According to the Homeland Security Today website, the statement lists "guidelines for dealing with the epidemic". For the Islamic State, the main advice is "to trust God and take refuge in Him from disease", but followers have an "obligation" to take protective measures to prevent it. Among these measures, the terrorist group emphasizes that "the healthy should not enter the land of the epidemic and the sick must not leave it". According to the council, terrorists should not travel to Europe and the United States, which are common targets in the West, nor to countries in the Middle East such as Iran, Iraq and Saudi Arabia. The group dominates provinces and has active cells in some countries still free of the disease, such as the Central and West Africa region, as well as Syria and Yemen, where civil war makes it difficult to collect information about epidemics. But cases have already been confirmed in Algeria, Egypt, Iraq, Afghanistan, India, the Philippines and Indonesia. The reorganization in Africa of ISIS - Evolution and progression in Mozambique In Mozambique, according to statements by the President of the Republic and the Minister of Defence, there are groups of terrorists in the district of Cabo Delgado and other groups in the centre, but who are considered to be affected by RENAMO. The situation is complicated because as these groups demonstrate, they show all the characteristics of IS members.
Discrete MDL Predicts in Total Variation
Creators: name: Hutter, Marcus
Publisher: name: arXiv
Year: 2009
Subjects: subject: Probability (math.PR)
subject: Information Theory (cs.IT)
subject: Machine Learning (cs.LG)
subject: Statistics Theory (math.ST)
subject: Machine Learning (stat.ML)
subject: FOS: Mathematics
subject: FOS: Computer and information sciences

description: The Minimum Description Length (MDL) principle selects the model that has the shortest code for data plus model. We show that for a countable class of models, MDL predictions are close to the true distribution in a strong sense. The result is completely general. No independence, ergodicity, stationarity, identifiability, or other assumption on the model class need to be made. More formally, we show that for any countable class of models, the distributions selected by MDL (or MAP) asymptotically predict (merge with) the true measure in the class in total variation distance. Implications for non-i.i.d. domains like time-series forecasting, discriminative learning, and reinforcement learning are discussed.
description: 15 LaTeX pages
Roman studies of the dawn of black holes and synergies with Lynx
Creators: name: Hickox, Ryan
Publisher: name: Zenodo
Year: 2021

description: Supermassive black holes are ubiquitous un the local Universe and appear to play key role in galaxy formation, but their ultimate origin remains a mystery. To solve this puzzle requires direct observations of the growth of these black holes in the early Universe (z > 6-10) as active galactic nuclei (AGN). I will give a brief overview of how these observations can constrain black hole seed models, for example distinguishing between direct collapse of pristine gas clouds or rapid accretion onto stellar-mass remnants. The Nancy Grace Roman Space Telescope will play a key role in these studies, primarily measuring host galaxy properties and redshifts for high-z AGN through deep observations over a wide area. I will discuss synergies with other future observatories (in particular in the infrared and X-ray bands) for identifying high-z AGN, with an emphasis on observations with NASA' Lynx concept X-ray observatory.
title: Ð­Ð½ÐµÑÐ³Ð¾ÑÑÑÐµÐºÑÐ¸Ð²Ð½ÑÐµ ÑÐ°ÑÐ°Ð´Ñ Ñ ÑÐ¾ÑÐ¾Ð±Ð¸Ð¾ÑÐµÐ°ÐºÑÐ¾ÑÐ¾Ð¼ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¾Ð² ÑÐ¾ÑÑÐ° Ð¼Ð¸ÐºÑÐ¾Ð²Ð¾Ð´Ð¾ÑÐ¾ÑÐ»ÐµÐ¹
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°ÑÐ°, 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Ð¸Ð¾Ð³Ð°Ð·
Ð¤Ð°ÑÐ°Ð´Ñ
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ÑÐ¾ÑÐ¾Ð±Ð¸Ð¾ÑÐµÐ°ÐºÑÐ¾ÑÑ
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description: ÐÐ°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ ÑÐ¾ÑÐ¾Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ ÑÑÑÑÐ¾Ð¹ÑÑÐ² Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¾Ð² ÑÐ¾ÑÑÐ° Ð¼Ð¸ÐºÑÐ¾Ð²Ð¾Ð´Ð¾ÑÐ¾ÑÐ»ÐµÐ¹ Ð´Ð»Ñ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð±Ð¸Ð¾Ð°Ð´Ð°Ð¿ÑÐ¸Ð²Ð½ÑÑ ÑÐ°ÑÐ°Ð´Ð¾Ð² Ð·Ð´Ð°Ð½Ð¸Ñ. ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¾ Ð½Ð° ÑÐµÑÐµÐ½Ð¸Ðµ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ñ Ð·Ð°Ð´Ð°Ñ Ð¿Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ ÑÐ½ÐµÑÐ³Ð¾ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð·Ð´Ð°Ð½Ð¸Ð¹ Ð¸ ÑÐ½Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð²ÑÐ±ÑÐ¾ÑÐ¾Ð² Ð¡Ð2 Ð² Ð°ÑÐ¼Ð¾ÑÑÐµÑÑ. Ð¦ÐµÐ»Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ â Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½ÑÑ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ ÑÐ°ÑÐ°Ð´Ð½Ð¾Ð¹ Ð¿Ð°Ð½ÐµÐ»Ð¸ Ð·Ð´Ð°Ð½Ð¸Ñ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÐ¾ÑÐ¾Ð±Ð¸Ð¾ÑÐµÐ°ÐºÑÐ¾ÑÐ¾Ð² Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¾Ð² ÑÐ¾ÑÑÐ° Ð¼Ð¸ÐºÑÐ¾Ð²Ð¾Ð´Ð¾ÑÐ¾ÑÐ»ÐµÐ¹ Ð² ÐºÐ»Ð¸Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÑÐ»Ð¾Ð²Ð¸ÑÑ Ð Ð¾ÑÑÐ¸Ð¸. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÑÑ ÑÐ°ÑÑÐµÑ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¼Ð¸ÐºÑÐ¾Ð²Ð¾Ð´Ð¾ÑÐ¾ÑÐ»ÐµÐ¹ Ð¿ÑÐ¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½ÑÑ ÐºÐ»Ð¸Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÑÐ»Ð¾Ð²Ð¸ÑÑ, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ°ÑÑÐµÑ ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²Ð° ÑÐ½ÐµÑÐ³Ð¸Ð¸, ÐºÐ¾ÑÐ¾ÑÑÑ Ð¼Ð¾Ð¶Ð½Ð¾ Ð¿Ð¾Ð»ÑÑÐ¸ÑÑ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð¿Ð°Ð½ÐµÐ»Ð¸ Ñ ÑÐ¾ÑÐ¾Ð±Ð¸Ð¾ÑÐµÐ°ÐºÑÐ¾ÑÐ°Ð¼Ð¸.
Size as a constraint on high-z galaxy selection
Creators: name: Holwerda, Benne
Publisher: name: Zenodo
Year: 2021

description: Redshift z=9-10 object selection is the effective limit of Hubble Space Telescope imaging capability, even when confirmed with Spitzer. If only a few photometry data points are available, it becomes attractive to add criteria based on their morphology in these J- and H-band images. One could do so through visual inspection, a size criterion, or alternate morphometrics. We explore a vetted sample of BoRG z~9 and z~10 candidate galaxies and the object rejected by Morishita+ to explore the utility of a size criterion in z=9-10 candidate selection. A stringent, PSF-corrected effective radius criterion (re<0.3") would result in the rejection of 65-70% of the interlopers visually rejected by Morishita+. It may also remove up to $\sim20$\% of bona-fide brightest (L>>L*) z=9 or 10 candidates from a BoRG selected sample based on the Mason+ luminosity functions, assuming the Holwerda+ (2015) z~9 size-luminosity relation. We argue that including a size constraint in lieu of a visual inspection may serve in wide-field searches for these objects in e.g. Roman Telescope or HST archival imaging with minimal loss of candidate objects while removing a large fraction of contaminants for z>6 selections.
Multiwavelength Observations of the Runaway Binary HD 15137
Creators: name: McSwain, M. Virginia
name: De Becker, Michael
name: Roberts, Mallory S. E.
name: Boyajian, Tabetha S.
name: Gies, Douglas R.
name: Grundstrom, Erika D.
name: Aragona, Christina
name: Marsh, Amber N.
name: Roettenbacher, Rachael M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: HD 15137 is an intriguing runaway O-type binary system that offers a rare opportunity to explore the mechanism by which it was ejected from the open cluster of its birth. Here we present recent blue optical spectra of HD 15137 and derive a new orbital solution for the spectroscopic binary and physical parameters of the O star primary. We also present the first XMM-Newton observations of the system. Fits of the EPIC spectra indicate soft, thermal X-ray emission consistent with an isolated O star. Upper limits on the undetected hard X-ray emission place limits on the emission from a proposed compact companion in the system, and we rule out a quiescent neutron star in the propellor regime or a weakly accreting neutron star. An unevolved secondary companion is also not detected in our optical spectra of the binary, and it is difficult to conclude that a gravitational interaction could have ejected this runaway binary with a low mass optical star. HD 15137 may contain an elusive neutron star in the ejector regime or a quiescent black hole with conditions unfavorable for accretion at the time of our observations.
description: Accepted to AJ
Indigenous librarianship
Creators: name: Burns, Kathleen
name: Doyle, Ann M.
name: Joseph, Gene
name: Krebs, Allison
Publisher: name: Taylor & Francis
Year: 2015

description: Indigenous librarianship unites the discipline of librarianship with Indigenous approaches to knowledge, theory, and research methodology. It has a developing bibliography and local, national and international professional associations devoted to its growth. A focus of Indigenous librarianship is the provision of culturally relevant library and information collections and services by, for and with Indigenous people. Grounded in the contemporary realities of Indigenous people and Indigenous aspirations for self governance and sovereignty, it has a critical theoretical base. Its practice may be carried out in places ranging from small Indigenous community libraries to specialized collections in large research institutions. As an emergent scholarship the field is in the process of defining itself. This article serves as an introductory overview to the history, practice, issues, and theoretical approaches associated with Indigenous librarianship. [This article was originally published in 2009 and updated in 2014].
Additional file 1 of The association between daily total physical activity and risk of cardiovascular disease among hypertensive patients: a 10-year prospective cohort study in China
Creators: name: Zhou, Tingyu
name: Su, Jian
name: Tao, Ran
name: Qin, Yu
name: Zhou, Jinyi
name: Lu, Yan
name: Hua, Yujie
name: Jin, Jianrong
name: Guo, Yu
name: Chen, Zhengming
name: Li, Liming
name: Wu, Ming
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: Environmental Sciences not elsewhere classified
subject: Science Policy
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified

description: Additional file 1 : Appendix 1. Hazard ratios (95%CI) of CVD across quartiles of total physical activity stratified by BP-levels with self-reported and new detected hypertension. Appendix 2. Hazard ratios (95% CI) of CVD across physical activity categorized by recommendation of guidelines. Appendix 3. Hazard ratios (95% CI) of CVD across quartiles of total physical activity for all participants and stratified by gender with sensitivity analyses. Appendix 4. Hazard ratios (95%CI) of CVD across quartiles of total physical activity stratified by age with sensitivity analyses. Appendix 5. Hazard ratios (95%CI) of CVD across quartiles of total physical activity stratified by BP-levels with sensitivity analyses. Appendix 6. Basic characteristics of respondent, non-respondent, death population of Respondent and respondents die of CVD at baseline.
title: ÐÐ¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐ¸ Ð½ÐµÐ¹ÑÐ¾ÑÐµÐ°Ð±Ð¸Ð»Ð¸ÑÐ°ÑÐ¸Ð¸ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÐ¸ÑÑÐµÐ¼Ñ Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¾Ð±ÑÐ°ÑÐ½Ð¾Ð¹ ÑÐ²ÑÐ·Ð¸
title: Possibilities of neurorehabilitation using a biofeedback system
Creators: name: ÐÐ°ÑÐ°Ð½Ð¾Ð²Ð°, ÐÐ°ÑÐ¸Ð½Ð°
name: Ð¨Ð¸ÑÐºÐ¸Ð½, ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2022
Subjects: Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ°Ñ ÑÐµÐ°Ð±Ð¸Ð»Ð¸ÑÐ°ÑÐ¸Ñ
Ð½ÐµÐ¹ÑÐ¾ÑÐµÐ°Ð±Ð¸Ð»Ð¸ÑÐ°ÑÐ¸Ñ
Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ°Ñ Ð¾Ð±ÑÐ°ÑÐ½Ð°Ñ ÑÐ²ÑÐ·Ñ
ÑÑÐ°Ð±Ð¸Ð»Ð¾Ð¿Ð»Ð°ÑÑÐ¾ÑÐ¼Ð°
medical rehabilitation
neurorehabilitation
biofeedback
stabiloplatform

description: ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð¼ÐµÑÐ¾Ð´ ÑÐµÐ°Ð±Ð¸Ð»Ð¸ÑÐ°ÑÐ¸Ð¸ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÐ¸ÑÑÐµÐ¼Ñ Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ²ÑÐ·Ð¸, ÐºÐ»Ð¸Ð½Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ»ÑÑÐ°Ð¸ Ð¾Ð½ÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð±Ð¾Ð»ÑÐ½ÑÑ, Ð² ÑÐµÐ°Ð±Ð¸Ð»Ð¸ÑÐ°ÑÐ¸Ð¸ ÐºÐ¾ÑÐ¾ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð»Ð¸ÑÑ ÑÑÐµÐ½Ð¸Ð½Ð³Ð¸ Ñ Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¾Ð±ÑÐ°ÑÐ½Ð¾Ð¹ ÑÐ²ÑÐ·ÑÑ.
description: The article presents a method of rehabilitation using a biological communication system, clinical cases of cancer patients in the rehabilitation of which biofeedback trainings were used.
Direct photon emission in Heavy Ion Collisions from Microscopic Transport Theory and Fluid Dynamics
Creators: name: Baeuchle, Bjoern
name: Bleicher, Marcus
Publisher: name: arXiv
Year: 2010
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Direct photon emission in heavy-ion collisions is calculated within a relativistic micro+macro hybrid model and compared to the microscopic transport model UrQMD. In the hybrid approach, the high-density part of the collision is calculated by an ideal 3+1-dimensional hydrodynamic calculation, while the early (pre-equilibrium-) and late (rescattering-) phase are calculated with the transport model. Different scenarios of the transition from the macroscopic description to the transport model description and their effects are studied. The calculations are compared to measurements by the WA98-collaboration and predictions for the future CBM-experiment are made.
description: 6 pages, 3 figures. XLVIII International Winter Meeting on Nuclear Physics, BORMIO2010 January 25-29, 2010, Bormio, Italy
Archivematica as a service : COPPUL's Shared Digital Preservation Platform
Creators: name: Sprout, Bronwen
name: Jordan, Mark
Publisher: name: The University of British Columbia
Year: 2015

description: The Council of Prairie and Pacific University Libraries (COPPUL) is piloting a cloud-based preservation service using the Archivematica digital preservation system. The service is offered to COPPUL member institutions that wish to preserve digital holdings but prefer a hosted service to installing and managing local Archivematica instances. This service is a joint effort of COPPUL, Artefactual Systems (Archivematica lead developers), and University of British Columbia (UBC) Library (the cloud storage provider). COPPUL is responsible for promoting the service, signing up new institutions and seeding the one-time set-up costs. Artefactual Systems provides account administration, installation, server administration, and user technical support. UBC Library provides fee- based server hosting and digital object storage service. This article discusses COPPUL’s Archivematica-as-a-service model generally and covers certain aspects of implementation in greater detail, concluding with a discussion of future directions.
title: Ð Ð°ÑÑÐµÑ ÐºÐ°Ð±ÐµÐ»ÑÐ½Ð¾Ð¹ Ð»Ð¸Ð½Ð¸Ð¸ Ðº ÐÐÐ¢Ð 6(10)/0,4 ÐºÐ
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±ÐµÐ´ÐµÐ², ÐÐ²Ð°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: ÐºÐ°Ð±ÐµÐ»ÑÐ½ÑÐµ Ð»Ð¸Ð½Ð¸Ð¸
Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½ÑÐµ Ð¿ÐµÑÐµÑÐµÑÐµÐ½Ð¸Ñ
Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð¿ÑÐ¾ÐºÐ»Ð°Ð´ÐºÐ° ÐºÐ°Ð±ÐµÐ»Ñ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÑÑ ÑÐ°ÑÑÐµÑ ÐºÐ°Ð±ÐµÐ»ÑÐ½ÑÑ Ð»Ð¸Ð½Ð¸Ð¹ Ñ Ð¿ÑÐµÐ´Ð²Ð°ÑÐ¸ÑÐµÐ»ÑÐ½ÑÐ¼ Ð²ÑÐ±Ð¾ÑÐ¾Ð¼ ÐºÐ°Ð±ÐµÐ»Ñ, Ð²ÑÐ±Ð¾ÑÐ¾Ð¼ Ð¿ÑÑÐ¸ ÑÑÐ°ÑÑÑ ÑÐºÐ»Ð°Ð´ÐºÐ¸ ÐºÐ°Ð±ÐµÐ»ÐµÐ¹. ÐÑÐµ ÑÐ°ÑÑÐµÑÑ Ð¸ Ð½Ð¾ÑÐ¼Ñ ÑÐºÐ»Ð°Ð´ÐºÐ¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ñ ÑÐ¾Ð³Ð»Ð°ÑÐ½Ð¾ Ð½Ð¾ÑÐ¼Ð°Ð¼ ÐÐ£Ð­ Ð¸ Ð¡ÐÐ¸Ð. Ð¢Ð°Ðº Ð¶Ðµ Ð² ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐ»ÑÑÐ°Ð¸ Ð¿ÐµÑÐµÑÐµÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÑÐµÐ¼Ð¾Ð¹ ÐºÐ°Ð±ÐµÐ»ÑÐ½Ð¾Ð¹ Ð»Ð¸Ð½Ð¸Ð¸ Ñ Ð´ÑÑÐ³Ð¸Ð¼Ð¸ Ð½Ð°Ð´Ð·ÐµÐ¼Ð½ÑÐ¼Ð¸ Ð¸ Ð¿Ð¾Ð´Ð·ÐµÐ¼Ð½ÑÐ¼Ð¸ Ð¿ÐµÑÐµÑÐµÑÐµÐ½Ð¸ÑÐ¼Ð¸. ÐÐ»Ð°Ð½ Ð¿ÑÐ¾ÐµÐºÑÐ° Ð±ÑÐ» Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½ Ð² Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ðµ Auto CAD.
Cross-correlation properties of cyclotomic sequences
Creators: name: Cai, Kai
name: Feng, Rongquan
name: Zheng, Zhiming
Publisher: name: arXiv
Year: 2009
Subjects: subject: Information Theory (cs.IT)
subject: Discrete Mathematics (cs.DM)
subject: Combinatorics (math.CO)
subject: FOS: Computer and information sciences
subject: FOS: Mathematics

description: Sequences with good correlation properties are widely used in engineering applications, especially in the area of communications. Among the known sequences, cyclotomic families have the optimal autocorrelation property. In this paper, we decide the cross-correlation function of the known cyclotomic sequences completely. Moreover, to get our results, the relations between the multiplier group and the decimations of the characteristic sequence are also established for an arbitrary difference set.
Klippel-Feil syndrome
Creators: name: Van Looveren, Kevin
Publisher: name: EURORAD
Year: 2014
Subjects: subject: Anatomy
subject: Musculoskeletal spine
subject: Paediatric
subject: Spine
subject: Conventional radiography
subject: Plain radiographic studies
subject: Comparative studies
subject: Diagnostic procedure
subject: Education
subject: Screening
subject: Congenital
subject: Dysplasias
subject: Pathology

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: male, 12 years
description: Clinical History: A 12-year-old boy with a previous medical history of tetralogy of Fallot,  bilateral hearing loss and small stature, presented with limitation of neck movement after a minor neck trauma.On clinical examination, mild dextroconvex thoracolumbar scolio... Final Diagnosis: Klippel-Feil syndrome with several associated anomalies.
title: ÐÐ¾Ð»Ð¸ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ°Ñ Ð²ÐµÑÐ½Ð°. ÐÑÐ¼Ð°Ð½Ð¸ÑÐ°ÑÐ½ÑÐµ Ð½Ð°ÑÐºÐ¸
title: Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ ÐÑÐµÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ ÑÑÑÐ´ÐµÐ½ÑÐµÑÐºÐ¾Ð¹ Ð½Ð°ÑÑÐ½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ð¸, 29-30 Ð¼Ð°ÑÑÐ° 2019 Ð³Ð¾Ð´Ð°
titleType: Subtitle
Creators: name: "ÐÐ¾Ð»Ð¸ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ°Ñ Ð²ÐµÑÐ½Ð°. ÐÑÐ¼Ð°Ð½Ð¸ÑÐ°ÑÐ½ÑÐµ Ð½Ð°ÑÐºÐ¸", Ð²ÑÐµÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ°Ñ ÑÑÑÐ´ÐµÐ½ÑÐµÑÐºÐ°Ñ Ð½Ð°ÑÑÐ½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (2; 2019; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2019
Subjects: Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½ÑÐµ ÑÐ·ÑÐºÐ¸
Ð»Ð¸Ð½Ð³Ð²Ð¸ÑÑÐ¸ÐºÐ°
Ð»Ð¸Ð½Ð³Ð²Ð¾Ð´Ð¸Ð´Ð°ÐºÑÐ¸ÐºÐ°
Ð¼ÐµÐ¶ÐºÑÐ»ÑÑÑÑÐ½ÑÐµ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ
Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ðµ Ð´ÐµÐ»Ð¾
Ð¿ÐµÐ´Ð°Ð³Ð¾Ð³Ð¸ÐºÐ°
Ð¿ÐµÑÐµÐ²Ð¾Ð´

description: Ð ÑÐ±Ð¾ÑÐ½Ð¸Ðº Ð²ÐºÐ»ÑÑÐµÐ½Ñ ÑÑÐ°ÑÑÐ¸ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ¾Ð² Ð¸ Ð¼Ð¾Ð»Ð¾Ð´ÑÑ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð² ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¸Ñ Ð¸ Ð·Ð°ÑÑÐ±ÐµÐ¶Ð½ÑÑ Ð²ÑÐ·Ð¾Ð². ÐÐ°ÑÐµÑÐ¸Ð°Ð»Ñ Ð¾ÑÐ¾Ð±ÑÐ°Ð½Ñ Ð¿Ð¾ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ°Ð¼
Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ ÑÐµÐºÑÐ¸Ð¾Ð½Ð½ÑÑ Ð·Ð°ÑÐµÐ´Ð°Ð½Ð¸Ð¹ II ÐÑÐµÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ ÑÑÑÐ´ÐµÐ½ÑÐµÑÐºÐ¾Ð¹ Ð½Ð°ÑÑÐ½Ð¾-
Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ð¸ Â«ÐÐ¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ°Ñ Ð²ÐµÑÐ½Ð°. ÐÑÐ¼Ð°Ð½Ð¸ÑÐ°ÑÐ½ÑÐµ Ð½Ð°ÑÐºÐ¸Â»
(Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³, 29â30 Ð¼Ð°ÑÑÐ° 2019 Ð³Ð¾Ð´Ð°), Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð½Ð¾Ð¹ 120-Ð»ÐµÑÐ¸Ñ Ð¡Ð°Ð½ÐºÑ-
ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°. Ð Ð¿ÑÐ±Ð»Ð¸ÐºÐ°ÑÐ¸ÑÑ Ð·Ð°ÑÑÐ°Ð³Ð¸Ð²Ð°ÑÑÑÑ Ð°ÐºÑÑÐ°Ð»ÑÐ½ÑÐµ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð³ÑÐ¼Ð°Ð½Ð¸ÑÐ°ÑÐ½Ð¾Ð³Ð¾ Ð·Ð½Ð°Ð½Ð¸Ñ, Ð² ÑÐ°ÑÑÐ½Ð¾ÑÑÐ¸ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¹
Ð»Ð¸Ð½Ð³Ð²Ð¸ÑÑÐ¸ÐºÐ¸, Ð»Ð¸Ð½Ð³Ð²Ð¾Ð´Ð¸Ð´Ð°ÐºÑÐ¸ÐºÐ¸, Ð¿ÐµÑÐµÐ²Ð¾Ð´Ð¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ, Ð¼ÐµÐ¶ÐºÑÐ»ÑÑÑÑÐ½Ð¾Ð¹ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¸, Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ Ð´ÐµÐ»Ð°, ÑÐ¸ÑÑÐ¾Ð²Ð¾Ð¹ Ð¿ÐµÐ´Ð°Ð³Ð¾Ð³Ð¸ÐºÐ¸ Ð¸ Ð´ÑÑÐ³Ð¸Ñ ÑÐ°Ð·Ð´ÐµÐ»Ð¾Ð².
ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÑÐµÑ Ð¸Ð½ÑÐµÑÐµÑ Ð´Ð»Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð² Ð² ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ Ð¾Ð±Ð»Ð°ÑÑÑÑ Ð³ÑÐ¼Ð°Ð½Ð¸ÑÐ°ÑÐ½ÑÑ Ð½Ð°ÑÐº, ÑÑÐ°ÑÐ¸ÑÑÑ Ð¸ Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»ÐµÐ¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ¾Ð² Ð¸ Ð¾Ð±ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½ÑÑ ÑÐºÐ¾Ð», Ð²ÑÐµÑ ÑÑÑÐµÐ¼ÑÑÐ¸ÑÑÑ Ðº ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ Ð³ÑÐ¼Ð°Ð½Ð¸ÑÐ°ÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ.
Traumatic pulmonary torsion leading to complete bronchovascular avulsion
Creators: name: Awwad, Amir
Publisher: name: EURORAD
Year: 2014
Subjects: subject: Arteries / Aorta
subject: Cardiovascular system
subject: Emergency
subject: Lung
subject: CT
subject: Diagnostic procedure
subject: Surgery
subject: Acute
subject: Trauma

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: female, 45 years
description: Clinical History: Following a fall from the 5th floor, an emergency admission of a severely shocked patient (GCS 3/15) has led to a clam shell thoracotomy and urgent laparotomy on arrival to the hospital. Intra-operatively, no clear source of acute haemorrhage was identifi... Final Diagnosis: Acute pulmonary torsion with bronchovascular avulsion.
Diagnóstico molecular rápido em ambulatório
Creators: name: Smal, Yulia
Publisher: name: Anais do Instituto de Higiene e Medicina Tropical
Year: 2024

description: A tecnologia em Ponto de Cuidado (POCT) revolucionou o diagnóstico clínico com testes mais rápidos e eficientes.
O avanço do teste molecular em POCT (mPOCT) combina a agilidade do POCT com a precisão da biologia molecular, permitindo diagnósticos precisos e eficazes. A biologia molecular amplia o espectro de diagnósticos, abrangendo desde infeções respiratórias até doenças genéticas. Os testes de biologia molecular, como a PCR (Polymerase Chain Reaction), são essenciais para o diagnóstico rápido e sensível de doenças infecciosas. A evolução de PCR em POCT evidencia sua relevância para ambientes com acesso limitado a laboratórios mais complexos e equipados. Contudo, a eficácia do mPOCT ainda exige formação adequada e seleção criteriosa dos sistemas, visando a simplicidade, robustez e clareza na interpretação dos resultados. Alem disso os patógenos comuns para países em desenvolvimento precisam de ter maior representação nos mPOCT. As tecnologias de diagnóstico mPOC buscam ser acessíveis, simples e portáteis.
Este artigo faz uma revisão breve de aspetos tecnológicos que aproximam cada vez mais o diagnóstico laboratorial de referência ao paciente. Começando pelas tecnologias tradicionais como PCR que em tempos revolucionou diagnóstico molecular permitindo a deteção e análise quantitativa em tempo real discutem-se agora as tecnologias que estão a mudar mPOCT moderno. Assim, a PCR digital oferece quantificação absoluta de genes-alvo. Inovações em primers e sondas otimizam a precisão do diagnóstico molecular. A eficácia e custo dos testes moleculares são influenciados pela escolha do detetor, com sensores eletroquímicos surgindo como opção promissora de baixo custo para ambientes com recursos limitados. Técnicas de amplificação isotérmica permitiram baixar as exigências energéticas e restrições de armazenamento de reagentes que são aspetos críticos de POCT. A nanotecnologia potencializa diagnósticos moleculares em relação à qualidade dos resultados e miniaturização. Sistemas microfluídicos compactam várias funções em dispositivos minúsculos permitindo a automação que por sua vez reduz significativamente os erros de utilizador nos testes. Microarrays detectam múltiplos ácidos nucleicos e anticorpos ao mesmo tempo permitindo paneis diagnósticos sintomáticos. Sequenciações de nova e terceira gerações têm potencial completamente substituir todas as outras tecnologias de mPOCT no futuro e já são fundamentais para diagnósticos e rastreamento de epidemias.
description: Anais do Instituto de Higiene e Medicina Tropical, v. 22 n. 2 (2023): Medicina Tropical e Desenvolvimento Sustentável - 6.º Congresso Nacional de Medicina Tropical
title: ÐÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¾ÑÐ¾ÑÐ½Ð¾Ð¹ ÑÐ°ÑÑÐ¸ ÐÐ¦ÐÐ Ð´Ð»Ñ ÑÐµÐ°ÐºÑÐ¾ÑÐ° ÑÐ´ÐµÑÐ½Ð¾Ð¹ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸ ÐÐ ÐÐ¡Ð¢ ÐÐ - 300
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ²Ð°Ð½Ð¾Ð², ÐÐ²Ð³ÐµÐ½Ð¸Ð¹
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: Ð¾ÑÐµÐ²ÑÐµ Ð½Ð°ÑÐ¾ÑÑ
ÑÐµÐ°ÐºÑÐ¾ÑÐ½ÑÐµ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸
Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¾ÑÐµÐ²Ð¾Ð³Ð¾ Ð½Ð°ÑÐ¾ÑÐ°

description: ÐÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð° Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¾ÑÐµÐ²Ð¾Ð³Ð¾ Ð½Ð°ÑÐ¾ÑÐ° Ð½Ð¸Ð·ÐºÐ¾Ð¹ Ð±ÑÑÑÑÐ¾ÑÐ¾Ð´Ð½Ð¾ÑÑÐ¸ Ñ Ð½ÐµÐ¿ÑÐµÑÑÐ²Ð½Ð¾ ÑÐ°ÑÑÑÑÐµÐ¹ Ð½Ð°Ð¿Ð¾ÑÐ½Ð¾Ð¹ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¾Ð¹ Ð¸ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð½ÑÐ¼Ð¸ ÐºÐ°Ð²Ð¸ÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐ¼Ð¸ ÐºÐ°ÑÐµÑÑÐ²Ð°Ð¼Ð¸. Ð¡ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸ÐµÐ¼ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð¿ÑÐ¾ÑÐ¾ÑÐ½Ð°Ñ ÑÐ°ÑÑÑ ÐÐ¦ÐÐ Ð´Ð»Ñ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ´ÐµÑÐ½Ð¾Ð¹ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸ Ð½Ð° Ð±ÑÑÑÑÑÑ Ð½ÐµÐ¹ÑÐ¾Ð½Ð°Ñ ÐÐ ÐÐ¡Ð¢ ÐÐ-300.
HNCO abundances in galaxies: Tracing the evolutionary state of starbursts
Creators: name: Martin, Sergio
name: Martin-Pintado, J.
name: Mauersberger, R.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The chemistry in the central regions of galaxies is expected to be strongly influenced by their nuclear activity. To find the best tracers of nuclear activity is of key importance to understand the processes taking place in the most obscured regions of galactic nuclei. In this work we present multi-line observations of CS, C34S, HNCO and C18O in a sample of 11 bright galaxies prototypical for different types of activity. The 32S/34S isotopic ratio is ~10, supporting the idea of an isotopical 34S enrichment due to massive star formation in the nuclear regions of galaxies. Although C32S and C34S do not seem to be significantly affected by the activity type, the HNCO abundance appears highly contrasted among starburst. We observed HNCO abundance variations of nearly two orders of magnitude. The HNCO molecule is shown to be a good tracer of the amount of molecular material fueling the starburst and therefore can be used as a diagnostics of the evolutionary state of a nuclear starburst.
description: 21 pages, 3 figures, Accepted by ApJ
title: ÐÐµÑÐ¾Ð´ ÐºÐ¾Ð¼Ð¿Ð¾Ð·Ð¸ÑÐ¸Ð¸ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¾Ð² Ð¼Ð°ÑÐ¸Ð½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Oracle data mining Ð´Ð»Ñ Ð¿ÑÐ¾Ð³Ð½Ð¾Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÑÐ´ÐµÑÐ½Ð¾-ÑÐ¾ÑÑÐ´Ð¸ÑÑÑÑ Ð·Ð°Ð±Ð¾Ð»ÐµÐ²Ð°Ð½Ð¸Ð¹
title: Ensemble learning method based on Oracle data mining for cardiovascular diseases prediction
Creators: name: Ð¡Ð¾Ð±Ð¾Ð»ÐµÐ²Ð°, ÐÐ»ÐµÐºÑÐ°Ð½Ð´ÑÐ°
name: Ð¡Ð°Ð±Ð¸Ð½Ð¸Ð½, ÐÐ»ÐµÐ³
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2020
Subjects: Ð¼Ð°ÑÐ¸Ð½Ð½Ð¾Ðµ Ð¾Ð±ÑÑÐµÐ½Ð¸Ðµ
ÑÐµÑÐ´ÐµÑÐ½Ð¾-ÑÐ¾ÑÑÐ´Ð¸ÑÑÑÐµ Ð·Ð°Ð±Ð¾Ð»ÐµÐ²Ð°Ð½Ð¸Ñ

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description: The prediction problem, the existing machine learning methods and related issues are considered in the chapter. The modification of the bagging method, which aggregates two fundamentally different machine learning algorithms (Generalized Liner Model and Support Vector Machine), is proposed and justified. The research of the method based on three different heart disease datasets. It confirms the effectiveness of the method for solving problem of risk estimation of the cardiovascular disease.
The Immunization Agenda 2030 strategy to reach zero-dose children in low- and middle-income countries: a living scoping review protocol
Creators: name: Bangaman Christian Akani
name: Reynolds, Heidi W.
name: Beaulieu, Audrey
name: Johri, Mira
name: Ducharme, Joelle
name: Correa, Gustavo Caetano
name: Thibeault, Céline
Publisher: name: OSF Registries
Year: 2024
Subjects: subject: Immunology and Infectious Disease
subject: Maternal and Child Health
subject: Public Health
subject: Medicine and Health Sciences
subject: Life Sciences
subject: International Public Health

description: Launched in 2021 by WHO, UNICEF and Gavi, the Immunization Agenda 2030 (IA2030) is a global strategy to leave no one behind with immunisation. An important target to achieve by 2030 is to reduce by 50% the number of children completely missing out on vaccines (referred to as “zero-dose children”). According to the latest WHO/UNICEF Estimates of National Immunization Coverage (WUENIC), there were still 14.3 million zero-dose children worldwide in 2022. In low-income countries, these children account for almost half of vaccine-preventable deaths. Zero-dose vaccination status is also linked with poor health and developmental outcomes for children and is an early indicator of systematic disadvantage over the life course. As we approach the end of the Gavi 5.0 strategy period and the mid-term of IA2030, the world is struggling to recover from significant setbacks in coverage of essential childhood vaccinations caused by the COVID-19 pandemic - which disproportionally affected low-income countries and jeopardise the success of IA2030. There is thus an urgent need to better understand how to sustainably reach zero-dose children and missed communities to strengthen policy actions.

This living scoping review aims to map and synthesise what is known from the scientific literature about zero-dose children in low- and middle-income countries, in the context of the global IA2030 strategy. It will provide evidence for decision-makers to consider when planning for the remainder of the IA2030 strategic period (2021-2030), and for Gavi’s next strategic period, Gavi 6.0 (2026-2030). It is intended to provide updates on an annual or bi-annual basis for the remainder of the IA2030 strategic period and the planning and operationalisation of Gavi 6.0.
The effect of ram pressure on the star formation, mass distribution and morphology of galaxies
Creators: name: Kapferer, W.
name: Sluka, C.
name: Schindler, S.
name: Ferrari, C.
name: Ziegler, B.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We investigate the dependence of star formation and the distribution of the components of galaxies on the strength of ram pressure. Several mock observations in X-ray, H$α$ and HI wavelength for different ram-pressure scenarios are presented. By applying a combined N-body/hydrodynamic description (GADGET-2) with radiative cooling and a recipe for star formation and stellar feedback 12 different ram-pressure stripping scenarios for disc galaxies were calculated. Special emphasis was put on the gas within the disc and in the surroundings. All gas particles within the computational domain having the same mass resolution. The relative velocity was varied from 100 km/s to 1000 km/s in different surrounding gas densities in the range from $1\times10^{-28}$ to $5\times10^{-27}$ g/cm$^3$. The temperature of the surrounding gas was initially $1\times10^{7}$ K. The star formation of a galaxy is enhanced by more than a magnitude in the simulation with a high ram-pressure ($5\times10^{-11}$ dyn/cm$^2$) in comparison to the same system evolving in isolation. The enhancement of the star formation depends more on the surrounding gas density than on the relative velocity. Up to 95% of all newly formed stars can be found in the wake of the galaxy out to distances of more than 350 kpc behind the stellar disc. Continuously stars fall back to the old stellar disc, building up a bulge-like structure. Young stars can be found throughout the stripped wake with surface densities locally comparable to values in the inner stellar disc. Ram-pressure stripping can shift the location of star formation from the disc into the wake on very short timescales. (Abridged)
description: 19 pages, 25 figures, A&A accepted, high resolution version can be found at http://astro.uibk.ac.at/~wolfgang/kapferer_rps_galaxies.pdf
In/formal Credentials : Governing Open Badges
Creators: name: Fields, Erin
Publisher: name: The University of British Columbia
Year: 2016

description: While many conversations around open badges in academia highlight the potential for co-curricular records, skills-based credentials, and personalized learning data, the impact they may have on the formal academic learning ecosystem is difficult to determine. Badges are at the innovation stage, where badge projects are emerging but their success remains undefined and unproven. What badges will mean for university environments will require not only a larger number of implementations and assessment of outcomes, but also a clear idea of what badges mean in the academic environment and how they are governed. With the UBC Open Badges pilots, questions about governance, new forms of credentialing and authority are fast becoming issues that need to be addressed.
An X-ray View of Star Formation in the Central 3 kpc of NGC 2403
Creators: name: Yukita, Mihoko
name: Swartz, Douglas A.
name: Tennant, Allyn F.
name: Soria, Roberto
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Archival Chandra observations are used to study the X-ray emission associated with star formation in the central region of the nearby SAB(s)cd galaxy NGC 2403. The distribution of X-ray emission is compared to the morphology visible at other wavelengths using complementary Spitzer, GALEX, and ground-based Halpha imagery. In general, the brightest extended X-ray emission is associated with HII regions and to other star-forming structures but is more pervasive; existing also in regions devoid of strong Halpha and UV emission. This X-ray emission has the spectral properties of diffuse hot gas (kT ~ 0.2keV) whose likely origin is in gas shock-heated by stellar winds and supernovae with < 20% coming from faint unresolved X-ray point sources. This hot gas may be slowly-cooling extra-planar remnants of past outflow events, or a disk component that either lingers after local star formation activity has ended or that has vented from active star-forming regions into a porous interstellar medium.
description: 25 pages, accepted to AJ
Sinus Pericrani
Creators: name: Gracey, Gavin
Publisher: name: EURORAD
Year: 2014
Subjects: subject: Paediatric
subject: Conventional radiography
subject: Digital radiography
subject: MR
subject: Ultrasound-Colour Doppler
subject: Decision analysis
subject: Congenital
subject: Varices

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: female, 14 weeks
description: Clinical History: A 14 week old infant presented with a slowing enlarging occipital soft tissue swelling.  There was discolouration of the overlying skin and an abnormal tuft of dark hair.  No other medical issues were reported. Final Diagnosis: Sinus Pericrani
Dicke-Type Energy Level Crossings in Cavity-Induced Atom Cooling: Another Superradiant Cooling
Creators: name: Hirokawa, Masao
Publisher: name: arXiv
Year: 2008
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: This paper is devoted to energy-spectral analysis for the system of a two-level atom coupled with photons in a cavity. It is shown that the Dicke-type energy level crossings take place when the atom-cavity interaction of the system undergoes changes between the weak coupling regime and the strong one. Using the phenomenon of the crossings we develop the idea of cavity-induced atom cooling proposed by the group of Ritsch, and we lay mathematical foundations of a possible mechanism for another superradiant cooling in addition to that proposed by Domokos and Ritsch. The process of our superradiant cooling can function well by cavity decay and by control of the position of the atom, at least in (mathematical) theory, even if there is neither atomic absorption nor atomic emission of photons.
description: 15 pages; 8 figures