CHERNOBYL EXCLUSION ZONE - A WORLD FAMOUS TOURIST BRAND OF UKRAINE

Annotation. The article identifies the main principles of of functioning and development of the tourism in the Chornobyl radiation and ecological biosphere reserveaffected by the technogenic disaster. The paper provides a rationale fortourismdevelopmentto the Chernobyl exclusion zone as anew direction of the international tourism service market.It defines the main principles of planning and development of thebrand of “Chornobyl radiation and ecological biosphere reserve” (Chernobyl exclusion zone) and providesproposals for itspromotion astheworld-famous tourist brand of Ukraineon the international tourism service market through popularisation of the safe tours to Chernobyl exclusion zone.This article examines the important role of the state in the optimization and arrangementof the market participants activity in this region and tourist offers.The study has confirmedthe safety of the proposed tours with the assistance of specialists of the State Agency of Ukraine on the Exclusion Zone Management, the Chornobyl radiation and ecological biosphere reserve, and State specialised enterprise "Ecocentre". This paper proposes a number ofpractical measures in the context of the formation of the renewed Strategy of the Chernobyl exclusion zone development for optimization of the international tourism service marketthat will ensure the highest level of the travel market consumer's interest in purchasing tours to this region of Ukraine.Annotation. The article identifies the main principles of of functioning and development of the tourism in the Chornobyl radiation and ecological biosphere reserveaffected by the technogenic disaster. The paper provides a rationale fortourismdevelopmentto the Chernobyl exclusion zone as anew direction of the international tourism service market.It defines the main principles of planning and development of thebrand of “Chornobyl radiation and ecological biosphere reserve” (Chernobyl exclusion zone) and providesproposals for itspromotion astheworld-famous tourist brand of Ukraineon the international tourism service market through popularisation of the safe tours to Chernobyl exclusion zone.This article examines the important role of the state in the optimization and arrangementof the market participants activity in this region and tourist offers.The study has confirmedthe safety of the proposed tours with the assistance of specialists of the State Agency of Ukraine on the Exclusion Zone Management, the Chornobyl radiation and ecological biosphere reserve, and State specialised enterprise "Ecocentre". This paper proposes a number ofpractical measures in the context of the formation of the renewed Strategy of the Chernobyl exclusion zone development for optimization of the international tourism service marketthat will ensure the highest level of the travel market consumer's interest in purchasing tours to this region of Ukraine

Correlation investigation of the brightness of GDE-grams using the methods of computer graphics and direct measurements

There are two methods of measuring the glow of a liquid under the conditions of gas-discharge imaging. This is a investigation of the brightness of GD-grams - a digital image of streamers created under these conditions, and a direct measurement of brightness using a luminometer, which is carried out during the formation of a streamer during a gas discharge. In the first case, the digital image is analyzed using computer graphics methods and certain software. In the second, the results of direct measurement are analyzed. We have analyzed these two methods using the example of the glow of water under the conditions of gas-discharge visualization. It is shown that with direct measurements the brightness values ​​are higher than when investigating the brightness of a digital image of the same streamer obtained in the same time period. Namely 1.5 cd/m2 and 1.7 cd/m2. The difference is 13% and significantly exceeds the measurement error of the brightness meter (± 7%). According to the results of our research, we suggest that, at the very least, when calibrating the devices that create the GDV-grams, use direct measurements of the glow of the liquid in photometric units. For example, in brightness units

New Computer System for Recognizing Micro- and Nano-Sized Objects in Semiconductors and Colloidal Solutions

In this paper it is describe a new approach developed for recognizing micro- and nano-sized objects and a method for quantitative analysis of these objects. For this purpose was developed the automated systems that can simplify and accelerate the process of nanoparticle tracks analysis under the microscope whereby engineers and scientists are able to recognize the structures of defects in semiconductor wafers, along with nanoparticles and other microscopic objects. This capability is important to both select appropriate crystals and also to apply the data to improve the production process

Совершенствование методов определения частотно-инерционных и кинематических свойств систем с распределенными параметрами путем анализа их собственных колебаний

Досліджено коливання (вільні) тонкого диску. Визначено співвідношення для товстих дисків, які враховують інерцію обертання та зсув. Побудовано залежності резонансної частоти коливань диску з вузловими колами.Free vibrations of the thin disc are studied. The equation for thick discs which include the inertia of rotation and the slide is determined. The dependencies of the resonant frequency of oscillation with knotty circles are made.Исследованы колебания (свободные) тонкого диска. Определены соотношения для толстых дисков, которые учитывают инерцию вращения и смещение. Построены зависимости резонансной частоты колебаний диска с узловыми кругами

ОСНОВНІ ВИМОГИ ДО СТРУКТУРИ ТИПОВИХ МЕДИЧНИХ ІНФОРМАЦІЙНИХ СИСТЕМ В УПРАВЛІННІ ОХОРОНОЮ ЗДОРОВ'Я

In modern development of health care for providing proper quality of medicare there is a necessity in accumulation and analysis of data during the long period, application of electronic and consulting models. The presented work determines basic principles of construction of the informative systems for optimization of management of health care establishments, first of all, at making decisions. Basic tasks and requirements to the informative systems on regional and local levels are considered. It is proven that typical structures of the medical informative systems must have possibilities of risks monitoring for patients and decisions as to danger identification for managers.В сучасних умовах розвитку охорони здоров’я для забезпечення належної якості медичної допомоги існує потреба в накопиченні й аналізі даних впродовж тривалого періоду, застосуванні електронних експертних систем. Представлена робота визначає основні принципи побудови інформаційних систем для оптимізації управління закладами охорони здоров’я, насамперед, при прийнятті рішень. Розглянуті основні завдання та вимоги до інформаційних систем на регіональному і локальному рівнях. Доведено, що типові структури медичних інформаційних систем повинні мати можливості моніторингу ризиків для пацієнтів і рішення щодо ідентифікації небезпеки для  управлінців

VODKA-JWST: Synchronized growth of two SMBHs in a massive gas disk? A 3.8 kpc separation dual quasar at cosmic noon with JWST NIRSpec IFU

The search for dual supermassive black holes (SMBHs) is of immense interest in modern astrophysics. Galaxy mergers may be an important route to fuel and to produce SMBH pairs. Actively accreting SMBH pairs can be observed as a dual quasar, which are vital probes of SMBH growth. Gaia observations have enabled a novel technique to systematically search for such dual quasars at previously unreachable sub-kpc scales, based on the small jitters of the light centroid as the two quasars vary stochastically. Here we present the first detailed study of a 0.46'', 3.8 kpc separation, VODKA-selected dual quasar, J0749+2255, at $z=2.17$ using JWST/NIRSpec integral field unit spectroscopy. This is one of the most distant, small separation dual quasars identified today. Dual quasars at cosmic noon are not well characterized. We detect the faint ionized gas of the host galaxy, best traced by the narrow \ha\ emission. Line ratio diagnostics show a mix of ionization from the two quasars and intense star formation. The spatially-resolved spectra of the two quasars suggest that they have very similar black hole properties (two $M_{BH}\sim 10^9\ \textrm{M}_{\odot}$with large Eddington ratio reaching$L/L_{Edd}\sim0.2$) hinting at the possible synchronized growth and accretion from the same gas supply. Surprisingly, the ionized gas kinematics suggest an extended, rotating disk rather than a disturbed system that would be expected in a major gas-rich galaxy merger. While it is unclear if J0749+2255 is representative of the dual quasar evolution, the observations with JWST revealed a major puzzle. It would be interesting to see what observations of other dual quasars will show.Comment: 21 pages, 9 figures, submitte

VODKA-JWST: A 3.8 kpc dual quasar at cosmic noon in a powerful starburst galaxy with JWST/MIRI IFU

Dual quasars, two active supermassive black holes at galactic scales, represent crucial objects for studying the impact of galaxy mergers and quasar activity on the star formation rate (SFR) within their host galaxies, particularly at cosmic noon when SFR peaks. We present JWST/MIRI mid-infrared integral field spectroscopy of J074922.96+225511.7, a dual quasar with a projected separation of 3.8 kilo-parsec at a redshift $z$ of 2.17. We detect spatially extended [Fe II] 5.34$\rm \mu$m and polycyclic aromatic hydrocarbon (PAH) 3.3$\mu$m emissions from the star formation activity in its host galaxy. We derive the SFR of 10$^{3.0\pm0.2}$ M$_{\odot}$ yr$^{-1}$ using PAH 3.3$\mu$m, which is five times higher than that derived from the cutoff luminosity of the infrared luminosity function for galaxies at $z\sim2$. While the SFR of J0749+2255 agrees with that of star-forming galaxies of comparable stellar mass at the same redshifts, its molecular gas content falls short of expectations based on the molecular Kennicutt-Schmidt law. This discrepancy may result from molecular gas depletion due to the longer elevated stage of star formation, even after the molecular gas reservoir is depleted. We do not observe any quasar-driven outflow that impacts PAH and [Fe II] in the host galaxy based on the spatially resolved maps. From the expected flux in PAH-based star formation, the [Fe II] line likely originates from the star-forming regions in the host galaxy. Our study highlights the stardust nature of J0749+2255, indicating a potential connection between the dual quasar phase and intense star formation activities.Comment: 12 pages, 7 figures, 1 table, submitted to ApJ, comments are welcom

ДОСВІД ВИЗНАЧЕННЯ ІНТРАТЕКАЛЬНОГО СИНТЕЗУ АНТИТІЛ У ПАЦІЄНТІВ З УРАЖЕННЯМИ ЦЕНТРАЛЬНОЇ НЕРВОВОЇ СИСТЕМИ

The aim of the work – to study the frequency of intrathecal synthesis of specific antibodies at patients with inflammatory lesions of the central nervous system.Patients and methods. In this work the data of the determination of intrathecal synthesis of specific antibodies (ITSA) in 90 patients are given who were treated at the Lev Hromashevskyi Institute of Epidemiology and Infectious Diseases. The research included quantitative definition of antibodies of the class IgG in serum (S) and cerebrospinal fluid (CSF) to neurotropic pathogens: herpes simplex virus 1/2, cytomegalovirus, Epstein-Barr virus, varicella zoster virus, rubella virus, Borrelies. Calculations of ITSA indicators were carried out according to the method of Reiber H. The condition of a hematoencephalic barrier (HEB) was estimated by means of coefficient of albumine (Qalb) taking into account age norms.Results. ITSA was established in (25.6±4.6) % of the examined patients with damages of the central nervous system. In patients with ITSA most often (in 52.2 %) simultaneously present antibodies to several neurotropic pathogens. Detection of ITSA at the examined patients didn’t depend on concentration of specific antibodies in S and CSF and wasn’t followed by malfunction of HEB. The incidence of HEB dysfunction at patients with ITSA and without ITSA appeared with an identical frequency (13,0 % and 13,6 % respectively).Мета роботи. Вивчити частоту інтратекального синтезу специфічних антитіл у пацієнтів зі запальними ураженнями центральної нервової системи.Пацієнти і методи. В роботі наведені дані визначення інтратекального синтезу специфічних антитіл (ІТСА) у 90 пацієнтів, які проходили лікування в клініці ДУ «Інститут епідеміології та інфекційних хвороб ім. Л.В. Громашевського». Дослідження включало кількісне визначення антитіл класу Ig G в сироватці крові (СК) та спинномозковій рідині (СМР) до нейротропних збудників: вірусу простого герпесу 1/2 типу, цитомегаловірусу, вірусу Епштейна-Барр, вірусу оперізувального лишаю, вірусу кору, вірусу краснухи, бореліям. Розрахунки показників ІТСА проведені за методикою Reiber H. Стан гематоенцефалічного бар’єру (ГЕБ) оцінювали за допомогою коефіцієнту альбуміну (Qalb) з урахуванням вікових норм.Результати. ІТСА встановлений у (25,6±4,6) % обстежених пацієнтів з ураженнями ЦНС. У пацієнтів з ІТСА найчастіше (у 52,2 %) одночасно були присутні антитіла до декількох нейротропних збудників. Виявлення ІТСА в обстежених пацієнтів не залежало від концентрації специфічних антитіл у СК і СМР і не супроводжувалося порушенням функції ГЕБ. Випадки дисфункції ГЕБ у пацієнтів з ІТСА та без ІТСА виявлялися з однаковою частотою (13,0 та 13,6 % відповідно)

First results from the JWST Early Release Science Program Q3D: Benchmark Comparison of Optical and Mid-IR Tracers of a Dusty, Ionized Red Quasar Wind at z=0.435

The [OIII] 5007 A emission line is the most common tracer of warm, ionized outflows in active galactic nuclei across cosmic time. JWST newly allows us to use mid-infrared spectral features at both high spatial and spectral resolution to probe these same winds. Here we present a comparison of ground-based, seeing-limited [OIII] and space-based, diffraction-limited [SIV] 10.51 micron maps of the powerful, kpc-scale outflow in the Type 1 red quasar SDSS J110648.32+480712.3. The JWST data are from the Mid-InfraRed Instrument (MIRI). There is a close match in resolution between the datasets (0."4--0."6), in ionization potential of the O+2 and S+3 ions (35 eV), and in line sensitivity (1e-17 to 2e-17 erg/s/cm2/arcsec2). The [OIII] and [SIV] line shapes match in velocity and linewidth over much of the 20 kpc outflowing nebula, and [SIV] is the brightest line in the rest-frame 3.5--19.5 micron range, demonstrating its usefulness as a mid-IR probe of quasar outflows. [OIII] is nevertheless intriniscally brighter and provides better contrast with the point-source continuum, which is strong in the mid-IR. There is a strong anticorrelation of [OIII]/[SIV] with average velocity, which is consistent with a scenario of differential obscuration between the approaching (blueshifted) and receding (redshifted) sides of the flow. The dust in the wind may also obscure the central quasar, consistent with models that attribute red quasar extinction to dusty winds.Comment: Submitted to ApJ

First results from the JWST Early Release Science Program Q3D: Ionization cone, clumpy star formation and shocks in a z=3z=3 extremely red quasar host

Massive galaxies formed most actively at redshifts $z=1-3$ during the period known as `cosmic noon.' Here we present an emission-line study of an extremely red quasar SDSSJ165202.64+172852.3 host galaxy at $z=2.94$, based on observations with the Near Infrared Spectrograph (NIRSpec) integral field unit (IFU) on board JWST. We use standard emission-line diagnostic ratios to map the sources of gas ionization across the host and a swarm of companion galaxies. The quasar dominates the photoionization, but we also discover shock-excited regions orthogonal to the ionization cone and the quasar-driven outflow. These shocks could be merger-induced or -- more likely, given the presence of a powerful galactic-scale quasar outflow -- these are signatures of wide-angle outflows that can reach parts of the galaxy that are not directly illuminated by the quasar. Finally, the kinematically narrow emission associated with the host galaxy presents as a collection of 1 kpc-scale clumps forming stars at a rate of at least 200 $M_{\odot}$ yr$^{-1}$. The ISM within these clumps shows high electron densities, reaching up to 3,000 cm$^{-3}$ with metallicities ranging from half to a third solar with a positive metallicity gradient and V band extinctions up to 3 magnitudes. The star formation conditions are far more extreme in these regions than in local star-forming galaxies but consistent with that of massive galaxies at cosmic noon. JWST observations reveal an archetypical rapidly forming massive galaxy undergoing a merger, a clumpy starburst, an episode of obscured near-Eddington quasar activity, and an extremely powerful quasar outflow simultaneously.Comment: 19 pages, 8 figures. Accepted for publication in Ap