A5024553013- Photocathodes and Microchannel Plates
- Atmospheric Ozone and Climate
- Astronomical Observations and Instrumentation
- Astro and Planetary Science
- Calibration and Measurement Techniques
- Astronomy and Astrophysical Research
- Stellar, planetary, and galactic studies
- Planetary Science and Exploration
- Adaptive optics and wavefront sensing
- CCD and CMOS Imaging Sensors
- Solar and Space Plasma Dynamics
- Gamma-ray bursts and supernovae
- Space exploration and regulation
- Space Satellite Systems and Control
- Spacecraft Design and Technology
- Advanced Semiconductor Detectors and Materials
- Astrophysics and Star Formation Studies
- solar cell performance optimization
- Spacecraft and Cryogenic Technologies
- Infrared Target Detection Methodologies
- Computational Physics and Python Applications
- History and Developments in Astronomy
- Field-Flow Fractionation Techniques
- Advanced X-ray Imaging Techniques
- Radioactive Decay and Measurement Techniques
Institute of Astronomy
2013-2024
Russian Academy of Sciences
2008-2024
Special Astrophysical Observatory
2024
Institute of Applied Astronomy
2009-2022
Space Research Institute
2021
P.N. Lebedev Physical Institute of the Russian Academy of Sciences
2020
Universidad Complutense de Madrid
2020
International Society for Optics and Photonics
2015
В работе предложена концепция широкоугольного УФ телескопа небольшой апертуры для проведения обзорных наблюдений в с поверхности Луны целью устранения неполноты каталога УФ-источников GALEX, а также решения ряда других научных задач, решение которых затруднено при использовании наземных телескопов. Кратко рассмотрены варианты оптической схемы, способов наведения телескопа, предложены научные светофильтры и современный КМОП детектор. We present the concept of a small-aperture wide field UV...
Spektr–UF (World Space Observatory Ultraviolet, WSO-UV) is a Russian-led international collaboration aiming to develop large space-borne 1.7 m Ritchey–Chretién telescope with science instruments study the Universe in ultraviolet wavelengths. The WSO-UV spectrograph (WUVS) consists of three channels: two high-resolution channels (R = 50,000) spectral ranges 115–176 nm and 174–310 nm, low-resolution 1000) channel range 115–305 nm. Each has an almost identical custom detector consisting CCD...
The WSO-UV project is an efficient multipurpose orbital observatory for high sensitivity imaging. imaging instrument Field Camera Unit (FCU) onboard will be the first UV camera to flown a geosynchronous orbit. planned operate at least five years and perhaps longer. open new opportunities in planetary science, stellar astrophysics, extragalactic astronomy cosmology. This paper provides information on updated FCU instrument.
As part of a strategy to provide increasingly complex systems customers, e2v is currently developing the sensor solution for focal plane array WSO-UV (World Space Observatory – Ultraviolet) programme, Russian led 170 cm space astronomical telescope. This fully integrated system detection UV light across 3 channels: 2 high resolution spectrometers covering wavelengths 115 176 nm and 174 310 Long-Slit Spectrometer nm. paper will describe systematic approach technical that has been developed...
Abstract Chelyabinsk event of Feb 15, 2013 clearly demonstrated that decameter sizeNear EarthObjects (NEO) should be considered as hazardous ones. Another important lesson is bodies approaching the Earth from day sky could not discovered by any ground-based or near space telescopes and only way to detect these reasonably well beforehand put telescope(s) relatively far fromthe Earth.We proposed project system SODA (System Observation Day-time Asteroids) for exhaustive detection (and larger)...
World Space Observatory Ultraviolet (WSO-UV) is a major Russian-led international collaboration to develop large Space-borne 1.7 m Ritchey-Chrétien telescope and instrumentation study the Universe in ultraviolet wavelengths. The WSO-UV WUVS spectrograph consists of three channels: two high resolution channels (R=50000) with spectral ranges 115-176 nm 174-310 nm, low (R=1000) channel range 115-305 nm. Each has an almost identical custom detector consisting CCD inside vacuum Enclosure, drive...
The World Space Observatory UltraViolet (WSO-UV) project is an international space observatory designed for observations in the ultraviolet domain. includes a single 170 cm aperture telescope capable of high-resolution spectroscopy, long slit low-resolution spectroscopy and deep UV optical imaging.
A new wide-field optical instrument of the Institute Astronomy Russian Academy Sciences (INASAN) is described. It has been implemented under bilateral Russia--Uzbekistan collaboration in astronomy 2023–2025. The comprises four identical 28-cm aperture telescopes on a common mount designed for all-sky surveys and photometry. For single exposure, cluster takes an image 7 square degree field photometric bands simultaneously with 1.26 $''$/px scale. technical optoelectronic characteristics are...
The international collaboration between Russia and Cuba in astronomical research first began 2017. 20-cm robotic telescope of the Russian-Cuban network has been operating since 2021 Havana. construction second 50-cm underway 2023, it is expected to be finished installed 2025 near Kislovodsk (Russia). By 2030, plan build third 1-m at Valle de Picadura (Cuba). We describe main parameters scientific equipment new discuss its role distributed global network.
The ``Milky Way'' space safety program is under development in Russia. A part of the implies launch a special spacecraft aimed to detect decameter asteroids coming from day sky (from sunward hemisphere) as well predict weather and monitor Sun's activity. will be launched Sun–Earth L1 point. payload SODA (System for Observation Daytime Asteroids) at INASAN. concept based on results previous, conceptual, phase project. We present general outline give some new features more detail. IKI RAS...
The main instrument of the space mission "Spectr-UF" (World Space Observatory-Ultraviolet) is a large telescope to work in UV wavelength domain (115 - 310 nm). WSO-UV feeds its focal plane two instruments: unit spectrographs WUVS, and field camera FCU, as well Fine Guidance System (FGS). imaging FCU onboard will be first flown geosynchronous orbit. Here we provide brief description on updated current status.
Spectr-UV/WSO-UV is the third and last of Spektr missions (Spektr-Radio, Spektr-RG, Spektr-UF), space-based observatories, Russian Scientific Space Program. Spektr-UF/WSO-UV a 2-m class ultraviolet (UV) observatory to be set in geosynchronous orbit 2025 from Vostochny launching pad. The equipped with instrumentation for UV spectroscopy imaging. Universidad Complutense de Madrid together Institute Astronomy Academy Sciences are developing jointly imaging instrument mission. has UV-optical...