Viktor Voropaev, Igor Molotov Roscosmos delegation KIAM RAS

Slides:

Advertisements

Similar presentations

HOU in Russia Irina GUSEVA St Petersburg - Central (Pulkovo) Astronomical Observatory of the Russian Academy of Sciences - St Petersburg State University,

Advertisements

Research Centre of Astronomy and Geophysics Mongolian Academy of Sciences Study of near-earth objects in Mongolia. Space debris, asteroids and comets Outreach.

Optical Astronomy Final Year Double Honours Presentation Eoin Cartwright & John Loughran. Supervisor: Dr Créidhe Ní Shúilleabháin.

4 th SONG WORKSHOP Charleston, SC Sep 2011 The Virgin Islands Robotic Telescope James E. Neff College of Charleston & David Morris University of.

David Haworth Copyright 2001 Imaging the Sky 2001.

An Introduction to mini-SONG Project Xiaojun Jiang Natioanl Astronomical Observatories Chinese Academy of Sciences.

The Nearby Supernovae Factory: Spectrograph Calibration Ben Dilday Advisor: Rick Kessler, CfCP Physics 335 Autumn 2003.

Model of the Seasons Josh Kratzer, Carly Reed, Feliciti Fredsti, Dr. Bruce Palmquist, Dr. Tim Sorey, Dan Durr* Department of Physics, Central Washington.

(1): Observatori Fabra, Reial Acadèmia de Ciències i Arts de Barcelona Fabra-ROA Baker-Nunn camera at Observatori Astronòmic del Montsec: an instrument.

International collaboration as a primary way for the ISON network development Igor Molotov, Vladimir Agapov Russian Academy of Sciences Keldysh Institute.

MONGOLIAN-RUSSIAN COOPERATION IN KHURELTOGOOT OBSERVATORY IN THE ISON PROJECT FRAMEWORK N.Tungalag 1, I.Molotov 2, V.Voropaev 2, V.Kouprianov 3, Yu.Krugly.

Prime Focus Option (Ming Liang) Actuator Intro/Overview/Status Prime focus slides from M. Liang (NOAO) M. Sholl University of California at Berkeley Space.

3rd Integral Bart Work Shop Chocerady - November 1-3, Patrizia Ferrero GRB Too observations in Loiano Patrizia Ferrero (IASF-BO, OACT & Universita’

Engineering: NAHUAL Ireland Acquisition Camera, Focal Plane Mechanisms and Layout Tully Peacocke, National University of Ireland Maynooth Carlos del Burgo,

Research and Imaging Program for the SVAS. Current Situation Society supports beginners well –Messier Group –Community Outreach programs Monthly star.

The Chinese SONG proposal: scientific concerns Jianning Fu (Beijing Normal University) and Chinese SONG team Beijing ─ March 29, 2010 The third workshop.

ISON dedicated survey instruments development Igor Molotov, Vladimir Agapov Russian Academy of Sciences Keldysh Institute of Applied Mathematics 64th International.

The Second International Workshop on Ultra-high-energy cosmic rays and their sources INR, Moscow, April 14-16, 2005 from Extreme Universe Space Observatory.

New dedicated observation facilities for near-Earth space monitoring Molotov I., Agapov V., Sokolov N. Roscosmos delegation 29th IADC Meeting Berlin, Germany.

Upgrade plan of the MOA 1.8-m telescope F. Abe MOA collaboration 19 Jan. 2009, 13th Microlensing Paris.

Mechanical Structure „Pi of the Sky” robotic telescope mgr inż. Robert Pietrzak mgr inż. Piotr Wawer mgr inż. Roman Wawrzaszek –

ISON-NM Observatory capabilities for Gaia-FUN-SSO support CoLiTeC image processing pipeline for moving objects detection L. Elenin¹, V. Savanevych², I.

is transparent ERAU Astronomical Observatory Meade inch Schmidt Cassegrain Reflecting Telescope.

Exoplanet Transit Observations at Weihai Observatory of Shandong University Chen CAO

Database of Variable Stars Bingqiu Chen Dept of Astronomy Beijing Normal University.

Pachon Sky Camera Christopher Stubbs Chuck Claver Jan 25, 2014.

Short overview of activities performed under Roscosmos and RAS auspices in 2014 in the area of space debris monitoring Nikolay Sakva, Vladimir Agapov,

Astronomical Institute University of Bern 31 th IADC Meeting, April , 2013, ESOC, Darmstadt, Germany Catalogue of High AMR GEO-like Debris T. Schildknecht,

Telescopes. Light Hitting a Telescope Mirror huge mirror near a star * * * small mirror far from 2 stars In the second case (reality), light rays from.

OBSERVATION OF SPACE DEBRIS AND GEO SATELLITES IN DERENIVKA, UKRIANE V.Yepishev, V.Kudak, V.Perig, I.Motrunych, I.Nojbauer. Laboratory of the space researches.

Vladimir Agapov and Igor Molotov

The Auger Observatory for High-Energy Cosmic Rays G.Matthiae University of Roma II and INFN For the Pierre Auger Collaboration The physics case Pierre.

Active Optics and Wavefront Sensing at the Upgraded 6.5-meter MMT Xiaoyin Zhu Dec 12, 2012 OPTI 521 Paper Synopsis By T.E. Pickering, etc.

Mahfuz Krueng Asteroid 1825 Klare (1954 QH) Klare Objectives What and Where? Observation Data Analysis Previous Research Further Works.

Telescopes Resolution - Degree to which fine detail can be distinguished Resolution - Degree to which fine detail can be distinguished Fundamentally an.

System Performance Metrics and Current Performance Status George Angeli.

Hubble Space Telescope By Brittany Bellows Physics 1040 – Spring 2011.

DAO Observations and Instrumentation Jason Grunhut.

Results of GEO and HEO monitoring by ISON network in th session of STSC COPUOS Vienna Feb 2013 Russian Academy of Sciences Keldysh Institute.

Updated information on high altitude HAMR objects tracking by ISON Vladimir Agapov, Igor Molotov Roscosmos delegation Presentation for the WG1 session.

ISON network development in Molotov I., Agapov V. Roscosmos delegation 30th IADC Meeting Montreal, Canada May 22-25, 2012.

Update on results of Molniya-type HEO surveys performed by ISON in 2014 Vladimir Agapov (KIAM RAS) Roscosmos delegation Presentation for the WG1 session.

Remote observatory ISON-NM Survey of Minor Solar System bodies L. Elenin¹, I. Molotov¹, V. Savanevich², A. Kozhukhov³, A. Bryukhovetskiy³, V. Vlasenko³,

HOW TO SELECT DOUBLE STARS FOR OBSERVATION GENERAL CONSIDERATIONS UNDERSTANDING WDS DATA USING THE SKY X ON BARC0 TO CONFIRM YOUR PLAN OTHER PLANETARIUM.

11 – 13 May 2016 Osservatorio Polifunzionale del Chianti Use of SMALL TELESCOPES in the GIANT ERA Italo Foppiani – Technical manager In collaboration with.

Telescopes I. Refraction: Refraction is the _____________ of light as it passes through glass. II. Reflection: Reflection occurs when light _____________.

ISON network development in

V. Agapov, N. Sakva, D.Davydov, E.Katkova

Indian Astronomical Observatory

Igor Molotov Keldysh Institute of Applied Mathematics RAS,

X Serbian-Bulgarian Astronomical Conference (X SBAC)

Recent Results and Future Improvements

Current status of the ISON optical network

Goal Automatize of the VORT

GMV/ISON COMBINED OPTICAL CAMPAIGNS

Vladimir Agapov, Igor Molotov, Victor Stepanyants

(1): Observatori Fabra, Reial Acadèmia de Ciències i Arts de Barcelona

C2PU TELESCOPES Version 02, 28/08/2016 Jean-Pierre Rivet CNRS, OCA,

Detectors of the New Projects at NAOC

ISON Network Tracking of Space Debris: current status and achievements

SLAC DOE Program Review

Vladimir Agapov, Igor Molotov, Nikolay Sakva

V. Agapov, D. Zelenov 35th IADC meeting Darmstadt, April 2017

NEARBY Platform for Automatic Asteroids Detection and EURONEAR Surveys

Texas Tech University Department of Physics and Astronomy

TRAINEE PRESENTATION The North and South Ecliptic Pole fields population Project supervisors: R. Saxton N. Loiseau Trainee student: Jaime Abella Payá.

7-th European Space Debris Conference 2017

Caucasian Mountain Observatory SAI MSU

Presentation transcript:

Viktor Voropaev, Igor Molotov Roscosmos delegation KIAM RAS First results of observations with 80-cm telescope at peak Terskol, North Caucasus Viktor Voropaev, Igor Molotov Roscosmos delegation KIAM RAS IADC 35th Darmstadt, Germany ― WG1 April 24 – 26, 2017

Terskol observatory Peak Terskol Observatory is situated at altitude of 3100 m in North Caucasus on the Elbrus mountainside

Map of observatories that send the data to KIAM

80-cm Cassegrain telescope K-800 It was installed in the 70-ies and working about 10 years. Then it was stopped and dismantled (secondary mirror was lost Telescope was upgraded by setting up the lens corrector for improving and enlarging of FOV and motors with controller for automation of operations

Setting up of lens corrector, CCD camera FLI PL09000 (3k x 3k, 12 µm) and Atlas focuser

Updated K-800: FOV=55 x 55 minutes

Observation statistics (telescope is exploited with expeditions)

Histogram of object size Data from telescope are used to calibrate the space debris population SDPA model Histogram of GEO SO magnitude in experimental measurements Histogram of object size estimations

Future update of K-800 telescope Re-aluminization of the main mirror to improve limiting magnitude Installation of new 2k x 2k CCD camera FLI PL4301E having 24µm pixels to enlarge FOV Installation UBVRI ﬁlter wheel to start photometry observations Control system renewal and stepper motors replacement by DC motors with encoders to improve the throughput of telescope To change CHAOS control software on FORTE to increase stability of operations

Conclusion ISON project is replenished with new respectively large telescope situated at 3100 m altitude in place with good quality of atmosphere This is very powerful instrument for faint space debris observations Now this is most large telescope that can spent 100% observation time for the project goals Limiting magnitude is down to 18.5 now. It is expected that it will be improved down to 19.5 after re-aluminization of the main mirror Current FOV is 55 x 55 minutes. It is expected that this will be enlarged to 75 x 75 minutes with new CCD camera Obtained measurements are used to calibrate the space debris population SDPA model