Ultra-Violet Imaging Telescope for ASTROSAT

Slides:



Advertisements
Similar presentations
1 ATST Imager and Slit Viewer Optics Ming Liang. 2 Optical layout of the telescope, relay optics, beam reducer and imager. Optical Layouts.
Advertisements

A detailed simulation study of the ASTROSAT-LAXPC WAPP-2013, Bose Institute, December 2013 Biplab Bijay
ASTROSAT LAXPC Biswajit Paul Raman Research Institute, Bangalore On behalf of the LAXPC Team.
ASTROSAT Prospects for a Hard X-ray Survey  ASTROSAT Overview  LAXPC Details  Science Prospects  Hard X-ray Survey Prospects  Beyond ASTROSAT Biswajit.
Coronas-Photon Project The RT-2 experiment. CORONAS-PHOTON mission is the third satellite of the Russian CORONAS program on the Solar activity observations.
Workshop „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, RHESSI and SPIRIT Instruments”, 6 – 8 December 2005, Wrocław Spectroscopy Department.
Light and Telescopes Please pick up your assigned transmitter
What we call “light” is only one type of … Electromagnetic Radiation – a way in which energy moves through space. Do not confuse EM radiation with Particle.
Optical Astronomy Imaging Chain: Telescopes & CCDs.
SWD 2005, Taormina, Jun,19-26 An EUV Imaging Detector of Space Solar Telescope Qian Song, Binxun Ye, Zhaowang Zhao National Astronomical Observatories,
The HEROES Balloon- borne Hard X-ray Telescope Colleen A. Wilson-Hodge, J. Gaskin, S. Christe, A. Shih, K. Kilaru, D.A. Swartz, A. F. Tennant, B. Ramsey.
Status of the Astrosat mission
X-ray transients with Astrosat
And a head sensor on a sun tracker What is PANDORA? Pandora is a small spectrometer system, which we have been developing since It consists of …
Low Energy, Low Cost Swift A design experiment June 2010.
5/21/2015G.C.Stewart Berlin 1 ASTROSAT: A Multi-Wavelength Satellite 1st Dedicated Indian Astronomical Mission ISRO Satellite Centre (ISAC), Bangalore.
A student satellite initiative Indian Institute of Technology Madras.
Astro-E2 and Japanese future space programs for high energy astrophysics Astro-E2 NeXT XEUS Small satellite programs Tadayasu Dotani (ISAS)
Telescopes and Spacecraft Astronomy 311 Professor Lee Carkner Lecture 7.
LXO/MagEX Meeting Greenbelt, 24/10/07 Telescope Baseline Configuration: Imaging Capability (Micropore Optic) Telescope Field of View ~ 30° x 30° Angular.
Swift 1 Swift Spacecraft and Instruments. Swift 2 Spacecraft Design 1 of 6 Reaction wheels Gyros Star Trackers.
Wide-field, triple spectrograph with R=5000 for a fast 22 m telescope Roger Angel, Steward Observatory 1 st draft, December 4, 2002 Summary This wide-field,
Radio Emission from Masuda Sources New Jersey Institute of Technology Sung-Hong Park.
2nd Zwicky Informal Workshop - Berkeley 2005 May 26, 2005John Vallerga John Vallerga, Barry Welsh, Anton Tremsin, Jason McPhate and Oswald Siegmund Experimental.
Science Specification of SOLAR-C payload SOLAR-C Working Group 2012 July 23.
SXT Soft X-Ray Telescope Onboard the Yohkoh Satellite SXT.ppt.
Indian Astronomy Satellite Mission (ASTROSAT) National Institutions 1.ISRO, Bangalore 2.TIFR, Mumbai 3.IIA, Bangalore 4.RRI, Bangalore 5.PRL, Ahmedabad.
X-ray Timing and Polarization mission & instrumentation DONG Yongwei Center for Particle Astrophysics Institute of High Energy Physics, Chinese Academy.
BRITE-Constellation consists of six nano-satellites: UniBRITE and BRITE-AUSTRIA (TUGSAT-1) are funded by Austria, two more by.
RELEC project (Relativistic ELECtrons). Unified platform “Karat” for small spacecraft 2 MICROSATELLITE KARAT FOR PLANETARY MISSIONS, ASTROPHYSICAL AND.
The Hard X-ray Modulation Telescope Mission
Cosmic Origins Spectrograph Hubble Space Telescope James C. Green University of Colorado Cosmic Origins Spectrograph Instrument Design and Capabilities.
TESIS on CORONAS-PHOTON S. V. Kuzin (XRAS) and TESIS Team.
Gamma-Ray Bursts observed with INTEGRAL and XMM- Newton Sinead McGlynn School of Physics University College Dublin.
5.1 Optical Observatories 5.1 a: Observatory Sites: One limitation: the time needed for optics to reach equilibrium shape when exposed to severe temperatures.
IIA Sept UVIT gratings and science Science meeting Sept 2006 J. Hutchings.
VLST workshop; STScI February UV astronomy in the post- GALEX era Noah Brosch Wise Observatory Tel Aviv University Israel.
1 5-9 October th ICATPP, Como, Italy S. Maltezos NITROGEN MOLECULAR SPECTRA OF AIR FLUORESCENCE EMULATOR USING A LN 2 COOLED CCD S. Maltezos, E.
What does mean neighbours ? At the same epoch –simultaneous (transient phenomenae) –before (can affect the SIMBOL-X observing plan) –after (can complement.
Scanning sky monitor (SSM) Technical Physics Division, ISAC & Astrophysics Group, RRI.
Silicon Optics for Wide Field X-ray Imaging Dick Willingale et al. – SPIE August 2013 Silicon Optics for Wide Field X-ray Imaging Dick Willingale University.
Science Lessons Learned from TESIS and their Relevance to SWAP V. Slemzin, LPI PROBA 2 SWT, La Roche, 14 June 2010.
MONITOR OF SOLAR EUV/XUV IRRADIATION PHOKA A. Kochemasov Astrophysics institute at Moscow engineering-physics institute.
Optical characteristics of the EUV spectrometer for the grazing-incidence region L. Poletto, G. Tondello Istituto Nazionale per la Fisica della Materia.
1 Overview of Existing and Planned X-ray Spectroscopy Missions Wilton Sanders Science Mission Directorate Universe Division NASA Headquarters ITAMP Workshop.
Observation of cosmic gamma-ray bursts and solar flares in the ''RELEC'' experiment on the ''VERNOV'' satellite.
Some results of observation of ultraviolet and infrared emission from lightning discharges at Aragats Cosmic Station LEAD workshop Armenia, NOR AMBERD.
MPI Semiconductor Laboratory, The XEUS Instrument Working Group, PNSensor The X-ray Evolving-Universe Spectroscopy (XEUS) mission is under study by the.
Highlights of the ASTROSAT Mission S. Seetha PI, ASTROSAT Programme Director Space Science Programme Office ISRO Headquarters Bangalore IACHEC, Pune 01.
ISUAL Design Concept S. Mende. SDR 7 Jun NCKU UCB Tohoku ISUAL Design Concept S. Mende Sprite Example Sprite Image obtained by Berkeley/NCKU 1999.
Space Solar Telescope (SST) —— 申请发改委 “ 十二五 ” 项目 Proposed by Chinese Academy of Sciences and China Aerospace Science and Technology Corporation.
Wide-field Infrared Survey Explorer (WISE) is a NASA infrared- wavelength astronomical space telescope launched on December 14, 2009 It’s an Earth-orbiting.
for Lomonosov-GRB collaboration
E. Ponce2-1, G. Garipov2, B. Khrenov2, P. Klimov2, H. Salazar1
Light and Telescopes
Onboard Instruments of ASTROSAT
Astronomy 04 The Solar System
Spectrophotometer Dr . S. Jayakumar.
Upcoming Facilities of IIA
Ch.1, Sec.2 - Telescopes Optical Telescopes
Detectors of the New Projects at NAOC
Telescopes and the Electromagnetic Spectrum Section 3
Overview Instrument Role Science Niches Consortium science
IR Telescopes Need relatively large objectives for reasonable resolution at infrared wavelengths. Need cooling to reduce thermal background “noise”
Tools of Astronomy.
Chapter 36—Optical Instruments
SSM onboard ASTROSAT Calibration and First Results
ME instrument and in-orbit performance
Electromagnetic Radiation
Sci. 1-3 Telescopes- then and Now Pages 18-23
Presentation transcript:

Ultra-Violet Imaging Telescope for ASTROSAT ASTROSAT is India’s first dedicated astronomy Satellite and is scheduled to launch on board the PSLV in 2014. Astrosat is currently proposed as a multi-wavelength astronomy mission on an IRS-class satellite into a near-Earth, equatorial orbit by the PSLV. The 4 instruments on-board cover the visible (320-530 nm), near UV (180-300 nm), far UV (130-180 nm), soft X-ray (0.3-8 keV and 2-10 keV) and hard X-ray (3-80 keV and 10-150 keV) regions of the electromagnetic spectrum. The satellite is a collaborative effort of the TIF, ISRO Satellite Centre, IIA, RRI, IUCAA and PRL, all of which are involved in the development of hardware for this mission. In addition, several centres of ISRO are involved in the designing of components and subsystems and several other institutes are involved in developing software for the mission. The Canadian Space Agency is also involved in the making of this satellite. Onboard Instruments of ASTROSAT Twin 40-cm Ultraviolet Imaging Telescopes (UVIT) covering Far- UV to optical bands. Three units of Large Area Xenon Proportional Counters (LAXPC) covering medium energy X-rays from 3 to 80 keV with an effective area of 6000 sq.cm. at 10 keV. A Soft X-ray Telescope (SXT) with conical foil mirrors and X-ray CCD detector, covering the energy range 0.3-8 keV. The effective area will be about 200 sq.cm. at 1 keV. A Cadmium-Zinc-Telluride coded-mask imager (CZTI), covering hard X-rays from 10 to 150 keV, with about 10 deg field of view and 1000 sq.cm. effective area. UVIT Technical Specification Telescope: Aperture : 375mm Optical Configuration: RC Focal Length: 4750mm Plate Scale: 23.2micron/arc Sec Field of View: 28arc min Detector: Microchannel Plate + Photon-counting CMOS 3 channels: FUV, NUV, VIS simultaneous Filters: FUV (130 -180nm): Caf2, Baf2, Sapphire, Silica, Grating, Block NUV ( 200 -300nm ) : Caf2, Silica, NUV13, NUV15, NUVB4, NUVN2 Grating, Block VIS: Bk7, VIS1, VIS2, VIS3, ND, Block Sensitivity: ~ 20 mag Image resol: 1.8 arc-sec Temporal resolution: 30 ms, full frame,< 5 ms, small window http://uvit.iiap.res.in/ http://www.iiap.res.in/iiaoutreach Poster Credit: Prasanna Deshmukh