Participación Española en SAFARI/SPICA
|
|
|
- Richard Ryan
- 8 years ago
- Views:
Transcription
1 Participación Española en SAFARI/SPICA F. Najarro (CAB) CAB J. R. Goicoechea J. Martín-Pintado J. Gómez-Elvira J. Torres L. Mora J. Bueno INTA L.M. González C. Pastor T. Belenguer M. Reina IAC I. Pérez-Fournón Paco Najarro SEA 2010
2 Themes Addressed by SPICA 1. What are the conditions for life and planetary formation? 2. How does the Solar System work? 3. What are the fundamental laws of the Universe? 4. How did the Universe originate and what is it made of? Paco Najarro SEA 2010
3 What is SPICA? PI:Takao Nakagawa (JAXA-lead)+ESA partnership+others * Observatory-class mission European access through ESA partnership *Telescope: 3.2m, Actively cooled to <6 K: monolithic mirror clean PSF * Core wavelength: 5-210μm: Δθ = arcsec * Orbit: Sun-Earth L2 Halo * Warm Launch Cooling in orbit Long lifetime ~ 3 yrs (5 yrs goal) * Launch: ~2018 Paco Najarro SEA 2010
4 The origins questions key science drivers and SPICA and SAFARI How do stars and galaxies form and evolve over cosmic ages? SAFARI will observe thousands of obscured, far away galaxies and determine what processes govern their evolution How does our solar system relate to other planetary systems and could life evolve elsewhere? SAFARI will characterize oxygen, water, ice and rock in young planet forming systems and study their relation to the rocks and ice in our own Solar System Science is the driver basis for the SAFARI Science Requirements Area and number of pixels on the sky, filters and wavebands, stability etc. ~1 degree 4
5 Why observe in the Mid and Far-IR? MIR FIR FIR MIR Galliano et al. Star light recycled by dust and gas Complete picture only seen by observing in the mid- and far-ir Paco Najarro SEA 2010
6 Why SPICA? IR Natural Sky Background VS Thermal Telescope Emission Paco Najarro SEA 2010
7 Why SPICA? 冷 却 方 法 の 革 新 Small Telescope Big Telescope ISO (60cm) (2000L He 2.6t) HERSCHEL (3.5 m) (No Cryogen 2.6t) Paco Najarro SEA 2010
8 Huge Gain of Sensitivity!!! 2.5 orders SPICA 1.5 orders SPICA Paco Najarro SEA 2010
9 SPICA/SAFARI: TES detectors TES SRON: a novel parallel, straight leg design and result Straight leg: not possible to realize required isolation for small pixels Ta absorber Si x N y legs
10 SPICA multiplexing capability SPICA FIR arcmin SPICA FIR m SPICA MIR m - 30x5 arcsec JWST MIRI 5-28 m - 4x4 to 8x8 arcsec SPICA/JWST spectral volumes superposed on deep GOODS 24 m image SPICA MIR/FIR: warm/cool gas + dust JWST: 3 settings/ full waveband 30 hrs to get 10 sources SPICA: 30 hrs integration ~ same sensitivity Multiple sources in field - comparable sensitivity Paco Najarro SEA 2010
11 SPICA instrument suite (NIR/MIR) Mid-IR Camera+Spectrometer (Japan) Operating wavelength 5-38 m Photometric + spectroscopic capability Camera: FoV ~6 x6 Spectroscopic: R~200 (5 slit), R~700 (12 x6 /12), R~30,000 (0.72/1.2 x3.5/6 : 4-8/12-18 m) High resolution spectroscopy NOT possible with JWST Mid-IR coronograph, SCI (Japan) Operating wavelength 5-27 m (possibly down to 3.5 m) ~1 x 1 FoV Pupil mask: >10 6 contrast; Inner Working Angle ~3.3 /D R~20 and 200 Spectroscopy NOT possible with JWST coronagraph (+ SCI cleaner PSF/higher contrast due to monolithic mirror) FPC-S: Focal plane guidance camera (Korea) H, K, 2-5um, Imaging (R~3) + low resolution spectroscopy (R~50 using LVF) 5 x 5 FoV
12 SAFARI (European-lead+Canada+Japan): SPICA instrument suite, cont. (FIR) Imaging FTS, various R resolutions m FoV 2 x2 R~3 (photometry); R~ (SED-mode); 100 µm (spectroscopy) 3 bands (simultaneous): 34-60/60-110/ µm 64x64, 38x38, 20x20 pixels (~6000 pixels total) Diffraction-limited PI: SRON, NL (P. Roelfsema) High sensitivity detectors NEP = 2x10-19 W/ Hz TES detectors (<100mK)
13 Participación española en SPICA (2006-7) CDTI ESAC Run second SOC User Support Proposal handling Observation planning Data processing, archiving and distribution Possible Spanish contributions: DAMIR, ICC, Electrónica de control IAC Warm-electronics, EGSE Coste aproximado de la participación española 4-5 M Paco Najarro SEA 2010
14 Participación española en SPICA (2008) CDTI ESAC Run second SOC User Support Proposal handling Observation planning Data processing, archiving and distribution ICC: pipeline?? Possible Spanish contributions: DAMIR, ICC, Electrónica de control (cryocooler), mecánica: FTS mechanism Subsystem structure IAC Warm-electronics, EGSE Coste aproximado de la participación española 5-8 M Paco Najarro SEA 2010
15 Participación española en SPICA (2010) (2008) Francisco Najarro (HoN) & Javier R. Goicoechea (Gal. Project Scientist) ICC. Ground Segment contribution + Running 2nd SOC (CDTI) Lead Structural Engineer (CAB) FPU chassis (horizontal & vertical Optical Bench, cover(s) and other structural elements (CAB + INDUSTRY) Camera Optics Bay on optical bench including warm alignment. All mirrors (INTA + INDUSTRY) Input Optics Module, Filter Wheels & Alignment Engineer (INTA) Test house for end-to-end optical performance testing (AITV) (INTA) Contributions to ICC (CAB) Contributions to EGSE (IAC) Cooperate in context of Calibration testing e.g. with CSL (CAB-INTA) FPA testing (incl. cryostat) of one of the TES bands (CAB) Coste aproximado de la participación española 25 M Co-PI Paco Najarro SEA 2010
16 The consortium task distribution On-going changes Filter wheel Spain Germany/Belgium; FTS mechanism and control NL Canada; AIV support by Poland TBD/TBC: Calibration source; Filters/dicroics UK Sweden ;Camera bay NL Spain SAFARI consortium meeting September PI/PM update 17
17 The SAFARI project SAFARI consortium meeting September PI/PM update 18
18 The SAFARI project who does what (now) SAFARI consortium meeting September PI/PM update 19
19 SPANISH ORGANIZATION & TEAM Paco Najarro (HoN) Galactic Project Scientist Javier R. Goicoechea Science Coordination Paco Najarro CAB Engineering Management Javier Gomez-Elvira (PM) Jesus Martin Pintado (CAB) Amaya Moro-Martin(CAB) José Cernicharo(CAB) Guillermo Muñoz-Caro(CAB) Luisa Lara (IAA-CSIC) Ismael Perez-Fournon (IAC) Ignasi Ribas (ICE-CSIC) Almudena Alonso Herrera (DAMIR) Pablo Perez Gonzalez( UCM) Armando Gil de Paz (UCM) FPU Filter Wheels & Opt. Input Module Josefina Torres (CAB) Luis Gonzalez Fernandez (INTA) Tomás Belenguer (INTA) Carmen Pastor (INTA) Detectors & Calibration Manuel Reina Aranda (INTA) Juan Bueno Lopez (CAB) Lola Sabau (INTA) Nuria Llombart (UCM) Electrical Eduardo Sebastian (CAB) EGSE Ismael Perez-Fournon ( IAC ) ICC Eduardo Sanchez(CAB) LNA Juan Daniel Gallego(Yebes) TBC
20 detailing of the reference design continues Structural Thermal SAFARI consortium meeting September PI/PM update 21
21 SAFARI project status Consortium well established Final iterations on detailed work distribution on-going PI institute (NL) funding secured, partners funded for phase B1 Science consortium final iterations on requirements Straw-man observing programmes Discussions with MCS on joint programme Development status - achieved fully viable reference design Science Verification Review closeout imminent Much unit level progress; eg. 50mK cooler in EM manufacture Much technology progress; eg. magnetic shielding, flex cables Detector concept review II (May 13) great progress! Schedule?/2014 instrument proposal to ESA End 2016 Preliminary Design Review Mid 2020 Flight Model delivery SAFARI consortium meeting September PI/PM update 22
22 The not so good last week news Japan cannot allocate mission within the current budget New mission implementation concept JAXA/ISAS service module the satellite + launch + ops. ESA payload ESA part is bigger than mission of opportunity envelope SPICA needs to be an M4 mission M4 proposal SPICA now will compete with other projects M4 proposal process takes time mission candidate selection late 2014 mission selection in late 2017 launch in late 2026 SAFARI consortium meeting September SPICA Plan-B 23
23 Posibles salidas: Pasamos del actual - Plan-A JAXA SPICA Project ESA Satellite System AIVT Launch Operation SAFARI BM AIVT PLM AIVT Satellite Operation Science Operation KASI Cryogenics AIVT SIA AIVT SAFARI Operation Other Instruments Operations Cryo Supports and Shields Cryocoolers STA FPIA AIVT Items in red: not exchangeable SAFARI MCS SCI FPC SAFARI consortium meeting September SPICA Plan-B 24
24 A un posible Plan-B1 ESA does payload JAXA SPICA Project ESA Satellite System AIVT Launch Operation SAFARI BM AIVT PLM AIVT Satellite Operation Science Operation KASI Cryogenics AIVT SIA AIVT SAFARI Operation Other Instruments Operations Cryo Supports and Shields Cryocoolers STA FPIA AIVT Items in red: not exchangeable SAFARI MCS SCI FPC SAFARI consortium meeting September SPICA Plan-B 25
El programa de ciencias del espacio de la ESA
El programa de ciencias del espacio de la ESA Fabio Favata European Space Agency Astronomy and Fundamental Physics Missions Coordinator A broad mission portfolio A long-term commitment to the excellence
Low noise millimeter wave receivers for Cosmic Microwave Background radiometers
Low noise millimeter wave receivers for Cosmic Microwave Background radiometers Eduardo Artal, Beatriz Aja, Luisa de la Fuente, Juan Luis Cano, Enrique Villa, Jaime Cagigas (1) Enrique Martínez-González,
TES microcalorimeters for future X ray missions. Athena and Beyond: TES detectors for future X-ray missions. Luigi Piro IAPS/INAF
Athena and Beyond: TES detectors for future X-ray missions IAPS/INAF 1 Setting the stage Science drivers for a Integral Field Spectrometer in X-rays Driving Requirements and mapping into detector Scenarios
Development of the Extreme Ultraviolet Spectrometer: EXCEED
Development of the Extreme Ultraviolet Spectrometer: EXCEED Go Murakami*, Kazuo Yoshioka, Atsushi Yamazaki, Tomoki Kimura Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency
WFIRST- AFTA: European Interests
WFIRST- AFTA: European Interests Mark Cropper Mullard Space Science Laboratory University College London Contents 1. WFI interests Europe- wide 2. Coronagraph interests, UK only see Anthony BoccaleJ s
Archival Science with the ESAC Science Archives and Virtual Observatory
Archival Science with the ESAC Science Archives and Virtual Observatory Deborah Baines Science Archives and VO Team Scientist European Space Agency (ESA) European Space Astronomy Centre (ESAC) Science
Yukikatsu Terada (Saitama Univ, Japan), on behalf of the Astro-H Software Calibration board
Yukikatsu Terada (Saitama Univ, Japan), on behalf of the Astro-H Software Calibration board SKIP (Rob Introduction) The sixth series of the Japanese X-ray satellite. Collaboration with JAXA, NASA, and
Are We Alone?! Exoplanet Characterization and Direct Imaging!
From Cosmic Birth to Living Earths A Vision for Space Astronomy in the 2020s and Beyond Are We Alone?! Exoplanet Characterization and Direct Imaging! A Study Commissioned by the Associated Universities
The Balloon Experimental Twin Telescope for Infrared Interferometry (BETTII)
The Balloon Experimental Twin Telescope for Infrared Interferometry (BETTII) Dr. Stephen Rinehart NASA s Goddard Space Flight Center Laboratory for Observational Cosmology What is BETTII? As proposed,
RESULTS FROM A SIMPLE INFRARED CLOUD DETECTOR
RESULTS FROM A SIMPLE INFRARED CLOUD DETECTOR A. Maghrabi 1 and R. Clay 2 1 Institute of Astronomical and Geophysical Research, King Abdulaziz City For Science and Technology, P.O. Box 6086 Riyadh 11442,
An Introduction to the MTG-IRS Mission
An Introduction to the MTG-IRS Mission Stefano Gigli, EUMETSAT IRS-NWC Workshop, Eumetsat HQ, 25-0713 Summary 1. Products and Performance 2. Design Overview 3. L1 Data Organisation 2 Part 1 1. Products
Fig.1. The DAWN spacecraft
Introduction Optical calibration of the DAWN framing cameras G. Abraham,G. Kovacs, B. Nagy Department of Mechatronics, Optics and Engineering Informatics Budapest University of Technology and Economics
Virtual Observatory tools for the detection of T dwarfs. Enrique Solano, LAEFF / SVO Eduardo Martín, J.A. Caballero, IAC
Virtual Observatory tools for the detection of T dwarfs Enrique Solano, LAEFF / SVO Eduardo Martín, J.A. Caballero, IAC T dwarfs Low-mass (60-13 MJup), low-temperature (< 1300-1500 K), low-luminosity brown
The Planck Legacy Archive: current status, contents and future development. Xavier Dupac ESA-ESAC Villanueva de la Cañada, Spain
The Planck Legacy Archive: current status, contents and future development Xavier Dupac ESA-ESAC Villanueva de la Cañada, Spain Outline Introduction Schedule Scientific contents of the PLA Additional contents
Mid InfraRed Instrument (MIRI) Cooler Subsystem Design
Mid InfraRed Instrument (MIRI) Cooler Subsystem Design D. Durand, D. Adachi, D. Harvey, C. Jaco, M. Michaelian, T. Nguyen, M. Petach, and J. Raab Northrop Grumman Space Technology Redondo Beach, California,
The Sino-French Gamma-Ray Burst Mission SVOM (Space-based multi-band astronomical Variable Objects Monitor)
The Sino-French Gamma-Ray Burst Mission SVOM (Space-based multi-band astronomical Variable Objects Monitor) Didier BARRET on behalf of the SVOM collaboration didier.barret@cesr.fr Outline SVOM background
CAUP s Astronomical Instrumentation and Surveys
CAUP s Astronomical Instrumentation and Surveys CENTRO DE ASTROFÍSICA DA UNIVERSIDADE DO PORTO www.astro.up.pt Sérgio A. G. Sousa Team presentation sousasag@astro.up.pt CAUP's Astronomical Instrumentation
The Virtual Observatory: What is it and how can it help me? Enrique Solano LAEFF / INTA Spanish Virtual Observatory
The Virtual Observatory: What is it and how can it help me? Enrique Solano LAEFF / INTA Spanish Virtual Observatory Astronomy in the XXI century The Internet revolution (the dot com boom ) has transformed
JWST and the Solar System
JWST and the Solar System P. Ferruit (ESA JWST project scientist) Presentation based on work and presentations done/prepared by the JWST solar system working group and a set of 10 focus groups (more later).
JWST Primer. Space Telescope Science Institute 3700 San Martin Drive Baltimore, Maryland 21218 help@stsci.edu. Version 1.
Version 1.0 October 2004 JWST Primer Space Telescope Science Institute 3700 San Martin Drive Baltimore, Maryland 21218 help@stsci.edu Operated by the Association of Universities for Research in Astronomy,
How To Make A High Energy Ion Detector
EPD: Energetic particle Detector Javier Rodríguez guez-pacheco Martín Grupo de Investigación n Espacial Universidad de Alcalá EPD: Energetic particle Detector STEIN (Supra-thermal Electrons, Ions & Neutrals)
The PAU Camera. Abstract
Highlights of Spanish Astrophysics VI, Proceedings of the IX Scientific Meeting of the Spanish Astronomical Society held on September 13-17, 2010, in Madrid, Spain. M. R. Zapatero Osorio et al. (eds.)
In studying the Milky Way, we have a classic problem of not being able to see the forest for the trees.
In studying the Milky Way, we have a classic problem of not being able to see the forest for the trees. A panoramic painting of the Milky Way as seen from Earth, done by Knut Lundmark in the 1940 s. The
Indiana University Science with the WIYN One Degree Imager
Indiana University Science with the WIYN One Degree Imager Katherine Rhode (Indiana University, WIYN SAC member) Indiana University Department of Astronomy Nine faculty members, plus active emeritus faculty
A THERMAL MAPPER FOR MARCO POLO-R
A THERMAL MAPPER FOR MARCO POLO-R Javier Licandro, Miquel Serra Ricart, Alex Oscoz Abad, Víctor Alí Lagoa, Ovidiu Vaduvescu, Marcos Reyes, Enrique Joven Reunión CV M3, MICIIN, Octubre 21, 2011 The
ID Objective Requirements Description of Test Date & Examiner 15 Verify that the optics?? OMC
NAOMI OMC/NCU Acceptance Tests at the University of Durham ATC Document number AOW/GEN/RAH/15.0/06/00 OMC/NCU acceptance tests DRAFT (Version date: 2 nd June 2000) wht-naomi-44 The ID numbers are those
PRESENTATION SPACE MISSIONS
GENERAL PRESENTATION SPACE MISSIONS CONTENTS 1. Who we are 2. What we do 3. Space main areas 4. Space missions Page 2 WHO WE ARE GENERAL Multinational conglomerate founded in 1984 Private capital Offices
FRACTAL S.L.N.E. A private company for engineering of scientific projects. Instrumentation and Software for Astronomy
FRACTAL S.L.N.E A private company for engineering of scientific projects Instrumentation and Software for Astronomy 1 Introducing FRACTAL FRACTAL S.L.N.E. is a private technological company funded in 2005.
Sviluppo di componenti per sottosistemi ottici basati su ottiche elettroformate altamente asferiche per applicazioni Spazio e Difesa
EMSOM Sviluppo di componenti per sottosistemi ottici basati su ottiche elettroformate altamente asferiche per applicazioni Spazio e Difesa Workshop Terzo bando P.M.I. Tema Materiali, Componenti e Sensori
Towards the Detection and Characterization of Smaller Transiting Planets
Towards the Detection and Characterization of Smaller Transiting Planets David W. Latham 27 July 2007 Kepler MISSION CONCEPT Kepler Mission is optimized for finding habitable planets ( 10 to 0.5 M )
Resultados Concurso Apex 2007
Resultados Concurso Apex 2007 Propuesta: CC-07-03 Investigador Principal: Leonardo Bronfman Título: ATLASGAL: APEX Telescope Large Area Survey of the Galaxy Resumen: The location of the APEX telescope
ALMA Overview. Leonardo Testi (European Southern Observatory)
ALMA Overview Leonardo Testi (European Southern Observatory) The ALMA Project Status Timeline towards Early and Full Science Operations Future Developments Atacama Large Millimeter Array At least 50x12m
16 th IOCCG Committee annual meeting. Plymouth, UK 15 17 February 2011. mission: Present status and near future
16 th IOCCG Committee annual meeting Plymouth, UK 15 17 February 2011 The Meteor 3M Mt satellite mission: Present status and near future plans MISSION AIMS Satellites of the series METEOR M M are purposed
High Resolution Planetary Imaging Workflow
High Resolution Planetary Imaging Workflow Fighting the Atmosphere Getting out of the Atmosphere Adaptive Optics Lucky Imaging Lucky Imaging is the process of capturing planets using a CCD video camera.
INTA AIRBORNE REMOTE SENSING FACILITY from the Hasselblad s cameras to the SensyTech-AHS sensor
INTA AIRBORNE REMOTE SENSING FACILITY from the Hasselblad s cameras to the SensyTech-AHS sensor José-Antonio Gómez-Sánchez gomezsj@inta.es Remote Sensing Laboratory INSTITUTO NACIONAL DE TÉCNICA AEROESPACIAL
Clouds and the Energy Cycle
August 1999 NF-207 The Earth Science Enterprise Series These articles discuss Earth's many dynamic processes and their interactions Clouds and the Energy Cycle he study of clouds, where they occur, and
Adaptive Optics (AO) TMT Partner Institutions Collaborating Institution Acknowledgements
THIRTY METER TELESCOPE The past century of astronomy research has yielded remarkable insights into the nature and origin of the Universe. This scientific advancement has been fueled by progressively larger
How To Use Laboca
Laboca in a nutshell Total power Bolometer Array operating at 850 µm 295 pixels Field of view 11 Science: cold dust nearby and far Bolometer Principle Neutron-Transmutation-Doped (NTD) Germanium 0.25mm
NASA s Future Missions in X-ray Astronomy
NASA s Future Missions in X-ray Astronomy Nicholas E. White NASA s Goddard Space Flight Center Laboratory for High Energy Astrophysics Greenbelt, MD 20771 USA nwhite@lheapop.gsfc.nasa.gov Abstract The
Herschel PACS Test Procedure STM PACS-KT-PR-011 Issue: 1 Revision: -
CASE GmbH Westendstrasse 125 80339 München Herschel PACS Test Procedure STM 1 Revision: - i Document Approval Sheet Title: Herschel PACS Subtitle: Test Procedure STM Doc. No: 1 Revision: - Prepared:......
Extreme-AO for GMT. Center for Astronomical Adaptive Optics, University of Arizona Subaru Telescope, National Astronomical Observatory of Japan
Extreme-AO for GMT Olivier Guyon Center for Astronomical Adaptive Optics, University of Arizona Subaru Telescope, National Astronomical Observatory of Japan guyon@naoj.org 1 Extreme-AO for GMT: Key science
A.-L. Maire, S. Desidera, S. Esposito, A. Skemer, P. Hinz, & the LEECH & HOSTS teams
A.-L. Maire, S. Desidera, S. Esposito, A. Skemer, P. Hinz, & the LEECH & HOSTS teams LEECH LBTI Exozodi Exoplanet Common Hunt PI: A. Skemer/Univ. Arizona (~130 nights) Search for & characterization young
CBERS Program Update Jacie 2011. Frederico dos Santos Liporace AMS Kepler liporace@amskepler.com
CBERS Program Update Jacie 2011 Frederico dos Santos Liporace AMS Kepler liporace@amskepler.com Overview CBERS 3 and 4 characteristics Differences from previous CBERS satellites (CBERS 1/2/2B) Geometric
Science and the Taiwan Airborne Telescope
Cosmic Variability Study in Taiwan Wen-Ping Chen Institute of Astronomy National Central University, Taiwan 2010 November 16@Jena/YETI Advantages in Taiwan: - Many high mountains - Western Pacific longitude
Science@ESA vodcast series. Script for Episode 6 Charting the Galaxy - from Hipparcos to Gaia
Science@ESA vodcast series Script for Episode 6 Charting the Galaxy - from Hipparcos to Gaia Available to download from http://sci.esa.int/gaia/vodcast Hello, I m Rebecca Barnes and welcome to the Science@ESA
Orientation. Contractors
Space Systems Forecast - Satellites & Spacecraft Outlook The Ariane 5 launch vehicle carrying blasted off from the Kourou Spaceport at 2:12 p.m. EST (18:12 GMT) on May 14, 2009 Before the launch, were
How To Celebrate The Industry Day Of The Euclid Spacecraft
Industry Day of the Euclid Spacecraft With the present announcement, the European Space Agency and Thales Alenia Space (Italy) inform the EITS Users (European Companies and Institutes) about a presentation
ESA Contribution to Astro-H
ESA Contribution to Astro-H P Kretschmar & D Lumb Rome 03/07/2012 Background 1. Follows on from the co-operative agreements between JAXA and ESA on data sharing in the XMM-Newton and Suzaku 2. To leverage
NASA s Dawn Mission Journey to the Asteroid Frontier
NASA s Dawn Mission Journey to the Asteroid Frontier Dawn Lucy McFadden, Co-Investigator University of Maryland College Park, MD January 12, 2009 SBAG update 9 th Discovery Mission Dawn Explores the Earliest
Esa Mandatory Programme Opportunities as seen by Astrium Satellites. Wolfram Lork // July 07
Esa Mandatory Programme Opportunities as seen by Astrium Satellites Wolfram Lork // July 07 Overview Esa member states are contributing to Esa by mandatory contributions, calculated along GNP Gross National
Data transport in radio astronomy. Arpad Szomoru, JIVE
Data transport in radio astronomy Arpad Szomoru, JIVE Some acronyms EVN: European VLBI Network Consortium of radio telescopes Involving 14 different organizations around the world: Europe, China, Puerto
PRELIMINARY DESIGN REVIEW
STUDENTS SPACE ASSOCIATION THE FACULTY OF POWER AND AERONAUTICAL ENGINEERING WARSAW UNIVERSITY OF TECHNOLOGY PRELIMINARY DESIGN REVIEW CAMERAS August 2015 Abstract The following document is a part of the
Assessments of LEDs IESNA LM-79, LM-80 & LM-82
Assessments of LEDs IESNA LM-79, LM-80 & LM-82 by Rolf S. Bergman Consultant 4/30/2012 1 ALA M Outline of Presentation Background Information EPA Energy Star specifications NVLAP Accreditation IESNA Technical
Spectrophotometry of Ap Stars
Spectrophotometry of Ap Stars ASTRA Status Report Barry Smalley Astrophysics Group Keele University Staffordshire United Kingdom bs@astro.keele.ac.uk What is Spectrophotometry? Spectroscopy through a wide
Using Photometric Data to Derive an HR Diagram for a Star Cluster
Using Photometric Data to Derive an HR Diagram for a Star Cluster In In this Activity, we will investigate: 1. How to use photometric data for an open cluster to derive an H-R Diagram for the stars and
SOLSPEC MEASUREMENT OF THE SOLAR ABSOLUTE SPECTRAL IRRADIANCE FROM 165 to 2900 nm ON BOARD THE INTERNATIONAL SPACE STATION
SOLSPEC MEASUREMENT OF THE SOLAR ABSOLUTE SPECTRAL IRRADIANCE FROM 165 to 2900 nm ON BOARD THE INTERNATIONAL SPACE STATION G. Thuillier1, D. Bolsee2 1 LATMOS-CNRS, France 2 Institut d Aéronomie Spatiale
The Milky Way Galaxy is Heading for a Major Cosmic Collision
The Milky Way Galaxy is Heading for a Major Cosmic Collision Roeland van der Marel (STScI) [based on work with a team of collaborators reported in the Astrophysical Journal July 2012] Hubble Science Briefing
Large FOV Mobile E-O Telescope for Searching and Tracking Low-orbit Micro-satellites and Space Debris
Large FOV Mobile E-O Telescope for earching and Tracking Low-orbit Micro-satellites and pace Debris WANG Jian-li 1, GAO Xin, TANG Jia, HAN Chang-yuan 1, ZHAO Jin-yu 1 1 Changchun Institute of Optics, Fine
Georgia Performance Standards Framework for Science Grade 6. Unit Organizer: UNIVERSE AND SOLAR SYSTEM (Approximate Time 3 Weeks)
The following instructional plan is part of a GaDOE collection of Unit Frameworks, Performance Tasks, examples of Student Work, and Teacher Commentary. Many more GaDOE approved instructional plans are
KZO Tactical UAV System Overview
KZO Tactical UAV System Overview KZO TUAV / FTS / 08.02.2006 / Chart 1 Content System Elements Air Vehicle Ground Control Station Data Link Vehicle Launch Vehicle Refurbishing Vehicle Technical Summary
A STEP 400 Technical development status
A STEP 400 Technical development status ARENA workshop, Catania, 17 sept 08 Authors: J.B. Daban (1), C. Gouvret (1), A. Agabi (1), T. Guillot (2), F. Fressin (2), L. Abe (1), N. Crouzet (2), Y. Fanteï-Caujolle
How To Process Data From A Casu.Com Computer System
CASU Processing: Overview and Updates for the VVV Survey Nicholas Walton Eduardo Gonalez-Solares, Simon Hodgkin, Mike Irwin (Institute of Astronomy) Pipeline Processing Summary Data organization (check
Overview of NASA s Laser Communications Relay Demonstration
Overview of NASA s Laser Communications Relay Demonstration April 2012 Bernard Edwards NASA Goddard Space Flight Center (301) 286-8926 Bernard.L.Edwards@nasa.gov 1 LCRD Demonstration Scenarios Mission
Image classification of night time images detected from the International Space Station
Image classification of night time images detected from the International Space Station Alejandro Sánchez de Miguel, José Gómez Castaño and Jaime Zamorano Calvo. Universidad Complutense de Madrid. Image
First Discoveries. Asteroids
First Discoveries The Sloan Digital Sky Survey began operating on June 8, 1998. Since that time, SDSS scientists have been hard at work analyzing data and drawing conclusions. This page describes seven
Lessons Learned from SOFIA
Lessons Learned from SOFIA Erick Young SOFIA Science Center 25 April 2012 1 Basic Parameters Mission Duration Facility designed for 20 year operational lifetime User Base General astronomical community
Software challenges in the implementation of large surveys: the case of J-PAS
Software challenges in the implementation of large surveys: the case of J-PAS 1/21 Paulo Penteado - IAG/USP pp.penteado@gmail.com http://www.ppenteado.net/ast/pp_lsst_201204.pdf (K. Taylor) (A. Fernández-Soto)
European Solar Telescope: Perspectives for the coming years. M. Collados Instituto de Astrofísica de Canarias
European Solar Telescope: Perspectives for the coming years M. Collados Instituto de Astrofísica de Canarias 2007: EAST Consortium formed EAST: European Association for Solar Telescopes AIM (among others):
High Resolution Planetary Imaging
High Resolution Planetary Imaging Fighting the Atmosphere Getting out of the Atmosphere Adaptive Optics Lucky Imaging Lucky Imaging is the process of capturing planets using a CCD video camera. A software
Light Telescopes. Grade Level: 5. 2-3 class periods (more if in-depth research occurs)
Light Telescopes Grade Level: 5 Time Required: Suggested TEKS: Science - 5.4 Suggested SCANS Information. Acquires and evaluates information. National Science and Math Standards Science as Inquiry, Earth
Robotic Pre-Cursor Contribution to Human NEA Mission. H. Kuninaka JSPEC/JAXA
Robotic Pre-Cursor Contribution to Human NEA Mission H. Kuninaka JSPEC/JAXA Asteroid Explorer Hayabusa Dimensions 1.0m x 1.6m x 1.1m Weight : 380kg(Dry) Chemical Fuel 70kg Xe Propellant 60kg Total 510kg
Teaching Astronomy in the University of Granada. Eduardo Battaner Departamento de Física Teórica y del Cosmos
Teaching Astronomy in the University of Granada Eduardo Battaner Departamento de Física Teórica y del Cosmos Some history University created by Charles V in the XVI century (An arabic Madraza was created
THE GOCI INSTRUMENT ON COMS MISSION THE FIRST GEOSTATIONARY OCEAN COLOR IMAGER
THE GOCI INSTRUMENT ON COMS MISSION THE FIRST GEOSTATIONARY OCEAN COLOR IMAGER Topic 1 - Optical instruments for Earth / Planets surface and atmosphere study François FAURE, Astrium SAS Satellite, Toulouse,
California Standards Grades 9 12 Boardworks 2009 Science Contents Standards Mapping
California Standards Grades 912 Boardworks 2009 Science Contents Standards Mapping Earth Sciences Earth s Place in the Universe 1. Astronomy and planetary exploration reveal the solar system s structure,
Astrophysical Techniques. C R Kitchin
Astrophysical Techniques C R Kitchin University of Hertfordshire Observatory Third Edition SUB Gottingen 7 210 119 268 99 A 8843 Institute of Physics Publishing Bristol and Philadelphia Contents Preface
Ten years of astronomical Field Trips to Tenerife: challenges and rewards
Ten years of astronomical Field Trips to Tenerife: challenges and rewards [Short title: UG astronomy from Tenerife] M J Coe Dept of Physics & Astronomy, University of Southampton, SO17 1BJ, UK. Email:
7th Agile Meeting & The Bright Gamma-Ray Sky Frascati, 29 September - 1 October, 2009. Carlotta Pittori, on behalf of the ADC
7th Agile Meeting & The Bright Gamma-Ray Sky Frascati, 29 September - 1 October, 2009 The AGILE Data Center and the First AGILE Catalog Carlotta Pittori, on behalf of the ADC AGILE GS Architecture Fucino,
Technical Data. FLIR T620 25 (incl. Wi-Fi)
Technical Data FLIR T620 25 (incl. WiFi) Part number: 559010102 Copyright 2012, FLIR Systems, Inc. All rights reserved worldwide. Names and marks appearing herein are either registered trademarks or trademarks
Alpy guiding User Guide. Olivier Thizy (olivier.thizy@shelyak.com) François Cochard (francois.cochard@shelyak.com)
Alpy guiding User Guide Olivier Thizy (olivier.thizy@shelyak.com) François Cochard (francois.cochard@shelyak.com) DC0017A : april 2013 Alpy guiding module User Guide Olivier Thizy (olivier.thizy@shelyak.com)
Remote Sensing of Clouds from Polarization
Remote Sensing of Clouds from Polarization What polarization can tell us about clouds... and what not? J. Riedi Laboratoire d'optique Atmosphérique University of Science and Technology Lille / CNRS FRANCE
The Gaia Archive. Center Forum, Heidelberg, June 10-11, 2013. Stefan Jordan. The Gaia Archive, COSADIE Astronomical Data
The Gaia Archive Astronomisches Rechen-Institut am Zentrum für Astronomie der Universität Heidelberg http://www.stefan-jordan.de 1 2 Gaia 2013-2018 and beyond Progress with Gaia 3 HIPPARCOS Gaia accuracy
United Nations - Nations Unies. COSPAR Symposium. Measuring the Universe. Looking Back in Time with Modern Astronomy. Monday, 2nd February 2015
United Nations - Nations Unies COSPAR Symposium Measuring the Universe Looking Back in Time with Modern Astronomy Monday, 2nd February 2015 15:00 18:00 Conference Rooms M1, Building M, Vienna International
Summary of Data Management Principles South Pole Telescope
Summary of Data Management Principles South Pole Telescope Experiment description - Where it is: The South Pole Telescope (SPT) is a 10-meter-diameter telescope located at the Amundsen-Scott South Pole
Amateur Astrophotography. Lauri Kangas Teekkarikamerat 2011-10-20
Amateur Astrophotography Lauri Kangas Teekkarikamerat Astrophotography Outline Introduction Knowing the sky objects to shoot Choosing equipment / focal lengths Long exposures Fixed tripod astrophotos Tracking
Dawn - Overview, Science Objectives, Mission Progress. Hap McSween For PI Chris Russell
Dawn - Overview, Science Objectives, Mission Progress Hap McSween For PI Chris Russell Presentation to Decadal Survey Primitive Bodies Panel, Washington, DC, Sep 2009 Spacecraft configuration, assembly
R1 The meeting endorses the recommendations from the ATMOS User Meeting in 2012. All of which are relevant
R1 The meeting endorses the recommendations from the ATMOS User Meeting in 2012. All of which are relevant We recognize that some projects have been initiated to address some of the deficits in 2012. However
The VHE future. A. Giuliani
The VHE future A. Giuliani 1 The Cherenkov Telescope Array Low energy Medium energy High energy 4.5o FoV 7o FoV 10o FoV 2000 pixels 2000 pixels 2000 pixels ~ 0.1 ~ 0.18 ~ 0.2-0.3 The Cherenkov Telescope
Ionospheric Research with the LOFAR Telescope
Ionospheric Research with the LOFAR Telescope Leszek P. Błaszkiewicz Faculty of Mathematics and Computer Science, UWM Olsztyn LOFAR - The LOw Frequency ARray The LOFAR interferometer consist of a large
Infrared Focal Plane Arrays. High Performance. Optics & Photonics News. Nonlinear Spatial Solitons Report from OFC/NFOEC 2008
PINHOLE EYES SILICONE OPTICS OSA 2008 AWARDS Optics & Photonics News June 2008 Vol. 19 No. 6 $8.25 www.osa-opn.org Nonlinear Spatial Solitons Report from OFC/NFOEC 2008 High Performance Infrared Focal
Temperature. LumaSense Technologies, Inc. supplies a unique selection of very precise calibration
Temperature Calibration Sources Highly accurate calibration equipment for pyrometers, thermal imaging cameras, radiometers, heatflux and spectrographic measurement sytems. Calibration sources are infrared
Space Algorithm Testbeds - Small Business Pipeline for Technology Innovation
AIAA SPACE 2009 Conference & Exposition 14-17 September 2009, Pasadena, California AIAA 2009-6821 Space Algorithm Testbeds - Small Business Pipeline for Technology Innovation Roberta M. Ewart and Jie Z.
Earth Sciences -- Grades 9, 10, 11, and 12. California State Science Content Standards. Mobile Climate Science Labs
Earth Sciences -- Grades 9, 10, 11, and 12 California State Science Content Standards Covered in: Hands-on science labs, demonstrations, & activities. Investigation and Experimentation. Lesson Plans. Presented
Space Weather Research and Forecasting in CRL, Japan
Space Weather Research and Forecasting in CRL, Japan Maki Akioka Hiraiso Solar Observatory Communications Research Laboratory Contact akioka@crl.go.jp 1 Contents of Presentation 1.Space Weather Observation
Thermal Imaging Test Target THERMAKIN Manufacture and Test Standard
Thermal Imaging Test Target THERMAKIN Manufacture and Test Standard June 2014 This document has been produced by CPNI as the standard for the physical design, manufacture and method of use of the Thermal
Spatially resolved spectroscopy of the exoplanet HR 8799 c
Spatially resolved spectroscopy of the exoplanet HR 8799 c M. Janson 1,4, C. Bergfors 2, M. Goto 2, W. Brandner 2, D. Lafrenière 3 janson@astro.utoronto.ca ABSTRACT HR 8799 is a multi-planet system detected
A Guide to Modern Planetary Imaging. Christopher Go
A Guide to Modern Planetary Imaging Christopher Go Fighting the Atmosphere Getting out of the Atmosphere Adaptive Optics Speckle/Lucky Imaging Speckle Imaging: Feeling Lucky Speckle or Lucky Imaging is
IRAIT project: future mid-ir operations at Dome C during summer
Mem. S.A.It. Suppl. Vol. 2, 82 c SAIt 2003 Memorie della Supplementi IRAIT project: future mid-ir operations at Dome C during summer Gino Tosti On behalf of the IRAIT Collaboration Osservatorio Astronomico
GAIA Science and Mission
GAIA Science and Mission Nicholas Walton Institute of Astronomy The University of Cambridge p1 Outline Gaia high level science drivers Example science objectives Gaia mission overview Gaia data analysis
Science Standard 4 Earth in Space Grade Level Expectations
Science Standard 4 Earth in Space Grade Level Expectations Science Standard 4 Earth in Space Our Solar System is a collection of gravitationally interacting bodies that include Earth and the Moon. Universal
Searching for space debris elements with the Pi of the Sky system
Searching for space debris elements with the Pi of the Sky system Marcin Sokołowski msok@fuw.edu.pl Soltan Institute for Nuclear Studies ( IPJ ) Warsaw, Poland 7th Integral / BART Workshop ( IBWS), 14-18