WFIRST- AFTA: European Interests
|
|
|
- Harry Barton
- 8 years ago
- Views:
Transcription
1 WFIRST- AFTA: European Interests Mark Cropper Mullard Space Science Laboratory University College London
2 Contents 1. WFI interests Europe- wide 2. Coronagraph interests, UK only see Anthony BoccaleJ s talk also 2
3 Europe and WFI: who Following groups were canvassed, mostly based on JWST NIRSpec and Euclid Germany: Bender (MPE), Rix (MPIA) Spain: Castander (Barcelona) France: le Fevre (LAM), Mellier (IAP) Italy: CimaJ (Bologna), Scaramella (Rome) UK: Sharples (Durham), Wright (UKATC), Davies (Oxford), Nichol (Portsmouth), Cropper (MSSL- UCL) All approached were asked if there were any others they knew who might be interested 3
4 Europe and WFI: who Following groups were canvassed, mostly based on JWST NIRSpec and Euclid Germany: Bender (MPE), Rix (MPIA) Spain: Castander (Barcelona) France: le Fevre (LAM), Mellier (IAP) Italy: CimaJ (Bologna), Scaramella (Rome) UK: Sharples (CfAI- Durham), Wright (UKATC), Davies (Oxford), Nichol (Portsmouth), Cropper (MSSL- UCL) All approached were asked if there were any others they knew who might be interested Those in blue replied with an expression of interest 4
5 IFU: Durham interest, NIRSpec Heritage IFU engineering model structure IFU opmcs mounted inside cryo- test facility for the NIRSpec IFU CollaboraMon with SSTL Durham CfAI lead in: conceptual design opmcs manufacture thermal vac test (35K) 30 slices 3.0 x 0.1 WFE < 100nm Ra < 5-10nm For WFIRST: high TRL low risk WFIRST- AFTA SDT MeeMng #5 20 November
6 Durham Centre for Advanced InstrumentaMon CapabiliMes: Opto- mechanical Design 5- axis diamond machining & metrology Thermal- vac tesmng 5- axis diamond diamond machining facility Specific interests: Integral field unit(s) gold coated opmcs for 8 of the 24 VLT- KMOS IFU channels 6
7 Laboratoire d Astrophysique de Marseille: interests in WFIRST- WFI Technical interests WFI design, manufacturing, tests IFU spectrograph: slicer, disperser, mechanical structure Opto- mechanical systems: opmcs, structure, Science & ground segment interests ExperMse in deep spectroscopy survey for cosmology and galaxy evolumon IFU spectroscopy processing MulM- wavelength analysis: photometric redshifs, SED fijng, Spectra analysis: redshifs, velocity maps, ExperMse on relevant space hardware: Herschel SPIRE FTS Lead ins)tute Euclid- NISP infrastructure for integramon and tests in space environment New 90m 3 vacuum chamber (all tests for Euclid- NISP) Euclid- NISP 90m 3 Space tes<ng chamber 7
8 IFU spectrograph prototype developed for SNAP study with CPPM and LBNL Prototype developed and tested at LAM Funded by CNES, CNRS, LBNL Main space requirements (cold, vibramon) samsfied TRL~6 as evaluated by CNES- chaired panel, including high surface accuracy glass slicer λ=900nm item specifica)on FOV Pixel size Spect Res 4 x ~ x,y SimulaMon λ x,y demonstrator λ Wavelength µm OperaMng Temperature 140 K +/-? Camera F/D F/36 8
9 CalibraMon Unit: MSSL interest, NIRSpec Heritage highly specified opmcal and bandpass- controlled performance in 1 5µm band low- dissipamon light sources comb and broadband filters delivered under contract to Astrium Germany NIRSpec CalibraMon Unit Flight Model 9
10 Mullard Space Science Lab, University College London NIRSpec ground calibramon cryo- GSE Over 50 satellite missions with NASA, ESA, JAXA, USSR/ Russia, China, India Recent relevant (cryogenic) missions: ISO LWS Herschel SPIRE JWST NIRSpec Gaia Swif UVOT Euclid (VIS instrument lead) Last NASA- led missions (JWST) Cassini CAPS SwiD UVOT GOES- SXI, - N, - O, - P Cryogenic mk ADR cryocoolers Science: astrophysics and cosmology 10
11 Spanish interests in WFIRST- WFI A consormum of Spanish insmtumons in Barcelona (ICE, IFAE) and Madrid (CIEMAT, IFT) are interested in a possible parmcipamon in WFIRST This consormum is focused on Dark Energy related research It is currently involved in several Dark Energy experiments: DES, PAU, DESI and Euclid The consormum acmvely parmcipates on several aspects of these projects like management, planning, instrumental development and construcmon, sofware development and scienmfic coordinamon and exploitamon We are interested in possible parmcipamon in the WFIRST WFI in the areas of mechanics, electronics and/or control sofware Euclid: leading FWA (Filter Wheel Assembly) of NISP and SimulaMons OrganizaMon Unit in Science Ground Segment; also, host the Spanish Data Centre 11
12 Spain: Dark Energy Experiments InstrumentaMon heritage DECam: front- end electronics and guider sofware PAUCam on WHT: overall design and construcmon: mechanics, electronics, sofware control also, DESI: negomamng leadership in the GFA: guiding, focus and alignment WFIRST- AFTA SDT MeeMng #5 20 November
13 InsMtute of Cosmology and GravitaMon (ICG) University of Portsmouth: interests in WFIRST Project and sofware experience Significant science leadership roles in DES, SDSS, DESI and Euclid Development of IFU data processing pipeline for SDSS MaNGA (IFU) Founding members of GalaxyZoo and conmnued development of cimzen science projects under Zooniverse Joint SN light curve analysis between DES and VISTA WFIRST interests IFU spectroscopy processing SN classificamon and analysis, leading to improved systemamcs (cosmology) and astrophysics (discoveries) Redshif determininamon from slitless spectroscopy Precision Large scale structure measurements (masks, esmmaorts, mocks) ExperMse on relevant space missions: Lead of galaxy clustering SWG in Euclid BAO scienmst on Euclid EST GalaxyZoo:Hubble 13
14 UK Science Interests: WFI UK has strong track record in cosmology; in parmcular heritage in redshif surveys (2dFGS, SDSS) in the weak lensing probe in Euclid (Science Working Group leads, Science Ground Segment, VIS instrument lead) in the galaxy clustering probe in Euclid (SWG lead) hence is highly interested in scienmfic complementarity offered by WFIRST- AFTA Supernova science is not supported by Euclid significant interest from UK Supernova community who have leading roles in key on- going SN surveys e.g. Portsmouth is leading the DES search and there is strong involvement in the PanSTARRS transient survey (Belfast, Southampton, Oxford). ExperMse in SN cosmology and SN astrophysics Not forgejng extensive UK galaxy evolumon interests In pracmce: involvement in WFIRST- AFTA science working groups would be welcomed Science links to ground segment sofware development 14
15 UK Interests in Coronagraph UK technology interest centred on e2v detector capability allied with research capability at Open Univ CEI MSSL- UCL camera capability (Eddington, Gaia, Euclid, PLATO) Highly integrated approach to system design, high performance, radiamon mimgamon Experience with operamon of and space qualificamon of L3CCDs via Gaia RVS programme (MSSL- UCL and CEI- OU partnership) Current WFIRST contract with CEI- OU on L3CCD development Euclid 12- channel camera electronics Science interests based on PLATO involvement at MSSL- UCL, Warwick, Cambridge, Open University 100 L3CCD97 provided by e2v for Gaia- RVS detector qualificamon 15
16 Summary Significant interest in WFI across Europe in both instrumentamon and science strong Euclid complementarity track record parmcularly with JWST instruments involvement in science working groups UK interests in Coronagraph science complementarity to PLATO track record in CCDs and large space CCD cameras 16
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.)
Euclid. Mapping the geometry of the dark Universe. Conseil scientifique de l IN2P3. 25 Octobre 2012. A Ealet (CPPM)
Euclid Mapping the geometry of the dark Universe Conseil scientifique de l IN2P3 25 Octobre 2012 A Ealet (CPPM) Participation of IN2P3 to an ESA space mission OVERVIEW Euclid Scientific objectives The
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 )
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
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
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
Dominique Fouchez. 12 Fevrier 2011
données données CPPM 12 Fevrier 2011 The Data données one 6.4-gigabyte image every 17 seconds 15 terabytes of raw scientific image data / night 60-petabyte final image data archive 20-petabyte final database
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)
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
Galaxy Survey data analysis using SDSS-III as an example
Galaxy Survey data analysis using SDSS-III as an example Will Percival (University of Portsmouth) showing work by the BOSS galaxy clustering working group" Cosmology from Spectroscopic Galaxy Surveys"
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
Status of NectarCAM camera project. J-F. Glicenstein (IRFU) for the NectarCAM consortium
Status of NectarCAM camera project J-F. Glicenstein (IRFU) for the NectarCAM consortium Outline NectarCAM Design and prototyping Focal plane instrumentation Readout and digitization Trigger Acquisition
Reduced data products in the ESO Phase 3 archive (Status: 15 May 2015)
Reduced data products in the ESO Phase 3 archive (Status: 15 May 2015) The ESO Phase 3 archive provides access to reduced and calibrated data products. All those data are stored in standard formats. The
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
High Energy Physics (HEP) Program Status Update to the AAAC Meeting. June 1, 2015
OFFICE OF SCIENCE High Energy Physics (HEP) Program Status Update to the AAAC Meeting June 1, 2015 Kathy Turner Program Manager, Cosmic Frontier Office of High Energy Physics Office of Science, U.S. Department
Participación Española en SAFARI/SPICA
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
Description of the Dark Energy Survey for Astronomers
Description of the Dark Energy Survey for Astronomers May 1, 2012 Abstract The Dark Energy Survey (DES) will use 525 nights on the CTIO Blanco 4-meter telescope with the new Dark Energy Camera built by
Keysight Technologies Using Fine Resolution to Improve Thermal Images. Application Note
Keysight Technologies Using Fine Resolution to Improve Thermal Images Application Note Introduction Digital imaging opened up new possibilities and has been very much part of our lives since social media
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
ING LA PALMA TECHNICAL NOTE No. 130. Investigation of Low Fringing Detectors on the ISIS Spectrograph.
ING LA PALMA TECHNICAL NOTE No. 130 Investigation of Low Fringing Detectors on the ISIS Spectrograph. Simon Tulloch (ING) June 2005 Investigation of Low Fringing Detectors on the ISIS Spectrograph. 1.
J-PAS: low-resolution (R 50) spectroscopy over 8000 deg 2
J-PAS: low-resolution (R 50) spectroscopy over 8000 deg 2 C. López-Sanjuan J. Cenarro, L. A. Díaz-García, J. Varela, K. Viironen, & the J-PAS team Centro de Estudio de Física del Cosmos de Aragón 10th
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
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
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
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
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
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
Big Data @ STScI. Enhancing STScI s Astronomical Data Science Capabilities over the Next Five Years
Big Data @ STScI Enhancing STScI s Astronomical Data Science Capabilities over the Next Five Years Science Definition Team Report March 15, 2016 1 Table of Contents 1 Executive Summary... 3 2 Charter of
Data Management Plan Extended Baryon Oscillation Spectroscopic Survey
Data Management Plan Extended Baryon Oscillation Spectroscopic Survey Experiment description: eboss is the cosmological component of the fourth generation of the Sloan Digital Sky Survey (SDSS-IV) located
Data, Computation, and the Fate of the Universe
Data, Computation, and the Fate of the Universe Saul Perlmutter University of California, Berkeley Lawrence Berkeley National Laboratory NERSC Lunchtime Nobel Keynote Lecture June 2014 Atomic Matter 4%
ALIGNMENT AND TESTING OF THE NIRSpec FILTER- AND GRATING WHEEL ASSEMBLY
ALIGNMENT AND TESTING OF THE NIRSpec FILTER- AND GRATING WHEEL ASSEMBLY Thomas Leikert (1), Torsten Groß (1), Hans-Ulrich Wieland (1), Kai Weidlich (1) (1) Carl-Zeiss Optronics GmbH, Carl-Zeiss-Straße
Tutor in Systems Engineering / Project Management (2 posts)
Tutor in Systems Engineering / Project Management (2 posts) University College London Mullard Space Science Laboratory Department of Space and Climate Physics Holmbury St Mary Dorking, Surrey Grade - 7
LSST/Euclid/WFIRST Synergies
LSST/Euclid/WFIRST Synergies Steven M. Kahn LSST Director Stanford/SLAC/AURA Astrononomy and Astrophysics Advisory Commi2ee Mee5ng NASA/Goddard Space Flight Center January 29, 2016 LSST/Euclid/WFIRST Synergies
C/KOSMOS Work Breakdown Structure Summary
C/OSMOS Work Breakdown Structure Summary Version 2.3 January 13, 2011 Version Date Changes 1.8 November 19, 2009 Final version prior to issuing contract 1.9 December 8, 2009 Added documentation control
Introduction FRIGERIO ETTORE spa Lecco (Italy) Rev.09 1 / 19
Introduction FRIGERIO ETTORE spa Lecco (Italy) Rev.09 1 / 19 HISTORY Frigerio Ettore S.p.A. is a family run company founded in 1948 with a strong presence in the European metal working market. Frigerio
Applications. Blue IF 039, Green IF 062, Yellow IF 022, Orange IF 041, Red IF 090,Dark Red IF 091 IR pass IF 092, IF098, IF 093 Surface 1 5/2 0.
Color Filters Blue, Green, Yellow, Orange, Red & NIR Color Filters Blue and Green filters, transmitts wavelength in a corresponding color as seen by the human eye, while yellow, orange and red are long
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
ESSENCE: Determining the Nature of Dark Energy with High-z Supernovae
ESSENCE: Determining the Nature of Dark Energy with High-z Supernovae Ryan Foley UC Berkeley ESSENCE Team Equation of State: SupErNovae trace Cosmic Expansion C. Aguilera (NOAO/CTIO) B. Barris (IfA/UH)
Realization of a UV fisheye hyperspectral camera
Realization of a UV fisheye hyperspectral camera Valentina Caricato, Andrea Egidi, Marco Pisani and Massimo Zucco, INRIM Outline Purpose of the instrument Required specs Hyperspectral technique Optical
Summary of Data Management Principles Dark Energy Survey V2.1, 7/16/15
Summary of Data Management Principles Dark Energy Survey V2.1, 7/16/15 This Summary of Data Management Principles (DMP) has been prepared at the request of the DOE Office of High Energy Physics, in support
Solutions Manufacturing Performance
Solutions Manufacturing Performance Let s partner up for your project At RI Research Instruments we develop, design, manufacture and test high performance components and systems to the needs of our customers
Euro-VO DCA. Board Meeting #1 Oct 2-3, 2006. Nic Walton for Mike Watson. CDS Strasbourg
Euro-VO DCA Board Meeting #1 Oct 2-3, 2006 Nic Walton for Mike Watson CDS Strasbourg AstroGrid AstroGrid: UK's Virtual Observatory Empowerment of scientists Improve the quality, ease, speed and cost effectiveness
Jeremy Sakstein Curriculum Vitae
Contact Information University of Portsmouth Dennis Sciama Building Burnaby Road Portsmouth PO1 3FX Email: jeremy.sakstein@port.ac.uk Website: jeremysakstein.com www.icg.port.ac.uk/author/saksteij/ Academic
SGS System Requirements Review
SGS System Requirements Review John Hoar Lausanne 09/06/2015 Quick recap The Science Ground Segment transforms measurements made by the Euclid instruments into data products ready for scientific use. This
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
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,
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,
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.
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
Refractive Index Measurement Principle
Refractive Index Measurement Principle Refractive index measurement principle Introduction Detection of liquid concentrations by optical means was already known in antiquity. The law of refraction was
Astroparticle theory in France. Pierre Binetruy, APC. ASPERA Theory Meting, Oxford, 17 March 2008
Astroparticle theory in France Pierre Binetruy, APC ASPERA Theory Meting, Oxford, 17 March 2008 Two kinds of laboratories: general theory labs with an astroparticle physics group: Laboratoire de Physique
COMPANY OVERVIEW. International Sourcing Tooling Management Design & Product Engineering Rapid Prototyping Supply Chain Management
COMPANY OVERVIEW COMPANY OVERVIEW SINO INTERNATIONAL PRODUCTS import, manufacture, assemble and supply components to the automotive, rail and other industrial sectors Warwick Office United Kingdom Shanghai
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
The Search for Dark Matter, Einstein s Cosmology and MOND. David B. Cline
The Search for Dark Matter, Einstein s Cosmology and MOND David B. Cline Astrophysics Division, Department of Physics & Astronomy University of California, Los Angeles, CA 90095 USA dcline@physics.ucla.edu
LSST All Hands Meeting SLAC, December 4-8 2006 (MAP)
LSST All Hands Meeting SLAC, December 4-8 2006 (MAP) Monday, December 4 th Plenary Session Day One, Kavli Auditorium Project Status 1:00 Welcome; Project and MREFC Status D. Sweeney 1:40 Directors Report
Data Pipelines & Archives for Large Surveys. Peter Nugent (LBNL)
Data Pipelines & Archives for Large Surveys Peter Nugent (LBNL) Overview Major Issues facing any large-area survey/search: Computational power for search - data transfer, processing, storage, databases
Mapping structure of the Universe. the very large scale. INAF IASF Milano
Mapping the large scale structure of the Universe the very large scale structure Marco Scodeggio INAF IASF Milano The large scale structure (100Mpc) Zero order approximation: the Universe is homegeneous
Exploring Multiwavelength AGN Variability with Swift Archival Data
Exploring Multiwavelength AGN Variability with Swift Archival Data, a Caryl Gronwall, b Dirk Grupe, c Dan Vanden Berk d and Jian Wu e a Spectral Sciences Inc., 4 Fourth Ave., Burlington MA 01803, USA b
A high accuracy, small field of view star guider with application to SNAP.
A high accuracy, small field of view star guider with application to SNAP. Aurélia Secroun and Michael Lampton Space Sciences Laboratory, U.C. Berkeley Michael Levi Lawrence Berkeley National Laboratory,
JDEM ISWG Report to NASA and DOE Headquarters May 4. 2010. Executive Summary
JDEM ISWG Report to NASA and DOE Headquarters May 4. 2010 Executive Summary In December 2009, NASA HQ and DOE HQ asked the Joint Dark Energy Mission Interim Science Working Group (ISWG) to provide science
Data analysis of L2-L3 products
Data analysis of L2-L3 products Emmanuel Gangler UBP Clermont-Ferrand (France) Emmanuel Gangler BIDS 14 1/13 Data management is a pillar of the project : L3 Telescope Caméra Data Management Outreach L1
Integration Services
Integration Services EXPERIENCED TEAM ADVANCED TECHNOLOGY PROVEN SOLUTIONS Integrations for large scale metrology applications Metris metrology to streamline your CAPABILITIES Advanced systems design Engineering
The Sentinel-4/UVN instrument on-board MTG-S
The Sentinel-4/UVN instrument on-board MTG-S Grégory Bazalgette Courrèges-Lacoste; Berit Ahlers; Benedikt Guldimann; Alex Short; Ben Veihelmann, Hendrik Stark ESA ESTEC European Space Technology & Research
R&D Support Services. Ad Astra Rocket Company
R&D Support Services About Us A Delaware Corporation, capitalizing on more than 25 years of NASA R&D PhD Scientists, engineers, technicians skilled in the design fabrication and testing of prototype hardware.
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
Ph.D., Particle Physics Theory Thesis title: FCNC Processes of B and K Mesons from Lattice QCD University of Edinburgh October 1995 July1999
Curriculum Vitae Date of Birth: 8 th April 1971 Nationality: Place of Birth: Work Address: Taiwanese Taipei City Institute for Physics National Chiao-Tung University Hsinchu 300 Taiwan Work Telephone:
Outline: Yb optical frequency standard The fiber link Applications and fundamental physics
Orologi ottici e link in fibra: metrologia primaria di frequenza e fisica fondamentale. Davide Calonico Physical Metrology Division ISTITUTO NAZIONALE DI RICERCA METROLOGICA d.calonico@inrim.it 1 Outline:
SKA Dish Array Elements
SKA Dish Array Elements Eduardo Artal (1) Francisco Casas (2) (1) Departamento de Ingeniería de Comunicaciones (DICOM) Universidad de Cantabria. Santander. (2) Instituto de Física de Cantabria (IFCA).
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):
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
Possible use of the dedicated MARLY one meter telescope for intensive supernovæ studies
LAL 01-71 October 2001 Possible use of the dedicated MARLY one meter telescope for intensive supernovæ studies M. Moniez (moniez@lal.in2p3.fr), O. Perdereau (perderos@lal.in2p3.fr) Laboratoire de l Accélérateur
Visualization and Analysis of Spectral Data Cubes an Hipe toolbox
Visualization and Analysis of Spectral Data Cubes an Hipe toolbox Madrid 4-5 December 2008 Alain Gueguen MPE-Garching agueguen@mpe.mpg.de 1 Goal of the tool Display and analysis toolbox for the spectral
Understanding the Accelerating Universe using the MSE. Gong-Bo Zhao NAOC
Understanding the Accelerating Universe using the MSE Gong-Bo Zhao NAOC Nobel Prize 2011 a > 0 The expansion of the Universe can accelerate if In GR, to add new repulsive matter, which contributes 70%
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,
MY FIRST STEPS IN SLIT SPECTROSCOPY
MY FIRST STEPS IN SLIT SPECTROSCOPY Andrew Wilson BAAVSS Spectroscopy Workshop Norman Lockyer Observatory October 2015 Overview My choice of spectrograph, camera and telescope Getting started and basic
WP3: Infrastructure Web- Based Database
WP3: Infrastructure Web- Based Database Peter McIntosh (STFC, Daresbury Laboratory) TIARA Mid-Term Review Meeting, Madrid, 12-14 th June 2012. WP3 Infrastructure Database: https://tiara.astec.ac.uk TIARA
LSST Data Management System Applications Layer Simulated Data Needs Description: Simulation Needs for DC3
LSST Data Management System Applications Layer Simulated Data Needs Description: Simulation Needs for DC3 Draft 25 September 2008 A joint document from the LSST Data Management Team and Image Simulation
LBS-300 Beam Sampler for C-mount Cameras. YAG Focal Spot Analysis Adapter. User Notes
LBS-300 Beam Sampler for C-mount Cameras P/N SP90183, SP90184, SP90185 and SP90186 YAG Focal Spot Analysis Adapter P/N SP90187, SP90188, SP90189, SP90190, SP90191 User Notes Ophir-Spiricon Inc. 60 West
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
Experiment #5: Qualitative Absorption Spectroscopy
Experiment #5: Qualitative Absorption Spectroscopy One of the most important areas in the field of analytical chemistry is that of spectroscopy. In general terms, spectroscopy deals with the interactions
Astronomical and space-based systems engineering
The Role of Astronomy in Society and Culture, E19, 1 of 8 Proceedings IAU Symposium No. 260, 2009 D. Valls-Gabaud & A. Boksenberg, eds. c International Astronomical Union 2011 doi:10.1017/s1743921311003395
The LSST Data management and French computing activities. Dominique Fouchez on behalf of the IN2P3 Computing Team. LSST France April 8th,2015
The LSST Data management and French computing activities Dominique Fouchez on behalf of the IN2P3 Computing Team LSST France April 8th,2015 OSG All Hands SLAC April 7-9, 2014 1 The LSST Data management
High Resolution Digital Surface Models and Orthoimages for Telecom Network Planning
Renouard, Lehmann 241 High Resolution Digital Surface Models and Orthoimages for Telecom Network Planning LAURENT RENOUARD, S ophia Antipolis FRANK LEHMANN, Berlin ABSTRACT DLR of Germany and ISTAR of
We bring quality to light. MAS 40 Mini-Array Spectrometer. light measurement
MAS 40 Mini-Array Spectrometer light measurement Features at a glance Cost-effective and robust CCD spectrometer technology Standard USB interface Compatible with all Instrument Systems measuring adapters
Computing Advisory Panel (CAP) Preliminary enquiry in respect of future PRACE membership. Jan- 2014
Computing Advisory Panel (CAP) Preliminary enquiry in respect of future PRACE membership Jan2014 To: STFC supported researchers who depend upon HPC facilities, including Cosmology, Particle Physics, Astrophysics,
How Does One Obtain Spectral +Imaging Data
How Does One Obtain Spectral +Imaging Data What we observe depends on the instruments that one observes with! In x and γ-ray spectroscopy we have a wide variety of instruments with different properties
SPIRIT/CORONAS-F experiment
SPIRIT/CORONAS-F experiment S.V. Kuzin, V.A. Slemzin, A.M. Urnov P.N. Lebedev Physics Institute of RAS Leninsky pr., 53, Moscow, Russia 1. Description of the SPIRIT instrument Spectral bands Optical design
CONTAMINATION CONTROL FOR ELECTRONIC AND SEMICONDUCTOR APPLICATIONS
CONTAMINATION CONTROL FOR ELECTRONIC AND SEMICONDUCTOR APPLICATIONS UNDERSTANDING, ACCELERATED TSI SETS THE STANDARD FOR PARTICLE COUNTING Performance Semiconductor, hard disk drive, and flat panel manufacturers
Exoplanet and Solar System Synergy with Future Missions
Exoplanet and Solar System Synergy with Future Missions Britney Schmidt Georgia Tech OPAG Steering Committee Steve Vance, Jet Propulsion Lab Kunio Sayanagi, Hampton University Solar System Targets for
Very Large Telescope
EUROPEAN SOUTHERN OBSERVATORY Organisation Européene pour des Recherches Astronomiques dans l Hémisphère Austral Europäische Organisation für astronomische Forschung in der südlichen Hemisphäre ESO - European
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)
1 Table of Contents 1.1 List of Tables 1.2 List of Figures 2 Introduction 3 Global Peripheral Vascular Devices Market - Market Characterization 3.
1 Table of Contents 1.1 List of Tables 1.2 List of Figures 2 Introduction 3 Global Peripheral Vascular Devices Market - Market Characterization 3.1 Peripheral Vascular Devices Market, Revenue ($m), 2004-3.2
Products - Microarray Scanners - SpotLight Two-Color Microarray Fluorescence Scanners New! SpotLight 2 now available!
Products - Microarray Scanners - SpotLight Two-Color Microarray Fluorescence Scanners New! SpotLight 2 now available! Arrayit SpotLight Two-Color Microarray Scanners provide the market s most affordable
Company Presentation Federico Toriello
Company Presentation Federico Toriello Support Systems Other Services Young and competent company Started in 2007 in Germany, in 2004 in Portugal Technology cooperation partner of DLR Staff with more than
Spectral Measurement Solutions for Industry and Research
Spectral Measurement Solutions for Industry and Research Hamamatsu Photonics offers a comprehensive range of products for spectroscopic applications, covering the, Visible and Infrared regions for Industrial,
How To Set Up A Rov-Dfd (Rov Zero Point) Du)
DU640 Radial Velocity Zero-Point Software Requirement Specifications prepared by: approved by: reference: issue: 4 revision: 1 date: 28-03-2008 status: Issued G. Jasniewicz, F. Crifo, D. Hestroffer, A.
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).
Computer Vision: Machine Vision Filters. Computer Vision. Optical Filters. 25 August 2014
Computer Vision Optical Filters 25 August 2014 Copyright 2001 2014 by NHL Hogeschool, Van de Loosdrecht Machine Vision BV and Klaas Dijkstra All rights reserved j.van.de.loosdrecht@nhl.nl, jaap@vdlmv.nl,
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
SITools2 as VO service provider: an example with Herschel at IDOC (Integrated Data and Operation Center)
SITools2 as VO service provider: an example with Herschel at IDOC (Integrated Data and Operation Center) SITools 2 SITools2 is a CNES generic tool performed by a joint effort between CNES and scienefic