Specsim An IFU Spectrometer Simulator

4. Future telescopes & IFU facilities. Next generation IFUs Adaptive optics Extremely large telescopes Next space telescope: JWST

4. Future telescopes & IFU facilities Next generation IFUs Adaptive optics Extremely large telescopes Next space telescope: JWST Next generation IFUs At ESO: KMOS (infrared) MUSE (optical) XSHOOTER & SPHERE

MIRI The Mid-InfraRed Instrument for JWST The James Webb Space Telescope

MIRI The Mid-InfraRed Instrument for JWST The James Webb Space Telescope Prof. Gillian Wright, MBE Science and Technology Facilities Council UK-Astronomy Technology Centre JWST MIRI European PI Talk Overview

Instruments for ESO s Extremely Large Telescope

Instruments for ESO s Extremely Large Telescope at Dispersing Elements for Astronomy, October 2017 Suzanne Ramsay, ELT Instrumentation Project Manager on behalf of many ESO colleagues and the consortia

The Mid-Infrared Instrument for JWST. Some background about infrared astronomy The Mid-Infrared Instrument Some science ideas

The Mid-Infrared Instrument for JWST George Rieke Steward Observatory The University of Arizona Some background about infrared astronomy The Mid-Infrared Instrument Some science ideas Because the most

Subaru GLAO: Comparisons with Space Missions. I. Iwata (Subaru Telescope) 2011/08/ /05/28 small revisions 2013/06/04 include JWST/NIRISS

Subaru GLAO: Comparisons with Space Missions I. Iwata (Subaru Telescope) 2011/08/25 2013/05/28 small revisions 2013/06/04 include JWST/NIRISS Space Missions in Near-Future JWST 6.5m Deployable Mirror,

Scientific Capability of the James Webb Space Telescope and the Mid-InfraRed Instrument

Scientific Capability of the James Webb Space Telescope and the Mid-InfraRed Instrument Oliver Krause (Max Planck Institute for Astronomy, Heidelberg) on behalf of Gillian Wright (Royal Observatory Edinburgh)

E-ELT Spectroscopic ETC: Detailed Description

E-ELT Spectroscopic ETC: Detailed Description Jochen Liske Based on a document originally written by Pascal Ballester, Andrés Jordán, Markus Kissler- Patig & Jakob Vinther. 1. Preliminaries As of Jan 2008

Herschel Photodetector Array Camera & Spectrometer

Herschel Photodetector Array Camera & Spectrometer Albrecht Poglitsch, MPE Garching Christoffel Waelkens, Katholieke Universiteit Leuven Otto H. Bauer, Max-Planck-Institut für extraterrestrische Physik

Improving the observing efficiency of SINFONI and KMOS at the VLT by factors of 2 to 4: sophisticated sky subtraction algorithms

Improving the observing efficiency of SINFONI and KMOS at the VLT by factors of 2 to 4: sophisticated sky subtraction algorithms Niranjan A. Thatte *a, Nicholas Scott b, Ryan Houghton a, Dieter Nuernberger

Imaging with Micado at the E-ELT. WORKSHOP: Imaging at the E-ELT

Imaging with Micado at the E-ELT Renato Falomo INAF Observatory of Padova, Italy WORKSHOP: Imaging at the E-ELT 29 May 2009, Garching Resolved stellar population in Virgo (high SB) Detailed View of high

The World's Largest (operating) Telescopes.

The World's Largest (operating) Telescopes http://astro.nineplanets.org/bigeyes.html Subaru (8.2 meter) Subaru (8.2 meter) IRCS (Infrared Camera and Spectrograph 1024x1024 Alladin-2 0.9-5.6um imager 20

JWST/NIRSpec. P. Ferruit. (ESA JWST project scientist) Slide #1

P. Ferruit (ESA JWST project scientist)! Slide #1 Acknowledgements Thanks for giving me the opportunity to present the NIRSpec instrument. All along this presentation you will see the results of work conducted

MAORY (Multi conjugate Adaptive Optics RelaY) for E-ELT. Paolo Ciliegi. On behalf of the MAORY Consortium

MAORY (Multi conjugate Adaptive Optics RelaY) for E-ELT Paolo Ciliegi INAF Osservatorio Astronomico di Bologna On behalf of the MAORY Consortium Science ELT Workshop Team Meeting ESO Garching, MPE Garching,

Goals of the meeting. Catch up with JWST news and developments: ERS and GO call for proposals are coming!!

Welcome Goals of the meeting Catch up with JWST news and developments: ERS and GO call for proposals are coming!! What is JWST capable of (focus on H 2 spectroscopy)? What do we need to do (models, lab)

The next-generation Infrared astronomy mission SPICA Space Infrared Telescope for Cosmology & Astrophysics

The next-generation Infrared astronomy mission SPICA Space Infrared Telescope for Cosmology & Astrophysics 3.5m cooled telescope mission for mid- and far-infrared astronomy Takao Nakagawa (ISAS/JAXA) for

Subaru Telescope Ground Layer AO System and New Near-IR Instrument

Subaru Telescope Ground Layer AO System and New Near-IR Instrument 2013/04/15 I. Iwata (New Development Group, Subaru Telescope, NAOJ) photo by Sebastian Egner Subaru Next-Gen AO Working Group Founded

GEMINI 8-M Telescopes Project

GEMINI 8-M Telescopes Project RPT-PS-G0065 The Gemini Instrumentation Program F. C. Gillett, D. A. Simons March 25, 1996 GEMINI PROJECT OFFICE 950 N. Cherry Ave. Tucson, Arizona 85719 Phone: (520) 318-8545

What will the future bring? Scientific discoveries expected from the E-ELT

What will the future bring? Scientific discoveries expected from the E-ELT Planets & Stars Stars & Galaxies Galaxies & Cosmology Eline Tolstoy Kapteyn Astronomical Institute, University of Groningen E-ELT

Introduction to SDSS -instruments, survey strategy, etc

Introduction to SDSS -instruments, survey strategy, etc (materials from http://www.sdss.org/) Shan Huang 17 February 2010 Survey type Status Imaging and Spectroscopy Basic Facts SDSS-II completed, SDSS-III

Integrated spectrographs in the era of ELTs

Integrated spectrographs in the era of ELTs N. Blind Max-Planck Institut fur Extraterrestrische Physik (MPE; Garching, D.) IPAG seminar - 04.02.2013! APE 1 Context: Extremely Large Telescopes... E-ELT

A Gigan2c Step into the Deep Universe

MOSAIC@ELT: A Gigan2c Step into the Deep Universe presented by François Hammer http://www.mosaic-elt.eu ESO is now building the future largest telescope First light: 2024 MOSAIC core team has developed,

Ongoing and upcoming observations and their implication for exoplanet and brown dwarf studies.

Giant planets in the Solar System Ongoing and upcoming observations and their implication for exoplanet and brown dwarf studies. Henrik Melin, Steve Miller, Leigh Fletcher, Pat Irwin, Glenn Orton, Kevin

Instrumentation for 2D Spectroscopy

Instrumentation for 2D Spectroscopy Suresh Sivanandam Assistant Professor Department of Astronomy and Astrophysics Dunlap Institute University of Toronto KIAA-PKU Astrophysics Forum Focus of Our Research

Large Area Imaging Survey of Near-Infrared Sky with Korean Compact Space Telescopes

Large Area Imaging Survey of Near-Infrared Sky with Korean Compact Space Telescopes Science & Technology Satellite Series (KARI) (2000 ~ 2013. 02) 1 st Satellite: FIMS (Far-ultraviolet IMaging Spectrograph)

Science Drivers for the European Extremely Large Telescope

Science Drivers for the European Extremely Large Telescope Suzanne Ramsay E-ELT Instrumentation Project Manager for Michele Cirasuolo E-ELT Programme Scientist Outline of the talk From an scientific idea

PROBING THE SURFACE COMPOSITION OF TRANSNEPTUNIAN OBJECTS WITH JWST/NIRSPEC. P. Ferruit & A. Guilbert Lepoutre

PROBING THE SURFACE COMPOSITION OF TRANSNEPTUNIAN OBJECTS WITH JWST/NIRSPEC P. Ferruit & A. Guilbert Lepoutre Trans-Neptunian Objects (TNOs) ~1600 known TNOs and Centaurs (between Jupiter & Neptune). Sub-populations

Integral Field Spectroscopy. David Burnham & Trystyn Berg

Integral Field Spectroscopy David Burnham & Trystyn Berg Introduc;on Integral Field Units (IFUs) are rela;vely new instruments in astronomy for obtaining spa;ally resolved spectra. The largest and most

Optimal resolutions for optical and NIR spectroscopy S. Villanueva Jr.* a, D.L. DePoy a, J. L. Marshall a

Optimal resolutions for optical and NIR spectroscopy S. Villanueva Jr.* a, D.L. DePoy a, J. L. Marshall a a Department of Physics and Astronomy, Texas A&M University, 4242 TAMU, College Station, TX, USA

Problem Solving. radians. 180 radians Stars & Elementary Astrophysics: Introduction Press F1 for Help 41. f s. picture. equation.

Problem Solving picture θ f = 10 m s =1 cm equation rearrange numbers with units θ factors to change units s θ = = f sinθ fθ = s / cm 10 m f 1 m 100 cm check dimensions 1 3 π 180 radians = 10 60 arcmin

Detectors for IR astronomy

Detectors for IR astronomy Where does infrared begin? Wavelength sensi?vity of the human eye vs. wavelength Note: the eye has some (limited) sensi?vity to IR light at ~1000nm (=0.5x energy of photons the

Outflows in regions of massive star formation. Suzanne Ramsay (ESO), Watson Varricatt (UKIRT), Chris Davis (NSF)

Outflows in regions of massive star formation Suzanne Ramsay (ESO), Watson Varricatt (UKIRT), Chris Davis (NSF) How do massive stars form? Do high mass stars (>8Msolar) form in the same way as low mass

Report to the GSMT Committee

Report to the GSMT Committee P. McCarthy GMT Science Working Group and GMT Board GMT Consortium Status Conceptual Design Review AO Systems GMT Instrument Candidates Instrument properties Potential scientific

1. Give short answers to the following questions. a. What limits the size of a corrected field of view in AO?

Astronomy 418/518 final practice exam 1. Give short answers to the following questions. a. What limits the size of a corrected field of view in AO? b. Describe the visibility vs. baseline for a two element,

The Austrian contribution to the European Extremely Large Telescope

The Austrian contribution to the European Extremely Large Telescope Werner W. Zeilinger consortium Evolution of Telescope Size Scientific American 2015 14/15.Dec.2015 From Ground to Space 2 Discoveries

CASE/ARIEL & FINESSE Briefing

CASE/ARIEL & FINESSE Briefing Presentation to NRC Committee for Exoplanet Science Strategy including material from the ARIEL consortium Mark Swain - JPL 19 April 2019 2018 California Institute of Technology.

The infrared imaging spectrograph (IRIS) for TMT: sensitivities and simulations

The infrared imaging spectrograph (IRIS) for TMT: sensitivities and simulations Shelley A. Wright a*, Elizabeth J. Barton b, James E. Larkin c, Anna M. Moore d, David Crampton e,f, Luc Simard e,f, and

NEON Archive School 2006

NEON Archive School 2006 Introduction to Spectroscopic Techniques (low dispersion) M. Dennefeld (IAP-Paris) Outline Basic optics of gratings and spectrographs (with emphasis on long-slit spectroscopy)

A Million Element Integral Field Unit (MEIFU)

A Million Element Integral Field Unit (MEIFU) Simon Morris 1, Robert Content 1, Ray Sharples 1, Richard Bower 1, Roger Davies 1, and Carlton Baugh 1 Physics Department, Durham University, South Rd., Durham,

The James Webb Telescope (NGST) to replace HST

PROLOGUE The James Webb Telescope (NGST) to replace HST Source: http://www.jwst.nasa.gov/ Key elements: 6.5m primary mirror (18 sections), lightweight, deployable (launch date 2013?) 1 Large sunshield

Reduction procedure of long-slit optical spectra. Astrophysical observatory of Asiago

Reduction procedure of long-slit optical spectra Astrophysical observatory of Asiago Spectrograph: slit + dispersion grating + detector (CCD) It produces two-dimension data: Spatial direction (x) along

Grand Canyon 8-m Telescope 1929

1 2 Grand Canyon 8-m Telescope 1929 3 A World-wide Sample of Instruments 4 Instrumentation Details Instrument name Observing Modes Start of operations Wavelength Coverage Field of View Instrument cost

Observations of First Light

Image from Space Telescope Science Institute Observations of First Light Betsy Barton (UC Irvine) Member, TMT SAC Project Scientist, IRIS on TMT Microwave Background What reionized the universe? The End

Adaptive Optics Status & Roadmap. Norbert Hubin Adaptive Optics Department European Southern Observatory November 2007

Adaptive Optics Status & Roadmap Norbert Hubin Adaptive Optics Department European Southern Observatory November 2007 1 Analysis CASIS: VLT MCAO Imager NACO upgrade Commissioning PAC The ESO Adaptive Optics

The Large UV Optical IR survey telescope. Debra Fischer

The Large UV Optical IR survey telescope Debra Fischer Yale University How do we identify worlds that are most promising for life? Host star insolation determines the probability of retaining water. Habitable

Million Element Integral Field Unit Design Study

Million Element Integral Field Unit Design Study Simon Morris, Robert Content, Cedric Lacey (University of Durham, UK) AURA contract No. 9414257-GEM00303 Milestone 1 Prepare and present a PowerPoint presentation

Instrumentation for The European Extremely Large Telescope Science and Technology with E-ELT Erice, October 2015

Instrumentation for The European Extremely Large Telescope Science and Technology with E-ELT Erice, October 2015 Suzanne Ramsay (sramsay@eso.org) Outline of the talk The environment for instruments on

On-sky test of sky subtraction methods for fiber-fed spectrograph

On-sky test of sky subtraction methods for fiber-fed spectrograph Myriam Rodrigues a, M. Cirasuolo c, F. Hammer b, F. Royer b, C. Evans c, M. Puech b, H. Flores b, I. Guinouard b, Gianluca Li Causi d,

Suresh Sivanandam (PI) University of Toronto

GIRMOS: Gemini Infrared Multi-Object Spectrograph A TMT Pathfinder Instrument Suresh Sivanandam (PI) University of Toronto A B A. SINFONI Velocity Map of z~2 Galaxy B. Hubble XDF with GIRMOS Fields Overlaid

Science with Micado. the high resolution camera for the E-ELT Renato Falomo. INAF Observatory of Padova, Italy. 25 February IASF, Milano

Science with Micado the high resolution camera for the E-ELT Renato Falomo INAF Observatory of Padova, Italy 25 February 2010 -- IASF, Milano Overview of MICADO (Tehnology & Science) Resolved stellar population

Very compact galaxies at high-z

Turbulent / High-density disks at high-z Typical galaxy seen in the local universe Very compact galaxies at high-z Clumpy galaxies at high-z Example image of a massive galaxy at z=1.0 Even if we put this

Preparing staff for ELT science operations activities

Preparing staff for ELT science operations activities Andres Pino Pavez European Southern Observatory ESA/ESO Sciops Workshop 2017 Working together in support of science 17-20 OCTOBER 2017 - EUROPEAN SPACE

JWST/NIRSpec. P. Ferruit. (ESA JWST project scientist) Slide #1

P. Ferruit (ESA JWST project scientist)! Slide #1 Acknowledgements Thanks for giving me the opportunity to present the NIRSpec instrument. All along this presentation you will see the results of work conducted

Hubble Science Briefing

Hubble Science Briefing Delivering JWST Science, from Exoplanets to First Light: The Near-InfraRed Imager and Slitless Spectrograph (NIRISS) March 6, 2014 Alex Fullerton (STScI) 1 Agenda for Today The

ABSTRACT. a Institute for Space Imaging Science, University of Lethbridge, Alberta, T1K 3M4, Canada; b Joint

The spectral response of the SCUBA-2 850 and 450 micron photometric bands David A. Naylor* a, Brad G. Gom a, Sherif AbdElazim a, Per Friberg b, Daniel Bintley b, Wayne S. Holland c, Michael J. MacIntosh

ULTIMATE-SUBARU: Science Cases. Ikuru Iwata (Subaru Telescope, NAOJ)

ULTIMATE-SUBARU: Science Cases Ikuru Iwata (Subaru Telescope, NAOJ) Subaru next-gen AO working group + Collaborators Subaru / NAOJ: Yutaka Hayano, Shin Oya, Yosuke Minowa, Tadayuki Kodama, Nobuo Arimoto,

ATHENA Mission Design and ESA Status. David Lumb ESA Study Scientist MPE Jan 13 th 2012

ATHENA Mission Design and ESA Status David Lumb ESA Study Scientist MPE Jan 13 th 2012 Topics covered ESA L class mission reformulation Current status & programmatics Athena Mission Design Spacecraft Optics

Characterisation & Use of Array Spectrometers

Characterisation & Use of Array Spectrometers Mike Shaw, Optical Technologies & Scientific Computing Team, National Physical Laboratory, Teddington Middlesex, UK 1 Overview Basic design and features of

Introduction of near-infrared (NIR) spectroscopy. Ken-ichi Tadaki (NAOJ)

Introduction of near-infrared (NIR) spectroscopy Ken-ichi Tadaki (NAOJ) Near-infrared in astronomy absorption by terrestrial atmosphere - wavelength range of 1-5 um - observable windows are limited (J,

Continuum Submillimetre Astronomy from UKIRT. Ian Robson UK ATC

Continuum Submillimetre Astronomy from UKIRT Ian Robson UK ATC Submillimetre means high - how high can we get? let s s go to Hawaii! (1975,( 76) We need a submillimetre photometer! Lots of lessons learned

Dynamics of High Redshift Galaxies M. Stiavelli, STScI Baltimore

Lecture plan: Dynamics of High Redshift Galaxies M. Stiavelli, STScI Baltimore 1. Introduction. Galaxy kinematics at high redshift. 2. Dynamics of elliptical galaxies at high redshift and evolution of

#JWSTnearbygalaxies @JWSTObserver #jwst @KISS_Caltech Welcome WebEx Participants To ask a question or contribute to the discussion: Select send to moderator and type your question/comment into the chat

Todays Topics 3/19/2018. Light and Telescope. PHYS 1403 Introduction to Astronomy. CCD Camera Makes Digital Images. Astronomical Detectors

PHYS 1403 Introduction to Astronomy Light and Telescope Chapter 6 Todays Topics Astronomical Detectors Radio Telescopes Why we need space telescopes? Hubble Space Telescopes Future Space Telescopes Astronomy

From the VLT to ALMA and to the E-ELT

From the VLT to ALMA and to the E-ELT Mission Develop and operate world-class observing facilities for astronomical research Organize collaborations in astronomy Intergovernmental treaty-level organization

These notes may contain copyrighted material! They are for your own use only during this course.

Licensed for Personal Use Only DO NOT DISTRIBUTE These notes may contain copyrighted material! They are for your own use only during this course. Distributing them in anyway will be considered a breach

The E-ELT Telescope, instruments, technology. Mark Casali

The E-ELT Telescope, instruments, technology Mark Casali Project Goal To deliver and commission, in 2024 and within budget, the fully functional and complete European Extremely Large Telescope 39.3 m segmented

Giant Magellan Telescope. ALMA/ELT Workshop March

Giant Magellan Telescope ALMA/ELT Workshop March 2009 1 GMT Partners Astronomy Australia Limited Australian National University Carnegie Institution of Washington Harvard University Korea Astronomy & Space

Technology Developments for ESO at the IAC

Jornada ESO 2011, Granada, 10-11/02/2011 Technology Developments for ESO at the IAC Head of Technology Division 1 Technology involvement in ESO Instruments: Espresso for the VLT CODEX and HARMONI for the

Spitzer Space Telescope

Spitzer Space Telescope (A.K.A. The Space Infrared Telescope Facility) The Infrared Imaging Chain 1/38 The infrared imaging chain Generally similar to the optical imaging chain... 1) Source (different

Presented by B. Neichel. Wide-Field Adaptive Optics for ground based telescopes: First science results and new challenges

Edinburgh 25 th March 2013 Presented by B. Neichel Wide-Field Adaptive Optics for ground based telescopes: First science results and new challenges Outline A brief Introduction to Adaptive Optics (AO)

G.Witzel Physics and Astronomy Department, University of California, Los Angeles, CA , USA

E-mail: shahzaman@ph1.uni-koeln.de A.Eckart E-mail: eckart@ph1.uni-koeln.de G.Witzel Physics and Astronomy Department, University of California, Los Angeles, CA 90095-1547, USA N. Sabha M. Zamaninasab

Planck and Virtual Observatories: Far Infra-red / Sub-mm Specificities

JF Sygnet (Planck HFI DPCM) Planck and Virtual Observatories: Far Infra-red / Sub-mm Specificities Planck Mission, Planck Data and its Specificities (4) Data Treatment and its Specificities (4) Planck

Universe Now. 2. Astronomical observations

Universe Now 2. Astronomical observations 2. Introduction to observations Astronomical observations are made in all wavelengths of light. Absorption and emission can reveal different things on different

CIRMOS. 4/26/2010 Tetsuo Nishimura

CIRMOS 4/26/2010 Tetsuo Nishimura About the name CIRMOS Thermos -- Hot Matters. Cold Matters. It Matters. How about Dark Matter?... Does it matter? Dark Matter Astronomy? Does Dark Matter deserve an astronomy?

Notes: Reference: Merline, W. J. and S. B. Howell (1995). "A Realistic Model for Point-sources Imaged on Array Detectors: The Model and Initial

Notes: Notes: Notes: Reference: Merline, W. J. and S. B. Howell (1995). "A Realistic Model for Point-sources Imaged on Array Detectors: The Model and Initial Results." Experimental Astronomy 6: 163-210.

arxiv: v1 [astro-ph.im] 20 Jul 2012

The Development of WIFIS: a Wide Integral Field Infrared Spectrograph arxiv:1207.5053v1 [astro-ph.im] 20 Jul 2012 Suresh Sivanandam a, Richard C. Y. Chou b, Dae-Sik Moon b, Ke Ma b, Maxwell Millar-Blanchaer

Status of the JWST Science Instrument Payload

Status of the JWST Science Instrument Payload Ma9 Greenhouse JWST Project Office NASA Goddard Space Flight Center 12 October 2015 @NASAWebbTelescp #JWST 12 October 2015 PresentaBon to: 49th ESLAB Symposium:

Spectroscopy at 8-10 m telescopes: the GTC perspective. Romano Corradi GRANTECAN

Spectroscopy at 8-10 m telescopes: the GTC perspective Romano Corradi GRANTECAN Spectroscopy from large ground-based telescope At the vanguard of observational astronomy is a growing family of >8m telescopes:

E-ELT/METIS. 1 Introduction to METIS

Conditions and Impact of Star Formation R. Simon, R. Schaaf and J. Stutzki (eds) EAS Publications Series, 75-76 (2015) 405 410 E-ELT/METIS B. Brandl 1, S. Quanz 2,M.Feldt 3,A.Glasse 4,M.Guedel 5,M.Meyer

The NFIRAOS MCAO System on the Thirty Meter Telescope. Paul Hickson, UBC MAD

The NFIRAOS MCAO System on the Thirty Meter Telescope Paul Hickson, UBC MAD2009 2009-06-10 TMT in a nutshell 30m f/1 primary, RC optics, 20 field of view Filled circular aperture high contrast PSF Integrated

TMT Overview Telescope / Instruments / Sites

1 SUBARU N a t io na l A s t r o n o m ic a l J a p an TMT Overview Telescope / Instruments / Sites of O b s e r v a t o r y Tomonori USUDA (SUBARU Telescope) TMT Reference Design (as of Dec 06)! Costs:

MIRI, METIS and the exoplanets. P.O. Lagage CEA Saclay

MIRI, METIS and the exoplanets P.O. Lagage CEA Saclay French Co-PI of JWST-MIRI and Coordinator of European MIRI GTO on exoplanets Member of the ELT-METIS science team Why MIRI and METIS? Because of my

Optical/IR Observational Astronomy Spectroscopy. David Buckley, SALT

David Buckley, SALT 1 Background is really just monochromatic photometry History 1637 Descartes explained the origin of the rainbow. 1666 Newton s classic experiments on the nature of colour. 1752 Melvil

ORBS and ORCS. Reduction and analysis of SITELLE's data

ORBS and ORCS Reduction and analysis of SITELLE's data omas Martin (Université Laval) Laurent Drissen (Université Laval) Laurie Rousseau-Nepton (Université Laval), Alexandre Alarie (Université Laval),

SIMULATIONS OF HIGH-Z GALAXY OBSERVATIONS WITH AN E-ELT/MOS

Florence, Italy. May 2013 ISBN: 978-88-908876-0-4 DOI: 10.12839/AO4ELT3.12389 SIMULATIONS OF HIGH-Z GALAXY OBSERVATIONS WITH AN E-ELT/MOS Mathieu Puech 1a, Karen Disseau 1, Laura Pentericci 2, and the

Tests of MATISSE on large spectral datasets from the ESO Archive

Tests of MATISSE on large spectral datasets from the ESO Archive Preparing MATISSE for the ESA Gaia Mission C.C. Worley, P. de Laverny, A. Recio-Blanco, V. Hill, Y. Vernisse, C. Ordenovic and A. Bijaoui

The First Billion Year of History - Galaxies in the Early Universe. Stephen Wilkins, Silvio Lorenzoni, Joseph Caruana, Holly Elbert, Matt Jarvis

The First Billion Year of History - Galaxies in the Early Universe Stephen Wilkins, Silvio Lorenzoni, Joseph Caruana, Holly Elbert, Matt Jarvis X recent z=8.3 GRB CCDs HST Keck Subaru Picture credit:

HIGH RESOLUTION IN THREE DIMENSIONS WITH SWIFT AND PALM3K

Florence, Italy. Adaptive May 2013 Optics for Extremely Large Telescopes III ISBN: 978-88-908876-0-4 DOI: 10.12839/AO4ELT3.13428 HIGH RESOLUTION IN THREE DIMENSIONS WITH SWIFT AND PALM3K Fraser Clarke

W. M. Keck Observatory Subaru Users Meeting

W. M. Keck Observatory Subaru Users Meeting Taft Armandroff, Director January 16, 2013 Table of Contents Keck / Subaru Exchange Program Recent Keck Observatory Instrumentation and Adaptive Optics Development

Gemini Integration Time Calculators

Gemini Integration Time Calculators Phil Puxley SPE-C-G0076 Version 1.1; June 1998 Version History: 1.0 June 1998; first draft. 1.1 June 1998; following comments from Ted von Hippel and Joe Jensen. 1.

ADAPTIVE OPTICS SYSTEMS FOR ASTRONOMY: ITALIAN INDUSTRIAL AND RESEARCH ESTABLISHMENTS

ADAPTIVE OPTICS SYSTEMS FOR ASTRONOMY: ITALIAN INDUSTRIAL AND RESEARCH ESTABLISHMENTS Daniele Gallieni A.D.S. International S.r.l. JINR, Dubna, Dec.21, 2010 Adaptive optics The wavefront sensor measures

SALT s Venture into Near Infrared Astronomy with RSS NIR

SALT s Venture into Near Infrared Astronomy with RSS NIR Marsha Wolf University of Wisconsin Madison IUCAA RSS VIS future RSS NIR 5 June 2015 SALT Science Conference 2015 2 Robert Stobie Spectrograph 5

TMT and Space-Based Survey Missions

TMT and Space-Based Survey Missions Daniel Stern Jet Propulsion Laboratory/ California Institute of Technology 2014 California Institute of Technology TMT Science Forum 2014 July 17 Outline Summary of

Hanle Echelle Spectrograph (HESP)

Hanle Echelle Spectrograph (HESP) Bench mounted High resolution echelle spectrograph fed by Optical Fiber Second generation instrument for HCT The project is a technical collaboration between Indian Institute

Studies for the first generation of instruments for the European ELT

Studies for the first generation of instruments for the European ELT Sandro D Odorico a, Mark Casali a, Juan-Carlos Gonzalez a, Markus Kasper a, Hans Ulrich Käufl a, Markus Kissler Patig a, Luca Pasquini

Astronomical Techniques I

Astronomical Techniques I Lecture 8 Yogesh Wadadekar Jan-Feb 2015 IUCAA-NCRA Grad School 1 / 28 Assignment 1 will be posted on the website by tonight or tomorrow morning. Kaustubh Vaghmare (kaustubh@iucaa.ernet.in)

MESSIER Unveiling galaxy formation

MESSIER Unveiling galaxy formation David Valls-Gabaud on behalf of the MESSIER consortium Challenges in UV astronomy ESO - 2013 Oct 09 Two driving science cases for critical tests of the ΛCDM paradigm

ALGORITHM TO CORRECT FOR ATMOSPHERIC DIFFERENTIAL REFRACTION ON OSIRIS DATA CUBES

ALGORITHM TO CORRECT FOR ATMOSPHERIC DIFFERENTIAL REFRACTION ON OSIRIS DATA CUBES Denny C. Dement III Department of Physics and Astronomy University of Hawai i at Hilo Hilo, HI 96720 ABSTRACT Near the

Keck Adaptive Optics Note 1069

Keck Adaptive Optics Note 1069 Tip-Tilt Sensing with Keck I Laser Guide Star Adaptive Optics: Sensor Selection and Performance Predictions DRAFT to be updated as more performance data becomes available

arxiv: v1 [astro-ph] 5 Mar 2008

X-shooter: a medium-resolution, wide-band spectrograph for the VLT arxiv:0803.0609v1 [astro-ph] 5 Mar 2008 L. Kaper 1, S. D Odorico 2, F. Hammer 3, R. Pallavicini 4, P. Kjaergaard Rasmussen 5, H. Dekker

Synergy between MOSAIC, MICADO, and MUSE:

Synergy between MOSAIC, MICADO, and MUSE: resolved stellar populations in nearby galaxies Martin M. Roth (P.I.) Andreas Kelz Leibniz-Institute for Astrophysics Potsdam (AIP) University of Potsdam Toledo,