CHARACTERIZING EXOPLANETS WITH HIGH DISPERSION CORONAGRAPHY ON TMT
|
|
- Charlene Shields
- 5 years ago
- Views:
Transcription
1 CHARACTERIZING EXOPLANETS WITH HIGH DISPERSION CORONAGRAPHY ON TMT DIMITRI MAWET, CALTECH, NOVEMBER 2017 HDC CALTECH/JPL: J. WANG, J. JOVANOVIC, J-R DELORME, J. LLOP, N. KLIMOVICH, Y. XIN, W. XUAN, J. WALLACE, J. FUCIK, G. RUANE EXOPLANET ATMOSPHERES: B. BENNEKE (NOW AT U. MONTREAL), R. HU (JPL), S. DOMOGAL-GOLDMAN (GSFC), G. ARNEY (GSFC), J. FORTNEY KPIC HDC COLLABORATORS: M. FITZGERALD (UCLA), FROM WMKO: P. WIZINOWICH, S. CETRE, B. FEMENIA, S. LILLEY, E. WETHERELL, S. RAGLAND
2 HIGH DISPERSION CORONAGRAPHY Wang et al. 2017, Mawet et al. 2017
3 HIGH RESOLUTION SPECTROSCOPIC CHARACTERIZATION OF EXOPLANETS Unambiguous identification of molecules such as CO, CH 4, CO 2, O 3, O 2
4 PROOF OF CONCEPT AT MEDIUM RESOLUTION WITH OSIRIS AND HR8799 Marois et al (2010)
5 HR8799c Konopacky et al. 2013
6 HR8799b Barman et al. 2015
7 HIGH RESOLUTION SPECTROSCOPIC CHARACTERIZATION OF EXOPLANETS Unambiguous identification of molecules such as CO, CH 4, CO 2, O 3, O 2 Line broadening: => spin measurements => planet accretion history => final mass and atmospheric composition => formation of moons and rings
8 MEASURE PLANET SPIN a Relative position ( ) Snellen et al (CRIRES@VLT) Stellar velocity Star position Planet position b CC signal Velocity (km s 1 ) Velocity (km s 1 ) Bryan et al Keck)
9 HIGH RESOLUTION SPECTROSCOPIC CHARACTERIZATION OF EXOPLANETS Unambiguous identification of molecules such as CO, CH 4, CO 2, O 3, O 2 Line broadening: => spin measurements => planet accretion history => final mass and atmospheric composition => formation of moons and rings Time Domain Analysis of line profile: => Doppler imaging => Global circulation => Cloud coverage and weather
10 DOPPLER MAPPING OF GIANT PLANETS Crossfield et al. 2014
11 HIGH RESOLUTION SPECTROSCOPIC CHARACTERIZATION OF EXOPLANETS Unambiguous identification of molecules such as CO, CH 4, CO 2, O 3, O 2 Line broadening: => spin measurements => planet accretion history => final mass and atmospheric composition => formation of moons and rings Time Domain Analysis of line profile: => Doppler imaging => Global circulation => Cloud coverage and weather Contrast gains: => gains α N lines (# lines resolved) => Sidesteps chromatic speckle noise present and inevitable at low res
12 ELTs GPI/SPHERE HDC CONTRAST GAINS N lines
13 ASTROBIOLOGIST S FLOWCHART TO CHAMPAGNE S. Domagal-Goldman (GSFC)
14 BIOSIGNATURES AT HIGH R Wang J., Mawet D., Hu R., Benneke B. 2017
15 DETECTING BIO-SIGNATURE GASES WITH HDC ON TMT SNR contour map SNR contour map M dwarf planet at 5 pc CO2 Proxima Cen b O2 planet signal is ~10-8 Wang et al. 2017
16 DETECTING BIO-SIGNATURE GASES WITH HDC AT TMT SNR contour map SNR contour map M dwarf planet at 5 pc CO2 Proxima Cen b O2 planet signal is ~10-8 Wang et al. 2017
17 DETECTING BIO-SIGNATURE GASES WITH HDC AT TMT SNR contour map SNR contour map M dwarf planet at 5 pc CO2 Proxima Cen b O2 planet signal is ~10-8 Wang et al. 2017
18 BOTTOM LINE HDC might be the only way to tease out biomarkers from Earth-like and super-earth exoplanets HDC enables detailed characterization from optical to infrared: composition, spin, cloud mapping Strong synergies with transit spectroscopy and RV: fiber-fed diffraction limited high-resolution spectrographs
19 PSI strawman concept PSI-Blue Vis WFS PSI-Red IR WFS Woofer DM Cold Coronagraph Coronagraph Tweeter DM 8-13 μm Imager μm IFU/Imager μm High-Res Cold Coronagraph 2-5 μm High-Res 2-5 μm IFU/Imager
20 HRS CONCEPTUAL DESIGN (MODIUS) 9-channel Multiplexing using H4RG, 25-channel possible (reduced bw) Echelle Gra*ng Fiber Ap. Stop Coll OAP CX Prism Camera M2 H4RG Detector Camera M1 RV ready J. Fucik (COO) Camera M3
21 HIGH DISPERSION CORONAGRAPHY DEMONSTRATOR IN THE CALTECH EXOPLANET TECHNOLOGY LAB Mawet et al. 2017
22 HIGH DISPERSION CORONAGRAPHY SCIENCE DEMONSTRATOR WITH KPIC Keck Planet Imager and Characterizer
23 KPIC HDC MODULE 2nd relay Tip-Tilt mirror Fiber port 1 Fiber port 2 FIU dichroic #2 MEMS DM FIU dichroic #1 Tracking camera AO focus 1st relay Up
24 PERSPECTIVES Theoretical studies/numerical simulations: Refine HDC simulators (exo-zodis, telescope/system emissivity, speckle chromaticity) Refine theoretical models of exoplanet atmospheres Better spectroscopic templates Capture diversity of planets Archean Earth modeling HDC science demonstrators: Keck/NIRSPEC Subaru/IRD VLT/CRIRES Palomar
25 COLLABORATORS Caltech: J. Wang, N. Jovanovic, G. Ruane, J.-R. Delorme, R. Dekany, J. Fucik, N. Klimovich, J. Llop, R. Riddle, K. Matthews JPL: J.K. Wallace, E. Serabyn, G. Vasisht, R. Bartos, M. Bottom, AJ Riggs W.M. Keck Observatory: P. Wizinowich, S. Cetre, B. Femenia, S. Lilley, E. Wetherell, S. Ragland University of Hawaii: M. Chun, C. Bond, C. Baranec, D. Hall, D. Atkinson, S. Goebel, C. Lockhart, E. Warmbier University of Liege: O. Absil, E. Huby*, B. Carlomagno, C. Gomez, A. Jolivet, J. Surdej, S. Habraken, C. Delacroix** Uppsala University: E. Vargas, P. Forsberg, M. Karlsson UCLA: M. Fitzgerald Subaru: O. Guyon LAM: T. Fusco Arcetri: S. Esposito, C. Plantet ANU: F. Rigault (*) ULg -> ObsPM (**) ULg -> Cornel
A FIBER INJECTION UNIT FOR EXOPLANET SPECTROSCOPY
A FIBER INJECTION UNIT FOR EXOPLANET SPECTROSCOPY Presenter: Wenhao Xuan Mentor: Dimitri Mawet Collaboratorsrs: Garreth Ruane, James Kent Wallace, Daniel Echeverri, Michael Randolph Marois et al. 2008
More informationExoplanet Instrumentation with an ASM
Exoplanet Instrumentation with an ASM Olivier Guyon1,2,3,4, Thayne Currie 1 (1) Subaru Telescope, National Astronomical Observatory of Japan (2) National Institutes for Natural Sciences (NINS) Astrobiology
More informationKeck Planet Imager and Characterizer: concept and phased implementation
Keck Planet Imager and Characterizer: concept and phased implementation D. Mawet a,b, P. Wizinowich c, R. Dekany a, M. Chun d, D. Hall d, S. Cetre c, O. Guyon e, J.K. Wallace b, B. Bowler f, M. Liu g,
More informationThe Planetary Systems Imager: 2-5 Micron Channel
The Planetary Systems Imager: 2-5 Micron Channel Andrew J. Skemer a, Deno Stelter a, Dimitri Mawet b, Michael Fitzgerald c, Benjamin Mazin d, Olivier Guyon e, Christian Marois f, Zackery Briesemeister
More informationlife detection capabilities of LUVOIR and HabEx and WFIRST
life detection capabilities of LUVOIR and HabEx and WFIRST Shawn Domagal-Goldman NASA Goddard Space Flight Center Deputy Study Scientist, LUVOIR Science and Technology Definition Team member, HabEx Image
More informationDirect imaging and characterization of habitable planets with Colossus
Direct imaging and characterization of habitable planets with Colossus Olivier Guyon Subaru Telescope, National Astronomical Observatory of Japan University of Arizona Contact: guyon@naoj.org 1 Large telescopes
More informationTMT High-Contrast Exoplanet Science. Michael Fitzgerald University of California, Los Angeles (UCLA)
TMT High-Contrast Exoplanet Science Michael Fitzgerald University of California, Los Angeles (UCLA) The Next Decade+ Demographics Kepler has provided rich census of radius/semimajoraxis space down to terrestrial
More informationExoplanet Science with E-ELT/METIS
Science with E-ELT/METIS Sascha P. Quanz (ETH Zurich) METIS Project Scientist EPSC 2015 - Nantes 1 Oct 2015 Image credit: BBC METIS is a 3-19 micron imager and spectrograph... METIS instrument baseline
More informationThe Fast Spin of β Pic b
The Fast Spin of β Pic b! Jayne Birkby 1,2,* Ignas Snellen 2, Bernhard Brandl 2, Remco de Kok 2, Matteo Brogi 2, Henriette Schwarz 2 1 Harvard-Smithsonian Center for Astrophysics, USA; 2 Leiden Observatory,
More informationCASE/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.
More informationUsing Ground-Based Telescopes to Mature Key Technologies and Advance Science for Future NASA Exoplanet Direct Imaging Missions
The first directly-imaged planetary system, HR 8799, discovered with Keck and Gemini. Using Ground-Based Telescopes to Mature Key Technologies and Advance Science for Future NASA Exoplanet Direct Imaging
More informationDirect Imaging in Reflected Light: Characterization of Older, Temperate Exoplanets With 30-m Telescopes
Direct Imaging in Reflected Light: Characterization of Older, Temperate Exoplanets With 3-m Telescopes arxiv:1.93v1 [astro-ph.im 9 Aug 1 A RESPONSE TO THE CALL FOR WHITE PAPERS ISSUED BY THE COMMITTEE
More informationExoplanet High Contrast Imaging Technologies Ground
Exoplanet High Contrast Imaging Technologies Ground KISS Short Course: The Hows and Whys of Exoplanet Imaging Jared Males University of Arizona Telescope Diameter (Bigger is Better) Diameter: Collecting
More informationHigh-Contrast Exoplanet Gemini. Christian Marois NRC-NSI, DAO GPI DA&A
High-Contrast Exoplanet Imaging @ Gemini Christian Marois NRC-NSI, DAO GPI DA&A Gemini Altair 2001 ADI first ever testing Exoplanet Science with Altair/NIRI GDPS/IDPS/SONIC/Janson/DavidL (young stars)
More informationSubaru-Australian collaboration on Technologies for Habitable Planet Spectroscopy
Subaru-Australian collaboration on Technologies for Habitable Planet Spectroscopy Mike Ireland Plus many others: thanks to Barnaby Norris and Nemanja Jovanovic for slides. Thanks to Yosuke Minowa for keeping
More informationE-ELT s View of Exoplanetary Atmospheres
Exo-Abundances Workshop, May 12th 14th, Grenoble E-ELT s View of Exoplanetary Atmospheres Gaël Chauvin - IPAG/CNRS - Institute of Planetology & Astrophysics of Grenoble/France In Collaboration with ESO-PST,
More informationThe Subaru Coronagraphic Extreme-AO system (SCExAO)
The Subaru Coronagraphic Extreme-AO system (SCExAO) O. Guyon, N. Jovanovic, F. Martinache, G. Singh, J. Lozi, C. Clergeon, T. Kudo, D. Doughty, S. Goebel, P. Phatak, J. Morino and J. Males Subaru Telescope,
More informationStudying Exoplanet Atmospheres with TMT. Ian Crossfield Sagan Fellow, UA/LPL 2014/07/18
Studying Exoplanet Atmospheres with TMT Ian Crossfield Sagan Fellow, UA/LPL 2014/07/18 What are conditions like on other worlds? Temperature @ 3 mbar Temperature @ 210 mbar Temperature @ 400 mbar Phosphine
More informationFinding bio-signatures on extrasolar planets, how close are we?
Finding bio-signatures on extrasolar planets, how close are we? Enric Palle Instituto de Astrofisica de Canarias TMT Forum 2017, Mysore Exoplanet discoveries 3703 planets 2773 system 621 multiple Exoplanets:
More informationSurvey of Present and Future Ground-Based Imaging Systems
Survey of Present and Future Ground-Based Imaging Systems Olivier Guyon (guyon@naoj.org) University of Arizona Subaru Telescope With material from : Rich Dekany, Ben Oppenheimer (Palm 3000, P1640) Bruce
More informationExoplanet atmosphere Spectroscopy present observations and expectations for the ELT
Exoplanet atmosphere Spectroscopy present observations and expectations for the ELT Hành tinh ngoại không khí phổ quan sát và kỳ vọng đối với các kính viễn vọng cực kỳ lớn Ignas Snellen, Leiden University
More informationHigh Contrast Imaging: New Techniques and Scientific Perspectives for ELTs
High Contrast Imaging: New Techniques and Scientific Perspectives for ELTs Is there a path to life What game changing finding with ELTs? technologies can get us there? Olivier Guyon Subaru Telescope &
More informationExoplanets Direct imaging. Direct method of exoplanet detection. Direct imaging: observational challenges
Black body flux (in units 10-26 W m -2 Hz -1 ) of some Solar System bodies as seen from 10 pc. A putative hot Jupiter is also shown. The planets have two peaks in their spectra. The short-wavelength peak
More informationHigh Contrast Imaging: Direct Detection of Extrasolar Planets
High Contrast Imaging: Direct Detection of Extrasolar Planets James R. Graham University of Toronto Dunlap Institute and Astronomy & Astrophysics September 16, 2010 Exoplanet Science How and where to planets
More informationSynergies of Subaru and CGI. Tyler D. Groff
1 Synergies of Subaru and CGI Tyler D. Groff High Level What can Subaru observations do for CGI 2 Precursor Observations with extreme adaptive optics (ExAO) Any CGI targets of opportunity are generally
More informationSubaru 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,
More informationTHE SUBARU CORONAGRAPHIC EXTREME AO HIGH SENSITIVITY VISIBLE WAVEFRONT SENSORS
Florence, Italy. May 2013 ISBN: 978-88-908876-0-4 DOI: 10.12839/AO4ELT3.13398 THE SUBARU CORONAGRAPHIC EXTREME AO HIGH SENSITIVITY VISIBLE WAVEFRONT SENSORS Christophe Clergeon 1a, Olivier Guyon 1, Frantz
More informationDirect imaging characterisation of (exo-) planets with METIS
Direct imaging characterisation of (exo-) planets with METIS Jupiter HR8799 Saturn VLT/ISAAC VLT/NACO Cassini/VIMS Wolfgang Brandner (MPIA) with contributions by Ian Crossfield, Lisa Kaltenegger (MPIA),
More informationPrincipal Author: Name: Thayne M. Currie Institution: NASA-Ames Research Center Phone: (857)
Astro2020 Science White Paper The Critical, Strategic Importance of Adaptive Optics-Assisted Ground-Based Telescopes for the Success of Future NASA Exoplanet Direct Imaging Missions Thematic Areas: Planetary
More informationA Fast Path to Imaging and Characterizing Habitable Exoplanets around the Nearest Stars with TMT
A Fast Path to Imaging and Characterizing Habitable Exoplanets around the Nearest Stars with TMT Olivier Guyon National Institutes for Natural Sciences (NINS) Astrobiology Center Subaru Telescope, National
More informationNEAR: Low-mass planets in Cen
NEAR: Low-mass planets in Cen M. Kasper 1, R. Arsenault 1, U. Käufl 1, G. Jakob 1, E. Fuenteseca 1, M. Riquelme 1, R. Siebenmorgen 1, M. Sterzik 1, G. Zins 1, N. Ageorges 2, S. Gutruf 2, A. Reutlinger
More informationPost-coronagraphic PSF sharpening with the vortex coronagraph
Post-coronagraphic PSF sharpening with the vortex coronagraph G. Orban de Xivry a, O. Absil a, E. Huby a, b, and A. Jolivet a a Space sciences, Technologies, and Astrophysics Research (STAR) Institute,
More informationExoplanets Direct imaging. Direct method of exoplanet detection. Direct imaging: observational challenges
Black body flux (in units 10-26 W m -2 Hz -1 ) of some Solar System bodies as seen from 10 pc. A putative hot Jupiter is also shown. The planets have two peaks in their spectra. The short-wavelength peak
More informationSSC Report UCSC. Jean Brodie and Chuck Steidel SSC co-chairs. June 20, 21
SSC Report June 20, 21 UCSC Jean Brodie and Chuck Steidel SSC co-chairs April Action Items-1 Prepare comparison of NIRES, NIRSPEC low RES, and MOSFIRE sensitivities in at least 1 band BY SCIENCE MEETING
More informationProxima Cen b: theoretical spectral signatures for different atmospheric scenarios
Proxima Cen b: theoretical spectral signatures for different atmospheric scenarios A. Léger(1), D. Defrère(2), J.L. Grenfell(3), M. Godolt(3), A Garcia Munoz(3), H. Rauer(3), and F. Tian(4) (1) University
More informationW.M. Keck Observatory s Next Generation Adaptive Optics Facility
W.M. Keck Observatory s Next Generation Adaptive Optics Facility P. Wizinowich a, R. Dekany b, D. Gavel c, C. Max c, S. Adkins a, B. Bauman c, J. Bell a, A. Bouchez b, M. Britton b, J. Chin a, R. Flicker
More informationOverview of Instrumentation Programs for Infrared Spectroscopy at the U.Toronto
Overview of Instrumentation Programs for Infrared Spectroscopy at the U.Toronto Dae-Sik Moon (Univ. of Toronto) (S. Sivanandam, E. Meyer, M. Millar-Blanchaer, J. Jilcote, J. Miranda, ) Three Key Elements
More informationCharacterizing exoplanetary atmospheres with a mid-infrared nulling spectrograph
Characterizing exoplanetary atmospheres with a mid-infrared nulling spectrograph D. Defrère (1), A. Léger (2), O. Absil (1) (1) University of Liège, Belgium, (2) University of Paris-Saclay, France June
More information2 More Science Cases, Summary & Close
2 More Science Cases, Summary & Close Chris Packham University of Texas at San Antonio On behalf of the MICHI team Physics&Astronomy THE UNIVERSITY OF TEXAS AT SAN ANTONIO ! Giant Planets - Giant Problems!
More informationPlanets Around M-dwarfs Astrometric Detection and Orbit Characterization
Planets Around M-dwarfs Page of 7 Planets Around M-dwarfs Astrometric Detection and Orbit Characterization N. M. Law (nlaw@astro.caltech.edu), S. R. Kulkarni, R. G. Dekany, C. Baranec California Institute
More informationThe Future of Exoplanet Science from Space
The Future of Exoplanet Science from Space Informed by a Clearer, Better, Faster, Stronger talk An Exoplanet Wishlist for ~2050 Based on talks with Giada Arney, Joshua Schlieder, Avi Mandell, Alexandra
More informationPolarimetry and spectral imaging of mature Jupiter and super-earth with SEE-COAST
Polarimetry and spectral imaging of mature Jupiter and super-earth with SEE-COAST Jean Schneider, A. Boccaletti, P. Baudoz, R. Galicher, R. Gratton, D. Stam et al. & E. Pantin, Complementarity of techniques
More informationThe 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
More informationarxiv: v1 [astro-ph.im] 5 Nov 2018
Letter Optics Letters 1 Vortex fiber nulling for exoplanet observations. I. Experimental demonstration in monochromatic light DANIEL ECHEVERRI 1,*, GARRETH RUANE 1,, NEMANJA JOVANOVIC 1, DIMITRI MAWET
More informationSPIRou status. and the SPIRou team.
SPIRou status René Doyon, Université de Montréal Jean-François Donati, IRAP (Toulouse) Xavier Delfosse, IPAG (Grenoble) Etienne Artigau, Université de Montréal Francesso Pepe, Observatoire de Genève and
More informationCIRMOS. 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?
More informationTMT 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:
More informationS. Rukdee 1, L. Vanzi 1, C. Schwab 2, M. Jones 1, M. Flores 1, A. Zapata 1, K. Motohara 3, Y. Yoshii 3, M. Tala 4
S. Rukdee 1, L. Vanzi 1, C. Schwab 2, M. Jones 1, M. Flores 1, A. Zapata 1, K. Motohara 3, Y. Yoshii 3, M. Tala 4 1. Center of Astro Engineering UC AIUC, Av. Vicuña Mackenna 4860, Macul - Santiago, Chile
More informationScientific context in 2025+
Outline Scientific context and goals O 2 detection on an Exoplanet with the E-ELT? PCS concept and technological challenges Timeframe for E-ELT high-contrast imaging Scientific context in 2025+ GAIA: Know
More informationReport 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
More informationThe James Webb Space Telescope: Capabilities for Transiting Exoplanet Observations
The James Webb Space Telescope: Capabilities for Transiting Exoplanet Observations Mark Clampin Observatory Project Scientist mark.clampin@nasa.gov Goddard Space Flight Center : How It Works Integrated
More informationW. M. Keck Observatory s Next Generation Adaptive Optics Facility
W. M. Keck Observatory s Next Generation Adaptive Optics Facility P. Wizinowich a, S. Adkins a, R. Dekany b, D. Gavel c, C. Max c, R. Bartos d, J. Bell a, A. Bouchez b, J. Chin a, A. Conrad a, A. Delacroix
More informationHIGH-CONTRAST IMAGING OF YOUNG PLANETS WITH JWST
ExSoCal Conference September 18-19th 2017, Pasadena HIGH-CONTRAST IMAGING OF YOUNG PLANETS WITH JWST Marie Ygouf HR 8799 planetary system Jason Wang / Christian Marois Keck data Giants planets and brown
More informationScientific 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)
More informationExoplanetary Science with the E-ELT
SF2A, MONTPELLIER, 4-7 JUNE 2013 Exoplanetary Science with the E-ELT Gaël Chauvin - IPAG/CNRS - Institute of Planetology & Astrophysics of Grenoble/France In Collaboration with ESO-PST, and E-ELT CAM,
More informationCharacterizing Exoplanets and Brown Dwarfs With JWST
Characterizing Exoplanets and Brown Dwarfs With JWST C. Beichman NASA Exoplanet Science Institute, Jet Propulsion Laboratory, California Institute of Technology On Behalf of the NIRCam Exoplanet Team September
More informationThe Status of AO Worldwide. State of AO Today UC Santa Cruz. Interim Director, UC Observatories Director, Center for Adaptive Optics
The Status of AO Worldwide Claire E. Max State of AO Today UC Santa Cruz Interim Director, UC Observatories Director, Center for Adaptive Optics Topics AO on current 8-10m telescopes Plans for AO on ELTs
More informationADVANCING HIGH-CONTRAST ADAPTIVE OPTICS
ADVANCING HIGH-CONTRAST ADAPTIVE OPTICS S. Mark Ammons LLNL Bruce Macintosh Stanford University Lisa Poyneer LLNL Dave Palmer LLNL and the Gemini Planet Imager Team ABSTRACT A long-standing challenge has
More informationSearch for Transiting Planets around Nearby M Dwarfs. Norio Narita (NAOJ)
Search for Transiting Planets around Nearby M Dwarfs Norio Narita (NAOJ) Outline Introduction of Current Status of Exoplanet Studies Motivation for Transiting Planets around Nearby M Dwarfs Roadmap and
More informationImaging polarimetry of exo-planets with the VLT and the E-ELT Hans Martin SCHMID, ETH Zurich
Imaging polarimetry of exo-planets with the VLT and the E-ELT Hans Martin SCHMID, ETH Zurich Collaborators: ETH Zurich: E. Buenzli, F. Joos, C. Thalmann (now at MPIA) VLT SPHERE: J.L. Beuzit, D. Mouillet,
More informationSPICA Science for Transiting Planetary Systems
SPICA Science for Transiting Planetary Systems Norio Narita Takuya Yamashita National Astronomical Observatory of Japan 2009/06/02 SPICA Science Workshop @ UT 1 Outline For Terrestrial/Jovian Planets 1.
More informationMIRI, 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
More informationCharacterization of Exoplanets in the mid-ir with JWST & ELTs
Characterization of Exoplanets in the mid-ir with JWST & ELTs Jupiter HR8799 Saturn VLT/ISAAC VLT/NACO Cassini/VIMS Wolfgang Brandner (MPIA), Eric Pantin (CEA Saclay), Ralf Siebenmorgen (ESO), Carolina
More informationTuesday Nov 18, 2014 Rapporteurs: Aki Roberge (NASA GSFC) & Matthew Penny (Ohio State)
Tuesday Nov 18, 2014 Rapporteurs: Aki Roberge (NASA GSFC) & Matthew Penny (Ohio State) Speaker Neil Zimmerman Mike McElwain Ilya Poberezhskiy Doug Lisman Tiffany Glassman Avi Shporer Jennifer Yee Dave
More informationarxiv: v3 [astro-ph.ep] 2 Nov 2018
to appear in ApJ Preprint typeset using L A TEX style emulateapj v. 12/16/11 DETECTING WATER IN THE ATMOSPHERE OF HR 8799 c WITH L-BAND HIGH DISPERSION SPECTROSCOPY AIDED BY ADAPTIVE OPTICS Ji Wang 1,2,
More informationSuper Earths: Reflection and Emission Spectra
National Aeronautics and Space Administration Jet Propulsion Laboratory California Institute of Technology tion Pr ogram ExoP Planet Explora Super Earths: Reflection and Emission Spectra Wes Traub 10 November
More informationRoadmap for PCS, the Planetary Camera and Spectrograph for the E-ELT
Florence, Italy. Adaptive May 2013 Optics for Extremely Large Telescopes III ISBN: 978-88-908876-0-4 DOI: 10.12839/AO4ELT3.12804 Roadmap for PCS, the Planetary Camera and Spectrograph for the E-ELT Markus
More informationExoplanets in the mid-ir with E-ELT & METIS
Exoplanets in the mid-ir with E-ELT & METIS Wolfgang Brandner (MPIA), Eric Pantin (CEA Saclay), Ralf Siebenmorgen (ESO), Sebastian Daemgen (MPIA/ESO), Kerstin Geißler (MPIA/ESO), Markus Janson (MPIA/Univ.
More informationProspects for ground-based characterization of Proxima Centauri b
Prospects for ground-based characterization of Proxima Centauri b Ma#eo Brogi Hubble Fellow, CU-Boulder Ignas Snellen, Remco de Kok, Henrie5e Schwarz (Leiden, NL) Jayne Birkby (CfA, USA), Simon Albrecht
More informationThe Instrumentation Plan for the Giant Magellan Telescope (GMT)
The Instrumentation Plan for the Giant Magellan Telescope (GMT) George Jacoby (GMTO/Carnegie) GMT Instrumentation Scientist SPIE Amsterdam July 4, 2012 1 Outline Project Overview Project Status Instrument
More informationTMT-J Project Office, National Institute of Natural Sciences/ National Astronomical Observatory of Japan TELESCOPE (TMT) ( NAOJ)
SPECIAL REPORT TMT~Thirty Meter Telescope Tomonori Usuda (TMT-J Project Director) and Miki Ishii (Public Relations) TMT-J Project Office, National Institute of Natural Sciences/ National Astronomical Observatory
More informationCoronagraphic Imaging of Exoplanets with NIRCam
Coronagraphic Imaging of Exoplanets with NIRCam C. Beichman NASA Exoplanet Science Institute, Jet Propulsion Laboratory, California Institute of Technology For the NIRCam Team September 27, 2016 Copyright
More informationNEAR: Low-mass Planets in α Cen with VISIR
Telescopes and Instrumentation DOI:.8727/0722-669/5033 NEAR: Low-mass Planets in α Cen with VISIR Markus Kasper Robin Arsenault Hans-Ulrich Käufl Gerd Jakob Eloy Fuenteseca Miguel Riquelme Ralf Siebenmorgen
More informationTechniques for direct imaging of exoplanets
Techniques for direct imaging of exoplanets Aglaé Kellerer Institute for Astronomy, Hawaii 1. Where lies the challenge? 2. Contrasts required for ground observations? 3. Push the contrast limit Recycle!
More informationADVANCEMENT OF AO TECHNOLOGY FOR THE NEXT GENERATION OF EXTREMELY LARGE TELESCOPES
ADVANCEMENT OF AO TECHNOLOGY FOR THE NEXT GENERATION OF EXTREMELY LARGE TELESCOPES Donald Gavel 1 University of California Observatories, UC Santa Cruz, 1156 High Street, Santa Cruz, CA, USA 95064 Abstract.
More informationExoPlanets Imaging Camera Spectrograph for the European ELT Simulations
ExoPlanets Imaging Camera Spectrograph for the European ELT Simulations Christophe Vérinaud,Visa Korkiakoski Laboratoire d Astrophysique - Observatoire de Grenoble, France and EPICS consortium EPICS for
More informationSYSTEM FOR CORONAGRAPHY WITH HIGH ORDER ADAPTIVE OPTICS FROM R TO K BAND THE NIR CHANNEL
1 SHARK-NIR@LBT SYSTEM FOR CORONAGRAPHY WITH HIGH ORDER ADAPTIVE OPTICS FROM R TO K BAND THE NIR CHANNEL Jacopo Farinato The SHARK-NIR Team: J.Farinato 1, F.Pedichini 2, E.Pinna 3, C.Baffa 3, A.Baruffolo
More informationExoplanets at the E-ELT era
Towards Other Earths II: The Star Planet Connection, Porto, September 15-19 th, 2014 Exoplanets at the E-ELT era Gaël Chauvin - IPAG/CNRS - Institute of Planetology & Astrophysics of Grenoble/France ESO-Project
More informationGEMINI 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
More informationDIRECT PLANET DETECTION
DIRECT PLANET DETECTION James R. Graham (UCB) Bruce Macintosh (LLNL) & Mitchell Troy (JPL) 1 High Contrast Imaging? Broad new frontier enabled by large telescopes & AO Exoplanet detection Direct methods
More informationScience of extrasolar Planets A focused update
Science of extrasolar Planets A focused update Raffaele Gratton, INAF Osservatorio Astronomico di Padova Extrasolar planets: a rapidly growing field of astronomy Top Tenz: Top 10 most important discoveries
More informationEarthFinder A NASA-selected Probe Mission Concept Study for input to the 2020 Astrophysics Decadal Survey
EarthFinder A NASA-selected Probe Mission Concept Study for input to the 2020 Astrophysics Decadal Survey Peter Plavchan Assistant Professor George Mason University 1 @PlavchanPeter http://exo.gmu.edu
More informationExoplanets. Wes Traub KISS Workshop on Planetary Magnetic Fields August 2013, Caltech
Jet Propulsion Laboratory California Institute of Technology Exoplanets Wes Traub KISS Workshop on Planetary Magnetic Fields 12 16 August 2013, Caltech 2013 California Institute of Technology. Government
More informationTriplespec: Motivations and Design. John Wilson
Triplespec: Motivations and Design John Wilson Slit Viewer Prisms Slit Collimator Reimager OAP #2 Window Spec Camera Tele Focus Reimager OAP #2 Grating Outline Scientific Rationale Heritage of Triplespec
More informationEPICS: A planet hunter for the European ELT
EPICS: A planet hunter for the European ELT M. Kasper, C. Verinaud, J.L. Beuzit, N. Yaitskova, A. Boccaletti, S. Desidera, K. Dohlen, T. Fusco, N. Hubin, A. Glindemann, R. Gratton, N. Thatte 42-m E-ELT
More informationTue 16:40-16:55 M. Tamura AO188
HiCIAO Early Result from SEEDS and The Subaru s Next Step 2011.5.3 Tue 16:40-16:55 M. Tamura AO188 SEEDS Strategic Exploration of Exoplanets and Disks with Subaru First Subaru Strategic Program (SSP) a
More information100 µas Astrometry with Adap2ve Op2cs on Moderate- Sized Telescopes
100 µas Astrometry with Adap2ve Op2cs on Moderate- Sized Telescopes Drs. Richard Dekany and Nick Law Caltech Optical Observatories Workshop on Astronomy with Adaptive Optics on Moderate-Sized Telescopes
More informationKeck/Subaru Exchange Program Subaru Users Meeting January 20, 2011
Keck/Subaru Exchange Program Subaru Users Meeting January 20, 2011 Taft Armandroff, Director W. M. Keck Observatory With science results from: Drew Newman and Richard Ellis, Caltech A. Romanowsky, J. Strader,
More informationA red / near-ir Spectrograph for GTC NEREA (Near Earths and high-res Exoplanet Atmospheres)
A red / near-ir Spectrograph for GTC NEREA (Near Earths and high-res Exoplanet Atmospheres) Enric Palle, Guillem Anglada, Ignasi Ribas Instituto de Astrofísica de Canarias Queen Mary University of London
More informationPotential Synergies Between MSE and the ELTs A Purely TMT-centric perspective But generally applicable to ALL ELTs
Potential Synergies Between MSE and the ELTs A Purely TMT-centric perspective But generally applicable to ALL ELTs Warren Skidmore, TMT Instrument System Scientist 2 nd May, 2018 IPAC Science Talk 1 TMT
More informationThe Search For Life in the Universe. Lecture 27
The Search For Life in the Universe Lecture 27 Our basic search technique: 1: Find the planets 2: Isolate the planets light from the stars light 3: Get a spectrum of the planet Its atmosphere, maybe is
More informationSubaru 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
More informationOngoing 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
More informationE-ELT Programme; ESO Instrumentation Project Office Ground-based Instrumentation for VLT, VLTI and E-ELT
Ground-based Instrumentation for VLT, VLTI and E-ELT Raffaele Gratton (with strong help by Sandro D Odorico) VLT 2 nd generation instruments Launched in 2001, completed 2012 HAWK-I (2007): wide field (7.5
More informationarxiv: v1 [astro-ph.im] 28 Apr 2016
Mid-IR AGPMs for ELT applications Brunella Carlomagno a, Christian Delacroix a, Olivier Absil a, Pontus Forsberg b, Serge Habraken a, Aïssa Jolivet a, Mikael Karlsson b, Dimitri Mawet c, Pierre Piron a,
More informationADAPTIVE PHASE MASK CORONAGRAPH
Florence, Italy. May 2013 ISBN: 978-88-908876-0-4 DOI: 10.12839/AO4ELT3.13183 ADAPTIVE PHASE MASK CORONAGRAPH Pierre Haguenauer 1,a, Pierre Bourget 1, Dimitri Mawet 1, and Nicolas Schuhler 1 1 European
More informationSpectroscopy. AST443, Lecture 14 Stanimir Metchev
Spectroscopy AST443, Lecture 14 Stanimir Metchev Administrative Homework 2: problem 5.4 extension: until Mon, Nov 2 Homework 3: problems 8.32, 8.41, 10.31, 11.32 of Bradt due in class Mon, Nov 9 Reading:
More informationTMT Instrumentation and Performance:
TMT Instrumentation and Performance: A Handbook for the July 2007 TMT Science Workshop May 24, 2007 TMT.INS.PRE.07.012.REL01 1 Important Note Feasibility studies for all TMT instrument concepts were conducted
More informationThe WFIRST Coronagraphic Instrument (CGI)
The WFIRST Coronagraphic Instrument (CGI) N. Jeremy Kasdin Princeton University CGI Adjutant Scientist WFIRST Pasadena Conference February 29, 2016 The Coronagraph Instrument Optical Bench Triangular Support
More informationMAORY (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,
More information