NIR Spectroscopy at Gemini South

Slides:



Advertisements
Similar presentations
Sarah Kendrew Leiden Instrumentation Group.  One of eight potential instruments for the European ELT, the largest planned optical/IR telescope for the.
Advertisements

General Astrophysics with TPF-C David Spergel Princeton.
HIRES Technical concept and design E. Oliva, HIRES meeting, Brera (Milan, Italy)1.
A detailed 2D spectroscopic study of the Central Region of NGC 5253 Ana Monreal Ibero (1) José Vílchez (1), Jeremy Walsh (2), Casiana Muñoz-Tuñón (3) (1)
GLAO instrument specifications and sensitivities
Studying Parsec Scale Jets in Star Forming Region Tae-Soo Pyo Subaru Telescope.
E-ELT VLT HARMONI – the first light integral field spectrograph for the E-ELT Niranjan Thatte On behalf of the HARMONI consortium Florence - 29 June 2013.
Integral Field Spectroscopy on Gemini Andrew Bunker (IoA, Cambridge) Euro3D Meeting July 2002 GMOS Gemini Multi-Object Spectrograph, optical IFU (Durham)
1 Palermo nd May Looking ahead to MOONS William Taylor on behalf of the MOONS consortium.
JWST IFUs and Data Tool Development Plans Tracy Beck JWST NIRSpec Instrument Scientist.
HST WFC3 IR channel: 1k x 1k HgCdTe detector, QE 80% 18 micron pixels (0.13”/pix), ~2’x2’ FOV Detector sensitivity engineered to cut off above 1.7 micron,
Keck NGAO Science Requirements Claire Max UC Santa Cruz Caltech NGAO Meeting November 14, 2006.
Science Team Management Claire Max Sept 14, 2006 NGAO Team Meeting.
Multi-long-slit Spectroscopy for Kinematic Studies II. Initial Results for Edge-on Galaxies NGC891 and NGC4244 Jiehae Choi, Sophia Cisneros, Cat Wu, Maria.
LIM: Near IR from a mini-satellite Dani Maoz. HST WFC3 IR channel: 1k x 1k HgCdTe detector, QE 80% 18 micron pixels (0.13”/pix), ~2’x2’ FOV Detector.
X-shooter A Wideband Spectrograph for GRBs
MMT Magellan Infrared Spectrograph ( MMIRS ) P.I. Brian McLeod Warren R. Brown SAO/CfA.
Black Holes in Nearby Galaxies Claire Max NGAO Team Meeting March 7, 2007.
PALM3K Review PALM3K Review Caltech Nov 12 th, 2007.
Astronomical Spectroscopy
FMOS and UKIDSS Galactic Astronomy Phil Lucas UHerts.
W. M. Keck Observatory Subaru Users’ Meeting
Masahiro Konishi (IoA, UTokyo), SWIMS Team S W I M S.
The Mid-Infrared Instrument (MIRI) Medium Resolution Spectrometer for JWST Martyn Wells MIRI EC & UKATC.
3D meeting Tenerife July 2002 Ian Parry, Andrew Dean, Dave King, Andy Bunker, Steve Medlen, Jim Pritchard, Rachel Johnson, Anamparabu Ramaprakash, Rob.
GMTNIRS (Giant Magellan Telescope Near-IR Spectrograph) Survey Science Group Workshop 3 조 김상혁 김재영 최나현
INTEGRAL FIELD SPECTROSCOPY AT THE VLT STAR (CLUSTER) FORMATION IN 3D : INTEGRAL FIELD SPECTROSCOPY AT THE VLT Markus Kissler-Patig (Instrument Scientist.
Integral Field Spectroscopy. David Lee, Anglo-Australian Observatory.
HIGH REDSHIFT GALAXIES and COSMOLOGY SUMMARY. RESOLUTION > (IGM metals, molecules, constants) ( would be fine too – turbulence?
ASTRO-F Survey as an Input Catalogue for FIRST Takao Nakagawa (ISAS, Japan) & ASTRO-F Team.
X-shooter Phase 2 Users Workshop | Vincenzo Mainieri (USD)
MIRI Optical System CDR, 6 th & 7 th December 2006 Mid InfraRed Instrument 07-1 Optical System Critical Design Review (CDR) TIPS Presentation: Margaret.
Central Engine of AGN Xi’ian October 2006 Black Hole Mass Measurements with Adaptive Optic Assisted 3D-Spectroscopy Courtesy ESO Guia Pastorini Osservatorio.
KMOS Instrument Overview & Data Processing Richard Davies Max Planck Institute for Extraterrestrial Physics  What does KMOS do?  When will it do it?
イメージスライサー型可視光 面分光ユニットの開発 Development of an integral field unit (IFU) with an image slicer Shinobu Ozaki, Satoshi Miyazaki, Takuya Yamashita, Takashi Hattori,
Submillimeter Array CH3OH A Cluster of Highly Collimated and Young Bipolar Outflows Emanating from OMC1 South. Luis A. Zapata 1,2, Luis.
November 14, 2007CTIO-Gemini Colloquium, La Serena1 Slicing Up Galactic HII Regions with NIFS and... The Incredible Shrinking Milky Way R. Blum NOAO Gemini.
A Detector Upgrade for LDSS3 Mike Gladders Jacob Bean (on the phone) with Andreas Seifart, Josh Frieman, John Carlstrom.
3D SPECTROSCOPY OF HERBIG HARO OBJECTS R. López 1, S.F. Sánchez 2, B. García-Lorenzo 3, R. Estalella 1, G. Gómez 3, A. Riera 4,1, K. Exter 3 (1) Departament.
Science with Giant Telescopes - Jun 15-18, Instrument Concepts InstrumentFunction range (microns) ResolutionFOV GMACSOptical Multi-Object Spectrometer.
Astronomical Observational Techniques and Instrumentation
David R. Law Hubble Fellow, UCLA The Physical Structure of Galaxies at z ~ John McDonald, CFHT Galaxies in the Distant Universe: Ringberg Castle.
Introduction NICMOS (Near-Infrared Camera and Multi-Object Spectroscopy) was installed on the Hubble Space Telescope during SM2 in 1997 and has been the.
Robo-AO Overview: System, capabilities, performance Christoph Baranec (PI)
GMT’s Near IR Multiple Object Spectrograph - NIRMOS Daniel Fabricant Center for Astrophysics.
Competitive Science with the WHT for Nearby Unresolved Galaxies Reynier Peletier Kapteyn Astronomical Institute Groningen.
Performance and sensitivity of Low Resolution Spectrographs for LAMOST Zhu Yongtian, Hou Yonghui, Hu Zhongwen Wang Lei, Wang Jianing.
June 3, 2010MIRI NL meeting Prelude to MIRI Herschel: A WISH come true RCW120 Herschel A. Zavagno.
Black Holes in Globular Clusters Karl Gebhardt (UT)
The Prime Focus Imaging Spectrograph for the Southern African Large Telescope: Operational Modes Chip Kobulnicky – Instrument Scientist, University of.
Spectrometer The instrument used for the astronomers MinGyu Kim
Gemini Observatory Giant Telescope Science J. Y. Seok.
VLT Integral Field Spectroscopy of Embedded Protostars Near-IR emission lines as tracers of accretion and outflow Chris Davis Joint Astronomy Centre Hilo,
GTC Commissioning (as of September 2008) Peter Hammersley (GTC)
January 30, 2008Subaru Users Meeting 2007 NAOJ, Mitaka, Tokyo 1 Slicing Up Galactic HII Regions with NIFS R. Blum NOAO Gemini Science Center, Tucson.
Single Object Spectroscopy and Time Series Observations with NIRSpec
Robo-AO: Demo Period Nicholas Law.
A.Zanichelli, B.Garilli, M.Scodeggio, D.Rizzo
Key Inputs / Requirements
Single Object & Time Series Spectroscopy with JWST NIRCam
Galaxy Evolution from z=2 to the present
Observing and Data Reduction
NIRSpec simulation data-package
ESAC 2017 JWST Workshop JWST User Documentation Hands on experience
A galaxy at redshift 10? Brigitta Eder Vera Könyves
Overview Instrument Role Science Niches Consortium science
Integral Field Spectroscopy
Astronomical Observational Techniques and Instrumentation
Observational Prospect of NIREBL
Fig. 1 Localization of GW and associated transient EM
Presentation transcript:

NIR Spectroscopy at Gemini South Cool Universe Valparaiso, Chile

Delivered November 2003 Cool Universe Valparaiso, Chile

Most modes now available to community First Light January 2004 Most modes now available to community Versatile, sensitive 1-5um instrument Long slit: R=1800,6000,18000; 100” slit; 0.15” and 0.05” pixels Cross-dispersed: Simultaneous JHK coverage at R=1800; select regions at R=6000 IFU: 3x5” FOV; R=1800 and R=6000 Cool Universe Valparaiso, Chile

Early Science Brown Dwarf Search (JHK R=2000) Z=2 Galaxy (JHK R=2000) K. Luhman Z=2 Galaxy (JHK R=2000) P. van Dokkum and M. Kriek HH120 (Long-slit J, R=6000) J. Elias Galactic Center in the IFU (R=6000) Cool Universe Valparaiso, Chile

Cross-dispersed (XD) Mode 1.9-2.5um Very popular mode in 2004B R=2000 (shown) Also R=6000 with reduced coverage Blue end extends into optical red, with reduced transmission 1.1-1.5um 0.9-1.28um 0.8-1.09um 1.4-1.9um Cool Universe Valparaiso, Chile

XD: R=2000 JHK Confirmed Brown dwarf, OTS 44, M=9.5 Observed Resolution 1800-2200 JHK Displayed R=300 OTS 7: H=15.9, 33mins on source (poor seeing) OTS 44: H=15.4, 13min on source Figure from Luhman 2004 (in press) Cool Universe Valparaiso, Chile

XD: R=2000 JHK z=2.22 non-active galaxy K=18.9; 63 minutes on source Figure by van Dokkum and Kriek (2004, in prep) Cool Universe Valparaiso, Chile

Long Slit: R=6000 Herbig-Haro outflow source (HH120) Acquisition image Cool Universe Valparaiso, Chile

Long Slit: R=6000 Herbig-Haro outflow source (HH120) Acquisition image Cool Universe Valparaiso, Chile

Long Slit: R=6000 Spatial, kinematic differences between [FeII] and H2 J band; 27 minutes on source Figure by Jay Elias Cool Universe Valparaiso, Chile

Integral Field Unit (IFU) Commissioning data of galactic center (IRS7) 60 second raw exposure (no sky subtraction) Strong velocity gradient in Br gamma Figure by J. Allington-Smith Cool Universe Valparaiso, Chile

High Resolution Near-IR Spectroscopy GNIRS R=18000 with the long camera and 0.1” slit Phoenix Long-term “visitor” instrument R~50,0000 with 0.005*lambda coverage Cool Universe Valparaiso, Chile

High Resolution Near-IR Spectroscopy Cool Universe Valparaiso, Chile