TMT-India Science Interests and Project Update G.C. Anupama & R. Srianand (On behalf of the TMT-India)‏ TMT-SAC Meeting: 22-23 November 2010, Pasadena,

Slides:



Advertisements
Similar presentations
Proposal for the Establishment and Funding of the Cluster of Excellence Origin and Structure of the Universe The Cluster of Excellence for Fundamental.
Advertisements

Xavier Barcons Instituto de Física de Cantabria (CSIC-UC) On behalf of The Athena+ Co-ordination Group, the Athena+ Working Groups and Supporters A theme.
Chapter 21: The Milky Way. William Herschel’s map of the Milky Way based on star counts In the early 1800’s William Herschel, the man who discovered the.
JWST Science 4-chart version follows. End of the dark ages: first light and reionization What are the first galaxies? When did reionization occur? –Once.
February 9, 11:00 am. The unusually bright centers found in some galaxies are called 1.active galactic nuclei. 2.starbursts. 3.halos. 4.supermassive.
Introduction to Astrophysics Ronald L. Westra Department Mathematics Maastricht University.
Edo Berger Carnegie Observatories Edo Berger Carnegie Observatories Probing Stellar to Galactic Scales with Gamma-Ray Bursts.
Measuring the Gas in Galaxies in the Distant Past Philip Lah Too late. Here comes the SKA.
Stars science questions Origin of the Elements Mass Loss, Enrichment High Mass Stars Binary Stars.
Research Astronomy In Southern NM: Insights From the Sloan Digital Sky Survey (SDSS) Jon Holtzman NMSU Department of Astronomy.
Imaging Science FundamentalsChester F. Carlson Center for Imaging Science The LASP* at RIT’s Center for Imaging Science *Laboratory for Astronomy in Strange.
NASA Living with a Star Program Targeted Research & Technology Steering Committee NASA HQ & LWS TR&T Update September 16, 2008 Doug Rowland On Detail to.
KDUST Supernova Cosmology
Outline  Introduction  The Life Cycles of Stars  The Creation of Elements  A History of the Milky Way  Nucleosynthesis since the Beginning of Time.
Astronomy Science combining all sciences. What is the Science of Astronomy? Astronomy is the scientific study of celestial objects (such as stars, planets,
Review for Exam 3.
European Southern Observatory Blois, 20 July 2010 From the VLT to ALMA and to the E-ELT.
Margaret Meixner (STScI, JHU) March 7, 2013
Instruments and Science with TMT Shude Mao. Outline International context Telescope overview and science instruments Some key science areas Summary.
Overview of Astronomy AST 200. Astronomy Nature designs the Experiment Nature designs the Experiment Tools Tools 1) Imaging 2) Spectroscopy 3) Computational.
What is Radio Astronomy? MIT Haystack Observatory This material was developed under a grant from the National Science Foundation.
 Galaxies with extremely violent energy release in their nuclei  Active Galactic Nuclei (AGN)  Up to many thousand times more luminous than the entire.
Gamma-ray Bursts in the E-ELT era Rhaana Starling University of Leicester.
Charles Hakes Fort Lewis College1. Charles Hakes Fort Lewis College2.
OWL Instrument Concept Studies Within the OWL Conceptual Design to be completed by ESO in 3Q 2005, ESO collaborates with external institutes in the study.
1 BDRv3 - November 26, Markus Kissler-Patig E-ELT Programme 1 E-ELT Science Case Markus Kissler-Patig.
The Formation and Evolution of Galaxies What were the first sources of light in the Universe? How were luminous parts of galaxies assembled? How did the.
The Galactic Habitable Zone Guillermo Gonzalez Iowa State University Fermilab August 21, 2002 Acknowledgements: Don Brownlee Peter Ward.
CELT Science Case. CELT Science Justification Process Put together a Science Working Group –Bolte, Chuck Steidel, Andrea Ghez, Mike Brown, Judy Cohen,
Expected progress and break-throughs in ground-based extragalactic astronomy Ralf Bender ESO Council FORS Deep Field.
The Far-Infrared Universe: from the Universe’s oldest light to the birth of its youngest stars Jeremy P. Scott, on behalf of Locke D. Spencer Physics and.
© Sierra College Astronomy Department 1 Astronomy 10 Elementary Astronomy COURSE GOALS & OBJECTIVES.
Mssl astrophysics group start Terribly hot stars. Liz Puchnarewicz Mullard Space Science Laboratory, UCL  -ray sources, missions.
Structure Formation in the Universe Concentrate on: the origin of structure in the Universe How do we make progress?How do we make progress? What are the.
What is Astronomy? Mr. Hibbetts Classical and Modern Astronomy.
Galaxies with Active Nuclei Chapter 14:. Active Galaxies Galaxies with extremely violent energy release in their nuclei (pl. of nucleus).  “active galactic.
ALMA Science Examples Min S. Yun (UMass/ANASAC). ALMA Science Requirements  High Fidelity Imaging  Precise Imaging at 0.1” Resolution  Routine Sub-mJy.
Active Galaxies and Supermassive Black Holes Chapter 17.
Astrophysics from Space Lecture 6: Supermassive black holes Prof. Dr. M. Baes (UGent) Prof. Dr. C. Waelkens (KUL) Academic year
Astrophysics Missions in ESA’s Cosmic Vision Program
What is Astronomy? An overview..
Caty PilachowskiIUB Astronomy Giant Telescopes, Ancient Skies:
A nebula is an interstellar cloud of dust, hydrogen gas and plasma. It is the first stage of a star's cycle. dusthydrogenplasmastar.
Copyright © 2010 Pearson Education, Inc. Clicker Questions Chapter 14 The Milky Way Galaxy.
19 vii 2011Astro-H Stanford1 Scientific Opportunities Roger Blandford KIPAC Stanford.
Introduction Education Cross-over fields Salaries Different fields of Astronomy.
Cosmology with ESO telescopes Bruno Leibundgut. Outline Past and current cosmology projects with ESO telescopes Future instrumentation capabilities (interferometry?)
BBN abundance observations Karl Young and Taryn Heilman Astronomy 5022 December 4, 2014.
FIRST LIGHT A selection of future facilities relevant to the formation and evolution of galaxies Wavelength Sensitivity Spatial resolution.
Homework for today was WORKBOOK EXERCISE: “Expansion of the Universe” (pg in workbook)
Competitive Science with the WHT for Nearby Unresolved Galaxies Reynier Peletier Kapteyn Astronomical Institute Groningen.
ST9 TPWS OSS Science Needs Overview Robert M. Nelson Lead Scientist New Millennium Program Offcie California Institute of Technology, Jet Propulsion.
Active Galaxies Galaxies with extremely violent energy release in their nuclei (pl. of nucleus). → “Active Galactic Nuclei” (= AGN) Up to many thousand.
Sample expanded template for one theme: Physics of Galaxy Evolution Mark Dickinson.
1 ASTRON is part of the Netherlands Organisation for Scientific Research (NWO) Netherlands Institute for Radio Astronomy Astronomy at ASTRON George Heald.
Research at Indian Institute of Astrophysics
The Science Case Hubble Space Telescope CELT+AO HDF.
2000 l.y. M87 Purdue.
Presolar Grains & Meteorites
Collaborative Indian Projects in Physics and Astronomy
Upcoming Facilities of IIA
The XENIA mission Cosmic chemical evolution of baryons
The “Milky Way”.
What is Astronomy? An overview..
What is Astronomy? An overview..
Note that the following lectures include animations and PowerPoint effects such as fly ins and transitions that require you to be in PowerPoint's Slide.
Galaxies With Active Nuclei
Galaxies With Active Nuclei
What is Astronomy? An overview..
Presentation transcript:

TMT-India Science Interests and Project Update G.C. Anupama & R. Srianand (On behalf of the TMT-India)‏ TMT-SAC Meeting: November 2010, Pasadena, CA, U.S.A

TMT-India Funding Agency – Department of Science and Technology, Govt. of India Principal Investigating Institutes –  Indian Institute of Astrophysics (IIA), Bangalore  Inter-University Center for Astronomy and Astrophysics (IUCAA), Pune  Aryabhatta Research Institute for Observational Sciences (ARIES), Nainital Members from Tata Institute of Fundamental Research (TIFR), Mumbai, Physical Research Laboratory (PRL), Ahmedabad and Universities

Steps towards TMT-India Nearly three years of deliberations – several national workshops and discussion meetings Astronomical community reached a consensus that the Thirty Meter Telescope (TMT) project was the best suited for Indian participation, among the three proposed international mega optical and infrared telescope projects. Submitted a detailed project report, in February, 2010, to the Department of Science and Technology (DST), Govt. of India. The DST approved the report, and, on 24th June 2010, made an announcement about India's participation in the TMT project as an observer, with a serious intent towards partnership.

Science Starformation Star forming regions (Galactic, nearby galaxies), YSOs and open clusters Stellar Physics Elemental abundances – evolved stars (AGB, RR Lyrae), hydrogen deficient, metal poor stars (CEMP), Lithium enriched Isotopic ratios Milky way structure Eruptive Variables and compact objects Novae, Supernovae, GRBs, LMXBs Galaxy formation and Evolution Stellar population in local group and nearby galaxies, kinematics of high redshift galaxies, central engines Early Universe Solar system objects and Exoplanets

Science Interests with TMT Formation and evolution of stars and planets  Star forming regions, YSOs, planetary atmospheres Formation and evolution of galaxies The Milky Way Galaxy – structures and their origin and dynamics – age, kinematics and chemical composition of stars Stellar population in the Local Group and nearby galaxies – kinematics and dark matter content Study of baryonic mass assembly in distant galaxies Kinematics of star-forming galaxies at z=2-3 Supermassive blackholes and AGNs Occurrence of AGN phenomenon and blackhole formation in the early universe

Science Interests with TMT The chemical evolution and composition of the Universe Nucleosynthesis in stars – chemical abundances The earliest stars: First stars, First Mass Function (FMF) Isotopic ratios - testing cosmic homogeneity Galaxy-Intergalactic medium interactions and metal enrichment Molecules at high-z Stellar explosions and extreme objects  Supernovae and their progenitors  GRB afterglows; GRB host galaxy  Compact star in LMXBs and isolated neutron stars Early Universe Cosmology with Ly-alpha forest Probing the fundamental physics – QSO absorption lines CMB temperature – using fine-structure excitation lines of carbon in DLAs

Instrument Requirements Generic instruments that are required to meet our science interests  Wide field optical imager  AO NIR imager  Low resolution NIR spectrometer (AO)‏  Multi-object low resolution spectrometer - optical and NIR (seeing limited, AO)‏  High resolution spectrometer – optical and NIR  Mid-infrared imager (AO)‏  Mid-infrared low resolution spectrometer ~30% of science proposals require high resolution spectrometer ~60-70% require imaging + low resolution spectroscopy ~20% require wide-field imaging and/or multi-object/IFU spectroscopy ~5-10% require mid-IR ~2% require polarisation

Instrument Requirements

TMT-India Update TMT-India has submitted a proposal to the Department of Science and Technology, Govt. of India for funds for development of technology/prototypes under the following work packages  M1 Segment Support Assemblies  Edge Sensor  Actuators  M1 segment polishing  Software  Interested in participation in instruments – either through hardware/software development, or through man power (currently under discussion)‏ Seeking ~5M USD funds during the observer period The performing institution/entity for all work packages approved by the TMT Project will be “TMT-India”