The Greenland Telescope
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Curriculum Vitae
CURRICULUM VITAE Ming-Tang Chen, Ph.D., Physics Research Fellow Deputy Director of ASIAA Hawaii Operations Academia Sinica, Institute of Astronomy and Astrophysics (Taiwan) PO Box 23-141, Taipei, Taiwan, ROC (USA) 645 N. A’ohoku Place, Hilo, HI 96720, USA Telephone (TW): +886-2-2366-5348 Telephone (US): +1-808-938-4708 Email: [email protected] CURRICULUM VITAE ................................................................................................... 1 Brief Biography: .............................................................................................................. 2 Person Data: ..................................................................................................................... 2 Education: ........................................................................................................................ 2 Knowledge & Skills: ....................................................................................................... 2 Professional TitleS: .......................................................................................................... 2 Committee Service: ......................................................................................................... 3 Grant Executed: ............................................................................................................... 4 International Invited Talks: ............................................................................................. 5 Current and Past Research Topics: ................................................................................. -
Seeing Black Holes: from the Computer to the Telescope
universe Review Seeing Black Holes: From the Computer to the Telescope Jean-Pierre Luminet 1,2,3 1 Aix Marseille University, CNRS, LAM, 13013 Marseille, France; [email protected] or [email protected] 2 Aix Marseille University, CNRS, CPT, 13009 Marseille, France 3 Observatoire de Paris, CNRS, LUTH, 92195 Meudon, France Received: 7 July 2018; Accepted: 6 August 2018; Published: 9 August 2018 Abstract: Astronomical observations are about to deliver the very first telescopic image of the massive black hole lurking at the Galactic Center. The mass of data collected in one night by the Event Horizon Telescope network, exceeding everything that has ever been done in any scientific field, should provide a recomposed image in 2018. All this, forty years after the first numerical simulations performed by the present author. Keywords: black hole; numerical simulation; observation; general relativity 1. Introduction According to the laws of general relativity (for recent overviews at the turn of its centennial, see, e.g., [1,2]), black holes are, by definition, invisible. Contrary to uncollapsed stars, their surface is neither a solid nor a gas; it is an intangible frontier known as the event horizon. Beyond this horizon, gravity is so strong that nothing escapes, not even light. Seen projected onto the background of the sky, the event horizon would probably resemble a perfectly black disk if the black hole is static (Schwarzschild black hole) or a slightly flattened disk if it is rotating (Kerr black hole). A black hole however, be it small and of stellar mass or giant and supermassive, is rarely “bare”; in typical astrophysical conditions it is usually surrounded by gaseous matter. -
Sub-Mm VLBI from the Arctic — Imaging Black Holes
Astrophysics from Antarctica Proceedings IAU Symposium No. 288, 2012 c International Astronomical Union 2013 M. G. Burton, X. Cui & N. F. H. Tothill, eds. doi:10.1017/S1743921312016870 Sub-mm VLBI from the Arctic — Imaging Black Holes Makoto Inoue1 and the Greenland Telescope team1,2,3,4 1 Academia Sinica Institute of Astronomy and Astrophysics, P.O. Box 23-141, Taipei, 10617 Taiwan, R.O.C. email: [email protected] 2 Smithsonian Astrophysical Observatory, 60 Garden Street, Cambridge, MA 02138, USA 3 MIT Haystack Observatory, Off Route 40, Westford, MA 01886-1299, USA 4 National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903-4608, USA Abstract. We are deploying a new station for sub-millimeter Very Long Baseline Interferom- etry (VLBI) to obtain shadow images of Supermassive Black Hole (SMBH). Sub-mm VLBI is thought to be the only way so far to get the direct image of SMBH by its shadow, thanks to the superb angular resolution and high transparency against dense plasma around SMBH. At the Summit Station on Greenland, we have started monitoring the opacity at sub-mm region. The Summit Station subtends long baselines with the Atacama Large Milimeter/submillimeter Array (ALMA) in Chile and Submillimeter Array (SMA) in Hawaii. In parallel, we started retrofitting the ALMA North America prototype telescope (renamed as Greenland Telescope: GLT) for the cold environment. Keywords. Supermassive Black Hole (SMBH), Sub-millimeter telescope, Very Long Baseline Interferometry (VLBI) 1. Introduction An experiment in the sub-millimeter (submm) Very Long Baseline Interferometry (VLBI) has shown the capability for direct imaging of Sumermassive Black Hole (SMBH) (Doelaman et al. -
First Results from the Event Horizon Telescope
First results from the Event Horizon Telescope Dom Pesce On behalf of the Event Horizon Telescope collaboration March 10, 2020 EDSU conference The goal (ca. 2017) The goal is to take a picture of a black hole The goal (ca. 2017) Subrahmanyan Chandrasekhar The goal is to take a picture of a black hole • General relativity makes a prediction for the apparent shape of a black hole “It is conceptually interesting, if not astrophysically very important, to calculate the precise apparent shape of the black hole… Unfortunately, there seems to be no hope of observing this effect.” - James Bardeen, 1973 James Bardeen Photon ring and black hole shadow The warped spacetime around a black hole causes photon trajectories to bend event horizon b photon orbit Photon ring and black hole shadow The warped spacetime around a black hole causes photon trajectories to bend The closer these trajectories get to a critical impact parameter, the more tightly wound they become Photon ring and black hole shadow The warped spacetime around a black hole causes photon trajectories to bend The closer these trajectories get to a critical impact parameter, the more tightly wound they become Photon ring and black hole shadow The warped spacetime around a black hole causes photon trajectories to bend The closer these trajectories get to a critical impact parameter, the more tightly wound they become The trajectories interior to this critical impact parameter intersect the horizon, and these collectively form the black hole “shadow” (Falcke, Melia, & Agol 2000) while the bright surrounding region constitutes the “photon ring” Adapted from: Asada et al. -
Greenland Telescope Project --- Direct Confirmation of Black Hole with Sub-Millimeter VLBI
Greenland Telescope Project --- Direct Confirmation of Black Hole with Sub-millimeter VLBI --- Inoue, M.§; Algaba-Marcos, J.C.; Asada, K.; Chang, C.-C.; Chen, M.-T.; Han, J.; Hirashita, H.; Ho, P.T.P.; Hsieh, S.-N.; Huang, T.; Jiang, H.; Koch, P.M.; Kubo, D.Y.; Kuo, C.-Y.; Liu, B.; Martin-Cocher, P.; Matsushita, S.; Meyer-Zhao, Z.; Nakamura, M.; Nishioka, H.; Nystrom, G.; Pradel, N.; Pu, H.-Y.; Raffin, P.A.; Shen, H.-Y.; Snow, W.; Srinivasan, R.; and Wei, T.-S. Academia Sinica Institute of Astronomy and Astrophysics 11F of Astronomy-Mathematics Building, AS/NTU, No.1, Sec. 4, Roosevelt Rd, Taipei 10617, Taiwan, R.O.C. Blundell, R.; Burgos, R.; Grimes, P.; Keto, E.; Paine, S.; Patel, N.; and Sridharan, T.K. Harvard-Smithsonian Center for Astrophysics 60 Garden Street, Cambridge, MA 02138, USA Doeleman, S.S.; and Fish, V. MIT Haystack Observatory Off Route 40, Westford, MA 01886-1299, USA and Brisken, W.; and Napier, P. National Radio Astronomy Observatory Array Operation Center, P.O. Box O, 1003 Lopezville Road, Socorro, NM 87801-0387, USA § Email address: [email protected] 1 Abstract A 12-m diameter radio telescope will be deployed to the Summit Station in Greenland to provide direct confirmation of a Super Massive Black Hole (SMBH) by observing its shadow image in the active galaxy M87. The telescope (Greenland Telescope: GLT) is to become one of the Very Long Baseline Interferometry (VLBI) stations at sub-millimeter (submm) regime, providing the longest baseline > 9,000 km to achieve an exceptional angular resolution of 20 µas at 350 GHz, which will enable us to resolve the shadow size of ~40 µas. -
Ejected Superluminal Features Associated with the VHE Flare in AGN Jets: Sites Constrained by Smbhs
Ejected Superluminal Features Associated with the VHE Flare in AGN Jets: Sites Constrained by SMBHs Image credit: W. B. Sparks (STScI) Masanori Nakamura (ASIAA) Collaborators: K. Asada (ASIAA), J. A. Biretta (STScI), D. A. Garofalo (CSUN), C. A. Norman (JHU), D. L. Meier (JPL), W. B. Sparks (STScI) TIARA WS on Transient Universe, Dec. 2011, NTHU Outline ✤ Evidence for magnetic acceleration & collimation M87 of the active galactic nuclei (AGN) jet in M87 ✤ Quad MHD shock model for sub/super-luminal ejections ✤ Stationary feature in AGN jets constrained by the SMBH ✤ ASIAA “Greenland Telescope Project”: sub-mm VLBI for exploring the SMBH shadow & origin of AGN jets Outline ✤ Evidence for magnetic acceleration & collimation of the active galactic nuclei (AGN) jet in M87 ✤ Quad MHD shock model for sub/super-luminal ejections ✤ Stationary feature in AGN jets constrained by the SMBH ✤ ASIAA “Greenland Telescope Project”: sub-mm VLBI for exploring the SMBH shadow & origin of AGN jets Observational Overview Observations • Good Resolution • Nearby: D 16 Mpc (1 mas = 0.08 pc) ∼ • FR I: Misaligned BL Lac (θ 14 ◦ ; Wang & Zhou 2009) view ∼ • SMBH mass: (6 . 6 0 . 4) 10 9 M (Gebhardt et al. 2011) ± × ⊙ • VLBA resolution: 20 RS at 43 GHz • Sub-mm VLBI resolution: 3 RS at 345 GHz (w/ GL) VLBA Movie at 43GHz (C. Walker, NRAO) • Well studied at wavelengths from radio to X-ray • Proper motions (sub/super-luminal feature) • Polarization (20-60%; ordered B-fields) • Substructure (limb-brightened, knots, wiggles, ...), indicating a role of B-fields • In situ particle acceleration (Fermi-I diffusive shock process ) HST Movie (J. -
Event Horizon Telescope: the Black Hole Seen Round the World
EVENT HORIZON TELESCOPE: THE BLACK HOLE SEEN ROUND THE WORLD HEARING BEFORE THE COMMITTEE ON SCIENCE, SPACE, AND TECHNOLOGY HOUSE OF REPRESENTATIVES ONE HUNDRED SIXTEENTH CONGRESS FIRST SESSION MAY 16, 2019 Serial No. 116–19 Printed for the use of the Committee on Science, Space, and Technology ( Available via the World Wide Web: http://science.house.gov U.S. GOVERNMENT PUBLISHING OFFICE 36–301PDF WASHINGTON : 2019 COMMITTEE ON SCIENCE, SPACE, AND TECHNOLOGY HON. EDDIE BERNICE JOHNSON, Texas, Chairwoman ZOE LOFGREN, California FRANK D. LUCAS, Oklahoma, DANIEL LIPINSKI, Illinois Ranking Member SUZANNE BONAMICI, Oregon MO BROOKS, Alabama AMI BERA, California, BILL POSEY, Florida Vice Chair RANDY WEBER, Texas CONOR LAMB, Pennsylvania BRIAN BABIN, Texas LIZZIE FLETCHER, Texas ANDY BIGGS, Arizona HALEY STEVENS, Michigan ROGER MARSHALL, Kansas KENDRA HORN, Oklahoma RALPH NORMAN, South Carolina MIKIE SHERRILL, New Jersey MICHAEL CLOUD, Texas BRAD SHERMAN, California TROY BALDERSON, Ohio STEVE COHEN, Tennessee PETE OLSON, Texas JERRY MCNERNEY, California ANTHONY GONZALEZ, Ohio ED PERLMUTTER, Colorado MICHAEL WALTZ, Florida PAUL TONKO, New York JIM BAIRD, Indiana BILL FOSTER, Illinois JAIME HERRERA BEUTLER, Washington DON BEYER, Virginia JENNIFFER GONZA´ LEZ-COLO´ N, Puerto CHARLIE CRIST, Florida Rico SEAN CASTEN, Illinois VACANCY KATIE HILL, California BEN MCADAMS, Utah JENNIFER WEXTON, Virginia (II) CONTENTS May 16, 2019 Page Hearing Charter ..................................................................................................... -
Greenland Telescope (GLT) Frontend/Backend Commissioning
Greenland Telescope (GLT): Imaging the Black Hole Shadow Satoki Matsushita (ASIAA; Academia Sinica Institute of Astronomy and Astrophysics, Taiwan) & the GLT Project Team (ASIAA & SAO) Primary Science Target: Direct Imaging of the Shadow of Black Holes Sizes of Black Holes Shadow Size Mass Distance (masec) (106 Mo) (Mpc) Sgr A* 50 4.1 +- 0.6 0.008 M87 39 6600 +- 400 17.0 M31 18 180 +- 80 0.80 M60 12 2100 +- 600 16.5 NGC 5128 (Cen A) 7 310 +- 30 4.5 Gebhardt et al. (2011) Note: Here we assume Rshadow ~ 5 x Rsch Spatial Resolution • Spatial resolution goes high with shorter wavelength (or higher frequency) and bigger telescope (or longer baseline): • Resolution ~ l/D l: Wavelength D: Diameter of telescope (or baseline length) • Spatial resolutions of the optical/infrared telescopes: • Hubble Space Telescope (HST): 0.04” (40 milliarcsec) • James Webb Space Telescope (JWST): 0.03” (30 milliarcsec) • VLT Interferometer (VLTI): 0.002” (2 milliarcsec) a Too large to image black holes, whose sizes are marcsec scale. ⇒ Submillimeter Interferometry !!! Feasibility of Submillimeter VLBI Doeleman et al. (2008) Doeleman et al. (2012) Sgr A* Vir A* (M 87) Size ≈ 40 µas (≈ 4 rsch) Size ≈ 40 µas (≈ 5 rsch) Why Greenland? Submillimeter Telescopes in the World • Atacama Large Millimeter Array (ALMA), Chile • ALMA Pathfinder Experiment (APEX), Chile • James Clerk Maxwell Telescope (JCMT), Hawaii • Large Millimeter Telescope (LMT), Mexico • IRAM 30-meter Telescope, Spain • South Pole Telescope (SPT), South Pole • Submillimeter Array (SMA), Hawaii • Submillimeter Telescope (SMT), Arizona M. Johnson/SAO Telescope Site Selection • Site selection criteria: • Precipitable water vapor (PWV) is low. -
Electronics Instrumentation for the Greenland Telescope
Electronics Instrumentation for the Greenland Telescope Derek Kubo1a, Chih-Chiang Hana, Hiroaki Nishiokaa, Ryan Chilsona, Ranjani Srinivasana, Sheng- Feng Yena, Kuo-Chieh Fua, Homin Jianga, Kuan-Yu Liua, Ta-Shun Weia, Chih-Wei Huanga, Chen- Yu Yua, Peter Oshiroa, Shu-Hao Changa, Chung-Cheng Chena, Philippe Raffina, Yau-De Huanga, Pierre Martin-Cochera, Ming-Tang Chena, Makoto Inouea, Satoki Matsushitaa, Keiichi Asadaa, Shoko Koyamaa, Patrick Kocha, Paul T. P. Hoa, Yang-Tai Shawa, Timothy J. Nortonb, Nimesh A. Patelb, Shepherd S. Doelemanb, Daniel Bintleyc, Craig Waltherc, Per Fribergc, Jessica Dempseyc, Hideo Ogawad, Kimihiro Kimurad, Yutaka Hasegawad, Ching-Tang Liue, Kou-Chang Hane, Song- Chu Change, Li-Ming Lue aAcademia Sinica, Institute of Astronomy & Astrophysics, No 1, Sec 4, Roosevelt Rd, Taipei 10617, Taiwan, ROC; bHarvard-Smithsonian Center for Astrophysics, 60 Garden St, Cambridge, MA 02138, USA; cEast Asian Observatory, 660 N Aohoku Pl, Hilo, HI 96720, USA; dOsaka Prefecture University, 1-1 Gakuen-cho, Naka-ku, Sakai, Osaka, 599-8531, Japan; eNational Chung-Shan Institute of Science and Technology, No 300-5, Ln 277, Xian St, Xitun Dist, Taichung City, 40722, Taiwan, ROC. ABSTRACT The Greenland Telescope project has recently participated in an experiment to image the supermassive black hole shadow at the center of M87 using Very Long Baseline Interferometry technique in April of 2018. The antenna consists of the 12-m ALMA North American prototype antenna that was modified to support two auxiliary side containers and to withstand an extremely cold environment. The telescope is currently at Thule Air Base in Greenland with the long-term goal to move the telescope over the Greenland ice sheet to Summit Station. -
Greenland Telescope (GLT) Project
EPJ W e b o f Con ferenc es 61 , 01008 (2013) / / DOI: 10.1051 epjconf 20136101008 C Owned by the authors, published by EDP Sciences, 2013 Greenland Telescope (GLT) Project ”A Direct Confirmation of Black Hole with Submillimeter VLBI” M. Nakamura1, J. C. Algaba1, K. Asada1, B. Chen1, M.-T. Chen1, J. Han1, P. H. P. Ho1, S.-N. Hsieh1, T. Huang1, M. Inoue1, P. Koch1, C.-Y. Kuo1, P. Martin-Cocher1, S. Matsushita1, Z. Meyer-Zhao1, H. Nishioka1, G. Nystrom2, N. Pradel1, H.-Y. Pu1, P. Raffin1, H.-Y. Shen1, C.-Y. Tseng1, and the Greenland Telescope Project Team1,2,3,4 1Institute of Astronomy and Astrophysics, Academia Sinica, 11F of Astronomy-Mathematics Building, AS/NTU No 1, Sec 4, Roosevelt Rd., Taipei 10617, Taiwan 2Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA 3MIT Haystack Observatory, Off Route 40, Westford, MA 01886-1299, USA 4NRAO, 520 Edgemont Road, Charlottesville, VA 22903-2475, USA Abstract. The GLT project is deploying a new submillimeter (submm) VLBI station in Greenland. Our primary scientific goal is to image a shadow of the supermassive black hole (SMBH) of six billion solar masses in M87 at the center of the Virgo cluster of galaxies. The expected SMBH shadow size of 40-50 µas requires superbly high angular resolution, suggesting that the submm VLBI would be the only way to obtain the shadow image. The Summit station in Greenland enables us to establish baselines longer than 9,000 km with ALMA in Chile and SMA in Hawaii as well as providing a unique u–v coverage for imaging M87. -
Danish Press Conference on First Result from the Event Horizon Telescope
Danish Press Conference on First Result from the Event Horizon Telescope Left panel : A simulated image showing turbulent plasma glowing as it is swallowed up by a supermassive black hole (credit: University of Arizona). Right panel: The Greenland Telescope, currently located at the Thule Air Base in northern Greenland. April 1, 2019 The Event Horizon Telescope (EHT) project and DTU Space, National Space Institute will hold a press conference to present a groundbreaking result from the EHT. ● What: Press conference announcing a groundbreaking result from the EHT. The Greenland Telescope is due to join the worldwide network of telescopes that make up the EHT thereby boosting its discovery capabilities, and presenting an opportunity for Danish astronomers to be part of future groundbreaking discoveries with the EHT. ● Who: Introductory remarks by Thomas R. Greve (DAWN/DTUSpace). A panel of expert astrophysicists from Denmark and Taiwan will answer questions: ○ VIP guest: Paul Ho, East Asian Observatories Director, PI of the Greenland Telescope, and coinvestigator of the EHT result. ○ Thomas R. Greve, DAWN, DTU Space, Technical University of Denmark ○ Marianne Vestergaard, DARK, The Niels Bohr Institute, University of Copenhagen ○ Jes K. Jørgensen, StarPlan, The Niels Bohr Institute, University of Copenhagen ○ Ivalu B. Christensen, Lund University and Astrophysicist from Greenland ● When: Wednesday, April 10, 2019, 15:00 CEST. ● Where: The press conference will be held at DTU Space, Elektrovej 328, 2800 Lyngby, Denmark. The conference will be streamed online on: ■ www.greenlandtelescope.dk/outreach/ ■ https://www.facebook.com/GLTdenmark/ . ■ http://www.facebook.com/darkcosmologycentre/ ● RSVP: Me dia representatives can register to attend the event in person by contacting [email protected]. -
Astro2020 APC White Paper Studying Black Holes on Horizon Scales with VLBI Ground Arrays
Astro2020 APC White Paper Studying Black Holes on Horizon Scales with VLBI Ground Arrays Lindy Blackburn1;2;∗ Sheperd Doeleman1;2;∗, Jason Dexter12, José L. Gómez16, Michael D. Johnson1;2, Daniel C. Palumbo1;2, Jonathan Weintroub1;2, Joseph R. Farah1;2;21, Vincent Fish4, Laurent Loinard18;19, Colin Lonsdale4, Gopal Narayanan28, Nimesh A. Patel2, Dominic W. Pesce1;2, Alexander Raymond1;2, Remo Tilanus17;22;23, Maciek Wielgus1;2, Kazunori Akiyama1;3;4;5, Geoffrey Bower6, Avery Broderick7;8;9, Roger Deane10;11, Christian Michael Fromm13, Charles Gammie14;15, Roman Gold13, Michael Janssen17, Tomohisa Kawashima4, Thomas Krichbaum29, Daniel P. Marrone20, Lynn D. Matthews4, Yosuke Mizuno13, Luciano Rezzolla13, Freek Roelofs17, Eduardo Ros29, Tuomas K. Savolainen29;30;31, Feng Yuan24;25;26, Guangyao Zhao27 1 Black Hole Initiative at Harvard University, 20 Garden Street, Cam- and Particle Physics (IMAPP), Radboud University, P.O. Box 9010, bridge, MA 02138, USA 6500 GL Nijmegen, The Netherlands 2 Center for Astrophysics j Harvard & Smithsonian, 60 Garden Street, 18 Instituto de Radioastronomía y Astrofísica, Universidad Nacional Cambridge, MA 02138, USA Autónoma de México, Morelia 58089, México 3 National Radio Astronomy Observatory, 520 Edgemont Road, Char- 19 Instituto de Astronomía, Universidad Nacional Autónoma de México, lottesville, VA 22903, USA CdMx 04510, México 4 Massachusetts Institute of Technology, Haystack Observatory, 99 Mill- 20 Steward Observatory and Department of Astronomy, University of stone Road, Westford, MA 01886, USA Arizona, 933 N. Cherry Ave., Tucson, AZ 85721, USA 5 National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, 21 University of Massachusetts Boston, 100 William T, Morrissey Blvd, Tokyo 181-8588, Japan Boston, MA 02125, USA 6 Institute of Astronomy and Astrophysics, Academia Sinica, 645 N.