Preliminary Cycle 6 Proposal Submission Statistics. Joint ALMA Observatory May 13, 2018
|
|
- Milton York
- 5 years ago
- Views:
Transcription
1 Preliminary Cycle 6 Proposal Submission Statistics Joint ALMA Observatory May 13, 2018
2 Number of Submitted Proposals and Time Requested Time requested (hours) Number 12-m 7-m Total Power All proposals ,698 10, ACA standalone Large Programs Polarization* Solar Target of Opportunity VLBI (3mm) VLBI (1mm) *Excludes VLBI Proposals
3 Subscription Rates: 12-m Array All Chile East Asia Europe Other Time requested (hours) 19, Offered see note Subscription N/A Note: All regions contribute observing time for proposals from PIs who are not affiliated with any of the ALMA regions.
4 Subscription Rates: 7-m Array All Chile East Asia Europe Other Time requested (hours) 10, Offered see note Subscription N/A Note: All regions contribute observing time for proposals from PIs who are not affiliated with any of the ALMA regions.
5 Subscription Rates: Total Power Array All Chile East Asia Europe Time requested (hours) Other Offered see note Subscription N/A Note: All regions contribute observing time for proposals from PIs who are not affiliated with any of the ALMA regions.
6 Requested 12-m Array Time per Proposal* *Excludes Large Programs
7 Requested 12-m Array Time by category* *Excludes Large Programs
8 Proposal Pressure per Configuration Dashed-line indicates nominal time available
9 East Asia 20% Number of Proposals for the 12-m Array Open Skies 3% Chile 6% Europe 43% 7 24% 8 4% 10 1% 9 4% 3 21% 4 8% Disks, Exoplanets & Solar System 22% Stellar evolution & Stars 8% Cosmology & High Redshift universe 24% 28% 6 33% 5 5% Interstellar medium, Star formation & Astrochemistry 23% Galaxies & Galactic nuclei 23%
10 East Asia 21% Open Skies 2% Chile 6% Requested Time on 12-m Array Europe 42% 7 23% 10 1% 8 3% 9 2% 3 25% Disks, Exoplanets & Solar System 18% Stellar evolution & Stars 7% Cosmology & High Redshift universe 30% 29% 6 36% 4 7% 5 3% Interstellar medium, Star formation & Astrochemistry 21% Galaxies & Galactic nuclei 24%
11 East Asia 22% Number of Proposals for the 7-m Array Open Skies Chile 4% 7% 28% Europe 39% 7 19% 8 6% 10 1% 9 3% 6 37% 3 26% 4 4% 5 4% Disks, Exoplanets & Solar System 9% Stellar evolution & Stars 13% Interstellar medium, Star formation & Astrochemistry 49% Cosmology & High Redshift universe 7% Galaxies & Galactic nuclei 22%
12 East Asia 19% 31% Open Skies Chile 3% 8% Requested Time on 7-m Array Europe 39% 7 16% 6 36% 10 < 1 % 8 7% 9 1% 4 2% 5 2% 3 36% Disks, Exoplanets & Solar System 7% Stellar evolution & Stars 5% Interstellar medium, Star formation & Astrochemistry 54% Cosmology & High Redshift universe 10% Galaxies & Galactic nuclei 24%
13 Number of Proposals for the Total Power Array East Asia 29% Open Skies Chile 7% 3% 27% Europe 34% 7 12% 6 43% 8 6% 9 1% 4 1% 3 34% 5 3% Stellar evolution & Stars 21% Disks, Exoplanets & Solar System 4% Cosmology & High Galaxies & Redshift Galactic universe nuclei < 1% 16% Interstellar medium, Star formation & Astrochemistry 59%
14 East Asia 28% Requested Time on Total Power Array Open Skies 1% Chile 5% Europe 36% 7 11% Requested Time TP 8 6% 3 45% Disks, Exoplanets & Solar System 1% Stellar evolution & Stars 2% Cosmology & High Redshift universe < 1% Galaxies & Galactic nuclei 21% 30% 6 36% 4 1% 5 1% Interstellar medium, Star formation & Astrochemistry 76%
15 Requested Time on 12-m Array for Large Programs East Asia 22% Chile 8 10% 7 2% 3 16% 20% 33% Europe 35% 6 54% 4 8% 5 < 1% Stellar evolution & Stars 6% Disks, Exoplanets & Solar System 14% Interstellar medium, Star formation & Astrochemistry 28% Cosmology & High Redshift universe 36% Galaxies & Galactic nuclei 16%
16 Requested Time on 7-m Array for Large Programs Chile 13% 7 10% East Asia 13% Europe 42% 6 36% 3 54% Interstellar medium, Star formation & Astrochemistry 65% Galaxies & Galactic nuclei 35% 32%
17 Requested Time on Total Power Array for Large Programs Chile 11% 7 20% East Asia 16% Europe 42% 3 45% Interstellar medium, Star formation & Astrochemistry 100% 31% 6 35%
18 Number of Submitted Proposals by Cycle Number of proposals Cycle 0 Cycle 1 Cycle 2 Cycle 3 Cycle 4 Cycle 5 Cycle 6
19 Time requested (hours) Time requested by Cycle Total Power Array 7-m Array 12-m Array 0 Cycle 0 Cycle 1 Cycle 2 Cycle 3 Cycle 4 Cycle 5 Cycle 6
20 Requested 12-m Array Time per Proposal by Cycle* *Excludes Large Programs
21 OversubscripRon rate Oversubscription Rate: 12-m Array Chile East Asia Europe 0 Cycle 0 Cycle 1 Cycle 2 Cycle 3 Cycle 4 Cycle 5 Cycle 6
an NSF Facility Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array
an NSF Facility Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array ALMA s Contributions to Outflows, Winds and Jets Al Wootten
More informationFirst Detection of an Intermediate-Mass Black Hole Candidate in the Milky Way
Press Release September 27, 2017 Keio University First Detection of an Intermediate-Mass Black Hole Candidate in the Milky Way Professor Tomoharu Oka of the Department of Physics, Faculty of Science and
More informationSpitzer Space Telescope Cycle-6 Exploration Science Programs
Spitzer Space Telescope Cycle-6 Exploration Science Programs LSL-1 Introduction Cryogen depletion expected in mid-april 2009 No changes in expected instrument performance since Call for Proposals issued
More informationCycle-5 Proposal. Submission Statistics
Cycle-5 Proposal Overview Cycle-5 is estimated to include 6 months of new observations Cycle-5 starts in July 2008 Expected cryogen depletion date is April 2009 2-3 months of previous cycle observations
More informationSolar research with ALMA: Czech node of European ARC as your user-support infrastructure
Solar research with ALMA: Czech node of European ARC as your user-support infrastructure M. Bárta 1, I. Skokič 1, R. Brajša 2,1 & the Czech ARC Node Team 1 European ARC Czech node, Astronomical Inst. CAS,
More informationALMA/ASTE/Mopra Report
1 ALMA/ASTE/Mopra Report Daisuke Iono (NAOJ) NRO UM 2014/7/24 2 ALMA Telescope 21 countries and regions (Japan, Taiwan, Korea, U.S., Canada, 15 European nations, and Chile) 4 regions East Asia: NAOJ North
More informationAn Introduction to the Cycle 4 ALMA Observing Tool
An Introduction to the Cycle 4 ALMA Observing Tool How to turn that great idea into ALMA data.. Harvey Liszt, Alison Peck, Tony Remijan, Sabrina Stierwalt Atacama Large Millimeter/submillimeter Array Expanded
More informationOpportunities of observing at ESO How to write a successful proposal. Bruno Leibundgut
Opportunities of observing at ESO How to write a successful proposal Bruno Leibundgut 1 European Southern Observatory n Mission Develop and operate world-class observing facilities for astronomical research
More informationALMA Cycle 6 Information and Cycle 4 and Cycle 5 Statistics
ALMA Cycle 6 Information and Cycle 4 and Cycle 5 Statistics Yu-Nung Su (ASIAA) on behalf of Taiwan ARC node ALMA Cycle 6 Users Workshop March 26, 2018 Photo Credit: Wei-Hao Wang Cycle 6 Timeline (23:00
More informationFrom 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
More informationIntroduction to Radio Interferometry Jim Braatz (NRAO)
Introduction to Radio Interferometry Jim Braatz (NRAO) Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Radio Astronomy
More informationTable of Contents and Executive Summary Final Report, ALTAIR Committee Access to Large Telescopes for Astronomical Instruction and Research (ALTAIR)
Complete report available from http://www.noao.edu/system/altair 1 TableofContentsandExecutiveSummary FinalReport,ALTAIRCommittee AccesstoLargeTelescopesforAstronomical InstructionandResearch(ALTAIR) ForthecompletereportandmoreinformationabouttheALTAIRcommittee,
More informationCycle 2 status Cycle 3 Policies
Cycle 2 status Cycle 3 Policies The Science Portal: entry point to ALMA operations and users support Evanthia will bring you through the science portal The SP contains all the information necessary to
More informationAstrochemistry In the Era of Broadband single dish and Interferometric observations
Astrochemistry In the Era of Broadband single dish and Interferometric observations Anthony J. Remijan NA ARC Manager 1 2014 ANASAC Meeting National Radio Astronomy Observatory Overview Why imaging? What
More informationALMA Science Ex am ples
ALMA Science Ex am ples Min S. Yun (UMass/ ANASAC) ALMA Science Requirements High Fidelity Imaging Precise Imaging at 0.1 Resolution Routine Sub- mjy Continuum Sensitivity Routine mk Spectral Sensitivity
More informationA Survey of GBT Science. Felix J. Lockman Green Bank Observatory, Green Bank, WV
A Survey of GBT Science Felix J. Lockman Green Bank Observatory, Green Bank, WV GBT Surveys Workshop November 13, 2018 National Radio Quiet Zone Unblocked Optics for High Dynamic Range GBT Surveys Workshop
More informationCharacterization of the exoplanet host stars. Exoplanets Properties of the host stars. Characterization of the exoplanet host stars
Characterization of the exoplanet host stars Exoplanets Properties of the host stars Properties of the host stars of exoplanets are derived from a combination of astrometric, photometric, and spectroscopic
More informationStudying MWG structure with VERA
Studying MWG structure with VERA Mareki Honma Mizusawa VLBI Observatory, NAOJ Milky Way & VERA Ogasawara station contents Galaxy scale astrometry with VERA + some more topics future prospect VERA and optical
More informationHighlights of the program of. The European Southern Observatory
Highlights of the program of The European Southern Observatory ESO, the European Southern Observatory Established in1962, with the main mission of providing its member states with world-class facilities
More informationAn Introduction to the Cycle 4 ALMA Observing Tool How to turn that great idea into ALMA data...
An Introduction to the Cycle 4 ALMA Observing Tool How to turn that great idea into ALMA data... Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope
More informationThe Potential of Ground Based Telescopes. Jerry Nelson UC Santa Cruz 5 April 2002
The Potential of Ground Based Telescopes Jerry Nelson UC Santa Cruz 5 April 2002 Contents Present and Future Telescopes Looking through the atmosphere Adaptive optics Extragalactic astronomy Planet searches
More informationAstronomy Today. Eighth edition. Eric Chaisson Steve McMillan
Global edition Astronomy Today Eighth edition Eric Chaisson Steve McMillan The Distance Scale ~1 Gpc Velocity L Distance Hubble s law Supernovae ~200 Mpc Time Tully-Fisher ~25 Mpc ~10,000 pc Time Variable
More informationService vs Visitor mode observing at ESO. Should I stay or should I go?
Service vs Visitor mode observing at ESO. Should I stay or should I go? Francesca Primas, Michael Hilker and Lowell Tacconi-Garman Directorate for Science & Directorate of Operations Observing Programmes
More informationBraneworld Cosmological Perturbations
2005 2005 2005 Spectropolarimetric Studies on Circumstellar Structure of Low-Mass Pre-Main-Sequence Stars ELT Statistical Properties of Lyman a Emitters at Redshift 5.7 Neutrino Probes of Galactic and
More informationTowards an accurate alignment of the VLBI frame with the future Gaia optical frame
Towards an accurate alignment of the VLBI frame with the future Gaia optical frame G. Bourda,, A. Collioud Laboratoire d Astrophysique de Bordeaux R. Porcas Max Planck Institut für Radioastronomie S. Garrington
More informationA review of (sub)mm band science and instruments in the ALMA era
A review of (sub)mm band science and instruments in the ALMA era Marcella Massardi INAF- Istituto di Radioastronomia Italian node of European ALMA Regional Centre SISSA March 2018 Outline Signals in the
More informationOrigin of the stellar Initial Mass Function (IMF) in the W43-MM1 ridge
Origin of the stellar Initial Mass Function (IMF) in the W43-MM1 ridge Fabien Louvet (Universidad de Chile & IPAG Grenoble) Special credits to: F. Motte, T. Nony, S. Bontemps, A. Gusdorf, P. Didelon, P.
More information2. Radio Astronomy. 3. AGN Research
The Korea Astronomy and Space Science Institute (KASI) is a government-funded research institute located in Daejeon, Republic of Korea. We conduct front-line research in various fields of astronomy, astrophysics
More informationGALAXY EVOLUTION STUDIES AND HIGH PERFORMANCE COMPUTING
GALAXY EVOLUTION STUDIES AND HIGH PERFORMANCE COMPUTING Andreas Efstathiou European University Cyprus Astrophysics and HPC group ACTIVE AREAS OF ASTRONOMY OPPORTUNITIES FOR THEORETICAL, OBSERVATIONAL AND
More informationTerahertz Science Cases for the Greenland Telescope
Terahertz Science Cases for the Greenland Telescope Hiroyuki Hirashita Satoki Matsushita, Patrick M. Koch ASIAA GLT Single Dish Science Discussion Group (ASIAA, Taiwan) Topics 1. GLT Project 2. Opening
More informationALMA: the project becomes real
Mem. S.A.It. Suppl. Vol. 3, 292 c SAIt 2003 Memorie della Supplementi ALMA: the project becomes real G. Tofani Istituto di Radioastronomia, Consiglio Nazionale delle Ricerche, via Gobetti 101, 40146 Bologna
More informationALMA Development Plan. ALMA Days 25 Jun 2012 Leonardo Testi
ALMA Development Plan ALMA Days 25 Jun 2012 Leonardo Testi Leonardo Testi: ALMA Development Plan, 25 Jun 2012 Atacama Large Millimeter Array At least 50x12m Antennas Frequency range 30-1000 GHz (0.3-10mm)
More informationHerschel Mission Overview and Key Programmes
Herschel Mission Overview and Key Programmes SPIE Astronomical Instrumentation 2008 Space Telescopes and Instrumentation I: Optical, Infrared, and Millimeter Wave Marseille, 23-28 June 2008 Göran L. Pilbratt
More information1 Birth of Galaxies. Millimeter/submillimeter Wave The vision for the Dark Universe. ALMA (Atacama Large Millimeter/ submillimeter Array)
The Universe Explored by ALMA can see what has never been observed at optical wavelengths, such as protogalaxies formed in the very early years of the universe, birth of stars and planets like our solar
More informationActive Galaxies and Galactic Structure Lecture 22 April 18th
Active Galaxies and Galactic Structure Lecture 22 April 18th FINAL Wednesday 5/9/2018 6-8 pm 100 questions, with ~20-30% based on material covered since test 3. Do not miss the final! Extra Credit: Thursday
More informationCzech ARC Node Bartosz Dąbrowski. ALMA Regional Centre, Czech Republic
Bartosz Dąbrowski ALMA Regional Centre, Republic Toruń, 22 23 October 2013 The interface between ALMA and the astronomy community is provided by the three ALMA Regional Centres (ARCs), in Europe, North
More informationTable of Contents and Executive Summary Final Report, ReSTAR Committee Renewing Small Telescopes for Astronomical Research (ReSTAR)
For the complete report, see http://www.noao.edu/system/restar 1 TableofContentsandExecutiveSummary FinalReport,ReSTARCommittee RenewingSmallTelescopesforAstronomical Research(ReSTAR) ForthecompletereportandmoreinformationabouttheReSTARcommittee,
More informationAtacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Observing with ALMA Introduction: ALMA and the NAASC Nine Antennas at
More informationGalactic environment The possibility of Galactic Paleoclimatology. Jun Makino with Takayuki Saito, Junichi Baba ELSI
Galactic environment The possibility of Galactic Paleoclimatology Jun Makino with Takayuki Saito, Junichi Baba ELSI In short... Q: Has the Milky Way Galaxy anything to do with Earth s environment? A: Yes,
More informationTransitional disks and their host stars
Transitional disks and their host stars Nienke vander dermarel Marel Nienke van Leiden Observatory rd September 23 2011 The Netherlands August 13th 2013 (ING) Star and planet formation Class II => III:
More informationThe Robert C. Byrd Green Bank Telescope
The Robert C. Byrd Green Bank Telescope Phil Jewell National Radio Astronomy Observatory 520 Edgemont Road Charlottesville, VA 22903-2475 USA pjewell@nrao.edu NAIC-NRAO School on Single Dish Radio Astronomy
More informationGalaxies with Active Nuclei. Active Galactic Nuclei Seyfert Galaxies Radio Galaxies Quasars Supermassive Black Holes
Galaxies with Active Nuclei Active Galactic Nuclei Seyfert Galaxies Radio Galaxies Quasars Supermassive Black Holes Active Galactic Nuclei About 20 25% of galaxies do not fit well into Hubble categories
More informationAstronomy across the spectrum: telescopes and where we put them. Martha Haynes Discovering Dusty Galaxies July 7, 2016
Astronomy across the spectrum: telescopes and where we put them Martha Haynes Discovering Dusty Galaxies July 7, 2016 CCAT-prime: next generation telescope CCAT Site on C. Chajnantor Me, at 18,400 feet
More informationCosmology, Black Holes, and AGNs with Water Megamasers
Cosmology, Black Holes, and AGNs with Water Megamasers Jim Braatz (NRAO) Mark Reid Jim Condon Fred Lo Christian Henkel Cheng-Yu Kuo Feng Gao Wei Zhao Violetta Impellizzeri Jan Wagner Dom Pesce Jenny Greene
More informationHomework 13 (not graded; only some example ques!ons for the material from the last week or so of class)
Homework 13 (not graded; only some example ques!ons for the material from the last week or so of class)! This is a preview of the draft version of the quiz Started: Apr 28 at 9:27am Quiz Instruc!ons Question
More informationCommensal observing: HI science with MIGHTEE
Commensal observing: HI science with MIGHTEE Natasha Maddox Postdoctoral Fellow at Image credit: SKA Organization 135 science chapters 10 HI chapters 24 hours in a day Time oversubscription 135 science
More informationThe ALMA Observing Preparation Tool
The ALMA Observing Preparation Tool Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Video versions of this material:
More informationExoplanet Detection and Characterization with Mid-Infrared Interferometry
Exoplanet Detection and Characterization with Mid-Infrared Interferometry Rachel Akeson NASA Exoplanet Science Institute With thanks to Peter Lawson for providing material Sagan Workshop July 21, 2009
More informationChapter 7: From theory to observations
Chapter 7: From theory to observations Given the stellar mass and chemical composition of a ZAMS, the stellar modeling can, in principle, predict the evolution of the stellar bolometric luminosity, effective
More informationWhy study plasma astrophysics?
Why study plasma astrophysics? Nick Murphy and Xuening Bai Harvard-Smithsonian Center for Astrophysics Astronomy 253: Plasma Astrophysics January 25, 2016 Today s plan Definition of a plasma Plasma astrophysics:
More informationA Supermassive Black Hole in the Dwarf Starburst Galaxy Henize Amy Reines Einstein Fellow National Radio Astronomy Observatory
A Supermassive Black Hole in the Dwarf Starburst Galaxy Henize 2-10 Amy Reines Einstein Fellow National Radio Astronomy Observatory Supermassive black holes and galaxy evolution Supermassive black holes
More informationRadio astronomical use of the electromagnetic spectrum at Onsala Space Observatory
Radio astronomical use of the electromagnetic spectrum at Onsala Space Observatory Magnus Thomasson, Onsala Space Observatory, Sweden Summary Radio astronomy is a vigorous science which provides both astrophysicists
More informationDesign Reference Mission for SKA1 P. Dewdney System Delta CoDR
Phasing of SKA science: Design Reference Mission for SKA1 P. Dewdney System Delta CoDR Feb. 23, 2011 21 st Century Astrophysics National Aeronautics and Space Administration Jet Propulsion Laboratory California
More informationRadio Interferometry and ALMA
Radio Interferometry and ALMA T. L. Wilson ESO 1 PLAN Basics of radio astronomy, especially interferometry ALMA technical details ALMA Science More details in Interferometry Schools such as the one at
More informationPerspectives for Future Groundbased Telescopes. Astronomy
Perspectives for Future Groundbased Telescopes Tim de Zeeuw 1 Astronomy Study of everything beyond the Earth Objects far away, hence small and faint Limited information about their nature Searches and
More informationALMA Early Science Cycle 3: Outcome of the Proposal Review Process
ALMA Early Science Cycle 3: Outcome of the Proposal Review Process Proposal Review Process In response to the Call for Proposals for Early Science Cycle 3, ALMA received 1578 valid proposals by the 23
More informationRadioNet: Advanced Radio Astronomy in Europe
RadioNet: Advanced Radio Astronomy in Europe An I3 funded by the EU through FP6 Philip Diamond RadioNet Co-ordinator University of Manchester Jodrell Bank Observatory ILIAS 2 nd ANNUAL MEETING 7 th /8
More informationAstro 32 - Galactic and Extragalactic Astrophysics/Spring 2016
Astro 32 - Galactic and Extragalactic Astrophysics/Spring 2016 The class meets Monday and Wednesday 10:30-11:45am (Block E+) in 574 Boston Ave, room 401 Instructor: Professor Anna Sajina email: Anna.Sajina@tufts.edu
More informationIAU General Assembly Block Schedule - Week 1 - August
Monday, 3 August 2015 10:00 am - 10:30 am 10:00 am - 4:00 pm Exhibits, Posters, and Cyber Café, Kamehameha Hall I S 318 Population Models/Collisions and S 317 Global Properties of Stellar Halos Cratering
More informationAstronomy in the Netherlands. Konrad Kuijken Leiden Observatory
Astronomy in the Netherlands Konrad Kuijken Leiden Observatory Landscape Four university departments, together form NOVA Two National research institutes, Space and Radio Funding agency NWO-exact sciences
More informationRadio-optical outliers a case study with ICRF2 and SDSS
Radio-optical outliers a case study with ICRF2 and SDSS Sándor Frey FÖMI Satellite Geodetic Observatory & MTA Research Group for Physical Geodesy and Geodynamics (Budapest, Hungary) Gábor Orosz Department
More informationGalaxies. The majority of known galaxies fall into one of three major classes: spirals (78 %), ellipticals (18 %) and irregulars (4 %).
Galaxies Collection of stars, gas and dust bound together by their common gravitational pull. Galaxies range from 10,000 to 200,000 light-years in size. 1781 Charles Messier 1923 Edwin Hubble The distribution
More informationSupernovae in Distant Galaxies
Hubble Space Telescope Cycle 11 General Observer Proposal Principal Investigator: Mr. Anthony Martorano Institution: Stony Brook University USA/NY Electronic mail: anthony.martorano@stonybrook.edu Scientific
More informationPART 3 Galaxies. Gas, Stars and stellar motion in the Milky Way
PART 3 Galaxies Gas, Stars and stellar motion in the Milky Way The Interstellar Medium The Sombrero Galaxy Space is far from empty! Clouds of cold gas Clouds of dust In a galaxy, gravity pulls the dust
More informationSECOND ANNOUNCEMENT. Science with the Hubble Space Telescope II
SECOND ANNOUNCEMENT Science with the Hubble Space Telescope II TOPICS A Scientific Conference co-organised by the Space Telescope Science Institute, Baltimore, MD, USA, and the Space Telescope European
More informationATACAMA LARGE MILLIMETER ARRAY
ATACAMA LARGE MILLIMETER ARRAY ATACAMA LARGE MILLIMETER ARRAY ALMA the Atacama Large Millimeter Array will be a single instrument composed of up to 64 high-precision antennas located on the Chajnantor
More informationTime Allocation at ESO
Time Allocation at ESO N&O P@@ Nando Patat Observing Programmes Office Somewhere, in Australia, September 2017 1 The Observing Programmes Office OPO is in charge of allocating the observing time and scheduling
More informatione-vlbi Radio interferometers How does VLBI work? What science do we do with VLBI? How has the technology changed? Advantages of e-vlbi e-astronomy
e-vlbi Radio interferometers How does VLBI work? What science do we do with VLBI? How has the technology changed? Advantages of e-vlbi e-astronomy Simple interferometer In a simple interferometer, two
More informationActive Galactic Nuclei (AGNs): A type of AGNs: Quasars. Whatever is powering these QSO s must be very small!!
Active Galactic Nuclei (AGNs): Galaxies with lots of activity AST 101 General Astronomy: Stars & Galaxies Some galaxies at high redshift (large lookback times) have extremely active centers More than 1000
More informationEuropean Southern Observatory ELT. The Extremely Large Telescope. The World s Biggest Eye on the Sky
European Southern Observatory ELT The Extremely Large The World s Biggest Eye on the Sky Building a Giant On a mountain in the Atacama Desert in northern Chile, ESO, the European Southern Observatory,
More informationSolar System Science with JWST!
Solar System Science with JWST! Dean C. Hines Space Telescope Science Institute JWST Imaging Modes! Mode Imaging Aperture Mask Interferometry Coronography Instrument Wavelength (microns) Pixel Scale (arcsec)
More informationA Random Walk Through Astrometry
A Random Walk Through Astrometry Astrometry: The Second Oldest Profession George H. Kaplan Astronomical Applications Department Astrometry Department U.S. Naval Observatory Random Topics to be Covered
More informationASTR Astrophysics 1 - Stellar and Interstellar. Phil Armitage. office: JILA tower A909
ASTR 3730 Astrophysics 1 - Stellar and Interstellar Phil Armitage office: JILA tower A909 email: pja@jilau1.colorado.edu Part one of a year-long introduction to astrophysics: Aim - develop physical understanding
More informationGreen Bank Telescope Science Program. Felix Jay Lockman NRAO, Green Bank WV
Green Bank Telescope Science Program Felix Jay Lockman NRAO, Green Bank WV The Green Bank Observatory A Showcase for the NSF 40,000-50,000 visitors each year NOAA Weather in Focus Photo Contest First Place:
More informationHistory of Astronomy on Mauna Kea
History of Astronomy on Mauna Kea CFHT: Interna-onal Partnership Work on the 3.6-meter Canada-France-Hawaii Telescope (CFHT) began in 1973. CFHT began operations in 1979, establishing their headquarters
More informationSubaru Telescope Director s Report CFHTUM 2016
Subaru Telescope Director s Report CFHTUM 2016 Nobuo ARIMOTO Subaru Telescope H.Fujiwara (2015) 2 Subaru Telescope Subaru-HiCIAO Spots Young Stars Surreptitiously Gluttonizing Their Birth Cloud (Liu et
More informationALMA: a new instrument for science in the submm band
ALMA: a new instrument for science in the submm band M. Massardi Italian node of ESO ALMA Regional Center INAF-Istituto di Radioastronomia (Bologna) ERIS school, 8th september 2011 ALMA basics and status
More informationALMA's Window on Molecular Emission: Small Ions to Complex Prebiotics
ALMA's Window on Molecular Emission: Small Ions to Complex Prebiotics Al Wootten Complex Molecules in Space Boom Time for IS Spectroscopy 1000 year anniversary of SN1006 this week! Correlator technology:
More informationMASSIVE BLACK HOLES AMY REINES IN NEARBY DWARF GALAXIES HUBBLE FELLOW NATIONAL OPTICAL ASTRONOMY OBSERVATROY
MASSIVE BLACK HOLES IN NEARBY DWARF GALAXIES AMY REINES HUBBLE FELLOW NATIONAL OPTICAL ASTRONOMY OBSERVATROY Motivation: The origin of massive black holes (BHs) Massive BHs are fundamental components of
More informationPDF hosted at the Radboud Repository of the Radboud University Nijmegen
PDF hosted at the Radboud Repository of the Radboud University Nijmegen The following full text is a publisher's version. For additional information about this publication click this link. http://hdl.handle.net/2066/84153
More informationASTERICS Astronomy ESFRI & Research Infrastructure Cluster
ASTERICS Astronomy ESFRI & Research Infrastructure Cluster Giuseppe Cimò Joint Institute for VLBI - ERIC (JIVE) Netherlands Institute for Radio Astronomy (ASTRON) 1 what is ASTERICS? A major collaboration
More informationMapping the Galaxy using hydrogen
The Swedish contribution to EU-HOU: A Hands-On Radio Astronomy exercise Mapping the Galaxy using hydrogen Daniel Johansson Christer Andersson Outline Introduction to radio astronomy Onsala Space Observatory
More informationESO: Status and perspectives
ESO: Status and perspectives ESO, the European Southern Observatory Established in1962, with the main mission of providing its member states with world-class facilities that individual European countries
More informationAstronomy across the spectrum: telescopes and where we put them. Martha Haynes Exploring Early Galaxies with the CCAT June 28, 2012
Astronomy across the spectrum: telescopes and where we put them Martha Haynes Exploring Early Galaxies with the CCAT June 28, 2012 CCAT: 25 meter submm telescope CCAT Site on C. Chajnantor Me, at 18,400
More informationTHE STRATEGIC VISION OF INAF
THE STRATEGIC VISION OF INAF 2015-2024 Scientific Council Enzo Brocato Stefano Covino Silvia Masi Francesca Matteucci Stefano Orsini Bianca Poggianti Pietro Schipani Scientific challenges in the 21th century
More informationALMA Observing Tool!
ALMA Observing Tool Phase I: Observing Proposal Yu-Nung Su" ALMA User Workshop 2015" March 28, 2015 Introduction What is Observing Tool (OT)? provides a comprehensive set of interfaces (form and tool)
More informationPAGaN II: The evolution of AGN jets on sub-parsec scales Junghwan Oh Seoul National University East-Asia AGN Workshop 2016
PAGaN II: The evolution of AGN jets on sub-parsec scales Junghwan Oh Seoul National University East-Asia AGN Workshop 2016 S. Trippe, S. Kang, D. Kim, M. Kino, SS. Lee, T. Lee, J. Park, B. Sohn AGN at
More informationHaystack astronomy VLBI progress/plans. Sheperd Doeleman Haystack Observatory
Haystack astronomy VLBI progress/plans Sheperd Doeleman Haystack Observatory Haystack Astronomy Context: General Mission and Interest: Develop new VLBI inst. that optimizes science for astronomical community.
More informationFormation, Detection and the Distribution of Complex Organic Molecules with the Atacama Large Millimeter/submillimeter Array (ALMA)
Formation, Detection and the Distribution of Complex Organic Molecules with the Atacama Large Millimeter/submillimeter Array (ALMA) Anthony J. Remijan, ALMA Program Scientist Joint ALMA Observatory National
More informationGalaxies & Introduction to Cosmology
Galaxies & Introduction to Cosmology Other Galaxies: How many are there? Hubble Deep Field Project 100 hour exposures over 10 days Covered an area of the sky about 1/100 the size of the full moon Probably
More informationChapter 19 Reading Quiz Clickers. The Cosmic Perspective Seventh Edition. Our Galaxy Pearson Education, Inc.
Reading Quiz Clickers The Cosmic Perspective Seventh Edition Our Galaxy 19.1 The Milky Way Revealed What does our galaxy look like? How do stars orbit in our galaxy? Where are globular clusters located
More informationMillimetre Science with the AT
Millimetre Science with the AT Astrochemistry with mm-wave Arrays G.A. Blake, Caltech 29Nov 2001 mm-arrays: Important Features - Spatial Filtering - Transform to image plane - Cross Correlation (Sub)Millimeter
More informationPlanning (VLA) observations
Planning () observations Loránt Sjouwerman, NRAO Sixteenth Synthesis Imaging Workshop 16-23 May 2018 Outline General advice on planning any (ground based) observation AUI telescopes: the GBT, ALMA, VLBA,
More informationActive Galactic Nuclei
Active Galactic Nuclei How were they discovered? How common are they? How do we know they are giant black holes? What are their distinctive properties? Active Galactic Nuclei for most galaxies the luminosity
More informationLARGE QUASAR GROUPS. Kevin Rahill Astrophysics
LARGE QUASAR GROUPS Kevin Rahill Astrophysics QUASARS Quasi-stellar Radio Sources Subset of Active Galactic Nuclei AGNs are compact and extremely luminous regions at the center of galaxies Identified as
More informationThe high angular resolution component of the SKA
The high angular resolution component of the SKA Tingay, S. 1, Bignall, H. 1, Colegate, T. 1, Aben, G. 2, Nicolls, J. 2 & Weston, S. 3 Prof. Steven Tingay SKA2010 Deputy Director, ICRAR March 22 25, 2010
More informationThe Redshift Evolution of Bulges and Disks of Spiral Galaxies in COSMOS
Pathways through an Eclectic Universe ASP Conference Series, Vol. 390, c 2008 J. H. Knapen, T. J. Mahoney, and A. Vazdekis, eds. The Redshift Evolution of Bulges and Disks of Spiral Galaxies in COSMOS
More informationChapter 23 The Milky Way Galaxy Pearson Education, Inc.
Chapter 23 The Milky Way Galaxy The Milky Way is our own galaxy viewed from the inside. It is a vast collection of more than 200 billion stars, planets, nebulae, clusters, dust and gas. Our own sun and
More informationNRAO Structural Changes: Announcing the Separation of the Green Bank Observatory and the Long Baseline Observatory
NRAO enews Volume 9, Issue 3 24 March 2016 NRAO Structural Changes: Announcing the Separation of the Green Bank Observatory and the Long Baseline Observatory Tony Beasley (NRAO Director) and Ethan Schreier
More informationChapter 15 Galaxies and the Foundation of Modern Cosmology
15.1 Islands of stars Chapter 15 Galaxies and the Foundation of Modern Cosmology Cosmology: study of galaxies What are they 3 major types of galaxies? Spiral galaxies: like the milky way, look like flat,
More information