German ARC node/Bonn, Cologne Host institute 1: Argelander Institute for Astronomy Research and educational institute, dep. of Physics and Astronomy, Univ.

Slides:

Advertisements

Similar presentations

SA/EE INCOSE 7/17/00 Systems Architecting/Engineering Education at The Aerospace Corporation INCOSE Academic Forum 17 July 2000 David J. Evans Executive.

Advertisements

Christian Endres, Universität zu Köln 69 th ISMS, Urbana-Champaign, 2014 IMPROVED INFRASTUCTURE FOR CDMS AND JPL MOLECULAR SPECTROSCOPY CATALOGUES Christian.

Data Analysis Plan GBT IDL Workshop October 15, 2004.

JWST IFUs and Data Tool Development Plans Tracy Beck JWST NIRSpec Instrument Scientist.

Symposium on Digital Curation in the Era of Big Data: Career Opportunities and Educational Requirements Workforce Demand and Career Opportunities From.

Canadian Virtual Observatory Project David Schade Canadian Astronomy Data Centre Herzberg Institute for Astrophysics National Research Council Canada.

Ch Viewing the Universe

Interactive Narrative Content and Context for Visualization Curtis Wong Group Manager Next Media Research Microsoft Research Visualization of Astrophysical.

Physics 202: Introduction to Astronomy – Lecture 22 Carsten Denker Physics Department Center for Solar–Terrestrial Research.

Michigan Math and Science Scholars 2006 Ice Cream Social July 10, 2006.

UK ARC Node – Manchester Host institute: Jodrell Bank Centre for Astrophysics, University of Manchester Part of Interferometry Centre of Excellence, Jodrell.

Galaxies and the Foundation of Modern Cosmology III.

Science Requirements Impacting AO Architecture Claire Max Architecture Meeting July

Definitive Science with Band 3 adapted from the ALMA Design Reference Science Plan (

Lecture 9: Quasars & “Active” Galaxies Astronomy 5: The Formation and Evolution of the Universe Sandra M. Faber Spring Quarter 2007 UC Santa Cruz.

Careers in Astronomy AST 200. Astronomy Primary Goal: Understanding the nature of the universe and its constituents Means: Equipment building, research,

1 Universities Space Research Association AAS January 7, 2008 Early Science Workshop Range of E&PO Office Responsibilities Public Affairs (Public Information,

Astronomy Science combining all sciences. What is the Science of Astronomy? Astronomy is the scientific study of celestial objects (such as stars, planets,

Migale Virtual Instrument to study the evolution of galaxies BulgariaFranceRussia

Status of the Korean ALMA project Jongsoo Kim Korea Astronomy and Space Science Institute.

NA5: Interferometry Forum Andreas Quirrenbach (U Leiden / U Heidelberg)

The Pisgah Astronomical Research Institute (PARI) is a not-for- profit foundation established in Located in the Pisgah Forest 30 miles southwest.

C. ChandlerEVLA Advisory Committee Meeting September 6-7, Scientific Commissioning Plan Claire Chandler.

1 ASTRONET PROGRAM STATUS as of Preliminary Board 1 st Meeting Paris, 31 May 2005.

Principal Investigators: W. Wild (Instrumentation R&D) M. Hogerheijde (Allegro) M. Hogerheijde (Allegro) NOVA-3 Proposal Advancing Submillimeter Astronomy.

ALMA Operations and the North American ALMA Science Center Al Wootten NRAO.

Molecular Gas and Dust in SMGs in COSMOS Left panel is the COSMOS field with overlays of single-dish mm surveys. Right panel is a 0.3 sq degree map at.

06/10/2006IRAM Interferometry School1 ARC node at IRAM F.Gueth – IRAM Grenoble.

… and AGN Marcello Giroletti Dipartimento di Astronomia, UniBO Istituto di Radioastronomia, INAF.

Research at Indian Institute of Astrophysics The Indian Institute of Astrophysics (IIA) conducts research in solar physics, astrophysics, theoretical physics.

An I3 funded by the EU through FP6 Alastair G Gunn University of Manchester Jodrell Bank Observatory OPTICON BOARD MEETING – 11 th /12 th October 2004,

ARC node name/location Host institute: Full name Structure Size Areas of expertise ARC node representative: Full name ARC node Expertise: ARC node key.

Czech/Ondrejov (Prague) Host institute: Astronomical Institute of Czech Academy of Sciences Public research institution 60 FTEs research staff + 60 technicians/support.

NRAO Users Committee Meeting May 20-21, National Radio Astronomy Observatory NRAO Users Committee Meeting – May 20-21, 2008 ALMA Operations Chris.

E/PO Activities in the HEASARC 1 James Lochner HEASARC E/PO Lead.

The North American ALMA Science Center North America’s ALMA Regional Center The North American ALMA Science Center acts as the gateway to ALMA for North.

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

Lecture 1: Introduction to Cosmology Astronomy 5: The Formation and Evolution of the Universe Sandra M. Faber Spring Quarter 2007 UC Santa Cruz.

MAST Users Group – July 9, 2009 other planned and ongoing projects within MAST.

Large Area Surveys - I Large area surveys can answer fundamental questions about the distribution of gas in galaxy clusters, how gas cycles in and out.

Galaxies with Active Nuclei Chapter 14:. Active Galaxies Galaxies with extremely violent energy release in their nuclei (pl. of nucleus).  “active galactic.

ALMA and the Call for Early Science The Atacama Large (Sub)Millimeter Array (ALMA) is now under construction on the Chajnantor plain of the Chilean Andes.

ALMA Science Examples Min S. Yun (UMass/ANASAC). ALMA Science Requirements  High Fidelity Imaging  Precise Imaging at 0.1” Resolution  Routine Sub-mJy.

What is Astronomy? An overview..

Italian ARC-node/Bologna Host institute: INAF – Istituto di Radioastronomia (IRA), Bologna, Italy ARC-node: 2 staff, 5 postdocs (1 Co-Fin with Dept. Astron.

UlvestadEVLA Advisory Committee Meeting September 6-7, Future EVLA Operations Jim Ulvestad.

Nordic ARC Update Nov 17 th 2008 ARC face-to-face ESO Garching John Conway.

1 LSST Town Hall 227 th meeting of the AAS 1/7/2016 Pat Eliason, LSSTC Executive Office Pat Osmer, LSSTC Senior Advisor.

CfAO Professional Development Workshop “Connecting Science Education Theory and Practice” Introduction Lisa Hunter Associate Director, Education.

FIRST LIGHT A selection of future facilities relevant to the formation and evolution of galaxies Wavelength Sensitivity Spatial resolution.

Host institute: Institut de Radio Astronomie Millimétrique (IRAM) French (CNRS) / German (MPG) / Spanish (IGN) institute About 120 staff, including ~20.

Stars, Galaxies, and the Universe Section 4 Section 4: The Big Bang Theory Preview Key Ideas Hubble’s Observations A Theory Emerges Big Bang Theory Universal.

ALMA and FP6 Opportunities and strategy Funded project – construction phase FP6 timeframe 2003 – Good timing - first science planned for.

A dynamic database of molecular model spectra

SCI 151 Academic Success /snaptutorial.com For more course Tutorials

Group Summary: Stars and Their Evolution ALMA Science Workshop.

Observatories: Local & Remote

Hosted by LBL Cosmology Workshop

Latest from the Sloan Digital Sky Surveys

The “Milky Way”.

ARTIST Adaptive Radiative Transfer Innovations for Submillimeter Telescopes J. JØrgensen1, F. Bertoldi5, C. Brinch1, P. Frau3, J.M. Girart3, M. Hogerheijde2,

Astronomy – A Study of “Our Space”

What is Astronomy? An overview..

12/6/2018 Course Overview.

What is Astronomy? An overview..

Observatory Science Operations

Observatory Science Operations

The Formation of Stars Where do they come from? How do they form?

What is Astronomy? An overview..

Welcome to ALMA Community Day!

Presentation transcript:

German ARC node/Bonn, Cologne Host institute 1: Argelander Institute for Astronomy Research and educational institute, dep. of Physics and Astronomy, Univ. of Bonn, ~60 staff, ~70 PhD and master students, 9 research groups Expertise: star formation, galaxy evolution, ISM in galaxies, obs. cosmology, Milky Way, AGN; grav. lensing, LS structure, dark energy, stellar evolution Close ties to Max-Planck-Institute for Radio Astronomy, Univ. of Cologne Representative: Frank Bertoldi NameStatusFTEExpertise/task Frank BertoldiARC node representative 0.1Funding, overall management Stefanie MuehleARC node manager 0.75management, training, outreach, user support, mmVLBI Reinhold SchaafStaff0.3IT support, user sup. Sandra BurkuteanPostdoc0.5Short-spacings, web CASA, user support Alexander KarimPostdoc0.25CASA, user support Benjamin MagnelliPostdoc0.5Polarization, user sup. Toma BadescuPhD student0.1User support

German ARC node/Bonn, Cologne Host institute 2: I. Physikalisches Institut Research and educational institute, Univ. of Cologne, 6 research groups Expertise: Galactic Center, galaxies, nearby QSOs, PDR (obs. + modelling), large-scale mapping, plan. atmospheres, turbulent clouds, instrumentation Expertise in the German ARC node: Cologne Database for Molecular Spectroscopy (CDMS) Spectral line analysis and radiative transfer tools Short spacings for continuum data Polarization NameStatusFTEExpertise/task Peter SchilkeARC node affiliate 0.2Funding, Cologne management Christian EndresPostdoc0.5CDMS Thomas MoellerPostdoc0.5myXCLASS, Spectral measurement Alvaro Sanchez-MongePostdoc0.5myXCLASS, user support

German ARC node/Bonn, Cologne Major current activities: User support (including CS, QA2, f2f) Community Training/Outreach (Community Days, hands-on workshops, lecture series, tutorials) Expansion of the Cologne Database for Molecular Spectroscopy XCLASS (CASA toolbox for spectral line identification and fitting) CASA tools for the combination of single-dish and interferometric data Integration of polarization tools into CASA Funding: Federal Ministry for Education and Research, 3-year cycle, last renewed in July 2014 (currently 5 postdocs + IT) Universities of Bonn and Cologne

German ARC node/Bonn, Cologne Future perspectives: Maintain current staffing level Maintain special expertise and involvement in development projects as added service to the community New area of expertise: mm-VLBI with ALMA (with MPIfR, EU-ARC) Expand training opportunities for broader astronomical community Issues/concerns: German constitution does not allow federal agencies long-term funding of science support structures at universities (under review) o Funding specifically for development projects/German community o Risk of brain-drain at end of each funding period o additional lines of funding important Additional comments: ES phase proven very useful for training staff, testing procedures etc. German community seems to prefer formal meetings/workshops over individual face-to-face visits