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Nachrichten, Termine, Experten
Nachrichten, Termine, Experten
APEX (Atacama Pathfinder Experiment), is the most efficient earthborn Instrument for studying the early Universe, galaxies and star formation processes. After a constructing period of 36 months - 5100 meters high in the Chilean Atacam desert - the results of "first light" show that the radio telescope gives an unique and almost unobscured view on of star forming regions and galactic nuclei,.
On the occasion of the Dediction and first light results you are invited to a
Background talk
On July 14th 2005, 11:00 - 16:00
At Max Planck Institut for Radio Astronomy
Auf dem Hügel 69, 53121 Bonn, Germany
The APEX Telescope was constructed by an international collaboration led by Prof. Dr. Karl Menten, Director at Max Planck Institute for Radio Astronomy, Bonn. The Atacama Pathfinder Experiment will:
· carry out research in submillimeter radio astronomy that is expected to bring rapid advances, particularly in studies of the early Universe, galaxies and star formation processes.
· study the southern celestial hemisphere at submillimeter wavelengths, a spectral range where it is almost unexplored, an
· serve as a pathfinder for the Atacama Large Millimeter Array (ALMA) by performing wide-field observations for later ALMA detailed follow-up studies.
The Max Planck Institute for Radio Astronomy, the European Southern Observatory (ESO) and the Onsala Space Observatory (OSO) share APEX funding and observing time, with 10% of the observing time set aside for Chilean astronomers.
Illustrations and footage are available free of charge.
Programme
11:00 Welcome Prof Dr Karl M. Menten Director Max Planck Institute for Radio Astronomy
11:05 Introduction of the APEX Consortium
Prof Dr Roy Booth, Onsala Space Observatory (OSO)
Dr Ian Corbett, European Southern Observatory (ESO)
Prof Dr Karl Menten, Max Planck Institute for Radio Astronomy
11:20 Submm astronomy & science perspectives with APEX Prof Dr Karl M. Menten Director Max Planck Institute for Radio Astronomy
11:50 Project Overview
- Introduction & Status of the Project: Dr Rolf Güsten
Projektmanager APEX (MPIfR)
- Infrastructure, Logistics, Operation: Dr. Lars-A. Nyman
Head of APEX Station
12:15 Design and Construction of the telescope
Dr Karl-Heinz Stenvers, Director VERTEX Antennentechnik
Dr. Konrad Pausch, Technical Director VERTEX Antennentechnik
12:35 Commissioning of the Telescope
Dr Rolf Güsten
12:55 -- Lunch Break --
13:45 Instrumentation for APEX (moderation: Dr Rolf Güsten)
Detector instruments for submillimeter telescopes fall into two broad categories: heterodyne and bolometric receivers. Heterodyne receivers allow splitting of the radiation into fine frequency intervals, creating spectra. Analysis of such spectra (spectroscopy) allows determination of the physical properties and chemical content of interstellar molecular clouds within and outside of our Galaxy.
Bolometers on the other hand, have very broad bandwidth and are thus extremely sensitive. Recent developments allow packaging of detectors into arrays, similar to the CCD array in your digital camera.
APEX will be equipped with both, bolometer and heterodyne arrays which, including the necessary readout electronics, are developed by the MPIfR and OSO, in some cases in collaboration with other partners.
Selected presentations by APEX instrument scientists will give an overview of APEX detectors and detector arrays - present and future.
14:15 First-light science results (moderation: Prof Dr Karl Menten)
A variety of scientific results have been obtained with APEX in the first few weeks of its operation. These include measurements of molecules in the immediate vicinity of hot massive very young stars, the central regions of galaxies containing active nuclei and the Magellanic Clouds, our nearest neighbour galaxies. Since these wavelengths have never before been explored with a similar telescope in the southern hemisphere, many of these results are genuine "firsts".
APEX scientists will present assorted first-light results.
15:00 Plans for the near future (2005/2006):
In a collaboration with the University of California at Berkeley and Bonn University an extremely sensitive survey for distortions in the spectrum of the cosmological microwave background radiation by the hot plasma of clusters of galaxies (the "Sunyaev-Zeldovich-Effekt") will be conducted, revealing thousands of galaxy clusters, placing constraints on the cosmological parameters, Dark Energy and structure formation in the Universe.
In a systematic survey of our Milky Way galaxy's plane we shall detect gas condensations harbouring newly-formed stars or protostars with masses as little as one solar mass at distances of thousands of light years.
Innovative receivers on the superb Atacama site will allow the first ground-based explorations of the few atmospheric "windows" beyond one Terahertz (wavelengths shorter than 300 micrometers). Such receivers are currently developed for APEX at OSO, the University at Cologne, and the Harvard-Smithsonian Center for Astrophysics.
As it name says, APEX is the pathfinder for other (sub)mm wavelength projects, most directly for the Atacama Large Millimeter Array (ALMA) - an interferometric array of dozens of submillimeter telescopes (of which APEX is actually one of the prototypes). There also is great complementarity to the Herschel Satellite (the 4th cornerstone in ESA's "Horizons 2000" program) and the Stratospheric Observatory for Infrared Wavelegths (SOFIA). Herschel's HIFI instrument overlaps with APEX's frequency range but also covers the large parts of the spectrum unaccessible to APEX because of atmospheric absorption. Herschel, like SOFIA, reaches to higher frequencies into the infrared range. The MPIfR Submillimeter Technology divison also builds instrumentation for HIFI and SOFIA.
A final presentation will summarize these exciting perspectives.
15:30 General Discussion
For further information please contact:
Susanne Milde
Milde Marketing Science Communications
Tel.: 0049 331 721 53 71
Fax: 0049 331 721 53 80
www.milde-marketing.de
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