eso1229-en-us — Organisation Release

APEX takes part in sharpest observation ever

Telescopes in Chile, Hawaii, and Arizona reach sharpness two million times finer than human vision

18 July 2012

An international team of astronomers has observed the heart of a distant quasar with unprecedented sharpness, two million times finer than human vision. The observations, made by connecting the Atacama Pathfinder Experiment (APEX) telescope [1] to two others on different continents for the first time, is a crucial step towards the dramatic scientific goal of the “Event Horizon Telescope” project [2]: imaging the supermassive black holes at the centre of our own galaxy and others.

Astronomers connected APEX, in Chile, to the Submillimeter Array (SMA) [3] in Hawaii, USA, and the Submillimeter Telescope (SMT) [4] in Arizona, USA. They were able to make the sharpest direct observation ever [5], of the centre of a distant galaxy, the bright quasar 3C 279, which contains a supermassive black hole with a mass about one billion times that of the Sun, and is so far from Earth that its light has taken more than 5 billion years to reach us. APEX is a collaboration between the Max Planck Institute for Radio Astronomy (MPIfR), the Onsala Space Observatory (OSO) and ESO. APEX is operated by ESO.

The telescopes were linked using a technique known as Very Long Baseline Interferometry (VLBI). Larger telescopes can make sharper observations, and interferometry allows multiple telescopes to act like a single telescope as large as the separation — or “baseline” — between them. Using VLBI, the sharpest observations can be achieved by making the separation between telescopes as large as possible. For their quasar observations, the team used the three telescopes to create an interferometer with transcontinental baseline lengths of 9447 km from Chile to Hawaii, 7174 km from Chile to Arizona and 4627 km from Arizona to Hawaii. Connecting APEX in Chile to the network was crucial, as it contributed the longest baselines.

The observations were made in radio waves with a wavelength of 1.3 millimetres. This is the first time observations at a wavelength as short as this have been made using such long baselines. The observations achieved a sharpness, or angular resolution, of just 28 microarcseconds  — about 8 billionths of a degree. This represents the ability to distinguish details an amazing two million times sharper than human vision. Observations this sharp can probe scales of less than a light-year across the quasar — a remarkable achievement for a target that is billions of light-years away.

The observations represent a new milestone towards imaging supermassive black holes and the regions around them. In future it is planned to connect even more telescopes in this way to create the so-called Event Horizon Telescope. The Event Horizon Telescope will be able to image the shadow of the supermassive black hole in the centre of our Milky Way galaxy, as well as others in nearby galaxies. The shadow — a dark region seen against a brighter background — is caused by the bending of light by the black hole, and would be the first direct observational evidence for the existence of a black hole’s event horizon, the boundary from within which not even light can escape.

The experiment marks the first time that APEX has taken part in VLBI observations, and is the culmination of three years hard work at APEX’s high altitude site on the 5000-metre plateau of Chajnantor in the Chilean Andes, where the atmospheric pressure is only about half that at sea level. To make APEX ready for VLBI, scientists from Germany and Sweden installed new digital data acquisition systems, a very precise atomic clock, and pressurised data recorders capable of recording 4 gigabits per second for many hours under challenging environmental conditions [6]. The data — 4 terabytes from each telescope — were shipped to Germany on hard drives and processed at the Max Planck Institute for Radio Astronomy in Bonn.

The successful addition of APEX is also important for another reason. It shares its location and many aspects of its technology with the new Atacama Large Millimeter/submillimeter Array (ALMA) telescope [7]. ALMA is currently under construction and will finally consist of 54 dishes with the same 12-metre diameter as APEX, plus 12 smaller dishes with a diameter of 7 metres. The possibility of connecting ALMA to the network is currently being studied. With the vastly increased collecting area of ALMA’s dishes, the observations could achieve 10 times better sensitivity than these initial tests. This would put the shadow of the Milky Way's supermassive black hole within reach for future observations.

Notes

[1] APEX is a collaboration between the Max Planck Institute for Radio Astronomy (MPIfR), the Onsala Space Observatory (OSO) and ESO. Operation of APEX at Chajnantor is entrusted to ESO. APEX is a pathfinder for the next-generation submillimetre telescope, the Atacama Large Millimeter/submillimeter Array (ALMA), which is being built and operated on the same plateau.

[2] The Event Horizon Telescope project is an international collaboration, coordinated by the MIT Haystack Observatory (USA).

[3] The Submillimeter Array (SMA) on Mauna Kea, Hawaii, consisting of 8 dishes of 6 m diameter each, is operated by the Smithsonian Astrophysical Observatory (USA) and the Academia Sinica Institute of Astronomy and Astrophysics (Taiwan).

[4] The Submillimeter Telescope (SMT) of 10 m diameter on top of Mount Graham, Arizona, is operated by the Arizona Radio Observatory (ARO) in Tucson, Arizona (USA).

[5] Some indirect techniques have been used to probe finer scales, for example using microlensing (see heic1116) or interstellar scintillation, but this is a record for direct observations.

[6] These systems were developed in parallel in the USA (MIT-Haystack observatory) and in Europe (MPIfR, INAF — Istituto di Radioastronomia Noto VLBI Station, and HAT-Lab). A hydrogen maser time standard (T4Science) was installed as the very precise atomic clock. The SMT and SMA had already been equipped similarly for VLBI.

[7] The Atacama Large Millimeter/submillimeter Array (ALMA), an international astronomy facility, is a partnership of Europe, North America and East Asia in cooperation with the Republic of Chile. ESO is the European partner in ALMA.

More information

The year 2012 marks the 50th anniversary of the founding of the European Southern Observatory (ESO). ESO is the foremost intergovernmental astronomy organisation in Europe and the world’s most productive astronomical observatory. It is supported by 15 countries: Austria, Belgium, Brazil, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Spain, Sweden, Switzerland and the United Kingdom. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the world’s most advanced visible-light astronomical observatory and two survey telescopes. VISTA works in the infrared and is the world’s largest survey telescope and the VLT Survey Telescope is the largest telescope designed to exclusively survey the skies in visible light. ESO is the European partner of a revolutionary astronomical telescope ALMA, the largest astronomical project in existence. ESO is currently planning a 40-metre-class European Extremely Large optical/near-infrared Telescope, the E-ELT, which will become “the world’s biggest eye on the sky”.

Links

Contacts

Alan Roy
APEX VLBI Project Lead, Max-Planck-Institut für Radioastronomie
Bonn, Germany
Tel: +49 228 525 191
Email: aroy@mpifr-bonn.mpg.de

Thomas Krichbaum
APEX VLBI Project Scientist, Max-Planck-Institut für Radioastronomie
Bonn, Germany
Tel: +49 228 525 295
Email: tkrichbaum@mpifr-bonn.mpg.de

Shep Doeleman
MIT Haystack Observatory
Westford, USA
Tel: +1 781 981 5400 x5904
Email: dole@haystack.mit.edu

Michael Lindqvist
Onsala Space Observatory
Onsala, Sweden
Tel: +46 31 772 5508
Email: michael.lindqvist@chalmers.se

Lucy Ziurys
Director, Arizona Radio Observatory
Tucson, USA
Tel: +1 520 621-6525
Email: lziurys@as.arizona.edu

Jonathan Weintroub
Harvard-Smithsonian Center for Astrophysics
Cambridge, USA
Tel: +1 617 495 7319
Email: jweintroub@cfa.harvard.edu

Douglas Pierce-Price
APEX Public Information Officer, ESO
Garching bei München, Germany
Tel: +49 89 3200 6759
Email: dpiercep@eso.org

This is a translation of ESO Press Release eso1229.

About the Release

Release No.:eso1229-en-us
Name:3C 279
Type:• Early Universe : Galaxy : Activity : AGN : Quasar
Facility:Atacama Pathfinder Experiment

Images

Artist’s impression of the quasar 3C 279
Artist’s impression of the quasar 3C 279
Positions of the telescopes used in the 1.3 mm VLBI observations of the quasar 3C 279
Positions of the telescopes used in the 1.3 mm VLBI observations of the quasar 3C 279
The Atacama Pathfinder Experiment (APEX)
The Atacama Pathfinder Experiment (APEX)
The Submillimeter Telescope (SMT) at the Arizona Radio Observatory
The Submillimeter Telescope (SMT) at the Arizona Radio Observatory
The Submillimeter Array (SMA) on Mauna Kea, Hawaii
The Submillimeter Array (SMA) on Mauna Kea, Hawaii
Position of the quasar 3C 279 in the constellation of Virgo
Position of the quasar 3C 279 in the constellation of Virgo

Videos

Artist’s impression of the quasar 3C 279
Artist’s impression of the quasar 3C 279
Positions of the telescopes used in the 1.3 mm VLBI observations of the quasar 3C 279
Positions of the telescopes used in the 1.3 mm VLBI observations of the quasar 3C 279
Artist’s impression of the quasar 3C 279 (alternative version)
Artist’s impression of the quasar 3C 279 (alternative version)

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