ann14065 — Announcement

ALMA Achieves New Short Wavelength Observing Capabilities

10 September 2014

The Atacama Large Millimeter/submillimeter Array (ALMA) has reached a major milestone by extending its vision fully into the realm of the submillimetre, the wavelengths of cosmic light that hold intriguing information about the cold, dark, and distant Universe.

This achievement opens an entirely new window on the Universe for ALMA beyond its existing capabilities with the Band 9 receivers. It also is a critical step in the telescope's commissioning process, which brings its full capabilities to bear and makes them available to the international astronomical community.

As a demonstration of its new capabilities, the commissioning team released a new image of planet Uranus as it appears in submillimetre wavelength light. The image — obtained with ALMA's shortest wavelength, Band 10 receivers — reveals the icy glow from the planet's atmosphere, which can reach temperatures as low as -224 C (giving Uranus the coldest atmosphere in the Solar System). ALMA's now broader range of capabilities will enable astronomers and planetary scientists to study and monitor temperature changes at different altitudes above the clouds of Uranus and other giant planets in our Solar System.

ALMA Astronomer Satoko Takahashi of the National Astronomical Observatory of Japan who leads this effort said: "Before astronomers could take advantage of the shorter wavelengths, we first had to take the telescope through its paces and establish observing strategies that yield the best, most accurate results. That’s why commissioning is so critical to our success."

ALMA observes the cosmos by using a series of precisely tuned receivers that are installed on each of the array's 66 antennas. Each receiver type is sensitive to a particular "band," or range of wavelengths of the electromagnetic spectrum. The shortest wavelength Band 10 receivers have already been installed and tested on a majority of the ALMA antennas and the remainder will be installed and integrated over the next several months.

To take full advantage of ALMA's new short-wavelength capabilities, the commissioning team is in the process of refining two new observing techniques which will greatly expand the amount of time ALMA can effectively study the Universe at shorter wavelengths.

The first, "band to band transfer," enables ALMA to observe at short wavelengths in less than optimal weather conditions by first observing an object at longer wavelengths, and then using that data to calibrate, or "tune," the telescope for a particular observation.

Another technique involves first observing at very broadband wavelengths and then tuning-in to more narrowband, shorter wavelengths. This technique will soon be routine operating procedure, even though it is unique to ALMA at these wavelengths. Combined, these two techniques open up many more hours of observations at shorter wavelengths than would otherwise be possible.

Teams from around the world are still on their way to ALMA to further verify these techniques and provide the optimal observing strategy for observing with ALMA at short wavelength.

More Information

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. ALMA is funded in Europe by the European Southern Observatory (ESO), in North America by the U.S. National Science Foundation (NSF) in cooperation with the National Research Council of Canada (NRC) and the National Science Council of Taiwan (NSC) and in East Asia by the National Institutes of Natural Sciences (NINS) of Japan in cooperation with the Academia Sinica (AS) in Taiwan.

The international commissioning team for the High Frequency Observing Campaign was led by Satoko Takasashi of the National Astronomical Observatory of Japan, ALMA’s representative East Asia and Anthony Remijan of the National Radio Astronomy Observatory and the ALMA Program Scientist for Extension and Optimization of Capabilities. Other members include Catherine Vlahakis, Neil Philips, Denis Barkats, Bill Dent (JAO/ESO), Ed Fomalont, Brian Mason, Jennifer Donovan Meyer (NRAO); Violette Impellizzeri, Paulo Cortes, Christian Lopez (JAO/NRAO); Christine Wilson (NRAO/McMaster University); Seiji Kameno, Tsyuoshi Sawada (JAO/NAOJ); Tim Van Kempen, Luke Maud & Remo Tilanus (Leiden); Robert Lucas (Grenoble); Richard Hills (Cambridge); Akihiko Hirota (JAO/NAOJ); James Chibueze (NAOJ).

Contacts

Lars Lindberg Christensen
Head of ESO ePOD
Garching bei München, Germany
Tel: +49 89 3200 6761
Cell: +49 173 3872 621
Email: lars@eso.org

Charles E. Blue
Public Information Officer
National Radio Astronomy Observatory
Tel: +1 434 296 0314
Cell: +1 202 236 6324
Email: cblue@nrao.edu

Masaaki Hiramatsu
National Astronomical Observatory of Japan
Japan
Tel: +81 422 34 3630
Email: hiramatsu.masaaki@nao.ac.jp

About the Announcement

Id:ann14065

Images

Band 10 receiver cartridge
Band 10 receiver cartridge
ALMA short wavelength image of Uranus
ALMA short wavelength image of Uranus