Onsala Space Observatory

Onsala Space Observatory

Logo of the Onsala Space Observatory
Organization Chalmers University of Technology
Location Onsala, Kungsbacka, Sweden
Coordinates 57°23′35″N 11°55′04″E / 57.39306°N 11.91778°E / 57.39306; 11.91778Coordinates: 57°23′35″N 11°55′04″E / 57.39306°N 11.91778°E / 57.39306; 11.91778
Altitude 20 m
Established 1949
Website www.chalmers.se/oso
Telescopes
20 metre single-dish movable
25 metre single-dish movable
LOFAR station interferometer
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Onsala Space Observatory (OSO), the Swedish National Facility for Radio Astronomy, provides scientists with equipment to study the Earth and the rest of the Universe. The observatory operates two radio telescopes in Onsala, 45 km south of Gothenburg, and takes part in several international projects. Examples of activities:

Onsala Space Observatory was founded in 1949 by professor Olof Rydbeck. The observatory is hosted by Department of Earth and Space Science at Chalmers University of Technology, and is operated on behalf of the Swedish Research Council.

25-metre telescope

The 25-metre telescope

The 25.6 m diameter, polar mount decimeter-wave telescope in Onsala is equipped with receivers for frequencies up to 7 GHz. It is used for astronomical VLBI observations. It is also operated as a single dish for studies of molecular clouds in the Galaxy. The telescope was built in 1963.

20-metre telescope

The 20-metre telescope enclosed in its radome
20m telescope inside the radome

The 20 m diameter millimetre wave telescope in Onsala is equipped with receivers for frequencies up to 116 GHz. It is used for observations of millimetre wave emission from molecules in comets, circumstellar envelopes, and the interstellar medium in the Galaxy and in extragalactic objects. The telescope is enclosed in a radome of diameter 30 m.[1]

It is also used for astronomical VLBI observations of star forming regions, radio stars, and active galactic nuclei, and for geodetic VLBI observations to study e.g. crustal dynamics and polar motion. The telescope was built in 1975-76 and upgraded in 1992.

It is also used, as part of the European and worldwide networks, for astronomical Very Long Baseline Interferometry (VLBI) observations of star forming regions, radio stars, and active galactic nuclei, and for geodetic VLBI observations to study e.g. crustal dynamics and polar motion.

Receivers

The telescope is equipped with the following receivers:

Frequency range Receiver temperature Receiver type Polarization
2.2–2.4 GHz 60 K HEMT amplifier Single
8.2–8.4 GHz 80 K HEMT amplifier Dual
18.0–26.0 GHz 30 K HEMT amplifier Dual
26.0–36.0 GHz 50 K HEMT amplifier Single
36.0–49.8 GHz 50 K HEMT amplifier Dual
85–116 GHz 80–130 K SIS mixer Single

LOFAR station

The LOFAR station at Onsala Space Observatory

The Swedish station in the international radio telescope LOFAR is located at Onsala Space Observatory. It was completed in 2011.[2]

Nordic ALMA node

The Onsala Space Observatory currently hosts the Nordic ALMA node, which is part of the European ALMA regional centre (ARC). The Nordic ALMA node provides face-to-face support for any astronomer than wants to use the ALMA telescope and primarily supports the Nordic scientific community.[3]

References

  1. ↑ Rydbeck, O.E.H.; Ronnang, B; Hansson, B.; Ellder, J.; Hjalmarson, A; Kollberg, E.; d'Amato, Richard (1977). "The Onsala 20 M Millimeter Wave Radio Telescope". Proc. 7th European Microwave Conference. doi:10.1109/EUMA.1977.332461.
  2. ↑ "Education minister to open Onsala's LOFAR station (Chalmers press release), 30 June 2011". LOFAR Sweden consortium.
  3. ↑ "Nordic ARC node".
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