Thermo-camera sees first light
The world's largest bolometer camera will study star formation and how galaxies emerged from the Big Bang.
August 10, 2007
Provided by ESO, Garching, Germany
The Large Bolometer Camera (LABOCA) is installed on the APEX telescope at the 5,100-meter-high Chajnantor site in Chile. LABOCA is a thermometer camera with 295 detectors and an 11.4-arcminute field of view.
Photo by ESO
|August 10, 2007|
The world's largest bolometer camera for submillimeter astronomy is now in service at the 12-meter Atacama Pathrinder Experiment (APEX) telescope, located on the 5,100-meter-high Chajnantor plateau in the Chilean Andes. The Large Bolometer Camera (LABOCA) was specifically designed for the study of extremely cold astronomical objects. With its large field of view and very high sensitivity, LABOCA will expand our knowledge of how stars form and how the first galaxies emerged from the Big Bang.
"A large fraction of all the gas in the universe has extremely cold temperatures of around minus 250° Celsius, a mere 20° above absolute zero," says Karl Menten, director at the Max Planck Institute for Radio Astronomy (MPIfR) in Bonn, Germany. "Studying these cold clouds requires looking at the light they radiate in the submillimetre range, with very sophisticated detectors."
Astronomers use bolometers for this task, which are essentially thermometers. They detect incoming radiation by registering the resulting rise in temperature. More specifically, a bolometer detector consists of an extremely thin foil that absorbs the incoming light. Any change of the radiation's intensity results in a slight change in temperature of the foil, which can then be registered by sensitive electronic thermometers. To be able to measure such minute temperature fluctuations requires the bolometers to be cooled down to less than 0.3° above absolute zero (–272.85° Celsius).
"Cooling to such low temperatures requires using liquid helium, which is no simple feat for an observatory located at 5,100-meter altitude," says Carlos De Breuck, the APEX instrument scientist at ESO.
Nor is it simple to measure the weak temperature radiation of astronomical objects. Millimeter and submillimeter radiation opens a window into the enigmatic, cold universe, but the signals from space are heavily absorbed by water vapor in Earth's atmosphere. "It is a bit as if you were trying to see stars during the day," explains Axel Weiss of the MPIfR and leader of the team that installed LABOCA on APEX.
This is why telescopes for this kind of astronomy must be built on high, dry sites, and why the 5,100-meter-high plateau at Chajnantor in the extremely dry Atacama Desert was chosen. Even under such optimal conditions, the heat from Earth's atmosphere is still a hundred thousand times more intense than the tiny astronomical signals from distant galaxies. Very special software is required to filter such weak signals from the overwhelming disturbances.
LABOCA and its associated software were developed by MPIfR. "Since so far there are no commercial applications for such instruments we have to develop them ourselves," explains Ernst Kreysa, head of the group that built the new instrument.
A bolometer camera combines many tiny bolometer units into a matrix, much like how pixels are combined in a digital camera. LABOCA observes at the wavelength of 0.87 millimeters, and consists of 295 channels arranged in 9 concentric hexagons around a central channel. The angular resolution is 18.6 arcseconds, and the total field of view is 11.4 arcmin, a remarkable size for instruments of this kind.
"The first astronomical observations with LABOCA have revealed its great potential. In particular, the large number of LABOCA's detectors is an enormous improvement over earlier instruments," says Giorgio Siringo, from MPIfR and member of the LABOCA team. "LABOCA is the first camera that will allow us to map large areas on the sky with high sensitivity."
APEX where LABOCA is installed is a new-technology, 12-meter telescope, based on an ALMA prototype antenna, and operating at the ALMA site. It has modified optics and an improved antenna surface accuracy, and is designed to take advantage of the excellent sky transparency working with wavelengths in the 0.2 to 1.4 mm range.
"APEX is located a mere 2 kilometers from the center of the future ALMA array. The new LABOCA camera will be very complementary to ALMA, as its very wide view will find thousands of galaxies which will be observed in great detail with ALMA," says De Breuck.