heic0112 — Science Release
Greater accuracy deepens understanding - Hubble's Faint Object Spectrograph re-calibrated
11 September 2001
The dedicated team effort to understand and correct systematic effects in observations from Hubble's Faint Object Spectrograph has now been concluded. In future astronomers who use the observations from this instrument will be able to measure the exact velocity of interstellar clouds, as well as the motions of individual parts of nebulae and galaxies. This will for instance lead to better determinations of black hole masses.
The Faint Object Spectrograph (FOS) has been one of the key instruments during the early life of the NASA/ESA Hubble Space Telescope. It was designed to reveal the chemical composition of both faint and remote targets, as well as to help unravel the mystery of black holes at the centres of galaxies by measuring the unusually large motions of gas and stars.
The observations collected by the Faint Object Spectrograph during its six-year lifetime from August 1990 to December 1996 have been carefully stored in the Hubble Science Archive - one of the finest and most valuable astronomical archives in existence. For example, many of the spectra taken by FOS have shown extraordinarily high mass black holes at the centres of nearby galaxies - a fact of great significance in the understanding of the formation and evolution of galaxies. The Hubble Science Archive has been one of the driving forces behind the increasing awareness in the astronomical community of the need for careful archiving of high-quality astronomical observations and calibrations.
The `blue part' of the FOS data have now been revived with a new calibration, adding substantially to their scientific value. A four-person team based at the Space Telescope-European Coordinating Facility (ST-ECF) in Garching, Germany, has carried out this `re- calibration' with support from scientists at the Space Telescope Science Institute and the Goddard Space Flight Center. ST-ECF's 'Instrument Physical Modelling Group' has expended ten man-years of effort in understanding the intricate details of the instrument and in developing a novel physical model of its operation. This has allowed them to develop routines to correct for unwanted instrumental and environmental effects in the measurements of stars and galaxies. Group leader Michael Rosa explains: 'We have shown that our concept of looking at the detailed physics of a scientific instrument first and then developing new methods for the calibration is a sound one. By using a physical model we have been able to remove complex effects that distorted valuable observations.' He adds: 'Only a full overview of the complete archive enables one to gain such detailed insight. That is why it was impossible to develop the physical model and improved calibration during the operational part of FOS' life.'
The group has clarified the exact way in which the instrument operated and has modified the calibration of the data so as to include the effects of the influence of the Earth's magnetic field and of temperature changes. The accuracy with which velocities can now be derived from the new calibration-enhanced Faint Object Spectrograph data has been increased five-fold.
Experienced FOS user Tim de Zeeuw explains the importance of the recent re-calibration for the scientific value of the FOS archive data: 'Using this new repository of enhanced observations will seem like receiving data from an entirely new instrument. The re-calibrated data can answer questions about the exact velocity of interstellar clouds, as well as about the motions of building blocks of nebulae and galaxies.'
During the Second Hubble Servicing Mission the Faint Object Spectrograph was replaced by the more powerful Space Telescope Imaging Spectrograph (STIS) and was brought back to Earth. It is now on permanent display at the Smithsonian National Air & Space Museum in Washington DC, USA.
The final products of the exacting re-calibration effort will be released on 11 September 2001. The success of the FOS project has confirmed that this approach has enormous potential for dealing with the much larger data sets typical of the newer Hubble instruments. The team has already begun the next task - the re-calibration of data from the Space Telescope Imaging Spectrograph - an increase of a factor of ten in data set size and complexity.
Credit: ESA & the Space Telescope-European Coordinating Facility (ST- ECF)
LinksThe Instrument Physical Modelling Group Web pages
The FOS Web pages
Space Telescope-European Coordinating Facility (ST-ECF)
The Hubble Science Archive
Space Telescope Science Institute
Lars Lindberg Christensen
Hubble European Space Agency Information Centre, Garching, Germany
Cellular (24 hr): +49-(0)173-38-72-621
Dr. Michael Rosa
Space Telescope-European Coordinating Facility (ST-ECF), Garching, Germany