Mathematics – Logic
Scientific paper
Jun 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..pres...85.&link_type=abstract
XMM Press Release SNR 9-2004
Mathematics
Logic
Scientific paper
Composite image hi-res
Size hi-res: 851 KB Credits: ESA/Univ. of Leicester/I. Stewart and M. Watson
XMM-Newton X-ray spectral colour composite image XMM-Newton X-ray spectral colour composite image of the Subaru/XMM-Newton Deep Field. The view gives an X-ray pseudo-colour representation of all the sources, coded according to their X-ray energy. More energetic sources are shown in blue and less energetic ones in red. This mosaic image, composed of 7 partially overlapping pointings, maps the full extent of the SXDF and corresponds to an exposure time exceeding one hundred hours. These data form the largest contiguous area over which deep X-ray observations have been performed.
Composite image hi-res
Size hi-res: 6215 KB Credits: NAOJ/Subaru Telescope
XMM-Newton/Subaru colour composite image A colour composite image obtained by combining data taken with the Subaru Telescope in blue, red and near-infrared light. The image, worth over two hundred hours of exposure time, covers an area of sky seven times larger than the full moon. The images in blue light show details several hundred million times fainter than what can be seen with the naked eye.
SXDS field hi-res
Size hi-res: 448 KB Credits: NAOJ/Subaru Telescope
SXDS field A particular of the SXDS field. The teardrop-shaped galaxy in the upper right portion of the frame is likely to have suffered from a collision with another galaxy.
SXDS field hi-res
Size hi-res: 358 KB Credits: NAOJ/Subaru Telescope
SXDS field A particular of the SXDS field. The prominent spiral galaxy near the centre may be ineracting with a less-conspicuous dwarf galaxy to its lower right.
One of the fundamental goals of modern astronomy is understanding the history of the Universe, and in particular learning about the processes that shape the formation and evolution of galaxies. To observe these processes as they unfold, astronomers must survey galaxies near and far, spanning a large enough volume of the Universe, so that local variations in the physical properties and distribution of galaxies do not skew the results.
About four years ago, ESA's XMM-Newton observatory and NAOJ's Subaru Telescope began a deep survey of a region of sky located in the southern constellation Cetus (the 'Whale'), now known as the Subaru/XMM-Newton Deep Survey (SXDS) field. The SXDS covers a roughly square patch in the sky, measuring about 1.3 degree on a side, or about seven times the area of the full moon and nearly 1000 times larger than the area of the famous Hubble Deep Field.
Both observatories have devoted a considerable amount of time to the SXDS. The XMM-Newton observations represent the deepest and most sensitive wide-area X-ray survey ever carried out by XMM-Newton, totalling over one hundred hours of exposure time. The Subaru Telescope has stared at this field for over two hundred hours, in four different colours, revealing details which are hundred million times fainter than what can be seen with the naked eye.
Over a thousand X-ray sources are found in the XMM-Newton images. Some of them are nearby stars with very active coronas that radiate in the X-ray domain, but the largest majority are far-flung active galaxies hiding powerful black holes in their nuclei. Other sources include distant clusters of galaxies, located up to eight thousand million light years away. Since X-rays travel in space at a finite speed, XMM-Newton gives us a view of these galaxies when they were much younger and less evolved than now. By comparing these images with those of nearby galaxies, astronomers can infer how they have evolved in the course of the last several thousand million years, or about three quarters of the life of the Universe.
The true virtue of the SXDS is that it allows for a seamless comparison and combination of the XMM-Newton images, which provide an X-ray view of the most energetic phenomena in the Universe, with the Subaru data, offering a picture in visible light of where stars form in galaxies. The combined SXDS images reveal over a million galaxies, of all types and sizes and in a range of environments, covering various phases of their evolution. "The SXDS multi-wavelength survey, with its unprecedented width and depth, is already bringing new insights into the structure of the Universe at earlier times," said Prof Mike Watson, head of the XMM-Newton Survey Science Centre, at the University of Leicester, United Kingdom, and one of the scientists involved in the SXDS.
The broad wavelength range spanned by the SXDS data also allows scientists to estimate distances to most galaxies in the field, providing in practice a three-dimensional map of this part of the Universe. With this information at hand, astronomers can study the history of the Universe in much more detail. For example, they can determine very accurately where and when stars formed in galaxies and whether larger galaxies formed before or after smaller objects. They can also measure how many galaxies formed together in the same cluster and which was originally their shape.
Some of the preliminary discoveries already made with these data will be presented and discussed at a scientific workshop taking place later this week in Kyoto, Japan. The SXDS team, however, believe that the only way to fully exploit the scientific potential of the data is to release them and make them available to researchers worldwide.
From today, professional astronomers, students and even amateur astronomers will be able to test their observational or theoretical results against the SXDS data. "With a large and comprehensive data set like this, there are innumerable research possibilities," said Dr Kazuhiro Sekiguchi from the NAOJ Subaru Telescope, Hawaii, USA, and the coordinator of the Japanese SXDS team. "Other researchers can look at our data with a new perspective and begin answering questions that we may have overlooked, or do not have the time or human resources to address," he added.
Besides the XMM-Newton and Subaru Telescope images, the SXDS archive already includes radio maps that further extend the range of wavelengths covered by the survey and provide information on the powerful quasars, the centres of distant galaxies which are releasing large amounts of energy.
Although the SXDS data are already a treasure trove of information, their scientific value will multiply when planned observations at wavelengths that complement the existing data are concluded. These include ultraviolet, infrared and sub-millimetre images as well as optical spectra from a wide range of international facilities. In five years, when the survey is scheduled to be complete, the SXDS should allow astronomers to place strong constraints on the cosmological models that determine the ultimate fate of the Universe, providing insights into both its past and future.
Note to Editors
The coordinated release issued by the National Astronomical Observatory of Japan can be found at the following address:
http://soaps.naoj.org
More on the Subaru/XMM-Newton Deep Survey
The SXDS is a project of international collaboration involving astronomers from the National Astronomical Observatory of Japan, Tokyo, Japan, the University of Tokyo, Japan, the Institute of Space and Astronautical Science, Sagamihara, Japan, the University of Durham, United Kingdom, and Tohoku University, Sendai, Japan, working in close collaboration with the XMM-Newton Survey Science Centre led by the University of Leicester, United Kingdom.
For more information about the SXDS project and the data please visit:
http://www.naoj.org/Science/SubaruProject/SDS
Direct public access to the XMM-Newton data is also possible at:
http://xmm.vilspa.esa.es/external/xmm_data_acc/xsa/index.shtml
More about XMM-Newton
XMM-Newton can detect more X-ray sources than any previous satellite and is helping to solve many cosmic mysteries of the violent Universe, from black holes to the formation of galaxies. It was launched on 10 December 1999, using an Ariane-5 rocket from French Guiana. It is expected to return data for a decade. XMM-Newton's high-tech design uses over 170 wafer-thin cylindrical
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