Institut für Astronomie und Astrophysik
Abteilung AstronomieSand 1, D-72076 Tübingen, Germany
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K. Giedke (1), J. Wilms (1), G.Lamer (2), H. Brunner (2), R. Staubert (1), and G. Hasinger (3)
(1) Institut für Astronomie und Astrophysik, Astronomie, Universität
Tübingen, Sand 1, D-72076 Tübingen, Germany
(2) AIP, An der Sternwarte 16, 14482 Potsdam, Germany
(3) MPE, Postfach 1312, 85741 Garching, Germany
in: New Visions of the X-ray Universe in the XMM-Newton and Chandra Era, eds. F. Jansen & TBD, ESA SP-488, 2002
The Marano Field is an area in the southern sky which was extensively surveyed in different wavelengths. In the optical, multicolor imaging, slitless and slit spectroscopy, and variability studies were performed. In the X-rays the field was observed with ROSAT for a total of ~60 ksec integration time, and in the radio band the region was surveyed with the ATCA at 1.4 and 2.4 GHz. Including the recently performed ISO observation and our new XMM-Newton deep pointing, it is one of the best studied regions of the sky at all wavelengths. We present first results of a deep (~100 ksec) XMM-Newton observation of the Marano Field which shows a great number of formerly unknown X-ray sources.
Key words: Missions: XMM-Newton - objects: Marano Field - galaxies: active - X-rays: galaxies - surveys
Paper (628k gzip'ed Postscript including figures)
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Last modified 14 Nov 2002