/ftp/cats/aliases/K/./KLS2007



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J/A+A/466/41        XMM-Newton survey in the Marano Field. I.    (Krumpe+, 2007)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	xray.dat opt.dat tabled1.dat notes.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/A+A/466/41
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drwxr-xr-x 29 cats archive 4096 Jul 17 2012 [Up] drwxr-xr-x 2 cats archive 4096 Jan 13 2023 [TAR file] -rw-r--r-- 1 cats archive 498 Dec 19 2022 .message -r--r--r-- 1 cats archive 14929 Aug 29 2008 ReadMe -rw-r--r-- 1 cats archive 1012 Aug 29 2008 +footg5.gif -rw-r--r-- 1 cats archive 2951 Aug 29 2008 +footg8.gif -r--r--r-- 1 cats archive 10005 Oct 18 2007 notes.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 22509 Nov 23 2007 opt.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 3180 Aug 29 2008 tabled1.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 34739 Jan 9 2008 xray.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+A/466/41 XMM-Newton survey in the Marano Field. I. (Krumpe+, 2007) ================================================================================ The XMM-Newton survey in the Marano Field. I. The X-ray data and optical follow-up. Krumpe M., Lamer G., Schwope A.D., Wagner S., Zamorani G., Mignoli M., Staubert R., Wisotzki L., Hasinger G <Astron. Astrophys. 466, 41 (2007)> =2007A&A...466...41K ================================================================================ ADC_Keywords: Surveys - X-ray sources ; Galaxies, photometry Keywords: surveys - X-rays: galaxies - galaxies: active - galaxies: quasars: general Abstract: We report on a medium deep XMM-Newton survey of the Marano Field and optical follow-up observations. The mosaicked XMM-Newton pointings in this optical quasar survey field cover 0.6 deg2 with a total of 120ks good observation time. We detected 328 X-ray sources in total. The turnover flux of our sample is f_X_ 5x10^-15^erg/cm2/s in the 0.2-10keV band. With VLT FORS1 and FORS2 spectroscopy we classified 96 new X-ray counterparts. The central 0.28deg^2^, where detailed optical follow-up observations were performed, contain 170 X-ray sources (detection likelihood ML>10), out of which 48 had already been detected by ROSAT. In this region we recover 23 out of 29 optically selected quasars. With a total of 110 classifications in our core sample we reach a completeness of  65%. About one-third of the XMM-Newton sources are classified as type II AGN with redshifts mostly below 1.0. Furthermore, we detect five high redshift type II AGN (2.2<=z<=2.8). Description: Optical and X-ray properties of spectroscopically investigated candidate counterparts of Marano XMM-Newton X-ray sources.