activity
19972007
most citedThe Chandra Deep Field South: Optical Spectroscopy I

591 citations · 2k across the 26 of their papers we have counts for

collaborators

26 papers

astro-ph2007★ 2 cited

The XMM-SSC survey of hard-spectrum XMM-Newton sources 1: optically bright sources

M. J. Page, I. Lehmann, Th. Boller +15

We present optical and X-ray data for a sample of serendipitous XMM-Newton sources that are selected to have 0.5-2 keV vs 2-4.5 keV X-ray hardness ratios which are harder than the…

astro-ph2006★ 175 cited

The XMM-Newton wide-field survey in the COSMOS field: III. optical identification and multiwavelength properties of a large sample of X-ray selected sources

M. Brusa, G. Zamorani, A. Comastri +31

[ABRIGED] We present the optical identification of a sample of 695 X-ray sources detected in the first 1.3 deg^2 of the XMM-COSMOS survey, down to a 0.5-2 keV (2-10 keV) limiting f…

astro-ph2006★ 353 cited

The XMM-Newton wide-field survey in the COSMOS field: I. Survey description

G. Hasinger, N. Cappelluti, H. Brunner +21

We present the first set of XMM-Newton EPIC observations in the 2 square degree COSMOS field. The strength of the COSMOS project is the unprecedented combination of a large solid a…

astro-ph2006★ 91 cited

Mid-infrared Spitzer spectra of X-ray selected Type 2 QSOs: QSO2s are not ULIRGs

E. Sturm, G. Hasinger, I. Lehmann +5

We have performed a spectroscopic study of 7 Type 2 QSOs using the mid-infrared spectrometer IRS on board the Spitzer Space Telescope. These are (to our knowledge) the first mid-IR…

astro-ph2005★ 45 cited

XMM-Newton observations of bright ROSAT selected active galactic nuclei with low intrinsic absorption

L. C. Gallo, I. Lehmann, W. Pietsch +4

We present a sample of twenty-one ROSAT bright active galactic nuclei (AGN), representing a range of spectral classes, and selected for follow-up snap-shot observations with XMM-Ne…

astro-ph2005★ 6 cited

Chandra Observations of Six QSOs at z 3

Takamitsu Miyaji, Guenther Hasinger, Ingo Lehmann +1

We report the results of our Chandra observations of six QSOs at from the Palomer Transit Grism Survey. Our primary goal is to investigate the possible systematic change…