[PDF] Top 20 The high redshift (z > 3) active galactic nucleus population in the 4 Ms Chandra Deep Field South

... providing the LADE model data, ...for the helpful suggestions which improved this ...from the agreement ASI-INAF I/009/10/0 and the ...thanks the Youth 1000 Plan (QingNianQianRen) ... See full document

... X-ray active galactic nucleus (AGN) hosts and non-AGN galaxies through the galaxy formation epoch (z ≈ 1–4) in the Chandra Deep Field-North and ... See full document

... with Chandra and XMM-Newton have resolved the vast majority of the ...into the X-ray point sources de- tected (see, ...characterize the extra- galactic X-ray source ... See full document

... to the above methods, which utilize observa- tional data directly and determine the selection criteria em- pirically, Daddi et ...including the component corresponding to the transmitted UV ... See full document

... present the first results of our optical spectroscopy program aimed to provide redshifts and identifications for the X-ray sources in the Extended Chandra Deep Field ... See full document

... of the rich multiwavelength data available in the Chandra Deep Field South (CDF-S), including the 4 Ms Chandra observations (the deepest ... See full document

... to the XRB in the 14–195 keV Swift/BAT band as a function of redshift, from the population synthesis model presented here (solid line; see the text for ...by the ... See full document

... a high-redshift com- parison to previous measurements of the XLF at hard ( 10 keV ) X-ray energies, which have been restricted to the local ( z  ...universe. In Figure 6 we ... See full document

... and high-quality photometric redshifts for the 462 X-ray sources in the ≈2 Ms Chandra Deep Field-South (CDF-S) ...using deep optical-to-radio ... See full document

... 5 in at least one of three X-ray bands ...(i.e., the probability of sources not being real is less than ...maximize the number of reliable sources ...to the previous 2 Ms CDF-S ... See full document

... that the remnants of massive Population III (Pop III) stars constitute BH progenitors (Haiman & Loeb 2001; Madau & Rees 2001; Bromm, Coppi & Larson 2002; Alvarez, Wise & Abel 2009; Johnson ... See full document

... spectroscopic redshift measurements, col- lected from Le F`evre et ...of the 419 spectroscopic redshift measure- ments are “secure,” in that they are measured at 95% confi- dence levels with ... See full document

... at High Redshifts, z > 3. As mentioned in Section 3, most measurements of black hole accretion at high redshift, z > 3, come from optical observations ... See full document

... If the X-ray emission from the stacked LBGs are dominated by star-forming processes and the X-ray–SFR correlation at z ≈ ...at z ≈ 3, then we find X-ray–derived SFRs of 341 M yr ... See full document

... 13. The average observed infrared SEDs of the AGNs in the Chandra Deep Fields and the local BAT/IRAS sample ...sample in terms of X-ray luminosity (left- and ... See full document

... For the computation of the space density in the 2 – 10 keV band, we applied the fl ux cuts described in Section ...avoid the Eddington bias at faint fl uxes. The fl ... See full document

... of the three standard-band images by first masking out point sources from our main catalogue using circular apertures with radii of ...times the ≈ 99.9 per cent PSF encircled-energy fraction radii as ... See full document

... assistance in the planning and scheduling of the extensive COSMOS observa- ...acknowledge the contributions of the entire COSMOS collaboration consisting of more than 70 ...on ... See full document

... and the referee, Andy Lawrence, for his insightful comments and ...and MS acknowledge financial support from the DFG cluster of excellence ‘Origin and structure of the universe’ ...by ... See full document

... determine the relative black- hole–galaxy growth of SMGs and explore their evolutionary ...status. The X-ray-obscured SMGs already have host-galaxy mass constraints ...of the SMG population. ... See full document