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Photoionization modeling and the K lines of iron
We calculate the efficiency of iron K line emission and iron K absorption in photoionized models using a new set of atomic data. These data are more comprehensive than those previously applied to theExpand
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The Herschel Multi-tiered Extragalactic Survey: HerMES
TLDR
The Herschel Multi-tiered Extragalactic Survey (HerMES) is a legacy programme designed to map a set of nested fields totalling ∼380 deg^2. Expand
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Emission-line diagnostics of low-metallicity active galactic nuclei
Current emission-line-based estimates of the metallicity of active galactic nuclei (AGN) at both high and low redshifts indicate that AGN have predominantly solar-to-supersolar metallicities. ThisExpand
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Radio faint AGN: a tale of two populations
We study the Extended Chandra Deep Field South (E-CDFS) Very Large Array sample, which reaches a flux density limit at 1.4 GHz of 32.5 microJy at the field centre and redshift ~ 4, and covers ~ 0.3Expand
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DYNAMICS OF LINE-DRIVEN DISK WINDS IN ACTIVE GALACTIC NUCLEI. II. EFFECTS OF DISK RADIATION
We explore consequences of a radiation-driven disk wind model for mass outflows from active galactic nuclei (AGNs). We performed axisymmetric time-dependent hydrodynamic calculations using the sameExpand
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UWISH2 – the UKIRT Widefield Infrared Survey for H2
The definitive version can be found at : http://onlinelibrary.wiley.com/ Copyright Wiley-Blackwell
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An XMM-Newton Observation of the Luminous Seyfert 1 Galaxy Markarian 509
We present the spectral analysis of an early XMM-Newton observation of the luminous Seyfert 1 galaxy Mrk 509. We find the hard (2-10 keV) continuum slope, including reflection, to be somewhat flatterExpand
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Measurements of cosmic-ray secondary nuclei at high energies with the first flight of the CREAM balloon-borne experiment
Abstract We present new measurements of heavy cosmic-ray nuclei at high energies performed during the first flight of the balloon-borne cosmic-ray experiment Cosmic-Ray Energetics and Mass (CREAM).Expand
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Do the Spectra of Soft X-Ray Transients Reveal Bulk-Motion Inflow Phenomenon?
We present our analysis of the high-energy radiation from black hole (BH) transients using archival data obtained primarily with RXTE and a comprehensive test of the bulk-motion Comptonization (BMC)Expand
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The size-luminosity relation at z=7 in CANDELS and its implication on reionization
Context. The exploration of the relation between galaxy sizes and other physical parameters (luminosity, mass, star formation rate) has provided important clues for understanding galaxy formation,Expand
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