[PDF] Top 20 The Evolution of Lyα emitting Galaxies between z = 2 1 and z = 3 1

... depth, the Gu10 data set is well suited for a comparative ...used the Chandra and GALEX source lists to eliminate some high-EW interlopers from their sample: as with our z ∼ ...true z ∼ ... See full document

... (2002), the X-ray spectrum of SF galaxies that do not have an AGN is dominated by HMXBs, which are best described by Γ = ...1.2 and a cutoff energy of 20 keV. Many SF galaxies ... See full document

... to the submm-detected quasars identified by Page et al. (2001, 2004) and Stevens et ...in the evolution of SMGs ...from the black hole have started to remove gas and dust ... See full document

... timespan between z = 1.6 and z ∼ 1.3 is only ∼1 Gyr, indicating possibly rapid evolution in environmental quenching efficiency in this redshift ...point the intracluster ... See full document

... where the lower mass central sub-halo descends into a satellite belonging to the descendant of the more massive central ...track the descendants until the two sub-halos merge, ... See full document

... to the strongest low- ionization lines that we detect at high significance: Si ii λ1260, O i λ1302 + Si ii λ1304, C ii λ1334, Si ii ...All of these features have been well studied in high-redshift LBGs ... See full document

... cluster evolution is intertwined with that of its constituent ...understand the former, we must explore the baryonic processes that shape the ...understanding of the ... See full document

... Given the much higher density of sources detected at optical wavelengths in COSMOS (Capak et ...cross-correlation between the 24 μm- selected catalogue and the optical ... See full document

... 243 z ≈ 3 quasars in nine Very Large Telescope (VLT) Visible Imaging and Multi-Object Spectrograph (VIMOS) Lyman-break galaxy (LBG) redshift survey areas, each of which is centred on a known ... See full document

... to the excellent sensitivity of Herschel PACS to rest frame far-infrared emission in the hosts of z = ...break the redshift / luminosity degen- eracy that affected previous ... See full document

... number of different lines of evidence suggest that a close relationship exists between the growth of supermassive black holes (SMBHs) and their host ...established and ... See full document

... ratio of the [4550–4650] ˚ A to the [4150–4250] ˚ A fluxes. The resulting values are given in Table ...increase of 16% in the G-step index between z = 0.65 ... See full document

... in the local universe between the presence of a cool core and radio emission from the BCG (Sun 2009), which may conspire to fill in the SZ signal for the strongest ... See full document

... (2008) and Bielby et al. (2011, here- after Paper I), both of whom showed that the clustering evolution of the LBG population may be more complicated, but is likely to produce ... See full document

... 1998) and the small volume available for z 0 ...case, the exclusion of GALEX-detected sources should rule out this ...capable of triggering a narrow- band excess through their ... See full document

... spectroscopy of 92 LAE candidates, along with other MUSYC targets, was performed with Magellan- Baade+IMACS on ...Nov. 2-3, 2005, ...2006 and Feb. 18-20, 2007. The 300 line/mm grism was ... See full document

... wavelengths of ∼ 1500 ˚ A and 2000 ˚ A at z = 3.1 and z = ...in the apparent sizes of LAEs between these two parts of the ...compared the sizes ... See full document

... on the measurement and the sample variance. The former was determined by the quality of the observations and the instrumentation, while the latter ... See full document

... on the X-ray cluster RXJ0054.0–2823 at z = 0.29 . We study the spectral evolution of galaxies from z = 1 down to the cluster redshift in a magnitude-limited ... See full document

... advantage of features in the spectral energy distribution (SED) to identify sets of galaxies at a particular redshift ...use the Lyman Break in the SED at z ∼ 4 and ... See full document