[PDF] Top 20 High Redshift Galaxies As Probes Of The Epoch Of Reionization

... the Epoch of Reionization (PAPER), who, although they do not have the required sensitivity to actu- ally detect the 21-cm signal due to reionization, were able to place a tight upper bound on it (Ali ... See full document

... first galaxies and black holes which reionized the ubiquitous ...This Epoch of Reionization (EoR) is the next major unexplored cosmological ...between galaxies is almost completely ionized, ... See full document

... the high redshift universe using a combination of observational data and numerical simulations/theoretical ...on reionization can be pushed beyond the two traditional probes (Gunn-Peterson ... See full document

... first galaxies reionized the intergalactic medium (IGM) promises to shed light on both the nature of the first objects and the cosmic history of ...between galaxies and the IGM near the reionization ... See full document

... reality, galaxies are unlikely to be closed systems ...for galaxies at a fixed gas-phase oxygen abundance (Gallazzi et ...at high redshift provide further indirect evidence that inflows are ... See full document

... higher redshift where the forest is completely absorbed (asides for in the “proximity zones” close to the quasar ...numerical reionization simulations of McQuinn et ...inhomogeneous reionization on ... See full document

... forming galaxies at z ≃ 2 − 3 based on a modest ...massive galaxies at similar redshifts ...forming galaxies at this epoch are undergoing mergers while the remaining ∼ 2/3 are isolated with ... See full document

... Instead of directly looking for a cutoff feature in the spectrum of the near‐ Infrared background it is also possible to measure fluctuations in the background (Cooray et al. 2004, Bock et al. 2006), much as is ... See full document

... elliptical galaxies will form in the cores of what will become the most massive galaxy clusters today, but the epoch of the bulk of star formation for these galaxies is ...of high ... See full document

... nearby galaxies, between black hole mass and stellar bulge mass im- plies that the formation of these two components must be ...with redshift is consistent with a high redshift epoch of ... See full document

... Our goal is to generate initial conditions that are consistent with our best knowledge of the power spectrum of matter fluctuations (Spergel et al., 2003), while at the same time we want to impose the constraint that we ... See full document

... and galaxies have been used to infer the nature of the early Universe ...cal probes, each of these object types have pros and cons (see Table ...and galaxies as cosmologi- cal ...host galaxies ... See full document

... fainter galaxies (leading to a higher ionisation parameter) or other differences in ISM ...dwarf galaxies (De Looze et ...of galaxies with strong Lyα emission is higher at low SFRs in the ob- served ... See full document

... with high galactic cirrus confusion, which would exhibit a negative power spectrum on these scales at SPIRE wavelengths (Martin et ...identify high cirrus ...a high- cirrus field here is identified ... See full document

... infrared galaxies (LIRGs and ULIRGs) in the local universe, particularly irregular morphologies correspond to major galaxy mergers ...with redshift out to z ∼ 3 to indicate a higher merger fraction in the ... See full document

... five galaxies with detected Lyman continuum ...these galaxies have among the lowest best- fit star-formation rate and below average dust ...leaking galaxies and thus their E(B − V ) and star- ... See full document

... nearby galaxies (e.g. Andromeda, Mattsson et al. 2014) and the earliest galaxies (Wang, Hirashita & Hou 2017) suggest that grain growth (via accretion) would need to be responsible for ∼ 90 per cent of ... See full document

... of reionization on the polarized large- scale CMB anisotropies, reionization generates CMB tempera- ture anisotropies through the kinetic Sunyaev-Zeldovich (kSZ) e ff ect (Sunyaev & Zeldovich 1980), ... See full document

... for high mass star forming regions located at several ...of high mass stars is cru- cial to understand their formation processes from cores to stars ...20 high-mass star forming regions with ... See full document

... Although dust is a minor component in galaxies, it cap- tures a large fraction of the stellar emission, especially at short wavelengths. This process makes the direct obser- vation of stellar populations from the ... See full document