Hubble Space Telescope And The High Redshift Universe, The - Proceedings Of The 37th Herstmonceux Conference


Book Description

Since the successful refurbishment mission, the Hubble Space Telescope has made dramatic and exciting progress in unravelling the nature of sources at high redshift. The upcoming installation of the next generation of instruments will give further impetus to the field, particularly in the infrared spectral region.The proceedings of this landmark meeting review the results of the first three years of post-repair data, including the deepest astronomical images ever obtained: the Hubble Deep Field. This was the first presentation of these exciting results at a major international conference. The interface between HST and ground-based facilities and planned programmes with forthcoming HST instruments are also extensively discussed.




Disentangling Redshift-Space Distortions and Nonlinear Bias Using the 2D Power Spectrum


Book Description

We present the nonlinear 2D galaxy power spectrum, P(k, æ), in redshift space, measured from the Dark Sky simulations, using galaxy catalogs constructed with both halo occupation distribution and subhalo abundance matching methods, chosen to represent an intermediate redshift sample of luminous red galaxies. We find that the information content in individual æ (cosine of the angle to the line of sight) bins is substantially richer then multipole moments, and show that this can be used to isolate the impact of nonlinear growth and redshift space distortion (RSD) effects. Using the æ 0.2 simulation data, which we show is not impacted by RSD effects, we can successfully measure the nonlinear bias to an accuracy of ̃5% at k




The Hy-redshift Universe


Book Description

Bunker (astronomy, U. of California) and van Breugel (Institute of Geophysics & Planetary Physics) present 87 papers from the June 1999 conference on the study of high-redshift galaxies (the pun in the title is a dedication to scientist Spinrad). The contributions are organized into sections on radio galaxies at large redshifts, galaxy stellar populations and scaling relations, deep field surveys, galaxy evolution in clusters, theory and observations of structure formation, the history of star formation, and future prospects.



















The First Galaxies in the Universe


Book Description

This book provides a comprehensive, self-contained introduction to one of the most exciting frontiers in astrophysics today: the quest to understand how the oldest and most distant galaxies in our universe first formed. Until now, most research on this question has been theoretical, but the next few years will bring about a new generation of large telescopes that promise to supply a flood of data about the infant universe during its first billion years after the big bang. This book bridges the gap between theory and observation. It is an invaluable reference for students and researchers on early galaxies. The First Galaxies in the Universe starts from basic physical principles before moving on to more advanced material. Topics include the gravitational growth of structure, the intergalactic medium, the formation and evolution of the first stars and black holes, feedback and galaxy evolution, reionization, 21-cm cosmology, and more. Provides a comprehensive introduction to this exciting frontier in astrophysics Begins from first principles Covers advanced topics such as the first stars and 21-cm cosmology Prepares students for research using the next generation of large telescopes Discusses many open questions to be explored in the coming decade