Absorption lines in the Ly{alpha} forest can be thought of as peaks in neutral hydrogen density along lines of sight. The column density distribution (the number density of absorption lines as a function of column density) is then a statistic of density peaks, which contains information about the underlying power spectrum. In particular, we show that the slope of the distribution provides a measure of power on scales smaller than those probed by studies of present day large scale structure. 2 refs., 1 fig
Lyman-alpha forest lines in QSO spectra have typical widths of 20-50 km/s. Low column density absorb...
Power laws describe frequent scaling trends found in nature, in areas as disparate as physics, biolo...
Numerical simulations indicate that the smooth, photoionized intergalactic medium (IGM) responsible ...
We develop a method to calculate the column density distribution of the Lyman-alpha forest for colum...
A simple consistency argument for hypothesis of the galactic halo origin of the Ly-alpha forest abso...
Knowledge of the evolution of the low column density end of the Ly alpha forest (12.8 < log N_HI < 1...
In this paper we review the importance of the Lyman alpha forest as a probe of structure formation i...
The cross-section of sky occupied by a particular neutral hydrogen column density provides insight i...
The spatial distribution of Ly-alpha forest absorption systems toward a group of 8, closely spaced Q...
We have analyzed the properties of low column density Lyman alpha forest clouds (12.8 < log N_HI < 1...
We study the physical properties of the Lyman-α forest by applying the inversion method described ...
In this thesis we investigate the large-scale distribution of Ly alphaforest absorption, the effect ...
We derive the distribution of neutral and ionized gas in high redshift clouds which are optically th...
Abstract: We present a measurement of the HI column density distribution function, f(N), at the pres...
We present a measurement of the HI column density distribution function f(N-HI) at the present epoch...
Lyman-alpha forest lines in QSO spectra have typical widths of 20-50 km/s. Low column density absorb...
Power laws describe frequent scaling trends found in nature, in areas as disparate as physics, biolo...
Numerical simulations indicate that the smooth, photoionized intergalactic medium (IGM) responsible ...
We develop a method to calculate the column density distribution of the Lyman-alpha forest for colum...
A simple consistency argument for hypothesis of the galactic halo origin of the Ly-alpha forest abso...
Knowledge of the evolution of the low column density end of the Ly alpha forest (12.8 < log N_HI < 1...
In this paper we review the importance of the Lyman alpha forest as a probe of structure formation i...
The cross-section of sky occupied by a particular neutral hydrogen column density provides insight i...
The spatial distribution of Ly-alpha forest absorption systems toward a group of 8, closely spaced Q...
We have analyzed the properties of low column density Lyman alpha forest clouds (12.8 < log N_HI < 1...
We study the physical properties of the Lyman-α forest by applying the inversion method described ...
In this thesis we investigate the large-scale distribution of Ly alphaforest absorption, the effect ...
We derive the distribution of neutral and ionized gas in high redshift clouds which are optically th...
Abstract: We present a measurement of the HI column density distribution function, f(N), at the pres...
We present a measurement of the HI column density distribution function f(N-HI) at the present epoch...
Lyman-alpha forest lines in QSO spectra have typical widths of 20-50 km/s. Low column density absorb...
Power laws describe frequent scaling trends found in nature, in areas as disparate as physics, biolo...
Numerical simulations indicate that the smooth, photoionized intergalactic medium (IGM) responsible ...