Neutral hydrogen traces gravitational potentials. In the nearby universe, 21cm emission-line surveys show that the bulk of the HI resides in well-formed, optically-luminous galaxies. At high redshift, 21cm line absorption against background radio quasars occurs in gas-rich systems identified with the highest HI column densities -- the ``damped Lyman alpha'' quasar absorption-line systems. High spatial-resolution observations of the redshifted 21cm line absorbers measure sizes and kinematics of the neutral absorbers
© 2011 Dr. Paul M. GeilThe measurement of the spatial distribution of neutral hydrogen in the high-r...
We study the distribution and nature of neutral hydrogen in various environments. We start by explor...
We study the distribution and nature of neutral hydrogen in various environments. We start by explor...
Damped Lyman-alpha and metal absorption lines in the spectra of quasars indicate the presence of int...
Using the Boolardy Engineering Test Array of the Australian Square Kilometre Array Pathfinder (ASKAP...
We present the results of a blind search for intervening H i 21 cm absorption towards 260 radio sour...
We have precisely characterised our Universe with the elegant LCDM model. However, this model predic...
We investigate the 21 cm absorption lines produced by non-linear structures during the early stage o...
The nature of the most abundant components of the Universe, dark energy and dark matter, is still to...
Distribution of cold gas in the post-reionization era provides an important link between distributio...
The baryonic processes in galaxy evolution include gas infall onto galaxies to form neutral atomic h...
The epoch of reionization, when photons from early galaxies ionized the intergalactic medium about a...
Measurements of hydrogen are important in our understanding of the Universe. Following reionization ...
Recent observations using the Hubble Space Telescope of the z = 0.156 QSO 3C 273 have discovered a s...
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2019, Tutor: ...
© 2011 Dr. Paul M. GeilThe measurement of the spatial distribution of neutral hydrogen in the high-r...
We study the distribution and nature of neutral hydrogen in various environments. We start by explor...
We study the distribution and nature of neutral hydrogen in various environments. We start by explor...
Damped Lyman-alpha and metal absorption lines in the spectra of quasars indicate the presence of int...
Using the Boolardy Engineering Test Array of the Australian Square Kilometre Array Pathfinder (ASKAP...
We present the results of a blind search for intervening H i 21 cm absorption towards 260 radio sour...
We have precisely characterised our Universe with the elegant LCDM model. However, this model predic...
We investigate the 21 cm absorption lines produced by non-linear structures during the early stage o...
The nature of the most abundant components of the Universe, dark energy and dark matter, is still to...
Distribution of cold gas in the post-reionization era provides an important link between distributio...
The baryonic processes in galaxy evolution include gas infall onto galaxies to form neutral atomic h...
The epoch of reionization, when photons from early galaxies ionized the intergalactic medium about a...
Measurements of hydrogen are important in our understanding of the Universe. Following reionization ...
Recent observations using the Hubble Space Telescope of the z = 0.156 QSO 3C 273 have discovered a s...
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2019, Tutor: ...
© 2011 Dr. Paul M. GeilThe measurement of the spatial distribution of neutral hydrogen in the high-r...
We study the distribution and nature of neutral hydrogen in various environments. We start by explor...
We study the distribution and nature of neutral hydrogen in various environments. We start by explor...