User profiles for Madau, P.
![]() | Piero MadauProfessor of Astrophysics, UC Santa Cruz and Università degli Studi di Milano-Bicocca Verified email at ucsc.edu Cited by 57453 |
Cosmic star-formation history
P Madau, M Dickinson - Annual Review of Astronomy and …, 2014 - annualreviews.org
Over the past two decades, an avalanche of new data from multiwavelength imaging and
spectroscopic surveys has revolutionized our view of galaxy formation and evolution. Here we …
spectroscopic surveys has revolutionized our view of galaxy formation and evolution. Here we …
The star formation history of field galaxies
P Madau, L Pozzetti, M Dickinson - The Astrophysical Journal, 1998 - iopscience.iop.org
We develop a method for interpreting faint galaxy data which focuses on the integrated light
radiated from the galaxy population as a whole. The emission history of the universe at …
radiated from the galaxy population as a whole. The emission history of the universe at …
High-redshift galaxies in the Hubble Deep Field: colour selection and star formation history to z ∼ 4
P Madau, HC Ferguson, ME Dickinson… - Monthly Notices of …, 1996 - academic.oup.com
… The technique used to analyse the HDF images we develop in this paper is based on the
theoretical study by Madau (1995) (see also Yoshii & Peterson 1994), and is an extension of …
theoretical study by Madau (1995) (see also Yoshii & Peterson 1994), and is an extension of …
Massive black holes as population III remnants
Recent numerical simulations of the fragmentation of primordial molecular clouds in hierarchical
cosmogonies have suggested that the very first stars (the so-called Population III) may …
cosmogonies have suggested that the very first stars (the so-called Population III) may …
21 centimeter tomography of the intergalactic medium at high redshift
We investigate the 21 cm signature that may arise from the intergalactic medium (IGM) prior
to the epoch of full reionization (z> 5). In scenarios in which the IGM is reionized by discrete …
to the epoch of full reionization (z> 5). In scenarios in which the IGM is reionized by discrete …
[HTML][HTML] Radiative transfer in a clumpy universe: The colors of high-redshift galaxies
P Madau - … Journal, Part 1 (ISSN 0004-637X), vol. 441, no. 1, p …, 1995 - adsabs.harvard.edu
… In Figure la we plot the distribution p(~c) as a function of the Ly~x line-blanketing optical depth
for … Figure lb depicts p(x) as a function of the continuum opacity alone. The optical depth is …
for … Figure lb depicts p(x) as a function of the continuum opacity alone. The optical depth is …
Radiative transfer in a clumpy universe. III. The nature of cosmological ionizing sources
… In Paper I (Madau 1995) we showed how the stochastic attenuation produced by neutral
hydrogen along the line of sight can seriously distort our view of objects at cosmological …
hydrogen along the line of sight can seriously distort our view of objects at cosmological …
Radiative transfer in a clumpy universe: Ii. the utraviolet extragalactic background
… In Paper I (Madau 1995), we have assessed the e ects of the stochastic attenuation produced
… From the numerical study of Madau & Meiksin (1994), we derive for thermally broadened …
… From the numerical study of Madau & Meiksin (1994), we derive for thermally broadened …
The great observatories origins deep survey: initial results from optical and near-infrared imaging
This special issue of the Astrophysical Journal Letters is dedicated to presenting initial
results from the Great Observatories Origins Deep Survey (GOODS) that are primarily, but not …
results from the Great Observatories Origins Deep Survey (GOODS) that are primarily, but not …
Early metal enrichment of the intergalactic medium by pregalactic outflows
… (z \ 3.5) B 0.6 ] 10~12 s~1, which is close to that inferred from quasars (Haardt & Madau
1996). They also show a clear correlation between the HI column, gas temperature, and …
1996). They also show a clear correlation between the HI column, gas temperature, and …