activity
19952004
most citedThe Gemini Deep Deep Survey: III. The abundance of massive galaxies 3-6 billion years after the Big Bang

365 citations · 365 across the 3 of their papers we have counts for

collaborators

12 papers

astro-ph2004

Metals in the Neutral Interstellar Medium of Starburst Galaxies

A. Aloisi, T. M. Heckman, C. G. Hoopes +3

Thanks to their proximity, local starbursts are perfectly suited for high-resolution and sensitivity multiwavelength observations aimed to test our ideas about star formation, evol…

astro-ph2004

Metals in the Neutral Interstellar Medium of Dwarf Star-Forming Galaxies

A. Aloisi, T. M. Heckman, C. G. Hoopes +3

The determination of the metal abundances in the neutral interstellar medium of dwarf star-forming galaxies is a key step in understanding their physical and chemical evolution. Th…

astro-ph2004365 cited

The Gemini Deep Deep Survey: III. The abundance of massive galaxies 3-6 billion years after the Big Bang

Karl Glazebrook, Roberto Abraham, Patrick McCarthy +9

Hierarchical galaxy formation is the model whereby massive galaxies form from an assembly of smaller units. The most massive objects therefore form last. The model succeeds in desc…

astro-ph2000

The Metallicity Evolution of Damped Lyman-alpha Systems

Sandra Savaglio

According to Pei, Fall & Hauser (1999), the global metallicity evolution of the Universe can be represented by the ratio of the total metal content to the total gas content measure…

astro-ph1999

The Metallicity evolution of Damped Lyman-alpha systems

S. Savaglio, N. Panagia, M. Stiavelli

We have collected data for 69 Damped Lyman-alpha (DLA) systems, to investigate the chemical evolution of galaxies in the redshift interval 0.0 < z < 4.4. In doing that, we have ado…

astro-ph1997

Clustering of Absorbers

S. Cristiani, S. D'Odorico, V. D'Odorico +4

The observed clustering of Lyman- lines is reviewed and compared with the clustering of CIV systems. We argue that a continuity of properties exists between Lyman- and metal…