activity
19962004
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 2 of their papers we have counts for

collaborators

12 papers

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-ph2003

Emission line galaxies at 9200 A, including a multi-component galaxy system at z =6.43

Simon Lilly, Kim-Vy Tran, Mark Brodwin +3

This paper has been temporarily withdrawn by the authors. Subsequent observations with the VLT have shown that the high equivalent width line emission from the candidate z=6.4 gala…

astro-ph1999

Focussing Image Slicers: Refractive and Reflective

E. H. Richardson, A. Moore, T. Tilleman +1

A number of design options for image slicers for NGST and Gemini are being investigated. These image slicers are all of the focussing type and both refractive and reflective soluti…

astro-ph1999

Photometric Redshifts in the CFDF

Mark Brodwin, Simon Lilly, David Crampton

The Canada-France Deep Fields (CFDF) is a large, deep, multi-colour imaging survey undertaken primarily at CFHT. It is about 10 times fainter than the CFRS (Lilly et al 1995a) and…

astro-ph1999

Internal Kinematics of Blue CFRS Galaxies at z ~ 0.6

Gabriela Mallen-Ornelas, Simon Lilly, David Crampton +1

We present the results of a study of the internal kinematics of luminous starforming galaxies in the 0 < z < 0.8 range, with the aim of investigating the nature of the blue galaxie…

astro-ph1998

15um ISO observations of a CFRS field: the cosmic SFR as derived from UV, optical, mid-IR and radio photometry

H. Flores, F. Hammer, T. Thuan +7

The CFRS 1452+52 field has been deeply imaged with the Infrared Space Observatory (ISO) using ISOCAM through the LW3 filter (12-18um). Careful data analysis and comparison to deep…