365 citations · 365 across the 2 of their papers we have counts for
10 papers · 1 filter
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…
Penetration at high-z of the Greenberg "yellow stuff": Eyes to the Future with NGST
David L. Block, Ivanio Puerari, Marianne Takamiya +1
Quantitative morphological dust-penetrated templates for galaxies in our Local Universe may also serve as excellent templates for galaxies at high-z, because of partial/total decou…
Observations of Disk Galaxy Evolution
Roberto G. Abraham, Sidney van den Bergh
The morphologies of disk galaxies begin to deviate systematically from those of nearby galaxies at surprisingly low redshifts, possibly as low as z=0.3. This corresponds to a time…
The z ~ 1.2 Galaxy Luminosity Function from The LCIR Survey
H. -W. Chen, P. J. McCarthy, R. O. Marzke +10
We present results from the Las Campanas Infrared Survey, designed to identify a statistically significant sample of z>=1 galaxies using photometric redshift techniques. Here we su…
The Duality of Spiral Structure, and a Quantitative Dust Penetrated Morphological Tuning Fork at Low and High Redshift
D. L. Block, I. Puerari, R. J. Buta +3
In the near-infrared, the morphology of older star-dominated disks indicates a simple classification scheme (1) H where is the dominant harmonic, (2) a pitch angle (derived…
Perspectives in Physical Morphology
R. G. Abraham
In the first section of these lectures I outline the classical framework of the Hubble classification system. Because of space limitations I will focus on points of controversy con…