scholarly journals Adaptive Optics Views of the Hubble Deep Fields Final report on LLNL LDRD Project 03-ERD-002

2007 ◽  
Author(s):  
C Max ◽  
D Gavel ◽  
D Pennington ◽  
S Gibbard ◽  
M van Dam ◽  
...  
Keyword(s):  
Adaptive Optics ◽  
Final Report ◽  
Hubble Deep Fields ◽  
Deep Fields

scholarly journals Photometric Redshifts and Selection of High-Redshift Galaxies in the NTT and Hubble Deep Fields

2000 ◽  
Vol 120 (5) ◽  
pp. 2206-2219 ◽  
Author(s):  
Adriano Fontana ◽  
Sandro D’Odorico ◽  
Francesco Poli ◽  
Emanuele Giallongo ◽  
Stephane Arnouts ◽  
...  
Keyword(s):  
High Redshift ◽  
Photometric Redshifts ◽  
High Redshift Galaxies ◽  
Hubble Deep Fields ◽  
Deep Fields ◽  
Selection Of ◽  
Redshift Galaxies

scholarly journals The evolution of barred spiral galaxies in the Hubble Deep Fields North and South

1999 ◽  
Vol 308 (2) ◽  
pp. 569-576 ◽  
Author(s):  
R. G. Abraham ◽  
M. R. Merrifield ◽  
R. S. Ellis ◽  
N. R. Tanvir ◽  
J. Brinchmann
Keyword(s):  
Spiral Galaxies ◽  
Hubble Deep Fields ◽  
Deep Fields ◽  
Barred Spiral Galaxies ◽  
North And South

scholarly journals Cloning Hubble Deep Fields. II. Models for Evolution by Bright Galaxy Image Transformation

1998 ◽  
Vol 506 (2) ◽  
pp. 579-589 ◽  
Author(s):  
Rychard Bouwens ◽  
Tom Broadhurst ◽  
Joseph Silk
Keyword(s):  
Bright Galaxy ◽  
Image Transformation ◽  
Hubble Deep Fields ◽  
Deep Fields

scholarly journals Galaxy number counts -- V. Ultradeep counts: the Herschel and Hubble Deep Fields

2001 ◽  
Vol 323 (4) ◽  
pp. 795-830 ◽  
Author(s):  
N. Metcalfe ◽  
T. Shanks ◽  
A. Campos ◽  
H. J. McCracken ◽  
R. Fong
Keyword(s):  
Hubble Deep Fields ◽  
Deep Fields ◽  
Number Counts

scholarly journals The Optical Extragalactic Background Light from Resolved Galaxies

2001 ◽  
Vol 204 ◽  
pp. 71-85 ◽  
Author(s):  
Lucia Pozzetti ◽  
Piero Madau
Keyword(s):  
Surface Brightness ◽  
Diffuse Light ◽  
Selection Effects ◽  
Extragalactic Background Light ◽  
Background Light ◽  
Number Magnitude ◽  
Near Ir ◽  
The Galaxy ◽  
Hubble Deep Fields ◽  
Deep Fields

We discuss the ultraviolet to near-IR galaxy counts from the deepest imaging surveys, including the northern and southern Hubble Deep Fields. The logarithmic slope of the galaxy number-magnitude relation is flatter than 0.4 in all seven UBVIJHK optical passbands at faint magnitudes, i.e. the light from resolved galaxies has converged from the UV to the near-IR. Most of the galaxy contribution to the extragalactic background light (BEL) comes from relatively bright, low-redshift objects (50% at VAB ≲ 21 and 90% at VAB ≲ 25.5). We find a lower limit to the surface brightness of the optical EBL of about 15 nW m−2 sr−1, comparable to the intensity of the far-IR background from COBE data. Diffuse light, lost because of surface brightness selection effects, may add substantially to the EBL.

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