Hubble Deep Field and the Distant Universe

Author(s):  
Robert Williams
Keyword(s):  
2000 ◽  
Vol 127 (1) ◽  
pp. 1-9 ◽  
Author(s):  
David W. Hogg ◽  
Michael A. Pahre ◽  
Kurt L. Adelberger ◽  
Roger Blandford ◽  
Judith G. Cohen ◽  
...  

2003 ◽  
Vol 324 (5) ◽  
pp. 506-506
Author(s):  
T. Miyaji ◽  
R.E. Griffiths ◽  
D. Lumb ◽  
V. Sarajedini ◽  
H. Siddiqui
Keyword(s):  

Author(s):  
R. A. Méndez ◽  
G. De Marchi ◽  
D. Minniti ◽  
A. Baker ◽  
W. J. Couch
Keyword(s):  

2002 ◽  
Vol 199 ◽  
pp. 32-33
Author(s):  
M.A. Garrett ◽  
G. de Bruyn ◽  
W. Baan ◽  
R.T. Schilizzi

We present WSRT 1.38 GHz observations of the Hubble Deep Field (and flanking fields). 72 hours of data were combined to produce the WSRT's deepest image yet, reaching an r.m.s. noise level of 8 microJy/beam. We detect radio emission from galaxies both in the HDF and HFF which have not been previously detected by recent MERLIN or VLA studies of the field.


1999 ◽  
Author(s):  
Christopher J. Conselice ◽  
Matthew A. Bershady
Keyword(s):  

1997 ◽  
Vol 475 (1) ◽  
pp. L5-L7 ◽  
Author(s):  
E. B. Fomalont ◽  
K. I. Kellermann ◽  
E. A. Richards ◽  
R. A. Windhorst ◽  
R. B. Partridge

2001 ◽  
Vol 562 (1) ◽  
pp. L23-L27 ◽  
Author(s):  
Felipe Menanteau ◽  
Raul Jimenez ◽  
Francesca Matteucci

1999 ◽  
Vol 186 ◽  
pp. 439-445
Author(s):  
R. D. Blandford

The Hubble Deep Field, henceforth HDF, (Williams et al 1996) is a unique data set for studies of faint galaxies. A small area was chosen well away from known local density enhancements and sources of obscuration. It was imaged for 30 complete orbits in each of four filters centered on wavelengths λ300, 450, 606, 814 nm. There are three, contiguous WFPC2 frames and a solid angle 15,500 arcsec2 is usable. This tiny region is teeming with galaxies. At least 2500 significant features can be identified down to R = 30, though it is not clear that these are all entire galaxies.


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