scholarly journals Radio Emission from Galaxies in the Hubble Deep Field

1998 ◽  
Vol 116 (3) ◽  
pp. 1039-1054 ◽  
Author(s):  
E. A. Richards ◽  
K. I. Kellermann ◽  
E. B. Fomalont ◽  
R. A. Windhorst ◽  
R. B. Partridge
Keyword(s):  
Radio Emission ◽  
Hubble Deep Field

scholarly journals WSRT 1.4 GHz Observations of the Hubble Deep Field

2002 ◽  
Vol 199 ◽  
pp. 32-33
Author(s):  
M.A. Garrett ◽  
G. de Bruyn ◽  
W. Baan ◽  
R.T. Schilizzi
Keyword(s):  
Radio Emission ◽  
Noise Level ◽  
Hubble Deep Field

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.

Radio Emission from Objects in the Hubble Deep Field

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

scholarly journals Radio Emission from High Redshift Galaxies: VLA Observations of the Hubble Deep Field

1998 ◽  
Vol 179 ◽  
pp. 356-357
Author(s):  
E.A. Richards
Keyword(s):  
Radio Emission ◽  
Small Area ◽  
High Redshift ◽  
Radio Galaxies ◽  
Radio Sources ◽  
High Redshift Galaxies ◽  
Area 5 ◽  
Moderate Power ◽  
Galaxy Populations ◽  
Hubble Deep Field

To study galaxy populations and their evolution at the highest possible redshifts, a small area of the sky, the Hubble Deep Field (HDF) was imaged to an unprecedented sensitivity of R = 29.5 (Williams et al. 1996). As a complement to the HST observations, we have used the VLA at 8 GHz to image an area 5.′4 in diameter (FWHM) centered on the HDF to an rms sensitivity of 2 μJy. With a radio resolution of about 3″, we have 33 sources above 9.5 μJy, seven in the 4 arcmin2 HDF field of which six have clear optical IDs. There are an additional 12 IDs in the HST flanking fields. The optical counterparts of the radio sources are a mixture of ellipticals, spirals, and irregulars, consistent with earlier surveys of comparable depth (Windhorst et al. 1995). With a median redshift <z> ∼ 1, the radio galaxies we are sampling are somewhat more distant than the classical starbursting galaxies which dominate less sensitive radio surveys. Our HDF identifications are predominately with post-starburst galaxies, moderate power AGN, and blue irregulars (Fomalont et al. 1996).

Nonlinear Phase Radio-Range Station for Measuring Distance to Radio Emission Sources

2007 ◽  
Vol 66 (1) ◽  
pp. 63-67
Author(s):  
N. I. Kozachek ◽  
Vladimir B. Avdeev ◽  
D. V. Senkevich ◽  
S. N. Panychev
Keyword(s):  
Radio Emission ◽  
Emission Sources ◽  
Nonlinear Phase ◽  
Radio Range
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