THE DEEP SWIRE FIELD. I. 20 cm CONTINUUM RADIO OBSERVATIONS: A CROWDED SKY

The VLA - VIRMOS Deep Field I . Radio observations probing the μ Jy source population

We have conducted a deep survey (r.m.s noise ≃ 17µJy) with the Very Large Array (VLA) at 1.4 GHz, with a resolution of 6 arcsec, of a 1 deg 2 region included in the VIRMOS VLT Deep Survey. In the same field we already have multiband photometry down to IAB = 25, and spectroscopic observations will be obtained during the VIRMOS VLT survey. The homogeneous sensitivity over the whole field has allo...

Radio Observations of the Hubble Deep Field South 3

Radio Observations of the Hubble Deep Field South region: I. Survey Description and Initial Results

This paper is the first of a series describing the results of the Australia Telescope Hubble Deep Field South (ATHDFS) radio survey. The survey was conducted at four wavelengths 20, 11, 6, and 3 cm, over a 4-year period, and achieves an rms sensitivity of about 10 μJy at each wavelength. We describe the observations and data reduction

T he ultra - deep 20 cm Australia telescope survey of the Chandra Deep Field South

The advent of ultra-deep X-ray surveys with telescopes such as Chandra and XMM, together with deep multi-waveband ground-based and HST imaging covering radio and optical /near-IR wavelengths, allows us to directly probe the detailed properties of the environments, host galaxies and central accretion disks of both radio-loud and radio-quiet active galaxies up to cosmological redshifts. Here we p...

Observations of the Hubble Deep Field with the Infrared Space Observatory - I. Data reduction, maps and sky coverage

We present deep imaging at 6.7 and 15 /lm from the CAM instrument on the Infrared Space Observatory (ISO), centred on the Hubble Deep Field (HDF). These are the deepest integrations published to date at these wavelengths in any region of sky. We discuss the observational strategy and the data reduction. The observed source density appears to approach the CAM confusion limit at 15 /lm, and fluct...