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Observations of the Hubble Deep Field with the Infrared Space Observatory. IV. Association of sources with Hubble Deep Field Galaxies
The ISO-HDF Consortium, :, Bob Mann
We discuss the identification of sources detected by ISO at 6.7 and 15 micron in the Hubble Deep Field (HDF) region. We conservatively associate ISO sources with objects in existin…
Observations of the Hubble Deep Field with the Infrared Space Observatory. V. Spectral Energy Distributions, Starburst Models and Star Formation History
The ISO-HDF Consortium, :, Michael Rowan-Robinson
We have modelled the spectral energy distributions of the 13 HDF galaxies reliably detected by ISO. For 2 galaxies the emission detected by ISO is consistent with being starlight o…
Observations of the Hubble Deep Field with the Infrared Space Observatory. III. Source counts and P(D) analysis
The ISO-HDF Consortium, :, Seb Oliver
We present source counts at 6.7 micron and 15 micron from our maps of the Hubble Deep Field region, reaching 38.6 microJy at 6.7 micron and 255 microJy at 15 micron. These are the…
Observations of the Hubble Deep Field with the Infrared Space Observatory. II. Source detection and photometry
The ISO-HDF Consortium, :, Pippa Goldschmidt
We present positions and fluxes of point sources found in the Infrared Space Observatory (ISO) images of the Hubble Deep Field (HDF) at 6.7 and 15 micron. We have constructed algor…
Observations of the Hubble Deep Field with the Infrared Space Observatory. I. Data reduction, maps and sky coverage
The ISO-HDF Consortium, :, Steve Serjeant
We present deep imaging at 6.7 micron and 15 micron from the CAM instrument on the Infrared Space Observatory (ISO), centred on the Hubble Deep Field (HDF). These are the deepest i…