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The discovery of a giant debris arc in the Coma Cluster
Neil Trentham, Bahram Mobasher
We present the discovery a giant low surface-brightness arc, of length luminous matrix with surface-brightness mu_B < 26.5 mag arcsec^{-2} and a number of embedded condensations. I…
Near-infrared luminosity function and colours of dwarf galaxies in the Coma Cluster
Bahram Mobasher, Neil Trentham
We present K-band observations of the low-luminosity galaxies in the Coma cluster, which are responsible for the steep upturn in the optical luminosity function at M_R ~ -16, disco…
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…