ISOCAM Observations of Normal Star-Forming Galaxies: The Key Project Sample
We present mid-infrared maps and preliminary analysis for 61 galaxies observed with the Infrared Space Observatory.
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Publications and source records attributed to Helou, G..
We present mid-infrared maps and preliminary analysis for 61 galaxies observed with the Infrared Space Observatory.
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The ISO-IRAS Faint Galaxy Survey (IIFGS) is a program designed to produce one of the largest and deepest samples of luminous galaxies possible with present facilities.
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The system consists of two counter-rotating spirals having suffered a nearly face-on collsion only ~10(sup 7) years ago.
In a search for lensed infrared galaxies, ISOCAM images have been obtained toward the rich clusters Abell 2218 and Abell 2219 at 15 micro m.
We report a mid-infrared color and surface brightness analysis of IC 10, NGC 1313, and NGC 6946, three of the nearby galaxies studied under the Infrared Space Observatory Key Project on Normal Galaxies.
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In this work we incorporate the newest ISO results on the mid-infrared spectral-energy-distributions (MIR SEDs) of galaxies into models for the number counts and redshift distributions of MIR surveys.
We have measured accurate celestial coordinates for 4741 extragalactic objects, primarily drawn from a list of MCG galaxies with no recently published accurate positions.
We present deep ISOCAM observations taken at 4.5 um (LW1) in search of a faint halo surrounding the edge-on spiral galaxy NGC4565.
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First results are reported from the four.
We have performed some quantitative tests of the smearing model for the radio emission in spiral galaxies.