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- W1517249737 abstract "The Spitzer Space Telescope is now providing new insights into the IR population contributing to the CIRB, in particular with the MIPS 24-μm band. The question raises on how to compare them with the previous ISOCAM counts at 15-μm. In this work, we present the 24-μm predictions, inferred accurately from a phenomenological 15-μm based model. We will show how extrapolating the ISOCAM populations at higher z, we can explain almost all the 24-μm sources." @default.
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- W1517249737 date "2005-01-01" @default.
- W1517249737 modified "2023-09-23" @default.
- W1517249737 title "What we learn from the comparison between ISOCAM 15-micron & Spitzer 24-micron source counts." @default.
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