A new model for the infrared emission of IRAS F10214+4724
We present a new model for the infrared emission of the high redshift hyperluminous infrared galaxy IRAS F10214+4724 which takes into account recent photometric data from Spitzer and Herschel that sample the peak of its spectral energy distribution. We first demonstrate that the combination of the A...
Main Authors: | , , , |
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Format: | Journal article |
Language: | English |
Published: |
2011
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