Abstract
We present a detailed study of the infrared spectral energy distribution of the high-redshift radio galaxy MRC1138-26 at z = 2.156, also known as the Spiderweb Galaxy. By combining photometry from Spitzer, Herschel and LABOCA we fit the rest-frame 5−300 μm emission using a two component, starburst and active galactic nucleus (AGN), model.
| Original language | English |
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| Article number | 146 |
| Number of pages | 8 |
| Journal | The Astrophysical Journal |
| Volume | 755 |
| Issue number | 2 |
| DOIs | |
| Publication status | Published - 1 Aug 2012 |