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 |
---|---|
Article number | 146 |
Number of pages | 8 |
Journal | The Astrophysical Journal |
Volume | 755 |
Issue number | 2 |
DOIs | |
Publication status | Published - 1 Aug 2012 |