Rapid coeval black hole and host galaxy growth in MRC1138-262: The hungry spider
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,...
Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
---|---|
Format: | Journal Article |
Published: |
2012
|
Online Access: | http://hdl.handle.net/20.500.11937/43788 |