Rapid Coeval Black Hole and Host Galaxy Growth in MRCnbsp1138-262 : The Hungry Spider
Seymour, N., Altieri, B., De Breuck, C., Barthel, P., Coia, D., Conversi, L., Dannerbauer, H., Dey, A., Dickinson, M., Drouart, G., Galametz, A., Greve, T.R., Haas, M., Hatch, N., Ibar, E., Ivison, R., Jarvis, M.J., Kovács, A., Kurk, J., Lehnert, M., Miley, G., Nesvadba, N., Rawlings, J.I., Rettura, A., Röttgering, H., Rocca-Volmerange, B., Sánchez-Portal, M., Santos, J. S., Stern, D., Stevens, J., Valtchanov, I., Vernet, J. and Wylezalek, D.
(2012)
Rapid Coeval Black Hole and Host Galaxy Growth in MRCnbsp1138-262 : The Hungry Spider.
The Astrophysical Journal, 755 (2): 146.
ISSN 0004-637X
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.
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