| |
 |
| Paper: |
Spitzer Observations of High Redshift Radio Galaxies |
| Volume: |
380, At the Edge of the Universe: Latest Results from the Deepest Astronomical Surveys |
| Page: |
393 |
| Authors: |
Seymour, N.; Stern, D.; De Breuck, C. |
| Abstract: |
We present the results of a comprehensive Spitzer survey of 70 radio galaxies across 1 < z < 5.2. Using IRAC (3.6 − 8.0 μm), IRS (16 μm) and MIPS (24 − 160 μm) imaging, we decompose the rest-frame optical to infrared spectral energy distributions into stellar, AGN, and dust components and determine the contribution of host galaxy stellar emission at rest-frame 1.6 μm (H-band). The resultant stellar luminosities imply stellar masses of 1011−12M⊙, independent of redshift, indicating that radio galaxies form early and are amongst the most massive galaxies observed over this redshift range. These powerful radio galaxies tend to lie in a similar region of mid-IR color-color space as unobscured AGN, despite the inferred stellar contribution to their shorter-wavelength, mid-IR SEDs. The observed rest-frame mid-IR luminosities are typically above 1011L⊙, similar to lower redshift AGN. As expected, these exceptionally high mid-IR luminosities are consistent with an obscured, highly-accreting AGN. A weak, but significant, correlation of stellar mass with radio luminosity is found, consistent with earlier results. |
|
|
|
|
|
