The Star Formation and Nuclear Accretion Histories of Normal Galaxies in the AGES Survey
arXiv:0903.2219 · doi:10.1088/0004-637X/696/2/2206
Abstract
We combine IR, optical and X-ray data from the overlapping, 9.3 square degree NOAO Deep Wide-Field Survey (NDWFS), AGN and Galaxy Evolution Survey (AGES), and XBootes Survey to measure the X-ray evolution of 6146 normal galaxies as a function of absolute optical luminosity, redshift, and spectral type over the largely unexplored redshift range 0.1 < z < 0.5. Because only the closest or brightest of the galaxies are individually detected in X-rays, we use a stacking analysis to determine the mean properties of the sample. Our results suggest that X-ray emission from spectroscopically late-type galaxies is dominated by star formation, while that from early-type galaxies is dominated by a combination of hot gas and AGN emission. We find that the mean star formation and supermassive black hole accretion rate densities evolve like (1+z)^3, in agreement with the trends found for samples of bright, individually detectable starburst galaxies and AGN. Our work also corroborates the results of many previous stacking analyses of faint source populations, with improved statistics.
19 pages, 15 figures, 3 tables, accepted for publication in ApJ
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Cited by in corpus (10)
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- Extended Hot Halos Around Isolated Galaxies Observed in the ROSAT All-Sky Survey
- The X-ray Star Formation Story as Told by Lyman Break Galaxies in the 4 Ms CDF-S
- Observational constraints on the co-evolution of supermassive black holes and galaxies
- The XXL Survey: VI. The 1000 brightest X-ray point sources
- The Cosmic History of Hot Gas Cooling and Radio AGN Activity in Massive Early-Type Galaxies
- The Wyoming Survey for H-alpha. III. A Multi-wavelength Look at Attenuation by Dust in Galaxies out to z~0.4