• Corpus ID: 18734913

National Optical Astronomy Observatory

@inproceedings{Physics2010NationalOA,
  title={National Optical Astronomy Observatory},
  author={astronomy Physics},
  year={2010}
}
We use an X-ray stacking technique to investigate the evolution of the mean X-ray luminosity of ∼21,000 red galaxies at 0.3 ≤ z < 0.9 as a function of their stellar mass and redshift. The red galaxies are selected from the 9.3 deg 2 Boötes field of the NOAO Deep Wide-Field Survey (NDWFS). The mean X-ray luminosity is an order of magnitude larger than we would expect from stellar sources alone and therefore must be primarily due to AGN emission. The X-ray luminosities (L x ≈ 10 41 ergs s −1… 

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