Tracing the Accretion History of the Universe by stacking X-rays from Red Galaxies in the NDWFS Kate Brand, NOAO, Tucson A. Dey, B. Jannuzi, M. Brown, J. Najita, C. Kochanek, C. Watson, D. Fabricant, G. Fazio, W. Forman, P. Green, C. Jones, A. Kenter, S. Murray, A. Vikhlinin, B. McNamara, J. Shields, M. Rieke AAS, Denver, June 2004
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Tracing the Accretion History of the Universe by stacking X-rays from Red Galaxies in the NDWFS
Tracing the Accretion History of the Universe by stacking X-rays from Red Galaxies in the NDWFS. Kate Brand, NOAO, Tucson - PowerPoint PPT Presentation
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Tracing the Accretion History of the Universe by stacking X-rays from
Red Galaxies in the NDWFS
Kate Brand, NOAO, Tucson A. Dey, B. Jannuzi, M. Brown, J. Najita, C. Kochanek, C. Watson, D. Fabricant, G. Fazio, W. Forman, P. Green, C. Jones, A. Kenter,
S. Murray, A. Vikhlinin, B. McNamara, J. Shields, M. Rieke
AAS, Denver, June 2004
The NDWFS / XBoÖtes fields
Summary
• Stacking analysis of X-rays from optically selected galaxies to determine mean X-ray properties and how this evolves.
• Wide field / deep multi-band optical data
• AGN / star formation.
The NDWFS red galaxy population (Brown et al. 2003)
3316 red galaxies in 1.4 deg2 region selected by model SED fitting to photometric dataPhotometric redshifts, z= 0.3-0.9Same evolution corrected absolute magnitude distribution over all redshifts (MR < -20.5) -> tracing same population
The stacked X-ray images
Evolution of X-ray Luminosity with Redshift
SOFT
HARD TOTAL
Future Work
• The full 9 deg2 -> ~ 7 x number of objects -> better number statistics-Smaller errors-Divide population into sub-populations-Mean X-ray spectra-Bimodality in number counts• Stacking of X-rays in different optical populations - AGN / Star formation• Multi-wavelength data - deep radio / FIR - star formation rates