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COSMOS Key Questions for AGN. Chris Impey and Jonathan Trump Steward Observatory Martin Elvis (CfA), John Huchra (CfA), Pat McCarthy (Carnegie), and Michael Westover (Harvard). COSMOS AGN Survey Science Goals. Deep, wide-field AGN survey, down to Seyfert luminosities at z ~ 3
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COSMOSKey Questions for AGN Chris Impey and Jonathan Trump Steward Observatory Martin Elvis (CfA), John Huchra (CfA), Pat McCarthy (Carnegie), and Michael Westover (Harvard)
COSMOS AGN SurveyScience Goals • Deep, wide-field AGN survey, down to Seyfert luminosities at z ~ 3 • Bolometric measures of activity from X-ray, optical, radio and IR data • Proxy for measure of supermassive black hole mass from broad lines • Statistical sensitivity to rare populations (obscured, BAL, etc) • New measure of AGN clustering relative to galaxy large scale structure • Environmental dependence of AGN luminosity and energy distributions • Host galaxies morphologies measured out to z ~ 1 with ACS data • Populations of high redshift (z > 4) quasars with superior statistics • 3D tomography of the IGM using COS spectroscopy of brightest quasars
IMACS limit IMACS limit AGN locus 0.1 < Fx/Fopt < 10 X-Ray Selection Most efficient way to select AGN with x-ray… follow up all objects of iAB < 23.5 with IMACS Secondary targets and objects with iAB > 23.5 picked up by V-COSMOS
z~2.1 QSO z~3.6 QSO z~1.8 QSO ~30 counts/pixel z~0.5 QSO + SF? First Results
Redshift Yields and Projections • Redshifts for targets of 20 counts/pixel or more • > Limited to i’<23.5 • Estimates from pointing 11 projected to 2 deg2