He also suggested that I talk to Yue Shen about his catalogs of black hole masses (or maybe it was line widths). I don't know how different this is to the catalog that Ian McGreer has given us.
He also thought that perhaps we might want to do a separation by Eddington ratio and see if there is a clustering dependence there.
He was very helpful, and overall a productive meeting.
I've been working on trying to get a stronger clustering signal separation. So far divided the QSO sample into even brighter/dimmer sets. As well as applying a uniform redshift selection to my two samples to see if what I am measuring is actually a redshift separation, not luminosity. Fun fun fun!
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