Michael Strauss

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n 5645 quasars with g < 21.85 selected from SDSS imaging, observed with 2dF at AAT. UV excess sources, almost all with z < 2.5. Best-fit slope b is -1.45 at faint end. A crucial question: the shape and slope of the LF at the faint end… end Richards et al. 2005a MNRAS
The nature of low-luminosity quasars n As we push to lower luminosities still (at low redshift), redshift), emission from the host galaxy becomes an ever-larger fraction of the total luminosity. n Here we select both Type I and Type II Seyfert galaxies from the SDSS main galaxy sample. Lei Hao 2003, PhD Thesis; Hao et al. 2005ab in AJ
Page 1 and 2: Nearly Normal Active Galactic Nucle
Page 3 and 4: Using SDSS for AGN Studies n A colo
Page 5 and 6: The Luminosity Function from the fu
Page 7: Comoving number density peaks betwe
Page 11 and 12: Ratios of various emission lines al
Page 13 and 14: The relative number of Type I and T
Page 15 and 16: n Very few high-luminosity Type II
Page 17 and 18: How do we determine intrinsic lumin
Page 19 and 20: • Multiband continuum imaging wit
Page 21 and 22: A montage of HST images of SDSSSDSS
Page 23 and 24: These objects have IRAC colors cons
Page 25 and 26: 19 quasars with z>5.7

Michael Strauss

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