Michael Strauss
Michael Strauss Michael Strauss
My collaborators on the work shown here: My former and current grad students: Xiaohui Fan, Lei Hao, Nadia Zakamska, Joe Hennawi Former Postdocs: Gordon Richards, Pat Hall Julian Krolik, Tim Heckman, Bob Becker, Richard White, Christy Tremonti, Guinevere Kauffmann. And the whole SDSS collaboration, especially: Jim Gunn, Jill Knapp, Robert Lupton, David Schlegel, Sebastian Jester, Don Schneider, Dan Vanden Berk, Zeljko Ivezic, and many others.
Using SDSS for AGN Studies n A color-selected sample of quasars, sensitive from z=0 to z>6. 90,000 quasars and counting. n A magnitude-limited sample of more than 500,000 galaxies, from which Seyferts can be selected. n Superb morphologies, photometry, astrometry, and R=2000 photometrically calibrated spectroscopy, 3800-9200 Å.
- Page 1: Nearly Normal Active Galactic Nucle
- Page 5 and 6: The Luminosity Function from the fu
- Page 7 and 8: Comoving number density peaks betwe
- Page 9 and 10: The nature of low-luminosity quasar
- 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
Using SDSS for AGN Studies<br />
n A color-selected sample of quasars,<br />
sensitive from z=0 to z>6. 90,000 quasars<br />
and counting.<br />
n A magnitude-limited sample of more than<br />
500,000 galaxies, from which Seyferts can<br />
be selected.<br />
n Superb morphologies, photometry,<br />
astrometry, and R=2000 photometrically<br />
calibrated spectroscopy, 3800-9200 Å.
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