Michael Strauss
Michael Strauss Michael Strauss
SDSS Quasar Sample Courtesy Xiaohui Fan
The Luminosity Function from the full SDSS (here, a complete sample of 15,000 quasars) n Can study luminous quasars over the full range of redshift with a single sample (note that we do not go to very low luminosities…) luminosities n Substantial (and quantifiable) incompleteness at z=2.7, 3.5. Richards et al. 2005c
- Page 1 and 2: Nearly Normal Active Galactic Nucle
- Page 3: Using SDSS for AGN Studies n A colo
- 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
The Luminosity Function from<br />
the full SDSS<br />
(here, a complete sample of<br />
15,000 quasars)<br />
n Can study luminous<br />
quasars over the full range<br />
of redshift with a single<br />
sample (note that we do not<br />
go to very low<br />
luminosities…)<br />
luminosities<br />
n Substantial (and<br />
quantifiable)<br />
incompleteness at z=2.7,<br />
3.5.<br />
Richards et al. 2005c
Change language