Michael Strauss

30.06.2013 • Views

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Michael Strauss

Michael Strauss

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Comoving number<br />

density peaks<br />

between z=2 =2 and 3<br />

LF slope increases at<br />

z=3 =3 and above.

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What is different about LINER Galaxies

Stephen Murray - Astronomy and Astrophysics - University of ...

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Light, Optics and Telescopes Trip to Lick Observatory

Frank van den Bosch

Jason X. Prochaska

Leo Blitz

Kathryn Johnston

Risa Wechsler - Astronomy and Astrophysics

Stéphane Courteau

Kim Griest

Ofer Lahav

Laurence Tresse

Systematic flattening of the LF above z~3

Comoving number density peaks between z=2 =2 and 3 LF slope increases at z=3 =3 and above.

Page 1 and 2: Nearly Normal Active Galactic Nucle
Page 3 and 4: Using SDSS for AGN Studies n A colo
Page 5: The Luminosity Function from the fu
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