output
19932026
most citedThe Seventh Data Release of the Sloan Digital Sky Survey

5.4k citations

Showing 2006 · astro-phShow all

48 papers · 2 filters

astro-ph2006★ 25 cited

On the Heterogeneity of Metal-Line and Ly-Alpha Absorption in Galaxy "Halos" at z~0.7

Christopher W. Churchill, Glenn G. Kacprzak, Charles C. Steidel +1

We examine the properties of two galaxy "halos" at z ~ 0.7 in the TON 153 (z_em = 1.01) quasar field. The first absorber-galaxy pair (G1) is a z = 0.672, L_B = 4.3 L*_B, E/S0 galax…

astro-ph2006★ 370 cited

Hubble Space Telescope Fine Guidance Sensor Parallaxes of Galactic Cepheid Variable Stars: Period-Luminosity Relations

G. Fritz Benedict, Barbara E. McArthur, Michael W. Feast +6

(abridged) We present new absolute trigonometric parallaxes and relative proper motions for nine Galactic Cepheid variable stars: l Car, zeta Gem, beta Dor, W Sgr, X Sgr, Y Sgr, FF…

astro-ph2006★ 173 cited

Formation of Double Compact Objects

V. Kalogera, K. Belczynski, C. Kim +2

Current observations of double neutron stars provide us with a wealth of information that we can use to investigate their evolutionary history and the physical conditions of neutro…

astro-ph2006★ 10 cited

Gravitational lensing as a probe of compact object population in the Galaxy

S. Oslowski, R. Moderski, T. Bulik +1

The population of solitary compact objects in the Galaxy is very diffcult to investigate. In this paper we analyze the possibility of using microlensing searches to detect and to a…

astro-ph2006★ 114 cited

The Intrinsically X-ray Weak Quasar PHL 1811. I. X-ray Observations and Spectral Energy Distribution

Karen M. Leighly, Jules P. Halpern, Edward B. Jenkins +3

This is the first of two papers reporting observations and analysis of the unusually bright (m_b=14.4), luminous (M_B=-25.5), nearby (z=0.192) narrow-line quasar PHL 1811, focusing…

astro-ph2006★ 222 cited

The Peculiar SN 2005hk: Do Some Type Ia Supernovae Explode as Deflagrations?

M. M. Phillips, W. Li, J. A. Frieman +41

We present extensive u'g'r'i'BVRIYJHKs photometry and optical spectroscopy of SN 2005hk. These data reveal that SN 2005hk was nearly identical in its observed properties to SN 2002…