activity
19952023
most citedThe Seventh Data Release of the Sloan Digital Sky Survey

5.4k citations · 39.3k across the 226 of their papers we have counts for

collaborators
Showing 2012Show all

7 papers · 1 filter

astro-ph.CO2012★ 5 cited

X-ray and Multiwavelength Insights into the Inner Structure of High-Luminosity Disc-Like Emitters

B. Luo, W. N. Brandt, M. Eracleous +5

We present X-ray and multiwavelength studies of a sample of eight high-luminosity active galactic nuclei (AGNs) with disc-like Hβemission-line profiles selected from the Sloan Digi…

astro-ph.CO2012★ 273 cited

The Sloan Digital Sky Survey quasar catalog: ninth data release

Isabelle Pâris, Patrick Petitjean, Eric Aubourg +73

We present the Data Release 9 Quasar (DR9Q) catalog from the Baryon Oscillation Spectroscopic Survey (BOSS) of the Sloan Digital Sky Survey III. The catalog includes all BOSS objec…

astro-ph.CO2012★ 2.1k cited

The Baryon Oscillation Spectroscopic Survey of SDSS-III

Kyle S. Dawson, David J. Schlegel, Christopher P. Ahn +162

The Baryon Oscillation Spectroscopic Survey (BOSS) is designed to measure the scale of baryon acoustic oscillations (BAO) in the clustering of matter over a larger volume than the…

astro-ph.GA2012★ 21 cited

Galaxies with Background QSOs, I: A Search for Strong Galactic H-alpha Lines

Donald G. York, Lorrie A. Straka, Michael Bishof +12

A search for emission lines in foreground galaxies in quasar spectra (z(gal) < z(QSO)) of the Sloan Digital Sky Survey (SDSS) data release 5 (DR5) reveals 23 examples of quasars sh…

astro-ph.CO2012★ 155 cited

The Sloan Digital Sky Survey Quasar Lens Search. V. Final Catalog from the Seventh Data Release

Naohisa Inada, Masamune Oguri, Min-Su Shin +13

We present the final statistical sample of lensed quasars from the Sloan Digital Sky Survey (SDSS) Quasar Lens Search (SQLS). The well-defined statistical lens sample consists of 2…

astro-ph.CO2012

Monitoring Quasar Colour Variability in Stripe 82

Jesse A. Rogerson, Patrick B. Hall, Chelsea MacLeod +1

Broad Absorption Line (BAL) trough variability is predominantly due to cloud motion transverse to our line of sight. The rate at which the variability occurs indicates the velocity…