activity
20042008
most citedThe Sloan Digital Sky Survey Quasar Catalog IV. Fifth Data Release

479 citations · 949 across the 6 of their papers we have counts for

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astro-ph200863 cited

First-Year Spectroscopy for the SDSS-II Supernova Survey

Chen Zheng, Roger W. Romani, Masao Sako +77

This paper presents spectroscopy of supernovae discovered in the first season of the Sloan Digital Sky Survey-II Supernova Survey. This program searches for and measures multi-band…

astro-ph2008165 cited

Light and Motion in SDSS Stripe 82: The Catalogues

D. M. Bramich, S. Vidrih, L. Wyrzykowski +19

We present a new public archive of light-motion curves in Sloan Digital Sky Survey (SDSS) Stripe 82, covering 99 deg in right ascension from RA = 20.7 h to 3.3 h and spanning 2.52…

astro-ph2007239 cited

The Sloan Digital Sky Survey-II Supernova Survey: Search Algorithm and Follow-up Observations

Masao Sako, B. Bassett, A. Becker +47

The Sloan Digital Sky Survey-II Supernova Survey has identified a large number of new transient sources in a 300 sq. deg. region along the celestial equator during its first two se…

astro-ph2007479 cited

The Sloan Digital Sky Survey Quasar Catalog IV. Fifth Data Release

Donald P. Schneider, Patrick B. Hall, Gordon T. Richards +41

We present the fourth edition of the Sloan Digital Sky Survey (SDSS) Quasar Catalog. The catalog contains 77,429 objects; this is an increase of over 30,000 entries since the previ…

astro-ph20073 cited

An Improved Photometric Calibration of the Sloan Digital Sky Survey Imaging Data

N. Padmanabhan, D. J. Schlegel, D. P. Finkbeiner +21

We present an algorithm to photometrically calibrate wide field optical imaging surveys, that simultaneously solves for the calibration parameters and relative stellar fluxes using…

astro-ph2004

Different Velocity Dependences of Physical Conditions of High- and Low-Ionization Lines in Broad-Line Regions

Stephanie A. Snedden, C. Martin Gaskell

We present results from a study of high- and low-ionization emission line ratios as a function of projected velocity for a sample of eight active galactic nuclei (AGNs). Our result…