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

@article{Sako2008TheSD,
  title={The Sloan Digital Sky Survey-II Supernova Survey: Search Algorithm and Follow-up Observations},
  author={M. Sako and B. Bassett and A. Becker and D. Cinabro and F. Dejongh and D. Depoy and B. Dilday and M. Doi and J. Frieman and P. Garnavich and C. Hogan and J. Holtzman and S. Jha and R. Kessler and K. Konishi and H. Lampeitl and J. Marriner and G. Miknaitis and R. Nichol and J. Prieto and A. Riess and M. Richmond and R. Romani and D. Schneider and M. Smith and M. SubbaRao and N. Takanashi and K. Tokita and K. V. Heyden and N. Yasuda and C. Zheng and J. Barentine and H. Brewington and C. Choi and J. Dembicky and M. Harnavek and Y. Ihara and M. Im and W. Ketzeback and S. Kleinman and J. Krzesi'nski and D. Long and E. Malanushenko and V. Malanushenko and R. Mcmillan and T. Morokuma and A. Nitta and K. Pan and G. Saurage and S. Snedden},
  journal={The Astronomical Journal},
  year={2008},
  volume={135},
  pages={348-373}
}
The Sloan Digital Sky Survey-II Supernova Survey has identified a large number of new transient sources in a 300 deg2 region along the celestial equator during its first two seasons of a three-season campaign. Multi-band (ugriz) light curves were measured for most of the sources, which include solar system objects, galactic variable stars, active galactic nuclei, supernovae (SNe), and other astronomical transients. The imaging survey is augmented by an extensive spectroscopic follow-up program… Expand
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