Photometry and Light Curves for the SDSS-II SN Survey

Details Photometry and Light Curves for the SDSS-II SN Survey Photometry and Light Curves for the SDSS-II SN Survey

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aas...209.2802h&link_type=abstract

2007 AAS/AAPT Joint Meeting, American Astronomical Society Meeting 209, #28.02; Bulletin of the American Astronomical Society, V

Astronomy and Astrophysics

Astronomy

Scientific paper

The SDSS-II SN Survey is detecting large numbers of supernovae. We discuss the techniques that are being used to extract brightnesses of these supernovae, including a new scene modelling technique that does not use template-subtracted images, and has the capability to work with data from multiple telescopes. We also describe how the data, which are often taken under non-photometric conditions, are calibrated onto the standard SDSS system. We present some information relative to the understanding of the absolute calibration of the SDSS system. Finally, we show some of the derived light curves.

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