HYPERCALIBRATION: A PAN-STARRS1-BASED RECALIBRATION OF THE SLOAN DIGITAL SKY SURVEY PHOTOMETRY
- Finkbeiner, Douglas P;
- Schlafly, Edward F;
- Schlegel, David J;
- Padmanabhan, Nikhil;
- Jurić, Mario;
- Burgett, William S;
- Chambers, Kenneth C;
- Denneau, Larry;
- Draper, Peter W;
- Flewelling, Heather;
- Hodapp, Klaus W;
- Kaiser, Nick;
- Magnier, EA;
- Metcalfe, N;
- Morgan, Jeffrey S;
- Price, Paul A;
- Stubbs, Christopher W;
- Tonry, John L
- et al.
Abstract
We present a recalibration of the Sloan Digital Sky Survey (SDSS) photometry with new flat fields and zero points derived from Pan-STARRS1. Using point-spread function (PSF) photometry of 60 million stars with 16 < r < 20, we derive a model of amplifier gain and flat-field corrections with per-run rms residuals of 3 millimagnitudes (mmag) in griz bands and 15 mmag in u band. The new photometric zero points are adjusted to leave the median in the Galactic north unchanged for compatibility with previous SDSS work. We also identify transient non-photometric periods in SDSS ("contrails") based on photometric deviations co-temporal in SDSS bands. The recalibrated stellar PSF photometry of SDSS and PS1 has an rms difference of {9, 7, 7, 8} mmag in griz, respectively, when averaged over 15′ regions.