Figure 4 from FEELING THE PULL: A STUDY OF NATURAL GALACTIC ACCELEROMETERS. I. PHOTOMETRY OF THE DELICATE STELLAR STREAM OF THE PALOMAR 5 GLOBULAR CLUSTER

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FEELING THE PULL: A STUDY OF NATURAL GALACTIC ACCELEROMETERS. I. PHOTOMETRY OF THE DELICATE STELLAR STREAM OF THE PALOMAR 5 GLOBULAR CLUSTER

Authors: Rodrigo A. Ibata, Geraint F. Lewis, and Nicolas F. Martin

2016 The Astrophysical Journal 819 1.

Provider: AAS Journals

Caption: Figure 4.

Photometric differences between SDSS photometry of stars in the small color–magnitude window ﹩0.3\lt {(g-r)}_{0}\lt 0.4﹩, ﹩16\lt {g}_{0}\lt 18﹩ and the DDO 51 and M-band magnitudes calibrated in this study. The rms of the differences (after clipping ﹩5\sigma ﹩ outliers) is ﹩\lt 0.03﹩ mag in each band.

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