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Recurring Planetary Debris Transits and Circumstellar Gas around White Dwarf ZTF J0328–1219

  • Authors: Zachary P. Vanderbosch, Saul Rappaport, Joseph A. Guidry, Bruce L. Gary, Simon Blouin, Thomas G. Kaye, Alycia J. Weinberger, Carl Melis, Beth L. Klein, B. Zuckerman, Andrew Vanderburg, J. J. Hermes, Ryan J. Hegedus, Matthew. R. Burleigh, Ramotholo Sefako, Hannah L. Worters, and Tyler M. Heintz

2021 The Astrophysical Journal 917 41.

  • Provider: AAS Journals

Caption: Figure 4.

Left: the TESS Sector 4 (top) and Sector 31 (bottom) light curves phase-folded on the best-fit B-periods determined from each sector and vertically shifted for clarity. We again split each TESS light curve into first- and second-half components to display changes that occur throughout their ≈26-day durations. The amount of data contained within each phase-folded segment is shown to the left of each light curve in parentheses. Right: the corresponding periodograms of each TESS sector, where solid lines indicate the first-half light curves and dashed lines the second-half ones. Frequencies corresponding to the A- and B-periods (fA and fB) are marked with vertical dotted lines. In TESS Sector 31, the B-period underwent a significant reduction in amplitude from 2.3% ± 0.2% in the first half to 0.8% ± 0.2% in the second half.

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