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Multiwavelength Transit Observations of the Candidate Disintegrating Planetesimals Orbiting WD 1145+017

  • Authors: Bryce Croll, Paul A. Dalba, Andrew Vanderburg, Jason Eastman, Saul Rappaport, John DeVore, Allyson Bieryla, Philip S. Muirhead, Eunkyu Han, David W. Latham, Thomas G. Beatty, Robert A. Wittenmyer, Jason T. Wright, John Asher Johnson, and Nate McCrady

2017 The Astrophysical Journal 836 82.

  • Provider: AAS Journals

Caption: Figure 1.

Perkins/PRISM, DCT/LMI, FLWO/KeplerCam, and MINERVA photometric observations of WD 1145+017. The UTC date of observations are given in the lower-left of each panel, while the telescope and band of observations are given in the legend at the lower-right. The minutes from mid-event for each night of observations are given from the deepest decrement in flux observed in each night, if this decrement in flux is believed to be statistically significant. For the “MINERVA air x2” and “MINERVA V-band x2” data, observations of two MINERVA telescopes in the “air” and V-bands respectively, have been combined using their weighted mean.

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