Using 3.4-micron Variability towards White Dwarfs as a Signpost of Remnant Planetary Systems

Here we provide the catalog of variables (Catalog_of_3p4um_Variable_WDs_Guidry+2024.csv) and full sample (Full_Variable_WDs_in_WISE_Sample_Guidry+2024.csv) generated by our analysis in https://arxiv.org/abs/2406.18646.

We also provide all of the light curves used in our analysis. Light curve files generated using 2-pixel circular apertures are available in .csv format in AP_Phot_LCs.tar.gz. Our PSF photometry extracted light curves (which we do not analyze in our study) are also provided in PSF_Phot_LCs.tar.gz.