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Title: Revealing the progenitor of SN 2021zby through analysis of the
    TESS shock-cooling light curve 
Authors: Wang Q., Armstrong P., Zenati Y., Ridden-Harper R., Rest A., 
    Arcavi I., Kilpatrick C.D., Foley R.J., Tucker B.E., Lidman C., 
    Killestein T.L., Shahbandeh M., Anderson J.P., Angulo R., Ashall C., 
    Burke J., Chen T.-C., von Coelln S., Dalrymple K.A., Davis K.W., 
    Fulton M.D., Galbany L., Padilla Gonzalez E., Gao B., Gromadzki M., 
    Howell D.A., Ihanec N., Jencson J.E., Jones D.O., Lyman J.D., McCully C., 
    Muller-Bravo T.E., Newsome M., Nicholl M., O'Neill D., Pellegrino C., 
    Rest S., Smartt S.J., Smith K., Srivastav S., Terreran G., Tinyanont S., 
    Young D.R., Zenteno A. 
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Description of contents: This tar.gz archive contains the data behind Figure
    1 of the accepted version of the manuscript listed above. These files
    include the optical light curves of SN 2021zby from TESS and 
    ground-based surveys. The specific files included in this archive are:
    
    21zby_tesslc.mrt                Unbinned TESS light curve
    21zby_tesslc_bin.mrt            Binned TESS light curve
    atlas_1120.mrt                  ATLAS light curve (multi-filter)
    decam_cali_lc.mrt               DECam light curve (multi-filter)
    
System requirements: The files are formatted according to the machine
    readable format used by the AAS Journals and CDS/VizieR. Specific
    information on the structure of MRT files can be found at:
    
        AAS: https://journals.aas.org/mrt-overview/
        CDS: http://cds.u-strasbg.fr/doc/catstd.htx
    
    These files can be read in python using the astropy package:
    
        from astropy.table import Table
        data = Table.read("decam_cali_lc.mrt", format="ascii.cds")
    
    or with the most recent version of TOPCAT (> Version 4.8)
    
Additional comments: ## Please replace this with additional comments
 or even text from the main paper useful for the AAS Journal reader. ##
    
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