Data Products for "An HST Transmission Spectrum of the Closest M-Dwarf Transiting Rocky Planet LTT 1445Ab"

Data for Figures 2, 3, 4, 6, 7, and 8 from the paper "An HST Transmission Spectrum of the Closest M-Dwarf Transiting Rocky Planet LTT 1445Ab".  All are given in .csv files and can easily be plotted in Python. 

Figure 2:  Flux (erg/s/cm^2/A) as a function of wavelength for the three exposures leading up to the flare, the exposure that was taken during the flare, and the first 10 exposures taken after the flare. 

Figure 3: Normalized flux and normalized error as a function of time (BJD_TDB) for the +1 and -1 orders of the WFC3/G280 grism are presented. Data from all three transits are included and are separated by a blank row. 

Figure 4: Wavelength-dependent transit depths for the +1 and -1 order of the WFC3/G280 grism are presented for all three visits. Each order within each visit has two columns, one corresponding to the transit depth value (e.g., "Visit 1 +1 Order (Rp/Rs)^2") and the adjacent column corresponding to the error (e.g., "Visit 1 +1 Order (Rp/Rs)^2 error"). 

Figure 6: Normalized flux and normalized error as a function of time (BJD_TDB) are presented for the WFC3/G141 observation. The first three columns correspond to the forward scan, then there is a gap, and the next three columns correspond to the reverse scan.

Figure 7: Wavelength-dependent transit depths for both reductions (WRECS and ExoTiC-ISM) of the WFC3/G141 observation are presented. Columns are: wavelength (microns), wavelength width (microns), followed by the transit depth and error for each reduction (e.g., "WRECS (Rp/Rs)^2" and "WRECS (Rp/Rs)^2 error". 

Figure 8: Final transmission spectrum including the weighted mean of the three WFC3/G280 observations and the WFC3/G141 observation are given. Columns are wavelength (microns), wavelength width (microns), transit depth, and transit depth error.