Table A.1
Remeasured 
.
| Galaxy name | Flit | Range | Ftotal | Fshadow | Range |
|
|
| (Å) | (Å) | % | % | ||||
|
|
|||||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
|
|
|||||||
| J0921+4509 | 0.30±0.07 | 902-912 | 0.26 |
0.26 |
880-912 | ~1 | ~1 |
| Tol0440−381 | 10.30±2.30 | 882-912 | 3.49 |
2.71 |
880-912 | <7.1 | 1.9 |
| Tol1247−232 | 22.60±6.20 | 882-912 | 2.80 |
2.04 |
880-912 | 4.5±1.2 | 0.40 |
| Mrk 54 | 9.76±2.94 | 882-912 | 1.44 |
<0.67 | 880-912 | 2.5±0.72 | <0.16 |
Notes. Column (1) gives the name of the galaxy, Col. (2) gives the measured LyC average flux level calculated in the range given in Col. (3). Column (4) gives the total LyC flux in our remeasured method, while Col. (5) gives the total flux in just the shadow. Larger Ftotal than Fshadow indicates significant geocoronal Lyman series emission or scattered geocoronal Lyman alpha emission. Both Cols. (4) and (5) are calculated in the range given in Col. (6). Columns (7) and (8) are the fractions measured from Flit and Fshadow, respectively. The errors for Ftotal and Fshadow are given as 1σ errors where we have broken out the statistical and systematic errors as the first and second terms, respectively. The fluxes are in units 10-16 erg cm-2 s-1 Å-1. They are not corrected for Galactic extinction. Note that MRK 54 is not considered a LyC leaker, and it is included in the control sample.
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