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Table 1
Comparison of estimated characteristics of residuals for 13 selected observatories: mode, “FWHM” and median.
Obs | NLC | Mode | FWHM | Median |
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Weight | Observatory name |
|
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608 | 2459 | 0.26 | 0.20 | 0.27 | 37 | 0 | Haleakala-AMOS |
644 | 2567 | 0.22 | 0.22 | 0.24 | 36 | 0 | Palomar Mountain/NEAT |
683 | 218 | 0.18 | 0.25 | 0.20 | 39 | 0 | Goodricke-Pigott Observatory, Tucson |
689 | 1970 | 0.14 | 0.12 | 0.15 | 118 | 0.3 | U.S. Naval Observatory, Flagstaff |
691 | 1893 | 0.23 | 0.22 | 0.24 | 39 | 0 | Steward Observatory, Kitt Peak-Spacewatch |
699 | 546 | 0.17 | 0.11 | 0.18 | 33 | 0.1 | Lowell Observatory-LONEOS |
703 | 8350 | 0.17 | 0.16 | 0.19 | 54 | 0.15 | Catalina Sky Survey |
704 | 8333 | 0.42 | 0.17 | 0.42 | 311 | 0 | Lincoln Laboratory ETS, New Mexico |
950 | 80 | 0.14 | 0.11 | 0.15 | 180 | 0.15 | La Palma |
E12 | 1354 | 0.14 | 0.16 | 0.15 | 41 | 0.1 | Siding Spring Survey |
G96 | 1810 | 0.14 | 0.22 | 0.17 | 43 | 0.1 | Mt. Lemmon Survey |
H07 | 161 | 0.20 | 0.18 | 0.23 | 47 | 0 | 7300 Observatory, Cloudcroft |
Hip | 49 | 0.10 | 0.10 | 0.11 | 53 | 0.3 | Hipparcos satellite |
Notes. For each observatory, the table gives also the number of sparse lightcurves NLC, and the average number of data points for a single lightcurve .
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