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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 Weight Observatory name

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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