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Table 1

Summary of the light curves of WASP-3b analyzed in this work.

N ID Evening Telescope Band Np τ σ σ120 Reference paper Notes
date (s) (mmag) (mmag)

250 G1 2008/05/18 LT-2.0 m (R + V) 4799 3.0 3.97 0.63 Gibson et al. (2008)
309 G2 2008/09/04 LT-2.0 m (R + V) 3900 3.0 3.81 0.61 Gibson et al. (2008) partial
248 T1 2008/05/15 FLWO-1.2 m Sloan i 403 33.8 1.38 0.73 Tripathi et al. (2010) partial
262 T2 2008/06/10 FLWO-1.2 m Sloan i 269 33.6 1.16 0.61 Tripathi et al. (2010) partial
268 T3 2008/06/21 FLWO-1.2 m Sloan i 522 34.2 1.59 0.85 Tripathi et al. (2010)
280 T4 2008/07/13 UH-2.2 m Sloan z 276 67.5 0.81 0.61 Tripathi et al. (2010)
444 T5 2009/05/12 FLWO-1.2 m Sloan g 224 78.3 1.17 0.95 Tripathi et al. (2010)
451 T6 2009/05/25 FLWO-1.2 m Sloan g 238 74.5 1.08 0.85 Tripathi et al. (2010)
486 M1 2009/07/28 Rohzen-0.6 m R 283 49.3 2.06 1.32 Maciejewski et al. (2010)
499 M2 2009/08/21 Rohzen-0.6 m R 200 72.2 2.36 1.83 Maciejewski et al. (2010)
506 M3 2009/09/03 Rohzen-0.6 m R 297 45.8 2.87 1.78 Maciejewski et al. (2010)
519 M4 2009/09/27 Jena-0.9 m R 259 59.6 2.72 1.92 Maciejewski et al. (2010)
539 M5 2009/11/03 Jena-0.9 m R 258 51.6 2.41 1.58 Maciejewski et al. (2010)
629 M6 2010/04/18 Jena-0.9 m R 206 78.0 1.50 1.21 Maciejewski et al. (2010)
486 D1 2009/07/28 OAVdA-0.25 m R 353 46.7 2.30 1.43 Damasso et al. (2010)
290 C1 2008/07/31 HRI-EPOXI clear 1157 53.2 0.89 0.59 Christiansen et al. (2011)
291 C2 2008/08/02 HRI-EPOXI clear 958 51.7 1.01 0.66 Christiansen et al. (2011)
292 C3 2008/08/04 HRI-EPOXI clear 985 51.3 1.03 0.67 Christiansen et al. (2011)
293 C4 2008/08/06 HRI-EPOXI clear 1138 51.3 0.98 0.64 Christiansen et al. (2011)
294 C5 2008/08/08 HRI-EPOXI clear 281 52.2 0.97 0.64 Christiansen et al. (2011) partial
296 C6 2008/08/12 HRI-EPOXI clear 954 54.6 0.93 0.63 Christiansen et al. (2011) partial
297 C7 2008/08/13 HRI-EPOXI clear 640 51.5 1.02 0.67 Christiansen et al. (2011)
298 C8 2008/08/15 HRI-EPOXI clear 852 51.5 1.07 0.70 Christiansen et al. (2011)
654 L1 2010/06/04 SC-11′′ clear 218 76.8 2.68 2.14 Littlefield (2011)
686 L2 2010/08/02 SC-11′′ clear 192 113. 2.38 2.31 Littlefield (2011)
706 L3 2010/09/08 SC-11′′ clear 192 65.5 2.70 1.99 Littlefield (2011)
488 Z1 2009/08/01 Weihai-1 m V 323 43.4 7.35 4.42 Zhang et al. (2011)
444 S1 2009/05/12 VCT-0.5 m Sloan z 177 94.7 2.25 1.99 Sada et al. (2012)
653 S2 2010/06/02 KPNO-2.0 m J 250 71.8 1.50 1.16 Sada et al. (2012)
653 S3 2010/06/02 VCT-0.5 m Sloan z 186 91.1 2.23 1.94 Sada et al. (2012)
842 S4 2011/05/17 VCT-0.5 m Sloan z 217 87.4 3.52 3.00 Sada et al. (2012)

194 E1 2009/04/22 Newton-0.2 m clear 194 74.2 3.36 2.64 ETD obs. Trnka
446 E2 2009/05/16 SC-12′′ I 181 104. 3.18 2.96 ETD obs. Gregorio
653 E3 2010/06/02 SC-12′′ R 177 72.7 2.90 2.26 ETD obs. Shadik & Patrick
666 E4 2010/06/26 Newton-0.3 m B 266 61.6 3.69 2.64 ETD obs. Garlitz
699 E5 2010/08/26 RC-12.5′′ R 119 124. 2.62 2.67 ETD obs. Hose
838 E6 2011/05/09 Monteboo-0.6 m R 393 35.3 2.55 1.38 ETD obs. Janov
849 E7 2011/05/30 RC-12′′ V 297 51.2 5.65 3.69 ETD obs. Dvorak

837 U1 2008/09/03 UDEM-0.36 m I 467 33.7 4.27 2.26 this work
844 U2 2009/06/05 UDEM-0.36 m I 566 34.1 3.78 2.01 this work
864 U3 2009/07/25 UDEM-0.36 m Sloan z 383 45.1 4.38 2.68 this work
877 U4 2009/08/05 UDEM-0.36 m Sloan z 371 44.2 5.03 3.05 this work low S/N
884 U5 2010/08/15 UDEM-0.36 m I 471 35.0 3.31 1.79 this work
837 N1 2011/05/07 IAC-0.8 m R 678 24.0 1.78 0.79 this work
844 N2 2011/05/21 IAC-0.8 m R 742 23.1 1.53 0.67 this work
851 N3 2011/06/02 IAC-0.8 m R 412 38.1 2.93 1.65 this work low S/N
864 N4 2011/06/26 IAC-0.8 m R 566 25.1 1.53 0.70 this work
877 N5 2011/07/20 IAC-0.8 m R 785 20.1 2.12 0.87 this work
884 N6 2011/08/02 IAC-0.8 m R 694 19.9 2.34 0.95 this work red noise

Notes. The columns give: the transit epoch N assuming T = T0 + NP and the original ephemeris (Eq. (1)) from Pollacco et al. (2008), the ID code, the “evening date” of the observation, the filter employed, the number of unbinned data points, the average net cadence τ in seconds, the photometric scatter σ measured as the 68.27th percentile of the residuals from the best-fit model, the normalized photometric scatter , the reference paper or database, and comments.

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