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Table 1:

Revised and new eclipse times of NN Ser ab with residuals for the light-travel-time effect produced by the two planets of Model 2a1.

E
BJD(TT) Error Residual
  JD2450000+ (days) (s) (s)
(a) Revised, VLT V-band and Wroclaw Obs. white light:
30721 1340.7165402 0.0000023 0.20 -0.03
33233 1667.4780058 0.0000960 8.29 0.35
(b) MONET/North 1.2-m white light photometry:
60489 5212.9418187 0.0000069 0.60 0.23
60505 5215.0230961 0.0000066 0.57 -0.15
60528 5218.0149380 0.0000043 0.37 -0.21
60735 5244.9415254 0.0000029 0.25 0.10
60743 5245.9821654 0.0000032 0.28 0.03
60751 5247.0228063 0.0000034 0.29 0.02
60774 5250.0146469 0.0000034 0.29 -0.16
(c) McDonald 2.1-m photometry with Schott BG40 filter:
60927 5269.9169047 0.0000014 0.12 -0.16
60950 5272.9087487 0.0000013 0.11 -0.04
61426 5334.8268834 0.0000018 0.16 -0.22
61440 5336.6480059 0.0000018 0.16 -0.15
61441 5336.7780894 0.0000015 0.13 0.15
61564 5352.7779443 0.0000016 0.14 0.15
(c) ESO NTT 3.5-m ULTRACAM Sloan g' photometry:
61219 5307.9003015 0.0000010 0.09 0.04
61579 5354.7291448 0.0000009 0.08 0.03

Notes. (1) Table 3 in the electronic version of the journal provides a list of all eclipse times used in this work.


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