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Table 2:

Log of the MIDI observations of $\ell $ Car and RS Pup. $\phi $ is the phase of the observation for the Cepheids, relative to the maximum light in V (see Sect. 1 for P and T0 values), B is the projected baseline length, PA is the position angle of the projected baseline (counted East of North = $0^\circ $), and AM is the airmass.
# MJD $\phi $ Target B (m) PA ($^\circ$) AM
A* 53 104.060 0.90 $\ell $ Car 40.82 48.7 1.27
B* 53 104.076   HD 67582 38.86 58.9 1.20
C* 53 104.090 0.90 $\ell $ Car 39.18 56.4 1.28
D* 53 104.104   HD 67582 35.85 63.5 1.31
E 53 842.082 0.66 $\ell $ Car 117.52 74.4 1.30
F 53 842.099   HD 67582 122.80 70.1 1.21
G** 54 045.290 0.90 RS Pup 121.25 31.1 1.29
H 54 046.275 0.92 RS Pup 119.80 27.5 1.36
I 54 046.312   HD 70555 122.87 37.2 1.20
J*** 54 046.343 0.41 $\ell $ Car 130.10 26.5 1.52
K 54 046.372   HD 94510 130.11 20.7 1.57
L 54 047.267 0.95 RS Pup 119.10 25.7 1.40
M 54 047.286   HD 70555 119.62 30.3 1.31
N 54 048.244   HD 70555 114.88 17.3 1.63
O 54 048.270 0.97 RS Pup 119.79 27.5 1.36
P 54 048.347 0.46 $\ell $ Car 130.03 29.3 1.48
Q 54 048.366   HD 94510 130.10 20.4 1.57
* $\ell $ Car observations obtained in 2004 (see Sect. 2.3); ** observation #G of RS Pup was not calibrated;
*** observation #J of $\ell $ Car has a low interferometric flux.

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