Table 1:

Logbook of the photometric observations of HD 180 642.
Observatory N $\Delta T$ HJD begin HJD end Filter(s) f1
La Silla 20 186.7 50 562.8 50749.6 UB1BB2V1VG 5.4870(2)
La Palma 171 11 83.8 52 421.6 53605.4 UB1BB2V1VG 5.48693(1)
SPMO 113 5.3 53 192.7 53 198.0 u,v,b,y 5.494(3)
SNO 222 359.2 53 205.4 53 564.6 u,v,b,y 5.48693(3)
KO 84 319.2 53 260.3 53 579.5 Johnson V 5.49(1)
KO CCD 261 26.1 53 921.4 53 947.5 Johnson V 5.4858(3)
ASAS 363 2797.6 51 979.9 54 777.5 Johnson V 5.486915(7)
Strömgren 335 371.9 53 192.7 53564.6 u,v,b,y 5.48693(2)
U 526 3042.6 50 562.8 53 605.4 U, u 5.48695(2)
B 526 3042.6 50 562.8 53 605.4 B, v 5.486947(2)
V 526 3042.6 50 562.8 53 605.4 V, y 5.486944(2)
V+ 1234 4214.7 50 562.8 54 777.5 V, y, V 5.486938(5)
The number N of datapoints retained for the analysis, the total timespan $\Delta T$ (in days) and the available filters are given. The last column gives the value of the dominant frequency (see Sect. 2.2) expressed in d-1 with its error between brackets. The HJD is given with respect to ${\it HJD}_0= 2~400~000$. Strömgren refers to merged SPMO and SNO Strömgren data. The merged Geneva U and Strömgren u, B and v, and V and y data, are denoted as U, B, V data, respectively. The V+ dataset corresponds to the V data to which the KO Johnson V data and ASAS Johnson V data are also added.

Source LaTeX | All tables | In the text

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