Table 1: Journal of all available MIDI observations.
Star UT date & time $\varphi_{\rm Mira}$ Config. Base[m] PA[deg]
HM Sge 2005-07-23 06:48:42 0.75 U2-U3 46.5 44
HD 188512 2005-07-23 07:12:10 ... - ... ...
HM Sge 2005-07-24 02:41:11 0.75 U2-U3 32.1 42
HD 188512 2005-07-24 02:58:55 ... - ... ...
HM Sge 2005-07-24 03:42:18 0.75 U2-U3 37.8 47
HD 188512 2005-07-24 04:03:14 ... - ... ...
HM Sge 2005-07-24 06:14:49 0.75 U2-U3 46.2 47
HD 188512 2005-07-24 06:37:58 ... - ... ...
HM Sge 2006-05-17 09:04:02 0.31 U3-U4 59.3 105
HD 187642 2006-05-17 09:27:14 ... - ... ...
HM Sge 2006-06-11 09:05:09 0.36 U3-U4 46.8 101
HD 187642 2006-06-11 08:42:52 ... - ... ...
HM Sge 2007-04-04 09:39:22 0.93 A0-G1 89 118
HD 187076 2007-04-04 09:06:17 ... - ... ...
HM Sge 2007-05-08 08:52:55 0.99 G1-D0 66 127
HD 167618 2007-05-08 10:16:28 ... - ... ...
HM Sge 2007-05-10 08:34:58 0.99 H0-D0 60 78
HD 187076 2007-05-10 08:55:17 ... - ... ...
HM Sge 2007-05-16 09:48:33 0.00 H0-D0 64 72
HD 206778 2007-05-16 09:20:11 ... - ... ...
HM Sge 2007-07-30 05:54:54 0.15 A0-G1 65 107
HD 206778 2007-07-30 05:23:12 ... - ... ...
The calibrators used to calibrate the visibilities are given below the science target. The phase of the Mira ( $\varphi_{\rm Mira}$) during the observations is indicated. The configuration used for the observations is given. The length and position angle of the projected baseline are also indicated.


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