This README file contains a description of single quasar stare data taken in the past long baseline tests/campains. These data were taken as "commissioning data," so that there is no script for data reduction. --------------------------------------------------------------- The list of the data with observation date, ExecBlock name, PWV, observation band, source name, longest baseline, and notes is written in 10kmBL-DataStatus.pdf. The data in the list have been observed by a manual command just to observe a single strong quasar without doing any calibration. This is to check and study the stability/fluctuation of amplitude and phase of the system and/or the atmosphere. The data have been taken at the long baseline tests/campaigns in 2012 (2 km baseline test), 2013 (3 km baseline test), and 2014 (10-15 km baseline campaign). All the data are taken in Time Domain Mode (TDM) with both XX and YY polarizations and 4 basebands (BBs) with 2 GHz bandwidth for each BB. Frequency bands that have been used are Bands 3, 6, 7, 8 and 9. Integration time for each data point is about 1 second, and the total observation time were varied data by data, from about 10 minutes to up to 40 minutes. Number of antennas that have been used were also varied data by data, from about 10 antennas to up to about 40 antennas. Further details of the observations are in the list. Due to the commissioning purpose of the data taking, various problems can be in the data, such as amplitude/phase jumps, water vapor radiometer problems, undetermined pad positions, etc., which needs to be carefully examined when using these data. Furthermore, since there is no calibration information as mentioned above, all the values in the data are arbitrary. Publications making use of these data must include the following statement in the acknowledgement: "This paper makes use of the following ALMA data: ADS/JAO.ALMA#2011.0.00003.E. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada) and NSC and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ." In addition, publications from NA authors must include the standard NRAO acknowledgement: "The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc."