Table 2
Source observation details.
| Code | Source | Class | Vlsr(IF1) | Vlsr(IF2) | Beam | RA0 | Dec0 | Date |
| (km s-1) | (km s-1) | (mas) | (J2000) | (J2000) | (mm/dd/yy) | |||
|
|
||||||||
| BV067A* | OH231.8+4.2 | pre-Planetary Nebula | +44.0 | +26.0 | 1.7 × 0.9 | 07h42m16.93s | –14°42′50 2 |
03/01/09 |
| BV067B | AP Lyn | Mira variable | –19.5 | –32.5 | – | 06h34m34.88s | +60°56′332 |
03/15/09 |
| BV067C | IK Tau | Mira variable | +42.5 | +29.5 | 1.2 × 0.5 | 03h53m28.84s | +11°24′226 |
02/20/09 |
| BV067D | RT Vir | Semi-regular variable | +25.5 | +12.5 | 1.2 × 0.9 | 13h02m37.98s | +05°11′084 |
03/15/09 |
| BV067E | IRC+60370 | Mira variable | –44.5 | –57.5 | 0.8 × 0.5 | 22h49m58.88s | +60°17′567 |
03/05/09 |
|
|
||||||||
| * Presented in Leal-Ferreira et al. (2012) | ||||||||
Notes.From left to right: The project code (Code), the name of the source (Source), the nature of the source (Class), the velocity center position of each of the 2 filters (vlsr), the PSF beam size (Beam), the center coordinates of the observations (RA0 and Dec0), and the starting observation date (Date).
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