Table 1
GC sample properties.
BAaDE name | OGLE name | RA (J2000) | Dec (J2000) | VLOS (km s-1) | Period (days) |
---|---|---|---|---|---|
ad3a-04238 | OGLE-BLG-LPV-251997 | 17:50:27.528 | –28:18:39.96 | –107 | 504.0 |
ad3a-04347 | OGLE-BLG-LPV-248279 | 17:43:25.800 | –28:12:12.96 | 210 | 405.5 |
ad3a-04350 | OGLE-BLG-LPV-138399 | 17:57:14.688 | –28:12:09.72 | 248 | 455.6 |
ad3a-04376 | OGLE-BLG-LPV-248715 | 17:44:06.456 | –28:10:45.12 | 201 | 362.7 |
ad3a-04404 | OGLE-BLG-LPV-177264 | 18:01:09.408 | –28:08:48.12 | –118 | 456.4 |
ad3a-04412 | OGLE-BLG-LPV-253293 | 17:53:00.000 | –28:08:15.00 | –218 | 482.2 |
ad3a-04415 | OGLE-BLG-LPV-252053 | 17:50:34.248 | –28:08:11.04 | –105 | 524.3 |
ad3a-04418 | OGLE-BLG-LPV-248322 | 17:43:30.312 | –28:07:55.56 | 147 | 273.0 |
ad3a-04425 | OGLE-BLG-LPV-247533 | 17:42:07.776 | –28:07:36.12 | 140 | 405.1 |
ad3a-04433 | OGLE-BLG-LPV-254833 | 17:56:10.656 | –28:07:17.04 | 293 | 557.0 |
Notes. BAaDE and OGLE names for the 370 GC sample sources, as well as source coordinates, maser-derived line-of-sight velocities, and I-band periods. Listed positions are those from 2MASS, accurate to within 0.015″ (Skrutskie et al. 2006) and generally within 1″ of the maser emission (Pihlströmetal. 2018),which are the coordinates used during the BAaDE survey. Coordinates ofthe corresponding OGLE source maybe different by as much as 3″. Uncertainties on the velocities are ±2 km s−1 for all sources and are dominated by the spectral resolution of the BAaDE survey. The full table is only available at the CDS. The first ten rows are presented here to demonstrate the form and content.
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