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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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