NGC 1326-A Table 5 - Astrometry for NGC 1326-A Cepheids ID PL X Y RA(J2000) DEC(J2000) Chip C1 + 185.15 385.24 3:25:05.91 -36:21:37.4 WF2 C2 + 547.56 542.25 3:25:04.95 -36:20:59.9 WF2 C3 + 97.11 690.93 3:25:08.30 -36:21:24.3 WF2 C4 610.93 493.90 3:25:10.40 -36:22:07.5 WF3 C5 + 225.81 312.48 3:25:07.01 -36:22:18.6 WF3 C6 + 463.41 510.73 3:25:05.20 -36:21:08.3 WF2 C7 + 412.55 527.10 3:25:05.58 -36:21:11.1 WF2 C8 299.18 ~94.68 3:25:06.31 -36:21:57.3 WF3 C9 + 224.76 274.70 3:25:05.01 -36:21:41.6 WF2 C10 356.75 221.03 3:25:07.34 -36:22:03.2 WF3 C11 421.88 269.38 3:25:08.01 -36:22:02.7 WF3 C12 + 459.80 303.39 3:25:03.93 -36:21:22.0 WF2 C13 + 239.58 302.26 3:25:07.04 -36:22:16.9 WF3 C14 + 192.82 ~88.33 3:25:05.61 -36:22:03.7 WF3 C15 + 200.38 238.98 3:25:04.91 -36:21:45.8 WF2 C16 + 419.14 189.51 3:25:03.43 -36:21:32.5 WF2 C17 + 435.19 394.31 3:25:08.76 -36:22:11.3 WF3 C18 + 242.22 221.38 3:25:04.32 -36:22:37.0 WF4 C19 485.98 662.95 3:25:06.03 -36:20:56.7 WF2 Notes: 1. Cepheids are ordered by increasing period. 2. PL column is flagged if the cepheid is used in fit to the period-luminosity relation for NGC 1326-A. 3. X and Y coordinates are derived from UT 1997 August 06 epoch. 4. RA and DEC are derived using the IRAF task stsdas.toolbox.imgtools.xy2rd, STSDAS V2.0.1.