NGC 3621 - Table 2
Cepheid Candidates -- Coordinates and Classification

ID  Chip   R.A.    Declination Comments ID  Chip   R.A.    Declination Comments
              (J2000.0)                               (J2000.0)        

C01 WF2 11:18:21.6 -32:50:19.2  ABfd *  C02 WF4 11:18:14.0 -32:50:58.8  ABC *
C03 PC1 11:18:16.6 -32:50:09.3  ABCd *  C04 WF3 11:18:22.4 -32:51:05.8  aBfd *
C05 WF2 11:18:19.5 -32:49:51.2  aBFs    C06 WF4 11:18:16.3 -32:50:47.7  ABfsd *
C07 WF3 11:18:22.5 -32:50:49.4  ABFFs   C08 PC1 11:18:18.3 -32:50:24.5  DEC  *
C09 WF2 11:18.19.7 -32:50:02.4  aBFFs   C10 PC1 11:18:16.8 -32:50:31.4  aBC *
C11 WF4 11:18:16.0 -32:50:50.5  aEFs    C12 PC1 11:18:18.8 -32:50:16.5  ABFFI 
C13 PC1 11:18:17.1 -32:50:12.7  ABCd *  C14 WF2 11:18:21.4 -32:49:32.7  ABFFs 
C15 WF2 11:18:20.5 -32:50:07.1  ABFFd   C16 PC1 11:18:18.2 -32:50:36.0  ABC *
C17 PC1 11:18:19.0 -32:50:36.3  ABC *   C18 WF2 11:18:19.8 -32:50:20.8  aBFsd 
C19 WF4 11:18:16.1 -32:51:34.8  ABFF    C20 WF2 11:18:22.3 -32:50:30.9  ABfd *
C21 PC1 11:18:18.3 -32:50:40.2  aBdF    C22 WF2 11:18:20.1 -32:49:55.0  aBFFs 
C23 WF2 11:18:19.6 -32:49:38.8  ABFsd   C24 WF3 11:18:23.5 -32:51:44.2  aBCd *
C25 WF2 11:18:24.4 -32:49:53.9  aBf *   C26 WF3 11:18:19.0 -32:51:38.0  DBF 
C27 WF4 11:18:17.3 -32:50:43.5  aBFF    C28 WF4 11:18:17.3 -32:51:12.8  aBfd *
C29 PC1 11:18:18.2 -32:50:39.9  ABCd *  C30 WF4 11:18:15.5 -32:51:44.8  DBF 
C31 WF2 11:18:21.3 -32:49:53.9  aBF     C32 WF2 11:18:19.4 -32:50:35.2  aBFF 
C33 WF2 11:18:20.3 -32:49:40.0  ABFs    C34 WF4 11:18:16.1 -32:51:26.2  aEFF 
C35 PC1 11:18:18.3 -32:50:26.0  aBC *   C36 WF4 11:18:14.7 -32:51:03.8  DEf *
C37 WF2 11:18:21.4 -32:50:18.3  aBfd *  C38 WF2 11:18:19.7 -32:50:10.8  aBFFsd 
C39 WF2 11:18:20.0 -32:50:16.1  ABFF    C40 WF3 11:18:18.7 -32:51:25.2  DBfsd *
C41 WF4 11:18:14.5 -32:51:10.7  ABC *   C42 WF2 11:18:21.6 -32:49:46.7  aBFFd 
C43 WF2 11:18:20.6 -32:50:01.2  DEFFs   C44 WF3 11:18:18.9 -32:51:08.3  ABFd 
C45 WF2 11:18:20.0 -32:49:48.5  aEfs *  C46 WF3 11:18:23.7 -32:50:52.7  ABf *
C47 WF4 11:18:18.0 -32:50:51.0  DBf *   C48 WF4 11:18:18.1 -32:51:11.5  aECd *
C49 WF2 11:18:19.8 -32:50:15.6  aBCs *  C50 WF2 11:18:20.3 -32:50:15.4  ABFs 
C51 PC1 11:18:17.6 -32:50:14.3  ABFF    C52 WF3 11:18:23.6 -32:51:47.3  aBf * 
C53 WF4 11:18:16.3 -32:51:26.4  ABf *   C54 WF2 11:18:20.7 -32:49:59.7  ABfd * 
C55 WF4 11:18:16.6 -32:51:00.9  aBf *   C56 WF2 11:18:23.2 -32:50:34.7  aBCd * 
C57 PC1 11:18:18.2 -32:50:12.5  aEfsd   C58 WF2 11:18:19.5 -32:49:56.6  aBfsd 
C59 WF2 11:18:20.2 -32:50:19.9  aEFs    C60 PC1 11:18:16.1 -32:50:20.2  ABC * 
C61 WF4 11:18:18.2 -32:51:05.7  aBf *   C62 PC1 11:18:18.0 -32:50:35.5  aECd * 
C63 WF3 11:18:20.5 -32:51:43.2  DBfd *  C64 WF2 11:18:19.3 -32:50:42.8  aBF 
C65 WF4 11:18:17.2 -32:51:09.6  DEF     C66 PC1 11:18:18.4 -32:50:37.5  ABfd * 
C67 PC1 11:18:17.4 -32:50:32.6  AECd *  C68 WF2 11:18:19.5 -32:50:29.3  aEFsd 
C69 WF3 11:18:21.3 -32:51:46.7  DBFd                                    

The key to the code used to describe each Cepheid is: (A) well-sampled rise
and decline in the lightcurve, (a) well-sampled decline only, (B) V-band
peak-to-peak lightcurve amplitude of 0.75~mag or greater, (C) isolated star,
(D) poorly sampled lightcurve, (E) low-amplitude lightcurve, (F) companion
within 4 pixel radius, (FF) two or more companion stars within 4 pixel radius,
(I) bad image defect, (d) affected by cosmic rays, (f) companion within 8
pixel radius, but not overlapping (ff) bad confusion in the wings, (i) minor
image defect, (s) large sky gradient. (*) indicates that the Cepheid was
incorporated into the final sample.