Based on observations collected at the Las Campanas Observatory of the Carnegie Institution of Washington.

.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.

The photometric data presented in this paper are available in electronic form at the CDS, via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/Abstract.html

.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.

...OGLE

The OGLE project is currently conducted, under the name OGLE-2, using a dedicated 1.3-m telescope located at Las Campanas Observatory.

.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.

...here)

In fact variability of OGLEGC212, 213, 214, 216, 243, 245 and 246 was reported recently by Kaluzny et al. (1997c). These authors surveyed a western part of the cluster covering a region overlapping with fields 104A and 104C. It is encouraging that all but one variable from Kaluzny et al. (1997c) were recovered in the current study. We missed variable V8 which is very faint and was not included on the list of template stars for the field 104A.

.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.

...Center

The OGLE data (FITS images) are accessible to astronomical community from the NASA NSS Data Center. Send e-mail to: archives@nssdc.gfc.nasa.gov with the subject line: REQUEST OGLE ALL and put requested frame numbers (in the form MR00NNNN where NNNN stands for frame number according to OGLE notation), one per line, in the body of the message. Requested frames will be available using an "anonymous ftp" service from nssdc.gfc.nasa.gov host in location shown in the return e-mail message from archives@nssdc.gsfc.nasa.gov

.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.