Las Campanas Observatory 1m Swope Telescope.
TEK 5 CCD, SITe 1 2048x2048 CCD
The NGC 3201 field was observed using a single pointing centered on the cluster center with a field-of-view of about 24° on the side.
Observations of NGC 3201 were conducted in both V and I filters. Exposure times were 600s in both filters for the time-series data, complemented by single-epoch shorter exposures for color-magnitude diagram purposes.
The data were processed using standard IRAF routines; photometry was done using DoPHOT, subsequent relative photometry using a customized pipeline (akin to standard differential ensemble photometry). Variability detection was based on a chi-squared algorithm, period determination on Minimum-String-Length and Analysis-of-Variance method.
The data parameters fall into the following approximate ranges:
| Field | Min | Max |
|---|---|---|
| RA (2000) | 10 16.466 | 10 18.685 |
| Dec (2000) | -46 36.693 | -46 12.920 |
| HJD of the observation |
2450244.476 | 2450940.531 |
| V magnitude | 16.07 | 23.74 |
| I magnitude | 15.46 | 22.36 |
| Total number of stars | - | 58666 |
| Number of epochs | - | ~120 |
Figure 1: Color image of NGC 3201 with location of detected variable stars.
| NGC 3201 summary file | IPAC ASCII format table |
| NGC 3201 light curves | Download scripts |