The Optical Gravitational lensing Experiment. Variable stars in globular clusters - IV. Fields 104A-E in 47 Tuc J/A+AS/128/19 J/A+AS/128/19 Variable stars in 47 Tuc fields 104A-E The Optical Gravitational lensing Experiment. Variable stars in globular clusters - IV. Fields 104A-E in 47 Tuc J Kaluzny M Kubiak M Szymanski A Udalski W Krzeminski M Mateo K Z Stanek Astron. Astrophys. Suppl. Ser. 128 19 1998 1998A&AS..128...19K I/244 : OGLE General Catalog of Stars. I. (Szymanski+ 1996) II/213 : OGLE Galactic Bulge periodic var. stars. (Udalski+ 1996) J/A+AS/112/407 : Variable Stars in the Sculptor dwarf galaxy (Kaluzny+, 1995) J/A+AS/120/139 : Variables in Omega Cen I. Fields 5139A-C (Kaluzny+ 1996) J/A+AS/122/471 : Variables in Omega Cen. II. Fields 5139D-F (Kaluzny+ 1997) J/A+AS/125/343 : Variables in Omega Cen. III. RR Lyr (Kaluzny+ 1997) Clusters, globular Photometry, CCD Stars, variable binaries: eclipsing blue stragglers globular clusters: individual (NGC 104) Hertzsprung-Russell (HR diagram) Magellanic Clouds stars: variables: other CCD photometry for 42 variables from the field of 47 Tuc = NGC 104 is presented. VI photometry for a large set of stars from the surveyed fields is also given.
NGC 10447 Tuc00 24 05.1-72 04 51
 V band light curve for variables OGLE 218, 239, 252 and 254 OGLE OGLE number --- HJD Heliocentric Julian date d Vmag V magnitude mag e_Vmag Internal error of V magnitude mag Phased V band light curve (tables 5 to 42) OGLE OGLE number --- HJD Heliocentric Julian date d Vmag V magnitude mag e_Vmag Internal error of V magnitude mag Phase Phase --- VI photometry for stars from 104A-E fields (tables 43 to 47) Field Field name (always 104) --- m_Field Multiplicity index in Field --- Xpos X coordinate number=1 The rectangular coordinates X & Y correspond to positions of stars on the "template" images (see paper for details). The X-axis points toward East an the Y axis points toward North. The scale is about 0.435 arcsec/pixel. pix Ypos Y coordinate number=1 The rectangular coordinates X & Y correspond to positions of stars on the "template" images (see paper for details). The X-axis points toward East an the Y axis points toward North. The scale is about 0.435 arcsec/pixel. pix RAdeg Right ascension in degrees, J2000 deg DEdeg Declination in degrees, J2000 deg Vmag V magnitude mag e_Vmag Internal error of V mag V-I V-I color mag e_V-I Internal error of V-I mag Patricia Bauer CDS 1997Sep09Janusz Kaluzny (OGLE-1 team) <jka@vela.astrouw.edu.pl> J_A+AS_128_19.xml