... 1.5 Completed WF/PC-2 8574 (Proper Motions in Baade'sWindow) The WF/PC-2 was used to obtain third epoch observations of a rich field in Baade'sWindow. ...
... 1.11 Completed WF/PC-2 6185 (Baade'sWindow Proper Motions) The WF/PC-2 was used to make second-epoch observations of the galactic bulge (FIELD-1803 within Baade'sWindow) to study its proper motion of the bulge stars. ...
... 1.4 Completed FOC/96 4546 (Imaging of UV Bright Stars in the galactic Bulge) The Faint Object Camera was used to make observation of the bright ultraviolet star SGR-I which is located in Baade'sWindow. ...
... 1.8 Completed FOC/96 4546 (Imaging of UV Bright Stars in the Galactic Bulge) The Faint Object Camera was used to make observation of the bright ultraviolet star SGR-I (i.e., Sagittarii-I) which is located in Baade'sWindow. ...
... 1.6 Completed FOC/96 4546 (Imaging of UV Bright Stars in the Galactic Bulge) The Faint Object Camera was used to make eight observations of the bright ultraviolet star SGR-I which is located in Baade'sWindow. ...
... Only p oint-like sources will b e observed, and in some regions of the sky, like the Baade'swindow, Centauri or other globular clusters, the star density of the two combined fields of view will b e of the order of 750 000 or more p er square degree ...
... et al. (1995) show that the MS luminosity function of the two clusters is indistinguishable to that of the stars in Baade'sWindow (the low-reddening bulge field at from the Galaxy center), that they have obtained with the ESO NTT with superb seeing ...