... 1.6 Completed FOS/BL 5349 (The UV Interstellar Extinction in M-31 and M-33) The Faint Object Spectrograph (Blue Side) was used to make observations of star M-31-OB8-17 which is located in galaxy M-31 (aka, The Andromeda Galaxy) to study interstellar ...
... 1.14 Completed FOS/BL 5349 (The UV Interstellar Extinction in M-31 and M-33) The Faint Object Spectrograph (Blue Side) was used to make observations of star M-31/OB78-2 which are located in galaxy M-31 (aka, The Andromeda Galaxy) to study interstellar ...
... 1.9 Completed NIC/2 7826 (Near-IR Photometry of M-31's Metal-Rich Globular Clusters) The Near Infrared Camera (Cameras Two) were used to make observations of the metal-rich globular clusters in galaxy M-31. ...
... from Accurate Multi-Color WF/PC-2 Photometry of A & B Supergiants in M-31 and M-33) The WF/PC-2 was used to make multi-color ... This is to study A and B supergiant stars in M-31 and M-33 with a precision far exceeding that of existing ground-based ...
... WF/PC-2 6125 (Imaging and Spectroscopy of SN 1885 in = M-31) The WF/PC-2 was used to make observations of Super Nova SN 1885 ... plan is to have the Faint Object Spectrograph = obtain spectra of both the supernova remnant (SNR) and the bulge of M-31 ...
... 2/3 7876 (The Giant Branch Luminosity Function of M-31's Bulge) The Near Infrared Camera (Cameras One, Two and Three) was used ... in the luminous M giant population of the bulge of M-31 is of considerable interest for stellar synthesis work and for ...
... The data range from low Galactic latitude star fields with bright (~16th mag) stars, to very crowded star fields in the surroundings of the M31 dwarf companions to very sparse fields of faint galaxies. ...