... Completed 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 ... plan is to have the Faint Object Spectrograph obtain spectra of both the supernova remnant (SNR) and the bulge of M-31 ...
... 1.15 Completed Two Sets of 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 stars M-31-OB48-2 and HD6201 which are located in galaxy M-31 (aka, The Andromeda Galaxy ...
... 1.18 Completed STIS/CCD/MA1 8033 (UV Extinction in M-31) The Space Telescope Imaging Spectrograph (CCD and MA1) was used to study the ultraviolet extinction in galaxy M-31 by making low dispersion spectra observations of the star M-31-OB6. ...
... 1.11 Completed STIS/CCD 8033 (UV Extinction in M-31) The Space Telescope Imaging Spectrograph (CCD) was used to study the ultraviolet extintion in galaxy M-31 by making low dispersion spectra observations of the star M-31-OB6. ...
... Redshifts of Galaxies in the Hubble Ultra Deep Field, Rafelski, M. et al. (including S. Ravindranath), 2015, AJ, 150, 31 ... 31) Giavalisco, M., et al., ...
... Study: Andromeda way bigger than thought POSTED: 3:31 p.m. EST, January 9, 2007 By Ker Than SPACE.com Adjust font size: (SPACE.com) -- The discovery of several large, metal -poor stars located far from the center of the Andromeda galaxy suggests our ...
... 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 ...
... 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 ...