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- 8. Surface Brightness Fluctuations
- Faint Dwarf Galaxies in the Next Generation Virgo Cluster Survey
- UV Surface Brightness of Galaxies from the Local Universe to Z
- Arxiv:Astro-Ph/9508054V2 13 Sep 1995
- Fornax, Virgo, Coma, Et Al. ESO, Garching, 27 June - 1 July 2011
- The Dragonfly Wide Field Survey. I. Telescope, Survey Design And
- The Structure of Galaxies I: Surface Photometry Techniques
- University of Groningen Photo-Ionization Studies of Nebulae
- Imaging and Photometry
- The Cosmic Distance Ladder
- Surface Brightness Fluctuation Measurements of Dwarf Elliptical
- Surface Brightness and Magnitude
- A Comprehensive View of the Virgo Stellar Stream?,??
- NGC-6543 (Caldwell 6) the Cat’S Eye Nebula Introduction the Purpose of the Observer’S Challenge Is to Encourage the Pursuit of Visual Observing
- Surface Brightness Luminosity, L, Is the Radiative Power (W ) Emitted by a Source
- Stellar Halos Across the Cosmos July 2-6, MPIA Heidelberg Talk and Poster Abstracts
- The Cosmic Distance Ladder
- Definitions of Magnitudes and Surface Brightness
- Rings and Arcs Around Evolved Stars. II. the Carbon Star AFGL 3068 and the Planetary Nebulae NGC 6543, NGC 7009 and NGC 7027
- What Are Planetary Nebulae?
- Measuring Galaxy Luminosities
- PHYS-638-07F: Problem Set #0 Solutions
- Cosmic Distance Scale
- Cosmic Distance Ladder
- Astronomy 730 / Galaxies
- Structure and Physical Conditions in the Huygens Region of the Orion Nebula C
- University of Groningen Photo-Ionization Studies Of
- Stars Are Made up Entirely of Gas. • Main Properties: Luminosity, Mass, Text Temperature, Chemical Composition, Radius, Evolutionary Stage • Main Sequence
- Lecture 5: Surface Brightness and the Sersic Profile Surface Brightness
- Scattered Light Systematically Distorts Conditions Derived from Emission Lines∗ C