Absolute Magnitude is a photometric quantity that denotes the intrinsic brightness of a celestial object, defined as the apparent magnitude it would exhibit if placed at a standard distance of 10 parsecs from the observer.
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Quantifying the Bimodal Color‐Magnitude Distribution of Galaxies
I. K. Baldry, Karl Glazebrook, J. Brinkmann et al. · The Astrophysical Journal · 2004 · 1.6K citations · Full text
Natural Sciences, Astronomy, Physics +13
Edwin Hubble · The Astrophysical Journal · 1926 · 1.2K citations
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California Institute of Technology
Pasadena, United States
40 h-index
246 publications
17.6K citations
University of Arizona
Tucson, United States
37 h-index
116 publications
8.2K citations
University of California, Berkeley
Berkeley, United States
36 h-index
179 publications
15.7K citations
University of Cambridge
Cambridge, United Kingdom
35 h-index
123 publications
25.5K citations
Space Telescope Science Institute
Baltimore, United States
34 h-index
90 publications
8.5K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
33 h-index
100 publications
11.6K citations
Princeton University
Princeton, United States
33 h-index
94 publications
26K citations
Centre National de la Recherche Scientifique
Paris, France
32 h-index
132 publications
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- The Astrophysical Journal
ApJ · 335 publications · 31.9K citations
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- Monthly Notices of the Royal Astronomical Society
237 publications · 13.4K citations
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AJ · 186 publications · 11.7K citations
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- Astronomy and Astrophysics
95 publications · 4.6K citations
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PASP · 42 publications · 1.9K citations
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