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- W2010845260 abstract "The Hubble Deep Field (HDF) offers the best view to date of the optical sky at faint magnitudes and small angular scales. Early reports suggested that faint source counts continue to rise to the completeness limit of the data, which implies a very large number of galaxies. In this Letter, we use the two-point angular correlation function and number-magnitude relation of sources within the HDF in order to assess their nature. We find that the correlation peaks between 025 and 04 with amplitude of 2 or greater and is much higher for the smallest objects. This angular scale corresponds to physical scales of order 1 kpc for redshifts z ≳ 1. The correlation must therefore derive from objects with subgalactic separations. At faint magnitudes, the counts satisfy the relation number ∝1/flux, which is expected for images that are subdivisions of larger ones." @default.
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- W2010845260 date "1996-12-20" @default.
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- W2010845260 title "Are Hubble Deep Field Galaxy Counts Whole Numbers?" @default.
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- W2010845260 doi "https://doi.org/10.1086/310394" @default.
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