Faint Blue Objects in the Hubble Deep Field South Revealed: White Dwarfs, Subdwarfs, and Quasars

Abstract

We explore the nature of the faint blue objects in the Hubble Deep Field South. We have derived proper motions for the point sources in the Hubble Deep Field South using a 3 year baseline. Combining our proper motion measurements with spectral energy distribution fitting enabled us to identify 4 quasars and 42 stars, including 3 white dwarf candidates. Two of these white dwarf candidates, HDFS 1444 and 895, are found to display significant proper motion, 21.1 $\pm$ 7.9 mas/yr and 34.9 $\pm$ 8.0 mas/yr, and are consistent with being thick disk or halo white dwarfs located at ~2 kpc. The other faint blue objects analyzed by Mendez & Minniti do not show any significant proper motion and are inconsistent with being halo white dwarfs; they do not contribute to the Galactic dark matter. The observed population of stars and white dwarfs is consistent with standard Galactic models.

arXiv commentApJ accepted, 39 pages, 13 figures

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Cited by in corpus (13)

• Evolutionary and pulsational properties of white dwarf stars
• The MUSE 3D view of the Hubble Deep Field South
• A study of the sensitivity of shape measurements to the input parameters of weak lensing image simulations
• The white dwarf luminosity function
• Spectrophotometrically Identified stars in the PEARS-N and PEARS-S fields
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• Trigonometric parallaxes of high velocity halo white dwarf candidates
• The contribution of red dwarfs and white dwarfs to the halo dark matter
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• Spitzer's View of the Candidate Cluster and Protocluster Catalog (CCPC)
• Moving Objects in the Hubble Ultra Deep Field