Hubble Deep Field Constraint on Baryonic Dark Matter
Open Access
- 1 August 1996
- journal article
- research article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 466 (2) , L55-L58
- https://doi.org/10.1086/310174
Abstract
We use a new technique to search for faint red stars in the Hubble deep field. We distinguish unambiguously between stars and galaxies to I = 26.3. Our results place strong and general constraints on the I-band luminosity of the constituents of the Galactic dark halo.Keywords
All Related Versions
This publication has 18 references indexed in Scilit:
- Are Hubble Deep Field Galaxy Counts Whole Numbers?The Astrophysical Journal, 1996
- Signatures of white dwarf galaxy halosThe Astrophysical Journal, 1995
- Experimental Limits on the Dark Matter Halo of the Galaxy from Gravitational MicrolensingPhysical Review Letters, 1995
- The Pop. II Lower Main Sequence: Some Properties and a Luminosity Function DeterminationPublished by Springer Nature ,1995
- M dwarfs, microlensing, and the mass budget of the GalaxyThe Astrophysical Journal, 1994
- Density of matter in the Galactic discMonthly Notices of the Royal Astronomical Society, 1994
- Evidence for gravitational microlensing by dark objects in the Galactic haloNature, 1993
- Possible gravitational microlensing of a star in the Large Magellanic CloudNature, 1993
- What the Longest Exposures from the Hubble Space Telescope Will RevealScience, 1990
- The galactic spheroidThe Astrophysical Journal, 1983