Survey for Planets and Exozodiacal Dust Around White Dwarfs

Details Survey for Planets and Exozodiacal Dust Around White Dwarfs Survey for Planets and Exozodiacal Dust Around White Dwarfs

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sptz.prop.2313k&link_type=abstract

Spitzer Proposal ID #2313

Computer Science

Scientific paper

We propose a survey of 134 infrared-bright white dwarfs (WDs) to study their spectral energy distributions and to look for excess emission from orbiting dust and faint companions. This survey will be sensitive to planets and brown dwarfs down to effective temperatures of 300K or less and to dust clouds with 1% of the optical depth of the cloud around G 29-38, the only WD known to host a dust disk.

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