TL;DR
This study assesses LSST's potential to detect transiting planets around white dwarfs, estimating detection rates for various planet sizes and habitable zones over a decade-long survey.
Contribution
It provides the first simulation-based estimate of LSST's capability to discover planets orbiting white dwarfs, highlighting its potential for detecting terrestrial planets in habitable zones.
Findings
Detection rates for Ceres to Earth-sized planets range from 5e-6 to 4e-4 per white dwarf.
LSST could detect hundreds of terrestrial planets in habitable zones with 1-10% occurrence.
Approximately 50 to 4,000 planets could be found assuming 100% occurrence rate.
Abstract
White dwarfs are one of the few types of stellar objects for which we know almost nothing about the possible existence of companion planets. Recent evidence for metal contaminated atmospheres, circumstellar debris disks and transiting planetary debris all indicate that planets may be likely. However, white dwarf transit surveys are challenging due to the intrinsic faintness of such objects, the short timescale of the transits and the low transit probabilities due to their compact radii. The Large Synoptic Survey Telescope (LSST) offers a remedy to these problems as a deep, half-sky survey with fast exposures encompassing approximately 10 million white dwarfs with apparent magnitude. We simulate LSST photometric observations of 3.5 million white dwarfs over a ten-year period and calculate the detectability of companion planets with d via transits. We find typical…
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