Outer Planet Single-transit Detections with LSST
Abstract
In our solar system massive outer planets dominate in terms of both mass and angular momentum, but few such planets are among the more than 4000 currently confirmed exoplanets, and none of these have accurately determined densities. Here I examine the detection rate of single-transit events anticipated from the LSST deep drilling fields for such planets with periods of 2 - 25 years. Using conservative detection criteria, I anticipate 3-30 such detections over the 10-year period of the project, though distinguishing detections from false positives may prove challenging. However, these few detections are likely to be of great value in understanding the formation, dynamics, and diversity of exoplanet systems.
- Publication:
-
Research Notes of the American Astronomical Society
- Pub Date:
- February 2020
- DOI:
- 10.3847/2515-5172/ab75e3
- arXiv:
- arXiv:2002.05453
- Bibcode:
- 2020RNAAS...4...27B
- Keywords:
-
- Exoplanets;
- Exoplanet detection methods;
- Transit photometry;
- Sky surveys;
- 498;
- 489;
- 1709;
- 1464;
- Astrophysics - Earth and Planetary Astrophysics;
- Astrophysics - Solar and Stellar Astrophysics
- E-Print:
- Accepted for publication in Research Notes of the American Astronomical Society (RNAAS)