Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21542111b&link_type=abstract
American Astronomical Society, AAS Meeting #215, #421.11; Bulletin of the American Astronomical Society, Vol. 42, p.288
Astronomy and Astrophysics
Astronomy
Scientific paper
We report on simulations of the exoplanet population detectable by LSST. The temporal coverage, large solid angle and photometric sensitivity of LSST make it a unique instrument for detecting exoplanet transits. We computed numerical detection probabilities for a grid of stellar/planetary radii, at varying inclinations, distances, and position on the sky, using the LSST Operations Simulations. We then conducted a large Monte Carlo simulation of the exoplanet population that LSST might detect. In general, large, super-Jupiter planets transiting M dwarfs present the most likely observed events. We also demonstrate LSST's sensitivity to super-Earth's and Neptune-sized planets, and compare our period-finding algorithm to standard methods. LSST has the potential to discover thousands of new exoplanets, including those around thick disk and halo members, which lie unexplored by current surveys.
Bochanski John J.
Claire Mark W.
No associations
LandOfFree
Simulating the Exoplanet Population Seen by LSST does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Simulating the Exoplanet Population Seen by LSST, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Simulating the Exoplanet Population Seen by LSST will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-967093