Results 91 to 100 of about 2,926,316 (134)
Searching for Free-floating Planets with TESS: Results from Sectors 61–65
Though free-floating planets (FFPs) may outpopulate their bound counterparts in the terrestrial-mass range, they remain one of the least explored exoplanet demographics.
Michelle Kunimoto +4 more
doaj +1 more source
Free-floating planets comprise one of the most enigmatic populations of exoplanets in the Galaxy. Though ground-based observations point to a large abundance of these worlds, little is known about their origins and demographics.
William DeRocco +4 more
doaj +1 more source
International audienceA galactic microlensing effect occurs when a luminous object (the source) located in the Bulge of the Milky Way is temporarily magnified by an intervening star (the "microlens'') passing close to its line of sight.
Cassan, Arnaud
core +2 more sources
The Persistent Missing Mass Problem in Planet Formation
Recent ground-based microlensing surveys suggest that our Galaxy may abound with small free-floating planets, potentially up to ∼21 such planets per star. We explore the implication of such possibility on the mass budget for planet formation.
Eve J. Lee +3 more
doaj +1 more source
Microlensing Constraints on the Stellar and Planetary Mass Functions
The mass function (MF) of isolated objects measured by microlensing consists of both a stellar and a planetary component. We compare the microlensing MFs of A. Gould et al. and T. Sumi et al. to other measurements of the MF. The abundance of brown dwarfs
Jennifer C. Yee, Scott J. Kenyon
doaj +1 more source
A Fast Concentric-disk Contour Integration Method for Microlensing Limb-darkening Effect
Incorporating limb darkening is a computationally demanding step in contour-integration-based microlensing modeling. Conventional concentric-ring integration is incompatible with high-order quadrature schemes, limiting efficiency.
Suwei Wang
doaj +1 more source
The WFIRST Exoplanet Microlensing Survey
The Wide Field Infrared Survey Telescope (WFIRST) was the top ranked large space mission in the 2010 New Worlds, New Horizons decadal survey, and it was formed by merging the science programs of 3 different mission concepts, including the Microlensing ...
Cole, Andrew +32 more
core
Exoplanet Biosignatures: Observational Prospects. [PDF]
Fujii Y +11 more
europepmc +1 more source
EXOPLANET MODULATION OF STELLAR CORONAL RADIO EMISSION. [PDF]
Cohen O +7 more
europepmc +1 more source
The frequency of snowline-region planets from four-years of OGLE-MOA-Wise second-generation microlensing. [PDF]
Shvartzvald Y +37 more
europepmc +1 more source

