We combined photometry, medium / high - resolution spectroscopy, adaptive optics / speckle imaging and archival survey images to rule out any false positive detection scenarios, validate the planet, and further characterize the system.
Not exact matches
We identified several candidates around known stellar members using a combination of color selection and spectral energy distribution... ▽ More We have
combined optical and NIR
photometry from Pan-STARRS 1 and UKIDSS to search the young (5 - 10 Myr) star - forming region of Upper Scorpius for wide (~ 400-4000 AU) substellar companions down to ~ 5 Mjup.
Here we
combine K2
photometry with spectroscopy, adaptive optics imaging, and archival survey images to analyze two small planets orbiting the nearby, field age, M dwarfs K2 - 26 (EPIC 202083828) and K2 - 9.
Abstract: We have
combined optical and NIR
photometry from Pan-STARRS 1 and UKIDSS to search the young (5 - 10 Myr) star - forming region of Upper Scorpius for wide (~ 400-4000 AU) substellar companions down to ~ 5 Mjup.
We
combine the estimate of Teff and [Fe / H] with an estimate o... ▽ More We present the discovery of the Kepler - 19 planetary system, which we first identified from a 9.3 - day periodic transit signal in the Kepler
photometry.
The results are the first from The Kepler Cluster Study which
combine Kepler's
photometry with ground - based spectroscopy for cluster membership and binarity.
Combined with resolved near - infrared
photometry and spectroscopic accretion diagnostics, we find that ~ 10 % of stars with a mid-infrared excess do not appear to be accreting.
We use spectroscopic data from a variety of large surveys
combined with infra - red
photometry from 2MASS and AllWISE and compare these in a Bayesian manner with PARSEC isochrones to derive probability density functions (PDFs) for stellar masses, ages and distances.
The characteristics of the host star are well constrained by high - resolution spectroscopy
combined with an asteroseismic analysis of the Kepler
photometry, leading to an estimated mass and radius of 0.970 + / - 0.060 M... ▽ More A search of the time - series
photometry from NASA's Kepler spacecraft reveals a transiting planet candidate orbiting the 11th magnitude G5 dwarf KIC 10593626 with a period of 290 days.
Combining these new images and
photometry with ancilliary data from the literature, we undertook simultaneous multi-wavelength modelling of the discs» radial profiles and spectral energy distributions using three different methodologies: single annulus, modified black body, and a radiative transfer code.