Not exact matches
The KELT images have a pixel
scale of ~ 23 arsec per pixel (similar to TESS) and a large point spread function, and the KELT reduction pipeline uses a weighted
photometric aperture with radius 3 arcmin.
At this angular
scale, multiple sta... ▽ More The Kilodegree Extremely Little Telescope (KELT) project has been conducting a
photometric survey for transiting planets orbiting bright stars for over ten years.
At this angular
scale, multiple stars are typically blended in the
photometric apertures.
The median combined (random and systematic) uncertainties are 2 % (0.01 dex; $ \ log -LCB- g -RCB- $), 3.4 % ($ \ rho $), 2.6 % ($ R$), 5.1 % ($ M$), and 19 % ($ \ tau $) for the
photometric Teff
scale and 2 % ($ \ log -LCB- g -RCB- $), 3.5 % ($ \ rho $), 2.7 % ($ R$), 6.3 % ($ M$), and 23 % ($ \ tau $) for the spectroscopic
scale.