VizieR Online Data Catalog: GTC transit light curves of HAT-P-11b (Murgas+, 2019)

We present here the transit light curves of the Neptune-sized exoplanet HAT-P-11b obtained on August 30, 2016 and September 25, 2017 using the 10.4-m GTC telescope. The spectra were obtained using OSIRIS instrument in its long-slit spectroscopy mode (40 arcsec slit, R1000B grism, wavelength coverage 360-780 nm). We provide auxiliary parameters of the observations that were use to detrend the original light curves. These parameters are: airmass, position of the stars in spatial and dispersion direction, the relative FWHM of the spectral profile in spatial and dispersion direction, and telescope rotator angle.

(5 data files).