CASCADe: Calibration of trAnsit Spectroscopy using CAusal Data

At present several thousand transiting exoplanet systems have been discovered. For relatively few systems, however, a spectro-photometric characterization of the planetary atmospheres could be performed due to the tiny photometric signatures of the atmospheres and the large systematic noise introduced by the used instruments or the earth atmosphere. Several methods have been developed to deal with instrument and atmospheric noise. These methods include high precision calibration and modeling of the instruments, modeling of the noise using methods like principle component analysis or Gaussian processes and the simultaneous observations of many reference stars. Though significant progress has been made, most of these methods have drawbacks as they either have to make too many assumptions or do not fully utilize all information available in the data to negate the noise terms.

The CASCADe package, developed within the EC Horizons 2020 project Exoplanets A, implements a full spectroscopic pipeline for HST/WFC3 and Spitzer/IRS spectroscopic timeseries observations as well as lightcurve calibration and fitting functionality. The CASCADe project implements a novel “data driven” method, pioneered by Schoelkopf et al (2016) utilizing the causal connections within a data set, and uses this to calibrate the spectral timeseries data of a transiting systems, observed in a single object mode. The current code has been tested successfully on spectroscopic data obtained with the Spitzer and HST observatories, as well as JWST MIRI simulations.

Document version: 1.2.11

CASCADe documentation

Indices and tables