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Expected performances of the Characterising Exoplanet Satellite (CHEOPS). III. Data reduction pipeline: architecture and simulated performances
DOI: 10.1051/0004-6361/201936325 Bibcode: 2020A&A...635A..24H

Guterman, P.; Deleuil, M.; Benz, W. +4 more

The CHaracterizing ExOPlanet Satellite (CHEOPS) is set to be launched in December 2019 and will detect and characterize small size exoplanets via ultra high precision photometry during transits. CHEOPS is designed as a follow-up telescope and therefore it will monitor a single target at a time. The scientific users will retrieve science-ready ligh…

2020 Astronomy and Astrophysics
CHEOPS Gaia 99
The hot dayside and asymmetric transit of WASP-189 b seen by CHEOPS
DOI: 10.1051/0004-6361/202038677 Bibcode: 2020A&A...643A..94L

Guterman, P.; Alonso, R.; Deleuil, M. +103 more

The CHEOPS space mission dedicated to exoplanet follow-up was launched in December 2019, equipped with the capacity to perform photometric measurements at the 20 ppm level. As CHEOPS carries out its observations in a broad optical passband, it can provide insights into the reflected light from exoplanets and constrain the short-wavelength thermal …

2020 Astronomy and Astrophysics
CHEOPS Gaia 85
Mitigating flicker noise in high-precision photometry. I. Characterization of the noise structure, impact on the inferred transit parameters, and predictions for CHEOPS observations
DOI: 10.1051/0004-6361/201937412 Bibcode: 2020A&A...636A..70S

Veronig, A.; Fossati, L.; Lendl, M. +4 more

Context. In photometry, the short-timescale stellar variability ("flicker"), such as that caused by granulation and solar-like oscillations, can reach amplitudes comparable to the transit depth of Earth-sized planets and is correlated over the typical transit timescales. It can introduce systematic errors on the inferred planetary parameters when …

2020 Astronomy and Astrophysics
CHEOPS 23
Expected performances of the Characterising Exoplanet Satellite (CHEOPS). II. The CHEOPS simulator
DOI: 10.1051/0004-6361/201936616 Bibcode: 2020A&A...635A..23F

Queloz, D.; Benz, W.; Deline, A. +14 more

Context. The CHaracterising ExOPlanet Satellite (CHEOPS) is a mission dedicated to the search for exoplanetary transits through high precision photometry of bright stars already known to host planets. The telescope will provide the unique capability of determining accurate radii for planets whose masses have already been measured from ground-based…

2020 Astronomy and Astrophysics
CHEOPS Gaia 15
Expected performances of the Characterising Exoplanet Satellite (CHEOPS). I. Photometric performances from ground-based calibration
DOI: 10.1051/0004-6361/201935977 Bibcode: 2020A&A...635A..22D

Queloz, D.; Benz, W.; Deline, A. +6 more

Context. The characterisation of Earth-size exoplanets through transit photometry has stimulated new generations of high-precision instruments. In that respect, the Characterising Exoplanet Satellite (CHEOPS) is designed to perform photometric observations of bright stars to obtain precise radii measurements of transiting planets. The CHEOPS instr…

2020 Astronomy and Astrophysics
CHEOPS Gaia 14