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TESS optical phase curve of KELT-1b
We present the detection and analysis of the phase curve of KELT-1b at optical wavelengths, analyzing data taken by the Transiting Exoplanet Survey Satellite (TESS). The light... -
GJ 740 radial velocities
M-dwarfs have proven to be ideal targets for planetary radial velocity (RV) searches due to their higher planet-star mass contrast, which favors the detection of low-mass... -
Transiting planet WASP-76
Binarity is a widespread phenomenon around solar-type stars, including the host stars of transiting extrasolar planets. We performed a detailed study of six transiting planetary... -
Multiplicity study of transiting exoplanet hosts. I.
Many main-sequence stars are part of multiple systems. The effect of stellar multiplicity on planet formation and migration, however, is poorly understood. We study the... -
WASP-18b HST/WFC3 spectroscopic phase curves
We present the analysis of a full-orbit, spectroscopic phase curve of the ultra hot Jupiter (UHJ) WASP-18b, obtained with the Wide Field Camera 3 aboard the Hubble Space... -
47 single-line eclipsing binaries BEBOP velocities
We introduce the BEBOP radial velocity survey for circumbinary planets. We initiated this survey using the CORALIE spectrograph on the Swiss Euler Telescope at La Silla, Chile.... -
HAT-P-32b differential photometry time series
We obtained 11 photometric time series of secondary eclipse events of the hot Jupiter HAT-P-32b in the Sloan z' band. We inferred the eclipse depth and employed this value to... -
Spectra of Earth-like planets around M-dwarfs
The characterisation of the atmosphere of exoplanets is one of the main goals of exoplanet science in the coming decades. We investigate the detectability of atmospheric... -
Radial velocities of K2-36
K2-36 is a K dwarf orbited by two small (R_b_=1.43+/-0.08R_{earth} and R_c=3.2+/-0.3R_{earth}, close-in (a_b=0.022AU and a_c_=0.054AU) transiting planets discovered by the... -
Kepler-411 mid-transit times
We present a detailed characterization of the Kepler-411 system (KOI 1781). This system was previously known to host two transiting planets: one with a period of 3 days... -
MASCARA-2 b (HD185603) light curves and spectra
In this paper we present MASCARA-2 b, a hot Jupiter transiting the m_V_=7.6 A2 star HD 185603. Since early 2015, MASCARA has taken more than 1.6 million flux measurements of the... -
HD 176986 HARPS + HARPS-N data
We report the discovery of a system of two super-Earths orbiting the moderately active K-dwarf HD 176986. This work is part of the RoPES RV program of G- and K-type stars that... -
Unistellar Exoplanet Campaign
This paper presents early results from and prospects for exoplanet science using a citizen science private/public partnership observer network managed by the SETI Institute in... -
Stellar obliquities in exoplanetary systems
The rotation of a star and the revolutions of its planets are not necessarily aligned. This article reviews the measurement techniques, key findings, and theoretical... -
Masses and RV of exoplanets
Being one of the most fundamental physical parameter of astronomical objects, mass plays a vital role in the study of exoplanets, including their temperature structure, chemical... -
TTVs & linear ephemerides of Kepler exoplanets
We determined new linear ephemerides of transiting exoplanets using long-cadence de-trended data from quarters Q1 to Q17 of Kepler mission. We analysed TTV diagrams of 2098... -
Spin-orbit connection of exoplanets
Star-planet interactions play, among other things, a crucial role in planetary orbital configurations by circularizing orbits, aligning the star and planet spin and... -
70 cool giant exoplanets
Exomoons represent a crucial missing puzzle piece in our efforts to understand extrasolar planetary systems. To address this deficiency, we here describe an exomoon survey of 70... -
nu2 Lupi CHEOPS light curves
Exoplanets transiting bright nearby stars are key objects for advancing our knowledge of planetary formation and evolution. The wealth of photons from the host star gives... -
EPIC 228801451 RV and activity indices
Earth, Venus, Mars and some extrasolar terrestrial planets1 have a mass and radius that is consistent with a mass fraction of about 30% metallic core and 70% silicate mantle. At...