activity
20172026
most citedA pair of Sub-Neptunes transiting the bright K-dwarf TOI-1064 characterised with CHEOPS

60 citations · 241 across the 16 of their papers we have counts for

collaborators

18 papers

astro-ph.EP2026

Uncovering temperate worlds: an updated look at the K2-3 system with ESPRESSO

Avidaan Srivastava, Emma Pimentel, Amélie Gressier +24

The K2-3 system is one of the most unique planetary systems as it features three transiting sub-Neptunes in decreasing order of radii, spanning the radius valley. In addition to th…

astro-ph.EP2026

Effect of stellar spot-only spectral lines in high-resolution transit spectroscopy

W. Dethier, E. Cristo, O. D. S. Demangeon +3

We investigate how a representative single spectral line present only in a stellar spot can introduce distortions in high-resolution planetary absorption spectra. Specifically, we…

physics.gen-ph2026

Predicting Radial Velocities from Rossiter-McLaughlin Time Series Observations

Vardan Adibekyan, Olivier Demangeon, Diogo Teixeira +7

The Rossiter-McLaughlin (RM) effect produces apparent radial velocity (RV) shifts through line-profile distortions caused by a transiting planet blocking different regions of the r…

cs.DL2026

Reinforcing Prestige: Journal Citation Biases in Astronomy

Vardan Adibekyan, Olivier Demangeon, Tiago Campante +3

Citations are essential for recognizing scientific contributions, yet citation behavior is shaped by more than just relevance or quality. We analyzed approximately 255,000 refereed…

astro-ph.SR2025★ 1 cited

PoET: the Paranal solar ESPRESSO Telescope

Nuno C. Santos, Alexandre Cabral, Inês Leite +42

The detection and characterisation of other "Earths", orbiting other suns, is a bold objective of present-day astrophysics. However, this quest is severely challenged by astrophysi…

astro-ph.EP2025

Exploring the Neptunian Desert: Insights from a Homogeneous Planetary Sample

Lauren Doyle, David J. Armstrong, Lorena Acuña +26

In this paper, we present a homogeneous analysis of close-in Neptune planets. To do this, we compile a sample of TESS-observed planets using a ranking criterion which takes into ac…

astro-ph.EP2024★ 23 cited

TOI-1408: Discovery and Photodynamical Modeling of a Small Inner Companion to a Hot Jupiter Revealed by TTVs

Judith Korth, Priyanka Chaturvedi, Hannu Parviainen +60

We report the discovery and characterization of a small planet, TOI-1408 c, on a 2.2-day orbit located interior to a previously known hot Jupiter, TOI-1408 b ( d, $M=1.86\p…

astro-ph.IM2024★ 13 cited

The PLATO Mission

Heike Rauer, Conny Aerts, Juan Cabrera +842

PLATO (PLAnetary Transits and Oscillations of stars) is ESA's M3 mission designed to detect and characterise extrasolar planets and perform asteroseismic monitoring of a large numb…

astro-ph.EP2023★ 13 cited

Giant Outer Transiting Exoplanet Mass (GOT 'EM) Survey: III. Recovery and Confirmation of a Temperate, Mildly Eccentric, Single-Transit Jupiter Orbiting TOI-2010

Christopher R. Mann, Paul A. Dalba, David Lafrenière +48

Large-scale exoplanet surveys like the TESS mission are powerful tools for discovering large numbers of exoplanet candidates. Single-transit events are commonplace within the resul…

astro-ph.EP2022★ 60 cited

A pair of Sub-Neptunes transiting the bright K-dwarf TOI-1064 characterised with CHEOPS

Thomas G. Wilson, Elisa Goffo, Yann Alibert +132

We report the discovery and characterisation of a pair of sub-Neptunes transiting the bright K-dwarf TOI-1064 (TIC 79748331), initially detected in TESS photometry. To characterise…

astro-ph.EP2021★ 3 cited

TOI-1431b/MASCARA-5b: A Highly Irradiated Ultra-Hot Jupiter Orbiting One of the Hottest & Brightest Known Exoplanet Host Stars

Brett Christopher Addison, Emil Knudstrup, Ian Wong +70

We present the discovery of a highly irradiated and moderately inflated ultra-hot Jupiter, TOI-1431b/MASCARA-5b (HD 201033b), first detected by NASA's Transiting Exoplanet Survey S…

astro-ph.IM2020

ARCHI: pipeline for light curve extraction of CHEOPS background star

André M. Silva, Sérgio G. Sousa, Nuno Santos +6

High precision time series photometry from space is being used for a number of scientific cases. In this context, the recently launched CHEOPS (ESA) mission promises to bring 20 pp…

astro-ph.EP2020★ 49 cited

Improving transit characterisation with Gaussian process modelling of stellar variability

S. C. C. Barros, O. Demangeon, R. F. Díaz +4

New photometric space missions to detect and characterise transiting exoplanets are focusing on bright stars to obtain high cadence, high signal-to-noise light curves. Since these…

astro-ph.SR2019★ 44 cited

Gaussian Process modelling of granulation and oscillations in red-giant stars

Filipe Pereira, Tiago L. Campante, Margarida S. Cunha +6

The analysis of photometric time series in the context of transiting planet surveys suffers from the presence of stellar signals, often dubbed "stellar noise". These signals, cause…

astro-ph.EP2018

Synergy between asteroseismology and exoplanet science: an outlook

Tiago L. Campante, Susana C. C. Barros, Olivier Demangeon +5

Space-based asteroseismology has been playing an important role in the characterization of exoplanet-host stars and their planetary systems. The future looks even brighter, with sp…

astro-ph.EP2018★ 4 cited

K2 Targets Observed with SPHERE/VLT: An M4-7 Dwarf Companion Resolved around EPIC 206011496

Roxanne Ligi, Olivier Demangeon, Susana Barros +6

The quest to discover exoplanets is one of the most important missions in astrophysics, and is widely performed using the transit method, which allows for the detection of exoplane…

astro-ph.EP2018★ 12 cited

KPS-1b: the first transiting exoplanet discovered using an amateur astronomer's wide-field CCD data

Artem Burdanov, Paul Benni, Eugene Sokov +19

We report the discovery of the transiting hot Jupiter KPS-1b. This exoplanet orbits a V=13.0 K1-type main-sequence star every 1.7 days, has a mass of $M_{…

astro-ph.EP2017★ 19 cited

Distinguishing the albedo of exoplanets from stellar activity

L. M. Serrano, S. C. C. Barros, M. Oshagh +5

Light curves show the flux variation from the target star and its orbiting planets as a function of time. In addition to the transit features created by the planets, the flux also…