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20112026
most citedThe CHEOPS mission

292 citations · 2.8k across the 97 of their papers we have counts for

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13 papers · 1 filter

astro-ph.SR2025★ 2 cited

SN 2016iog: A fast declining Type II-L supernova with an ultra-faint tail, persistently interacting with circumstellar material

Z. -H. Peng, S. Benetti, Y. -Z. Cai +26

We present optical photometric and spectroscopic observations of the rapidly declining Type IIL supernova (SN) 2016iog. SN 2016iog reached its peak 14 days after explosion,…

astro-ph.SR2025★ 3 cited

SN2017ckj: A linearly declining Type IIb supernova with a relatively massive hydrogen envelope

L. -H. Li, S. Benetti, Y. -Z. Cai +26

We present optical observations of the Type IIb supernova (SN) 2017ckj, covering approximately 180 days after the explosion. Its early-time multi-band light curves display no clear…

astro-ph.SR2024

Detailed cool star flare morphology with CHEOPS and TESS

G. Bruno, I. Pagano, G. Scandariato +79

Context. White-light stellar flares are proxies for some of the most energetic types of flares, but their triggering mechanism is still poorly understood. As they are associated wi…

astro-ph.SR2023

The EBLM Project XI. Mass, radius and effective temperature measurements for 23 M-dwarf companions to solar-type stars observed with CHEOPS

M. I. Swayne, P. F. L. Maxted, A. H. M. J. Triaud +104

Observations of low-mass stars have frequently shown a disagreement between observed stellar radii and radii predicted by theoretical stellar structure models. This ``radius inflat…

astro-ph.SR2022★ 25 cited

Connecting photometric and spectroscopic granulation signals with CHEOPS and ESPRESSO

S. Sulis, M. Lendl, H. Cegla +83

Stellar granulation generates fluctuations in photometric and spectroscopic data whose properties depend on the stellar type, composition, and evolutionary state. In this study, we…

astro-ph.SR2021★ 16 cited

A new photometric and dynamical study of the eclipsing binary star HW Virginis

S. B. Brown-Sevilla, V. Nascimbeni, L. Borsato +12

A growing number of eclipsing binary systems of the "HW Vir" kind (i. e., composed by a subdwarf-B/O primary star and an M dwarf secondary) show variations in their orbital period,…

astro-ph.SR2019★ 73 cited

A PSF-based Approach to TESS High quality data Of Stellar clusters (PATHOS) -- I. Search for exoplanets and variable stars in the field of 47 Tuc

D. Nardiello, L. Borsato, G. Piotto +9

The TESS mission will survey ~85 % of the sky, giving us the opportunity of extracting high-precision light curves of millions of stars, including stellar cluster members. In this…

astro-ph.SR2019★ 63 cited

A possibly inflated planet around the bright, young star DS Tuc A

S. Benatti, D. Nardiello, L. Malavolta +13

The origin of the observed diversity of planetary system architectures is one of the main topic of the exoplanetary research. The detection of a statistically significant sample of…

astro-ph.SR2016★ 36 cited

A PSF-based approach to Kepler/K2 data - III. Search for exoplanets and variable stars within the open cluster M 67 (NGC 2682)

D. Nardiello, M. Libralato, L. R. Bedin +5

In the third paper of this series we continue the exploitation of Kepler/K2 data in dense stellar fields using our PSF-based method. This work is focused on a ~720-arcmin^2 region…

astro-ph.SR2015★ 50 cited

Variable stars in one open cluster within the Kepler/K2-Campaign-5 field: M 67 (NGC 2682)

D. Nardiello, M. Libralato, L. R. Bedin +5

In this paper we continue the release of high-level data products from the multiyear photometric survey collected at the 67/92 cm Schmidt Telescope in Asiago. The primary goal of t…

astro-ph.SR2015★ 59 cited

The GAPS Programme with HARPS-N@TNG V. A comprehensive analysis of the XO-2 stellar and planetary systems

M. Damasso, K. Biazzo, A. S. Bonomo +56

XO-2 is the first confirmed wide stellar binary system where the almost twin components XO-2N and XO-2S have planets. This stimulated a detailed characterization study of the stell…

astro-ph.SR2014★ 42 cited

Variable stars in two open clusters within the Kepler 2-Campaign-0 field: M 35 and NGC 2158

D. Nardiello, L. R. Bedin, V. Nascimbeni +15

We present a multi-year survey aimed at collecting (1) high-precision (~5 milli-mag), (2) fast-cadence (~3 min), and (3) relatively long duration (~10 days) multi-band photometric…

astro-ph.SR2013★ 139 cited

The GAPS programme with HARPS-N at TNG. I: Observations of the Rossiter-McLaughlin effect and characterisation of the transiting system Qatar-1

E. Covino, M. Esposito, M. Barbieri +67

A long-term multi-purpose observational programme has started with HARPS-N@TNG aimed to characterise the global architectural properties of exoplanetary systems. In this first pape…