activity
20182022
most citedCHEOPS observations of the HD 108236 planetary system: A fifth planet, improved ephemerides, and planetary radii

82 citations · 178 across the 17 of their papers we have counts for

collaborators

41 papers

astro-ph.IM2022

The Ingot WFS ON an ELT-like telescope: the project and simulations

Elisa Portaluri, Simone Di Filippo, Valentina Viotto +12

The Ingot WFS represents an innovative and indispensable class of sensors conceived to overcome some limitations due to the LGSs geometry, which is significantly different from the…

astro-ph.IM2022

Laboratory testing of the Ingot WFS

Simone Di Filippo, Davide Greggio, Maria Bergomi +9

The ingot WFS is a new kind of wavefront sensor specifically designed to deal with the elongation of LGS reference sources on ELT-class telescopes. Like the pyramid, it belongs to…

astro-ph.IM2022

SOXS AIT: a paradigm for system engineering of a medium class telescope instrument

Riccardo Claudi, Kalyan Radhakrishnan, Federico Battaini +40

SOXS (SOn of X-Shooter) is a high-efficiency spectrograph with a mean Resolution-Slit product of 3500 over the entire band capable of simultaneously observing the complete spectral…

astro-ph.IM20224 cited

From Assembly to the Complete Integration and Verification of the SOXS Common Path

Kalyan Kumar Radhakrishnan Santhakumari, Federico Battaini, Riccardo Claudi +50

The Son Of X-Shooter (SOXS) is a single object spectrograph offering simultaneous spectral coverage in UV-VIS (350-850 nm) and NIR (800-2000 nm) wavelength regimes with an average…

astro-ph.EP202242 cited

Investigating the architecture and internal structure of the TOI-561 system planets with CHEOPS, HARPS-N and TESS

G. Lacedelli, T. G. Wilson, L. Malavolta +115

We present a precise characterization of the TOI-561 planetary system obtained by combining previously published data with TESS and CHEOPS photometry, and a new set of HARPS-N…

astro-ph.SR202129 cited

The EBLM project -- VIII. First results for M-dwarf mass, radius and effective temperature measurements using CHEOPS light curves

M. I. Swayne, P. F. L. Maxted, A. H. M. J. Triaud +93

The accuracy of theoretical mass, radius and effective temperature values for M-dwarf stars is an active topic of debate. Differences between observed and theoretical values have r…