activity
20172021
most citedOptical and ultraviolet pulsed emission from an accreting millisecond pulsar

23 citations · 50 across the 5 of their papers we have counts for

collaborators

7 papers

astro-ph.HE202123 cited

Optical and ultraviolet pulsed emission from an accreting millisecond pulsar

F. Ambrosino, A. Miraval Zanon, A. Papitto +28

Millisecond spinning, low magnetic field neutron stars are believed to attain their fast rotation in a 0.1-1 Gyr-long phase during which they accrete matter endowed with angular mo…

astro-ph.EP202118 cited

The GAPS Programme at TNG. XXIX. No detection of reflected light from 51 Peg b using optical high-resolution spectroscopy

G. Scandariato, F. Borsa, D. Sicilia +44

The analysis of exoplanetary atmospheres by means of high-resolution spectroscopy is an expanding research field which provides information on chemical composition, thermal structu…

astro-ph.IM20209 cited

SOXS End-to-End simulator: development and applications for pipeline design

M. Genoni, M. Landoni, G. Li Causi +44

We present the development of the End-to-End simulator for the SOXS instrument at the ESO-NTT 3.5-m telescope. SOXS will be a spectroscopic facility, made by two arms high efficien…

astro-ph.IM2020

The AIV strategy of the Common Path of Son of X-Shooter

Federico Biondi, Kalyan Kumar Radhakrishnan Santhakumari, Riccardo Claudi +48

Son Of X-Shooter (SOXS) is a double-armed (UV-VIS, NIR) spectrograph designed to be mounted at the ESO-NTT in La Silla, now in its Assembly Integration and Verification (AIV) phase…

astro-ph.IM2018

GIARPS: commissioning and first scientific results

R. Claudi, S. Benatti, I. Carleo +41

GIARPS (GIAno \& haRPS) is a project devoted to have on the same focal station of the Telescopio Nazionale Galileo (TNG) both high resolution spectrographs, HARPS-N (VIS) and GIANO…

astro-ph.EP2018

Multi-band high resolution spectroscopy rules out the hot Jupiter BD+20 1790b - First data from the GIARPS Commissioning

I. Carleo, S. Benatti, A. F. Lanza +51

Context. Stellar activity is currently challenging the detection of young planets via the radial velocity (RV) technique. Aims. We attempt to definitively discriminate the nature o…