activity
19942022
most citedHigh-precision photometry by telescope defocussing. I. The transiting planetary system WASP-5

212 citations · 1.7k across the 47 of their papers we have counts for

collaborators

48 papers

astro-ph.SR2022

An Isolated Stellar-Mass Black Hole Detected Through Astrometric Microlensing

Kailash C. Sahu, Jay Anderson, Stefano Casertano +90

We report the first unambiguous detection and mass measurement of an isolated stellar-mass black hole (BH). We used the Hubble Space Telescope (HST) to carry out precise astrometry…

astro-ph.IM2021★ 3 cited

Time delay estimation in unresolved lensed quasars

L. Biggio, A. Domi, S. Tosi +4

Time-delay cosmography can be used to infer the Hubble parameter by measuring the relative time delays between multiple images of gravitationally-lensed quasars. A few of suc…

astro-ph.EP2021★ 14 cited

The ultra-hot-Jupiter KELT-16 b: Dynamical Evolution and Atmospheric Properties

L. Mancini, J. Southworth, L. Naponiello +15

We present broad-band photometry of 30 planetary transits of the ultra-hot Jupiter KELT-16b, using five medium-class telescopes. The transits were monitored through standard B, V,…

astro-ph.IM2020★ 2 cited

Commissioning and improvements of the instrumentation and launch of the scientific exploitation of OARPAF, the Regional Astronomical Observatory of the Antola Park

Davide Ricci, Silvano Tosi, Lorenzo Cabona +17

The \oarpaf telescope is an -diameter optical telescope installed in the Antola Mount Regional Reserve, in Northern Italy. This work presents the results of the character…

astro-ph.IM2018★ 1 cited

The VIS detector system of SOXS

Rosario Cosentino, Matteo Aliverti, Salvatore Scuderi +46

SOXS will be a unique spectroscopic facility for the ESO NTT telescope able to cover the optical and NIR bands thanks to two different arms: the UV-VIS (350-850 nm), and the NIR (8…

astro-ph.IM2018★ 29 cited

Architecture of the SOXS instrument control software

Davide Ricci, Andrea Baruffolo, Bernardo Salasnich +45

SOXS (Son Of X-Shooter) is a new spectrograph for the ESO NTT telescope, currently in the final design phase. The main instrument goal is to allow the characterization of transient…