activity
19992022
most citedThe VLT-FLAMES Tarantula Survey I: Introduction and observational overview

287 citations · 410 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.HE2022★ 34 cited

The rise and fall of the iron-strong nuclear transient PS16dtm

T. Petrushevska, G. Leloudas, D. Ilic +30

Thanks to the advent of large-scale optical surveys, a diverse set of flares from the nuclear regions of galaxies has recently been discovered. These include the disruption of star…

astro-ph.IM2022★ 4 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.IM2018

The mechanical design of SOXS for the NTT

M Aliverti, O Hershko, O Diner +45

SOXS (Son of X-shooter) is a wide band, medium resolution spectrograph for the ESO NTT with a first light expected in 2021. The instrument will be composed by five semi-independent…

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★ 4 cited

MITS: the Multi-Imaging Transient Spectrograph for SOXS

Adam Rubin, Sagi Ben-Ami, Ofir Hershko +45

The Son Of X-Shooter (SOXS) is a medium resolution spectrograph R~4500 proposed for the ESO 3.6 m NTT. We present the optical design of the UV-VIS arm of SOXS which employs high ef…

astro-ph.HE2016★ 8 cited

Optical photometry and spectroscopy of the low-luminosity, broad-lined Ic supernova iPTF15dld

E. Pian, L. Tomasella, E. Cappellaro +37

Core-collapse stripped-envelope supernova (SN) explosions reflect the diversity of physical parameters and evolutionary paths of their massive star progenitors. We have observed th…