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20052026
most citedObservation of a Large-scale Anisotropy in the Arrival Directions of Cosmic Rays above eV

409 citations · 1k across the 21 of their papers we have counts for

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Showing astro-ph.SRShow all

6 papers · 1 filter

astro-ph.SR2025★ 1 cited

COSMIC-S: a photometric Catalogue of Observed Stars in the Small MagellanIc Cloud

A. Franco, A. A. Nucita, F. De Paolis +1

The Dark Energy Camera (DECam) is a wide-field instrument mounted on the 4m V. Blanco Telescope (CTIO). Its impressive technical characteristics makes it one of the most suitable g…

astro-ph.SR2023★ 3 cited

New variable sources revealed by DECam toward the LMC: the first 15 deg2

A. Franco, A. A. Nucita, F. De Paolis +2

The Dark Energy Camera (DECam) is a sensitive, wide field instrument mounted at the prime focus of the 4 m V. Blanco Telescope in Chile. Beside its main objectives, i.e. understand…

astro-ph.SR2020

Do subsequent outbursts of the same EXor source present similar features?

T. Giannini, A. Giunta, D. Lorenzetti +4

V1118 Ori is a classical EXor source whose light curve has been monitored over the past thirty years (although not continuously). It underwent a powerful outburst in 2005, followed…

astro-ph.SR2019

Dense cores and star formation in the giant molecular cloud Vela~C

F. Massi, A. Weiss, D. Elia +12

Context The Vela Molecular Ridge is one of the nearest (700 pc) giant molecular cloud (GMC) complexes hosting intermediate-mass (up to early B, late O stars) star formation, and is…

astro-ph.SR2017

The 2015-2016 outburst of the classical EXor V1118 Ori

T. Giannini, S. Antoniucci, D. Lorenzetti +15

After a quiescence period of about 10 years, the classical EXor source V1118 Ori has undergone an accretion outburst in 2015 September. The maximum brightness (DV > 4 mag) was reac…

astro-ph.SR2009★ 10 cited

Pre-Main Sequence variables in the VMR-D : identification of T Tauri-like accreting protostars through Spitzer-IRAC variability

T. Giannini, D. Lorenzetti, D. Elia +6

We present a study of the infrared variability of young stellar objects by means of two Spitzer-IRAC images of the Vela Molecular Cloud D (VMR-D) obtained in observations separated…