activity
20172020
most citedExperimental characterization of modal noise in multimode fibers for astronomical spectrometers

19 citations · 43 across the 5 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2020

MOONS Surveys of the Milky Way and its Satellites

O. A. Gonzalez, A. Mucciarelli, L. Origlia +37

The study of resolved stellar populations in the Milky Way and other Local Group galaxies can provide us with a fossil record of their chemo-dynamical and star-formation histories…

astro-ph.IM201919 cited

Experimental characterization of modal noise in multimode fibers for astronomical spectrometers

E. Oliva, M. Rainer, A. Tozzi +3

Starting from our puzzling on-sky experience with the GIANO-TNG spectrometer we set up an infrared high resolution spectrometer in our laboratory and used this instrument to charac…

astro-ph.SR20191 cited

Stellar Population Astrophysics (SPA) with the TNG: Identification of a Sulphur line at lambda(air) = 1063.600nm in GIANO-B stellar spectra

N. Ryde, H. Hartman, E. Oliva +6

Context. In the advent of new infrared, high-resolution spectrometers, accurate and precise atomic data in the infrared is urgently needed. Identifications, wavelengths, strengths,…

astro-ph.SR20193 cited

Stellar population astrophysics (SPA) with the TNG. Characterization of the young open cluster ASCC 123

A. Frasca, J. Alonso-Santiago, G. Catanzaro +10

Star clusters are key to understand the stellar and Galactic evolution. ASCC 123 is a little-studied, nearby and very sparse open cluster. We performed the first high-resolution sp…

astro-ph.SR2019

Stellar population astrophysics (SPA) with the TNG. GIANO-B spectroscopy of red supergiants in Alicante 7 and Alicante 10

L. Origlia, E. Dalessandro, N. Sanna +6

The Scutum complex in the inner disk of the Galaxy hosts a number of young clusters and associations of red supergiant stars that are heavily obscured by dust extinction. These sta…

astro-ph.SR20176 cited

The GAPS Programme with HARPS-N at TNG XV. A substellar companion around a K giant star identified with quasi-simultaneous HARPS-N and GIANO measurements

E. González - Álvarez, L. Affer, G. Micela +34

Context. Identification of planetary companions of giant stars is made difficult because of the astrophysical noise, that may produce radial velocity (RV) variations similar to tho…