activity
20172020
most citedAccurate sub-millimetre rest-frequencies for HOCO and DOCO ions

81 citations · 230 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2020★ 27 cited

Distribution of methanol and cyclopropenylidene around starless cores

S. Spezzano, P. Caselli, J. E. Pineda +3

Context. The spatial distribution of molecules around starless cores is a powerful tool for studying the physics and chemistry governing the earliest stages of star formation. Aims…

astro-ph.GA2020★ 4 cited

Extensive ro-vibrational analysis of deuterated-cyanoacetylene (DCN) from millimeter-wavelengths to the infrared domain

M. Melosso, L. Bizzocchi, A. Adamczyk +12

Cyanoacetylene, the simplest cyanopolyyne, is an abundant interstellar molecule commonly observed in a vast variety of astronomical sources. Despite its importance as a potential t…

astro-ph.GA2020★ 66 cited

Propargylimine in the laboratory and in space: millimetre-wave spectroscopy and first detection in the ISM

Luca Bizzocchi, Domenico Prudenzano, Victor M. Rivilla +10

Small imines containing up to three carbon atoms are present in the interstellar medium. As alkynyl compounds are abundant in this medium, propargylimine thus represents a promisin…

physics.comp-ph2019★ 5 cited

Collisional excitation of NH(3Σ-) by Ar: A new ab initio 3D potential energy surface and scattering calculations

D. Prudenzano, F. Lique, R. Ramachandran +2

Collisional excitation of light hydrides is important to fully understand the complex chemical and physical processes of atmospheric and astrophysical environments. Here, we focus…

astro-ph.GA2019★ 34 cited

The chemical structure of the very young starless core L1521E

Z. Nagy, S. Spezzano, P. Caselli +5

L1521E is a dense starless core in Taurus that was found to have relatively low molecular depletion by earlier studies, thus suggesting a recent formation. We aim to characterize t…

astro-ph.GA2018★ 13 cited

Accurate millimetre and submillimetre rest frequencies for - and -dithioformic acid, HCSSH

D. Prudenzano, J. Laas, L. Bizzocchi +6

A better understanding of sulphur chemistry is needed to solve the interstellar sulphur depletion problem. A way to achieve this goal is to study new S-bearing molecules in the lab…