activity
20152021
most citedYebes 40 m radio telescope and the broad band NANOCOSMOS receivers at 7 mm and 3 mm for line surveys

143 citations · 517 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2021★ 38 cited

Ultra-deep 31.0-50.3 GHz spectral survey of IRC+10216

J. R. Pardo, J. Cernicharo, B. Tercero +8

Context. IRC+10216, the carbon-rich envelope of the asymptotic giant branch (AGB) star CW Leo, is one of the richest molecular sources in the sky. Available spectral surveys below…

astro-ph.GA2021★ 104 cited

TMC-1, the starless core sulfur factory: Discovery of NCS, HCCS, H2CCS, H2CCCS, and C4S and detection of C5S

J. Cernicharo, C. Cabezas, M. Agundez +7

We report the detection of the sulfur-bearing species NCS, HCCS, H2CCS, H2CCCS, and C4S for the first time in space. These molecules were found towards TMC-1 through the observatio…

astro-ph.GA2021★ 11 cited

Discovery of allenyl acetylene, H2CCCHCCH, in TMC-1. A study of the isomers of C5H4

J. Cernicharo, C. Cabezas, M. Agundez +7

We present the discovery in TMC-1 of allenyl acetylene, H2CCCHCCH, through the observation of nineteen lines with a signal-to-noise ratio ~4-15. For this species, we derived a rota…

astro-ph.GA2021★ 74 cited

Discovery of CH2CHCCH and detection of HCCN, HC4N, CH3CH2CN, and, tentatively, CH3CH2CCH in TMC-1

J. Cernicharo, M. Agundez, C. Cabezas +7

We present the discovery in TMC-1 of vinyl acetylene, CH2CHCCH, and the detection, for the first time in a cold dark cloud, of HCCN, HC4N, and CH3CH2CN. A tentative detection of CH…

astro-ph.IM2020★ 143 cited

Yebes 40 m radio telescope and the broad band NANOCOSMOS receivers at 7 mm and 3 mm for line surveys

F. Tercero, J. A. López-Pérez, J. D. Gallego +23

Yebes 40\,m radio telescope is the main and largest observing instrument at Yebes Observatory and it is devoted to Very Long Baseline Interferometry (VLBI) and single dish observat…

astro-ph.IM2017★ 14 cited

Using radio astronomical receivers for molecular spectroscopic characterization in astrochemical laboratory simulations: A proof of concept

I. Tanarro, B. Alemán, P. de Vicente +26

We present a proof of concept on the coupling of radio astronomical receivers and spectrometers with chemical reactorsand the performances of the resulting setup for spectroscopy a…

astro-ph.GA2016★ 31 cited

28 SiO v=0 J=1-0 emission from evolved stars

P. de Vicente, V. Bujarrabal, A. Díaz-Pulido +18

Observations of 28SiO v=0 J=1-0 line emission (7-mm wavelength) from AGB stars show in some cases peculiar profiles, composed of a central intense component plus a wider plateau. V…

astro-ph.GA2015★ 102 cited

Probing non polar interstellar molecules through their protonated form: Detection of protonated cyanogen (NCCNH+)

M. Agundez, J. Cernicharo, P. de Vicente +19

Cyanogen (NCCN) is the simplest member of the series of dicyanopolyynes. It has been hypothesized that this family of molecules can be important constituents of interstellar and ci…